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<rss xmlns:itunes="http://www.itunes.com/dtds/podcast-1.0.dtd" xmlns:atom="http://www.w3.org/2005/Atom" xmlns:podcast="https://podcastindex.org/namespace/1.0" xmlns:media="http://search.yahoo.com/mrss/" version="2.0"><channel><title>CiTR -- AstroTalk</title><link>https://www.spreaker.com/podcast/citr-astrotalk--4253829</link><description><![CDATA[Space is an interesting place. Marco slices up the night sky with a new topic every week. Death Stars, Black Holes, Big Bang, Red Giants, the Milky Way, G-Bands, Pulsars, Super Stars and the Solar System.]]></description><atom:link href="https://www.spreaker.com/show/4253829/episodes/feed" rel="self" type="application/rss+xml"/><language>en</language><category>Society &amp; Culture</category><copyright>Copyright CiTR &amp; Discorder Magazine</copyright><image><url>https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg</url><title>CiTR -- AstroTalk</title><link>https://www.spreaker.com/podcast/citr-astrotalk--4253829</link></image><lastBuildDate>Wed, 15 Mar 2023 21:19:07 +0000</lastBuildDate><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:owner><itunes:name>CiTR &amp; Discorder Magazine</itunes:name><itunes:email>feeds@spreaker.com</itunes:email></itunes:owner><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:subtitle>Space is an interesting place. Marco slices up the night sky with a new topic every week. Death Stars, Black Holes, Big Bang, Red Giants, the Milky Way, G-Bands, Pulsars, Super Stars and the Solar System.</itunes:subtitle><itunes:summary><![CDATA[Space is an interesting place. Marco slices up the night sky with a new topic every week. Death Stars, Black Holes, Big Bang, Red Giants, the Milky Way, G-Bands, Pulsars, Super Stars and the Solar System.]]></itunes:summary><itunes:category text="Society &amp; Culture"/><itunes:explicit>clean</itunes:explicit><itunes:type>episodic</itunes:type><item><title>AstroTalk - October 24, 2022</title><link>https://www.spreaker.com/episode/astrotalk-october-24-2022--51698474</link><description><![CDATA[AstroTalk - October 24, 2022]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46479-162153-October-24-12-00-00.mp3</guid><pubDate>Mon, 24 Oct 2022 19:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/51698474/astrotalk_46479_162153_october_24_12_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>AstroTalk - October 24, 2022</itunes:subtitle><itunes:summary><![CDATA[AstroTalk - October 24, 2022]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>AstroTalk - Sept 29, 2022</title><link>https://www.spreaker.com/episode/astrotalk-sept-29-2022--51698473</link><description><![CDATA[AstroTalk - Sept 29, 2022]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46478-162152-September-29-14-00-00.mp3</guid><pubDate>Thu, 29 Sep 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/51698473/astrotalk_46478_162152_september_29_14_00_00.mp3" length="59810483" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>AstroTalk - Sept 29, 2022</itunes:subtitle><itunes:summary><![CDATA[AstroTalk - Sept 29, 2022]]></itunes:summary><itunes:duration>3739</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>AstroTalk - Sept 22, 2022</title><link>https://www.spreaker.com/episode/astrotalk-sept-22-2022--51698475</link><description><![CDATA[AstroTalk - Sept 22, 2022]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46477-162151-September-22-14-00-00.mp3</guid><pubDate>Thu, 22 Sep 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/51698475/astrotalk_46477_162151_september_22_14_00_00.mp3" length="49345617" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>AstroTalk - Sept 22, 2022</itunes:subtitle><itunes:summary><![CDATA[AstroTalk - Sept 22, 2022]]></itunes:summary><itunes:duration>3085</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>AstroTalk - Sept 15, 2022</title><link>https://www.spreaker.com/episode/astrotalk-sept-15-2022--51698482</link><description><![CDATA[AstroTalk - Sept 15, 2022]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46476-162150-September-15-14-00-00.mp3</guid><pubDate>Thu, 15 Sep 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/51698482/astrotalk_46476_162150_september_15_14_00_00.mp3" length="55791537" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>AstroTalk - Sept 15, 2022</itunes:subtitle><itunes:summary><![CDATA[AstroTalk - Sept 15, 2022]]></itunes:summary><itunes:duration>3487</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>AstroTalk - Sept 8, 2022</title><link>https://www.spreaker.com/episode/astrotalk-sept-8-2022--51698478</link><description><![CDATA[AstroTalk - Sept 8, 2022]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46475-162149-September-08-14-00-00.mp3</guid><pubDate>Thu, 08 Sep 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/51698478/astrotalk_46475_162149_september_08_14_00_00.mp3" length="55791530" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>AstroTalk - Sept 8, 2022</itunes:subtitle><itunes:summary><![CDATA[AstroTalk - Sept 8, 2022]]></itunes:summary><itunes:duration>3487</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Astrotalk - Sept 1, 2022</title><link>https://www.spreaker.com/episode/astrotalk-sept-1-2022--51261666</link><description><![CDATA[Astrotalk - Sept 1, 2022]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46234-161908-September-01-14-00-00.mp3</guid><pubDate>Thu, 01 Sep 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/51261666/astrotalk_46234_161908_september_01_14_00_00.mp3" length="55763797" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Astrotalk - Sept 1, 2022</itunes:subtitle><itunes:summary><![CDATA[Astrotalk - Sept 1, 2022]]></itunes:summary><itunes:duration>3486</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Astrotalk - August 25, 2022</title><link>https://www.spreaker.com/episode/astrotalk-august-25-2022--51261665</link><description><![CDATA[Astrotalk - August 25, 2022]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46233-161907-August-25-14-00-00.mp3</guid><pubDate>Thu, 25 Aug 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/51261665/astrotalk_46233_161907_august_25_14_00_00.mp3" length="44981711" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Astrotalk - August 25, 2022</itunes:subtitle><itunes:summary><![CDATA[Astrotalk - August 25, 2022]]></itunes:summary><itunes:duration>2812</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Astrotalk - August 18, 2022</title><link>https://www.spreaker.com/episode/astrotalk-august-18-2022--51261669</link><description><![CDATA[Astrotalk - August 18, 2022]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46232-161906-August-18-14-00-00.mp3</guid><pubDate>Thu, 18 Aug 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/51261669/astrotalk_46232_161906_august_18_14_00_00.mp3" length="59172827" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Astrotalk - August 18, 2022</itunes:subtitle><itunes:summary><![CDATA[Astrotalk - August 18, 2022]]></itunes:summary><itunes:duration>3699</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Astrotalk - August 11, 2022</title><link>https://www.spreaker.com/episode/astrotalk-august-11-2022--51261668</link><description><![CDATA[Astrotalk - August 11, 2022]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46231-161905-August-11-14-00-00.mp3</guid><pubDate>Thu, 11 Aug 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/51261668/astrotalk_46231_161905_august_11_14_00_00.mp3" length="55380499" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Astrotalk - August 11, 2022</itunes:subtitle><itunes:summary><![CDATA[Astrotalk - August 11, 2022]]></itunes:summary><itunes:duration>3462</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--50810628</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46060-161734-July-21-14-00-00.mp3</guid><pubDate>Thu, 21 Jul 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/50810628/astrotalk_46060_161734_july_21_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>July 21 2022 Show</title><link>https://www.spreaker.com/episode/july-21-2022-show--50795721</link><description><![CDATA[NASATV. There are many interesting shows by the hour on NASAA TV. aeach sghow last 1/2 hour and is packed with interesting info about Astronomy. Reaswons why AWebbh Telescope was delayed from orignal launch dat eo f2007 until Dec 2021? Complexity of building the telescope and over optimisti8c projections. The mirros, for example, operate at cold temps, close to aboslute zero, in wspace. But they are tested at romm temperature on ASEarth. AWhen the mirros are unfolded in space, they will warp differently than they do on AEarth, so fitting them together is crucial. Also, on a typical NASA launch are are 5 to 10 failure opoints. If any oif these 10 go wrong, the mission is mostl likely scrubbed. On the AWsebb launch, there were 344 fgilure points. Much more comp[licate, risky abnd dangerous. ISS research on flames and fire. Flames burn differently in space anbd micro-G. Learning about this can make engines burn efficiently on Aearth. Building protections in power grids on Aearth, against solar storms. SAcienties are studying a very dangerous solar storm 9,200 years ago and during the Carrington AEvenmt in SApet 1859. It any of these 2 storms hit now, AEarth's power grids would not be protected. There could be ctostrophic damage. It is dangerous when solar storms smah into AEarth's atmosphere at the wrong part of the solar cycle. Need to build in better protections. The SLS SApace Launch SAystem of rocket s are being tested for a treturn to the moon, and possible Mars. THE SLSA Mego Moon Roacke twas rollde out in June on a dress rehearsal.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46043-161717-July-21-14-00-00.mp3</guid><pubDate>Thu, 21 Jul 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/50795721/astrotalk_46060_161734_july_21_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>NASATV. There are many interesting shows by the hour on NASAA TV. aeach sghow last 1/2 hour and is packed with interesting info about Astronomy. Reaswons why AWebbh Telescope was delayed from orignal launch dat eo f2007 until Dec 2021? Complexity of...</itunes:subtitle><itunes:summary><![CDATA[NASATV. There are many interesting shows by the hour on NASAA TV. aeach sghow last 1/2 hour and is packed with interesting info about Astronomy. Reaswons why AWebbh Telescope was delayed from orignal launch dat eo f2007 until Dec 2021? Complexity of building the telescope and over optimisti8c projections. The mirros, for example, operate at cold temps, close to aboslute zero, in wspace. But they are tested at romm temperature on ASEarth. AWhen the mirros are unfolded in space, they will warp differently than they do on AEarth, so fitting them together is crucial. Also, on a typical NASA launch are are 5 to 10 failure opoints. If any oif these 10 go wrong, the mission is mostl likely scrubbed. On the AWsebb launch, there were 344 fgilure points. Much more comp[licate, risky abnd dangerous. ISS research on flames and fire. Flames burn differently in space anbd micro-G. Learning about this can make engines burn efficiently on Aearth. Building protections in power grids on Aearth, against solar storms. SAcienties are studying a very dangerous solar storm 9,200 years ago and during the Carrington AEvenmt in SApet 1859. It any of these 2 storms hit now, AEarth's power grids would not be protected. There could be ctostrophic damage. It is dangerous when solar storms smah into AEarth's atmosphere at the wrong part of the solar cycle. Need to build in better protections. The SLS SApace Launch SAystem of rocket s are being tested for a treturn to the moon, and possible Mars. THE SLSA Mego Moon Roacke twas rollde out in June on a dress rehearsal.]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--50810629</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46059-161733-July-14-14-00-00.mp3</guid><pubDate>Thu, 14 Jul 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/50810629/astrotalk_46059_161733_july_14_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--50810388</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46058-161732-July-07-14-00-00.mp3</guid><pubDate>Thu, 07 Jul 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/50810388/astrotalk_46058_161732_july_07_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--50810387</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46057-161731-July-07-14-00-00.mp3</guid><pubDate>Thu, 07 Jul 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/50810387/astrotalk_46057_161731_july_07_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>June 30 2022 SAhow</title><link>https://www.spreaker.com/episode/june-30-2022-sahow--50806772</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46054-161728-June-30-14-00-00.mp3</guid><pubDate>Thu, 30 Jun 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/50806772/astrotalk_46054_161728_june_30_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--50805880</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46052-161726-June-23-14-00-00.mp3</guid><pubDate>Thu, 23 Jun 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/50805880/astrotalk_46052_161726_june_23_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>June 16 Show</title><link>https://www.spreaker.com/episode/june-16-show--50795984</link><description><![CDATA[Is global warming responsible for our cool spring? Major planetary alignmnent on the way. All planets, will be aligned, in order, in the night sky. WAill next happen in 186 years. The Chginese are threatening to shoot down aelon Musk's satellites because he believes they are spyting on Chinese interests. VChina has a telescope, FAST, the world's bigfest radio telescope. 500 meters across. FAAST picks up anaomolouys signals. Are they alien signals? Might just be radio interference. Also picking up Fast Periodic Bu8rsts, ir fast radio bursts, FRBs. Carry more energy in 1 milliseconde than the sun emits in 11 year. FRBs come and go quickly . 2020 first FRB found in the Milky AWay. Came from a magnetar, ahighly magnetized neutron star. 3 B LYs away. goes in different cyklces. 90 days of powerful radio bursts,m then 57 days of mild radio bursts. Then 157 flares across 47 days. Video of AWebb and its insturment suite. A micro-meteor impact occurred on one of AWebb's mirros on May 23 - 25. Did damage that cannot be fixed./  AWe4bb is going to open views of the most distant galaxies, but it will also allow scientists to see in m ore clarity inside our own solar stystem. Things like planets, asteroids and the Puiper Belt. More excitment in sotre with AWebb.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46045-161719-June-16-14-00-00.mp3</guid><pubDate>Thu, 16 Jun 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/50795984/astrotalk_46045_161719_june_16_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Is global warming responsible for our cool spring? Major planetary alignmnent on the way. All planets, will be aligned, in order, in the night sky. WAill next happen in 186 years. The Chginese are threatening to shoot down aelon Musk's satellites...</itunes:subtitle><itunes:summary><![CDATA[Is global warming responsible for our cool spring? Major planetary alignmnent on the way. All planets, will be aligned, in order, in the night sky. WAill next happen in 186 years. The Chginese are threatening to shoot down aelon Musk's satellites because he believes they are spyting on Chinese interests. VChina has a telescope, FAST, the world's bigfest radio telescope. 500 meters across. FAAST picks up anaomolouys signals. Are they alien signals? Might just be radio interference. Also picking up Fast Periodic Bu8rsts, ir fast radio bursts, FRBs. Carry more energy in 1 milliseconde than the sun emits in 11 year. FRBs come and go quickly . 2020 first FRB found in the Milky AWay. Came from a magnetar, ahighly magnetized neutron star. 3 B LYs away. goes in different cyklces. 90 days of powerful radio bursts,m then 57 days of mild radio bursts. Then 157 flares across 47 days. Video of AWebb and its insturment suite. A micro-meteor impact occurred on one of AWebb's mirros on May 23 - 25. Did damage that cannot be fixed./  AWe4bb is going to open views of the most distant galaxies, but it will also allow scientists to see in m ore clarity inside our own solar stystem. Things like planets, asteroids and the Puiper Belt. More excitment in sotre with AWebb.]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--50795985</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46046-161720-June-09-14-00-00.mp3</guid><pubDate>Thu, 09 Jun 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/50795985/astrotalk_46046_161720_june_09_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>June 2, 2022</title><link>https://www.spreaker.com/episode/june-2-2022--50795986</link><description><![CDATA[Blah]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-46044-161718-June-02-14-00-00.mp3</guid><pubDate>Thu, 02 Jun 2022 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/50795986/astrotalk_46044_161718_june_02_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Blah</itunes:subtitle><itunes:summary><![CDATA[Blah]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Astrotalk - Jan 27, 2022</title><link>https://www.spreaker.com/episode/astrotalk-jan-27-2022--48849287</link><description><![CDATA[Astrotalk - Jan 27, 2022]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2022/AstroTalk-45272-160946-January-27-14-00-00.mp3</guid><pubDate>Thu, 27 Jan 2022 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/48849287/astrotalk_45272_160946_january_27_14_00_00.mp3" length="53296065" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Astrotalk - Jan 27, 2022</itunes:subtitle><itunes:summary><![CDATA[Astrotalk - Jan 27, 2022]]></itunes:summary><itunes:duration>3331</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>A</title><link>https://www.spreaker.com/episode/a--43983189</link><description><![CDATA[A]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2021/AstroTalk-43638-159313-March-18-14-00-00.mp3</guid><pubDate>Thu, 18 Mar 2021 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/43983189/astrotalk_43638_159313_march_18_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>A</itunes:subtitle><itunes:summary><![CDATA[A]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--43968206</link><description><![CDATA[aa]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2021/AstroTalk-43628-159303-March-11-14-00-00.mp3</guid><pubDate>Thu, 11 Mar 2021 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/43968206/astrotalk_43628_159303_march_11_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>aa</itunes:subtitle><itunes:summary><![CDATA[aa]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>1</title><link>https://www.spreaker.com/episode/1--43968205</link><description><![CDATA[1]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2021/AstroTalk-43626-159301-March-04-14-00-00.mp3</guid><pubDate>Thu, 04 Mar 2021 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/43968205/astrotalk_43626_159301_march_04_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>1</itunes:subtitle><itunes:summary><![CDATA[1]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>`</title><link>https://www.spreaker.com/episode/kyzh2--43968208</link><description><![CDATA[1]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2021/AstroTalk-43625-159300-February-25-14-00-00.mp3</guid><pubDate>Thu, 25 Feb 2021 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/43968208/astrotalk_43625_159300_february_25_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>1</itunes:subtitle><itunes:summary><![CDATA[1]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>`</title><link>https://www.spreaker.com/episode/kyzh2--43968207</link><description><![CDATA[s]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2021/AstroTalk-43627-159302-February-18-14-00-00.mp3</guid><pubDate>Thu, 18 Feb 2021 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/43968207/astrotalk_43627_159302_february_18_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>s</itunes:subtitle><itunes:summary><![CDATA[s]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--43650231</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2021/AstroTalk-43526-159201-February-11-14-00-00.mp3</guid><pubDate>Thu, 11 Feb 2021 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/43650231/astrotalk_43526_159201_february_11_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--43650234</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2021/AstroTalk-43525-159200-February-04-14-00-00.mp3</guid><pubDate>Thu, 04 Feb 2021 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/43650234/astrotalk_43525_159200_february_04_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Wolf Moon. 3 Minutes After The Big Bang. Dark Matter Discussion.</title><link>https://www.spreaker.com/episode/wolf-moon-3-minutes-after-the-big-bang-dark-matter-discussion--43650232</link><description><![CDATA[`A Wolf Moon in January. New Research suggests an early kick just after the Big Bangt created Dark Matter. <br /><br />Dark Matter Discussion.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2021/AstroTalk-43524-159199-January-28-14-00-00.mp3</guid><pubDate>Thu, 28 Jan 2021 21:00:17 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/43650232/astrotalk_43524_159199_january_28_14_00_00.mp3" length="57344000" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>`A Wolf Moon in January. New Research suggests an early kick just after the Big Bangt created Dark Matter. 

Dark Matter Discussion.</itunes:subtitle><itunes:summary><![CDATA[`A Wolf Moon in January. New Research suggests an early kick just after the Big Bangt created Dark Matter. <br /><br />Dark Matter Discussion.]]></itunes:summary><itunes:duration>3584</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--43650233</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2021/AstroTalk-43523-159198-January-21-14-00-00.mp3</guid><pubDate>Thu, 21 Jan 2021 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/43650233/astrotalk_43523_159198_january_21_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>A</title><link>https://www.spreaker.com/episode/a--43648395</link><description><![CDATA[A]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2021/AstroTalk-43522-159197-January-14-14-00-00.mp3</guid><pubDate>Thu, 14 Jan 2021 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/43648395/astrotalk_43522_159197_january_14_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>A</itunes:subtitle><itunes:summary><![CDATA[A]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Planck Length. Finding Exoplanets Similar to Earth. 77% of Stars in MW are Red Dwarf Stars. A Giant Black Hole Keeps Avoiding Detection. Nin</title><link>https://www.spreaker.com/episode/planck-length-finding-exoplanets-similar-to-earth-77-of-stars-in-mw-are-red-dwarf-stars-a-giant-black-hole-keeps-avoiding-detection-nin--43648394</link><description><![CDATA[Planck Length. Zepo-second. Review of the significanace of this data. 77% of Stars in MW are Red Dwarf Stars. Astros are trying to find Earth-like planets around Red Dwarfs.  But some rocky exo-planets are close to their Red Dwarf stars. A Giant Black Hole Keeps Avoiding Detection.  A big galaxy at the core of cluster Abell 2261,  2.7 billion light-years from Earth, should have an even larger central black hole — a light-gobbling monster that weighs as much as 3 billion to 100 billion suns, astronomers estimate from the galaxy's mass. But the exotic object has evaded detection so far. Largest canyon in Solar System revealed on  Mars.  Look on Hi-Rise website Nine epic astronomy discoveries you may have missed in 2020. Fermi Bubbles discovered  in the X-Ray bublbles.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2021/AstroTalk-43521-159196-January-07-14-00-00.mp3</guid><pubDate>Thu, 07 Jan 2021 21:01:29 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/43648394/astrotalk_43521_159196_january_07_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Planck Length. Zepo-second. Review of the significanace of this data. 77% of Stars in MW are Red Dwarf Stars. Astros are trying to find Earth-like planets around Red Dwarfs.  But some rocky exo-planets are close to their Red Dwarf stars. A Giant Black...</itunes:subtitle><itunes:summary><![CDATA[Planck Length. Zepo-second. Review of the significanace of this data. 77% of Stars in MW are Red Dwarf Stars. Astros are trying to find Earth-like planets around Red Dwarfs.  But some rocky exo-planets are close to their Red Dwarf stars. A Giant Black Hole Keeps Avoiding Detection.  A big galaxy at the core of cluster Abell 2261,  2.7 billion light-years from Earth, should have an even larger central black hole — a light-gobbling monster that weighs as much as 3 billion to 100 billion suns, astronomers estimate from the galaxy's mass. But the exotic object has evaded detection so far. Largest canyon in Solar System revealed on  Mars.  Look on Hi-Rise website Nine epic astronomy discoveries you may have missed in 2020. Fermi Bubbles discovered  in the X-Ray bublbles.]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--43648397</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-43520-159195-December-31-14-00-00.mp3</guid><pubDate>Thu, 31 Dec 2020 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/43648397/astrotalk_43520_159195_december_31_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>A</title><link>https://www.spreaker.com/episode/a--42653668</link><description><![CDATA[AA]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-43258-158938-December-24-14-00-00.mp3</guid><pubDate>Thu, 24 Dec 2020 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/42653668/astrotalk_43258_158938_december_24_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>AA</itunes:subtitle><itunes:summary><![CDATA[AA]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>A</title><link>https://www.spreaker.com/episode/a--42644836</link><description><![CDATA[A]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-43256-158936-December-17-14-00-00.mp3</guid><pubDate>Thu, 17 Dec 2020 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/42644836/astrotalk_43256_158936_december_17_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>A</itunes:subtitle><itunes:summary><![CDATA[A]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>A</title><link>https://www.spreaker.com/episode/a--42342122</link><description><![CDATA[A]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-43175-158855-December-03-14-00-00.mp3</guid><pubDate>Thu, 03 Dec 2020 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/42342122/astrotalk_43175_158855_december_03_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>A</itunes:subtitle><itunes:summary><![CDATA[A]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Moving Planets and Exo-Planets. Locating Brown Dwarfs, or Super Planets. Solar Power Statins in Space. Radio Telescope in Space.</title><link>https://www.spreaker.com/episode/moving-planets-and-exo-planets-locating-brown-dwarfs-or-super-planets-solar-power-statins-in-space-radio-telescope-in-space--42367129</link><description><![CDATA[By studying exo-planet formation, this adds to the knowledge base of how planets form, and how they can move. Jupiter moved in its orbit a lot in the early solar system, and this had a profound effect on how our solar system and its planets formed. Super planet or brown dwarf? New theories are coming out about brown dwarfs. A brown dwarf, or planet, BDR J1750+3802, or Elegast,  has been discovered by a radio telescope. The BD was not visioned previously. Solar power stations in space could be the answer to our energy/power needs on Earth. A new radio telescope in space is envisioned. This could also be placed on the moon. Millions of signals are detected in space from intelligent civilizations: the problem is, the intelligent civilization is us. Very few anamolous signals from supposed aliens have been detected. The search for extra-terrestrial signals are for techno-signatures. Some of these signals have been received by the Aricebo telescope, but, unfortunately, in the next week, the Aricebo telescope di4ed a slow but certain death.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-43183-158863-November-26-14-00-00.mp3</guid><pubDate>Thu, 26 Nov 2020 21:02:14 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/42367129/astrotalk_43183_158863_november_26_14_00_00.mp3" length="53904196" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>By studying exo-planet formation, this adds to the knowledge base of how planets form, and how they can move. Jupiter moved in its orbit a lot in the early solar system, and this had a profound effect on how our solar system and its planets formed....</itunes:subtitle><itunes:summary><![CDATA[By studying exo-planet formation, this adds to the knowledge base of how planets form, and how they can move. Jupiter moved in its orbit a lot in the early solar system, and this had a profound effect on how our solar system and its planets formed. Super planet or brown dwarf? New theories are coming out about brown dwarfs. A brown dwarf, or planet, BDR J1750+3802, or Elegast,  has been discovered by a radio telescope. The BD was not visioned previously. Solar power stations in space could be the answer to our energy/power needs on Earth. A new radio telescope in space is envisioned. This could also be placed on the moon. Millions of signals are detected in space from intelligent civilizations: the problem is, the intelligent civilization is us. Very few anamolous signals from supposed aliens have been detected. The search for extra-terrestrial signals are for techno-signatures. Some of these signals have been received by the Aricebo telescope, but, unfortunately, in the next week, the Aricebo telescope di4ed a slow but certain death.]]></itunes:summary><itunes:duration>3370</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--42374866</link><description><![CDATA[aa]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-43189-158869-November-19-14-00-00.mp3</guid><pubDate>Thu, 19 Nov 2020 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/42374866/astrotalk_43189_158869_november_19_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>aa</itunes:subtitle><itunes:summary><![CDATA[aa]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>ESA Michael Frelick Sentinel Satellite Launch. Fast Radio Bursts From A Magnetar. 12 Strangest Galaxies in the Universe. Trojan Asteroid1014</title><link>https://www.spreaker.com/episode/esa-michael-frelick-sentinel-satellite-launch-fast-radio-bursts-from-a-magnetar-12-strangest-galaxies-in-the-universe-trojan-asteroid1014--42392770</link><description><![CDATA[The European Space Agency's Sentinel 5 Michael Frelick weather/climate satellite was launched Nov 23. It will track seal level rise, which is due to global warming.  Fast Radio bursts FRBs have been tracked from the Milky Way, for the first time. (30.00 light years away)  SGR 1935+2154 provides the first evidence for the origins of FRBs. Scientists have some ideas about other objects tat might create FRBs, but they are not 100% sure.  12 strangest galaxies in the uiniverse. Contact has been re-established with Voyager II. With repairs ot DSS 43 in Canberra Australia, part of the Deep Space Network, contact was not possible for about 3 months because of repairs to DSS 43. An asteroid,  101429,  is an trojan asteroid thought to have possibly come from the moon.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-43195-158875-November-12-14-00-00.mp3</guid><pubDate>Thu, 12 Nov 2020 21:01:09 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/42392770/astrotalk_43195_158875_november_12_14_00_00.mp3" length="48527987" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The European Space Agency's Sentinel 5 Michael Frelick weather/climate satellite was launched Nov 23. It will track seal level rise, which is due to global warming.  Fast Radio bursts FRBs have been tracked from the Milky Way, for the first time....</itunes:subtitle><itunes:summary><![CDATA[The European Space Agency's Sentinel 5 Michael Frelick weather/climate satellite was launched Nov 23. It will track seal level rise, which is due to global warming.  Fast Radio bursts FRBs have been tracked from the Milky Way, for the first time. (30.00 light years away)  SGR 1935+2154 provides the first evidence for the origins of FRBs. Scientists have some ideas about other objects tat might create FRBs, but they are not 100% sure.  12 strangest galaxies in the uiniverse. Contact has been re-established with Voyager II. With repairs ot DSS 43 in Canberra Australia, part of the Deep Space Network, contact was not possible for about 3 months because of repairs to DSS 43. An asteroid,  101429,  is an trojan asteroid thought to have possibly come from the moon.]]></itunes:summary><itunes:duration>3033</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--42409297</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-43201-158881-November-05-14-00-00.mp3</guid><pubDate>Thu, 05 Nov 2020 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/42409297/astrotalk_43201_158881_november_05_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--42643520</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-43250-158930-October-29-14-00-00.mp3</guid><pubDate>Thu, 29 Oct 2020 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/42643520/astrotalk_43250_158930_october_29_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Proton Gradient And Life. Entropy In The Universe. Why Are Galaxies Different Shapes? Elon Musk Testing And Launching Its Space-X Rockets. Z</title><link>https://www.spreaker.com/episode/proton-gradient-and-life-entropy-in-the-universe-why-are-galaxies-different-shapes-elon-musk-testing-and-launching-its-space-x-rockets-z--42643994</link><description><![CDATA[Entropy, order, disorder, and its meaning for life in the universe, and the eventual fate of the universe. When the universe first came into existence atoms, and light, did not exist. Galaxies come in different sizes, but also different shapes. The shape of a galaxy gives us a break down of the events in that galaxy's ultra-long life. There are 2 basic designations of a galaxy's shape, a disk, and an elliptical. Both the Milky Way and Andromeda are disks, formed from clouds of hydrogen gas. Ellipticals appear to be older and the movement of their stars appear to be more random. They are also thought to have formed from a galaxy merger. Galaxy mergers are thought to take millions or billions of years. The mergers that form irregular galaxies merging are thought to look like a big train wreck. There are also lenticular shaped galaxies. Elon Musk is testing his rockets to go to Mars. The window to go to Mars is every 26 months. Musk will launch on vehicle to Mars in 2024. Musk only plans to ferry humans and cargo to Mars. He does not want to build a settlement on Mars.  A sepo-second is the shortest unit of time ever measured. A particle of light, a photon, produces waves. By measuring how long it takes for the waves of a photon to cross a hydorgen atom, a sepo-second can be measure. A zepo-second is 1.o x 10-20 of a second. Eleven fascinating facts about the Milky Way, Dirty grease, or aliphatic carbon compounds are interspersed thought out the Milky Way. The study of Fermi Bubbles, gamma ray emissions, and x-ray emissions, can tell about previous mergers of galaxies into the Milky Way. The Mily Way is also being bombarder by FRBs, Fast Radio Bursts, from other parts of the universe.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-43251-158931-October-22-14-00-00.mp3</guid><pubDate>Thu, 22 Oct 2020 21:03:39 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/42643994/astrotalk_43251_158931_october_22_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Entropy, order, disorder, and its meaning for life in the universe, and the eventual fate of the universe. When the universe first came into existence atoms, and light, did not exist. Galaxies come in different sizes, but also different shapes. The...</itunes:subtitle><itunes:summary><![CDATA[Entropy, order, disorder, and its meaning for life in the universe, and the eventual fate of the universe. When the universe first came into existence atoms, and light, did not exist. Galaxies come in different sizes, but also different shapes. The shape of a galaxy gives us a break down of the events in that galaxy's ultra-long life. There are 2 basic designations of a galaxy's shape, a disk, and an elliptical. Both the Milky Way and Andromeda are disks, formed from clouds of hydrogen gas. Ellipticals appear to be older and the movement of their stars appear to be more random. They are also thought to have formed from a galaxy merger. Galaxy mergers are thought to take millions or billions of years. The mergers that form irregular galaxies merging are thought to look like a big train wreck. There are also lenticular shaped galaxies. Elon Musk is testing his rockets to go to Mars. The window to go to Mars is every 26 months. Musk will launch on vehicle to Mars in 2024. Musk only plans to ferry humans and cargo to Mars. He does not want to build a settlement on Mars.  A sepo-second is the shortest unit of time ever measured. A particle of light, a photon, produces waves. By measuring how long it takes for the waves of a photon to cross a hydorgen atom, a sepo-second can be measure. A zepo-second is 1.o x 10-20 of a second. Eleven fascinating facts about the Milky Way, Dirty grease, or aliphatic carbon compounds are interspersed thought out the Milky Way. The study of Fermi Bubbles, gamma ray emissions, and x-ray emissions, can tell about previous mergers of galaxies into the Milky Way. The Mily Way is also being bombarder by FRBs, Fast Radio Bursts, from other parts of the universe.]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Jupiter In The Early Solar System. Proton Gradients And Entropy. Nobel Prize In Physics For Black Hole Discoveries. Dark Matter And Dark Ene</title><link>https://www.spreaker.com/episode/jupiter-in-the-early-solar-system-proton-gradients-and-entropy-nobel-prize-in-physics-for-black-hole-discoveries-dark-matter-and-dark-ene--42644469</link><description><![CDATA[Apparently, Jupiter moved from its present orbit in the early solar system, and had a role in sculpting out and influencing how the inner planets developed. Proton gradients and their roles in the development, or sparking of life, on Earth. Entropy is always increasing in the universe. Life forms, like us, have low entropy, and are very ordered systems. Non living things have very high entropy, but all things in the universe are tending toward a state of higher entropy. Life takes energy and does useful things with it. three people were awarded for Black Hole work. Roger Penrose received half the prize for the discovery that black hole formation is a robust prediction of the general theory of relativity" and the other half jointly to Reinhard Genzel and Andrea Ghez "for the discovery of a black hole at the center of the Milky Way. Improving the exactness of the expansion rate of our universe will apparently help astros discover what dark matter is. Nuclear Fusion reactor could be here by 2025.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-43253-158933-October-08-14-00-00.mp3</guid><pubDate>Thu, 08 Oct 2020 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/42644469/astrotalk_43253_158933_october_08_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Apparently, Jupiter moved from its present orbit in the early solar system, and had a role in sculpting out and influencing how the inner planets developed. Proton gradients and their roles in the development, or sparking of life, on Earth. Entropy is...</itunes:subtitle><itunes:summary><![CDATA[Apparently, Jupiter moved from its present orbit in the early solar system, and had a role in sculpting out and influencing how the inner planets developed. Proton gradients and their roles in the development, or sparking of life, on Earth. Entropy is always increasing in the universe. Life forms, like us, have low entropy, and are very ordered systems. Non living things have very high entropy, but all things in the universe are tending toward a state of higher entropy. Life takes energy and does useful things with it. three people were awarded for Black Hole work. Roger Penrose received half the prize for the discovery that black hole formation is a robust prediction of the general theory of relativity" and the other half jointly to Reinhard Genzel and Andrea Ghez "for the discovery of a black hole at the center of the Milky Way. Improving the exactness of the expansion rate of our universe will apparently help astros discover what dark matter is. Nuclear Fusion reactor could be here by 2025.]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>A</title><link>https://www.spreaker.com/episode/a--42644471</link><description><![CDATA[A]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-43254-158934-October-01-14-00-00.mp3</guid><pubDate>Thu, 01 Oct 2020 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/42644471/astrotalk_43254_158934_october_01_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>A</itunes:subtitle><itunes:summary><![CDATA[A]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Artemis Gateway</title><link>https://www.spreaker.com/episode/artemis-gateway--23886019</link><description><![CDATA[NASA has begun to choose equipment for the Gateway Station. This station will be a fixture, orbiting the Moon. Astronauts can deploy to and from Gateway to the Moon. These first sets of instruments selected for Gateway will observe space weather and monitor the Sun’s radiation environment. Other instruments will be choosen within the next few years. The Canadian Space Agency, ESA, and JAXA will also take part. One of the most important funcntions of Gatelway is prepare and rehearse for flights to Mars.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-42117-157844-March-12-14-04-50.mp3</guid><pubDate>Thu, 12 Mar 2020 21:04:50 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23886019/astrotalk_42117_157844_march_12_14_04_50.mp3" length="52191817" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>NASA has begun to choose equipment for the Gateway Station. This station will be a fixture, orbiting the Moon. Astronauts can deploy to and from Gateway to the Moon. These first sets of instruments selected for Gateway will observe space weather and...</itunes:subtitle><itunes:summary><![CDATA[NASA has begun to choose equipment for the Gateway Station. This station will be a fixture, orbiting the Moon. Astronauts can deploy to and from Gateway to the Moon. These first sets of instruments selected for Gateway will observe space weather and monitor the Sun’s radiation environment. Other instruments will be choosen within the next few years. The Canadian Space Agency, ESA, and JAXA will also take part. One of the most important funcntions of Gatelway is prepare and rehearse for flights to Mars.]]></itunes:summary><itunes:duration>3262</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Explosion!!!!</title><link>https://www.spreaker.com/episode/explosion--23886017</link><description><![CDATA[Biggest explosion in universe, and,,,,,,,,, they saw a cavity being blown out, maybe not the explosion itself.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-42121-157848-March-12-14-00-00.mp3</guid><pubDate>Thu, 12 Mar 2020 21:04:48 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23886017/astrotalk_42121_157848_march_12_14_00_00.mp3" length="52208118" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Biggest explosion in universe, and,,,,,,,,, they saw a cavity being blown out, maybe not the explosion itself.</itunes:subtitle><itunes:summary><![CDATA[Biggest explosion in universe, and,,,,,,,,, they saw a cavity being blown out, maybe not the explosion itself.]]></itunes:summary><itunes:duration>3264</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>AstroTalk with Marco - Episode 3</title><link>https://www.spreaker.com/episode/astrotalk-with-marco-episode-3--23525017</link><description><![CDATA[Black Holes. What are they and how are they formed? We will distinguish between black holes that are produced by core-collapse supernova, and black holes that exist at centers of galaxies. Our sun will not  turn into a supernova at the end of its life-cycle, but will instead become a carbon white dwarf. The life stages and fates of stars of different sizes will be discussed, as well as the processes involved when and after big stars go supernova. Guess what? Well also talk about aspects of relatively associated with black holes, and things like event horizons and space-time.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2014/AstroTalk-May-15-15-02-50.mp3</guid><pubDate>Thu, 05 Mar 2020 23:15:59 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525017/astrotalk_may_15_15_02_50.mp3" length="52717189" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Black Holes. What are they and how are they formed? We will distinguish between black holes that are produced by core-collapse supernova, and black holes that exist at centers of galaxies. Our sun will not  turn into a supernova at the end of its...</itunes:subtitle><itunes:summary><![CDATA[Black Holes. What are they and how are they formed? We will distinguish between black holes that are produced by core-collapse supernova, and black holes that exist at centers of galaxies. Our sun will not  turn into a supernova at the end of its life-cycle, but will instead become a carbon white dwarf. The life stages and fates of stars of different sizes will be discussed, as well as the processes involved when and after big stars go supernova. Guess what? Well also talk about aspects of relatively associated with black holes, and things like event horizons and space-time.]]></itunes:summary><itunes:duration>3295</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Astronaut Training: Supermassive Blackhole. Development of Intelligent Life in the Universe</title><link>https://www.spreaker.com/episode/astronaut-training-supermassive-blackhole-development-of-intelligent-life-in-the-universe--23886016</link><description><![CDATA[Watching Astronauts train: Fun!!! Bigest exkplosion in history from Ophiuchus galaxy cluster about 390 million light-years from Earth. Galaxy clusters are the largest structures in the universe held together by gravity, containing thousands of individual galaxies, dark matter, and hot gas. The explosion blew out a hole in the wall of the cluster. This explosion was 5 x bigger than the previous record holder. The biggest explosion of course, was the Big Bang.  The previous record holder, MS 0735+74, and hundreds and thousands of times greater than typical clusters.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-42118-157845-March-05-14-00-00.mp3</guid><pubDate>Thu, 05 Mar 2020 21:06:30 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23886016/astrotalk_42118_157845_march_05_14_00_00.mp3" length="46896274" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Watching Astronauts train: Fun!!! Bigest exkplosion in history from Ophiuchus galaxy cluster about 390 million light-years from Earth. Galaxy clusters are the largest structures in the universe held together by gravity, containing thousands of...</itunes:subtitle><itunes:summary><![CDATA[Watching Astronauts train: Fun!!! Bigest exkplosion in history from Ophiuchus galaxy cluster about 390 million light-years from Earth. Galaxy clusters are the largest structures in the universe held together by gravity, containing thousands of individual galaxies, dark matter, and hot gas. The explosion blew out a hole in the wall of the cluster. This explosion was 5 x bigger than the previous record holder. The biggest explosion of course, was the Big Bang.  The previous record holder, MS 0735+74, and hundreds and thousands of times greater than typical clusters.]]></itunes:summary><itunes:duration>2932</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--23886015</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-42119-157846-February-27-14-00-00.mp3</guid><pubDate>Thu, 27 Feb 2020 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23886015/astrotalk_42119_157846_february_27_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Jupiter</title><link>https://www.spreaker.com/episode/jupiter--23886018</link><description><![CDATA[Jupiter Migrated In and Out in the early solar system, and carved out the solar system. Discussion about the early universe. When U turned 380,000 years old, U started to change. Discussion about LiveScience website. More exciting stories than NASA.gov.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-42120-157847-February-20-14-00-00.mp3</guid><pubDate>Thu, 20 Feb 2020 21:03:15 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23886018/astrotalk_42120_157847_february_20_14_00_00.mp3" length="53551856" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Jupiter Migrated In and Out in the early solar system, and carved out the solar system. Discussion about the early universe. When U turned 380,000 years old, U started to change. Discussion about LiveScience website. More exciting stories than NASA.gov.</itunes:subtitle><itunes:summary><![CDATA[Jupiter Migrated In and Out in the early solar system, and carved out the solar system. Discussion about the early universe. When U turned 380,000 years old, U started to change. Discussion about LiveScience website. More exciting stories than NASA.gov.]]></itunes:summary><itunes:duration>3347</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--23886014</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-42122-157849-February-13-14-00-00.mp3</guid><pubDate>Thu, 13 Feb 2020 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23886014/astrotalk_42122_157849_february_13_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--23886020</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2020/AstroTalk-42123-157850-February-06-14-00-00.mp3</guid><pubDate>Thu, 06 Feb 2020 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23886020/astrotalk_42123_157850_february_06_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>All About Space Time</title><link>https://www.spreaker.com/episode/all-about-space-time--23524903</link><description><![CDATA[An examination of space time from an article in Livescience.com. What Is Space-Time? By Adam Mann - Live Science Contributor . this article deals with the theories behind space time, and more specifically, the fabric of space time. Einstein combined space and time into 4 dimensions. This article deals with how space-time works, and what scientists still don't know.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-41514-157241-December-19-14-00-00.mp3</guid><pubDate>Thu, 19 Dec 2019 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524903/astrotalk_41514_157241_december_19_14_00_00.mp3" length="51392261" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>An examination of space time from an article in Livescience.com. What Is Space-Time? By Adam Mann - Live Science Contributor . this article deals with the theories behind space time, and more specifically, the fabric of space time. Einstein combined...</itunes:subtitle><itunes:summary><![CDATA[An examination of space time from an article in Livescience.com. What Is Space-Time? By Adam Mann - Live Science Contributor . this article deals with the theories behind space time, and more specifically, the fabric of space time. Einstein combined space and time into 4 dimensions. This article deals with how space-time works, and what scientists still don't know.]]></itunes:summary><itunes:duration>3213</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Space Time, White Holes and Worm Holes</title><link>https://www.spreaker.com/episode/space-time-white-holes-and-worm-holes--23887321</link><description><![CDATA[Space Time, White Holes and Worm Holes.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-42124-157851-December-19-14-00-00.mp3</guid><pubDate>Thu, 19 Dec 2019 20:59:47 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23887321/astrotalk_42124_157851_december_19_14_00_00.mp3" length="51791831" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Space Time, White Holes and Worm Holes.</itunes:subtitle><itunes:summary><![CDATA[Space Time, White Holes and Worm Holes.]]></itunes:summary><itunes:duration>3237</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Space Junk. Gravitational Waves. New Particle X17????</title><link>https://www.spreaker.com/episode/space-junk-gravitational-waves-new-particle-x17--23887320</link><description><![CDATA[A new satellite (spacecraft?) will be deployed to clear the space junk from outer space. About time. The universe remembers gravitational waves. Evidence of an intermediate sized particle called X17. Does X17 contain a fiftth force that could help explain dark matter?]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-42125-157852-December-12-14-00-00.mp3</guid><pubDate>Thu, 12 Dec 2019 21:13:14 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23887320/astrotalk_42125_157852_december_12_14_00_00.mp3" length="46240078" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>A new satellite (spacecraft?) will be deployed to clear the space junk from outer space. About time. The universe remembers gravitational waves. Evidence of an intermediate sized particle called X17. Does X17 contain a fiftth force that could help...</itunes:subtitle><itunes:summary><![CDATA[A new satellite (spacecraft?) will be deployed to clear the space junk from outer space. About time. The universe remembers gravitational waves. Evidence of an intermediate sized particle called X17. Does X17 contain a fiftth force that could help explain dark matter?]]></itunes:summary><itunes:duration>2890</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>UFO Reports Now Available in Canada. The Echos and Memories of Gravitational Waves. Particle X 17. Robot Hugs and Space Garbage.</title><link>https://www.spreaker.com/episode/ufo-reports-now-available-in-canada-the-echos-and-memories-of-gravitational-waves-particle-x-17-robot-hugs-and-space-garbage--23524859</link><description><![CDATA[UFO Reports Now Available in Canada.  The Universe remembers gravitational waves. G waves warp space time and leave their imprint. When G waves wash over you, they leave their imprint. This echo can be measured, or so scientists think. But gravity is a weak force so its hard to measure so multiple events of g waves must be combined in order to measure them. 2,000 combined waves are needed.  A few scientists believe a new particle, X 17, will reveal a 5th force of nature.  Scientists hope this particle can help define what dark matter is. Space is littered with space garbage. ESA is proposing a robot that will hug garbage in space, and then clear the garbage out. The 4 armed robot will drag itself and the garbage to be burned up in the Earth's atmosphere.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-41515-157242-December-12-14-00-00.mp3</guid><pubDate>Thu, 12 Dec 2019 21:13:14 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524859/astrotalk_41515_157242_december_12_14_00_00.mp3" length="44911804" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>UFO Reports Now Available in Canada.  The Universe remembers gravitational waves. G waves warp space time and leave their imprint. When G waves wash over you, they leave their imprint. This echo can be measured, or so scientists think. But gravity is...</itunes:subtitle><itunes:summary><![CDATA[UFO Reports Now Available in Canada.  The Universe remembers gravitational waves. G waves warp space time and leave their imprint. When G waves wash over you, they leave their imprint. This echo can be measured, or so scientists think. But gravity is a weak force so its hard to measure so multiple events of g waves must be combined in order to measure them. 2,000 combined waves are needed.  A few scientists believe a new particle, X 17, will reveal a 5th force of nature.  Scientists hope this particle can help define what dark matter is. Space is littered with space garbage. ESA is proposing a robot that will hug garbage in space, and then clear the garbage out. The 4 armed robot will drag itself and the garbage to be burned up in the Earth's atmosphere.]]></itunes:summary><itunes:duration>2807</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Parker Solar Probe. Is the Universe Curved? Amazing Moon Photos.</title><link>https://www.spreaker.com/episode/parker-solar-probe-is-the-universe-curved-amazing-moon-photos--23524789</link><description><![CDATA[Parker has many new finds about the mysteries of the corona. Parker is doing many flybys between Venus and the Sun, and has already challenged some of the current theories of the Sun. The probe will run until 2025. The first details about the Sun are HOOOOOOT. The probe is 23 million miles from the Sun to measure the solar wind and the corona. Our previous views of the sun were simple. Parker has found cosmic dust stops at a distance of 3.5 million miles from the sun. Parker also saw magnetic waves from the sun flip in a whip like motion 180 degrees in a matter of seconds. These switchbacks came in clusters. The solar wind now is known to have rough irregular texture. The plasma lacks an orderly sense of direction. Some flies out but some falls back. Parker also found a transition point in the solar wind. The corona rotates with the visible surface  before it transitions and Parker  spotted signs of the transition, and it now is known that it happens farther out than expected. Parker also observed several outbursts of solar energetic particles. They have never seen to be this small before. Amazing photos of the terrain of the moon.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-41516-157243-December-05-14-00-00.mp3</guid><pubDate>Thu, 05 Dec 2019 21:01:35 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524789/astrotalk_41516_157243_december_05_14_00_00.mp3" length="56095974" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Parker has many new finds about the mysteries of the corona. Parker is doing many flybys between Venus and the Sun, and has already challenged some of the current theories of the Sun. The probe will run until 2025. The first details about the Sun are...</itunes:subtitle><itunes:summary><![CDATA[Parker has many new finds about the mysteries of the corona. Parker is doing many flybys between Venus and the Sun, and has already challenged some of the current theories of the Sun. The probe will run until 2025. The first details about the Sun are HOOOOOOT. The probe is 23 million miles from the Sun to measure the solar wind and the corona. Our previous views of the sun were simple. Parker has found cosmic dust stops at a distance of 3.5 million miles from the sun. Parker also saw magnetic waves from the sun flip in a whip like motion 180 degrees in a matter of seconds. These switchbacks came in clusters. The solar wind now is known to have rough irregular texture. The plasma lacks an orderly sense of direction. Some flies out but some falls back. Parker also found a transition point in the solar wind. The corona rotates with the visible surface  before it transitions and Parker  spotted signs of the transition, and it now is known that it happens farther out than expected. Parker also observed several outbursts of solar energetic particles. They have never seen to be this small before. Amazing photos of the terrain of the moon.]]></itunes:summary><itunes:duration>3506</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Parker Solar Probe. New Moon Photos.</title><link>https://www.spreaker.com/episode/parker-solar-probe-new-moon-photos--23887323</link><description><![CDATA[The Parker Solar Probe has given a bonanza of new info about our star. Launched August 2018. It is targetting the solar wind and the solar corona. New lovely moon photos from LRO.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-42126-157853-December-05-14-00-00.mp3</guid><pubDate>Thu, 05 Dec 2019 21:01:34 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23887323/astrotalk_42126_157853_december_05_14_00_00.mp3" length="57664157" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The Parker Solar Probe has given a bonanza of new info about our star. Launched August 2018. It is targetting the solar wind and the solar corona. New lovely moon photos from LRO.</itunes:subtitle><itunes:summary><![CDATA[The Parker Solar Probe has given a bonanza of new info about our star. Launched August 2018. It is targetting the solar wind and the solar corona. New lovely moon photos from LRO.]]></itunes:summary><itunes:duration>3605</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Ice Fossil Gives Clues About Early Solar System. Voyager II Went Through A Violent Conflict Between the Solar Wind and Cosmic Rays. 18 Unsol</title><link>https://www.spreaker.com/episode/ice-fossil-gives-clues-about-early-solar-system-voyager-ii-went-through-a-violent-conflict-between-the-solar-wind-and-cosmic-rays-18-unsol--23524828</link><description><![CDATA[ACFER 094 crashed in the Sahara desert in the 1990s. Voyager !! went through a violent battle between the solar wind and cosmic rays from interstellar space. Voyager ! couldn't measure through this area because of a senfor malfunction. V II went through the heliopause, the edge of our solar system. The helippause protects us from interstellar space. Temperatures in the heliopause reached temperatures of  31,000 degrees Celcius, double what scientists previously predicted. This suggests a far more violent clash between the solar wind and interstellar space. The heliopauses' thick walls protect us from interstellar space. There were also 2 holes in our side of the heliopause. The 18 biggest unsolved mysteries in Physics. Bubbles of cooler universe cooled in the beginning after the Big Bang. <br /><br />V883 Orionis]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-41517-157244-November-28-14-00-00.mp3</guid><pubDate>Thu, 28 Nov 2019 21:02:05 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524828/astrotalk_41517_157244_november_28_14_00_00.mp3" length="55615739" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>ACFER 094 crashed in the Sahara desert in the 1990s. Voyager !! went through a violent battle between the solar wind and cosmic rays from interstellar space. Voyager ! couldn't measure through this area because of a senfor malfunction. V II went...</itunes:subtitle><itunes:summary><![CDATA[ACFER 094 crashed in the Sahara desert in the 1990s. Voyager !! went through a violent battle between the solar wind and cosmic rays from interstellar space. Voyager ! couldn't measure through this area because of a senfor malfunction. V II went through the heliopause, the edge of our solar system. The helippause protects us from interstellar space. Temperatures in the heliopause reached temperatures of  31,000 degrees Celcius, double what scientists previously predicted. This suggests a far more violent clash between the solar wind and interstellar space. The heliopauses' thick walls protect us from interstellar space. There were also 2 holes in our side of the heliopause. The 18 biggest unsolved mysteries in Physics. Bubbles of cooler universe cooled in the beginning after the Big Bang. <br /><br />V883 Orionis]]></itunes:summary><itunes:duration>3476</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Solar Wind Discussion. Voyager II Goes Through the Helio-pause. 3 Black Holes Cooking Their Galaxies Alive.</title><link>https://www.spreaker.com/episode/solar-wind-discussion-voyager-ii-goes-through-the-helio-pause-3-black-holes-cooking-their-galaxies-alive--23887322</link><description><![CDATA[The solar wind sends out a solar bubble all the way to the -, our cosmic border which protects us from the dangerous things in interstellar space. Quasi particles messing up my mind. Blah, blah, blah. 3 Black Holes cooking their galaxies alive. Cool (or hot?) How does this gas stay so hot??????]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-42127-157854-November-28-14-00-00.mp3</guid><pubDate>Thu, 28 Nov 2019 21:02:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23887322/astrotalk_42127_157854_november_28_14_00_00.mp3" length="55152222" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The solar wind sends out a solar bubble all the way to the -, our cosmic border which protects us from the dangerous things in interstellar space. Quasi particles messing up my mind. Blah, blah, blah. 3 Black Holes cooking their galaxies alive. Cool...</itunes:subtitle><itunes:summary><![CDATA[The solar wind sends out a solar bubble all the way to the -, our cosmic border which protects us from the dangerous things in interstellar space. Quasi particles messing up my mind. Blah, blah, blah. 3 Black Holes cooking their galaxies alive. Cool (or hot?) How does this gas stay so hot??????]]></itunes:summary><itunes:duration>3448</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--23887324</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-42128-157855-November-21-14-00-00.mp3</guid><pubDate>Thu, 21 Nov 2019 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23887324/astrotalk_42128_157855_november_21_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Stellar Mysteries. A Singles Club - The Top 10 Star Mysteries. A Grim Reaper Star. Where Do Black Holes Lead?</title><link>https://www.spreaker.com/episode/stellar-mysteries-a-singles-club-the-top-10-star-mysteries-a-grim-reaper-star-where-do-black-holes-lead--23524790</link><description><![CDATA[Different freaky stars are examined. BPM a white dwarf weighed 5 million trillion pounds and was the equivalent of  10 billion trillion trillion karats. 85% of the stars in the Milky Way system are 2 or higher order star systems. Where do Black Holes lead? The Oldest Known Black Hole.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-41518-157245-November-21-14-00-00.mp3</guid><pubDate>Thu, 14 Nov 2019 21:09:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524790/astrotalk_41518_157245_november_21_14_00_00.mp3" length="46688131" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Different freaky stars are examined. BPM a white dwarf weighed 5 million trillion pounds and was the equivalent of  10 billion trillion trillion karats. 85% of the stars in the Milky Way system are 2 or higher order star systems. Where do Black Holes...</itunes:subtitle><itunes:summary><![CDATA[Different freaky stars are examined. BPM a white dwarf weighed 5 million trillion pounds and was the equivalent of  10 billion trillion trillion karats. 85% of the stars in the Milky Way system are 2 or higher order star systems. Where do Black Holes lead? The Oldest Known Black Hole.]]></itunes:summary><itunes:duration>2919</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Mercury Transits in Front of the Sun. Turning the Universe Transparent. Top 10 Star Mysteries of All Time. Black Holes. Star Quakes. Light a</title><link>https://www.spreaker.com/episode/mercury-transits-in-front-of-the-sun-turning-the-universe-transparent-top-10-star-mysteries-of-all-time-black-holes-star-quakes-light-a--23524764</link><description><![CDATA[Mercury recently transitted the Sun. Hubble photoed how light escaped from the earliest galaxes, turning the universe transparent. Top 10 star mysteries of all time. Star Quakes give strong magnetic wavesl. Super Stars. Rotating Radio Transers give off powerful magnetic fields. How light escaped from the earlies galaxies, and how this made the universe transparent.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-41519-157246-November-14-14-00-00.mp3</guid><pubDate>Thu, 14 Nov 2019 21:08:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524764/astrotalk_41519_157246_november_14_14_00_00.mp3" length="47648183" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Mercury recently transitted the Sun. Hubble photoed how light escaped from the earliest galaxes, turning the universe transparent. Top 10 star mysteries of all time. Star Quakes give strong magnetic wavesl. Super Stars. Rotating Radio Transers give...</itunes:subtitle><itunes:summary><![CDATA[Mercury recently transitted the Sun. Hubble photoed how light escaped from the earliest galaxes, turning the universe transparent. Top 10 star mysteries of all time. Star Quakes give strong magnetic wavesl. Super Stars. Rotating Radio Transers give off powerful magnetic fields. How light escaped from the earlies galaxies, and how this made the universe transparent.]]></itunes:summary><itunes:duration>2979</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>50th NASA Anniversaries. NASA Satellites Saving the World. Earthlings Ruining the Earth. Voyager II.</title><link>https://www.spreaker.com/episode/50th-nasa-anniversaries-nasa-satellites-saving-the-world-earthlings-ruining-the-earth-voyager-ii--23524826</link><description><![CDATA[50 Anniv launch of NASA rockets. Rainforests are burning and NASA is helping monitor this. Voayger II deliniates the boundaries of interstellar space. It is unknown how far out Voyayger II is from the heliopause. The plasma outside of the heliopause is considerably denser than astronauts believed.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-41520-157247-November-07-14-00-00.mp3</guid><pubDate>Thu, 07 Nov 2019 21:13:39 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524826/astrotalk_41520_157247_november_07_14_00_00.mp3" length="102015896" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>50 Anniv launch of NASA rockets. Rainforests are burning and NASA is helping monitor this. Voayger II deliniates the boundaries of interstellar space. It is unknown how far out Voyayger II is from the heliopause. The plasma outside of the heliopause...</itunes:subtitle><itunes:summary><![CDATA[50 Anniv launch of NASA rockets. Rainforests are burning and NASA is helping monitor this. Voayger II deliniates the boundaries of interstellar space. It is unknown how far out Voyayger II is from the heliopause. The plasma outside of the heliopause is considerably denser than astronauts believed.]]></itunes:summary><itunes:duration>6376</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Gas Escapes Galaxies, Creates Stars. Glowing Galactic Goo. CGM --&gt; Circum Galactic Medium. TOP 15 Weirdest Galaxies in Our Universe. Mars an</title><link>https://www.spreaker.com/episode/gas-escapes-galaxies-creates-stars-glowing-galactic-goo-cgm-circum-galactic-medium-top-15-weirdest-galaxies-in-our-universe-mars-an--23524773</link><description><![CDATA[Interstellar Medium Intergalactic Medium. Winds are transporting gases between these mediums. Oxygen Ions are emitting gas in galaxies. GCM --> seeing for the first time how the CGM is being mixed. This is called cosmic goo, the stuff in between galaxies. Top 15 Weirdest Galaxies in our Universe. How NASA might bring home pieces of Mars in a Darth Vader. Colliding Galaxies form piercing eyes of ghost face.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-41521-157248-October-31-14-00-00.mp3</guid><pubDate>Thu, 31 Oct 2019 21:02:40 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524773/astrotalk_41521_157248_october_31_14_00_00.mp3" length="51104288" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Interstellar Medium Intergalactic Medium. Winds are transporting gases between these mediums. Oxygen Ions are emitting gas in galaxies. GCM --&gt; seeing for the first time how the CGM is being mixed. This is called cosmic goo, the stuff in between...</itunes:subtitle><itunes:summary><![CDATA[Interstellar Medium Intergalactic Medium. Winds are transporting gases between these mediums. Oxygen Ions are emitting gas in galaxies. GCM --> seeing for the first time how the CGM is being mixed. This is called cosmic goo, the stuff in between galaxies. Top 15 Weirdest Galaxies in our Universe. How NASA might bring home pieces of Mars in a Darth Vader. Colliding Galaxies form piercing eyes of ghost face.]]></itunes:summary><itunes:duration>3195</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>NASA and Google Partner Up. Quantum Computers. Taking a Picture of a Black Hole. Trojan Asteroids.</title><link>https://www.spreaker.com/episode/nasa-and-google-partner-up-quantum-computers-taking-a-picture-of-a-black-hole-trojan-asteroids--23524770</link><description><![CDATA[NASA and Google partner up. Quantum computers are demystifying the future of computing. A quantum is a the minimum of any physical thing that is needed to interact with something else. In QM, particles radiate in quantums. Computer scientists try to harness the properties of quantum mechanics in computing. Hopefully, computer can be done much faster. The event horizon telescope, which is the link up of 8 telescopes around the world, is trying to take a picture of a black hole. Trojan Asteroids.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-41522-157249-October-24-14-00-00.mp3</guid><pubDate>Thu, 24 Oct 2019 21:15:37 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524770/astrotalk_41522_157249_october_24_14_00_00.mp3" length="37248105" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>NASA and Google partner up. Quantum computers are demystifying the future of computing. A quantum is a the minimum of any physical thing that is needed to interact with something else. In QM, particles radiate in quantums. Computer scientists try to...</itunes:subtitle><itunes:summary><![CDATA[NASA and Google partner up. Quantum computers are demystifying the future of computing. A quantum is a the minimum of any physical thing that is needed to interact with something else. In QM, particles radiate in quantums. Computer scientists try to harness the properties of quantum mechanics in computing. Hopefully, computer can be done much faster. The event horizon telescope, which is the link up of 8 telescopes around the world, is trying to take a picture of a black hole. Trojan Asteroids.]]></itunes:summary><itunes:duration>2329</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Computers and Viewing Black Holes. Why the Milky Way Is Getting So Gassy. Earth Like Planet. How the Universe Expands and How It Evolves.</title><link>https://www.spreaker.com/episode/computers-and-viewing-black-holes-why-the-milky-way-is-getting-so-gassy-earth-like-planet-how-the-universe-expands-and-how-it-evolves--23524814</link><description><![CDATA[Computers and Viewing Black Holes and the Intracacies. Why is the MW getting so gassy? Star clusters are born together.  The first planet orbiting a sun like star outside our solar system. Scientists believe we will not be able to get to other stars, and especially we will not be able to habitate them. Going to Mars or another planet? Is it possible. Steven Kane says we might be able to send people to Mars in the next 50 years. To Jupiter? Noooooooo. To other stars? Noooooooooooooooooooooooooo. How the universe stopped making sense.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-41523-157250-October-17-14-00-00.mp3</guid><pubDate>Thu, 17 Oct 2019 21:03:09 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524814/astrotalk_41523_157250_october_17_14_00_00.mp3" length="46416040" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Computers and Viewing Black Holes and the Intracacies. Why is the MW getting so gassy? Star clusters are born together.  The first planet orbiting a sun like star outside our solar system. Scientists believe we will not be able to get to other stars,...</itunes:subtitle><itunes:summary><![CDATA[Computers and Viewing Black Holes and the Intracacies. Why is the MW getting so gassy? Star clusters are born together.  The first planet orbiting a sun like star outside our solar system. Scientists believe we will not be able to get to other stars, and especially we will not be able to habitate them. Going to Mars or another planet? Is it possible. Steven Kane says we might be able to send people to Mars in the next 50 years. To Jupiter? Noooooooo. To other stars? Noooooooooooooooooooooooooo. How the universe stopped making sense.]]></itunes:summary><itunes:duration>2901</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Telescopes, Space Probes and Satellites, NASA's great Successes. The Science Community and the Nobel.    Empty Void Galaxy. Mega Merger of G</title><link>https://www.spreaker.com/episode/telescopes-space-probes-and-satellites-nasa-s-great-successes-the-science-community-and-the-nobel-empty-void-galaxy-mega-merger-of-g--23524835</link><description><![CDATA[The Nobel was split between cosmology research to a Canadian and exoplanet research. The science community was upset about how the Nobel was awarded. Exoplanet research. Marcy and Butler research was finally awarded. A jet or trail of gas is arriving in our direction from the Magellanic Clouds. A large empty void is forming in space, far, far away, in Eridanus. Largest exoplanet, GQ LUPI B, has a radius 3.5 times that of Jupiter. UI SCUTI with a radius of 1,700 times that of the Sun. Largest Nebula Tarantula 1,800 LYs. or galaxy, IC 1101   weighing  200,000 more than the Milky Way.  TON 618 Supermassive black hole, 66,000,000,000 Suns. Largest Fermi Bubble is 25,000 LYs tall. A large structure, a galactic cluster, is SPT 2349-56 weighing 10 trillion times the mass of the sun.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-41524-157251-October-10-14-00-00.mp3</guid><pubDate>Thu, 10 Oct 2019 21:07:06 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524835/astrotalk_41524_157251_october_10_14_00_00.mp3" length="42928170" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The Nobel was split between cosmology research to a Canadian and exoplanet research. The science community was upset about how the Nobel was awarded. Exoplanet research. Marcy and Butler research was finally awarded. A jet or trail of gas is arriving...</itunes:subtitle><itunes:summary><![CDATA[The Nobel was split between cosmology research to a Canadian and exoplanet research. The science community was upset about how the Nobel was awarded. Exoplanet research. Marcy and Butler research was finally awarded. A jet or trail of gas is arriving in our direction from the Magellanic Clouds. A large empty void is forming in space, far, far away, in Eridanus. Largest exoplanet, GQ LUPI B, has a radius 3.5 times that of Jupiter. UI SCUTI with a radius of 1,700 times that of the Sun. Largest Nebula Tarantula 1,800 LYs. or galaxy, IC 1101   weighing  200,000 more than the Milky Way.  TON 618 Supermassive black hole, 66,000,000,000 Suns. Largest Fermi Bubble is 25,000 LYs tall. A large structure, a galactic cluster, is SPT 2349-56 weighing 10 trillion times the mass of the sun.]]></itunes:summary><itunes:duration>2684</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Fast Moving Stars. The Deep Space Network. Andromeda the Cannibal. Where is Planet 9? Primordial Black Holes.</title><link>https://www.spreaker.com/episode/fast-moving-stars-the-deep-space-network-andromeda-the-cannibal-where-is-planet-9-primordial-black-holes--23524899</link><description><![CDATA[The Deep Space Network. Fast Moving Stars. Why? How to photograph a black hole? Creating complicated computer algorthrims is necessary. The Cannibal next store. Andrormeda is going to cannibalize the Milky Way one day. Planet 9 and TNOs, trans Neptunian objects, orbit in a different plane than the other planets. This suggests that something else, Planet 9, is tugging on them.  Where can we find primordial, or grapefruit-sized, black holes.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-41525-157252-October-03-14-00-00.mp3</guid><pubDate>Thu, 03 Oct 2019 21:08:02 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524899/astrotalk_41525_157252_october_03_14_00_00.mp3" length="34416013" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The Deep Space Network. Fast Moving Stars. Why? How to photograph a black hole? Creating complicated computer algorthrims is necessary. The Cannibal next store. Andrormeda is going to cannibalize the Milky Way one day. Planet 9 and TNOs, trans...</itunes:subtitle><itunes:summary><![CDATA[The Deep Space Network. Fast Moving Stars. Why? How to photograph a black hole? Creating complicated computer algorthrims is necessary. The Cannibal next store. Andrormeda is going to cannibalize the Milky Way one day. Planet 9 and TNOs, trans Neptunian objects, orbit in a different plane than the other planets. This suggests that something else, Planet 9, is tugging on them.  Where can we find primordial, or grapefruit-sized, black holes.]]></itunes:summary><itunes:duration>2151</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>q</title><link>https://www.spreaker.com/episode/q--23524779</link><description><![CDATA[q]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-41526-157253-September-26-14-00-00.mp3</guid><pubDate>Thu, 26 Sep 2019 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524779/astrotalk_41526_157253_september_26_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>q</itunes:subtitle><itunes:summary><![CDATA[q]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>q</title><link>https://www.spreaker.com/episode/q--23524845</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-41527-157254-September-19-14-00-00.mp3</guid><pubDate>Thu, 19 Sep 2019 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524845/astrotalk_41527_157254_september_19_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>OSIRIS-REx Sample Sites at Bennu. 30th  Year Anniversay of Voyager 2's Visit to Neptune.</title><link>https://www.spreaker.com/episode/osiris-rex-sample-sites-at-bennu-30th-year-anniversay-of-voyager-2-s-visit-to-neptune--23524822</link><description><![CDATA[OSIRIS-REx has narrowed down its list to 4 potential sample sites at the asteroid Bennu.  Scenarios NASA has to plan for on a mission like OSIRIS-REx.  30 year anniversary of Voyager 2's visit to the planet Neptune.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40643-156370-August-22-14-00-00.mp3</guid><pubDate>Thu, 22 Aug 2019 21:01:39 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524822/astrotalk_40643_156370_august_22_14_00_00.mp3" length="56335883" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>OSIRIS-REx has narrowed down its list to 4 potential sample sites at the asteroid Bennu.  Scenarios NASA has to plan for on a mission like OSIRIS-REx.  30 year anniversary of Voyager 2's visit to the planet Neptune.</itunes:subtitle><itunes:summary><![CDATA[OSIRIS-REx has narrowed down its list to 4 potential sample sites at the asteroid Bennu.  Scenarios NASA has to plan for on a mission like OSIRIS-REx.  30 year anniversary of Voyager 2's visit to the planet Neptune.]]></itunes:summary><itunes:duration>3521</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>50th Aniiversay Neil Armstrong Celebrates Birthday In Quarantine. Jupiter and its Effects on the Formation of the Inner Solar System. Conami</title><link>https://www.spreaker.com/episode/50th-aniiversay-neil-armstrong-celebrates-birthday-in-quarantine-jupiter-and-its-effects-on-the-formation-of-the-inner-solar-system-conami--23524788</link><description><![CDATA[No one know if astronauts would return from the Moon with contaminants, so Neil Armstrong was quarantined for 3 weeks after returning from the Moon.  Titanium was found in higher proportion in moon rocks than on Earth. LRRRs or solar arrays left on the Moon by the Apollo astronauts.  Jupiter marauds through the inner solar system, causing havoc, in its formative younger years.  Saturn  moves in, then pulls Jupiter out of its marauding in the inner solar system.  Jupiter can also fling asteroids or comets on a path toward Earth, or, it can be a vacuum cleaner and suck up dangerous asteroids or comets that could eventually, or potentially, hit Earth. Contaminants on space mission. How NASA will protect astronauts from space radiation at the moon.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40642-156369-August-15-14-00-01.mp3</guid><pubDate>Thu, 15 Aug 2019 21:01:01 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524788/astrotalk_40642_156369_august_15_14_00_01.mp3" length="53711935" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>No one know if astronauts would return from the Moon with contaminants, so Neil Armstrong was quarantined for 3 weeks after returning from the Moon.  Titanium was found in higher proportion in moon rocks than on Earth. LRRRs or solar arrays left on...</itunes:subtitle><itunes:summary><![CDATA[No one know if astronauts would return from the Moon with contaminants, so Neil Armstrong was quarantined for 3 weeks after returning from the Moon.  Titanium was found in higher proportion in moon rocks than on Earth. LRRRs or solar arrays left on the Moon by the Apollo astronauts.  Jupiter marauds through the inner solar system, causing havoc, in its formative younger years.  Saturn  moves in, then pulls Jupiter out of its marauding in the inner solar system.  Jupiter can also fling asteroids or comets on a path toward Earth, or, it can be a vacuum cleaner and suck up dangerous asteroids or comets that could eventually, or potentially, hit Earth. Contaminants on space mission. How NASA will protect astronauts from space radiation at the moon.]]></itunes:summary><itunes:duration>3357</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Northern Lights in South Western B.C. Sky. Protecting Astronauts From Space Radiation. Hubble's New Portrait of Jupiter. Extended Use of Sma</title><link>https://www.spreaker.com/episode/northern-lights-in-south-western-b-c-sky-protecting-astronauts-from-space-radiation-hubble-s-new-portrait-of-jupiter-extended-use-of-sma--23524823</link><description><![CDATA[Northern Lights appear in southwestern B.C. sky. Protecting Astronauts From Space Radiation.  hubble's new portarait of Jupiter.  Extended Use of Small Spacecraft in and Beyond Earth Orbit.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40641-156368-August-08-14-00-00.mp3</guid><pubDate>Thu, 08 Aug 2019 21:04:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524823/astrotalk_40641_156368_august_08_14_00_00.mp3" length="51439909" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Northern Lights appear in southwestern B.C. sky. Protecting Astronauts From Space Radiation.  hubble's new portarait of Jupiter.  Extended Use of Small Spacecraft in and Beyond Earth Orbit.</itunes:subtitle><itunes:summary><![CDATA[Northern Lights appear in southwestern B.C. sky. Protecting Astronauts From Space Radiation.  hubble's new portarait of Jupiter.  Extended Use of Small Spacecraft in and Beyond Earth Orbit.]]></itunes:summary><itunes:duration>3215</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Voyager 1 and Voyager 2 Mission Recap.</title><link>https://www.spreaker.com/episode/voyager-1-and-voyager-2-mission-recap--23524851</link><description><![CDATA[Recap of the Voyager mission from a PBS broadcoast from Wednesday August 1.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40487-156214-August-01-14-00-00.mp3</guid><pubDate>Thu, 01 Aug 2019 21:07:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524851/astrotalk_40487_156214_august_01_14_00_00.mp3" length="53311947" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Recap of the Voyager mission from a PBS broadcoast from Wednesday August 1.</itunes:subtitle><itunes:summary><![CDATA[Recap of the Voyager mission from a PBS broadcoast from Wednesday August 1.]]></itunes:summary><itunes:duration>3332</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Joe Kittinger.</title><link>https://www.spreaker.com/episode/joe-kittinger--23524829</link><description><![CDATA[Joe Kittinger was the first human to jump from space to the Earth. It took bravado true bravado. KIittinger first went up in a balloon in the upper reaches of the atmosphere. then he jump from heights as high as 100,000 feet in free falls to Earth. He almost died once and on one mission, a leak in his spacesuit caused his hand to swell up to several times its size. He also fell unconsious once on a dive. His dives were necessary so that NASA could test the effect of radiation, and of being in space, on the human body. Jon Kittinger: a true pioneer, hero and brave man.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40640-156367-July-25-14-00-00.mp3</guid><pubDate>Thu, 25 Jul 2019 21:05:34 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524829/astrotalk_40640_156367_july_25_14_00_00.mp3" length="56384366" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Joe Kittinger was the first human to jump from space to the Earth. It took bravado true bravado. KIittinger first went up in a balloon in the upper reaches of the atmosphere. then he jump from heights as high as 100,000 feet in free falls to Earth. He...</itunes:subtitle><itunes:summary><![CDATA[Joe Kittinger was the first human to jump from space to the Earth. It took bravado true bravado. KIittinger first went up in a balloon in the upper reaches of the atmosphere. then he jump from heights as high as 100,000 feet in free falls to Earth. He almost died once and on one mission, a leak in his spacesuit caused his hand to swell up to several times its size. He also fell unconsious once on a dive. His dives were necessary so that NASA could test the effect of radiation, and of being in space, on the human body. Jon Kittinger: a true pioneer, hero and brave man.]]></itunes:summary><itunes:duration>3525</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Moon Walking. 50th Anniversary Upcoming. The Birth of the Apollo Missions.</title><link>https://www.spreaker.com/episode/moon-walking-50th-anniversary-upcoming-the-birth-of-the-apollo-missions--23524853</link><description><![CDATA[President Kennedy sets a goal to have men walk on the moon by the end of the 1960s. The competition between the US and the Soviets motivated Kennedy to have America be the first to land on the moon. Looing at all of the considerations NASA had to look at to successfully reach the moon.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40639-156366-July-18-14-00-00.mp3</guid><pubDate>Thu, 18 Jul 2019 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524853/astrotalk_40639_156366_july_18_14_00_00.mp3" length="53087921" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>President Kennedy sets a goal to have men walk on the moon by the end of the 1960s. The competition between the US and the Soviets motivated Kennedy to have America be the first to land on the moon. Looing at all of the considerations NASA had to look...</itunes:subtitle><itunes:summary><![CDATA[President Kennedy sets a goal to have men walk on the moon by the end of the 1960s. The competition between the US and the Soviets motivated Kennedy to have America be the first to land on the moon. Looing at all of the considerations NASA had to look at to successfully reach the moon.]]></itunes:summary><itunes:duration>3318</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--23524831</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40637-156364-July-11-14-00-00.mp3</guid><pubDate>Thu, 11 Jul 2019 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524831/astrotalk_40637_156364_july_11_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Another Show.</title><link>https://www.spreaker.com/episode/another-show--23524791</link><description><![CDATA[Another show.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40638-156365-July-11-14-00-00.mp3</guid><pubDate>Thu, 11 Jul 2019 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524791/astrotalk_40637_156364_july_11_14_00_00.mp3" length="57616092" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Another show.</itunes:subtitle><itunes:summary><![CDATA[Another show.]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Another Show.</title><link>https://www.spreaker.com/episode/another-show--23524838</link><description><![CDATA[Another show.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40636-156363-July-04-14-00-00.mp3</guid><pubDate>Thu, 04 Jul 2019 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524838/astrotalk_40636_156363_july_04_14_00_00.mp3" length="57632392" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Another show.</itunes:subtitle><itunes:summary><![CDATA[Another show.]]></itunes:summary><itunes:duration>3603</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Another Show.</title><link>https://www.spreaker.com/episode/another-show--23524850</link><description><![CDATA[Another show.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40635-156362-June-20-14-00-00.mp3</guid><pubDate>Thu, 27 Jun 2019 21:00:01 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524850/astrotalk_40635_156362_june_20_14_00_00.mp3" length="57600209" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Another show.</itunes:subtitle><itunes:summary><![CDATA[Another show.]]></itunes:summary><itunes:duration>3601</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Mars 2020. Safer Guidance and Landing Systems for Mars. MOXIE. Telescopes. Spitzer Space Telescope. Fermi and Intense Gamma Bursts.</title><link>https://www.spreaker.com/episode/mars-2020-safer-guidance-and-landing-systems-for-mars-moxie-telescopes-spitzer-space-telescope-fermi-and-intense-gamma-bursts--23524868</link><description><![CDATA[Mars 2020 will blaze a trail for human flight to Mars. Entry into the Martian atmosphere for spacecraft from Earth.  7 minutes of terror. Mars 2020 guidance system makes safer landings on Mars. MOXIE.  Telescopes. Fermi Observatory. Hubble ST. How Spitzer has stayed alive for such a long time. But it will be shut down in January 2020. Fermi Mission reveals its most intense Gamma Ray Bursts yet.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40634-156361-June-20-14-03-19.mp3</guid><pubDate>Thu, 20 Jun 2019 21:03:19 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524868/astrotalk_40634_156361_june_20_14_03_19.mp3" length="55472379" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Mars 2020 will blaze a trail for human flight to Mars. Entry into the Martian atmosphere for spacecraft from Earth.  7 minutes of terror. Mars 2020 guidance system makes safer landings on Mars. MOXIE.  Telescopes. Fermi Observatory. Hubble ST. How...</itunes:subtitle><itunes:summary><![CDATA[Mars 2020 will blaze a trail for human flight to Mars. Entry into the Martian atmosphere for spacecraft from Earth.  7 minutes of terror. Mars 2020 guidance system makes safer landings on Mars. MOXIE.  Telescopes. Fermi Observatory. Hubble ST. How Spitzer has stayed alive for such a long time. But it will be shut down in January 2020. Fermi Mission reveals its most intense Gamma Ray Bursts yet.]]></itunes:summary><itunes:duration>3468</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Another Show.</title><link>https://www.spreaker.com/episode/another-show--23524794</link><description><![CDATA[Another show.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40633-156360-June-13-14-00-00.mp3</guid><pubDate>Thu, 13 Jun 2019 21:00:01 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524794/astrotalk_40633_156360_june_13_14_00_00.mp3" length="57599791" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Another show.</itunes:subtitle><itunes:summary><![CDATA[Another show.]]></itunes:summary><itunes:duration>3600</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Another Show.</title><link>https://www.spreaker.com/episode/another-show--23524918</link><description><![CDATA[Another show.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40632-156359-June-06-14-00-00.mp3</guid><pubDate>Thu, 06 Jun 2019 21:00:01 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524918/astrotalk_40632_156359_june_06_14_00_00.mp3" length="57599791" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Another show.</itunes:subtitle><itunes:summary><![CDATA[Another show.]]></itunes:summary><itunes:duration>3600</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>50th Anniversary 1st Moon Walk Coming. Celebrations of 50th Anniv in U.S. Artemis Moon Program. Building Rockets for Space. Goddard. NICER M</title><link>https://www.spreaker.com/episode/50th-anniversary-1st-moon-walk-coming-celebrations-of-50th-anniv-in-u-s-artemis-moon-program-building-rockets-for-space-goddard-nicer-m--23524847</link><description><![CDATA[50th Anniversary 1st moon walk Many exhibits and celebrations in US for the 50 th Anniv. Building rockets for space. NICER Mission Maps ‘Light Echoes’ of New Black Hole.  A newky discovered black hole, MAXI J1820+070 (J1820), is consuming material from a companion star. Waves of X-rays formed “light echoes” that reflected off the swirling gas near the black hole and revealed changes in the environment’s size and shape. <a href="https://www.nasa.gov/feature/goddard/2019/nasa-s-nicer-mission-maps-light-echoes-of-new-black-hole" rel="noopener">https://www.nasa.gov/feature/goddard/2019/nasa-s-nicer-mission-maps-light-echoes-of-new-black-hole</a>. Building large rockets to launch to the Moon in the Artemis Moon Program.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40631-156358-May-30-14-00-00.mp3</guid><pubDate>Thu, 30 May 2019 21:13:39 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524847/astrotalk_40631_156358_may_30_14_00_00.mp3" length="39471647" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>50th Anniversary 1st moon walk Many exhibits and celebrations in US for the 50 th Anniv. Building rockets for space. NICER Mission Maps ‘Light Echoes’ of New Black Hole.  A newky discovered black hole, MAXI J1820+070 (J1820), is consuming material...</itunes:subtitle><itunes:summary><![CDATA[50th Anniversary 1st moon walk Many exhibits and celebrations in US for the 50 th Anniv. Building rockets for space. NICER Mission Maps ‘Light Echoes’ of New Black Hole.  A newky discovered black hole, MAXI J1820+070 (J1820), is consuming material from a companion star. Waves of X-rays formed “light echoes” that reflected off the swirling gas near the black hole and revealed changes in the environment’s size and shape. <a href="https://www.nasa.gov/feature/goddard/2019/nasa-s-nicer-mission-maps-light-echoes-of-new-black-hole" rel="noopener">https://www.nasa.gov/feature/goddard/2019/nasa-s-nicer-mission-maps-light-echoes-of-new-black-hole</a>. Building large rockets to launch to the Moon in the Artemis Moon Program.]]></itunes:summary><itunes:duration>2467</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--23524931</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40630-156357-May-23-14-00-00.mp3</guid><pubDate>Thu, 23 May 2019 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524931/astrotalk_40630_156357_may_23_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Another Program</title><link>https://www.spreaker.com/episode/another-program--23524800</link><description><![CDATA[Another Program]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40629-156356-May-16-14-00-00.mp3</guid><pubDate>Thu, 16 May 2019 21:15:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524800/astrotalk_40629_156356_may_16_14_00_00.mp3" length="43215726" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Another Program</itunes:subtitle><itunes:summary><![CDATA[Another Program]]></itunes:summary><itunes:duration>2701</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>New Clues How Ancient Galaxies Lit Up the Ancient Universe. NASAs Goddard Celebrates its 60 Year Anniversary. Honoring Ellison Onizuka, The</title><link>https://www.spreaker.com/episode/new-clues-how-ancient-galaxies-lit-up-the-ancient-universe-nasas-goddard-celebrates-its-60-year-anniversary-honoring-ellison-onizuka-the--23524867</link><description><![CDATA[Cosmologists: How do they  up with their obscure and exotic theories? Infinite universes? Why is the space between galaxies expanding? Spitzer has revealed that some of the Us earliest galaxies were brighter than expected, because they released incredibly high levels of ionizing radiation. This Epoch of Reionization  transformed the U from being mostly opaque to the brilliant U of stars we have today.  The ancient galaxies were found to be especially bright in a few wavelengths of infrared light, explaining their brilliant glow. 100 million - million years after the big bang, the universe was filled with neutral hydrogen gas that probably had begun to coalesce into stars, which then formed the first galaxies. 1 billion years after the BB, the U began sparkling. Electrons of the neutral hydrogen gas had been stripped away in a process known as ionization. The Epoch of Reionization - the changeover from a universe full of neutral hydrogen to one filled with ionized hydrogen - is well documented. See <a href="https://www.jpl.nasa.gov/news/news.php?feature=7397." rel="noopener">https://www.jpl.nasa.gov/news/news.php?feature=7397.</a> NASAs Goddard Space Flight Center celebrates its 60 year anniversary. Robert H. Goddard is considered the father of modern rocket science. Goddard experimented on his aunt's farm by launching the first liquid fueled rocket.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40488-156215-August-01-14-00-00.mp3</guid><pubDate>Thu, 09 May 2019 21:06:10 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524867/astrotalk_40488_156215_august_01_14_00_00.mp3" length="46576117" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Cosmologists: How do they  up with their obscure and exotic theories? Infinite universes? Why is the space between galaxies expanding? Spitzer has revealed that some of the Us earliest galaxies were brighter than expected, because they released...</itunes:subtitle><itunes:summary><![CDATA[Cosmologists: How do they  up with their obscure and exotic theories? Infinite universes? Why is the space between galaxies expanding? Spitzer has revealed that some of the Us earliest galaxies were brighter than expected, because they released incredibly high levels of ionizing radiation. This Epoch of Reionization  transformed the U from being mostly opaque to the brilliant U of stars we have today.  The ancient galaxies were found to be especially bright in a few wavelengths of infrared light, explaining their brilliant glow. 100 million - million years after the big bang, the universe was filled with neutral hydrogen gas that probably had begun to coalesce into stars, which then formed the first galaxies. 1 billion years after the BB, the U began sparkling. Electrons of the neutral hydrogen gas had been stripped away in a process known as ionization. The Epoch of Reionization - the changeover from a universe full of neutral hydrogen to one filled with ionized hydrogen - is well documented. See <a href="https://www.jpl.nasa.gov/news/news.php?feature=7397." rel="noopener">https://www.jpl.nasa.gov/news/news.php?feature=7397.</a> NASAs Goddard Space Flight Center celebrates its 60 year anniversary. Robert H. Goddard is considered the father of modern rocket science. Goddard experimented on his aunt's farm by launching the first liquid fueled rocket.]]></itunes:summary><itunes:duration>2912</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Giant Galaxy Around A Giant Black Hole. Plans for Asteroid Flyby One Decade Away. Insight Captures Sunset and Sunrise on Mars.</title><link>https://www.spreaker.com/episode/giant-galaxy-around-a-giant-black-hole-plans-for-asteroid-flyby-one-decade-away-insight-captures-sunset-and-sunrise-on-mars--23524924</link><description><![CDATA[The event horizon of a black hole has been photographed for the first time. The black hole has a mass of 6.5 Million suns. The image was made by the Spitzer Space Telescope in infrared light. The image from M87 is 55 million light years away. 99942 Apophis that will fly  harmlessly by the Earth on April 13 2029, coming within  19,000 miles or 31,000 kilometers from Earth. Scientists are planning for this incredible opportunity to study this asteroid.  The Insight Lander captures Sunset and Sunrise on Mars. The photos were snapped April 24 and 25, the 145th Martian day, or sol, of the mission, by a camera on the spacecraft's robotic arm. The length of day's on other planets in the Solar System.<br /><br /><br />The Giant Galaxy Around the Giant Black Hole<br />The galaxy M87, imaged here by NASA's Spitzer Space Telescope, is home to a supermassive black hole that spews two jets of material out into space at nearly the speed of light. The inset shows a close-up view of the shockwaves created by the two jets.Credit: NASA/JPL-Caltech/IPAC <br />› Full image and caption<br />On April 10, 2019, the Event Horizon Telescope (EHT) unveiled the first-ever image of a black hole's event horizon, the area beyond which light cannot escape the immense gravity of the black hole. That giant black hole, with a mass of 6.5 billion Suns, is located in the elliptical galaxy Messier 87 (M87). EHT is an international collaboration whose support in the U.S. includes the National Science Foundation.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40485-156212-May-02-13-59-37.mp3</guid><pubDate>Thu, 02 May 2019 20:59:37 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524924/astrotalk_40485_156212_may_02_13_59_37.mp3" length="52608105" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The event horizon of a black hole has been photographed for the first time. The black hole has a mass of 6.5 Million suns. The image was made by the Spitzer Space Telescope in infrared light. The image from M87 is 55 million light years away. 99942...</itunes:subtitle><itunes:summary><![CDATA[The event horizon of a black hole has been photographed for the first time. The black hole has a mass of 6.5 Million suns. The image was made by the Spitzer Space Telescope in infrared light. The image from M87 is 55 million light years away. 99942 Apophis that will fly  harmlessly by the Earth on April 13 2029, coming within  19,000 miles or 31,000 kilometers from Earth. Scientists are planning for this incredible opportunity to study this asteroid.  The Insight Lander captures Sunset and Sunrise on Mars. The photos were snapped April 24 and 25, the 145th Martian day, or sol, of the mission, by a camera on the spacecraft's robotic arm. The length of day's on other planets in the Solar System.<br /><br /><br />The Giant Galaxy Around the Giant Black Hole<br />The galaxy M87, imaged here by NASA's Spitzer Space Telescope, is home to a supermassive black hole that spews two jets of material out into space at nearly the speed of light. The inset shows a close-up view of the shockwaves created by the two jets.Credit: NASA/JPL-Caltech/IPAC <br />› Full image and caption<br />On April 10, 2019, the Event Horizon Telescope (EHT) unveiled the first-ever image of a black hole's event horizon, the area beyond which light cannot escape the immense gravity of the black hole. That giant black hole, with a mass of 6.5 billion Suns, is located in the elliptical galaxy Messier 87 (M87). EHT is an international collaboration whose support in the U.S. includes the National Science Foundation.]]></itunes:summary><itunes:duration>3289</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Expansion Rate of the Universe. Stephen Hawking Theories on the Universe. Universe Expanding Ever-Faster. Apollo 10 and Snoopy.</title><link>https://www.spreaker.com/episode/expansion-rate-of-the-universe-stephen-hawking-theories-on-the-universe-universe-expanding-ever-faster-apollo-10-and-snoopy--23524897</link><description><![CDATA[Hubble shows that the expansion rate of the universe is increasing (accelerating?) A cosmic distance ladder is getting more accurate with this data. DASH. Drift and shift method used in the study. Apollo 10 in the spacecrafts Snoopy and Chral;ie Brown circled the moon to scout for the best landing sites of the Apollo 11 mission, when Neil Armstrong was the first person to set foor on the moon. NASA is using a new instrument, a flux radiometer, to make new measurerments of Jupiter, Neptune and Uranus. the hope is to probe the heat engine driving the gas giants' atmospheric circulation. <br /><br /><br /><a href="https://www.nasa.gov/feature/goddard/2019/mystery-of-the-universe-s-expansion-rate-widens-with-new-hubble-data" rel="noopener">https://www.nasa.gov/feature/goddard/2019/mystery-of-the-universe-s-expansion-rate-widens-with-new-hubble-data</a><br /><a href="https://www.nasa.gov/feature/50-years-ago-apollo-10-a-great-amount-of-team-work" rel="noopener">https://www.nasa.gov/feature/50-years-ago-apollo-10-a-great-amount-of-team-work</a><br /><a href="https://www.nasa.gov/feature/goddard/2019/next-generation-nasa-instrument-advanced-to-study-the-atmospheres-of-uranus-and-neptune" rel="noopener">https://www.nasa.gov/feature/goddard/2019/next-generation-nasa-instrument-advanced-to-study-the-atmospheres-of-uranus-and-neptune</a>]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40444-156171-April-25-14-00-00.mp3</guid><pubDate>Thu, 25 Apr 2019 21:03:01 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524897/astrotalk_40444_156171_april_25_14_00_00.mp3" length="54720053" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Hubble shows that the expansion rate of the universe is increasing (accelerating?) A cosmic distance ladder is getting more accurate with this data. DASH. Drift and shift method used in the study. Apollo 10 in the spacecrafts Snoopy and Chral;ie Brown...</itunes:subtitle><itunes:summary><![CDATA[Hubble shows that the expansion rate of the universe is increasing (accelerating?) A cosmic distance ladder is getting more accurate with this data. DASH. Drift and shift method used in the study. Apollo 10 in the spacecrafts Snoopy and Chral;ie Brown circled the moon to scout for the best landing sites of the Apollo 11 mission, when Neil Armstrong was the first person to set foor on the moon. NASA is using a new instrument, a flux radiometer, to make new measurerments of Jupiter, Neptune and Uranus. the hope is to probe the heat engine driving the gas giants' atmospheric circulation. <br /><br /><br /><a href="https://www.nasa.gov/feature/goddard/2019/mystery-of-the-universe-s-expansion-rate-widens-with-new-hubble-data" rel="noopener">https://www.nasa.gov/feature/goddard/2019/mystery-of-the-universe-s-expansion-rate-widens-with-new-hubble-data</a><br /><a href="https://www.nasa.gov/feature/50-years-ago-apollo-10-a-great-amount-of-team-work" rel="noopener">https://www.nasa.gov/feature/50-years-ago-apollo-10-a-great-amount-of-team-work</a><br /><a href="https://www.nasa.gov/feature/goddard/2019/next-generation-nasa-instrument-advanced-to-study-the-atmospheres-of-uranus-and-neptune" rel="noopener">https://www.nasa.gov/feature/goddard/2019/next-generation-nasa-instrument-advanced-to-study-the-atmospheres-of-uranus-and-neptune</a>]]></itunes:summary><itunes:duration>3420</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Universe's First Molecule Found, Hydrocarban Cycle, Titan. A New Signal for a Neutron Star Colliision</title><link>https://www.spreaker.com/episode/universe-s-first-molecule-found-hydrocarban-cycle-titan-a-new-signal-for-a-neutron-star-colliision--23524854</link><description><![CDATA[Universe's first molecule, helium huydride, has been found in the planetary nebula NGC 7027, 3,000 light years away. The observatory SOFIA made the discovery. 100,000 years after the Big Band, helium and huydrogen combined to form helium hydride. this is the first time it has been detected. Cassini reveals that the small liquid lakes on Titan, Saturn's largest moon, are surprisingly large. Ethane and methane are gases on earth, but on Titan, they exist in the liquid state. These liquids therefore rain down onto Titan. Tiitan has a hydrocarbon cycle, where on Earth, we have a water cycle. A new signal for a neutron star collision.<br /><br /><a href="https://www.nasa.gov/feature/the-universe-s-first-type-of-molecule-is-found-at-last" rel="noopener">https://www.nasa.gov/feature/the-universe-s-first-type-of-molecule-is-found-at-last</a><br /><a href="https://www.jpl.nasa.gov/news/news.php?feature=4635" rel="noopener">https://www.jpl.nasa.gov/news/news.php?feature=4635</a><br /><a href="https://www.nasa.gov/mission_pages/chandra/images/a-new-signal-for-a-neutron-star-collision-discovered.html" rel="noopener">https://www.nasa.gov/mission_pages/chandra/images/a-new-signal-for-a-neutron-star-collision-discovered.html</a><br /><br /><br /><br /><br />3,000 light-years away near the constellation Cygnus, this planetary nebula, called]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-40442-156169-April-18-14-03-18.mp3</guid><pubDate>Thu, 18 Apr 2019 21:03:18 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524854/astrotalk_40442_156169_april_18_14_03_18.mp3" length="52320130" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Universe's first molecule, helium huydride, has been found in the planetary nebula NGC 7027, 3,000 light years away. The observatory SOFIA made the discovery. 100,000 years after the Big Band, helium and huydrogen combined to form helium hydride. this...</itunes:subtitle><itunes:summary><![CDATA[Universe's first molecule, helium huydride, has been found in the planetary nebula NGC 7027, 3,000 light years away. The observatory SOFIA made the discovery. 100,000 years after the Big Band, helium and huydrogen combined to form helium hydride. this is the first time it has been detected. Cassini reveals that the small liquid lakes on Titan, Saturn's largest moon, are surprisingly large. Ethane and methane are gases on earth, but on Titan, they exist in the liquid state. These liquids therefore rain down onto Titan. Tiitan has a hydrocarbon cycle, where on Earth, we have a water cycle. A new signal for a neutron star collision.<br /><br /><a href="https://www.nasa.gov/feature/the-universe-s-first-type-of-molecule-is-found-at-last" rel="noopener">https://www.nasa.gov/feature/the-universe-s-first-type-of-molecule-is-found-at-last</a><br /><a href="https://www.jpl.nasa.gov/news/news.php?feature=4635" rel="noopener">https://www.jpl.nasa.gov/news/news.php?feature=4635</a><br /><a href="https://www.nasa.gov/mission_pages/chandra/images/a-new-signal-for-a-neutron-star-collision-discovered.html" rel="noopener">https://www.nasa.gov/mission_pages/chandra/images/a-new-signal-for-a-neutron-star-collision-discovered.html</a><br /><br /><br /><br /><br />3,000 light-years away near the constellation Cygnus, this planetary nebula, called]]></itunes:summary><itunes:duration>3271</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>International Space Station Spinoffs</title><link>https://www.spreaker.com/episode/international-space-station-spinoffs--23524914</link><description><![CDATA[Counting the Many Ways the Space Station Benefits Humankind. There are many spinoffs  from research done on the ISS that benefit humans on Earth. Go to <a href="https://www.nasa.gov/stationbenefits" rel="noopener">https://www.nasa.gov/stationbenefits</a> to find out more.  These range from improved water filtration systems to medical advances that help patients with heart problems. Also, NASA  is studying plants from space. The OCO-2 is a polar oribiting satelllite that studies carbon, CO2, oxygen and other gas signatures in the Arctic, from space. OCO-3, soon to be launched, will make its home on ISS, and will study carbon, and other gas signatures in the tropics. In the Arctic, CO2 & C is primarily buried in the ground, under ice sheets. In the tropics, OCO-3 will study leaves and plants.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-39674-155406-April-11-14-00-00.mp3</guid><pubDate>Thu, 11 Apr 2019 21:00:41 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524914/astrotalk_39674_155406_april_11_14_00_00.mp3" length="52287948" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Counting the Many Ways the Space Station Benefits Humankind. There are many spinoffs  from research done on the ISS that benefit humans on Earth. Go to https://www.nasa.gov/stationbenefits to find out more.  These range from improved water filtration...</itunes:subtitle><itunes:summary><![CDATA[Counting the Many Ways the Space Station Benefits Humankind. There are many spinoffs  from research done on the ISS that benefit humans on Earth. Go to <a href="https://www.nasa.gov/stationbenefits" rel="noopener">https://www.nasa.gov/stationbenefits</a> to find out more.  These range from improved water filtration systems to medical advances that help patients with heart problems. Also, NASA  is studying plants from space. The OCO-2 is a polar oribiting satelllite that studies carbon, CO2, oxygen and other gas signatures in the Arctic, from space. OCO-3, soon to be launched, will make its home on ISS, and will study carbon, and other gas signatures in the tropics. In the Arctic, CO2 & C is primarily buried in the ground, under ice sheets. In the tropics, OCO-3 will study leaves and plants.]]></itunes:summary><itunes:duration>3268</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Spinoff Technology. 30 Dangers to Humans in Space. Studying Glaciers from Space.</title><link>https://www.spreaker.com/episode/spinoff-technology-30-dangers-to-humans-in-space-studying-glaciers-from-space--23524799</link><description><![CDATA[More on NASA Spinoff Technology. NASA has identified 30 dangers to humans in space.  One example is how blood flow is impacted by micro-gravity in space.  NASA is studying glaciers from space. Jane Stupic looks through a telescope for women's history month. Review of  NASA's Europa Clipper mission.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-39679-155411-April-04-14-00-00.mp3</guid><pubDate>Thu, 04 Apr 2019 21:02:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524799/astrotalk_39679_155411_april_04_14_00_00.mp3" length="50479857" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>More on NASA Spinoff Technology. NASA has identified 30 dangers to humans in space.  One example is how blood flow is impacted by micro-gravity in space.  NASA is studying glaciers from space. Jane Stupic looks through a telescope for women's history...</itunes:subtitle><itunes:summary><![CDATA[More on NASA Spinoff Technology. NASA has identified 30 dangers to humans in space.  One example is how blood flow is impacted by micro-gravity in space.  NASA is studying glaciers from space. Jane Stupic looks through a telescope for women's history month. Review of  NASA's Europa Clipper mission.]]></itunes:summary><itunes:duration>3155</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>NASA viewing Glaciers Melting in the Arctic. Nasa Spinoff Technology.</title><link>https://www.spreaker.com/episode/nasa-viewing-glaciers-melting-in-the-arctic-nasa-spinoff-technology--23524927</link><description><![CDATA[Glaciers are melting in the Arctic.  Clipper is going to Europa to test, among other things, to determine if life is present in the sub-surface ocean in Europa, a Jovian moon.   HGA is a high gain attena that Clipper will use to monitor Europa. New Spinoff publication highlights NASA technology in use in the civilian sector.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-39740-155472-April-04-14-00-00.mp3</guid><pubDate>Thu, 04 Apr 2019 21:01:57 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524927/astrotalk_39740_155472_april_04_14_00_00.mp3" length="50560104" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Glaciers are melting in the Arctic.  Clipper is going to Europa to test, among other things, to determine if life is present in the sub-surface ocean in Europa, a Jovian moon.   HGA is a high gain attena that Clipper will use to monitor Europa. New...</itunes:subtitle><itunes:summary><![CDATA[Glaciers are melting in the Arctic.  Clipper is going to Europa to test, among other things, to determine if life is present in the sub-surface ocean in Europa, a Jovian moon.   HGA is a high gain attena that Clipper will use to monitor Europa. New Spinoff publication highlights NASA technology in use in the civilian sector.]]></itunes:summary><itunes:duration>3161</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Humans Back to the Moon. Review of Voyager missions entering Interstellar Space. A Space Butterfly in Space Studied by the Spitzer Space Tel</title><link>https://www.spreaker.com/episode/humans-back-to-the-moon-review-of-voyager-missions-entering-interstellar-space-a-space-butterfly-in-space-studied-by-the-spitzer-space-tel--23524858</link><description><![CDATA[NASA is going back to the Moon with  its Gateway  mission.  NASA is putting US astronauts back on the moon within 5 years. NASA will go their on the Orion spacecraft.  The moon has a very important  and stabilizing influence on the Earth.  The Voyager mission  has now placed its 2 spacecraft V1 & V2 in interstellar space (IS).  Voyager 2's magnetometer and other cosmic ray telescopes on-board are making measurements of the IS it is now in.  The high energy particles that were expected in IS are present,  The low energy particles were also present before V 2 crossed into IS.  Hubble and the Spitzer Space telescope are looking at a nebula, W40, called the butterfly, which is 1,400 light years away. the images are in infrared and x-ray. The lit up nebula glowing in different colors. To the right of W40 is another cluster of stars, known as Serpens South.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-39769-155501-March-28-14-00-00.mp3</guid><pubDate>Thu, 28 Mar 2019 21:00:05 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524858/astrotalk_39769_155501_march_28_14_00_00.mp3" length="53872013" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>NASA is going back to the Moon with  its Gateway  mission.  NASA is putting US astronauts back on the moon within 5 years. NASA will go their on the Orion spacecraft.  The moon has a very important  and stabilizing influence on the Earth.  The Voyager...</itunes:subtitle><itunes:summary><![CDATA[NASA is going back to the Moon with  its Gateway  mission.  NASA is putting US astronauts back on the moon within 5 years. NASA will go their on the Orion spacecraft.  The moon has a very important  and stabilizing influence on the Earth.  The Voyager mission  has now placed its 2 spacecraft V1 & V2 in interstellar space (IS).  Voyager 2's magnetometer and other cosmic ray telescopes on-board are making measurements of the IS it is now in.  The high energy particles that were expected in IS are present,  The low energy particles were also present before V 2 crossed into IS.  Hubble and the Spitzer Space telescope are looking at a nebula, W40, called the butterfly, which is 1,400 light years away. the images are in infrared and x-ray. The lit up nebula glowing in different colors. To the right of W40 is another cluster of stars, known as Serpens South.]]></itunes:summary><itunes:duration>3367</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>US Going Back to the Moon Within Five Years. Voyager II Reaches Interstellar Space.  Giant Butterfly Forming In Nebula 1,400 light Years Fro</title><link>https://www.spreaker.com/episode/us-going-back-to-the-moon-within-five-years-voyager-ii-reaches-interstellar-space-giant-butterfly-forming-in-nebula-1-400-light-years-fro--23524879</link><description><![CDATA[VP Mike Pence announces US going back to the Moon within 5 years.  The Moon is our Buddy. Yah!!  Voyager II has reached Interstellar Space (IS).  Four decades after launch, the 2 Voyager spacecraft have travelled farther into space than any spacecrafts in our history. Measurements were made just before the Voyagers left our solar system, and then just after they entered IS. The measurements confirm that both Voyagers have indeed entered IS.  WD 40  and the Space Butterfly. A space butterfly has been detected in space by Hubble. WD 40 is a nebula, which is home to  hundreds of baby stars. WD 40 shows an examples of how the dust that creates stars is destroyed by the very stars they make. The giant wings of the nebula are giant bubbles of gas that are blown out of the inside of the nebula, by the massive stars forming from within the nebula.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-39924-155656-March-28-14-00-00.mp3</guid><pubDate>Thu, 28 Mar 2019 21:00:04 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524879/astrotalk_39924_155656_march_28_14_00_00.mp3" length="53872013" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>VP Mike Pence announces US going back to the Moon within 5 years.  The Moon is our Buddy. Yah!!  Voyager II has reached Interstellar Space (IS).  Four decades after launch, the 2 Voyager spacecraft have travelled farther into space than any...</itunes:subtitle><itunes:summary><![CDATA[VP Mike Pence announces US going back to the Moon within 5 years.  The Moon is our Buddy. Yah!!  Voyager II has reached Interstellar Space (IS).  Four decades after launch, the 2 Voyager spacecraft have travelled farther into space than any spacecrafts in our history. Measurements were made just before the Voyagers left our solar system, and then just after they entered IS. The measurements confirm that both Voyagers have indeed entered IS.  WD 40  and the Space Butterfly. A space butterfly has been detected in space by Hubble. WD 40 is a nebula, which is home to  hundreds of baby stars. WD 40 shows an examples of how the dust that creates stars is destroyed by the very stars they make. The giant wings of the nebula are giant bubbles of gas that are blown out of the inside of the nebula, by the massive stars forming from within the nebula.]]></itunes:summary><itunes:duration>3367</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Super Worm Vernal Equinox Moon. Hopping Water on the Moon.</title><link>https://www.spreaker.com/episode/super-worm-vernal-equinox-moon-hopping-water-on-the-moon--23524861</link><description><![CDATA[Worm Moon  of Wednesday March 20.  A type of super moon, a full moon,a super worm moon occurs when the sun crosses the celestial equator.  It will be closest to the Earth on its monthly orbit.  Full moons tend to be named from earlier Aborigiinal tribes.  The moon will rise due East while the Sun sets in the West, shine all night for 12 hours, then set in the West while the Sun rises in the East.  The worm moon will be the smallest of 2019's super moons.  water hops around on the moon. Knowledge of how water behaves on the moon will be important when we return to the moon in the next few years.  The moon is a complex geological body, so more studying is needed.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-39922-155654-March-21-14-00-00.mp3</guid><pubDate>Thu, 21 Mar 2019 21:03:22 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524861/astrotalk_39922_155654_march_21_14_00_00.mp3" length="49631817" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Worm Moon  of Wednesday March 20.  A type of super moon, a full moon,a super worm moon occurs when the sun crosses the celestial equator.  It will be closest to the Earth on its monthly orbit.  Full moons tend to be named from earlier Aborigiinal...</itunes:subtitle><itunes:summary><![CDATA[Worm Moon  of Wednesday March 20.  A type of super moon, a full moon,a super worm moon occurs when the sun crosses the celestial equator.  It will be closest to the Earth on its monthly orbit.  Full moons tend to be named from earlier Aborigiinal tribes.  The moon will rise due East while the Sun sets in the West, shine all night for 12 hours, then set in the West while the Sun rises in the East.  The worm moon will be the smallest of 2019's super moons.  water hops around on the moon. Knowledge of how water behaves on the moon will be important when we return to the moon in the next few years.  The moon is a complex geological body, so more studying is needed.]]></itunes:summary><itunes:duration>3102</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Dust in the Universe. Goddard Prepares for New Era of Moon Exploration.</title><link>https://www.spreaker.com/episode/dust-in-the-universe-goddard-prepares-for-new-era-of-moon-exploration--23524863</link><description><![CDATA[Dust is prevalent in the universe. Around the sun, in the paths of planets, in beautiful nebualas, dust is everywhere. Dust also accumulates in strange places.  How strange? Dust co-orbits with Venus, but not with other planets. Part of the rings of Saturn are made of dust. Dust rings circle the sun. Nebulas are made largely of dust, and it is in nebulas where stars are born. Dust also moves around the solar system, and in the universe in ordered patterns.  Goddard prepares for a new of exploration for the Moon and Mars..]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-39921-155653-March-14-14-00-00.mp3</guid><pubDate>Thu, 14 Mar 2019 21:02:40 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524863/astrotalk_39921_155653_march_14_14_00_00.mp3" length="51344196" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Dust is prevalent in the universe. Around the sun, in the paths of planets, in beautiful nebualas, dust is everywhere. Dust also accumulates in strange places.  How strange? Dust co-orbits with Venus, but not with other planets. Part of the rings of...</itunes:subtitle><itunes:summary><![CDATA[Dust is prevalent in the universe. Around the sun, in the paths of planets, in beautiful nebualas, dust is everywhere. Dust also accumulates in strange places.  How strange? Dust co-orbits with Venus, but not with other planets. Part of the rings of Saturn are made of dust. Dust rings circle the sun. Nebulas are made largely of dust, and it is in nebulas where stars are born. Dust also moves around the solar system, and in the universe in ordered patterns.  Goddard prepares for a new of exploration for the Moon and Mars..]]></itunes:summary><itunes:duration>3210</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--23524866</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-39923-155655-March-14-14-00-00.mp3</guid><pubDate>Thu, 14 Mar 2019 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524866/astrotalk_39923_155655_march_14_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Fundrive</title><link>https://www.spreaker.com/episode/fundrive--23524943</link><description><![CDATA[Fundrive show.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-39915-155647-March-07-14-00-00.mp3</guid><pubDate>Thu, 07 Mar 2019 21:04:49 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524943/astrotalk_39915_155647_march_07_14_00_00.mp3" length="49072170" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Fundrive show.</itunes:subtitle><itunes:summary><![CDATA[Fundrive show.]]></itunes:summary><itunes:duration>3068</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--23524952</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-39914-155646-February-28-14-00-00.mp3</guid><pubDate>Thu, 28 Feb 2019 21:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524952/astrotalk_39914_155646_february_28_14_00_00.mp3" length="57616091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>3602</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Alex Filipenko Supernovas and Timescales. Star Clusters. Galaxy Clusters. My guest Mr. Dave.</title><link>https://www.spreaker.com/episode/alex-filipenko-supernovas-and-timescales-star-clusters-galaxy-clusters-my-guest-mr-dave--23524738</link><description><![CDATA[Hunting Supernovas. SN allows scientists to study something  that is occuring on a timescale through which we can study the whole process. A SN might shine brightly for a few weeks, whereas if a solar system is forming, it might take millions of years to form, and we don't live for millions of years. Star Clusters - globular clusters and open clusters. Most if not all stars form in star clusters.  NASA show how ingredients for water on the water can allows astronauts to make water on the moon.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2019/AstroTalk-39913-155645-February-21-14-00-00.mp3</guid><pubDate>Thu, 21 Feb 2019 21:00:31 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524738/astrotalk_39913_155645_february_21_14_00_00.mp3" length="54911896" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Hunting Supernovas. SN allows scientists to study something  that is occuring on a timescale through which we can study the whole process. A SN might shine brightly for a few weeks, whereas if a solar system is forming, it might take millions of years...</itunes:subtitle><itunes:summary><![CDATA[Hunting Supernovas. SN allows scientists to study something  that is occuring on a timescale through which we can study the whole process. A SN might shine brightly for a few weeks, whereas if a solar system is forming, it might take millions of years to form, and we don't live for millions of years. Star Clusters - globular clusters and open clusters. Most if not all stars form in star clusters.  NASA show how ingredients for water on the water can allows astronauts to make water on the moon.]]></itunes:summary><itunes:duration>3432</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>NASA's 60th Birthday. NASA Satellites View California Wildfires. ECOSTRESS. TESS Begins Operating.</title><link>https://www.spreaker.com/episode/nasa-s-60th-birthday-nasa-satellites-view-california-wildfires-ecostress-tess-begins-operating--23524862</link><description><![CDATA[NASA celebrates it's 60th birthday  NASA Satellites View California Wildfires. NASA's Terra satellite is viewing Northern California' raging wildfires with its  Multi-angle Imaging SpectroRadiometer (MISR) instrument. Terra passed over California July 27 and July 29, observing the Carr Fire on July 27 and the Ferguson Fire on July 29.  MISR's 9 cameras view Earth at different angles, and is able to measure the height of the fire's plumes. The plumes don't go up a very great height, so the air quality closer to the Earth is affected more. The drought from 2012 on is a major reason for the ferocity of the  fires. ECOSTRESS can see 4 other things. What's ECOSTRESS? Ecosystem Spaceborne Thermal Radiometer Experiment on Space Station  is designed to study how plants respond to heat and water stress. ECOSTRESS" precise temperature measurements of the Earth  ES monitors fires, volcanoes, urban heat and coastal and inland waters. NASA's TESS Spacecraft has started its science operations on July 25, 2018. TESS will transmit ifs first data to Earth beginning August, and after that, data will be sent back to Earthy every 13.5 days. TESS will search for exoplanets in our Milky Way neighborhood. by monitoring periodic dips in light intensity from a star, as a planet (or planets) pass in front of the star.  <br /><br /><a href="https://climate.nasa.gov/news/2774/nasas-misr-views-raging-fires-in-california/" rel="noopener">https://climate.nasa.gov/news/2774/nasas-misr-views-raging-fires-in-california/</a><br /><a href="https://climate.nasa.gov/news/2758/four-things-ecostress-can-see-from-space-in-addition-to-plants/" rel="noopener">https://climate.nasa.gov/news/2758/four-things-ecostress-can-see-from-space-in-addition-to-plants/</a><br /><a href="https://www.nasa.gov/feature/goddard/2018/nasa-s-tess-spacecraft-starts-science-operations" rel="noopener">https://www.nasa.gov/feature/goddard/2018/nasa-s-tess-spacecraft-starts-science-operations</a>]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-August-02-14-00-00.mp3</guid><pubDate>Thu, 02 Aug 2018 21:02:42 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524862/astrotalk_august_02_14_00_00.mp3" length="52944144" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>NASA celebrates it's 60th birthday  NASA Satellites View California Wildfires. NASA's Terra satellite is viewing Northern California' raging wildfires with its  Multi-angle Imaging SpectroRadiometer (MISR) instrument. Terra passed over California July...</itunes:subtitle><itunes:summary><![CDATA[NASA celebrates it's 60th birthday  NASA Satellites View California Wildfires. NASA's Terra satellite is viewing Northern California' raging wildfires with its  Multi-angle Imaging SpectroRadiometer (MISR) instrument. Terra passed over California July 27 and July 29, observing the Carr Fire on July 27 and the Ferguson Fire on July 29.  MISR's 9 cameras view Earth at different angles, and is able to measure the height of the fire's plumes. The plumes don't go up a very great height, so the air quality closer to the Earth is affected more. The drought from 2012 on is a major reason for the ferocity of the  fires. ECOSTRESS can see 4 other things. What's ECOSTRESS? Ecosystem Spaceborne Thermal Radiometer Experiment on Space Station  is designed to study how plants respond to heat and water stress. ECOSTRESS" precise temperature measurements of the Earth  ES monitors fires, volcanoes, urban heat and coastal and inland waters. NASA's TESS Spacecraft has started its science operations on July 25, 2018. TESS will transmit ifs first data to Earth beginning August, and after that, data will be sent back to Earthy every 13.5 days. TESS will search for exoplanets in our Milky Way neighborhood. by monitoring periodic dips in light intensity from a star, as a planet (or planets) pass in front of the star.  <br /><br /><a href="https://climate.nasa.gov/news/2774/nasas-misr-views-raging-fires-in-california/" rel="noopener">https://climate.nasa.gov/news/2774/nasas-misr-views-raging-fires-in-california/</a><br /><a href="https://climate.nasa.gov/news/2758/four-things-ecostress-can-see-from-space-in-addition-to-plants/" rel="noopener">https://climate.nasa.gov/news/2758/four-things-ecostress-can-see-from-space-in-addition-to-plants/</a><br /><a href="https://www.nasa.gov/feature/goddard/2018/nasa-s-tess-spacecraft-starts-science-operations" rel="noopener">https://www.nasa.gov/feature/goddard/2018/nasa-s-tess-spacecraft-starts-science-operations</a>]]></itunes:summary><itunes:duration>3310</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Radiation Map of Europa. Extension for Juno Mission Orbiting Jupiter.</title><link>https://www.spreaker.com/episode/radiation-map-of-europa-extension-for-juno-mission-orbiting-jupiter--23524864</link><description><![CDATA[Europa could be a promising place for life outside Earth. Problem is: Jupiter is pummeling Europa with radiation, so detecting possible life signs is nearly impossible because Jupiter's radiation bombards Europa, and any of the water that makes it to Europa's Surface.  This material could be altered or destroyed by Jupiter's radiation. In planning for future missions to Europa, scientists are making maps of the radiation to learn where the rad is most intense, and least intense. NASA is planning to send a spacecraft, called Clipper, to Europa in 2022, but for now, Juno is mapping Europa. The Juno spacecraft's original plan was to make orbits of Jupiter every 14 days, but due to technical issues, it is now orbiting Jupiter (around the Pole) every 53 days. <br /><br /><a href="https://www.jpl.nasa.gov/news/news.php?release=2018-170Surface" rel="noopener">https://www.jpl.nasa.gov/news/news.php?release=2018-170Surface</a>]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-July-26-14-00-00.mp3</guid><pubDate>Thu, 26 Jul 2018 21:08:44 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524864/astrotalk_july_26_14_00_00.mp3" length="47311726" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Europa could be a promising place for life outside Earth. Problem is: Jupiter is pummeling Europa with radiation, so detecting possible life signs is nearly impossible because Jupiter's radiation bombards Europa, and any of the water that makes it to...</itunes:subtitle><itunes:summary><![CDATA[Europa could be a promising place for life outside Earth. Problem is: Jupiter is pummeling Europa with radiation, so detecting possible life signs is nearly impossible because Jupiter's radiation bombards Europa, and any of the water that makes it to Europa's Surface.  This material could be altered or destroyed by Jupiter's radiation. In planning for future missions to Europa, scientists are making maps of the radiation to learn where the rad is most intense, and least intense. NASA is planning to send a spacecraft, called Clipper, to Europa in 2022, but for now, Juno is mapping Europa. The Juno spacecraft's original plan was to make orbits of Jupiter every 14 days, but due to technical issues, it is now orbiting Jupiter (around the Pole) every 53 days. <br /><br /><a href="https://www.jpl.nasa.gov/news/news.php?release=2018-170Surface" rel="noopener">https://www.jpl.nasa.gov/news/news.php?release=2018-170Surface</a>]]></itunes:summary><itunes:duration>2957</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Proton Proton Chain. A Planet Devouring Star. Red Nugget Galaxies.</title><link>https://www.spreaker.com/episode/proton-proton-chain-a-planet-devouring-star-red-nugget-galaxies--23524801</link><description><![CDATA[The Proton Proton chain takes place in the center of the Sun. This makes 2 neutrinos, those little ghost particles. The neutrinos leave the Sun right away and some of them head to Earth. 6 billion neutrinos go through your thumb every second. This is just one source of neutrinos. Last week, we talked about n black hole producing neutrinos. Today, our first topic is Chandra sees first evidence of star devouring a planet. RW Aur A is star that is located in the Taurus-Auriga Dark Clouds, which has stellar nurseries containing thousands of infant stars. Scientists believe that planetesimals colliding close to the star are producing gas and dust that obscure or dim the light from the star, that can be seen from Earth.  Since the last decade, astronomers are observing dense, distant galaxies they have called Red Nugget Galaxies. The RNG have masses that are similar to giant elliptical galaxies, but have only 1/5 of the mass of the giant galaxies. Most red nuggets merged with other galaxies billions of years, but a small number slipped through a long history  untouched. These unscathed red nuggets givea golden opportunity to study how the galaxies, and the supermassive black hole at their centers, act over billions of years of isolation.<br /><br /><a href="https://www.nasa.gov/mission_pages/chandra/news/chandra-may-have-first-evidence-of-a-young-star-devouring-a-planet.htmleutrinos" rel="noopener">https://www.nasa.gov/mission_pages/chandra/news/chandra-may-have-first-evidence-of-a-young-star-devouring-a-planet.htmleutrinos</a> coming from black holes. <br /><a href="https://www.nasa.gov/mission_pages/chandra/news/red-nuggets-are-galactic-gold-for-astronomers.html" rel="noopener">https://www.nasa.gov/mission_pages/chandra/news/red-nuggets-are-galactic-gold-for-astronomers.html</a>]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-July-19-14-00-00.mp3</guid><pubDate>Thu, 19 Jul 2018 21:02:57 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524801/astrotalk_july_19_14_00_00.mp3" length="52623987" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The Proton Proton chain takes place in the center of the Sun. This makes 2 neutrinos, those little ghost particles. The neutrinos leave the Sun right away and some of them head to Earth. 6 billion neutrinos go through your thumb every second. This is...</itunes:subtitle><itunes:summary><![CDATA[The Proton Proton chain takes place in the center of the Sun. This makes 2 neutrinos, those little ghost particles. The neutrinos leave the Sun right away and some of them head to Earth. 6 billion neutrinos go through your thumb every second. This is just one source of neutrinos. Last week, we talked about n black hole producing neutrinos. Today, our first topic is Chandra sees first evidence of star devouring a planet. RW Aur A is star that is located in the Taurus-Auriga Dark Clouds, which has stellar nurseries containing thousands of infant stars. Scientists believe that planetesimals colliding close to the star are producing gas and dust that obscure or dim the light from the star, that can be seen from Earth.  Since the last decade, astronomers are observing dense, distant galaxies they have called Red Nugget Galaxies. The RNG have masses that are similar to giant elliptical galaxies, but have only 1/5 of the mass of the giant galaxies. Most red nuggets merged with other galaxies billions of years, but a small number slipped through a long history  untouched. These unscathed red nuggets givea golden opportunity to study how the galaxies, and the supermassive black hole at their centers, act over billions of years of isolation.<br /><br /><a href="https://www.nasa.gov/mission_pages/chandra/news/chandra-may-have-first-evidence-of-a-young-star-devouring-a-planet.htmleutrinos" rel="noopener">https://www.nasa.gov/mission_pages/chandra/news/chandra-may-have-first-evidence-of-a-young-star-devouring-a-planet.htmleutrinos</a> coming from black holes. <br /><a href="https://www.nasa.gov/mission_pages/chandra/news/red-nuggets-are-galactic-gold-for-astronomers.html" rel="noopener">https://www.nasa.gov/mission_pages/chandra/news/red-nuggets-are-galactic-gold-for-astronomers.html</a>]]></itunes:summary><itunes:duration>3289</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>My Guest India. Neutrinos.. Fermi Observatory.</title><link>https://www.spreaker.com/episode/my-guest-india-neutrinos-fermi-observatory--23524919</link><description><![CDATA[My friend India from Los Angeles joined in for this show. Thanks for your perceptiveness on the topic, and your interesting inputs. Neutrinos have been detected emerging from a monster black hole. This would mark the first clear detection of cosmologically-distant neutrinos and the dawn of an observed association between energetic neutrinos and cosmic rays created by powerful jets emanating from blazing quasars (blazars). Once the Antarctican IceCube detector measured an energetic neutrino in 2017 September, many of humanity's premier observatories sprang into action to try to identify a counterpart in light. And they did. An erupting counterpart was pinpointed by high energy observatories including AGILE, Fermi, HAWC, H.E.S.S., INTEGRAL, MAGIC, NuSTAR, Swift, and VERITAS, which found that gamma-ray blazar TXS 0506+056 was in the right direction and with gamma-rays from a flare arriving nearly coincidental in time with the neutrino. Even though this and other position and time coincidences are statistically strong, astronomers will await other similar neutrino - blazar light associations to be absolutely sure. TESS continues testing before beginning first observations. Transit Exoplanet Survey Satellite TESS has reached its final science orbit, and testing is continuing to optimize TESS' operations. \<br /><br /><a href="https://apod.nasa.gov/apod/ap180716.html" rel="noopener">https://apod.nasa.gov/apod/ap180716.html</a><br /><a href="https://www.nasa.gov/feature/goddard/2018/nasa-s-tess-spacecraft-continues-testing-prior-to-first-observations" rel="noopener">https://www.nasa.gov/feature/goddard/2018/nasa-s-tess-spacecraft-continues-testing-prior-to-first-observations</a>]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-July-12-14-00-00.mp3</guid><pubDate>Thu, 12 Jul 2018 21:01:57 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524919/astrotalk_july_12_14_00_00.mp3" length="55744053" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>My friend India from Los Angeles joined in for this show. Thanks for your perceptiveness on the topic, and your interesting inputs. Neutrinos have been detected emerging from a monster black hole. This would mark the first clear detection of...</itunes:subtitle><itunes:summary><![CDATA[My friend India from Los Angeles joined in for this show. Thanks for your perceptiveness on the topic, and your interesting inputs. Neutrinos have been detected emerging from a monster black hole. This would mark the first clear detection of cosmologically-distant neutrinos and the dawn of an observed association between energetic neutrinos and cosmic rays created by powerful jets emanating from blazing quasars (blazars). Once the Antarctican IceCube detector measured an energetic neutrino in 2017 September, many of humanity's premier observatories sprang into action to try to identify a counterpart in light. And they did. An erupting counterpart was pinpointed by high energy observatories including AGILE, Fermi, HAWC, H.E.S.S., INTEGRAL, MAGIC, NuSTAR, Swift, and VERITAS, which found that gamma-ray blazar TXS 0506+056 was in the right direction and with gamma-rays from a flare arriving nearly coincidental in time with the neutrino. Even though this and other position and time coincidences are statistically strong, astronomers will await other similar neutrino - blazar light associations to be absolutely sure. TESS continues testing before beginning first observations. Transit Exoplanet Survey Satellite TESS has reached its final science orbit, and testing is continuing to optimize TESS' operations. \<br /><br /><a href="https://apod.nasa.gov/apod/ap180716.html" rel="noopener">https://apod.nasa.gov/apod/ap180716.html</a><br /><a href="https://www.nasa.gov/feature/goddard/2018/nasa-s-tess-spacecraft-continues-testing-prior-to-first-observations" rel="noopener">https://www.nasa.gov/feature/goddard/2018/nasa-s-tess-spacecraft-continues-testing-prior-to-first-observations</a>]]></itunes:summary><itunes:duration>3484</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>A Tiny Asteroid Over Africa. NEOWISE.</title><link>https://www.spreaker.com/episode/a-tiny-asteroid-over-africa-neowise--23524871</link><description><![CDATA[A tiny asteroid named 2018 A (6 feet) disintegrated over Botswana on June 2, 9:44 AM PDT. No damage was reported. NASA's NEOWISE mission is using infrared to characterize 122 asteroids. The imagery will help determine the surface properties of these asteroids. Thermophysical modeling of the asteroids will help scientists better understand the surface properties of these asteroids. Engineers are testing baffles on the James Webb Telescope. The telescope will examine in infrared light, so the baffles are intended to dissipate the heat (that is generated by Webb's electronics) away from the mirrors of the telescope. The gold-plated baffles will direct this heat into space and away from the mirrors. The telescope's mirrors are also gold plated, because gold has a high reflectivity in the infrared spectrum.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-June-07-14-00-00.mp3</guid><pubDate>Thu, 07 Jun 2018 21:02:07 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524871/astrotalk_june_07_14_00_00.mp3" length="56895948" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>A tiny asteroid named 2018 A (6 feet) disintegrated over Botswana on June 2, 9:44 AM PDT. No damage was reported. NASA's NEOWISE mission is using infrared to characterize 122 asteroids. The imagery will help determine the surface properties of these...</itunes:subtitle><itunes:summary><![CDATA[A tiny asteroid named 2018 A (6 feet) disintegrated over Botswana on June 2, 9:44 AM PDT. No damage was reported. NASA's NEOWISE mission is using infrared to characterize 122 asteroids. The imagery will help determine the surface properties of these asteroids. Thermophysical modeling of the asteroids will help scientists better understand the surface properties of these asteroids. Engineers are testing baffles on the James Webb Telescope. The telescope will examine in infrared light, so the baffles are intended to dissipate the heat (that is generated by Webb's electronics) away from the mirrors of the telescope. The gold-plated baffles will direct this heat into space and away from the mirrors. The telescope's mirrors are also gold plated, because gold has a high reflectivity in the infrared spectrum.]]></itunes:summary><itunes:duration>3556</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Relativistic Particles in the Van Allen Radiation Belts. A Distant and Lonely Neutron Star. Ultraviolet Light Survey of Nearby Galaxies.</title><link>https://www.spreaker.com/episode/relativistic-particles-in-the-van-allen-radiation-belts-a-distant-and-lonely-neutron-star-ultraviolet-light-survey-of-nearby-galaxies--23524812</link><description><![CDATA[Intro Einstein and his super large enormous brain, and how he figured out all of these difficult theories. Astronomers have determined why relativistic particles are flying through the Van Allen Radiation Belts. Electromagnetic waves, called chorus waves, speed up particles, just like an adult's hand would when speeding up a child on a swing, by pushing the swing. The chorus waves are thought to continuously push the particles to relativistic speeds. Astronomers would like to know the cause of the acceleration of the particles so they can learn more about the radiation in the Van Allen Belts, something which is hazardous to spacecraft and astronauts which pass through the belts. A lonely neutron star has been found in the Large Magellanic Cloud, about 200,00 light years from us. Images are shown in X-ray, from the Chandra X-Ray Observatory, and visible light from Hubble nd the Very Large Telescope (VLT) in Chile. The debris around the corpse neutron star is rich in oxygen, and scientists are studying E0102 because they want to learn more about how massive stars fuse lighter elements into heavier ones before they explode. Seen up to a few thousand years after the original explosion, oxygen-rich remnants contain the debris ejected from the dead star’s interior. Also, astronomers have released the most completer survey of nearby stars and galaxies. The stars studied are all bigger than the sun, and are from 11 - 58 million light years from us. The galaxies were chosen for study based on their mass, star-formation rate, and abundances of elements that are heavier than hydrogen and helium. The data provide detailed information on young, massive stars and star clusters, and how their environment affects their development.  from among 500 galaxies, compiled in ground-based surveys, located between 11 million and 58 million light-years from Earth. Team members chose the galaxies based on their mass, star-formation rate, and abundances of elements that are heavier than hydrogen and helium. The star cluster catalogs contain about 8,000 young clusters whose ages range from 1 million to roughly 500 million years old. These stellar groupings are as much as 10 times more massive than the largest clusters seen in our Milky Way galaxy. Astronomers hope to form the most complete catalog of star clusters and a  stellar catalog in ultraviolet light. Ultraviolet light is a major tracer of the youngest and hottest star populations, which astronomers need to derive the ages of stars and get a complete stellar history. The synergy of the two catalogs combined offers an unprecedented potential for understanding star formation.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-May-31-14-00-00.mp3</guid><pubDate>Thu, 31 May 2018 21:01:45 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524812/astrotalk_may_31_14_00_00.mp3" length="56544026" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Intro Einstein and his super large enormous brain, and how he figured out all of these difficult theories. Astronomers have determined why relativistic particles are flying through the Van Allen Radiation Belts. Electromagnetic waves, called chorus...</itunes:subtitle><itunes:summary><![CDATA[Intro Einstein and his super large enormous brain, and how he figured out all of these difficult theories. Astronomers have determined why relativistic particles are flying through the Van Allen Radiation Belts. Electromagnetic waves, called chorus waves, speed up particles, just like an adult's hand would when speeding up a child on a swing, by pushing the swing. The chorus waves are thought to continuously push the particles to relativistic speeds. Astronomers would like to know the cause of the acceleration of the particles so they can learn more about the radiation in the Van Allen Belts, something which is hazardous to spacecraft and astronauts which pass through the belts. A lonely neutron star has been found in the Large Magellanic Cloud, about 200,00 light years from us. Images are shown in X-ray, from the Chandra X-Ray Observatory, and visible light from Hubble nd the Very Large Telescope (VLT) in Chile. The debris around the corpse neutron star is rich in oxygen, and scientists are studying E0102 because they want to learn more about how massive stars fuse lighter elements into heavier ones before they explode. Seen up to a few thousand years after the original explosion, oxygen-rich remnants contain the debris ejected from the dead star’s interior. Also, astronomers have released the most completer survey of nearby stars and galaxies. The stars studied are all bigger than the sun, and are from 11 - 58 million light years from us. The galaxies were chosen for study based on their mass, star-formation rate, and abundances of elements that are heavier than hydrogen and helium. The data provide detailed information on young, massive stars and star clusters, and how their environment affects their development.  from among 500 galaxies, compiled in ground-based surveys, located between 11 million and 58 million light-years from Earth. Team members chose the galaxies based on their mass, star-formation rate, and abundances of elements that are heavier than hydrogen and helium. The star cluster catalogs contain about 8,000 young clusters whose ages range from 1 million to roughly 500 million years old. These stellar groupings are as much as 10 times more massive than the largest clusters seen in our Milky Way galaxy. Astronomers hope to form the most complete catalog of star clusters and a  stellar catalog in ultraviolet light. Ultraviolet light is a major tracer of the youngest and hottest star populations, which astronomers need to derive the ages of stars and get a complete stellar history. The synergy of the two catalogs combined offers an unprecedented potential for understanding star formation.]]></itunes:summary><itunes:duration>3534</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Course Corrections for Insight. Black Holes Around Sgr A*.</title><link>https://www.spreaker.com/episode/course-corrections-for-insight-black-holes-around-sgr-a--23524902</link><description><![CDATA[The Insight Spacecraft has to deal with as many 6 course corrections on its way to Mars. NASA has to keep Insight free from contaminants, so this affected the way Insight was launched. The course corrections are therefore necessary to get Insight in the right place at the right time, when it eventually gets to Mars in later October. Scientists are discovering the bounty of solar mass black holes that are thought to exist around our galaxy's central, supermassive black hole, Sgr A* The Chandra X-Ray observatory is doing the necessary snooping, to locate these black holes. NASA's NASA’s Magnetospheric Multiscale spacecraft — MMS, is also discovering fascinating things about the magnetic happenings in Earth's magnetosphere. Magnetic reconnection, a complicated process which takes place in Earth's magnetosphere, has an affect on space weather, and therefore the weather on Earth. MMS is finding out interesting things about magnetic reconnection in near-Earth space.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-May-24-14-00-00.mp3</guid><pubDate>Thu, 24 May 2018 21:01:27 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524902/astrotalk_may_24_14_00_00.mp3" length="58816052" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The Insight Spacecraft has to deal with as many 6 course corrections on its way to Mars. NASA has to keep Insight free from contaminants, so this affected the way Insight was launched. The course corrections are therefore necessary to get Insight in...</itunes:subtitle><itunes:summary><![CDATA[The Insight Spacecraft has to deal with as many 6 course corrections on its way to Mars. NASA has to keep Insight free from contaminants, so this affected the way Insight was launched. The course corrections are therefore necessary to get Insight in the right place at the right time, when it eventually gets to Mars in later October. Scientists are discovering the bounty of solar mass black holes that are thought to exist around our galaxy's central, supermassive black hole, Sgr A* The Chandra X-Ray observatory is doing the necessary snooping, to locate these black holes. NASA's NASA’s Magnetospheric Multiscale spacecraft — MMS, is also discovering fascinating things about the magnetic happenings in Earth's magnetosphere. Magnetic reconnection, a complicated process which takes place in Earth's magnetosphere, has an affect on space weather, and therefore the weather on Earth. MMS is finding out interesting things about magnetic reconnection in near-Earth space.]]></itunes:summary><itunes:duration>3676</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Neutrinos</title><link>https://www.spreaker.com/episode/neutrinos--23524967</link><description><![CDATA[Neutrinos are sometimes called ghost particles because they are difficult to trap, or locate. If your thumb is perpendicular to the sun, then about 65 billion neutrinos are going through your thumb each second. Neutrinos are produced in the heart of the sun, in supernova explosions, in nuclear reactions, and in a few other ways. Neutrinos are almost massless, they carry 1/2 integer spin, and they interact only through the weak force and gravity. It was long of matter of debate for physicists whether neutrinos even had mass, but Canadian physicist Dr. Art MacDonald of the Sudbury Neutrino Observatory received a Nobel prize in physics in 2015 for proving that neutrinos do have mass. Since neutrinos can oscillate between different flavors, or kinds, that was the necessary item needed to prove they have mass. Neutrino physics took off in 1987 when neutrinos from Supernova SN1987A were detected on Earth, just before the light from the SN reached us.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-May-10-14-03-00.mp3</guid><pubDate>Thu, 10 May 2018 21:03:12 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524967/astrotalk_may_10_14_03_00.mp3" length="55376248" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Neutrinos are sometimes called ghost particles because they are difficult to trap, or locate. If your thumb is perpendicular to the sun, then about 65 billion neutrinos are going through your thumb each second. Neutrinos are produced in the heart of...</itunes:subtitle><itunes:summary><![CDATA[Neutrinos are sometimes called ghost particles because they are difficult to trap, or locate. If your thumb is perpendicular to the sun, then about 65 billion neutrinos are going through your thumb each second. Neutrinos are produced in the heart of the sun, in supernova explosions, in nuclear reactions, and in a few other ways. Neutrinos are almost massless, they carry 1/2 integer spin, and they interact only through the weak force and gravity. It was long of matter of debate for physicists whether neutrinos even had mass, but Canadian physicist Dr. Art MacDonald of the Sudbury Neutrino Observatory received a Nobel prize in physics in 2015 for proving that neutrinos do have mass. Since neutrinos can oscillate between different flavors, or kinds, that was the necessary item needed to prove they have mass. Neutrino physics took off in 1987 when neutrinos from Supernova SN1987A were detected on Earth, just before the light from the SN reached us.]]></itunes:summary><itunes:duration>3462</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Intro to Wormholes. A Stellar Thief, or Survivor to a Supernova Explosion.</title><link>https://www.spreaker.com/episode/intro-to-wormholes-a-stellar-thief-or-survivor-to-a-supernova-explosion--23524972</link><description><![CDATA[Intro to Wormholes. A supernova, 2001ig, in galaxy NGC 7424, 40 million light years away, has been spotted with a surviving companion star. This proves that some supernovas originate in double-star systems. The  majority of massive stars are in binary pairs, and many of these binary pairs will interact and transfer gas from one star to the other when their orbits bring them close together. The companion siphoned off almost all of the hydrogen from the doomed star’s stellar envelope, the region that transports energy from the star’s core to its atmosphere. Millions of years before the primary star went supernova, the companion’s thievery created an instability in the primary star, causing it to episodically blow off a cocoon and shells of hydrogen gas before the catastrophe. How stripped-envelope supernovas lose that outer envelope is not entirely clear. They were originally thought to come from single stars with very fast winds that pushed off the outer envelopes. The problem was that when astronomers started looking for the primary stars from which supernovas were spawned, they couldn’t find them for many stripped-envelope supernovas. Now they have. Astronomers hope to use the James Webb Space Telescope in the future to study this pair in more detail. A brief discussion of multi-star systems. Details are published in the March 2018 issue of Astrophysical Journal. Thanks for visiting Giorgio.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-April-26-14-00-00.mp3</guid><pubDate>Thu, 26 Apr 2018 21:01:34 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524972/astrotalk_april_26_14_00_00.mp3" length="55744053" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Intro to Wormholes. A supernova, 2001ig, in galaxy NGC 7424, 40 million light years away, has been spotted with a surviving companion star. This proves that some supernovas originate in double-star systems. The  majority of massive stars are in binary...</itunes:subtitle><itunes:summary><![CDATA[Intro to Wormholes. A supernova, 2001ig, in galaxy NGC 7424, 40 million light years away, has been spotted with a surviving companion star. This proves that some supernovas originate in double-star systems. The  majority of massive stars are in binary pairs, and many of these binary pairs will interact and transfer gas from one star to the other when their orbits bring them close together. The companion siphoned off almost all of the hydrogen from the doomed star’s stellar envelope, the region that transports energy from the star’s core to its atmosphere. Millions of years before the primary star went supernova, the companion’s thievery created an instability in the primary star, causing it to episodically blow off a cocoon and shells of hydrogen gas before the catastrophe. How stripped-envelope supernovas lose that outer envelope is not entirely clear. They were originally thought to come from single stars with very fast winds that pushed off the outer envelopes. The problem was that when astronomers started looking for the primary stars from which supernovas were spawned, they couldn’t find them for many stripped-envelope supernovas. Now they have. Astronomers hope to use the James Webb Space Telescope in the future to study this pair in more detail. A brief discussion of multi-star systems. Details are published in the March 2018 issue of Astrophysical Journal. Thanks for visiting Giorgio.]]></itunes:summary><itunes:duration>3484</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Tsugunska Sized Asteroid, 2018CGE,  Just Misses Earth. Wormholes, Wormholes, Wormholes.</title><link>https://www.spreaker.com/episode/tsugunska-sized-asteroid-2018cge-just-misses-earth-wormholes-wormholes-wormholes--23524877</link><description><![CDATA[An asteroid similar in size to one that exploded more than 100 years ago in Russia's Tunguska region in Siberia gave Earth a close shave on Sunday (April 15), just one day after astronomers discovered the object. The asteroid, 2018 GE3, made its closest approach to Earth at around 2:41 a.m. EDT , whizzing by at a distance of 119,400 miles (192,000 kilometers), or about half the average distance between Earth and the moon, according to NASA's Center for Near Earth Object Studies (CNEOS). The asteroid, discovered just 1 day before it whizzed past Earth, is .6 times the size of the asteroid that leveled 500,000 acres (2,000 square kilometers) of Siberian forest over Tunguska in 1908. 2018 GE3 is 3 times bigger than the asteroid that caused a lot of damage when it broke up 58 miles from  Chelyabinsk, Russia, in 2013. It could have caused a lot of regional damage if it hit Earth. Another asteroid also just nicked Earth in April. Now, lets talk about wormholes. Talking about wormholes seemed to be more in vogue a few decades ago. Wormholes are theoretical constructs, or bridges, that could potentially connect different parts of the universe, so that astronauts or space travelers could theoretically travel very vast distances in a very, very short amount of time. In fact, it would allow faster than light speed travel. Some theorists believe that some type of special exotic matter, is necessary in order to prop open the mouth of the wormhole. Travelers could then theoretically travel through the bridge or portal that the wormholes create, or other distance parts of the universe, or to other universes. A wormhole, by the way, represents one solution to Einstein's equations of General Relativity. Some scientists actually believe that wormholes in our Milky Way are casting shadows that could be spotted. The shadows would be tiny, so scientists are using the Event Horizon Telescope to detect these shadows. Wormholes are thought to cast bigger shadows than black holes. The shadows would also be more distorted for wormholes. wormholes.  (Hmmm, heady stuff). The detection of these wormholes could provide an alternative explanation to gravity.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-April-19-14-00-00.mp3</guid><pubDate>Thu, 19 Apr 2018 21:02:14 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524877/astrotalk_april_19_14_00_00.mp3" length="54752235" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>An asteroid similar in size to one that exploded more than 100 years ago in Russia's Tunguska region in Siberia gave Earth a close shave on Sunday (April 15), just one day after astronomers discovered the object. The asteroid, 2018 GE3, made its...</itunes:subtitle><itunes:summary><![CDATA[An asteroid similar in size to one that exploded more than 100 years ago in Russia's Tunguska region in Siberia gave Earth a close shave on Sunday (April 15), just one day after astronomers discovered the object. The asteroid, 2018 GE3, made its closest approach to Earth at around 2:41 a.m. EDT , whizzing by at a distance of 119,400 miles (192,000 kilometers), or about half the average distance between Earth and the moon, according to NASA's Center for Near Earth Object Studies (CNEOS). The asteroid, discovered just 1 day before it whizzed past Earth, is .6 times the size of the asteroid that leveled 500,000 acres (2,000 square kilometers) of Siberian forest over Tunguska in 1908. 2018 GE3 is 3 times bigger than the asteroid that caused a lot of damage when it broke up 58 miles from  Chelyabinsk, Russia, in 2013. It could have caused a lot of regional damage if it hit Earth. Another asteroid also just nicked Earth in April. Now, lets talk about wormholes. Talking about wormholes seemed to be more in vogue a few decades ago. Wormholes are theoretical constructs, or bridges, that could potentially connect different parts of the universe, so that astronauts or space travelers could theoretically travel very vast distances in a very, very short amount of time. In fact, it would allow faster than light speed travel. Some theorists believe that some type of special exotic matter, is necessary in order to prop open the mouth of the wormhole. Travelers could then theoretically travel through the bridge or portal that the wormholes create, or other distance parts of the universe, or to other universes. A wormhole, by the way, represents one solution to Einstein's equations of General Relativity. Some scientists actually believe that wormholes in our Milky Way are casting shadows that could be spotted. The shadows would be tiny, so scientists are using the Event Horizon Telescope to detect these shadows. Wormholes are thought to cast bigger shadows than black holes. The shadows would also be more distorted for wormholes. wormholes.  (Hmmm, heady stuff). The detection of these wormholes could provide an alternative explanation to gravity.]]></itunes:summary><itunes:duration>3423</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Dark Stars in the Early Universe. Planet Hunter TESS. Opportunity Rover 5,000.</title><link>https://www.spreaker.com/episode/dark-stars-in-the-early-universe-planet-hunter-tess-opportunity-rover-5-000--23524882</link><description><![CDATA[Types of dark stars could have existed in the early universe that contained a high concentration of neutrolino dark matter. These dark stars had a say on how stars would later form in the later universe. A little talk about gravity assists and NASA's gravity assist podcasts. TESS NASA's planet hunter has been launched. TESS stands for Transiting Exoplanet Survey Satellite and it will hunt for exoplanets by surveying the sky in a new way. TESS will divide the sky into 26 sections each 24 degrees by 96 degrees across. TESS's cameras will look at each sector for 27 days. TESS will study stars that are 30 - 100 times brighter than the stars that were studied by the Kepler Space telescope and  cover a sky area 400 times larger than that monitored by Kepler.. Opportunity rover recently celebrated its 5,000 sol on Mars. A sol is a Martian day, and Opportunity was only built to last for about 90 days. Opportunity is now studying stripes in the  Perseverance Valley. PV also holds rocks that were affected by Mars' winds. Opportunity is studying this valley for ancient signs of life on Mars.<br /><br />The powerful cameras on the spacecraft will stare at each sector for at least 27 days, looking at the brightest stars at a two-minute cadence. From Earth, the Moon occupies half a degree, which is less than 1/9,000th the size of the TESS tiles.The stars TESS will study are 30 to 100 times brighter than those the Kepler mission]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-April-12-14-00-00.mp3</guid><pubDate>Thu, 12 Apr 2018 21:08:12 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524882/astrotalk_april_12_14_00_00.mp3" length="50336079" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Types of dark stars could have existed in the early universe that contained a high concentration of neutrolino dark matter. These dark stars had a say on how stars would later form in the later universe. A little talk about gravity assists and NASA's...</itunes:subtitle><itunes:summary><![CDATA[Types of dark stars could have existed in the early universe that contained a high concentration of neutrolino dark matter. These dark stars had a say on how stars would later form in the later universe. A little talk about gravity assists and NASA's gravity assist podcasts. TESS NASA's planet hunter has been launched. TESS stands for Transiting Exoplanet Survey Satellite and it will hunt for exoplanets by surveying the sky in a new way. TESS will divide the sky into 26 sections each 24 degrees by 96 degrees across. TESS's cameras will look at each sector for 27 days. TESS will study stars that are 30 - 100 times brighter than the stars that were studied by the Kepler Space telescope and  cover a sky area 400 times larger than that monitored by Kepler.. Opportunity rover recently celebrated its 5,000 sol on Mars. A sol is a Martian day, and Opportunity was only built to last for about 90 days. Opportunity is now studying stripes in the  Perseverance Valley. PV also holds rocks that were affected by Mars' winds. Opportunity is studying this valley for ancient signs of life on Mars.<br /><br />The powerful cameras on the spacecraft will stare at each sector for at least 27 days, looking at the brightest stars at a two-minute cadence. From Earth, the Moon occupies half a degree, which is less than 1/9,000th the size of the TESS tiles.The stars TESS will study are 30 to 100 times brighter than those the Kepler mission]]></itunes:summary><itunes:duration>3146</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Vast Black Hole Swarm and A Galaxy With NO Dark Matter</title><link>https://www.spreaker.com/episode/vast-black-hole-swarm-and-a-galaxy-with-no-dark-matter--23524816</link><description><![CDATA[Chuck Hailey from Columbia University is searching for a vast swarm of black holes, called a DENSITY CUSP, that he believes should exist around the central supermassive black hole in our Milky Way, Sagittarius A* (Sag A*). Trouble is, he cannot find this swath, or DENSITY CUSP. Hailey theorizes that in a 6 light year diameter around Sag A*, there should be 10,000 - 20,000 solar mass black holes floating around. Currently, though, only 5 dozen (~60) solar mass black holes are know to exist in our galaxy, and that's with a Milky Way diameter of 100,000 light years. It is difficult to spot black holes, and till now, there presence has only been inferred by indirect methods. Hailey is now looking for less-energetic sources of X-ray emissions around Sag A*, to locate these so-called missing solar mass black holes. Black holes are difficult to find, and since Sag A* is  26,000 light years from Earth, this makes them all the more difficult to locate. In the next story, astronomers from the University of Toronto, and Yale University, have found a galaxy which they believe contains very little, or no, dark matter. The galaxy is known as NGC 1052-DF2. Dark matter is the stuff which builds galaxies. Its gravity pulls all the mass of stars together to form the galaxy. An analogy: its like having a cup of coffee, but without the cup. If someone were to pour coffee onto a table, then the coffee would spill everywhere; on the table, on the floor, on the books. There would be nothing to hold the coffee together, and the results would just be pools of coffee splattered everywhere. Astronomers therefore are puzzled that NGC 105-DF2 is holding itself together, because there is very little, or next to no, Dark Matter in this galaxy. The weight of the galaxy is 1/400 of the weight that astronomers believe it should have, so it seems that the dark matter is missing from this galaxy. Dark matter and dark energy cannot be seen, and it is believed that 95% of our universe is either dark matter or dark energy. The normal matter that we can see only makes up 5 % of our universe. So astronomers are wondering how this galaxy could have formed, and how it could still be held together, without any dark matter there to do the holding. Its like coffee without the cup. But the galaxy is still somehow holding itself together, even though it is a diffuse galaxy. In fact, astronomers can see right through the galaxy, to the background stars and galaxies behind NGC 1052-DF2. It has tagged as being a "FLUFFY GALAXY", or a "UDG", and Ultra Diffuse Galaxy. Researchers are looking for others galaxies like NGC 1052-DF2 to try to explain how this peculiar galaxy came to form, or how it is holding itself together, without dark matter. Its like coffee without a cup, or a skyscraper without its supports, or the human body without its skeleton.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-April-05-14-04-32.mp3</guid><pubDate>Thu, 05 Apr 2018 21:04:32 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524816/astrotalk_april_05_14_04_32.mp3" length="55263817" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Chuck Hailey from Columbia University is searching for a vast swarm of black holes, called a DENSITY CUSP, that he believes should exist around the central supermassive black hole in our Milky Way, Sagittarius A* (Sag A*). Trouble is, he cannot find...</itunes:subtitle><itunes:summary><![CDATA[Chuck Hailey from Columbia University is searching for a vast swarm of black holes, called a DENSITY CUSP, that he believes should exist around the central supermassive black hole in our Milky Way, Sagittarius A* (Sag A*). Trouble is, he cannot find this swath, or DENSITY CUSP. Hailey theorizes that in a 6 light year diameter around Sag A*, there should be 10,000 - 20,000 solar mass black holes floating around. Currently, though, only 5 dozen (~60) solar mass black holes are know to exist in our galaxy, and that's with a Milky Way diameter of 100,000 light years. It is difficult to spot black holes, and till now, there presence has only been inferred by indirect methods. Hailey is now looking for less-energetic sources of X-ray emissions around Sag A*, to locate these so-called missing solar mass black holes. Black holes are difficult to find, and since Sag A* is  26,000 light years from Earth, this makes them all the more difficult to locate. In the next story, astronomers from the University of Toronto, and Yale University, have found a galaxy which they believe contains very little, or no, dark matter. The galaxy is known as NGC 1052-DF2. Dark matter is the stuff which builds galaxies. Its gravity pulls all the mass of stars together to form the galaxy. An analogy: its like having a cup of coffee, but without the cup. If someone were to pour coffee onto a table, then the coffee would spill everywhere; on the table, on the floor, on the books. There would be nothing to hold the coffee together, and the results would just be pools of coffee splattered everywhere. Astronomers therefore are puzzled that NGC 105-DF2 is holding itself together, because there is very little, or next to no, Dark Matter in this galaxy. The weight of the galaxy is 1/400 of the weight that astronomers believe it should have, so it seems that the dark matter is missing from this galaxy. Dark matter and dark energy cannot be seen, and it is believed that 95% of our universe is either dark matter or dark energy. The normal matter that we can see only makes up 5 % of our universe. So astronomers are wondering how this galaxy could have formed, and how it could still be held together, without any dark matter there to do the holding. Its like coffee without the cup. But the galaxy is still somehow holding itself together, even though it is a diffuse galaxy. In fact, astronomers can see right through the galaxy, to the background stars and galaxies behind NGC 1052-DF2. It has tagged as being a "FLUFFY GALAXY", or a "UDG", and Ultra Diffuse Galaxy. Researchers are looking for others galaxies like NGC 1052-DF2 to try to explain how this peculiar galaxy came to form, or how it is holding itself together, without dark matter. Its like coffee without a cup, or a skyscraper without its supports, or the human body without its skeleton.]]></itunes:summary><itunes:duration>3454</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Peggy Whitson's Space Record. Twins in Space (Or one of the Twins).</title><link>https://www.spreaker.com/episode/peggy-whitson-s-space-record-twins-in-space-or-one-of-the-twins--23524891</link><description><![CDATA[Peggy Whitson has just come back from n space. The astronaut has set a record for the length of a spacewalk, and the longest duration in space for any US astronaut, at 665 days. Mark and Scott Kelly are now re-united. Scott Kelly spent 1 year in space, while his twin brother, Mark, stayed on Earth. During this time, any potential changes in Scott's genes, or gene expression, was measured. Telomeres and Telomerase of genes were focused on. It is understood that when looked at over many years, telomeres decrease in length as a person ages. Interestingly, on a time scale of just one year, Bailey found Scott’s telomeres on the ends of chromosomes in his white blood cells increased in length while in space. This could be linked to increased exercise and reduced caloric intake during the mission. However, upon his return to Earth they began to shorten again. There was also a decrease in Scott's bone formation during his last 6 months in space.  In the DNA within Scott’s white blood cells, he found that the level of methylation, or chemical modifications to DNA, decreased while inflight – including a gene regulating telomeres, but returned to normal upon return. On the ground, Mark’s level of methylation in the DNA derived from his white blood cells increased at the midpoint of the study but returned to normal in the end. Variability was observed in the methylation patterns from both twins; however, this epigenetic noise was slightly higher in Scott during spaceflight and then returned to baseline levels after return to Earth. These results could indicate genes that are more sensitive to a changing environment whether on Earth or in space. Other long term changes will appear in upcoming articles. <br />James Webb Space Telescope's launch has been delayed again, until may 2020.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-March-29-14-00-00.mp3</guid><pubDate>Thu, 29 Mar 2018 21:11:57 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524891/astrotalk_march_29_14_00_00.mp3" length="46064117" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Peggy Whitson has just come back from n space. The astronaut has set a record for the length of a spacewalk, and the longest duration in space for any US astronaut, at 665 days. Mark and Scott Kelly are now re-united. Scott Kelly spent 1 year in...</itunes:subtitle><itunes:summary><![CDATA[Peggy Whitson has just come back from n space. The astronaut has set a record for the length of a spacewalk, and the longest duration in space for any US astronaut, at 665 days. Mark and Scott Kelly are now re-united. Scott Kelly spent 1 year in space, while his twin brother, Mark, stayed on Earth. During this time, any potential changes in Scott's genes, or gene expression, was measured. Telomeres and Telomerase of genes were focused on. It is understood that when looked at over many years, telomeres decrease in length as a person ages. Interestingly, on a time scale of just one year, Bailey found Scott’s telomeres on the ends of chromosomes in his white blood cells increased in length while in space. This could be linked to increased exercise and reduced caloric intake during the mission. However, upon his return to Earth they began to shorten again. There was also a decrease in Scott's bone formation during his last 6 months in space.  In the DNA within Scott’s white blood cells, he found that the level of methylation, or chemical modifications to DNA, decreased while inflight – including a gene regulating telomeres, but returned to normal upon return. On the ground, Mark’s level of methylation in the DNA derived from his white blood cells increased at the midpoint of the study but returned to normal in the end. Variability was observed in the methylation patterns from both twins; however, this epigenetic noise was slightly higher in Scott during spaceflight and then returned to baseline levels after return to Earth. These results could indicate genes that are more sensitive to a changing environment whether on Earth or in space. Other long term changes will appear in upcoming articles. <br />James Webb Space Telescope's launch has been delayed again, until may 2020.]]></itunes:summary><itunes:duration>2880</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Star Grazes Our Solar System 70,000 years Ago, Lithium in Comes or Asteroids? A Cosmic Tug of War</title><link>https://www.spreaker.com/episode/star-grazes-our-solar-system-70-000-years-ago-lithium-in-comes-or-asteroids-a-cosmic-tug-of-war--23524895</link><description><![CDATA[Lithium is becoming a hot commodity on Earth. In less than 100 years, so will every other metal. The solution to this coming mineral crunch? Mine minerals on comets or asteroids, or mine the moon. We will have to soon go out in our solar system to survive. Top 10 Star Mysteries. A tug of war is also going on between 2 dwarf galaxies that orbit our Milky Way. the Large Magellanic Cloud, and the Small Magellanic Cloud, are waging a pulling match. Scientists have determined the Large Cloud is pulling material off the small cloud. The stream of gas, known as the Leading Arm, is then feeding its way into the Milky Way, and making i9ts way across our galaxy. This gas will, in the future, most likely feed star birth in the Milky Way, when new stars are being born. Now, let's talk about TESS. What is TESS? TESS stands for, Transiting Exoplanet Survey Satellite. TESS is scheduled to launch April 16, and when in orbit, it will search out for the existence of exo-planets. The James Webb Telescope will then analyze the atmospheres and compositions of these exoplanets.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-March-22-14-04-43.mp3</guid><pubDate>Thu, 22 Mar 2018 21:04:43 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524895/astrotalk_march_22_14_04_43.mp3" length="53087921" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Lithium is becoming a hot commodity on Earth. In less than 100 years, so will every other metal. The solution to this coming mineral crunch? Mine minerals on comets or asteroids, or mine the moon. We will have to soon go out in our solar system to...</itunes:subtitle><itunes:summary><![CDATA[Lithium is becoming a hot commodity on Earth. In less than 100 years, so will every other metal. The solution to this coming mineral crunch? Mine minerals on comets or asteroids, or mine the moon. We will have to soon go out in our solar system to survive. Top 10 Star Mysteries. A tug of war is also going on between 2 dwarf galaxies that orbit our Milky Way. the Large Magellanic Cloud, and the Small Magellanic Cloud, are waging a pulling match. Scientists have determined the Large Cloud is pulling material off the small cloud. The stream of gas, known as the Leading Arm, is then feeding its way into the Milky Way, and making i9ts way across our galaxy. This gas will, in the future, most likely feed star birth in the Milky Way, when new stars are being born. Now, let's talk about TESS. What is TESS? TESS stands for, Transiting Exoplanet Survey Satellite. TESS is scheduled to launch April 16, and when in orbit, it will search out for the existence of exo-planets. The James Webb Telescope will then analyze the atmospheres and compositions of these exoplanets.]]></itunes:summary><itunes:duration>3318</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>500th Sol</title><link>https://www.spreaker.com/episode/500th-sol--23524876</link><description><![CDATA[The Mars Solar powered Opportunity Rover has just finished its 5000th sol on Mars. A "SOL" is a Martian day, and it is 2 hours longer than an Earth day. A Martian year is also 2 Earth years. The Rover is explo9ring the rim of the Endeavour Crater, an area known as the Perseverance Valley. Scientists have noted a series of stripes on the rocks there, and are unsure as what the origins of the stripes are. On its 5000th Martian sunrise, Opportunity will see the Sun rise over the basin's eastern rim, about 14 miles (22 kilometers) away. Perseverance Valley is a shallow channel incised from the rim's crest of the crater's floor. Opportunity has returned about 225,000 images, and they are available to the public. NASA is also set to launch the TESS Sattelite from Cape Canaveral Florida, after February 38, 2018. TESS is an exoplanet hunter. TESS will monitor the entire sky, and the 200,00 closest stars to Earth. TESS works by monitoring the dip in the light intensity when an exoplanet transits in front of its host star. TESS will work in colloboration with the upcoming James Webb Telescope, in an attempt to examine the atmospheres of, and to search for life on newly discovered exoplanets.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-February-19-16-00-00.mp3</guid><pubDate>Mon, 19 Feb 2018 23:00:02 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524876/astrotalk_february_19_16_00_00.mp3" length="52799947" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The Mars Solar powered Opportunity Rover has just finished its 5000th sol on Mars. A "SOL" is a Martian day, and it is 2 hours longer than an Earth day. A Martian year is also 2 Earth years. The Rover is explo9ring the rim of the Endeavour Crater, an...</itunes:subtitle><itunes:summary><![CDATA[The Mars Solar powered Opportunity Rover has just finished its 5000th sol on Mars. A "SOL" is a Martian day, and it is 2 hours longer than an Earth day. A Martian year is also 2 Earth years. The Rover is explo9ring the rim of the Endeavour Crater, an area known as the Perseverance Valley. Scientists have noted a series of stripes on the rocks there, and are unsure as what the origins of the stripes are. On its 5000th Martian sunrise, Opportunity will see the Sun rise over the basin's eastern rim, about 14 miles (22 kilometers) away. Perseverance Valley is a shallow channel incised from the rim's crest of the crater's floor. Opportunity has returned about 225,000 images, and they are available to the public. NASA is also set to launch the TESS Sattelite from Cape Canaveral Florida, after February 38, 2018. TESS is an exoplanet hunter. TESS will monitor the entire sky, and the 200,00 closest stars to Earth. TESS works by monitoring the dip in the light intensity when an exoplanet transits in front of its host star. TESS will work in colloboration with the upcoming James Webb Telescope, in an attempt to examine the atmospheres of, and to search for life on newly discovered exoplanets.]]></itunes:summary><itunes:duration>3300</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Annie Jump Cannon, Henrietta Swan Leavitt</title><link>https://www.spreaker.com/episode/annie-jump-cannon-henrietta-swan-leavitt--23524975</link><description><![CDATA[Early women astronomers, like Annie Jump Cannon and Henrietta Swan Leavitt, made extraordinary contributions to Astronomy, even though as women, they were not permitted to operate telescopes in the great observatories. Prior to the mass use of computers in astrono0my, and in the world at large, NASA required a whole host of calculations to be carried out: trouble was, before the 1960s, computers, or even efficient computers, did not exist. Groups of women, called human calculators, were tasked with doing the vital calculation work that NASA needed on things like trajectories for their rockets. One of these women, Henrietta Swan Leavitt, calculated a whole lot more. Her supervisor, Edward Charles Pickering, tasked her with studying the luminous stars whose luminosity varies over time. Pickering never expected Henrietta Leavitt to come up with any new discoveries, but she did just that. She calculated the period-luminosity relationship for Cepheid Variable stars. Edwin Hubble could not have made his fantastic discoveries without this relationship. Hubble claimed that Leavitt deserved the Nobel Prize in Physics for her work. Gösta Mittag-Leffler of the Swedish Academy of Sciences tried to nominate Leavitt for the Nobel Prize in 1924, but unfortunately she had passed away 3 years earlier. Ms. Leavitt did much groundbreaking work in the field of Astronomy. Annie Jump Cannon was also a noted, early, female Astronomer. She is largely credited with establishing the first star classification system. Cannon, as with Leavitt, was lauded and acknowledged for her work many, many times. She received 2 honorary doctorates, and had many honors bestowed upon her. Henrietta Swan Leavitt and Annie Jump Cannon were 2 women that made amazing contributions to the field of Astronomy. They did so at times when women were underrepresented, and also were not whole-heartedly accepted, in the field of Astronomy.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-February-12-16-01-46.mp3</guid><pubDate>Tue, 13 Feb 2018 00:01:46 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524975/astrotalk_february_12_16_01_46.mp3" length="53472026" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Early women astronomers, like Annie Jump Cannon and Henrietta Swan Leavitt, made extraordinary contributions to Astronomy, even though as women, they were not permitted to operate telescopes in the great observatories. Prior to the mass use of...</itunes:subtitle><itunes:summary><![CDATA[Early women astronomers, like Annie Jump Cannon and Henrietta Swan Leavitt, made extraordinary contributions to Astronomy, even though as women, they were not permitted to operate telescopes in the great observatories. Prior to the mass use of computers in astrono0my, and in the world at large, NASA required a whole host of calculations to be carried out: trouble was, before the 1960s, computers, or even efficient computers, did not exist. Groups of women, called human calculators, were tasked with doing the vital calculation work that NASA needed on things like trajectories for their rockets. One of these women, Henrietta Swan Leavitt, calculated a whole lot more. Her supervisor, Edward Charles Pickering, tasked her with studying the luminous stars whose luminosity varies over time. Pickering never expected Henrietta Leavitt to come up with any new discoveries, but she did just that. She calculated the period-luminosity relationship for Cepheid Variable stars. Edwin Hubble could not have made his fantastic discoveries without this relationship. Hubble claimed that Leavitt deserved the Nobel Prize in Physics for her work. Gösta Mittag-Leffler of the Swedish Academy of Sciences tried to nominate Leavitt for the Nobel Prize in 1924, but unfortunately she had passed away 3 years earlier. Ms. Leavitt did much groundbreaking work in the field of Astronomy. Annie Jump Cannon was also a noted, early, female Astronomer. She is largely credited with establishing the first star classification system. Cannon, as with Leavitt, was lauded and acknowledged for her work many, many times. She received 2 honorary doctorates, and had many honors bestowed upon her. Henrietta Swan Leavitt and Annie Jump Cannon were 2 women that made amazing contributions to the field of Astronomy. They did so at times when women were underrepresented, and also were not whole-heartedly accepted, in the field of Astronomy.]]></itunes:summary><itunes:duration>3342</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Van Allen 60 Year Anniversary, the Penguin and The Egg, Hubble and a Giant Spiral, and 3oo Million Billion Suns</title><link>https://www.spreaker.com/episode/van-allen-60-year-anniversary-the-penguin-and-the-egg-hubble-and-a-giant-spiral-and-3oo-million-billion-suns--23524884</link><description><![CDATA[NASA is celebrating the 60 year anniversary of the discovery of the Van Allen radiation belts with 3 satellites now in orbit, studying the belts. They are 2012 launch of the twin Van Allen Probes, and the subsequent launch of  THEMIS, and Magnetospheric Multiscale, or MMS, missions, to learn about the belts. It is vital to understand the radiation in the belts, because the radiation from them can affect spacecraft, satellites, and humans, in space. Hubble and the Spitzer Space Telescope are also revealing interesting things. A galaxy merger is being viewed in NGC 2336. One galaxy looks like a penguin, and the other like an egg, so the pair is being called, The Penguin and the Egg. The egg is distorting the other galaxy, making it resemble a penguin. The 2 galaxies are 23 million light-years away. The image of the 2 galaxies is a blend of a visible image from Hubble, and an infrared image from Spitzer. Hubble is also showing us another galaxy, NGC 7331, about 45 million LYs away. A supernova is prominent in the middle area of 7331. SN 2014C is surprising us, because within the last year, it went from a supernova that contained little hydrogen, to one that is now hydrogen-rich. NGC 7331 is similar to the Milky Way in all but one respect: it does not have a central bar, like the Milky Way does. Hubble is also viewing a cartwheel shaped galaxy, the Cartwheel Galaxy, which is 500 million LYs away, toward Pegasus. A smaller galaxy passed right through the Cartwheel, sending a blue colored shockwave out from the center of Cartwheel. Cartwheel is known as a ringed-type galaxy. Finally, Hubble is weighing in on 300 million billion suns. Hubble is viewing ACT-CLJ0102-4915, or EL Gordo, a group of galaxy clusters that weighs more than 300,000,000,000,000,000 suns. El Gordo is actually 2 galaxy clusters that are colliding and merging, at a speed of 1 million kilometers per hour. 2014 measurements show that gas and dust is being is being torn from El Gordo by dark matter. Scientists believe that visible matter and dark matter are colliding in the merger. The normal matter is slowing down, but the dark matter is not.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2018/AstroTalk-February-05-16-03-40.mp3</guid><pubDate>Tue, 06 Feb 2018 00:03:40 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524884/astrotalk_february_05_16_03_40.mp3" length="46816026" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>NASA is celebrating the 60 year anniversary of the discovery of the Van Allen radiation belts with 3 satellites now in orbit, studying the belts. They are 2012 launch of the twin Van Allen Probes, and the subsequent launch of  THEMIS, and...</itunes:subtitle><itunes:summary><![CDATA[NASA is celebrating the 60 year anniversary of the discovery of the Van Allen radiation belts with 3 satellites now in orbit, studying the belts. They are 2012 launch of the twin Van Allen Probes, and the subsequent launch of  THEMIS, and Magnetospheric Multiscale, or MMS, missions, to learn about the belts. It is vital to understand the radiation in the belts, because the radiation from them can affect spacecraft, satellites, and humans, in space. Hubble and the Spitzer Space Telescope are also revealing interesting things. A galaxy merger is being viewed in NGC 2336. One galaxy looks like a penguin, and the other like an egg, so the pair is being called, The Penguin and the Egg. The egg is distorting the other galaxy, making it resemble a penguin. The 2 galaxies are 23 million light-years away. The image of the 2 galaxies is a blend of a visible image from Hubble, and an infrared image from Spitzer. Hubble is also showing us another galaxy, NGC 7331, about 45 million LYs away. A supernova is prominent in the middle area of 7331. SN 2014C is surprising us, because within the last year, it went from a supernova that contained little hydrogen, to one that is now hydrogen-rich. NGC 7331 is similar to the Milky Way in all but one respect: it does not have a central bar, like the Milky Way does. Hubble is also viewing a cartwheel shaped galaxy, the Cartwheel Galaxy, which is 500 million LYs away, toward Pegasus. A smaller galaxy passed right through the Cartwheel, sending a blue colored shockwave out from the center of Cartwheel. Cartwheel is known as a ringed-type galaxy. Finally, Hubble is weighing in on 300 million billion suns. Hubble is viewing ACT-CLJ0102-4915, or EL Gordo, a group of galaxy clusters that weighs more than 300,000,000,000,000,000 suns. El Gordo is actually 2 galaxy clusters that are colliding and merging, at a speed of 1 million kilometers per hour. 2014 measurements show that gas and dust is being is being torn from El Gordo by dark matter. Scientists believe that visible matter and dark matter are colliding in the merger. The normal matter is slowing down, but the dark matter is not.]]></itunes:summary><itunes:duration>2926</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Water and Electronegativity, Superworms? Worms in Space. Orbital Dance of Icy Worlds</title><link>https://www.spreaker.com/episode/water-and-electronegativity-superworms-worms-in-space-orbital-dance-of-icy-worlds--23524870</link><description><![CDATA[<a href="https://www.nasa.gov/audience/foreducators/9-12/features/F_Worms_in_Space.html" rel="noopener">https://www.nasa.gov/audience/foreducators/9-12/features/F_Worms_in_Space.html</a><br /><br />Electronegativity of Water. Worms in Space.  C. elegans (worm) is often used in biomedical research, to help learn more about human development, genetics, aging and disease.  Tests are being done on the worms to understand how their biological processes can be affected in a micro-gravity, or zero gravity environment. Researchers hope to use what they learn about the effect on the worms to hypothesize, or build models, on how spaceflight might affect humans. This knowledge can then hopefully be used to prepare humans for the long flight to Mars. Although the worm's biology is very simple in comparison to the comlex biology of a human, worms and humans share many of the same biological processes. Another advantage of studying the worms is that their lifespan is about  2 -3 weeks, so that s cientists can get a gd ideaa on the affects of microo-gravity on the whole lifetime of a creature. This knowledge can then be applied to humans, in predicting how affects a long spaceflight would have on the human anatomy. All 959 cells of a worm are visible through a microscope, and worms have a nervous system, a brain, muscles and a gut. It exhibits behavior and is capable of rudimentary learning. It produces sperm and eggs, and reproduces, although normally as a hermaphrodite. After reproduction, the worm gradually ages, loses vigor and finally dies. All these characteristics, which are similar to humans, make the worm an ideal candidate for study in space. Info on this experiment can be found at <a href="http://weboflife.nasa.gov/" rel="noopener">http://weboflife.nasa.gov/</a>. <br /><a href="https://www.nasa.gov/press-release/goddard/2017/dance-preserves-oceans" rel="noopener">https://www.nasa.gov/press-release/goddard/2017/dance-preserves-oceans</a>. The mid and far-reaches of our solar system is populated by many icy worlds, both planet and moon. Liquid water may not have a chance to exist here, but, on icy moons like Enceladus, the gravitational tug or pull of its home planet, Saturn, may provide the heat necessary to Enceladus' sub-surface ocean in a liquid state. When talking about TNO's, Trans-Neptunian Objects, well then, water would have an even more difficult probability of being found, especially with typical temperatures of -200 deg C out there. But traces of sub-surface water, crystalline ice, and sub-surface ammonia hydrates have been found on some of these TNOs. The analysis was done by reflecting light onto the surface of these TNOs. Sicentists believe that the water may have come to the surface through a process known as "Cryovolcanism". Many of the moons, or TNOs, are thought to have been formed through collisions. When orbits stabilize and a TNO or moon achieves a stable orbit with its parent, then frictional hearing, or tidal heating, from gravitational interaction, can then create enough heat to allow water or other compounds to exist in this cold environment. Without the frictional heating, then the water could only exist as a form of very hard ice. With water and other compounds, comes the possibility that life could evolve way out yonder in the outer reaches of the Solar System. The tidal heating could also provide the chemical compounds and the heat that is necessary for life to evolve.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-December-07-15-09-55.mp3</guid><pubDate>Thu, 07 Dec 2017 23:09:55 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524870/astrotalk_december_07_15_09_55.mp3" length="18272339" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>https://www.nasa.gov/audience/foreducators/9-12/features/F_Worms_in_Space.html

Electronegativity of Water. Worms in Space.  C. elegans (worm) is often used in biomedical research, to help learn more about human development, genetics, aging and...</itunes:subtitle><itunes:summary><![CDATA[<a href="https://www.nasa.gov/audience/foreducators/9-12/features/F_Worms_in_Space.html" rel="noopener">https://www.nasa.gov/audience/foreducators/9-12/features/F_Worms_in_Space.html</a><br /><br />Electronegativity of Water. Worms in Space.  C. elegans (worm) is often used in biomedical research, to help learn more about human development, genetics, aging and disease.  Tests are being done on the worms to understand how their biological processes can be affected in a micro-gravity, or zero gravity environment. Researchers hope to use what they learn about the effect on the worms to hypothesize, or build models, on how spaceflight might affect humans. This knowledge can then hopefully be used to prepare humans for the long flight to Mars. Although the worm's biology is very simple in comparison to the comlex biology of a human, worms and humans share many of the same biological processes. Another advantage of studying the worms is that their lifespan is about  2 -3 weeks, so that s cientists can get a gd ideaa on the affects of microo-gravity on the whole lifetime of a creature. This knowledge can then be applied to humans, in predicting how affects a long spaceflight would have on the human anatomy. All 959 cells of a worm are visible through a microscope, and worms have a nervous system, a brain, muscles and a gut. It exhibits behavior and is capable of rudimentary learning. It produces sperm and eggs, and reproduces, although normally as a hermaphrodite. After reproduction, the worm gradually ages, loses vigor and finally dies. All these characteristics, which are similar to humans, make the worm an ideal candidate for study in space. Info on this experiment can be found at <a href="http://weboflife.nasa.gov/" rel="noopener">http://weboflife.nasa.gov/</a>. <br /><a href="https://www.nasa.gov/press-release/goddard/2017/dance-preserves-oceans" rel="noopener">https://www.nasa.gov/press-release/goddard/2017/dance-preserves-oceans</a>. The mid and far-reaches of our solar system is populated by many icy worlds, both planet and moon. Liquid water may not have a chance to exist here, but, on icy moons like Enceladus, the gravitational tug or pull of its home planet, Saturn, may provide the heat necessary to Enceladus' sub-surface ocean in a liquid state. When talking about TNO's, Trans-Neptunian Objects, well then, water would have an even more difficult probability of being found, especially with typical temperatures of -200 deg C out there. But traces of sub-surface water, crystalline ice, and sub-surface ammonia hydrates have been found on some of these TNOs. The analysis was done by reflecting light onto the surface of these TNOs. Sicentists believe that the water may have come to the surface through a process known as "Cryovolcanism". Many of the moons, or TNOs, are thought to have been formed through collisions. When orbits stabilize and a TNO or moon achieves a stable orbit with its parent, then frictional hearing, or tidal heating, from gravitational interaction, can then create enough heat to allow water or other compounds to exist in this cold environment. Without the frictional heating, then the water could only exist as a form of very hard ice. With water and other compounds, comes the possibility that life could evolve way out yonder in the outer reaches of the Solar System. The tidal heating could also provide the chemical compounds and the heat that is necessary for life to evolve.]]></itunes:summary><itunes:duration>1143</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Pulsars, Gravitational Waves, Hubble Unravels a Twisted Cosmic Knot</title><link>https://www.spreaker.com/episode/pulsars-gravitational-waves-hubble-unravels-a-twisted-cosmic-knot--23524896</link><description><![CDATA[Review from last show. How pulsars are being used to detect gravitational waves. <br />Hubble Space Telescope (HST) is viewing a galaxy merger. The galaxy NCG 2623, or Arp 243, is 250 million LYs away in the constellation Cancer. The merging galaxy is taking on an odd, irregular shape, and star formation is prominent, as marked by the bright blue glow of parts of the galaxy. When galaxies merge, dust and gas is stirred and becomes turbulent, resulting in increased star formation. Since the separate galaxies were harbouring super-massive black holes before the merger, these black holes will surely merge in the future. In other news, NASA is locating whistling electrons in orbit around Earth, in its Van Allen Belts. Scientists believe fluctuating magnetic and electric fields, are causing the electrons to be lost from Earth's atmosphere. These high energy electrons are known by the term, Whistler Mode Chorus. The electrons chirp in rising tones, much like birds do. The results are in Geophysical Review Letters. 15:00:30    15:29:10<br /><br /><a href="https://www.nasa.gov/image-feature/goddard/2017/hubble-unravels-a-twisted-cosmic-knot" rel="noopener">https://www.nasa.gov/image-feature/goddard/2017/hubble-unravels-a-twisted-cosmic-knot</a>]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-November-23-15-00-00.mp3</guid><pubDate>Thu, 23 Nov 2017 22:00:30 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524896/astrotalk_november_23_15_00_00.mp3" length="27535987" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Review from last show. How pulsars are being used to detect gravitational waves. 
Hubble Space Telescope (HST) is viewing a galaxy merger. The galaxy NCG 2623, or Arp 243, is 250 million LYs away in the constellation Cancer. The merging galaxy is...</itunes:subtitle><itunes:summary><![CDATA[Review from last show. How pulsars are being used to detect gravitational waves. <br />Hubble Space Telescope (HST) is viewing a galaxy merger. The galaxy NCG 2623, or Arp 243, is 250 million LYs away in the constellation Cancer. The merging galaxy is taking on an odd, irregular shape, and star formation is prominent, as marked by the bright blue glow of parts of the galaxy. When galaxies merge, dust and gas is stirred and becomes turbulent, resulting in increased star formation. Since the separate galaxies were harbouring super-massive black holes before the merger, these black holes will surely merge in the future. In other news, NASA is locating whistling electrons in orbit around Earth, in its Van Allen Belts. Scientists believe fluctuating magnetic and electric fields, are causing the electrons to be lost from Earth's atmosphere. These high energy electrons are known by the term, Whistler Mode Chorus. The electrons chirp in rising tones, much like birds do. The results are in Geophysical Review Letters. 15:00:30    15:29:10<br /><br /><a href="https://www.nasa.gov/image-feature/goddard/2017/hubble-unravels-a-twisted-cosmic-knot" rel="noopener">https://www.nasa.gov/image-feature/goddard/2017/hubble-unravels-a-twisted-cosmic-knot</a>]]></itunes:summary><itunes:duration>1721</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Ice Cream and Pizza in Space, Finding Gravitational Waves Using a Pulsar</title><link>https://www.spreaker.com/episode/ice-cream-and-pizza-in-space-finding-gravitational-waves-using-a-pulsar--23524977</link><description><![CDATA[<a href="https://www.jpl.nasa.gov/news/news.php?release=2017-293&rn=news.xml&rst=6998" rel="noopener">https://www.jpl.nasa.gov/news/news.php?release=2017-293&rn=news.xml&rst=6998</a><br /><br />Ice-cream and pizza are being delivered to the International Space Station (ISS). YUM. Venus and Jupiter were aligned and were very close to each other in the morning sky on November 13, 2017. Also, astronomers are using pulsars to track G Waves. Gravitational waves are ripples in space-time. They are created from the collision of black holes or neutron stars, amongst other things. They occur from masses accelerating in space. G waves also result from black holes or neutron stars as they do they dance around each other, before they merge. Most galaxies harbour super-massive black holes at their centers. When 2 galaxies merge (that have super-massive black holes) they produce low-frequency G waves. These G waves from the collision of 2 super massive black holes have not yet been detected. Remember, super massive black holes can have the mass of millions or billions of solar masses. To try to find these kind of G waves, astronomers are using pulsars to help. Pulsars are neutron stars that spin. They spin so fast, that they emit many pulses of radio waves each second. Some pulsars can spin hundreds of times each second. The North American Nanohertz Observatory for Gravitational Waves (NANOGrav), is one group using pulsars to search for G waves. A pulsar, or pulsar timing array, emits radio waves in such a predictable pattern, that if a G wave hits the pulsar, then the distortion in space-time of the G waves can be measured from the distortion, or the offset, of the pulse from the pulsar. Observatories like LIGO detect G waves in the seconds just before 2 black holes or 2 neutron stars merge, but it can take millions of years for 2 BHs or 2 NSs to merge. While they are engaged in this cosmic death dance around each other for millions of years before they merge, G waves are emitted. LIGO cannot detect these types of G waves, but astronomers believe that they can detect these types of G waves. When 2 galaxies merge, their black holes (BHs) will usually merge millions of years later. They will emit G waves while they are doing their death dance around each other, and astronomers believe they can detect the G waves that are emitted in this process.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-November-16-15-05-51.mp3</guid><pubDate>Thu, 16 Nov 2017 22:02:40 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524977/astrotalk_november_16_15_05_51.mp3" length="22095830" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>https://www.jpl.nasa.gov/news/news.php?release=2017-293&amp;rn=news.xml&amp;rst=6998

Ice-cream and pizza are being delivered to the International Space Station (ISS). YUM. Venus and Jupiter were aligned and were very close to each other in the morning sky on...</itunes:subtitle><itunes:summary><![CDATA[<a href="https://www.jpl.nasa.gov/news/news.php?release=2017-293&rn=news.xml&rst=6998" rel="noopener">https://www.jpl.nasa.gov/news/news.php?release=2017-293&rn=news.xml&rst=6998</a><br /><br />Ice-cream and pizza are being delivered to the International Space Station (ISS). YUM. Venus and Jupiter were aligned and were very close to each other in the morning sky on November 13, 2017. Also, astronomers are using pulsars to track G Waves. Gravitational waves are ripples in space-time. They are created from the collision of black holes or neutron stars, amongst other things. They occur from masses accelerating in space. G waves also result from black holes or neutron stars as they do they dance around each other, before they merge. Most galaxies harbour super-massive black holes at their centers. When 2 galaxies merge (that have super-massive black holes) they produce low-frequency G waves. These G waves from the collision of 2 super massive black holes have not yet been detected. Remember, super massive black holes can have the mass of millions or billions of solar masses. To try to find these kind of G waves, astronomers are using pulsars to help. Pulsars are neutron stars that spin. They spin so fast, that they emit many pulses of radio waves each second. Some pulsars can spin hundreds of times each second. The North American Nanohertz Observatory for Gravitational Waves (NANOGrav), is one group using pulsars to search for G waves. A pulsar, or pulsar timing array, emits radio waves in such a predictable pattern, that if a G wave hits the pulsar, then the distortion in space-time of the G waves can be measured from the distortion, or the offset, of the pulse from the pulsar. Observatories like LIGO detect G waves in the seconds just before 2 black holes or 2 neutron stars merge, but it can take millions of years for 2 BHs or 2 NSs to merge. While they are engaged in this cosmic death dance around each other for millions of years before they merge, G waves are emitted. LIGO cannot detect these types of G waves, but astronomers believe that they can detect these types of G waves. When 2 galaxies merge, their black holes (BHs) will usually merge millions of years later. They will emit G waves while they are doing their death dance around each other, and astronomers believe they can detect the G waves that are emitted in this process.]]></itunes:summary><itunes:duration>1381</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Gravitational Lensing, Monitoring Antarctic Penguin Populations, and What Provides Heat for Enceladus' Subsurface Ocean?</title><link>https://www.spreaker.com/episode/gravitational-lensing-monitoring-antarctic-penguin-populations-and-what-provides-heat-for-enceladus-subsurface-ocean--23524915</link><description><![CDATA[Introduction: Talk about Gravitational Lensing. <br />NASA Satellites are monitoring Antarctic Penguin population. Penguins are important ecosystem indicators. Penguins are part of the vast food web in the Antarctic area. Data bases for penguin populations are being updated, so scientists can monitor not only the survival of the penguins, but also the populations of things like krill and polar bears in the Antarctic. A NASA app, MAPPDD, (Mapping Applications for Penguin Populations and Projection Dynamics) allows anyone, including scientists and citizen scientists, to monitor the penguin populations. NASA is accepting proposals on how to best model the penguin population using MAPPDD. Existing datasets for penguin populations are limited and patchy, so NASA hopes that it can help scientists better forecast trends for penguin populations. Penguin scientists have not had much luck in accurately predicting future penguin populations so a competition is now on for citizen scientists to develop a new model, using MAPPPD, to more accurately forecast penguin population dynamics. Do you have it in you to become a penguin detective?<br />Powering Enceladuds' Active Icy Ocean. (Enceladus is a moon of Saturn). Scientists are trying to figure out what power source is providing heat for Enceladus' subsurface ocean. Scientists believe it is possible that the moon's rocky core is responsible for the heating. Simulations show that as Enceladus orbits Saturn, the rocks in the porous core rub together, and thus provides heat that rises up and interacts with the water in Enceladus' subsurface ocean. The scientists cannot explain, though, why the moon's North pole is so different than the South pole. Geyers spewing water are found in the South but not the North.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-November-09-15-02-18.mp3</guid><pubDate>Thu, 09 Nov 2017 23:02:18 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524915/astrotalk_november_09_15_02_18.mp3" length="25839908" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Introduction: Talk about Gravitational Lensing. 
NASA Satellites are monitoring Antarctic Penguin population. Penguins are important ecosystem indicators. Penguins are part of the vast food web in the Antarctic area. Data bases for penguin populations...</itunes:subtitle><itunes:summary><![CDATA[Introduction: Talk about Gravitational Lensing. <br />NASA Satellites are monitoring Antarctic Penguin population. Penguins are important ecosystem indicators. Penguins are part of the vast food web in the Antarctic area. Data bases for penguin populations are being updated, so scientists can monitor not only the survival of the penguins, but also the populations of things like krill and polar bears in the Antarctic. A NASA app, MAPPDD, (Mapping Applications for Penguin Populations and Projection Dynamics) allows anyone, including scientists and citizen scientists, to monitor the penguin populations. NASA is accepting proposals on how to best model the penguin population using MAPPDD. Existing datasets for penguin populations are limited and patchy, so NASA hopes that it can help scientists better forecast trends for penguin populations. Penguin scientists have not had much luck in accurately predicting future penguin populations so a competition is now on for citizen scientists to develop a new model, using MAPPPD, to more accurately forecast penguin population dynamics. Do you have it in you to become a penguin detective?<br />Powering Enceladuds' Active Icy Ocean. (Enceladus is a moon of Saturn). Scientists are trying to figure out what power source is providing heat for Enceladus' subsurface ocean. Scientists believe it is possible that the moon's rocky core is responsible for the heating. Simulations show that as Enceladus orbits Saturn, the rocks in the porous core rub together, and thus provides heat that rises up and interacts with the water in Enceladus' subsurface ocean. The scientists cannot explain, though, why the moon's North pole is so different than the South pole. Geyers spewing water are found in the South but not the North.]]></itunes:summary><itunes:duration>1615</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Water? Gravitational Waves in Neutron Star Collision</title><link>https://www.spreaker.com/episode/water-gravitational-waves-in-neutron-star-collision--23524906</link><description><![CDATA[2 LIGO stations and the Virgo detector detected Gravitational waves, named  GW170817, on August 17 2017 from the collision of 2 neutron stars in NGC 4993. Historically, this was the 5th disturbance or detection of G waves, but in this, the 5th instance, other radiation was detected as well. In the first 4 disturbances, only G waves were detected, because light cannot escape a black hole. But in this collision of 2 neutron stars, radio, light, and other types of waves were detected. Another feature of  the August 17 event was the length of time that it lasted. The first 4 events lasted for at most, just a few mere seconds, but the 5th event lasted for about 100 seconds, at frequencies climbing to 1000s of cycles per seconds. The neutron stars that collided were 1.1 and 1.6 solar masses. NASA's Fermi Gamma Ray Space Telescope also picked up a flood of gamma rays from the collision just seconds after it happened. Other observatories around the Earth detected the electromagnetic radiation just after the event, as well. A number of observatories were therefore able to jump in and monitor the event, in many different wavelengths. A high level of collaboration allowed scientists to pinpoint the location of the event, which was in NGC 4993. Heavy elements were generated in the event.  The 3 big finds in the event were   1. The collision explains the origins of some gamma ray bursts GRB, short bursts <br />                           2. The event revealed the occurence of a kilonova<br />                           3. The event solved the puzzle of elements that are produced in the R Process,<br />                               or Rapid Process. These heavy nuclei were shown to be produced in the<br />                               neutron star collision.<br /><br />The neutron star collision produced some other puzzles as well. The GRBs were relatively faint, and you can listen to the podcast at about 22 minutes to hear why. May the force be with us all as we wait for more G wave events. NGC 4993 is 130 Million light years away, by the way.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-November-02-15-00-00.mp3</guid><pubDate>Thu, 02 Nov 2017 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524906/astrotalk_november_02_15_00_00.mp3" length="28815778" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>2 LIGO stations and the Virgo detector detected Gravitational waves, named  GW170817, on August 17 2017 from the collision of 2 neutron stars in NGC 4993. Historically, this was the 5th disturbance or detection of G waves, but in this, the 5th...</itunes:subtitle><itunes:summary><![CDATA[2 LIGO stations and the Virgo detector detected Gravitational waves, named  GW170817, on August 17 2017 from the collision of 2 neutron stars in NGC 4993. Historically, this was the 5th disturbance or detection of G waves, but in this, the 5th instance, other radiation was detected as well. In the first 4 disturbances, only G waves were detected, because light cannot escape a black hole. But in this collision of 2 neutron stars, radio, light, and other types of waves were detected. Another feature of  the August 17 event was the length of time that it lasted. The first 4 events lasted for at most, just a few mere seconds, but the 5th event lasted for about 100 seconds, at frequencies climbing to 1000s of cycles per seconds. The neutron stars that collided were 1.1 and 1.6 solar masses. NASA's Fermi Gamma Ray Space Telescope also picked up a flood of gamma rays from the collision just seconds after it happened. Other observatories around the Earth detected the electromagnetic radiation just after the event, as well. A number of observatories were therefore able to jump in and monitor the event, in many different wavelengths. A high level of collaboration allowed scientists to pinpoint the location of the event, which was in NGC 4993. Heavy elements were generated in the event.  The 3 big finds in the event were   1. The collision explains the origins of some gamma ray bursts GRB, short bursts <br />                           2. The event revealed the occurence of a kilonova<br />                           3. The event solved the puzzle of elements that are produced in the R Process,<br />                               or Rapid Process. These heavy nuclei were shown to be produced in the<br />                               neutron star collision.<br /><br />The neutron star collision produced some other puzzles as well. The GRBs were relatively faint, and you can listen to the podcast at about 22 minutes to hear why. May the force be with us all as we wait for more G wave events. NGC 4993 is 130 Million light years away, by the way.]]></itunes:summary><itunes:duration>1801</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Water</title><link>https://www.spreaker.com/episode/water--23524880</link><description><![CDATA[All the rage about water. From extrapolation made from the periodic table, H2O, or water, should freeze at lower temperatures. How would this affect the existence of life on Earth if water were to freeze at a much lower temperature? The water molecule has a high polarity, and because of this, water molecules stick together, thus making it harder for water to freeze at lower temperatures. Water is present in different forms in the Solar System, and, as we know, it is essential for life as we know it.  Also, heavy water is present in different percentages in comets and asteroids. The percentage of heavy water on Earth matches the percentage of    XXXXX, so scientists have concluded that the water on Earth comes from     XXXXXX.    3 / 10,000 water molecules on Earth contain heavy water, but in a 1986 flyby of Halley's Comet, the ESA Giotto spacecraft found Halley contained a ratio of 6 / 10,000 heavy water molecules. So comets from the Kuiper Belt were ruled out as providers of Earth's water. From this, scientists concluded that most of Earth's water were delivered by asteroids, billions of years ago, in a period known as the Late Heavy Bombardment.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-October-26-15-09-15.mp3</guid><pubDate>Thu, 26 Oct 2017 22:03:10 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524880/astrotalk_october_26_15_09_15.mp3" length="25487987" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>All the rage about water. From extrapolation made from the periodic table, H2O, or water, should freeze at lower temperatures. How would this affect the existence of life on Earth if water were to freeze at a much lower temperature? The water molecule...</itunes:subtitle><itunes:summary><![CDATA[All the rage about water. From extrapolation made from the periodic table, H2O, or water, should freeze at lower temperatures. How would this affect the existence of life on Earth if water were to freeze at a much lower temperature? The water molecule has a high polarity, and because of this, water molecules stick together, thus making it harder for water to freeze at lower temperatures. Water is present in different forms in the Solar System, and, as we know, it is essential for life as we know it.  Also, heavy water is present in different percentages in comets and asteroids. The percentage of heavy water on Earth matches the percentage of    XXXXX, so scientists have concluded that the water on Earth comes from     XXXXXX.    3 / 10,000 water molecules on Earth contain heavy water, but in a 1986 flyby of Halley's Comet, the ESA Giotto spacecraft found Halley contained a ratio of 6 / 10,000 heavy water molecules. So comets from the Kuiper Belt were ruled out as providers of Earth's water. From this, scientists concluded that most of Earth's water were delivered by asteroids, billions of years ago, in a period known as the Late Heavy Bombardment.]]></itunes:summary><itunes:duration>1593</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Collision of Neutron Stars</title><link>https://www.spreaker.com/episode/collision-of-neutron-stars--23524925</link><description><![CDATA[Light cannot escape a black hole, so when astronomers at LIGO detected the collision of 2 black holes a few years ago, LIGO detected gravitational waves only. But when 2 neutron stars (that were 130 million light years away, in the galaxy NGC 4993)  collided, and their signal was received on Earth on August 17, 2017,  gravitational waves, and a whole array of electromagnetic radiation was detected. Astronomers were able to confirm their theories on many aspects about neutron stars from the collision. The newspaper, the Independent, claims that "  the event has kickstarted a "new chapter in astrophysics" and confirmed theories about the origin of the mysterious neutron stars". Astronomers detected the formation of many precious and heavy metals from the collision. This kilonova, which was apparently 1000s of times stronger than a mere nova, flung out a whole host of knowledge, along with gravitational waves, electromagnetic radiation, gold, plantinum and lanthanides, among a host of other heavy elements. The mass of the colliding neutron stars was 1.4 and 1.6 solar masses. This was the first detection of gravitational waves from anything other than black holes. The neutron stars stretched and warped space-time as they approached each other, and then collided. A burst of short gamma ray bursts, short GRBs, was detected 2 seconds after the detection of the gravitational waves. The event also was detected for 100 seconds, whereas in the collision of black holes, the 4 previous detections lasted at most only 2 seconds. When the event, called GW170817, occurred, dinosaurs roamed the Earth. The findings were published in the journals, Nature, Nature Astronomy, and Physical Review Letters. The collision answered 3 questions about neutron stars: (1) What happens when neutron stars merge   (2) What causes the short duration gamma ray bursts, short GRBs   (3) Where are heavy elements like gold made.    Astronomers feel this is a new chapter in astrophysics. <br />Dr. BS Sathyaprakash from Cardiff University remarked that the 12 hours following the collision of the 2 neutron stars was the most exciting period of his entire scientific life. The collision also helped astronomers more accurately measure the expansion rate of the universe. The explosion will help explain the inner workings of neutron stars, as well as confirming the theories in general relativity.  <br /><br /><a href="http://www.independent.co.uk/news/science/neutron-star-collision-gravitational-waves-gold-metal-precious-ligo-a8003146.html" rel="noopener">http://www.independent.co.uk/news/science/neutron-star-collision-gravitational-waves-gold-metal-precious-ligo-a8003146.html</a>   15:08:33       15:38:38]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-October-19-15-00-00.mp3</guid><pubDate>Thu, 19 Oct 2017 22:08:33 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524925/astrotalk_october_19_15_00_00.mp3" length="28896026" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Light cannot escape a black hole, so when astronomers at LIGO detected the collision of 2 black holes a few years ago, LIGO detected gravitational waves only. But when 2 neutron stars (that were 130 million light years away, in the galaxy NGC 4993)...</itunes:subtitle><itunes:summary><![CDATA[Light cannot escape a black hole, so when astronomers at LIGO detected the collision of 2 black holes a few years ago, LIGO detected gravitational waves only. But when 2 neutron stars (that were 130 million light years away, in the galaxy NGC 4993)  collided, and their signal was received on Earth on August 17, 2017,  gravitational waves, and a whole array of electromagnetic radiation was detected. Astronomers were able to confirm their theories on many aspects about neutron stars from the collision. The newspaper, the Independent, claims that "  the event has kickstarted a "new chapter in astrophysics" and confirmed theories about the origin of the mysterious neutron stars". Astronomers detected the formation of many precious and heavy metals from the collision. This kilonova, which was apparently 1000s of times stronger than a mere nova, flung out a whole host of knowledge, along with gravitational waves, electromagnetic radiation, gold, plantinum and lanthanides, among a host of other heavy elements. The mass of the colliding neutron stars was 1.4 and 1.6 solar masses. This was the first detection of gravitational waves from anything other than black holes. The neutron stars stretched and warped space-time as they approached each other, and then collided. A burst of short gamma ray bursts, short GRBs, was detected 2 seconds after the detection of the gravitational waves. The event also was detected for 100 seconds, whereas in the collision of black holes, the 4 previous detections lasted at most only 2 seconds. When the event, called GW170817, occurred, dinosaurs roamed the Earth. The findings were published in the journals, Nature, Nature Astronomy, and Physical Review Letters. The collision answered 3 questions about neutron stars: (1) What happens when neutron stars merge   (2) What causes the short duration gamma ray bursts, short GRBs   (3) Where are heavy elements like gold made.    Astronomers feel this is a new chapter in astrophysics. <br />Dr. BS Sathyaprakash from Cardiff University remarked that the 12 hours following the collision of the 2 neutron stars was the most exciting period of his entire scientific life. The collision also helped astronomers more accurately measure the expansion rate of the universe. The explosion will help explain the inner workings of neutron stars, as well as confirming the theories in general relativity.  <br /><br /><a href="http://www.independent.co.uk/news/science/neutron-star-collision-gravitational-waves-gold-metal-precious-ligo-a8003146.html" rel="noopener">http://www.independent.co.uk/news/science/neutron-star-collision-gravitational-waves-gold-metal-precious-ligo-a8003146.html</a>   15:08:33       15:38:38]]></itunes:summary><itunes:duration>1806</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Solar Mass, Intermediate and Super-Massive Black Holes.</title><link>https://www.spreaker.com/episode/solar-mass-intermediate-and-super-massive-black-holes--23524990</link><description><![CDATA[Astronomers have spotted a super-massive black hole, 12 Billion light-years from us. The black hole weighs in at about 12 billion solar masses, so astronomers are puzzled how such a super massive black hole could have formed, only 1.3 billion years after the Big Bang. Astronomers have detected many solar mass black holes, and many super-massive black holes (millions or billions times the mass of the Sun), but apparently, very few, if any, intermediate black holes have been detected. How then could super-massive black holes have formed, given that there is a lack of a middle-men, or interrnediate sized black holes, that could have grouped together, or combined, to form the super-massive black holes. <br />In another black hole topic, a super-massive black hole is on the move. This black hole, 160 million times the mass of our Sun, and located 3.9 billion light years away in an elliptical galaxy. is moving. Speculation is that 2 black holes merged to formed this black hole, and the black hole was then kicked out, or was recoiled, by the gravitational waves coming from the collision. Since the amount of kick depends on the spin of the original black holes, properties of the original colliding black holes could be deduced. The strong x-rays emitted from this galaxy was the clue that led scientists to this moving monster. Strong x-ray can indicate that a black hole is growing rapidly. Other optical data led scientists to conclude that the black hole was moving away from the center of its galaxy, and that disturbances in the outer regions of the galaxy were signs of a recent merger of 2 galaxies, to make the present galaxy. The detection of a high rate of star formation was another clue of a recent merger between 2 separate galaxies. The findings are published in the paper, A Potential Recoiling Supermassive Black Hole CXO J101527.2+625911, and can be found on the internet at,<br /><a href="https://arxiv.org/abs/1704.05549" rel="noopener">https://arxiv.org/abs/1704.05549</a>       15:13:05       15:38:18]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-October-12-15-00-00.mp3</guid><pubDate>Thu, 12 Oct 2017 22:13:05 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524990/astrotalk_october_12_15_00_00.mp3" length="24224078" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Astronomers have spotted a super-massive black hole, 12 Billion light-years from us. The black hole weighs in at about 12 billion solar masses, so astronomers are puzzled how such a super massive black hole could have formed, only 1.3 billion years...</itunes:subtitle><itunes:summary><![CDATA[Astronomers have spotted a super-massive black hole, 12 Billion light-years from us. The black hole weighs in at about 12 billion solar masses, so astronomers are puzzled how such a super massive black hole could have formed, only 1.3 billion years after the Big Bang. Astronomers have detected many solar mass black holes, and many super-massive black holes (millions or billions times the mass of the Sun), but apparently, very few, if any, intermediate black holes have been detected. How then could super-massive black holes have formed, given that there is a lack of a middle-men, or interrnediate sized black holes, that could have grouped together, or combined, to form the super-massive black holes. <br />In another black hole topic, a super-massive black hole is on the move. This black hole, 160 million times the mass of our Sun, and located 3.9 billion light years away in an elliptical galaxy. is moving. Speculation is that 2 black holes merged to formed this black hole, and the black hole was then kicked out, or was recoiled, by the gravitational waves coming from the collision. Since the amount of kick depends on the spin of the original black holes, properties of the original colliding black holes could be deduced. The strong x-rays emitted from this galaxy was the clue that led scientists to this moving monster. Strong x-ray can indicate that a black hole is growing rapidly. Other optical data led scientists to conclude that the black hole was moving away from the center of its galaxy, and that disturbances in the outer regions of the galaxy were signs of a recent merger of 2 galaxies, to make the present galaxy. The detection of a high rate of star formation was another clue of a recent merger between 2 separate galaxies. The findings are published in the paper, A Potential Recoiling Supermassive Black Hole CXO J101527.2+625911, and can be found on the internet at,<br /><a href="https://arxiv.org/abs/1704.05549" rel="noopener">https://arxiv.org/abs/1704.05549</a>       15:13:05       15:38:18]]></itunes:summary><itunes:duration>1514</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>NASA’s Webb Telescope to Witness Galactic Infancy</title><link>https://www.spreaker.com/episode/nasa-s-webb-telescope-to-witness-galactic-infancy--23524872</link><description><![CDATA[NASA's James Webb Space Telescope (JWST or JW) (long overdue for its launch, by the way) has a mission to look at the universe's first galaxies and stars. JW will focus on the Hubble Ultra-Deep Field (HUDF) and the Great Observatories Origins Deep Survey (GOODS). HUDF is a photo (photo?) of a tiny patch of sky that contains 10,000 or so galaxies. The galaxy are so faint, and so old, so it is hoped JW will reveal info on the temperature, mass and composition of the galaxies, through spectroscopic studies. Scientists then hope to determine, or to see, how gas was transformed into stars in the first galaxies, and how super-massive black holes in the galaxies formed. MIRI, Webb's mid-infrared instrument, and NIRCam, Webb's near infrared camera, will be the main instruments used. Webb will be able to see objects with 8 times more spatial resolution, and objects that are 250 times fainter, than the Spitzer Space Telescope could see. Webb will also see things in a different spatial band than Hubble did, so Webb will improve on all previous instruments. And Webb will be able to see with twice the spatial resolution, and at 50 times fainter, than Hubble can. The universe is expanding, so light from distant galaxies (that are moving away from us) are red-shifted. The galaxies that are farthest away have their light red-shifted in the infrared and mid-infrared bands. Webb will be ideally suited to image this light. This will make Webb ideal for looking at the early universe. Says Pablo Pérez-González, from tbe Complutense University of Madrid in Spain: “When you build an observatory with unprecedented capabilities, most probably the most interesting results will not be those that you can expect or predict, but those that no one can imagine.” <br /><br /><br />For more information about Webb telescope, visit: <a href="http://www.webb.nasa.gov" rel="noopener">www.webb.nasa.gov</a> or <a href="http://www.nasa.gov/webb" rel="noopener">www.nasa.gov/webb</a><br /><br />For more information about Hubble telescope, visit: <a href="http://www.nasa.gov/hubble" rel="noopener">www.nasa.gov/hubble</a><br /><br />For more information about Spitzer telescope, visit: <a href="http://www.nasa.gov/spitzer" rel="noopener">www.nasa.gov/spitzer</a><br /><br />Article :https://www.nasa.gov/feature/goddard/2017/nasa-s-webb-telescope-to-witness-galactic-infancy]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-October-05-15-12-10.mp3</guid><pubDate>Thu, 05 Oct 2017 22:12:10 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524872/astrotalk_october_05_15_12_10.mp3" length="20431934" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>NASA's James Webb Space Telescope (JWST or JW) (long overdue for its launch, by the way) has a mission to look at the universe's first galaxies and stars. JW will focus on the Hubble Ultra-Deep Field (HUDF) and the Great Observatories Origins Deep...</itunes:subtitle><itunes:summary><![CDATA[NASA's James Webb Space Telescope (JWST or JW) (long overdue for its launch, by the way) has a mission to look at the universe's first galaxies and stars. JW will focus on the Hubble Ultra-Deep Field (HUDF) and the Great Observatories Origins Deep Survey (GOODS). HUDF is a photo (photo?) of a tiny patch of sky that contains 10,000 or so galaxies. The galaxy are so faint, and so old, so it is hoped JW will reveal info on the temperature, mass and composition of the galaxies, through spectroscopic studies. Scientists then hope to determine, or to see, how gas was transformed into stars in the first galaxies, and how super-massive black holes in the galaxies formed. MIRI, Webb's mid-infrared instrument, and NIRCam, Webb's near infrared camera, will be the main instruments used. Webb will be able to see objects with 8 times more spatial resolution, and objects that are 250 times fainter, than the Spitzer Space Telescope could see. Webb will also see things in a different spatial band than Hubble did, so Webb will improve on all previous instruments. And Webb will be able to see with twice the spatial resolution, and at 50 times fainter, than Hubble can. The universe is expanding, so light from distant galaxies (that are moving away from us) are red-shifted. The galaxies that are farthest away have their light red-shifted in the infrared and mid-infrared bands. Webb will be ideally suited to image this light. This will make Webb ideal for looking at the early universe. Says Pablo Pérez-González, from tbe Complutense University of Madrid in Spain: “When you build an observatory with unprecedented capabilities, most probably the most interesting results will not be those that you can expect or predict, but those that no one can imagine.” <br /><br /><br />For more information about Webb telescope, visit: <a href="http://www.webb.nasa.gov" rel="noopener">www.webb.nasa.gov</a> or <a href="http://www.nasa.gov/webb" rel="noopener">www.nasa.gov/webb</a><br /><br />For more information about Hubble telescope, visit: <a href="http://www.nasa.gov/hubble" rel="noopener">www.nasa.gov/hubble</a><br /><br />For more information about Spitzer telescope, visit: <a href="http://www.nasa.gov/spitzer" rel="noopener">www.nasa.gov/spitzer</a><br /><br />Article :https://www.nasa.gov/feature/goddard/2017/nasa-s-webb-telescope-to-witness-galactic-infancy]]></itunes:summary><itunes:duration>1277</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Muana Kea Telescopes, Hurricane Maria, and the end of the Cassini Mission</title><link>https://www.spreaker.com/episode/muana-kea-telescopes-hurricane-maria-and-the-end-of-the-cassini-mission--23524940</link><description><![CDATA[I ventured to Hawaii, and then Mount Muana Kea, to visit the various telescopes on the mountain. <br />Gemini 8.1 meter diameter, Optical/Infrared Telescope, operated by a consortium of 7 countries, of which Canada is one.  Canada, France, Hawaii Telescope, 3.6 meter Optical Telescope, the UK 3.8 m Infrared Telescope, University of Hawaii 0.6 m educational reflector Telescope,  James Clerk Maxwell 15 m Telescope for submillimeter astronomy, operated the UK and Canada, the Submillieter Array, an array of  8, 6 m, submillimeter antennas, Subaru 8.3  m Telescope operated by Japan, W.M. Keck Observatory, housed in 2 buildings, with 2, 10 m Telescopes, in which Canada is involved, and the NASA INFRARED Telescope, operated for NASA by the University of Hawaii.  I saw the Milky Way in Hawaii after the sun went down. NICE. In other news, let's talk about MARIA, the storm that his hitting Puerto Rico. NASA is using satellites and GPS systems. Among these are the Hubble Telescope, and GEOS- 16. NASA is getting data on the amount of rain, where it is hitting, where it is heavier, and it is also providing information about the eye of the storm. In our third story, the Cassini Spacecraft ended its historic 13 year mission on Saturn, by crashlanding into the ringed planet, on Friday, September 15, 2017. This was done because the fuel supply was used up, and NASA wanted to ensure that Cassini would not crash on any of the moons which harbour subsurface oceans, particularly Enceladus, and also Titan. the telemetry recieved from Cassini during its final plunge showed that the spacecraft entered Saturn's atmosphere, using its thrusters to maintain stablility. Loss of contact with the spacecraft occurred on t 7:55 a.m. EDT (4:55 a.m. PDT), with the signal received by NASA's Deep Space Network antenna complex in Canberra, Australia. NASA was monitored the data as Cassini made its plunge. The spacecraft started its drama, by diving between Saturn and its rings. This is expected to give valuable information about Saturn's atmosphere. With the all of the enormous amount of data received from Cassini during its 13 year mission to Saturn, and also during its 4 year flight to reach the ringed planet, the textbooks will definitely be re-written for Saturn, and its rings, and its moons. Hopefully I can talk to Trina Ray, a mission scientist at the Jet Propulsion Laboratory, to ask here about all of the interesting things about Saturn. I had Trina Ray on a year or two ago. Thank you Cassini, NASA, and the Jet Propulsion Laboratory in Pasadena.<br /><br /><a href="https://www.nasa.gov/feature/goddard/2017/maria-atlantic-ocean" rel="noopener">https://www.nasa.gov/feature/goddard/2017/maria-atlantic-ocean</a><br /><a href="https://www.nasa.gov/press-release/nasa-s-cassini-spacecraft-ends-its-historic-exploration-of-saturn" rel="noopener">https://www.nasa.gov/press-release/nasa-s-cassini-spacecraft-ends-its-historic-exploration-of-saturn</a>]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-September-21-15-00-00.mp3</guid><pubDate>Thu, 21 Sep 2017 21:59:44 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524940/astrotalk_september_21_15_00_00.mp3" length="24736079" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>I ventured to Hawaii, and then Mount Muana Kea, to visit the various telescopes on the mountain. 
Gemini 8.1 meter diameter, Optical/Infrared Telescope, operated by a consortium of 7 countries, of which Canada is one.  Canada, France, Hawaii...</itunes:subtitle><itunes:summary><![CDATA[I ventured to Hawaii, and then Mount Muana Kea, to visit the various telescopes on the mountain. <br />Gemini 8.1 meter diameter, Optical/Infrared Telescope, operated by a consortium of 7 countries, of which Canada is one.  Canada, France, Hawaii Telescope, 3.6 meter Optical Telescope, the UK 3.8 m Infrared Telescope, University of Hawaii 0.6 m educational reflector Telescope,  James Clerk Maxwell 15 m Telescope for submillimeter astronomy, operated the UK and Canada, the Submillieter Array, an array of  8, 6 m, submillimeter antennas, Subaru 8.3  m Telescope operated by Japan, W.M. Keck Observatory, housed in 2 buildings, with 2, 10 m Telescopes, in which Canada is involved, and the NASA INFRARED Telescope, operated for NASA by the University of Hawaii.  I saw the Milky Way in Hawaii after the sun went down. NICE. In other news, let's talk about MARIA, the storm that his hitting Puerto Rico. NASA is using satellites and GPS systems. Among these are the Hubble Telescope, and GEOS- 16. NASA is getting data on the amount of rain, where it is hitting, where it is heavier, and it is also providing information about the eye of the storm. In our third story, the Cassini Spacecraft ended its historic 13 year mission on Saturn, by crashlanding into the ringed planet, on Friday, September 15, 2017. This was done because the fuel supply was used up, and NASA wanted to ensure that Cassini would not crash on any of the moons which harbour subsurface oceans, particularly Enceladus, and also Titan. the telemetry recieved from Cassini during its final plunge showed that the spacecraft entered Saturn's atmosphere, using its thrusters to maintain stablility. Loss of contact with the spacecraft occurred on t 7:55 a.m. EDT (4:55 a.m. PDT), with the signal received by NASA's Deep Space Network antenna complex in Canberra, Australia. NASA was monitored the data as Cassini made its plunge. The spacecraft started its drama, by diving between Saturn and its rings. This is expected to give valuable information about Saturn's atmosphere. With the all of the enormous amount of data received from Cassini during its 13 year mission to Saturn, and also during its 4 year flight to reach the ringed planet, the textbooks will definitely be re-written for Saturn, and its rings, and its moons. Hopefully I can talk to Trina Ray, a mission scientist at the Jet Propulsion Laboratory, to ask here about all of the interesting things about Saturn. I had Trina Ray on a year or two ago. Thank you Cassini, NASA, and the Jet Propulsion Laboratory in Pasadena.<br /><br /><a href="https://www.nasa.gov/feature/goddard/2017/maria-atlantic-ocean" rel="noopener">https://www.nasa.gov/feature/goddard/2017/maria-atlantic-ocean</a><br /><a href="https://www.nasa.gov/press-release/nasa-s-cassini-spacecraft-ends-its-historic-exploration-of-saturn" rel="noopener">https://www.nasa.gov/press-release/nasa-s-cassini-spacecraft-ends-its-historic-exploration-of-saturn</a>]]></itunes:summary><itunes:duration>1546</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>ELectronegativity of Hydrogen and Oxygen, Different Universes? Dark Energy and Dark Matter</title><link>https://www.spreaker.com/episode/electronegativity-of-hydrogen-and-oxygen-different-universes-dark-energy-and-dark-matter--23524885</link><description><![CDATA[Dark Matter Map of 26 million galaxies in the Dark Energy Survey, by using gravitational lensing. The map covers about 1/30th of the entire sky and spans several billion light years. The map will be useful for 2 planned missions, ESA's Euclid mission, and NASA's WFIRST. (I interviewed Dr. Dominic Benford about WFIRST a few years ago). WFIRST is NASA's next big outer-space observatory mission after the James Webb Telescope. WF will help scientists learn more about cosmology, the beginning and ultimate fate of our universe, by learning more about Dark Matter and Dark Energy. DM is thought to hold the universe together, and DE is thought to be responsible for the accelerated expansion of the universe. Planck measurements have provided astronomers with a very suitable model of the universe at its beginning, and as the universe is now. 70 % of the energy in the universe is believed to be dark energy. Dark matter makes up 25 % of the universe, and the stuff that we can see, is thought to compose about 5 % of the universe. Scientists have used gravitational lensing and galaxy clustering to make their measurements. <br /><br /><br /><br /><a href="https://www.jpl.nasa.gov/news/news.php?feature=6913" rel="noopener">https://www.jpl.nasa.gov/news/news.php?feature=6913</a>]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-September-07-15-00-00.mp3</guid><pubDate>Thu, 07 Sep 2017 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524885/astrotalk_september_07_15_00_00.mp3" length="28815778" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Dark Matter Map of 26 million galaxies in the Dark Energy Survey, by using gravitational lensing. The map covers about 1/30th of the entire sky and spans several billion light years. The map will be useful for 2 planned missions, ESA's Euclid mission,...</itunes:subtitle><itunes:summary><![CDATA[Dark Matter Map of 26 million galaxies in the Dark Energy Survey, by using gravitational lensing. The map covers about 1/30th of the entire sky and spans several billion light years. The map will be useful for 2 planned missions, ESA's Euclid mission, and NASA's WFIRST. (I interviewed Dr. Dominic Benford about WFIRST a few years ago). WFIRST is NASA's next big outer-space observatory mission after the James Webb Telescope. WF will help scientists learn more about cosmology, the beginning and ultimate fate of our universe, by learning more about Dark Matter and Dark Energy. DM is thought to hold the universe together, and DE is thought to be responsible for the accelerated expansion of the universe. Planck measurements have provided astronomers with a very suitable model of the universe at its beginning, and as the universe is now. 70 % of the energy in the universe is believed to be dark energy. Dark matter makes up 25 % of the universe, and the stuff that we can see, is thought to compose about 5 % of the universe. Scientists have used gravitational lensing and galaxy clustering to make their measurements. <br /><br /><br /><br /><a href="https://www.jpl.nasa.gov/news/news.php?feature=6913" rel="noopener">https://www.jpl.nasa.gov/news/news.php?feature=6913</a>]]></itunes:summary><itunes:duration>1801</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Fueling Super-Massive Black Holes and A Fleeting Blue Glow</title><link>https://www.spreaker.com/episode/fueling-super-massive-black-holes-and-a-fleeting-blue-glow--23524887</link><description><![CDATA[Italian astronomers using the MUSE (Multi-Unit Spectroscopic Explorer) instrument on the Very Large Telescope (VLT) at ESO’s Paranal Observatory in Chile are studying how gas is being stripped away from some nearby galaxies. The galaxies are nicknamed jellyfish galaxies, because streams of gas resembling tentacles, are being stripped away, and are being fed into their central black holes, causing these galaxies to shine brightly. The tentacles are formed by a process called "Ram Pressure Stripping", where the mutual gravitational attraction of the galaxies (which are falling into a galaxy cluster) create a hot, dense gas. This gas acts as a powerful wind that forces the gas out of the galaxies, and creates the long tentacles, which are tens of thousands of light-years long. It is these tentacles that fuel the super-massive black holes in the centers of the galaxies, and make them shine brightly. Astronomers are surprised at the extent of the feeding of the black holes. 6 of the 7 galaxies in the survey exhibit the phenomenon of Ram Pressure Stripping, far more than expected. The astronomers working on this project claim that the strong link between RPS and the feeding of the black hole with gas was not expected (at least not to this extent). The astronomers are puzzled as to why the gas emissions are reaching the central black holes, instead of being removed from the galaxy. In general, only a very small fraction of super-massive black holes (that inhabit the centers of galaxies) are active, or are devouring matter.<br />In other astronomy news, A Fleeting Blue Glow is being seen with a star that is "only" 55 million light-years away. An exploding star (or supernova) is seen to be gobbling up a companion star, but, to the surprise of astronomers, the companion is not a white dwarf star. The exploding star emits  very bright blue radiation, something that could not have happened if the companion star was another white dwarf. Because of the brightness of the blue emission, astronomers believe that the companion star had to be about 20 times the mass of the white dwarf. In ordinary supernovae of this type (type 1a), the white dwarf that goes supernova usually steals gas from a companion star that is much the same size that it is. Supernova SN 2017cbv is in galaxy NGC 5643, and at 55 million light-years away, is one of the closest supernovae that have recently been discovered. Linking their PROMPT telescope in Chile to a "Panchromatic Robotic Optical Monitoring and Polarimetry" system allowed the astronomers to capture a supernova explosion in a much quicker time than was previously possible.  The event was then looked at by 17 other robotic telescopic networks around the world. With this revolution in data acquisition, much was learned about supernovae in this explosion. In particular, the astronomers viewing the SN were seeing how the exploding star could wreak havoc on its companion. Additionally, astronomers were not expecting the companion to be approximately 20 times the mass of the exploding white dwarf star.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-August-17-15-02-12.mp3</guid><pubDate>Thu, 17 Aug 2017 22:02:13 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524887/astrotalk_august_17_15_02_12.mp3" length="27520104" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Italian astronomers using the MUSE (Multi-Unit Spectroscopic Explorer) instrument on the Very Large Telescope (VLT) at ESO’s Paranal Observatory in Chile are studying how gas is being stripped away from some nearby galaxies. The galaxies are nicknamed...</itunes:subtitle><itunes:summary><![CDATA[Italian astronomers using the MUSE (Multi-Unit Spectroscopic Explorer) instrument on the Very Large Telescope (VLT) at ESO’s Paranal Observatory in Chile are studying how gas is being stripped away from some nearby galaxies. The galaxies are nicknamed jellyfish galaxies, because streams of gas resembling tentacles, are being stripped away, and are being fed into their central black holes, causing these galaxies to shine brightly. The tentacles are formed by a process called "Ram Pressure Stripping", where the mutual gravitational attraction of the galaxies (which are falling into a galaxy cluster) create a hot, dense gas. This gas acts as a powerful wind that forces the gas out of the galaxies, and creates the long tentacles, which are tens of thousands of light-years long. It is these tentacles that fuel the super-massive black holes in the centers of the galaxies, and make them shine brightly. Astronomers are surprised at the extent of the feeding of the black holes. 6 of the 7 galaxies in the survey exhibit the phenomenon of Ram Pressure Stripping, far more than expected. The astronomers working on this project claim that the strong link between RPS and the feeding of the black hole with gas was not expected (at least not to this extent). The astronomers are puzzled as to why the gas emissions are reaching the central black holes, instead of being removed from the galaxy. In general, only a very small fraction of super-massive black holes (that inhabit the centers of galaxies) are active, or are devouring matter.<br />In other astronomy news, A Fleeting Blue Glow is being seen with a star that is "only" 55 million light-years away. An exploding star (or supernova) is seen to be gobbling up a companion star, but, to the surprise of astronomers, the companion is not a white dwarf star. The exploding star emits  very bright blue radiation, something that could not have happened if the companion star was another white dwarf. Because of the brightness of the blue emission, astronomers believe that the companion star had to be about 20 times the mass of the white dwarf. In ordinary supernovae of this type (type 1a), the white dwarf that goes supernova usually steals gas from a companion star that is much the same size that it is. Supernova SN 2017cbv is in galaxy NGC 5643, and at 55 million light-years away, is one of the closest supernovae that have recently been discovered. Linking their PROMPT telescope in Chile to a "Panchromatic Robotic Optical Monitoring and Polarimetry" system allowed the astronomers to capture a supernova explosion in a much quicker time than was previously possible.  The event was then looked at by 17 other robotic telescopic networks around the world. With this revolution in data acquisition, much was learned about supernovae in this explosion. In particular, the astronomers viewing the SN were seeing how the exploding star could wreak havoc on its companion. Additionally, astronomers were not expecting the companion to be approximately 20 times the mass of the exploding white dwarf star.]]></itunes:summary><itunes:duration>1721</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>ELectronegativity of Hydrogen and Oxygen, Different Universes? Dark Energy and Dark Matter</title><link>https://www.spreaker.com/episode/electronegativity-of-hydrogen-and-oxygen-different-universes-dark-energy-and-dark-matter--23524926</link><description><![CDATA[ELectronegativity of Hydrogen and Oxygen, Different Universes? Introduction on how our universe forms. Dr. and Professor Brian Cox, on his TV show, discusses the parameters and variables that were responsible for giving us the universe we have today. Dark Energy and Dark Matter <br />Dark Matter Map of 26 million galaxies in the Dark Energy Survey, by using gravitational lensing. The map covers about 1/30th of the entire sky and spans several billion light years. The map will be useful for 2 planned missions, ESA's Euclid mission, and NASA's WFIRST. (I interviewed Dr. Dominic Benford about WFIRST a few years ago). WFIRST is NASA's next big outer-space observatory mission after the James Webb Telescope. WF will help scientists learn more about cosmology, the beginning and ultimate fate of our universe, by learning more about Dark Matter and Dark Energy. DM is thought to hold the universe together, and DE is thought to be responsible for the accelerated expansion of the universe. Planck measurements have provided astronomers with a very suitable model of the universe at its beginning, and as the universe is now. 70 % of the energy in the universe is believed to be dark energy. Dark matter makes up 25 % of the universe, and the stuff that we can see, is thought to compose about 5 % of the universe. Scientists have used gravitational lensing and galaxy clustering to make their measurements. Also, brief introduction to the NUSTAR Observatory <br /> before the show finished. <a href="https://www.jpl.nasa.gov/news/news.php?feature=6913" rel="noopener">https://www.jpl.nasa.gov/news/news.php?feature=6913</a>     <a href="https://www.nasa.gov/feature/jpl/nustars-first-five-years-in-space" rel="noopener">https://www.nasa.gov/feature/jpl/nustars-first-five-years-in-space</a>]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-August-10-15-00-00.mp3</guid><pubDate>Thu, 10 Aug 2017 22:02:30 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524926/astrotalk_august_10_15_00_00.mp3" length="23296209" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>ELectronegativity of Hydrogen and Oxygen, Different Universes? Introduction on how our universe forms. Dr. and Professor Brian Cox, on his TV show, discusses the parameters and variables that were responsible for giving us the universe we have today....</itunes:subtitle><itunes:summary><![CDATA[ELectronegativity of Hydrogen and Oxygen, Different Universes? Introduction on how our universe forms. Dr. and Professor Brian Cox, on his TV show, discusses the parameters and variables that were responsible for giving us the universe we have today. Dark Energy and Dark Matter <br />Dark Matter Map of 26 million galaxies in the Dark Energy Survey, by using gravitational lensing. The map covers about 1/30th of the entire sky and spans several billion light years. The map will be useful for 2 planned missions, ESA's Euclid mission, and NASA's WFIRST. (I interviewed Dr. Dominic Benford about WFIRST a few years ago). WFIRST is NASA's next big outer-space observatory mission after the James Webb Telescope. WF will help scientists learn more about cosmology, the beginning and ultimate fate of our universe, by learning more about Dark Matter and Dark Energy. DM is thought to hold the universe together, and DE is thought to be responsible for the accelerated expansion of the universe. Planck measurements have provided astronomers with a very suitable model of the universe at its beginning, and as the universe is now. 70 % of the energy in the universe is believed to be dark energy. Dark matter makes up 25 % of the universe, and the stuff that we can see, is thought to compose about 5 % of the universe. Scientists have used gravitational lensing and galaxy clustering to make their measurements. Also, brief introduction to the NUSTAR Observatory <br /> before the show finished. <a href="https://www.jpl.nasa.gov/news/news.php?feature=6913" rel="noopener">https://www.jpl.nasa.gov/news/news.php?feature=6913</a>     <a href="https://www.nasa.gov/feature/jpl/nustars-first-five-years-in-space" rel="noopener">https://www.nasa.gov/feature/jpl/nustars-first-five-years-in-space</a>]]></itunes:summary><itunes:duration>1457</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>a</title><link>https://www.spreaker.com/episode/a--23524993</link><description><![CDATA[a]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-August-03-15-00-00.mp3</guid><pubDate>Thu, 03 Aug 2017 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524993/astrotalk_august_03_15_00_00.mp3" length="28816196" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>a</itunes:subtitle><itunes:summary><![CDATA[a]]></itunes:summary><itunes:duration>1802</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>August 21 Solar Eclipse</title><link>https://www.spreaker.com/episode/august-21-solar-eclipse--23524998</link><description><![CDATA[Most of North America will be taking in the total, or partial, solar eclipse, on August 21, 2017. The eclipse will be total as viewed in Portland Oregon, while in Vancouver, the magnitude of the eclipse will be 0.88. So the eclipse from Vancouver will be partial. The magnitude of the eclipse as seen from Seattle will be 0.91.The eclipse will move from Oregon, across the USA, and into South Carolina. NASA has enlisted 50 high schools in the USA to study the eclipse. Each school will launch a balloon, containing 1 metal plate of bacteria. The balloon will float high into Earth's atmosphere, and since UV rays are blocked by the Moon during the eclipse, this will be like simulating a Martian-like atmosphere, and how the bacteria react to it. The bacteria will then be compared to bacteria on Earth, which has not been exposed to the higher "eclipsed" atmosphere. The conditions of a "wispy-like" atmosphere high on Earth are thought to be similar to the wispy-like conditions with Mars' atmosphere in general. With the Moon blocking the UV rays from the Sun, this will also be similar to conditions in the Martian atmosphere. NASA is also sending up 2 of its WB-F57 jets, with telescopes mounted on their noses, to better view the eclipse.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-July-27-15-00-00.mp3</guid><pubDate>Thu, 27 Jul 2017 22:00:10 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524998/astrotalk_july_27_15_00_00.mp3" length="28816196" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Most of North America will be taking in the total, or partial, solar eclipse, on August 21, 2017. The eclipse will be total as viewed in Portland Oregon, while in Vancouver, the magnitude of the eclipse will be 0.88. So the eclipse from Vancouver will...</itunes:subtitle><itunes:summary><![CDATA[Most of North America will be taking in the total, or partial, solar eclipse, on August 21, 2017. The eclipse will be total as viewed in Portland Oregon, while in Vancouver, the magnitude of the eclipse will be 0.88. So the eclipse from Vancouver will be partial. The magnitude of the eclipse as seen from Seattle will be 0.91.The eclipse will move from Oregon, across the USA, and into South Carolina. NASA has enlisted 50 high schools in the USA to study the eclipse. Each school will launch a balloon, containing 1 metal plate of bacteria. The balloon will float high into Earth's atmosphere, and since UV rays are blocked by the Moon during the eclipse, this will be like simulating a Martian-like atmosphere, and how the bacteria react to it. The bacteria will then be compared to bacteria on Earth, which has not been exposed to the higher "eclipsed" atmosphere. The conditions of a "wispy-like" atmosphere high on Earth are thought to be similar to the wispy-like conditions with Mars' atmosphere in general. With the Moon blocking the UV rays from the Sun, this will also be similar to conditions in the Martian atmosphere. NASA is also sending up 2 of its WB-F57 jets, with telescopes mounted on their noses, to better view the eclipse.]]></itunes:summary><itunes:duration>1802</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Brown Dwarfs</title><link>https://www.spreaker.com/episode/brown-dwarfs--23524909</link><description><![CDATA[Rosa Castro is an amateur astronomer by night. She is involved in the Backyard Worlds: Planet 9 citizen science project. NASA is using the WISE Space Telescope (Wide-field Infrared Survey Explorer) to scour the sky for a 9th planet that is supposedly lurking somewhere beyond Pluto. But they are also wise enough to use WISE to search for Brown Dwarfs (BD). A BD is essentially a failed sun, or a failed star. It is bigger than Jupiter, roughly 13 - 80 Jupiter masses, but a BD dose not have enough mass to force itself to begin the process of nuclear fusion. Rosa Castro found 1 such BD, WISEA J110125.95+540052.8, when she was combing through some data provided by NASA. Backyard Worlds: Planet 9 is a citizen science project, where ordinary citizens comb through data from WISE, that NASA has provided for the public to examine. Planet 9 has identified 117 potential BDs. BDs were first discovered roughly 20 years ago. Because BDs do not have the necessary mass to sustain nuclear fusion, they are intrinsically dim, so their temperatures are therefore relatively low. This makes them hard to spot. The WISE telescope was designed to observe cold objects that emit light at long wavelengths.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-July-20-15-00-00.mp3</guid><pubDate>Thu, 20 Jul 2017 22:01:25 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524909/astrotalk_july_20_15_00_00.mp3" length="27232131" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Rosa Castro is an amateur astronomer by night. She is involved in the Backyard Worlds: Planet 9 citizen science project. NASA is using the WISE Space Telescope (Wide-field Infrared Survey Explorer) to scour the sky for a 9th planet that is supposedly...</itunes:subtitle><itunes:summary><![CDATA[Rosa Castro is an amateur astronomer by night. She is involved in the Backyard Worlds: Planet 9 citizen science project. NASA is using the WISE Space Telescope (Wide-field Infrared Survey Explorer) to scour the sky for a 9th planet that is supposedly lurking somewhere beyond Pluto. But they are also wise enough to use WISE to search for Brown Dwarfs (BD). A BD is essentially a failed sun, or a failed star. It is bigger than Jupiter, roughly 13 - 80 Jupiter masses, but a BD dose not have enough mass to force itself to begin the process of nuclear fusion. Rosa Castro found 1 such BD, WISEA J110125.95+540052.8, when she was combing through some data provided by NASA. Backyard Worlds: Planet 9 is a citizen science project, where ordinary citizens comb through data from WISE, that NASA has provided for the public to examine. Planet 9 has identified 117 potential BDs. BDs were first discovered roughly 20 years ago. Because BDs do not have the necessary mass to sustain nuclear fusion, they are intrinsically dim, so their temperatures are therefore relatively low. This makes them hard to spot. The WISE telescope was designed to observe cold objects that emit light at long wavelengths.]]></itunes:summary><itunes:duration>1703</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Astronomers Track the Birth of a Super-Earth</title><link>https://www.spreaker.com/episode/astronomers-track-the-birth-of-a-super-earth--23524904</link><description><![CDATA[Researchers at Arizona's Steward Observatory and at the Los Alamos National Laboratory in Los Alamos, New Mexico, are tracking the formation of a super-Earth, an exoplanet anywhere from the mass of the Earth, to the mass of Neptune (~ 14 Earth masses). The features of this exoplanet, and of other similar-sized exoplanets, did not match the model for most of the exoplanetsfound in the Milky Way. The features observed with this exo-planet were thought to require more massive planets, in the size range of Jupiter, or even bigger.  These astronomers were observing a super-Earth carving out a disk in the gas that surrounds its Sun, in a scenario similar to how the rings in Saturn are carved out. Previous models assumed this could only occur with Jupiter-sized exoplanets. This particular exoplanet was in a much younger stage of its formation, different than many of the other older exoplanets in our Solar System, which orbit stars that are billions of years old. When astronomers previously studied these senior citizens of our galaxy, they had no way of knowing how these planets were born. In studying this particular super-Earth, these scientists are now getting a first-hand look at the younger stages of star and planet formation. In essence, they are getting the chance to study a younger proto-planetary disk, in the younger, or "baby" stages of its formation. Seeing an actual planet forming in a proto-planetary disk is not such an easy thing to do, so the scientists are relying on being able to see the gaps and tracks these planet make as they travel through the gas and dust that surrounds the proto-star. The gaps and their relative positions are posing questions, as scientists try to reconcile their previous models from what they are now seeing.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-July-13-15-00-00.mp3</guid><pubDate>Thu, 13 Jul 2017 22:00:15 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524904/astrotalk_july_13_15_00_00.mp3" length="29375844" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Researchers at Arizona's Steward Observatory and at the Los Alamos National Laboratory in Los Alamos, New Mexico, are tracking the formation of a super-Earth, an exoplanet anywhere from the mass of the Earth, to the mass of Neptune (~ 14 Earth...</itunes:subtitle><itunes:summary><![CDATA[Researchers at Arizona's Steward Observatory and at the Los Alamos National Laboratory in Los Alamos, New Mexico, are tracking the formation of a super-Earth, an exoplanet anywhere from the mass of the Earth, to the mass of Neptune (~ 14 Earth masses). The features of this exoplanet, and of other similar-sized exoplanets, did not match the model for most of the exoplanetsfound in the Milky Way. The features observed with this exo-planet were thought to require more massive planets, in the size range of Jupiter, or even bigger.  These astronomers were observing a super-Earth carving out a disk in the gas that surrounds its Sun, in a scenario similar to how the rings in Saturn are carved out. Previous models assumed this could only occur with Jupiter-sized exoplanets. This particular exoplanet was in a much younger stage of its formation, different than many of the other older exoplanets in our Solar System, which orbit stars that are billions of years old. When astronomers previously studied these senior citizens of our galaxy, they had no way of knowing how these planets were born. In studying this particular super-Earth, these scientists are now getting a first-hand look at the younger stages of star and planet formation. In essence, they are getting the chance to study a younger proto-planetary disk, in the younger, or "baby" stages of its formation. Seeing an actual planet forming in a proto-planetary disk is not such an easy thing to do, so the scientists are relying on being able to see the gaps and tracks these planet make as they travel through the gas and dust that surrounds the proto-star. The gaps and their relative positions are posing questions, as scientists try to reconcile their previous models from what they are now seeing.]]></itunes:summary><itunes:duration>1836</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Hubble and Gravitational Lensing</title><link>https://www.spreaker.com/episode/hubble-and-gravitational-lensing--23525001</link><description><![CDATA[With help from the Hubble Space Telescope, scientists have viewed a distant cluster of galaxies, that has been microlensed, and then capture by the lens of HST. J143450.5+033843 lies 11 Billion light years away, and without the aid of gravitational lensing, and HST, it would not be visible. The light of the faint galaxy is being magnified by a cluster of foreground, or closer, galaxies, and without this magnification, HST would not be able to image it well. The strong gravity of the galaxy cluster acts as a magnifier, multiplying the light intensity coming from this far away galaxy. Presently, HST is only able to image the younger stars in this galaxy, but when the James Webb Telescope becomes operational, JSWT will be able to image the older stars in the galaxy. As for the HST, the images it would produce would seem unremarkable without the lensing effect. Astronomers would not be able to make out or spot the hundreds of galaxies, or the knots of galaxies, as astronomers are calling them. Knots of stars, forming in galaxies 200 -- 300 light years across are now visible. Without the lensing and the HST, the light would appear to be smooth; so the formation of the stars would not be visible.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-July-06-15-07-26.mp3</guid><pubDate>Thu, 06 Jul 2017 22:07:26 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525001/astrotalk_july_06_15_07_26.mp3" length="26608118" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>With help from the Hubble Space Telescope, scientists have viewed a distant cluster of galaxies, that has been microlensed, and then capture by the lens of HST. J143450.5+033843 lies 11 Billion light years away, and without the aid of gravitational...</itunes:subtitle><itunes:summary><![CDATA[With help from the Hubble Space Telescope, scientists have viewed a distant cluster of galaxies, that has been microlensed, and then capture by the lens of HST. J143450.5+033843 lies 11 Billion light years away, and without the aid of gravitational lensing, and HST, it would not be visible. The light of the faint galaxy is being magnified by a cluster of foreground, or closer, galaxies, and without this magnification, HST would not be able to image it well. The strong gravity of the galaxy cluster acts as a magnifier, multiplying the light intensity coming from this far away galaxy. Presently, HST is only able to image the younger stars in this galaxy, but when the James Webb Telescope becomes operational, JSWT will be able to image the older stars in the galaxy. As for the HST, the images it would produce would seem unremarkable without the lensing effect. Astronomers would not be able to make out or spot the hundreds of galaxies, or the knots of galaxies, as astronomers are calling them. Knots of stars, forming in galaxies 200 -- 300 light years across are now visible. Without the lensing and the HST, the light would appear to be smooth; so the formation of the stars would not be visible.]]></itunes:summary><itunes:duration>1664</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Cassini and Astronomer Trina Ray</title><link>https://www.spreaker.com/episode/cassini-and-astronomer-trina-ray--23524869</link><description><![CDATA[Ms. Trina Ray is a scientist working on the Cassini Mission, which is winding down its operations in its orbit around the Saturn. Listen to Trina talk about Saturn's Moon Titan, the remarkable composition of Titan's atmosphere, and about the planned crash landing of Cassini into Saturn's atmosphere, which will take place in summer/fall 2017. Also, listen to Trina talk about her involvement  in the Voyager program. Voyager I & II are 2 spacecraft launched in 1977, and both spacecraft are still operational. Voyager I has left the Solar System, and Voyager II will also leave the Solar System, and enter Interplanetary Space, in the near future.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-June-29-15-00-00.mp3</guid><pubDate>Thu, 29 Jun 2017 22:03:25 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524869/astrotalk_june_29_15_00_00.mp3" length="33232353" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Ms. Trina Ray is a scientist working on the Cassini Mission, which is winding down its operations in its orbit around the Saturn. Listen to Trina talk about Saturn's Moon Titan, the remarkable composition of Titan's atmosphere, and about the planned...</itunes:subtitle><itunes:summary><![CDATA[Ms. Trina Ray is a scientist working on the Cassini Mission, which is winding down its operations in its orbit around the Saturn. Listen to Trina talk about Saturn's Moon Titan, the remarkable composition of Titan's atmosphere, and about the planned crash landing of Cassini into Saturn's atmosphere, which will take place in summer/fall 2017. Also, listen to Trina talk about her involvement  in the Voyager program. Voyager I & II are 2 spacecraft launched in 1977, and both spacecraft are still operational. Voyager I has left the Solar System, and Voyager II will also leave the Solar System, and enter Interplanetary Space, in the near future.]]></itunes:summary><itunes:duration>2078</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>August 21 Total Solar Eclipse and Dead Galaxy MACS2129-1</title><link>https://www.spreaker.com/episode/august-21-total-solar-eclipse-and-dead-galaxy-macs2129-1--23524907</link><description><![CDATA[NASA is preparing the public for the total solar eclipse of August 21, 2017.  NASA has also found a "dead" galaxy, that stopped making stars only a few billion years after the Big Bang. The galaxy,   , was thought to have originally been a Milky Way type galaxy, but then it evolved into a giant elliptical-type galaxy. The galaxy is also noteworthy because is now considered a "dead galaxy", one that stopped forming stars only a few billion years after the Big Bang. This type of galaxy not only changed its  structure but also the motions of its stars to make a shape of an elliptical galaxy. The findings are making scientists rethink their earlier theories on how galaxies can burn out. Scientists now wonder whether this particular galaxy may not have fit the earlier models, simply because scientists were unable to image it. This was therefore the firast time that this type of galaxy evolution has been imaged.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-June-22-15-00-00.mp3</guid><pubDate>Thu, 22 Jun 2017 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524907/astrotalk_june_22_15_00_00.mp3" length="26287961" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>NASA is preparing the public for the total solar eclipse of August 21, 2017.  NASA has also found a "dead" galaxy, that stopped making stars only a few billion years after the Big Bang. The galaxy,   , was thought to have originally been a Milky Way...</itunes:subtitle><itunes:summary><![CDATA[NASA is preparing the public for the total solar eclipse of August 21, 2017.  NASA has also found a "dead" galaxy, that stopped making stars only a few billion years after the Big Bang. The galaxy,   , was thought to have originally been a Milky Way type galaxy, but then it evolved into a giant elliptical-type galaxy. The galaxy is also noteworthy because is now considered a "dead galaxy", one that stopped forming stars only a few billion years after the Big Bang. This type of galaxy not only changed its  structure but also the motions of its stars to make a shape of an elliptical galaxy. The findings are making scientists rethink their earlier theories on how galaxies can burn out. Scientists now wonder whether this particular galaxy may not have fit the earlier models, simply because scientists were unable to image it. This was therefore the firast time that this type of galaxy evolution has been imaged.]]></itunes:summary><itunes:duration>1643</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Cancer Research Aboard the International Space Station</title><link>https://www.spreaker.com/episode/cancer-research-aboard-the-international-space-station--23524881</link><description><![CDATA[Researchers are testing how drugs, and combinations of drugs, are affected in treating cancer, in a micro-gravity environment on the ISS. Larger cancer tumors, and tumors that are more spherical in shape, can be grown aboard the ISS. This gives researchers a more accurate picture of how cancer tumors form in the human body, and what is happening with the cancer tumors in the body. On Earth,  the cancer cells being studied are not spherical. This research is just one example of what NASA is doing, in order to study how differently the human body reacts in a gravity free environment, which would be the case on a mission to a place like Mars. Researchers are also using rodents for stem cell research, and, they are also studying how "mold" behaves in a micro-gravity environment.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-June-15-15-00-00.mp3</guid><pubDate>Thu, 15 Jun 2017 22:10:59 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524881/astrotalk_june_15_15_00_00.mp3" length="18992065" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Researchers are testing how drugs, and combinations of drugs, are affected in treating cancer, in a micro-gravity environment on the ISS. Larger cancer tumors, and tumors that are more spherical in shape, can be grown aboard the ISS. This gives...</itunes:subtitle><itunes:summary><![CDATA[Researchers are testing how drugs, and combinations of drugs, are affected in treating cancer, in a micro-gravity environment on the ISS. Larger cancer tumors, and tumors that are more spherical in shape, can be grown aboard the ISS. This gives researchers a more accurate picture of how cancer tumors form in the human body, and what is happening with the cancer tumors in the body. On Earth,  the cancer cells being studied are not spherical. This research is just one example of what NASA is doing, in order to study how differently the human body reacts in a gravity free environment, which would be the case on a mission to a place like Mars. Researchers are also using rodents for stem cell research, and, they are also studying how "mold" behaves in a micro-gravity environment.]]></itunes:summary><itunes:duration>1187</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Blobs of X-Ray Emissions Imaged by the Chandra X-Ray Observatory</title><link>https://www.spreaker.com/episode/blobs-of-x-ray-emissions-imaged-by-the-chandra-x-ray-observatory--23524910</link><description><![CDATA[Astronomers using Chandra are studying a MIra type star , a type of symbiotic star, which co-exists with another star. R Aquair, or R Aqr, is 710 light years from Earth, and is emitting blobs of X-ray emissions. It is a cool, red giant star (a Mira variable star), orbiting a dense white dwarf. The red giant is pulsating and its brightness can change by a factor of 250. The surface temperature of the white dwarf is 20,000 degrees, while the red giant measures in at 3,000. The 2 stars are comparable in mass, but since the WD is much more compact, it is much more dense. This means that is has a stronger gravitational tug, and it is therefore pulling off gas from the red giant, and onto itself. This has resulted in nova explosions on the WD in 1073 and 1773. NASA scientists now believe NOVA explosions occurred from the WD in the early 2000s, and in the 1950s and 1980s. With the NOVA, matter is ejected from the WD at 10 million miles per hour. With this a ring of ejecta is seen.The NOVA explosions are thought to give rise to 2 jets of X-ray emissions that stream away from the pair of stars at 14. & 1.9 millions miles per hour. With these observations, scientists are trying to understand the volatile relationships that can occur between pairs of stars like these.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-June-08-15-11-28.mp3</guid><pubDate>Thu, 08 Jun 2017 22:10:43 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524910/astrotalk_june_08_15_11_28.mp3" length="13887948" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Astronomers using Chandra are studying a MIra type star , a type of symbiotic star, which co-exists with another star. R Aquair, or R Aqr, is 710 light years from Earth, and is emitting blobs of X-ray emissions. It is a cool, red giant star (a Mira...</itunes:subtitle><itunes:summary><![CDATA[Astronomers using Chandra are studying a MIra type star , a type of symbiotic star, which co-exists with another star. R Aquair, or R Aqr, is 710 light years from Earth, and is emitting blobs of X-ray emissions. It is a cool, red giant star (a Mira variable star), orbiting a dense white dwarf. The red giant is pulsating and its brightness can change by a factor of 250. The surface temperature of the white dwarf is 20,000 degrees, while the red giant measures in at 3,000. The 2 stars are comparable in mass, but since the WD is much more compact, it is much more dense. This means that is has a stronger gravitational tug, and it is therefore pulling off gas from the red giant, and onto itself. This has resulted in nova explosions on the WD in 1073 and 1773. NASA scientists now believe NOVA explosions occurred from the WD in the early 2000s, and in the 1950s and 1980s. With the NOVA, matter is ejected from the WD at 10 million miles per hour. With this a ring of ejecta is seen.The NOVA explosions are thought to give rise to 2 jets of X-ray emissions that stream away from the pair of stars at 14. & 1.9 millions miles per hour. With these observations, scientists are trying to understand the volatile relationships that can occur between pairs of stars like these.]]></itunes:summary><itunes:duration>868</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>A Dance of Electrons in Space</title><link>https://www.spreaker.com/episode/a-dance-of-electrons-in-space--23524934</link><description><![CDATA[A strange or "bizarre" dance of electrons has been detected in Earth's magnetosphere. Electrons will travel in spiral patterns around magnetic filed lines, where there is a strong magnetic field. In weak magnetic fields, the electrons wag around in a free style motion. NASA has now uncovered what the electrons do in intermediate strength magnetic fields. The motion is a combination of spiraling and meandering, before the electrons are finally ejected into space. With this, large amounts of magnetic energy can be released. Scientists in NASA'S Magnetospheric Multiscale Mission (MMS) studied the electrons in these intermediate strength fields, and a process they call magnetic reconnection. Magnetic reconnection is thought to occur in the sun, where large amounts of energy that have been stored for days or hours, are released . <br />The magnetic field environment where the electrons’ motions were observed was uniquely created by magnetic reconnection, which caused a current sheet (through which the electrons travel) to be tightly confined by bunched-up magnetic fields. The electrons then travel in large spirals, before they are finally ejected, along with an enormous amount of stored magnetic energy. The new research will hopefully help the scientists better understand the role of electrons in reconnection, and how magnetic fields lose energy. Magnetic reconnection is an important process in the universe as a whole, and is thought to be responsible for the formation of some shock waves and cosmic rays.  In this study, scientists are looking to gain a better understanding of what role electrons play in magnetic reconnection.  Some of the most explosive releases of energy in the universe are thought to occur through magnetic reconnection. With this knowledge, scientists are gaining knowledge of our magnetic environment, and its affect on spacecraft and satellites. MMS obtained their data with a daring flight of 4  spacecraft through the Earth's magnetosphere.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-June-01-15-09-31.mp3</guid><pubDate>Thu, 01 Jun 2017 22:09:31 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524934/astrotalk_june_01_15_09_31.mp3" length="18783922" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>A strange or "bizarre" dance of electrons has been detected in Earth's magnetosphere. Electrons will travel in spiral patterns around magnetic filed lines, where there is a strong magnetic field. In weak magnetic fields, the electrons wag around in a...</itunes:subtitle><itunes:summary><![CDATA[A strange or "bizarre" dance of electrons has been detected in Earth's magnetosphere. Electrons will travel in spiral patterns around magnetic filed lines, where there is a strong magnetic field. In weak magnetic fields, the electrons wag around in a free style motion. NASA has now uncovered what the electrons do in intermediate strength magnetic fields. The motion is a combination of spiraling and meandering, before the electrons are finally ejected into space. With this, large amounts of magnetic energy can be released. Scientists in NASA'S Magnetospheric Multiscale Mission (MMS) studied the electrons in these intermediate strength fields, and a process they call magnetic reconnection. Magnetic reconnection is thought to occur in the sun, where large amounts of energy that have been stored for days or hours, are released . <br />The magnetic field environment where the electrons’ motions were observed was uniquely created by magnetic reconnection, which caused a current sheet (through which the electrons travel) to be tightly confined by bunched-up magnetic fields. The electrons then travel in large spirals, before they are finally ejected, along with an enormous amount of stored magnetic energy. The new research will hopefully help the scientists better understand the role of electrons in reconnection, and how magnetic fields lose energy. Magnetic reconnection is an important process in the universe as a whole, and is thought to be responsible for the formation of some shock waves and cosmic rays.  In this study, scientists are looking to gain a better understanding of what role electrons play in magnetic reconnection.  Some of the most explosive releases of energy in the universe are thought to occur through magnetic reconnection. With this knowledge, scientists are gaining knowledge of our magnetic environment, and its affect on spacecraft and satellites. MMS obtained their data with a daring flight of 4  spacecraft through the Earth's magnetosphere.]]></itunes:summary><itunes:duration>1174</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Juno Mission for Jupiter</title><link>https://www.spreaker.com/episode/juno-mission-for-jupiter--23524916</link><description><![CDATA[Juno blasted off from Earth in August 5, 2011, and entered the orbit in the Jovian system on July 5, 2016.  In its long, elliptical orbits around Jupiter, Juno is conducting various experiments. First data show cyclones at the poles of this turbulent world, that can be as big as the Earth, and that can travel at great speeds. The atmospheric content of ammonia on the planet can vary, and the magnetic filed surround Jupiter is bigger and more irregular than previously thought. Juno gets its closest to Jupiter every 53 days, as it approaches the gas giant in line with its north pole. The science coming in is endless and surprising. The Juno mission to Jupiter is being overseen by the Jet Propulsion Laboratory (JPL) in Pasadena. Stay tuned for more.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-May-25-15-00-26.mp3</guid><pubDate>Thu, 25 May 2017 22:00:26 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524916/astrotalk_may_25_15_00_26.mp3" length="26208130" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Juno blasted off from Earth in August 5, 2011, and entered the orbit in the Jovian system on July 5, 2016.  In its long, elliptical orbits around Jupiter, Juno is conducting various experiments. First data show cyclones at the poles of this turbulent...</itunes:subtitle><itunes:summary><![CDATA[Juno blasted off from Earth in August 5, 2011, and entered the orbit in the Jovian system on July 5, 2016.  In its long, elliptical orbits around Jupiter, Juno is conducting various experiments. First data show cyclones at the poles of this turbulent world, that can be as big as the Earth, and that can travel at great speeds. The atmospheric content of ammonia on the planet can vary, and the magnetic filed surround Jupiter is bigger and more irregular than previously thought. Juno gets its closest to Jupiter every 53 days, as it approaches the gas giant in line with its north pole. The science coming in is endless and surprising. The Juno mission to Jupiter is being overseen by the Jet Propulsion Laboratory (JPL) in Pasadena. Stay tuned for more.]]></itunes:summary><itunes:duration>1639</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>No show?</title><link>https://www.spreaker.com/episode/no-show--23524920</link><description><![CDATA[No show?]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-May-11-15-00-00.mp3</guid><pubDate>Thu, 11 May 2017 22:15:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524920/astrotalk_may_11_15_00_00.mp3" length="28816196" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>No show?</itunes:subtitle><itunes:summary><![CDATA[No show?]]></itunes:summary><itunes:duration>1802</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Galaxy Cluster Abell 370 and May the 4th Be With You</title><link>https://www.spreaker.com/episode/galaxy-cluster-abell-370-and-may-the-4th-be-with-you--23524905</link><description><![CDATA[Galaxy cluster Abell 370 is made up of hundreds of galaxies that are held together as a group, by the mutual pull of gravity each member galaxy exerts on other members of the group.  A recent Hubble photo, taken in the infrared, shows these galaxies, but it also shows arcs and/or streaks. Other photos were also taken in visible light, and then both the visible and infrared images were overlapped to provide more detailed images. These arcs/streaks are actually far-flung galaxies that lie behind the Abell 370 cluster. They have been magnified by gravitational lensing. The collective mass and gravity of the stars and matter of Abell 370 warp space and time, and act as the magnifier.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-May-04-15-00-00.mp3</guid><pubDate>Thu, 04 May 2017 22:03:50 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524905/astrotalk_may_04_15_00_00.mp3" length="24351974" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Galaxy cluster Abell 370 is made up of hundreds of galaxies that are held together as a group, by the mutual pull of gravity each member galaxy exerts on other members of the group.  A recent Hubble photo, taken in the infrared, shows these galaxies,...</itunes:subtitle><itunes:summary><![CDATA[Galaxy cluster Abell 370 is made up of hundreds of galaxies that are held together as a group, by the mutual pull of gravity each member galaxy exerts on other members of the group.  A recent Hubble photo, taken in the infrared, shows these galaxies, but it also shows arcs and/or streaks. Other photos were also taken in visible light, and then both the visible and infrared images were overlapped to provide more detailed images. These arcs/streaks are actually far-flung galaxies that lie behind the Abell 370 cluster. They have been magnified by gravitational lensing. The collective mass and gravity of the stars and matter of Abell 370 warp space and time, and act as the magnifier.]]></itunes:summary><itunes:duration>1522</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Earhart Propellor in Saturn`s A Ring</title><link>https://www.spreaker.com/episode/earhart-propellor-in-saturn-s-a-ring--23524886</link><description><![CDATA[on March 22, 2017, NASA`s Cassini Spacecraft took close up pictures of something called an Èarhart Propellor``, in Saturn`s A Ring. This is the second time NASA has targeted an individula propellor in a ring in Saturn. The first such propellor tarteted was the Santos-Dumont (PIA21433) propellor, one month earlier. Moonlets are sometimes thought to form in Saturn`s rings, and when they do, objects called ``Porpellors`form as well.  Prpellors are disturbances in a ring, that are caused by the formation, or presence, of a moonlet. Earhart is brighter than Santos-Dumont, and the third propellor which will be flimed in the near future,"Bleriot," will be imaged in April 2017. Earhart is close the Encke Gap, which is 200 miles wide. The Encke gap is thought to be held open by the moon Pan. Pan is 100os of times more massive than Earhart, so it can open up a gap that extends all the way around the ring it inhabits. The mass of the ring itself closes off the gap made by Earhart, before the gap can extend too far. Wave features are also seen to the left of Earhart. These are caused by the moons, Promehteus, Pandora and Pan.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-April-27-15-04-10.mp3</guid><pubDate>Thu, 27 Apr 2017 22:16:45 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524886/astrotalk_april_27_15_04_10.mp3" length="20416052" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>on March 22, 2017, NASA`s Cassini Spacecraft took close up pictures of something called an Èarhart Propellor``, in Saturn`s A Ring. This is the second time NASA has targeted an individula propellor in a ring in Saturn. The first such propellor...</itunes:subtitle><itunes:summary><![CDATA[on March 22, 2017, NASA`s Cassini Spacecraft took close up pictures of something called an Èarhart Propellor``, in Saturn`s A Ring. This is the second time NASA has targeted an individula propellor in a ring in Saturn. The first such propellor tarteted was the Santos-Dumont (PIA21433) propellor, one month earlier. Moonlets are sometimes thought to form in Saturn`s rings, and when they do, objects called ``Porpellors`form as well.  Prpellors are disturbances in a ring, that are caused by the formation, or presence, of a moonlet. Earhart is brighter than Santos-Dumont, and the third propellor which will be flimed in the near future,"Bleriot," will be imaged in April 2017. Earhart is close the Encke Gap, which is 200 miles wide. The Encke gap is thought to be held open by the moon Pan. Pan is 100os of times more massive than Earhart, so it can open up a gap that extends all the way around the ring it inhabits. The mass of the ring itself closes off the gap made by Earhart, before the gap can extend too far. Wave features are also seen to the left of Earhart. These are caused by the moons, Promehteus, Pandora and Pan.]]></itunes:summary><itunes:duration>1276</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>The Arrythmic Beating of a Black Hole Heart</title><link>https://www.spreaker.com/episode/the-arrythmic-beating-of-a-black-hole-heart--23524929</link><description><![CDATA[A large elliptical galaxy, NGC 4696, located 145 light years from Earth, lurks at the heart of the Centaurus galaxy cluster. And hiding deep in the heart of NGC 4696, lurks a massive black hole. Even though black holes are known to devour matter around it, this particular black hole is pumping energy into the galaxy around it. The bursts of energy are thought to occur every 5 - 10 million years. The bursts create cavities in the hot gas that inhabits the space in between neighboring galaxies. Sonic booms, which have been measured to travel tens of thousands of light years, are also created when the black hole pumps out its energy. The process is being imaged by the Chandra Observatory in x-rays, Hubble in visible light, and in radio from the Very Large Array Telescope. When the images are combined, astronomers get a better picture of what is going on. Chandra was used to highlight 9 special cavities in the hot gas. Astronomers have also measured the "pitch" of the resonance in the cavities, and have marked it as having a note near middle C. The hot gas that fills the cluster of galaxies has allowed the sound to travel. The black hole bursts seem to be full of elements that are generated in previous supernova explosions in NGC 4696. Oddly, the energy coming from the black hole has prevented the gas around it from cooling. New stars form from cool gas, so the higher temperature of the gas has prevented large numbers of stars from forming in the vicinity of the black hole. <br /><br />A different type of processing of the X-ray data reveals a sequence of curved and approximately equally spaced features in the hot gas. These may be caused by sound waves generated by the black hole’s repeated bursts. In a galaxy cluster, the hot gas that fills the cluster enables sound waves – albeit at frequencies far too low for the human hear to detect – to propagate.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-April-20-14-59-18.mp3</guid><pubDate>Thu, 20 Apr 2017 21:59:18 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524929/astrotalk_april_20_14_59_18.mp3" length="27023987" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>A large elliptical galaxy, NGC 4696, located 145 light years from Earth, lurks at the heart of the Centaurus galaxy cluster. And hiding deep in the heart of NGC 4696, lurks a massive black hole. Even though black holes are known to devour matter...</itunes:subtitle><itunes:summary><![CDATA[A large elliptical galaxy, NGC 4696, located 145 light years from Earth, lurks at the heart of the Centaurus galaxy cluster. And hiding deep in the heart of NGC 4696, lurks a massive black hole. Even though black holes are known to devour matter around it, this particular black hole is pumping energy into the galaxy around it. The bursts of energy are thought to occur every 5 - 10 million years. The bursts create cavities in the hot gas that inhabits the space in between neighboring galaxies. Sonic booms, which have been measured to travel tens of thousands of light years, are also created when the black hole pumps out its energy. The process is being imaged by the Chandra Observatory in x-rays, Hubble in visible light, and in radio from the Very Large Array Telescope. When the images are combined, astronomers get a better picture of what is going on. Chandra was used to highlight 9 special cavities in the hot gas. Astronomers have also measured the "pitch" of the resonance in the cavities, and have marked it as having a note near middle C. The hot gas that fills the cluster of galaxies has allowed the sound to travel. The black hole bursts seem to be full of elements that are generated in previous supernova explosions in NGC 4696. Oddly, the energy coming from the black hole has prevented the gas around it from cooling. New stars form from cool gas, so the higher temperature of the gas has prevented large numbers of stars from forming in the vicinity of the black hole. <br /><br />A different type of processing of the X-ray data reveals a sequence of curved and approximately equally spaced features in the hot gas. These may be caused by sound waves generated by the black hole’s repeated bursts. In a galaxy cluster, the hot gas that fills the cluster enables sound waves – albeit at frequencies far too low for the human hear to detect – to propagate.]]></itunes:summary><itunes:duration>1689</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Enceladus and Images of Mars from MRO and HIRISE and MAVEN</title><link>https://www.spreaker.com/episode/enceladus-and-images-of-mars-from-mro-and-hirise-and-maven--23524935</link><description><![CDATA[Cassini is showing off: well, just a little. NASA is revealing details of information gleamed from a Cassini dive through plumes of vapor as it flies through Enceladus' atmosphere. Enceladus is the icy moon of Saturn. A sub-surface ocean is thought to exist on Enceladus, hightening the possibility that life could exist on the moon. For life to exist (as we know it) 3 ingredients are necessary: liquid water, the right chemical ingredients, and a source of energy for metabloism. Enceladus is thought to have all of these. The article describing this research can be found on <a href="http://www.nasa.gov" rel="noopener">www.nasa.gov</a>, in  "NASA Missions Provide New Insights into 'Ocean Worlds' in Our Solar System", dated April 13, 2017.<br />Also, in another region of our Solar System, the Mars Reconnaissance Orbiter (MRO) is exploring a region called, "Noctis Labyrinthus". MRO has captured a striking image of a mesa, just one of several in the region known as Valles Marineris. The mesa is ~ 0.4 km wide, probably composed of sedimentary deposits that are also eroding. The image is magnificent, and can be found on <a href="https://www.nasa.gov/image-feature/jpl/pia21585/a-mesa-in-noctis-labyrinthus" rel="noopener">https://www.nasa.gov/image-feature/jpl/pia21585/a-mesa-in-noctis-labyrinthus</a>. Another image from MRO shows a hill on Mars, on the South Pole layered deposits. The hill protects the icy layers from erosion, so the image shows the hill with beautiful spiral patterns. In another finding from MRO, over 500 new impact events have been exposed from before and after images of the Southern Middle Latitudes. The new images show shallow sheets of ice that have interested scientists, because ice has not been previously detected on Mars at these latitudes. The scientists hope to better map the ice distribution on Mars, with help from this new data. Staying with Mars, NASA is using the MAVEN spacecraft (Mars Atmosphere and Volatile Evolution) to examine the charged metal atoms that exist high in Mars' whismy upper atmosphere, or ionosphere. This is the first direct detection of atoms like these in a planet other than Earth.  Metallic ions have long lifetimes, so studying these ions can help scientists infer the motion of Mars' ionosphere. With this information, it is hoped scientists can better understand how Mars lost most of its atmosphere, making it the dry, dusty world it is today. Scientists believe that ions exist in the atmospheres of other planets in our Solar System. When other spacecraft have tried to send signals to Earth from locations on other planets, such as Jupiter or Saturn, parts of these signals have sometimes been blocked. Scientists have inferred that the presence of metal ions in the ionospheres of these other planets have been responsible for the signal blockage, but no direct proof of this has been offered. Another curious find on Mars was that the metal ions in Mars' ionosphere behave differently than the ions in Earth's ionoshpere. This could be due to the presence of a magnetosphere on Earth, and a lack of one on Mars. Scientists with MAVEN are also trying to learn about the formation of high altitude clouds on Earth and Mars, and what role the ions in the ionospheres have on this phenomenon.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-April-13-15-05-30.mp3</guid><pubDate>Thu, 13 Apr 2017 22:05:30 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524935/astrotalk_april_13_15_05_30.mp3" length="22655895" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Cassini is showing off: well, just a little. NASA is revealing details of information gleamed from a Cassini dive through plumes of vapor as it flies through Enceladus' atmosphere. Enceladus is the icy moon of Saturn. A sub-surface ocean is thought to...</itunes:subtitle><itunes:summary><![CDATA[Cassini is showing off: well, just a little. NASA is revealing details of information gleamed from a Cassini dive through plumes of vapor as it flies through Enceladus' atmosphere. Enceladus is the icy moon of Saturn. A sub-surface ocean is thought to exist on Enceladus, hightening the possibility that life could exist on the moon. For life to exist (as we know it) 3 ingredients are necessary: liquid water, the right chemical ingredients, and a source of energy for metabloism. Enceladus is thought to have all of these. The article describing this research can be found on <a href="http://www.nasa.gov" rel="noopener">www.nasa.gov</a>, in  "NASA Missions Provide New Insights into 'Ocean Worlds' in Our Solar System", dated April 13, 2017.<br />Also, in another region of our Solar System, the Mars Reconnaissance Orbiter (MRO) is exploring a region called, "Noctis Labyrinthus". MRO has captured a striking image of a mesa, just one of several in the region known as Valles Marineris. The mesa is ~ 0.4 km wide, probably composed of sedimentary deposits that are also eroding. The image is magnificent, and can be found on <a href="https://www.nasa.gov/image-feature/jpl/pia21585/a-mesa-in-noctis-labyrinthus" rel="noopener">https://www.nasa.gov/image-feature/jpl/pia21585/a-mesa-in-noctis-labyrinthus</a>. Another image from MRO shows a hill on Mars, on the South Pole layered deposits. The hill protects the icy layers from erosion, so the image shows the hill with beautiful spiral patterns. In another finding from MRO, over 500 new impact events have been exposed from before and after images of the Southern Middle Latitudes. The new images show shallow sheets of ice that have interested scientists, because ice has not been previously detected on Mars at these latitudes. The scientists hope to better map the ice distribution on Mars, with help from this new data. Staying with Mars, NASA is using the MAVEN spacecraft (Mars Atmosphere and Volatile Evolution) to examine the charged metal atoms that exist high in Mars' whismy upper atmosphere, or ionosphere. This is the first direct detection of atoms like these in a planet other than Earth.  Metallic ions have long lifetimes, so studying these ions can help scientists infer the motion of Mars' ionosphere. With this information, it is hoped scientists can better understand how Mars lost most of its atmosphere, making it the dry, dusty world it is today. Scientists believe that ions exist in the atmospheres of other planets in our Solar System. When other spacecraft have tried to send signals to Earth from locations on other planets, such as Jupiter or Saturn, parts of these signals have sometimes been blocked. Scientists have inferred that the presence of metal ions in the ionospheres of these other planets have been responsible for the signal blockage, but no direct proof of this has been offered. Another curious find on Mars was that the metal ions in Mars' ionosphere behave differently than the ions in Earth's ionoshpere. This could be due to the presence of a magnetosphere on Earth, and a lack of one on Mars. Scientists with MAVEN are also trying to learn about the formation of high altitude clouds on Earth and Mars, and what role the ions in the ionospheres have on this phenomenon.]]></itunes:summary><itunes:duration>1416</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>New Horizons and Cassini Missions</title><link>https://www.spreaker.com/episode/new-horizons-and-cassini-missions--23524947</link><description><![CDATA[<a href="http://www.nasa.gov/feature/new-horizons-halfway-from-pluto-to-next-flyby-target" rel="noopener">www.nasa.gov/feature/new-horizons-halfway-from-pluto-to-next-flyby-target</a><br />On April 17, 2016, the New Horizons spacecraft (NH) will have reached its halfway point on its flight from Pluto, to its next target in the Kuiper Belt, 2014 MU69 (486.19 million miles from Pluto). When NH does reach 2014 NMU69, it will become the most distant world ever explored in our Solar System. NH is actually slowly down slightly due to the gravitational pull of the Sun. It will therefore reach its midpoint in distance 5 days before it reaches its midpoint in time. And, to add more intrigue to this unfolding drama, NH will also be asleep on April 7, before it reaches the midpoint. This will be done to preserve the systems on the spacecraft. The spacedraft will be put in hibernation for 157 days, but it needs the time off. NH would have been "awake" for 1 and 1/2 years, since December 2014. In that time period, NH flew by Pluto, relayed data back to Earth for 16 months, and also studied a dozen other Kuiper Belt Objects (KBOs). The busy little spacecraft has also studied the outer reaches of the heliosphere (the Sun's atmosphere), and the Kuiper Belt's dusty, ionicly charged environment. Another interesting fact: a signal sent between NH and Earth takes 5 hours and 20 minutes (at the speed of light)  to travel the  3.5 billion mile distance between Earth and the New Horizons spacecraft. Now, off to Saturn. Cassini is preparing for its Grand Finale at Saturn, where it will dive between Saturn and its rings, then burn up in Saturn's atmosphere. It will actually go through a total of 22 dives before its grand finale. Cassini has been in the Saturn system for 13 years, and since then it has learned much about things like the moon Enceldus, its icy surface, and its sub-surface ocean, and also about the moon Titan, and its liquid methane seas. With the ocean of information it has gained in this 13 years, mission scientists are using all this information to make the final dive very purposeful. During the final plunge, Cassini will sample Saturn`s atmosphere, sample particles from the rings, and relay back to Earth the closest ever pictures of Saturn, its clouds, and its inner rings. The duties that the robotic probe on Cassini will be assinged to undertake will be downloaded to the probe in what is called a sequence, on April 11. Cassini will study the moon Titan one last time, on April 22, then will carry out other experiments, all in anticipation for its grand finale dive on September 15. This will truly be the end of something special, as Cassini has given the scientists at the Jet Propulsion Laboratory (JPL), anc citizen astronomers, more than they could have ever hoped for.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-April-06-15-01-19.mp3</guid><pubDate>Thu, 06 Apr 2017 22:01:19 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524947/astrotalk_april_06_15_01_19.mp3" length="27440274" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>www.nasa.gov/feature/new-horizons-halfway-from-pluto-to-next-flyby-target
On April 17, 2016, the New Horizons spacecraft (NH) will have reached its halfway point on its flight from Pluto, to its next target in the Kuiper Belt, 2014 MU69 (486.19...</itunes:subtitle><itunes:summary><![CDATA[<a href="http://www.nasa.gov/feature/new-horizons-halfway-from-pluto-to-next-flyby-target" rel="noopener">www.nasa.gov/feature/new-horizons-halfway-from-pluto-to-next-flyby-target</a><br />On April 17, 2016, the New Horizons spacecraft (NH) will have reached its halfway point on its flight from Pluto, to its next target in the Kuiper Belt, 2014 MU69 (486.19 million miles from Pluto). When NH does reach 2014 NMU69, it will become the most distant world ever explored in our Solar System. NH is actually slowly down slightly due to the gravitational pull of the Sun. It will therefore reach its midpoint in distance 5 days before it reaches its midpoint in time. And, to add more intrigue to this unfolding drama, NH will also be asleep on April 7, before it reaches the midpoint. This will be done to preserve the systems on the spacecraft. The spacedraft will be put in hibernation for 157 days, but it needs the time off. NH would have been "awake" for 1 and 1/2 years, since December 2014. In that time period, NH flew by Pluto, relayed data back to Earth for 16 months, and also studied a dozen other Kuiper Belt Objects (KBOs). The busy little spacecraft has also studied the outer reaches of the heliosphere (the Sun's atmosphere), and the Kuiper Belt's dusty, ionicly charged environment. Another interesting fact: a signal sent between NH and Earth takes 5 hours and 20 minutes (at the speed of light)  to travel the  3.5 billion mile distance between Earth and the New Horizons spacecraft. Now, off to Saturn. Cassini is preparing for its Grand Finale at Saturn, where it will dive between Saturn and its rings, then burn up in Saturn's atmosphere. It will actually go through a total of 22 dives before its grand finale. Cassini has been in the Saturn system for 13 years, and since then it has learned much about things like the moon Enceldus, its icy surface, and its sub-surface ocean, and also about the moon Titan, and its liquid methane seas. With the ocean of information it has gained in this 13 years, mission scientists are using all this information to make the final dive very purposeful. During the final plunge, Cassini will sample Saturn`s atmosphere, sample particles from the rings, and relay back to Earth the closest ever pictures of Saturn, its clouds, and its inner rings. The duties that the robotic probe on Cassini will be assinged to undertake will be downloaded to the probe in what is called a sequence, on April 11. Cassini will study the moon Titan one last time, on April 22, then will carry out other experiments, all in anticipation for its grand finale dive on September 15. This will truly be the end of something special, as Cassini has given the scientists at the Jet Propulsion Laboratory (JPL), anc citizen astronomers, more than they could have ever hoped for.]]></itunes:summary><itunes:duration>1716</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>A Lost Planet the Size of Neptune and Exoplanets Kepler A B C D E, and a Caldera on the Moon</title><link>https://www.spreaker.com/episode/a-lost-planet-the-size-of-neptune-and-exoplanets-kepler-a-b-c-d-e-and-a-caldera-on-the-moon--23525005</link><description><![CDATA[Astronomers at Yale have discovered a lost planet about the size of Neptune, in a solar system 3,000 light-years from Earth.  Kepler-150 was overlooked for several years, probably because of its long orbit. The planet takes 637 Earth days to make 1 orbit around its star. This is probably the longest orbit of any planet that is in a 5 (or more) planet system. The other planets in the system, Kepler A B C & D were identified several years ago. Their orbits are much shorter.  Kepler 150's orbit was harder to tease out, because it was hiding in the orbits of its sister planets. The oribtal signatures of the other 4 planets had to be subtracted out before Kepler 150's orbit could be nailed down. Switching to our beloved Moon now. Scientists at Brown University are studying the suignature of the aftermath of a volacno on the Moon called Ina.  Previously, the eruption was thought to have taken place within the past 100 million years, 1 Billion years after volcanic activity on the Moon was thought to have ended. A caldera the sicentists are studying is testing everyone's theories. The caldera is much lighter than the surrounding area in which it lies, leading some scientists to speculate that this caldera is much younger than its surroundings. Because the caldera is much lighter, there is specualtion that it has not had as much time to collect the surrounding regolith, which is the layer of darker rock that accumulates over time. The 80 or so smooth rocks inside of Ina also confuses the issue. The lack of iimpact craters on these smooth hills also suggest Ina is younger the surrounding area, which has many more signs of impact. In their science, other astronomers used the amount of impact cratering in Ina to estimagte that the area saw volcanic activity 50 - 100 million years ago. But the scientists at Brown dispute these ideas. They compared Ina to Hawaii's Kilauea volcano in Hawai, and the aftermaths there from a 1959 eruption. In the Kilauea volcano, lava from the eruption solidified, then created a highly porous rock layer. This same process was thought to occur inside Ina's caldera, and it is this highly porous rock layer the Brown scientists say is responsible for hiding the amount of regolith in Ina. The porosity of the rock layer throws off the count of the craters, and is responsible for the caldera's relatively light color.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-March-30-15-12-30.mp3</guid><pubDate>Thu, 30 Mar 2017 22:12:01 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525005/astrotalk_march_30_15_12_30.mp3" length="14079791" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Astronomers at Yale have discovered a lost planet about the size of Neptune, in a solar system 3,000 light-years from Earth.  Kepler-150 was overlooked for several years, probably because of its long orbit. The planet takes 637 Earth days to make 1...</itunes:subtitle><itunes:summary><![CDATA[Astronomers at Yale have discovered a lost planet about the size of Neptune, in a solar system 3,000 light-years from Earth.  Kepler-150 was overlooked for several years, probably because of its long orbit. The planet takes 637 Earth days to make 1 orbit around its star. This is probably the longest orbit of any planet that is in a 5 (or more) planet system. The other planets in the system, Kepler A B C & D were identified several years ago. Their orbits are much shorter.  Kepler 150's orbit was harder to tease out, because it was hiding in the orbits of its sister planets. The oribtal signatures of the other 4 planets had to be subtracted out before Kepler 150's orbit could be nailed down. Switching to our beloved Moon now. Scientists at Brown University are studying the suignature of the aftermath of a volacno on the Moon called Ina.  Previously, the eruption was thought to have taken place within the past 100 million years, 1 Billion years after volcanic activity on the Moon was thought to have ended. A caldera the sicentists are studying is testing everyone's theories. The caldera is much lighter than the surrounding area in which it lies, leading some scientists to speculate that this caldera is much younger than its surroundings. Because the caldera is much lighter, there is specualtion that it has not had as much time to collect the surrounding regolith, which is the layer of darker rock that accumulates over time. The 80 or so smooth rocks inside of Ina also confuses the issue. The lack of iimpact craters on these smooth hills also suggest Ina is younger the surrounding area, which has many more signs of impact. In their science, other astronomers used the amount of impact cratering in Ina to estimagte that the area saw volcanic activity 50 - 100 million years ago. But the scientists at Brown dispute these ideas. They compared Ina to Hawaii's Kilauea volcano in Hawai, and the aftermaths there from a 1959 eruption. In the Kilauea volcano, lava from the eruption solidified, then created a highly porous rock layer. This same process was thought to occur inside Ina's caldera, and it is this highly porous rock layer the Brown scientists say is responsible for hiding the amount of regolith in Ina. The porosity of the rock layer throws off the count of the craters, and is responsible for the caldera's relatively light color.]]></itunes:summary><itunes:duration>880</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Nothing but music here</title><link>https://www.spreaker.com/episode/nothing-but-music-here--23524955</link><description><![CDATA[Nothing but music here]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-March-23-15-00-00.mp3</guid><pubDate>Thu, 23 Mar 2017 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524955/astrotalk_march_23_15_00_00.mp3" length="28816196" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Nothing but music here</itunes:subtitle><itunes:summary><![CDATA[Nothing but music here]]></itunes:summary><itunes:duration>1802</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Fundrive</title><link>https://www.spreaker.com/episode/fundrive--23524965</link><description><![CDATA[Fundrive]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-March-16-15-00-00.mp3</guid><pubDate>Thu, 16 Mar 2017 22:06:35 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524965/astrotalk_march_16_15_00_00.mp3" length="20128078" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Fundrive</itunes:subtitle><itunes:summary><![CDATA[Fundrive]]></itunes:summary><itunes:duration>1258</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Glutinous Star May Hold Clues To Planet Formation</title><link>https://www.spreaker.com/episode/glutinous-star-may-hold-clues-to-planet-formation--23524893</link><description><![CDATA[The young star FU Orionis suddenly began devouring material from the gas and dust surrounding it, in 1936. Over a 3 month super-binge, the star flared up 100 times brighter, and its termperature rose to 7,000 degrees Kelvin. Since 1936, FU Ornionis has continued to gobble up surrounding gas, but not at quite the same rate. The star is roughly the size of our Sun, and to this point, FU Ornionis has reached the point of being the brightest young star ever seen, for a star the size of our Sun. Scientists are now trying to figure out what the implications of this sudde4n heating is for how planets form. The chemistry of FU Orionis is thought to have changed with its heating, so the material in the disk that would make up planets also changed. Scientists believe this look at FU Orionis is just like looking back at the younger, formative, or baby years of the formation of our solar system. The intense baking of the star's surrounding disk likely changed its chemistry, permanently altering material that could one day turn into planets.  Our solar system could have gone through a similar brightening change when it was forming. Scientists will now turn to studying FU Orionis at infrared wavelengths, to gather more data about this Sun-like star. Over the past years, FU O has devoured or eaten the equivalent weight of 80 Jupiters (or about 8,000 Earths). Scientists estimate that FU O will continue to snack on surrounding gas and dust for a few hundred more years, before it returns to its pre-1936 brightening level. The amount of visible and infrred light energy coming from FU O has decreased by 13% over the past 1 2 years.  The dimming is thought to have occurred at shorter infrared wavelengths, not at longer wavelengths. This implies that 13% of the hotter material material has disappeared, while colder material remains, so it seems that only the inner part of the proto-lanetary disk has been eaten by FU O. The colder outer part has remained intact. This could have tremendous implications for how planets closer of farther from a star, like Earth or Mars, could have formed, or could have been influenced. The heating of the disk, and the changing of its chemical compositon at certain distances out from a star, could help explain the relative abundance of certain elements on Earth as opposed to Mars, or vice versa. FU Orionis is 1,500 light years from Earth, in the constellation of Orion.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-March-09-15-00-00.mp3</guid><pubDate>Thu, 09 Mar 2017 22:05:39 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524893/astrotalk_march_09_15_00_00.mp3" length="19904052" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The young star FU Orionis suddenly began devouring material from the gas and dust surrounding it, in 1936. Over a 3 month super-binge, the star flared up 100 times brighter, and its termperature rose to 7,000 degrees Kelvin. Since 1936, FU Ornionis...</itunes:subtitle><itunes:summary><![CDATA[The young star FU Orionis suddenly began devouring material from the gas and dust surrounding it, in 1936. Over a 3 month super-binge, the star flared up 100 times brighter, and its termperature rose to 7,000 degrees Kelvin. Since 1936, FU Ornionis has continued to gobble up surrounding gas, but not at quite the same rate. The star is roughly the size of our Sun, and to this point, FU Ornionis has reached the point of being the brightest young star ever seen, for a star the size of our Sun. Scientists are now trying to figure out what the implications of this sudde4n heating is for how planets form. The chemistry of FU Orionis is thought to have changed with its heating, so the material in the disk that would make up planets also changed. Scientists believe this look at FU Orionis is just like looking back at the younger, formative, or baby years of the formation of our solar system. The intense baking of the star's surrounding disk likely changed its chemistry, permanently altering material that could one day turn into planets.  Our solar system could have gone through a similar brightening change when it was forming. Scientists will now turn to studying FU Orionis at infrared wavelengths, to gather more data about this Sun-like star. Over the past years, FU O has devoured or eaten the equivalent weight of 80 Jupiters (or about 8,000 Earths). Scientists estimate that FU O will continue to snack on surrounding gas and dust for a few hundred more years, before it returns to its pre-1936 brightening level. The amount of visible and infrred light energy coming from FU O has decreased by 13% over the past 1 2 years.  The dimming is thought to have occurred at shorter infrared wavelengths, not at longer wavelengths. This implies that 13% of the hotter material material has disappeared, while colder material remains, so it seems that only the inner part of the proto-lanetary disk has been eaten by FU O. The colder outer part has remained intact. This could have tremendous implications for how planets closer of farther from a star, like Earth or Mars, could have formed, or could have been influenced. The heating of the disk, and the changing of its chemical compositon at certain distances out from a star, could help explain the relative abundance of certain elements on Earth as opposed to Mars, or vice versa. FU Orionis is 1,500 light years from Earth, in the constellation of Orion.]]></itunes:summary><itunes:duration>1244</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Pre-emption</title><link>https://www.spreaker.com/episode/pre-emption--23525012</link><description><![CDATA[Pre-emption from Vancouver Convention Centre East Ballrooom]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-March-02-15-00-00.mp3</guid><pubDate>Thu, 02 Mar 2017 22:01:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525012/astrotalk_march_02_15_00_00.mp3" length="28816196" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Pre-emption from Vancouver Convention Centre East Ballrooom</itunes:subtitle><itunes:summary><![CDATA[Pre-emption from Vancouver Convention Centre East Ballrooom]]></itunes:summary><itunes:duration>1802</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Blazars In The Early Universe</title><link>https://www.spreaker.com/episode/blazars-in-the-early-universe--23524959</link><description><![CDATA[Blazars are very compact quasars (quasi-stellar radio sources) that are associated with presumed supermassive black holes. They are located at the center of  active, giant elliptical galaxies. Blazars are among the most energetic phenomena in the universe. Scientists working with NASA's Fermi Gamma Ray Telescope have detected a blazar that breaks the record for the most distant blazar ever detected. The previous record holder sent its light toward Earth when the universe was only 2.1 Billion years old, but this newly discovered blazar breaks that record. Its light started coming toward Earth when the universe was only 1.4 Billion years old. In this galaxy, light and matter is pulled toward the central black hole, then gathers in an accretion disk, like cars gather on a road in a traffic jam. The matter heats up, and when the matter falls into toward the black hole, a small amount of it gathers and gets redirected into 2 particle jets, which shoot the matter out in opposite directions, along the central axis of rotation of the galaxy. When either of these jets is direct into the direction of the the Earth, then scientists can detect the jet. The energy output of the accretion disk has the output equivalent to 2 trillion times the energy output of our Sun. Scientists are surprised that a massive black hole such as this one, which is billions times the mass of our Sun, could have formed at such an early stage in our early universe. They are now trying to determine what caused the rapid development of this black hole. Scientists also detected 4 other blazars which appeared on a time scale when our universe was only 1.4 - 1.9 billion years old. Two of these blazars are powered by black holes that have the mass of more than 1 billion Suns. The detection of these blazars, at such an early stage in the universe, challenges some of the models that n ow describe how black holes formed and grow.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-February-02-15-00-00.mp3</guid><pubDate>Thu, 02 Feb 2017 22:10:48 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524959/astrotalk_february_02_15_00_00.mp3" length="17088261" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Blazars are very compact quasars (quasi-stellar radio sources) that are associated with presumed supermassive black holes. They are located at the center of  active, giant elliptical galaxies. Blazars are among the most energetic phenomena in the...</itunes:subtitle><itunes:summary><![CDATA[Blazars are very compact quasars (quasi-stellar radio sources) that are associated with presumed supermassive black holes. They are located at the center of  active, giant elliptical galaxies. Blazars are among the most energetic phenomena in the universe. Scientists working with NASA's Fermi Gamma Ray Telescope have detected a blazar that breaks the record for the most distant blazar ever detected. The previous record holder sent its light toward Earth when the universe was only 2.1 Billion years old, but this newly discovered blazar breaks that record. Its light started coming toward Earth when the universe was only 1.4 Billion years old. In this galaxy, light and matter is pulled toward the central black hole, then gathers in an accretion disk, like cars gather on a road in a traffic jam. The matter heats up, and when the matter falls into toward the black hole, a small amount of it gathers and gets redirected into 2 particle jets, which shoot the matter out in opposite directions, along the central axis of rotation of the galaxy. When either of these jets is direct into the direction of the the Earth, then scientists can detect the jet. The energy output of the accretion disk has the output equivalent to 2 trillion times the energy output of our Sun. Scientists are surprised that a massive black hole such as this one, which is billions times the mass of our Sun, could have formed at such an early stage in our early universe. They are now trying to determine what caused the rapid development of this black hole. Scientists also detected 4 other blazars which appeared on a time scale when our universe was only 1.4 - 1.9 billion years old. Two of these blazars are powered by black holes that have the mass of more than 1 billion Suns. The detection of these blazars, at such an early stage in the universe, challenges some of the models that n ow describe how black holes formed and grow.]]></itunes:summary><itunes:duration>1069</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Gravity, Pluto, Saturn and Monster Black Holes</title><link>https://www.spreaker.com/episode/gravity-pluto-saturn-and-monster-black-holes--23524969</link><description><![CDATA[A discussion about gravity. Do earthquakes occur more often when the Moon is in its nearest orbit to the Earth? Some scientists think so. When the Moon is closest to the Earth, its gravity is 20 % stronger than when it is at its furthest point from the Earth. Some scientists believe when the Moon is at its closest to Earth, it tugs on fault lines and initiates earthquakes. Some scientists are also speculate that if an asteroid or meteor were captured, and then put in orbit around Earth, it could tug Earth further away from the Sun. This would be useful when the Sun expands, and then makes it too hot to live on Earth. Einstein's analysis of gravity and space time is also discussed. All these three topics have to do with gravity. New images of Pluto keep coming in, adding more data to Pluto's file. In the picture discussed, Pluto's surface resembles that of the Moon, with craters, uplands and valleys. A stunning picture of Saturn is also discussed. Scientists could never get this type of shot of Saturn's rings. It is taken from the Cassini spacecraft now in orbit around Saturn. The photo was taken with Cassini's Wide Angle Camera on October 28, 2016, in violet light. The photo is on the dim, sunlit side of Saturn, at a ring angle of about 25 degrees. A previously hidden  black hole in NGC 1448 in an active galactic nuclei AGN is also featured. Gas and dust would usually hide this image, but this black hole gives itself away by emitting X-rays. The rays come from the black hole feeding on material behind the cloak of the gas and dust. The  NUStar Telescope is able to detect the x-rays coming from area around this black hole. This black hole is super massive, weighing in at million times the mass of the Sun. An AGN is super bright,  emitting light across the full electromagnetic spectrum. IC 3639, a galaxy with another sumpermassive black hole,  is also being examined by these astronomers. Its light is detected beyond its obscuring gas and dust with NUStar. Both these galaxies are described as monsters or ogres under our bed, because we cannot see them, unless we use NUStar, of course.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2017/AstroTalk-January-19-15-00-00.mp3</guid><pubDate>Thu, 19 Jan 2017 22:02:41 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524969/astrotalk_january_19_15_00_00.mp3" length="25088000" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>A discussion about gravity. Do earthquakes occur more often when the Moon is in its nearest orbit to the Earth? Some scientists think so. When the Moon is closest to the Earth, its gravity is 20 % stronger than when it is at its furthest point from...</itunes:subtitle><itunes:summary><![CDATA[A discussion about gravity. Do earthquakes occur more often when the Moon is in its nearest orbit to the Earth? Some scientists think so. When the Moon is closest to the Earth, its gravity is 20 % stronger than when it is at its furthest point from the Earth. Some scientists believe when the Moon is at its closest to Earth, it tugs on fault lines and initiates earthquakes. Some scientists are also speculate that if an asteroid or meteor were captured, and then put in orbit around Earth, it could tug Earth further away from the Sun. This would be useful when the Sun expands, and then makes it too hot to live on Earth. Einstein's analysis of gravity and space time is also discussed. All these three topics have to do with gravity. New images of Pluto keep coming in, adding more data to Pluto's file. In the picture discussed, Pluto's surface resembles that of the Moon, with craters, uplands and valleys. A stunning picture of Saturn is also discussed. Scientists could never get this type of shot of Saturn's rings. It is taken from the Cassini spacecraft now in orbit around Saturn. The photo was taken with Cassini's Wide Angle Camera on October 28, 2016, in violet light. The photo is on the dim, sunlit side of Saturn, at a ring angle of about 25 degrees. A previously hidden  black hole in NGC 1448 in an active galactic nuclei AGN is also featured. Gas and dust would usually hide this image, but this black hole gives itself away by emitting X-rays. The rays come from the black hole feeding on material behind the cloak of the gas and dust. The  NUStar Telescope is able to detect the x-rays coming from area around this black hole. This black hole is super massive, weighing in at million times the mass of the Sun. An AGN is super bright,  emitting light across the full electromagnetic spectrum. IC 3639, a galaxy with another sumpermassive black hole,  is also being examined by these astronomers. Its light is detected beyond its obscuring gas and dust with NUStar. Both these galaxies are described as monsters or ogres under our bed, because we cannot see them, unless we use NUStar, of course.]]></itunes:summary><itunes:duration>1568</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>A New Home On Mars and Hubble Spies a Megmaser</title><link>https://www.spreaker.com/episode/a-new-home-on-mars-and-hubble-spies-a-megmaser--23524979</link><description><![CDATA[NASA ran a contest for scientists to design a futuristic home on Mars for astronauts to live in. Instead of digging a hole in the ground and living beneath the surface, a revolutionary design, called a Ice Home, took home the prize. When astronauts do eventually set foot on Mars, one of the most important considerations will be, where will they live? A novel, new design of an ice home is now being talked about. Guarding against space radiation will be critical, because Mars' atmosphere is practically non-existent. To guard against space radiation, which Earth's atmosphere does for us here on Earth, astronauts must live in a radiative protective environment. The Ice Home can provide this environment. The Ice Home  is envisioned as a large inflatable torus, that would be surrounded by a shell of water ice. Another shell of carbon dioxide gas would be placed inside the layer of water ice, to provide the necessary heat. The water ice shell would serve as a good protector against space radiation, because water, naturally, contains hydrogen, and hydrogen does an excellent job of protecting against cosmic rays. And both water and carbon dioxide are readily available on Mars. The Ice Home has several advantages. Water can be let out, so it can be easily deflated, and then moved. Water that is extracted from the Ice Home can then be converted to rocket fuel. The Ice Home therefore looks promising. <br />Hubble also keeps doing its magnificent work by letting us look at a Cosmic Megamaser, in a galaxy that is 370 million light years away. Instead of the typical visible laser light that we know here on Earth, the Galaxy IRAS 16399 is emitting microwave type light, hence the name maser. The galaxy has a double nucleus, and one of the nuclei sport a black hole that weighs in at 100 million times the mass of the Sun. The megamaser galaxy is extremely bright, so the galaxy is essentially acting as an astronomical laser that beams out microwave emission. Lasers are set so that a majority of the excited radiation exists above its ground state energy, and can thus be made to oscillate in unison, and then be amplified. The gas clouds in this galaxy are essentially replicating this process, but with microwave radiation, rather than visible light. Hence the name maser, or megamaser.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-December-29-15-00-00.mp3</guid><pubDate>Thu, 29 Dec 2016 22:06:46 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524979/astrotalk_december_29_15_00_00.mp3" length="24272143" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>NASA ran a contest for scientists to design a futuristic home on Mars for astronauts to live in. Instead of digging a hole in the ground and living beneath the surface, a revolutionary design, called a Ice Home, took home the prize. When astronauts do...</itunes:subtitle><itunes:summary><![CDATA[NASA ran a contest for scientists to design a futuristic home on Mars for astronauts to live in. Instead of digging a hole in the ground and living beneath the surface, a revolutionary design, called a Ice Home, took home the prize. When astronauts do eventually set foot on Mars, one of the most important considerations will be, where will they live? A novel, new design of an ice home is now being talked about. Guarding against space radiation will be critical, because Mars' atmosphere is practically non-existent. To guard against space radiation, which Earth's atmosphere does for us here on Earth, astronauts must live in a radiative protective environment. The Ice Home can provide this environment. The Ice Home  is envisioned as a large inflatable torus, that would be surrounded by a shell of water ice. Another shell of carbon dioxide gas would be placed inside the layer of water ice, to provide the necessary heat. The water ice shell would serve as a good protector against space radiation, because water, naturally, contains hydrogen, and hydrogen does an excellent job of protecting against cosmic rays. And both water and carbon dioxide are readily available on Mars. The Ice Home has several advantages. Water can be let out, so it can be easily deflated, and then moved. Water that is extracted from the Ice Home can then be converted to rocket fuel. The Ice Home therefore looks promising. <br />Hubble also keeps doing its magnificent work by letting us look at a Cosmic Megamaser, in a galaxy that is 370 million light years away. Instead of the typical visible laser light that we know here on Earth, the Galaxy IRAS 16399 is emitting microwave type light, hence the name maser. The galaxy has a double nucleus, and one of the nuclei sport a black hole that weighs in at 100 million times the mass of the Sun. The megamaser galaxy is extremely bright, so the galaxy is essentially acting as an astronomical laser that beams out microwave emission. Lasers are set so that a majority of the excited radiation exists above its ground state energy, and can thus be made to oscillate in unison, and then be amplified. The gas clouds in this galaxy are essentially replicating this process, but with microwave radiation, rather than visible light. Hence the name maser, or megamaser.]]></itunes:summary><itunes:duration>1518</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Blankets for Space and Interstellar Travel</title><link>https://www.spreaker.com/episode/blankets-for-space-and-interstellar-travel--23525020</link><description><![CDATA[Meet Liem Pham, a spacecraft dressmaker for NASA. Pham makes the blankets that must cover every NASA vehicle before it is sent into space. Pham started at NASA 19 years ago, putting cables in the Cassini spacecraft. After 3 years of this, she was hired on to make the blankets that must cover every NASA vehicle before it is launched. Pham is part of the Flight Technician Services group, a group that contributes to all stages of spacecraft assembly. Pham constructs blankets from different materials, for all kinds of different uses. Blankets can be made a carbon type material called Kapton, which is used for a charged environment, to dissipate the charge on a space vehicle. She also makes blankets with materials such as Teflon, or Mylar netting with Dacron films. Work done by Pham is just another example of an integral part of the process of getting spaceships off the ground.<br />Interstellar travel, or interstellar space exploration, is occupying the minds of many scientists. Voyager 1 is now in interstellar space, but it took 36 years to get there. Voyager 1 is so low on energy though, so it does not have the capacity to do much science while it is in interstellar space. The faint signal that scientists on Earth are receiving from Voyager has the power of a refrigerator light bulb, or about 20 watts. Scientists are now hoping they can develop technology where they can get probes to interstellar space in a 10 year time frame, and then have the probes "live" in interstellar space so that they could do some science while there. Scientists also hope that these probes can visit some Kuiper Belt objects, like dwarf planets, on their way to interstellar space. Scientists are also dreaming up ideas of sending humans to interstellar space, or even to the nearest star system, Alpha Centauri, which is 4.3 light-years away. Hibernation experiments are now being dreamt up, where humans would be put into a state of hibernation on these long voyages. To do all these things, humans would have to develop exotic technology, because our present chemical-jet-fuel based propulsion systems can get us nowhere near to interstellar space or the next star system, because they do not have the ability to propel a space anywhere near a fraction of the speed of light that would be required to get us there.<br />Exotic, futuristic telescope systems are also being thought up. These would use the gravitational lensing properties of the Sun to magnify a distant star or planet, to the point that we could make out surface features on these objects. Pretty heady stuff.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-December-22-15-15-00.mp3</guid><pubDate>Thu, 22 Dec 2016 22:13:12 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525020/astrotalk_december_22_15_15_00.mp3" length="45231960" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Meet Liem Pham, a spacecraft dressmaker for NASA. Pham makes the blankets that must cover every NASA vehicle before it is sent into space. Pham started at NASA 19 years ago, putting cables in the Cassini spacecraft. After 3 years of this, she was...</itunes:subtitle><itunes:summary><![CDATA[Meet Liem Pham, a spacecraft dressmaker for NASA. Pham makes the blankets that must cover every NASA vehicle before it is sent into space. Pham started at NASA 19 years ago, putting cables in the Cassini spacecraft. After 3 years of this, she was hired on to make the blankets that must cover every NASA vehicle before it is launched. Pham is part of the Flight Technician Services group, a group that contributes to all stages of spacecraft assembly. Pham constructs blankets from different materials, for all kinds of different uses. Blankets can be made a carbon type material called Kapton, which is used for a charged environment, to dissipate the charge on a space vehicle. She also makes blankets with materials such as Teflon, or Mylar netting with Dacron films. Work done by Pham is just another example of an integral part of the process of getting spaceships off the ground.<br />Interstellar travel, or interstellar space exploration, is occupying the minds of many scientists. Voyager 1 is now in interstellar space, but it took 36 years to get there. Voyager 1 is so low on energy though, so it does not have the capacity to do much science while it is in interstellar space. The faint signal that scientists on Earth are receiving from Voyager has the power of a refrigerator light bulb, or about 20 watts. Scientists are now hoping they can develop technology where they can get probes to interstellar space in a 10 year time frame, and then have the probes "live" in interstellar space so that they could do some science while there. Scientists also hope that these probes can visit some Kuiper Belt objects, like dwarf planets, on their way to interstellar space. Scientists are also dreaming up ideas of sending humans to interstellar space, or even to the nearest star system, Alpha Centauri, which is 4.3 light-years away. Hibernation experiments are now being dreamt up, where humans would be put into a state of hibernation on these long voyages. To do all these things, humans would have to develop exotic technology, because our present chemical-jet-fuel based propulsion systems can get us nowhere near to interstellar space or the next star system, because they do not have the ability to propel a space anywhere near a fraction of the speed of light that would be required to get us there.<br />Exotic, futuristic telescope systems are also being thought up. These would use the gravitational lensing properties of the Sun to magnify a distant star or planet, to the point that we could make out surface features on these objects. Pretty heady stuff.]]></itunes:summary><itunes:duration>2827</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Are We Alone? John Glenn</title><link>https://www.spreaker.com/episode/are-we-alone-john-glenn--23524988</link><description><![CDATA[The Star Wars series has thrilled us with intriguing worlds like the ice planet Toth, or even Luke Skywalker's desert planet of Tattooine. These planets have also intrigued scientists, as many scientists who have discovered actual worlds similar to Toth or Tattooine have now taken to nicknaming their exoplanet discoveries after the Star Wars worlds. Kepler 16-b is 200 light years away, and it is a Saturn-sized planet that orbits a star in the constellation Cygnus. This planet orbits in a double star system, so if a person were on Kepler 16-b, they would see a double sunset, just like Luke saw on his home planet of Tattooine. A person on Kepler 16-b would have 2 shadows, and would also see two suns set every day. Planet OGLE 2005-BLG-390L, discovered in 2006, resembles the ice planet Toth, featured on the second Star Wars movie, so scientists have nicknamed it Toth. Scientists also believe that desert worlds, ice worlds or water worlds exist in abundance in our galaxy, and they also believe some of these planets may harbour life. With the launch of The James Webb Space Telescope, the W-First Telescope, and also the Transiting Exoplanet Survey Satellite (TESS), scientists believe that they can prove whether or not the planets they find are ice worlds, water worlds or desert worlds. <br />Also, John Glenn, the first US astronaut sent into space, passed away last week. In 1962, Glenn launched into space aboard a Friendship 7 spacecraft. Glenn was also the oldest person to ever launch into space, aboard the space shuttle Discovery on October 29, 1998. At that time, Glenn was 77 years old. Glenn was also one of the original crew members for the Mercury series of launches. Glenn loved meeting with the public, and especially children, to talk about NASA and his career as an astronaut. John Glenn was 95.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-December-15-15-00-00.mp3</guid><pubDate>Thu, 15 Dec 2016 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524988/astrotalk_december_15_15_00_00.mp3" length="43215725" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The Star Wars series has thrilled us with intriguing worlds like the ice planet Toth, or even Luke Skywalker's desert planet of Tattooine. These planets have also intrigued scientists, as many scientists who have discovered actual worlds similar to...</itunes:subtitle><itunes:summary><![CDATA[The Star Wars series has thrilled us with intriguing worlds like the ice planet Toth, or even Luke Skywalker's desert planet of Tattooine. These planets have also intrigued scientists, as many scientists who have discovered actual worlds similar to Toth or Tattooine have now taken to nicknaming their exoplanet discoveries after the Star Wars worlds. Kepler 16-b is 200 light years away, and it is a Saturn-sized planet that orbits a star in the constellation Cygnus. This planet orbits in a double star system, so if a person were on Kepler 16-b, they would see a double sunset, just like Luke saw on his home planet of Tattooine. A person on Kepler 16-b would have 2 shadows, and would also see two suns set every day. Planet OGLE 2005-BLG-390L, discovered in 2006, resembles the ice planet Toth, featured on the second Star Wars movie, so scientists have nicknamed it Toth. Scientists also believe that desert worlds, ice worlds or water worlds exist in abundance in our galaxy, and they also believe some of these planets may harbour life. With the launch of The James Webb Space Telescope, the W-First Telescope, and also the Transiting Exoplanet Survey Satellite (TESS), scientists believe that they can prove whether or not the planets they find are ice worlds, water worlds or desert worlds. <br />Also, John Glenn, the first US astronaut sent into space, passed away last week. In 1962, Glenn launched into space aboard a Friendship 7 spacecraft. Glenn was also the oldest person to ever launch into space, aboard the space shuttle Discovery on October 29, 1998. At that time, Glenn was 77 years old. Glenn was also one of the original crew members for the Mercury series of launches. Glenn loved meeting with the public, and especially children, to talk about NASA and his career as an astronaut. John Glenn was 95.]]></itunes:summary><itunes:duration>2701</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Food In Space</title><link>https://www.spreaker.com/episode/food-in-space--23525026</link><description><![CDATA[NASA is working with food scientists like Takiyah Simons and Jessica Vos to develop breakfast bars that are nutritious and filling, but also light enough so that they will not burden a space craft with too much weight on any potential long flight mission to Mars. Astronauts on the International Space Station (ISS) have a great choice from among 200 foods, but on long flight missions, astronauts cannot count on resupply ships coming to their rescue to bring them this great selection of food. Orion has limited room inside it to accommodate the supplies and food astronauts will need during their missions. Because flights to deep space cannot rely on resupply spacecraft to deliver what astronauts need, and to dispose of trash, the Orion crew will have to take everything they need with them and bring it all back home. Given the distances Orion will travel, teams also must limit Orion’s mass, since a heavier spacecraft requires more fuel and energy to propel it to its ultimate destination.  The Orion spacecraft, which will be counted on to deliver astronauts to Mars, will carry great tasting food bars, with flavours including organge cranberry, for breakfast. Lunch and dinner meals will have more selection, and astros will have a food warmer to heat the food. Still, carrying food for a year long mission on a smallish spacecraft is a challenge NASA is looking to conquer.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-December-08-15-00-00.mp3</guid><pubDate>Thu, 08 Dec 2016 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525026/astrotalk_december_08_15_00_00.mp3" length="28816196" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>NASA is working with food scientists like Takiyah Simons and Jessica Vos to develop breakfast bars that are nutritious and filling, but also light enough so that they will not burden a space craft with too much weight on any potential long flight...</itunes:subtitle><itunes:summary><![CDATA[NASA is working with food scientists like Takiyah Simons and Jessica Vos to develop breakfast bars that are nutritious and filling, but also light enough so that they will not burden a space craft with too much weight on any potential long flight mission to Mars. Astronauts on the International Space Station (ISS) have a great choice from among 200 foods, but on long flight missions, astronauts cannot count on resupply ships coming to their rescue to bring them this great selection of food. Orion has limited room inside it to accommodate the supplies and food astronauts will need during their missions. Because flights to deep space cannot rely on resupply spacecraft to deliver what astronauts need, and to dispose of trash, the Orion crew will have to take everything they need with them and bring it all back home. Given the distances Orion will travel, teams also must limit Orion’s mass, since a heavier spacecraft requires more fuel and energy to propel it to its ultimate destination.  The Orion spacecraft, which will be counted on to deliver astronauts to Mars, will carry great tasting food bars, with flavours including organge cranberry, for breakfast. Lunch and dinner meals will have more selection, and astros will have a food warmer to heat the food. Still, carrying food for a year long mission on a smallish spacecraft is a challenge NASA is looking to conquer.]]></itunes:summary><itunes:duration>1802</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Space Food Bars and a Stellar Circle of Life</title><link>https://www.spreaker.com/episode/space-food-bars-and-a-stellar-circle-of-life--23524956</link><description><![CDATA[NASA is designing breakfast food bars for astronauts for potential long distance space voyages in the future. NASA's Orion spacecraft has limited storage capacity, so it cannot carry all the food supplies astronauts would need on a long voyage. So to save space, NASA is creating nutritious, delicious breakfasts, with an eye toward saving storage space on long space flights. NASA will definitely have to figure out how to grow food for lunch or breakfast on such long range missions.<br />NASA scientists are also viewing a  cloud of dust and gas located 24,000 light years from Earth in Cygnus X-3. The Chandra X-ray telescope is receiving x-ray transmissions from the cloud, and believe the x-rays are coming from a neutron star, or a black hole, consuming a large star.  The cloud is acting like a mirror and is reflecting some of the x-rays toward Earth. Because of this, the cloud has been nicknamed the LITTLE FRIEND. The Little Friend is allowing NASA to more accurately make the distance measurement, but they don't know why the Little Friend is reflecting the x-rays. Most stars are now being formed in the spiral arms of our galaxy, but Cygnus X-3 is not in the spiral arms. It is odd, then, to have star formation in these region. NASA is studying the Little Friend's properties to determine why  they are seeing what they are seeing.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-December-01-15-00-00.mp3</guid><pubDate>Thu, 01 Dec 2016 21:59:41 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524956/astrotalk_december_01_15_00_00.mp3" length="24944222" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>NASA is designing breakfast food bars for astronauts for potential long distance space voyages in the future. NASA's Orion spacecraft has limited storage capacity, so it cannot carry all the food supplies astronauts would need on a long voyage. So to...</itunes:subtitle><itunes:summary><![CDATA[NASA is designing breakfast food bars for astronauts for potential long distance space voyages in the future. NASA's Orion spacecraft has limited storage capacity, so it cannot carry all the food supplies astronauts would need on a long voyage. So to save space, NASA is creating nutritious, delicious breakfasts, with an eye toward saving storage space on long space flights. NASA will definitely have to figure out how to grow food for lunch or breakfast on such long range missions.<br />NASA scientists are also viewing a  cloud of dust and gas located 24,000 light years from Earth in Cygnus X-3. The Chandra X-ray telescope is receiving x-ray transmissions from the cloud, and believe the x-rays are coming from a neutron star, or a black hole, consuming a large star.  The cloud is acting like a mirror and is reflecting some of the x-rays toward Earth. Because of this, the cloud has been nicknamed the LITTLE FRIEND. The Little Friend is allowing NASA to more accurately make the distance measurement, but they don't know why the Little Friend is reflecting the x-rays. Most stars are now being formed in the spiral arms of our galaxy, but Cygnus X-3 is not in the spiral arms. It is odd, then, to have star formation in these region. NASA is studying the Little Friend's properties to determine why  they are seeing what they are seeing.]]></itunes:summary><itunes:duration>1560</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Cassini in Orbit Around Saturn's Rings and Mars Ice Deposits</title><link>https://www.spreaker.com/episode/cassini-in-orbit-around-saturn-s-rings-and-mars-ice-deposits--23524894</link><description><![CDATA[Scientists have determined that the Utopia Planatia region on Mars holds as much water as Lake Superior, the largest of the Great Lakes. The deposits are under a layer of soil, in the form of frozen matter. If the water ice mixture were exposed to the Martian atmosphere, then it would sublime into the atmosphere and be lost. The deposit is thought to be away from the poles, and the tilt of Mars, which varies in cycles of 120,000 years has an effect on the water ice mixture. When the poles are heated during this cycle, then this drives the water-ice towards the equator.<br />The Cassini mission on Saturn is heading for another experiment. In this one, beginning on November 30, the spacecraft will make orbits, at a high tilt to the plane of the rings, in an effort to orbit, and then come close to, the rings of Saturn. The A, B & F rings will be studied in these orbits. The spacecraft will come close enough to the rings so as to be able to sample gas and some small particles from the rings. If the particles are too big, though, they could easily damage the spacecraft, rendering it useless. The A ring is one main target, as scientists want to study the propellers in the A rings. Propellers are the signatures of unknown moonlets. Many of Saturn's smallest moons are thought to originate, and form, inside the rings. The tiny moonlets Pan, Atlas, Pandora and Daphnis are presently orbiting close to the A ring. Because of this, these small moonlets will also be studied, in effort to reveal more of their secrets. The Cassini spacecraft is running low on fuel, so in April 2017, the spacecraft will make a final, daring dive into history, burning up in Saturn's atmosphere. Thank you for all the beautiful pictures, and memories, Cassini.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-November-24-15-00-00.mp3</guid><pubDate>Thu, 24 Nov 2016 22:03:56 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524894/astrotalk_november_24_15_00_00.mp3" length="24656249" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Scientists have determined that the Utopia Planatia region on Mars holds as much water as Lake Superior, the largest of the Great Lakes. The deposits are under a layer of soil, in the form of frozen matter. If the water ice mixture were exposed to the...</itunes:subtitle><itunes:summary><![CDATA[Scientists have determined that the Utopia Planatia region on Mars holds as much water as Lake Superior, the largest of the Great Lakes. The deposits are under a layer of soil, in the form of frozen matter. If the water ice mixture were exposed to the Martian atmosphere, then it would sublime into the atmosphere and be lost. The deposit is thought to be away from the poles, and the tilt of Mars, which varies in cycles of 120,000 years has an effect on the water ice mixture. When the poles are heated during this cycle, then this drives the water-ice towards the equator.<br />The Cassini mission on Saturn is heading for another experiment. In this one, beginning on November 30, the spacecraft will make orbits, at a high tilt to the plane of the rings, in an effort to orbit, and then come close to, the rings of Saturn. The A, B & F rings will be studied in these orbits. The spacecraft will come close enough to the rings so as to be able to sample gas and some small particles from the rings. If the particles are too big, though, they could easily damage the spacecraft, rendering it useless. The A ring is one main target, as scientists want to study the propellers in the A rings. Propellers are the signatures of unknown moonlets. Many of Saturn's smallest moons are thought to originate, and form, inside the rings. The tiny moonlets Pan, Atlas, Pandora and Daphnis are presently orbiting close to the A ring. Because of this, these small moonlets will also be studied, in effort to reveal more of their secrets. The Cassini spacecraft is running low on fuel, so in April 2017, the spacecraft will make a final, daring dive into history, burning up in Saturn's atmosphere. Thank you for all the beautiful pictures, and memories, Cassini.]]></itunes:summary><itunes:duration>1542</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Mercury, Arctic Ice and Saturn's Watercolours</title><link>https://www.spreaker.com/episode/mercury-arctic-ice-and-saturn-s-watercolours--23524901</link><description><![CDATA[Mercury is shrinking. A newly discovered valley on Mercury, close to the Rembrandt Basin, is being studied by NASA scientists. The valley, which is 620 miles long, (longer than the Grand Canyon) is caused by the global contraction of the planet. On Earth, similar valleys are often formed by the pulling apart of lithospheric plates due to plate tectonics. On Mercury, the great valley is thought to have formed from long-wavelength buckling of the planet's outermost shell in response to the global contraction of the planet. Valley formation on Earth is well-known process, but this may the first evidence of similar processes occurring on Mercury.<br />NASA is also monitoring conditions on Earth from satellites orbiting our planet. The Goddard Institute for Spaces Studies in New York  has presented data that suggest the past three Octobers, 2014, 2015 & 2016, have seen the highest global temperatures on record for that month. Global temperatures have been monitored for 136 years, and October 2016 was the second warmest October on our planet for the past 136 years, the warmest October happening in October 2015. The 10 warmest Octobers on record have also been recorded after the year 2,000. Goddard scientists also suggest that the study of trends are more important than just year-to-year data. Data after 2,000 therefore suggest that our planet is, indeed, warming up.<br />Perhaps tied in with these findings are other findings relating to a cyclone in the Arctic. In their monitoring of our planet, NASA scientists have detected the damage done to the ice pack in the Arctic by a cyclone that passed through that region in late December 2015. The cyclone brought a lot of humidity and an increase in air temperature of 10 degrees F to the air over the Arctic. The warm air thinned and shrunk the sea ice cover in the Arctic, at a time when ice there should have been growing stronger and thicker. The warm air from the storm, and the storm itself, compacted the ice pack, pushing it further North. More evidence seems to floating in that our planet is warming up, leading to more loss of ice in the polar regions.<br />NASA also released more images from Saturn, showing a kaleidoscope of water swirl colours painted on the northern pole of Saturn. The hexagon shape is again noted in the images provided, but the main highlight is the colorful representation of the latitudinal bands, which come about from air flowing at different speeds, and at different heights, in Saturn's atmosphere. Many eddies and swirls are also noted where the separate bands meet. Just another fascinating, gorgeous breathtaking image from the planet Saturn.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-November-17-15-00-00.mp3</guid><pubDate>Thu, 17 Nov 2016 21:57:26 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524901/astrotalk_november_17_15_00_00.mp3" length="32239699" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Mercury is shrinking. A newly discovered valley on Mercury, close to the Rembrandt Basin, is being studied by NASA scientists. The valley, which is 620 miles long, (longer than the Grand Canyon) is caused by the global contraction of the planet. On...</itunes:subtitle><itunes:summary><![CDATA[Mercury is shrinking. A newly discovered valley on Mercury, close to the Rembrandt Basin, is being studied by NASA scientists. The valley, which is 620 miles long, (longer than the Grand Canyon) is caused by the global contraction of the planet. On Earth, similar valleys are often formed by the pulling apart of lithospheric plates due to plate tectonics. On Mercury, the great valley is thought to have formed from long-wavelength buckling of the planet's outermost shell in response to the global contraction of the planet. Valley formation on Earth is well-known process, but this may the first evidence of similar processes occurring on Mercury.<br />NASA is also monitoring conditions on Earth from satellites orbiting our planet. The Goddard Institute for Spaces Studies in New York  has presented data that suggest the past three Octobers, 2014, 2015 & 2016, have seen the highest global temperatures on record for that month. Global temperatures have been monitored for 136 years, and October 2016 was the second warmest October on our planet for the past 136 years, the warmest October happening in October 2015. The 10 warmest Octobers on record have also been recorded after the year 2,000. Goddard scientists also suggest that the study of trends are more important than just year-to-year data. Data after 2,000 therefore suggest that our planet is, indeed, warming up.<br />Perhaps tied in with these findings are other findings relating to a cyclone in the Arctic. In their monitoring of our planet, NASA scientists have detected the damage done to the ice pack in the Arctic by a cyclone that passed through that region in late December 2015. The cyclone brought a lot of humidity and an increase in air temperature of 10 degrees F to the air over the Arctic. The warm air thinned and shrunk the sea ice cover in the Arctic, at a time when ice there should have been growing stronger and thicker. The warm air from the storm, and the storm itself, compacted the ice pack, pushing it further North. More evidence seems to floating in that our planet is warming up, leading to more loss of ice in the polar regions.<br />NASA also released more images from Saturn, showing a kaleidoscope of water swirl colours painted on the northern pole of Saturn. The hexagon shape is again noted in the images provided, but the main highlight is the colorful representation of the latitudinal bands, which come about from air flowing at different speeds, and at different heights, in Saturn's atmosphere. Many eddies and swirls are also noted where the separate bands meet. Just another fascinating, gorgeous breathtaking image from the planet Saturn.]]></itunes:summary><itunes:duration>2015</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Black Holes, Threatening Asteroids, and Active Galatic Nuclei</title><link>https://www.spreaker.com/episode/black-holes-threatening-asteroids-and-active-galatic-nuclei--23525113</link><description><![CDATA[By observing a  super-massive black hole in the center of galaxy (with HUBBLE and the Chandra X-Ray telescope) during the past 10 years, scientists have concluded that the BH is no longer being fed enough fuel to make its surroundings shine brightly.  The cores of many galaxies shine brightly, due to the presence of super massive BHs that feed on surrounding matter. These active galatic nuclei or AGN, are amongst the brightest shining things in the universe. They are powered by matter that falls into a BH. Scientists are unsure at to the cause, but it does seem that the infall of matter into the nucleus is being disrupted by some unknown process.<br />NASA and FEMA are planning emergency response exercises in the case of an asteroid impact on Earth. NASA monitors asteroids ion near Earth orbit, and other asteroids in longer orbits, but NASA and FEMA are regularly conducting emergency response exercises in case an asteroid does break through and then impacts our planet. Through the simulation, in which an steroid would impact the Los Angeles area in 2020, NASA and FEMA are developing response scenarios that all places on the planet can respond to.<br />HUBBLE is viewing a galaxy, NGC 1222, a peculiar example of a lenticular type galaxy, that is swallowing up 2 dwarf galaxies that are in orbit around NGC 1222. The gas matter that is falling into NGC 1222 is thought to be the agent that is triggered starbursts and star formation in NGC 1222. The moral of the story: don't stray in too close to a big galaxy because you will be ripped apart if you do so.<br /><br /><br />Astronomers classify AGN into two main types based on the properties of the light they emit. One type of AGN tends to be brighter than the other. The brightness is generally thought to depend on either or both of two factors: the AGN could be obscured by surrounding gas and dust, or it could be intrinsically dim because the rate of feeding of the supermassive black hole is low.<br /><br />Some AGN have been observed to change once between these two types over the course of only 10 years, a blink of an eye in astronomical terms. However, the AGN associated with the galaxy Markarian 1018 stands out by changing type twice, from a faint to a bright AGN in the 1980s and then changing back to a faint AGN within the last five years. A handful of AGN have been observed to make this full-cycle change, but never before has one been studied in such detail. During the second change in type the Markarian 1018 AGN became eight times fainter in X-rays between 2010 and 2016.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-November-10-15-00-00.mp3</guid><pubDate>Thu, 10 Nov 2016 22:05:49 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525113/astrotalk_november_10_15_00_00.mp3" length="24384157" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>By observing a  super-massive black hole in the center of galaxy (with HUBBLE and the Chandra X-Ray telescope) during the past 10 years, scientists have concluded that the BH is no longer being fed enough fuel to make its surroundings shine brightly....</itunes:subtitle><itunes:summary><![CDATA[By observing a  super-massive black hole in the center of galaxy (with HUBBLE and the Chandra X-Ray telescope) during the past 10 years, scientists have concluded that the BH is no longer being fed enough fuel to make its surroundings shine brightly.  The cores of many galaxies shine brightly, due to the presence of super massive BHs that feed on surrounding matter. These active galatic nuclei or AGN, are amongst the brightest shining things in the universe. They are powered by matter that falls into a BH. Scientists are unsure at to the cause, but it does seem that the infall of matter into the nucleus is being disrupted by some unknown process.<br />NASA and FEMA are planning emergency response exercises in the case of an asteroid impact on Earth. NASA monitors asteroids ion near Earth orbit, and other asteroids in longer orbits, but NASA and FEMA are regularly conducting emergency response exercises in case an asteroid does break through and then impacts our planet. Through the simulation, in which an steroid would impact the Los Angeles area in 2020, NASA and FEMA are developing response scenarios that all places on the planet can respond to.<br />HUBBLE is viewing a galaxy, NGC 1222, a peculiar example of a lenticular type galaxy, that is swallowing up 2 dwarf galaxies that are in orbit around NGC 1222. The gas matter that is falling into NGC 1222 is thought to be the agent that is triggered starbursts and star formation in NGC 1222. The moral of the story: don't stray in too close to a big galaxy because you will be ripped apart if you do so.<br /><br /><br />Astronomers classify AGN into two main types based on the properties of the light they emit. One type of AGN tends to be brighter than the other. The brightness is generally thought to depend on either or both of two factors: the AGN could be obscured by surrounding gas and dust, or it could be intrinsically dim because the rate of feeding of the supermassive black hole is low.<br /><br />Some AGN have been observed to change once between these two types over the course of only 10 years, a blink of an eye in astronomical terms. However, the AGN associated with the galaxy Markarian 1018 stands out by changing type twice, from a faint to a bright AGN in the 1980s and then changing back to a faint AGN within the last five years. A handful of AGN have been observed to make this full-cycle change, but never before has one been studied in such detail. During the second change in type the Markarian 1018 AGN became eight times fainter in X-rays between 2010 and 2016.]]></itunes:summary><itunes:duration>1525</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Sequencing DNA Aboard the International Space Station and Measuring the Length of a Day on Saturn</title><link>https://www.spreaker.com/episode/sequencing-dna-aboard-the-international-space-station-and-measuring-the-length-of-a-day-on-saturn--23524900</link><description><![CDATA[For the first time ever, a NASA scientist, Kate Reubens, has carried out an experiment for sequencing DNA in space, on the International Space Station. This opens up a whole new world of possibilities for research in the biological and medical communities. DNA in human cells contains instructions that scientists believe they can now manipulate. The ability to humanly manipulate this sequencing of DNA, which is now being done in space, can possibly help scientists learn how to control DNA, supposedly for human benefit. <br />Scientists, up till now, have found it difficult to get a precise measurement of the length of a day on the planet Saturn. One of the problems in getting this measurement is the inability, so far, to get a precise measurement of the rotation rate of Saturn. The notion of a day has to do with motion (???????) or so say NASA Scientists. When we think of a day on Earth, we think of the motion of the Sun across the sky, where it rises, and where it sets.  person does not have to be on Earth to measure the length of an Earth day. For Saturn, this is more difficult, because the gaseous surface (surface?) of Mars lies beneath 1,000s of miles of gaseous atmosphere. The poles also spin at different rates than the equator. So determining the precise length of a Saturnian day is not an easy task. Saturn has swirling gas clouds that move at different rates, so it is next to impossible to get anything resembling an accurate measurement from measuring the rotation rate of clouds or parcels of the atmosphere circling high above Saturn. Scientists can use the magnetic fields of Saturn, and the radio wave emissions from the planet, to get a much more accurate measurement on the rotation rate of Saturn. Saturn's magnetic field wobbles like a hula hoop does, and since the magnetic field is generated from deep within the planet, then 1 wobble in the magnetic filed is equal to the exact rotation rate of the planet Saturn. This, then, helps scientists determine the length of a day on Saturn.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-November-24-15-00-39.mp3</guid><pubDate>Thu, 03 Nov 2016 22:12:30 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524900/astrotalk_november_24_15_00_39.mp3" length="16815752" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>For the first time ever, a NASA scientist, Kate Reubens, has carried out an experiment for sequencing DNA in space, on the International Space Station. This opens up a whole new world of possibilities for research in the biological and medical...</itunes:subtitle><itunes:summary><![CDATA[For the first time ever, a NASA scientist, Kate Reubens, has carried out an experiment for sequencing DNA in space, on the International Space Station. This opens up a whole new world of possibilities for research in the biological and medical communities. DNA in human cells contains instructions that scientists believe they can now manipulate. The ability to humanly manipulate this sequencing of DNA, which is now being done in space, can possibly help scientists learn how to control DNA, supposedly for human benefit. <br />Scientists, up till now, have found it difficult to get a precise measurement of the length of a day on the planet Saturn. One of the problems in getting this measurement is the inability, so far, to get a precise measurement of the rotation rate of Saturn. The notion of a day has to do with motion (???????) or so say NASA Scientists. When we think of a day on Earth, we think of the motion of the Sun across the sky, where it rises, and where it sets.  person does not have to be on Earth to measure the length of an Earth day. For Saturn, this is more difficult, because the gaseous surface (surface?) of Mars lies beneath 1,000s of miles of gaseous atmosphere. The poles also spin at different rates than the equator. So determining the precise length of a Saturnian day is not an easy task. Saturn has swirling gas clouds that move at different rates, so it is next to impossible to get anything resembling an accurate measurement from measuring the rotation rate of clouds or parcels of the atmosphere circling high above Saturn. Scientists can use the magnetic fields of Saturn, and the radio wave emissions from the planet, to get a much more accurate measurement on the rotation rate of Saturn. Saturn's magnetic field wobbles like a hula hoop does, and since the magnetic field is generated from deep within the planet, then 1 wobble in the magnetic filed is equal to the exact rotation rate of the planet Saturn. This, then, helps scientists determine the length of a day on Saturn.]]></itunes:summary><itunes:duration>1051</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Penguins in the Antartica</title><link>https://www.spreaker.com/episode/penguins-in-the-antartica--23524911</link><description><![CDATA[Anther citizen scientist topic is covered today. NASA is studying penguin habitats in the Antartica using the Mapping Application for Penguin Populations and Projected Dynamics (MAPPPD) satellite. Information is available at  <a href="http://www.penguinmap.com" rel="noopener">www.penguinmap.com</a>. Citizens can now access information to understand how environmental change, fishing, and tourism are affecting Antarctica’s penguins. Population estimates for the penguins, for example, can be done by tracking the guana stains female penguins leave behind when they incubate their nests. The article does not make it exactly clear what things citizen scientists are doing, or can do, to help NASA. Go to the website to find out more about NASA's work on these interesting birds.<br />Centauri b is a planet orbiting the White Dwarf star in the triple-star Centauri system, the closest star system to Earth. There is still more to discover about this planet, but because the planet does not transit its host star, the information so far is limited. What is known is that Centauri b orbits its host star at 0.05 AU, and that it is approximately 1.3 times the mass of Earth. More research is needed before scientists at NASA can discover more about this exoplanet.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-October-27-15-00-00.mp3</guid><pubDate>Thu, 27 Oct 2016 21:59:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524911/astrotalk_october_27_15_00_00.mp3" length="29776248" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Anther citizen scientist topic is covered today. NASA is studying penguin habitats in the Antartica using the Mapping Application for Penguin Populations and Projected Dynamics (MAPPPD) satellite. Information is available at  www.penguinmap.com....</itunes:subtitle><itunes:summary><![CDATA[Anther citizen scientist topic is covered today. NASA is studying penguin habitats in the Antartica using the Mapping Application for Penguin Populations and Projected Dynamics (MAPPPD) satellite. Information is available at  <a href="http://www.penguinmap.com" rel="noopener">www.penguinmap.com</a>. Citizens can now access information to understand how environmental change, fishing, and tourism are affecting Antarctica’s penguins. Population estimates for the penguins, for example, can be done by tracking the guana stains female penguins leave behind when they incubate their nests. The article does not make it exactly clear what things citizen scientists are doing, or can do, to help NASA. Go to the website to find out more about NASA's work on these interesting birds.<br />Centauri b is a planet orbiting the White Dwarf star in the triple-star Centauri system, the closest star system to Earth. There is still more to discover about this planet, but because the planet does not transit its host star, the information so far is limited. What is known is that Centauri b orbits its host star at 0.05 AU, and that it is approximately 1.3 times the mass of Earth. More research is needed before scientists at NASA can discover more about this exoplanet.]]></itunes:summary><itunes:duration>1862</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Citizen Scientist</title><link>https://www.spreaker.com/episode/citizen-scientist--23525129</link><description><![CDATA[Citizen scientist are helping NASA big time. New formations on Mars, known as "SPIDERS", are receiving the once-over from 10,000 citizen scientists. 10,000 citizen scientists, or citizen volunteers, are pouring over data from the Mars Reconnaissance Orbiter (MRO) to help identify the spiders.  The spiders are long cracks or lines on the surface of Mars caused by CO2 gas, which escapes from under the surface of Mars, when slabs of sub-surface ice melts, producing the CO2 ice. NASA could not hope to do the work that the 10,000 citizen scientists do, so NASA is obviously very thankful to have this volunteer workforce aid it in its work. <br /><br />Work done by citizen scientists  is also aiding NASA scientists doing work on Jupiter. NASA has released images from the JUNO mission with its JunoCam public outreach camera on the JunoCam website  <a href="http://www.missionjuno.swri.edu/junocam" rel="noopener">www.missionjuno.swri.edu/junocam</a>. JunoCam apparently has a small operations team, but no image processing team, so the public is being invited to process the image data into final image products. JunoCam is the first outreach camera to venture beyond the asteroid belt. So says Candy Hansen, JunoCam imaging scientist from the Planetary Science Institute in Tucson, Arizona. “All sorts of people are coming to the JunoCam site and providing their own aesthetic. We have volunteers from all over the world, and they are doing beautiful work. So far all our expectations for JunoCam have not only been met but are being exceeded, and we’re just getting started.”<br /><br />There are other citizen scientist ventures ongoing, and probably the most important one from Vancouver was the marvelous work done by Michelle Kunimoto of UBC. Michelle identified 4 new planets from data from NASA, so congratulations again Michelle.<br /><br />2 links for citizen scientist participation are:   <a href="http://terrains.planetfour.org" rel="noopener">http://terrains.planetfour.org</a>   and   <a href="https://www.missionjuno.swri.edu/junocam" rel="noopener">https://www.missionjuno.swri.edu/junocam</a>.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-October-20-15-00-00.mp3</guid><pubDate>Thu, 20 Oct 2016 22:02:27 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525129/astrotalk_october_20_15_00_00.mp3" length="25055817" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Citizen scientist are helping NASA big time. New formations on Mars, known as "SPIDERS", are receiving the once-over from 10,000 citizen scientists. 10,000 citizen scientists, or citizen volunteers, are pouring over data from the Mars Reconnaissance...</itunes:subtitle><itunes:summary><![CDATA[Citizen scientist are helping NASA big time. New formations on Mars, known as "SPIDERS", are receiving the once-over from 10,000 citizen scientists. 10,000 citizen scientists, or citizen volunteers, are pouring over data from the Mars Reconnaissance Orbiter (MRO) to help identify the spiders.  The spiders are long cracks or lines on the surface of Mars caused by CO2 gas, which escapes from under the surface of Mars, when slabs of sub-surface ice melts, producing the CO2 ice. NASA could not hope to do the work that the 10,000 citizen scientists do, so NASA is obviously very thankful to have this volunteer workforce aid it in its work. <br /><br />Work done by citizen scientists  is also aiding NASA scientists doing work on Jupiter. NASA has released images from the JUNO mission with its JunoCam public outreach camera on the JunoCam website  <a href="http://www.missionjuno.swri.edu/junocam" rel="noopener">www.missionjuno.swri.edu/junocam</a>. JunoCam apparently has a small operations team, but no image processing team, so the public is being invited to process the image data into final image products. JunoCam is the first outreach camera to venture beyond the asteroid belt. So says Candy Hansen, JunoCam imaging scientist from the Planetary Science Institute in Tucson, Arizona. “All sorts of people are coming to the JunoCam site and providing their own aesthetic. We have volunteers from all over the world, and they are doing beautiful work. So far all our expectations for JunoCam have not only been met but are being exceeded, and we’re just getting started.”<br /><br />There are other citizen scientist ventures ongoing, and probably the most important one from Vancouver was the marvelous work done by Michelle Kunimoto of UBC. Michelle identified 4 new planets from data from NASA, so congratulations again Michelle.<br /><br />2 links for citizen scientist participation are:   <a href="http://terrains.planetfour.org" rel="noopener">http://terrains.planetfour.org</a>   and   <a href="https://www.missionjuno.swri.edu/junocam" rel="noopener">https://www.missionjuno.swri.edu/junocam</a>.]]></itunes:summary><itunes:duration>1566</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Opportunity Rover to Explore Mars Gully, Factors in Travelling to Mars</title><link>https://www.spreaker.com/episode/opportunity-rover-to-explore-mars-gully-factors-in-travelling-to-mars--23524912</link><description><![CDATA[The NASA Mars Opportunity Rover is just about to drive down into a large gully to look for signs of water. No space vehicle has driven down a gully on Mars before. The gully lies in the Bitterroot Valley, on the western rim of Endeavour Crater, a basin which was thought to have been excavated by a meteor impact billions of years ago. In craters that opportunity previously examined, it never drove down into the craters. This is the first time that Opportunity will actually drive down into one of those craters. The water in the crater is thought to be below the surface. If it wasn't beneath the surface, it would have already evaporated into the thin Martian atmosphere. The gully is the length of 2 football fields, and scientists are confident they will find signs of water in the gully.<br />In other news, a lot of consideration needs to be given to many factors in travelling to Mars. When humans went to the Moon, for example, the spacecrafts did not travel very fast: in relative terms that is. When travelling to Mars, the spacecrafts will have to travel at a far greater speed, because Mars is so much farther from Earth than is the Moon. Since the spacecraft's speeds will be much higher, a lot more of something will be needed to brake the spacecraft and slow it down enough so it can begin to orbit Mars. Can the firing of rockets brake the spacecraft enough? Maybe not, because that would require too much fuel, and these spacecrafts cannot carry endless supplies of fuel. NASA is therefore working with a new type of power fuel called a scudaradite. These materials can conduct electricity like a metal, heat up like a glass, and generate size-able voltages. Materials such as this new thermo-electrical material is apparently hard to come by. This material is being designed at the Jet Propulsion Laboratory in Pasadena. Scudaradites are composed of heavy atoms like Antimony. They can be used as thermocouples, which generate voltage due to the difference in temperature between its components. Thermocouples made of scudaradites need a lot less of a difference in temperature to produce a useful amount of power, so they are more efficient at generating power. This type of performance would be very advantageous  on a long term mission to Mars. An RTG generator, which is now being tested, contains 768 thermocouples all facing in the same direction. The scudaradite material would replace the now used Teluride in the RTG generator, and would provide better heat generation.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-October-13-15-00-00.mp3</guid><pubDate>Thu, 13 Oct 2016 21:58:12 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524912/astrotalk_october_13_15_00_00.mp3" length="30176235" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The NASA Mars Opportunity Rover is just about to drive down into a large gully to look for signs of water. No space vehicle has driven down a gully on Mars before. The gully lies in the Bitterroot Valley, on the western rim of Endeavour Crater, a...</itunes:subtitle><itunes:summary><![CDATA[The NASA Mars Opportunity Rover is just about to drive down into a large gully to look for signs of water. No space vehicle has driven down a gully on Mars before. The gully lies in the Bitterroot Valley, on the western rim of Endeavour Crater, a basin which was thought to have been excavated by a meteor impact billions of years ago. In craters that opportunity previously examined, it never drove down into the craters. This is the first time that Opportunity will actually drive down into one of those craters. The water in the crater is thought to be below the surface. If it wasn't beneath the surface, it would have already evaporated into the thin Martian atmosphere. The gully is the length of 2 football fields, and scientists are confident they will find signs of water in the gully.<br />In other news, a lot of consideration needs to be given to many factors in travelling to Mars. When humans went to the Moon, for example, the spacecrafts did not travel very fast: in relative terms that is. When travelling to Mars, the spacecrafts will have to travel at a far greater speed, because Mars is so much farther from Earth than is the Moon. Since the spacecraft's speeds will be much higher, a lot more of something will be needed to brake the spacecraft and slow it down enough so it can begin to orbit Mars. Can the firing of rockets brake the spacecraft enough? Maybe not, because that would require too much fuel, and these spacecrafts cannot carry endless supplies of fuel. NASA is therefore working with a new type of power fuel called a scudaradite. These materials can conduct electricity like a metal, heat up like a glass, and generate size-able voltages. Materials such as this new thermo-electrical material is apparently hard to come by. This material is being designed at the Jet Propulsion Laboratory in Pasadena. Scudaradites are composed of heavy atoms like Antimony. They can be used as thermocouples, which generate voltage due to the difference in temperature between its components. Thermocouples made of scudaradites need a lot less of a difference in temperature to produce a useful amount of power, so they are more efficient at generating power. This type of performance would be very advantageous  on a long term mission to Mars. An RTG generator, which is now being tested, contains 768 thermocouples all facing in the same direction. The scudaradite material would replace the now used Teluride in the RTG generator, and would provide better heat generation.]]></itunes:summary><itunes:duration>1887</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Hurricane Matthew</title><link>https://www.spreaker.com/episode/hurricane-matthew--23524985</link><description><![CDATA[Hurricane Matthew is the news story these days. The big hurricane, which began off the coast of Africa, has moved across the Atlantic, where it has brought devastating winds and heavy rainfall through much of the Caribbean. NASA has been tracking the storms with its numerous satellites, providing much needed data on the progression of the storm. NASA maps show Matthew moving West through much of the Caribbean, and then unexplicably heading directly North,  where it hit Haiti and many other Caribbean islands. The storm has been categorized as a  category 4 storm, on the Saffir-Simpson Hurricane Wind Scale. The strongest hurricane is a category 5 on this scale. For parts of its journey, the storm has been clocked as a category 5. Through most of its journey, the storm has been the strongest at the eye of the hurrincane. There are times though, when a combination of the cyclonic counter-clockwise rotation of the storm, in combination with how this wind reacts with the topography of any particular area, causes the rainfall and winds to be higher just off the eastern edge of the eye. Matthew has caused devastation as it has made its round through the Caribbean. Much of the eastern coast of Florida and South Carolina has been evacuated as Americans await the awful wrath of Matthew to hit their shores. Also today, we briefly touched on a lovely photo of the Saturn ring system, taken by the Cassini spacecraft. In the photo, the tiny  moon Atlas, which is farther out in its orbit than the tiny Pan, is slowly being overtaken in its orbit by Pan.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-October-06-15-00-00.mp3</guid><pubDate>Thu, 06 Oct 2016 22:01:04 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524985/astrotalk_october_06_15_00_00.mp3" length="25903857" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Hurricane Matthew is the news story these days. The big hurricane, which began off the coast of Africa, has moved across the Atlantic, where it has brought devastating winds and heavy rainfall through much of the Caribbean. NASA has been tracking the...</itunes:subtitle><itunes:summary><![CDATA[Hurricane Matthew is the news story these days. The big hurricane, which began off the coast of Africa, has moved across the Atlantic, where it has brought devastating winds and heavy rainfall through much of the Caribbean. NASA has been tracking the storms with its numerous satellites, providing much needed data on the progression of the storm. NASA maps show Matthew moving West through much of the Caribbean, and then unexplicably heading directly North,  where it hit Haiti and many other Caribbean islands. The storm has been categorized as a  category 4 storm, on the Saffir-Simpson Hurricane Wind Scale. The strongest hurricane is a category 5 on this scale. For parts of its journey, the storm has been clocked as a category 5. Through most of its journey, the storm has been the strongest at the eye of the hurrincane. There are times though, when a combination of the cyclonic counter-clockwise rotation of the storm, in combination with how this wind reacts with the topography of any particular area, causes the rainfall and winds to be higher just off the eastern edge of the eye. Matthew has caused devastation as it has made its round through the Caribbean. Much of the eastern coast of Florida and South Carolina has been evacuated as Americans await the awful wrath of Matthew to hit their shores. Also today, we briefly touched on a lovely photo of the Saturn ring system, taken by the Cassini spacecraft. In the photo, the tiny  moon Atlas, which is farther out in its orbit than the tiny Pan, is slowly being overtaken in its orbit by Pan.]]></itunes:summary><itunes:duration>1619</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Mercury and Elon Musk</title><link>https://www.spreaker.com/episode/mercury-and-elon-musk--23524936</link><description><![CDATA[The Messenger spacecraft has sent back some more data about tectonic activity on the planet Mercury. In article titled, The Shrinking Mercury is Active After All, the authors suggest that Mercury is shrinking, due to the cooling of the planet, which causes the appearance of scarps on its surface. As the planet contracts, the surface crust breaks, and small scarps, or fault lines, appear on the surface. The small scarps had to be very young, because due to the constant bombardment of Mercury by meteors, the scarps will not stay there for long. Earth and Mercury are the only 2 tectonically active planets in our Solar System. Also discussed was Elon Musk's ambitious plan to send spacecrafts full of humans to live on Mars by 2030. In an article on gizmodo.com, Maddie Stone argues that Musks' plan was long on hyperbole and promise, but Musk did not explain how it would be done, or who would pay for his ambitous plan. Still, you have to had to Musk: he is an ambitious dude.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-September-29-15-05-00.mp3</guid><pubDate>Thu, 29 Sep 2016 22:07:10 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524936/astrotalk_september_29_15_05_00.mp3" length="21295856" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The Messenger spacecraft has sent back some more data about tectonic activity on the planet Mercury. In article titled, The Shrinking Mercury is Active After All, the authors suggest that Mercury is shrinking, due to the cooling of the planet, which...</itunes:subtitle><itunes:summary><![CDATA[The Messenger spacecraft has sent back some more data about tectonic activity on the planet Mercury. In article titled, The Shrinking Mercury is Active After All, the authors suggest that Mercury is shrinking, due to the cooling of the planet, which causes the appearance of scarps on its surface. As the planet contracts, the surface crust breaks, and small scarps, or fault lines, appear on the surface. The small scarps had to be very young, because due to the constant bombardment of Mercury by meteors, the scarps will not stay there for long. Earth and Mercury are the only 2 tectonically active planets in our Solar System. Also discussed was Elon Musk's ambitious plan to send spacecrafts full of humans to live on Mars by 2030. In an article on gizmodo.com, Maddie Stone argues that Musks' plan was long on hyperbole and promise, but Musk did not explain how it would be done, or who would pay for his ambitous plan. Still, you have to had to Musk: he is an ambitious dude.]]></itunes:summary><itunes:duration>1331</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>An Impossible Cloud Forms on Titan - Again</title><link>https://www.spreaker.com/episode/an-impossible-cloud-forms-on-titan-again--23524923</link><description><![CDATA[Scientists working on the Cassini Mission in the Saturn system have discovered an impossible cloud on Saturn's largest moon Titan. A similar type ice cloud was found decades ago by the Voyager 1 Spacecraft. At that time, V1 scientists were puzzled by the fact that the cloud contained less than 1% of the dicyaniacetylene gas that was needed in order for the cloud to condense. At that time, scientists believed that V1's instruments may not have been sensitive enough to detect the gas. The same thing has happened again: just this week, scientists that work with the Cassini spacecraft have found less than 1% of the gas they thought would be needed in order for the cloud to condense. Clouds are thought to form on Titan in the same way that they form on Earth: through the condensation of gases in a evaporation/condensation cycle. Instead of water, the gas in Titan's atmosphere is methane. This puzzling occurrence of the formation of the cloud has led to another theory: the cloud on Titan forms through a similar type of solid-state chemical process that occurs over the N & S poles on Earth. The polar stratospheres on Titan and Earth could not be more different, so Titan has yielded another surprise. It seems that the underlying physical processes in Titans's and Earth's atmospheres have led to analogous cloud chemistry in both places.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-September-22-15-02-00.mp3</guid><pubDate>Thu, 22 Sep 2016 22:02:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524923/astrotalk_september_22_15_02_00.mp3" length="28816196" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Scientists working on the Cassini Mission in the Saturn system have discovered an impossible cloud on Saturn's largest moon Titan. A similar type ice cloud was found decades ago by the Voyager 1 Spacecraft. At that time, V1 scientists were puzzled by...</itunes:subtitle><itunes:summary><![CDATA[Scientists working on the Cassini Mission in the Saturn system have discovered an impossible cloud on Saturn's largest moon Titan. A similar type ice cloud was found decades ago by the Voyager 1 Spacecraft. At that time, V1 scientists were puzzled by the fact that the cloud contained less than 1% of the dicyaniacetylene gas that was needed in order for the cloud to condense. At that time, scientists believed that V1's instruments may not have been sensitive enough to detect the gas. The same thing has happened again: just this week, scientists that work with the Cassini spacecraft have found less than 1% of the gas they thought would be needed in order for the cloud to condense. Clouds are thought to form on Titan in the same way that they form on Earth: through the condensation of gases in a evaporation/condensation cycle. Instead of water, the gas in Titan's atmosphere is methane. This puzzling occurrence of the formation of the cloud has led to another theory: the cloud on Titan forms through a similar type of solid-state chemical process that occurs over the N & S poles on Earth. The polar stratospheres on Titan and Earth could not be more different, so Titan has yielded another surprise. It seems that the underlying physical processes in Titans's and Earth's atmospheres have led to analogous cloud chemistry in both places.]]></itunes:summary><itunes:duration>1802</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Star Trek Fifthieth Anniversary</title><link>https://www.spreaker.com/episode/star-trek-fifthieth-anniversary--23524922</link><description><![CDATA[Today is 50th anniversary of the 1st episode of the TV show Star Trek. Fittingly, on this anniversary, NASA has imaged 2 nebulas in the Infrared that look a lot like the startrek entrprise spaceships that were captained by Captain Kirk and Captain Jean-Luc Picard. The nebulas, dubbed the Enterprise Nebula, falls within the disk of the Milky Way galaxy, displaying 2 two regions that feature a lot of star formation, but that are hidden behind a haze of dust when viewed in visible light. A young magnetar whose rotation period, 66.7 hours, has also been discovered. This is the 30th magnetar ever discovered, and its rotation period is also the slowest ever discovered for a magnetar. The OSIRIS-Rex asteroid retrieval mission is also being launched today, Thursday, September 8, 2016. This  mission will be the 1st ever to fly to an asteroid, and then retrieve a sample, which it will bring back to Earth in 2023. OSIRIS-Rex will reach Bennu in 2018.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-September-08-15-07-00.mp3</guid><pubDate>Thu, 08 Sep 2016 22:07:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524922/astrotalk_september_08_15_07_00.mp3" length="28815778" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Today is 50th anniversary of the 1st episode of the TV show Star Trek. Fittingly, on this anniversary, NASA has imaged 2 nebulas in the Infrared that look a lot like the startrek entrprise spaceships that were captained by Captain Kirk and Captain...</itunes:subtitle><itunes:summary><![CDATA[Today is 50th anniversary of the 1st episode of the TV show Star Trek. Fittingly, on this anniversary, NASA has imaged 2 nebulas in the Infrared that look a lot like the startrek entrprise spaceships that were captained by Captain Kirk and Captain Jean-Luc Picard. The nebulas, dubbed the Enterprise Nebula, falls within the disk of the Milky Way galaxy, displaying 2 two regions that feature a lot of star formation, but that are hidden behind a haze of dust when viewed in visible light. A young magnetar whose rotation period, 66.7 hours, has also been discovered. This is the 30th magnetar ever discovered, and its rotation period is also the slowest ever discovered for a magnetar. The OSIRIS-Rex asteroid retrieval mission is also being launched today, Thursday, September 8, 2016. This  mission will be the 1st ever to fly to an asteroid, and then retrieve a sample, which it will bring back to Earth in 2023. OSIRIS-Rex will reach Bennu in 2018.]]></itunes:summary><itunes:duration>1801</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Saturn and Its Moon Enceladus</title><link>https://www.spreaker.com/episode/saturn-and-its-moon-enceladus--23525280</link><description><![CDATA[NASA's Cassini Spacecraft has discovered a large assortment of canyons on Titan, the biggest moon in the Saturn system. Large hydrocarbon lakes were also detected in the steep canyons. The depths of the canyons were measured by bouncing radar pings off the surface of Titan. The narrow branching channels of the canyon areas, named Vid Flumina, are quite narrow, but they are also quite deep, measuring anywhere from 790 - 1,870 feet. Titan is an interesting moon, featuring flowing hydrocarbon river, and hydrocarbon lakes. The clouds in Saturn's northern hemisphere, were imaged with infrared, IR, light, at wavelengths of 750, 727and  619 nanometers. Filters at these wavelengths were used because they are sensitive to the absorption and scattering of light with the methane that is found in Saturn's atmosphere. The water-moon Enceladus of Saturn, was also imaged. It appeared like a drop of dew floating on a leaf. But, it was just hovering Saturn's ring system.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-August-11-15-12-00.mp3</guid><pubDate>Thu, 11 Aug 2016 22:09:48 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525280/astrotalk_august_11_15_12_00.mp3" length="34991961" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>NASA's Cassini Spacecraft has discovered a large assortment of canyons on Titan, the biggest moon in the Saturn system. Large hydrocarbon lakes were also detected in the steep canyons. The depths of the canyons were measured by bouncing radar pings...</itunes:subtitle><itunes:summary><![CDATA[NASA's Cassini Spacecraft has discovered a large assortment of canyons on Titan, the biggest moon in the Saturn system. Large hydrocarbon lakes were also detected in the steep canyons. The depths of the canyons were measured by bouncing radar pings off the surface of Titan. The narrow branching channels of the canyon areas, named Vid Flumina, are quite narrow, but they are also quite deep, measuring anywhere from 790 - 1,870 feet. Titan is an interesting moon, featuring flowing hydrocarbon river, and hydrocarbon lakes. The clouds in Saturn's northern hemisphere, were imaged with infrared, IR, light, at wavelengths of 750, 727and  619 nanometers. Filters at these wavelengths were used because they are sensitive to the absorption and scattering of light with the methane that is found in Saturn's atmosphere. The water-moon Enceladus of Saturn, was also imaged. It appeared like a drop of dew floating on a leaf. But, it was just hovering Saturn's ring system.]]></itunes:summary><itunes:duration>2187</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Jupiter</title><link>https://www.spreaker.com/episode/jupiter--23524937</link><description><![CDATA[Jupiter's moon Io is the most volcanicaly active moon in the solar system. Scientists have now discovered that Io's atmosphere is variable, and this phenomenon is affected by whether iO is or isn't hiding from the Sun in the shadow of its host planet Jupiter. The Juno mission to Jupiter is also talked about. The Great Red Spot on Jupiter, (GRS) which is as wide as 3 Earth diameters, also has an effect on the heating of Jupiter's atmosphere. There is therefore a lot of atmosphere on the show today.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-August-04-15-00-00.mp3</guid><pubDate>Thu, 04 Aug 2016 22:06:29 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524937/astrotalk_august_04_15_00_00.mp3" length="33088157" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Jupiter's moon Io is the most volcanicaly active moon in the solar system. Scientists have now discovered that Io's atmosphere is variable, and this phenomenon is affected by whether iO is or isn't hiding from the Sun in the shadow of its host planet...</itunes:subtitle><itunes:summary><![CDATA[Jupiter's moon Io is the most volcanicaly active moon in the solar system. Scientists have now discovered that Io's atmosphere is variable, and this phenomenon is affected by whether iO is or isn't hiding from the Sun in the shadow of its host planet Jupiter. The Juno mission to Jupiter is also talked about. The Great Red Spot on Jupiter, (GRS) which is as wide as 3 Earth diameters, also has an effect on the heating of Jupiter's atmosphere. There is therefore a lot of atmosphere on the show today.]]></itunes:summary><itunes:duration>2069</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Titan</title><link>https://www.spreaker.com/episode/titan--23525342</link><description><![CDATA[Signals can reveal marvelous things. The Cassini spacecraft, which has been in orbit in the Saturn system for many years, uses interesting techniques to study Saturn's moon Titan. Radio, light and radar signals from Cassini are bounced off Titan, and then received on Earth on the Deep Space Network (DSN). The way that these signals are bounced or absorbed reveals telling features about Titan. These can features relate to the chemical composition of Titan's atmosphere, the density or temperature of the constituents of the gases in Titan's atmosphere, the composition of the seas and rivers on Titan's surface, as well as the make-up of the sea beds. Scientists are also using these techniques to study the atmospheres of exoplanets. When the light of a host star shines through the atmospheres of theses distant exoplanets, scientists can use techniques they have developed from studying Titan's features, to study the features of exoplanets, which reside many, many light years from Earth.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-July-28-15-08-00.mp3</guid><pubDate>Thu, 28 Jul 2016 22:06:37 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525342/astrotalk_july_28_15_08_00.mp3" length="45775726" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Signals can reveal marvelous things. The Cassini spacecraft, which has been in orbit in the Saturn system for many years, uses interesting techniques to study Saturn's moon Titan. Radio, light and radar signals from Cassini are bounced off Titan, and...</itunes:subtitle><itunes:summary><![CDATA[Signals can reveal marvelous things. The Cassini spacecraft, which has been in orbit in the Saturn system for many years, uses interesting techniques to study Saturn's moon Titan. Radio, light and radar signals from Cassini are bounced off Titan, and then received on Earth on the Deep Space Network (DSN). The way that these signals are bounced or absorbed reveals telling features about Titan. These can features relate to the chemical composition of Titan's atmosphere, the density or temperature of the constituents of the gases in Titan's atmosphere, the composition of the seas and rivers on Titan's surface, as well as the make-up of the sea beds. Scientists are also using these techniques to study the atmospheres of exoplanets. When the light of a host star shines through the atmospheres of theses distant exoplanets, scientists can use techniques they have developed from studying Titan's features, to study the features of exoplanets, which reside many, many light years from Earth.]]></itunes:summary><itunes:duration>2861</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Juno Spacecraft</title><link>https://www.spreaker.com/episode/juno-spacecraft--23524992</link><description><![CDATA[Titan, the solar system's second biggest moon, is the topic today. Review of the Cassini spacecrafts efforts at Titan, to learn more about this moon's atmosphere, when it is inside Saturn's protective magnetosphere, and when it wanders outside of this magnetosphere.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-July-14-15-00-00.mp3</guid><pubDate>Thu, 14 Jul 2016 22:03:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524992/astrotalk_july_14_15_00_00.mp3" length="39999948" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Titan, the solar system's second biggest moon, is the topic today. Review of the Cassini spacecrafts efforts at Titan, to learn more about this moon's atmosphere, when it is inside Saturn's protective magnetosphere, and when it wanders outside of this...</itunes:subtitle><itunes:summary><![CDATA[Titan, the solar system's second biggest moon, is the topic today. Review of the Cassini spacecrafts efforts at Titan, to learn more about this moon's atmosphere, when it is inside Saturn's protective magnetosphere, and when it wanders outside of this magnetosphere.]]></itunes:summary><itunes:duration>2500</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Juno Spacecraft In Orbit Jupiter</title><link>https://www.spreaker.com/episode/juno-spacecraft-in-orbit-jupiter--23524941</link><description><![CDATA[The Juno Spacecraft, which launched from Earth on August 5, 2011, and then traveled 1.7 Billion miles, executed maneuvers, and then was successfully captured by Jupiter, to go into orbit around the giant gas planet on July 4, 2016. Juno then turned itself toward a more beneficial position so that its solar panels could capture rays from the Sun, as the spacecraft is powered by solar energy. Over the next few months, scientists at the Jet Propulsion Laboratory in Pasadena will perform final tests on Juno's subsystems, do final calibrations on Juno's science instruments,and also do some minor science collection activities. The official science collection phase begins 53.5 days after July 4, on October 19. Juno will try to help uncover more secrets about Jupiter's atmosphere, and gather more info about Jupiter's solid, rocky core, and the liquid material that circles just outside that core.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-July-07-15-00-00.mp3</guid><pubDate>Thu, 07 Jul 2016 22:03:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524941/astrotalk_july_07_15_00_00.mp3" length="39375935" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The Juno Spacecraft, which launched from Earth on August 5, 2011, and then traveled 1.7 Billion miles, executed maneuvers, and then was successfully captured by Jupiter, to go into orbit around the giant gas planet on July 4, 2016. Juno then turned...</itunes:subtitle><itunes:summary><![CDATA[The Juno Spacecraft, which launched from Earth on August 5, 2011, and then traveled 1.7 Billion miles, executed maneuvers, and then was successfully captured by Jupiter, to go into orbit around the giant gas planet on July 4, 2016. Juno then turned itself toward a more beneficial position so that its solar panels could capture rays from the Sun, as the spacecraft is powered by solar energy. Over the next few months, scientists at the Jet Propulsion Laboratory in Pasadena will perform final tests on Juno's subsystems, do final calibrations on Juno's science instruments,and also do some minor science collection activities. The official science collection phase begins 53.5 days after July 4, on October 19. Juno will try to help uncover more secrets about Jupiter's atmosphere, and gather more info about Jupiter's solid, rocky core, and the liquid material that circles just outside that core.]]></itunes:summary><itunes:duration>2461</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Jupiter and Pluto</title><link>https://www.spreaker.com/episode/jupiter-and-pluto--23525533</link><description><![CDATA[Pluto keeps revealing more of its secrets. Pluto's Sputnik Planum, a nitrogen ice plane on the surface of Pluto, is a topic today. The New Horizons Spacecraft, which zipped past Pluto in July 2015, has sent back data that shows Pluto's icy nitrogen surface has some smooth areas, but also some rough and ridgey areas. Sunlight is reflected in different ways on this diverse ice surface, and the surface seems to be quite dynamic, as it constantly changes shape and form. The Juno mission to Jupiter has now entered the Jovian system. Juno left the solar wind imbedded reach of the Sun, and is now in the upper reaches of Jupiter's magnetosphere. Listen in as we track the progress of Juno, as it moves closer into toward Jupiter. The Juno spacecraft launched from Cape Canaveral Florida on August 11, 2011, entered Jupiter's magnetosphere on June 24, 2016, and is expected to go into orbit around Jupiter on July 4, 2016, and begin sampling the lower reaches of Jupiter's magnetosphere on July 25. The upper reaches of Jupiter's magnetosphere, or bow shock, has proven to be incredibly complex, as scientists are now pouring pour over data that was sent back to them, beginning June 24.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-June-30-15-20-00.mp3</guid><pubDate>Thu, 30 Jun 2016 22:18:20 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525533/astrotalk_june_30_15_20_00.mp3" length="31440144" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Pluto keeps revealing more of its secrets. Pluto's Sputnik Planum, a nitrogen ice plane on the surface of Pluto, is a topic today. The New Horizons Spacecraft, which zipped past Pluto in July 2015, has sent back data that shows Pluto's icy nitrogen...</itunes:subtitle><itunes:summary><![CDATA[Pluto keeps revealing more of its secrets. Pluto's Sputnik Planum, a nitrogen ice plane on the surface of Pluto, is a topic today. The New Horizons Spacecraft, which zipped past Pluto in July 2015, has sent back data that shows Pluto's icy nitrogen surface has some smooth areas, but also some rough and ridgey areas. Sunlight is reflected in different ways on this diverse ice surface, and the surface seems to be quite dynamic, as it constantly changes shape and form. The Juno mission to Jupiter has now entered the Jovian system. Juno left the solar wind imbedded reach of the Sun, and is now in the upper reaches of Jupiter's magnetosphere. Listen in as we track the progress of Juno, as it moves closer into toward Jupiter. The Juno spacecraft launched from Cape Canaveral Florida on August 11, 2011, entered Jupiter's magnetosphere on June 24, 2016, and is expected to go into orbit around Jupiter on July 4, 2016, and begin sampling the lower reaches of Jupiter's magnetosphere on July 25. The upper reaches of Jupiter's magnetosphere, or bow shock, has proven to be incredibly complex, as scientists are now pouring pour over data that was sent back to them, beginning June 24.]]></itunes:summary><itunes:duration>1966</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Pluto</title><link>https://www.spreaker.com/episode/pluto--23524984</link><description><![CDATA[Pluto and it moons. Canyons in the Pluto system are deeper and longer than the Grand Canyon on Earth. New Horizons, the spacecraft which flew by Pluto on July 14, 2015, continues to send back data and pictures of the mysterious Pluto system, such as how Pluto interacts with the Solar Wind. Listen to this, and all other mysteries Pluto continues to reveal to us.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-June-23-15-02-00.mp3</guid><pubDate>Thu, 23 Jun 2016 22:02:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524984/astrotalk_june_23_15_02_00.mp3" length="26896091" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Pluto and it moons. Canyons in the Pluto system are deeper and longer than the Grand Canyon on Earth. New Horizons, the spacecraft which flew by Pluto on July 14, 2015, continues to send back data and pictures of the mysterious Pluto system, such as...</itunes:subtitle><itunes:summary><![CDATA[Pluto and it moons. Canyons in the Pluto system are deeper and longer than the Grand Canyon on Earth. New Horizons, the spacecraft which flew by Pluto on July 14, 2015, continues to send back data and pictures of the mysterious Pluto system, such as how Pluto interacts with the Solar Wind. Listen to this, and all other mysteries Pluto continues to reveal to us.]]></itunes:summary><itunes:duration>1682</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Pluto</title><link>https://www.spreaker.com/episode/pluto--23524917</link><description><![CDATA[Today, I will read a few articles about our friend Pluto. Yes, Pluto was demoted to the status of dwarf planet a few years ago, but there's hope ahead for all you Plutoites. Today, I talk about some interesting things about Pluto, so you Plutonians out there might talk comfort in what I found. Pluto interacts with the solar wind (SW) in ways that are more similar to how the SW interacts with planets such as Venus or Mars. Scientists speculated before that Pluto might interact with SW in ways that are more similar to how a comet interacts with the SW, but apparently, that ain't so. I also talk about other things that scientists have gleamed from the data that the New Horizons spacecraft sent back to Earth as it flew by Pluto in July 2015. Scientists are still deciphering the data sent back by NH, and are discovering more fascinating things about Pluto. Hope you Plutocratonians enjoy this show.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-June-09-15-00-00.mp3</guid><pubDate>Thu, 09 Jun 2016 22:03:21 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524917/astrotalk_june_09_15_00_00.mp3" length="35120274" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Today, I will read a few articles about our friend Pluto. Yes, Pluto was demoted to the status of dwarf planet a few years ago, but there's hope ahead for all you Plutoites. Today, I talk about some interesting things about Pluto, so you Plutonians...</itunes:subtitle><itunes:summary><![CDATA[Today, I will read a few articles about our friend Pluto. Yes, Pluto was demoted to the status of dwarf planet a few years ago, but there's hope ahead for all you Plutoites. Today, I talk about some interesting things about Pluto, so you Plutonians out there might talk comfort in what I found. Pluto interacts with the solar wind (SW) in ways that are more similar to how the SW interacts with planets such as Venus or Mars. Scientists speculated before that Pluto might interact with SW in ways that are more similar to how a comet interacts with the SW, but apparently, that ain't so. I also talk about other things that scientists have gleamed from the data that the New Horizons spacecraft sent back to Earth as it flew by Pluto in July 2015. Scientists are still deciphering the data sent back by NH, and are discovering more fascinating things about Pluto. Hope you Plutocratonians enjoy this show.]]></itunes:summary><itunes:duration>2196</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Weird Things in the Universe</title><link>https://www.spreaker.com/episode/weird-things-in-the-universe--23525601</link><description><![CDATA[The biggest, smallest, coldest, weirdest, strangest things in the Universe. Discussion will involve the most massive black holes, the biggest galaxy clusters, the coldest place in the solar system, and many other weird and cool things about our universe.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-May-12-15-01-55.mp3</guid><pubDate>Thu, 12 May 2016 22:01:55 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525601/astrotalk_may_12_15_01_55.mp3" length="36936943" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The biggest, smallest, coldest, weirdest, strangest things in the Universe. Discussion will involve the most massive black holes, the biggest galaxy clusters, the coldest place in the solar system, and many other weird and cool things about our universe.</itunes:subtitle><itunes:summary><![CDATA[The biggest, smallest, coldest, weirdest, strangest things in the Universe. Discussion will involve the most massive black holes, the biggest galaxy clusters, the coldest place in the solar system, and many other weird and cool things about our universe.]]></itunes:summary><itunes:duration>1542</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Black Holes from Kip Thorne's Book Part III</title><link>https://www.spreaker.com/episode/black-holes-from-kip-thorne-s-book-part-iii--23524930</link><description><![CDATA[This is the third and last show on Kip Thorn'es book, Black Holes and Time Warps. This show discusses the contributions of British physicist Roger Penrose,who introduced the branch of mathematics of Topology into the study of black holes. Topology proved to be a powerful new tool in helping develop a theory on the formation and final stages of the development of black holes and singularities. Before Penrose's contribution, physicists were divided into a number of schools concerning black holes and singularities, but none of the theories proved satisfactory. Topology revolutionized black hole theory, and allowed scientists to forge ahead and develop final theories concerning black holes and their formation, that all physicists could agree on.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-May-05-15-08-45.mp3</guid><pubDate>Thu, 05 May 2016 22:08:45 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524930/astrotalk_may_05_15_08_45.mp3" length="27280196" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>This is the third and last show on Kip Thorn'es book, Black Holes and Time Warps. This show discusses the contributions of British physicist Roger Penrose,who introduced the branch of mathematics of Topology into the study of black holes. Topology...</itunes:subtitle><itunes:summary><![CDATA[This is the third and last show on Kip Thorn'es book, Black Holes and Time Warps. This show discusses the contributions of British physicist Roger Penrose,who introduced the branch of mathematics of Topology into the study of black holes. Topology proved to be a powerful new tool in helping develop a theory on the formation and final stages of the development of black holes and singularities. Before Penrose's contribution, physicists were divided into a number of schools concerning black holes and singularities, but none of the theories proved satisfactory. Topology revolutionized black hole theory, and allowed scientists to forge ahead and develop final theories concerning black holes and their formation, that all physicists could agree on.]]></itunes:summary><itunes:duration>1706</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Black Holes from Kip Thorne's Book Part II</title><link>https://www.spreaker.com/episode/black-holes-from-kip-thorne-s-book-part-ii--23525636</link><description><![CDATA[In this episode, World War II impacts the study of black holes. The efforts of top scientists are devoted to the war effort, as they are busy developing weapons, and more specifically, nuclear weapons, both in the West and in the Soviet Union. An arms race takes place, where scientists on both side develop the atomic bomb, and then the hydrogen bomb. These scientists do not realize at the time that the theories they use and then apply in the development of nuclear bombs can then easily be applied to the study of the processes of what goes on inside stars, both during their lifetime, and at their death. The knowledge that physicists gained and developed in making the bomb are then transferred to the study of stars, after these scientists return to their laboratories and universities at war's end. There is no unanimity amongst scientists on singularities, or even if black holes can form, so its takes Roger Penrose, and his insertion of the mathematics of Topology into the discussion, before am acceptable  theory on black hole and singularity development can be formulated.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-April-28-15-00-00.mp3</guid><pubDate>Thu, 28 Apr 2016 22:00:45 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525636/astrotalk_april_28_15_00_00.mp3" length="51999974" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>In this episode, World War II impacts the study of black holes. The efforts of top scientists are devoted to the war effort, as they are busy developing weapons, and more specifically, nuclear weapons, both in the West and in the Soviet Union. An arms...</itunes:subtitle><itunes:summary><![CDATA[In this episode, World War II impacts the study of black holes. The efforts of top scientists are devoted to the war effort, as they are busy developing weapons, and more specifically, nuclear weapons, both in the West and in the Soviet Union. An arms race takes place, where scientists on both side develop the atomic bomb, and then the hydrogen bomb. These scientists do not realize at the time that the theories they use and then apply in the development of nuclear bombs can then easily be applied to the study of the processes of what goes on inside stars, both during their lifetime, and at their death. The knowledge that physicists gained and developed in making the bomb are then transferred to the study of stars, after these scientists return to their laboratories and universities at war's end. There is no unanimity amongst scientists on singularities, or even if black holes can form, so its takes Roger Penrose, and his insertion of the mathematics of Topology into the discussion, before am acceptable  theory on black hole and singularity development can be formulated.]]></itunes:summary><itunes:duration>3250</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Black Holes from Kip Thorne's Book Part I</title><link>https://www.spreaker.com/episode/black-holes-from-kip-thorne-s-book-part-i--23525807</link><description><![CDATA[Kip Thorne's book, Black Holes and Time Warps, is discussed. Kip Thorne is one of the world's pre-eminent theorists on Black Holes. Today, Dr. Thorne gives a lecture on his work, talks about his books, and discusses the discovery of Gravitational Waves at LIGO.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-April-21-15-00-00.mp3</guid><pubDate>Thu, 21 Apr 2016 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525807/astrotalk_april_21_15_00_00.mp3" length="28816196" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Kip Thorne's book, Black Holes and Time Warps, is discussed. Kip Thorne is one of the world's pre-eminent theorists on Black Holes. Today, Dr. Thorne gives a lecture on his work, talks about his books, and discusses the discovery of Gravitational...</itunes:subtitle><itunes:summary><![CDATA[Kip Thorne's book, Black Holes and Time Warps, is discussed. Kip Thorne is one of the world's pre-eminent theorists on Black Holes. Today, Dr. Thorne gives a lecture on his work, talks about his books, and discusses the discovery of Gravitational Waves at LIGO.]]></itunes:summary><itunes:duration>1802</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Space Shuttle Challenger</title><link>https://www.spreaker.com/episode/space-shuttle-challenger--23525003</link><description><![CDATA[30 years ago, on January 28, 1986  NASA experienced one of its worst setbacks when the Space Shuttle Challenger exploded in ruins, only 73 seconds after lift-off. A faulty O-Ring was determined to be at fault, but engineers had warned NASA of safety concerns with the O-Rings. Challenger was also launched when the outside temperature was 41 degrees Fahrenheit, 9 degrees below the established safe operating temperature of 50 degrees. Engineers had issued warnings about the dangers of operating below 50 degrees, but these warnings, like the warnings about the O-Rings, were disregarded and not passed on to top NASA officials. The Challenger disaster grounded the space shuttle program for 32 months. Human space flight was more common in the last quarter of the 21st century, and even though humankind is now experiencing a golden age in Astronomy, nothing could match the excitement of the human space missions of the last century. After the Space Shuttle Columbia disintegrated over Texas upon re-entry on a February 1, 2003 flight, the Space Shuttle program was grounded again. Even though NASA suffered setbacks on these 2 Space Shuttle missions, the Space Shuttle program operated 135 missions from 1981 - 2011, and returned some of the best science of our time . This show talks about how the projected benefits of operating a reusable low-Earth orbit space vehicle clashed with the realities of how difficult it became to maintain the fleet of 5 space shuttles. During each launch, 1 million things had to go right, but only 1 thing, like underestimating the problems that could be caused by 1 faulty O-Ring, could lead to disasters like Challenger and Columbia. The Space Shuttle program was nevertheless one of NASA's final accomplishments, and from them, a myriad of astronomy buffs grew out of the skies.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-January-28-15-01-00.mp3</guid><pubDate>Thu, 28 Jan 2016 23:01:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525003/astrotalk_january_28_15_01_00.mp3" length="27760013" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>30 years ago, on January 28, 1986  NASA experienced one of its worst setbacks when the Space Shuttle Challenger exploded in ruins, only 73 seconds after lift-off. A faulty O-Ring was determined to be at fault, but engineers had warned NASA of safety...</itunes:subtitle><itunes:summary><![CDATA[30 years ago, on January 28, 1986  NASA experienced one of its worst setbacks when the Space Shuttle Challenger exploded in ruins, only 73 seconds after lift-off. A faulty O-Ring was determined to be at fault, but engineers had warned NASA of safety concerns with the O-Rings. Challenger was also launched when the outside temperature was 41 degrees Fahrenheit, 9 degrees below the established safe operating temperature of 50 degrees. Engineers had issued warnings about the dangers of operating below 50 degrees, but these warnings, like the warnings about the O-Rings, were disregarded and not passed on to top NASA officials. The Challenger disaster grounded the space shuttle program for 32 months. Human space flight was more common in the last quarter of the 21st century, and even though humankind is now experiencing a golden age in Astronomy, nothing could match the excitement of the human space missions of the last century. After the Space Shuttle Columbia disintegrated over Texas upon re-entry on a February 1, 2003 flight, the Space Shuttle program was grounded again. Even though NASA suffered setbacks on these 2 Space Shuttle missions, the Space Shuttle program operated 135 missions from 1981 - 2011, and returned some of the best science of our time . This show talks about how the projected benefits of operating a reusable low-Earth orbit space vehicle clashed with the realities of how difficult it became to maintain the fleet of 5 space shuttles. During each launch, 1 million things had to go right, but only 1 thing, like underestimating the problems that could be caused by 1 faulty O-Ring, could lead to disasters like Challenger and Columbia. The Space Shuttle program was nevertheless one of NASA's final accomplishments, and from them, a myriad of astronomy buffs grew out of the skies.]]></itunes:summary><itunes:duration>1735</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>The Large Magellanic Cloud</title><link>https://www.spreaker.com/episode/the-large-magellanic-cloud--23524946</link><description><![CDATA[The Large and Small Magellanic Clouds (LMC & SMC) are 2 irregular dwarf galaxies that are part of the local group of galaxies. The LMC & SMC orbit our Milky Way galaxy, and because of this, they are currently being shredded or torn apart by the gravitational tidal forces that the Milky Way exert on them. These galaxies can only be viewed in the southern hemisphere. Features and interesting facts about the LMC & SMC will be discussed.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2016/AstroTalk-January-21-15-00-56.mp3</guid><pubDate>Thu, 21 Jan 2016 23:00:56 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524946/astrotalk_january_21_15_00_56.mp3" length="28080170" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>The Large and Small Magellanic Clouds (LMC &amp; SMC) are 2 irregular dwarf galaxies that are part of the local group of galaxies. The LMC &amp; SMC orbit our Milky Way galaxy, and because of this, they are currently being shredded or torn apart by the...</itunes:subtitle><itunes:summary><![CDATA[The Large and Small Magellanic Clouds (LMC & SMC) are 2 irregular dwarf galaxies that are part of the local group of galaxies. The LMC & SMC orbit our Milky Way galaxy, and because of this, they are currently being shredded or torn apart by the gravitational tidal forces that the Milky Way exert on them. These galaxies can only be viewed in the southern hemisphere. Features and interesting facts about the LMC & SMC will be discussed.]]></itunes:summary><itunes:duration>1756</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Water on Mars and Canadian Wins Nobel Prize in Physics</title><link>https://www.spreaker.com/episode/water-on-mars-and-canadian-wins-nobel-prize-in-physics--23524939</link><description><![CDATA[Water on Mars may be easy to detect, well, not really so easy, but finding where the water comes from is going to be much harder. Spelunkers or hikers may need to search out where the water comes from. So it may be much, much harder to find the source of the water, than it was to actually say that WE HAVE WATER ON MARS!!! A Canadian, Arthur B. McDonald, from the Sudbury Neutrino Observatory Collaboration and Queen’s University, is this year's winner of the Nobel Prize for Physics. Dr. McDonald is sharing the prize with Takaaki Kajita, from the Super-Kamiokande Collaboration, University of Tokyo, Kashiwa, Japan. The prize was awarded for the pair's research in neutrino research. Neutrinos are tiny particles that are produced in the cores of stars. They are also produced in abundance when a star explodes in a supernova explosion. 99% of the energy from a supernova explosion is thought to be carried away by neutrinos. According to the Standard Model of Particle Physics, it was assumed that neutrinos have zero mass.The Standard Model has worked very well in providing excellent descriptions for the behavior of nearly all elementary particles, but it seems to have failed for the neutrino.  Dr. McDonald and Kajita have shown that neutrinos oscillate. If they oscillate, then they  must have mass. This discovery will surely affect our view of the universe. Will the Standard Model have to be revised after these finding on neutrinos? Finally, photos from the New Horizons Spacecraft were discussed. New Horizons whizzed by the dwarf planet Pluto on July 14, 2015, coming within 7,800 kilomteres of the dwarf planet. On September 5, New Horizons began sending back data and pictures on its close encounter with Pluto. All the data will take approximately 1 year to be intercepted and downloaded on Earth. Today, some of the findings from the pictures were discussed. More pictures on the encounter can be seen at www. nasa. gov.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2015/AstroTalk-October-08-15-00-00.mp3</guid><pubDate>Thu, 08 Oct 2015 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524939/astrotalk_october_08_15_00_00.mp3" length="26879791" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Water on Mars may be easy to detect, well, not really so easy, but finding where the water comes from is going to be much harder. Spelunkers or hikers may need to search out where the water comes from. So it may be much, much harder to find the source...</itunes:subtitle><itunes:summary><![CDATA[Water on Mars may be easy to detect, well, not really so easy, but finding where the water comes from is going to be much harder. Spelunkers or hikers may need to search out where the water comes from. So it may be much, much harder to find the source of the water, than it was to actually say that WE HAVE WATER ON MARS!!! A Canadian, Arthur B. McDonald, from the Sudbury Neutrino Observatory Collaboration and Queen’s University, is this year's winner of the Nobel Prize for Physics. Dr. McDonald is sharing the prize with Takaaki Kajita, from the Super-Kamiokande Collaboration, University of Tokyo, Kashiwa, Japan. The prize was awarded for the pair's research in neutrino research. Neutrinos are tiny particles that are produced in the cores of stars. They are also produced in abundance when a star explodes in a supernova explosion. 99% of the energy from a supernova explosion is thought to be carried away by neutrinos. According to the Standard Model of Particle Physics, it was assumed that neutrinos have zero mass.The Standard Model has worked very well in providing excellent descriptions for the behavior of nearly all elementary particles, but it seems to have failed for the neutrino.  Dr. McDonald and Kajita have shown that neutrinos oscillate. If they oscillate, then they  must have mass. This discovery will surely affect our view of the universe. Will the Standard Model have to be revised after these finding on neutrinos? Finally, photos from the New Horizons Spacecraft were discussed. New Horizons whizzed by the dwarf planet Pluto on July 14, 2015, coming within 7,800 kilomteres of the dwarf planet. On September 5, New Horizons began sending back data and pictures on its close encounter with Pluto. All the data will take approximately 1 year to be intercepted and downloaded on Earth. Today, some of the findings from the pictures were discussed. More pictures on the encounter can be seen at www. nasa. gov.]]></itunes:summary><itunes:duration>1680</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Planets of the Solar System and Pluto</title><link>https://www.spreaker.com/episode/planets-of-the-solar-system-and-pluto--23525987</link><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2015/AstroTalk-September-24-15-02-00.mp3</guid><pubDate>Thu, 24 Sep 2015 22:02:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525987/astrotalk_september_24_15_02_00.mp3" length="27008105" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:duration>1689</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Astrotalk with Marco - Episode December 4, 2014</title><link>https://www.spreaker.com/episode/astrotalk-with-marco-episode-december-4-2014--23524951</link><description><![CDATA[Neutrinos are elementary particles that are nearly massless, and that have half integer spin. They come in many flavors, and the anti-neutrino also exists. Neutrinos are produced in the core of stars, in nuclear reactors, or when atoms are hit by cosmic rays. Each second on Earth, 65 billion neutrinos travel through 1 square inch of matter. If your thumb is 1 square inch in size, then 65 billion neutrinos travel through your thumb each second. Neutrinos are almost impossible to detect, but on February 23 , 1987, 24 neutrinos were detected on Earth. 3 hours later, Earthlings in the southern hemisphere then saw a supernova, Supernova 1987a, about 3 hours after the neutrinos were detected. 99% of the energy radiated away by a star during a core-collapse supernova is carried away by neutrinos. This event marked the first time in history that neutrinos from a supernova were observed directly. The science of Neutrino Astronomy was then born. It is very difficult to detect nuclear reactions in the Sun using visible light, because photons can take hundreds of thousands of years to reach the Sun's surface. Since neutrinos are created in the core then move out at the speed of light, neutrino astronomy can be used to observe the core of the Sun directly.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2014/20141204-150000-to-20141204-153500.mp3</guid><pubDate>Thu, 04 Dec 2014 23:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524951/20141204_150000_to_20141204_153500.mp3" length="33453119" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Neutrinos are elementary particles that are nearly massless, and that have half integer spin. They come in many flavors, and the anti-neutrino also exists. Neutrinos are produced in the core of stars, in nuclear reactors, or when atoms are hit by...</itunes:subtitle><itunes:summary><![CDATA[Neutrinos are elementary particles that are nearly massless, and that have half integer spin. They come in many flavors, and the anti-neutrino also exists. Neutrinos are produced in the core of stars, in nuclear reactors, or when atoms are hit by cosmic rays. Each second on Earth, 65 billion neutrinos travel through 1 square inch of matter. If your thumb is 1 square inch in size, then 65 billion neutrinos travel through your thumb each second. Neutrinos are almost impossible to detect, but on February 23 , 1987, 24 neutrinos were detected on Earth. 3 hours later, Earthlings in the southern hemisphere then saw a supernova, Supernova 1987a, about 3 hours after the neutrinos were detected. 99% of the energy radiated away by a star during a core-collapse supernova is carried away by neutrinos. This event marked the first time in history that neutrinos from a supernova were observed directly. The science of Neutrino Astronomy was then born. It is very difficult to detect nuclear reactions in the Sun using visible light, because photons can take hundreds of thousands of years to reach the Sun's surface. Since neutrinos are created in the core then move out at the speed of light, neutrino astronomy can be used to observe the core of the Sun directly.]]></itunes:summary><itunes:duration>2096</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Astrotalk with Marco - Episode November 27, 2014</title><link>https://www.spreaker.com/episode/astrotalk-with-marco-episode-november-27-2014--23525000</link><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2014/20141127-150000-to-20141127-153500.mp3</guid><pubDate>Thu, 27 Nov 2014 23:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525000/20141127_150000_to_20141127_153500.mp3" length="33524843" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:duration>2101</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Astrotalk</title><link>https://www.spreaker.com/episode/astrotalk--23526068</link><description><![CDATA[Comets have been in the news lately. The Philae Lander from ESA's Rosetta spacecraft touched down on Comet 67 P, and other comets, such as Comet Siding Spring and ISON have come close to Mars in the last year. Comets have a lot less gravity than our Earth, so this made it very challenging for the Philae Lander to land on 67 P. As 67 P gets closer to the Sun, then it is hoped that the Philae Lander on 67 P will receive more sunlight and then will finally wake up, and start talking to Earth. Asteroid Bennu will also discussed.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2014/AstroTalk-November-20-15-00-00.mp3</guid><pubDate>Thu, 20 Nov 2014 23:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23526068/astrotalk_november_20_15_00_00.mp3" length="28352267" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Comets have been in the news lately. The Philae Lander from ESA's Rosetta spacecraft touched down on Comet 67 P, and other comets, such as Comet Siding Spring and ISON have come close to Mars in the last year. Comets have a lot less gravity than our...</itunes:subtitle><itunes:summary><![CDATA[Comets have been in the news lately. The Philae Lander from ESA's Rosetta spacecraft touched down on Comet 67 P, and other comets, such as Comet Siding Spring and ISON have come close to Mars in the last year. Comets have a lot less gravity than our Earth, so this made it very challenging for the Philae Lander to land on 67 P. As 67 P gets closer to the Sun, then it is hoped that the Philae Lander on 67 P will receive more sunlight and then will finally wake up, and start talking to Earth. Asteroid Bennu will also discussed.]]></itunes:summary><itunes:duration>1773</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Astrotalk with Marco - Episode August 21</title><link>https://www.spreaker.com/episode/astrotalk-with-marco-episode-august-21--23525009</link><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2014/20140821-150000-to-20140821-154500.mp3</guid><pubDate>Thu, 21 Aug 2014 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525009/20140821_150000_to_20140821_154500.mp3" length="43013261" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:duration>2695</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Astrotalk with Marco - Episode 14</title><link>https://www.spreaker.com/episode/astrotalk-with-marco-episode-14--23524953</link><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2014/20140731-150000-to-20140731-154500.mp3</guid><pubDate>Thu, 31 Jul 2014 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524953/20140731_150000_to_20140731_154500.mp3" length="42930278" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:duration>2690</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Astrotalk with Marco - Episode 13</title><link>https://www.spreaker.com/episode/astrotalk-with-marco-episode-13--23524958</link><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2014/20140724-150000-to-20140724-160000.mp3</guid><pubDate>Thu, 24 Jul 2014 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524958/20140724_150000_to_20140724_160000.mp3" length="57336794" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:duration>3592</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>Astrotalk with Marco - Episode 12</title><link>https://www.spreaker.com/episode/astrotalk-with-marco-episode-12--23526083</link><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2014/20140717-150000-to-20140717-160000.mp3</guid><pubDate>Thu, 17 Jul 2014 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23526083/20140717_150000_to_20140717_160000.mp3" length="57177917" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:duration>3582</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>AstroTalk with Marco - Episode 6</title><link>https://www.spreaker.com/episode/astrotalk-with-marco-episode-6--23525016</link><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2014/20140605-150000-to-20140605-160000.mp3</guid><pubDate>Thu, 05 Jun 2014 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525016/20140605_150000_to_20140605_160000.mp3" length="57227123" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:duration>3585</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>AstroTalk with Marco - Episode 4</title><link>https://www.spreaker.com/episode/astrotalk-with-marco-episode-4--23525013</link><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2014/20140522-150000-to-20140522-154500.mp3</guid><pubDate>Thu, 22 May 2014 22:00:00 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23525013/20140522_150000_to_20140522_154500.mp3" length="42913598" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:duration>2689</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>AstroTalk with Marco - Episode 2</title><link>https://www.spreaker.com/episode/astrotalk-with-marco-episode-2--23524954</link><description><![CDATA[Second episode on Magnetars and Death Stars.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2014/20140508-150000-to-20140508-154500.mp3</guid><pubDate>Thu, 08 May 2014 22:09:57 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524954/20140508_150000_to_20140508_154500.mp3" length="43022852" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>Second episode on Magnetars and Death Stars.</itunes:subtitle><itunes:summary><![CDATA[Second episode on Magnetars and Death Stars.]]></itunes:summary><itunes:duration>2696</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item><item><title>AstroTalk with Marco - Episode 1: Death Star</title><link>https://www.spreaker.com/episode/astrotalk-with-marco-episode-1-death-star--23524982</link><description><![CDATA[In 1967 Jocelyn Bell, then a graduate student, discovered the first neutron star. The pulse emitted by this neutron star puzzled astronomers.  Neutron stars emit beams of electromagnetic radiation as they spin, and spin very rapidly they do. Unable to classify this object, it was dubbed LGM1, or Little Green Men. Some people believed that the pulse of radiation from this neutron star was a signal sent by an alien civilization, because the pulses it was emitting were at regular intervals. This neutron star was later dubbed PSR B1919+2. The P stands for pulsar, because neutron stars emit radiation in regular, pulsed intervals. Neutron stars are made of neutrons, but they are not really stars. They are the remains of a star that has died in a supernova explosion. Some neutron stars become magnetars, the most magnetized objects in our universe. In 2007, the magnetar SGR 1806 underwent a starquake. In a fraction of a second, more energy was emittted by this neutron star than our Sun emits in 100,000 years. Magnetars can be death stars if they are too close to Earth, and if their axes of rotation are pointed at the Earth. When stars like SGR 1806 emit powerful gammar rays bursts, GBRs, then we'd better watch out. GBRs are amongst the most powerful bursts of energy in our universe. Today , you will learn about magnetars and death stars.]]></description><guid isPermaLink="false">https://playlist.citr.ca/podcasting/audio/2014/20140501-150000-to-20140501-154500.mp3</guid><pubDate>Thu, 01 May 2014 22:07:48 +0000</pubDate><enclosure url="https://api.spreaker.com/download/episode/23524982/20140501_150000_to_20140501_154500.mp3" length="43012427" type="audio/mpeg"/><itunes:author>CiTR &amp; Discorder Magazine</itunes:author><itunes:subtitle>In 1967 Jocelyn Bell, then a graduate student, discovered the first neutron star. The pulse emitted by this neutron star puzzled astronomers.  Neutron stars emit beams of electromagnetic radiation as they spin, and spin very rapidly they do. Unable to...</itunes:subtitle><itunes:summary><![CDATA[In 1967 Jocelyn Bell, then a graduate student, discovered the first neutron star. The pulse emitted by this neutron star puzzled astronomers.  Neutron stars emit beams of electromagnetic radiation as they spin, and spin very rapidly they do. Unable to classify this object, it was dubbed LGM1, or Little Green Men. Some people believed that the pulse of radiation from this neutron star was a signal sent by an alien civilization, because the pulses it was emitting were at regular intervals. This neutron star was later dubbed PSR B1919+2. The P stands for pulsar, because neutron stars emit radiation in regular, pulsed intervals. Neutron stars are made of neutrons, but they are not really stars. They are the remains of a star that has died in a supernova explosion. Some neutron stars become magnetars, the most magnetized objects in our universe. In 2007, the magnetar SGR 1806 underwent a starquake. In a fraction of a second, more energy was emittted by this neutron star than our Sun emits in 100,000 years. Magnetars can be death stars if they are too close to Earth, and if their axes of rotation are pointed at the Earth. When stars like SGR 1806 emit powerful gammar rays bursts, GBRs, then we'd better watch out. GBRs are amongst the most powerful bursts of energy in our universe. Today , you will learn about magnetars and death stars.]]></itunes:summary><itunes:duration>2695</itunes:duration><itunes:explicit>clean</itunes:explicit><itunes:image href="https://d3wo5wojvuv7l.cloudfront.net/images.spreaker.com/nuvolari-assets/light_blue_square_mic.jpg"/><itunes:episodeType>full</itunes:episodeType></item></channel></rss>
