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<title>NASA's Chandra X-ray Observatory Podcasts</title>
<link>http://chandra.harvard.edu/resources/podcasts/</link>
<description>NASA's Chandra X-ray Observatory Podcasts :: Recent Discoveries from NASA's Chandra X-ray Observatory in an Audio/Video Format</description>
<language>en-us</language>
<copyright>no copyright</copyright>
<managingEditor>cxcpub@cfa.harvard.edu (Chandra webmaster)</managingEditor>
<webMaster>cxcpub@cfa.harvard.edu (Chandra webmaster)</webMaster>
<category>Science &amp; Technology</category>
<category>Government</category>
<itunes:category text="Science &amp; Medicine">
<itunes:category text="Natural Sciences" />
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<itunes:category text="Science &amp; Medicine" />
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<itunes:keywords>Chandra, X-ray, Astronomy, NASA, Observatory</itunes:keywords>
<itunes:author>NASA/Chandra X-ray Center</itunes:author>
<itunes:subtitle>
The latest audio/video features from NASA's Chandra X-ray Observatory 
</itunes:subtitle>
<itunes:owner>
<itunes:name>Kim Kowal Arcand</itunes:name>
<itunes:email>cxcpub@cfa.harvard.edu </itunes:email>
</itunes:owner>
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<title>Chandra X-ray Observatory Podcasts</title>
<link>http://chandra.harvard.edu/resources/podcasts/</link>
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	<item>
		<title>GRS 1915 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts250609.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts250609.html</guid>
		<pubDate>Thu, 25 Jun 2009 12:00:00 EST</pubDate>
		<description>We start with an optical and infrared image that shows the crowded area around the object known as GRS 1915+105, or GRS 1915 for short.</description>
		<enclosure type="video/x-m4v" url="http://chandra.harvard.edu/resources/podcasts/media/pod250609.m4v" length="15070000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:27</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod250609.m4v" fileSize="15070000" type="video/x-m4v" duration="87" isDefault="true">
		<media:title>GRS 1915 in 60 Seconds</media:title>
		<media:description>We start with an optical and infrared image that shows the crowded area around the object known as GRS 1915+105, or GRS 1915 for short.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod250609_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Galactic Ridge in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts290509.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts290509.html</guid>
		<pubDate>Fri, 29 May 2009 12:00:00 EST</pubDate>
		<description>This sequence begins with an infrared view from the Spitzer Space Telescope of the central region of the Milky Way.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod290509.m4v" length="8290000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:01</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod290509.m4v" fileSize="8290000" type="audio/aiff" duration="61" isDefault="true">
		<media:title>Galactic Ridge in 60 Seconds</media:title>
		<media:description>This sequence begins with an infrared view from the Spitzer Space Telescope of the central region of the Milky Way.</media:description>
		<media:thumbnail url=" http://chandra.harvard.edu/resources/podcasts/images/pod290509_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>MacsJ0717 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts150509.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts150509.html</guid>
		<pubDate>Fri, 15 May 2009 12:00:00 EST</pubDate>
		<description>This image contains one of the most complex galaxy clusters known, which is located about 5.4 billion light years from Earth.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod150509.m4v" length="12740000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:15</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod150509.m4v" fileSize="12740000" type="audio/aiff" duration="75" isDefault="true">
		<media:title>MacsJ0717 in 60 Seconds</media:title>
		<media:description>This image contains one of the most complex galaxy clusters known, which is located about 5.4 billion light years from Earth.</media:description>
		<media:thumbnail url=" http://chandra.harvard.edu/resources/podcasts/images/pod150509_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Peering Into the X-ray Future</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts050509.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts050509.html</guid>
		<pubDate>Tue, 05 May 2009 12:00:00 EST</pubDate>
		<description>This episode will touch on some of the areas in which astronomers hope X-ray telescopes will push our knowledge forward in the years to come.</description>
		<enclosure type="video/x-m4v" url="http://chandra.harvard.edu/resources/podcasts/media/pod050509.m4v" length="62830000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:05:22</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod050509.m4v" fileSize="62830000" type="video/x-m4v" duration="322" isDefault="true">
		<media:title>Peering Into the X-ray Future</media:title>
		<media:description>This episode will touch on some of the areas in which astronomers hope X-ray telescopes will push our knowledge forward in the years to come.</media:description>
		<media:thumbnail url=" http://chandra.harvard.edu/resources/podcasts/images/pod050509_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Medusa in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts010509.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts010509.html</guid>
		<pubDate>Fri, 01 May 2009 12:00:00 EST</pubDate>
		<description>NGC 4194 is a galaxy that is found about 110 million light years from Earth.</description>
		<enclosure type="video/x-m4v" url="http://chandra.harvard.edu/resources/podcasts/media/pod010509.m4v" length="13280000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:17</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod010509.m4v" fileSize="13280000" type="video/x-m4v" duration="77" isDefault="true">
		<media:title>Medusa in 60 Seconds</media:title>
		<media:description>NGC 4194 is a galaxy that is found about 110 million light years from Earth.</media:description>
		<media:thumbnail url=" http://chandra.harvard.edu/resources/podcasts/images/pod010509_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>30 Doradus in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts170409.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts170409.html</guid>
		<pubDate>Fri, 17 Apr 2009 12:00:00 EST</pubDate>
		<description>Chandra's X-ray image of the Tarantula Nebula gives scientists a close-up view of the drama of star formation and star evolution.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod170409.m4v" length="7950000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:12</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod170409.m4v" fileSize="7950000" type="audio/aiff" duration="72" isDefault="true">
		<media:title>30 Doradus in 60 Seconds</media:title>
		<media:description>Chandra's X-ray image of the Tarantula Nebula gives scientists a close-up view of the drama of star formation and star evolution.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod170409_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>PSR B1509-58 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts030409.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts030409.html</guid>
		<pubDate>Fri, 03 Apr 2009 12:00:00 EST</pubDate>
		<description>A small dense object is responsible for the remarkably complex and intriguing structures seen in this image from the Chandra X-ray Observatory.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod030409.m4v" length="14410000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:23</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod030409.m4v" fileSize="14410000" type="audio/aiff" duration="83" isDefault="true">
		<media:title>PSR B1509-58 in 60 Seconds</media:title>
		<media:description>A small dense object is responsible for the remarkably complex and intriguing structures seen in this image from the Chandra X-ray Observatory.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod030409_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>NGC 604 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts230309.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts230309.html</guid>
		<pubDate>Mon, 23 Mar 2009 12:00:00 EST</pubDate>
		<description>NGC 604 is a divided neighborhood in the galaxy M33, where some 200 hot, young massive stars reside.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod230309.m4v" length="13030000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:16</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod230309.m4v" fileSize="13030000" type="audio/aiff" duration="76" isDefault="true">
		<media:title>NGC 604 in 60 Seconds</media:title>
		<media:description>NGC 604 is a divided neighborhood in the galaxy M33, where some 200 hot, young massive stars reside.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod230309_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Crab Nebula in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts050309.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts050309.html</guid>
		<pubDate>Thu, 05 Mar 2009 12:00:00 EST</pubDate>
		<description>The Crab Nebula is one of the best-known images ever taken by the Chandra X-ray Observatory.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod050309.m4v" length="13426000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:18</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod050309.m4v" fileSize="13426000" type="audio/aiff" duration="78" isDefault="true">
		<media:title>Crab Nebula in 60 Seconds</media:title>
		<media:description>The Crab Nebula is one of the best-known images ever taken by the Chandra X-ray Observatory.</media:description>
		<media:thumbnail url=" http://chandra.harvard.edu/resources/podcasts/images/pod050309_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>M101 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts100209.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts100209.html</guid>
		<pubDate>Tue, 10 Feb 2009 12:00:00 EST</pubDate>
		<description>This image of the spiral galaxy Messier 101 is a composite of observations from NASA's three Great Observatories.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod100209.m4v" length="12830000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:12</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod100209.m4v" fileSize="12830000" type="audio/aiff" duration="72" isDefault="true">
		<media:title>M101 in 60 Seconds</media:title>
		<media:description>This image of the spiral galaxy Messier 101 is a composite of observations from NASA's three Great Observatories.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod100209_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Abell 85 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts230109.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts230109.html</guid>
		<pubDate>Fri, 23 Jan 2009 12:00:00 EST</pubDate>
		<description>The composite image shows the galaxy cluster known as Abell 85, which is located about 740 million light years from Earth.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod230109.m4v" length="13210000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:17</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod230109.m4v" fileSize="13210000" type="audio/aiff" duration="77" isDefault="true">
		<media:title>Abell 85 in 60 Seconds</media:title>
		<media:description>The composite image shows the galaxy cluster known as Abell 85, which is located about 740 million light years from Earth.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod230109_thm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>3-D Fly-Through of Cassiopeia A</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts080109.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts080109.html</guid>
		<pubDate>Thu, 08 Jan 2009 12:00:00 EST</pubDate>
		<description>For the first time, a multiwavelength three-dimensional (3-D) reconstruction of a supernova remnant has been created.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod080109.m4v" length="14580000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:23</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod080109.m4v" fileSize="14580000" type="audio/aiff" duration="83" isDefault="true">
		<media:title>3-D Fly-Through of Cassiopeia A</media:title>
		<media:description>For the first time, a multiwavelength three-dimensional (3-D) reconstruction of a supernova remnant has been created.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod080109_thm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>G292.01+8 in 60 Seconds </title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts221208.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts221208.html</guid>
		<pubDate>Mon, 22 Dec 2008 12:00:00 EST</pubDate>
		<description>This image shows how complex a star's afterlife can be.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod221208.m4v" length="16770000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:35</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod221208.m4v" fileSize="16770000" type="audio/aiff" duration="95" isDefault="true">
		<media:title>G292.01+8 in 60 Seconds </media:title>
		<media:description>This image shows how complex a star's afterlife can be.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod221208_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>M84 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts121208.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts121208.html</guid>
		<pubDate>Fri, 12 Dec 2008 12:00:00 EST</pubDate>
		<description>M84 is a massive elliptical galaxy located about 55 million light years from Earth in the Virgo Cluster.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod121208.m4v" length="10170000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:04</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod121208.m4v" fileSize="10170000" type="audio/aiff" duration="64" isDefault="true">
		<media:title>M84 in 60 Seconds</media:title>
		<media:description>M84 is a massive elliptical galaxy located about 55 million light years from Earth in the Virgo Cluster.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod121208_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>M87 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts251108.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts251108.html</guid>
		<pubDate>Tue, 25 Nov 2008 12:00:00 EST</pubDate>
		<description>M87 is a giant elliptical galaxy. At a distance of about 60 million light-years from Earth, M87 is the largest galaxy in the Virgo cluster of some 2,000 galaxies.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod251108.m4v" length="14667000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:22</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod251108.m4v" fileSize="14667000" type="audio/aiff" duration="82" isDefault="true">
		<media:title>M87 in 60 Seconds</media:title>
		<media:description>M87 is a giant elliptical galaxy. At a distance of about 60 million light-years from Earth, M87 is the largest galaxy in the Virgo cluster of some 2,000 galaxies.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod251108_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Abell 1689 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts141108.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts141108.html</guid>
		<pubDate>Fri, 14 Nov 2008 12:00:00 EST</pubDate>
		<description>Abell 1689 is a massive cluster of galaxies located about 2.3 billion light-years away. </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod141108.m4v" length="15610000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:30</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod141108.m4v" fileSize="15610000" type="audio/aiff" duration="90" isDefault="true">
		<media:title>Abell 1689 in 60 Seconds</media:title>
		<media:description>Abell 1689 is a massive cluster of galaxies located about 2.3 billion light-years away. </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod141108_thm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>SN1996cr in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts311008.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts311008.html</guid>
		<pubDate>Fri, 31 Oct 2008 12:00:00 EST</pubDate>
		<description>In 1995 or 1996 a supernova exploded in a nearby galaxy, but no one on Earth knew it at the time. </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod311008.m4v" length="9560000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:13</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod311008.m4v" fileSize="9560000" type="audio/aiff" duration="73" isDefault="true">
		<media:title>SN1996cr in 60 Seconds</media:title>
		<media:description>In 1995 or 1996 a supernova exploded in a nearby galaxy, but no one on Earth knew it at the time. </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod311008_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>RCW 108 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts161008.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts161008.html</guid>
		<pubDate>Thu, 16 Oct 2008 12:00:00 EST</pubDate>
		<description>RCW 108 is a region where stars are actively forming about 4,000 light-years from Earth.  </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod161008.m4v" length="8330000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:29</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod161008.m4v" fileSize="8330000" type="audio/aiff" duration="89" isDefault="true">
		<media:title>RCW 108 in 60 Seconds</media:title>
		<media:description>RCW 108 is a region where stars are actively forming about 4,000 light-years from Earth.  </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod161008_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Perseus A in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts021008.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts021008.html</guid>
		<pubDate>Thu, 02 Oct 2008 12:00:00 EST</pubDate>
		<description>The giant galaxy, Perseus A, which is also known as NGC 1275, is a well-known source of strong radio radiation.  </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod021008.m4v" length="7290000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:31</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod021008.m4v" fileSize="7290000" type="audio/aiff" duration="91" isDefault="true">
		<media:title>Perseus A in 60 Seconds</media:title>
		<media:description>The giant galaxy, Perseus A, which is also known as NGC 1275, is a well-known source of strong radio radiation.  </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod021008_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Cat's Eye Nebula in 60 Seconds Plus</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts190908.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts190908.html</guid>
		<pubDate>Fri, 19 Sep 2008 12:00:00 EST</pubDate>
		<description>This composite of data from NASA's Chandra X-ray Observatory and the Hubble Space Telescope is another look for NGC 6543, better known as the Cat's Eye nebula.  </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod190908.m4v" length="6820000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:48</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod190908.m4v" fileSize="6820000" type="audio/aiff" duration="108" isDefault="true">
		<media:title>Cat's Eye Nebula in 60 Seconds Plus</media:title>
		<media:description>This composite of data from NASA's Chandra X-ray Observatory and the Hubble Space Telescope is another look for NGC 6543, better known as the Cat's Eye nebula.  </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod190908_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Macs J0025.4-1222 in 60 Seconds Plus</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts040908.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts040908.html</guid>
		<pubDate>Thu, 04 Sep 2008 12:00:00 EST</pubDate>
		<description>Two galaxy clusters, each a quadrillion times the mass of the Sun, collided to form the system formally known as Macs J0025.4-1222. </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod040908.m4v" length="8532000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:49</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod040908.m4v" fileSize="8532000" type="audio/aiff" duration="109" isDefault="true">
		<media:title>Macs J0025.4-1222 in 60 Seconds Plus</media:title>
		<media:description>Two galaxy clusters, each a quadrillion times the mass of the Sun, collided to form the system formally known as Macs J0025.4-1222. </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod040908_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>M81 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts210808.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts210808.html</guid>
		<pubDate>Thu, 21 Aug 2008 12:00:00 EST</pubDate>
		<description>This image of the mammoth spiral galaxy M81, located about 12 million light years away, contains data from four different NASA satellites. </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod210808.m4v" length="6430000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:06</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod210808.m4v" fileSize="6430000" type="audio/aiff" duration="66" isDefault="true">
		<media:title>M81 in 60 Seconds</media:title>
		<media:description>This image of the mammoth spiral galaxy M81, located about 12 million light years away, contains data from four different NASA satellites. </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod210808_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>SN 1006 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts080808.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts080808.html</guid>
		<pubDate>Fri, 08 Aug 2008 12:00:00 EST</pubDate>
		<description>The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world. It was brighter than Venus, and visible during the day for weeks.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod080808.m4v" length="6820000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:09</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod080808.m4v" fileSize="6820000" type="audio/aiff" duration="69" isDefault="true">
		<media:title>SN 1006 in 60 Seconds</media:title>
		<media:description>The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world. It was brighter than Venus, and visible during the day for weeks.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod080808_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Centaurus A in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts240708.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts240708.html</guid>
		<pubDate>Thu, 24 Jul 2008 12:00:00 EST</pubDate>
		<description>There is nothing subtle about the black hole in the galaxy Centaurus A.  First off, it's about 10 million times more massive than the sun, and Chandra's X-ray image shows it's not just sitting quietly as a bright point in the middle.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod240708.m4v" length="6500000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:14</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod240708.m4v" fileSize="6500000" type="audio/aiff" duration="74" isDefault="true">
		<media:title>Centaurus A in 60 Seconds</media:title>
		<media:description>There is nothing subtle about the black hole in the galaxy Centaurus A.  First off, it's about 10 million times more massive than the sun, and Chandra's X-ray image shows it's not just sitting quietly as a bright point in the middle.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod240708_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>NGC 4258 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts110708.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts110708.html</guid>
		<pubDate>Fri, 11 Jul 2008 12:00:00 EST</pubDate>
		<description> A composite image of NGC 4258, about 25 million light-years from Earth, shows an X-shaped pattern when seen in different types of light.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod110708.m4v" length="4130000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:09</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod110708.m4v" fileSize="4130000" type="audio/aiff" duration="69" isDefault="true">
		<media:title>NGC 4258 in 60 Seconds</media:title>
		<media:description> A composite image of NGC 4258, about 25 million light-years from Earth, shows an X-shaped pattern when seen in different types of light.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod110708_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>G1.9+0.3 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts300608.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts300608.html</guid>
		<pubDate>Mon, 30 Jun 2008 12:00:00 EST</pubDate>
		<description>About a hundred and forty years ago, the light from a supernova explosion in our galaxy reached the Earth, but no one saw it.  The discovery of this supernova remnant helps astronomers better understand how often these stellar time-bombs go off in our galaxy.  </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod300608.m4v" length="5850000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:11</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod300608.m4v" fileSize="5850000" type="audio/aiff" duration="71" isDefault="true">
		<media:title>G1.9+0.3 in 60 Seconds</media:title>
		<media:description>About a hundred and forty years ago, the light from a supernova explosion in our galaxy reached the Earth, but no one saw it.  The discovery of this supernova remnant helps astronomers better understand how often these stellar time-bombs go off in our galaxy.  </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod300608_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>3C321 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts120608.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts120608.html</guid>
		<pubDate>Thu, 12 Jun 2008 12:00:00 EST</pubDate>
		<description>In 3C321, a jet from a black hole in one of the galaxies is pummeling its neighbor galaxy, the first time this type of galactic violence has ever been seen.  The jet could bring big trouble for any planets in its path, but could also trigger a burst of star formation in its wake. </description>
		<enclosure type="video/x-m4v" url="http://chandra.harvard.edu/resources/podcasts/media/pod120608.m4v" length="3360000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:29</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod120608.m4v" fileSize="3360000" type="video/x-m4v" duration="89" isDefault="true">
		<media:title>3C321 in 60 Seconds</media:title>
		<media:description>In 3C321, a jet from a black hole in one of the galaxies is pummeling its neighbor galaxy, the first time this type of galactic violence has ever been seen.  The jet could bring big trouble for any planets in its path, but could also trigger a burst of star formation in its wake. </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod120608_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Just Two Numbers Is All You Need</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts020608.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts020608.html</guid>
		<pubDate>Mon, 02 Jun 2008 12:00:00 EST</pubDate>
		<description>Black holes sound wildly complicated.  After all, there are all sorts of bizarre things going on: intense gravity, the warping of the fabric of space, the distortion of time itself.  But when it comes to describing black holes, it comes down to just two numbers: the mass of the black hole and its spin. </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod020608.m4v" length="42460000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:05:47</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod020608.m4v" fileSize="42460000" type="audio/aiff" duration="347" isDefault="true">
		<media:title>Just Two Numbers Is All You Need</media:title>
		<media:description>Black holes sound wildly complicated.  After all, there are all sorts of bizarre things going on: intense gravity, the warping of the fabric of space, the distortion of time itself.  But when it comes to describing black holes, it comes down to just two numbers: the mass of the black hole and its spin. </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod020608_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Sombrero Galaxy in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts210508.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts210508.html</guid>
		<pubDate>Wed, 21 May 2008 12:00:00 EST</pubDate>
		<description>Like the Milky Way, Sombrero is a spiral galaxy. However, we see Sombrero edge-on from our vantage point from Earth, rather than the face-down perspective that is more familiar. </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod210508.m4v" length="7970000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:45</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod210508.m4v" fileSize="7970000" type="audio/aiff" duration="105" isDefault="true">
		<media:title>Sombrero Galaxy in 60 Seconds</media:title>
		<media:description>Like the Milky Way, Sombrero is a spiral galaxy. However, we see Sombrero edge-on from our vantage point from Earth, rather than the face-down perspective that is more familiar. </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod210508_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Kepler's Supernova Remnant in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts070508.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts070508.html</guid>
		<pubDate>Wed, 07 May 2008 12:00:00 EST</pubDate>
		<description>The supernova explosion that created this object was witnessed on Earth about 400 ago years by many skywatchers, including the astronomer Johannes Kepler. This object, which now bears Kepler's name, is the remains of a massive star's demise. </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod070508.m4v" length="6695000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:11</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod070508.m4v" fileSize="6695000" type="audio/aiff" duration="71" isDefault="true">
		<media:title>Kepler's Supernova Remnant in 60 Seconds</media:title>
		<media:description>The supernova explosion that created this object was witnessed on Earth about 400 ago years by many skywatchers, including the astronomer Johannes Kepler. This object, which now bears Kepler's name, is the remains of a massive star's demise. </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod070508_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>M82 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts140408.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts140408.html</guid>
		<pubDate>Mon, 14 Apr 2008 12:00:00 EST</pubDate>
		<description>When seen in visible light from the Hubble Space Telescope, M82 looks like an ordinary spiral galaxy. </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod140408.m4v" length="5467000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:58</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod140408.m4v" fileSize="5467000" type="audio/aiff" duration="58" isDefault="true">
		<media:title>M82 in 60 Seconds</media:title>
		<media:description>When seen in visible light from the Hubble Space Telescope, M82 looks like an ordinary spiral galaxy. </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod140408_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Exploring The Large Magellanic Cloud</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts040208.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts040208.html</guid>
		<pubDate>Wed, 02 Apr 2008 12:00:00 EST</pubDate>
		<description>The Large Magellanic Cloud, known as the LMC, is a nearby satellite galaxy of our own Milky Way. At a distance of around 160,000 light-years, the LMC is the third closest galaxy to us. But the LMC is more than just a nice little sidekick.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod040208.m4v" length="44340000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:06:32</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod040208.m4v" fileSize="44340000" type="audio/aiff" duration="392" isDefault="true">
		<media:title>Exploring The Large Magellanic Cloud</media:title>
		<media:description>The Large Magellanic Cloud, known as the LMC, is a nearby satellite galaxy of our own Milky Way. At a distance of around 160,000 light-years, the LMC is the third closest galaxy to us. But the LMC is more than just a nice little sidekick.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod040208_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>The Crab Nebula in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts310308.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts310308.html</guid>
		<pubDate>Mon, 31 Mar 2008 12:00:00 EST</pubDate>
		<description>In 1054 A.D., a star's death in the constellation Taurus was observed on Earth. Now, almost a thousand years later, a superdense neutron star left behind by the explosion is spewing out a blizzard of extremely high-energy particles into the expanding debris field known as the Crab Nebula. </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod310308.m4v" length="6950000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:08</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod310308.m4v" fileSize="6950000" type="audio/aiff" duration="68" isDefault="true">
		<media:title>The Crab Nebula in 60 Seconds</media:title>
		<media:description>In 1054 A.D., a star's death in the constellation Taurus was observed on Earth. Now, almost a thousand years later, a superdense neutron star left behind by the explosion is spewing out a blizzard of extremely high-energy particles into the expanding debris field known as the Crab Nebula. </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod310308_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>M51 in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts180308.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts180308.html</guid>
		<pubDate>Tue, 18 Mar 2008 12:00:00 EST</pubDate>
		<description>Hubble's image of M51, also known as the Whirlpool Galaxy, shows the majestic spiral arms that are actually long lanes of stars and gas laced with dust. The infrared image from Spitzer also reveals stars and the glow from clouds of interstellar dust. </description>
		<enclosure type="video/x-m4v" url="http://chandra.harvard.edu/resources/podcasts/media/pod180308.m4v" length="7139000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:11</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod180308.m4v" fileSize="7139000" type="video/x-m4v" duration="71" isDefault="true">
		<media:title>M51 in 60 Seconds</media:title>
		<media:description>Hubble's image of M51, also known as the Whirlpool Galaxy, shows the majestic spiral arms that are actually long lanes of stars and gas laced with dust. The infrared image from Spitzer also reveals stars and the glow from clouds of interstellar dust. </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod180308_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>The Universe Darkly</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts022908.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts022908.html</guid>
		<pubDate>Fri, 29 Feb 2008 12:00:00 EST</pubDate>
		<description>When you look up at the night sky, you see a lot of things glowing like stars, planets, and galaxies.  So it might sound strange to hear that most of the Universe is actually dark.  The truth is the protons, neutrons and electrons that make up everything we can see, and that means everything with telescopes we've got, accounts for only about 4% of the mass and energy of the Universe.  The rest is dark and mysterious.  More specifically, about 70% of the Universe is what is known as dark energy; about 26% is so-called dark matter. Modern day astronomers have developed many tactics to explore the dark Universe, including using telescopes like Chandra.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod022908.m4v" length="38300000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:05:23</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod022908.m4v" fileSize="38300000" type="audio/aiff" duration="323" isDefault="true">
		<media:title>The Universe Darkly</media:title>
		<media:description>When you look up at the night sky, you see a lot of things glowing like stars, planets, and galaxies.  So it might sound strange to hear that most of the Universe is actually dark.  The truth is the protons, neutrons and electrons that make up everything we can see, and that means everything with telescopes we've got, accounts for only about 4% of the mass and energy of the Universe.  The rest is dark and mysterious.  More specifically, about 70% of the Universe is what is known as dark energy; about 26% is so-called dark matter. Modern day astronomers have developed many tactics to explore the dark Universe, including using telescopes like Chandra.</media:description>
		<media:thumbnail url="/resources/podcasts/images/pod022908_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Cassiopeia A in 60 Seconds</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts021108.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts021108.html</guid>
		<pubDate>Mon, 11 Feb 2008 12:00:00 EST</pubDate>
		<description>Cassiopeia A is the 300-year-old remnant created by the supernova explosion of a massive star. Each Great Observatory image highlights different characteristics of the remnant.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod021108.m4v" length="6740000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:01:08</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod021108.m4v" fileSize="6740000" type="audio/aiff" duration="68" isDefault="true">
		<media:title>Cassiopeia A in 60 Seconds</media:title>
		<media:description>Cassiopeia A is the 300-year-old remnant created by the supernova explosion of a massive star. Each Great Observatory image highlights different characteristics of the remnant.</media:description>
		<media:thumbnail url="/resources/podcasts/images/pod021108_thm.jpg" />
		</media:content>
	</item>
	<item>
		<title>Chandra in the (Google) Sky</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts290108.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts290108.html</guid>
		<pubDate>Tue, 29 Jan 2008 12:00:00 EST</pubDate>
		<description>Astronomy is truly in a golden age. With a fleet of space-based observatories, including the Chandra X-ray Observatory, astronomers now have a suite of amazing tools to study the Universe. Simultaneously to this bonanza in astronomy has been the growth and expansion of the Internet. Think back to before 1990. The Internet was barely a rumor and there were no Great Observatories! But now people are taking advantage of these two seemingly separate advances to do some amazing things</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod290108.m4v" length="21800000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:04:27</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod290108.m4v" fileSize="21800000" type="audio/aiff" duration="267" isDefault="true">
		<media:title>Chandra in the (Google) Sky</media:title>
		<media:description>Astronomy is truly in a golden age. With a fleet of space-based observatories, including the Chandra X-ray Observatory, astronomers now have a suite of amazing tools to study the Universe. Simultaneously to this bonanza in astronomy has been the growth and expansion of the Internet. Think back to before 1990. The Internet was barely a rumor and there were no Great Observatories! But now people are taking advantage of these two seemingly separate advances to do some amazing things</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod290108_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>What's in a Name?</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts020108.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts020108.html</guid>
		<pubDate>Wed, 02 Jan 2008 12:00:00 EST</pubDate>
		<description>Names in astronomy don't always tell the whole story.  Let's take, for example, radio galaxies.  Why, might you ask, would a Chandra podcast talk about such an object?  The answer is that radio galaxies are, yes, very bright in radio emission.  But they are also powerful emitters of X-rays, optical light and from other parts of the electromagnetic spectrum.  More than that, they are important objects that really have played a very big role in how the Universe has evolved.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod020108.m4v" length="36000000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:05:20</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod020108.m4v" fileSize="36000000" type="audio/aiff" duration="320" isDefault="true">
		<media:title>What's in a Name?</media:title>
		<media:description>Names in astronomy don't always tell the whole story.  Let's take, for example, radio galaxies.  Why, might you ask, would a Chandra podcast talk about such an object?  The answer is that radio galaxies are, yes, very bright in radio emission.  But they are also powerful emitters of X-rays, optical light and from other parts of the electromagnetic spectrum.  More than that, they are important objects that really have played a very big role in how the Universe has evolved.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod020108_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>The Truth and Lies about Black Holes</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts301107.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts301107.html</guid>
		<pubDate>Fri, 30 Nov 2007 12:00:00 EST</pubDate>
		<description>Black holes have a bad reputation.  After all, something that could swallow you completely sounds pretty scary. They&#39;re invisible, so maybe there&#39;s one just around the corner and we dont know it!  Also, arent they enormous vacuum cleaners capable of destroying anything that gets near them?  Once the black hole starts pulling on something, isnt that just a one-way ticket to oblivion?  Well, not all of these things are exactly true.  </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod301107.m4v" length="34100000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:05:00</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod301107.m4v" fileSize="34100000" type="audio/aiff" duration="300" isDefault="true">
		<media:title>The Truth and Lies about Black Holes</media:title>
		<media:description>Black holes have a bad reputation.  After all, something that could swallow you completely sounds pretty scary. They&#39;re invisible, so maybe there&#39;s one just around the corner and we dont know it!  Also, arent they enormous vacuum cleaners capable of destroying anything that gets near them?  Once the black hole starts pulling on something, isnt that just a one-way ticket to oblivion?  Well, not all of these things are exactly true.  </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod301107_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>When Will History Repeat Itself?</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts311007.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts311007.html</guid>
		<pubDate>Wed, 31 Oct 2007 12:00:00 EST</pubDate>
		<description>Astronomers think that a supernova should go off in our own Milky Way galaxy every 50 years or so. When was the last one we've seen? Probably 1604. Yes, that's over 400 years ago. This being astronomy however, things will undoubtedly average out over the long run, but in the meantime, we're left without a recent supernova in our Galaxy to study. Luckily for us, astronomers from previous centuries were on the case. </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod311007.m4v" length="38000000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:05:34</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod311007.m4v" fileSize="38000000" type="audio/aiff" duration="334" isDefault="true">
		<media:title>When Will History Repeat Itself?</media:title>
		<media:description>Astronomers think that a supernova should go off in our own Milky Way galaxy every 50 years or so. When was the last one we've seen? Probably 1604. Yes, that's over 400 years ago. This being astronomy however, things will undoubtedly average out over the long run, but in the meantime, we're left without a recent supernova in our Galaxy to study. Luckily for us, astronomers from previous centuries were on the case. </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod311007_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>In A Galaxy Far, Far Away and Also Those Nearby</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts280907.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts280907.html</guid>
		<pubDate>Fri, 28 Sep 2007 12:00:00 EST</pubDate>
		<description>"In a galaxy far, far away..." These are some of the most famous words in movie history. But what do we already know about galaxies, and what do astronomers, like those using the Chandra X- ray Observatory, still hope to learn about them? </description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod280907.m4v" length="34500000"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:05:03</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod280907.m4v" fileSize="34500000" type="audio/aiff" duration="303" isDefault="true">
		<media:title>In A Galaxy Far, Far Away and Also Those Nearby</media:title>
		<media:description>"In a galaxy far, far away..." These are some of the most famous words in movie history. But what do we already know about galaxies, and what do astronomers, like those using the Chandra X- ray Observatory, still hope to learn about them? </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod280907_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>From First Light to Eighth Anniversary</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts240807.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts240807.html</guid>
		<pubDate>Fri, 24 Aug 2007 12:00:00 EST</pubDate>
		<description>Chandra's launch aboard the Space Shuttle Columbia on July 23, 1999, was obviously a very important event. However, you might say it wasn't until about a month later that the Chandra mission really got started. In late August, after weeks of getting the spacecraft into the correct orbit and testing out various aspects of the satellite, Chandra was ready for its debut to the public. This was Chandra's First Light. Chandra's director, Dr. Harvey Tananbaum, explains the significance of that early image.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod240807.m4v" length="31112052"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:04:21</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod240807.m4v" fileSize="31112052" type="audio/aiff" duration="261" isDefault="true">
		<media:title>From First Light to Eighth Anniversary</media:title>
		<media:description>Chandra's launch aboard the Space Shuttle Columbia on July 23, 1999, was obviously a very important event. However, you might say it wasn't until about a month later that the Chandra mission really got started. In late August, after weeks of getting the spacecraft into the correct orbit and testing out various aspects of the satellite, Chandra was ready for its debut to the public. This was Chandra's First Light. Chandra's director, Dr. Harvey Tananbaum, explains the significance of that early image.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod240807_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>How It All Started</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts072607.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts072607.html</guid>
		<pubDate>Thu, 26 Jul 2007 12:00:00 EST</pubDate>
		<description>Just after midnight on July 23, 1999, the Space Shuttle Columbia launched in orbit with the heaviest payload ever carried by a shuttle.  Its precious cargo was the Chandra X-ray Observatory, which has helped revolutionize our understanding of the Universe.</description>
		<enclosure type="video/x-m4v" url="http://chandra.harvard.edu/resources/podcasts/media/pod072607.m4v" length="32364081"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:04:32</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod072607.m4v" fileSize="32364081" type="video/x-m4v" duration="272" isDefault="true">
		<media:title>How It All Started</media:title>
		<media:description>Just after midnight on July 23, 1999, the Space Shuttle Columbia launched in orbit with the heaviest payload ever carried by a shuttle.  Its precious cargo was the Chandra X-ray Observatory, which has helped revolutionize our understanding of the Universe.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod072607_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Mergers And Acquisitions In The Cosmos</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts280607.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts280607.html</guid>
		<pubDate>Thu, 28 Jun 2007 12:00:00 EST</pubDate>
		<description>News about mergers is usually found in the business section.  But many objects in the Universe, from black holes to clusters of galaxies, are also prone to mergers.  Like the corporate world, cosmic mergers are dictated by where the most assets lie.</description>
		<enclosure type="video/x-m4v" url="http://chandra.harvard.edu/resources/podcasts/media/pod280607.m4v" length="40954731"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:05:26</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod280607.m4v" fileSize="40954731" type="video/x-m4v" duration="326" isDefault="true">
		<media:title>Mergers And Acquisitions In The Cosmos</media:title>
		<media:description>News about mergers is usually found in the business section.  But many objects in the Universe, from black holes to clusters of galaxies, are also prone to mergers.  Like the corporate world, cosmic mergers are dictated by where the most assets lie.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/podcast14_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>The Bigger They Are, The Harder They Fall</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts240507.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts240507.html</guid>
		<pubDate>Thu, 24 May 2007 12:00:00 EST</pubDate>
		<description>When you look at the night sky, stars look like permanent fixtures of light. However, stars are born, live for a period of time, and then ultimately die. How they die is directly linked to how massive they were when they were born. </description>
		<enclosure type="video/x-m4v" url="http://chandra.harvard.edu/resources/podcasts/media/pod240507.m4v" length="32174964"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:04:32</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod240507.m4v" fileSize="32174964" type="video/x-m4v" duration="272" isDefault="true">
		<media:title>The Bigger They Are, The Harder They Fall</media:title>
		<media:description>When you look at the night sky, stars look like permanent fixtures of light. However, stars are born, live for a period of time, and then ultimately die. How they die is directly linked to how massive they were when they were born. </media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod240507_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>The Exotic World of Neutron Stars</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts300407.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts300407.html</guid>
		<pubDate>Mon, 30 Apr 2007 12:00:00 EST</pubDate>
		<description>Neutron stars are created when a massive star runs out of fuel and collapses.  As the star collapses, the density becomes so immense that protons and electrons are squeezed tightly together to form neutrons. The end result is a star only 20 km across but weighing 1 1/2 times more than our sun and made up mostly of neutrons.</description>
		<enclosure type="video/x-m4v" url="http://chandra.harvard.edu/resources/podcasts/media/pod300407.m4v" length="31271125"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:04:23</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod300407.m4v" fileSize="31271125" type="video/x-m4v" duration="263" isDefault="true">
		<media:title>The Exotic World of Neutron Stars</media:title>
		<media:description>Neutron stars are created when a massive star runs out of fuel and collapses.  As the star collapses, the density becomes so immense that protons and electrons are squeezed tightly together to form neutrons. The end result is a star only 20 km across but weighing 1 1/2 times more than our sun and made up mostly of neutrons.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod300407_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>The Giant Planets: X-ray Secrets Revealed</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts190307.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts190307.html</guid>
		<pubDate>Mon, 19 Mar 2007 12:00:00 EST</pubDate>
		<description>Jupiter and Saturn are the two largest planets in our Solar System, best known for very different reasons.  Most people think of Jupiter's famous Great Red Spot, while Saturn is, of course, most loved for those excellent rings.  These two planets, however, offer much, much more for astronomers looking to learn more about our Solar System.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod190307.m4v" length="30191534"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:04:13</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod190307.m4v" fileSize="30191534" type="audio/aiff" duration="253" isDefault="true">
		<media:title>The Giant Planets: X-ray Secrets Revealed</media:title>
		<media:description>Jupiter and Saturn are the two largest planets in our Solar System, best known for very different reasons.  Most people think of Jupiter's famous Great Red Spot, while Saturn is, of course, most loved for those excellent rings.  These two planets, however, offer much, much more for astronomers looking to learn more about our Solar System.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod190307_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Star (X-ray) Light, Star (X-ray) Bright</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts280207.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts280207.html</guid>
		<pubDate>Wed, 28 Feb 2007 12:00:00 EST</pubDate>
		<description>Remember the line from the children's saying that goes: "Starlight, star bright, first star I see tonight"?   Looking at the light from stars is exactly how astronomers can learn about them.</description>
		<enclosure type="video/x-m4v" url="http://chandra.harvard.edu/resources/podcasts/media/pod280207.m4v" length="30123633"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:04:13</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod280207.m4v" fileSize="30123633" type="video/x-m4v" duration="253" isDefault="true">
		<media:title>Star (X-ray) Light, Star (X-ray) Bright</media:title>
		<media:description>Remember the line from the children's saying that goes: "Starlight, star bright, first star I see tonight"?   Looking at the light from stars is exactly how astronomers can learn about them.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod280207_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Snowball Fight in the Solar System</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts220107.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts220107.html</guid>
		<pubDate>Mon, 22 Jan 2007 12:00:00 EST</pubDate>
		<description>One of the most surprising objects observed in X-rays are comets.  X-rays are normally associated with the hottest things in the Universe, such as black holes.  Comets, however, were described by Fred Whipple as being "dirty snowballs". So how does a snowball make X-rays?</description>
		<enclosure type="video/x-m4v" url="http://chandra.harvard.edu/resources/podcasts/media/pod220107.m4v" length="27977732"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:04:36</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod220107.m4v" fileSize="27977732" type="video/x-m4v" duration="276" isDefault="true">
		<media:title>Snowball Fight in the Solar System</media:title>
		<media:description>One of the most surprising objects observed in X-rays are comets.  X-rays are normally associated with the hottest things in the Universe, such as black holes.  Comets, however, were described by Fred Whipple as being "dirty snowballs". So how does a snowball make X-rays?</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod220107_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Black Holes: Tall, Grande, Venti</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts291206.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts291206.html</guid>
		<pubDate>Sun, 31 Dec 2006 12:00:00 EST</pubDate>
		<description>Long before astronomers found evidence that black holes existed, these exotic objects have captured imaginations. In the 21st century, scientists not only have proof that black holes are real, they continue to make startling discoveries both about individual black holes examples and about their populations across the Universe.</description>
		<enclosure type="audio/aiff" url="http://chandra.harvard.edu/resources/podcasts/media/pod291206.m4v" length="25171171"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:05:25</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod291206.m4v" fileSize="25171171" type="audio/aiff" duration="325" isDefault="true">
		<media:title>Black Holes: Tall, Grande, Venti</media:title>
		<media:description>Long before astronomers found evidence that black holes existed, these exotic objects have captured imaginations. In the 21st century, scientists not only have proof that black holes are real, they continue to make startling discoveries both about individual black holes examples and about their populations across the Universe.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod291206_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Giants of the Universe Probe Cosmic Questions</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts301106.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts301106.html</guid>
		<pubDate>Thu, 30 Nov 2006 12:00:00 EST</pubDate>
		<description>Clusters of galaxies are the largest structures in the Universe that are held together by gravity.  Because of their immense size and mass, galaxy clusters are extremely useful as tools to probe a variety of questions about the Universe as a whole as well as properties of the clusters themselves.</description>
		<enclosure type="video/x-m4v" url="http://chandra.harvard.edu/resources/podcasts/media/pod301106.m4v" length="25171171"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:05:25</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod301106.m4v" fileSize="25171171" type="video/x-m4v" duration="325" isDefault="true">
		<media:title>Giants of the Universe Probe Cosmic Questions</media:title>
		<media:description>Clusters of galaxies are the largest structures in the Universe that are held together by gravity.  Because of their immense size and mass, galaxy clusters are extremely useful as tools to probe a variety of questions about the Universe as a whole as well as properties of the clusters themselves.</media:description>
		<media:thumbnail url="http://chandra.harvard.edu/resources/podcasts/images/pod301106_sm100.jpg" />
		</media:content>
	</item>
	<item>
		<title>Supernovas: When Stars Die</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts301006.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts301006.html</guid>
		<pubDate>Mon, 30 Oct 2006 12:00:00 EST</pubDate>
		<description>When a star explodes, it leaves behind a debris field of stellar material and high-energy particles known as a supernova remnant. Astronomers use Chandra to study these remnants that can produce intense X-ray radiation for thousands of years. Supernova remnants are responsible for seeding cloud that formed our Sun, planets, and ultimately us with elements like nitrogen and oxygen.</description>
		<enclosure type="video/x-m4v" url="http://chandra.harvard.edu/resources/podcasts/media/pod301006.m4v" length="23374632"/>
		<itunes:explicit>clean</itunes:explicit>
		<itunes:duration>00:04:39</itunes:duration>
		<media:content url="http://chandra.harvard.edu/resources/podcasts/media/pod301006.m4v" fileSize="23374632" type="video/x-m4v" duration="279" isDefault="true">
		<media:title>Supernovas: When Stars Die</media:title>
		<media:description>When a star explodes, it leaves behind a debris field of stellar material and high-energy particles known as a supernova remnant. Astronomers use Chandra to study these remnants that can produce intense X-ray radiation for thousands of years. Supernova remnants are responsible for seeding cloud that formed our Sun, planets, and ultimately us with elements like nitrogen and oxygen.</media:description>
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		<title>Until Their Dying Day: Stars on the Brink</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts260906.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts260906.html</guid>
		<pubDate>Tue, 26 Sep 2006 12:00:00 EST</pubDate>
		<description>Supernovas are the remnants of catastrophic explosions, and they are among the favorite targets of scientists who use Chandra, for good reason too. Supernovas and their remnants have proven to be extremely important in understanding topics ranging from the birth of our Solar System to the history and composition of the Universe itself.</description>
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		<itunes:duration>00:04:40</itunes:duration>
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		<media:title>Until Their Dying Day: Stars on the Brink</media:title>
		<media:description>Supernovas are the remnants of catastrophic explosions, and they are among the favorite targets of scientists who use Chandra, for good reason too. Supernovas and their remnants have proven to be extremely important in understanding topics ranging from the birth of our Solar System to the history and composition of the Universe itself.</media:description>
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		<title>Peering into the Heart of the Milky Way</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts300806.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts300806.html</guid>
		<pubDate>Thu, 31 Aug 2006 12:00:00 EST</pubDate>
		<description>Humanity has long sought to learn about the Milky Way, our home galaxy. Even after the advent of optical telescopes, the Milky Way's center remained mysterious because gas and dust blocks most visible light along our line of sight. Fortunately, X-ray telescopes like Chandra can detect higher-energy radiation that penetrates this veil of galactic debris.</description>
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		<itunes:duration>00:04:40</itunes:duration>
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		<media:title>Peering into the Heart of the Milky Way</media:title>
		<media:description>Humanity has long sought to learn about the Milky Way, our home galaxy. Even after the advent of optical telescopes, the Milky Way's center remained mysterious because gas and dust blocks most visible light along our line of sight. Fortunately, X-ray telescopes like Chandra can detect higher-energy radiation that penetrates this veil of galactic debris.</media:description>
		<media:thumbnail url="/resources/podcasts/images/pod300806_sm100.jpg" />
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		<title>Putting Chandra In Its Place</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts260706.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts260706.html</guid>
		<pubDate>Thu, 27 Jul 2006 12:00:00 EST</pubDate>
		<description>How the Chandra X-ray Observatory fits into the modern astronomer's toolkit.  Chandra is one of NASA's "Great Observatories."  The Great Observatories were four missions selected by NASA to explore different types of radiation and really tackle the biggest questions in astronomy. </description>
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		<media:title>Putting Chandra In Its Place</media:title>
		<media:description>How the Chandra X-ray Observatory fits into the modern astronomer's toolkit.  Chandra is one of NASA's "Great Observatories."  The Great Observatories were four missions selected by NASA to explore different types of radiation and really tackle the biggest questions in astronomy. </media:description>
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		<title>Chandra,  Not Your Backyard Telescope</title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts090606.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts090606.html</guid>
		<pubDate>Fri, 09 Jun 2006 12:00:00 EST</pubDate>
		<description>X-ray telescopes like Chandra are not like the telescopes you find in backyards or at the local observatory.  In addition to being above the Earth's atmosphere, they need to have special mirrors to detect the X-rays that pass through most objects.  </description>
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		<itunes:duration>00:05:48</itunes:duration>
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		<media:title>Chandra,  Not Your Backyard Telescope</media:title>
		<media:description>X-ray telescopes like Chandra are not like the telescopes you find in backyards or at the local observatory.  In addition to being above the Earth's atmosphere, they need to have special mirrors to detect the X-rays that pass through most objects.  </media:description>
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		<title>How Chandra Does What It Does </title>
		<link>http://chandra.harvard.edu/resources/podcasts/ts/ts060506.html</link>
		<guid>http://chandra.harvard.edu/resources/podcasts/ts/ts060506.html</guid>
		<pubDate>Thu, 11 May 2006 12:00:00 EST</pubDate>
		<description>NASA's Chandra X-ray Observatory, in orbit since 1999, studies the high-energy Universe, where black holes, exploding stars, and mysterious matter hold sway. </description>
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		<media:title>How Chandra Does What It Does </media:title>
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