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      <title>Enectali (Tali) Figueroa-Feliciano</title>
      <pubDate>2007-07-12 19:22:00 -0400</pubDate>
      <itunes:author>msrp2007</itunes:author>
      <itunes:summary>
Searching for Dark Needles in the Cosmic Particle Haystack
</itunes:summary>
      <itunes:duration>4441</itunes:duration>
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      <guid>tag:techtv.mit.edu,:Array/224573080</guid>
      <title>Student Presentation #3</title>
      <pubDate>2007-07-12 18:38:50 -0400</pubDate>
      <itunes:author>msrp2007</itunes:author>
      <itunes:summary>
The existence of dark matter.
</itunes:summary>
      <itunes:duration>1818</itunes:duration>
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      <guid>tag:techtv.mit.edu,:Array/224554120</guid>
      <title>Mareena Robinson</title>
      <pubDate>2008-11-26 14:00:26 -0500</pubDate>
      <itunes:author>msrp2008</itunes:author>
      <itunes:summary>&quot;The whole point of this program is to expose you to things you never would have been exposed to.&quot;
--Mareena Robinson, Junior, Florida A&amp;M University</itunes:summary>
      <itunes:duration>102</itunes:duration>
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      <guid>tag:techtv.mit.edu,:Array/224533380</guid>
      <title>Student Presentation #1</title>
      <pubDate>2009-06-25 14:11:12 -0400</pubDate>
      <itunes:author>MSRP 2009</itunes:author>
      <itunes:summary>&quot;Neutrino Backgrounds to Dark Matter Searches and Directionality,&quot; presented 6/18/2009</itunes:summary>
      <itunes:duration>2364</itunes:duration>
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      <title>Jocelyn Monroe</title>
      <pubDate>2009-06-25 14:14:54 -0400</pubDate>
      <itunes:author>MSRP 2009</itunes:author>
      <itunes:summary>&quot;The Search for Dark Matter.&quot; Recorded 6/18/2009</itunes:summary>
      <itunes:duration>0</itunes:duration>
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      <guid>tag:techtv.mit.edu,:Array/226874160</guid>
      <title>BLOSSOMS - Dark Matter</title>
      <pubDate>2009-10-19 15:05:17 -0400</pubDate>
      <itunes:author>Blended Learning Open Source Science or Math Studies (BLOSSOMS)</itunes:author>
      <itunes:summary>This video lesson has the goal of introducing students to galaxies as large collections of gravitationally bound stars.  It explores the amount of matter needed for a star to remain bound and then brings in the idea of Dark Matter, a new kind of matter that does not interact with light.  </itunes:summary>
      <itunes:duration>3854</itunes:duration>
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