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      <title>LIFE CYCLE OF STARS GRAPHIC ORGANIZER by Joseph Gussie</title>
      <link>https://padlet.com/jg26190/hj0ofro25gzj</link>
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      <pubDate>2019-02-07 13:42:39 UTC</pubDate>
      <lastBuildDate>2019-02-07 13:43:31 UTC</lastBuildDate>
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      <item>
         <title>MASSIVE STAR LIFE CYCLE </title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328719578</link>
         <description><![CDATA[]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 13:47:51 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328719578</guid>
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      <item>
         <title>Stage 1 </title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328720898</link>
         <description><![CDATA[<div>Nebular cloud<br>Gases (mostly hydrogen) and dust begin spinning around together forming a ball.</div>]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 13:50:07 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328720898</guid>
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      <item>
         <title>Stage 2 </title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328722532</link>
         <description><![CDATA[<div>Protostar <br>Gravity puts huge pressure on the ball of gas as it spins.  This causes the temperature to increase and gases to start shooting out.</div>]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 13:52:47 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328722532</guid>
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      <item>
         <title>Stage 3 </title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328724838</link>
         <description><![CDATA[<div>Main Sequence<br>Hydrogen fuses and becomes helium.  This happens for <strong>billions</strong> of years, sending light and heat out of the star. </div>]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 13:56:21 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328724838</guid>
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      <item>
         <title>Stage 4  </title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328727049</link>
         <description><![CDATA[<div>Red Super giant <br>The <strong>iron core</strong> of the star is so heavy that the gravitational force causes the core to collapse and the star to explode.  The heaviest elements are made by the fusion that occurs during the explosion and these elements are spread through the universe.</div>]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 13:59:52 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328727049</guid>
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      <item>
         <title>Stage 5 </title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328728085</link>
         <description><![CDATA[<div>Super Nova <br>The outer shell of the Red Giant ejects (shoots out) gases as the star is in the last part of its Red Giant stage.</div>]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 14:01:37 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328728085</guid>
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      <item>
         <title>Stage 6 </title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328729241</link>
         <description><![CDATA[<div> Neutron Star<br>The core of a star after an explosion.  The core is so dense that a sugar cube (1 cm3) sized piece would have a mass as much as Mount Everest. </div>]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 14:03:14 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328729241</guid>
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      <item>
         <title>Stage 7</title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328730697</link>
         <description><![CDATA[<div>Black Hole <br>A place in space where gravity is so large, even light cannot escape.  It happens because the core of the star is squeezed into a tiny place.</div>]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 14:05:30 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328730697</guid>
      </item>
      <item>
         <title>SMALL STAR LIFE CYCLE </title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328732596</link>
         <description><![CDATA[]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 14:08:44 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328732596</guid>
      </item>
      <item>
         <title>Stage 1 </title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328733265</link>
         <description><![CDATA[<div>Planetary nebula<br>Gases (mostly hydrogen) and dust begin spinning around together forming a ball.</div>]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 14:09:44 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328733265</guid>
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      <item>
         <title>Stage 2 </title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328734840</link>
         <description><![CDATA[<div>Protostar<br>Gravity puts huge pressure on the ball of gas as it spins.  This causes the temperature to increase and gases to start shooting out.</div>]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 14:12:14 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328734840</guid>
      </item>
      <item>
         <title>Stage 3 </title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328735431</link>
         <description><![CDATA[<div>Main sequence (Our Sun)<br>Helium gases are almost all used and the star begins forming iron at the core.  The star’s core is extremely hot and the star is expanding outward.</div>]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 14:13:10 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328735431</guid>
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      <item>
         <title>Stage 4 </title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328737533</link>
         <description><![CDATA[<div>Red Giant<br>Hydrogen gases are almost all used and the star begins forming other elements including carbon.  The star expands outward while the <strong>carbon core</strong> is squeezed by gravity.  The outside is cool but the inside hot.</div>]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 14:16:23 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328737533</guid>
      </item>
      <item>
         <title>Stage 5 </title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328738092</link>
         <description><![CDATA[<div>Planetary nebula<br>Hydrogen fuses and becomes helium.  This happens for <strong>millions</strong> of years, sending light and heat out of the star.<br><br></div>]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 14:17:20 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328738092</guid>
      </item>
      <item>
         <title>Stage 6</title>
         <author>jg26190</author>
         <link>https://padlet.com/jg26190/hj0ofro25gzj/wish/328738489</link>
         <description><![CDATA[<div>White Dwarf<br>The core of the star is pressurized carbon; possibly a giant diamond.  The star is the size of Earth.</div><div><br></div>]]></description>
         <enclosure url="" />
         <pubDate>2019-02-07 14:18:01 UTC</pubDate>
         <guid>https://padlet.com/jg26190/hj0ofro25gzj/wish/328738489</guid>
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