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      <pubDate>2018-04-07 19:03:23 UTC</pubDate>
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         <description><![CDATA[<div>The HR Diagram</div>]]></description>
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         <description><![CDATA[<div>Planetary Nebulae</div>]]></description>
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         <description><![CDATA[<div>When fusion in the core of a high mass star starts fusing Iron in its core the star almost instantaneously collapses and "goes supernova". This is because the Iron fusion is an endothermic reaction.</div>]]></description>
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