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	<title>Comments on: How Big Stars Die</title>
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	<description>Basic Astronomy and Night Sky Sights For Busy People</description>
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		<title>By: Type II Supernovae: Very Big Explosions &#124; One-Minute Astronomer</title>
		<link>http://www.oneminuteastronomer.com/2009/06/18/how-big-stars-die/comment-page-1/#comment-28</link>
		<dc:creator>Type II Supernovae: Very Big Explosions &#124; One-Minute Astronomer</dc:creator>
		<pubDate>Mon, 20 Jul 2009 22:28:31 +0000</pubDate>
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		<description>[...] As you learned before, when a big star has burned through its stock of hydrogen, helium, carbon, etc., it&#8217;s eventually left with iron and nickel in the core.  But iron and nickel can&#8217;t fuse together to release any more energy.  So the game is finally up&#8230; and when burning stops, there is no more energy to hold the star up against its own gravity, and the star&#8217;s hot core suddenly collapses into a neutron star or a black hole.  This releases a huge amount of gravitational energy. [...]</description>
		<content:encoded><![CDATA[<p>[...] As you learned before, when a big star has burned through its stock of hydrogen, helium, carbon, etc., it&#8217;s eventually left with iron and nickel in the core.  But iron and nickel can&#8217;t fuse together to release any more energy.  So the game is finally up&#8230; and when burning stops, there is no more energy to hold the star up against its own gravity, and the star&#8217;s hot core suddenly collapses into a neutron star or a black hole.  This releases a huge amount of gravitational energy. [...]</p>
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