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	<title>StarCitizen:White dwarf - Revision history</title>
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	<updated>2026-04-09T23:10:17Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<id>https://wiki.sasgaming.net/index.php?title=StarCitizen:White_dwarf&amp;diff=66098&amp;oldid=prev</id>
		<title>imported&gt;TheBookfinder: cat</title>
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		<updated>2025-07-04T09:54:36Z</updated>

		<summary type="html">&lt;p&gt;cat&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;A &amp;#039;&amp;#039;&amp;#039;white dwarf&amp;#039;&amp;#039;&amp;#039; is a stellar core remnant composed mostly of electron-degenerate matter. A white dwarf is very dense: its mass is comparable to the Sun&amp;#039;s, while its volume is comparable to the Earth&amp;#039;s. A white dwarf&amp;#039;s faint luminosity comes from the emission of residual thermal energy; no fusion takes place in a white dwarf.&lt;br /&gt;
&lt;br /&gt;
The material in a white dwarf no longer undergoes fusion reactions, so the star has no source of energy. As a result, it cannot support itself by the heat generated by fusion against gravitational collapse, but is supported only by electron degeneracy pressure, causing it to be extremely dense.&lt;br /&gt;
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=== Systems White Dwarfs ===&lt;br /&gt;
&lt;br /&gt;
* [[StarCitizen:Odin system]]&lt;br /&gt;
* [[StarCitizen:Tyrol system]]&lt;br /&gt;
* [[StarCitizen:UDS-2943-01-22]]&lt;br /&gt;
&lt;br /&gt;
[[Category:Astronomy]]&lt;/div&gt;</summary>
		<author><name>imported&gt;TheBookfinder</name></author>
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