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	<id>http://galactic-crucibles.com/index.php?action=history&amp;feed=atom&amp;title=Star</id>
	<title>Star - Revision history</title>
	<link rel="self" type="application/atom+xml" href="http://galactic-crucibles.com/index.php?action=history&amp;feed=atom&amp;title=Star"/>
	<link rel="alternate" type="text/html" href="http://galactic-crucibles.com/index.php?title=Star&amp;action=history"/>
	<updated>2026-05-15T19:20:31Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.42.5</generator>
	<entry>
		<id>http://galactic-crucibles.com/index.php?title=Star&amp;diff=1310&amp;oldid=prev</id>
		<title>Krayfishkarl: Krayfishkarl moved page Star terminology to Star</title>
		<link rel="alternate" type="text/html" href="http://galactic-crucibles.com/index.php?title=Star&amp;diff=1310&amp;oldid=prev"/>
		<updated>2022-12-03T17:59:16Z</updated>

		<summary type="html">&lt;p&gt;Krayfishkarl moved page &lt;a href=&quot;/wiki/Star_terminology&quot; class=&quot;mw-redirect&quot; title=&quot;Star terminology&quot;&gt;Star terminology&lt;/a&gt; to &lt;a href=&quot;/wiki/Star&quot; title=&quot;Star&quot;&gt;Star&lt;/a&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;1&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;1&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 17:59, 3 December 2022&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-notice&quot; lang=&quot;en&quot;&gt;&lt;div class=&quot;mw-diff-empty&quot;&gt;(No difference)&lt;/div&gt;
&lt;/td&gt;&lt;/tr&gt;&lt;/table&gt;</summary>
		<author><name>Krayfishkarl</name></author>
	</entry>
	<entry>
		<id>http://galactic-crucibles.com/index.php?title=Star&amp;diff=738&amp;oldid=prev</id>
		<title>Krayfishkarl at 16:32, 22 June 2022</title>
		<link rel="alternate" type="text/html" href="http://galactic-crucibles.com/index.php?title=Star&amp;diff=738&amp;oldid=prev"/>
		<updated>2022-06-22T16:32:35Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 16:32, 22 June 2022&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l1&quot;&gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[File:StarTypes.png|thumb|200px]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[File:StarTypes.png|thumb|200px]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Stars are divided by type.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&#039;&#039;&#039;&lt;/ins&gt;Stars&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&#039;&#039;&#039; &lt;/ins&gt;are divided by type.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==Main Sequence Stars==&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;==Main Sequence Stars==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*Class M - A small red star that is generally a red dwarf but also sometimes a brown dwarf, these stars are extremely common and can last trillions of years.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*Class M - A small red star that is generally a red dwarf but also sometimes a brown dwarf, these stars are extremely common and can last trillions of years.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l30&quot;&gt;Line 30:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 30:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*Darkmatter Star - A primitive, early star which predated the formation of the conventional stars, it was not composed of dark matter despite it&amp;#039;s name (a star primarily composed of non-baryonic matter is called a Q-star) but instead simply had large densities of neutralino dark matter which produced heat through annihilation reactors within the star. The Darkmatter Star would be a 2-4000 AU black cloud with surface temperatures so cold that radiation on it could be observed by the naked eye.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*Darkmatter Star - A primitive, early star which predated the formation of the conventional stars, it was not composed of dark matter despite it&amp;#039;s name (a star primarily composed of non-baryonic matter is called a Q-star) but instead simply had large densities of neutralino dark matter which produced heat through annihilation reactors within the star. The Darkmatter Star would be a 2-4000 AU black cloud with surface temperatures so cold that radiation on it could be observed by the naked eye.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Category:&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Guides&lt;/del&gt;]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Category:&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Cosmology&lt;/ins&gt;]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Category:Articles by User:Majoras Revenge!!!]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Category:Articles by User:Majoras Revenge!!!]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Krayfishkarl</name></author>
	</entry>
	<entry>
		<id>http://galactic-crucibles.com/index.php?title=Star&amp;diff=565&amp;oldid=prev</id>
		<title>Krayfishkarl: Created page with &quot;200px Stars are divided by type. ==Main Sequence Stars== *Class M - A small red star that is generally a red dwarf but also sometimes a brown dwarf, these stars are extremely common and can last trillions of years. *Class K - Orange stars smaller than the sun, which are very common. *Class G - Yellow stars much like Sol. *Class F - A yellow-white star which is the brightest capable of supporting habitable planets naturally. *Class A - The sma...&quot;</title>
		<link rel="alternate" type="text/html" href="http://galactic-crucibles.com/index.php?title=Star&amp;diff=565&amp;oldid=prev"/>
		<updated>2022-05-19T00:37:09Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;&lt;a href=&quot;/wiki/File:StarTypes.png&quot; title=&quot;File:StarTypes.png&quot;&gt;thumb|200px&lt;/a&gt; Stars are divided by type. ==Main Sequence Stars== *Class M - A small red star that is generally a red dwarf but also sometimes a brown dwarf, these stars are extremely common and can last trillions of years. *Class K - Orange stars smaller than the sun, which are very common. *Class G - Yellow stars much like Sol. *Class F - A yellow-white star which is the brightest capable of supporting habitable planets naturally. *Class A - The sma...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;[[File:StarTypes.png|thumb|200px]]&lt;br /&gt;
Stars are divided by type.&lt;br /&gt;
==Main Sequence Stars==&lt;br /&gt;
*Class M - A small red star that is generally a red dwarf but also sometimes a brown dwarf, these stars are extremely common and can last trillions of years.&lt;br /&gt;
*Class K - Orange stars smaller than the sun, which are very common.&lt;br /&gt;
*Class G - Yellow stars much like Sol.&lt;br /&gt;
*Class F - A yellow-white star which is the brightest capable of supporting habitable planets naturally.&lt;br /&gt;
*Class A - The smallest blue star, it isn&amp;#039;t able to form habitable worlds.&lt;br /&gt;
*Class B - A blue star between classes O and A in size. They cannot support habitable worlds.&lt;br /&gt;
*Class O - A very rare giant blue star which is incapable of supporting habitable worlds.&lt;br /&gt;
&lt;br /&gt;
==Non-Main Sequence Stars==&lt;br /&gt;
*Class D - A degenerate white dwarf star no longer producing energy at it&amp;#039;s core. White dwarves are as dense as G-class stars but as small in volume as some terrestrial planets. It is theorized that 97% of stars in the universe will eventually become white dwarves.&lt;br /&gt;
*Class T - Class T Brown Dwarves are rare and cool dwarves which can reach temperatures as low as 250 K.&lt;br /&gt;
*Class Y - Class Y Brown Dwarves are similar to Class T, but are hotter. T-Class Dwarves would persist several times the lifespan of the Universe.&lt;br /&gt;
*Class L - The L-class Red Dwarves are unable to support Hydrogen fusion due to their limited masses.&lt;br /&gt;
*Class S - Class S stars have a roughly equal amount of Oxygen and Hydrogen in their atmospheres (Main-Sequence Stars have mostly Oxygen), it is similar in heat to the K class of stars&lt;br /&gt;
*Class C - The Carbon Stars, class C, have a higher amount of Carbon within their atmospheres than Oxygen, giving them a ruby red appearance and a variable temperature range.&lt;br /&gt;
*Class W - Class W or WR, the Wolf-Rayet Star, is immensely hot and outclasses even the O-type star by several magnitudes in heat, reaching as much as 200,000 K.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Abnormal Stars==&lt;br /&gt;
*Neutron Stars - Neutron Stars have densities similar to those of G-class stars but extremely small volumes only a few kilometers across. The Neutron Star possesses an elephantine amount of heat that can be in excess of 600,000 K.&lt;br /&gt;
*Exotic Stars - Stars not made of electrons, protons, neutrons, or muons, such as &lt;br /&gt;
**Quark Stars - Stars made up only of quarks. &lt;br /&gt;
**Strange Stars - made up only of strange quark matter, which is composed of Up Quarks, Down Quarks, and Strange Quarks.&lt;br /&gt;
**Preon Stars - made up of sub-quark particles called Preons, which have not yet been proven to exist.&lt;br /&gt;
**Boson Stars - A star made of Boson particles, rather than the Fermion particles that make up all other stars.&lt;br /&gt;
*Dark Star - A star with an escape velocity greater to the speed of light, causing it to appear black to outside observers. Not to be confused with a black hole.&lt;br /&gt;
*Darkmatter Star - A primitive, early star which predated the formation of the conventional stars, it was not composed of dark matter despite it&amp;#039;s name (a star primarily composed of non-baryonic matter is called a Q-star) but instead simply had large densities of neutralino dark matter which produced heat through annihilation reactors within the star. The Darkmatter Star would be a 2-4000 AU black cloud with surface temperatures so cold that radiation on it could be observed by the naked eye.&lt;br /&gt;
&lt;br /&gt;
[[Category:Guides]]&lt;br /&gt;
&lt;br /&gt;
[[Category:Articles by User:Majoras Revenge!!!]]&lt;/div&gt;</summary>
		<author><name>Krayfishkarl</name></author>
	</entry>
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