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	<id>https://keystagewiki.com/index.php?action=history&amp;feed=atom&amp;title=Low_Mass_Star</id>
	<title>Low Mass Star - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://keystagewiki.com/index.php?action=history&amp;feed=atom&amp;title=Low_Mass_Star"/>
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	<updated>2026-05-04T08:46:11Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
		<id>https://keystagewiki.com/index.php?title=Low_Mass_Star&amp;diff=14182&amp;oldid=prev</id>
		<title>NRJC: /* Lifecycle */</title>
		<link rel="alternate" type="text/html" href="https://keystagewiki.com/index.php?title=Low_Mass_Star&amp;diff=14182&amp;oldid=prev"/>
		<updated>2019-04-07T21:01:03Z</updated>

		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Lifecycle&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;col class=&quot;diff-content&quot; /&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 21:01, 7 April 2019&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-l12&quot; &gt;Line 12:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 12:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;#[[Red Giant]] - A [[star]] that has run out of [[Hydrogen]] for [[Nuclear Fusion|fusion]] so the [[pressure]]s are no longer balanced and its core collapses under [[gravity]] until the core is hot enough to [[Nuclear Fusion|fuse]] [[Helium]] into more [[massive]] [[element]]s. During this time the outer layers expand as the [[star]] cools but becomes brighter as it becomes much bigger.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;#[[Red Giant]] - A [[star]] that has run out of [[Hydrogen]] for [[Nuclear Fusion|fusion]] so the [[pressure]]s are no longer balanced and its core collapses under [[gravity]] until the core is hot enough to [[Nuclear Fusion|fuse]] [[Helium]] into more [[massive]] [[element]]s. During this time the outer layers expand as the [[star]] cools but becomes brighter as it becomes much bigger.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;#[[White Dwarf]] - A [[star]] which as run out of low [[mass]] [[element]]s to [[Nuclear Fusion|fuse]]. There is no more outward [[pressure]] due to [[Nuclear Fusion|fusion]] so the core collapses due to [[gravity]] into a ball of [[Iron]] and continues to glow for millions of years as it [[radiation|radiates]] its [[Thermal Energy Store|thermal energy]].&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;#[[White Dwarf]] - A [[star]] which as run out of low [[mass]] [[element]]s to [[Nuclear Fusion|fuse]]. There is no more outward [[pressure]] due to [[Nuclear Fusion|fusion]] so the core collapses due to [[gravity]] into a ball of [[Iron]] and continues to glow for millions of years as it [[radiation|radiates]] its [[Thermal Energy Store|thermal energy]].&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; 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;#[[Black Dwarf]] - Once a [[White Dwarf]] has cooled enough it will no longer glow and become a [[Black Dwarf]]. These [[star]]s do not yet exist because the [[Universe]] has not existed long enough for [[White &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Drawf&lt;/del&gt;|White Dwarves]] to cool.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;#[[Black Dwarf]] - Once a [[White Dwarf]] has cooled enough it will no longer glow and become a [[Black Dwarf]]. These [[star]]s do not yet exist because the [[Universe]] has not existed long enough for [[White &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Dwarf&lt;/ins&gt;|White Dwarves]] to cool.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>NRJC</name></author>
		
	</entry>
	<entry>
		<id>https://keystagewiki.com/index.php?title=Low_Mass_Star&amp;diff=10591&amp;oldid=prev</id>
		<title>NRJC: Created page with &quot;==Key Stage 4== ===Meaning=== A '''low mass star''' is a star with up to 3 times the mass of The Sun.  ===About Low Mass Stars=== : '''Low mass stars''' have a dif...&quot;</title>
		<link rel="alternate" type="text/html" href="https://keystagewiki.com/index.php?title=Low_Mass_Star&amp;diff=10591&amp;oldid=prev"/>
		<updated>2019-03-13T10:43:39Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;==Key Stage 4== ===Meaning=== A &amp;#039;&amp;#039;&amp;#039;low mass star&amp;#039;&amp;#039;&amp;#039; is a &lt;a href=&quot;/index.php/Star&quot; title=&quot;Star&quot;&gt;star&lt;/a&gt; with up to 3 times the &lt;a href=&quot;/index.php/Mass&quot; title=&quot;Mass&quot;&gt;mass&lt;/a&gt; of &lt;a href=&quot;/index.php/The_Sun&quot; title=&quot;The Sun&quot;&gt;The Sun&lt;/a&gt;.  ===About Low Mass Stars=== : &amp;#039;&amp;#039;&amp;#039;Low mass stars&amp;#039;&amp;#039;&amp;#039; have a dif...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;==Key Stage 4==&lt;br /&gt;
===Meaning===&lt;br /&gt;
A '''low mass star''' is a [[star]] with up to 3 times the [[mass]] of [[The Sun]].&lt;br /&gt;
&lt;br /&gt;
===About Low Mass Stars===&lt;br /&gt;
: '''Low mass stars''' have a different life cycle to [[High Mass Star|high mass stars]] and exist for far longer than [[High Mass Star|high mass stars]].&lt;br /&gt;
&lt;br /&gt;
====Lifecycle====&lt;br /&gt;
#[[Nebula]] - A huge cloud of [[gas]] and dust stretching across space which collapses due to [[gravity]] to form [[star]]s.&lt;br /&gt;
#[[Protostar]] - A glowing ball of [[gas]] and dust that is not yet hot enough for [[Nuclear Fusion|fusion]] to occur in its core.&lt;br /&gt;
#[[Main Sequence Star]] - The longest and most stable period of a [[star]]s life when the outward pressure caused by [[Nuclear Fusion|fusion]] of [[Hydrogen]] in its core is balanced by the inward [[pressure]] caused by [[gravity]].&lt;br /&gt;
#[[Red Giant]] - A [[star]] that has run out of [[Hydrogen]] for [[Nuclear Fusion|fusion]] so the [[pressure]]s are no longer balanced and its core collapses under [[gravity]] until the core is hot enough to [[Nuclear Fusion|fuse]] [[Helium]] into more [[massive]] [[element]]s. During this time the outer layers expand as the [[star]] cools but becomes brighter as it becomes much bigger.&lt;br /&gt;
#[[White Dwarf]] - A [[star]] which as run out of low [[mass]] [[element]]s to [[Nuclear Fusion|fuse]]. There is no more outward [[pressure]] due to [[Nuclear Fusion|fusion]] so the core collapses due to [[gravity]] into a ball of [[Iron]] and continues to glow for millions of years as it [[radiation|radiates]] its [[Thermal Energy Store|thermal energy]].&lt;br /&gt;
#[[Black Dwarf]] - Once a [[White Dwarf]] has cooled enough it will no longer glow and become a [[Black Dwarf]]. These [[star]]s do not yet exist because the [[Universe]] has not existed long enough for [[White Drawf|White Dwarves]] to cool.&lt;/div&gt;</summary>
		<author><name>NRJC</name></author>
		
	</entry>
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