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	<id>https://nyssls.info/index.php?action=history&amp;feed=atom&amp;title=H-R_Diagram</id>
	<title>H-R Diagram - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://nyssls.info/index.php?action=history&amp;feed=atom&amp;title=H-R_Diagram"/>
	<link rel="alternate" type="text/html" href="https://nyssls.info/index.php?title=H-R_Diagram&amp;action=history"/>
	<updated>2026-10-17T00:55:43Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
		<id>https://nyssls.info/index.php?title=H-R_Diagram&amp;diff=5821&amp;oldid=prev</id>
		<title>Conrad: SEO: short lead above the diagram, fuller description in its own section below it</title>
		<link rel="alternate" type="text/html" href="https://nyssls.info/index.php?title=H-R_Diagram&amp;diff=5821&amp;oldid=prev"/>
		<updated>2026-10-13T15:18:45Z</updated>

		<summary type="html">&lt;p&gt;SEO: short lead above the diagram, fuller description in its own section below it&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&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 15:18, 13 October 2026&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-l5&quot; &gt;Line 5:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 5:&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: #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;  |desc=H-R Diagram from the NYS Earth and Space Sciences Reference Tables (ESSRT): star luminosity against surface temperature and spectral class, with the main sequence, giants, supergiants and white dwarfs. Supports HS-ESS1-3.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;  |desc=H-R Diagram from the NYS Earth and Space Sciences Reference Tables (ESSRT): star luminosity against surface temperature and spectral class, with the main sequence, giants, supergiants and white dwarfs. Supports HS-ESS1-3.&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: #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;}}&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;}}&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: #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;The '''H-R Diagram''' (Hertzsprung–Russell diagram) from the ''Reference Tables for Earth and Space Sciences'' (ESSRT) plots the luminosity of stars&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;, in solar units, &lt;/del&gt;against their surface temperature &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;in kelvins, with spectral class (O, B, A, F, G, K, M) and color from blue to red along the bottom&lt;/del&gt;. It &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;shows where the main sequence, giants, supergiants and white dwarfs fall and places well-known stars on the diagram, including the Sun, Sirius, Polaris, Rigel and Betelgeuse. Diagonal lines mark stellar size from 10&amp;lt;sup&amp;gt;−3&amp;lt;/sup&amp;gt; to 10&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt; solar radii, labels along the main sequence give stellar lifetimes from 10&amp;lt;sup&amp;gt;7&amp;lt;/sup&amp;gt; to 10&amp;lt;sup&amp;gt;11&amp;lt;/sup&amp;gt; years, and an arrow at the right shows mass increasing toward the top. This table &lt;/del&gt;primarily supports [[HS-ESS1-3]].&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;The '''H-R Diagram''' (Hertzsprung–Russell diagram) from the ''Reference Tables for Earth and Space Sciences'' (ESSRT) plots the luminosity of stars against their surface temperature. It primarily supports [[HS-ESS1-3]].&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: #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;/td&gt;&lt;td class='diff-marker'&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;/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: #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:H-R Diagram.png|800px|class=img-fluid|alt=H-R Diagram from the Earth and Space Sciences Reference Tables (ESSRT): luminosity of stars plotted against surface temperature and spectral class, showing the main sequence, giants, supergiants and white dwarfs]]&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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:H-R Diagram.png|800px|class=img-fluid|alt=H-R Diagram from the Earth and Space Sciences Reference Tables (ESSRT): luminosity of stars plotted against surface temperature and spectral class, showing the main sequence, giants, supergiants and white dwarfs]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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;== What the H-R Diagram shows ==&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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;Luminosity is given in solar units and surface temperature in kelvins, with spectral class (O, B, A, F, G, K, M) and color from blue to red along the bottom. The diagram shows where the main sequence, giants, supergiants and white dwarfs fall and places well-known stars on it, including the Sun, Sirius, Polaris, Rigel and Betelgeuse. Diagonal lines mark stellar size from 10&amp;lt;sup&amp;gt;−3&amp;lt;/sup&amp;gt; to 10&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt; solar radii, labels along the main sequence give stellar lifetimes from 10&amp;lt;sup&amp;gt;7&amp;lt;/sup&amp;gt; to 10&amp;lt;sup&amp;gt;11&amp;lt;/sup&amp;gt; years, and an arrow at the right shows mass increasing toward the top.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key mw_main_23:diff::1.12:old-5819:rev-5821 --&gt;
&lt;/table&gt;</summary>
		<author><name>Conrad</name></author>
	</entry>
	<entry>
		<id>https://nyssls.info/index.php?title=H-R_Diagram&amp;diff=5819&amp;oldid=prev</id>
		<title>Conrad: SEO: image scales down to fit phone screens (no more sideways scrolling)</title>
		<link rel="alternate" type="text/html" href="https://nyssls.info/index.php?title=H-R_Diagram&amp;diff=5819&amp;oldid=prev"/>
		<updated>2026-10-13T15:17:58Z</updated>

		<summary type="html">&lt;p&gt;SEO: image scales down to fit phone screens (no more sideways scrolling)&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&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 15:17, 13 October 2026&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-l7&quot; &gt;Line 7:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 7:&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: #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;The '''H-R Diagram''' (Hertzsprung–Russell diagram) from the ''Reference Tables for Earth and Space Sciences'' (ESSRT) plots the luminosity of stars, in solar units, against their surface temperature in kelvins, with spectral class (O, B, A, F, G, K, M) and color from blue to red along the bottom. It shows where the main sequence, giants, supergiants and white dwarfs fall and places well-known stars on the diagram, including the Sun, Sirius, Polaris, Rigel and Betelgeuse. Diagonal lines mark stellar size from 10&amp;lt;sup&amp;gt;−3&amp;lt;/sup&amp;gt; to 10&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt; solar radii, labels along the main sequence give stellar lifetimes from 10&amp;lt;sup&amp;gt;7&amp;lt;/sup&amp;gt; to 10&amp;lt;sup&amp;gt;11&amp;lt;/sup&amp;gt; years, and an arrow at the right shows mass increasing toward the top. This table primarily supports [[HS-ESS1-3]].&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;The '''H-R Diagram''' (Hertzsprung–Russell diagram) from the ''Reference Tables for Earth and Space Sciences'' (ESSRT) plots the luminosity of stars, in solar units, against their surface temperature in kelvins, with spectral class (O, B, A, F, G, K, M) and color from blue to red along the bottom. It shows where the main sequence, giants, supergiants and white dwarfs fall and places well-known stars on the diagram, including the Sun, Sirius, Polaris, Rigel and Betelgeuse. Diagonal lines mark stellar size from 10&amp;lt;sup&amp;gt;−3&amp;lt;/sup&amp;gt; to 10&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt; solar radii, labels along the main sequence give stellar lifetimes from 10&amp;lt;sup&amp;gt;7&amp;lt;/sup&amp;gt; to 10&amp;lt;sup&amp;gt;11&amp;lt;/sup&amp;gt; years, and an arrow at the right shows mass increasing toward the top. This table primarily supports [[HS-ESS1-3]].&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: #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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;[[File:H-R Diagram.png|800px|alt=H-R Diagram from the Earth and Space Sciences Reference Tables (ESSRT): luminosity of stars plotted against surface temperature and spectral class, showing the main sequence, giants, supergiants and white dwarfs]]&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;[[File:H-R Diagram.png|800px&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;|class=img-fluid&lt;/ins&gt;|alt=H-R Diagram from the Earth and Space Sciences Reference Tables (ESSRT): luminosity of stars plotted against surface temperature and spectral class, showing the main sequence, giants, supergiants and white dwarfs]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key mw_main_23:diff::1.12:old-5817:rev-5819 --&gt;
&lt;/table&gt;</summary>
		<author><name>Conrad</name></author>
	</entry>
	<entry>
		<id>https://nyssls.info/index.php?title=H-R_Diagram&amp;diff=5817&amp;oldid=prev</id>
		<title>Conrad: SEO: title subtitle, description of the diagram, alt text, links to the neighboring tables and the standard it supports</title>
		<link rel="alternate" type="text/html" href="https://nyssls.info/index.php?title=H-R_Diagram&amp;diff=5817&amp;oldid=prev"/>
		<updated>2026-10-13T15:08:24Z</updated>

		<summary type="html">&lt;p&gt;SEO: title subtitle, description of the diagram, alt text, links to the neighboring tables and the standard it supports&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&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 15:08, 13 October 2026&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='diff-marker'&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;{| &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;style&lt;/del&gt;=&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;&amp;quot;width:100%; table&lt;/del&gt;-&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;layout:fixed; margin&lt;/del&gt;-&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;top&lt;/del&gt;:-&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;1.0em; margin&lt;/del&gt;-&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;bottom:1&lt;/del&gt;.&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;2em; background&lt;/del&gt;-&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;color:rgb&lt;/del&gt;(&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;245&lt;/del&gt;, &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;250&lt;/del&gt;, &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;255&lt;/del&gt;)&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;;&amp;quot;&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt;{Reftable&lt;/ins&gt;&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: #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;&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;| style=&amp;quot;text-align:left; font&lt;/del&gt;-size&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;:1&lt;/del&gt;.&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;12em; padding:5px 8px;&amp;quot; | &lt;/del&gt;[[&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Earth and Space Science Reference Tables|⇱ See all reference tables&lt;/del&gt;]]&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt; &lt;/ins&gt;|&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;name&lt;/ins&gt;=&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;H&lt;/ins&gt;-&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;R Diagram&lt;/ins&gt;&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: #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;&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;|}&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt; |prev=Emission Spectra of Some Elements from Stars&lt;/ins&gt;&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: #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;[[File:H-R Diagram.png|800px]]&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt; |next=Life Cycles of Stars Model&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt; |desc=H&lt;/ins&gt;-&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;R Diagram from the NYS Earth and Space Sciences Reference Tables (ESSRT)&lt;/ins&gt;: &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;star luminosity against surface temperature and spectral class, with the main sequence, giants, supergiants and white dwarfs. Supports HS&lt;/ins&gt;-&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;ESS1&lt;/ins&gt;-&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;3&lt;/ins&gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt;}}&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt;The '''H&lt;/ins&gt;-&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;R Diagram''' (Hertzsprung–Russell diagram) from the ''Reference Tables for Earth and Space Sciences'' (ESSRT) plots the luminosity of stars, in solar units, against their surface temperature in kelvins, with spectral class &lt;/ins&gt;(&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;O, B, A, F, G&lt;/ins&gt;, &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;K&lt;/ins&gt;, &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;M&lt;/ins&gt;) &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;and color from blue to red along the bottom. It shows where the main sequence, giants, supergiants and white dwarfs fall and places well&lt;/ins&gt;-&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;known stars on the diagram, including the Sun, Sirius, Polaris, Rigel and Betelgeuse. Diagonal lines mark stellar &lt;/ins&gt;size &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;from 10&amp;lt;sup&amp;gt;−3&amp;lt;/sup&amp;gt; to 10&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt; solar radii, labels along the main sequence give stellar lifetimes from 10&amp;lt;sup&amp;gt;7&amp;lt;/sup&amp;gt; to 10&amp;lt;sup&amp;gt;11&amp;lt;/sup&amp;gt; years, and an arrow at the right shows mass increasing toward the top&lt;/ins&gt;. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;This table primarily supports &lt;/ins&gt;[[&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;HS-ESS1-3&lt;/ins&gt;]]&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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;[[File:H-R Diagram.png|800px&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;|alt=H-R Diagram from the Earth and Space Sciences Reference Tables (ESSRT): luminosity of stars plotted against surface temperature and spectral class, showing the main sequence, giants, supergiants and white dwarfs&lt;/ins&gt;]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key mw_main_23:diff::1.12:old-5635:rev-5817 --&gt;
&lt;/table&gt;</summary>
		<author><name>Conrad</name></author>
	</entry>
	<entry>
		<id>https://nyssls.info/index.php?title=H-R_Diagram&amp;diff=5635&amp;oldid=prev</id>
		<title>Conradrichman: Slightly larger directory link with more space above the table</title>
		<link rel="alternate" type="text/html" href="https://nyssls.info/index.php?title=H-R_Diagram&amp;diff=5635&amp;oldid=prev"/>
		<updated>2026-09-25T13:54:34Z</updated>

		<summary type="html">&lt;p&gt;Slightly larger directory link with more space above the table&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&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 13:54, 25 September 2026&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='diff-marker'&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;{| style=&amp;quot;width:100%; table-layout:fixed; margin-top:-1.0em; margin-bottom:&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;0&lt;/del&gt;.&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;3em&lt;/del&gt;; background-color:rgb(245, 250, 255);&amp;quot;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;{| style=&amp;quot;width:100%; table-layout:fixed; margin-top:-1.0em; margin-bottom:&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;1&lt;/ins&gt;.&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;2em&lt;/ins&gt;; background-color:rgb(245, 250, 255);&amp;quot;&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: #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;| style=&amp;quot;text-align:left;&amp;quot; | [[Earth and Space Science Reference Tables|⇱ See all reference tables]]&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;| style=&amp;quot;text-align:left&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;; font-size:1.12em; padding:5px 8px&lt;/ins&gt;;&amp;quot; | [[Earth and Space Science Reference Tables|⇱ See all reference tables]]&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: #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;|}&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;|}&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: #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:H-R Diagram.png|800px]]&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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:H-R Diagram.png|800px]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key mw_main_23:diff::1.12:old-5611:rev-5635 --&gt;
&lt;/table&gt;</summary>
		<author><name>Conradrichman</name></author>
	</entry>
	<entry>
		<id>https://nyssls.info/index.php?title=H-R_Diagram&amp;diff=5611&amp;oldid=prev</id>
		<title>Conradrichman: Link back to the reference tables directory</title>
		<link rel="alternate" type="text/html" href="https://nyssls.info/index.php?title=H-R_Diagram&amp;diff=5611&amp;oldid=prev"/>
		<updated>2026-09-25T13:49:31Z</updated>

		<summary type="html">&lt;p&gt;Link back to the reference tables directory&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&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 13:49, 25 September 2026&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 colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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;{| style=&amp;quot;width:100%; table-layout:fixed; margin-top:-1.0em; margin-bottom:0.3em; background-color:rgb(245, 250, 255);&amp;quot;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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;| style=&amp;quot;text-align:left;&amp;quot; | [[Earth and Space Science Reference Tables|⇱ See all reference tables]]&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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;|}&lt;/ins&gt;&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: #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:H-R Diagram.png|800px]]&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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:H-R Diagram.png|800px]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key mw_main_23:diff::1.12:old-1157:rev-5611 --&gt;
&lt;/table&gt;</summary>
		<author><name>Conradrichman</name></author>
	</entry>
	<entry>
		<id>https://nyssls.info/index.php?title=H-R_Diagram&amp;diff=1157&amp;oldid=prev</id>
		<title>Conradrichman: Created page with &quot;800px&quot;</title>
		<link rel="alternate" type="text/html" href="https://nyssls.info/index.php?title=H-R_Diagram&amp;diff=1157&amp;oldid=prev"/>
		<updated>2025-04-11T16:29:49Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;&lt;a href=&quot;/index.php/File:H-R_Diagram.png&quot; title=&quot;File:H-R Diagram.png&quot;&gt;800px&lt;/a&gt;&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;[[File:H-R Diagram.png|800px]]&lt;/div&gt;</summary>
		<author><name>Conradrichman</name></author>
	</entry>
</feed>