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	<title>3Dconfigurations/RiemannEllipsoids - Revision history</title>
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	<updated>2026-04-28T22:26:02Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<id>https://selfgravitatingfluids.education/JETohline/index.php?title=3Dconfigurations/RiemannEllipsoids&amp;diff=1819&amp;oldid=prev</id>
		<title>Joel2: Created page with &quot;__FORCETOC__  &lt;!-- __NOTOC__ will force TOC off --&gt;  =Riemann (1826 - 1866)=  ==Background==  Excerpt from p. 539 of R. Baker, C. Christenson &amp;amp; H. Orde (2004): &lt;table border=&quot;0&quot; width=&quot;90%&quot; align=&quot;center&quot;&gt;&lt;tr&gt;&lt;td align=&quot;left&quot;&gt; &lt;font color=&quot;darkgreen&quot;&gt;&quot;Newton first showed that the departure of the figure of the earth from a sphere is due to its rotation.  Jacobi showed in 1834 that gravitational equilibrium of a rotating spheroid is consistent with three distinct axes...&quot;</title>
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		<updated>2024-07-03T00:58:05Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;__FORCETOC__  &amp;lt;!-- __NOTOC__ will force TOC off --&amp;gt;  =Riemann (1826 - 1866)=  ==Background==  Excerpt from p. 539 of R. Baker, C. Christenson &amp;amp; H. Orde (2004): &amp;lt;table border=&amp;quot;0&amp;quot; width=&amp;quot;90%&amp;quot; align=&amp;quot;center&amp;quot;&amp;gt;&amp;lt;tr&amp;gt;&amp;lt;td align=&amp;quot;left&amp;quot;&amp;gt; &amp;lt;font color=&amp;quot;darkgreen&amp;quot;&amp;gt;&amp;quot;Newton first showed that the departure of the figure of the earth from a sphere is due to its rotation.  Jacobi showed in 1834 that gravitational equilibrium of a rotating spheroid is consistent with three distinct axes...&amp;quot;&lt;/p&gt;
&lt;a href=&quot;https://selfgravitatingfluids.education/JETohline/index.php?title=3Dconfigurations/RiemannEllipsoids&amp;amp;diff=1819&quot;&gt;Show changes&lt;/a&gt;</summary>
		<author><name>Joel2</name></author>
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