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	<title>Satellites and Binding Energy EX 10 - Revision history</title>
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	<updated>2026-06-01T19:34:57Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<id>https://euler.vaniercollege.qc.ca/gwikis/pwiki/index.php?title=Satellites_and_Binding_Energy_EX_10&amp;diff=629&amp;oldid=prev</id>
		<title>imported&gt;Patrick: Created page with &#039;The distance between the Earth and the Sun is &lt;math&gt;1.5 \times 10^{11} m&lt;/math&gt; and the masses of these objects are &lt;math&gt;6 \times 10^{24} kg&lt;/math&gt; and &lt;math&gt;2 \times 10^{30} kg…&#039;</title>
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		<updated>2011-09-29T22:12:16Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;#039;The distance between the Earth and the Sun is &amp;lt;math&amp;gt;1.5 \times 10^{11} m&amp;lt;/math&amp;gt; and the masses of these objects are &amp;lt;math&amp;gt;6 \times 10^{24} kg&amp;lt;/math&amp;gt; and &amp;lt;math&amp;gt;2 \times 10^{30} kg…&amp;#039;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;The distance between the Earth and the Sun is &amp;lt;math&amp;gt;1.5 \times 10^{11} m&amp;lt;/math&amp;gt; and the masses of these objects are &amp;lt;math&amp;gt;6 \times 10^{24} kg&amp;lt;/math&amp;gt; and &amp;lt;math&amp;gt;2 \times 10^{30} kg&amp;lt;/math&amp;gt;. The Earth is orbiting the Sun and therefore the energy of the system is&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;E = \frac{1}{2} U = -\frac{1}{2} {G M_S M_E \over r} = -\frac{1}{2} {(6.67 \times 10^{-11})(2 \times 10^{30})(6 \times 10^{24}) \over 1.5 \times 10^{11}} = -5.3 \times 10^{33} J&amp;lt;/math&amp;gt;&lt;br /&gt;
&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
The escape velocity at the distance &amp;lt;math&amp;gt;r = 1.5 \times 10^{11} m&amp;lt;/math&amp;gt; is given by&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;v = \sqrt{2 G M_S \over r} = \sqrt{2 (6.67 \times 10^{-11}) (2 \times 10^{30}) \over 1.5 \times 10^{11}} = 4.22 \times 10^4 m/s = 42.2 km/s&amp;lt;/math&amp;gt;&lt;/div&gt;</summary>
		<author><name>imported&gt;Patrick</name></author>
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