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	<title>Satellites and Binding Energy EX 13 - Revision history</title>
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	<updated>2026-04-20T23:14:51Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<title>imported&gt;Patrick: Created page with &#039;The shuttle is in an orbit of radius &lt;math&gt;r&lt;/math&gt; which 5% smaller than rg. Therefore the radius of this orbit &lt;math&gt;r = 0.95 r_g&lt;/math&gt;.  First we have to determine the radius…&#039;</title>
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		<updated>2011-09-30T03:49:17Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;#039;The shuttle is in an orbit of radius &amp;lt;math&amp;gt;r&amp;lt;/math&amp;gt; which 5% smaller than rg. Therefore the radius of this orbit &amp;lt;math&amp;gt;r = 0.95 r_g&amp;lt;/math&amp;gt;.  First we have to determine the radius…&amp;#039;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;The shuttle is in an orbit of radius &amp;lt;math&amp;gt;r&amp;lt;/math&amp;gt; which 5% smaller than rg. Therefore the radius of this orbit &amp;lt;math&amp;gt;r = 0.95 r_g&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
First we have to determine the radius in the geosynchroneous orbit using Kepler&amp;#039;s Law:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;r = \left ( {G M_E T^2 \over 4 \pi^2} \right )^{\frac{1}{3}} = \left ( {(6.67 \times 10^{-11})(6 \times 10^{24})(8.64 \times 10^4)^2 \over 4 \pi^2} \right )^{\frac{1}{3}} = 4.16 \times 10^7 m&amp;lt;/math&amp;gt;&lt;br /&gt;
&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
Then &amp;lt;math&amp;gt;r = 0.95 r_g = 0.95 \times 4.16 \times 10^7 = 3.94 \times 10^7 m&amp;lt;/math&amp;gt; and the energy of the shuttle in this orbit is&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;E_i = -\frac{1}{2}{G M_E m \over r} = -\frac{1}{2}{(6.67 \times 10^{-11})(6 \times 10^{24})(10^4) \over 3.94 \times 10^7} = -5.1 \times 10^{10} J&amp;lt;/math&amp;gt;&lt;br /&gt;
&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
To get into the geosynchroneous orbit the shuttle needs to have the energy&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;E_f = -\frac{1}{2}{G M_E m \over r} = -\frac{1}{2}{(6.67 \times 10^{-11})(6 \times 10^{24})(10^4) \over 4.16 \times 10^7} = -4.8 \times 10^{10} J&amp;lt;/math&amp;gt;&lt;br /&gt;
&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
The boosters must provide the difference between these two energies.&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;\Delta E = E_f - E_i = -4.8 \times 10^{10} - (-5.1 \times 10^{10}) = 3 \times 10^9 J&amp;lt;/math&amp;gt;&lt;/div&gt;</summary>
		<author><name>imported&gt;Patrick</name></author>
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