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	<id>https://euler.vaniercollege.qc.ca/gwikis/pwiki/index.php?action=history&amp;feed=atom&amp;title=Newtons_Laws_EX_38</id>
	<title>Newtons Laws EX 38 - Revision history</title>
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	<updated>2026-04-20T19:48:45Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
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		<title>imported&gt;Patrick: Created page with &#039;The strength of the gravitational field is also called the &lt;u&gt;gravitational acceleration&lt;/u&gt;. The gravitational acceleration of a particle which is placed at some distance &lt;math&gt;…&#039;</title>
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		<updated>2011-05-27T03:39:39Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;#039;The strength of the gravitational field is also called the &amp;lt;u&amp;gt;gravitational acceleration&amp;lt;/u&amp;gt;. The gravitational acceleration of a particle which is placed at some distance &amp;lt;math&amp;gt;…&amp;#039;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;The strength of the gravitational field is also called the &amp;lt;u&amp;gt;gravitational acceleration&amp;lt;/u&amp;gt;. The gravitational acceleration of a particle which is placed at some distance &amp;lt;math&amp;gt;r&amp;lt;/math&amp;gt; from an object of mass &amp;lt;math&amp;gt;m&amp;lt;/math&amp;gt; is equal to:&lt;br /&gt;
&lt;br /&gt;
 &amp;lt;math&amp;gt;g = {G m \over r^2}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;G = 6.67 \times 10^{-11}&amp;lt;/math&amp;gt;.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;(a)&amp;#039;&amp;#039;&amp;#039; Neptune: &amp;lt;math&amp;gt;g = {(6.67 \times 10^{-11})(1.03 \times 10^{26}) \over (2.43 \times 10^7)^2} = 11.6 m/s^2&amp;lt;/math&amp;gt;&lt;br /&gt;
&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;(b)&amp;#039;&amp;#039;&amp;#039; Jupiter: &amp;lt;math&amp;gt;g = {(6.67 \times 10^{-11})(1.9 \times 10^{27}) \over (7.14 \times 10^7)^2} = 24.8 m/s^2&amp;lt;/math&amp;gt;&lt;br /&gt;
&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;(c)&amp;#039;&amp;#039;&amp;#039; Neutron star: &amp;lt;math&amp;gt;g = {(6.67 \times 10^{-11})(10^{30}) \over (2 \times 10^4)^2} = 1.67 \times 10^{11} m/s^2&amp;lt;/math&amp;gt;&lt;/div&gt;</summary>
		<author><name>imported&gt;Patrick</name></author>
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