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	<id>https://marspedia.org/index.php?action=history&amp;feed=atom&amp;title=Talk%3AGravitational_parameter</id>
	<title>Talk:Gravitational parameter - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://marspedia.org/index.php?action=history&amp;feed=atom&amp;title=Talk%3AGravitational_parameter"/>
	<link rel="alternate" type="text/html" href="https://marspedia.org/index.php?title=Talk:Gravitational_parameter&amp;action=history"/>
	<updated>2026-06-15T17:39:52Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
		<id>https://marspedia.org/index.php?title=Talk:Gravitational_parameter&amp;diff=8510&amp;oldid=prev</id>
		<title>Rfc: Undo revision 8503 by 18.7.125.24 (Talk)</title>
		<link rel="alternate" type="text/html" href="https://marspedia.org/index.php?title=Talk:Gravitational_parameter&amp;diff=8510&amp;oldid=prev"/>
		<updated>2013-03-11T21:05:57Z</updated>

		<summary type="html">&lt;p&gt;Undo revision 8503 by &lt;a href=&quot;/Special:Contributions/18.7.125.24&quot; title=&quot;Special:Contributions/18.7.125.24&quot;&gt;18.7.125.24&lt;/a&gt; (&lt;a href=&quot;/index.php?title=User_talk:18.7.125.24&amp;amp;action=edit&amp;amp;redlink=1&quot; class=&quot;new&quot; title=&quot;User talk:18.7.125.24 (page does not exist)&quot;&gt;Talk&lt;/a&gt;)&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
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				&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: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 21:05, 11 March 2013&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-l4&quot; &gt;Line 4:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 4:&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: #222; 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;::However g is calculated, it is the value that I find in some references.  If I do not have mu but have g and r from a reference naturally that is what I would use.  Actually I have seldom found mu tabulated in the references that I have used.  Where it was tabulated, it was referred to as g*r&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  I just do not have the sort of references that are available to you.  - [[User:Farred|Farred]] 18:38, 20 February 2013 (UTC)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;::However g is calculated, it is the value that I find in some references.  If I do not have mu but have g and r from a reference naturally that is what I would use.  Actually I have seldom found mu tabulated in the references that I have used.  Where it was tabulated, it was referred to as g*r&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  I just do not have the sort of references that are available to you.  - [[User:Farred|Farred]] 18:38, 20 February 2013 (UTC)&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: #222; 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;:::Of course you should use the available values if that is all you have. That's why I tabulated mu values in the first place -- so everyone can see them. Perhaps we should nevertheless add a &amp;quot;relation to gravity&amp;quot; section showing how g = mu*r^-2 at distance r. If you have money to burn and want to expand your technical book collection, I can recommend [http://astrobooks.com Microcosm's bookstore]. Perhaps we should add a section for spaceflight related bookstores to [[Links and Resources]]. [[User:ChristiaanK|ChristiaanK]] 08:16, 22 February 2013 (UTC)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;:::Of course you should use the available values if that is all you have. That's why I tabulated mu values in the first place -- so everyone can see them. Perhaps we should nevertheless add a &amp;quot;relation to gravity&amp;quot; section showing how g = mu*r^-2 at distance r. If you have money to burn and want to expand your technical book collection, I can recommend [http://astrobooks.com Microcosm's bookstore]. Perhaps we should add a section for spaceflight related bookstores to [[Links and Resources]]. [[User:ChristiaanK|ChristiaanK]] 08:16, 22 February 2013 (UTC)&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: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&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: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;== SGPXgcUOwGHMnqSse ==&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&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: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&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: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Beth - Wow, so handsome Lailah!  You're going to have a line of girls outsdie your house pretty soon!  Erin is going to be first in line.  =) It was so cute how sweet he was with her when you guys visited!&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Rfc</name></author>
		
	</entry>
	<entry>
		<id>https://marspedia.org/index.php?title=Talk:Gravitational_parameter&amp;diff=8503&amp;oldid=prev</id>
		<title>18.7.125.24: /* SGPXgcUOwGHMnqSse */ new section</title>
		<link rel="alternate" type="text/html" href="https://marspedia.org/index.php?title=Talk:Gravitational_parameter&amp;diff=8503&amp;oldid=prev"/>
		<updated>2013-03-11T17:14:49Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;SGPXgcUOwGHMnqSse: &lt;/span&gt; new section&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
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				&lt;col class=&quot;diff-marker&quot; /&gt;
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				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 17:14, 11 March 2013&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-l4&quot; &gt;Line 4:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 4:&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: #222; 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;::However g is calculated, it is the value that I find in some references.  If I do not have mu but have g and r from a reference naturally that is what I would use.  Actually I have seldom found mu tabulated in the references that I have used.  Where it was tabulated, it was referred to as g*r&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  I just do not have the sort of references that are available to you.  - [[User:Farred|Farred]] 18:38, 20 February 2013 (UTC)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;::However g is calculated, it is the value that I find in some references.  If I do not have mu but have g and r from a reference naturally that is what I would use.  Actually I have seldom found mu tabulated in the references that I have used.  Where it was tabulated, it was referred to as g*r&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  I just do not have the sort of references that are available to you.  - [[User:Farred|Farred]] 18:38, 20 February 2013 (UTC)&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: #222; 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;:::Of course you should use the available values if that is all you have. That's why I tabulated mu values in the first place -- so everyone can see them. Perhaps we should nevertheless add a &amp;quot;relation to gravity&amp;quot; section showing how g = mu*r^-2 at distance r. If you have money to burn and want to expand your technical book collection, I can recommend [http://astrobooks.com Microcosm's bookstore]. Perhaps we should add a section for spaceflight related bookstores to [[Links and Resources]]. [[User:ChristiaanK|ChristiaanK]] 08:16, 22 February 2013 (UTC)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;:::Of course you should use the available values if that is all you have. That's why I tabulated mu values in the first place -- so everyone can see them. Perhaps we should nevertheless add a &amp;quot;relation to gravity&amp;quot; section showing how g = mu*r^-2 at distance r. If you have money to burn and want to expand your technical book collection, I can recommend [http://astrobooks.com Microcosm's bookstore]. Perhaps we should add a section for spaceflight related bookstores to [[Links and Resources]]. [[User:ChristiaanK|ChristiaanK]] 08:16, 22 February 2013 (UTC)&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: #222; 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: #222; 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;== SGPXgcUOwGHMnqSse ==&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: #222; 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: #222; 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;Beth - Wow, so handsome Lailah!  You're going to have a line of girls outsdie your house pretty soon!  Erin is going to be first in line.  =) It was so cute how sweet he was with her when you guys visited!&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>18.7.125.24</name></author>
		
	</entry>
	<entry>
		<id>https://marspedia.org/index.php?title=Talk:Gravitational_parameter&amp;diff=8374&amp;oldid=prev</id>
		<title>ChristiaanK: /* Alternate value of mu */</title>
		<link rel="alternate" type="text/html" href="https://marspedia.org/index.php?title=Talk:Gravitational_parameter&amp;diff=8374&amp;oldid=prev"/>
		<updated>2013-02-22T08:16:22Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Alternate value of mu&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
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				&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: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 08:16, 22 February 2013&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-l3&quot; &gt;Line 3:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 3:&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: #222; 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;:I'm not sure why you would want to do that. For heavenly bodies, the average surface gravity g is calculated from mu using the very formula that you just gave (mu and r being determined from astronomical observation). Why would you want to work backwards from this to get mu? I agree that inaccurate values are fine for most ballpark feasibility studies, but finding accurate values takes little time and offers several advantages. A small force over an Earth-Mars transit orbit makes a big difference and inaccurate values are compounded when you work backwards from the fuel needed for the last leg of a mission to determine the fuel needed at the beginning. [[User:ChristiaanK|ChristiaanK]] 17:01, 20 February 2013 (UTC)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;:I'm not sure why you would want to do that. For heavenly bodies, the average surface gravity g is calculated from mu using the very formula that you just gave (mu and r being determined from astronomical observation). Why would you want to work backwards from this to get mu? I agree that inaccurate values are fine for most ballpark feasibility studies, but finding accurate values takes little time and offers several advantages. A small force over an Earth-Mars transit orbit makes a big difference and inaccurate values are compounded when you work backwards from the fuel needed for the last leg of a mission to determine the fuel needed at the beginning. [[User:ChristiaanK|ChristiaanK]] 17:01, 20 February 2013 (UTC)&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: #222; 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;::However g is calculated, it is the value that I find in some references.  If I do not have mu but have g and r from a reference naturally that is what I would use.  Actually I have seldom found mu tabulated in the references that I have used.  Where it was tabulated, it was referred to as g*r&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  I just do not have the sort of references that are available to you.  - [[User:Farred|Farred]] 18:38, 20 February 2013 (UTC)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;::However g is calculated, it is the value that I find in some references.  If I do not have mu but have g and r from a reference naturally that is what I would use.  Actually I have seldom found mu tabulated in the references that I have used.  Where it was tabulated, it was referred to as g*r&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  I just do not have the sort of references that are available to you.  - [[User:Farred|Farred]] 18:38, 20 February 2013 (UTC)&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: #222; 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;:::Of course you should use the available values if that is all you have. That's why I tabulated mu values in the first place -- so everyone can see them. Perhaps we should nevertheless add a &amp;quot;relation to gravity&amp;quot; section showing how g = mu*r^-2 at distance r. If you have money to burn and want to expand your technical book collection, I can recommend [http://astrobooks.com Microcosm's bookstore]. Perhaps we should add a section for spaceflight related bookstores to [[Links and Resources]]. [[User:ChristiaanK|ChristiaanK]] 08:16, 22 February 2013 (UTC)&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>ChristiaanK</name></author>
		
	</entry>
	<entry>
		<id>https://marspedia.org/index.php?title=Talk:Gravitational_parameter&amp;diff=8368&amp;oldid=prev</id>
		<title>Farred: talk</title>
		<link rel="alternate" type="text/html" href="https://marspedia.org/index.php?title=Talk:Gravitational_parameter&amp;diff=8368&amp;oldid=prev"/>
		<updated>2013-02-20T18:38:40Z</updated>

		<summary type="html">&lt;p&gt;talk&lt;/p&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 18:38, 20 February 2013&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-l2&quot; &gt;Line 2:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 2:&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: #222; 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;I would like to point out that mu also equals g*r^2.  Gravity, g, = G * m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;/r^2.  So G = g * r^2 /m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;.  Substituting that into mu = GM, we get mu = g*r^2, QED.  This is the form of mu that I have been in the habit of using since gravity and radius are usually more available to me than G and m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;.  I have done paper missions with less accurate values but they were sufficient for my purposes.  See [[People from Earth to Mars in 30 days]]  - [[User:Farred|Farred]] 04:35, 19 February 2013 (UTC)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;I would like to point out that mu also equals g*r^2.  Gravity, g, = G * m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;/r^2.  So G = g * r^2 /m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;.  Substituting that into mu = GM, we get mu = g*r^2, QED.  This is the form of mu that I have been in the habit of using since gravity and radius are usually more available to me than G and m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;.  I have done paper missions with less accurate values but they were sufficient for my purposes.  See [[People from Earth to Mars in 30 days]]  - [[User:Farred|Farred]] 04:35, 19 February 2013 (UTC)&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: #222; 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;:I'm not sure why you would want to do that. For heavenly bodies, the average surface gravity g is calculated from mu using the very formula that you just gave (mu and r being determined from astronomical observation). Why would you want to work backwards from this to get mu? I agree that inaccurate values are fine for most ballpark feasibility studies, but finding accurate values takes little time and offers several advantages. A small force over an Earth-Mars transit orbit makes a big difference and inaccurate values are compounded when you work backwards from the fuel needed for the last leg of a mission to determine the fuel needed at the beginning. [[User:ChristiaanK|ChristiaanK]] 17:01, 20 February 2013 (UTC)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;:I'm not sure why you would want to do that. For heavenly bodies, the average surface gravity g is calculated from mu using the very formula that you just gave (mu and r being determined from astronomical observation). Why would you want to work backwards from this to get mu? I agree that inaccurate values are fine for most ballpark feasibility studies, but finding accurate values takes little time and offers several advantages. A small force over an Earth-Mars transit orbit makes a big difference and inaccurate values are compounded when you work backwards from the fuel needed for the last leg of a mission to determine the fuel needed at the beginning. [[User:ChristiaanK|ChristiaanK]] 17:01, 20 February 2013 (UTC)&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: #222; 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;::However g is calculated, it is the value that I find in some references.  If I do not have mu but have g and r from a reference naturally that is what I would use.  Actually I have seldom found mu tabulated in the references that I have used.  Where it was tabulated, it was referred to as g*r&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  I just do not have the sort of references that are available to you.  - [[User:Farred|Farred]] 18:38, 20 February 2013 (UTC)&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Farred</name></author>
		
	</entry>
	<entry>
		<id>https://marspedia.org/index.php?title=Talk:Gravitational_parameter&amp;diff=8360&amp;oldid=prev</id>
		<title>ChristiaanK: /* Alternate value of mu */</title>
		<link rel="alternate" type="text/html" href="https://marspedia.org/index.php?title=Talk:Gravitational_parameter&amp;diff=8360&amp;oldid=prev"/>
		<updated>2013-02-20T17:01:02Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Alternate value of mu&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 17:01, 20 February 2013&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;background-color: #f8f9fa; color: #222; 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;==Alternate value of mu==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;==Alternate value of mu==&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: #222; 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;I would like to point out that mu also equals g*r^2.  Gravity, g, = G * m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;/r^2.  So G = g * r^2 /m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;.  Substituting that into mu = GM, we get mu = g*r^2, QED.  This is the form of mu that I have been in the habit of using since gravity and radius are usually more available to me than G and m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;.  I have done paper missions with less accurate values but they were sufficient for my purposes.  See [[People from Earth to Mars in 30 days]]  - [[User:Farred|Farred]] 04:35, 19 February 2013 (UTC)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;I would like to point out that mu also equals g*r^2.  Gravity, g, = G * m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;/r^2.  So G = g * r^2 /m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;.  Substituting that into mu = GM, we get mu = g*r^2, QED.  This is the form of mu that I have been in the habit of using since gravity and radius are usually more available to me than G and m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;.  I have done paper missions with less accurate values but they were sufficient for my purposes.  See [[People from Earth to Mars in 30 days]]  - [[User:Farred|Farred]] 04:35, 19 February 2013 (UTC)&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: #222; 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;:I'm not sure why you would want to do that. For heavenly bodies, the average surface gravity g is calculated from mu using the very formula that you just gave (mu and r being determined from astronomical observation). Why would you want to work backwards from this to get mu? I agree that inaccurate values are fine for most ballpark feasibility studies, but finding accurate values takes little time and offers several advantages. A small force over an Earth-Mars transit orbit makes a big difference and inaccurate values are compounded when you work backwards from the fuel needed for the last leg of a mission to determine the fuel needed at the beginning. [[User:ChristiaanK|ChristiaanK]] 17:01, 20 February 2013 (UTC)&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>ChristiaanK</name></author>
		
	</entry>
	<entry>
		<id>https://marspedia.org/index.php?title=Talk:Gravitational_parameter&amp;diff=8339&amp;oldid=prev</id>
		<title>Farred: Alternate value of mu</title>
		<link rel="alternate" type="text/html" href="https://marspedia.org/index.php?title=Talk:Gravitational_parameter&amp;diff=8339&amp;oldid=prev"/>
		<updated>2013-02-19T04:35:24Z</updated>

		<summary type="html">&lt;p&gt;Alternate value of mu&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;==Alternate value of mu==&lt;br /&gt;
I would like to point out that mu also equals g*r^2.  Gravity, g, = G * m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;/r^2.  So G = g * r^2 /m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;.  Substituting that into mu = GM, we get mu = g*r^2, QED.  This is the form of mu that I have been in the habit of using since gravity and radius are usually more available to me than G and m&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;.  I have done paper missions with less accurate values but they were sufficient for my purposes.  See [[People from Earth to Mars in 30 days]]  - [[User:Farred|Farred]] 04:35, 19 February 2013 (UTC)&lt;/div&gt;</summary>
		<author><name>Farred</name></author>
		
	</entry>
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