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		<id>http://wiki.newmars.com/index.php?action=history&amp;feed=atom&amp;title=Sabatier_reaction</id>
		<title>Sabatier reaction - Revision history</title>
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		<updated>2026-05-24T11:41:38Z</updated>
		<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
		<id>http://wiki.newmars.com/index.php?title=Sabatier_reaction&amp;diff=497&amp;oldid=prev</id>
		<title>Josh Cryer: 1 revision</title>
		<link rel="alternate" type="text/html" href="http://wiki.newmars.com/index.php?title=Sabatier_reaction&amp;diff=497&amp;oldid=prev"/>
				<updated>2009-01-21T11:02:37Z</updated>
		
		<summary type="html">&lt;p&gt;1 revision&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=&#039;1&#039; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&#039;1&#039; style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 11:02, 21 January 2009&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&#039;2&#039; style=&#039;text-align: center;&#039; lang=&#039;en&#039;&gt;&lt;div class=&quot;mw-diff-empty&quot;&gt;(No difference)&lt;/div&gt;
&lt;/td&gt;&lt;/tr&gt;&lt;/table&gt;</summary>
		<author><name>Josh Cryer</name></author>	</entry>

	<entry>
		<id>http://wiki.newmars.com/index.php?title=Sabatier_reaction&amp;diff=496&amp;oldid=prev</id>
		<title>Maxie at 22:17, 29 January 2006</title>
		<link rel="alternate" type="text/html" href="http://wiki.newmars.com/index.php?title=Sabatier_reaction&amp;diff=496&amp;oldid=prev"/>
				<updated>2006-01-29T22:17:46Z</updated>
		
		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;The Sabatier reaction creates methane (a possible fuel for launch vehicles and rovers) and water from hydrogen and carbon dioxide, at high temperature and elevated pressure, and in the presence of a catalyst (nickel, or better, ruthenium and alumina).&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;CO_2  + 4H_2  \to \limits^{300^\circ C} CH_4  + 2H_2 O&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
For Marsian [[ISRU]], hydrogen could be imported from Earth, or produced by [[Water electrolysis|water electrolysis]]. Water could be collected from Marsian sources (&amp;#039;&amp;#039;see&amp;#039;&amp;#039;: [[Water on Mars]]), and also could be reused from the above reaction itself.&lt;br /&gt;
&lt;br /&gt;
==External links and references==&lt;br /&gt;
* [http://www.isso.uh.edu/publications/A9900/mini-richardson.htm Improved Sabatier Reactions for In Situ Resource Utilization on Mars Missions]&lt;br /&gt;
*Zubrin, Robert M., Price, S., Mason, L., Clark, L. (1994) &amp;quot;Report on the Construction and Operation of a Mars In-Situ Propellant Production Unit&amp;quot;, AIAA 94-2844, AIAA Joint Propellant Conference, Indianapolis, IN, [http://citeseer.ist.psu.edu/cache/papers/cs/24349/http:zSzzSzwww.nw.netzSzmarszSzdocszSzisrudemo.pdf/report-on-the-construction.pdf pdf available here].&lt;br /&gt;
&lt;br /&gt;
[[Category:In-situ Resource Utilization]]&lt;/div&gt;</summary>
		<author><name>Maxie</name></author>	</entry>

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