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		<title>Magnetic fields of Mars - Revision history</title>
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		<updated>2026-05-25T12:18:57Z</updated>
		<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
		<id>http://wiki.newmars.com/index.php?title=Magnetic_fields_of_Mars&amp;diff=299&amp;oldid=prev</id>
		<title>Josh Cryer: 1 revision</title>
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				<updated>2009-01-21T11:02:31Z</updated>
		
		<summary type="html">&lt;p&gt;1 revision&lt;/p&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;
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		<author><name>Josh Cryer</name></author>	</entry>

	<entry>
		<id>http://wiki.newmars.com/index.php?title=Magnetic_fields_of_Mars&amp;diff=298&amp;oldid=prev</id>
		<title>Josh Cryer: Reverted edit of TadroNcnab, changed back to last version by Noosfractal</title>
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				<updated>2009-01-20T13:14:20Z</updated>
		
		<summary type="html">&lt;p&gt;Reverted edit of TadroNcnab, changed back to last version by Noosfractal&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;[[Image:Mars magnetic fields 01.jpg|thumb|200px|right|Local magnetic fields on Mars]]&lt;br /&gt;
Unlike Earth, Mars has no strong global magnetic field, only weak local ones are present.&lt;br /&gt;
&lt;br /&gt;
Surveys in the 1990s of magnetic fields on Mars, by the orbiting [[Mars Global Surveyor]], detected the signatures of relatively intense magnetism in some of the planet&amp;#039;s more modern surfaces. But the fields were found to be very weak in two large and old impact basis, Hellas and Argyre. Each basin, carved out by a colossal space asteroid, is more than 3 billion years old. The data implied that Mars had a weak magnetic field back then.&lt;br /&gt;
&lt;br /&gt;
New research calls into question the validity of measuring magnetism from an orbital perch. It has been found that rocks in the 2-billion-year-old Vredefort impact crater in South Africa -- the oldest such structure on Earth -- are highly magnetized, yet from above the magnetism appears weak. Two other ancient craters reveal similar differences.&lt;br /&gt;
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The basic reason is simple: While magnetism is strong in individual rocks, the direction varies from rock to rock in these impact craters, so when examined from a distance, they cancel each other out.&lt;br /&gt;
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So, viewed from a high altitude of 100-400 km, certain areas of Mars might appear magnetically featureless if the magnetic vectors of their source rocks vary in direction over distances of a few kilometers or less.&lt;br /&gt;
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==Geological implications==&lt;br /&gt;
Magnetic fields on Mars are &amp;quot;striped&amp;quot;, a feature that clearly shows that Mars had crustal plates movement in its history. Stripe patterns like these are widespread on Earth – particularly along the Mid-Atlantic Ridge.&lt;br /&gt;
&lt;br /&gt;
{{MainArticle|[[Geology of Mars]]}}&lt;br /&gt;
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[[Category:Marsian features]]&lt;/div&gt;</summary>
		<author><name>Josh Cryer</name></author>	</entry>

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