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	<id>https://marspedia.org/index.php?action=history&amp;feed=atom&amp;title=Recent_Liquid_Flow_on_Mars</id>
	<title>Recent Liquid Flow on Mars - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://marspedia.org/index.php?action=history&amp;feed=atom&amp;title=Recent_Liquid_Flow_on_Mars"/>
	<link rel="alternate" type="text/html" href="https://marspedia.org/index.php?title=Recent_Liquid_Flow_on_Mars&amp;action=history"/>
	<updated>2026-06-06T21:37:17Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
		<id>https://marspedia.org/index.php?title=Recent_Liquid_Flow_on_Mars&amp;diff=136680&amp;oldid=prev</id>
		<title>Michel Lamontagne at 20:57, 10 November 2020</title>
		<link rel="alternate" type="text/html" href="https://marspedia.org/index.php?title=Recent_Liquid_Flow_on_Mars&amp;diff=136680&amp;oldid=prev"/>
		<updated>2020-11-10T20:57:06Z</updated>

		<summary type="html">&lt;p&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;
				&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 20:57, 10 November 2020&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;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;== Recent liquid flow on Mars? ==  &lt;/div&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;==Recent liquid flow on Mars?==  &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;Photographs of Hebes Chasma were recently published&amp;lt;ref&amp;gt;[http://spacefellowship.com/news/art35520/martian-scars.html &amp;quot;Martian scars&amp;quot; at SPACE FELLOWSHIP]&amp;lt;/ref&amp;gt; which show considerable resemblance to liquid flow features.  The dark stains seem to show something that &amp;quot;pool[ed] like spilt ink&amp;quot;.  Commentator(s) bent over backwards trying to not seem to be guilty of sensationalism.  The stains were suggested to be probably dust movement that produced a &amp;quot;flow-like feature&amp;quot;.  There is a possibility that wind can become heavily laden with dust and flow downwards to leave the dust collected in a broad flat pool, but the images in this case make that explanation seem unlikely.  The possibility of a petroleum seep suggests itself but the flow pattern that would result in the actual images is hard to imagine.  Perhaps some unknown dense gas of volcanic origin collected in Hebes Chasma and then condensed as dew on the surfaces that cooled the most by radiation.  This dew then slowly drained from those surfaces into inky pools in deep depressions in the eastern and central parts of Hebes Chasma.  If there is a liquid on Mars of petroleum nature, it could be an advantage for colonization efforts some day.   &lt;/div&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;Photographs of Hebes Chasma were recently published&amp;lt;ref&amp;gt;[http://spacefellowship.com/news/art35520/martian-scars.html &amp;quot;Martian scars&amp;quot; at SPACE FELLOWSHIP]&amp;lt;/ref&amp;gt; which show considerable resemblance to &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;[[Liquid Water on Mars|&lt;/ins&gt;liquid flow&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;]] &lt;/ins&gt;features.  The dark stains seem to show something that &amp;quot;pool[ed] like spilt ink&amp;quot;.  Commentator(s) bent over backwards trying to not seem to be guilty of sensationalism.  The stains were suggested to be probably dust movement that produced a &amp;quot;flow-like feature&amp;quot;.  There is a possibility that wind can become heavily laden with dust and flow downwards to leave the dust collected in a broad flat pool, but the images in this case make that explanation seem unlikely.  The possibility of a petroleum seep suggests itself but the flow pattern that would result in the actual images is hard to imagine.  Perhaps some unknown dense gas of volcanic origin collected in Hebes Chasma and then condensed as dew on the surfaces that cooled the most by radiation.  This dew then slowly drained from those surfaces into inky pools in deep depressions in the eastern and central parts of Hebes Chasma.  If there is a liquid on Mars of petroleum nature, it could be an advantage for colonization efforts some day.   &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;   &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;   &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;== Reference ==  &lt;/div&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;==Reference==  &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;&amp;lt;references/&amp;gt;  &lt;/div&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;&amp;lt;references /&amp;gt;  &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;   &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;   &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;[[Category:Areology]]&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;[[Category:Areology]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key marspediaorg_www-mwmars_:diff::1.12:old-126953:rev-136680 --&gt;
&lt;/table&gt;</summary>
		<author><name>Michel Lamontagne</name></author>
		
	</entry>
	<entry>
		<id>https://marspedia.org/index.php?title=Recent_Liquid_Flow_on_Mars&amp;diff=126953&amp;oldid=prev</id>
		<title>Jburk at 18:18, 17 December 2018</title>
		<link rel="alternate" type="text/html" href="https://marspedia.org/index.php?title=Recent_Liquid_Flow_on_Mars&amp;diff=126953&amp;oldid=prev"/>
		<updated>2018-12-17T18:18:03Z</updated>

		<summary type="html">&lt;p&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-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 18:18, 17 December 2018&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-l5&quot; &gt;Line 5:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 5:&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;&amp;lt;references/&amp;gt;  &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;&amp;lt;references/&amp;gt;  &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;   &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;   &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;[[Category:&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Geology&lt;/del&gt;]]&lt;/div&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;[[Category:&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Areology&lt;/ins&gt;]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key marspediaorg_www-mwmars_:diff::1.12:old-14220:rev-126953 --&gt;
&lt;/table&gt;</summary>
		<author><name>Jburk</name></author>
		
	</entry>
	<entry>
		<id>https://marspedia.org/index.php?title=Recent_Liquid_Flow_on_Mars&amp;diff=14220&amp;oldid=prev</id>
		<title>Farred: tweak</title>
		<link rel="alternate" type="text/html" href="https://marspedia.org/index.php?title=Recent_Liquid_Flow_on_Mars&amp;diff=14220&amp;oldid=prev"/>
		<updated>2013-10-16T15:51:14Z</updated>

		<summary type="html">&lt;p&gt;tweak&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;
				&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 15:51, 16 October 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;== Recent liquid flow on Mars? ==  &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;== Recent liquid flow on Mars? ==  &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;Photographs of Hebes Chasma were recently published&amp;lt;ref&amp;gt;[http://spacefellowship.com/news/art35520/martian-scars.html &amp;quot;Martian scars&amp;quot; at SPACE FELLOWSHIP]&amp;lt;/ref&amp;gt; which show considerable resemblance to liquid flow features.  The dark stains seem to show something that &amp;quot;pool[ed] like spilt ink&amp;quot;.  Commentator(s) bent over backwards trying to not seem to be guilty of sensationalism.  The stains were suggested to be probably dust movement that produced a &amp;quot;flow-like feature&amp;quot;.  There is a possibility that wind can become heavily laden with dust and flow downwards to leave the dust collected in a broad flat pool, but the images in this case make that explanation seem unlikely.  The possibility of a petroleum seep suggests itself but the flow pattern that would result in the actual images is hard to imagine.  Perhaps some unknown gas of volcanic origin collected in Hebes Chasma and then condensed as dew on the surfaces that cooled the most by radiation.  This dew then slowly drained from those surfaces into inky pools in deep depressions in the eastern and central parts of Hebes Chasma.  If there is a liquid on Mars of petroleum nature, it could be an advantage for colonization efforts some day.   &lt;/div&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;Photographs of Hebes Chasma were recently published&amp;lt;ref&amp;gt;[http://spacefellowship.com/news/art35520/martian-scars.html &amp;quot;Martian scars&amp;quot; at SPACE FELLOWSHIP]&amp;lt;/ref&amp;gt; which show considerable resemblance to liquid flow features.  The dark stains seem to show something that &amp;quot;pool[ed] like spilt ink&amp;quot;.  Commentator(s) bent over backwards trying to not seem to be guilty of sensationalism.  The stains were suggested to be probably dust movement that produced a &amp;quot;flow-like feature&amp;quot;.  There is a possibility that wind can become heavily laden with dust and flow downwards to leave the dust collected in a broad flat pool, but the images in this case make that explanation seem unlikely.  The possibility of a petroleum seep suggests itself but the flow pattern that would result in the actual images is hard to imagine.  Perhaps some unknown &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;dense &lt;/ins&gt;gas of volcanic origin collected in Hebes Chasma and then condensed as dew on the surfaces that cooled the most by radiation.  This dew then slowly drained from those surfaces into inky pools in deep depressions in the eastern and central parts of Hebes Chasma.  If there is a liquid on Mars of petroleum nature, it could be an advantage for colonization efforts some day.   &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;   &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;   &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;== Reference ==  &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;== Reference ==  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key marspediaorg_www-mwmars_:diff::1.12:old-14205:rev-14220 --&gt;
&lt;/table&gt;</summary>
		<author><name>Farred</name></author>
		
	</entry>
	<entry>
		<id>https://marspedia.org/index.php?title=Recent_Liquid_Flow_on_Mars&amp;diff=14205&amp;oldid=prev</id>
		<title>Farred: Recent liquid flow on Mars?</title>
		<link rel="alternate" type="text/html" href="https://marspedia.org/index.php?title=Recent_Liquid_Flow_on_Mars&amp;diff=14205&amp;oldid=prev"/>
		<updated>2013-10-16T08:28:02Z</updated>

		<summary type="html">&lt;p&gt;Recent liquid flow on Mars?&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;== Recent liquid flow on Mars? == &lt;br /&gt;
Photographs of Hebes Chasma were recently published&amp;lt;ref&amp;gt;[http://spacefellowship.com/news/art35520/martian-scars.html &amp;quot;Martian scars&amp;quot; at SPACE FELLOWSHIP]&amp;lt;/ref&amp;gt; which show considerable resemblance to liquid flow features.  The dark stains seem to show something that &amp;quot;pool[ed] like spilt ink&amp;quot;.  Commentator(s) bent over backwards trying to not seem to be guilty of sensationalism.  The stains were suggested to be probably dust movement that produced a &amp;quot;flow-like feature&amp;quot;.  There is a possibility that wind can become heavily laden with dust and flow downwards to leave the dust collected in a broad flat pool, but the images in this case make that explanation seem unlikely.  The possibility of a petroleum seep suggests itself but the flow pattern that would result in the actual images is hard to imagine.  Perhaps some unknown gas of volcanic origin collected in Hebes Chasma and then condensed as dew on the surfaces that cooled the most by radiation.  This dew then slowly drained from those surfaces into inky pools in deep depressions in the eastern and central parts of Hebes Chasma.  If there is a liquid on Mars of petroleum nature, it could be an advantage for colonization efforts some day.  &lt;br /&gt;
 &lt;br /&gt;
== Reference == &lt;br /&gt;
&amp;lt;references/&amp;gt; &lt;br /&gt;
 &lt;br /&gt;
[[Category:Geology]]&lt;/div&gt;</summary>
		<author><name>Farred</name></author>
		
	</entry>
</feed>