Surface Runoff Features on Mars: Testing the Carbon Dioxide Formation Hypothesis

Details Surface Runoff Features on Mars: Testing the Carbon Dioxide Formation Hypothesis Surface Runoff Features on Mars: Testing the Carbon Dioxide Formation Hypothesis

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1780s&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1780

Computer Science

Scientific paper

We examine the hypothesis that carbon dioxide or clathrate formed the
recent Martian gullies, and conclude that it is unlikely, based on the
likely reservoirs and flow characteristics of these compounds.

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