Martian Gullies: Morphologies and Possible Processes in their Formation

Details Martian Gullies: Morphologies and Possible Processes in their Formation Martian Gullies: Morphologies and Possible Processes in their Formation

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1331c&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1331

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Martian gullies are often morphologically similar to terrestrial gullies
and also appear young. The current environment on Mars does not support
liquid water. Several processes may have been involved in their
formation. At least some gullies were formed by dry mass wasting.

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