Orientation and Distribution of Recent Gullies in the Southern Hemisphere of Mars: Observations from HRSC/MEX and MOC/MGS Data

Details Orientation and Distribution of Recent Gullies in the Southern Hemisphere of Mars: Observations from HRSC/MEX and MOC/MGS Data Orientation and Distribution of Recent Gullies in the Southern Hemisphere of Mars: Observations from HRSC/MEX and MOC/MGS Data

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1610b&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1610

Physics

Scientific paper

MOC and HRSC data reveal martian gullies form most commonly on pole
facing slopes in the mid latitudes. Impact crater walls are the most
common setting for gullies but many are found on isolated knobs and
hills. Lengths up to ~7 km have been observed.

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