Geologic and Topographic Mapping of Tooting Crater, Mars, from HiRISE and CTX Data: Rim Slumping Controls the Distribution of Impact Melt, Pitted Terrain, Mudflows and Cavity Dewatering

Details Geologic and Topographic Mapping of Tooting Crater, Mars, from HiRISE and CTX Data: Rim Slumping Controls the Distribution of Impact Melt, Pitted Terrain, Mudflows and Cavity Dewatering Geologic and Topographic Mapping of Tooting Crater, Mars, from HiRISE and CTX Data: Rim Slumping Controls the Distribution of Impact Melt, Pitted Terrain, Mudflows and Cavity Dewatering

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1497m&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1497

Physics

Scientific paper

CTX and HiRISE data of Tooting crater, Mars, reveal a strong link
between ejecta volume, rim slumping, and the distribution of pitted
terrain and floor fractures. Tooting provides a benchmark against which
fresh large craters on Mars can be studied.

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