Small Crater Morphology Within Gusev Crater and Isidis Planitia: Evidence for Widespread Secondaries on Mars

Details Small Crater Morphology Within Gusev Crater and Isidis Planitia: Evidence for Widespread Secondaries on Mars Small Crater Morphology Within Gusev Crater and Isidis Planitia: Evidence for Widespread Secondaries on Mars

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.2068h&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.2068

Physics

4

Scientific paper

Through the use of digital elevation models created from
stereogrammetry, we determined the diameter, rim height, and crater
depth of small (<1 km) craters on the martian surface. The morphology
of these craters suggests that they are secondaries.

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