Constraints on the Impact Process from Observations of Oblique Impacts on the Terrestrial Planets

Details Constraints on the Impact Process from Observations of Oblique Impacts on the Terrestrial Planets Constraints on the Impact Process from Observations of Oblique Impacts on the Terrestrial Planets

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icbg.conf...31h&link_type=abstract

Impact Cratering: Bridging the Gap Between Modeling and Observations, February 7-9, 2003. LPI Contribution No. 1155. Houston,

Mathematics

Craters, Mathematical Models, Terrestrial Planets, Impact, Cratering, Mars (Planet), Moon, Venus (Planet)

Scientific paper

Recently there have been significant advances in both experimental and numerical modeling techniques that hold promise for providing details on how the cratering process is affected by impact at a non-vertical angle. Anecdotal observations of craters on the terrestrial planets validated initial experimental efforts. Recent and ongoing systematic characterizations of craters resulting from oblique impact on the Moon, Mars, and Venus provide important constraints for the detailed modeling efforts currently being conducted.

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