Small crater clasters: Findings from HiRise

Details Small crater clasters: Findings from HiRise Small crater clasters: Findings from HiRise

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008epsc.conf..340i&link_type=abstract

European Planetary Science Congress 2008, Proceedings of the conference held 21-25 September, 2008 in Münster, Germany. Online a

Physics

Scientific paper

Abstract Due to the small density of the atmosphere on Mars, the size of clusters controlled by lateral motion of fragments is about 10 to n×100 meters. The HiRISE image scale of 0.25-0.32 meters per pixel allows us for the first time to resolve details of small crater fields on Mars. The presentation demonstrates new primary data and a set of models aimed to interpret data in terms of density and strength of small bodies impacted Mars nowadays.

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