Identifying Martian Secondary Craters by Their Ejected Boulders

Details Identifying Martian Secondary Craters by Their Ejected Boulders Identifying Martian Secondary Craters by Their Ejected Boulders

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1461b&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

Bart and Melosh (2007) demonstrated that distant lunar secondary craters
could be distinguished from primary craters by the sizes of the largest
ejected boulders. The work presented in this abstract tests the validity
of that method for use on Mars.

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