Fluvial Processes Modifications of the Impact Craters in the Greater Hellas Region, Mars

Details Fluvial Processes Modifications of the Impact Craters in the Greater Hellas Region, Mars Fluvial Processes Modifications of the Impact Craters in the Greater Hellas Region, Mars

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1538a&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1538

Mathematics

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Scientific paper

The appearance of Martian impact craters is due to a number of pre- and
post-impact factors. The changes in their appearance may provide
information on the local surface geology and on the whole post-impact
geological evolution of the area studied.

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