Martian Surface Properties: Inferences from Resolved Differences in Crater Geometries

Details Martian Surface Properties: Inferences from Resolved Differences in Crater Geometries Martian Surface Properties: Inferences from Resolved Differences in Crater Geometries

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1293v&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1293

Computer Science

1

Scientific paper

We find large differences in geometry between fresh crater populations
in Utopia and Lunae Pl. Crater cavities and ejecta volumes in Utopia are
significantly larger, probably due to different composition or
subsurface structure in the two terrains.

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