Impact Cratering on Porous Low-Density Bodies

Details Impact Cratering on Porous Low-Density Bodies Impact Cratering on Porous Low-Density Bodies

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1228h&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1228

Mathematics

1

Scientific paper

Impact experiments indicate that large craters on porous bodies form
primarily by compaction with little deposition of ejecta exterior to the
crater. This may explain the fact that large craters formed on Mathilde
without destroying nearby craters.

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