Modeling of the Mantle Rebound for the Giant Impact Craters on Mars

Details Modeling of the Mantle Rebound for the Giant Impact Craters on Mars Modeling of the Mantle Rebound for the Giant Impact Craters on Mars

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1874f&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1874

Physics

Scientific paper

We assumed that large impact craters on Mars are axial symmetry with
respect to the basin center for topography and gravity, and calculated
mantle rebound model. In all large craters, the crustal thickness at the
center of the basin is quite thin.

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