Small Primaries Versus Large Secondaries on Mars -- Numerical Approach

Details Small Primaries Versus Large Secondaries on Mars -- Numerical Approach Small Primaries Versus Large Secondaries on Mars -- Numerical Approach

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1589a&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1589

Computer Science

1

Scientific paper

Using numerical simulations we compare crater strewn fields created by a
disrupted and dispersed projectile with distal secondary craters formed
by high-velocity ejecta from 10-km-diameter Zunil crater.

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