Numerical Modeling of Impact Cratering on Titan with Implications for the Age of Titan's Surface

Details Numerical Modeling of Impact Cratering on Titan with Implications for the Age of Titan's Surface Numerical Modeling of Impact Cratering on Titan with Implications for the Age of Titan's Surface

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1504l&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1504

Mathematics

Logic

6

Scientific paper

Results reported from the first two Cassini flybys of Titan reveal few
if any impact craters, suggesting that geological or atmospheric
processes, or both, have worked to prevent the formation of craters or
to hide or erase them after formation. Here we quantify some of these
processes.

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