Mar 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1756m&link_type=abstract
35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1756
Physics
1
Scientific paper
The youngest terrains on Mars could be older than previously believed
because impact craters smaller than ~250 m are largely secondaries and
lunar-derived production functions predict far too many small primary
craters.
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