Determining the Main Belt Size Distribution Using Asteroid Crater Records and Crater Saturation Models

Details Determining the Main Belt Size Distribution Using Asteroid Crater Records and Crater Saturation Models Determining the Main Belt Size Distribution Using Asteroid Crater Records and Crater Saturation Models

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1349b&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1349

Mathematics

4

Scientific paper

Craters on Eros, Ida and Mathilde were formed by a shallow main belt
size distribution (SD) w/differential q ~ -3.5. The steep crater SD on
Gaspra was the by-product of a recent event and does not represent
time-averaged main belt conditions.

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