Combining Saturnian Craters and Kuiper Belt Observations to Build an Outer Solar System Impactor Size-Frequency Distribution

Details Combining Saturnian Craters and Kuiper Belt Observations to Build an Outer Solar System Impactor Size-Frequency Distribution Combining Saturnian Craters and Kuiper Belt Observations to Build an Outer Solar System Impactor Size-Frequency Distribution

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2669m&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2669

Physics

Scientific paper

Using Cassini mission imagery of the icy satellites of Saturn, numerical
simulations, and telescopic observation data we produce a model size
frequency distribution for outer solar system impactors spanning tens of
meters to thousands of kilometers.

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