Analysis of Processes of Iapetus' Terrain Darkening

Details Analysis of Processes of Iapetus' Terrain Darkening Analysis of Processes of Iapetus' Terrain Darkening

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1928g&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1928

Physics

Scientific paper

In images of the trailing side of Iapetus, dark crater bottoms are
common at low latitudes. The typical length of a drop-off in albedo is
below Cassini ISS' resolution limit. To determine the threshold
necessary for the process, we simulated different crater
characteristics.

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