Shape, Topography and Roughness of 433 Eros

Details Shape, Topography and Roughness of 433 Eros Shape, Topography and Roughness of 433 Eros

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1522c&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1522

Physics

Scientific paper

A global topographic map of Eros shows that Himeros and Shoemaker Region
are giant craters. The slope distributions as inferred from tracks and
as inferred from surface elements are distinct, and the former is
Gaussian at small slopes.

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