Large-Scale Topographic Roughness of Terrestrial Planets: A Comparison

Details Large-Scale Topographic Roughness of Terrestrial Planets: A Comparison Large-Scale Topographic Roughness of Terrestrial Planets: A Comparison

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1472k&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Computer Science

1

Scientific paper

We compare topographic roughness of typical terrains on Mercury, Venus,
the Earth, the Moon, and Mars at the spatial scales from 30 to 200 km.
We specifically discuss differences in heavily cratered terrains on the
Moon, Mercury and Mars.

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