Thicknesses of Lunar Mare Flow Units: A New Investigation Based on Crater Size-Frequency Distribution Measurements

Details Thicknesses of Lunar Mare Flow Units: A New Investigation Based on Crater Size-Frequency Distribution Measurements Thicknesses of Lunar Mare Flow Units: A New Investigation Based on Crater Size-Frequency Distribution Measurements

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1065h&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1065

Physics

Scientific paper

We used crater size-frequency distribution measurements in order to
estimate the thickness and the volume of flow units in several nearside
basins. We found that thicknesses of flow units are on the order of
30-60 m and volumes are about 590-940 km3.

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