Differences in the Mega-Regolith Depth Across the Moon's Southern Highlands

Details Differences in the Mega-Regolith Depth Across the Moon's Southern Highlands Differences in the Mega-Regolith Depth Across the Moon's Southern Highlands

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1240t&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

Differences in the frequencies of small (1-16 km diameter) radar-bright
craters is not uniform across the southeastern nearside lunar highlands
indicating a deeper megaregolith depth of 1 km associated with the South
Pole Aitken Basin ejecta.

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