Lunar Gravity Models: Large, Near Side Impact Basins

Details Lunar Gravity Models: Large, Near Side Impact Basins Lunar Gravity Models: Large, Near Side Impact Basins

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1995k&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1995

Physics

Scientific paper

Lunar mascon gravity highs and surrounding lows are generally due to
mare basalt fill, flanked by impact basin ejecta. Super-isostatic moho
uplift is important for some impact basins and is possibly due to
non-Newtonian lower crustal flow during the impact event.

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