Lunar Volcanism Induced by Heat Advected from the Lower Mantle: Results of 2D and 3D Mantle Convection Calculations

Details Lunar Volcanism Induced by Heat Advected from the Lower Mantle: Results of 2D and 3D Mantle Convection Calculations Lunar Volcanism Induced by Heat Advected from the Lower Mantle: Results of 2D and 3D Mantle Convection Calculations

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1768s&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1768

Physics

Scientific paper

Lunar thermal histories from 2d and 3d convection calculations are
presented that study the partial remelting of the magma ocean. The melt
zone forms at the likely source depth of the mare basalts and may exist
well into the Eratosthenian period.

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