Gravity Constraints on the Subsurface Structure of the Marius Hills: A Sharper View of the Magmatic Pluming System Based on Improved Topography Data and New Lunar Density Measurements

Details Gravity Constraints on the Subsurface Structure of the Marius Hills: A Sharper View of the Magmatic Pluming System Based on Improved Topography Data and New Lunar Density Measurements Gravity Constraints on the Subsurface Structure of the Marius Hills: A Sharper View of the Magmatic Pluming System Based on Improved Topography Data and New Lunar Density Measurements

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1274k&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1274

Physics

1

Scientific paper

Gravity observations require the presence of a thick, high density
batholith beneath much of the Marius Hills. The likely cause is basalt
that has flooded the pore space within the brecciated anorthosite crust.

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