Constraints of the Density and Porosity of the Lunar Highlands Crust from Gravity and Topography

Details Constraints of the Density and Porosity of the Lunar Highlands Crust from Gravity and Topography Constraints of the Density and Porosity of the Lunar Highlands Crust from Gravity and Topography

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1879h&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1879

Physics

1

Scientific paper

In order to estimate the bulk density of the upper crust, localized
spectral analysis has been applied to several highland regions on the
Moon. Combined with pore-free density from geochemistry, porosity of the
upper crust is implied to be 2-3%.

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