An improved gravity model from Doppler tracking of the Lunar Prospecto
r (LP) spacecraft reveals three new Large mass concentrations (mascons
) on the nearside of the moon beneath the impact basins Mare Humboltia
num, Mendel-Ryberg, and Schiller-Zucchius, where the Latter basin has
no visible mare fill. Although there is no direct measurement of the L
unar farside gravity, LP partially resolves four mascons in the Large
farside basins of Hertzsprung, Coulomb-Sarton, Freundlich-Sharonov, an
d Mare Moscoviense. The center of each of these basins contains a grav
ity maximum relative to the surrounding basin. The improved normalized
polar moment of inertia (0.3932 +/- 0.0002) is consistent with an iro
n core with a radius of 220 to 450 kilometers.