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. Author manuscript; available in PMC: 2019 Aug 14.
Published in final edited form as: Science. 2012 Dec 5;339(6120):671–675. doi: 10.1126/science.1231530

Fig. 3.

Fig. 3.

Crustal thickness of the Moon from GRAIL gravity and Lunar Reconnaissance Orbiter topography. With a crustal porosity of 12% and a mantle density of 3220 kg m−3, the minimum crustal thickness is less than 1 km in the interior of the farside basin Moscoviense, and the thickness at the Apollo 12 and 14 landing sites is 30 km. Image format the same as in Fig. 1, and each image is overlain by a shaded relief map derived from the surface topography.