Exploring the Lunar Interior with Tides, Gravity and Orientation

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Exploration of the internal structure and properties of the Moon continues. Existing information from gravity field, tides and 3-dimensional orientation includes moments of inertia, mean density, tidal Love numbers, tidal dissipation, and fluid-core/solid-mantle interactions from dissipation and oblateness. Tracking orbiting spacecraft gives gravity field and a Love number k2. Lunar laser ranging (LLR) determined tides and orientation give Love numbers k2 and h2, four tidal dissipation and two fluid-core/solid-mantle effects. Spacecraft gravity and LLR combined give the moment of inertia of the solid Moon, currently estimated to be 0.3929 MR2. The detections of the two core/mantle boundary effects require a fluid core. Love numbers are becoming accurate enough to constrain deep interior models for fluid core and deepest mantle. Future possibilities include (LLR) determination of the fluid core moment and a (GRAIL and LLR) search for a solid inner core. Interior explorations would be much expanded by a network of geophysical landers.

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