GRAIL, LLR, and LOLA constraints on the interior structure of the Moon

GRAIL, LLR, and LOLA constraints on the interior structure of the Moon

The interior structure of the Moon is constrained by its mass, moment of inertia, and k(2) and h(2) tidal Love numbers. We infer the likely radius, density, and (elastic limit) rigidity of all interior layers by solving the inverse problem using these observational constraints assuming spherical sym...

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Bibliographic Details
Main Authors: Matsuyama, Isamu, Nimmo, Francis, Keane, James T., Chan, Ngai H., Taylor, G. Jeffrey, Wieczorek, Mark A., Kiefer, Walter S., Williams, James G.
Other Authors: Univ Arizona, Dept Planetary Sci, Lunar & Planetary Lab
Language:en
Published: GEOPHYSICAL RESEARCH LETTERS 2016
Subjects:
lunar interior
Online Access:http://hdl.handle.net/10150/621595
http://arizona.openrepository.com/arizona/handle/10150/621595

Internet

http://hdl.handle.net/10150/621595
http://arizona.openrepository.com/arizona/handle/10150/621595

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