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

@article{Matsuyama2016GRAILLA,
  title={GRAIL, LLR, and LOLA constraints on the interior structure of the Moon},
  author={Isamu Matsuyama and Francis Nimmo and James Tuttle Keane and Ngai Ham Chan and G. Jeffrey Taylor and Mark A. Wieczorek and Walter S. Kiefer and James G. Williams},
  journal={Geophysical Research Letters},
  year={2016},
  volume={43},
  pages={8365 - 8375}
}
The interior structure of the Moon is constrained by its mass, moment of inertia, and k2 and h2 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 symmetry. Our results do not favor the presence of a low rigidity transition layer between a liquid outer core and mantle. If a transition layer exists, its rigidity is constrained to 43−9+26 GPa, with a… 

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