Introduction
The lunar crust provides a record of the planetary formation and early evolutionary processes and contains a wealth of information about the origin and evolution of the Earth-Moon system (e.g., Taylor 1982; NRC 2007; Canup 2008, 2012; Cuk and Stewart 2012; Young et al. 2016). Understanding these processes is crucial for the reconstruction of the early evolutionary stages of the Earth, e.g., the early geological evolution of a terrestrial planet, inner Solar System impact bombardment, and the solar and galactic environment throughout the last 4.5 billion years (Ga) (e.g., NRC 2007; Crawford et al. 2012).
Our knowledge of the lunar highland crust has advanced enormously. Studies of lunar meteorites; experimental and computational studies; remote sensing of mineralogy, chemistry, and topography of the lunar surface; new gravity data; geochronology; geochemistry, especially isotopic constraints; and the abundances and source reservoirs of lunar volatiles have brought, and...
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Acknowledgments
JG acknowledges NASA grant NNX15AU25G; KHJ acknowledges STFC Grant ST/M001253/1 and Royal Society grant RS/UF140190. Some of the material used was modified from text presented in K. Joy’s Ph.D. thesis (Joy 2007), for which she thanks Ian Crawford for his help and support.
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Gross, J., Joy, K.H. (2016). Evolution, Lunar: From Magma Ocean to Crust Formation. In: Cudnik, B. (eds) Encyclopedia of Lunar Science. Springer, Cham. https://doi.org/10.1007/978-3-319-05546-6_39-1
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