期刊
NATURE COMMUNICATIONS
卷 12, 期 1, 页码 -出版社
NATURE PORTFOLIO
DOI: 10.1038/s41467-021-24626-3
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资金
- University of Maryland [80GSFC21M0002]
- NASA
The lunar surface holds ancient and well-preserved records of Solar System history and planetary evolution processes. There is debate among scientists about the lithologies of the upper lunar mantle and where they may be exposed on the surface. By reviewing dynamical models and recent data, researchers are assessing candidate lithologies and their implications for lunar evolution.
The lunar surface is ancient and well-preserved, recording Solar System history and planetary evolution processes. Ancient basin-scale impacts excavated lunar mantle rocks, which are expected to remain present on the surface. Sampling these rocks would provide insight into fundamental planetary processes, including differentiation and magmatic evolution. There is contention among lunar scientists as to what lithologies make up the upper lunar mantle, and where they may have been exposed on the surface. We review dynamical models of lunar differentiation in the context of recent experiments and spacecraft data, assessing candidate lithologies, their distribution, and implications for lunar evolution.
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