The search for lunar mantle rocks exposed on the surface of the Moon

被引:40
|
作者
Moriarty, Daniel P., III [1 ,2 ]
Dygert, Nick [3 ]
Valencia, Sarah N. [1 ,2 ]
Watkins, Ryan N. [4 ]
Petro, Noah E. [1 ]
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Univ Maryland, College Pk, MD 20742 USA
[3] Univ Tennessee, Dept Earth & Planetary Sci, Knoxville, TN USA
[4] Planetary Sci Inst, Tucson, AZ USA
关键词
POLE-AITKEN BASIN; MAGMA OCEAN; FRACTIONAL CRYSTALLIZATION; THERMAL EVOLUTION; ORIGIN; DIFFERENTIATION; CRUST; PETROGENESIS; OVERTURN; FARSIDE;
D O I
10.1038/s41467-021-24626-3
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
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.
引用
收藏
页数:11
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