A shallow (<100 km) ilmenite-bearing pyroxenitic source for young lunar volcanism

Author:

Wang ChengyuanORCID,Xu Yi-GangORCID,Zhang Le,Chen ZhimingORCID,Xia XiaopingORCID,Lin MangORCID,Guo Feng

Funder

Guangzhou Institute of Geochemistry

China National Space Administration

Chinese Academy of Sciences

Publisher

Elsevier BV

Reference67 articles.

1. Olivine-melt and orthopyroxene-melt equilibria;Beattie;Contribut. Mineral. Petrol.,1993

2. Parameterization of the Fe= Mg exchange coefficient (Kd) between clinopyroxene and silicate melts;Bédard;Chem. Geol.,2010

3. Mechanisms for incompatible-element enrichment on the Moon deduced from the lunar basaltic meteorite Northwest Africa 032;Borg;Geochim. Cosmochim. Acta,2009

4. Timing of mantle overturn during magma ocean solidification;Boukaré;Earth Planet. Sci. Lett.,2018

5. Analysis of lunar samples: implications for planet formation and evolution;Carlson;Science (1979),2019

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