The origin of ferroan and magnesian anorthosites in the lunar crust

【Author】

Zhu Dan;Zhang Mingming;Xu Yingkui;State Key Laboratory of Ore Deposit Geochemistry, Institute of Geochemistry, Chinese Academy of Sciences;Lunar and Planetary Science Research Center, Institute of Geochemistry, Chinese Academy of Sciences;

【Institution】

State Key Laboratory of Ore Deposit Geochemistry, Institute of Geochemistry, Chinese Academy of Sciences;Lunar and Planetary Science Research Center, Institute of Geochemistry, Chinese Academy of Sciences;

【Abstract】

<正>1 Introduction The widely accepted standard model for the lunar feldspathic crust is:the early Moon was wholly or mostly molten,forming Lunar Magma Ocean(LMO).Olivine and pyroxene crystallized first from that magma ocean and sank

【Keywords】

lunar;crust;magma;ocean;wholly;Lunar;crystallized;mostly;mantle;molten;

References

To explore the background and basis of the node document

Springer Journals Database

Total: 12 articles

  • [1] XU YingKui;LI XiongYao;ZHU Dan;WANG ShiJie;Lunar and Planetary Science Research Center,Institute of Geochemistry,Chinese Academy of Sciences;State Key Laboratory of Ore Deposit Geochemistry,Institute of Geochemistry,Chinese Academy of Sciences;State Key Laboratory of Environmental Geochemistry,Institute of Geochemistry,Chinese Academy of Sciences;, Evolution of lunar magma ocean and crust formation under initial conductive lid, Acta Petrologica Sinica,
  • [2] D. Walker;;S. E. DeLong, Soret separation of mid-ocean ridge basalt magma, Contributions to Mineralogy and Petrology,
  • [3] Frank M. Richter;;Yan Liang;;Andrew M. Davis, Isotope fractionation by diffusion in molten oxides, Geochimica et Cosmochimica Acta,
  • [4] Yang Chen;;Youxue Zhang, Olivine dissolution in basaltic melt, Geochimica et Cosmochimica Acta,

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