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- W2024982016 abstract "Statistical cluster analysis of 635 individual bulk chemical compositions of lunar rocks distinguishes three major chemical groups which correspond respectively to highland rocks, high titanium mare basalts and mare basalts with moderate titanium contents. Petrochemical variations are plotted on “A-S” diagrams and on “any major oxide-S” diagrams, where A = Al2O3+CaO+Na2O+K2O and S = SiO2(FeO+MgO+MnO). Considering firstly the K2OS variations and the SiO2-MGO-and Al2O3S variations, eight chemical subgroups are distinguished in the lunar rocks. Each subgroup is defined by vatiation curves on chemical diagrams and on an Ol-An-Q ternary normative diagram. The petrogenetic meaning of these characteristic trends are discussed. Also, the similarities with or differences from terrestrial basic magmatism are demonstrated. The evidence for two different (continental and mare) early stages of crustal formation on the moon and terrestrial planets is emphasized and it is considered to be impossible to construct, at the present time, a single universal model for the formation of the earth's crust." @default.
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- W2024982016 date "1979-01-01" @default.
- W2024982016 modified "2023-09-27" @default.
- W2024982016 title "The main features of the geochemistry of lunar rocks" @default.
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- W2024982016 doi "https://doi.org/10.1016/0079-1946(79)90016-8" @default.
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