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- W2006435210 abstract "An hypothesis for mare basalt petrogenesis is presented. In the proposed model, both high- and low-Ti mare basalts are produced by partial melting and hybridization at depth accompanied by equilibrium between the hybrid liquids and the local olivine-pyroxenite residuum. The energy source for mare basalt formation is ultimately provided by radiogenic heating in the primordial lunar interior. The proposed dynamic model explains similarities in the Mg/(Mg+Fe) ratios and Cr2O3 contents of high-Ti and low-Ti basalts and avoids thermal problems inherent in previous models." @default.
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- W2006435210 date "1976-05-01" @default.
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- W2006435210 title "Mare basalt petrogenesis in a dynamic moon" @default.
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- W2006435210 doi "https://doi.org/10.1016/0012-821x(76)90241-7" @default.
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