A High-Temperature Al–Ca Condensate in the Lunar Regolith


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For the first time, a high-temperature condensate in the form of two-component glass beads of about 200–400 nm size, consisting of an Al–Ca oxide core rimmed by a uniform oxide film of high-silica glass containing iron nano-inclusions, has been found in natural samples of the lunar regolith from Mare Crisium (Luna-24). Earlier, a high-temperature condensate was only theoretically predicted on the basis of laser evaporation experiments.

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A. Mokhov

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)

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Email: avm8okhov@gmail.com
俄罗斯联邦, Moscow, 119017

T. Gornostaeva

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)

Email: avm8okhov@gmail.com
俄罗斯联邦, Moscow, 119017

P. Kartashov

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)

Email: avm8okhov@gmail.com
俄罗斯联邦, Moscow, 119017

A. Rybchuk

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)

Email: avm8okhov@gmail.com
俄罗斯联邦, Moscow, 119017

O. Bogatikov

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences (IGEM RAS)

Email: avm8okhov@gmail.com
俄罗斯联邦, Moscow, 119017

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