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


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Resumo

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.

Sobre autores

A. Mokhov

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

Autor responsável pela correspondência
Email: avm8okhov@gmail.com
Rússia, Moscow, 119017

T. Gornostaeva

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

Email: avm8okhov@gmail.com
Rússia, Moscow, 119017

P. Kartashov

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

Email: avm8okhov@gmail.com
Rússia, Moscow, 119017

A. Rybchuk

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

Email: avm8okhov@gmail.com
Rússia, Moscow, 119017

O. Bogatikov

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

Email: avm8okhov@gmail.com
Rússia, Moscow, 119017

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