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


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Аннотация

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.

Авторлар туралы

A. Mokhov

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

Хат алмасуға жауапты Автор.
Email: avm8okhov@gmail.com
Ресей, Moscow, 119017

T. Gornostaeva

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

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

P. Kartashov

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

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

A. Rybchuk

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

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

O. Bogatikov

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

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

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