Structural state of native molybdenum in the lunar regolith


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Abstract

The structural state was determined for zero-valence molybdenum in the lunar regolith. The body- and face-centered molybdenum forms (BCC and FCC, respectively) were identified. Disruption of the structure down to complete amorphization was noted. This might be caused by the long-term influence of the solar wind.

About the authors

A. V. Mokhov

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry

Author for correspondence.
Email: avm8okhov@gmail.com
Russian Federation, Staromonetny per. 35, Moscow, 119017

T. A. Gornostaeva

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry

Email: avm8okhov@gmail.com
Russian Federation, Staromonetny per. 35, Moscow, 119017

P. M. Kartashov

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry

Email: avm8okhov@gmail.com
Russian Federation, Staromonetny per. 35, Moscow, 119017

O. A. Bogatikov

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry

Email: avm8okhov@gmail.com
Russian Federation, Staromonetny per. 35, Moscow, 119017

O. A. Sakharov

National Research University of Electronic Technology

Email: avm8okhov@gmail.com
Russian Federation, Moscow

N. V. Trubkin

Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry

Email: avm8okhov@gmail.com
Russian Federation, Staromonetny per. 35, Moscow, 119017


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