Eskolaite in the regolith of the Taurus-Littrow Valley


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Eskolaite crystals were discovered in the course of Scanning Electron Microscopy (SEM) studies of the regolith sample, which was delivered from the continental area between Serenitatis and Tranquilitatis Maria during the Apollo 17 mission. The finding was compared with an analogue sampled from Mare Crisium (Luna 24 mission). A condensate-impact origin of eskolaite is assumed for both findings. It was demonstrated that the eskolaite of the Apollo 17 probe is genetically and morphologically identical to the eskolaite from the Luna 24 probes.

作者简介

A. Mokhov

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

编辑信件的主要联系方式.
Email: avm8okhov@gmail.com
俄罗斯联邦, Moscow, 119017

A. Rybchuk

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

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

P. Kartashov

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

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

T. Gornostaeva

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

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

O. Bogatikov

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

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

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