Eskolaite in the regolith of the Taurus-Littrow Valley


Дәйексөз келтіру

Толық мәтін

Ашық рұқсат Ашық рұқсат
Рұқсат жабық Рұқсат берілді
Рұқсат жабық Тек жазылушылар үшін

Аннотация

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.

Авторлар туралы

A. Mokhov

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

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

A. Rybchuk

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

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

P. Kartashov

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

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

T. Gornostaeva

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

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

O. Bogatikov

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

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

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