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Antarctic Lunar Meteorites from Cryptomaria of the Moon

T. Arai, Bernard Ray Hawke, T. A. Giguere

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Abstract

Mineralogical, geochemical, isotopic compositions and cosmic-ray exposure history, combined with the orbital data revealed that Antarctic lunar meteorites, Yamato-793169, Asuka-881757, Meteorites Hills 01210, and Miller Range 05035 represent the first ground truth of lunar cryptomaria, originated from the 3870 Ma-aged basalt flow buried beneath the floor of the Schickard crater on the nearside of the Moon.

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What this paper is about

Mineralogical, geochemical, isotopic compositions and cosmic-ray exposure history, combined with the orbital data revealed that Antarctic lunar meteorites, Yamato-793169, Asuka-881757, Meteorites Hills 01210, and Miller Range 05035 represent the first ground truth of lunar cryptomaria, originated from the 3870 Ma-aged basalt flow buried beneath the floor of the Schickard crater on the nearside of the Moon.

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Available abstract

Mineralogical, geochemical, isotopic compositions and cosmic-ray exposure history, combined with the orbital data revealed that Antarctic lunar meteorites, Yamato-793169, Asuka-881757, Meteorites Hills 01210, and Miller Range 05035 represent the first ground truth of lunar cryptomaria, originated from the 3870 Ma-aged basalt flow buried beneath the floor of the Schickard crater on the nearside of the Moon.

Key concepts: Meteorite, Basalt, Geology, Regolith, Impact crater, Lunar mare, Ejecta, Astrobiology

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