Radiation-Thermal Effects in the Lunar Meteorites EET87521 and MAC88105 by the Track and Thermoluminescence Data in the Olivine Crystals

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Meteorites: Lunar, Olivine, Thermoluminescence, Tracks: Vh-Nuclei

Scientific paper

The study of lunar meteorites contributes essential data about radiation history of matter on the lunar surface and shock thermal effects due to impact ejection from the Moon. We report further results from our fossil track and thermoluminescence (TL) analyses on the olivine grain samples extracted from the two lunar meteorites EET87521 and MAC88105, the matrix chips of which (~0.1 g) were obtained from the meteoritic group of the NASA Cosmic Center. The first meteorite is a mixture of mare and highlands components (ratio about 2:1) and second ones is a regolith breccia from the lunar highlands.

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