Abundance, Distribution, and Isotopic Composition of Water in the Moon as Revealed by Basaltic Lunar Meteorites
نویسندگان
چکیده
Introduction: Lunar meteorites arguably provide a wider sampling of the lunar surface compared to the samples collected during the Apollo and Luna Missions. Apatite is the main hydroxyl-bearing (proxy for water) mineral in lunar samples, especially in basaltic rocks. The ages of lunar basaltic meteorites also span a larger range compared to basaltic samples collected during Apollo and Luna missions. Thus, by determining the H-content and the H isotopic composition of apatites from lunar basaltic meteorites of different ages it is possible to investigate the abundance, distribution and isotopic composition of water in the lunar interior.
منابع مشابه
Tracking secular changes in the “water” content of lunar interior using basaltic lunar meteorites
Lunar meteorites provide a wider sampling of the lunar surface compared to the samples collected during the Apollo and Luna Missions. Apatite is the main hydroxyl-bearing (proxy for water) mineral in lunar samples, especially in basaltic rocks. Apatite is also amenable to in-situ U-Pb age dating studies. The ages of lunar basaltic meteorites also span over a larger range compared to basaltic sa...
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