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• W2034196372 abstract "Ion microprobe studies of hydrous amphibole, biotite, and apatite in shergottite-nakhlite-chassignite (SNC) meteorites, probable igneous rocks from Mars, indicate high deuterium/hydrogen (D/H) ratios relative to terrestrial values. The amphiboles contain roughly one-tentn as much water as expected, suggesting that SNC magmas were less hydrous than previously proposed. The high but variable D/H values of these minerals are best explained by postcrystallization D enrichment of initially D-poor phases by martian crustal fluids with near atmospheric D/H (about five times the terrestrial value). These igneous phases do not directly reflect the D/H ratios of martian magmatic water but provide evidence for a D-enriched martian crustal water reservoir." @default.
• W2034196372 created "2016-06-24" @default.
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• W2034196372 date "1994-07-01" @default.
• W2034196372 modified "2023-09-24" @default.
• W2034196372 title "Water on Mars: Clues from Deuterium/Hydrogen and Water Contents of Hydrous Phases in SNC Meteorites" @default.
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• W2034196372 doi "https://doi.org/10.1126/science.265.5168.86" @default.
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