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- W2373896272 abstract "The detection of abundant olivine on Mars has led to hot debate over the history of water since olivine readily evolves to other minerals in the presence of water. Based on the experimental results, the hypothesis that early Mars may have had a methanol ocean has been published in Icarus. Olivine-rich basaltic materials are weathered in the laboratory under methanol-thermal conditions at temperatures of 80~160 ℃ and the alteration products are characterized. No additional secondary mineral phases are formed after methanol treatment, SEM images show physical weathering features. The experiment results presented here support the hypothesis that early Mars may have had a methanol ocean, suggesting that there has no substantial amount of liquid water on Mars since the formation of a large olivine deposits." @default.
- W2373896272 created "2016-06-24" @default.
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- W2373896272 date "2008-01-01" @default.
- W2373896272 modified "2023-09-25" @default.
- W2373896272 title "Laboratory-simulated Weathering of Olivine-rich Basalt in Methanol-thermal System: Implication for Early Martian Climate" @default.
- W2373896272 hasPublicationYear "2008" @default.
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