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- W2077813834 abstract "The basic thermal evolution model, described by Weizman et al. [1996], was modified to include the effect of phase transitions and the dependence of melting temperatures on pressure. The total amount of water release through Martian history was estimated from this model using the wet solidus of peridotite. Assuming a water content of 0.1% in the basalt, we find that the total amount of water released would be sufficient to cover the planet with a layer at least 3–300 m thick." @default.
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- W2077813834 date "1997-04-01" @default.
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- W2077813834 title "Phase transitions and melting in Mars" @default.
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- W2077813834 doi "https://doi.org/10.1029/96je03992" @default.
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