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- W2076283947 abstract "One of the most important inferences of the Lunar Prospector mission data was the existence of subsurface water ice in the permanently shadowed craters near both lunar poles [ Feldman et al. , 1998]. We propose and substantiate an alternative explanation that hydrogen can exist in the shallow lunar subsurface in the form of clathrate hydrates: CH 4 · 6H 2 O and/or CO 2 · 6H 2 O." @default.
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- W2076283947 date "2001-11-01" @default.
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- W2076283947 title "On the possibility of clathrate hydrates on the Moon" @default.
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- W2076283947 doi "https://doi.org/10.1029/2000je001425" @default.
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