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: CH4 . 6H(2)o and/or CO2 . 6H(2)o.


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    Titel :

    On the possibilty of clathrate hydrates on the Moon


    Beteiligte:
    Duxbury, N. (Autor:in) / Nealson, K. (Autor:in) / Romanovsky, V. (Autor:in)


    Erscheinungsdatum :

    2000-11-01


    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch






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