Data on terrestrial eruptions of pyroclastic material and ballistic considerations suggest that in the lunar environment (vacuum and reduced gravity) low-rimmed pyroclastic rings are formed rather than the high-rimmed cinder cones so abundant on the earth. Dark blanketing deposits in the Taurus-Littrow region (Apollo 17 landing area) are interpreted as being at least partly composed of lunar counterparts of terrestrial cinder cones.


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    Titel :

    Lunar cinder cones.


    Beteiligte:
    Mcgetchin, T. R. (Autor:in) / Head, J. W. (Autor:in)

    Erschienen in:

    Science ; 180


    Erscheinungsdatum :

    06.04.1973


    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


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