On the assumption that the vast majority of craters are of impact origin, relative age dates can be obtained by counting craters. Returned lunar samples are helping to resolve problems regarding the magnitude of the meteoritic flux. The samples provide a means for empirically calibrating crater count data. The characteristics of the Taurus-Littrow area are considered, giving attention to four different units. The crater frequency distribution is discussed, together with its significance for the age of the corresponding lunar features.


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    Titel :

    Crater frequency age determinations for the proposed Apollo 17 site at Taurus-Littrow.


    Beteiligte:
    Greeley, R. (Autor:in) / Gault, D. E. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    01.02.1973


    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Apollo 17: At Taurus Littrow

    Anderton, D. A. | NTRS | 1973


    Apollo 17: At Taurus Littrow

    D. A. Anderton | NTIS | 1973


    APOLLO 17 Mare Basalts: Serenely Sampling Taurus-Littrow

    C. R. Neal / L. A. Taylor | NTIS | 1992


    The Apollo 17 mare basalts: Serenely sampling Taurus-Littrow

    Neal, Clive R. / Taylor, Lawrence A. | NTRS | 1992