An experiment using Earth based remote sensing radar, infrared eclipse, and color difference data to deduce surface properties not visible in Apollo photography is reported. The Earth based data provided information on the small scale (centimeter sized) blockiness and on the surface chemical composition (titanium and iron contents) of the lunar surface. These deduced surface properties complemented the new Apollo photography, leading to refined geologic interpretations of the lunar surface.


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    Titel :

    Apollo experiment S-217 IR/radar study of Apollo data


    Beteiligte:
    Thompson, T. W. (Autor:in) / Moore, H. J. (Autor:in) / Schaber, G. G. (Autor:in) / Shorthill, R. W. (Autor:in) / Whitaker, E. A. (Autor:in) / Zisk, S. H. (Autor:in)

    Erscheinungsdatum :

    01.10.1976


    Medientyp :

    Report


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Apollo Experiment S-217 IR/Radar Study of APOLLO Data

    T. W. Thompson / H. J. Moore / G. G. Schaber et al. | NTIS | 1976


    APOLLO Entry Radar Acquistion Study

    J. R. Moore | NTIS | 1965


    Apollo entry radar acquistion study

    Moore, J. R. | NTRS | 1965


    Radar observations of Apollo

    Goldstein, R. M. / Jurgens, R. F. / Yeomans, D. K. | NTRS | 1981


    Apollo window meteoroid experiment

    Cour-Palais, B. G. / Brown, M. L. / Mckay, D. S. | NTRS | 1972