Voyager 2 images of Miranda revealed a significant history of geological activity. Overlying an apparently ancient cratered terrain are assemblages of concentric ridges, scarps, and dark banded material. The problems that evolutionary thermal and structural modes of Miranda must face, to provide a convincing explanation for such topographic complexity, are examined.


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    Titel :

    The viscosity of Miranda


    Beteiligte:
    Thomas, P. J. (Autor:in) / Reynolds, R. T. (Autor:in) / Squyres, S. W. (Autor:in) / Cassen, P. M. (Autor:in)


    Erscheinungsdatum :

    1987-05-01


    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch




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