Abstract T. C. Chamberlin suggested in 1897, on the basis of geological and climatological arguments, that the planets were formed by accretion of cold solid particles. With F. R. Moulton he developed convincing arguments against the Laplace nebular hypothesis and published a comprehensive ‘planetesimal theory’ of the origin of the solar system in 1905. The Chamberlin-Moulton theory has current as well as historical interest.


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    Titel :

    The origin of the planetesimal theory


    Beteiligte:

    Erschienen in:

    Erscheinungsdatum :

    1977




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Print


    Sprache :

    Englisch



    Klassifikation :

    Lokalklassifikation TIB:    535/3908/4290
    BKL:    44.71 Verkehrsmedizin



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