The general features of a new numerical simulation of planetesimal accretion which models multiple heliocentric distance zones, together with a detailed model for the planetesimal size and orbital distribution in each zone, are described. A restricted version of this model which allows only a single heliocentric distance zone has been used to test the validity of the code by comparing with results from earlier authors when the same physical phenomena are included. Generally, very good agreement is found.


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    Titel :

    Multizone accretional evolution of planetesimal swarms


    Beteiligte:
    Spaute, D. (Autor:in) / Davis, D. R. (Autor:in) / Weidenschilling, S. J. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1990-01-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Multizone accretional evolution of planetesimal swarms

    Spaute, D. / Davis, D.R. / Weidenschilling, S.J. | Elsevier | 1989


    Accretional heating of the satellites of Saturn and Uranus

    Squyres, Steven W. / Reynolds, Ray T. / Summers, Audrey L. et al. | NTRS | 1987


    Programmable Multizone Furnace

    Ting, Edmund Y. / Larson, David J., Jr. | NTRS | 1990


    Thermal History of the Moon: Implications for an Early Core Dynamo and Post-accretional Magmatism

    Konrad, W. / Spohn, T. / International Council of Scientific Unions; Committee on Space Research; Scientific Commission B | British Library Conference Proceedings | 1997


    DÉTECTEUR ROUTIER PIÉZOÉLECTRIQUE MULTIZONE

    ZEIDAN MARWAN / POQUE MATHIEU / RAMOND ALAIN et al. | Europäisches Patentamt | 2015

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