Coagulation of grains in the solar nebula should result in formation of low-density aggregates with fractal structure. The opacity of the nebula remains much higher than computed for the assumption that particles are compact. Timescales for particle growth, settling to the central plane of the nebula, and formation of planetesimals are lengthened significantly.


    Zugriff

    Zugriff über TIB

    Verfügbarkeit in meiner Bibliothek prüfen


    Exportieren, teilen und zitieren



    Titel :

    Early stages of accumulation in the solar nebula


    Beteiligte:

    Erschienen in:

    Erscheinungsdatum :

    1990-01-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Early stages of accumulation in the solar nebula

    Weidenschilling, S.J. | Elsevier | 1989


    Shock Processing of Interstellar Nitrogen Compounds in the Solar Nebula

    Kress, M. E. / Desch, S. J. / Dateo, C. E. et al. | British Library Conference Proceedings | 2002


    Solar thermal upper stages

    Calabro, M. | IEEE | 2003



    Dynamic Positioning in Early Design Stages

    Lübcke, A. / Krüger, S. | TIBKAT | 2014