Abstract Evolution of a system consisting of a great number of bodies that are gravitationally interacting and aggregating in contacts is considered. Body motions take place in the gravitational field of a central massive body (Sun or planet) in the same plane and at the initial time of system evolution orbits of all bodies are circular. It is shown that during evolution of the protoplanetary cloud, ring zones of matter rarefaction and condensation develop. Development of the condensation zones leads to the formation of planets, the most part of which acquire a direct rotation about their axes. In the case under consideration, approximate agreement between the law of planetary distances and that of geometric progression takes place as it is observed in planetary and satellite systems. The formation of the terrestrial planets and Jovian planets has been simulated. The principal numerical results have been obtained through digital simulation of planetary accumulation.


    Access

    Check access

    Check availability in my library

    Order at Subito €


    Export, share and cite



    Title :

    The problems of simulation of planetary systems accumulation processes


    Contributors:
    Eneev, T.M. (author) / Kozlov, N.N. (author)

    Published in:

    Publication date :

    1981-01-01


    Size :

    15 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



    Materials problems for planetary missions

    Moura, D. J. P. | British Library Online Contents | 1994


    Vehicle Planetary Gearbox Simulation

    Gajdosik Tomas / Brumercik Frantisek / Lukac Michal et al. | DOAJ | 2018

    Free access


    Planetary dune systems

    Bourke, Mary C. | TIBKAT | 2010


    Heatshielding problems of planetary entry - A review

    Park, Chul / Tauber, Michael | AIAA | 1999