Long term dynamical evolution of the Oort cloud comets: galactic and planetary perturbations

Details Long term dynamical evolution of the Oort cloud comets: galactic and planetary perturbations Long term dynamical evolution of the Oort cloud comets: galactic and planetary perturbations

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005dpps.conf..335d&link_type=abstract

Dynamics of Populations of Planetary Systems, Proceedings of IAU Colloquium #197, held 31 August - 4 Spetember, 2004 in Belgrade

Physics

Comets: General, Oort Cloud.

Scientific paper

The source of long-period comets can be numerically modeled by means of Monte Carlo simulation of the Oort cloud dynamics. Tracing a comet motion under the galactic perturbations over a long time interval requires taking into account of planetary perturbations. A method for the approximate treating of the planetary perturbations in such simulations is described. Some peculiarities found in planetary action on long-period simulated cometary sample are also discussed.

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