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Long term dynamical evolution of the Oort cloud comets: galactic and planetary perturbations
Published online by Cambridge University Press: 28 February 2005
Abstract
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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.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUC197 , August 2004 , pp. 335 - 340
- Copyright
- © 2005 International Astronomical Union
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