Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983m%26p....28...69r&link_type=abstract
Moon and the Planets (ISSN 0165-0807), vol. 28, Feb. 1983, p. 69-86. Research supported by the Centre National de la Recherche S
Astronomy and Astrophysics
Astronomy
11
Astronomical Models, Kepler Laws, Orbit Perturbation, Solar System, Three Body Problem, Comets, Dynamic Models, Jupiter (Planet), Monte Carlo Method, Planets, Sun
Scientific paper
A new and fast method to estimate perturbations by a planet on cometary orbits is developed. This method makes it possible to identify accurately the cases of large perturbations in a set of fictitious orbits. Hence, it can be used in constructing perturbation samples for Monte Carlo simulations in order to maximize the amount of information. Furthermore, the estimated perturbations are found to yield a good approximation to the real perturbation sample. This is shown by a comparison of the perturbations obtained by the new estimator with the results of numerical integration of regularized equations of motion for the same orbits in the same dynamical model: the three-dimensional elliptic restricted three-body problem (sun-Jupiter-comet).
Froeschle Cl.
Rickman Hans
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