Tridimensional Dissipative Semi-Numerical Model

Details Tridimensional Dissipative Semi-Numerical Model Tridimensional Dissipative Semi-Numerical Model

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003em%26p...92...63j&link_type=abstract

Earth, Moon, and Planets, v. 92, Issue 1, p. 63-71 (2003).

Physics

Scientific paper

Our research combines mean motion resonances and dissipative forces in the averaged elliptic spatial restricted three-body problem. The models presented can be applied in many contexts mixing resonances and dissipations, e.g., asteroid belt, transneptunian region, exoplanets, systems of planetary rings, etc. We propose a semi-numerical model that simulates the behaviour of test particles under the effect of generic forces, functions of powers of the position and/or of the velocity. This model is valid for any orbital eccentricities or inclinations, even at high values. Captures around symmetric and asymmetric equilibria are reproduced and the apparitions of a plateau of inclination for long periods of time are dectected.

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