The influence of the orbital eccentricity of a primary on the chaotic region

Details The influence of the orbital eccentricity of a primary on the chaotic region The influence of the orbital eccentricity of a primary on the chaotic region

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991acasn..32..222l&link_type=abstract

(Acta Astronomica Sinica, vol. 32, no. 2, 1991, p. 222-224) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 15, Dec. 1

Astronomy and Astrophysics

Astrophysics

Chaos, Eccentric Orbits, Orbital Resonances (Celestial Mechanics), Three Body Problem, Astronomical Models, Eccentricity

Scientific paper

The influence of the orbital eccentricity of a perturbing body (ep) on the chaotic region is investigated by applying the theory of resonance overlap to the elliptic restricted three-body model. Results of the analysis show that, the orbital (ep) increases the size of the chaotic region, confirming the conjecture of Duncan et al. (1988). This finding is helpful in overcoming the difficulty encountered in the choice of the 'feeding zone' in numerical simulations of the formation of the solar system (Wetherill, 1980).

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