Asteroids - 2/1 resonance and high eccentricity

Details Asteroids - 2/1 resonance and high eccentricity Asteroids - 2/1 resonance and high eccentricity

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993cemda..56..273m&link_type=abstract

Celestial Mechanics and Dynamical Astronomy (ISSN 0923-2958), vol. 56, no. 1-2, p. 273-276.

Astronomy and Astrophysics

Astronomy

1

Asteroids, Eccentric Orbits, Hamiltonian Functions, Orbital Resonances (Celestial Mechanics), Perturbation Theory, Solar Orbits, Jupiter (Planet), Resonant Frequencies, Saturn (Planet)

Scientific paper

Preliminary results of a systematic study of the dynamics in mean motion
resonances are reported for a case of a 2:1 resonance for the planar
restricted three-body problem of sun-Jupiter-asteroid. The study is
based on a seminumerical method of Henrard (1990).

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