The characteristics of the phase trajectories of asteroids in the case of first-order commensurabilities

Details The characteristics of the phase trajectories of asteroids in the case of first-order commensurabilities The characteristics of the phase trajectories of asteroids in the case of first-order commensurabilities

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65.1086g&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Sept.-Oct. 1988, p. 1086-1093. In Russian.

Astronomy and Astrophysics

Astronomy

Asteroids, Celestial Mechanics, Three Body Problem, Trajectory Analysis, Eccentric Orbits, Extremum Values, Phase Deviation, Steady State

Scientific paper

For Gecuba-, Gilda-, and Thyle-type asteroids, phase trajectories in the coordinates p = e cos s, q = e sin s (e is the eccentricity and s is the Delaunay anomaly) are discussed within the framework of the planar variant of the circular restricted three-body problem. Maximum disturbances of eccentricity and expressions for the period of variation of e are found.

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