Evolution of asteroid orbits in the case of commensurabilities of the mean motions - Fundamental equations

Details Evolution of asteroid orbits in the case of commensurabilities of the mean motions - Fundamental equations Evolution of asteroid orbits in the case of commensurabilities of the mean motions - Fundamental equations

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986azh....63..567g&link_type=abstract

(Astronomicheskii Zhurnal, vol. 63, May-June 1986, p. 567-573) Soviet Astronomy (ISSN 0038-5301), vol. 30, May-June 1986, p. 337

Astronomy and Astrophysics

Astronomy

6

Asteroids, Equations Of Motion, Gravitational Fields, Orbit Calculation, Solar Orbits, Three Body Problem, Kepler Laws

Scientific paper

Equations describing the evolution of the orbits of resonance asteroids
are derived within the framework of the inner variant of the circular,
restricted three-body problem using Zeipel's method. A simplified system
of equations is considered for lower-order resonances.

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