A characteristic parameter of librating orbits

Details A characteristic parameter of librating orbits A characteristic parameter of librating orbits

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984avest..18...28k&link_type=abstract

(Astronomicheskii Vestnik, vol. 18, Jan.-Mar. 1984, p. 28-34) Solar System Research (ISSN 0038-0946), vol. 18, no. 1, July 1984,

Astronomy and Astrophysics

Astronomy

Asteroids, Jupiter (Planet), Librational Motion, Solar Orbits, Eccentric Orbits, Orbital Resonances (Celestial Mechanics)

Scientific paper

A certain parameter M(asterisk) connecting the positions of Jupiter and an asteroid in a resonance orbit at the initial time is introduced. For a given commensurability with a fixed initial eccentricity the parameter M(asterisk) uniquely determines the evolution of the resonance orbit. It has high temporal stability, which can be used for numerical calculations of the evolution of resonance orbits over long time intervals.

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