Motion of the Jovian commensurability resonances and the character of the celestial mechanics in the asteroid zone - Implication for kinematics and structure

Details Motion of the Jovian commensurability resonances and the character of the celestial mechanics in the asteroid zone - Implication for kinematics and structure Motion of the Jovian commensurability resonances and the character of the celestial mechanics in the asteroid zone - Implication for kinematics and structure

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...110...43t&link_type=abstract

Astronomy and Astrophysics, vol. 110, no. 1, June 1982, p.43-49.

Astronomy and Astrophysics

Astrophysics

17

Asteroid Belts, Celestial Mechanics, Jupiter (Planet), Planetary Evolution, Solar Orbits, Eccentric Orbits, Kinematics, Long Term Effects, Numerical Integration, Resonance, Jupiter, Motion, Celestial Mechanics, Kinematics, Structure, Asteroids, Kirkwood Gaps, Equations Of Motion, Eccentricity, Evolution, Observations, Widths, Data

Scientific paper

The motion of the Jovian commensurability resonances during the early evolution of the solar system induced by the dissipation of the accretion disk results in fundamental differences in the celestial mechanics of objects over which a resonance passes from that observed for a stationary resonance. Objects experiencing resonance passage acquire irreversible increases of average eccentricity to large values accounting for the present-day random velocities of the asteroids. Semi-major axes are similarly irreversibly decreased by amounts capable of clearing the Kirkwood gaps. The gap widths are in agreement with observation.

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