Numerical investigation of motions of resonant asteroids in the three-dimensional space

Details Numerical investigation of motions of resonant asteroids in the three-dimensional space Numerical investigation of motions of resonant asteroids in the three-dimensional space

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992cemda..54..287y&link_type=abstract

Celestial Mechanics and Dynamical Astronomy (ISSN 0923-2958), vol. 54, no. 1-3, p. 287-290.

Astronomy and Astrophysics

Astronomy

2

Asteroids, Orbital Resonances (Celestial Mechanics), Three Dimensional Models, Astronomical Models, Eccentric Orbits, Equations Of Motion

Scientific paper

The paper examines motions of asteroids in mean motion resonances with Jupiter. Orbital changes of fictitious asteroids in the Kirkwood gaps are calculated by numerical integrations for 100,000-1,000,000 yr. There are various motions of resonant asteroids, some of them very complicated and chaotic, and others regular. The eccentricity of some asteroids becomes very large, and the variation of the inclination is large while the eccentricity is large. In the 7:3 resonance, the variation of the inclination of some resonant asteroids is so large that prograde motion becomes retrograde. Some asteroids in the 7:3 resonance can collide with the sun as well as with the inner planets.

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