The secular resonance nu6 in the asteroidal belt

Details The secular resonance nu6 in the asteroidal belt The secular resonance nu6 in the asteroidal belt

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...166..326f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 166, no. 1-2, Sept. 1986, p. 326-332. DFG-supported research.

Astronomy and Astrophysics

Astrophysics

28

Asteroid Belts, Celestial Mechanics, Resonance, Secular Variations, Solar Orbits, Eccentricity, Inclination, Numerical Integration, Orbital Elements, Temporal Distribution

Scientific paper

The authors present results obtained from numerical integrations over 1 M years for orbital evolution in the secular resonance ν6 at 2.05 AU. The resonance cases found show a libration of the secular argument ω~-ω~s about 180° only. Strong variations in eccentricity yield direct earth-crossers from this secular resonance. According to the numerical results, secular resonances should be considered as sources of meteorites as conjectured by Wetherill and Williams.

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