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Secular resonancesTheories and numerical experiments regarding secular resonances are reviewed. The basic dynamics and the positions of secular resonances are discussed, and secular perturbation theories for the nu16 resonance case, the nu6 resonance, and the nu5 resonance are addressed. What numerical experiments have revealed about asteroids located in secular resonances, the stability of secular resonances, variations of eccentricities and inclinations, and chaotic orbits is considered. Resonant transport of meteorites is discussed.
Document ID
19900039984
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Scholl, H. (Observatoire du Mont-Gros Nice, France)
Froeschle, CH. (Nice Observatoire, France)
Kinoshita, H. (Observatoire du Mont-Gros Nice, France)
Yoshikawa, M. (Tokyo Astronomical Observatory Mitaka, Japan)
Williams, J. G. (JPL Pasadena, CA, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Subject Category
Astronomy
Meeting Information
Meeting: Asteroids II
Location: Tucson, AZ
Country: United States
Start Date: March 8, 1988
End Date: March 11, 1988
Accession Number
90A27039
Distribution Limits
Public
Copyright
Other

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