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- W4248174768 abstract "Abstract Resonant asteroidal motion is investigated over 17 000 years in a three-dimensional elliptical model Sun-Jupiter-Asteroid averaged by Schubart's method à la Poincarè. Orbits remain trapped in the resonance over this period. The various stability mechanisms are discussed. With respect to their behaviour of ω and ῶ, our resulting orbits reveal 5 distinct classes. These 5 classes can be described in Schubart's topology for the planar problem. As compared to the planar case, eccentricities of orbits in the three-dimensional model vary more strongly. This is an important result for the problem of the delivery of meteorites." @default.
- W4248174768 created "2022-05-12" @default.
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- W4248174768 date "1983-01-01" @default.
- W4248174768 modified "2023-09-26" @default.
- W4248174768 title "Resonant Asteroidal Motion in the Kirkwood Gaps: A Three-Dimensional Study" @default.
- W4248174768 doi "https://doi.org/10.1017/s0252921100097050" @default.
- W4248174768 hasPublicationYear "1983" @default.
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