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Analysis of a Simple Mechanism to Deplete the Kirkwood Gaps

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 106))

Abstract

In most applications resonance problems are implicitely or explicitely modelized by the Fundamental Model of Resonance i.e. the pendulum, characterized by its Hamiltonian function:

$$H = \frac{a}{2}{I^2} - b cos \psi $$
(1)

This reduction is performed in two steps: first, the action-angles variables are introduced to get a “one degree of freedom” Hamiltonian system, given by (2):

$$K = {k_o}(S) + \varepsilon {K_1}(S,s)$$
(2)

where K1 is 2π — periodic in s (the resonant angle).

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References

  • HENRARD, J.; 1982a. “Capture into Resonance: An extension of the use of Adiabatic invariants”. Celest. Mech. 27, 3–22.

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  • HENRARD, J.; 1982b. “The Adiabatic Invariant: Its use in Celestial Mechanics” in Application of Modern Dynamics to Celestial Mechanics and Astrodynamics (V. Szebehely editor). D. Rei-del Publ. Co.,Holland.

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  • HENRARD, J.; LEMAITRE, A.; 1983. “A second fundamental model for resonance” submitted for publication in Celestial Mechanics, 30, 197.

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  • SCHUBART, J.; 1966. “Special cases of the restricted problem of three bodies”, Proc. I.A.U., Symposium n° 25, 187–193.

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  • TORBETT, M.; SMOLUCHOWSKI, R.; 1980. “Sweeping of the Jovian Resonances and the Evolution of the Asteroids”, Icarus n°44, 722–729.

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© 1983 D. Reidel Publishing Company, Dordrecht, Holland

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Lemaitre, A. (1983). Analysis of a Simple Mechanism to Deplete the Kirkwood Gaps. In: Markellos, V.V., Kozai, Y. (eds) Dynamical Trapping and Evolution in the Solar System. Astrophysics and Space Science Library, vol 106. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7214-8_23

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  • DOI: https://doi.org/10.1007/978-94-009-7214-8_23

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-7216-2

  • Online ISBN: 978-94-009-7214-8

  • eBook Packages: Springer Book Archive

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