The main secular resonances \(\nu{}_ 6,\nu{}_ 5\) and \(\nu{}_{16}\) in the asteroid belt

DOI10.1007/BF00048607zbMath0850.70123OpenAlexW2076217358MaRDI QIDQ1186265

Jacques Henrard, Alessandro Morbidelli

Publication date: 28 June 1992

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00048607

Mathematics Subject Classification ID

Celestial mechanics (70F15)

Related Items (4)

Formal solution of the asteroid motion near the 2:1 commensurability ⋮ Collective resonant phenomena on small bodies in the solar system ⋮ Are the analytical proper elements of asteroids still needed? ⋮ On the successive elimination of perturbation harmonics

Cites Work

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• A semi-numerical perturbation method for separable Hamiltonian systems
• Secular resonances in the asteroid belt: Theoretical perturbation approach and the problem of their location
• A second fundamental model for resonance
• Secular perturbations of asteroids in secular resonance

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