Secular resonances between bodies on close orbits: a case study of the Himalia prograde group of Jovian irregular satellites

DOI10.1007/s10569-016-9676-1zbMath1478.70010arXiv1603.05125OpenAlexW3101733991MaRDI QIDQ531170

Daohai Li, Apostolos A. Christou

Publication date: 3 August 2016

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

Full work available at URL: https://arxiv.org/abs/1603.05125

zbMATH Keywords

secular resonancesKozai-Lidov mechanismcoorbital interactionsirregular satellitesKozai cyclenodal resonancesolar perturbations

Mathematics Subject Classification ID

Orbital mechanics (70M20)

Related Items (1)

Secular resonances between bodies on close orbits. II: Prograde and retrograde orbits for irregular satellites

Uses Software

• FFTW

Cites Work

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• A semi-numerical perturbation method for separable Hamiltonian systems
• On the evection resonance and its connection to the stability of outer satellites
• Review of the dynamics in the Kirkwood gaps
• About the dynamics of the evection resonance
• Dislocation lines in the hyperbolic umbilic diffraction catastrophe
• Non-restricted double-averaged three body problem in Hill's case
• Solar System Dynamics
• Series expansions for encounter-type solutions of Hill's problem
• The long-term dynamics of the Jovian irregular satellites

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