A non-planar circular model for the 4/7 resonance

DOI10.1007/s10569-005-7872-5zbMath1129.70311OpenAlexW2095876603MaRDI QIDQ816919

Miloš Šidlichovský

Publication date: 2 March 2006

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

Full work available at URL: https://doi.org/10.1007/s10569-005-7872-5

zbMATH Keywords

resonancesEdgeworth-Kuiper beltsolar system dynamics

Mathematics Subject Classification ID

Three-body problems (70F07) Celestial mechanics (70F15)

Related Items (3)

An analytically treatable model of long-term dynamics in a mean motion resonance with coexisting resonant modes ⋮ Quasi-satellite orbits in the general context of dynamics in the \(1:1\) mean motion resonance: perturbative treatment ⋮ Long-term orbital dynamics of trans-Neptunian objects

Uses Software

• Mathematica

Cites Work

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• The Kozai resonance in the outer solar system and the dynamics of long-period comets
• Wisdom system: dynamics in the adiabatic approximation
• Comparative study of the \(2:3\) and \(3:4\) resonant motion with Neptune: an application of symplectic mappings and low frequency analysis
• A symplectic mapping model for the study of 2:3 resonant trans-Neptunian motion
• Solar System Dynamics

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