Effective Hamiltonian for the D'Alembert planetary model near a spin/orbit resonance

DOI10.1023/A:1020151319725zbMath1083.70014OpenAlexW4247579050MaRDI QIDQ1871115

Luca Biasco, Luigi Chierchia

Publication date: 6 May 2003

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

Full work available at URL: https://doi.org/10.1023/a:1020151319725

zbMATH Keywords

stabilityproper degeneraciesfast averagingNekhoroshev normal forms

Mathematics Subject Classification ID

Completely integrable systems and methods of integration for problems in Hamiltonian and Lagrangian mechanics (70H06) Celestial mechanics (70F15) Dynamical systems in classical and celestial mechanics (37N05) Stability problems for problems in Hamiltonian and Lagrangian mechanics (70H14)

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Adiabatic chaos in the spin-orbit problem ⋮ A resonant-term-based model including a nascent disk, precession, and oblateness: application to GJ 876 ⋮ Long term stability of proper rotations of the perturbed Euler rigid body

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