The \(3:2\) spin-orbit resonant motion of Mercury

DOI10.1007/S10569-006-9032-YzbMath1109.70012OpenAlexW2041533858MaRDI QIDQ850711

Nicolas Rambaux, Sandrine D'Hoedt, Anne Lemaitre

Publication date: 6 November 2006

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

Full work available at URL: https://doi.org/10.1007/s10569-006-9032-y

zbMATH Keywords

Hamiltonian formalismMercuryResonance spin-orbit

Mathematics Subject Classification ID

Hamilton's equations (70H05) Celestial mechanics (70F15)

Related Items (7)

Note on Mercury's rotation: the four equilibria of the Hamiltonian model ⋮ A symplectic mapping for the synchronous spin-orbit problem ⋮ Planetary long periodic terms in Mercury's rotation: a two-dimensional adiabatic approach ⋮ Tidal friction in close-in satellites and exoplanets: the Darwin theory re-visited ⋮ Planetary perturbations on Mercury's libration in longitude ⋮ Regions of stability in rotational dynamics ⋮ Effective stability around the Cassini state in the spin-orbit problem

Cites Work

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• Note on Mercury's rotation: the four equilibria of the Hamiltonian model
• The spin-orbit resonant rotation of Mercury: a two degree of freedom Hamiltonian model
• Solar System Dynamics
• Introduction to Hamiltonian dynamical systems and the \(N\)-body problem

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