Steady state obliquity of a rigid body in the spin-orbit resonant problem: application to Mercury
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Publication:680978
DOI10.1007/s10569-017-9787-3zbMath1479.70072OpenAlexW2755866663MaRDI QIDQ680978
Publication date: 29 January 2018
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10569-017-9787-3
Related Items (2)
On the exo-planet precession under torqes due to three celestial bodies with the evolution of the satellite's orbit ⋮ Impact of a Moon on the evolution of a planet's rotation axis: a non-resonant case
Cites Work
- Effective stability around the Cassini state in the spin-orbit problem
- Mercury's resonant rotation from secular orbital elements
- Analysis of resonances in the spin-orbit problem in celestial mechanics. II: Higher order resonances and some numerical experiments
- Planetary long periodic terms in Mercury's rotation: a two-dimensional adiabatic approach
- Measures of basins of attraction in spin-orbit dynamics
- A symplectic mapping for the synchronous spin-orbit problem
- Transient times, resonances and drifts of attractors in dissipative rotational dynamics
- Celestial Dynamics
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