Titan's rotation: A 3-dimensional theory
arXiv:0710.4950 · doi:10.1051/0004-6361:20077991
Abstract
We study the forced rotation of Titan seen as a rigid body at the equilibrium Cassini state, involving the spin-orbit synchronization. We used both the analytical and the numerical ways. We analytically determined the equilibrium positions and the frequencies of the 3 free librations around it, while a numerical integration associated to frequency analysis gave us a more synthetic, complete theory, where the free solution split from the forced one. We find a mean obliquity of 2.2 arcmin and the fundamental frequencies of the free librations of about 2.0977, 167.4883, and 306.3360 years. Moreover, we bring out the main role played by Titan's inclination on its rotation, and we suspect a likely resonance involving Titan's wobble.
accepted for publication in Astronomy ans Astrophysics
References in corpus (1)
Cited by in corpus (12)
- Global dynamics of high area-to-mass ratios GEO space debris by means of the MEGNO indicator
- Theory of the rotation of Janus and Epimetheus
- Secular Dynamics of S-type Planetary Orbits in Binary Star Systems: Applicability Domains of First- and Second-Order Theories
- Interpreting the librations of a synchronous satellite -- How their phase assesses Mimas' global ocean
- Secular Orbit Evolution in Systems with a Strong External Perturber - A Simple and Accurate Model
- Long-Term Stability of Planets in the Centauri System, II: Forced Eccentricities
- Titan's rotational state : The effects of a forced "free" resonant wobble
- The rotation of Mimas
- Behavior of nearby synchronous rotation of a Poincaré-Hough satellite at low eccentricity
- Effective resonant stability of Mercury
- Rotation of a synchronous viscoelastic shell
- New insights on Titan's interior from its obliquity