Long-term numerical simulations of the orbits of the Galilean satellites are carried out using a realistic physical model. The free libration of the Laplace angle, which plays a central role in the classical description of the tidal evolution of the Laplace resonance, is isolated from the simulated
โฆ LIBER โฆ
Orbital evolution of the Galilean satellites: Capture into resonance
โ Scribed by J. Henrard
- Publisher
- Elsevier Science
- Year
- 1983
- Tongue
- English
- Weight
- 811 KB
- Volume
- 53
- Category
- Article
- ISSN
- 0019-1035
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1 / 2 ศ 3/2 and 1 / 2 ศ 2 resonances can pump Ganymede's free eccentricity up to ศ10 ุ3 independent of Q Gany /Q J . We also We use the numerical model of R. Malhotra (1991, Icarus show that Ganymede's free eccentricity cannot have been 94, 399-412) to explore the orbital history of Io, Europa, and