Fig. 6.

Typical evolution of the eccentricities in simulations where the Laplace resonance and all the current resonances are preserved. Panel a: case A with λ2 − 2λ3 + ϖ3 in libration; all the eccentricities rapidly settle to new low values. Panel b: case A with λ2 − 2λ3 + ϖ3 in circulation; Callisto’s eccentricity increases slowly as it exits its resonance with Ganymede. Panel c: case B with λ2 − 2λ3 + ϖ2 in libration; after an abrupt increase the eccentricities converge to new values.
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