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Fig. 8.

image

Typical evolution of the eccentricities in simulations where the Laplace resonance is disrupted. Column a: case B with ϖ2 − ϖ3 ∼ 0; all the eccentricities remain below 0.04. Column b: case B with ϖ2 − ϖ3 in circulation and ϖ3 − ϖ4 ∼ 0; the eccentricity of Callisto increases until the pure three-body resonance is disrupted. Column c: case B with ϖ2 − ϖ3 in circulation and ϖ3 − ϖ4 ∼ π; the eccentricity of Ganymede increases until the pure three-body resonance is disrupted.

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