Fig. 14
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Evolution of the ratio of the mean motions of S3 and S4 (top panel) and the evolution of the resonant angles involving the mean longitudes of S2, S3, and S4 (bottom panel) in the case of the 2:1&3:2 resonance of the three innermost moons considering the tidal dissipation assuming a fast-rotating central body. The tidal effects are multiplied by a factor 104.
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