Fig. 12
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Typical behaviour of the orbits in Region 1 (Fig. 11a). The temporal variations of n1/n2, n2/n3, e1, e2, e3 are in left panels, while right panels are for resonant angles θ12, Δϖ12, θ23, Δϖ23, φ0. The orbits are librating quasi-periodically around the stable symmetric ACR solution S6. The eccentricities of S6 are indicated by horizontal dashed lines.
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