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Fig. 5
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Random resonant solutions in the semimajor axis and eccentricity planet for the two different chains (3:2, 2:1, and 3:2 on the left and 3:2, 2:1, and 2:1 on the right). The solutions are scalable in semimajor axes, and the three inner planet semimajor axes can be shifted until they coincide with the observed ones.
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