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Fig. 2

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Same as Fig. 1 but for Kepler-88 b. We neglect the permanent deformation of the planet (C22,r = 0), and show the spin dynamics for C22 = 2.2 × 10-6 (top, maximum deformation in the sub/super-synchronous resonances), and 6.7 × 10-6 (bottom, maximum deformation in the synchronous resonance).

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