Fig. 6
Evolution of HD 80606 b with time for different τ values. We plot the semi-major axis (in AU) and the eccentricity (top), the ratio between the planet rotation rate and the orbital mean motion (middle), and the planet J2 and ϵ (bottom). The green line gives the pseudo-synchronous equilibrium (Eq. (60)) (middle), and the average equilibrium values for J2 and ϵ, respectively (Eqs. (85) and (86)) (bottom).
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