Fig. 9
Evolution of J2 (in red) and prolateness ϵ (in blue) of HD 80606 b as a function of the eccentricity for different τ values. The green dashed line shows the average equilibrium value of these two quantities over one orbital period (Eqs. (85), (86)). The cyan dashed line shows the average equilibrium value of the prolateness for a specific spin-orbit resonance (Eq. (87)).
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