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Fig. D.1

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Illustration of the evolution of Q* as function of time for the different models considered. In orange our stellar model combined to the upper boundary of the planetary tidal dissipation found previously Q* = 3 × 105. In black our stellar model is combined to the lower value of the planetary dissipation Q* → ∞. We can notice that the black and orange line are close to be superimposed. In green is represented the model with σ* = const, as done in Bolmont & Mathis (2016), the constant was calibrated at value in the MS (σ* = 5.536 × 10−66 at t = 0.83 Gyr). Finally the shaded areas correspond to the different evolutionary phases of the star, in yellow the MS, in orange, the sub-Giant phase, and in red the RGB phase.

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