Secular evolution of a star–planet system formed by a 1 M⊙ star with P*,ini = 5 days, orbited by a planet at initial distance aini = 0.035 AU, for three planets of differing mass: mp = 0.1 MJup (black lines),1 MJup (red), and 5 MJup (orange). Top panel: rotation rate of the envelope (solid lines) and of the radiative zone (dashed lines) of the star. Middle panel: semi-major axis (solid lines), corotation radius of the star (dashed lines) and limit of excitation of the dynamical tide (dotted lines). Bottom panel: modified quality factor.
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