Evolution of the orbital distance of a Jupiter-mass planet with different initial SMA (top panel) ranging from 0.8 R_co (black), 1.0 R_co (dark grey), and 1.2 R_co (light grey), δP_rot (middle panel), and the stellar rotation period (bottom panel) during the evolution of a 1.0 M_⊙ star with an initial rotation period of three days and a coupling timescale τ_c-e of 0.5 Myr. Upper panel: the orbital distance of the planet is represented in full coloured lines. The upper dotted lines correspond to P_orb = P_rot,⋆ (the corotation limit) and the lower dotted lines correspond to P_orb = 1/2 P_rot,⋆ limit, which marks the region above which the dynamical tide operates. The red long-dashed line is the evolution of the Roche lobe radius. Middle panel: departure of the rotation rate of the host star (P_rot,⋆ ) from an isolated star (P_rot,isol.). The horizontal dashed line indicates no difference with an isolated star, and the vertical dashed line represents the localisation of the ZAMS (around 50 Myr for a 1.0 M_⊙ star). Lower panel: rotation period (in days) of the host star. The horizontal dashed line correspond to the transition between saturated and unsaturated magnetic regimes (1.6 days ≈ 16 Ω_⊙), and the circle represents the rotation rate of the present Sun. The time on the x-axis is given from an initial time t_init of 5 Myr.