Formation and evolution tracks of one giant planet that ends up being accreted by the star during the evolution stage due to tidal migration. Top left: total mass M_tot versus distance; top right: total mass M_tot (black) and core mass M_core (red) versus time; bottom left: total luminosity L_tot (black) and the bloating contribution L_bloat (red) versus time; bottom centre: distance versus time; bottom right: total radius R_tot (black) and outer (attached phase) or Hill (detached phase) radius (red) versus time.