Tidal evolution of 10   M_⊕ mass planets starting with different initial semi-major axes around either a rapidly rotating or a slowly rotating 0.1 M_⊙ star with a mean dissipation factor. Top panel: evolution of the semi-major axis. The full colored lines correspond to rapidly rotating stars and the dash-dotted lines correspond to slowly rotating stars. The solid and dash-dotted red lines represent the evolution of the corotation radius in both cases when there is no planet. The long black dashes represent the Roche limit. Middle panel: the corresponding stellar rotation evolution (the same line code is used). The black long dashes represent T_sat = 2π/ω_sat. Bottom panel: equatorial velocity of the star vs. time (the same line code is used).