Fate of planets of different masses (in Jupiter masses), starting their evolution at various distances (in au) from their host star. The left panels show the fate of planets during the PMS phase. The right panels show the fate of planets during the RGB phase. The left panels cover a much wider range of distances (more than 10 times larger) than the right panel. From top to bottom panels, the host star is a 1 M_⊙ star (see its surface rotation in Fig.), a fast- and a slow-rotating 1.5 M_⊙ star, respectively. The domain of planet masses considered for the 1.5 M_⊙ is smaller than the domain covered for the 1 M_⊙ plot. Planets in the upper blue regions show no change in their orbit. Planets in the salmon region are engulfed. The orbits of planets in skyblue and turquoise regions are widened by tides. Orbits of planets in the pink regions were shrunken bytides. The light gray zones correspond to the domains where no planet should be observed, either because they have been engulfed during the PMS phase or because they have been kicked out from their original to a more distant orbit.