Fate of planets of different masses (in Jupiter masses), starting their evolution at various distances (in au) from their host star during the PMS phase. The left and right panels show respectively, the fate of planets without accounting for the evaporation process and with account of the evaporation process. Planets in the salmon-colored region are engulfed or evaporated. For low-mass planets, evaporation usually occurs before engulfment, and vice-versa for high-mass planets. Therefore, the transition of the fate happens somewhere in the intermediate-mass region. Planets in sky-blue regions and in turquoise regions have their orbits widened by tides.