Transition from solid planets to planets with H/He in the plane of mass (left panel) and corresponding radius (right panel) versus semimajor axis for the nominal simulation M0 at 5 Gyr. Colored points are planets that still have primordial H/He whereas gray diamonds are bare rocky planets. The color code shows the fraction of initial H/He that was evaporated (same color scale as in Fig. 3). The red line is a power law fit to the most massive respectively largest planet that has lost the envelope, representing the transition at M_bare respectively R_bare, with the fit parameters indicated in the inset (M_bare in M_⊕, R_bare in R_⊕). Planets below the red line are solid planets in the bare core triangle. In the mass plane the transition is continuous, whereas in the radius plane, there is a gap separating solid planets from planets with gas (the evaporation valley).