Mass-radius diagram of simulated planets (blue dots) and TRAPPIST-1 planets (red crosses), data taken from Dorn et al. (2018). The solid, dotted, and dashed lines correspond to mass-radius relations for a rocky composition and a waterfraction of 0, 10, and 20%, respectively. The mass-radius relations are the same as the ones used in Dorn et al. (2018). The arrows starting from the simulated planets depict the trajectories on the mass-radius diagram that the simulated planets would cover if they were to lose their entire water content.