Fig. 20
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Orbital distance, planetary radius diagram of synthetic planets around a 0.1 M⊙ star. For comparison, the Trappist-1 system (Agol et al. 2021) and the subsample of synthetic planets around them is shown. The core ice mass fraction is here colored using a logarithmic scale for better visibility of the low values derived assuming a core iron mass fraction of 32.5% in Trappist-1.
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