Fig. 8

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Mass–radius relationship. Planetary radii are plotted as a function of planetary masses for the planets in the KMPS 100-embryo population. For planets with non-zero H–He envelopes, the colour denotes their envelope mass fraction,
. Planets without envelopes and without volatiles in their cores are in brown, while planets without envelopes that have volatiles in their cores are in blue.
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