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Fig. 5
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Mass–radius relations of bare silicate core radii (dashed lines) and with the outgassed atmosphere as a function of ΔIWeq (colored contours) for Φ = 0.1 (a), Φ = 0.5 (b), and Φ = 1 (c), and relative sizes (to scale) of the solid, liquid, and gaseous part of the planets for the fiducial volatile contents and ΔIWeq = −5.
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