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Fig. 20

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Radii versus semimajor axes of our simulated planetary systems, both the radii of planets as homogeneous spheres calculated based on ρ = 3 g cm–3 (in magenta), and the compressed radii with individual ρ (in orange), compared to the currently known systems around K dwarfs (in blue). Only planets with known masses of 7 M or less are presented. The point size indicates the masses in M of the planets.

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