Fig. 10
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Bulk elemental planetary compositions (in wt%) of rocky planets formed around Kepler-62 star (the lowest metallicity star), and Kepler-94 star (the highest metallicity star in the sample) assuming the same planetesimal formation time of 0.2 Myr. The outcome of the same planet formation simulation is shown in both cases. Only planets with semi-major axes within 0.25 AU are displayed.
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