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Fig. 17
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Core mass fraction versus Fe/Mg and Si/Mg molar ratios, where the ranges reflect the uncertainties in the stellar abundances. The core mass fractions, computed using ExoPlex (Unterborn et al. 2023), are of a typical simulated planet of 1 M⊕ around Kepler-94 assuming the planetesimal formation time of 0.2 Myr.
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