Fig. 3
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Predicted bulk compositions (in wt%) of rocky planetary bodies as a function of temperature based on the condensation sequences computed using ECCOplanets code (Timmermann et al. 2023) for Kepler-94 metal-rich and Kepler-62 metal-poor stars (see Fig. 2). Stellar abundances are from Brewer et al. (2016), with S abundances estimated based on [Fe/H] values.
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