The formation and structure of iron-dominated planetesimals

Open Access

Fig. A.1

The metal-silicate partition coefficients, $L o g D_{i}^{met-sil}$ $\[Log D_i^{\text {met-sil}}\]$ plotted for key elements C, Si, S, and Ni as a function of fO₂, calculated at 1900 K and 0.1 GPa for the initial bulk compositions considered in this study. $L o g D_{i}^{met-sil}$ $\[Log D_{i}^{\text {met-sil}}\]$ functions are based on literature studies (Boujibar et al. 2014; Steenstra et al. 2016; Chi et al. 2014; Fischer et al. 2015; Steenstra et al. 2020a).

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