Extended Data Table 4 Oxidation states of rocky bodies in the solar system

From: Accretion of the earliest inner Solar System planetesimals beyond the water snowline

  1. Note that the fO2 values were reported using an ideal solution model (\({\gamma }_{{\rm{Fe}}}^{{\rm{metal}}}\) and \({\gamma }_{{\rm{FeO}}}^{{\rm{silicate}}}=1\)).
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