The research dataset of "Earth's water features shaped by deep core-mantle differentiation and volatile-rich accretion"

This dataset presents the research data of "Earth's water features shaped by deep core-mantle differentiation and volatile-rich accretion", including the following six tables: Table 1. Calculated reaction Gibbs free energy (∆G_r) for transferring one H2O from silicate melt to liquid iron via molecule exchange reaction, and the corresponding hydrogen partition coefficients (D_H^(met/sil)) at various pressure, temperature and chemical composition conditions. Table 2. Calculated reaction Gibbs free energy (∆G_r) for transferring one H2O from silicate melt to liquid iron via redox reaction, and corresponding hydrogen partition coefficients (D_H^(met/sil)) at various pressure, temperature and chemical composition conditions. Table 3. Summary of calculated interatomic distances (dij) and coordination numbers (CNij) in Fe-bearing silicate melt at different pressure-temperature conditions. Table 4. Summary of calculated interatomic distances (dij) and coordination numbers (CNij) in liquid iron with light elements (O, S, Si) at different pressure-temperature conditions. Table 5. Modeling results of water content in the bulk silicate Earth (BSE) and Earth’s core after core-mantle differentiation under different depths of magma ocean for various building block compositions. Table 6. Summary of calculated Bulk (Total) partition coefficients of hydrogen (Bulk D_H^(met/sil)) and oxygen (Bulk D_O^(met/sil)) between silicate melt (with and without Fe component) and liquid iron (LEs-free) at different pressures and temperatures under coexistence of exchange and redox reactions.