[S-IT31] 惑星中心核：構造，形成と進化

[SIT31-P04] Thermodynamic analysis of density of Fe-Ni-S melts at high pressure

*浦川 啓¹、寺崎 英紀²、町田 晃彦³ (1.岡山大学大学院自然科学研究科、2.大阪大学大学院理学研究科、3.量子科学技術研究開発機構)

キーワード：密度、モル体積、熱膨張、液体鉄合金

Density of liquid Fe-alloy is one of the important physical properties to understand dynamics of planetary liquid core. However, we have only limited information on the pressure, temperature and composition dependency of density of liquid Fe-alloy. We have focused on Fe-Ni-S alloy, which are thought to be universally present as core constituents of planets and satellites, and measured their densities at high-temperatures and pressures by X-ray absorption technique. Here we report the results of thermodynamic analysis of the density of liquid Fe-Ni-S alloy. Density (molar volume) of liquid Fe-Ni-S alloy measured at 3 GPa was analyzed by associated solution model assuming the associated compounds, Fe, FeS, NiS and Ni. We evaluated the molar volume and the thermal expansivity of each associated compound as well as the interaction parameters between associated compounds. As a result, we can express the temperature and composition dependence of the density of liquid Fe-Ni-S alloy at 3 GPa. We found a negative excess volume between Fe-FeS and FeS-NiS and a positive excess volume between Ni-NiS. We will also discuss the pressure evolution of the phase relationships of the Fe-FeS.