Structure type and bulk modulus of Fe3S, a new iron-sulfur compound

By Y. Fei, Jie Li, C. Bertka, C. Prewitt. 2000

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Phase equilibria at high temperatures (2006, background): “Subsequently, Fei et al. (1997, 2000) synthesized three Fe-S alloy phases (Fe3S2, Fe3S and Fe2S) at subsolidus temperatures and high pressures (Fig.”
Thermal evolution of the Martian core: Implications for an early dynamo (2004, background): “The melting temperatures of pure Fe and the Fe 1 FeS eutectic of ;2200 K and ;1500 K, respectively, at Martian core pressures, imply that u 5 2.41 (Fei et al., 2000).”
Geodesy constraints on the interior structure and composition of Mars (2011, background): “This large fraction of sulfur in the core results in a significant depression of the melting temperature of the core material aggregate compared to pure iron (Fei et al., 2000; Stewart et al., 2007) and implies that models based on the above bulk composition most likely have a molten outer core.”
Sulfur's impact on core evolution and magnetic field generation on Ganymede (2005, methodology): “The liquidus slope as a function of composition, ac, is determined from available data for the Fe-FeS system [Fei et al., 1997, 2000] by the following equation, with the parameters listed in Table 2: ac ¼ Tm0; Fe;FeSð Þ 1þ Tm1; Fe;FeSð ÞP þ Tm2; Fe;FeSð ÞP2 Teu0 1þ Teu1P½ Tm0; Fe;FeSð Þceu0 1þ…”