Thermal equation of state of Fe3S and implications for sulfur in Earth's core
Thermal equation of state of Fe3S and implications for sulfur in Earth's core
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DOI:
10.1029/2005jb004091
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发表时间:
2006-06-29
影响因子:
3.9
通讯作者:
Prakapenka, Vitali B.
中科院分区:
文献类型:
--
作者:
Seagle, Christopher T.;Campbell, Andrew J.;Prakapenka, Vitali B.
[1] Iron ( Fe) and coexisting Fe3S were studied simultaneously using synchrotron X- ray diffraction and a laser-heated diamond anvil cell (DAC). The thermal equation of state (EOS) of Fe3S was investigated up to pressures of 80 GPa and temperatures of 2500 K. Fitting a third-order Birch-Murnaghan EOS to the room temperature data yielded bulk modulus K-0 = 156( 7) GPa ( values in parentheses are standard deviation) and pressure derivative K-0'= 3.8( 3) calibrated against NaCl in the B2 structure. The room temperature data were also calibrated against the EOS of hcp-Fe for comparison and aid in the determination of the thermal pressure contribution of Fe3S. This fit yielded bulk modulus K-0 = 113( 9) GPa and pressure derivative K-0'= 5.2( 6). The thermal pressure contribution of Fe3S was assumed to be of the form Delta P-thermal = alpha K-T Delta T, where alpha K-T is constant. The best fit to the data yielded alpha K-T = 0.011( 2) GPa K-1. Iron and Fe3S coexisted in the high-pressure, high-temperature experiments, and a density relationship between Fe and Fe3S was found to be linear and independent of temperature. Extrapolation of the data to the core-mantle boundary (CMB), using an assumed temperature of 3500 K at the CMB, a 2% volume change associated with melting, and applying a small adjustment to account for the nickel content of the core indicates that 14.7(11) wt % sulfur is adequate to resolve the density deficit of the outer core.