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Published December 2015 | public
Journal Article

Thermal equation of state and stability of (Mg₀.₀₆Fe₀.₉₄)O

Abstract

We present the pressure-volume-temperature (P-V-T) equation of state of polycrystalline (Mg_(0.06)Fe_(0.94))O (Mw94) determined from laser-heated x-ray diffraction experiments up to 122 GPa and 2100 K, conditions approaching those of the deep mantle. We conducted two sets of experiments, one with an in situ Fe metal oxygen fugacity buffer and one without such a buffer. The internal pressure markers used in these experiments were B2-NaCl and hcp-Fe in the buffered experiment and B2-NaCl in the unbuffered experiment. In the sampled P-T range of the high temperature part of this study, only the B1 structure of Mw94 was observed, indicating that the addition of Mg to FeO stabilizes the B1 phase with respect to the B8 phase at these conditions. Both datasets were fit to a Birch-Murnaghan and Mie-Grüneisen-Debye thermal equation of state using a new open-source fitting routine, also presented here. Analysis of these data sets using the same internal pressure marker shows that the P–V–T data of Mw94 obtained in the unbuffered experiment are well explained by the equation of state parameters determined from the buffered data set. We have also compared the thermal equation of state of Mw94 with that of wüstite and conclude that Mw94 has measurably distinct thermoelastic properties compared with those of wüstite. We use the results obtained in the buffered experiment to determine the density and bulk sound velocity of Mw94 at the base of the mantle and compare these values to geophysical observations of ultralow-velocity zones.

Additional Information

© 2015 Elsevier B.V. Received Date: 16 January 2015; Revised Date: 15 August 2015; Accepted Date: 3 September 2015. Available online 11 September 2015. We thank D. Zhang and C.A. Murphy for assistance with the measurements, A.S. Wolf and D.B. Bower for discussions, and NSF-EAR 0711542 and CSEDI EAR-0855815 for financial support. We thank E.E. Alp for conducting the conventional Mössbauer spectroscopy measurements at Argonne National Laboratory. This work was performed at GeoSoilEnviroCARS (Sector 13), Advanced Photon Source (APS), Argonne National Laboratory. GeoSoilEnviroCARS is supported by the National Science Foundation - Earth Sciences (EAR-1128799) and Department of Energy - Geosciences (DE-FG02-94ER14466). Use of the Advanced Photon Source was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under contract No. DE-AC02-06CH11357. The gas-loading system at GSECARS and conventional Mössbauer spectroscopy laboratory are supported in part by COMPRES under NSF Cooperative Agreement EAR 06-49658. Sample synthesis was carried out in the petrological facilities at Caltech. Microprobe analyses were carried out at the Caltech GPS Division Analytical Facility (funded in part by the MRSEC Program of the NSF under DMR-0080065). Finally, we would like to acknowledge two anonymous reviewers, whose feedback helped to improve the manuscript.

Additional details

Created:
August 23, 2023
Modified:
October 24, 2023