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Published November 13, 2023 | Published
Journal Article Open

Melting and defect transitions in FeO up to pressures of Earth's core-mantle boundary

Abstract

The high-pressure melting curve of FeO controls key aspects of Earth's deep interior and the evolution of rocky planets more broadly. However, existing melting studies on wüstite were conducted across a limited pressure range and exhibit substantial disagreement. Here we use an in-situ dual-technique approach that combines a suite of >1000 x-ray diffraction and synchrotron Mössbauer measurements to report the melting curve for Fe₁₋O wüstite to pressures of Earth's lowermost mantle. We further observe features in the data suggesting an order-disorder transition in the iron defect structure several hundred kelvin below melting. This solid-solid transition, suggested by decades of ambient pressure research, is detected across the full pressure range of the study (30 to 140 GPa). At 136 GPa, our results constrain a relatively high melting temperature of 4140 ± 110 K, which falls above recent temperature estimates for Earth's present-day core-mantle boundary and supports the viability of solid FeO-rich structures at the roots of mantle plumes. The coincidence of the defect order-disorder transition with pressure-temperature conditions of Earth's mantle base raises broad questions about its possible influence on key physical properties of the region, including rheology and conductivity.

Copyright and License

© The Author(s) 2023. This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.

Acknowledgement

We thank June Wicks for sample synthesis. We thank Paul Asimow, Michael Gurnis, and Zhongwen Zhan for valuable discussions. We are grateful to the National Science Foundation for supporting this work under EAR-1727020 and EAR-CSEDI—2009935 (J.M.J.). We acknowledge the JPL Strategic Research & Technology Development Program, "Venus Science Into The Next Decade". GeoSoilEnviroCARS and Sector 3 operations are partially supported by COMPRES (NSF-EAR-1661511). GeoSoilEnviroCARS is supported by the National Science Foundation—Earth Sciences (NSF-EAR-1634415) and Department of Energy- GeoSciences (DE-FG02-94ER14466). Use of APS is supported by the U.S. DOE, Office of Science (DE-AC02-06CH11357). SMS data collected during hybrid mode of the APS used a dual, fast-shutter spectrometer built by T.S.T. and supported by Laboratory Directed Research and Development (LDRD) funding from Argonne National Laboratory, provided by the Director, Office of Science, of the U.S. DOE under Contract No. DE-AC02-06CH11357.

Contributions

V.V.D. and J.M.J. designed the study. V.V.D. prepared the samples, led the XRD and SMS experiments, analyzed the data, produced the figures, and wrote the manuscript. J.M.J. and W.S. contributed to validating the data analysis. V.V.D., W.S., and D.Z. developed software for data analysis. J.M.J., D.Z., W.S., S.C., V.B.P., J.Z., T.S.T., and O.S.P. contributed to performing the experiments and editing the manuscript.

Data Availability

All data used to construct Fig. 6 are available in the main text and supplementary materials, in the Source Data file, and in a Zenodo data depository (https://doi.org/10.5281/zenodo.10048208). Additional data are available from the corresponding author upon request. Source data are provided with this paper.

Conflict of Interest

The authors declare no competing interests.

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Additional details

Created:
November 20, 2023
Modified:
November 20, 2023