Abstract
The redox state of Earth’s mantle is governed by the oxidation state of iron and carbon and influences key physical and chemical mantle parameters. Mantle xenoliths, and experimental and thermodynamic studies reveal a decrease in oxygen fugacity with depth, down to ~250 km. A further more modest drop is linked to the predicted stabilization of nickel-rich metallic alloy at 250–300 km. However, garnets from 250–500 km record more oxidized conditions, and no nickel-rich alloy has been reported from these depths to account as natural evidence for the predictions. Here we report nickel–iron metallic nanoinclusions and Ni-rich carbonate microinclusions in two diamonds from the Voorspoed mine, South Africa. Various pressure indicators confirm their origin in the deep upper mantle or the shallow transition zone (280–470 km). The coexistence of nickel-rich metal and carbonate indicates a reaction between oxidized carbonatitic melt and reduced metal-bearing peridotite that led to nickel enrichment and diamond growth. This reaction captures a snapshot of the dynamics of metasomatism, including the formation of intermediate products that may later react. The diamonds provide direct evidence for nickel-rich alloy at its predicted depth within the mantle. They also indicate the presence of deep carbonatitic–silicic melts, which episodically oxidize small volumes of the mantle and play a role in the formation of kimberlites and alkali basalts.
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Data availability
Source data for this paper are provided in Supplementary Tables and Supplementary Figs. 1–11 and can be found on the EarthChem Library at https://doi.org/10.60520/IEDA/113984 (ref. 77).
Change history
25 September 2025
A Correction to this paper has been published: https://doi.org/10.1038/s41561-025-01826-w
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Acknowledgements
We thank A. Radko for help with the Raman analyses, W. Liu (Advanced Photon Source (APS), Argonne National Laboratory) and S. Atray, N. Tamura, H. Bechtel and S. Gilbert-Corder (Advanced Light Source (ALS), Lawrence Berkeley Laboratory) for help with the synchrotron beamline analyses, and E. Brosh for calculating the Fe–Ni alloy a–x relations. I. Chinn and De Beers Consolidated Mines are thanked for the donation of diamonds used in this study and R. Hamman and G. Bartlette for selecting them. We thank E. Stolper, R. Angel and A. Matthews for discussions, and A. Meltzer and O. Elazar for moral support. This research was supported by the Israel Science Foundation grant numbers 2015/18 and 779/22 to Y.W. and NSF-BSF grant number 2020639 to O.N. Use of the APS and the ALS was supported by the US DOE-BES contracts DE-AC02-06CH11357 and DE-AC02-05CH11231.
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Y.K. and Y.W. conceived of and developed the project. Y.K. performed the EPMA, FTIR and Raman analyses, and Y.K. and S.R. performed STEM analyses, all at HUJI. O.T. performed the synchrotron X-ray analyses at ANL and LBL. T.J.B.H. carried out the thermodynamic calculations. Y.K. wrote the first draft of the paper and together with Y.W. wrote the present version. S.R. and O.T. helped describe the STEM and X-ray methods and results, and Y.K., T.J.B.H. and O.N. described the thermodynamic calculations. All authors contributed intellectually to the paper.
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Extended data
Extended Data Fig. 2 X-ray diffraction (XRD) spectrum of the inclusions in the diamond clouds.
a. ON-VRS-664 shows three major lines that fit those of δ-N2 and yield a volume of 26.37 ± 4 Å3 corresponding to pressure of 8.1 GPa at room temperature. Other peaks and shoulders fit CO2 under pressure of 8 GPa and gaspeite. Because of the difference in composition between the trapped and the reference gaspeite, no pressure could be estimated based on that phase. See Supplementary Data 2, Supplementary Fig. 2.3 for the full spectrum. b. X-ray diffraction of the high Ni concentration zone in the inclusions cloud of diamond ON-VRS-866. The lines are fitted by diffractograms of deltanitrogen (δ-N2, main phase), taenite (metallic, Ni-rich phase), and possibly Ni11N2 (or (Ni,Fe)11N2), an ordered supercell of fcc-type Ni with some sites unoccupied and some sites occupied by nitrogen.
Extended Data Fig. 3 TEM images of selected area diffraction patterns taken from a single (Ni,Fe)CO3 microinclusion at different orientations.
The solution of these diffraction patterns and the angles between their orientations are in good agreement with the crystallographic structure of trigonal NiCO3 phase with lattice parameters a = b = 4.6117 Å, c = 14.735 Å (ICSD# 61067)65. Pattern of ZA [0001] contain double diffraction due to orientation relationship between diamond and gaspeite crystal structure. Additional diffraction patterns are presented in Supplementary Data 4, Supplementary Figs. 4.3-4.5.
Extended Data Fig. 4 Raman spectra of mineral inclusions in diamond ON-VRS-664.
a. Coesite (a photo of one of the inclusions is shown). All spectra are shifted from the one-atmosphere peak at ~520 cm−1 (RRUFF #X050094). b. Ulvöspinel – the Raman spectrum is very close to that of a synthetic ulvöspinel (Fe2TiO4)24. The spectrum of magnetite (RRUFF Project database number R060191) is shown for comparison. c. Na-Al pyroxene – the upper left inclusion in the photo. Raman peaks at 362, 681 and 1020 cm−1 resemble those of a high-pressure Na-Al pyroxene11 at 348, 680 and 1021 cm−1; the two peaks at 825 and 857 cm−1 fit those of olivine (RRUFF Project database number X050085), suggesting that the two phases co-occupy the inclusion. d. The Raman spectrum was collected before the inclusion was exposed. Two of the peaks fall close to two of the four peaks associated with a Na-NAL phase28, the other two do not show in the present spectrum of the K-NAL inclusions. e. A spectrum collected from the inclusion cloud in diamond ON-VRS-664. The peaks at ~1140 cm−1 correspond to the main line of Mg-gaspeite at a pressure of more than 13.6 GPa43. The photo presents a representative gaspeite microinclusion.
Extended Data Fig. 5 Pressure estimation of the diamond source.
Diamond symbols: internal pressure at room temperature (black dashed line) recorded by the various trapped phases in the inclusions. Blue diamonds: 8.4 and 8.7 GPa (shift of Raman lines) and 8.1 GPa (not shown) based on the X-ray peak. The blue lines: isochores (equal-volume lines) of fluid N2 at high pressure and temperature. The volume was determined based on the pressure in the deltanitrogen inclusions in the two diamonds and the EOS of solid δ-N234. It was extrapolated to high temperatures using the EOS of fluid N235,36. Volume change due to thermal expansion and compressibility of the diamond were neglected and would lead to somewhat higher pressure if included18. Cyan diamond: solid CO2-I at 8 GPa based on the shift of the FTIR line38 (Supplementary Data 5, Supplementary Fig. 5.2) Cyan lines: isochores for fluid CO2, using the volume calculated using the EOS of CO2-I40 and of fluid CO2 (a41, b42). Brown diamond and line: The maximum internal pressure at room temperature (3-9 GPa, by the Raman spectra) and the isomeke for coesite in diamond (the line along which the diamond and the coesite have the same P, T and volume, calculated using the software of Angel et al.44). Dashed grey line – the diamond graphite phase boundary78, Black line – the melting curve of solid N279. Orange line – the 38 mW/m2 geotherm80 connected to the mantle adiabate37. Orange thick line – the inferred possible range of pressure and temperature for the two diamonds.
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Supplementary Data
Supplementary Data 1–11, including all analysis data of the diamonds and inclusions (FTIR, EPMA, TEM, Raman, thermodynamic calculations and XRD).
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Kempe, Y., Remennik, S., Tschauner, O. et al. Redox state of the deep upper mantle recorded by nickel-rich diamond inclusions. Nat. Geosci. (2025). https://doi.org/10.1038/s41561-025-01791-4
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DOI: https://doi.org/10.1038/s41561-025-01791-4