| Literature DB >> 30635572 |
Jin Liu1,2, Qingyang Hu3, Wenli Bi4,5, Liuxiang Yang1,6, Yuming Xiao7, Paul Chow7, Yue Meng7, Vitali B Prakapenka8, Ho-Kwang Mao9,10, Wendy L Mao11,12.
Abstract
A drastically altered chemistry was recently discovered in the Fe-O-H system under deep Earth conditions, involving the formation of iron superoxide (FeO2Hx with x = 0 to 1), but the puzzling crystal chemistry of this system at high pressures is largely unknown. Here we present evidence that despite the high O/Fe ratio in FeO2Hx, iron remains in the ferrous, spin-paired and non-magnetic state at 60-133 GPa, while the presence of hydrogen has minimal effects on the valence of iron. The reduced iron is accompanied by oxidized oxygen due to oxygen-oxygen interactions. The valence of oxygen is not -2 as in all other major mantle minerals, instead it varies around -1. This result indicates that like iron, oxygen may have multiple valence states in our planet's interior. Our study suggests a possible change in the chemical paradigm of how oxygen, iron, and hydrogen behave under deep Earth conditions.Entities:
Year: 2019 PMID: 30635572 PMCID: PMC6329810 DOI: 10.1038/s41467-018-08071-3
Source DB: PubMed Journal: Nat Commun ISSN: 2041-1723 Impact factor: 14.919
Fig. 1Representative XAS and XRS spectra of iron oxide compounds. a PFY-XAS spectra at Fe K-edge of iron oxide compounds at room temperature. Black, olive, blue, and cyan lines: Fe0, Fe2+O, Fe3+2O3, and CaFe4+O3 at ambient conditions, respectively; light and dark magenta lines: Py-FeO2 at 53 and 81 GPa, respectively; red line: Py-FeO2Hx at 133 GPa; gray arrow: the link from the dashed outline to the inset. Inset: the area zoomed for the dashed outline in Fig. 1a. b XRS spectra of Py-FeO2Hx at 110 GPa. Circles: experimental data; shaded areas: fitted peaks
Fig. 2Representative SMS spectra and hyperfine parameters. a High pressure Mössbauer spectra of FeO2Hx collected upon decompression at 300 K. Circles: experimental SMS spectra; red solid lines: modeled spectra using CONUSS program. Comparison of isomer shift (b) and quadrupole splitting (c) of iron in iron-rich compounds at high pressure and room temperature. Solid and half-filled diamonds: pyrite-structured FeO2Hx and FeO2, respectively, this study; open diamonds: pyrite FeS2 (ref. [29]); solid squares: Fe2O3, this study; open squares: Fe2O3 (ref. [58]); left-, right-, and top-pointing triangles: (Fe0.48Mg0.52)O (ref. [27]), Fe0.94O (ref. [26]), and (Fe0.25Mg0.75)O (ref. [28]), respectively; dashed lines: linear fits to experimental data. The errors on the experimental data are ±2 SD, which are smaller than symbols and not shown for clarity
Fig. 3High-pressure XES spectra of pyrite-structured FeO2Hx at 300 K. The integrated intensity of the XES spectra was normalized to unity. Inset: the satellite emission peak between 7030 and 7048 eV after the iron main emission peaks was aligned to that at 133 GPa. The changes of the satellite peak intensity in FeO2Hx are attributed to the high-spin to low-spin transition, as the disappearance of the satellite peak has been used as a robust criterion for the electronic spin-pairing transition of iron in other iron-bearing compounds[30]
Fig. 4The calculated charge density landscape of pyrite-structured FeO2 at 100 GPa. a Gold surface represents charge density of 0.15 e/Å3. The section cut through the plane shows the weak O–O bonding feature. Brown balls are Fe atoms and red balls are O atoms. b Charge density distribution projected on the plane. The level of charge density is reflected by the color bar
The valence state of Fe and O atoms from the electron charge density of Py-phase at 100 GPa and 0 K
| FeO2 | DFT + U | HSE |
|---|---|---|
| Fe | 1.62 | 1.68 |
| O | −0.81 | −0.84 |
|
| 0.367 | 0.362 |