Published June 12, 2024 | Version v1
Journal article Open

High Sodium Solubility in Magnesiowüstite in Iron-Rich Deep Lower Mantle

  • 1. Michigan State University
  • 2. National Central University
  • 3. Mediatek
  • 4. Ecole polytechnique fédérale de Lausanne
  • 5. University of Chicago

Description

(Mg,Fe)O ferropericlase-magnesiowüstite has been proposed to host the majority of Earth's sodium, but the mechanism and capacity for incorporating the alkali cation remain unclear. In this work, experiments in the laser-heated diamond anvil cell and first-principles calculations determine the solubility of sodium and favorability of sodium incorporation in iron-rich magnesiowüstite relative to (Mg,Fe)SiO3 bridgmanite. Reaction of Mg/(Mg + Fe) (Mg#) 55 and 28 olivine with NaCl at 33–128 GPa and 1600–3000 K produces iron-rich magnesiowüstite containing several percent sodium, while iron-rich bridgmanite contains little to no detectable sodium. In sodium-saturated magnesiowüstite, sodium number [Na/(Na + Mg + Fe)] is 2–5 atomic percent at pressures below 60 GPa and drastically increases to 10–20 atomic percent at deep lower mantle pressures. For these two compositions, there is no significant dependence of the results on Mg#. Our calculations not only show consistent results with experiments but further indicate that such an increase in solubility and partitioning of Na into magnesiowüstite is driven by the spin transition in iron. These results provide fundamental constraints on the crystal chemistry of sodium at lower-mantle conditions. If the sodium capacity of (Mg,Fe)O is not strongly dependent on Mg#, (Mg,Fe)O in the lower mantle may have the capacity to store the entire sodium budget of the Earth.

Data availability

In this work, all calculations are performed using the Quantum ESPRESSO (QE) codes, as described in Section 2 Materials and Methods. QE is an open-source package and can be downloaded for free (Giannozzi et al., 2009, 2017). Detailed information for the compilation and installation of QE can be found on the project webpage. Example input/output files of our calculations, data used to plot Figure 7, and a brief description of the data are available at Zenodo (Hsu, 2023). All composition data obtained by energy-dispersive X-ray spectroscopy and plotted in Figures 4 and 5 are available as Data Set S1.

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Additional details

Identifiers

DOI
10.1029/2023GC011390
Other
oai:uchicago.tind.io:12655

Funding

Swiss National Science Foundation
PMPDP2_151256
National Science Foundation
EAR-1751664
National Science Foundation
EAR-2242904
National Science and Technology Council of Taiwan
NSTC 112-2112-M-008-038
National Science and Technology Council of Taiwan
111-2112-M-008-032
National Science and Technology Council of Taiwan
MOST 110-2112-M-008-033
Sorbonne Paris Cité
UnivEarthS Labex program
Sorbonne Paris Cité
UnivEarthS Labex program

UChicago Information

Division(s)
Physical Sciences Division
Center(s) or Institute(s)
Center for Advanced Radiation Sources