Abstract

Basalts and peridotites from mid-ocean ridges record fO2 near the quartz-fayalite-magnetite buffer (QFM), but peridotite partial melting experiments have mostly been performed in graphite capsules (~ QFM-3), precluding evaluation of ferric iron’s behavior during basalt generation. We performed experiments at 1.5 GPa, 1350–1400 °C, and fO2 from about QFM-3 to QFM+3 to investigate the anhydrous partitioning behavior of Fe2O3 between silicate melts and coexisting peridotite mineral phases. We find spinel/melt partitioning of Fe2O3 ({D}_{mathrm{Fe}2mathrm{O}3}^{mathrm{spl}/mathrm{melt}}) increases as spinel Fe2O3 concentrations increase, independent of increases in fO2, and decreases with temperature, which is consistent with new and previous experiments at 0.1 MPa. We find {D}_{mathrm{Fe}2mathrm{O}3}^{mathrm{opx}/mathrm{melt}} = 0.63 ± 0.10 and {D}_{mathrm{Fe}2mathrm{O}3}^{mathrm{cpx}/mathrm{melt}} = 0.78 ± 0.30. MORB Fe2O3 and Na2O concentrations are consistent with a modeled MORB source with Fe2O3 = 0.48 ± 0.03 wt% (Fe3+/ΣFe = 0.053 ± 0.003) at potential temperatures (TP) from 1320 to 1440 °C. The temperature-dependence of the {D}_{mathrm{Fe}2mathrm{O}3}^{mathrm{spl}/mathrm{melt}} function alone allows ~ 40% of the variation in MORB compositions. If we allow {D}_{mathrm{Fe}2mathrm{O}3}^{mathrm{opx}/mathrm{melt}} and {D}_{mathrm{Fe}2mathrm{O}3}^{mathrm{opx}/mathrm{melt}} to also vary with temperature by tying them to spinel Fe2O3 through intermineral partitioning, then all the MORB data are within error of the model. Our model Fe2O3 concentration for the MORB source would require that the convecting mantle be more oxidized at a given depth than recorded by continental mantle xenoliths. Our result is supported by thermodynamic models of mantle with Fe3+/ΣFe = 0.03 that predict fO2 of ~ QFM-1 near the garnet-spinel transition, which is inconsistent with fO2 of MORB. Our results support previous suggestions that redox melting may occur between 200 and 250 km depth.

Highlights

  • Estimates of upper mantle oxygen fugacity and the bulk ferric iron content of the upper mantle inform petrological and geophysical models of the mantle

  • Our results suggest that F­ e2O3-Na2O systematics in MORB can be accounted for by variations in F­ e2O3 partitioning with temperature

  • All experiments contained large glass pools, similar to those pictured in Fig. 2, that allowed us to analyze glasses by Electron probe microanalysis (EPMA) and X-ray absorption near-edge structure spectroscopy (XANES) at least 100 μm away from crystals or quench mattes

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Summary

Introduction

Estimates of upper mantle oxygen fugacity (fO2) and the bulk ferric iron content of the upper mantle inform petrological and geophysical models of the mantle. The absence of a deep xenolith record from the convecting mantle forces workers to assume that the continental xenolith record (e.g., Frost and McCammon, 2008) can stand in for the fO2-depth profile of the convecting oceanic upper mantle; the absence of a deep xenolith record from the convecting mantle prevents evaluation of this assumption or even any direct assessment of the fO2 of the unmelted oceanic upper mantle. This shortfall in the geologic record highlights the importance of ridge fO2 as an anchor for modeling fO2 deeper in the convecting mantle. Even correcting for the effects of depressurization upon ascent, which are well-characterized for ascending melts (Kress and Carmichael 1991) but poorly understood for peridotites (Birner et al 2018), does not account for the redistribution of F­ e2O3 between minerals and melt during partial melting and melt extraction

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