Abstract

The extent of lithological heterogeneity in the Earth's convecting mantle is highly debated. Whilst the presence of pyroxenite in the mantle source regions of Ocean Island Basalts (OIBs) has traditionally been constrained using the minor-element chemistry of olivine phenocrysts, recent studies have shown that the Ni and Mn contents of primitive olivines are influenced by the conditions of mantle melting, as well as magma chamber processes. Nevertheless, constraining the lithological properties of the mantle is important due to its influence on the P-T path followed by solid mantle material during adiabatic ascent, as well as the density of upwelling mantle plumes. We have therefore explored the use of Fe-isotopes as a novel method of tracing lithological heterogeneity in the mantle source regions beneath plume-influenced segments of the global Mid-Ocean Ridge system as well as OIBs.We present new Fe-isotope (δ56Fe) and trace-element data for 26 basaltic glasses from the plume-influenced Galápagos Spreading Centre to investigate the relative roles of pyroxenite and peridotite in the mantle source region of oceanic basalts. Our data reveals significant heterogeneity in the Fe-isotope composition of the Galápagos Spreading Centre basalts (+0.05 to +0.25‰ δ56Fe), which correlates with key major- and trace-element parameters (e.g. CaO(8)/Al2O3(8), [La/Sm]n). Application of new models developed to calculate Fe-isotope fractionation during mantle melting, alongside Monte Carlo simulations for melting of a 2-component peridotite mantle, show that this variation cannot be caused by changes in melting processes and/or oxygen fugacity of a peridotitic mantle. Instead, our new δ56Fe data is best explained by variations in the proportion of isotopically-heavy pyroxenite-derived melt that contributes to the GSC basalts, and conclusively shows that lithological heterogeneity exists in the Galápagos mantle plume. Our findings have implications for the moderately-heavy δ56Fe compositions measured in plume-influenced basalts from the Society Islands, Rochambeau Ridges of the Lau back-arc basin, and the FAMOUS segment of the Mid-Atlantic Ridge, which we suggest may also represent contribution from pyroxenite-derived melts.

Highlights

  • 35 Seismic tomography and distinctive geochemical signatures of Ocean Island Basalts (OIBs) and Mid36 Ocean Ridge Basalts (MORBs) provide compelling evidence for recycling of lithospheric components into the convecting mantle, and subsequent incorporation of this material into upwelling mantle plumes (Hofmann, 1997; van der Hilst et al, 1997)

  • Here we investigate the use of stable Fe-isotopes (δ56Fe) as an alternative method for identifying lithological heterogeneity in the mantle source region of oceanic basalts (Konter et al, 2016; Nebel et al., 2019; Williams and Bizimis, 2014)

  • 205 Clear differences are seen in the major-element systematics of D-MORBs, N-MORBs, and E206 MORBs from the Galápagos Spreading Centre (GSC)

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Summary

Introduction

35 Seismic tomography and distinctive geochemical signatures of Ocean Island Basalts (OIBs) and Mid Ocean Ridge Basalts (MORBs) provide compelling evidence for recycling of lithospheric components into the convecting mantle, and subsequent incorporation of this material into upwelling mantle plumes (Hofmann, 1997; van der Hilst et al, 1997). Incorporation of recycled oceanic lithosphere into the convecting mantle is widely believed to result in the presence of lithologically-distinct components via high-pressure melting of eclogite (metamorphosed remnants of recycled slabs), and subsequent reaction of these melts with surrounding peridotite (Sobolev et al, 2007) This results in the formation of pyroxene-rich (and highly fusible) components in the mantle (pyroxenite; Sobolev et al, 2007; Yaxley and Green, 1998). These methods are subject to considerable uncertainties regarding: (i) the influence of temperature, pressure, and oxygen fugacity (fO2) during mantle melting (Matzen et al, 2017b); and (ii) the influence that crustal processes may play (Gleeson and Gibson, 2019). It is still uncertain whether Ca, Ni, and Mn concentrations in magmatic olivines can be used, unambiguously, to distinguish between peridotite and pyroxenite derived melts and it is important to develop additional tracers for pyroxenite melting (Gleeson and Gibson, 2019; Matzen et al, 2017b, 2017a; Putirka et al, 2011; Rhodes et al, 2012)

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