Abstract

We report the results of experiments designed to separate the effects of temperature and pressure from liquid composition on the partitioning of Ni between olivine and liquid, D_{text{Ni}}^{text{ol/liq}}. Experiments were performed from 1300 to 1600 °C and 1 atm to 3.0 GPa, using mid-ocean ridge basalt (MORB) glass surrounded by powdered olivine in graphite–Pt double capsules at high pressure and powdered MORB in crucibles fabricated from single crystals of San Carlos olivine at one atmosphere. In these experiments, pressure and temperature were varied in such a way that we produced a series of liquids, each with an approximately constant composition (~12, ~15, and ~21 wt% MgO). Previously, we used a similar approach to show that D_{text{Ni}}^{text{ol/liq}} for a liquid with ~18 wt% MgO is a strong function of temperature. Combining the new data presented here with our previous results allows us to separate the effects of temperature from composition. We fit our data based on a Ni–Mg exchange reaction, which yields ln left( {D_{text{Ni}}^{text{molar}} } right) = frac{{ -Delta _{r(1)} H_{{T_{text{ref}} ,P_{text{ref}} }}^{ circ } }}{RT} + frac{{Delta _{r(1)} S_{{T_{text{ref}} ,P_{text{ref}} }}^{ circ } }}{R} - ln left( {frac{{X_{text{MgO}}^{text{liq}} }}{{X_{{{text{MgSi}}_{ 0. 5} {text{O}}_{ 2} }}^{text{ol}} }}} right). Each subset of constant composition experiments displays roughly the same temperature dependence of D_{text{Ni}}^{text{ol/liq}} (i.e.,-Delta _{r(1)} H_{{T_{text{ref}} ,P_{text{ref}} }}^{ circ } /R) as previously reported for liquids with ~18 wt% MgO. Fitting new data presented here (15 experiments) in conjunction with our 13 previously published experiments (those with ~18 wt% MgO in the silicate liquid) to the above expression gives -Delta _{r(1)} H_{{T_{text{ref}} ,P_{text{ref}} }}^{ circ } /R = 3641 ± 396 (K) and Delta _{r(1)} S_{{T_{text{ref}} ,P_{text{ref}} }}^{ circ } /R = − 1.597 ± 0.229. Adding data from the literature yields -Delta _{r(1)} H_{{T_{text{ref}} ,P_{text{ref}} }}^{ circ } /R = 4505 ± 196 (K) and Delta _{r(1)} S_{{T_{text{ref}} ,P_{text{ref}} }}^{ circ } /R = − 2.075 ± 0.120, a set of coefficients that leads to a predictive equation for D_{text{Ni}}^{text{ol/liq}} applicable to a wide range of melt compositions. We use the results of our work to model the melting of peridotite beneath lithosphere of varying thickness and show that: (1) a positive correlation between NiO in magnesian olivine phenocrysts and lithospheric thickness is expected given a temperature-dependent D_{text{Ni}}^{text{ol/liq}} , and (2) the magnitude of the slope for natural samples is consistent with our experimentally determined temperature dependence. Alternative processes to generate the positive correlation between NiO in magnesian olivines and lithospheric thickness, such as the melting of olivine-free pyroxenite, are possible, but they are not required to explain the observed correlation of NiO concentration in initially crystallizing olivine with lithospheric thickness.

Highlights

  • Unlike most other minor and trace elements, Ni is compatible in olivine over a broad range of temperatures, pressures, and silicate liquid compositions (i.e., DNoli/liq = NiOol/NiOliq is greater than one, where NiOφ refers to the concentration of NiO in phase φ by weight).One consequence of the compatibility of Ni in olivine and other mantle phases (e.g., Mysen 1978) is that the NiO contents of residual lherzolites are insensitive to low degrees of partial melting; this is consistent with the observed narrow distribution of the NiO contents of olivines from spinel lherzolites: 0.37 ± 0.03 [mean absolute deviation (MAD)], 308 analyses (Korenaga and Kelemen2000; Jun Korenaga, personal communication, 2011) and0.37 ± 0.01, 172 analyses (Herzberg et al 2013)

  • One consequence of the compatibility of Ni in olivine and other mantle phases (e.g., Mysen 1978) is that the NiO contents of residual lherzolites are insensitive to low degrees of partial melting; this is consistent with the observed narrow distribution of the NiO contents of olivines from spinel lherzolites: 0.37 ± 0.03 [mean absolute deviation (MAD)], 308 analyses (Korenaga and Kelemen 2000; Jun Korenaga, personal communication, 2011) and

  • Keeping in mind that increasing temperature can be associated with increasing pressure, the results shown in Fig. 2 confirm the conclusion of Matzen et al (2013) that, for constant liquid and olivine compositions, DNoli/liq decreases with increasing temperature and pressure

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Summary

Introduction

NiO contents exceeding 0.5 wt% (e.g., Clague et al 1991; Sobolev et al 2005, 2007) Possible explanations for these elevated NiO concentrations in olivine—and the melts from which they are derived—include an olivine-free component in the mantle produced by metasomatism of peridotite by silicic partial melts of recycled oceanic crust (Sobolev et al.2005, 2007), Ni-enrichment in the mantle source due to interaction with the Ni-rich core (Ryabchikov 2003; Herzberg et al 2013), or a DNoli/liq that is a function of temperature (T) and/or pressure (P), in addition to composition (Leeman and Lindstrom 1978; Mysen and Kushiro 1979; Li and Ripley 2010; Putirka et al 2011; Matzen et al 2013).

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