The oxidation state of europium in silicate melts as a function of oxygen fugacity, composition and temperature
Introduction
Europium is the only rare earth element (REE) that can occur in significant proportions as an oxidation state other than REE3 + in natural silicate melts (e.g., Drake, 1975). The oxidation state of Eu is of geochemical interest because Eu2 + and Eu3 + partition differently (e.g., Drake, 1975) and thus the behaviour of Eu in a magma depends on the oxygen fugacity (f O2) and the phase(s) crystallising. Chondrite-normalised REE patterns with anomalous Eu concentrations, quantified as Eu/Eu*, are frequently observed and are attributed to the redox-variability of Eu (e.g., Morris et al., 1974a, Drake, 1975, Hoskin et al., 2000). Experimental studies have calibrated the fO2-dependency of Eu partitioning between feldspars and melt and shown DEu2 + (where Di is the ratio of the weight fraction of i in the crystal to that in the melt) to be an order of magnitude greater than DEu3 + (Aigner-Torres et al., 2007, Drake, 1975, McKay et al., 1994, Wilke and Behrens, 1999). Conversely, Eu2 + is far less compatible than REE3 + in pyroxenes (McKay et al., 1994, Wadhwa, 2001; see Eby, 1975 for exceptions). The resulting positive or negative Eu anomalies can provide an indication of crystal fractionation (e.g., Brophy and Basu, 1990, Hoskin et al., 2000). Alternately, these anomalies could be used to estimate the fO2 at which a sample crystallised. For example, the partitioning of Eu between pyroxene and melt as a function of f O2 has potential as an oxybarometer, particularly for meteoritic samples (Karner et al., 2010, McKay et al., 1994, Shearer et al., 2006). Anomalous concentrations of Eu are also commonly exhibited by zircon and similarly could record the f O2 of crystallisation (Burnham and Berry, 2012, Hoskin and Schaltegger, 2003, Trail et al., 2012).
Partitioning between feldspar, or other minerals, and melt allows the oxidation state ratio of Eu in the melt to be estimated, because the observed DEu can be modelled as an average of DSr (a proxy for DEu2 +) and DGd or DSm (a proxy for DEu3 +) weighted by the relative proportions of Eu2 + and Eu3 + in the melt (e.g., McKay et al., 1994). However, such experiments ideally require melts with a compositionally invariant phase on the liquidus and thus cannot fully address the roles of composition and temperature, as neither can be varied freely. Spectroscopic determinations of Eu3 +/Eu2 +, or Eu3 +/ΣEu where ΣEu = Eu2 + + Eu3 +, are not subject to this constraint.
151Eu (47.8% natural abundance) Mössbauer spectroscopy has been used to determine Eu3 +/ΣEu in silicate glasses (Nemov et al., 2007, Virgo et al., 1981), though the limited applications and the long spectral acquisition times (several days) have probably hampered greater uptake of this technique. Eu3 +/ΣEu can also be determined by electron paramagnetic resonance (EPR) spectroscopy (Eu2 + is EPR active), however, the method is restricted to Fe-free compositions since the resonances of other paramagnetic ions will overlap with the Eu signal (Morris et al., 1974a, Morris et al., 1974b, Schreiber, 1977).
Eu LIII-edge X-ray absorption near edge structure (XANES) spectroscopy has been used to provide information on the oxidation state ratio and coordination environment of Eu in aqueous solutions, silicate melts and minerals (Antonio et al., 1997, Cicconi et al., 2012, Karner et al., 2010, Mayanovic et al., 2007, Rakovan et al., 2001, Shearer et al., 2011). Eu2 + spectra are characterised by an intense peak (white line) at ~ 6974 eV and Eu3 + spectra by a white line at ~ 6982 eV (Rakovan et al., 2001, Shimizugawa et al., 1999, Takahashi et al., 2005). The peaks are assigned to the 2p3/2 → 5d transitions of Eu2 + and Eu3 + (Rakovan et al., 2001, Takahashi et al., 2005). The ~ 8 eV difference in energy between these features is large compared to the core hole width of 3.91 eV (Krause and Oliver, 1979), and hence for mixed valence systems the two peaks are well resolved and the relative contributions from each oxidation state can be determined. This resolution makes quantification of redox ratios potentially easier than for many other elements (e.g., Berry and O'Neill, 2004, Sutton et al., 2005). For example, Eu3 +/ΣEu has been determined with a precision of 0.01 for a sample of apatite containing only 700 ppm Eu (Rakovan et al., 2001). XANES spectroscopy can also be used to determine oxidation state ratios in situ; oxidation states present in a melt may not be preserved in a glass, even with rapid quenching, due to electron exchange reactions (Berry et al., 2006). In situ experiments on melts have suggested that electron exchange may occur between Eu and Fe (Cicconi et al., 2015).
In order to use Eu anomalies in minerals as an oxybarometer it is necessary to understand the separate effects of f O2, melt composition, and temperature on Eu3 +/ΣEu in magmas. The work of Morris et al., 1974a, Morris et al., 1974b represents the most comprehensive study to date of the controls on the oxidation state ratio of Eu in glasses, covering temperatures from 1415 to 1650 °C, 12 log units of f O2 and over 20 compositions in the system CMAS; they found that Eu3 + was stabilised by high f O2s, melt compositions with high Ca/Mg ratios, and low temperatures. More recently, XANES spectroscopy has been used to determine Eu3 +/ΣEu in a number of glass compositions equilibrated at four values of f O2, although the data were too limited to model or interpret accurately (Cicconi et al, 2012).
Here we use XANES spectroscopy to determine Eu3 +/ΣEu as a function of fO2 for a range of silicate glasses and melts, thereby extending the work of Morris et al., 1974a, Morris et al., 1974b to other melt compositions and to lower temperatures. We also use an X-ray absorption spectroscopy furnace (Berry et al., 2003) to make the first in situ determinations of Eu3 +/ΣEu in silicate melts as a function of f O2. Pressure may also affect Eu3 +/ΣEu although this variable will not be addressed here.
Section snippets
Experimental
Eleven glass compositions in the system SiO2–Al2O3–MgO–CaO, a ZrO2-bearing glass and a synthetic mid-ocean ridge basalt (MORB), all with 0.5 wt.% Eu2O3, were prepared at a range of f O2s (log f O2s from − 20 to 0 at 1400 °C, equivalent to QFM − 13.7 to QFM + 6.3, where QFM is the quartz–fayalite–magnetite f O2 buffer) and temperatures (1300–1500 °C) at atmospheric pressure. The compositions were selected to span a range of major element oxide components, and consequently compositional and structural
Results
All glasses are homogeneous and vary in colour from yellow-green (reduced) to colourless (oxidised) for the Fe-free samples, and from green (reduced) to dark brown (oxidised) for MORB. The compositions determined by electron probe microanalysis (EPMA) are given in Table 1.
Representative normalised Eu LIII-edge XANES spectra of the quenched glasses (AD) and in situ melts (MORB) are shown in Fig. 1. Spectra obtained from MORB included the Fe K-edge in the far post-edge region (~ 7115 eV) but
XANES analysis
For the reaction Eu2 +O + n/4 O2 = Eu2+nO1+n/2 it follows that Eu3 +/ΣEu should vary with f O2 according to the sigmoidal relationship:where n relates to the stoichiometric number of electrons involved in the redox reaction (i.e., n = 1 for Eu) and logK′ is a modified equilibrium constant (see Berry and O'Neill, 2004). Eq. (1) can be modified to describe any spectral feature (e.g., peak height, peak area, and centroid energy) that varies with f O2:
Discussion
For AD the average values of logK′ determined from the Eu2 + and Eu3 + peaks for both the glasses and in situ melts are identical, within error, despite the differences in the spectra. These differences are unlikely to be due to the effect of temperature (spectral broadening) because the line shapes (half width and Lorentz fraction) of the glass and melt spectra are indistinguishable. The differences in the a and c parameters between AD melt and glass corresponds to a difference in Eu3 +/ΣEu of ~
Conclusions
The widespread occurrence of Eu anomalies in minerals and rocks is generally regarded as evidence of Eu depletion due to the uptake and removal of Eu2 + by plagioclase fractionation, however, the anomalies could also arise from variable Eu3 +/ΣEu (thus reducing the activity of Eu3 + relative to the other REE3 +) and may record the f O2. This paper presents quantitative results that describe the dependence of Eu3 +/ΣEu on f O2, temperature and melt composition, which will aid the interpretation of
Acknowledgements
Beamtime awards SP3771, SP6300, SP7452 and NT5576 (DLS) and EC-657 (ESRF) are gratefully acknowledged. We thank Hugh O'Neill and Jonathan Paul for their help with collecting some of the XANES spectra, and John Spratt for assistance with the electron probe analyses. A.D.B. thanks Imperial College London for the award of a Janet Watson Scholarship and A.J.B. thanks the Australian Research Council for the award of a Future Fellowship (FT120100766).
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