The Fe3+/ΣFe ratios of MORB glasses and their implications for mantle melting

The Fe3+/SigmaFe ratio of 104 MORB glasses from the Pacific, the Atlantic, the Indian, and the Red Sea spreading centers have been determined using wet chemical Fe2+ analyses and electron microprobe FeOtotal measurements. The data provide a new estimate for the MORB oxygen fugacity (fO(2)) of 0.41 +/- 0.43 (tsigma, N = 100) log units below the fayalite-magnetite-quartz buffer (FMQ), equivalent to a Fe3+/SigmaFe = 0.12 +/- 0.02 (1sigma, N = 104). This new fO(2) estimate is 0.8 log units more oxidized than the average fO(2) proposed by Christie et al. (1986) (FMQ-1.20 +/- 0.44; Fe3+/SigmaFe = 0.07 +/- 0.01; N = 87). This slight difference may be related in part to the 3.5% underestimation of the Fe2+ concentration determined by Christie et al. (1986) compared with this study. MORB oxygen fugacity does not display any significant difference between the three main oceanic domains, or between enriched and depleted MORB. Yet. the iron red-ox State ratio shows a broad increase during fractional crystallization. Detailed study of magmatic suites highlights the lack of systematic Fe3+/SigmaFe ratio fractionation during differentiation. Despite the large variations of inferred partial melting degrees (from 5 to 20%), the present data set does not provide any evidence of Fe3+/SigmaFe relationships with partial melting proxies such as Na-8.0. Based on the Fe3+ systematics during partial melting, it is suggested that the oxidation state of MORB reflects a "buffered mantle melting process" resulting in the apparent compatible behavior of Fe3+ durings partial melting, and in the relatively constant Fe3+/SigmaFe ratio irrespective of the extent of melting. This result implies that partial melting processes may be open relative to oxygen. We propose a model where the Fe3+/SigmaFe ratio in the melt is buffered during partial melting. The MORB Fe2O3 systematics can be accounted for by using a fO(2) of FMQ-1 that is equivalent to the average fO(2) reported for abyssal peridotites. Copyright (C) 2005 Elsevier Ltd.