We investigate the relationship between sulfur and oxygen fugacity at Erta Ale and Masaya volcanoes. Oxygen fugacity was assessed utilizing Fe 3+ /∑Fe and major element compositions measured in olivine‐hosted melt inclusions and matrix glasses. Erta Ale melts have Fe 3+ /∑Fe of 0.15–0.16, reflecting f O 2 of ΔQFM 0.0 ± 0.3, which is indistinguishable from f O 2 calculated from CO 2 /CO ratios in high‐temperature gases. Masaya is more oxidized at ΔQFM +1.7 ± 0.4, typical of arc settings. Sulfur isotope compositions of gases and scoria at Erta Ale (δ 34 S gas − 0.5‰; δ 34 S scoria + 0.9‰) and Masaya (δ 34 S gas + 4.8‰; δ 34 S scoria + 7.4‰) reflect distinct sulfur sources, as well as isotopic fractionation during degassing (equilibrium and kinetic fractionation effects). Sulfur speciation in melts plays an important role in isotope fractionation during degassing and S 6+ /∑S is <0.07 in Erta Ale melt inclusions compared to >0.67 in Masaya melt inclusions. No change is observed in Fe 3+ /∑Fe or S 6+ /∑S with extent of S degassing at Erta Ale, indicating negligible effect on f O 2 , and further suggesting that H 2 S is the dominant gas species exsolved from the S 2− ‐rich melt (i.e., no redistribution of electrons). High SO 2 /H 2 S observed in Erta Ale gas emissions is due to gas re‐equilibration at low pressure and fixed f O 2. Sulfur budget considerations indicate that the majority of S injected into the systems is emitted as gas, which is therefore representative of the magmatic S isotope composition. The composition of the Masaya gas plume (+4.8‰) cannot be explained by fractionation effects but rather reflects recycling of high δ 34 S oxidized sulfur through the subduction zone.
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Moor et al. (2013) studied this question.
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