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Published May 1, 2007 | Supplemental Material
Journal Article Open

Rare sulfur and triple oxygen isotope geochemistry of volcanogenic sulfate aerosols

Abstract

We present analyses of stable isotopic ratios ^(17)O/^(16)O, ^(18)O/^(16)O, ^(34)S/^(32)S, and ^(33)S/^(32)S, ^(36)S/^(32)S in sulfate leached from volcanic ash of a series of well known, large and small volcanic eruptions. We consider eruptions of Mt. St. Helens (Washington, 1980, ∼1 km^3), Mt. Spurr (Alaska, 1953, <1 km3), Gjalp (Iceland, 1996, 1998, <1 km^3), Pinatubo (Phillipines, 1991, 10 km^3), Bishop tuff (Long Valley, California, 0.76 Ma, 750 km^3), Lower Bandelier tuff (Toledo Caldera, New Mexico, 1.61 Ma, 600 km^3), and Lava Creek and Huckleberry Ridge tuffs (Yellowstone, Wyoming, 0.64 Ma, 1000 km^3 and 2.04 Ma 2500 km^3, respectively). This list covers much of the diversity of sizes and the character of silicic volcanic eruptions. Particular emphasis is paid to the Lava Creek tuff for which we present wide geographic sample coverage. This global dataset spans a significant range in δ^(34)S, δ^(18)O, and Δ^(17)O of sulfate (29‰, 30‰, and 3.3‰, respectively) with oxygen isotopes recording mass-independent (Δ^(17)O > 0.2‰) and sulfur isotopes exhibiting mass-dependent behavior. Products of large eruptions account for most of' these isotopic ranges. Sulfate with Δ^(17)O > 0.2‰ is present as 1–10 μm gypsum crystals on distal ash particles and records the isotopic signature of stratospheric photochemical reactions. Sediments that embed ash layers do not contain sulfate or contain little sulfate with Δ^(17)O near 0‰, suggesting that the observed sulfate in ash is of volcanic origin. Mass-dependent fractionation of sulfur isotopic ratios suggests that sulfate-forming reactions did not involve photolysis of SO2, like that inferred for pre-2.3 Ga sulfates from Archean sediments or Antarctic ice-core sulfate associated with few dated eruptions. Even though the sulfate sulfur isotopic compositions reflect mass-dependent processes, the products of caldera-forming eruptions display a large δ^(34)S range and exhibit fractionation relationships that do not follow the expected equilibrium slopes of 0.515 and 1.90 for ^(33)S/^(32)S vs. ^(34)S/^(32)S and ^(36)S/^(32)S vs. ^(34)S/^(32)S, respectively. The data presented here are consistent with modification of a chemical mass-dependent fractionation of sulfur isotopes in the volcanic plume by either a kinetic gas phase reaction of volcanic SO_2 with OH and/or a Rayleigh processes involving a residual Rayleigh reactant—volcanic SO_2 gas, rather than a Rayleigh product. These results may also imply at least two removal pathways for SO_2 in volcanic plumes. Above-zero Δ^(17)O values and their positive correlation with δ^(18)O in sulfate can be explained by oxidation by high-δ^(18)O and high-Δ^(17)O compounds such as ozone and radicals such as OH that result from ozone break down. Large caldera-forming eruptions have the highest Δ^(17)O values, and the largest range of δ^(18)O, which can be explained by stratospheric reaction with ozone-derived OH radicals. These results suggest that massive eruptions are capable of causing a temporary depletion of the ozone layer. Such depletion may be many times that of the measured 3–8% depletion following 1991 Pinatubo eruption, if the amount of sulfur dioxide released scales with the amount of ozone depletion.

Additional Information

© 2007 Elsevier Ltd. Received 25 April 2006; accepted in revised form 29 January 2007; available online 8 February 2007. Associate editor: Thomas Chacko. We thank John Fournelle, John Pallister, and Olgeir Sigmarsson for sample donation, Kelli McCormick for help during S. Dakota field sampling, Art Bettis for Iowa and Nebraska sampling assistance, and Lena Bogolyubova for help with California sampling. John Valley for long-term collaboration on Yellowstone, Simon Poulson for analyses of barite for sulfur isotopes, Pat Shanks for providing barite standards, Axel Schmitt for trying barite analyses by SIMS, Nathan Dalleska for ICP-MS analyses of leachate solutions, and Paul Engelking for analysis of solutions using an ion chromatograph. Alex Pavlov and Jim Lyons are thanked for discussions on the atmospheric chemistry of sulfur and oxygen. University of Oregon (EAR-0537872 IB), Caltech (EAR-0345905 JE) are thanked for support of fieldwork and oxygen isotope analyses. Work at the University of Maryland was funded by EAR-0348382, NAG51235, and a fellowship of the Hanse Wissenschaftsk olleg (J.F.), as well as NNG05GF86G and NNG05GQ96G (J.F., B.A.W.). Reviews of two anonymous reviewers and Alex Pavlov, and editorial handling by Tom Chacko are acknowledged.

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