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Oxygen isotope biogeochemistry of pore water sulfate in the deep ...

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4224 U.G. Wortmann et al. / Geochimica et Cosmochimica Acta 71 (2007) 4221–4232567 mmol/l Cl - 567 mmol/l Cl -1300 mmol/l Cl - 1300 mmol/l Cl -Fig. 3. Isohal<strong>in</strong>e surfaces derived from <strong>in</strong>terpolation <strong>of</strong> <strong>the</strong> Cl data <strong>of</strong> Sites 1130 and 1132. The fact that <strong>the</strong> Cl concentrations stabilize at asub-horizontal level, suggests that <strong>the</strong> br<strong>in</strong>e is constantly replenished at depth, possibly by lateral advection. The horizontal distance between<strong>the</strong> two sites is about 11.6 km, seismic data courtesy <strong>of</strong> D.A. Feary.Depth [m]-50 0 500SO 4 [mM] DataH 2 S [mM] Data50δ 34 S SO 4 [ 0 / 00 VCDT] Dataδ 34 S H 2 S[ 0 / 00 VCDT] Data1001502002500 / 00[VCDT]SO 4 [mM] ModelH 2 S [mM] Modelδ 34 S SO 4 [ 0 / 00 VCDT] Modelδ 34 S H 2 S [ 0 / 00 VCDT] Model300-50 0 50[mM]Fig. 4. Wortmann et al. (2001) reported d 34 S data from ODP Site 1130 which showed an isotopic difference <strong>of</strong> more than 70‰ between coexist<strong>in</strong>gdissolved H 2 S and SO 24. They argued that under hypersulfidic conditions and <strong>in</strong> <strong>the</strong> absence <strong>of</strong> any oxidants, this difference must becaused by unusually high S-fractionation factors dur<strong>in</strong>g microbial <strong>sulfate</strong> reduction. Reaction transport model<strong>in</strong>g <strong>of</strong> this system suggests that<strong>the</strong> fractionation factor was at least 65‰ (Wortmann et al., 2001). A <strong>the</strong>oretical framework how to expla<strong>in</strong> <strong>the</strong>se large fractionation factorswas given by Brunner and Bernasconi (2005). Note that <strong>the</strong> model<strong>in</strong>g results presented <strong>in</strong> this figure have been obta<strong>in</strong>ed by <strong>the</strong> same nonsteadystate parametrization used throughout <strong>in</strong> this paper, and that Fig. 7 demonstrates that <strong>the</strong> observed d 34 S-signatures are not an artifact<strong>of</strong> <strong>the</strong> 1-D model<strong>in</strong>g approach.However, <strong>the</strong> <strong>in</strong>terstitial <strong>water</strong> data <strong>of</strong> <strong>the</strong> upper 30 mbsfat ODP Site 182 are difficult to expla<strong>in</strong> with<strong>in</strong> <strong>the</strong> framework<strong>of</strong> a steady state diagenetic model. Previous publications(Wortmann et al., 2001; Wortmann, 2006) suggestedthat <strong>the</strong> upper 30 mbsf might be affected by an unknownmix<strong>in</strong>g process. While it is difficult to envision a physicalprocess which provides for a steady state mix<strong>in</strong>g depth <strong>of</strong>30 mbsf, non-steady state mix<strong>in</strong>g by sedimentation eventsis a plausible process. Huuse and Feary (2005) suggestedthat <strong>the</strong> youngest sediments <strong>in</strong> <strong>the</strong> Great Australian Bightsediments might be contourites. Thus we assume that <strong>the</strong>sediments at Site 1130 are redeposited older sediments,which provides a plausible mechanism for sea<strong>water</strong> irrigation,and allows us for <strong>the</strong> first time, to successfully model<strong>the</strong> upper 30 mbsf <strong>of</strong> OPD Site 1130 (see Fig. 5).2. METHODSThe <strong>in</strong>terstitial <strong>water</strong> samples were taken on board <strong>the</strong>JOIDES Resolution follow<strong>in</strong>g <strong>the</strong> procedures given <strong>in</strong>

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