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The AAPG/Datapages Combined Publications Database

Journal of Sedimentary Research (SEPM)

Abstract


Journal of Sedimentary Research
Vol. 80 (2010), No. 11. (November), Pages 943-954
Research Articles: Paleosols

Micromorphology and Stable-Isotope Geochemistry of Historical Pedogenic Siderite Formed in PAH-Contaminated Alluvial Clay Soils, Tennessee, U.S.A.

Steven G. Driese, Greg A. Ludvigson, Jennifer A. Roberts, David A. Fowle, Luis A. Gonzalez, Jon Jay Smith, Vijay M. Vulava, Larry D. McKay

Abstract

Alluvial clay Previous HitsoilNext Hit samples from six boreholes advanced to depths of 400–450 cm (top of limestone bedrock) from the Chattanooga Coke Plant (CCP) site were examined micromorphologically and geochemically in order to determine if pedogenic siderite (FeCO3) was present and whether siderite occurrence was related to organic contaminant distribution. Samples from shallow depths were generally more heavily contaminated with polycyclic aromatic hydrocarbons (PAHs) than those at greater depth. The upper 1 m in most boreholes consisted of mixtures of anthropogenically remolded clay Previous HitsoilNext Hit fill containing coal clinker, cinder grains, and limestone gravel; most layers of coarse fill were impregnated with creosote and coal tar. Most undisturbed Previous HitsoilNext Hit (below 1 m depth) consisted of highly structured clays exhibiting fine subangular blocky ped structures, as well as redox-related features. Pedogenic siderite was abundant in the upper 2 m of most cores and in demonstrably historical (< 100 years old) Previous HitsoilTop matrices. Two morphologies were identified: (1) sphaerosiderite crystal spherulites ranging from 10 to 200 μm in diameter, and (2) coccoid siderite comprising grape-like “clusters” of crystals 5–20 μm in diameter. The siderite, formed in both macropores and within fine-grained clay matrices, indicates development of localized anaerobic, low-Eh conditions, possibly due to microbial degradation of organic contaminants. Stable-isotope compositions of the siderite have δ13C values spanning over 25‰ (+7 to −18‰ VPDB) indicating fractionation of DIC by multiple microbial metabolic pathways, but with relatively constant δ18O values (−4.8 ± 0.66‰ VPDB) defining a meteoric sphaerosiderite line (MSL). Calculated isotope equilibrium water δ18O values from pedogenic siderites at the CCP site are from 1 to 5 per mil lighter than the groundwater δ18O values that we estimate for the site. If confirmed by field studies in progress, this observation might call for a reevaluation of low-temperature siderite-water 18O fractionations. Investigations at the CCP site thus provide valuable information on the geochemical conditions under which siderite can form in modern soils, and thus insight on controls on siderite formation in ancient soils.


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