T137 Mercury Cycling, Fate, and Bioaccumulation in Coastal Zones: The Next Big Stage for Mercury Research?
Sunday, 5 October 2008
8:00 AM - 12:00 PM
Mercury Isotopic Composition of Marine Sediments in the Baltic Sea
Paper number: T137-13
Program: Technical Sessions
Time: 11:00 AM – 11:15 AM
Authors
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J.D. BlumUniversity of Michigan, Ann Arbor, MI
Abstract
Mass dependent (d202Hg) and mass independent (Δ199Hg) variation in the isotopic composition of Hg has been observed in a wide range of natural materials. In this study we measured the Hg isotopic composition of marine sediments from the Baltic Sea that predate and post-date the Industrial Revolution to see whether anthropogenic inputs of Hg had altered the isotopic composition of the sediments. We analyzed surface (0-4 cm) and pre-Industrial (24-34 cm) sediments from spatially distributed, hydrographically separated locations in the Baltic Sea. Sediments from the Baltic Proper and Arkona basins demonstrate a three-fold enrichment in Hg concentration between pre-Industrial and post-Industrial sediments, with Hg concentrations increasing from an average of 19 ng/g to 51 ng/g in the Baltic Proper basin and from 51 ng/g to 155 ng/g in the Arkona basin. All sediments analyzed have a narrow range of d202Hg and Δ199Hg values. Deeper sediments from the two basins have d202Hg values ranging from -1.2‰ to -0.9‰ and Δ199Hg values of +0.14‰ to +0.15‰. Near-surface sediments from each site have d202Hg values ranging between -0.9‰ and -0.8‰ and Δ199Hg values of +0.09‰. The sediments analyzed have indistinguishable Hg isotopic compositions within analytical uncertainty (d202Hg = ±0.1‰, Δ199Hg = ±0.05‰). The isotopic composition of Baltic Sea sediments is nearly identical to mid-Pleistocene Mediterranean Sea marine sediments. The similar Hg isotopic composition of these marine sediments deposited at different times and locations suggests a characteristic marine Hg isotopic signature preserved in sediments of d202Hg » -0.9‰ and Δ199Hg » +0.1‰. Implications of this isotopic signature for global Hg cycling will be discussed.