Mercury Speciation by X-ray Absorption Fine Structure Spectroscopy and Sequential Chemical Extractions:  A Comparison of Speciation Methods

Christopher S. Kim,* Nicolas S. Bloom, James J. Rytuba,§ and Gordon E. Brown, Jr.
Surface and Aqueous Geochemistry Group, Department of Geological and Environmental Sciences, Stanford University, Stanford, California 94305-2115, Frontier Geosciences, 414 Pontius North, Seattle, Washington 98109, U.S. Geological Survey, 345 Middlefield Road, MS 901, Menlo Park, California 94025, and Stanford Synchrotron Radiation Laboratory, SLAC, 2575 Sand Hill Road, MS 99, Menlo Park, California 94025
Environ. Sci. Technol., 2003, 37 (22), pp 5102–5108
DOI: 10.1021/es0341485
Publication Date (Web): October 22, 2003
Copyright © 2003 American Chemical Society

Abstract

Determining the chemical speciation of mercury in contaminated mining and industrial environments is essential for predicting its solubility, transport behavior, and potential bioavailability as well as for designing effective remediation strategies. In this study, two techniques for determining Hg speciationX-ray absorption fine structure (XAFS) spectroscopy and sequential chemical extractions (SCE)are independently applied to a set of samples with Hg concentrations ranging from 132 to 7539 mg/kg to determine if the two techniques provide comparable Hg speciation results. Generally, the proportions of insoluble HgS (cinnabar, metacinnabar) and HgSe identified by XAFS correlate well with the proportion of Hg removed in the aqua regia extraction demonstrated to remove HgS and HgSe. Statistically significant (>10%) differences are observed however in samples containing more soluble Hg-containing phases (HgCl2, HgO, Hg3S2O4). Such differences may be related to matrix, particle size, or crystallinity effects, which could affect the apparent solubility of Hg phases present. In more highly concentrated samples, microscopy techniques can help characterize the Hg-bearing species in complex multiphase natural samples.

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History

  • Published In Issue November 15, 2003
  • Received for review February 19, 2003
    Revised manuscript received August 12, 2003
    Accepted August 28, 2003

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