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VERTICAL STABILITY OF MERCURY IN HISTORIC AND PREHISTORIC SEDIMENTS FROM CLEAR LAKE, CALIFORNIA
Author(s) -
Suchanek Thomas H.,
Richerson Peter J.,
Zierenberg Robert A.,
Slotton Darell G.,
Mullen Lauri H.
Publication year - 2008
Publication title -
ecological applications
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.864
H-Index - 213
eISSN - 1939-5582
pISSN - 1051-0761
DOI - 10.1890/06-1544.1
Subject(s) - mercury (programming language) , methylmercury , sediment , geology , tailings , sedimentation , diagenesis , ecosystem , environmental science , deposition (geology) , hydrology (agriculture) , environmental chemistry , geochemistry , ecology , bioaccumulation , geomorphology , chemistry , geotechnical engineering , computer science , biology , programming language
Clear Lake, California, USA, is the site of the Sulphur Bank Mercury Mine, now a U.S. Environmental Protection Agency Superfund Site. Intermittent mining from 1873 to 1957 resulted in ∼100 Mg of mercury (Hg) being deposited into the lake's ecosystem. Sediment cores to ∼2.5 m depth (dated using 210 Pb and 14 C) represent ∼3000 years of sedimentation. Clear Lake sediments have experienced Hg deposition from anthropogenic sources (mining) during historic times (to the mid‐1900s) and geologic sources during prehistoric times (prior to the mid‐1800s). This provides a unique opportunity to evaluate hypotheses relating to (1) the influence of the mine on Hg loading to the lake and (2) the potential upward mobilization of Hg by diagenetic processes proposed by some as an alternative explanation for increased Hg concentrations at the surface of the sediment column believed to be caused by increased global atmospheric deposition. Although Hg mining began in 1873, no significant evidence of anthropogenic Hg loading was detected in cores prior to open‐pit mining ca. 1927, which also involved bulldozing mine waste rock and tailings into the lake. Exponential increases in total Hg (TotHg) and methylmercury (MeHg) were observed above the 1927 horizon, where estimated sedimentation rates were 2.2–20.4 mm/yr and peaks of both forms of Hg maintained vertical stability within the sediment column. Below the 1927 horizon, a slow increase in both TotHg and MeHg with depth was observed from ∼1000 to 3000 years before present, where sedimentation rates ranged from ∼0.6 to 2.0 mm/yr and elevated Hg profiles appear stable. Vertical stability of Hg in the shallow and deep sediment column suggests that both TotHg and MeHg do not undergo diagenetic upward mobilization within the sediment column under rapid or slow sedimentation rates. Because (1) these data were collected at a site with known anthropogenic and geologic sources and (2) regions of elevated Hg concentrations from both sources remain stable within the sediment column under very different sedimentation regimes, these results also support the hypothesis that elevated Hg at the surface of cores in other worldwide locations likely represents global atmospheric deposition rather than upward diagenetic mobilization.