Methylmercury in environmental compartments of a hydroelectric reservoir in the Western Amazon, Brazil.

Chemosphere

Ecology and Natural Resources Postgraduate Program, Laboratory of Environmental Sciences, Biosciences and Biotechnology Center, Norte Fluminense Darcy Ribeiro State University, Av. Alberto Lamego, 2000, Parque Califórnia, CEP 28013-602, Campos dos Goytacazes, Rio de Janeiro, Brazil.

Published: January 2019

Damming rivers to generate electricity creates a lentic environment that favors methylmercury (MeHg) formation. Reservoirs in the Amazon are critical environments for MeHg formation, considering its old soils and the use of Hg in gold mining in the region. The objective of this study was to evaluate MeHg accumulation in three environmental compartments (aquatic macrophytes, suspended particulate matter (SPM) and sediment) of the Samuel reservoir (Western Amazon, Brazil), during the low water, ebb and high water hydrological periods, characterizing the dry season, the end of the rainy season and the rainy season, respectively. MeHg concentrations were determined through GC-AFS. The aquatic macrophytes presented higher %MeHg in their roots (up to 12%) compared to their other tissues. This ratio was 1.7 and 5.9 times higher than those observed for SPM and the sediment, but MeHg concentrations were the lowest (0.5-4.5 ng g) among the three environmental compartments. Contrary, the highest MeHg concentration was observed in SPM (104 ng g) during the low water period. The MeHg concentration in the sediment profile decreased with increasing depth (0.93-0.48 ng g) and with decreasing organic matter lability (increasing C:N ratio). In the SPM, on the other hand, MeHg concentration showed a positive association with increasing C:N ratio. We conclude that MeHg dynamics in the SPM are associated with the hydrological periods, with peaks during the low water period. The organic matter lability of the sediments is more limiting to the production of MeHg than the total Hg concentrations.

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http://dx.doi.org/10.1016/j.chemosphere.2018.10.106DOI Listing

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