Comparative effects of mercury contamination and wastewater effluent input on Gram-negative merA gene abundance in mudflats of an anthropized estuary (Seine, France): a microcosm approach.

The macrotidal Seine estuary (France) is one of the most man-altered and mercury-contaminated European estuaries. Molecular quantification by competitive PCR has shown that the highest quantities of Gram-negative merA genes in intertidal freshwater mudflat sediments are located in recent sediment deposits independently of mercury concentrations, suggesting that particle-attached allochtonous mercury-resistant merA bacteria are deposited on mudflat surfaces. To investigate this hypothesis, a microcosm experiment was carried out to evaluate the respective contributions of (i) the input of allochtonous merA bacteria supplied by WWTP-treated effluents and (ii) merA gene abundance corresponding to a response of the sediment's autochthonous bacterial community to mercury contamination. Gram-negative merA gene quantification and T-RFLP analysis of both 16S rDNA and merA genes demonstrated that deposited allochtonous bacteria did not develop in estuarine sediments, whereas mercury contamination (10microg g(-1) wet sediment) selected an autochthonous mercury-resistant merA bacterial community. Thus, in mudflats of highly anthropized macrotidal estuaries, i.e. those subjected to intense hydrosedimentary processes and continuously contaminated by mercury and fecal bacteria, inputs of allochtonous merA bacteria are largely responsible for the high quantities of merA genes on the surface of mudflat sediments.