Microbial stable isotope fractionation of mercury: A synthesis of present understanding and future directions

Abstract

Mercury (Hg) is a trace metal with potentially serious public health consequences, especially when its neurotoxic form, monomethylmercury (MMHg), accumulates in aquatic and terrestrial food chains. Given the variation in Hg stable isotope abundances (up to 6‰ in δ202/198Hg and 11‰ in Δ201/198Hg) in natural environmental samples and evidence for Hg isotopic fractionation during microbial (e.g., reduction of Hg(II), degradation and formation of MMHg) and abiotic processes (e.g., photo-degradation of MMHg and volatilization, evaporation and diffusion of Hg(0)), Hg isotope biogeochemistry is currently being developed as a tool to study sources, sinks, and transformations of Hg in the environment. The use of Hg stable isotopes to identify sources of MMHg in aquatic and terrestrial food chains depends on the knowledge of reasonably precise fractionation factors for individual Hg transformations that influence speciation and accumulation of Hg. Microbial transformations are critical to the formation of MMHg and Hg(0) and to the degradation of MMHg. This article a) highlights the importance of experimental determination of microbial fractionation factors for the development of Hg stable isotope systematics because of the limitations of theoretical calculations; b) provides a summary of the current understanding of microbial stable isotope fractionation of Hg, especially during kinetically controlled processes; and c) demonstrates the various factors likely to affect cell-level fractionation during microbial transformations through use of an iterative finite-step model. We also identify future directions, conditions and controls that could help rigorously advance the development of mass-dependent Hg isotope systematics at the enzymatic, cellular and ecosystem level.