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Properly interpret metabolic inhibition results to identify primary mercury methylating microbes

, , , , , , , , & ORCID Icon show all
Pages 1757-1773 | Published online: 24 Feb 2023
 

Abstract

Distinguishing the respective contributions of various microbes to methylmercury (MeHg) production is critical for predicting MeHg bioaccumulation and exposure risk. Metabolic inhibitors have been commonly used to block the activity of specific microbial groups and identify primary Hg methylating microbes. By reviewing literatures and our empirical data, we demonstrate how multiple factors, including (1) the addition of inappropriate amounts of inhibitors, (2) a tendency to overlook microbial syntrophy, and (3) the absence of comprehensive proxy systems of Hg methylation, would impact result interpretation of this approach. We thus suggest that the design of inhibition assays should consider the environmental properties, e.g., background levels of electron acceptors, concentrations of metabolic substrates, and abundances of Hg methylating microbes. We also recommend that inhibitors should be added at multiple concentrations and that observed changes in Hg methylation should be assessed with comprehensive indicators. Revealing the key factors responsible for the improper usage of this method and inadequate interpretation of the results would help optimize inhibition assays for robust predictions of MeHg production in nature.

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Disclosure statement

The authors have no competing or conflicting interests in relation to the issues tackled in this paper.

Correction Statement

This article has been corrected with minor changes. These changes do not impact the academic content of the article.

Additional information

Funding

This work was supported by the Natural Science Foundation of Jiangsu Province10.13039/501100004608 (BK20200322), the National Natural Science Foundation of China10.13039/501100001809 (42107383, U2032201), and the Scientific research start-up fund for high-level talents of Nanjing Normal University (184080H202B357).

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