Atmospheric source of mercury to the ocean constrained by isotopic model.
basic_science · Level V
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- Record sourced from PubMed, PMID 40595712.
- Also identified by DOI 10.1038/s41467-025-60981-1 and PMC identifier 12217555.
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Abstract
Mercury is a potent neurotoxin that poses significant health risks to humans, primarily through seafood consumption. Atmospheric deposition is the largest source of oceanic mercury, in either oxidized (Hg<sup>II</sup>) or elemental (Hg<sup>0</sup>) form. Understanding the relative contributions of atmospheric Hg<sup>II</sup> and Hg<sup>0</sup> to the ocean is essential for accurately assessing global mercury budgets. Earlier even mercury isotope (Δ<sup>200</sup>Hg) analyses suggested equivalent Hg<sup>II</sup>/Hg<sup>0</sup> contributions but neglected spatial variations in atmospheric Δ<sup>200</sup>Hg signatures. Here, we developed a 3D atmospheric model incorporating mercury chemistry and isotopic fractionation to address this limitation. Our simulations reveal distinct atmospheric Δ<sup>200</sup>Hg patterns and quantify their deposition to the ocean. Constrained by observed Δ<sup>200</sup>Hg data in the ocean, we propose an updated deposition ratio of atmospheric Hg<sup>II</sup> to Hg<sup>0</sup> to the ocean, which may exceed 2:1, higher than the previously reported 1:1. Our findings are crucial for assessing atmospheric mercury dispersal and predicting the recovery of marine ecosystems.