Mercury
(Hg) is a globally spread trace metal due to its long atmospheric
residence time. Yet, our understanding of atmospheric processes (e.g.,
redox reactions and deposition) driving Hg cycling is still limited,
especially in polar regions. The Antarctic continent, by virtue of
its remoteness, is the perfect location to investigate Hg atmospheric
processes in the absence of significant local anthropogenic impact.
Here, we present the first 2 year record (2016–2017) of total
suspended particulate mercury (PHg) concentrations along with a year-round
determination of an Hg stable isotopic composition in particles collected
at Zhongshan Station (ZSS), eastern Antarctic coast. The mean PHg
concentration is 21.8 ± 32.1 pg/m3, ranging from 0.9
to 195.6 pg/m3, and peaks in spring and summer. The negative
mass-independent fractionation of odd Hg isotopes (odd-MIF, average
−0.38 ± 0.12‰ for Δ199Hg) and
the slope of Δ199Hg/Δ201Hg with
0.91 ± 0.12 suggest that the springtime isotope variation of
PHg is likely caused by in situ photo-oxidation and reduction reactions.
On the other hand, the increase of PHg concentrations and the observed
odd-MIF values in summer are attributed to the transport by katabatic
winds of divalent species derived from the oxidation of elemental
Hg in the inland Antarctic Plateau.