Elemental gaseous Hg is emitted into the atmosphere through
various
anthropogenic and natural processes. Mercury's different species
and
respective transport ranges, atmospheric physical and chemical transformations,
and interaction with the earth’s surfaces all contribute to
the global cycling of toxic mercury. Under sunlight, halogens, ozone,
and nitro species oxidize the emitted elemental Hg to gaseous Hg (II)
molecules, which deposit onto the snow and ice surfaces in the Arctic.
To investigate the fate of deposited mercury, a quantum chemical investigation
was conducted using first-principles density functional theory (DFT)
to analyze the interaction between various mercury molecules and snow
clusters of differing sizes. Results show that all oxidized mercury
molecules: XHgY, BrHgOX, BrHgXO XHgOH, XHgO2H, and XHgNO2, with X, Y = Cl, Br, and I atoms have thermodynamically stable
interactions with snow clusters. Further, the adsorption energy of
all mercury molecules increases with increasing size of snow clusters.
Additionally, the orientations of deposited mercury molecules on the
cluster surface also influence the mercury–snow interactions.