Mt. Etna is a major natural source of Hg to the Mediterranean region. Total mercury concentrations, [Hg]tot, in
Castanea sativa (sweet chestnut) leaves sampled 7–13 km from Etna's vents (during six campaigns in
2005–2011) were determined using atomic absorption spectroscopy. [Hg]tot in C. sativa was greatest on
Etna's SE flank reflecting Hg deposition from the typically overhead volcanic plume. [Hg]tot also showed Hg
accumulation over the growing season, increasing with leaf age and recent eruptive activity. [Hg]tot in C.
sativa was not controlled by [Hg]tot in soils, which instead was greatest on Etna's NW flank, and was
correlated with the proportion of organic matter in the soil (% Org). An elevated [Hg]tot/% Org ratio in soils on
Etna's SE flank is indicative of increased Hg deposition. This ratio was also found to decrease with local soil
pH, suggesting that Hg deposited to the low pH and organic-poor soils on Etna's SE flank may not be retained
but will instead be released to groundwater or re-emitted to the atmosphere. These results show that the
deposition of volcanic Hg
