Deep oceans receive mercury (Hg)
from upper oceans, sediment
diagenesis,
and submarine volcanism; meanwhile, sinking particles shuttle Hg to
marine sediments. Recent studies showed that Hg in the trench fauna
mostly originated from monomethylmercury (MMHg) of the upper marine
photosynthetic food webs. Yet, Hg sources in the deep-sea chemosynthetic
food webs are still uncertain. Here, we report Hg concentrations and
stable isotopic compositions of indigenous biota living at hydrothermal
fields of the Indian Ocean Ridge and a cold seep of the South China
Sea along with hydrothermal sulfide deposits. We find that Hg is highly
enriched in hydrothermal sulfides, which correlated with varying Hg
concentrations in inhabited biota. Both the hydrothermal and cold
seep biota have small fractions (<10%) of Hg as MMHg and slightly
positive Δ199Hg values. These Δ199Hg values are slightly higher than those in near-field sulfides but
are 1 order of magnitude lower than the trench counterparts. We suggest
that deep-sea chemosynthetic food webs mainly assimilate Hg from ambient
seawater/sediments and hydrothermal fluids formed by percolated seawater
through magmatic/mantle rocks. The MMHg transfer from photosynthetic
to chemosynthetic food webs is likely limited. The contrasting Hg
sources between chemosynthetic and trench food webs highlight Hg isotopes
as promising tools to trace the deep-sea Hg biogeochemical cycle.