H2020Individual fellowship2015–2017

MEROXRE · Understanding the fate of Arctic atmospheric mercury (Hg) deposition – A Hg stable isotope investigation of redox processes and Hg re-emissions

Horizon 2020 — Marie Skłodowska-Curie Actions

Duration
2015-04-01 → 2017-03-31
EU contribution
€173,076
Participants
1
Scheme
MSCA-IF

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Results in brief

Understanding the fate of Arctic atmospheric mercury (Hg) deposition – A Hg stable isotope investigation of redox processes and Hg re-emissions

Mercury (Hg) is a pollutant of global concern for human and ecosystem health. This is particularly true in the Arctic where indigenous populations are excessively exposed to dietary Hg from fish and marine mammal consumption. The deposition of Hg from the atmosphere to Earth surfaces and its re-emission via biogeochemical reduction processes determine Hg concentrations in Earth surface reservoirs, such as soils, snow, and runoff into Arctic lakes and surface Ocean. Stable Hg isotopes are a promising new tool to identify the dominant pathways of atmospheric Hg deposition and potential re-emission processes. We investigated the Hg isotope signatures of different plant species, organic and mineral soil horizons and bedrock of the Arctic tundra at Toolik Field Station, Alaska. We measured stable Hg isotope signatures of atmospheric Hg0, Hg0 in interstitial snow and soil air and Hg in snow, representing atmospheric HgII scavenged during snowfall or deposited during halogen-driven atmospheric mercury depletion events (AMDE). The results suggest that vegetation uptake of gaseous elemental mercury from the atmosphere is the dominant deposition pathway to the terrestrial ecosystem, and contributes about 70% to Hg in organic soils. We have observed large mass-independent Hg isotope anomalies in snow during spring, with minimal D199Hg values of -1.4‰, which are in agreement with previously observed Hg isotope signatures during the AMDE season at the Arctic coast. However, the transfer of HgII from AMDE's to the terrestrial ecosystem does not represent a significant source (0-5 %), suggesting that most HgII deposited during AMDE's was re-emitted prior to snow-melt. The Hg isotope signatures in the soils and the atmosphere showed no indication for substantial re-emission of gaseous elemental mercury from the soils. The Hg stable isotope results agreed well with micro-metrological flux measurements conducted at the same location. Both independent approaches suggest that vegetation uptake of gaseous elemental Hg represents the dominant Hg flux between the atmosphere and Arctic tundra soils and they thus represent a net sink for atmospheric Hg. Changes in environmental conditions, such as warming and thawing of permafrost due to climate change or fires could however lead to a remobilization of the large Hg pool stored in Arctic tundra soils.

Data: CORDIS, © European Union

Project objective

Mercury (Hg) is a pollutant of global concern for human and ecosystem health. This is particularly true in the Arctic where indigenous populations are excessively exposed to dietary Hg from fish and marine mammal consumption. The deposition of Hg from the atmosphere to Earth surfaces and its re-emission via biogeochemical reduction processes determine Hg concentrations in Earth surface reservoirs, such as soils, snow, and runoff into Arctic lakes and surface Ocean. In order to predict the impact of anthropogenic Hg emissions on net atmospheric Hg deposition and ultimately Hg concentrations in biota, it is important to understand these deposition and re-emission processes. The reduction of deposited Hg2+ to volatile gaseous Hg0 and the oxidation of gaseous Hg0 to reactive Hg2+, which is rapidly deposited from the atmosphere, control the global fate of Hg. Major knowledge gaps concerning the mechanisms of these redox processes exist. Different photochemical and non-photochemical Hg2+ reduction mechanisms were found to fractionate Hg stable isotopes in distinct, identifiable ways. Also, different atmospheric Hg0 and Hg2+ pools have been shown to have distinguishable Hg isotope signatures. Hg isotopes can thus provide new insights in the sources of Hg and redox transformation processes at the Earth-atmosphere interface, which are inaccessible by means of concentration and flux measurements alone. In the MEROXRE project proposed here we will combine the latest innovations in gaseous Hg measurements in porous media (soils, snow) with state-of-the-art Hg isotope techniques to investigate:(i)Hg isotope fractionation of Hg2+ reduction and gaseous Hg0 oxidation in interstitial snow air and soil pores. (ii)Hg isotope fractionation factors associated with net gaseous Hg0 re-emission fluxes from soil and snow(iii)the importance of gaseous Hg0 oxidation and Hg2+ reduction and re-emission for the global Hg cycle by incorporating the results in a global Hg isotope model.

Original text from CORDIS.

Participants

  • CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS · ParisCoordinatorFrance

Links

Data: CORDIS, © European Union