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Copyright Copernicus GmbH 2012

Abstract

The abrupt warming across the Younger Dryas termination (~11 600 yr before present) was marked by a large increase in the global atmospheric methane mixing ratio. The debate over sources responsible for the rise in methane centers on the roles of global wetlands, marine gas hydrates, and thermokarst lakes. We present a new, higher-precision methane stable carbon isotope ratio (δ13 CH4 ) dataset from ice sampled at Påkitsoq, Greenland that shows distinct 13 C-enrichment associated with this rise. We investigate the validity of this finding in face of known anomalous methane concentrations that occur at Påkitsoq. Comparison with previously published datasets to determine the robustness of our results indicates a similar trend in ice from both an Antarctic ice core and previously published Påkitsoq data measured using four different extraction and analytical techniques. The δ13 CH4 trend suggests that 13 C-enriched CH4 sources played an important role in the concentration increase. In a first attempt at quantifying the various contributions from our data, we apply a methane triple mass balance of stable carbon and hydrogen isotope ratios and radiocarbon. The mass balance results suggest biomass burning (42-66% of total methane flux increase) and thermokarst lakes (27-59%) as the dominant contributing sources. Given the high uncertainty and low temporal resolution of the 14 CH4 dataset used in the triple mass balance, we also performed a mass balance test using just δ13 C and δD. These results further support biomass burning as a dominant source, but do not allow distinguishing of thermokarst lake contributions from boreal wetlands, aerobic plant methane, or termites. Our results in both mass balance tests do not suggest as large a role for tropical wetlands or marine gas hydrates as commonly proposed.

Details

Title
Enrichment in 13C of atmospheric CH4 during the Younger Dryas termination
Author
Melton, J. R.; Schaefer, H.; Whiticar, M. J.
First page
1177
Publication year
2012
Publication date
2012
Publisher
Copernicus GmbH
ISSN
18149324
e-ISSN
18149332
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
1038359724
Copyright
Copyright Copernicus GmbH 2012