GC14C-06
Methane emissions in the East Siberian Arctic Shelf: issues addressed and questions raised

Monday, 14 December 2015: 17:15
3005 (Moscone West)
Natalia E Shakhova, University of Alaska Fairbanks, Fairbanks, AK, United States; Tomsk Polytechnic University, Institute of Natural Resources, Tomsk, Russia and The International Siberian Shelf Study Team
Abstract:
Methane (CH4) emissions in the East Siberian Arctic Shelf (ESAS) has been studied during the last decade. Our investigation, including observational studies using hydrological, biogeochemical, geophysical, geo-electrical, microbiological, and isotopic methods, and modeling efforts to assess current subsea permafrost state and the ESAS’ contribution to the regional CH4 budget, have clarified processes driving CH4 emissions in the ESAS and spilt some light on possible sources involvement. Despite some authors believe that CH4 fluxes from subsea permafrost in the ESAS will depend on rates of CH4 production in gradually thawing sediments while subsea permafrost will remain frozen for millennia, results of our investigation showed the opposite. Permafrost failure caused by long-lasting warming by sea water due to sea level rise, deep/open taliks formation due to combined heating effects of seawater, river runoff, geothermal flux, and pre-existing thermokarst and global-change-induced warming, determines destabilization of massive gas reservoirs, leading to large-scale CH4 releases, including release of pre-formed CH4 long preserved within/beneath subsea permafrost. Resultant rates of CH4 emissions over the ESAS vary spatially by 3-5 orders of magnitude. Re-drilling of subsea permafrost performed from the fast ice 30 years after it was first drilled in 1982-1983, revealed modern rates of subsea permafrost degradation. These results contradict previous hypotheses that: 1) taliks beneath thermokarst lakes always freeze after submergence; 2) rates of permafrost degradation after inundation decrease over time; and 3) thousands of years required to form escape paths for permafrost-preserved gas. Involvement of shallow relic hydrates is suggested based on results of experimental work with sediment cores extracted from the near-shore zone of the ESAS. In-situ investigations revealed that dissolved CH4 could remain in the seawater up to 1000 days, because oxidation rates are low. Storms could release some aqueous CH4 to atmosphere; dissolved CH4, captured beneath ice in winter, can spread via currents and escape to atmosphere through breaks in the ice. Progressive subsea permafrost thawing and decreasing ice extent could significantly increase CH4 emissions from the ESAS.