EGU26-9799, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-9799
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Monday, 04 May, 16:15–18:00 (CEST), Display time Monday, 04 May, 14:00–18:00
 
Hall X5, X5.190
Investigating the CH4 isotopic signature of debris rich basal ice: insight from Camp Century ice core. 
Lisa Ardoin1, Carina Van der Veen2, Saïda El Amari1, Dorthe Dahl-Jensen3, Jørgen Peder Steffensen3, Jean-Louis Tison1, Thomas Röckmann2, and François Fripiat1
Lisa Ardoin et al.
  • 1Université Libre de Bruxelles (ULB), Laboratory of Glaciology, Belgium (lisa.ardoin@ulb.be)
  • 2Institute for Marine and Atmospheric research Utrecht (IMAU), Utrecht University, Netherlands
  • 3Centre for Ice and Climate, Niels Bohr Institute, University of Copenhagen, Denmark

Runoff waters at the margin of the Greenland Ice Sheet export CH₄-supersaturated waters originating from the ice-sheet bed, contributing to the global atmospheric CH₄ budget [1, 2]. This methane is of microbial origin, likely produced from a mixture of inorganic and ancient organic carbon buried beneath the ice sheet [1, 2, 3].

Debris-rich basal ice layers provide a unique opportunity to investigate the sources and sink of methane at the ice/bedrock interface. Previous studies have shown that Greenland debris-rich basal ice preserves large methane accumulations [4, 5, 6] and may represent a potential endmember contributing to CH4-rich meltwaters released during the melting season. At Camp Century, CH4 mixing ratios increase sharply from ~200 ppm to up to 30 000 ppm within 1 m above the ice/bed material transition [6]. Prokaryotic DNA analyses support the microbial origin, and indicate the presence of in situ methanotrophic communities, suggesting active CH4 consumption and oxidation to CO2 within the debris-rich ice [6].

Here, we present methane stable isotope measurements (δ13C-CH4 and δD-CH4) from 7 samples spanning this transition zone. Despite the large methane accumulation, debris-rich ice is strongly gas-depleted, and the limited sample size combined with high CH4 variability makes isotopic analyses technically challenging. CH4 was extracted using a melting-freeze extraction coupled to a cold-trap finger filled with HayeSep Q at Université Libre de Buxelles (ULB, Belgium) laboratory, allowing gases to be sealed in glass tubes to prevent atmospheric contamination. CH4 isotope analyses were performed at the Institute for Marine and Atmospheric Research Utrecht (IMAU, Netherlands) using a Thermo Delta Plus XP (δ13C and δD) [7].

The overall isotopic signature supports a microbial origin of CH4 via methanogenesis, consistent with GRIP values [4]. Despite substantial scatter in δ13C-CH4, a negative correlation is reported between CH4 concentration and both δ13C-CH4 and δD-CH4, consistent with preferential oxidation of lighter isotopes during methanotrophy. However, the observed relationship suggests a relatively low apparent fractionation factor compared to literature estimates. This could result from under-expression of the true isotope effect due to superimposed processes such as mixing or diffusion, or because the fractionation is intrinsically smaller under low-temperature conditions.

 

[1] Lamarche-Gagnon et al., 2019, Nature, 565(7737), 73-77. [2] Christiansen et al., 2021, Journal of Geophysical Research: Biogeosciences126(11), e2021JG006308. [3] Adnew et al., 2023, Geochimica et Cosmochimica Acta389, 249-264. [4] Souchez et al., 2006, Geophys. Res. Lett., 33, L24503. [5] Verbeke et al., 2002, Annals of Glaciology 35, 231-236. [6] Ardoin et al., submitted, The Cryosphere. [7] Menoud et al., 2020, Tellus B: Chemical and Physical Meteorology72(1), 1-20.

How to cite: Ardoin, L., Van der Veen, C., El Amari, S., Dahl-Jensen, D., Steffensen, J. P., Tison, J.-L., Röckmann, T., and Fripiat, F.: Investigating the CH4 isotopic signature of debris rich basal ice: insight from Camp Century ice core. , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9799, https://doi.org/10.5194/egusphere-egu26-9799, 2026.