Anaerobic oxidation of methane by Mn oxides in sulfate-poor environments

Author:

Cai Chunfang12,Li Kaikai3,Liu Dawei2,John Cedric M.4,Wang Daowei3,Fu Bin5,Fakhraee Mojtaba6,He Hong7,Feng Lianjun1,Jiang Lei1

Affiliation:

1. Key Laboratory of Cenozoic Geology and Environment, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China

2. College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China

3. School of Energy Resources, China University of Geosciences (Beijing), Beijing 100083, China

4. Department of Earth Science and Engineering, Imperial College London, SW7 2BU London, UK

5. Research School of Earth Science, The Australian National University, Canberra, Australian Capital Territory 2601, Australia

6. Department of Geology and Geophysics, Yale University, New Haven, Connecticut 06520, USA

7. Petroleum Exploration and Production Research Institute, SINOPEC, Beijing 100083, China

Abstract

Strongly 13C-depleted authigenic carbonates (e.g., δ13CVPDB <−30‰; VPDB—Vienna Peedee belemnite) in nature are generally believed to form by sulfate-dependent anaerobic oxidation of methane (AOM). However, we demonstrate using geochemical data and thermodynamic calculation that such calcites are most likely derived from biogenic oxidation of methane in sulfate-poor, nonmarine environments during early diagenesis, as observed in the Triassic sandy conglomerates from the Junggar Basin, northwestern China. This process operated through preferential oxidation of 13C-depleted methane by Mn oxides in closed conditions, producing calcites with higher Mn contents and δ13C values in association with more 13C-enriched residual methane as a result of kinetic isotope fractionation. Thus, the Mn-rich and 13C-depleted carbonates are proposed as tracers of Mn-dependent AOM, which should have served as an important sink of greenhouse methane in low-sulfate early Earth’s oceans.

Publisher

Geological Society of America

Subject

Geology

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