Clumped isotopes constrain thermogenic and secondary microbial methane origins in coal bed methane
- 1. Tianjin University
- 2. Haihe Laboratory of Sustainable Chemical Transformations, Tianjin 300072, China
- 3. California Institute of Technology
- 4. Tokyo Institute of Technology
- 5. Swiss Federal Laboratories for Materials Science and Technology
- 6. University of California, Berkeley
- 7. University of Arizona
Abstract
Methane is an economic energy resource and potent greenhouse gas. Distinguishing secondary microbial methane from thermogenic gas is important for natural gas exploration and consideration of subsurface microbial activity in the global carbon cycle, but remains challenging. To understand controls on methane origins in natural gas systems, we investigated the methane clumped isotopologue distributions in the Qinshui Basin high-thermal maturity coal bed methane (CBM) reservoir. Here, near-equilibrium clumped isotopologues distribution (Δ13CH3D and Δ12CH2D2) inferred a temperature interval of 21.6–252.3 °C. The high-temperature thermodynamic equilibrium most likely represents original thermogenic CBM characteristics during coalification. The low-temperature equilibrium clumped isotopologue distributions suggest microbial alteration to CH4 isotopic bond ordering by increased enzymatically catalyzed isotopic exchange. The independent constraints from clumped isotopes, integrated with other geochemical and genomic evidence, confirm notable secondary microbial methane from biodegradation in the highly mature reservoir. Thus, methane clumped isotopes can be used as unequivocal tracers to distinguish secondary microbial methane from thermogenic gases and hence provide the ability to incorporate them separately into global methane budgets.
Copyright and License
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Acknowledgement
This work was supported by National Natural Science Foundation of China (Grant no. 42150710532), the Tianjin Municipal Science and Technology Bureau (Grant no. 24JRRCRC00020) and the Haihe Laboratory of Sustainable Chemical Transformations. Xinchu Wang was supported by the Postdoctoral Fellowship Program of CPSF (Grant no. GZC20241195), the China Postdoctoral Science Foundation - Tianjin Joint Support Program (Grant no. 2024T019TJ). Naizhong Zhang was supported by the JSPS KAKENHI Grant (Grant no. 22K14134) and the Astrobiology Center Program of NINS (Grant no. AB0513). Jennifer McIntosh was supported by the NSF EAR FRES SMRFS project (Grant no. 2120733). We are grateful to Shanxi Lanyan Coalbed Methane Group Co., Ltd for permission to collect samples and providing relevant information. Y. Liu, Z.-J. Xu and Y. Yang are appreciated for field assistance.
Contributions
Xinchu Wang: Writing – original draft, Visualization, Validation, Methodology, Investigation, Formal analysis, Data curation, Conceptualization. Biying Chen: Writing – review & editing, Methodology, Investigation, Formal analysis, Data curation, Conceptualization. Hui Nai: Writing – review & editing, Data curation. Cong-Qiang Liu: Writing – review & editing, Validation, Supervision, Project administration, Funding acquisition. Guannan Dong: Writing – review & editing, Methodology. Naizhong Zhang: Writing – review & editing, Validation. Si-Liang Li: Writing – review & editing, Validation, Supervision. Jonathan Gropp: Writing – review & editing. Jennifer McIntosh: Writing – review & editing, Data curation. Rob M. Ellam: Writing – review & editing. John M. Eiler: Writing – review & editing, Validation. Sheng Xu: Writing – review & editing, Supervision, Project administration, Methodology.
Data Availability
All data needed to evaluate the conclusions in the paper are present in the paper and the Source Data file, Supplementary Materials.
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Additional details
- National Natural Science Foundation of China
- Accepted
-
2024-09-18Accepted
- Available
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2024-10-03Published online
- Available
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2024-10-03Version of record
- Caltech groups
- Division of Geological and Planetary Sciences
- Publication Status
- Published