The Clumped Isotope Signatures of Multiple Methanogenic Metabolisms
- Creators
-
Li, Jiawen1
- Ash, Jeanine L.2
-
Cobban, Alec1
- Kubik, Briana C.3
- Rizzo, Gabriella3
- Thompson, Mia1
- Guibourdenche, Laetitia4
- Berger, Stefanie5
- Morra, Kaycee6
- Lin, Ying6
-
Mueller, Elliott P.7
- Masterson, Andrew L.8
- Stein, Rebekah9
- Fogel, Marilyn6
-
Torres, Mark A.2
- Feng, Xiahong1
- Holden, James F.3
- Martini, Anna10
- Welte, Cornelia U.5
- M. Jetten, Mike S.5
- Young, Edward D.4
- Leavitt, William D.1, 11
-
1.
Dartmouth College
-
2.
Rice University
-
3.
University of Massachusetts Amherst
-
4.
University of California, Los Angeles
-
5.
Radboud University Nijmegen
-
6.
University of California, Riverside
-
7.
California Institute of Technology
-
8.
Northwestern University
- 9. Cooperative Programs for the Advancement of Earth System Science, University Corporation for Atmospheric Research, Boulder, Colorado 80307, United States.
-
10.
Amherst College
-
11.
University of Utah
Abstract
Methane is a potent greenhouse gas, an important energy source, and an important part of the global carbon cycle. The relative abundances of doubly substituted (“clumped”) methane isotopologues (13CH3D and 12CH2D2) offer important information on the sources and sinks of methane. However, the clumped isotope signatures of microbially produced methane from different methanogenic pathways lack a systematic investigation. In this study, we provide a data set encompassing isotopic signatures of hydrogenotrophic, methylotrophic, acetoclastic, and methoxydotrophic methanogenesis. We find that a statistical “combinatorial effect” generates significant differences in 12CH2D2 compositions between hydrogenotrophic methanogenesis and the other pathways, while variations in the fractionation factors of clumped isotopologues result in differences in 13CH3D compositions between the methylotrophic, acetoclastic, and methoxydotrophic pathways. The energy yield of methanogenesis and the energy conservation approaches implemented by different microbial strains may also influence the isotope values of methane. Further analysis suggests that previously observed isotopic signatures of methane in freshwater environments are potentially due to mixing between hydrogenotrophic and other methanogenesis pathways. This study provides new experimental constraints on the isotope signatures of different microbial methanogenic pathways and evidence of the mechanisms responsible for the observed differences. This enables a better understanding of the sources and sinks of methane in the environment.
Copyright and License
© 2025 The Authors. Published by American Chemical Society
This publication is licensed under CC-BY 4.0.
Acknowledgement
We thank Daniel Stolper for the contributions to the isotopic measurements of substrates. We thank Jonathan Gropp and Jiarui Liu for their in-depth discussions on the interpretation of the data. We also thank William Metcalf for offering the microbial strain Methanosarcina barkeri strain WWM603 used in this study.
Funding
Simons Foundation Award 62388 (W.D.L.), NASA Exobiology grant 80NSSC21K0477 (E.D.Y., W.D.L.), NASA Exobiology grant 80NSSC21K1240 (J.F.H.), Netherlands Organization for Scientific Research (N.W.O.)/Ministry of Education (OCW) grant SIAM 024002002 (S.B., C.U.W., M.J.), ERC Synergy grant MARIX 854088 (M.J.)
Supplemental Material
The experimental details, materials, methods, measured isotope values, calculations of isotope fractionations, and modeling details, including Figure S1–S4, Table S1–S7, and Text S1–S7 (PDF)
Files
Name | Size | Download all |
---|---|---|
md5:e1dcdb8508ffbb9821b3cfb71f43f2ff
|
3.8 MB | Preview Download |
md5:f9533741301082812a13408af1c13fff
|
2.2 MB | Preview Download |
Additional details
- Alternative title
- The clumped isotope signatures of multiple methanogenesis metabolisms
- Simons Foundation
- 62388
- National Aeronautics and Space Administration
- 80NSSC21K0477
- National Aeronautics and Space Administration
- 80NSSC21K1240
- Dutch Research Council
- 024002002
- Ministry of Education Culture and Science
- 024002002
- European Research Council
- 854088
- Accepted
-
2025-06-25
- Available
-
2025-07-03Published
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)
- Publication Status
- Published