Repository logo
Log in(current)
Repository logoMIT Open ScholarshipDSpace@MIT
  1. Home
  2. MIT Open Access Articles
  3. MIT Open Access Articles
  4. Microbial methanogenesis fueled by freshwater infiltration and oil biodegradation in the Siljan impact structure, Sweden

Microbial methanogenesis fueled by freshwater infiltration and oil biodegradation in the Siljan impact structure, Sweden

Thumbnail Image
Download
Name

42452_2024_Article_6418.pdf

Size

2.38 MB

Format

Adobe PDF

Checksum (MD5)

2ba1dabf74518c1f134d32a3e85805e8

Download all files submitted through automated deposit
art_3849510747680360082.zip (2.07 MB)
Author(s)
van Dam, Femke
•
Kietäväinen, Riikka
•
Westmeijer, George
•
Reinhardt, Manuel
•
Ono, Shuhei
•
Dopson, Mark
•
Ketzer, Marcelo
•
McIntosh, Jennifer C.
•
Drake, Henrik
Date Issued
January 3, 2025
Journal
Discover Applied Sciences
Publisher
Springer International Publishing
Citation
van Dam, F., Kietäväinen, R., Westmeijer, G. et al. Microbial methanogenesis fueled by freshwater infiltration and oil biodegradation in the Siljan impact structure, Sweden. Discov Appl Sci 7, 51 (2025).
Version
Final published version
Abstract
Deeply fractured rocks of meteorite impact craters are suggested as prime niches for subsurface microbial colonization. Methane can be a product of such microbial communities and seeps of methane from impact craters on Earth are of strong interest as they act as analogs for Mars. Previous studies report signs of ancient microbial methanogenesis in the Devonian Siljan meteorite impact structure in Sweden, but the proportion of microbial methane, metabolic pathways, and potential modern activity remain elusive. In this study, gas composition, hydrochemistry, oil organic geochemistry, and microbial community analyses are reported in 400 m deep fractures of the Siljan impact structure. The results showed a dominantly microbial origin for methane, which was supported by highly negative δ13CCH4 and positive δ13CCO2 values along with multiply substituted isotopologues (Δ13CH3D) that indicated disequilibrium fractionation due to microbial kinetic isotope effects. The presence of C2 to C5 hydrocarbons suggested a minor thermogenic input in the gas mix. Characterization of the microbial community via 16S rRNA gene amplicon sequencing and real-time PCR indicated a low abundance of several methanogenic archaeal populations, which is common for settings with active methanogenesis. Evidence of oil biodegradation suggested that secondary microbial hydrocarbon utilization was involved in the methanogenesis. Low sulfate and high alkalinity in the groundwaters also suggested a dominantly microbial methane formation driven by infiltration of freshwater that was coupled to sulfate reduction and secondary utilization of early mature thermogenic hydrocarbons.
MIT Department
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Terms of Use
Creative Commons Attribution
https://creativecommons.org/licenses/by/4.0/
Persistent DSpace Link
https://hdl.handle.net/1721.1/157943
DOI of Published Version
https://doi.org/10.1007/s42452-024-06418-8
Repository logo
PrivacyPermissionsAccessibilityContact us
Repository logo
Notify us about copyright concerns.