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Anaerobic oxidation of methane (AOM) is an important microbial process mitigating methane (CH) emission from natural sediments. Anaerobic methanotrophic archaea (ANME) have been shown to mediate AOM coupled to the reduction of several compounds, either directly (i.e. nitrate, metal oxides) or in consortia with syntrophic bacterial partners (i.e. sulfate). However, the mechanisms underlying extracellular electron transfer (EET) between ANME and their bacterial partners or external electron acceptors are poorly understood. In this study, we investigated electron and carbon flow for an anaerobic methanotrophic consortium dominated by 'Candidatus Methanoperedens nitroreducens' in a CH-fed microbial electrolysis cell (MEC). Acetate was identified as a likely intermediate for the methanotrophic consortium, which stimulated the growth of the known electroactive genus Geobacter. Electrochemical characterization, stoichiometric calculations of the system, along with stable isotope-based assays, revealed that acetate was not produced from CH directly. In the absence of CH, current was still generated and the microbial community remained largely unchanged. A substantial portion of the generated current in the absence of CH was linked to the oxidation of the intracellular polyhydroxybutyrate (PHB) and the breakdown of extracellular polymeric substances (EPSs). The ability of 'Ca. M. nitroreducens' to use stored PHB as a carbon and energy source, and its ability to donate acetate as a diffusible electron carrier expands the known metabolic diversity of this lineage that likely underpins its success in natural systems.
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http://dx.doi.org/10.1016/j.watres.2022.118743 | DOI Listing |
Anaerobic methanotrophic archaea (ANME) are crucial to planetary carbon cycling. They oxidise methane in anoxic niches by transferring electrons to nitrate, metal oxides, or sulfate-reducing bacteria. No ANMEs have been isolated, hampering the biochemical investigation of anaerobic methane oxidation.
View Article and Find Full Text PDFISME J
January 2025
Division of Biology and Biological Engineering, California Institute of Technology, Pasadena, CA 91125, United States.
At methane seeps worldwide, syntrophic anaerobic methane-oxidizing archaea and sulfate-reducing bacteria promote carbonate precipitation and rock formation, acting as methane and carbon sinks. Although maintenance of anaerobic oxidation of methane (AOM) within seep carbonates has been documented, its reactivation upon methane exposure remains uncertain. Surface-associated microbes may metabolize sulfide from AOM, maintain carbonate anoxia, contribute to carbonate dissolution, and support higher trophic levels; however, these communities are poorly described.
View Article and Find Full Text PDFSci Adv
August 2025
Department of Physics and Astronomy, University of Southern California, Los Angeles, CA 90089, USA.
Anaerobic methanotrophic archaea (ANME) and sulfate-reducing bacteria (SRB) form syntrophic partnerships in marine sediments to consume greenhouse gas methane. While direct interspecies electron transport is proposed to enable ANME/SRB symbiosis, its electrochemical properties remain uncharacterized. Here, using sediment-free enrichment cultures, we measured the electron transport capabilities of marine consortia under physiological conditions.
View Article and Find Full Text PDFEnviron Sci Technol
September 2025
Department of Earth, Energy, and Environment, University of Calgary, Calgary, AB T2N 1N4, Canada.
Nitrogen fixation is an energy-intensive process critical for microbial survival in nitrogen-depleted environments. Groundwater, the Earth's largest accessible freshwater reservoir, is typically oligotrophic. However, recent studies have identified productive groundwater habitats where nitrogen fixation may become important to support the productivity.
View Article and Find Full Text PDFPhilos Trans R Soc Lond B Biol Sci
August 2025
Research School of Astronomy and Astrophysics, Australian National University, Weston Creek, Australian Capital Territory, Australia.
In our galaxy, tens of billions of wet, rocky Earth-like planets orbit in the habitable zones of their host stars. Stellar spectra and models of devolatilization yield ranges of plausible chemistries on these Earths. The early emergence of biology on Earth from similar chemistry has a chance of being universally relevant to the origins of life elsewhere.
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