Anaerobic methane oxidation by archaea/sulfate-reducing bacteria aggregates: 2. Isotopic constraints
Clicks: 3
ID: 295899
2009
Article Quality & Performance Metrics
Overall Quality
Not rated
Combines reader engagement with the AI quality analysis. This
article has not been analysed, so there is no overall score —
reader engagement is measured and shown alongside.
Reader Engagement
Emerging Content
0.6
/100
3 views
0 readers
AI Quality Assessment
Not analyzed
Readership in this journal
EmergingRanked #512 of 8,486 articles by views in american journal of science
Most read
Least read
Bar heights use a square-root scale. Only the 120 most-read articles are drawn; the journal has 8,486 in total.
Mint this article as an NFT
Not yet mintedCreate a permanent, verifiable on-chain record of this article on the Scimatic Network. The NFT is held in your Journament account, and you can withdraw it to your own wallet at any time.
5
SUSD
one-off · no wallet required
Abstract
Recent studies employing novel analytical tools provide detailed, microscopic portraits of archaea/sulfate-reducing bacteria aggregates in sediments from methane seep and vent sites. One of the most striking features of these aggregates is that lipid and cell carbon are highly depleted in 13C (δ13C < −60‰). Biogenic methane, with δ13C values of −50 to −110 permil, is a logical candidate for carbon source of these aggregates. Accordingly, it is widely assumed that the archaea oxidize and assimilate methane, and that methane-derived carbon is transferred to the sulfate-reducing bacteria (SRB) symbionts as CO2 or as a partially oxidized intermediate. However, methane is not the only possible source of 13C-depleted carbon in archaea/SRB aggregates. ΣCO2 in sediments at seep and vent sites tends to be isotopically "light" due to decomposition of organic matter derived from chemoautotrophic organisms. In addition, CO2 is depleted in 13C by ∼10 permil compared to ΣCO2 owing to the equilibrium isotope effect. Assimilation of this "light" CO2 by methanogenic archaea and autotrophic SRB, combined with enzymatic isotope effects, could also yield lipid and biomass that are highly depleted in 13C. We derive general equations based on isotope mass-balance and calibrated with laboratory and field data to predict the isotopic composition of archaeal cell carbon and lipids derived from autotrophic methanogenesis and anaerobic methane oxidation. The calculations show that observed δ13C values for archaeal biomass and lipids at methane seep and vent sites are readily accounted for by isotope fractionation during methane production from CO2, and that biomass produced during anaerobic methane oxidation is only slightly depleted in 13C relative to methane unless the enzymatic isotope effect associated with the anabolic arm of the assimilation-dissimilation branch point is considerably larger than the isotope effect associated with the catabolic arm. We also apply an isotope diffusion-reaction model to demonstrate that micro-gradients in δ13C-CO2 cannot be maintained within archaea/SRB aggregates. However, 13C-depleted carbon in SRB members of the aggregate is readily explained by autotrophic sulfate-reduction with bulk porewater CO2 as carbon source. These results illustrate that 13C-depleted biomass and lipids observed in sediments from methane seep and vent sites may be derived from CO2-reducing archaea and autotrophic sulfate-reducing bacteria. The inference of anaerobic methanotrophy based on 13C depletion in archaeal and sulfate-reducing bacterial cell carbon and/or lipids should be considered tentative unless corroborated by independent, concordant evidence of net methane consumption.
| Reference Key |
openalex_W2034818194
Use this key to autocite in the manuscript while using
SciMatic Manuscript Manager or Thesis Manager
|
|---|---|
| Authors | Marc J. Alperin, Tori M. Hoehler |
| Journal | american journal of science |
| Year | 2009 |
| DOI |
10.2475/10.2009.02
|
| URL | |
| Keywords | Keywords not found |
Citations
No citations found. To add a citation, contact the admin at info@scimatic.org
Comments
No comments yet. Be the first to comment on this article.