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dc.contributor.authorOno, Shuhei
dc.contributor.authorSim, Min Sub
dc.contributor.authorBosak, Tanja
dc.date.accessioned2017-01-09T15:51:53Z
dc.date.available2017-01-09T15:51:53Z
dc.date.issued2014-12
dc.identifier.issn0027-8424
dc.identifier.issn1091-6490
dc.identifier.urihttp://hdl.handle.net/1721.1/106288
dc.description.abstractIn PNAS, Wing and Halevy present a new model that quantitatively describes the magnitude of sulfur isotope fractionation produced by dissimilatory microbial sulfate reduction (MSR). MSR is a major player in the global biogeochemical cycles and is responsible for the respiration of up to 30% of organic matter in marine sediments. This metabolism produces large isotope effects, in which the product, sulfide, is depleted in the heavy isotopes ([superscript 33]S, [superscript 34]S, and [superscript 36]S) relative to the most abundant isotope [superscript 32]S (3), enriching modern seawater sulfate in [superscript 34]S by about 21‰ (parts per thousand) compared with mantle sulfur. Sedimentary sulfur minerals preserve a record of this effect and are used to track changes in the sulfur isotope composition of seawater and the biogeochemical sulfur, carbon, and oxygen cycles through geologic time (4). Such reconstructions require an understanding of factors that control the magnitude of sulfur isotope effects and dictate the fractionation of sulfur isotopes by sulfate reducers under a range of growth conditions.en_US
dc.language.isoen_US
dc.publisherNational Academy of Sciences (U.S.)en_US
dc.relation.isversionofhttp://dx.doi.org/10.1073/pnas.1420670111en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourcePNASen_US
dc.titlePredictive isotope model connects microbes in culture and natureen_US
dc.typeArticleen_US
dc.identifier.citationOno, Shuhei, Min Sub Sim, and Tanja Bosak. “Predictive Isotope Model Connects Microbes in Culture and Nature.” Proceedings of the National Academy of Sciences 111.51 (2014): 18102–18103. © 2014 National Academy of Scienceen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.contributor.mitauthorOno, Shuhei
dc.contributor.mitauthorSim, Min Sub
dc.contributor.mitauthorBosak, Tanja
dc.relation.journalProceedings of the National Academy of Sciencesen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsOno, Shuhei; Sim, Min Sub; Bosak, Tanjaen_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-1348-9584
dc.identifier.orcidhttps://orcid.org/0000-0001-5179-5323
mit.licensePUBLISHER_POLICYen_US


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