Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/87544
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dc.contributorDepartment of Civil and Environmental Engineering-
dc.creatorZerkle, AL-
dc.creatorYin, R-
dc.creatorChen, C-
dc.creatorLi, X-
dc.creatorIzon, GJ-
dc.creatorGrasby, SE-
dc.date.accessioned2020-07-16T03:58:08Z-
dc.date.available2020-07-16T03:58:08Z-
dc.identifier.urihttp://hdl.handle.net/10397/87544-
dc.language.isoenen_US
dc.publisherNature Publishing Groupen_US
dc.rights© The Author(s) 2020. This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.en_US
dc.rightsThe following publication Zerkle, A.L., Yin, R., Chen, C. et al. Anomalous fractionation of mercury isotopes in the Late Archean atmosphere. Nat Commun 11, 1709 (2020), is available at https://doi.org/10.1038/s41467-020-15495-3en_US
dc.titleAnomalous fractionation of mercury isotopes in the Late Archean atmosphereen_US
dc.typeJournal/Magazine Articleen_US
dc.identifier.volume11-
dc.identifier.issue1-
dc.identifier.doi10.1038/s41467-020-15495-3-
dcterms.abstractEarth’s surface underwent a dramatic transition ~2.3 billion years ago when atmospheric oxygen first accumulated during the Great Oxidation Event, but the detailed composition of the reducing early atmosphere is not well known. Here we develop mercury (Hg) stable isotopes as a proxy for paleoatmospheric chemistry and use Hg isotope data from 2.5 billion-year-old sedimentary rocks to examine changes in the Late Archean atmosphere immediately prior to the Great Oxidation Event. These sediments preserve evidence of strong photochemical transformations of mercury in the absence of molecular oxygen. In addition, these geochemical records combined with previously published multi-proxy data support a vital role for methane in Earth’s early atmosphere.-
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationNature communications, 2020, v. 11, no. 1, 1709-
dcterms.isPartOfNature communications-
dcterms.issued2020-
dc.identifier.scopus2-s2.0-85083022494-
dc.identifier.pmid32249783-
dc.identifier.eissn2041-1723-
dc.identifier.artn1709-
dc.description.validate202007 bcma-
dc.description.oaVersion of Recorden_US
dc.identifier.FolderNumberOA_Scopus/WOSen_US
dc.description.pubStatusPublisheden_US
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