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dc.contributor.authorKipp, Michael A.
dc.contributor.authorStüeken, Eva E.
dc.contributor.authorYun, Misuk
dc.contributor.authorBekker, Andrey
dc.contributor.authorBuick, Roger
dc.date.accessioned2019-08-16T23:42:35Z
dc.date.available2019-08-16T23:42:35Z
dc.date.issued2018-10-15
dc.identifier.citationKipp , M A , Stüeken , E E , Yun , M , Bekker , A & Buick , R 2018 , ' Pervasive aerobic nitrogen cycling in the surface ocean across the Paleoproterozoic Era ' , Earth and Planetary Science Letters , vol. 500 , pp. 117-126 . https://doi.org/10.1016/j.epsl.2018.08.007en
dc.identifier.issn0012-821X
dc.identifier.otherPURE: 255480700
dc.identifier.otherPURE UUID: a402203b-d6da-45f4-8c37-b89c91a10d4f
dc.identifier.otherRIS: urn:E32DB2B2C271D0DE5AAAAA1530AE7D8B
dc.identifier.otherScopus: 85051625682
dc.identifier.otherWOS: 000445718700012
dc.identifier.otherORCID: /0000-0001-6861-2490/work/65014409
dc.identifier.urihttps://hdl.handle.net/10023/18329
dc.descriptionMAK acknowledges support from NSF Graduate Research Fellowship DGE-1256082. AB acknowledges funding from NSERC Discovery and Accelerator grants. Funding for isotopic analyses was provided by the UW Department of Earth & Space Sciences to MAK and by NASA Exobiology grant NNX16AI37G to RB.en
dc.description.abstractNitrogen isotope ratios in marine sedimentary rocks have become a widely used biogeochemical proxy that records information about nutrient cycling and redox conditions in Earth's distant past. While the past two decades have seen considerable progress in our understanding of the Precambrian sedimentary nitrogen isotope record, it is still compromised by substantial temporal gaps. Furthermore, quantitative links between nitrogen isotope data, marine redox conditions, and nutrient availability are largely lacking in a Precambrian context. Here we present new nitrogen isotope data from a suite of marine sedimentary rocks with ca. 2.4 to 1.8 Ga ages, spanning the Great Oxidation Event in the Paleoproterozoic, to better constrain the response of the nitrogen cycle to the first major redox transition in Earth's history. We further construct a simple box model to describe the major pathways that influenced the nitrogen isotope mass balance of the Precambrian ocean and use this as a platform to evaluate the Precambrian nitrogen isotope record. Within this framework, we find that consistently positive nitrogen isotope values, ranging from +1.1 to +7.7‰, across the early Paleoproterozoic are strong evidence for an expansion of oxygenated surface waters. Since the isotopic signature of aerobic nitrogen cycling is recorded in the biomass of nitrate-assimilating organisms, this implicates widespread nitrate bioavailability in this time interval. The decline in offshore nitrogen isotope ratios in the Mesoproterozoic is consistent with the contraction of oxic waters, which could have inhibited the expansion of nitrate-fueled ecosystems to pelagic waters until the widespread oxygenation of the ocean in the latest Neoproterozoic to early Phanerozoic.
dc.format.extent10
dc.language.isoeng
dc.relation.ispartofEarth and Planetary Science Lettersen
dc.rights© 2018 Elsevier B.V. This work has been made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at: https://doi.org/10.1016/j.epsl.2018.08.007en
dc.subjectPaleoproterozoicen
dc.subjectNitrogen isotopesen
dc.subjectPaleoredoxen
dc.subjectEukaryote evolutionen
dc.subjectGreat Oxidation Eventen
dc.subjectLomagundi Eventen
dc.subjectQE Geologyen
dc.subjectDASen
dc.subjectSDG 14 - Life Below Wateren
dc.subject.lccQEen
dc.titlePervasive aerobic nitrogen cycling in the surface ocean across the Paleoproterozoic Eraen
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews. School of Earth & Environmental Sciencesen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.identifier.doihttps://doi.org/10.1016/j.epsl.2018.08.007
dc.description.statusPeer revieweden
dc.date.embargoedUntil2019-08-17


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