Uranium isotope systematics of a low-productivity ferruginous ocean analog: Implications for the uranium isotope record of early Earth

IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Geochimica et Cosmochimica Acta Pub Date : 2025-03-01 Epub Date: 2025-01-13 DOI:10.1016/j.gca.2025.01.011
Geoffrey J. Gilleaudeau , Xinming Chen , Stephen J. Romaniello , Sajjad A. Akam , Chad Wittkop , Sergei Katsev , Ariel D. Anbar , Elizabeth D. Swanner
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Abstract

The uranium isotope (δ238U) paleo-redox proxy has emerged as a premier tool for understanding ocean oxygenation through Earth’s history. The fidelity of this important proxy depends, however, on our mechanistic understanding of the pathways that induce uranium isotope fractionation during U(VI) reduction to U(IV). Uranium reduction has been extensively studied in euxinic (anoxic + sulfidic) environments, yet relatively few constraints currently exist on δ238U fractionation in ferruginous (anoxic + iron-rich) environments, even though ferruginous conditions may have been a dominant feature of Earth’s oceans for much of the geologic past. Here, we present a comprehensive uranium isotope study of modern, meromictic, oligotrophic to mesotrophic, ferruginous Canyon Lake, Upper Peninsula, Michigan (USA), including investigation of a high-resolution profile of lake waters, lake inlet and outlet waters, and groundwater, as well as shallow cores through both oxic and ferruginous sediments. The key observation of this study is that the entire water column, oxic sediments, and ferruginous sediments have indistinguishable δ238U values near the composition of the upper continental crust. This implies a lack of δ238U fractionation in the low-productivity, ferruginous environments of Canyon Lake. We suggest that uranium cycling in Canyon Lake is dominated by adsorption and co-precipitation with iron oxides, with only a limited role for U(VI) reduction. These processes result partly from aqueous uranium speciation in the lake, with the dominance of UO2-CO3 complexes in the upper water column leading to a high partition coefficient of uranium during sorption to iron oxides. In addition, the dominance of CaUO2(CO3)32– and Ca2UO2(CO3)3(aq) in bottom waters kinetically inhibits U(VI) reduction by Fe(II)(aq). The lack of U(VI) reduction and hence δ238U fractionation in Canyon Lake, despite Fe(II)(aq) concentrations >1.5 mM, is potentially analogous to the lack of δ238U fractionation that occurred in the Archean and Proterozoic oceans, as indicated by the carbonate δ238U record. In contrast with predictions that U(VI) should be rapidly reduced and scavenged from the water column in the presence of Fe(II)(aq), our data suggest a limited role for U(VI) reduction and δ238U fractionation under the low-nutrient, low-productivity, ferruginous conditions that characterized the oceans on the early Earth.
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低生产力含铁海洋类似物的铀同位素系统:对早期地球铀同位素记录的启示
铀同位素(δ238U)古氧化还原代理已成为了解地球历史上海洋氧化作用的首要工具。然而,这一重要代理的保真度取决于我们对铀(VI)还原为铀(IV)过程中诱导铀同位素分馏途径的机制理解。铀的还原已经在缺氧(缺氧+硫化物)环境中进行了广泛的研究,但目前在含铁(缺氧+富铁)环境中δ238U分异的限制相对较少,尽管含铁条件可能是地球海洋的主要特征在地质过去的大部分时间里。在这里,我们提出了一个全面的铀同位素研究,现代,分生,贫营养到中营养,含铁峡谷湖,上半岛,密歇根州(美国),包括湖水,湖泊进出口水,地下水的高分辨率剖面的调查,以及浅层岩心含氧和含铁沉积物。本研究的关键观察结果是整个水柱、含氧沉积物和含铁沉积物在上陆地壳组成附近具有难以区分的δ238U值。这表明在峡谷湖的低生产力、含铁环境中缺乏δ238U分选。结果表明,峡谷湖中铀的循环主要以吸附和与氧化铁共沉淀为主,U(VI)的还原作用有限。这些过程的部分原因是湖水中铀的形态形成,上层水柱中UO2-CO3络合物的优势导致铀在铁氧化物吸附过程中的分配系数很高。此外,底水中Ca2UO2(CO3) 32 -和Ca2UO2(CO3)3(aq)在动力学上抑制了Fe(II)(aq)对U(VI)的还原。尽管Fe(II)(aq)浓度为>;1.5 mM,但峡谷湖缺乏U(VI)还原,因此δ238U分异,这与碳酸盐岩δ238U记录表明的太古宙和元古代海洋中δ238U分异的缺乏可能类似。与预测在Fe(II)(aq)存在的情况下U(VI)会被迅速还原并从水柱中清除相反,我们的数据表明,在地球早期海洋的低营养、低生产力、含铁条件下,U(VI)的还原和δ238U的分馏作用有限。
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来源期刊
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta 地学-地球化学与地球物理
CiteScore
9.60
自引率
14.00%
发文量
437
审稿时长
6 months
期刊介绍: Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes: 1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids 2). Igneous and metamorphic petrology 3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth 4). Organic geochemistry 5). Isotope geochemistry 6). Meteoritics and meteorite impacts 7). Lunar science; and 8). Planetary geochemistry.
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