IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Yuanyuan Wang , Wenshuai Li , Ryoichi Nakada , Makoto Nagasawa , Jianxi Zhu , Hongping He , Yoshio Takahashi
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引用次数: 0

摘要

本研究调查了田上山地区的碎屑岩中的铈(Ce)地球化学组成,以评估在碎屑岩形成过程中使用铈替代物进行氧化还原追踪的有效性。根据剖面上的铈同位素模式,我们将该碎屑岩分为三个不同的层:I层(0-2.0米)、II层(2.0-5.0米)和III层(5.0-8.0米)。该碎屑岩的Ce异常(Ce/Ce∗)从0.2到4.2不等,Ce主要以四价形式存在(85.3%)。值得注意的是,δ142Ce 值在 0.060 至 0.307 ‰ 之间,主要重于基岩中的δ142Ce 值(- 0.1 至 0 ‰),这与之前在风化剖面中观察到的情况相反。风化沉积对沉积岩中的δ142Ce成分影响较小,εNd模式也证明了这一点。在弱酸性条件下(pH:4.88-6.91),O2驱动的自发氧化和MnO2上的氧化吸附都会导致同位素较轻的Ce优先保留下来,而较重的Ce同位素则向下迁移。我们认为,富含较轻同位素 Ce 的原有表层(E 层)很可能已被侵蚀,而富含较重 Ce 同位素的较深 I 层(δ142Ce:0.131-0.307 ‰)则被保留了下来。此外,锰在 II 层的氧化还原循环促进了同位素较重的 Ce(δ142Ce:0.139-0.248 ‰)向下迁移,δ142Ce 值随深度增加而增加。锰氧化物的再沉淀和随后的氧化吸附作用将Ⅱ层中的Ce转化为四价形式(Bir-Ce4+,吸附在桦锰矿上的Ce4+)。底部 III 层接近基质,有微弱的风化信号,表现出有限的 Ce 同位素分馏(δ142Ce:0.078-0.161 ‰,几乎与基岩相同)。总之,结合 Ce 的元素、同位素和物种信息,可以全面了解陆地氧化还原状态和波动情况。此外,我们的研究结果还强调,在使用氧化还原敏感元素(包括 Ce 和其他氧化还原敏感元素,如 S、Fe、Mn 和 Mo)对地球表面环境进行氧化还原追踪时,需要考虑侵蚀过程。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Abnormally heavy cerium stable isotope composition in regolith: Implications for redox tracing
This study investigated the cerium (Ce) geochemical composition in the regolith at Tanakami Mountain to assess the effectiveness of using Ce proxies for redox tracing during regolith formation. Based on the in-profile Ce isotope pattern, we divided this regolith into three different layers: I (0–2.0 m), II (2.0–5.0 m), and III layers (5.0–8.0 m). The regolith exhibits Ce anomalies (Ce/Ce) ranging from 0.2 to 4.2, with Ce primarily in its tetravalent form (85.3 %). Notably, δ142Ce values range from 0.060 to 0.307 ‰, predominantly heavier than those in the bedrock (∼ − 0.1 to 0 ‰), which is contrary to previous observations in weathering profiles. Eolian deposition has a minor impact on the δ142Ce composition in the regolith, as supported by the εNd pattern. Under weakly acidic conditions (pH: 4.88–6.91), both O2-driven spontaneous oxidation and oxidative adsorption on MnO2 cause preferential retention of isotopically lighter Ce while heavier Ce isotopes migrate downward. We suggest that the pre-existing surface layer (E layer), which is enriched in isotopically lighter Ce, has likely been eroded, while the deeper I layer (δ142Ce: 0.131–0.307 ‰), enriched in heavier Ce isotopes, has been preserved. In addition, the oxidation–reduction cycling of Mn in the II layer promotes the downward migration of isotopically heavier Ce (δ142Ce: 0.139–0.248 ‰) and an increase in δ142Ce value with depth. The reprecipitation of Mn oxides and subsequent oxidative adsorption transforms Ce into its tetravalent form (Bir-Ce4+, Ce4+ adsorbed on birnessite) in the II layer. The bottom III layer, close to the substrate with subtle weathering signals exhibits limited Ce isotope fractionation (δ142Ce: 0.078–0.161 ‰, nearly identical to the bedrock). In summary, the combination of elemental, isotopic, and speciation information of Ce provides a comprehensive picture of terrestrial redox status and fluctuations. Moreover, our findings emphasize the need to consider erosion processes when using redox-sensitive elements, including Ce and other redox-sensitive elements (e.g. S, Fe, Mn, and Mo), for redox tracing in Earth’s surface environment.
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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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