Titanium transport and isotopic fractionation in the Critical Zone

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Geochimica et Cosmochimica Acta Pub Date : 2023-07-01 DOI:10.1016/j.gca.2023.05.008
Sarah M. Aarons , Nicolas Dauphas , Nicolas D. Greber , Mathieu Roskosz , Julien Bouchez , Tamara Carley , Xiao-Ming Liu , Roberta L. Rudnick , Jérôme Gaillardet
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Abstract

Stable Ti isotopes have been applied in the detrital sediment record to reconstruct the bulk composition of Earth’s continental crust due to the relationship between magmatic differentiation and Ti isotopic compositions. However, no study has systematically evaluated the influence of provenance, physical, and chemical weathering on the composition of sediments relative to the protolith they originated from. To test the influence of these processes on Ti isotopic compositions we investigate the Ti isotope composition of 82 surface samples including loess, volcaniclastic rocks, river sediment, and two separate weathering profiles through igneous rocks, collected from a broad geographical area and a range of environmental conditions. Limited but significant Ti isotope fractionation exists in samples subjected to extreme chemical weathering processes, potentially as a result of elemental mobilization. For example, the δ49Ti isotopic composition of bauxites developed on Columbia River basalt varies by up to 0.1‰, becoming isotopically heavier with increasing weathering intensity. However, negligible variation in δ49Ti was found in a second profile of saprolites developed on weathered diabase. Titanium isotope variations in loess do not correlate with chemical weathering intensity or size sorting, but may instead be related to the provenance of the sediment. We find that the δ49Ti of Amazon River sediments is correlated with the Al/Zr ratio, indicating that δ49Ti is impacted by sediment sorting. At our study sites, the river averaged offset between the isotopic composition of the bedload and the suspended sediment fraction is 0.051‰, with the largest offset being + 0.116‰. Our data suggest that during chemical weathering, heavy Ti isotopes are preferentially incorporated into secondary minerals producing higher δ49Ti in intensely weathered soils. During fluvial transport, the Ti isotopic composition of fine-grained sediment is heavier than that of its coarser counterpart. Crustal protolith composition and sorting during transport and sedimentation have a stronger effect on the Ti isotopic composition than chemical weathering. Our results have implications for studies that utilize the Ti elemental concentration to calculate relative enrichment or depletion during chemical weathering and physical transport processes in the Critical Zone and for studies using Ti isotopes in terrigenous sediments to infer the composition of their provenance.

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临界带钛输运与同位素分馏
由于岩浆分异与钛同位素组成的关系,稳定的钛同位素已被应用于碎屑沉积物记录中,以重建地球大陆地壳的总体组成。然而,目前还没有研究系统地评估物源、物理和化学风化对沉积物成分相对于其起源的原岩的影响。为了测试这些过程对Ti同位素组成的影响,我们研究了82个表面样品的Ti同位素组成,包括黄土,火山碎屑岩,河流沉积物和两个单独的风化剖面,通过火成岩,从广泛的地理区域和一系列环境条件中收集。在经受极端化学风化过程的样品中存在有限但显著的钛同位素分馏,这可能是元素动员的结果。例如,哥伦比亚河玄武岩上发育的铝土矿δ49Ti同位素组成差异最大可达0.1‰,随着风化强度的增加,其同位素组成逐渐变重。然而,在风化辉绿岩上发育的第二剖面中,δ49Ti的变化可以忽略不计。黄土中钛同位素的变化与化学风化强度或粒度分选无关,而可能与沉积物的物源有关。发现亚马逊河沉积物的δ49Ti与Al/Zr比值相关,表明δ49Ti受沉积物分选的影响。在研究点,河床沉积物同位素组成与悬沙组分的平均偏移量为0.051‰,最大偏移量为+ 0.116‰。我们的数据表明,在化学风化过程中,重Ti同位素优先结合到次生矿物中,在强风化土壤中产生较高的δ49Ti。在河流搬运过程中,细粒沉积物的钛同位素组成比粗粒沉积物重。搬运和沉积过程中地壳原岩组成和分选对钛同位素组成的影响大于化学风化作用。我们的研究结果对利用Ti元素浓度来计算临界带化学风化和物理搬运过程中的相对富集或亏缺的研究以及利用陆源沉积物中的Ti同位素来推断其物源组成的研究具有指导意义。
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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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