Experimental pathways of clay formation and kinetics of basalt alteration in poor drainage systems: Implications for weathering

IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Geochimica et Cosmochimica Acta Pub Date : 2025-01-31 DOI:10.1016/j.gca.2025.01.042
Piyush Sriwastava , Vijay Kumar Saini , George Mathew , Anil D. Shukla
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Abstract

Basalt being the most dominant rock on the earth’s crust, contributes significantly to the global elemental cycle through weathering. In recent years, the potential of basalt weathering has been continuously scrutinized as a carbon dioxide removal (CDR) strategy. An accurate estimation of such large-scale processes requires a deeper insight into the mechanism controlling the basalt glass dissolution under field conditions. This contribution assesses the chemical evolution of fluid interacting with basalt glass in poorly drained regimes. Experiments showed a drop in kinetics of alteration (r0 = 1.7 × 10-9 mol.m−2. s−1) by two orders of magnitude in 24 days and emphasizes the onset of secondary mineral formation within 20 hr of the start of dissolution. At first, Mg starts fractionating from the solution due to brucite oversaturation and reaches undersaturation after 60th hour due to onset of other Mg-bearing minerals. From the 54th hour, montmorillonite remains oversaturated until Mg is entirely consumed by precipitation at the 164th hour. SEM-EDS investigation shows the presence of two major morphologies of secondary products: (a) honeycomb shape (smectite), with high Mg (>3 wt%) and octahedral composition similar [(Si/Al + Fe + Mg) and Al/Si] to smectite, (b) aggregate of ellipsoid and/or equant granular phases. Compositionally, elliptical and granular aggregates show affinity towards low Mg and high Fe variety of smectite amorphous precursor. The absence of pure brucite grains indicates epitaxial growth of Mg-rich, honeycomb-shaped phyllosilicate precursor on the brucite template due to well-reported structural similarity between the brucite layer and 2:1 phyllosilicate octahedral sheet. Elliptical and equant-shaped grains with or without compositional similarity with smectite phases have high Fe and low Mg, indicating their formation under a low Mg concentration stage in solution. Precipitation of the secondary phases at various stages of reaction progress affects the total reaction affinity in a closed system. Coupled dissolution and precipitation at the fluid-rock interface are responsible for lowering the kinetics of dissolution reactions in a closed system, previously explaining the slow kinetics of natural weathering regimes. The damped kinetics of dissolution and cations fractionation in secondary products within a few hours of onset of dissolution reaction can result in an overestimation (ten times) of CDR potential estimation by enhanced rock weathering (ERW) if calculations do not involve the nature of closed system evolution during basalt glass alteration.
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不良排水系统中粘土形成和玄武岩蚀变动力学的实验路径:对风化的影响
玄武岩是地壳上最主要的岩石,通过风化作用对全球元素循环有重要贡献。近年来,玄武岩风化的潜力作为一种二氧化碳去除(CDR)策略不断受到关注。要准确估计这种大规模的过程,需要更深入地了解在野外条件下控制玄武岩玻璃溶解的机制。这一贡献评估了在不良排水条件下流体与玄武岩玻璃相互作用的化学演化。实验表明,蚀变动力学下降(r0 = 1.7 × 10-9 mol.m−2)。S−1)在24天内增加了两个数量级,并强调在溶解开始后20小时内开始形成次生矿物。一开始,由于水镁石的过饱和,Mg开始从溶液中析出,60小时后,由于其他含镁矿物的开始,Mg达到欠饱和状态。从第54小时开始,蒙脱石保持过饱和状态,直到第164小时Mg被沉淀完全消耗。SEM-EDS研究表明,二次产物存在两种主要形态:(a)蜂窝状(蒙脱石),具有高Mg (> 3wt %)和类似于蒙脱石的八面体组成[(Si/Al + Fe + Mg)和Al/Si], (b)椭球和/或等颗粒相聚集。在成分上,椭圆和粒状团聚体对低Mg和高Fe的蒙脱石非晶态前驱体表现出亲和力。纯水镁石颗粒的缺失表明富镁的蜂窝状层状硅酸盐前驱体在水镁石模板上外延生长,这是由于已有报道的水镁石层与2:1层状硅酸盐八面体片的结构相似。与蒙脱石相成分相似或不相似的椭圆和等形晶粒具有高Fe和低Mg的特征,表明它们是在溶液中低Mg浓度阶段形成的。在封闭体系中,反应过程中各阶段次级相的析出影响着反应的总亲和度。流体-岩石界面处的耦合溶解和沉淀降低了封闭系统中溶解反应的动力学,从而解释了自然风化机制的缓慢动力学。如果不考虑玄武岩玻璃蚀变过程中封闭体系演化的性质,溶蚀反应开始后数小时内二次产物中溶蚀和阳离子分异的阻尼动力学可能导致增强岩石风化作用(ERW)对CDR电位估计的高估(10倍)。
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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.
期刊最新文献
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