Zhao Wang , Michael F. Hochella Jr , Yiren Duan , Ganlin Zhang , Xiancai Lu , Wei Li
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引用次数: 0
Abstract
Goethite is essential in controlling Zn mobility and behavior in surface environments and can strongly influence Zn isotope fractionation through adsorption processes. However, the influence of particle size of goethite on stable isotopic fractionation remains poorly understood. This research investigates the fractionation of Zn stable isotopes during adsorption onto nano- and micro-goethite, focusing on factors such as reaction duration, Zn concentrations, and pH. The findings reveal that equilibrium in Zn isotope fractionation is achieved after roughly 48 h at pH 6 in both nano- and micro-goethite systems. For nano-goethite, the isotopic fractionation between adsorbed and aqueous Zn (Δ66Znadsorbed–aqueous) remains around −0.1 ± 0.04 ‰, regardless of pH and initial Zn concentrations. During Zn adsorption on micro-goethite, a significantly more negative fractionation of Δ66Znadsorbed–aqueous = − 0.40 ± 0.04 ‰ is observed. Extended X-ray absorption fine structure (EXAFS) spectroscopy shows that Zn binds to the surface of nano-goethite as a combination of inner-sphere octahedral and tetrahedral surface complexes, with average ZnO bond lengths ranging from 2.00 to 2.02 Å. In contrast, on micro-goethite, Zn predominantly exists as a distorted octahedral structure, exhibiting an average ZnO interatomic distance of 2.09 Å. Our findings suggest that the size-dependent Zn isotope fractionation in goethite is driven by the structural differences in the Zn surface complexes formed on nano- and micro-goethite. These results provide valuable insights into Zn isotope signatures in natural iron-rich soils, supporting the use of Zn isotopes as tracers for understanding the fate of Zn influenced by iron minerals in soil environments.
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.