Potassium isotope composition in global loess: Origins and implications

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Wenshuai Li, Xiao-Ming Liu, Kun Wang, Mohsen Shakouri, Catherine Chauvel
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Abstract

Potassium (K) isotope compositions (δ41K) in global loess deposits can provide valuable insights into the average upper continental crust (UCC). However, current knowledge of δ41K in the UCC is limited due to the lithological complexity of the continental crust, which results in highly variable K isotope compositions. Accurately estimating the K isotope composition of the UCC remains a challenge. Here, we investigated the concentration, phase, and isotopic composition of K in loess samples from Asia, Europe, Oceania, North America, and South America to identify the dominant controls on loess δ41K and better constrain the average composition of the UCC. Our results show that the δ41K value in globally compiled loess ranges from −0.60 ± 0.08 ‰ to −0.33 ± 0.04 ‰, with an average of −0.46 ± 0.12 ‰ (2 S.D.). This loess-based δ41K value of the average UCC is comparable to the average δ41K value established from various crustal materials by Huang et al. (2020). Nonetheless, our new range is slightly narrower compared with the previous estimation. We infer the measured K isotope variation in loess reflects a result of eolian sorting rather than chemical weathering. The abundance of 39K-rich illite is the primary driver of the δ41K variability in these loess samples. We suggest that the K isotope composition in bulk loess record provide more reliable information of the grain size sorting effect and thus inferring regional wind patterns (e.g., past monsoon variation).
全球黄土钾同位素组成:成因及其意义
全球黄土沉积物中钾(K)同位素组成(δ41K)为研究平均上大陆地壳(UCC)提供了有价值的信息。然而,由于大陆地壳的岩性复杂性,目前对UCC中δ41K的认识有限,这导致了K同位素组成的高度变化。准确估计UCC的K同位素组成仍然是一个挑战。本文研究了亚洲、欧洲、大洋洲、北美和南美黄土样品中K的浓度、相和同位素组成,以确定黄土δ41K的主要控制因素,并更好地约束UCC的平均组成。结果表明,全球黄土的δ41K值在−0.60±0.08‰~−0.33±0.04‰之间,平均值为−0.46±0.12‰(2 S.D.)。这种基于黄土的平均UCC δ41K值与Huang等(2020)基于各种地壳物质建立的平均δ41K值相当。尽管如此,与之前的估计相比,我们的新范围略窄。我们推测黄土中K同位素的变化反映了风成分选的结果,而不是化学风化的结果。富39k伊利石的丰度是黄土样品δ41K变化的主要驱动因素。我们认为,大块黄土记录中的K同位素组成提供了更可靠的粒度分选效应信息,从而推断区域风型(如过去季风变化)。
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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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