Of zircons and zircons: The tumultuous story of Zr-Hf and REE during cooling of peralkaline granites

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Loïs Monnier, Oscar Laurent, Stefano Salvi, Cyrielle Bernard, Mathieu Leisen, Guillaume Estrade, Philippe de Parseval, Claudie Josse, Armel Descamps-Mandine, Zhenpeng Duan, Sophie Gouy, Caliméria Passos do Carmo, Camille Dusséaux
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引用次数: 0

Abstract

Understanding the behavior of trace elements such as Zr-Hf, REE, and Th-U during magmatic and hydrothermal processes is crucial for unraveling the evolution of rare-metal peralkaline granites. These elements play key roles in geochemical cycles, mineral formation, and economic mineral deposits. The Evisa intrusion, a rare-metal peralkaline granite, is an ideal setting to study such processes due to its diverse zircon population, which records a continuous transition from early igneous to late hydrothermal precipitation and alteration. This evolution spans temperatures from more than 600 °C to approximately 150 °C, with zircon demonstrating exceptional diversity in textures and compositions. In-situ U-Pb dating of both igneous and hydrothermal zircon suggests they precipitated coevally at ∼ 270 Ma, indicating the synchronous formation and alteration of zircon during the crystallization and cooling of the Evisa granite. Hf isotopic compositions vary from 0 to + 10 εHf(t) for igneous zircon and from −5 to + 5 εHf(t) for hydrothermal zircon, reflecting a shift from a mantle-derived to a more crustal signature. Both U-Pb and Hf isotopic data support a rift-related context for the Corsica terrane during the late Permian. Zircon in this granite is highly enriched in REE (median value > 2 wt% for Y + REE) and variably enriched in U and Th (up to several wt.%), with igneous zircon exhibiting higher Ce anomalies and HREE/LREE ratios than hydrothermal zircon. Alteration of zircon results in the formation of pores (ranging from nm to µm scale) and the redistribution of trace metals between newly-formed mineral inclusions, newly-crystallized zircon, and the aqueous fluid. This redistribution, combined with the breakdown of other REE-minerals and availability of suitable ligands in the fluid, controlled the cyclic enrichment of REE in hydrothermal zircon and influenced their fate in the Evisa granite. Hydrothermal remobilization of Hf at low temperature led to significant Hf isotopic variations (up to > 20 εHf(t) unit) in newly crystallized zircon, likely due to mass-dependent kinetic fractionation. Discrepancies in the Zr/Hf ratio (from ∼ 0.5 to 2.5) in successive growth zones of hydrothermal zircon were interpreted as resulting from fractionation due to mass-independent effects on bond strength during transport, probably in the form of fluoride complexes. This study not only provides new insights into the behavior of Zr-Hf, Th-U and REE in rare-metal peralkaline granites but also underscores the need for caution when interpreting zircon compositions, particularly when using commonly employed geochemical tools, such as Ti-based thermometers.
锆石与锆石:过碱性花岗岩冷却过程中Zr-Hf和REE的动荡故事
了解Zr-Hf、REE、Th-U等微量元素在岩浆和热液过程中的行为对揭示稀土过碱性花岗岩的演化具有重要意义。这些元素在地球化学旋回、矿物形成和经济矿床中起着关键作用。Evisa岩体是一种稀有金属的过碱性花岗岩,其锆石种群多样化,记录了从早期火成岩到晚期热液沉淀和蚀变的连续转变,是研究这一过程的理想环境。锆石的演化范围从600°C到大约150°C,锆石在结构和成分上表现出异常的多样性。火成岩锆石和热液锆石的原位U-Pb测年结果表明,它们在~ 270 Ma时共卵状沉积,表明在Evisa花岗岩的结晶和冷却过程中,锆石是同步形成和蚀变的。火成岩锆石的Hf同位素组成变化范围为0 ~ + 10 εHf(t),热液锆石的Hf同位素组成变化范围为- 5 ~ + 5 εHf(t),反映了地幔演化特征向地壳演化特征的转变。U-Pb和Hf同位素数据均支持科西嘉地体在晚二叠纪时期与裂谷相关的背景。该花岗岩中锆石高度富集稀土元素(中值>;2 wt% (Y + REE), U和Th的富集程度不同(可达数wt%),火成岩锆石的Ce异常和HREE/LREE比值高于热液锆石。锆石蚀变导致孔隙(nm ~µm)的形成,微量金属在新形成的矿物包裹体、新结晶的锆石和水流体之间重新分布。这种再分配,结合流体中其他稀土矿物的分解和合适配体的可用性,控制了热液锆石中稀土元素的循环富集,并影响了它们在Evisa花岗岩中的命运。低温水热再活化Hf导致Hf同位素显著变化(高达>;20 εHf(t)单位),可能是由于质量依赖的动力学分馏作用。在热液锆石的连续生长带中,Zr/Hf比值的差异(从~ 0.5到2.5)被解释为由于运输过程中对键强度的质量无关效应而产生的分馏,可能以氟化物配合物的形式出现。这项研究不仅对稀土过碱性花岗岩中Zr-Hf、Th-U和REE的行为提供了新的见解,而且还强调了在解释锆石成分时需要谨慎,特别是在使用常用的地球化学工具(如ti基温度计)时。
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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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