Qi-Wei Li , Qiang Wang , Lin Ma , Andrew C. Kerr , Jing-Jing Fan , Jun-Hong Zhao , Hai-Ou Gu , Wei Wang , Zhi-Kun Su
{"title":"Light iron isotopes in high-silica granites record fluid evolution in magmatic-hydrothermal systems","authors":"Qi-Wei Li , Qiang Wang , Lin Ma , Andrew C. Kerr , Jing-Jing Fan , Jun-Hong Zhao , Hai-Ou Gu , Wei Wang , Zhi-Kun Su","doi":"10.1016/j.gca.2024.12.034","DOIUrl":null,"url":null,"abstract":"<div><div>High-silica (SiO<sub>2</sub> > 70 wt%) granites in continental collisional zones are crucial for understanding formation and evolution of the upper continental crust. Fluids released from felsic magmas can help drive the transition from magmatic to magmatic-hydrothermal systems in shallow magma chambers. However, the influence of these fluids on compositional variations and Fe isotope fractionation during the later stages of evolution of felsic magmas are unclear. In this contribution, we report stable Fe–Mg isotope compositions for the Paleocene Zhengga leucogranite pluton, part of the Gangdese batholith in southern Tibet. The pluton consists of both biotite granite and garnet-bearing two-mica granite, the latter of which contains zoned plagioclase and patchy K-feldspar that show fluid-mediated partial replacement textures, recording complicated magmatic and hydrothermal processes. Compared to high-silica granites worldwide (δ<sup>57</sup>Fe = +0.10 ‰ to +0.74 ‰), all rocks from the Zhengga leucogranite pluton have light and variable δ<sup>57</sup>Fe values (+0.03 ‰ to +0.28 ‰ relative to IRMM-014), which display wave-shaped variations with progressive magmatic differentiation. However, their δ<sup>26</sup>Mg values (relative to DSM-3) decrease from −0.12 ‰ to −0.72 ‰ with increasing SiO<sub>2</sub>. The variable Fe and Mg isotope signatures of the Zhengga pluton can be best explained by a three-stage process, comprising initial fractional crystallization of biotite and magnetite, followed by deuteric fluid exsolution with decreasing temperatures and pressures, and final interaction between trapped fluids and residual melts in the highly crystalline magma mush. In combination with previously published Sr–Nd–Mo isotopes on the same samples, our new results suggest that fluid exsolution is required to elevate the δ<sup>57</sup>Fe of the felsic melts by up to 0.15 permil, but subsequent fluid-melt reaction reduces the Fe isotopes and leads to similar light-Fe isotope compositions of final residual melts to their primary magma. Therefore, the high-silica granites can be enriched in light Fe isotopes due to the effects of magmatic fluids, which make a significant contribution to the formation and evolution of upper continental crust.</div></div>","PeriodicalId":327,"journal":{"name":"Geochimica et Cosmochimica Acta","volume":"391 ","pages":"Pages 277-290"},"PeriodicalIF":4.5000,"publicationDate":"2025-01-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Geochimica et Cosmochimica Acta","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0016703724006859","RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
High-silica (SiO2 > 70 wt%) granites in continental collisional zones are crucial for understanding formation and evolution of the upper continental crust. Fluids released from felsic magmas can help drive the transition from magmatic to magmatic-hydrothermal systems in shallow magma chambers. However, the influence of these fluids on compositional variations and Fe isotope fractionation during the later stages of evolution of felsic magmas are unclear. In this contribution, we report stable Fe–Mg isotope compositions for the Paleocene Zhengga leucogranite pluton, part of the Gangdese batholith in southern Tibet. The pluton consists of both biotite granite and garnet-bearing two-mica granite, the latter of which contains zoned plagioclase and patchy K-feldspar that show fluid-mediated partial replacement textures, recording complicated magmatic and hydrothermal processes. Compared to high-silica granites worldwide (δ57Fe = +0.10 ‰ to +0.74 ‰), all rocks from the Zhengga leucogranite pluton have light and variable δ57Fe values (+0.03 ‰ to +0.28 ‰ relative to IRMM-014), which display wave-shaped variations with progressive magmatic differentiation. However, their δ26Mg values (relative to DSM-3) decrease from −0.12 ‰ to −0.72 ‰ with increasing SiO2. The variable Fe and Mg isotope signatures of the Zhengga pluton can be best explained by a three-stage process, comprising initial fractional crystallization of biotite and magnetite, followed by deuteric fluid exsolution with decreasing temperatures and pressures, and final interaction between trapped fluids and residual melts in the highly crystalline magma mush. In combination with previously published Sr–Nd–Mo isotopes on the same samples, our new results suggest that fluid exsolution is required to elevate the δ57Fe of the felsic melts by up to 0.15 permil, but subsequent fluid-melt reaction reduces the Fe isotopes and leads to similar light-Fe isotope compositions of final residual melts to their primary magma. Therefore, the high-silica granites can be enriched in light Fe isotopes due to the effects of magmatic fluids, which make a significant contribution to the formation and evolution of upper continental crust.
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.