Fluid systems captured by giant amethyst-hosted fluid inclusions from continental flood basalts

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Marta Sośnicka , Samuel Niedermann , Rudolph Erasmus , Sharad Master
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Abstract

Continental flood basalt (CFB) provinces, defined by the rapid emplacement of large volumes of mafic lava, represent some of the most significant large-scale magmatic events in Earth’s geological record. Gaining insight into the origin and evolution of fluid systems within these settings is critical for understanding the geodynamic architecture of large igneous provinces (LIPs) and accompanying mineralisation processes. However, the provenance and reservoirs of hydrothermal fluid systems in CFB settings remain poorly constrained. This study provides new evidence on the origin and sources of fluids responsible for the formation of amethyst mineralisation within a CFB context. Unique, giant fluid inclusions entrapped in amethyst crystals enabled reconstruction of variations in fluid system dynamics during incremental crystal growth in the geodes, which developed in the LTZ.L series Goboboseb basalts in an active continental flood basalt volcanic setting of the Paraná-Etendeka CFB Province.
Three compositionally different types of fluid inclusions, namely H2O-NaCl-N2-CH4, N2-CH4-CO2 and N2-CH4, preserved in individual amethyst and quartz crystals have archived an intricate fluid evolution history. Amethyst crystallisation commenced at moderate temperatures (281–327 °C) from low salinity (0.3–8.7 wt% NaCl equiv.) aqueous H2O-NaCl-N2-CH4 fluid. As crystal growth rates decreased and the fluid system cooled to 160–211 °C, some crystals captured fluid boiling/phase separation in the environment of ongoing magmatic CO2 degassing. Fluid properties and fluid-host rock thermal equilibrium, coupled with high SiO2 and H2O contents of the low Ti/Zr LTZ.L series basalts, support a magmatic-hydrothermal origin of the aqueous fluid. For the first time, fluid inclusion noble gas data reveal unequivocal evidence of deep primordial mantle contributions (3He) to magmatic-hydrothermal fluids involved in amethyst formation. The results provide convincing evidence for the Tristan da Cunha plume-related magmatism in the Paraná-Etendeka CFB Province and confirm that deep-sourced volatiles can migrate into shallow crustal levels via magmatic degassing. Strongly elevated 40Ar*/4He, nucleogenic 21Ne/22Ne isotope ratios and crustal δ15N signatures of fluids indicate significant assimilation of continental crust and entrainment of old crustal fluids during magma fractionation in feeder chambers at different crustal levels above the Tristan da Cunha mantle plume, supporting models of lithospheric recycling and magma-crust interaction. The engagement of multi-source fluid systems, predominantly mantle and crust-derived, across different evolution stages shows the complexity of fluid systems in CFB volcanic settings. Moreover, the findings of this study demonstrate that not only post-magmatic, but also syn-magmatic fluids are capable of generating gemstone-grade amethyst mineralisation and thus bring to light the untapped mineral potential of underexplored areas in the CFB settings worldwide.
大陆洪泛玄武岩中巨型紫水晶包裹体捕获的流体系统
大陆洪水玄武岩(CFB)省,以大量岩浆的快速就位为特征,代表了地球地质记录中一些最重要的大规模岩浆事件。了解这些环境中流体系统的起源和演化对于理解大火成岩省(lip)的地球动力学结构和伴随的矿化过程至关重要。然而,在循环流化床环境下,热液流体系统的物源和储层仍然知之甚少。本研究为CFB环境下紫水晶矿化形成流体的起源和来源提供了新的证据。紫水晶晶体中包裹着独特的巨大流体包裹体,可以重建在LTZ中形成的晶洞中晶体增量生长过程中流体系统动力学的变化。Paraná-Etendeka CFB省活大陆洪水玄武岩火山背景下L系列Goboboseb玄武岩
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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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