Barium isotope variation during granitic magma differentiation: implications for the discrimination of crystal fractionation and fluid-magma interaction

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Nian-Qin Zhang, Kun Zhou, Yi-Xiang Chen, Fang Huang, Xiao-Feng Gu, Lin-Hui Dong, Gengxin Deng, Peng Gao
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Abstract

The genesis and compositional diversity of granites are primarily controlled by multiple processes, including partial melting and magma differentiation. However, discriminating the individual effects of processes such as partial melting, fractional crystallization, and fluid-magma interaction on the evolution of granitic magma remains challenging. Barium isotopes serve as a potentially powerful tracer for discrimination between fractional crystallization and fluid-magma interaction processes, yet the effect of fractionation crystallization on Ba isotope composition variation remains poorly constrained. To tackle this challenge, we measured the Ba isotope compositions of syn-exhumation granites from the Sulu orogen in eastern China. These high-Si granites exhibit significant variations in δ138/134Ba values (–0.69 ‰ to 0.36 ‰). Using phase equilibrium modeling, we estimate that the Ba isotope variation during partial melting process can result in an increase of less than ca. 0.20 ‰ between melts and protoliths, which cannot account for the observed light Ba isotope compositions. Additionally, the content of SiO2 is significantly correlated with contents of other major and trace elements, such as Al2O3, TiO2, Fe2O3t, Ba, Sr and Eu/Eu*, suggesting extensive fractional crystallization in these granites. Moreover, δ138/134Ba values exhibit good correlations with the compositions of such major and trace elements, indicating large Ba isotopic variation during the fractional crystallization of granitic magmas. In contrast, the Zr/Hf, K/Rb, Nb/Ta ratios and REE patterns of the syn-exhumation granites indicate the absence of fluid-magma interaction. These observations indicate that fractional crystallization, rather than fluid-magma interaction, is the primary factor driving significant Ba isotope fractionation in the granites, resulting in δ138/134Ba values as low as −0.69 ‰. Using fractional crystallization modelling with rhyolite-MELTS, we demonstrate that the fractional crystallization of K-feldspar, biotite and muscovite controls the Ba isotope variation of granites, consistent with the petrological observations. Combined with previous results from leucogranites and strongly fractionated granites, we document that it should be taken caution when using Ba isotope compositions to trace the fluid-magma interaction. While crystal fractionation can lead to δ138/134Ba values as low as ca. −0.7 ‰ in granites, values lower than this can be more unambiguously attributed to fluid-magma interaction during the late-stage differentiation of granitic magma.
花岗岩岩浆分异过程中钡同位素的变化:对晶体分异和流体-岩浆相互作用鉴别的意义
花岗岩的成因和成分多样性主要受部分熔融和岩浆分异等多种作用的控制。然而,区分部分熔融、分离结晶和流体-岩浆相互作用等过程对花岗质岩浆演化的个别影响仍然具有挑战性。钡同位素可作为区分分馏结晶和流体-岩浆相互作用过程的潜在有力示踪剂,但分馏结晶对钡同位素组成变化的影响尚不明确。为了应对这一挑战,我们测量了中国东部苏鲁造山带同出土花岗岩的Ba同位素组成。高硅花岗岩δ138/134Ba值变化显著(-0.69‰~ 0.36‰)。利用相平衡模型,我们估计部分熔融过程中Ba同位素的变化可能导致熔体与原岩之间的增加小于0.20‰,这不能解释观测到的轻Ba同位素组成。此外,SiO2含量与Al2O3、TiO2、Fe2O3t、Ba、Sr、Eu/Eu*等主微量元素含量呈显著相关,表明这些花岗岩中存在广泛的分馏结晶。此外,δ138/134Ba值与这些主微量元素的组成具有良好的相关性,表明在花岗质岩浆分馏结晶过程中Ba同位素变化较大。与此相反,同出土花岗岩的Zr/Hf、K/Rb、Nb/Ta比值和稀土元素模式表明岩浆与流体的相互作用不存在。这些观测结果表明,分馏结晶作用,而不是流体-岩浆相互作用,是导致花岗岩中Ba同位素分馏显著的主要因素,导致δ138/134Ba值低至- 0.69‰。利用流纹岩- melts分馏结晶模拟表明,钾长石、黑云母和白云母的分馏结晶控制了花岗岩Ba同位素的变化,与岩石学观测结果一致。结合前人对浅花岗岩和强分选花岗岩的研究结果,认为利用Ba同位素组成进行流体-岩浆相互作用的示踪需要谨慎。虽然晶体分馏作用可导致花岗岩δ138/134Ba值低至约- 0.7‰,但较低的δ138/134Ba值更明确地归因于花岗岩岩浆后期分化过程中的流体-岩浆相互作用。
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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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