Whole-rock Mg isotopes distinguishing high- and low-temperature S-type granites

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Yan Wang, Peng Gao, Zi-Fu Zhao, Hai-Ou Gu, Guo-Chao Sun, Hui-Chan Huang, Zhang-Jian Wu, Changqing Yin
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Abstract

Determining the temperature of crustal anatexis associated with granitic magmatism is vital for understanding the petrogenesis of granites and the processes underlying crustal anatexis. During the partial melting of metasedimentary rocks, the breakdown of biotite at elevated temperatures can lead to the formation of peritectic garnet, which is typically rare or absent at lower temperatures when melting is predominantly driven by muscovite breakdown. This distinction makes magnesium (Mg) isotopes a valuable tool for tracing relative variations in crustal melting temperatures, as garnet exhibits the lowest δ26Mg values compared to other Mg-bearing phases under equilibrium fractionation. However, the extent to which temperature variations influence melt Mg isotope compositions remains inadequately understood. In this study, we present Mg and oxygen isotope data for high- and low-temperature leucogranites from the Himalayan orogen, alongside whole-rock major and trace element data, and zircon Ti content from previous studies. Low-temperature leucogranites, with maximum Ti-in-zircon temperatures ranging from 739 to 801 °C, display negative δ26Mg values between −0.70 and −0.14 ‰, aligning with most global S-type granites. Conversely, high-temperature leucogranites, exhibiting maximum Ti-in-zircon temperatures of 800 to 855 °C, possess positive δ26Mg values ranging from 0.46 to 0.53 ‰, significantly exceeding those of Himalayan metasedimentary rocks and most global S-type granites. The high-temperature leucogranites also demonstrate relatively elevated Nb/Ta and Eu/Eu* ratios, while their whole-rock δ18O and CIA values are comparable to those of low-temperature leucogranites. These findings suggest that fluid alteration, fractional crystallization, and crustal assimilation have a minimal impact on the Mg isotope discrepancies between the two granite groups. We propose that the positive δ26Mg values of the high-temperature leucogranites result from a greater fraction of peritectic garnet in the melting residue, attributable to higher anatectic temperatures. Phase equilibrium modeling indicates that the peritectic reaction involving muscovite breakdown is swiftly replaced by biotite breakdown as temperatures rise, leading to a steady increase in the corresponding fraction of garnet. Equilibrium fractionation calculations further corroborate that melt δ26Mg values rise with an increasing fraction of peritectic garnet, with values at high temperatures significantly surpassing those at lower temperatures. Consequently, this study elucidates a causal relationship between Mg isotope composition and anatectic temperature, highlighting that whole-rock Mg isotopes can serve as a reliable indicator for distinguishing between high- and low-temperature S-type granites.
区分高低温s型花岗岩的全岩Mg同位素
确定与花岗质岩浆作用相关的地壳深熔温度对于了解花岗岩的岩石成因和地壳深熔过程至关重要。在变质沉积岩的部分熔融过程中,黑云母在高温下的分解可形成包晶石榴石,而在较低温度下,当熔融主要由白云母分解驱动时,包晶石榴石通常很少或不存在。这种区别使得镁(Mg)同位素成为追踪地壳熔融温度相对变化的有价值的工具,因为在平衡分馏下,石榴石的δ26Mg值与其他含镁相相比最低。然而,温度变化对熔体Mg同位素组成的影响程度仍未得到充分了解。在这项研究中,我们提供了喜马拉雅造山带高低温亮花岗岩的Mg和氧同位素数据,以及整个岩石的主要和微量元素数据,以及锆石Ti含量。低温白花岗岩的最大ti -in-锆石温度范围为739 ~ 801℃,δ26Mg值为- 0.70 ~ - 0.14‰,与全球大多数s型花岗岩一致。高温亮花岗岩的最大ti -in-锆石温度为800 ~ 855℃,δ26Mg值为0.46 ~ 0.53‰,显著高于喜马拉雅变质沉积岩和全球大多数s型花岗岩。高温白花岗岩的Nb/Ta和Eu/Eu*比值也相对较高,全岩δ18O和CIA值与低温白花岗岩相当。这些结果表明,流体蚀变、分离结晶和地壳同化作用对两组花岗岩Mg同位素差异的影响很小。我们认为高温亮花岗岩的正δ26Mg值是由于熔渣中含有更多的包晶石榴石,这是由于较高的析晶温度造成的。相平衡模型表明,随着温度的升高,涉及白云母分解的包晶反应迅速被黑云母分解所取代,导致相应的石榴石分数稳步增加。平衡分馏计算进一步证实,熔体δ26Mg值随着包晶石榴石含量的增加而增加,高温时的值明显超过低温时的值。因此,本研究阐明了镁同位素组成与深熔温度之间的因果关系,强调全岩镁同位素可以作为区分高低温s型花岗岩的可靠指标。
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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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