Tracing hydrous eclogite melts in the source of sanukitoids

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Earth and Planetary Science Letters Pub Date : 2024-10-15 DOI:10.1016/j.epsl.2024.119067
L.M. Spencer , C. Albert , H.M. Williams , O. Nebel , I.J. Parkinson , R.H. Smithies , H. Bruno , M. Fowler , H. Moreira , C.J. Lissenberg , M.-A. Millet
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Abstract

Sanukitoids are unique Archean and early Proterozoic igneous rocks. They contain high amounts of Mg, Ni and Cr, showing they are mantle-derived melts, while they are also enriched in Sr and Ba and have relatively high K contents, requiring the involvement of an incompatible element-enriched component likely derived from recycled crustal material. The appearance of sanukitoids in the geological record coincides with a shift in continental crust composition, and both events have been linked to a change in geodynamic processes on Earth. However, uncertainties remain about sanukitoid petrogenesis, in particular whether their mantle source was metasomatised by a metabasite-derived silicate melt or by an aqueous fluid. Titanium (Ti) stable isotopes can trace magmatic processes where silicate melts are in equilibrium with Fe-Ti oxides and amphibole but are insensitive to fluid-driven processes, making them a suitable tool to investigate not only the formation of sanukitoid magmas but also their subsequent evolution. Here we present Ti isotope data (δ49Ti) for a series of Neoarchean sanukitoids from the Yilgarn Craton that continuously covers the full compositional range of sanukitoids. These are complemented by Mesoarchean sanukitoids and Paleoarchean “sanukitoid-like” rocks from the Pilbara Craton, and by Paleoproterozoic sanukitoids from the São Francisco Craton/Paleocontinent. In addition, we analysed Paleozoic high Ba-Sr granite suites from Scotland, which are proposed to be Phanerozoic sanukitoid analogues.
Evolved sanukitoids, which formed after Fe-Ti oxide saturation, show a more muted δ49Ti increase during differentiation compared to currently analysed modern calc-alkaline suites. This difference is best explained by removal of significant proportions of Ti during sanukitoid differentiation by magmatic hornblende, which fractionates Ti isotopes less strongly than Fe-Ti oxides. Combined with early oxide saturation at high Mg#, this suggests that sanukitoid parental magmas had H2O contents and fO2 at least as high as modern arc magmas. Primitive (pre-oxide saturation) sanukitoids, however, have significantly higher δ49Ti (0.11–0.20‰) than modern arc basalts, the depleted mantle and the bulk silicate Earth (BSE). Their elevated δ49Ti values cannot be explained by aqueous fluids alone in their mantle source, and instead require the involvement of a hydrous eclogite melt component formed in equilibrium with residual rutile. We favour generation of this metasomatic melt by fluid-fluxed eclogite partial melting, demonstrating that both metabasite melts and aqueous fluids are important for sanukitoid formation. The Ti isotope compositions of Archean and Paleoproterozoic sanukitoids therefore favour formation of the sanukitoid mantle source by a subduction-like process at least ∼2.7 Ga.
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追踪萨努基托岩源中的含水蚀变岩熔体
萨努基托岩是一种独特的阿新世和新生代早期火成岩。它们含有大量的镁、镍和铬,表明它们是地幔熔体,同时还富含锶和钡,钾含量也相对较高,这就要求有不相容元素富集的成分参与其中,而这些不相容元素富集的成分很可能来自回收的地壳物质。地质记录中出现萨努基多岩的时间与大陆地壳成分的变化相吻合,这两个事件都与地球地球动力过程的变化有关。然而,萨努基托岩成岩过程仍存在不确定性,特别是它们的地幔源是由新元古代硅酸盐熔体还是由水流体变质而成。钛(Ti)稳定同位素可以追踪硅酸盐熔体与铁钛氧化物和闪石处于平衡状态的岩浆过程,但对流体驱动过程不敏感,因此钛同位素不仅是研究萨努基特类岩浆形成过程的合适工具,也是研究其后续演化过程的合适工具。在这里,我们展示了来自伊尔加恩克拉通的一系列新元古代萨努基特岩的钛同位素数据(δ49Ti),这些数据连续涵盖了萨努基特岩的全部成分范围。皮尔巴拉克拉通的中新世砂岩和古新世 "类砂岩 "以及圣弗朗西斯科克拉通/古陆的古近纪砂岩对这些岩石进行了补充。此外,我们还分析了来自苏格兰的古生代高钡锶花岗岩套件,这些套件被认为是新生代sanukitoid的类似物。与目前分析的现代钙碱性套件相比,在铁钛氧化物饱和之后形成的进化sanukitoids在分化过程中显示出更为柔和的δ49Ti增加。这种差异的最佳解释是,岩浆角闪石在三绢云母分异过程中去除了大量的Ti,而角闪石对Ti同位素的分馏作用不如Fe-Ti氧化物强烈。结合高 Mg# 时的早期氧化物饱和,这表明三琉球母岩的 H2O 含量和 fO2 至少与现代弧岩浆一样高。然而,原始(氧化物饱和前)萨努基托岩浆的δ49Ti(0.11-0.20‰)明显高于现代弧玄武岩、贫化地幔和大块硅酸盐地球(BSE)。它们升高的δ49Ti值不能仅用地幔源中的水性流体来解释,而需要与残余金红石平衡形成的含水闪长岩熔体成分的参与。我们倾向于通过流体通量的斜长岩部分熔融来生成这种偏闪长岩熔体,从而证明偏闪长岩熔体和水成流体对于砂岩的形成都很重要。因此,阿新世和古新生代沙努基托岩的Ti同位素组成倾向于沙努基托岩地幔源是通过至少∼2.7 Ga的类似俯冲过程形成的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Earth and Planetary Science Letters
Earth and Planetary Science Letters 地学-地球化学与地球物理
CiteScore
10.30
自引率
5.70%
发文量
475
审稿时长
2.8 months
期刊介绍: Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.
期刊最新文献
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