海底太古宙马长岩的水化作用:来自微量元素和氧同位素的证据

IF 2.5 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Renée Tamblyn , Jörg Hermann , Daniela Rubatto , Anne-Sophie Bouvier
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引用次数: 0

摘要

在现代地球上,由海底蛇纹石作用水化的地幔岩石在地质(深层)水循环中起着重要作用。然而,在太古宙,地质水循环可能有所不同。超镁铁质岩石以高镁铁质岩浆、高镁铁质羽流衍生的熔岩等形式存在于海洋高原或大陆边缘。先前的研究表明,这些科马长岩主要在海底环境中喷发,并且含有大量的水结合在反长花岗岩、绿泥石和透闪石中(约6 wt%)。本文给出了Kaapvaal、Superior、Singhbhum、Yilgarn和Pilbara克拉通水化科马铁矿的原位微量元素和氧同位素数据,进一步约束了海底水化过程中的热条件和元素吸收。与可能的科马长岩熔体组成相比,硅酸盐相富含B、W、as、Sb和Pb等可流动元素。这些流体流动元素来源于海水,或者可能是海水-沉积物平衡流体。橄榄石的δ18O组成呈地幔状(~ 5.5‰),反长岩的δ18O组成在样品内均匀分布,大部分落在+1.5 ~ 4.1‰之间。对太古宙δ18O组成为- 1‰的平衡态蛇纹石的氧同位素模拟表明,这些样品在科马铁矿结晶后,在~ 150-210℃的温度下水化。科马提岩熔岩的普遍水化可能是由于它们的高表面积,因为它们喷发时是广泛而薄的流动。温度驱动的流体循环可能是由于下伏和上覆熔岩流的冷却、岩浆注入或靠近地幔柱而促进的。尽管在地质记录中它们的丰度相对较低,但太古代的科马提岩熔岩流可能影响了海洋和大气的地球化学。此外,这些含水科马岩深埋会在高温下释放水分,促进玄武岩的流体熔融,从而形成早期的闪长岩-闪长岩-花岗闪长岩(TTG)大陆地壳。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Hydration of Archean komatiites on the seafloor: Evidence from trace elements and oxygen isotopes
In the modern Earth, mantle rocks hydrated by seafloor serpentinisation play an important role in the geological (deep) water cycle. In the Archean, however, the geological water cycle may have been different. Ultramafic rocks were present as komatiites, high-MgO plume derived lavas which erupted onto oceanic plateaux or the margins of continents. Previous work has shown that these komatiites dominantly erupted in submarine environments and contain significant amounts of water bound in antigorite, chlorite and tremolite (∼6 wt%). We present in situ trace element and oxygen isotopic data of hydrated komatiites from the Kaapvaal, Superior, Singhbhum, Yilgarn and Pilbara Cratons, which further constrain thermal conditions and element uptake during seafloor hydration. Silicate phases are enriched in fluid mobile elements such as B, W, As, Sb and Pb, compared to likely komatiitic melt compositions. These fluid mobile elements were derived from seawater, or possibly seawater-sediment equilibrated fluids. The δ18O composition of olivine is mantle-like (∼5.5 ‰), and the δ18O compositions of antigorite are homogenous within sample, with most falling in a range between +1.5–4.1 ‰. Oxygen isotope modelling of serpentine in equilibrium with Archean seawater with a δ18O composition of −1 ‰ suggests that these samples were hydrated at temperatures of ∼150–210 °C, after komatiite crystallisation. The pervasive hydration of komatiite lavas was likely due to their high surface area, as they erupted as extensive but thin flows. Temperature-driven fluid circulation in the komatiites may have been promoted by the cooling of underlying and overlying lava flows, magmatic injections or proximity to the mantle plume. Despite their relatively low abundance in the geological record, komatiite lava flows in the Archean may have impacted the geochemistry of the oceans and atmosphere. Additionally, deep burial of these hydrated komatiites would release water at high temperatures, promoting the fluid-fluxed melting of basalts and in turn contributing to the formation of the early tonalite-trondhjemite-granodiorite (TTG) continental crust.
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来源期刊
Lithos
Lithos 地学-地球化学与地球物理
CiteScore
6.80
自引率
11.40%
发文量
286
审稿时长
3.5 months
期刊介绍: Lithos publishes original research papers on the petrology, geochemistry and petrogenesis of igneous and metamorphic rocks. Papers on mineralogy/mineral physics related to petrology and petrogenetic problems are also welcomed.
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