南非3.48 Ga Barberton科马地岩套的火山构造、岩石学和地球动力学背景

IF 1.2 4区 地球科学 Q2 GEOLOGY
E. Grosch, J. Sláma
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引用次数: 2

摘要

本文结合地球化学资料,对南非巴伯顿绿岩带约3.48 Ga科马提组中下类型剖面的一系列科马提岩-拉斑岩火山岩进行了新的野外和岩石学观察。在1.44公里的剖面上发现了一系列基性-超基性岩石,从而提出了中下科马提组类型剖面的新的初步火山结构。主要元素、痕量元素和稀土元素(REE)数据结合Lu-Hf同位素约束表明,火山层序中的拉斑岩、新发现的高镁玄武岩、玄武质科马岩和科马岩具有原始地幔特征,与太古宙或现代超俯冲带的博长岩没有地球化学亲缘关系。科马提型剖面最下部的尖砾岩和块状科马提岩流动的全岩初始εHf值为负值,范围在-1.9 ~ -3.1之间,而上覆的第二个尖砾岩和块状科马提岩单元的初始εHf值为正,范围在+0.5 ~ +4.7之间。针对巴伯顿中下科马提组类型剖面,提出了一种涉及幔柱-壳相互作用的基性-超基性熔岩地壳污染的新地球动力学模型。新的观测和资料表明,科马岩浆岩的喷发是由于中太古代热地幔(> - 1 600℃)的地幔柱,其中最早的火山流在上升和喷发过程中受到地壳污染的不同影响。不能排除地幔源区存在下地壳物质和/或再循环地壳的可能性。这表明现代板块构造作用,如俯冲作用,可能不是3.48 Ga Barberton komatiite套件形成的必要条件,这对太古宙地幔的水化状态、地球动力学过程和长期热演化具有重要意义。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
On the volcanic architecture, petrology and geodynamic setting of the 3.48 Ga Barberton komatiite suite, South Africa
This study presents new field and petrological observations combined with geochemical data on a range of komatiitic to tholeiitic volcanic rocks from the ca. 3.48 Ga mid-lower Komati Formation type-section of the Barberton Greenstone Belt, South Africa. A range of mafic-ultramafic rocks is identified across a 1.44 km profile, leading to the proposition of a new preliminary volcanic architecture for the mid-lower Komati Formation type-section. Major, trace and rare earth element (REE) data in conjunction with Lu-Hf isotopic constraints indicate that the tholeiites, newly recognized high-magnesium basalts, basaltic komatiites and komatiites in the volcanic sequence have a primitive mantle signature with no geochemical affinity to Archaean or modern-day supra-subduction zone boninites. The whole rock initial εHf values of spinifex and massive komatiite flows in the lowermost part of the Komati type-section are negative, ranging between -1.9 and -3.1, whereas the second overlying spinifex and massive flow unit records positive initial εHf values between +0.5 and +4.7. A new geodynamic model involving crustal contamination of the mafic-ultramafic lavas is proposed for the Barberton mid-lower Komati Formation type-section, involving mantle plume-crust interaction. The new observations and data indicate that the komatiites erupted as a result of a mantle plume from a hot (>1 600oC) mid-Archaean mantle, in which the earliest volcanic flows were variably affected by crustal contamination during their ascent and eruption. The possibility of incorporation of lower crustal material and/or recycled crust residing in the mantle source region cannot be excluded. This indicates that modern-style plate tectonic processes, such as subduction, may not have been a requirement for the formation of the 3.48 Ga Barberton komatiite suite, with implications for the hydration state, geodynamic processes and secular thermal evolution of the Archaean mantle.
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来源期刊
CiteScore
3.60
自引率
5.60%
发文量
18
审稿时长
>12 weeks
期刊介绍: The South African Journal of Geology publishes scientific papers, notes, stratigraphic descriptions and discussions in the broadly defined fields of geoscience that are related directly or indirectly to the geology of Africa. Contributions relevant to former supercontinental entities such as Gondwana and Rodinia are also welcome as are topical studies on any geoscience-related discipline. Review papers are welcome as long as they represent original, new syntheses. Special issues are also encouraged but terms for these must be negotiated with the Editors.
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