2.7 Ga时,强烈的裂谷岩浆活动导致伊尔甘克拉通地壳迅速增厚

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Alan R.A. Aitken, Q. Masurel, N. Thébaud, Lu Li, Abdul Azim bin Rossalim
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引用次数: 0

摘要

许多太古宙克拉通的地壳结构符合相对薄壳的范例(<;35公里),具有长英质成分,低速下地壳和尖锐的莫霍不连续。这与元古代地区的地壳形成鲜明对比,后者的典型特征是地壳较厚(>;40公里),通常具有高速下地壳和弥散莫霍。有人提出了地壳性质的全球性转变,但其时间和性质尚不清楚。西澳大利亚的伊尔甘克拉通的地壳厚度从~ 30 km到>;45公里,并可能保留这种转变的一个关键例子。本研究采用地震约束重力反演技术详细解析了伊尔甘克拉通的地壳厚度和密度。确定了地壳较厚致密的区域,并探讨了其发展的两种情景:情景1为地壳缩短、侵蚀和含石榴石下地壳的发育,情景2为伸展过程中添加基性岩浆岩。情景2更符合克拉通的新太古代地质和推断出的2.73 ~ 2.65 Ga之间的幼年岩浆活动程度。约2.73 Ga的区域地层不整合被认为是克拉通演化的转折点,标志着地球动力稳定下地壳的热流变阈值的跨越。我们认为净地壳增厚发生在接下来的~ 40 Ma,其中基性岩浆输入总量为5.0 Mkm3,由中等扩展(β-因子~ 1.1)平衡。蒙特卡罗模拟使用持续时间为40 Ma,体积为10 Mkm3的一系列时空分布事件,成功地解释了模拟的全球平均地壳厚度随时间的变化。这里发现的事件与构造倾向的峰值一致,支持新太古代全球下地壳的历时性和幕式生长。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Intense rift magmatism caused rapid thickening of Yilgarn Craton crust at 2.7 Ga
The crustal structure of many Archean cratons fits a paradigm of relatively thin crust (< 35 km), with felsic compositions, low-velocity lower crust and a sharp Moho discontinuity. This contrasts with the crusts of Proterozoic regions, which are typified by thicker crust (> 40 km), often with a high-velocity lower crust and a diffuse Moho. A global-scale transition in the nature of the crust is suggested, but its timing and nature remain unclear. The Yilgarn Craton in Western Australia has crustal thickness from ∼ 30 km to > 45 km and may preserve a key example of this transition. This study employs seismic-constrained gravity inversion to resolve in detail the thickness and density of the Yilgarn Craton crust. Regions with thick and dense crust are identified, and we explore two scenarios for their development: scenario 1 involves crustal shortening, erosion, and the development of a garnet-bearing lower crust, and scenario 2 involves addition of mafic magmatic rocks during extension. Scenario 2 is more consistent with the Neoarchean geology of the craton and the inferred extents of juvenile magmatism between 2.73 to 2.65 Ga. A regional stratigraphic unconformity at ca. 2.73 Ga is recognised as a turning point in the evolution of the craton, marking the crossing of thermo-rheological thresholds for geodynamically-stable lower crust. We suggest that net crustal thickening occurred over the next ∼40 Ma with a mafic magmatic input totalling 5.0 Mkm3 balanced by moderate extension (β-factor ∼ 1.1) Monte-Carlo simulations use a time-and-space distributed series of events of <40 Ma duration and <10 MKm3 vol to successfully explain modelled variations in global average crustal thickness through time. The event identified here aligns with a peak in constructive tendency, supporting the diachronous and episodic growth of the global lower crust during the Neoarchean.
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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.
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