次大陆岩石圈地幔熔化和再肥化的热力学模型和年代测定法

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Yujian Wang, Jingao Liu
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引用次数: 0

摘要

从地球化学角度区分熔体耗竭和再充填的产物,并确定次大陆岩石圈(SCLM)中这种地幔-熔体相互作用的时间,仍然是悬而未决的研究课题。在这里,我们利用 alphaMELTS 对部分熔融和再肥化的热力学建模,重新审视了比利牛斯造山地幔丘陵的勒尔兹地幔岩的起源。热力学建模揭示了再富集(即整块岩石和clinopyroxenes中的TiO2/Al2O3和HREE含量升高)和部分熔融过程之间微妙而关键的差异。来自勒尔茨山丘的哈兹博格岩主要由部分熔融的原始残留物和熔体/岩石比率较低的次级再肥化产物组成。与橄榄石菱锰矿层在空间上有密切联系的勒尔兹沸石是次生岩石,由原始的难熔哈兹堡垒岩和上涌的 N-MORB 类熔体再充填而成。与橄榄石网状岩没有密切空间联系的海尔兹堡岩有可能是另一种起源,即通过岩石圈底部的静止冷却,在天体层地幔适度绝热上涌之后形成的。难熔哈兹堡垒岩的再损耗模型年龄(TRD)得出的系统峰值熔融年龄为 2.0 Ga。我们开发了一种新的解决方案,通过评估Re-Os和Lu-Hf同位素系统的行为,采用一种经过调整的渗滤模型来制约相对较早的再增殖年龄(∼ 1.5 - 2.0 Ga)。该研究结合全球弧上和弧下SCLM的综合数据集,成功地区分了硅酸盐熔融诱导的再热化和元素层面的部分熔融,证明了不同熔融机制对历史上SCLM成分演化的独特贡献,并强调了再热化对地球化学浮力和力学稳健性的变化,以及最终对古SCLM的稳定性和寿命所起的深远作用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Thermodynamic modelling and chronometric dating of melting and refertilization in the subcontinental lithospheric mantle

Geochemically distinguishing the products of melt depletion from refertilization and constraining the timing of such mantle-melt interactions in the subcontinental lithosphere (SCLM) remain outstanding research issues. Here we utilize alphaMELTS thermodynamic modeling of both partial melting and refertilization to revisit the origins of the Lherz mantle rocks from the Pyrenean orogenic mantle massifs. Thermodynamic modeling reveals subtle but critical differences between refertilization (i.e., elevated TiO2/Al2O3 and higher HREE in both whole rocks and clinopyroxenes) and partial melting processes. Harzburgites from the Lherz massif comprise predominantly pristine residues of partial melting and subordinately refertilized products with low melt/rock ratios. The Lherz lherzolites that show close spatial associations with olivine websterite layers represent secondary rocks, derived from refertilization involving the pristine, refractory harzburgites and upwelling N-MORB-like melts. Lherzolites with no intimate spatial association to olivine websterites are open to an additional origin, i.e., via stationary cooling at the base of lithosphere after moderate adiabatic upwelling of asthenospheric mantle. The Re-depletion model ages (TRD) of refractory harzburgites yield a systematic peak melting age of 2.0 Ga. We have developed a novel solution for constraining the relatively ancient age of refertilization (∼ 1.5 – 2.0 Ga) through the approach of an adapted percolation model to assess the behavior of Re-Os and Lu-Hf isotopic systems. Together with a comprehensive dataset of global on- and off-cratonic SCLM, this study has successfully distinguished silicate-melt induced refertilization from partial melting on elemental level, demonstrated the contribution of different melting mechanisms to the distinctive SCLM compositional evolution in the history, and highlighted how profound a role that refertilization has played on the variations of geochemical buoyancy and mechanical robustness and eventually on the stability and longevity of the ancient SCLM.

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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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