T. McIntyre, P. Waterton, L. Li, B. Gong, X. Zha, K. Szilas, D. G. Pearson
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The Ussuit peridotite was emplaced in the crust during the Nagssugtoqidian orogeny between 1,870 Ma and 1,775 Ma and preserves primary melt depleted characteristics that reflect >30% melting, for example, Al<sub>2</sub>O<sub>3</sub> < 0.4 wt.%, Ti < 10 ppm, Lu/Yb > 0.25, and Mg #s up to 93. Cryptic signatures of hydrous melting, for example, spinel Cr #’s >65, Os/Ir ratios between 0.3 and 6, and supramantle olivine δ<sup>18</sup>O values, suggest that the high degree of melt depletion was partly inherited from a forearc or sub-arc melting environment. Re-Os isotopic systematics show melt depletion occurred at ∼2 Ga overlapping the juvenile oceanic arc crust that hosts the peridotites. This age coincides with a peak in the global production of juvenile cratonic lithosphere. Furthermore, the global Paleoproterozoic cratonic mantle has strong geochemical similarities with the Ussuit peridotites. 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引用次数: 0
摘要
太古宙克拉通核下的地幔残余物已被广泛研究,而连接这些核的元古代活动带下的地幔岩石圈研究较少。古元古代活动带构造模数内的稀有地幔构造岩为理解克拉通地幔岩石圈的构造过程提供了重要的信息。本文介绍了西格陵兰岛古元古代地幔构造岩-乌苏塞橄榄岩的矿物组成、大块岩石主元素、微量元素和铂族元素、Re-Os同位素和橄榄石氧同位素。乌苏特橄榄岩是在1870 ~ 1775 Ma的那苏木—祁甸造山运动时期侵位在地壳中的,保留了反映30%熔融的初级熔体衰竭特征,如Al2O3 <;0.4 wt.%, Ti <;10 ppm, Lu/Yb >;0.25, Mg #s可达93。尖晶石Cr # s >;65、Os/Ir比值在0.3 ~ 6之间、上地幔橄榄石δ18O值等水熔特征表明,高熔体损耗部分继承自弧前或弧次熔融环境。Re-Os同位素系统显示熔体耗损发生在~ 2ga,与孕育橄榄岩的幼年洋弧地壳重叠。这个时代与全球幼年克拉通岩石圈的生产高峰相吻合。此外,全球古元古代克拉通地幔与乌苏特橄榄岩具有很强的地球化学相似性。俯冲带橄榄岩是古元古代克拉通岩石圈地幔的重要组成部分,形成了一个粘性、浮力强的地幔岩石圈,有助于大克拉通块体的长期稳定。
A Rare Glimpse of Paleoproterozoic Sub-Arc Mantle: The Ussuit Peridotite, West Greenland
Mantle residues beneath Archean cratonic nuclei have been extensively studied, whereas less attention has been given to the mantle lithosphere beneath Proterozoic mobile belts that link these nuclei. Rare mantle tectonites within tectonic mélanges of Paleoproterozoic mobile belts provide information important to understanding the broader processes involved in the construction of the cratonic mantle lithosphere. Here we present mineral compositions, bulk-rock major, trace, and platinum group elements, Re-Os isotopes, and olivine oxygen isotopes from a Paleoproterozoic mantle tectonite in West Greenland–the Ussuit peridotite. The Ussuit peridotite was emplaced in the crust during the Nagssugtoqidian orogeny between 1,870 Ma and 1,775 Ma and preserves primary melt depleted characteristics that reflect >30% melting, for example, Al2O3 < 0.4 wt.%, Ti < 10 ppm, Lu/Yb > 0.25, and Mg #s up to 93. Cryptic signatures of hydrous melting, for example, spinel Cr #’s >65, Os/Ir ratios between 0.3 and 6, and supramantle olivine δ18O values, suggest that the high degree of melt depletion was partly inherited from a forearc or sub-arc melting environment. Re-Os isotopic systematics show melt depletion occurred at ∼2 Ga overlapping the juvenile oceanic arc crust that hosts the peridotites. This age coincides with a peak in the global production of juvenile cratonic lithosphere. Furthermore, the global Paleoproterozoic cratonic mantle has strong geochemical similarities with the Ussuit peridotites. It is suggested that subduction zone peridotites form key components of the Paleoproterozoic cratonic lithospheric mantle, creating a viscous, buoyant mantle lithosphere that contributed to the long-term stability of the greater cratonic masses.
期刊介绍:
Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged.
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The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution
Principles and applications of geochemical proxies to studies of Earth history
The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them
The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales
Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets
The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets
Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.