MORBs 的 142Nd 和 182W 对比研究以及上地幔的 4.5 Gyr 演变

IF 3.4 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
D. Peters, H. Rizo, J. O’Neil, C. Hamelin, S.B. Shirey
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引用次数: 0

摘要

在太平洋-南极海脊的同一玄武岩样本上获得了新的高精度钕和钨同位素组成。这些数据提供了迄今为止对被称为 DMM 的洋中脊玄武岩贫化地幔源的μ142Nd 和 μ182W 值的最佳估计。PAR 玄武岩的平均 μ142Nd = -1.6 ± 5.0 (2 个标准差)和 μ182W = -1.9 ± 3.5 (2 个标准差),这些数据与文献数据一起,可以对 DMM 的同位素组成进行约束。现今DMM的μ182W比Archean地幔的μ182W低10-20 ppm。这种降低可能与24亿至30亿年前开始的深冷板块俯冲及其随之而来的地幔回流造成的地幔羽流物质广泛进入上地幔有关。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Comparative 142Nd and 182W study of MORBs and the 4.5 Gyr evolution of the upper mantle

Comparative 142Nd and 182W study of MORBs and the 4.5 Gyr evolution of the upper mantle
New high precision Nd and W isotopic compositions were obtained on the same basalt samples from the Pacific-Antarctic Ridge. These provide the best estimate so far for the μ142Nd and μ182W values of the depleted mantle source of mid-ocean ridge basalts known as DMM. The PAR basalts yield a mean μ142Nd = −1.6 ± 5.0 (2 s.d.) and μ182W = −1.9 ± 3.5 (2 s.d.), which together with the literature data allow the isotope composition of the DMM to be constrained. The present-day DMM μ182W is 10–20 ppm lower than that of the Archean mantle. This decrease could be related to the broad incorporation of mantle plume material into the upper mantle, starting between 2.4 and 3 billion years ago, due to the onset of deep cold slab subduction, and its attendant return mantle flow.
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来源期刊
Geochemical Perspectives Letters
Geochemical Perspectives Letters Earth and Planetary Sciences-Geochemistry and Petrology
CiteScore
7.00
自引率
2.00%
发文量
42
审稿时长
15 weeks
期刊介绍: Geochemical Perspectives Letters is an open access, internationally peer-reviewed journal of the European Association of Geochemistry (EAG) that publishes short, highest-quality articles spanning geochemical sciences. The journal aims at rapid publication of the most novel research in geochemistry with a focus on outstanding quality, international importance, originality, and stimulating new developments across the vast array of geochemical disciplines.
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