东南亚晚新生代海南类obb玄武岩记录了深地幔柱与滞流板块的相互作用

IF 5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Ming Lei , Katsuhiko Suzuki , Minako Kurisu , Teruhiko Kashiwabara , Jifeng Xu , Zhengfu Guo , Jie Li , Jianlin Chen
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引用次数: 0

摘要

东南亚晚新生代玄武岩是否记录了地幔过渡带(MTZ)内的柱-板相互作用仍未定论。为此,我们报道了海南玄武岩中橄榄石He同位素、全岩主微量元素组成和Sr-Nd-Hf-Fe-Mo同位素比值的新数据。海南玄武岩MgO含量高,SiO2含量低,具有洋岛玄武岩的微量元素特征,如轻稀土元素和高场强元素富集。同时,这些玄武岩具有贫Sr-Nd-Hf同位素组成特征(87Sr/86Sr = 0.7031-0.7043,εNd = +3.3 ~ +5.5,εHf = +6.8 ~ +10.3),形成类似洋中脊玄武岩(MORBs)的3He/4He比值(7.0 ~ 9.2 Ra)。海南玄武岩地球化学特征说明其地幔源包括贫和富两种成分。与源自上地幔橄榄岩的morb相比,海南玄武岩的分馏校正δ56Fe值(+0.07 ‰~ +0.17 ‰)较高,δ98Mo值(- 0.38 ‰~ - 0.07 ‰)变化较大,表明其源岩性为环境橄榄岩与含碳酸盐的再循环洋壳相互作用形成的辉石岩。综合地球物理约束,我们将海南玄武岩地幔源的亏缺和富缺特征分别归结为来自MTZ的橄榄岩FOZO羽流和来自MTZ的含太平洋碳酸盐岩洋壳。晚新生代,来自深部地幔的上升地幔柱到达MTZ,与停滞的太平洋板块反应形成辉石岩。由于MTZ厚度的变化和停滞板块的存在,深部地幔柱发生了分叉,导致了次级地幔柱的形成。来自MTZ的次级地幔柱上涌将新形成的地幔辉石岩输送到上地幔,在上地幔中辉石岩经过部分熔融形成海南玄武岩和东南亚其他玄武岩。因此,我们的深地幔柱与中山带内滞流板块相互作用的模型可以用来解释该地区晚新生代玄武岩的形成。我们进一步提出,玄武岩(如海南玄武岩)中类似morb的3He/4He值不能简单地作为一个强有力的指标来否定它们可能来自深部地幔柱的可能性。此外,玄武岩放射性成因(Sr-Nd-Hf)和稳定同位素(Fe-Mo)数据的整合是揭示玄武岩地幔源中辉石岩存在并揭示其成因的有力方法。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Late Cenozoic Hainan OIB-like basalts in SE Asia record the interaction between a deep mantle plume and stagnant slab
Whether Late Cenozoic basalts in SE Asia record plume-slab interactions within the mantle transition zone (MTZ) remains unresolved. To investigate this, we report new data on He isotopes measured in olivine, together with whole-rock major and trace element compositions and Sr–Nd–Hf–Fe–Mo isotope ratios for the Hainan basalts. The Hainan basalts have high MgO and low SiO2 contents and display trace-element signatures of ocean island basalts (OIBs), such as the enrichments in light rare earth elements and high-field-strength elements. Meanwhile, these basalts are characterized by the depleted Sr–Nd–Hf isotopic compositions (87Sr/86Sr = 0.7031–0.7043; εNd = +3.3 to +5.5; εHf = +6.8 to +10.3) and yield mid-ocean ridge basalts (MORBs)-like 3He/4He ratios (7.0–9.2 Ra). The geochemical characteristics of Hainan basalts illuminate that their mantle source includes depleted and enriched components. Compared with MORBs derived from upper mantle peridotite, the Hainan basalts have higher fractionation-corrected δ56Fe values (+0.07 ‰ to +0.17 ‰) and variable δ98Mo values (−0.38 ‰ to −0.07 ‰), indicating their source lithology was a pyroxenite formed by the interaction between ambient peridotite and recycled carbonate-bearing oceanic crust. Integrating geophysical constraints, we attribute the depleted and enriched signatures in the mantle source of Hainan basalts to a peridotitic FOZO plume and Pacific carbonate-bearing oceanic crust entrained from the MTZ, respectively. During the Late Cenozoic, an ascending mantle plume from the deep mantle reached the MTZ and reacted with the stagnant Pacific oceanic slab to form pyroxenite. Given the variable thickness and presence of a stagnant slab in the MTZ, the deep mantle plume bifurcated, leading to the formation of secondary mantle plumes. The upwelling secondary mantle plumes from the MTZ transported newly formed mantle pyroxenite into the upper mantle, where pyroxenite underwent partial melting to form the Hainan basalts and other basaltic rocks in SE Asia. Therefore, our model of the interplay between a deep mantle plume and a stagnant slab within the MTZ might be applied to explain the formation of Late Cenozoic basalts in this region. We further propose that MORB-like 3He/4He values in basaltic rocks (e.g., Hainan basalts) cannot be simply used as a robust indicator to negate the possibility that they may be sourced from a deep mantle plume. Moreover, the integration of radiogenic (Sr–Nd–Hf) and stable (Fe–Mo) isotope data for basaltic rocks is a robust method to reveal the presence of pyroxenite in the mantle source of basalts and shed light on its genesis.
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来源期刊
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta 地学-地球化学与地球物理
CiteScore
9.60
自引率
14.00%
发文量
437
审稿时长
6 months
期刊介绍: Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes: 1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids 2). Igneous and metamorphic petrology 3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth 4). Organic geochemistry 5). Isotope geochemistry 6). Meteoritics and meteorite impacts 7). Lunar science; and 8). Planetary geochemistry.
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