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首页> 外文期刊>International Geology Review >Quaternary high-Nb basalts: existence of young oceanic crust under the Sanandaj-Sirjan Zone, NW Iran
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Quaternary high-Nb basalts: existence of young oceanic crust under the Sanandaj-Sirjan Zone, NW Iran

机译:第四纪高Nb玄武岩:伊朗西北部Sanandaj-Sirjan区之下存在年轻的洋壳

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Quaternary basaltic volcanoes are distributed in the northern part of the Sanandaj-Sirjan Zone (N-SSZ). Those in the Ghorveh area of the N-SSZ are characterized by low SiO_2, high alkalis, and LILE + LREE enrichment. They also have high Mg numbers (Mg# = 65-70) and high contents of Cr (>300 ppm), Ni (> 177 ppm), and TiO_2 (> 1.5 wt.%), suggesting that they crystallized directly from primary magma. The basalts are classified as high-Nb basalts (HNB), with Nb concentrations greater than 20 ppm. Their ~(87)Sr/~(86)Sr values range from 0.7049 to 0.7053 and their ε~0_(Nd) values lie between -0.2 and 1.1. The small negative values of ε~0_(Nd) indicate involvement of continental material in the evolution of the source magma in the area. Based on these new chemical and isotopic data and their relationship to the Plio-Quaternary volcanic adakites in northern Ghorveh, we propose that the partial fusion of metasomatized mantle associated with adakitic magma was responsible for generation of the HNB rocks following late Miocene collision of the Arabian and Iranian plates. Rollback of Neotethyan oceanic spreading and mantle plume activity caused a thinning of the northern SSZ lithosphere;;furthermore, the S wave tomography model beneath the N-SSZ supports this hypothesized lithospheric thinning. The HNB rocks have close spatial proximity and temporal association with adakites, which were formed by the subduction of young (<25 Ma) oceanic crust. Our discussion clarifies the role of the oceanic slab in the post-collision generation of the HNB basalts in this area. Our data confirm the relationship of the HNB rocks to the subduction zone instead of to the oceanic island basalt (OIB) type magma in extensional zones.
机译:第四纪玄武质火山分布在Sanandaj-Sirjan区(N-SSZ)的北部。 N-SSZ的Ghorveh区域的特征是SiO_2低,碱度高和LILE + LREE富集。它们还具有高的Mg值(Mg#= 65-70)和高含量的Cr(> 300 ppm),Ni(> 177 ppm)和TiO_2(> 1.5 wt。%),表明它们直接从原生岩浆中结晶。 。玄武岩归为高Nb玄武岩(HNB),其Nb浓度大于20 ppm。它们的〜(87)Sr /〜(86)Sr值在0.7049至0.7053之间,并且其ε〜0_(Nd)值在-0.2至1.1之间。 ε〜0_(Nd)的较小负值表明大陆物质参与了该地区的源岩浆演化。基于这些新的化学和同位素数据,以及它们与古尔维北部的上新世-第四纪火山埃达克特岩的关系,我们认为,与阿拉伯格达克岩浆相关的交代地幔的部分融合是造成阿拉伯中新世晚期碰撞后HNB岩石生成的原因。和伊朗板块。新特提斯洋洋扩张和地幔柱活动的回滚导致北部SSZ岩石圈变薄;此外,N-SSZ下方的S波层析成像模型支持这种假设的岩石圈变薄。 HNB岩石具有接近的空间接近性,并且与Adakite具有时间相关性,后者是由年轻(<25 Ma)洋壳俯冲形成的。我们的讨论阐明了海洋平板在该区域HNB玄武岩碰撞后生成中的作用。我们的数据证实了HNB岩石与俯冲带的关系,而不是与伸展带中的海洋岛玄武岩(OIB)型岩浆的关系。

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