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Unexpected HIMU-type late-stage volcanism on the Walvis Ridge

机译:沃尔维斯山脊上意外的HIMU型后期火山

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Volcanic activity at many oceanic volcanoes, ridges and plateaus often reawakens after hiatuses of up to several million years. Compared to the earlier magmatic phases, this late-stage (rejuvenated/posterosional) volcanism is commonly characterized by a distinct geochemical composition. Late-stage volcanism raises two hitherto unanswered questions: Why does volcanism restart after an extended hiatus and what is the origin of this volcanism? Here we present the first Ar-40/Ar-39 age and comprehensive trace element and Sr-Nd-Pb-Hf isotopic data from seamounts located on and adjacent to the Walvis Ridge in the South Atlantic ocean basin. The Walvis Ridge is the oldest submarine part of the Tristan-Gough hotspot track and is famous as the original type locality for the enriched mantle one (EM I) end member. Consistent with the bathymetric data, the age data indicates that most of these seamounts are 20-40 Myr younger than the underlying or nearby Walvis Ridge basement. The trace element and isotope data reveal a distinct compositional range from the EM 1-type basement. The composition of the seamounts extend from the St. Helena HIMU (high time-integrated U-238/(204)pb mantle with radiogenic Pb isotope ratios) end member to an enriched (E) Mid-Ocean-Ridge Basalt (MORB) type composition, reflecting a two-component mixing trend on all isotope diagrams. The EMORB end member could have been generated through mixing of Walvis Ridge EM 1 with normal (N) MORB source mantle, reflecting interaction of Tristan-Gough (EM l-type) plume melts with the upper mantle. The long volcanic quiescence and the HIMU-like geochemical signature of the seamounts are unusual for classical hotspot related late-stage volcanism, indicating that these seamounts are not related to the Tristan-Gough hotspot volcanism. Two volcanic arrays in southwestern Africa (Gibeon-Dicker Willem and Western Cape province) display similar ages to the late-stage Walvis seamounts and also have HIMU-like compositions, su
机译:许多海洋火山,山脊和高原的火山活动经常在高达数百万年后重新制造。与早期的岩浆阶段相比,这种晚期(恢复活力/后退)的火山常见于不同的地球化学组合物。阶段的火山主义提出了两个迄今为止未解决的问题:为什么火山主义在延长的中断后重新启动,这座火山的起源是什么?在这里,我们介绍了位于南大西洋盆地的Walvis山脊上的海山的第一个AR-40 / AR-39年龄和综合微量元素和SR-ND-PB-HF同位素数据。 Walvis Ridge是Tristan-Gough热点轨道的最古老的潜艇部分,并且作为富集的地幔(EM I)最终成员的原始型位置而闻名。与碱基数据一致,年龄数据表明,这些海山的大多数比底层或附近的Walvis Ridge地下室更年轻20-40 Myr。痕量元素和同位素数据显示来自EM 1型地下室的不同的组成范围。海山的组成从St. Helena Himu(高时间 - 集成的U-238 /(204)Pb幔含有辐射性Pb同位素比)末端成员到富集(E)中海脊玄武岩(Morb)类型构成,反映了所有同位素图的双组分混合趋势。可以通过使用正常(n)Morb源幔的Walvis脊Em1混合来产生透光端构件,反射三氮(EM L型)羽状熔体的相互作用。海山的长火山静态和HIMU样地球化学签名对于经典热点相关的晚期火山是不寻常的,这表明这些海山与Tristan-Gough热点Volcanism无关。两座非洲(Gibeon-Dicker Willem和西开普省)的两座火山阵列展示了类似年龄的沃尔维斯海山,也有纯粹的组合物,苏

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