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首页> 外文期刊>Chemical geology >Geochemical temporal evolution of Brava Island magmatism: Constraints on the variability of Cape Verde mantle sources and on carbonatite-silicate magma link
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Geochemical temporal evolution of Brava Island magmatism: Constraints on the variability of Cape Verde mantle sources and on carbonatite-silicate magma link

机译:布拉瓦岛岩浆作用的地球化学时间演化:佛得角地幔源变化和碳酸盐岩-硅酸盐岩浆链接的制约

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摘要

Elemental and isotopic (Sr, Nd and Pb) analyses of silicate and carbonatite rocks from Brava, the southernmost island of the Cape Verde archipelago, are reported here to assess the nature, origin and location of the main contributors to magma composition and to evaluate the chemical evolution of magma through time. In contrast to other islands of the archipelago where a continuous range is usually observed, Brava is clearly characterized by two groups of distinct isotopic compositions. Rocks from the Upper Unit (<. 0.5. Ma) are less Nd- and Pb-radiogenic and more Sr-radiogenic than rocks belonging to the Basal Complex (~. 3 to 1.4. Ma), which are also characterized by more unradiogenic He signatures. Here, the chemistry of the Basal Complex is mainly explained by the mixing of a high-μ (HIMU)-type local end-member, which represents an ancient (~. 1.3. Ga) recycled oceanic crust, with the lower mantle. For the Upper Unit, elemental and isotopic signatures suggest the involvement of an additional local end-member akin to the EM1-type. Such differences in the contributing end-members to the Upper Unit and Basal Complex sources mirror those usually assigned to the southern and northern Cape Verde islands, respectively. This temporal evolution is discussed in light of plume interaction with a shallow EM1-type domain, which is considered to represent the subcontinental lithosphere floating in the asthenosphere. Brava carbonatites define two distinct groups with similar isotopic ranges as those observed for the coeval alkaline silicate rocks. This observation suggests that, in each of the volcano-stratigraphic units, carbonatite and silicate magmas are ultimately derived from the same sources. We propose that calciocarbonatites from either the Basal Complex or the Upper Unit resulted from nephelinite-carbonatite liquid immiscibility, while the subordinate Basal Complex magnesiocarbonatites represent residual liquids after calcite fractionation from carbonatite magma.
机译:此处报道了佛得角群岛最南端布拉瓦岛的硅酸盐和碳酸盐岩的元素和同位素(Sr,Nd和Pb)分析,以评估造成岩浆成分的主要性质,来源和位置,并评估岩浆的化学演化。与通常观察到连续范围的群岛的其他岛屿相反,布拉瓦岛的明显特征是两组不同的同位素组成。来自上层单元(<。0.5。Ma)的岩石比属于基础复合体(〜。3-1.4。Ma)的岩石具有更少的Nd和Pb放射源和更多的Sr放射源,其特征还在于非放射源的He签名。在这里,主要通过将高μ(HIMU)型局部端构件与下地幔混合,来表示基础复合物的化学作用,该高μ(HIMU)型局部端构件代表着古老的(〜。1.3。Ga)再生海洋地壳。对于上层单元,元素和同位素特征表明存在与EM1型相似的其他局部末端成员。上层部队和基层建筑群来源的最终成员之间的这种差异反映了通常分别分配给佛得角南部和北部岛屿的那些差异。根据羽流与浅层EM1型域的相互作用来讨论这种时间演化,该域被认为代表了漂浮在软流圈中的次大陆岩石圈。布拉瓦碳酸盐岩定义了两个不同的组,它们的同位素范围与同时代碱性硅酸盐岩所观察到的同位素范围相似。这一观察结果表明,在每个火山地层单元中,碳酸盐岩和硅酸盐岩浆最终都来自相同的来源。我们认为,基底复合物或上部单元中的钙碳酸盐岩是由霞石-碳酸盐岩液体不混溶性产生的,而从属基底络合物的镁碳碳酸盐岩代表了方解石从碳酸盐岩浆分离后的残余液体。

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