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The origin of decoupled Hf-Nd isotope compositions in Eoarchean rocks from southern West Greenland

机译:西格陵兰南部欧陶统岩石中Hf-Nd同位素解耦的成因

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摘要

Radiogenic isotope compositions of Hf and Nd are typically coupled in Phanerozoic and Proterozoic mafic rocks due to a similar behaviour of Lu-Hf and Sm-Nd during mantle melting. Eoarchean rocks, for instance those from southern West Greenland, exhibit an apparent decoupling of Hf and Nd isotope compositions. This apparent decoupling may either indicate metamorphic disturbance or, alternatively, mirror early differentiation processes in the silicate Earth. To evaluate the issue, we performed combined measurements of Hf-Nd isotope compositions together with major and trace element concentrations for well preserved >3720 to >3800. Ma old tholeiitic metabasalts and gabbros from the ~3700. Ma and ~3800. Ma old terranes of the Isua Supracrustal Belt, southern West Greenland. In contrast to younger mafic rocks, calculated initial εHf-εNd values of the Isua tholeiites show similar spreads and are both near chondritic to strongly depleted (-0.7 to +6.3 and -0.8 to +4.4, respectively), also in contrast to previously reported more depleted signatures in nearby boninite-like metabasalts of the Garbenschiefer unit. An evaluation of alteration effects based on preserved major and trace element arrays reveals pristine magmatic trends and therefore the measured isotope compositions indeed in most cases characterize contrasting Eoarchean mantle sources. In accord with this view, compositions of the Isua metabasalts yield Eoarchean regression ages in Sm-Nd and Lu-Hf isochron spaces, overlapping with emplacement ages inferred from crosscutting relationships with tonalites. Lutetium-Hf systematics of the Isua metabasalts studied here, yield clear isochron relationships. For both terranes, there is some scatter in Sm-Nd space, indicating early disturbance of the Sm-Nd system close in time to the extrusion ages, possibly by seafloor alteration. Trace element compositions of the metabasalts indicate an arc setting and a strong source overprint by melt-like subduction components. It is likely, that the source overprint may have caused partial decoupling of the εHf-εNd values, due to selective addition of Nd as observed in modern subduction settings. In this case, the most radiogenic initial εNd and εHf isotope values characterize the most depleted mantle sources, and less radiogenic values would reflect increased contributions of isotopically more enriched subduction components. However, the most depleted samples still exhibit decoupled Hf-Nd compositions, making a case for the presence of even older mantle heterogeneities. A proposed superchondritic composition of the silicate Earth (SCHEM), however, cannot account for the most depleted sample compositions. Conversely, a depleted upper mantle formed by crystallization of perovskite-rich cumulates in the early Hadean may well explain these observed compositions. A literature survey reveals an overlap in initial Hf-Nd compositions between southern West Greenland TTGs and the metabasalts analyzed here. This overlap suggests a genetic relationship between these lithologies, where the TTGs may have inherited their unusual Hf-Nd compositions from mafic precursors isotopically similar in composition to the Isua tholeiites.
机译:Hf和Nd的放射性同位素组成通常在古生代和元古代镁铁质岩石中耦合,这是由于在地幔融化过程中Lu-Hf和Sm-Nd具有相似的行为。欧archean岩石,例如来自西格陵兰南部的岩石,表现出Hf和Nd同位素组成的明显脱钩。这种明显的解耦可能表明变质扰动,或者反映了硅酸盐地球的早期分化过程。为了评估该问题,我们对Hf-Nd同位素组成以及主要和痕量元素浓度进行了组合测量,以保存良好的> 3720至> 3800。距今约3700年的Ma老的变质玄武岩和辉长岩。马和〜3800。西格陵兰南部伊苏阿(Isua)地壳带的Ma老地。与年轻的镁铁质岩石相反,Isua辉绿岩的初始εHf-εNd初始值显示出相似的展布,并且均接近于软骨状至强烈耗尽(分别为-0.7至+6.3和-0.8至+4.4), Garbenschiefer单元附近的类似邦尼石的玄武岩中有更多的枯竭签名。基于保留的主要元素和微量元素阵列对蚀变作用的评估揭示了原始岩浆趋势,因此,在大多数情况下,所测量的同位素组成确实的确表征了对比欧陶统地幔源。按照这种观点,伊苏亚变玄武岩的成分在Sm-Nd和Lu-Hf等时空间产生了Eoarchean回归年龄,与从与同辉石的横切关系推断出的年代年龄重叠。此处研究的Isua偏玄武岩的ute-Hf系统学,产生清晰的等时线关系。对于这两种地貌,Sm-Nd空间都有一定的散射,这表明Sm-Nd系统的早期扰动可能在接近挤压年龄的时候就可能是由于海底的变化。偏玄武岩的痕量元素组成显示出电弧凝结和类似熔体俯冲成分的强烈源叠印。如在现代俯冲环境中观察到的那样,由于有选择地添加了Nd,源套印很可能导致εHf-εNd值部分解耦。在这种情况下,最放射源的初始εNd和εHf同位素值表征了最贫乏的地幔源,而较少的放射源值将反映同位素更富集的俯冲成分的增加贡献。但是,最贫乏的样品仍表现出解耦的Hf-Nd成分,这说明甚至存在更古老的地幔非均质性。但是,建议的硅酸盐地球(SCHEM)的超软骨质成分不能解释最消耗的样品成分。相反,在哈代早期,富含钙钛矿的堆积物结晶形成的贫化上地幔可能很好地解释了这些观察到的成分。文献调查显示,南部格陵兰岛TTG与此处分析的偏玄武岩之间的初始Hf-Nd成分重叠。这种重叠暗示了这些岩性之间的遗传关系,其中TTG可能已经从同位素组成类似于Isua硫铁矿的镁铁质前体继承了它们不寻常的Hf-Nd组成。

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