首页> 外文会议>Conference on Composition, Deep Structure and Evolution of Continents Harvard University,Cambridge,Mass.,15-17 October 1997 >Evidence for Archean ocean crust with low high field strength element signature from diamondiferous eclogite xenoliths
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Evidence for Archean ocean crust with low high field strength element signature from diamondiferous eclogite xenoliths

机译:含刚玉榴辉岩异岩的高场强元素特征低的太古代海洋地壳的证据

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late Archean (2.57 Ga) diamond-bearing eclogite xenoliths from Udachnaya, Siberia, exhibit geochemical characteristics including variation in oxygen isotope values, and correlations of delta ~(18)O with major elements and radiogenic isotopes which can be explained by an origin as subducted oceanic crust. Trace element analyses of constituent garnet and clinopyroxene by Laser-ICPMS are used to reconstruct whole-rock trace element compositions, which indicate that the eclogites have very low high field strength element (HFSE) concentrations and Zr/Hf and Nb/Ta ratios most similar to modern island arcs or ultradepleted mantle. Although hydrothermal alteration on the Archean sea floor had enough geochemical effect to allow the recognition of its effects in the eclogites and thus diagnose them as former oceanic crust, it was not severe enough to erase many other geochemical features ofthe original igneous rocks, particularly the relatively immobile HFSEs. Correlations of the trace element patterns with oxygen isotopes show that some, generaly Mg-richer, eclogites originated as lavas, whereas others have lower delta ~(18)O and higher Sr and Eu contents indicating an origin as plagioclase-bearing intrusive rocks formed in magma chambers witin the ocean crust. Major and trace element correlations demonstrate that the ecolgites are residues after partial melting during the subduction process, and that their present compositions were enriched in MgO by this process. The original lava compositions were picritic, but not komatiitic, whereas the intrusives had lower, basaltic MgO contents. The HFSE signature of the eclogites may indicate that ocean floor basalts of the time were relatively close to island arcs and recvcled material, which would be consistent with a larger number of smaller oceanic plates. Their composition appears to indicate that komatiitic ocean crust compositions were restricted to the early Archean which is not known to be represented among the eclogite xenolith population.
机译:来自西伯利亚Udachnaya的晚太古代(2.57 Ga)含钻石的榴辉岩异岩,具有地球化学特征,包括氧同位素值的变化,δ〜(18)O与主要元素和放射性同位素的相关性,可以解释为起源为俯冲大洋地壳。用Laser-ICPMS对石榴石和斜生辉石中的微量元素进行分析,以重建全岩石中的微量元素组成,这表明榴辉岩的场强元素(HFSE)浓度非常低,Zr / Hf和Nb / Ta的比值最相似到现代岛屿弧或超耗尽的地幔。尽管太古代海底的热液蚀变具有足够的地球化学作用,可以识别其在榴辉岩中的作用,从而将其诊断为前洋壳,但还不足以消除原始火成岩的许多其他地球化学特征,特别是相对较早的火成岩。固定式HFSE。微量元素形态与氧同位素的关系表明,一些富含镁的榴辉岩起源于熔岩,而其他的δ-(18)O较低,而Sr和Eu含量较高,表明其起源为形成于斜长石的侵入岩。地壳中的岩浆室。主要元素和痕量元素的相关性表明,镁橄榄石是俯冲过程中部分熔融后的残余物,并且通过该过程,它们的当前组成富含MgO。最初的熔岩成分是苦味的,但不是科马提质的,而侵入岩的玄武质MgO含量较低。榴辉岩的HFSE标记可能表明当时的海底玄武岩相对接近岛弧和倾斜的物质,这与大量较小的洋盘相一致。它们的组成似乎表明,科迈特洋洋壳的组成仅限于太古宙时期,尚不知道在榴辉岩异种岩种群中有这种成分。

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