首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >~(187)Os-enriched domain in an Archean mantle plume: evidence from 2.8 Ga komatiites of the Kostomuksha greenstone belt, NW Baltic Shield
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~(187)Os-enriched domain in an Archean mantle plume: evidence from 2.8 Ga komatiites of the Kostomuksha greenstone belt, NW Baltic Shield

机译:太古代地幔柱中〜(187)Os富集区域:来自西北波罗的海盾构Kostomuksha绿岩带的2.8 Ga科马提岩的证据

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The Re-Os data on Archean komatiites from the Kostomuksha greenstone belt in the Baltic Shield are presented. This greenstone belt has been previously interpreted to represent a former oceanic plateau formed by the emplacement of an ancient plume head [Puchtel et al., Earth Planet. Sci. Lett. 155 (1998) 57-74]. Samples of flowtop breccia, spinifextextured and cumulate komatiites and a chromite separate, all collected from the core of a 300 m deep diamond drill hole, yielded a Re-Os isochron with an age of 2795 ± 40 Ma and an initial ~(187)Os/~(188)Os of 0.1117 ± 0.0011 (γ~(187)Os = + 3.6 ± 1.0). The high positive γ~(187)Os(T) implies that the komatiites were derived from a mantle source with a time-integrated suprachondritic Re/Os ratio. Recycling of oceanic lithosphere to produce the enriched ~(187)Os isotope signature is considered unlikely, as 15-25% crustal component is required to be incorporated into the plume source as early as 3.5-4.3 Ga. Such a substantial proportion of mafic material in the source would likely destroy the major and trace element characteristics of the komatiites. Our tentative interpretation is that the ~(187)Os-enrichment in the Kostomuksha plume represents an outer core signature. If confirmed by the ongoing Pt-Os isotope studies, the results would provide evidence for the existence of whole-mantle convection in the late Archean, and might place constraints on the timing of core differentiation in the early Earth.
机译:给出了来自波罗的海盾的科斯图穆克沙绿岩带的太古代科马提岩的Re-Os数据。该绿岩带先前已被解释为代表由古代羽状头的位置形成的前洋洋高原[Puchtel等,地球行星。科学来吧155(1998)57-74]。从300 m深的金刚石钻孔的岩心中采集的流顶角砾岩,刺状结构和累积的科马蒂岩样品以及亚铬酸盐分离样品,产生了Re-Os等时线,年龄为2795±40 Ma,初始〜(187)Os /〜(188)Os为0.1117±0.0011(γ〜(187)Os = + 3.6±1.0)。较高的正γ〜(187)Os(T)表示,孔雀石是从幔源中衍生出来的,具有时间积分的超胶质岩Re / Os比。人们认为不可能再利用海洋岩石圈产生富集的〜(187)Os同位素标记,因为早在3.5-4.3 Ga时就需要将15-25%的地壳成分掺入烟羽中。如此大量的镁铁质物质源中的钙可能会破坏科马铁矿的主要和微量元素特征。我们的初步解释是,Kostomuksha羽中〜(187)Os的富集代表了外部核特征。如果得到正在进行的Pt-Os同位素研究的证实,那么该结果将为太古宙晚期存在完整的对流对流提供证据,并且可能会限制地球早期的核心分化时间。

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