首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Non-chondritic Sm/Nd ratio in the terrestrial planets: Consequences for the geochemical evolution of the mantle-crust system
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Non-chondritic Sm/Nd ratio in the terrestrial planets: Consequences for the geochemical evolution of the mantle-crust system

机译:地行星中的非软骨状Sm / Nd比:地幔-地壳系统地球化学演化的结果

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摘要

Super-chondritic ~(142)Nd signatures are ubiquitous in terrestrial, Martian and lunar samples, and indicate that the terrestrial planets may have accreted from material with Sm/Nd ratio higher than chondritic. This contradicts the long-held view that chondrites represent a reference composition for the ~(147)Sm-~(143)Nd system. Using coupled ~(146)Sm-~(142)Nd and ~(147)Sm-~(143)Nd systematics in planetary samples, we have proposed a new set of values for the ~(147)Sm/~(144)Nd and ~(143)Nd/~(144)Nd ratios of the bulk silicate Earth (Caro et al., 2008). Here, we revise the Bulk Silicate Earth estimates for the ~(87)Rb-~(87)Sr and ~(176)Lu-~(176)Hf systems using coupled Sr-Nd-Hf systematics in terrestrial rocks. These estimates are consistent with Hf-Nd systematics in lunar samples. The implications of a slightly non-chondritic silicate Earth with respect to the geochemical evolution of the mantle-crust system are then examined. We show that the Archean mantle has evolved with a composition indistinguishable from that of the primitive mantle until about 2Gyr. Positive ε~(143)Nd and ε~(176)Hf values ubiquitous in the Archean mantle are thus accounted for by the non-chondritic Sm/Nd and Lu/Hf composition of the primitive mantle rather than by massive early crustal formation, which solves the paradox that early Archean domains only have a limited extension in the present-day continents. The Sm-Nd and Lu-Hf evolution of the depleted mantle for the past 3.5Gyr can be entirely explained by continuous extraction of the continents from a well-mixed mantle. Thus, in contrast to the chondritic Earth model, Sm-Nd mass balance relationships can be satisfied without the need to call upon hidden reservoirs or layered mantle convection. This new Sm-Nd mass balance yields a scenario of mantle evolution consistent with trace element and noble gas systematics. The high ~3He/~4He mantle component is associated with ~(143)Nd/~(144)Nd compositions indistinguishable from the bulk silicate Earth, suggesting that the less degassed mantle sources did not experience significant fractionation for moderately incompatible elements.
机译:在陆,火星和月球样品中普遍存在超软骨形〜(142)Nd特征,这表明陆地行星可能从Sm / Nd比值高于软骨的物质中增生。这与长久以来的观点相矛盾,即球粒陨石代表〜(147)Sm-〜(143)Nd系统的参考组成。使用行星样本中的〜(146)Sm-〜(142)Nd和〜(147)Sm-〜(143)Nd耦合系统,我们提出了〜(147)Sm /〜(144)的一组新值。整体硅酸盐地球的Nd和〜(143)Nd /〜(144)Nd比(Caro et al。,2008)。在此,我们使用耦合的Sr-Nd-Hf系统,在地面岩石中修改了〜(87)Rb-〜(87)Sr和〜(176)Lu-〜(176)Hf系统的硅酸盐块体估计。这些估计值与月球样品中的Hf-Nd系统分析结果一致。然后研究了略呈非软骨状的硅酸盐地球对地幔-地壳系统地球化学演化的影响。我们表明,太古宙地幔的演化与原始地幔的成分一直没有区别,直到大约2Gyr。因此,太古代地幔中普遍存在的ε〜(143)Nd和ε〜(176)Hf正值是由原始地幔的非粒状Sm / Nd和Lu / Hf组成而不是由大量早期地壳形成引起的。解决了一个悖论,即早期的太古宙域在当今大陆仅具有有限的扩展。过去3.5Gyr耗尽地幔的Sm-Nd和Lu-Hf演化可以完全由不断混合的地幔中连续提取大陆来解释。因此,与软骨状地球模型相反,可以满足Sm-Nd质量平衡关系,而无需调用隐藏的储层或分层的地幔对流。这种新的Sm-Nd质量平衡产生了与微量元素和稀有气体系统一致的地幔演化情景。 〜3He /〜4He较高的地幔组分与〜(143)Nd /〜(144)Nd成分与大块硅酸盐地球无法区分,这表明脱气程度较低的地幔源对于中等程度不相容的元素没有明显的分馏作用。

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