e球粒陨石变质过程中微量元素的再分布:对还原体和地球的影响

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Jean-Alix Barrat , Addi Bischoff , Brigitte Zanda
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引用次数: 0

摘要

本文报道了对顽辉石球粒陨石(ECs)微量元素的新分析,以阐明它们在变质过程中的行为。在由3型向5型或更高型转变的过程中,硅酸盐的大部分微量元素流失到硫化物中。我们的程序使我们能够很容易地获得EC的硅酸盐部分的微量元素丰度。EH和EL球粒陨石的这些组分的元素模式(尤其是REE模式)有很大的不同,并且与变质品位有关。这种方法对陨石分类很有用,特别是当硫化物发生变化时。将其应用于异常ec,可以直接识别QUE 94204的EH亲和力,并表明Zakłodzie, NWA 4301和NWA 4799来自先前未采样的相同EH样体。我们利用最变质球粒陨石的硅酸盐组分的浓度来讨论EH或EL亲和还原体(即岩心分离后)的原始地幔的化学特征。我们的数据表明,这些地幔中难熔亲石元素(RLEs),特别是稀土元素(ree)非常缺乏,并且在Sr, Zr, Hf和Ti中表现出显著的正异常。这些估计表明,这些天体的大部分稀土、铀和钍元素都包含在地核中。有趣的是,推断出的这些缩小天体的原始地幔与地球的形成了对比。如果地球基本上是由ec吸积而来,人们会期望类似的特征被保留下来,但事实并非如此。这种不匹配可以解释为块状硅酸盐土后来的均质化,或者是被吸积的物质在同位素上与ec相似,但在矿物学上不同(即不含oldoldmine)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Trace element redistributions during metamorphism of E-chondrites: Implications for reduced bodies and the Earth

We report on new trace element analyses of enstatite chondrites (ECs) to clarify their behavior during the metamorphism. During the transition from a type 3 to a type 5 or higher, silicates lose a large portion of their trace elements to sulfides. Our procedure allows us to obtain trace element abundances of the silicate fraction of an EC quite easily. The element patterns of these fractions (especially REE patterns) are quite different for EH and EL chondrites, and are furthermore dependent on the metamorphic grade. This procedure can be usefull to classify meteorites, in particular when the sulfides are altered. Applied to anomalous ECs, it allows direct recognition of the EH affinity of QUE 94204, and suggests that Zakłodzie, NWA 4301, and NWA 4799 derive from the same EH-like body of previously unsampled composition.

We have used the concentrations obtained on the silicate fractions of the most metamorphosed chondrites to discuss the chemical characteristics of the primitive mantles of reduced bodies of EH or EL affinity (i.e., after core segregation). Our data indicate that these mantles are very depleted in refractory lithophile elements (RLEs), particularly in rare earth elements (REEs), and notably show significant positive anomalies in Sr, Zr, Hf, and Ti. These estimates imply that the cores contain most of the REEs, U and Th of these bodies. Interestingly, the inferred primitive mantles of these reduced bodies contrast with that of the Earth. If the Earth accreted essentially from ECs, one would expect similar signatures to be preserved, which is not the case. This mismatch can be explained either by a later homogenization of the bulk silicate Earth, or alternatively, that the materials that were accreted were isotopically similar to ECs, but mineralogically different (i.e., oldhamite-free).

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来源期刊
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta 地学-地球化学与地球物理
CiteScore
9.60
自引率
14.00%
发文量
437
审稿时长
6 months
期刊介绍: Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes: 1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids 2). Igneous and metamorphic petrology 3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth 4). Organic geochemistry 5). Isotope geochemistry 6). Meteoritics and meteorite impacts 7). Lunar science; and 8). Planetary geochemistry.
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