Experimental Results on Fractionation of the Highly Siderophile Elements (HSE) at Variable Pressures and Temperatures during Planetary and Magmatic Differentiation

1区 地球科学 Q1 Earth and Planetary Sciences
J. Brenan, N. Bennett, Z. Zajacz
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引用次数: 85

Abstract

The platinum-group elements (PGEs; Os, Ir, Ru, Rh, Pt, Pd), along with rhenium and gold, are grouped together as the highly siderophile elements (HSEs), defined by their extreme partitioning into the metallic, relative to the oxide phase (> 104). The HSEs are highly refractory, as gauged by their high melting and condensation temperatures, and were therefore relatively concentrated in the feedstock for the terrestrial planets, as defined by the composition of chondritic meteorites (e.g., Anders and Ebihara 1982; Horan et al. 2003; Fischer-Godde et al. 2010). However, the planetary formation and differentiation process has since acted on this chemical group to produce a rich variety of absolute and relative inter-element fractionations. For example, analysis of iron meteorites suggests a significant decoupling of the HSE in the cores of planetesimals, and likely Earth’s core, with Os, Ir, Ru (IPGE-group) and Re concentrated in the metal phase, and Pt, Rh, Pd (PPGE-group) plus Au usually concentrated in the residual liquid (Goldstein et al. 2009). In terms of the silicate Earth, analysis of mantle rocks reveals very low levels of the HSE, but relative abundances similar to chondrites (see review by Day et al. 2016, this volume), in part reflecting HSE segregation into core-forming iron (Ringwood 1966; Ganapathy et al. 1970). This is in contrast to mantle-derived melts, whose HSE abundances are highly fractionated, with relative depletions in the IPGE-group compared to PPGE-group, as well as Re and Au (Barnes et al. 1985). Resulting Re/Os and Pt/Os fractionation also influence the long-term evolution of the 187Re to 187Os and 190Pt to 186Os decay systems, and, hence, the development of distinctive Os-isotope reservoirs (Walker et al. 1997; Shirey and Walker 1998; Day 2013). The emplacement of mantle-derived magmas into Earth’s crust results in …
行星和岩浆分异过程中高亲铁元素(HSE)在变压变温条件下分馏的实验结果
铂族元素(PGEs;Os, Ir, Ru, Rh, Pt, Pd),以及铼和金,被归类为高度亲铁元素(hsse),由它们相对于氧化物相(> 104)的极端分配到金属中来定义。根据球粒陨石的组成(例如,Anders and Ebihara 1982;Horan et al. 2003;fisher - godde et al. 2010)。然而,行星的形成和分化过程自此作用于这一化学群,产生了丰富多样的绝对和相对元素间分馏。例如,对铁陨石的分析表明,星子核心(很可能是地核)中的HSE存在明显的解耦,Os、Ir、Ru (IPGE-group)和Re集中在金属相中,而Pt、Rh、Pd (PPGE-group)和Au通常集中在残液中(Goldstein etal . 2009)。就硅酸盐地球而言,对地幔岩石的分析显示,HSE含量非常低,但相对丰度与球粒陨石相似(见Day等人2016年的评论,本卷),部分反映了HSE分离成核形成铁(Ringwood 1966;Ganapathy et al. 1970)。这与地幔源熔体相反,地幔源熔体的HSE丰度是高度分散的,与ppge组相比,ipge组相对减少,Re和Au也相对减少(Barnes et al. 1985)。由此产生的Re/Os和Pt/Os分馏也影响了187Re - 187Os和190Pt - 186Os衰变系统的长期演化,从而影响了独特的Os同位素储层的发育(Walker等,1997;Shirey and Walker 1998;天,2013)。地幔岩浆进入地壳的位置导致…
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来源期刊
Reviews in Mineralogy & Geochemistry
Reviews in Mineralogy & Geochemistry 地学-地球化学与地球物理
CiteScore
8.30
自引率
0.00%
发文量
39
期刊介绍: RiMG is a series of multi-authored, soft-bound volumes containing concise reviews of the literature and advances in theoretical and/or applied mineralogy, crystallography, petrology, and geochemistry. The content of each volume consists of fully developed text which can be used for self-study, research, or as a text-book for graduate-level courses. RiMG volumes are typically produced in conjunction with a short course but can also be published without a short course. The series is jointly published by the Mineralogical Society of America (MSA) and the Geochemical Society.
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