23 GPa流变性转变前后顽辉石球粒质地幔的部分熔体成分:对地幔化学分异的启示

IF 2.4 3区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Hideharu Kuwahara
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引用次数: 0

摘要

类地行星被认为是由球粒质物质构成的。然而,以往的研究表明,与球粒测量值相比,地球上地幔中一些不相容的难熔亲石元素(RLEs),如U和Th,已被耗尽。为了解释上地幔和球粒陨石之间的成分矛盾,提出了下地幔中存在不相容RLEs的隐伏储层。这些研究提出了岩浆海洋凝固过程中不相容RLEs隐藏储层的可能,以及由于富铁致密堆积的引力不稳定导致的后续地幔倾覆。然而,部分熔体的密度及其在结晶的深部岩浆海洋中的命运仍然存在争议。在这里,我们报告了23 GPa的顽辉石球粒质地幔的部分熔融成分作为熔化程度的函数。结果表明:在球粒岩浆海洋中结晶的桥辉石随着熔融程度的降低而富集Fe和Ca,阻止了铁长石和CaSiO3钙钛矿(Davemaoite)的结晶;在流变过渡阶段(根据质量平衡计算,熔融程度为40%),即使在平衡结晶的情况下,固液分离也能有效地发生,固体部分主要由桥菱石和微量镁铁石组成,与初始球粒陨石组成相比,熔体中FeO和CaO的含量变得丰富。流变转变处熔体的密度比桥辉石轻,但比镁铁镁石密度大,表明熔体可能在地幔过渡带的底部发生了沉积。660 km深度附近的熔池如果对后续地幔对流稳定,可能富集了不相容RLEs,形成了缺失RLEs的隐伏储层。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Partial melt composition of enstatite chondritic mantle around the rheological transition at 23 GPa: Implications for the chemical differentiation of the Earth's mantle

Partial melt composition of enstatite chondritic mantle around the rheological transition at 23 GPa: Implications for the chemical differentiation of the Earth's mantle

Terrestrial planets are thought to be made of chondritic materials. However, previous studies have suggested that the Earth's upper mantle is depleted in some incompatible refractory lithophile elements (RLEs), such as U and Th in comparison with chondritic values. To explain the compositional contradiction between the upper mantle and chondrites, a hidden reservoir for incompatible RLEs in the lower mantle has been proposed. These studies have invoked a possible formation of hidden reservoir for incompatible RLEs during magma ocean solidification and by subsequent mantle overturn due to the gravitational instability of Fe-rich dense cumulates. However, the density of partial melt and its fate in a crystallizing deep magma ocean is still debated. Here we report partial melt compositions of enstatite chondritic mantle at 23 GPa as a function of the extent of melting. The results show that bridgmanite crystallized in a chondritic magma ocean becomes enriched in Fe and Ca with decreasing extent of melting and prevents the crystallization of ferropericlase and CaSiO3 perovskite (Davemaoite). At the rheological transition (the extent of melting of 40% based on mass balance calculation), where the solid-liquid separation efficiently occurs even in the case of equilibrium crystallization, the solid part is mostly composed of bridgmanite with a trace amount of majorite, and the melt becomes enriched in FeO and CaO compared to the initial chondritic composition. The calculated density of the melt at the rheological transition is lighter than bridgmanite, but denser than majorite, suggesting that the melt may have ponded at the bottom of the mantle transition zone. The melt ponded around 660 km depth may have been enriched in incompatible RLEs and formed the hidden reservoir for missing RLEs if this melt-bearing region is stable against subsequent mantle convection.

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来源期刊
Physics of the Earth and Planetary Interiors
Physics of the Earth and Planetary Interiors 地学天文-地球化学与地球物理
CiteScore
5.00
自引率
4.30%
发文量
78
审稿时长
18.5 weeks
期刊介绍: Launched in 1968 to fill the need for an international journal in the field of planetary physics, geodesy and geophysics, Physics of the Earth and Planetary Interiors has now grown to become important reading matter for all geophysicists. It is the only journal to be entirely devoted to the physical and chemical processes of planetary interiors. Original research papers, review articles, short communications and book reviews are all published on a regular basis; and from time to time special issues of the journal are devoted to the publication of the proceedings of symposia and congresses which the editors feel will be of particular interest to the reader.
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