Rare earth elements in apatite: A proxy for unravelling carbonatite melt compositions

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Earth and Planetary Science Letters Pub Date : 2024-07-04 DOI:10.1016/j.epsl.2024.118863
Haihao Guo , Johann Tuduri , Zineb Nabyl , Saskia Erdmann , Xiaochun Li , Fabrice Gaillard
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Abstract

Carbonatites are fascinating magmatic rocks because of their anomalous compositions, including the fact that some of these rocks host major rare earth element (REE) deposits. Despite much recent work, our understanding of their genesis and the composition of initial carbonatite melts is hindered by two major obstacles: most carbonatites we see are intrusive rocks, and they are commonly affected by metasomatic overprint. Here, we report experimental data in which we use apatite as a geochemical proxy to see back through crystallization and metasomatic events, thus making it possible to decipher the composition of carbonatite melts. We determined partition coefficients between apatite and carbonatite melts for a broad range of elements. The Na-rich nature of carbonatite melts plays an important role in apatite-melt partition coefficients, which are in the range of 1–7 for Sr, Y and REE in carbonatite systems. Using our new experimental data combined with >700 apatite composition data from carbonatites in various geodynamic settings, we show that carbonatite melt REE contents vary by more than two orders of magnitude. This variation cannot be solely produced by crystal-melt fractionation, implying that some carbonatite melts must be REE-rich or REE-poor initially, and that they mostly remain so during differentiation. We conclude that the degree of REE enrichment reflects carbonatite melts produced by immiscibility from variably differentiated alkaline magmas.

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磷灰石中的稀土元素:揭示碳酸盐岩熔体成分的替代物
碳酸盐岩是令人着迷的岩浆岩,因为它们的成分异常,包括其中一些岩石蕴藏着主要的稀土元素(REE)矿床。尽管最近做了大量工作,但我们对碳酸盐岩成因和初始碳酸盐岩熔体成分的了解仍受到两大障碍的阻碍:我们看到的大多数碳酸盐岩都是侵入岩,而且它们通常受到元古代叠印的影响。在这里,我们报告了一些实验数据,其中我们使用磷灰石作为地球化学替代物来回溯结晶和元成岩事件,从而有可能破译碳酸盐岩熔体的成分。我们测定了磷灰石和碳酸盐岩熔体之间多种元素的分配系数。碳酸盐岩熔体富含 Na 的性质在磷灰石-熔体分配系数中发挥了重要作用,碳酸盐岩体系中 Sr、Y 和 REE 的分配系数在 1-7 之间。利用我们的新实验数据以及来自不同地球动力环境下碳酸盐岩的 700 个磷灰石成分数据,我们发现碳酸盐岩熔体中的 REE 含量相差两个数量级以上。这种变化不可能完全由晶体-熔体分馏产生,这意味着一些碳酸盐岩熔体最初一定是富含或贫含REE的,而且在分化过程中它们大多保持这种状态。我们的结论是,REE富集程度反映了从不同分异的碱性岩浆中通过不熔性产生的碳酸盐岩熔体。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Earth and Planetary Science Letters
Earth and Planetary Science Letters 地学-地球化学与地球物理
CiteScore
10.30
自引率
5.70%
发文量
475
审稿时长
2.8 months
期刊介绍: Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.
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