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克拉通边缘富含硫化物的大陆根由碳酸盐熔体形成。

Sulfide-rich continental roots at cratonic margins formed by carbonated melts.

作者信息

Chen Chunfei, Förster Michael W, Shcheka Svyatoslav S, Ezad Isra S, Shea Joshua J, Liu Yongsheng, Jacob Dorrit E, Foley Stephen F

机构信息

State Key Laboratory of Geological Processes and Mineral Resources, School of Earth Sciences, China University of Geosciences, Wuhan, China.

School of Natural Sciences, Macquarie University, North Ryde, New South Wales, Australia.

出版信息

Nature. 2025 Jan;637(8046):615-621. doi: 10.1038/s41586-024-08316-w. Epub 2025 Jan 8.

DOI:10.1038/s41586-024-08316-w
PMID:39779858
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11735387/
Abstract

The cratonic crust contains abundant mineral deposits of metals such as gold, copper and rare earths and is underlain by a thick mantle lithosphere rich in the volatiles carbon, sulfur and water. Although volatiles are known to be key components in metallogenesis, how and where they are distributed in the cratonic lithosphere mantle and their role in the initial enrichment of metals have not been sufficiently explored. Here we compile sulfur and copper contents of global cratonic peridotites, identifying sulfide-rich and copper-rich continental roots at depths of 160-190 km at cratonic margins. Our new high-pressure experiments show that carbonated silicate melts originating from the asthenosphere lose silicate components during reaction with lithospheric peridotite, evolving to carbonatite melts that become concentrated at cratonic margins. Sulfur solubility in melts substantially decreases as the SiO content of melts decreases during this process, forcing sulfide precipitation and the formation of sulfide-rich continental roots at the base of the mantle lithosphere. The migration of carbonated melts towards cratonic margins replenishes the continental roots there with sulfur, explaining the co-location of magmatic metal deposits with carbonatites close to cratonic margins. These findings highlight the notable role of carbonated melts in metallogenesis and provide a potential platform for metal ore exploration.

摘要

克拉通地壳含有丰富的金、铜和稀土等金属矿床,其下是富含挥发性碳、硫和水的厚地幔岩石圈。尽管已知挥发性物质是成矿作用的关键成分,但它们在克拉通岩石圈地幔中的分布方式和位置以及它们在金属初始富集过程中的作用尚未得到充分探索。在这里,我们汇编了全球克拉通橄榄岩的硫和铜含量,确定了克拉通边缘160 - 190公里深处富含硫化物和铜的大陆根。我们新的高压实验表明,来自软流圈的碳酸化硅酸盐熔体在与岩石圈橄榄岩反应过程中会失去硅酸盐成分,演变成碳酸岩熔体,并在克拉通边缘富集。在此过程中,随着熔体SiO含量的降低,熔体中的硫溶解度大幅下降,促使硫化物沉淀并在岩石圈地幔底部形成富含硫化物的大陆根。碳酸化熔体向克拉通边缘的迁移为那里的大陆根补充了硫,解释了岩浆金属矿床与靠近克拉通边缘的碳酸岩的共存现象。这些发现突出了碳酸化熔体在成矿作用中的显著作用,并为金属矿勘探提供了一个潜在平台。

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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8ff7/11735387/504e2b6f7f58/41586_2024_8316_Fig9_ESM.jpg
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本文引用的文献

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Incipient carbonate melting drives metal and sulfur mobilization in the mantle.初始碳酸盐熔融驱动地幔中的金属和硫迁移。
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