Sublithospheric Diamonds: Plate Tectonics from Earth's Deepest Mantle Samples

IF 11.3 1区 地球科学 Q1 ASTRONOMY & ASTROPHYSICS Annual Review of Earth and Planetary Sciences Pub Date : 2024-01-18 DOI:10.1146/annurev-earth-032320-105438
Steven B. Shirey, D. Graham Pearson, Thomas Stachel, Michael J. Walter
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Abstract

Sublithospheric diamonds and the inclusions they may carry crystallize in the asthenosphere, transition zone, or uppermost lower mantle (from 300 to ∼800 km), and are the deepest minerals so far recognized to form by plate tectonics. These diamonds are distinctive in their deformation features, low nitrogen content, and inclusions of these major mantle minerals: majoritic garnet, clinopyroxene, ringwoodite, CaSi perovskite, ferropericlase, and bridgmanite or their retrograde equivalents. The stable isotopic compositions of elements within these diamonds (δ11B, δ13C, δ15N) and their inclusions (δ18O, δ56Fe) are typically well outside normal mantle ranges, showing that these elements were either organic (C) or modified by seawater alteration (B, O, Fe) at relatively low temperatures. Metamorphic minerals in cold slabs are effective hosts that transport C as CO3 and H as H2O, OH, or CH4 below the island arc and mantle wedge. Warming of the slab generates carbonatitic melts, supercritical aqueous fluids, or metallic liquids, forming three types of sublithospheric diamonds. Diamond crystallization occurs by movement and reduction of mobile fluids as they pass through host mantle via fractures—a process that creates chemical heterogeneity and may promote deep focus earthquakes. Geobarometry of majoritic garnet inclusions and diamond ages suggest upward transport, perhaps to the base of mantle lithosphere. From there, diamonds are carried to Earth's surface by eruptions of kimberlite magma. Mineral assemblages in sublithospheric diamonds directly trace Earth's deep volatile cycle, demonstrating how the hydrosphere of a rocky planet can connect to its solid interior. ▪ Sublithospheric diamonds from the deep upper mantle, transition zone, and lower mantle host Earth's deepest obtainable mineral samples. ▪ Low-temperature seawater alteration of the ocean floor captures organic and inorganic carbon at the surface eventually to become some of the most precious gem diamonds. ▪ Subduction transports fluids in metamorphic minerals to great depth. Fluids released by slab heating migrate, react with host mantle to induce diamond crystallization, and may trigger earthquakes. ▪ Sublithospheric diamonds are powerful tracers of subduction—a plate tectonic process that deeply recycles part of Earth's planetary volatile budget.Expected final online publication date for the Annual Review of Earth and Planetary Sciences, Volume 52 is May 2024. Please see http://www.annualreviews.org/page/journal/pubdates for revised estimates.
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岩石圈下的钻石:从地球最深的地幔样本看板块构造
岩石圈下金刚石及其可能携带的包裹体在星体层、过渡带或最上层下地幔(300 至 800 千米)中结晶,是迄今公认的由板块构造形成的最深层矿物。这些金刚石的独特之处在于它们的变形特征、低含氮量以及这些主要地幔矿物的包裹体:主石榴石、倩辉石、环钨矿、CaSi透辉石、铁闪长岩、桥粒岩或它们的逆行等价物。这些金刚石中的元素(δ11B、δ13C、δ15N)及其包裹体(δ18O、δ56Fe)的稳定同位素组成通常远远超出正常地幔范围,表明这些元素要么是有机元素(C),要么是在相对较低的温度下被海水蚀变(B、O、Fe)而改变的。冷板块中的变质矿物是有效的宿主,它们以 CO3 的形式将 C 和以 H2O、OH 或 CH4 的形式将 H 运送到岛弧和地幔楔以下。板块升温产生碳酸盐熔体、超临界水液或金属液,形成三种岩石圈下金刚石。金刚石的结晶是由流动流体在通过裂缝穿过主地幔时的移动和还原而产生的--这一过程会产生化学异质性,并可能促进深部聚焦地震。橄榄榴石包裹体的测地线和钻石的年龄表明,钻石是向上迁移的,可能迁移到地幔岩石圈的底部。从那里,金伯利岩浆的喷发将钻石带到地球表面。岩石圈下钻石中的矿物组合直接追溯了地球的深层挥发循环,展示了岩石行星的水圈是如何与其固体内部相联系的。来自深层上地幔、过渡带和下地幔的岩石圈下金刚石拥有地球上可获得的最深矿物样本。洋底的低温海水蜕变在表层捕获有机碳和无机碳,最终成为一些最珍贵的宝石钻石。俯冲作用将变质矿物中的流体带到很深的地方。板块加热释放的流体迁移,与主地幔发生反应,诱发钻石结晶,并可能引发地震。岩石圈下的钻石是俯冲--板块构造过程--的强大示踪剂,它深度回收了地球行星挥发性预算的一部分。《地球与行星科学年刊》第52卷的最终在线出版日期预计为2024年5月。修订后的预计日期请参见 http://www.annualreviews.org/page/journal/pubdates。
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来源期刊
Annual Review of Earth and Planetary Sciences
Annual Review of Earth and Planetary Sciences 地学天文-地球科学综合
CiteScore
25.10
自引率
0.00%
发文量
25
期刊介绍: Since its establishment in 1973, the Annual Review of Earth and Planetary Sciences has been dedicated to providing comprehensive coverage of advancements in the field. This esteemed publication examines various aspects of earth and planetary sciences, encompassing climate, environment, geological hazards, planet formation, and the evolution of life. To ensure wider accessibility, the latest volume of the journal has transitioned from a gated model to open access through the Subscribe to Open program by Annual Reviews. Consequently, all articles published in this volume are now available under the Creative Commons Attribution (CC BY) license.
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