Jing Sun , Sebastian Tappe , Sergey Kostrovitsky , Tatiana Kalashnikova , Sheng-Hua Zhou , Katie A. Smart
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Although the majority of eclogite samples are characterized by equilibrium temperatures higher than the closure temperatures of the Lu-Hf and Sm-Nd isotope systems, they might have experienced rapid cooling and uplift to shallower lithospheric mantle depths, or fast heating immediately prior to kimberlite eruption, without resetting of the isotopic systems. If this assumption is correct, then the mineral pair two-point isochron ages represent a cooling episode during the Proterozoic between 2.2 and 0.8 Ga. The age peak at 1.9 Ga for the Obnazhennaya eclogites falls within the 2.1–1.8 Ga age range for eclogite xenolith suites from cratons worldwide, which supports the evidence for widespread oceanic lithosphere subduction during the Paleoproterozoic. The timing of this global subduction event coincides with the formation of orogenic belts at ca. 1.8 Ga during the final assembly of the Paleoproterozoic Columbia supercontinent, which was completed by 1.6 Ga. Age complexity is revealed by the majority of eclogite samples, which equilibrated close to or above the closure temperatures for the Lu-Hf and Sm-Nd isotope systems. Isochron ages as young as 185 Ma for a single low-MgO eclogite xenolith suggest that these mantle-derived materials resided deep within the Siberian cratonic root, and that radiogenic Hf and Nd only accumulated in the constituent garnet and clinopyroxene after xenolith entrainment into the host kimberlite magma. The presence of garnet exsolution lamellae in clinopyroxene also records protracted cooling, but presents a challenge for producing clean mineral separates in an attempt to obtain robust Lu-Hf and Sm-Nd isochron ages.</div></div>","PeriodicalId":18070,"journal":{"name":"Lithos","volume":"508 ","pages":"Article 108062"},"PeriodicalIF":2.9000,"publicationDate":"2025-03-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Timing of subduction along the northern margin of the Siberian craton: Lu-Hf and Sm-Nd isochrons for kimberlite-borne mantle eclogite xenoliths\",\"authors\":\"Jing Sun , Sebastian Tappe , Sergey Kostrovitsky , Tatiana Kalashnikova , Sheng-Hua Zhou , Katie A. 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引用次数: 0
摘要
由西伯利亚陨石坑上约 152 Ma 年前的奥布纳真纳亚金伯利岩带出的蚀变地幔异长岩是变质玄武岩洋壳的典范。西伯利亚陨石坑上距今约 152 Ma 的奥布纳真纳亚金伯利岩是变质玄武岩洋壳的典范,其形成通常归因于陨石坑东北边缘的古老俯冲机制。在这项研究中,获得了来自 Obnazhennaya 金伯利岩的高氧化镁和低氧化镁夕闪岩的霞石和石榴石的 Lu-Hf 和 Sm-Nd 同位素数据。虽然大多数斜长岩样品的平衡温度高于 Lu-Hf 和 Sm-Nd 同位素系统的闭合温度,但它们可能在金伯利岩喷发前经历了快速冷却和隆起到较浅岩石圈地幔深度,或快速加热,而没有重新设置同位素系统。如果这一假设是正确的,那么矿物对的两点等时线年龄就代表了在 2.2 Ga 到 0.8 Ga 之间的新生代冷却过程。Obnazhennaya斜长岩的年龄峰值为1.9 Ga,属于全球陨石坑斜长岩异长岩套件的2.1-1.8 Ga年龄范围,这支持了古新生代期间大洋岩石圈广泛俯冲的证据。这一全球俯冲事件的时间与造山带形成的时间(约 1.8 Ga)相吻合。在古近代哥伦比亚超大陆的最终组装过程中,造山带的形成时间约为 1.8 Ga,而哥伦比亚超大陆的组装则在 1.6 Ga 时完成。大多数斜长岩样品显示了年龄的复杂性,这些样品的平衡温度接近或超过了Lu-Hf和Sm-Nd同位素系统的闭合温度。一块低氧化镁夕闪岩异质岩的等时年龄早至185Ma,这表明这些地幔衍生物质深藏于西伯利亚板块根部,而放射性Hf和Nd只是在异质岩夹带进入主金伯利岩浆后才在成分石榴石和鳞片辉石中积累起来的。霞石中石榴石外溶解片层的存在也记录了长时间的冷却,但这对生产干净的矿物分离物以试图获得可靠的lu-hf和sm-nd等时线年龄提出了挑战。
Timing of subduction along the northern margin of the Siberian craton: Lu-Hf and Sm-Nd isochrons for kimberlite-borne mantle eclogite xenoliths
Eclogitic mantle xenoliths brought up by the ca. 152 Ma old Obnazhennaya kimberlite on the Siberian craton are examples of metamorphosed basaltic oceanic crust, and their formation is commonly attributed to ancient subduction regimes along the northeastern craton margin. In this study, Lu-Hf and Sm-Nd isotope data for clinopyroxene and garnet were obtained for high-MgO and low-MgO eclogite xenoliths from the Obnazhennaya kimberlite. Although the majority of eclogite samples are characterized by equilibrium temperatures higher than the closure temperatures of the Lu-Hf and Sm-Nd isotope systems, they might have experienced rapid cooling and uplift to shallower lithospheric mantle depths, or fast heating immediately prior to kimberlite eruption, without resetting of the isotopic systems. If this assumption is correct, then the mineral pair two-point isochron ages represent a cooling episode during the Proterozoic between 2.2 and 0.8 Ga. The age peak at 1.9 Ga for the Obnazhennaya eclogites falls within the 2.1–1.8 Ga age range for eclogite xenolith suites from cratons worldwide, which supports the evidence for widespread oceanic lithosphere subduction during the Paleoproterozoic. The timing of this global subduction event coincides with the formation of orogenic belts at ca. 1.8 Ga during the final assembly of the Paleoproterozoic Columbia supercontinent, which was completed by 1.6 Ga. Age complexity is revealed by the majority of eclogite samples, which equilibrated close to or above the closure temperatures for the Lu-Hf and Sm-Nd isotope systems. Isochron ages as young as 185 Ma for a single low-MgO eclogite xenolith suggest that these mantle-derived materials resided deep within the Siberian cratonic root, and that radiogenic Hf and Nd only accumulated in the constituent garnet and clinopyroxene after xenolith entrainment into the host kimberlite magma. The presence of garnet exsolution lamellae in clinopyroxene also records protracted cooling, but presents a challenge for producing clean mineral separates in an attempt to obtain robust Lu-Hf and Sm-Nd isochron ages.
期刊介绍:
Lithos publishes original research papers on the petrology, geochemistry and petrogenesis of igneous and metamorphic rocks. Papers on mineralogy/mineral physics related to petrology and petrogenetic problems are also welcomed.