科米大火成岩带的岩浆-岩石圈相互作用:中国西藏江孜南部两种岩浆岩堤的证据

IF 4.6 3区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY
China Geology Pub Date : 2024-01-01 DOI:10.31035/cg2023023
Ya-ying Wang , Ling-sen Zeng , Li-e Gao , Li-long Yan , Ling-hao Zhao , Jia-hao Gao , Ying-long Di , Guang-xu Li , Yi-hong Tian
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引用次数: 0

摘要

西藏东南部江孜地区出露了两套岩浆岩堤,分别为T1193-A和T1194-A。它们位于康美LIP地区,与江孜地区的另外两块堤坝--锆石年龄为137.7±1.3Ma的T0902堤坝和锆石年龄为142±1.4Ma的T0907堤坝(Wang YY et al.综合所有四条辉绿岩堤,可归纳出两种不同类型,即 OIB 型和弱富集型。OIB型 "样品(包括T1193-A和T0907堤坝)显示出类似OIB的地球化学特征,其初始Sr-Nd同位素值与科米大火成岩带(LIP)中的大多数岩浆产物相似,表明它们代表了直接从凯尔盖朗地幔羽流中生成的熔体。包括T1194-A和T0902岩堤在内的 "弱富集型 "样品的REEs和微量元素模式显示出板块内的亲缘关系,但具有明显的Nb-Ta-Ti负异常。它们显示出均匀的较低的εNd(t)值(-6--2)和较高的87Sr/86Sr(t)值(0.706-0.709),这与它们的氧化镁变化无关,表明它们是一个富集地幔源。这些 "弱富集型 "样品与德令哈喜马拉雅地区广泛存在的科米低成岩期岩浆产物有着密切的时空关系,因此它们与来自地幔羽流的熔融物和上述古老的德令哈喜马拉雅次大陆岩石圈地幔(SCLM)中不同比例的熔融物的混合是一致的。科米大裂隙中的这些弱富集岩浆岩形成了一个特殊的岩石群,很可能表明大规模的热地幔羽流-大陆岩石圈相互作用。这一过程可能导致早白垩世哲支喜马拉雅岩石圈的强烈改造。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Plume-lithosphere interaction in the Comei Large Igneous Province: Evidence from two types of mafic dykes in Gyangze, south Tibet, China

Two suites of mafic dykes, T1193-A and T1194-A, outcrop in Gyangze area, southeast Tibet. They are in the area of Comei LIP and have indistinguishable field occurrences with two other dykes in Gyangze, T0902 dyke with 137.7±1.3 Ma zircon age and T0907 dyke with 142±1.4 Ma zircon age reported by Wang YY et al. (2016), indicating coeval formation time. Taking all the four diabase dykes into consideration, two different types, OIB-type and weak enriched-type, can be summarized. The “OIB-type” samples, including T1193-A and T0907 dykes, show OIB-like geochemical features and have initial Sr-Nd isotopic values similar with most mafic products in Comei Large Igneous Provinces (LIP), suggesting that they represent melts directly generated from the Kerguelen mantle plume. The “weak enriched-type ” samples, including T1194-A and T0902 dykes, have REEs and trace element patterns showing within-plate affinity but have obvious Nb-Ta-Ti negative anomalies. They show uniform lower εNd(t) values (–6––2) and higher 87Sr/86Sr(t) values (0.706–0.709) independent of their MgO variation, indicating one enriched mantle source. Considering their closely spatial and temporal relationship with the widespread Comei LIP magmatic products in Tethyan Himalaya, these “weak enriched-type” samples are consistent with mixing of melts from mantle plume and the above ancient Tethyan Himalaya subcontinental lithospheric mantle (SCLM) in different proportions. These weak enriched mafic rocks in Comei LIP form one special rock group and most likely suggest large scale hot mantle plume-continental lithosphere interaction. This process may lead to strong modification of the Tethyan Himalaya lithosphere in the Early Cretaceous.

©2024 China Geology Editorial Office.

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来源期刊
China Geology
China Geology GEOLOGY-
CiteScore
7.80
自引率
11.10%
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275
审稿时长
16 weeks
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