冈瓦纳超大陆中部变质岩浆岩地球化学特征揭示的板内伸展环境

IF 3.2 2区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY
Sanjeewa P.K. Malaviarachchi , Lei Zhao , Jinghui Guo , Xianhua Li , Mingguo Zhai , Prasanna L. Dharmapriya
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引用次数: 0

摘要

尽管对挤压构造有广泛的研究,但与寒武纪造山带崩塌形成冈瓦南边缘有关的伸展期尚未得到深入的研究。在斯里兰卡,在Kadugannawa和Highland Complexes(分别为KC和HC)东部边界地带的裂谷背景可能对应于印度、南极洲和马达加斯加附近的Gondwanan中部段。因此,该研究为大陆内伸展边缘的地球化学表征提供了一条途径,为全球构造地球化学知识增添了新的价值。分析的KC变质基性岩石显示出光滑的球粒陨石归一化稀土元素(REE)模式,大多数岩石具有明显的重稀土(HREE)消耗,(La/Yb)N比值在2 ~ 20之间,Eu有轻微的负-正异常。多数长英岩还表现出高轻稀土(LREE)富集的HREE亏缺,并伴有变正至微负Eu异常。HC变质基性岩石多呈中、中稀土(MREE) ~三稀土(HREE)模式,低稀土(LREE)变化富集,多数呈离散负异常或无Eu异常。所有变质基性岩的原岩均来源于富集的地幔/OIB源。研究的变质长英质岩石均不具有弧岩浆特征,均符合a2型造山特征的成因特征。因此,本文研究的变质基性岩和变质长英质岩原岩熔体的整体地球化学特征表明,它们的成因处于板块内伸展环境,而不是以往主要研究的弧形构造环境。我们的U- pb年龄数据对应于约2250 ~ 550 Ma的岩浆脉冲(约2250 ~ 1750 Ma, 1050 ~ 850 Ma, 700 ~ 627 Ma和550 ~ 575 Ma),随后与地壳成分在约580 ~ 530 Ma的显著相互作用,这与锆石中Th/U和Ce/Ce*值的上升一致。主要年龄峰与全球超克拉通(如苏superia)、超大陆(如Columbia、Rodinia和Gondwana)和区域微大陆(如Azania)的分散和融合相关的碰撞和裂陷事件吻合良好,时间跨度为约2250 ~约500 Ma的早期到晚期全球地球动力学史。因此,这项研究为冈瓦纳中部内陆迄今未知的大陆内裂谷/伸展构造环境提供了新的见解。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Insights for intraplate extensional settings revealed from geochemistry of metamorphosed magmatic rocks of the central Gondwana supercontinent
The extensional episodes related to the shaping of the Gondwanan margins with the collapse of the Cambrian Orogens have not been deeply investigated despite extensive studies on compressional tectonics. The rift-setting considered here in Sri Lanka at the boundary zone of eastern parts of Kadugannawa and Highland Complexes (KC and HC, respectively) may correspond to the central Gondwanan segments in the vicinity of India, Antarctica, and Madagascar. Hence this study offers a pathway to geochemical characterization of intra-continental extensional margins adding a new value for global tectono-geochemical knowledge. Analysed meta-mafic rocks of the KC display smooth Chondrite normalized rare earth element (REE) patterns with most of them having distinct heavy REE (HREE) depletions, with (La/Yb)N ratios in the range of 2–20, and slightly negative to positive Eu anomaly. The majority of felsic-rocks also show HREE depletion with high light REE (LREE) enrichment accompanying variably-positive to slightly-negative Eu anomalies. In contrast, meta-mafic rocks of the HC mostly show flat middle REE (MREE) to HREE patterns with variably-enriched LREE with the majority showing discrete-negative or no Eu anomalies. All the meta-mafic rocks show that their protoliths were derived from enriched mantle/OIB sources. Characteristically, none of the meta-felsic rocks studied exhibits arc magmatic signatures, while all of them were consistent with the origin of A2-type anorogenic characteristics. Hence, the overall geochemistry of the protolith melts of both meta-mafic and meta-felsic rocks studied here mostly suggests their genesis at an intra-plate extensional setting, contrary to arc-tectonic settting observed in predominant previous studies. Our U-Pb age data correspond to magmatic pulses from ca. 2250 to ca. 550 Ma (ca. 2250–1750 Ma, 1050–850 Ma, 700–627 Ma, and 550–575 Ma) followed by a significant interaction with crustal components at ∼580––530 Ma which is consistent with the escalation of the Th/U and Ce/Ce* values in Zircon. The predominant age peaks match well with both collisional and rifting events associated with the dispersal and amalgamation of global supercratons (e.g. Superia), supercontinents (e.g. Columbia, Rodinia, and Gondwana) and regional micro-continents (e.g. Azania), spanning from early to late global geodynamic history from ca. 2250 to ca. 500 Ma. Hence, this study provides new insights into intra-continental rifting/extensional tectonic settings hitherto-unknown from the inner-central Gondwana.
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来源期刊
Precambrian Research
Precambrian Research 地学-地球科学综合
CiteScore
7.20
自引率
28.90%
发文量
325
审稿时长
12 months
期刊介绍: Precambrian Research publishes studies on all aspects of the early stages of the composition, structure and evolution of the Earth and its planetary neighbours. With a focus on process-oriented and comparative studies, it covers, but is not restricted to, subjects such as: (1) Chemical, biological, biochemical and cosmochemical evolution; the origin of life; the evolution of the oceans and atmosphere; the early fossil record; palaeobiology; (2) Geochronology and isotope and elemental geochemistry; (3) Precambrian mineral deposits; (4) Geophysical aspects of the early Earth and Precambrian terrains; (5) Nature, formation and evolution of the Precambrian lithosphere and mantle including magmatic, depositional, metamorphic and tectonic processes. In addition, the editors particularly welcome integrated process-oriented studies that involve a combination of the above fields and comparative studies that demonstrate the effect of Precambrian evolution on Phanerozoic earth system processes. Regional and localised studies of Precambrian phenomena are considered appropriate only when the detail and quality allow illustration of a wider process, or when significant gaps in basic knowledge of a particular area can be filled.
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