Reassessment of continental growth during the accretionary history of the Central Asian Orogenic Belt

被引:798
|
作者
Kroener, A. [1 ,2 ]
Kovach, V. [3 ]
Belousova, E. [4 ]
Hegner, E. [5 ]
Armstrong, R. [6 ]
Dolgopolova, A. [6 ]
Seltmann, R. [6 ]
Alexeiev, D. V. [7 ]
Hoffmann, J. E. [8 ]
Wong, J. [9 ]
Sun, M. [9 ]
Cai, K. [9 ]
Wang, T. [10 ]
Tong, Y. [10 ]
Wilde, S. A. [11 ]
Degtyarev, K. E. [7 ]
Rytsk, E. [3 ]
机构
[1] Chinese Acad Geol Sci, Beijing SHRIMP Ctr, Beijing, Peoples R China
[2] Johannes Gutenberg Univ Mainz, Dept Geosci, Mainz, Germany
[3] Russian Acad Sci, Inst Precambrian Geol & Geochronol, St Petersburg, Russia
[4] Macquarie Univ, Dept Earth & Planetary Sci, Australian Res Council Ctr Excellence Core Crust, Sydney, NSW 2109, Australia
[5] Univ Munich, Dept Geo & Environm Sci, D-81377 Munich, Germany
[6] Nat Hist Museum, Dept Earth Sci, CERCAMS, London SW7 5BD, England
[7] Russian Acad Sci, Inst Geol, Moscow V71, Russia
[8] Univ Cologne, Dept Geol & Mineral, Cologne, Germany
[9] Univ Hong Kong, Dept Earth Sci, Hong Kong, Hong Kong, Peoples R China
[10] Chinese Acad Geol Sci, Inst Geol, Beijing, Peoples R China
[11] Curtin Univ Technol, Dept Appl Geol, Inst Geosci Res, Perth, WA 6845, Australia
基金
俄罗斯基础研究基金会;
关键词
Central Asian Orogenic Belt; Nd-Hf isotopes; Crustal growth; Crustal reworking; Juvenile crust; ZIRCON U-PB; EARLY CALEDONIAN SUPERTERRANE; PHANEROZOIC CRUSTAL GROWTH; PALEOASIAN OCEAN FORMATION; HF ISOTOPIC CONSTRAINTS; LARGE IGNEOUS PROVINCE; TUVA-MONGOLIA MASSIF; ISLAND-ARC SYSTEM; ND-SR ISOTOPES; SM-ND;
D O I
10.1016/j.gr.2012.12.023
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We argue that the production of mantle-derived or juvenile continental crust during the accretionary history of the Central Asian Orogenic Belt (CAOB) has been grossly overestimated. This is because previous assessments only considered the Palaeozoic evolution of the belt, whereas its accretionary history already began in the latest Mesoproterozoic. Furthermore, much of the juvenile growth in Central Asia occurred in late Permian and Mesozoic times, after completion of CAOB evolution, and perhaps related to major plume activity. We demonstrate from zircon ages and Nd-Hf isotopic systematics from selected terranes within the CAOB that many Neoproterozoic to Palaeozoic granitoids in the accreted terranes of the belt are derived from melting of heterogeneous Precambrian crust or through mixing of old continental crust with juvenile or short-lived material, most likely in continental arc settings. At the same time, juvenile growth in the CAOB occurred during the latest Neoproterozoic to Palaeozoic in oceanic island arc settings and during accretion of oceanic, island arc, and Precambrian terranes. However, taking together, our data do not support unusually high crust-production rates during evolution of the CAOB. Significant variations in zircon epsilon(Hf) values at a given magmatic age suggest that granitoid magmas were assembled from small batches of melt that seem to mirror the isotopic characteristics of compositionally and chronologically heterogeneous crustal sources. We reiterate that the chemical characteristics of crustally-derived granitoids are inherited from their source(s) and cannot be used to reconstruct tectonic settings, and thus many tectonic models solely based on chemical data may need re-evaluation. Crustal evolution in the CAOB involved both juvenile material and abundant reworking of older crust with varying proportions throughout its accretionary history, and we see many similarities with the evolution of the SW Pacific and the Tasmanides of eastern Australia. (C) 2013 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved.
引用
收藏
页码:103 / 125
页数:23
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