A Tale of Amalgamation of Three Permo-Triassic Collage Systems in Central Asia: Oroclines, Sutures, and Terminal Accretion

Author:

Xiao Wenjiao123,Windley Brian F.4,Sun Shu1,Li Jiliang1,Huang Baochun5,Han Chunming12,Yuan Chao6,Sun Min7,Chen Hanlin8

Affiliation:

1. State Key Laboratory of Lithospheric Evolution, Institute of Geology and Geophysics and

2. CAS Center for Excellence in Tibetan Plateau Earth Science, Chinese Academy of Sciences, Beijing 100029, China;

3. Xinjiang Institute of Ecology and Geography, Chinese Academy of Sciences, Urumqi 100029, China

4. Department of Geology, University of Leicester, Leicester LE1 7RH, United Kingdom

5. School of Earth and Space Science, Peking University, Beijing 100871, China

6. Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, Guangzhou 510640, China

7. Department of Earth Sciences, University of Hong Kong, Hong Kong, China

8. Department of Earth Sciences, Zhejiang University, Hangzhou 310027, China

Abstract

The Central Asian Orogenic Belt records the accretion and convergence of three collage systems that were finally rotated into two major oroclines. The Mongolia collage system was a long, N–S-oriented composite ribbon that was rotated to its current orientation when the Mongol-Okhotsk orocline was formed. The components of the Kazakhstan collage system were welded together into a long, single composite arc that was bent to form the Kazakhstan orocline. The cratons of Tarim and North China were united and sutured by the Beishan orogen, which terminated with formation of the Solonker suture in northern China. All components of the three collage systems were generated by the Neoproterozoic and were amalgamated in the Permo-Triassic. The Central Asian Orogenic Belt evolved by multiple convergence and accretion of many orogenic components during multiple phases of amalgamation, followed by two phases of orocline rotation.

Publisher

Annual Reviews

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Astronomy and Astrophysics

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