Volume 93, Issue S2 pp. 120-121
2 Earth System Science
Free Access

Accreted Terranes in the Paleo-Asian Ocean

Gaoxue YANG

Corresponding Author

Gaoxue YANG

School of Earth Science & Resources, Chang'an University, Xi'an, Shaanxi 710054 China

Ministry of Education, Key Laboratory of Western China's Mineral Resources and Geological Engineering Xi'an, Shaanxi 710054 China

Corresponding author. E-mail: [email protected]Search for more papers by this author
Yongjun LI

Yongjun LI

School of Earth Science & Resources, Chang'an University, Xi'an, Shaanxi 710054 China

Ministry of Education, Key Laboratory of Western China's Mineral Resources and Geological Engineering Xi'an, Shaanxi 710054 China

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Lili TONG

Lili TONG

School of Earth Science & Resources, Chang'an University, Xi'an, Shaanxi 710054 China

Ministry of Education, Key Laboratory of Western China's Mineral Resources and Geological Engineering Xi'an, Shaanxi 710054 China

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Zuopeng WANG

Zuopeng WANG

School of Earth Science & Resources, Chang'an University, Xi'an, Shaanxi 710054 China

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Fenghao DUAN

Fenghao DUAN

School of Earth Science & Resources, Chang'an University, Xi'an, Shaanxi 710054 China

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First published: 31 May 2019

Abstract

Terrane accretion is considered to be one of the main contributors to the growth of continental crust (Stern and Scholl, 2010). Allochthonous terranes can be categorized into three general groups, including island arcs, seamounts (oceanic plateaus, submarine ridges), and continental fragments. The Central Asian Orogenic Belt (CAOB) is one of the largest and long-lived accretionary collages on the globe, and is composed of numerous island arcs, and accretionary wedges, seamounts, and microcontinents associated with the growth and consumption of the Paleo-Asian Ocean (Fig.1; Şengör et al., 1993; Windley et al., 2007; Xiao et al., 2015; Yang et al., 2015).

 

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