Neoproterozoic to Paleozoic long-lived accretionary orogeny in the northern Tarim Craton

被引:314
作者
Ge, Rongfeng [1 ,2 ]
Zhu, Wenbin [1 ]
Wilde, Simon A. [2 ]
He, Jingwen [1 ]
Cui, Xiang [1 ]
Wang, Xi [1 ]
Zheng Bihai [1 ]
机构
[1] Nanjing Univ, State Key Lab Mineral Deposits Res, Sch Earth Sci & Engn, Nanjing 210008, Jiangsu, Peoples R China
[2] Curtin Univ, Dept Appl Geol, Perth, WA 6845, Australia
关键词
zircon isotopic data; granitoids; accretionary orogens; Tarim Craton; ZIRCON U-PB; NW CHINA CONSTRAINTS; A-TYPE GRANITES; NORTHWEST CHINA; TECTONIC EVOLUTION; VOLCANIC-ROCKS; GEOCHEMICAL CHARACTERISTICS; PRECAMBRIAN EVOLUTION; NORTHEASTERN MARGIN; CARBONATITE COMPLEX;
D O I
10.1002/2013TC003501
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The Tarim Craton, located in the center of Asia, was involved in the assembly and breakup of the Rodinia supercontinent during the Neoproterozoic and the subduction-accretion of the Central Asian Orogenic Belt (CAOB) during the Paleozoic. However, its tectonic evolution during these events is controversial, and a link between the Neoproterozoic and Paleozoic tectonic processes is missing. Here we present zircon U-Pb ages, Hf isotopes, and whole-rock geochemical data for the extensive granitoids in the western Kuruktag area, northeastern Tarim Craton. Three distinct periods of granitoid magmatism are evident: circa 830-820Ma, 660-630Ma, and 420-400Ma. The magma sources, melting conditions (pressure, temperature, and water availability), and tectonic settings of various granitoids from each period are determined. Based on our results and the geological, geochronological, geochemical, and isotopic data from adjacent areas, a long-lived accretionary orogenic model is proposed. This model involves an early phase (circa 950-780Ma) of southward advancing accretion from the Tianshan to northern Tarim and a late phase (circa 780-600Ma) of northward retreating accretion, followed by back-arc opening and subsequent bidirectional subduction (circa 460-400Ma) of a composite back-arc basin (i.e., the South Tianshan Ocean). Our model highlights a long-lived accretionary history of the southwestern CAOB, which may have initiated as part of the circum-Rodinia subduction zone and was comparable with events occurring at the southern margin of the Siberian Craton, thus challenging the traditional southward migrating accretionary models for the CAOB.
引用
收藏
页码:302 / 329
页数:28
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