Origin of the early Permian Wajilitag igneous complex and associated Fe-Ti oxide mineralization in the Tarim large igneous province, NW China

被引:38
作者
Cao, Jun [1 ,3 ]
Wang, Christina Yan [2 ]
Xing, Chang-Ming [2 ,3 ]
Xu, Yi-Gang [1 ]
机构
[1] Chinese Acad Sci, Guangzhou Inst Geochem, State Key Lab Isotope Geochem, Guangzhou 510640, Guangdong, Peoples R China
[2] Chinese Acad Sci, Guangzhou Inst Geochem, CAS Key Lab Mineral & Metallogeny, Guangzhou 510640, Guangdong, Peoples R China
[3] Univ Chinese Acad Sci, Beijing 100049, Peoples R China
关键词
Layered mafic-ultramafic intrusion; Syenitic pluton; Fe-Ti oxides; Wajilitag; Tarim large igneous province; PB ZIRCON GEOCHRONOLOGY; A-TYPE GRANITOIDS; BUSHVELD COMPLEX; LIQUID IMMISCIBILITY; MAGNETITE LAYERS; PANXI DISTRICT; HOST ROCKS; SW CHINA; GEOCHEMISTRY; BASIN;
D O I
10.1016/j.jseaes.2013.09.014
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The Wajilitag igneous complex is part of the early Permian Tarim large igneous province in NW China, and is composed of a layered mafic-ultramafic intrusion and associated syenitic plutons. In order to better constrain its origin, and the conditions of associated Fe-Ti oxide mineralization, we carried out an integrated study of mineralogical, geochemical and Sr-Nd-Hf isotopic analyses on selected samples. The Wajilitag igneous rocks have an OIB-like compositional affinity, similar to the coeval mafic dykes in the Bachu region. The layered intrusion consists of olivine clinopyroxenite, coarse-grained clinopyroxenite, fine-grained clinopyroxenite and gabbro from the base upwards. Fe-Ti oxide ores are mainly hosted in fine-grained clinopyroxenite. Forsterite contents in olivines from the olivine clinopyroxenite range from 71 to 76 mol%, indicating crystallization from an evolved magma. Reconstructed composition of the parental magma of the layered intrusion is Fe-Ti-rich, similar to that of the Bachu mafic dykes. Syenite and quartz syenite plutons have epsilon(Nd)(t) values ranging from +1.4 to +2.9, identical to that for the layered intrusion. They may have formed by differentiation of underplated magmas at depth and subsequent fractional crystallization. Magnetites enclosed in olivines and clinopyroxenes have Cr2O3 contents higher than those interstitial to silicates in the layered intrusion. This suggests that the Cr-rich magnetite is an early crystallized phase, whereas interstitial magnetite may have accumulated from evolved Fe-Ti-rich melts that percolated through a crystal mush. Low V content in Cr-poor magnetite (< 6600 ppm), is consistent with an estimate of oxygen fugacity of FMQ + 1.1 to FMQ + 3.5. We propose that accumulation of Fe-Ti oxides during the late stage of magmatic differentiation may have followed crystallization of Fe-Ti-melt under high fO(2) and a volatile-rich condition. (C) 2013 Elsevier Ltd. All rights reserved.
引用
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页码:51 / 68
页数:18
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