Ji Zheng, Meng Qi-An, Wan Chuan-Biao, Zhu De-Feng, Ge Wen-Chun, Zhang Yan-Long, Yang Hao, Dong Yu, Jing Yan
College of Earth Sciences, Jilin University, Changchun, 130061, China.
Exploration and Development Research Institute, Daqing Oilfield Limited Company, Daqing, 163712, China.
Sci Rep. 2019 Nov 1;9(1):15854. doi: 10.1038/s41598-019-52181-x.
We performed zircon U-Pb age dating and geochemical analyses of late Mesozoic felsic volcanic rocks in the Hailar Basin, NE China, with the aim of eclucidating their emplacement ages, origin and geodynamic significance. The volcanic rocks consist of dacites, rhyolites and rhyolitic tuffs. Laser ablation-inductively coupled plasma-mass spectrometry zircon U-Pb dating results suggest that the rocks were erupted during the Late Jurassic-Early Cretaceous (161-117 Ma). They belong to the high-K calc-alkaline series and can be divided into two groups. Group I rocks are metaluminous to weakly peraluminous, contain low concentrations of heavy rare earth elements (HREEs) and high field strength elements (HFSEs), and have low zircon saturation temperatures (average 786 °C), all of which indicate an I-type affinity. In contrast, Group II rocks have higher HREE and HFSE concentrations and zircon saturation temperatures (average 918 °C), suggesting an A-type affinity. All the felsic volcanic rocks have positive ε(t) values of 1.43-12.32 with two-stage model ages of 1110-401 Ma. Our data indicate that the I-type felsic volcanic rocks formed from magmas generated by partial melting of a dominantly juvenile mica-bearing K-rich basaltic lower crust, whereas the A-type felsic volcanic rocks originated from the partial melting of a dry mafic-intermediate middle-lower crust that was dehydrated but not melt depleted. Based on the present results and previous research, we propose that the Late Jurassic I- and A-type felsic volcanic rocks in the Hailar Basin were formed in a post-collisional environment related to break-off of the subducted oceanic slab of the Mongol-Okhotsk Ocean and the subsequent gravitational collapse of the orogenically-thickened crust after closure of the ocean. In contrast, the Early Cretaceous I- and A-type felsic volcanic rocks were erupted in an extensional setting related to rollback of the subducted Paleo-Pacific Plate.
我们对中国东北海拉尔盆地晚中生代长英质火山岩进行了锆石U-Pb年龄测定和地球化学分析,旨在阐明其就位年龄、成因及地球动力学意义。这些火山岩由英安岩、流纹岩和流纹质凝灰岩组成。激光烧蚀-电感耦合等离子体质谱锆石U-Pb定年结果表明,这些岩石喷发于晚侏罗世-早白垩世(161-117Ma)。它们属于高钾钙碱性系列,可分为两组。第一组岩石为准铝质至弱过铝质,重稀土元素(HREE)和高场强元素(HFSE)含量低,锆石饱和温度低(平均786°C),所有这些都表明其具有I型亲缘性。相比之下,第二组岩石的HREE和HFSE浓度以及锆石饱和温度较高(平均918°C),表明具有A型亲缘性。所有长英质火山岩的ε(t)值为1.43-12.32,两阶段模式年龄为1110-401Ma。我们的数据表明,I型长英质火山岩由主要为新生的含云母富钾玄武质下地壳部分熔融产生的岩浆形成,而A型长英质火山岩起源于脱水但未熔体亏损的干镁铁质-中性中-下地壳的部分熔融。基于目前的结果和先前的研究,我们认为海拉尔盆地晚侏罗世的I型和A型长英质火山岩形成于与蒙古-鄂霍次克洋俯冲洋壳的拆沉以及洋盆闭合后造山增厚地壳的随后重力垮塌相关的碰撞后环境。相比之下,早白垩世的I型和A型长英质火山岩喷发于与古太平洋板块俯冲回撤相关的伸展环境。