Neoproterozoic bimodal magmatism in the eastern Himalayan orogen: Tectonic implications for the Rodinia supercontinent evolution
Graphical abstract
Introduction
The global Neoproterozoic magmatism is commonly related to the assembly, configuration, and breakup of the Rodinia supercontinent and has evoked geoscientific attention regarding its petrogenesis and tectonic settings (Heaman et al., 1992; Li et al., 1999, Li et al., 2002, Li et al., 2006, Li et al., 2008, Li et al., 2013; Wang et al., 2009, Wang et al., 2018; Bybee et al., 2010; Spencer et al., 2013; Cawood et al., 2018). The evidences of Neoproterozoic magmatism have been reported from several continental fragments, such as South China (e.g., Li et al., 1999, Li et al., 2002, Li et al., 2003, Li et al., 2008, Li et al., 2010; Cawood et al., 2013; Zhao et al., 2013; Liu et al., 2020), India (e.g., Bhushan, 2000; Gyani et al., 2001; Gregory et al., 2009; Santosh et al., 2012, Santosh et al., 2014, Santosh et al., 2017; Ashwal et al., 2013; He et al., 2016; Wang et al., 2018; Zhao et al., 2018; Yang et al., 2020), Seychelles (e.g., Torsvik et al., 2001; Tucker et al., 2001; Ashwal et al., 2002; Hammond et al., 2013), Madagascar (e.g., Nédélec et al., 1995, Nédélec et al., 2016; Handke et al., 1999; Bybee et al., 2010; Boger et al., 2014; Zhou et al., 2015), Lhasa (e.g., Zhang et al., 2012a, Zhang et al., 2012b; Hu et al., 2018a, Hu et al., 2018b, Hu et al., 2018c; Dong et al., 2020), Tarim (e.g., Xu et al., 2005, Xu et al., 2013; He et al., 2012; Zhang et al., 2012c, 2016; Wu et al., 2017; Wen et al., 2019), Australia (e.g., Michael et al., 1998; Li et al., 2006; Huang et al., 2015), Pakistan (e.g., Khan et al., 2012; Ahmad et al., 2013; Qasim et al., 2018), and Laurentia (e.g., Goodge and Vervoort, 2006; Goodge et al., 2017; Cawood and Pisarevsky, 2017). However, the paleogeographic settings of diffenent terranes are still controversial. This caused long debates about the petrogenesis and tectonic settings of Neoproterozoic magmatism from diffenent terranes. As has been stated in previous studies, most of the Neoproterozoic magmatic events are attributed to mantle plumes or a mantle superplume that caused the rifting and fragmentation of the Neoproterozoic Rodinia supercontinent (e.g., Heaman et al., 1992; Park et al., 1995; Shellnutt et al., 2004; Maruyama et al., 2007; Li et al., 1999, Li et al., 2002, Li et al., 2006, Li et al., 2008, Li et al., 2013; Cui et al., 2015; Lyu et al., 2017; Zhang et al., 2017a; Zhu et al., 2018). However, a few other studies have suggested that the Neoproterozoic magmas from northwestern India, Madagascar, Seychelles, and Tarim were formed in a continental arc setting, pointing to active Andean-type orogeny on the northwestern margin of the Rodinia supercontinent (e.g., Torsvik et al., 1996; Tucker et al., 2001; Rino et al., 2008; Gregory et al., 2009; Bybee et al., 2010; He et al., 2012; Tang et al., 2016; Ding and Zhang, 2016; Liao et al., 2017; Wu et al., 2017; Wang et al., 2018; Zhao et al., 2018). Although this debate has not been well resolved so far, there is no doubt that studies on the origin and geodynamics of Neoproterozoic magmas will contribute to our understanding of the Rodinia supercontinent evolution.
Thus far, only a few studies have focused on the Neoproterozoic granitoids from the eastern Himalayan orogeny (Ding and Zhang, 2016; Wang et al., 2017a), and no coeval mafic rocks have been reported elsewhere. Moreover, the origin and geodynamics of these Neoproterozoic granitoids remain controversial. Ding and Zhang (2016) proposed that these granitoids display arc geochemical features, indicating that an Andean-type orogen may have existed along the northwestern margin of the Rodinia supercontinent. In contrast, Wang et al. (2017a) suggested that these Neoproterozoic granitoids are derived from the melting of ancient crustal rocks, possibly due to the breakup of the Rodinia supercontinent associated with episodic plume events. This contradiction is attributed to the lack of coeval mafic rock constraints, limiting the comprehensive understanding of the Neoproterozoic magmas in the eastern Himalayan orogen. Herein, we present new geochronological and geochemical data for the Neoproterozoic bimodal magmatism from the eastern Himalayan orogen (Fig. 1). In addition, we reanalyzed previously published results and revisited the petrogenesis of the Neoproterozoic bimodal magmatic rocks in the eastern Himalayan orogen to construct a new geodynamic model, propose the formation mechanism of these Neoproterozoic bimodal magmas, and correlate them with the geological evolution of the Rodinia supercontinent. We anticipate that this study can provide key clues for Neoproterozoic tectonothermal evolution of the India-Himalayan terrane in the northwestern Rodinia supercontinent.
Section snippets
Geological setting
As one of the largest collisional orogens in Earth history, the Himalayan orogenic belt consists of three parallel east-west-striking tectonic units, including the Lesser Himalayan Sequence (LHS), Greater Himalayan Crystalline Sequence (GHS), and Tethys Himalayan Sequence (THS), separated by the Main Boundary Thrust (MBT), Main Central Thrust (MCT), and South Tibetan Detachment System (STDS), respectively (Fig. 1A).
The THS zone extends in an east-west direction for more than 1300 km and is
Whole rock major and trace elements
Five fresh amphibolite samples and eleven fresh granitic gneiss samples were collected from outcrops. All the samples were analyzed for major and trace elements at the Analytical Laboratory Beijing Research Institute of Uranium Geology. Major element analyses were completed using a Philips PW2404 XRF with a precision of less than ±1%. Trace elements were determined using a Finnigan MAT Element XR ICP-MS. The uncertainties of the ICP-MS analyses are estimated to be better than ±5% for most trace
Zircon UPb ages
The results of zircon UPb testing are presented in Supplementary Table S1. The zircons from sample CNDXCJ (amphibolite) are euhedral to subhedral and approximately 40–150-μm long and 35–100-μm wide, with length to width ratios of 2:1 to 1:1 (Fig. 4A). Most of the Th/U ratios (0.46–1.94) are >0.1, indicating magmatic crystallization (Wu and Zheng, 2004). It is noteworthy that Most of these zircons have no clear oscillatory zoning and show core–rim structure in Cathodoluminescence (CL) images (
Rock metamorphism and alteration
Both the granitic gneiss and amphibolite samples reveal low loss-on-ignition (LOI) values (0.29–1.06). However, the petrographic investigations indicate that though these rocks have undergone various degrees of metamorphism and alteration, they still preserved igneous textures. Thus, the alkali elements and LILEs may have been modified by the metamorphic and alteration processes (Verma, 1981; Hart and Staudigel, 1982). However, REEs, HFSEs, V, Cr, and Ni are considered immobile and are likely
Conclusions
The new data presented herein and combined with previous studies allow for a better understanding of the petrogenesis of the Neoproterozoic bimodal magmatism in the eastern Himalayan orogen. Our key conclusions are as follows:
- (1)
The in situ zircon UPb dating reveal that the protoliths of amphibolites were emplaced at Ca. 826 Ma and the granitoids have crystallization ages of 825–820 Ma. An extensive Neoproterozoic magmatic rock belt likely existed in the eastern Himalayan orogeny.
- (2)
The granitic
Declaration of Competing Interest
The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.
Acknowledgements
This research was supported by National Natural Science Foundation of China (grant 41702080, 91955208), the National Key R&D Program of China (grants 2018YFC0604103, 2016YFC0600308) and the China Geological Survey (grant DD20190147). We are deeply grateful to the anonymous reviewers for constructive suggestions.
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2022, Earth-Science ReviewsCitation Excerpt :The Himalayas are bordered from east to west by the syntaxial massifs—the Namche Barwa massif in the east (Eastern Himalayan Syntaxis) and the Nanga Parbat massif in the west (Western Himalayan Syntaxis) (Guevara et al., 2022). Multiple stages of magmatism are recognized from the available data in the Himalayan orogenic belt: Paleoproterozoic (1900–1700 Ma; Imayama et al., 2019), Neoproterozoic (1000–800 Ma; Zhang et al., 2021), early Paleozoic (520–460 Ma; Zhang et al., 2019a), Permian (290–260 Ma; Tian et al., 2021), late Triassic (240–210 Ma; Huang et al., 2018), late Jurassic–early Cretaceous (150–120 Ma; Chen et al., 2021a) and Cenozoic (45–1 Ma; Burg and Bouilhol, 2019). Among these, the magmatic rocks emplaced during the Proterozoic and early Paleozoic underwent Cenozoic intermediate- to high-grade metamorphism to form orthogneiss and are mainly exposed in the LHS and GHC.