Elsevier

Gondwana Research

Volume 111, November 2022, Pages 53-63
Gondwana Research

In-situ mineralogical interpretation of the mantle geophysical signature of the Gangdese Cu-porphyry mineral system

https://doi.org/10.1016/j.gr.2022.07.005Get rights and content

Highlights

  • The phlogopites in Bairong lamprophyres reveal asthenospheric components.

  • The asthenosphere upwelling is the main mechanism for heat and material exchange.

  • The mafic magmas expelled volatiles and metals to form ore-bearing magmas.

Abstract

The lithosphere provides a reservoir for ore-forming elements introduced by repeated fertilisation during asthenosphere-lithosphere interaction by the slab subduction. Here we use the Gangdese copper metallogenic belt to show how mineralogical study can help to interpret these mantle signatures. We present insights into the in-situ geochronological, geochemical and whole-rock isotopic analyses of minerals from mantle-derived lamprophyres that intruded the Bairong Cu-porphyry deposit in the Gangdese metallogenic belt. Zircon U-Pb dating yields weighted-mean concordant 206Pb/238U ages of 11.69 ± 0.27 Ma to 12.41 ± 0.83 Ma. These zircons show juvenile εHf (t) (+1.0 ∼ +10.9) and low δ18O (5.5‰ ∼ 7.7‰) values. Variable initial 87Sr/86Sr ratios (0.7073–0.7080), εNd(t) values (−6.3 ∼ −5.0) and initial 187Os/188Os ratios (0.1382–0.1591) suggest hybridization between lithosphere mantle and asthenospheric melts. Phlogopites in the lamprophyres reflect partial dissolution and incipient melting with low Mg# values but high Al2O3 contents in core. And these phlogopites are surrounded by a zone with high Mg# values. We interpret this as superheating and hybridization of refractory lithosphere mantle and asthenosphere. The 3-D magnetotelluric and seismic signature of the Gangdese mineral belt reflect a mantle source region comprising asthenosphere, old refractory lithosphere, ponded mafic melts near the crust-mantle boundary, and higher-level magma chambers where more extensive mixing between crust- and mantle-derived melts occurs. The asthenospheric upwelling provides a mechanism for heat transfer and the expulsion of volatile elements. It is generating a new young, fertile lithosphere beneath the southeast Lhasa block, which has driven the mineralization processes in the Gangdese metallogenic belt.

Introduction

Most of the continental lithosphere formed in the Archaean eon (e.g, Griffin et al., 2009) and provides stability to Earth’s surface, which is critical for maintaining habitability. While providing stable continental blocks, the continental lithosphere is reshaped during tectonic processes by chemical and physical modification. This cratonic lithosphere may also provide a long-term stable reservoir for ore-forming elements introduced by repeated fertilization (e.g., Griffin et al., 2013, Tassara et al., 2017). Hence, this fertilization, and the exchange of mass and heat between asthenosphere and lithosphere, may be a major factor in the generation of large ore systems (e.g., Holwell, et al., 2019). Here we examine this exchange within the lithosphere beneath a major Miocene Cu-Au porphyry metallogenic belt in a continental-collision environment in the Lhasa block of southern Tibet.

The Lhasa block, situated at the front of the India-Asia collisional belt, is a good place to explore the exchange of mass and heat during continental convergence (e.g., Zhu et al., 2011). Recent geophysical observations have identified contrasts in the present-day thermal regime from west to east in the Lhasa block using seismic tomography (e.g., Liang et al., 2016), seismic anisotropy (Chen et al., 2015a, Chen et al., 2015b) and magnetotelluric (MT) methods (Wang et al., 2017). The geophysical signature of the Gangdese metallogenic system comprises significant low velocity zones, large time lags (1.0–2.0 s) of shear-wave splitting (SKS) travel-time residuals, and a deep conductor in the eastern part.

Lamprophyres and related ultra-potassic rocks (UPRs) occur over much of the Lhasa block (Li et al., 2020, Li et al., 2021). They represent low-volume melts, and carry vital information on the state of the continental root at the time of major mineralization (Fig. 1, e.g., Zhao et al., 2009, Huang et al., 2015). These erupted and/or injected mafic magmas also provide an opportunity to study the enrichment processes and the compositionally heterogeneous mantle sources associated with the generation of these unusual magmas (e.g., Tappe et al., 2005). Several studies of UPRs have indicated the involvement of a subcontinental lithospheric mantle (SCLM) with radiogenic Rb-Sr and Lu-Hf isotopes and unradiogenic Sm-Nd isotopes beneath the western part of the Lhasa block (Zhao et al., 2009). In this study, we use mantle-derived mafic lamprophyres in the Bairong porphyry deposit in the southeastern part of the Lhasa block (Fig. 1) to provide temporal constraints on the thermal and chemical evolution of the continental lithosphere to identify the mechanisms reflected in the geophysical signature of the mineralization of the Gangdese belt.

Section snippets

Geological setting and samples

The Lhasa continental fragment is a Precambrian block (e.g., Zhu et al., 2011), that rifted from eastern Gondwana and moved across the Tethyan Ocean during the early Mesozoic (e.g., Yin and Harrison, 2000). The long-term subduction of Neo-Tethyan slabs beneath the Lhasa block built juvenile magmatic arcs on this older core (e.g., Zhu et al., 2011). After the closure of the Neo-Tethyan Ocean, a nearly east–west belt of Miocene UPRs, as well as a coeval world-class porphyry Cu-Mo metallogenic

Geophysical observations

Recent magnetotelluric (MT) data reveal the 3-D electrical structure of the lithosphere across southern Tibet. The inversion found an electrically conductive body beneath the Bairong area (89°-90°), with a lower boundary at depths of approximately 80 km. This lower boundary has been interpreted as reflecting increasing temperature induced by asthenospheric upwelling (Wang et al., 2017). The difference in mantle composition and thermal state beneath the southeastern parts of the UPR belt is also

Petrography and mineral chemistry

The Bairong lamprophyres are porphyritic, with phlogopite (∼10 vol%), amphibole (∼7 vol%) and diopside (∼3 vol%) phenocrysts. The fine-grained groundmass is comprised of phlogopite, amphibole, K-feldspar, zircon and titanomagnetite. Phlogopite is ubiquitous in the lamprophyres and shows large textural and compositional variations (Table DR2). Three textural types can be found. 1) Phl-A: tabular euhedral phenocrysts with inclusion-free cores and rims containing inclusions of groundmass phases

Effects of crustal assimilation

Based on geochemical classifications, the Bairong mafic rocks can be characterized as primitive lamprophyres with a mantle origin. In the framework of southern Tibet, the geochemical features of the Bairong lamprophyres distinguish them from UPRs in the western part, which are proposed to reflect interactions of K-rich magmas with the continental crust of the Lhasa block (Liu et al., 2015). The isotopic compositions are more sensitive than trace elements to the assimilation of distinct

Conclusions

The Bairong lamprophyres have distinct phlogopite compositions and Sr-Nd-Os-Hf-O isotopic characteristics, revealing the presence of asthenospheric components. They are most plausibly derived from a mixed mantle source region composed of asthenosphere and preexisting lithosphere. The upwelling of asthenospheric mantle is the main mechanism for the exchange of heat and material involved in the generation of young and fertile lithosphere beneath the southeast Lhasa block. The mafic magmas

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 funded by National Key Technologies R&D Program 2020YFA0714804, 2019YFA0708602; National Natural Science Foundation of China (42073038, 41803045), Young Talent Support Project of CAST, the Fundamental Research Funds for the Central Universities (Grant no. 265QZ2021012), and IGCP-662. We thank the editor Santosh Madhava W. and another two anonymous reviewers, which helped in improving our paper. This is the 7th contribution of BX for National Mineral Rock and Fossil Specimens

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