Back to Search Start Over

Two episodes of Eocene mafic magmatism in the southern Lhasa terrane imply an eastward propagation of slab breakoff

Authors :
Wang, Zhenzhen
Zhao, Zhidan
Asimow, Paul D.
Li, Xuping
Meng, Yuanku
Liu, Dong
Mo, Xuanxue
Zhu, Di-Cheng
Tang, Yan
Cong, Fuyun
Source :
Gondwana Research. 110:31-43
Publication Year :
2022
Publisher :
Elsevier BV, 2022.

Abstract

Past geodynamic events can be reconstructed using the spatial and temporal patterns of geochemical variability in igneous rocks. Here we apply this principle to define the timing and geometry of breakoff of the Neo-Tethyan slab after the India-Asia collision. Two episodes of mafic magmatism (∼53 Ma and ∼ 48 Ma) are preserved in the Quxu area of the southern Lhasa terrane (SL). We present their whole-rock geochemistry, zircon U-Pb ages, and in situ zircon Hf isotope ratios. The early gabbro (∼53 Ma) exhibits typical arc basalt characteristics, including enrichment of large-ion lithophile elements (LILEs), depletion of high-field strength elements (HFSEs), and radiogenic Nd and zircon Hf isotopes, implying that they were formed by partial melting of metasomatized lithospheric mantle. In comparison to the early gabbro, the late hornblende gabbro (∼48 Ma) contains higher contents of HFSEs (e.g., Nb, Zr) and relatively less radiogenic Nd and zircon Hf isotopes, suggesting interaction between the enriched sub-continental lithospheric mantle and asthenospheric mantle. It is likely that upwelling asthenosphere reached the central SL around 50 Ma and that the Neo-Tethyan slab tore off under this area at this time. The spatial and temporal distribution of mafic rocks across the whole southern Lhasa terrane show that this geochemical transition and hence, presumably, the tearing off of the Neo-Tethyan slab, propagated eastward along the collision zone throughout Paleocene-Eocene time.

Subjects

Subjects :
Geology

Details

ISSN :
1342937X
Volume :
110
Database :
OpenAIRE
Journal :
Gondwana Research
Accession number :
edsair.doi.dedup.....21b06eeeacaf317696dad1f5456e856c
Full Text :
https://doi.org/10.1016/j.gr.2022.05.019