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Understanding the genesis of ore-bearing and ore-barren adakitic rocks: insights from geochronology and geochemical analysis of the Tuncang intrusion and enclaves along the South Tan-Lu Fault.

Authors :
Zi, Feng
Xiao, Wenzhou
Sami, Mabrouk
Zhang, Chenguang
Xie, Fenquan
Liu, Ye
Li, Shuanglian
Source :
International Journal of Earth Sciences; Oct2024, Vol. 113 Issue 7, p1579-1598, 20p
Publication Year :
2024

Abstract

The relationships between metallogenic capacity and geochemical features of adakitic rocks along the South Tan-Lu Fault (STLF) remain unclear. In this study, the ore-barren adakitic rocks (Tuncang, Guandian and Wawuliu) exhibit higher K<subscript>2</subscript>O/Na<subscript>2</subscript>O ratios and lower Sr/Y ratios than the ore-bearing adakitic rocks (Chuzhou and Shangyaopu). These differences strongly suggest that the ore-barren adakitic rocks originated from the thickened lower continental crust (LCC), whereas the ore-bearing adakitic rocks were derived from oceanic slabs. Notably, the Tuncang granite exhibits higher Y/Yb and (Ho/Yb)<subscript>N</subscript> ratios than the Guandian granodiorite and Wawuliu intrusion. Accordingly, we suggest that the Tuncang granite likely originated from a delaminated eclogitic LCC, whereas the Guandian and Wawuliu intrusions were derived from a thickened basaltic LCC sources. The occurrence of diorite and gabbro mafic microgranular enclaves (MMEs) within the Tuncang granite strongly suggests a magma-mixing process. Considering their MgO contents and εNd(t) and (<superscript>87</superscript>Sr/<superscript>86</superscript>Sr)<subscript>i</subscript> values, we suggest that the gabbro MMEs were likely derived from an enriched mantle source previously metasomatized by subduction-related components and that the diorite MMEs were subsequently formed by magma mixing. Due to the slightly younger ages of the ore-bearing adakitic rocks, we propose a model in which the ore-barren adakitic rocks formed through LCC delamination at 130 Ma and the ore-bearing adakitic rocks formed through oceanic slab remelting at 125 Ma. Consequently, the exploration of Cu–Au mineralization along the STLF should focus on younger oceanic slab-derived adakitic rocks. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
14373254
Volume :
113
Issue :
7
Database :
Complementary Index
Journal :
International Journal of Earth Sciences
Publication Type :
Academic Journal
Accession number :
180733341
Full Text :
https://doi.org/10.1007/s00531-024-02465-z