Abstract
Granitoids and coeval mafic microgranular enclaves (MMEs) provide important insights into petrogenesis and crustal evolution. In the eastern sector of the East Kunlun Orogen, the Halazha (HLZ) pluton contains abundant MMEs, recording magma mingling processes. The HLZ pluton comprises quartz diorites and granodiorites, whereas the MMEs have a gabbroic-dioritic composition. This paper provides a detailed description of the petrography and mineralogy of the HLZ pluton and MMEs, and presents new ages and geochemical data. The zircon UâPb dating results indicate that quartz diorites and granodiorites are ranging from 243âŻÂ±âŻ2âŻMa to 244.8âŻÂ±âŻ1.3âŻMa and from 233.3âŻÂ±âŻ1.1âŻMa to 233.6âŻÂ±âŻ1.5âŻMa, respectively. The zircon ages of the coeval MMEs are identical to the host rocks, i.e., 244.5âŻÂ±âŻ1.1âŻMaâŻââŻ244.5âŻÂ±âŻ1.2âŻMa, and 233.7âŻÂ±âŻ1.3âŻMa, respectively. Both quartz diorites and granodiorites contain hornblende, display metaluminous characteristics with average A/CNK values of 0.93 and 0.99, respectively, and thus belong to I-type granite. Both of them are enriched in large-ion lithophile elements such as Rb and Ba and depleted in high-field-strength elements such as Nb and Ta. In addition, they both have low ΔHf(t) values, ranging from â5.6 to â1.7 and â5.4 to â1.79, respectively. Results suggest that HLZ pluton is derived from magmas formed by the partially melting juvenile mafic lower crust. Quartz diorites experienced hornblende accumulation for its low SiO2 contents. Whereas, the high Sr/Y ratio of granodiorites attributes to the fractional crystallization of apatite. Notably, the crystallization pressure and temperature (average 3.43 kbar and 764âŻÂ°C) of the hornblende xenocrysts in MMEs is close to it of the hornblende phenocryst in quartz diorite (average 3.68 kbar and 766âŻÂ°C). This similarity indicates that MMEs in the quartz diorites resulted from magmatic mingling between the mafic magma and the host rock within the deep crust. The hornblende xenocrysts present in MMEs of the granodiorites contain a higher number of inclusions, reveal higher crystallization pressures (average 2.73 kbar) and temperatures (average 825âŻÂ°C) compared to their host rocks (average 1.35 kbar and 702âŻÂ°C). These results suggest that MMEs in granodiorites underwent two distinct magmatic mixing processes: the magmatic mixing of mafic magma in the deep crust and then during the upwelling process after this mixed mafic magma entered the granodiorites.
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