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a Simplified geological map showing location of Liaodong Peninsula and study area in the North China Craton; b Geological map of the Gudaoling batholith in the Liaodong Peninsula and c Mafic microgranular enclaves occurring within monzogranite. The pen in c is 14 cm long  

a Simplified geological map showing location of Liaodong Peninsula and study area in the North China Craton; b Geological map of the Gudaoling batholith in the Liaodong Peninsula and c Mafic microgranular enclaves occurring within monzogranite. The pen in c is 14 cm long  

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In situ zircon U–Pb and Hf-isotopic data have been determined for mafic microgranular enclaves and host granitoids from the Early Cretaceous Gudaoling batholith in the Liaodong Peninsula, NE China, in order to constrain the sources and petrogenesis of granites. The zircon U–Pb age of the enclaves (120 ± 1 Ma) is identical to that of the host monzog...

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... The geodynamic evolution of granites remains a subject of debate, and many studies have been conducted to understand the origin of different granitic rock types. Several petrogenetic schemes have been reconstructed to explain the origin of granites, including the following: (1) dehydration melting of tonalite-granodiorte rocks [52]; (2) fractional crystallization of basaltic magma that is derived from the mantle [53]; (3) partial melting of the residual sources after I-type granite extraction [33]; (4) low-pressure melting of the calc-alkaline magmas at the upper crust [54]; and (5) hybridization of the mantle-derived magmas with those of crustal melts [55]. ...
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... Numerous studies have inferred that MMEs result from the mixing of mafic and silicic magmas, based on their fine-grained texture and the absence of cumulate texture. These studies have argued that magma mixing is an essential mechanism for granite formation (Kazemi et al., 2019;Yang et al., 2007). However, other studies have demonstrated that Table S8. ...
... The MMEs are ubiquitous in felsic plutons as isolated inclusions or 'enclave swarms' (Rodríguez and Castro, 2018). Several models have been proposed for the origin of MMEs, including refractory solid restites (Chappell and Wyborn, 2012), xenoliths from country rocks (Watson and Jurewicz, 1984), mafic blobs resulting from magma mixing of magmas with different compositions (Yang et al., 2007), and autoliths (Chen et al., 2021a;Zhang et al., 2023). The mineral assemblage of MMEs is similar to that of the host granitoids (Fig. 2), and they have identical crystallisation ages and zircon REEs pattern (Fig. 7c, d) as well as overlapping Sr-Nd-Hf isotopic compositions, which rule out the possibility that the MMEs are restites or xenoliths. ...
... Moreover, in situ zircon Hf isotopes can elucidate the role of magma mixing processes in the generation of granitoids, if such processes take place. The MMEs generated by the mixing of mantle-derived mafic magmas with crustal-derived felsic magmas should have distinct Hf isotopes with host granites (e.g., Yang et al., 2007). However, Qingshan MMEs have indistinguishable zircon Hf isotopes with Qingshan granodiorite, indicating a cognate origin. ...
... The zircon grains from the coarse-grained and medium-to fine-grained monzodiorite samples had similar initial 176 Hf/ 177 Hf ratios ranging from 0.282329 to 0.282401, with corresponding initial ε Hf (t) values restricted to −13.4 to −10.9 (−12.2 ± 0.6 on average, 1σ, n = 52). These values are comparable to those of coeval enriched lithospheric mantle-derived mafic intrusions from the North China Craton (−11.7 ± 2.6 on average) but are distinct from those of coeval asthenospheric mantle-and ancient lower crust-derived magmas from the North China Craton (0.5 ± 1.8 and −22.2 ± 2.3 on average, respectively; Fig. 13; Wu et al., 2005b;Yang et al., 2007aYang et al., , 2007bZhang et al., 2010;Ma et al., 2014aMa et al., , 2014b. ...
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... 18,48 Generally, MMEs formed from mixing between a mantle-derived mafic and a crust-derived felsic magma should exhibit distinct chemical and isotopic compositions from their host rocks. 60,61 However, the MMEs in the Triassic EKOB granites, including the Yuegelu MMEs, have similar mineral assemblages (with variations in mineral proportions) and isotopic characteristics as the host rocks (Figures 2 and 8). 3,12,13,16,20,62 Some researchers have attributed the isotopic similarity between the MMEs and the host granites to the isotopic equilibrium during the magma mixing process. ...
... In general, zircon crystallizes early and preserves the initial isotopic information on the magmas, preventing the isotope composition from being altered by the subsequent magmatic processes (such as magma mixing). 17,61 The Yuegelu MMEs share similar zircon Hf isotopic compositions (ε Hf (t) = −1.7 to +1.4) as the host rocks (ε Hf (t) = −1.8 to +1.0) (Figure 8b, Table S7), which implies their close connections in the magma source rather than the isotopic equilibration during magma mixing. 20,67 Moreover, the distinct boundary between the MMEs and the host rocks (Figure 2a,b) also indicates that no chemical equilibrium was reached during the formation of the Yuegelu MMEs. ...
... In the MgO and Mg# vs. SiO 2 diagrams, the biotite granodiorites plot in the area of experimental crustal melts, and some rocks exhibit a higher MgO and Mg# than those of these melts (Figures 8(3) and 11(1)), suggesting the involvement of mafic magma. All these data imply the key role of the magma mixing process in the formation of the biotite granodiorites [23,99]. In the Th/Nd vs. Th diagram (Figure 13(1)), these rocks follow the geochemical trend of partial melting or magma mixing processes. ...
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... 289 Ma; ε Hf (t) = +8.24 to +11.38) are distinct from those of the slightly older zircons (ca. 450 Ma; ε Hf (t) = −11.39 to +6.01), but similar to the values in zircons in the Permian ultramafic-felsic intrusions within the Kanggur Accretionary Complex (Fig. 9A), which indicates that the gneissic magma mixed with depleted mantle components during its formation (Yang et al., 2007). Based on the variable and distinct isotope signatures of the sources of the gneiss and granitic vein (Fig. 9), their old Nd-Hf model ages, low Mg# (0.14-0.27), elevated K 2 O (1.55-4.53 ...
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... respectively. This ratio, observed at low values in enclaves, reflects a melting regime dominated by relatively large melting fractions or the accompanying spinel-dominated residual phase [91,92]. The magma which has formed at the boundary of the upper mantle and lower continental crust would either interact with the continental crust or mix with magma derived from the continental crust in this melting regime. ...
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Leucogranites of Kalebalta in Central Anatolia are composed of plagioclase, quartz, orthoclase, and biotite and contains mafic microgranular enclaves (MME) in sizes ranging from few cm to 70 cm. In the total alkali-silica diagram, they fall typically in the granite field and show a calc-alkaline nature in the alkalis-iron-magnesium diagram whereas enclaves are Medium K series calc-alkaline, which represents the transition from tholeiitic to calc-alkaline. Leucogranites which have A/CNK(mol%) > 1 are strong peraluminous and seen as the products of magma derived from a metasedimentary source. Signs of magma mixing expressing the mantle inputs are also observed in many bivariation diagrams. Zircon and apatite saturation temperatures calculated on the basis of whole rock chemistry are 744–829°C for leucogranites and 761–832°C for their enclaves. According to the Raman spectra, biotite and plagioclase minerals in leucogranites and their enclaves show similar Raman spectrums. The biotite minerals have Mg–O and/or Fe–O translational (transformation) bonds between 182 and 552 cm⁻¹, Si–O–Si bending between 552 and 1,100 cm⁻¹ and Si–O–Si vibrational bonds between 1,100 and 1,200 cm⁻¹. The results of this study suggest that the leucogranites and enclaves are most probably derived from different magmas. In addition, according to geochemical and spectroscopic data, they may also have fractional crystallization, which is effective after the mixing process.
... Originally, I-type granitoids were considered as produced by reworking of pre-existing crustal rocks, precluding a direct mantle input (e.g., Chappell and Stephens, 1988;Chappell and White, 1992;Wyllie, 1977). However, it has subsequently been proposed that mantle-derived magmas (Bonin, 2004;Kemp et al., 2007;Kemp and Hawkesworth, 2006), magma mixing, and amphibole fractionation are responsible for some I-type granites (e.g., De Paolo, 1981;Collins, 1998;Barbarin, 1999;Millar et al., 2001;Yang et al., 2004Yang et al., , 2007Davidson et al., 2007;Rooney et al., 2010;Richards, 2011). ...
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... In contrast, the lower crust, which is composed mainly of meta-igneous rocks with low tungsten concentrations, is not considered a source for the formation of such deposits (Ishihara, 1977;Song et al., 2021). The zircon Lu -Hf isotope system is widely considered to provide a powerful tool for deciphering the evolution of the crust and mantle (Iizuka et al., 2017;Kemp et al., 2009;Kinny and Maas, 2003;Vervoort and Kemp, 2016;Wu et al., 2006;Yang et al., 2007). Zircon Hf isotope data compiled for granites associated with tungsten deposits in the Nanling region are characterized by ε Hf (t) values of − 8 to − 11.6 and Paleoproterozoic T DM2 (1.7-1.9 ...
Article
Tungsten is a critical and strategic metal used widely in the aerospace, automotive, electronic, and defense in­ dustries. Most tungsten deposits are genetically related to granitic rocks and a small number of them are giant deposits that supply much of the World’s demand for tungsten. Understanding the genesis of these giant deposits and developing models based on this understanding that can guide exploration for them is, therefore, a matter of considerable interest. China hosts nearly 50% of the global tungsten resource, much of which is contained in a few giant deposits. This makes it an ideal location in which to study the processes that lead to the formation of giant tungsten deposits. Here, we use a compilation of the whole-rock geochemical and zircon Hf–O isotopic compositions of granitic rocks associated with tungsten deposits in China and elsewhere, in conjunction with Rayleigh fractionation modeling and Monte Carlo simulations, to quantitatively evaluate the role of the source region, oxygen fugacity, and the degree of magma differentiation in the formation of giant tungsten deposits. The zircon Hf–O isotopic compositions are very heterogeneous, indicating that there is no source either in the upper crust, the lower crust, or one representing a mixture of crust and mantle that can explain the existence of giant tungsten deposits. Our modeling also shows that changes in oxygen fugacity have little impact on the formation of giant tungsten deposits. Instead, the modeling demonstrates that a combination of a pre-enriched source and a high degree of magma differentiation are pre-requisites for forming a giant tungsten deposit.
... Liu et al. (2010) reported a 176 Hf/ 177 Hf value of 0.282015 6 0.000025 for the GJ-82C standard, while Woodhead and Hergt (2005) reported an 176 Hf/ 177 Hf value of 0.282306 6 0.000006 for the 91500 standard. The parameters ɛHf and T DM were then calculated using the formulas of Yang et al. (2007). All the U-Pb and Lu-Hf zircon data are provided as supplemental material (U-Pb Data and Lu-Hf Data excel files). ...
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This work focuses on the sedimentary provenance of the Villavicencio Formation of the Mendoza Precordillera and integrates the information obtained with previous work on other coeval units of the Precordillera Central of San Juan province (Gualilán Group: Talacasto and Punta Negra formations) in western Argentina. Multiproxy provenance analyses are carried out from different applied methodologies (petrography, geochemistry, morphological, and cathodoluminescence studies of detrital zircon grains, and analysis of U-Pb and Lu-Hf isotopes). The Villavicencio Formation is mostly composed of pelites and very fine-grained psammites. The major components are quartz, both monocrystalline and polycrystalline, and metamorphic lithics that associate this unit with a recycled orogen. Regarding geochemistry, the Chemical Index of Alteration (CIA) values are similar to the Post-Archean Australian Shales (PAAS), indicating a null to incipient degree of weathering. The ratios between different trace elements and rare earth elements (REEs) suggest the felsic composition of the source area. Th/U ratios differ, but a secondary uranium enrichment is inferred. The morphological analysis of the zircon grains reveals their mainly plutonic origin. The integration of U-Pb data with Lu-Hf data shows a juvenile-mantle origin in which the populations are dominantly Mesoproterozoic and ɛHf of positive values (up to 12), indicating poor differentiation. The Villavicencio Formation would be the product of deltaic deposits in which its components are dominantly from the Western Pampean Sierras associated with the Grenville orogen, assuming exhumation and erosion of the Mesoproterozoic basement. The data support the hypothesis of equivalence and correlation with the Punta Negra Formation in the Devonian depocenters of the south-central region of the San Juan Precordillera.