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Article

Petrogenesis of Early Cretaceous High Ba-Sr Granitoids in the Jiaodong Peninsula, East China: Insights into Regional Tectonic Transition

1
School of Earth Sciences and Resources, China University of Geosciences, Beijing 100083, China
2
Jiaojia Gold Company, Shandong Gold Mining Stock Co., Ltd., Laizhou 261438, China
3
Yunfu Natural Resources Bureau, Yunfu 527300, China
4
MNR Key Laboratory of Metallogeny and Mineral Assesment, Institute of Mineral Resources, Chinese Academy of Geological Sciences, Beijing 100037, China
5
School of Earth and Space Sciences, Peking University, Beijing 100871, China
6
Yingkou Essential Industries High Quality Development Promotion Center, Yingkou 115003, China
*
Author to whom correspondence should be addressed.
Appl. Sci. 2023, 13(2), 1000; https://doi.org/10.3390/app13021000
Submission received: 16 November 2022 / Revised: 16 December 2022 / Accepted: 23 December 2022 / Published: 11 January 2023
(This article belongs to the Section Earth Sciences)

Abstract

:
Element geochemistry, Sr and Nd isotope, and LA-ICP-MS zircon U-Pb isotope data have been obtained for the granitoids of Dazesan pluton in the Jiaodong Peninsula, East China, and their intermediate microgranular dark enclaves so as to reveal their petrogenesis and tectonic implications. These granitoids have high SiO2 (68.25–71.56 wt.%), K2O (3.44–5.50 wt.%), total alkalis (K2O + Na2O = 7.29–9.00 wt.%), Sr (451–638 ppm), Ba (1157–2842 ppm) and light rare earth elements (LREEs) (131.57–210.08), with strong depletion both in heavy rare earth element (HREE) and high field strength element (HFSE) concentrations as well as unclearly Eu anomalies, showing typical signatures of high Ba-Sr granitoids. They possess high (La/Yb)N (32–50) and Sr/Y (50–79) values and low MgO (0.76–1.11 wt.%), Cr (9.9–19.6 ppm) and Ni (4.51–7.04 ppm) concentrations. All the above geochemical compositions are similar to those of late Early Cretaceous granitoids, in combination with zircon LA-ICP-MS U-Pb ages of 119.6 ± 1.3 to 120 ± 1 Ma for these granitoids obtained in this study, indicating c. 120 Ma probably represents the lower limit of ages when late Early Cretaceous granitoids emplaced in the Jiaodong Peninsula. The microgranular dark enclaves, forming a linear trend with their host granitoids on the oxide against SiO2 plots, display higher MgO contents of 3.05–4.39 wt.% at lower SiO2 concentrations of 54.25–56.84 wt.% and possess a zircon LA-ICP-MS U-Pb age of 119 ± 2 Ma, identical to those of these granitoids, indicating the acid magma and intermediate magma were coeval. Furthermore, dark enclaves and their host granitoids have indistinguishable (87Sr/86Sr)i values of 0.709523–0.70972 and 0.709361–0.709858, respectively, and plot within a two-liquid immiscible field on the Greig pseudoternary phase diagram. In addition, they have markedly parallel REE patterns, with the dark enclaves having much greater REE and HFSE abundances than those of their host granitoids. Therefore, it is suggested that liquid immiscibility is a viable model to explain the chemical compositional variations between the Dazeshan granitoids and their dark enclaves. Based on the element geochemistry, geochronology and Sr- and Nd-isotope of the Dazeshan granitoids and their dark enclaves, it is envisaged the crust-derived acid melts due to partial melting of ancient continental lower crust in the Jiaodong Peninsula (mainly Neoarchean-Palaeoproterozoic basement in the Jiaobei terrane) containing a subduction-related material, resulting from the addition of the enriched subcontinental lithospheric mantle-derived melts, assimilated the lithospheric mantle-derived basic melts and formed the homogeneous magma chamber at the crust base, then split into two immiscible liquids, with one granitic liquid producing the Dazeshan granitoids and the other intermediate one forming the dark enclave during its ascent. Combined with previous studies, the identification of a lithospheric mantle-derived material in the Dazeshan granitoids suggests a catastrophic lithospheric thinning at c. 120 Ma, reflecting an abrupt change in the direction of Palaeo-Pacific plate subducting and the corresponding regional tectonic transition from E–W extension to NW–SE extension.

1. Introduction

East China, towards the west Pacific Ocean (Figure 1a), was transformed into an active continental margin due to Palaeo-Pacific plate subducting under East Asia at a shallow angle, which was initiated at c. 180 Ma [1,2,3], following the collision of the North China Craton (NCC) with the Yangtze Craton (YC) in the Middle-Late Triassic (244–220 Ma) [4]. The latter orogenesis resulted in the formation of the Jiaodong Peninsula, by the combination of Jiaobei terrane in the northwest with Sulu terrane in the southeast by way of the NE- to NNE-trending lithospheric-scale Wulian-Qingdao-Yantai Fault (WQYF), on the East China continental margin (Figure 1a,b) [5,6]. The Mesozoic tectonic evolution in the Jiaodong Peninsula was closely associated with the Palaeo-Pacific plate subduction [7,8], the varying velocity, angle, and direction of which caused the crustal deformations and changed the geodynamics of the overlying East China continental margin [8,9]. In particular, it has been suggested that a tectonic transition occurred in the Jiaodong Peninsula because of the changes in the direction of Palaeo-Pacific plate subducting during the late Early Cretaceous [8,9,10,11]. A shift of this period from extension to transpression, corresponding to a change from SW to NW in the direction of Palaeo-Pacific plate subducting during c. 125–122 Ma [8], has been inferred from the development of basins, extension-related igneous rocks and gold deposits in the Jiaodong Peninsula [8,10,11]. However, it was suggested that the stress regimes shifted from transpression to extension at c. 120 Ma, which was indicated by the sinistral to normal movement that the Tan-Lu Fault (TLF) experienced [12]. Furthermore, fault-slip data from the Jiaobei terrane showed an overall extensional tectonic regime during Early Cretaceous only with the extensional direction rotating from E–W to NW–SE at c. 120 Ma [13], corresponding to a change of the Palaeo-Pacific plate subduction direction from WNW (139–122 Ma) to NW (121–95 Ma) [14].
High Ba-Sr granitoids, occurring in Phanerozoic (especially Early Cretaceous and Tertiary) orogenic belts globally [16,17,18], were first defined by [16] based on their geochemical features, which are marked by high Ba (>500 ppm), Sr (>300 ppm), LREEs and K/Rb, as well as low Rb, U, Th, Ta, Y and HREEs, with strong Nb depletion and insignificant Eu anomaly [16,19,20]. It has been proposed that the genetic mechanisms for high Ba-Sr granitoids include the partial melting of subducted ocean plateau resulting from mafic high Ba-Sr magma underplating [16], partial melting of metasomatized lithospheric mantle by asthenosphere-derived carbonatitic [16] or continental slab-derived melts [19,20], partial melting of mafic lower crust involving enriched mantle-derived magmas [18,21], mixing of acid and basic magmas produced from lower crust and enriched mantle, respectively [22,23], and crystal fractionation from the associated enriched lithospheric mantle-derived alkaline magmas accompanied with minor crustal assimilation [24,25,26]. The variable origins of high Ba-Sr granitoids play an important role in revealing the tectonic evolution of orogenic belts [27].
Mesozoic giant igneous magmatism in Jiaodong Peninsula is one of the principal geological events closely associated with Palaeo-Pacific plate subducting [28,29]. In particular, the Cretaceous giant igneous magmatism was coincident with the shift of Palaeo-Pacific plate drifting [8]. Furthermore, it is noted that a great number of high Ba-Sr granitoids (c. 162–110 Ma) have been discovered in the Jiaobei terrane [30,31]. Therefore, the tectonic-magmatic processes of high Ba-Sr granitoids are the key to unravel the tectonic evolution in Jiaodong Peninsula associated with late Early Cretaceous Palaeo-Pacific plate subducting. However, the formation of the late Early Cretaceous magmas is still not well constrained [8]. Here, we analyze element compositions and Sr-Nd isotopes as well as zircon LA-ICP-MS U-Pb dating so as to illustrate the tectonic-magmatic processes of the late Early Cretaceous granitoids and offer new insight into the tectonic transition in the Jiaodong Peninsula.

2. Geological Setting and Sampling

The Jiaodong Peninsula, on the East China continental margin, is bounded by the Pacific Plate to the east and separated from the Luxi Block in NCC by the NNE-trending TLF to the west (Figure 1a,b) [6]. It can be separated into Sulu terrane in the southeast and Jiaobei terrane in the northwest based on the lithospheric-scale ENE- to NE-oriented WQYF [32,33]. The Jiaobei terrane basement rocks consist of Mesoarchean-Neoarchean Jiaodong Group TTG gneisses with Neoarchean amphibolites and mafic granulites [34,35], Palaeoproterozoic Jingshan and Fenzishan Groups, including metasedimentary marbles, calc-silicate rocks, and amphibolites [36,37] undergoing a c. 1.8 Ga amphibolite- to granulite-facies metamorphism [35,38], and the Neoproterozoic Penglai Group, consisting of slates, marbles and quartzites [39]. The crystalline basement in the Sulu terrane mainly includes Neoproterozoic and Palaeoproterozoic basement rocks of YC [40,41,42], which underwent a c. 244–220 Ma ultrahigh-pressure (UHP) metamorphic event [43,44]. Coesite-bearing eclogite, granitic gneiss, marble and quartzite composed the UHP metamorphic rocks [36,45], which were overprinted by the 220–205 Ma amphibolite to granulite-facies metamorphism locally [46]. The Palaeo-Pacific plate subduction resulted in the large scale Mesozoic magmatism in the Jiaodong Peninsula (Figure 1b) [8]. These Mesozoic magmatic rocks mainly occurred during two major episodes [47]: (a) Late Jurassic monzogranite and biotite granite (166–149 Ma) [3,48] and (b) Early Cretaceous (130–110 Ma) porphyritic-like monzogranite, granodiorite and syenogranite [49,50]. In addition, in the Jiaodong Peninsula, a great number of Mesozoic mafic dykes also occurred [51,52].
The Dazeshan granitic pluton, with an area of c. 25 km2, intruding into the southwest part of the Late Jurassic Linglong batholith in Jiaobei terrane (Figure 1), is a sheet-like NE- to NNE-trending intrusive body (Figure 2a,b). It is composed of massive and homogeneous monzogranites, showing the sharp contact with the host rock (Figure 2c,d). These monzogranites are medium- to coarse-grained and light flesh-pink in appearance (Figure 2e) and generally show typically porphyritic-like texture with a large amount of megacrysts of K-feldspar (Figure 2e). In addition, microgranular dark enclaves occur widely but are scarce (less than 1%) in these monzogranites (Figure 2f). They range from a few centimeters to decimeters in size (Figure 2f) and are oval to tabular in shape, commonly showing abrupt contacts with their host granitoids (Figure 2g,f). Some enclaves contain K-feldspar megacrysts (Figure 2h), suggesting that the granitic and mafic magmas were coeval. Samples for this paper, consisting of monzogranites and their dark enclaves, were collected from the Dazeshan granitic pluton, the locations of which are given in Figure 2b.
The main mineralogy of monzogranite includes plagioclase (32–36%), K-feldspar (30–33%), quartz (22–25%), biotite (3–6%) and amphibole (<3%), with few accessory minerals of sphene, apatite and zircon (Figure 3a–c). K-feldspar is generally subhedral, with inclusions of biotite, plagioclase and quartz (Figure 3d). The dark enclaves are dioritic in composition and usually show fine-grained subhedral equigranular textures (Figure 3e,f). The minerals are mainly of plagioclase, hornblende and quartz, without or with K-feldspar and biotite, and the accessory minerals are apatite, zircon, magnetite and titanite (Figure 3f). No hydrothermal alteration and ductile structures are observed both in these granitoids and their dark enclaves (Figure 3).

3. Analytical Methods

3.1. LA-ICP-MS Zircon U-Pb Dating

Over 500 zircon crystals were extracted from each sample after being crushed to c. 80–100 mesh for a grain size, using standard gravimetric-magnetic separation techniques at Langfang Technology Service Co., Ltd. of Geoscience Exploration, Hebei Province, China. Then, under a binocular microscope, at least 200 grains larger than 40 um in diameter containing no visible fractures and inclusions were handpicked, mounted in epoxy resin and polished in order to expose the centre of zircon crystals. To choose the zircon grains without fluid/mineral inclusions and microcracks for U-Pb analyses, zircon internal textures were identified by examining the reflected and transmitted light micrographs in detail, which were obtained by optical microscopy at the geochemical research laboratory at China University of Geosciences (Beijing), as well as the cathodoluminescence (CL) images, which were obtained through a Quanta 200FEG environmental scanning electron microscope (SEM) at Beijing University.
Zircon U-Pb dating was performed by laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) at the Hefei University of Technology, China, through an Agilent 7500a ICP-Mass furnished with a GeolasPro laser. The laser frequency was 6 Hz, and the spot diameter used for the analyse was 32 um. The external standard used as U-Pb dating was Harvard zircon 91500, and the external standard for calculating the contents of Th, U and Pb was NIST610. ICPMSDataCal 8.3 software was used to calculate the 206Pb/238U and 207Pb/206Pb ratios [53], and on the basis of the method of [54], we corrected the common Pb. The calculation of the weighted average ages and the concordia ages plotting were obtained using the Isoplot 4.16 program [55]. Detailed analytical techniques resembled those documented by [31,56].

3.2. Major- and Trace-Element Analyses

In this study, whole-rock major- and trace-element contents (including REEs) for twenty-one samples (sixteen monzogranites and five dark enclaves) were determined at the Research Institute of Uranium Geology, Beijing, China. The major elements were measured using a Philips PW2404 X-Ray Fluorescence Spectrometer (XRF), and the trace elements were determined by an ELEMENT-1 plasma mass spectrometer made by Finnigan-MAT Ltd. For major- and trace- elements, which included REEs, the analytical uncertainties were less than ±1% and ±5%, respectively. Ref. [57] introduced the detailed analytical procedures.

3.3. Whole Rock Sr and Nd Isotope Analyses

In this study, whole-rock Sr and Nd isotope analyses for twenty samples (sixteen monzogranites and four dark enclaves) were determined by a Finnigan MAT 262 multi-channel mass spectrometer at the Research Institute of Uranium Geology, Beijing, China. The powder (c. 110 –160 mg) of each sample was dissolved with the acid mixture of HNO3 + HF (ratio of 1:2) in Teflon beakers. The separation of Sr and REEs was made through the combination of special Sr resin with standard cation-exchange columns. Then, the separation of Nd from the REEs was obtained through cation-exchange resin, with HIBA being eluent. The analytical procedures were introduced in detail by [58,59]. All the 143Nd/144Nd and 87Sr/86Sr fractionations measured were corrected according to the ratios of 143Nd/144Nd = 0.7219 and 87Sr/86Sr = 0.1194, respectively. During the analyses, the repeated analysis of the standard JNDi-1 for Nd produced 143Nd/144Nd = 0.512117 ± 0.000005 (2σ, n = 12), and the standard NBS-987 for Sr yielded 87Sr/86Sr = 0.710260 ± 0.000010 (2σ, n = 30). For Rb and Sr, total analytical blanks were (2–5) × 10−10 g, and they were 5 × 10−11 g for Sm and Nd.

4. Analytical Results

4.1. Zircon LA-ICP-MS U-Pb Age

The zircon LA-ICP-MS U-Pb isotope data obtained from the two monzogranite samples (DZS18D004B3 and DZS18D006B2-6) and one enclave sample (DZS18D004B1) are presented in Table 1. Figure 4 provides the U-Pb concordia age diagrams and histograms accompanied with the weighted average 206Pb/238U ages and the representative zircon cathodoluminescence (CL) images.
Zircons of both the monzogranites and their enclaves are prismatic and short, having length/width ratios and lengths of 1:1 to 3:1, and between 50 and 200 um, respectively. All the analyzed zircons are magmatic in origin as indicated by the oscillatory zoning shown on the CL images [60]. They have large variations in Th (88–4121 ppm) and U (129–1362 ppm) concentrations, with their Th/U ratios ranging between 0.4 and 2.5 (Table 1).
For monzogranite sample DZS18D004B3, we analyzed twenty-five zircon spots, which produced 206Pb/238U ages ranging between 115 ± 2 and 625 ± 8 Ma (Table 1; Figure 4a,b). Twenty-one of the twenty-five U-Pb isotopic data gave the concordant ages varying between 115 ± 2 and 123 ±2 Ma, with a weighted average age of 120 ± 1 Ma (2 σ , MSWD = 1.2) (Figure 4a,b), and the four analyses of inherited zircons yielded the concordant ages between 345 ± 11 and 625 ± 8 Ma (Figure 4a,b).
Among the fifteen zircon spots performed for monzogranite sample DZS18D006B2-6, fourteen U-Pb isotopic data showed the concordant ages between 114 ± 3 and 125 ± 2 Ma, with a weighted average age of 119.6 ± 1.3 Ma (2 σ , MSWD = 1.5) (Table 1; Figure 4c,d), and the remaining one, having the old and concordant age at 688 ± 13Ma, was from inherited zircon (Figure 4d).
For the enclave sample (DZS18D004B1), the eleven zircon spots were analyzed, which gave concordant ages between 112 ± 3 and 134 ± 8 Ma, with a weighted average age of 119 ± 2 Ma (2 σ , MSWD = 2.4) (Table 1; Figure 4e,f).

4.2. Whole-Rock Geochemistry

The major- and trace-element compositions for the monzogranites and their dark enclaves are shown in Figure 5 and Table A1. The rocks analyzed all have small loss on ignition (LOI) between 0.43% and 1.33% (Table A1), suggesting that these samples did not suffer any significant post-magmatic alteration, which is in accordance with the petrographic observations both in the field and from the thin sections (Figure 2).
Granitoids of the Dazeshan pluton are acidic in composition and have SiO2 contents ranging from 68.25 wt.% to 71.56 wt.% (Table A1; Figure 5a). They show high total alkalis (Na2O + K2O = 7.29–9.00 wt.%), mainly falling into the domain of the sub-alkaline monzogranite on the diagram of SiO2 vs. (Na2O + K2O) (Figure 5a). These samples have relatively high K2O concentrations of 3.44–5.50 wt.%, with K2O/Na2O of 0.89–1.57, and are in the domains of high-K calc-alkaline and shoshonite on the K2O vs. SiO2 diagram (Figure 5b) [62], indicating the overall potassic character (Figure 5b). They have a narrow range in contents of Al2O3 (13.91–15.70 wt.%), CaO (2.17–2.79 wt.%), TiO2 (0.26–0.36 wt.%), TFe2O3 (1.98–2.69 wt.%) and P2O5 (0.10–0.161 wt.%) (Table A1). Based on the aluminum saturation index A/CNK (molar Al2O3/(CaO + Na2O + K2O)), granitoids of the Dazeshan pluton show metaluminous to weakly peraluminous character, with A/CNK of 0.94–1.01 (Figure 5c). All these analyzed granitoids have a very narrow range of low MgO concentrations (0.76–1.11%), with the Mg# molar 100*MgO/(MgO + FeOT) of 40–43. Enclaves in the Dazeshan pluton, having the SiO2 concentrations of 54.25–56.84 wt.%, are intermediate in composition and correspond to syenodiorite (Figure 5a). They have higher contents of TiO2 (0.70–1.02 wt.%), Al2O3 (16.93–17.96 wt.%), TFe2O3 (6.86–8.65 wt.%), CaO (3.81–4.85 wt.%), P2O5 (0.45–0.67 wt.%) and MgO (3.05–4.39 wt.%), with a higher Mg# of 44–49 as compared those of the host granitoids (Table A1). These enclave samples have relatively high total alkalis concentrations of 7.69–9.97%, with variable K2O contents of 2.64–6.15 wt.% and K2O/Na2O ratios of 0.49–1.61, showing alkaline and shoshonitic characteristics (Figure 5b), and they are metaluminous, having A/CNK of 0.84–0.91 (Figure 5c). For granitoids and their enclaves, the major oxides of MgO, Al2O3 and CaO concentrations generally have negative correlations with SiO2 values (Figure 5d–f).
As shown in Table A1 and the chondrite-normalized REE diagrams (Figure 6a), both granitoids of the Dazeshan pluton and their enclaves are characterized by high total REE concentrations, with the ΣREE being 138–220 ppm and 359–572 ppm, respectively. Both are rich in LREE, with the ratios of (La/Yb)N varying between 32 and 50 for the granitoids and varying between 15 and 47 for the enclaves. The enclaves show moderate negative Eu anomalies, having Eu/Eu* values of 0.45–0.65 (Figure 6a), whereas the granitoids possess unclearly negative Eu anomalies (Eu/Eu* = 0.73–1.00), except that one sample has Eu/Eu* ratio of 0.66 (Figure 6a).
Granitoids of Dazeshan pluton are obviously rich in large ion lithophile element (LILE) concentrations, such as Rb (94–137 ppm), Sr (451–638 ppm) and Ba (1157–2842 ppm), with Rb/Sr and Sr/Y values of 0.18–0.27 and 50–79, respectively (Table A1; Figure 7a). The enclaves have Rb (162–220 ppm), Sr (387–544 ppm), Ba (629–1413 ppm), Rb/Sr (0.30–0.56) and Sr/Y (15–25) (Table A1; Figure 7a). Contents of HFSEs for the granitoids and their enclaves are Nb (6.9–9.7 and 15.6–31.4 ppm), Hf (0.47–1.10 and 1.55–1.89 ppm), Ta (0.63–0.88 and 1.09–2.95 ppm), Y(7.2–10.9 and 19.2–35.6 ppm) and Th (10–29 and 19–35 ppm), respectively. The enclaves show higher concentrations of compatible elements such as V (102–124 ppm), Ni (10–30 ppm) and Cr (12–133 ppm) than those of their host rocks, with V (21.4–44.8 ppm), Ni (4.51–7.04 ppm) and Cr (9.9–19.6 ppm). Both the enclaves and their host granitoids show strong negative Ta and Nb anomalies and positive Pb and K peaks on the primitive mantle-normalized spidergrams (Figure 7a).

4.3. Whole-Rock Sr-Nd Isotopes

Twenty representative samples (sixteen granitoids and four enclaves) were analyzed for Sr and Nd isotopic compositions in this study; they are listed in Table 2.
Granitoids of the Dazeshan pluton show 87Sr/86Sr ratios of 0.710638–0.710876 and 143Nd/144Nd values of 0.511434–0.511578, whereas their enclaves have slightly higher 87Sr/86Sr ratios of 0.711018–0.712482 and 143Nd/144Nd ratios of 0.511439–0.511633.
The initial 87Sr/86Sr ratios (87Sr/86Sr)i and εNd(t) values were obtained at 120 Ma according to the zircon LA-ICP-MS U-Pb dating for both granitoids and their enclaves in this study. The data are plotted in the diagram of εNd(t) vs. (87Sr/86Sr)i (Figure 8). Granitoids show a narrow range of (87Sr/86Sr)i ratios of 0.709361–0.709858, and strongly negative εNd(t) values of –21.6 to –18.8, with the two-stage Nd model ages (TDM2) varying between 2449 and 2679 Ma, consistent with those of their enclaves, with (87Sr/86Sr)i = 0.709523–0.709726, εNd(t) = –21.8 to –17.8 and TDM2 = 2365–2691 Ma.

5. Discussion

5.1. Petrological Classification and Petrogenesis

As mentioned above, the large scale Early Cretaceous intrusive rocks (130–110 Ma) occurred in the Jiaodong Peninsula (Figure 1) [8,33,49]. Based on the lithology, geochemistry and geochronology, as well as their attitudes and spatial relationships, they can be traditionally divided into two subgroups [33,49,65,73]: (a) the middle Early Cretaceous granitoids (132–122 Ma), mainly consisting of quartz monzonite, granodiorite and porphyritic-like monzogranite, and trending E–W to ENE (Figure 1b); and (b) the late Early Cretaceous granitoids (118–110 Ma), mainly including porphyritic-like monzogranites, granodiorite and syenogranites, and trending NE to NNE (Figure 1b). The LA-ICP-MS zircon U-Pb ages obtained in this study provide the first precise geochronology on granitoids of the Dazeshan pluton and show ages of 119.6 ± 1.3 to 120 ± 1 Ma, which are between those of middle Early Cretaceous granitoids and late Early Cretaceous granitoids. Given that the granitoids in this study have the same petrology (Figure 3), attitude (Figure 1b), major-element composition (Figure 5), and REE and trace-element distribution patterns as those of the late Early Cretaceous granitoids (Figure 6 and Figure 7), it is logical to infer that the Dazeshan pluton belongs to the late Early Cretaceous granitoids, and the crystallization age of c. 120 Ma probably represents the lower limit of emplacement ages for the late Early Cretaceous granitoids in the Peninsula. In addition, the LA-ICP-MS zircon U-Pb age of 119 ± 2 Ma obtained for the dioritic microgranular enclaves is the same as those of the host granitoids (119.6 ± 1.3 to 120 ± 1 Ma), suggesting that the felsic and intermediate magmas were coeval.
All the analyzed samples for granitoids of the Dazeshan pluton and their enclaves produced very low LOI (0.42–1.33 wt.%), as well as low La/Th ratios (1.0–6.4) and low to medium K/Sr ratios (49–160), suggesting that their element composition was not modified by the element migration [74,75]; therefore, all the major- and trace-element data obtained can be used to interpret their petrogenesis.
All the samples for granitoids of the Dazeshan pluton in this study have higher alkali contents (Na2O + K2O = 7.29–9.00%), and lower Al2O3 (13.91–15.70%) and MgO values (0.76–1.11%) (Table A1; Figure 5) and flatter HREE patterns (Figure 7a) as compared to the calc-alkaline geochemical features that the typical adakitic rocks possess. In addition, they reflect a dominant calc-alkaline trend in the Na-K-Ca plot, instead of the trondhjemitic affinities of the adakitic rocks (Figure 9a). Furthermore, they show high Ba (>629 ppm), Sr (>451 ppm), K/Rb (>320) and LREEs (>132 ppm), as well as low Rb (<137 ppm), Th (<29 ppm), U (<2.4 ppm), Nb (<9.7 ppm), Ta (<0.9 ppm), Y (<10.9 ppm) and HREEs (<9.6 ppm) (Table 2), have no clearly negative Eu anomalies (Figure 6a) and are depleted in Nb in spidergrams (Figure 7a), which separate them from the traditional A-, M-, S- and I-type granites.
However, the very high Sr (451–638 ppm) and Ba (1157–2842 ppm) contents indicate Dazeshan granitoids are similar to the high Ba-Sr granitoids proposed by [16], which are characterized by high Sr (>300 ppm) and Ba (>500 ppm) concentrations. Based on the difference in Sr and Ba contents, in the Sr-Rb-Ba plot, all the analyzed Dazeshan granitoids plot inside the domain of the high Ba-Sr granite [16], which is different from the low Ba-Sr granite (Figure 9b). Furthermore, the lack of clearly negative Eu anomalies (Figure 6a), the apparent fractionated REE patterns (Figure 6a) as well as the prominent depletion in Ti, P, Nb and Ta (Figure 7a), together with the very low Yb and Y concentrations against high (La/Yb)N (32–50) and Sr/Y (50–79) ratios, are also similar to the typical geochemical characteristics of high Ba-Sr granitoids (Figure 6d and Figure 7d) [20,76]. Therefore, it is logical to classify the Dazeshan granitoids as high Ba-Sr granitoids.
It was proposed that late Early Cretaceous granitoids (118–110 Ma) in the Jiaodong Peninsula resulted from the partial melting of continental lower-middle crust followed by crystal fractionation [65]. The microgranular dark enclaves were widely developed in late Early Cretaceous granitoids, such as Sanfoshan pluton [30], Yashan pluton [65], Changshannan pluton [64], Gushan pluton [66] and Weidesan plutons [77], which were considered to be a result of magma mixing between crust-derived and mantle-derived magmas [30,64,65,66,77]. Likewise, the microgranular dark enclaves were also observed in the Dazeshan pluton in this study. However, all the dark enclaves are dioritic, with SiO2 concentrations of 52.46–58.06 wt.% (Figure 5a) [64,65,66,77], and they have negative εHf (t) values ranging from –19.6 to –16.1 [78], indicating a crustal derivation for these dark enclaves, although a mantle origin followed by the crustal contamination remains a possibility [79]. Furthermore, the indistinguishable (87Sr/86Sr)i values for the dark enclaves and their host granitoids (Table 2; Figure 8) suggest a cogenetic origin, which may be associated with a common evolution process, such as restite unmixing, crystal accumulation, crystal fractionation or liquid immiscibility, instead of the magma mixing, co-mingling or wall-rock assimilation models [47,52,79,80,81,82,83,84,85].
However, the primary igneous rather than metamorphic textures of the enclaves from the Dazeshan pluton (Figure 3) preclude an origin resulting from restite unmixing [69,81,84,86]. In addition, the much higher REE, Zr, Nb and P concentrations in the dark enclaves than those in their host granitoids (Table A1; Figure 6 and Figure 7) rule out their relation to fractional crystallization [80,82,87,88]. Furthermore, a crystal accumulation model is also eliminated because of the greater REE and the moderately negative Eu anomalies (Eu/Eu* = 0.45–0.65) in contrast to the positive Eu anomaly shown in the dark enclaves (Table A1; Figure 6) [79,89,90]. Thus, it seems that liquid immiscibility is a viable model to explain the origin of the Dazeshan granitoids and their dark enclaves, which is also supported by the major-, trace-, and REE-element composition presented below, except for their identical (87Sr/86Sr)i values (Table 2; Figure 8).
Experimental studies show that silicate melts rich in MgO, CaO, P2O5, FeO and TiO2 tend to split into one immiscible liquid pair, consisting of a quartzo-feldspathic acid liquid and an iron-rich intermediate-basic liquid, producing a gap in SiO2 composition with a linear trend on the oxide against SiO2 plots [91,92,93,94]. On a Greig pseudoternary phase diagram [SiO2-(CaO + MgO + TFe2O3 + TiO2 + P2O5)-(Na2O + K2O + Al2O3)], the Dazeshan granitoids and dark enclaves plot within a two-liquid immiscible field (Figure 10). In addition, they show a gap between 56.84 wt.% and 68.25 wt.% in SiO2 composition, and the oxides have a decreasing trend against SiO2 increasing (Figure 5). Thus, the major-element compositional variation between the Dazeshan granitoids and dark enclaves could be related to a liquid immiscible process.
Furthermore, the relative contents of trace and REE elements in the silicic rocks and their dark enclaves can also be used to judge if they were derived from a liquid immiscible process [80,87,93,94]. In this study, the concentration of each trace element in the granitoid (acid material) was divided by that in the corresponding dark enclave pair (intermediate material). The distributions of resulting ratios are shown in Figure 11, which agree well with the distribution fields defined by the experimental two-liquid partitioning coefficients of [93,94], as well as the elemental rations between the acid and intermediate-basic materials that indicate one immiscible liquid pair [80,89,96]. In addition, it was suggested that the two immiscible liquids could have parallel REE distribution patterns, whereas REE abundances in immiscible intermediate-basic liquids are much greater than those in acid liquids [80]. It can be found that the REE distribution patterns between the Dazeshan granitoids and their enclaves are markedly parallel, and the dark enclaves have much greater rare earth element (REE) and HFSE abundances than those of their host granitoids, which is similar to those for the Rosetown diorite and granodiorite, representing two immiscible end-member liquids [80]. Therefore, it is logical to suggest that liquid immiscibility is a viable model to explain the chemical compositional variations between the Dazeshan granitoids and their dark enclaves.
It was suggested that the dioritic enclaves formed before and during liquid immiscibility are characterized by the typical textural features of distorted angular shapes with inward pointing cusps on their edges [80,97]. Hence, the spherical to tabular shape for the dark enclaves, which are lack of the inward pointing cusps, trapped in the Dazeshan granitoids may indicate the two immiscible end-member liquids during separation would have been almost free of crystals. Thus, the compositions of Dazeshan granitoids and their enclaves may represent those of the original melts. However, given the scarce dark enclaves in the Dazeshan granitoids, though they are widely distributed, the dioritic liquid could be an infinitesimal fraction compared to the parent; therefore, the acid liquid will have the composition approximating that of the parent magma.
All the samples of Dazeshan granitoids studied show great SiO2 (>68.25 wt.%) and low MgO (<1.11 wt.%), TiO2 (0.26–0.36 wt.%) and TFe2O3 (1.98–2.69 wt.%) concentrations (Table A1; Figure 5), as well as high (87Sr/86Sr)i values (0.709361–0.709858) and highly negative εNd(t) values of –21.6 to –18.8 (Table 2; Figure 8), indicating their derivation from strongly evolved or crust-involved magmas. However, the almost homogeneous major and trace element concentrations within all the Dazeshan granitoids studied (Table A1), which is consistent with the petrographical homogeneity of the granitoids, as well as the insignificant negative Eu anomalies (Figure 6), suggest that no significant fractionation occurred during magma evolution. In addition, their TDM2 ages vary from 2449 to 2679 Ma (Table 2), in accordance with the ages of Neoarchean-Palaeoproterozoic amphibolite- to granulite-facies basement rocks in the Jiaobei terrane, reflecting a derivation from an ancient crust. Nevertheless, the enrichment in LILE and LREE but depletion in HFSE (Figure 6), the highly positive anomaly in Pb accompanied by the strong negative Nb, Ta, P and Ti anomalies (Figure 7), as well as the low Ce/Pb ratios of 2.22–5.82 (Table A1), suggest that the granitic magmas are likely generated from the partial melting of continental crust, related to an existing subduction event.
It was suggested that the mafic to felsic granulite, constituting the Archean-Proterozoic lower crust in the NCC, typically shows low K2O (average 0.8 wt.%), Rb (average 16.4 ppm), Sr (average 232 ppm) and Ba (average 193 ppm) and is strongly depleted in Zr, U and Th as well as rich in Hf [41,98]. However, all these features contradict those shown in the Dazeshan granitoids studied here. Thus, it is impossible that the NCC Archean lower crust is the exclusive or direct source for these granitoids. Furthermore, the melting of the mafic to felsic granulite rocks need high melting temperatures [85,99]. In addition, the middle Early Cretaceous granitoids (132–122 Ma), which have higher SiO2 (>70.89 wt.%) and lower MgO (<0.62 wt.%) concentrations, and higher (87Sr/86Sr)i values (0.71071–0.71172), were suggested to be derived from the mingling of the felsic melts, produced by the partial melting of Precambrian basement rocks of the Jiaobei terrane, with the intermediate magmas generated by the partial melting of juvenile mafic lower crust [100]. Therefore, it was proposed that Dazeshan granitoids are products of partial melting of the continental lower crust containing subduction-related materials induced by the injection of mantle-derived basic magmas. However, given the very low MgO concentrations and relatively high (87Sr/86Sr)i combined with the lack of any significant fractionation, it is suggested that likely only a few melts or mainly fluids came from the mantle, which is in accordance with the small portion of dark enclaves presented in the Dazeshan granitoids.
In the Jiaodong Peninsula, two types of coeval lamprophyres, i.e., low-Ti and high-Ti lamprophyres, were identified to be emplaced at c. 121 Ma. The low-Ti lamprophyres have high SiO2 concentrations of 49.5–53.9 wt.% and high Mg# (63–74), and show enrichment in both LILEs and LREEs but high depletion in HFSEs, with strongly negative anomalies in Zr, Hf, Nb, Ti and Ta (Figure 6e and Figure 7e). They possess highly negative εNd(t) values (–13.9 to –15.5) and εHf(t) values (–23.1 to –19.3) and are considered to originate from an enriched subcontinental lithospheric mantle that was metasomatized by subduction-related fluids [47]. The high-Ti lamprophyres have low SiO2 concentrations of 46.9–49.2 wt.% and Mg# (51–58) and show enrichment in LREEs, but lack Nb-Ta depletion and LILE enrichment (Figure 6f and Figure 7f). They possess higher εNd(t) values (–0.79 to 1.76) and εHf(t) values (–4.7 to 2.1) and are considered to originate from an asthenospheric mantle unaffected by subduction-related materials [47]. The elemental and isotopic compositions of the dark enclaves in the Dazeshan granitoids are much closer to those of enriched subcontinental lithospheric mantle beneath the Jiaodong Peninsula as indicated by low-Ti lamprophyres (Figure 6e, Figure 7e and Figure 8), distinct from those of asthenospheric mantle-derived high-Ti lamprophyres in the Jiaodong Peninsula (Figure 6f, Figure 7f and Figure 8). Therefore, it is most likely the enriched subcontinental lithospheric mantle is the source for the mantle-derived materials.
Given the very small variations in major- and trace-element contents, such as SiO2 (68.25–71.56 wt.%), Al2O3 (13.91–15.70%), CaO (2.17–2.79%), Y (7.2–10.9 ppm) and Yb (0.66–1.00 ppm), and the narrow ranges of (La/Yb)N ratios (32–50) for the Dazeshan granitoids, it is suggested that the crust-derived materials were likely from almost the same depth. Combined with the lack of both Neoarchean to Palaeoproterozoic inherited zircons and metamorphic wall rock enclaves in the Dazeshan granitoids and their dark enclaves, which are common in Late Jurassic (166–149 Ma) and middle Early Cretaceous granitoids (132–122 Ma), it is most likely that almost all the crust-derived components contained in the region of the magma source were melted, except for few Neoproterozoic to Palaeozoic inherited zircons, indicating their melting at higher crustal levels, likely due to the removal of the Archean lithospheric mantle as a consequence of delamination (Figure 12) [29,65]. In addition, the Dazeshan granitoids show the homogeneous Sr–Nd isotopic compositions, as are also indicated by other late Early Cretaceous granitoids (118–110 Ma), including the Changshannan pluton [64] and Gushan pluton [66]. Therefore, magma homogenization could have been obtained in the magma chamber at the crust base, and a MASH (melting, assimilation, storage, and homogenization) process [101] was responsible for the Dazeshan granitoids.
In summary, on the basis of the petrography, major and trace element geochemistry, geochronology and Sr- and Nd-isotope data of the Dazeshan granitoids and their microgranular dark enclaves, a MASH process followed by the liquid immiscible is envisaged for the origin of late Early Cretaceous granitoids in the Jiaodong Peninsula (Figure 12). It is suggested that at c. 120 Ma, partial melting of ancient continental lower crust in the Jiaodong Peninsula (mainly the Neoarchean-Palaeoproterozoic basement rocks in the Jiaobei terrane) containing a subduction-related material, which resulted from the addition of the enriched subcontinental lithospheric mantle-derived melts, generated the major melts of the Dazeshan granitoids. Then, the mantle-derived basic melts were assimilated by the crust-derived acid melts, forming the homogeneous magma chamber at the crust base (Figure 12). During the homogeneous magma ascent, the single melt split into two immiscible liquids due to the variations in densities, viscosities and temperatures, with one granitic liquid producing Dazeshan granitoids, whereas the other intermediate melt formed the dark enclave (Figure 12).

5.2. Implication for a Shift in Tectonic Setting

Early Cretaceous tectonic evolution history in the Jiaodong Peninsula remains unclear, although it is well documented that its Mesozoic geodynamics are closely associated with the Palaeo-Pacific plate subducting beneath the East China continental margin [11,102,103], and an Early Cretaceous tectonic transition has been identified [8,13]. Large-scale extension-related magmatism [47,52,104] and gold mineralization [6,105], as well as the normal movement along the TLF [9] all suggest an extensional tectonic setting during c. 130–110 Ma in the Jiaodong Peninsula. However, [8] proposed that a tectonic transition from extension to compression occurred in the Jiaodong Peninsula during c. 125–122 Ma, resulting from the shift in subduction direction of the Palaeo-Pacific Plate.
It is widely accepted that the Jiaodong Peninsula has undergone lithospheric thinning during an extensional tectonic setting since the Mesozoic [106,107,108], which is evidenced by Early Cretaceous high Ba-Sr granitoids in the Jiaobei terrane [33]. However, there is an abrupt change in composition between these two subgroups of Early Cretaceous high Ba-Sr granitoids (Figure 5, Figure 6, Figure 7, Figure 8 and Figure 9), which indicates a change from juvenile mafic lower crust and continental lower crust sources in the middle Early Cretaceous (132–122 Ma) [33] to continental lower crust and enriched subcontinental lithospheric mantle-derived sources in the late Early Cretaceous (120–110 Ma). Furthermore, the two types of coeval lamprophyres (i.e., low-Ti and high-Ti lamprophyres) emplaced at c. 121 Ma are suggested to originate from an enriched subcontinental lithospheric mantle and an asthenospheric mantle, respectively [47]. It was suggested that the melting of inferred lower crust and juvenile mafic lower crust was caused by asthenosphere upwelling and lithospheric thinning (Figure 13 in [48]), which is in accordance with the Palaeo-Pacific plate WNW-ward subduction, leading to E–W extension in the Jiaodong Peninsula during the middle Early Cretaceous (132–122 Ma) [13,109]. The lithospheric mantle-derived melt for the late Early Cretaceous granitoids (120–110 Ma), combined with the asthenosphere mantle melting for the high-Ti lamprophyres, indicates the Jiaodong Peninsula probably underwent a catastrophic lithospheric thinning event at c. 120 Ma, which is consistent with an abrupt change in the direction of the Palaeo-Pacific plate subducting from WNW to NW at c. 121 Ma [13]. Therefore, this suggests a transition in tectonic setting from E–W extension to NW–SE extension (Figure 12), as also supported by the least principal stress axis shifting from E–W through WNW–ESE to NW–SE c. 119 Ma based on the Palaeostress analysis by the quartz veins and lamprophyre dikes at the Sizhuang gold deposit in the Jiaobei terrane [6].

6. Conclusions

(1)
The granitoids of Dazesan pluton consist of medium- to coarse-grained porphyritic-like homogeneous monzogranites, with large amounts of megacrysts of K-feldspar. These rocks possess acid composition, with SiO2 ranging between 68.25 wt.% and 71.56 wt.% and high K2O (3.44–5.50 wt.%) and total alkalis (K2O + Na2O = 7.29–9.00 wt.%), with very high Sr (451–638 ppm) and Ba (1157–2842 ppm), showing the typical signatures of high Ba-Sr granitoids.
(2)
These granitoids share the same geochemical compositions as those of late Early Cretaceous granitoids. The zircon LA-ICP-MS U-Pb ages of 119.6 ± 1.3 to 120 ± 1 Ma for the granitoids obtained in this study likely represent the lower limit of emplacement ages for the late Early Cretaceous granitoids in the Jiaodong Peninsula.
(3)
The microgranular dark enclaves with higher MgO contents of 3.05–4.39 wt.% at lower SiO2 concentrations of 54.25–56.84 wt.% form a linear trend on the oxide against SiO2 plots with their host granitoids and have the zircon LA-ICP-MS U-Pb age of 119 ± 2 Ma, identical to those of the host granitoids. Combined with the major-element compositional variation, the relative concentrations of trace and REE elements as well as the similar Sr-Nd isotopic compositions between silicic rocks and their dark enclaves support the liquid immiscibility for their origin.
(4)
Partial melting of the ancient continental lower crust in the Jiaodong Peninsula (mainly the Neoarchean-Palaeoproterozoic basement rocks in the Jiaobei terrane) containing a subduction-related material, resulting from the addition of the enriched subcontinental lithospheric mantle-derived melts, generated the crust-derived acid melts, which assimilated the lithospheric mantle-derived basic melts and formed the homogeneous magma chamber at the crust base, then split into two immiscible liquids, with one granitic liquid producing Dazeshan granitoids and the other intermediate one forming the dark enclave during its ascent.
(5)
Identification of a lithospheric mantle-derived material in the Dazeshan granitoids suggests a catastrophic lithospheric thinning at c. 120 Ma, in accordance with an abrupt change in direction of Palaeo-Pacific plate subducting, indicating regional tectonic transition from E–W extension to NW–SE extension.

Author Contributions

Conceptualization, Z.W.; Data curation, Z.W.; Formal analysis, R.Z. (Rongxin Zhao), T.Y. and Y.W.; Funding acquisition, Z.W.; Investigation, Z.W., R.Z. (Rongxin Zhao), T.Y., Y.W. and M.W.; Methodology, Z.W.; Project administration, Z.W.; Resources, Z.W. and R.Z. (Rongxin Zhao); Software, X.W., R.Z. (Rifeng Zhang), M.L., Y.L. and J.Q.; Supervision, Z.W.; Validation, Z.W.; Visualization, Z.W.; Writing—original draft, Z.W.; Writing—review and editing, Z.W. All authors have read and agreed to the published version of the manuscript.

Funding

This study was financially supported by the National Key Research and Development Program of China (2022YFC2903602) and the National Natural Science Foundation of China (Grant No. 41772061).

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

The datasets presented in this study can be obtained upon request to the corresponding author.

Acknowledgments

Constructive comments from the editors, and the revisions from three anonymous reviewers greatly improved the manuscript of this paper. We thank the team members at China University of Geosciences (Beijing) for their field support and comments.

Conflicts of Interest

The authors declare no conflict of interest.

Appendix A

Table A1. Major (wt.%) and trace element (ppm) compositions for dark enclaves and granitoids of the Dazeshan pluton.
Table A1. Major (wt.%) and trace element (ppm) compositions for dark enclaves and granitoids of the Dazeshan pluton.
Rock TypePorphyritic-like MonzograniteSyenodioritic Enclaves
SampleDZSD04B1DZSD04B2-1DZSD04B2-2DZSD04B3DZSD05B1DZSD06B2-1DZSD06B2-2DZSD06B2-3DZSD06B2-4DZSD06B2-5DZSD06B2-6DZSD14B1-1DZSD14B1-2DZSD14B1-3DZSD14B1-4DZSD14B1-5DZSD04B1(bt)DZSD04B2-1(bt)DZSD04B2-2(bt)DZSD05B1(bt)DZSD06B1(bt)
SiO269.0169.2768.6568.2570.0769.5470.1970.0169.156970.2570.871.5671.4470.9268.9654.3356.2456.7856.8454.25
TiO20.360.3270.3210.3120.2750.3210.280.3180.3230.2960.3290.2950.2620.3260.2850.3420.9931.020.8440.6980.94
Al2O315.1115.0215.3315.715.0314.8214.9714.8915.2515.4714.3314.3114.3913.9114.4915.2117.1817.6316.9816.9317.96
TFe2O32.692.372.332.262.092.471.982.352.42.192.622.351.982.412.192.598.657.097.146.868.02
MnO0.0370.0330.0310.0340.0290.0350.030.0370.0350.0320.0360.040.0350.040.0380.0430.1450.1030.1160.1270.133
MgO1.110.9750.9570.940.8731.010.830.9610.9960.8821.0910.7550.9920.9241.14.393.363.563.054.24
CaO2.622.42.262.442.282.292.172.52.482.242.792.452.172.372.352.554.524.694.483.814.85
Na2O3.553.513.53.713.643.493.393.83.743.63.853.633.663.53.643.714.675.414.673.824.57
K2O4.224.795.55.114.574.434.853.864.264.973.443.883.93.863.964.373.582.643.966.153.12
P2O50.1610.1360.1360.1340.1250.1370.1180.1330.1350.120.1520.140.10.140.1270.150.4820.4510.50.6710.622
LOI0.580.610.420.540.470.910.650.580.660.640.530.540.620.450.520.431.011.330.921.010.73
TOTAL99.44899.44199.43599.4399.45299.45399.45899.43999.42999.4499.41799.43599.43299.43899.44499.45599.9599.96499.9599.96699.435
Na2O/K2O0.8410.733 0.636 0.726 0.796 0.788 0.699 0.984 0.878 0.724 1.119 0.936 0.938 0.907 0.919 0.849 1.304 2.049 1.179 0.6211.465
Mg#42.442.342.342.642.742.242.842.242.541.842.643.140.542.342.943.147.545.847.144.248.5
A/CNK0.9950.979 0.968 0.976 0.995 1.007 1.012 0.993 0.997 1.005 0.946 0.977 1.013 0.975 0.995 0.982 0.868 0.868 0.843 0.8510.910
A/NK1.4501.369 1.307 1.348 1.373 1.405 1.381 1.426 1.415 1.367 1.424 1.405 1.403 1.398 1.409 1.402 1.485 1.499 1.417 1.3071.647
Li22.618.92020.119.8252024.921.72221.124.328.32221.626.87659.262.747.672.9
Be1.431.341.381.271.661.721.561.722.921.561.751.571.661.251.551.555.455.314.723.384.03
Sc4.123.583.663.453.574.873.413.454.663.534.113.882.913.633.814.262114.116.816.219.7
V33.73133.129.83637.1293034.428.930.132.721.440.744.834.4124102122124106
Cr17.815.615.714.413.319.613.215.217.615.41714.59.881615.118.913331.722.211.917
Co4.984.544.864.345.085.284.034.74.964.194.674.943.594.564.415.7821.716.317.315.420
Ni7.046.056.156.196.085.315.566.24.515.86.756.964.866.196.585.5930.420.813.310.122.8
Cu4.965.579.44.410.20.9514.394.70.944.274.594.944.215.354.691.187.599.5110.45.8623
Zn29.746.641.439.940.326.425.33028.225.72736.333.931.832.939.411798.510110397.6
Ga18.818.919.918.920.218.918.72019.818.518.320.219.117.617.319.433.931.530.127.134.5
Rb1081221371131331271221061231319510812294.4101105202162191216220
Sr593594638638590602632601632609523555451486564553454535442387544
Nb7.366.977.5176.859.527.447.639.77.187.597.547.588.717.869.042431.420.115.620.9
Mo0.280.9550.5980.4840.5770.0970.3930.3680.1670.2810.2840.3840.2760.3530.360.1850.3471.421.180.2890.705
Cd0.0510.0850.0850.0580.10.0280.0670.0570.0380.0560.0490.0640.080.070.1810.0180.0910.0930.0790.1340.1
In0.0160.0210.0170.0170.0170.0140.0130.0130.010.0140.0140.020.0160.0220.0230.0130.0650.050.0730.0740.073
Sb0.0270.3370.3730.3260.3070.030.040.0230.0340.0250.0150.0310.0170.0220.0210.0410.2820.3380.2360.2030.019
Cs1.271.31.611.111.571.91.431.341.571.221.40.9591.810.9530.8791.267.2765.713.767.24
Ba192621312842240320082161230416302228213211571170132012801779192669262911351413682
Ta0.6720.6560.7090.6320.6250.7250.7370.7110.8020.7320.7430.6920.6850.8840.7230.7711.742.951.361.091.4
W0.0910.0930.0920.130.5340.190.110.1920.160.220.1190.2080.2460.1780.160.1360.2640.2470.2270.2280.309
Tl0.5050.5580.6780.5940.580.6380.5950.520.5980.5980.4770.5050.6530.4740.4620.5961.251.011.061.121.08
Pb18.721.224.12423.921.52522.121.525.118.225.728.52125.126.414.413.416.531.614.5
Bi2.030.0270.0220.0210.0780.030.0240.0320.0330.0430.0220.040.030.0310.0360.0540.0440.0320.040.0590.045
Th12.69.8214.59.511112.710.510.812.910.4152911.212.511.712.834.520.519.123.922.2
U1.551.622.131.312.131.631.511.311.71.351.452.41.481.231.43213.98.125.431.863.59
Zr12.211.7118.299.5114.4121418.41812.525.226.413.314.313.430.352.548.76160.8
Hf0.6570.6040.6070.4670.6350.8790.660.8141.10.7920.7741.021.060.8140.7930.8971.581.831.551.621.89
La51.644.646.441.137.357.143.738.345.241.15854.436.14741.347.710070.7105154113
Ce98.889.487.978.372.19771.266.178.573.610691.363.283.769.581.5165145179260189
Pr9.227.978.567.197.019.937.676.958.438.1710.49.116.418.587.398.5917.62021.429.520.8
Nd30.326.7282522.234.926.72530.826.630.329.421.8282631.257.380.172.892.659.6
Sm4.173.924.223.753.394.663.853.674.514.024.364.143.284.193.974.167.613.29.9910.68.21
Eu0.9651.021.051.131.040.9711.10.9570.9571.211.021.020.7760.8510.9420.9841.352.481.741.611.49
Gd3.893.583.833.382.973.513.473.343.293.434.083.852.893.723.413.497.1710.38.9117.89
Tb0.520.4740.5220.4130.3960.4370.4630.4150.4440.4750.5140.4730.3770.470.4550.4840.8591.541.11.211.04
Dy2.452.352.441.951.981.962.061.982.12.372.452.271.692.282.062.043.867.084.885.084.82
Ho0.3460.3170.3440.2980.2850.3010.3190.3140.3550.3330.3260.3030.2510.3370.3010.3350.6221.20.7840.7340.693
Er1.141.021.070.9770.8230.9350.9921.051.041.091.081.140.8381.141.061.071.833.272.212.392.66
Tm0.1370.1370.140.1210.1150.1380.1360.1250.1610.1360.1420.1440.110.1550.1440.1460.3090.550.3730.3420.357
Yb0.9070.8260.8770.7950.7650.8230.8720.84710.9190.8690.9650.65610.9260.9272.093.372.42.332.32
Lu0.1270.1190.1270.1120.1070.1220.1260.1230.1340.1330.1310.1480.1030.1440.1380.1240.3210.4690.3470.3640.356
Y9.238.559.118.17.6110.28.628.6810.98.919.119.27.29.789.19.6919.235.623.522.921.7
ΣREE204.572182.433185.48164.516150.481212.787162.658149.171176.921163.586219.672198.663138.481181.567157.596182.75365.911359.259410.924571.76412.236
LREE195.055173.61176.13156.47143.04204.561154.22140.977168.397154.7210.08189.37131.566172.321149.102174.134348.85331.48389.93548.31392.1
HREE9.5178.8239.358.0467.4418.2268.4388.1948.5248.8869.5929.2936.9159.2468.4948.61617.06127.77920.99423.4520.136
LR/HR20.495 19.677 18.837 19.447 19.223 24.868 18.277 17.205 19.756 17.409 21.902 20.378 19.026 18.637 17.554 20.211 20.447 11.933 18.573 23.38219.473
LaN/YbN40.80838.73137.95137.80334.97449.76635.94732.43532.42232.07947.87540.43639.47333.71331.99236.91034.32115.04831.38247.4134.937
δEu0.7330.8320.7980.9701.0020.7340.9200.8360.7600.9960.7390.7810.7710.6590.7830.7900.5590.6500.5640.4560.566
Sr/Y64.247 69.474 70.033 78.765 77.530 59.020 73.318 69.240 57.982 68.350 57.409 60.326 62.639 49.693 61.978 57.069 23.646 15.028 18.809 16.925.069
Rb/Sr0.182 0.205 0.215 0.177 0.225 0.211 0.193 0.176 0.195 0.215 0.182 0.195 0.271 0.194 0.179 0.190 0.445 0.303 0.432 0.5580.404
Nb/La0.143 0.156 0.162 0.170 0.184 0.167 0.170 0.199 0.215 0.175 0.131 0.139 0.210 0.185 0.190 0.190 0.240 0.444 0.191 0.1010.185

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Figure 1. (a) Simplified tectonic map of East China illustrating the locations of Palaeo-Pacific subduction zone and Jiaodong Peninsula. Adapted with permission from [15]. (b) Simplified geological map of the Jiaodong Peninsula illustrating the major faults, large-scale Mesozoic magmatism, and typical gold deposits. Adapted with permission from [6]. Main faults: TLF, Tan-Lu Fault; WQYF, Wulian-Qingdao-Yantai Fault.
Figure 1. (a) Simplified tectonic map of East China illustrating the locations of Palaeo-Pacific subduction zone and Jiaodong Peninsula. Adapted with permission from [15]. (b) Simplified geological map of the Jiaodong Peninsula illustrating the major faults, large-scale Mesozoic magmatism, and typical gold deposits. Adapted with permission from [6]. Main faults: TLF, Tan-Lu Fault; WQYF, Wulian-Qingdao-Yantai Fault.
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Figure 2. (a) Geological map of the Dazeshan pluton, illustrating its location and relation with Linglong batholith. (b) Enlarged geological map of Dazeshan granitoids illustrating sample locations. (c,d) Contact between fine-grained biotite granite and porphyritic-like monzogranite. (e) Porphyritic-like monzogranite with megacrysts of K-feldspar. (f) Dark microgranular enclaves in host monzogranites. (g) Tabular enclaves with abrupt contacts with their host. (h) Oval dark enclaves containing K-feldspar megacrysts.
Figure 2. (a) Geological map of the Dazeshan pluton, illustrating its location and relation with Linglong batholith. (b) Enlarged geological map of Dazeshan granitoids illustrating sample locations. (c,d) Contact between fine-grained biotite granite and porphyritic-like monzogranite. (e) Porphyritic-like monzogranite with megacrysts of K-feldspar. (f) Dark microgranular enclaves in host monzogranites. (g) Tabular enclaves with abrupt contacts with their host. (h) Oval dark enclaves containing K-feldspar megacrysts.
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Figure 3. (a,b) Representative monzogranite samples for zircon LA-ICP-MS U-Pb dating and element analysis. (c) Euhedral to subhedral quartz, K-feldspar, plagioclase and biotite. (d) Subhedral K-feldspar with inclusions of biotite, plagioclase and quartz. (e) Representative fine-grained dark enclave sample for zircon LA-ICP-MS U-Pb dating and element analysis. (f) Fine-grained subhedral plagioclase, hornblende and quartz, K-feldspar and biotite. Mineral abbreviations: Pl: plagioclase, Qtz: quartz, Kfs: K-feldspar, Hbl: hornblende, Bt: biotite.
Figure 3. (a,b) Representative monzogranite samples for zircon LA-ICP-MS U-Pb dating and element analysis. (c) Euhedral to subhedral quartz, K-feldspar, plagioclase and biotite. (d) Subhedral K-feldspar with inclusions of biotite, plagioclase and quartz. (e) Representative fine-grained dark enclave sample for zircon LA-ICP-MS U-Pb dating and element analysis. (f) Fine-grained subhedral plagioclase, hornblende and quartz, K-feldspar and biotite. Mineral abbreviations: Pl: plagioclase, Qtz: quartz, Kfs: K-feldspar, Hbl: hornblende, Bt: biotite.
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Figure 4. Zircon LA-ICP-MS U-Pb concordia age diagrams and histograms of Dazeshan monzogranites (ad) and their enclaves (e,f). The insets show the typical zircon CL images with U-Pb apparent ages.
Figure 4. Zircon LA-ICP-MS U-Pb concordia age diagrams and histograms of Dazeshan monzogranites (ad) and their enclaves (e,f). The insets show the typical zircon CL images with U-Pb apparent ages.
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Figure 5. (a) Total alkali versus silica (TAS) diagram [61]. (b) K2O vs. SiO2 classification diagram [62]. (c) A/NK (molar Al2O3/(Na2O + K2O)) vs. A/CNK (molar Al2O3/(CaO + Na2O + K2O)) diagram [63]. (df) Harker variation diagrams show the correlations of Al2O3, MgO and CaO with SiO2. The data for middle Early Cretaceous granitoids (132–122 Ma) [64,65,66] and Late Early Cretaceous granitoids (118–110 Ma) [49,50] previously published are also shown on the Figures.
Figure 5. (a) Total alkali versus silica (TAS) diagram [61]. (b) K2O vs. SiO2 classification diagram [62]. (c) A/NK (molar Al2O3/(Na2O + K2O)) vs. A/CNK (molar Al2O3/(CaO + Na2O + K2O)) diagram [63]. (df) Harker variation diagrams show the correlations of Al2O3, MgO and CaO with SiO2. The data for middle Early Cretaceous granitoids (132–122 Ma) [64,65,66] and Late Early Cretaceous granitoids (118–110 Ma) [49,50] previously published are also shown on the Figures.
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Figure 6. Comparison of chondrite-normalized REE patterns between granitoids of the Dazeshan and their enclaves (a), Dazeshan granitoids and middle Early Cretaceous granitoids (132–122 Ma) (b), Dazeshan granitoids and late Early Cretaceous granitoids (118–110 Ma) (c), Dazeshan granitoids and high Ba–Sr granitoids (d), Dark microgranular enclaves and low-Ti (Lithospheric mantle-derived) lamprophyres (e), and Dark microgranular enclaves and high-Ti (Asthenospheric mantle-derived) lamprophyres (f). The published data for middle Early Cretaceous granitoids (132–122 Ma) are from [64,65,66], for Late Early Cretaceous granitoids (118–110 Ma) from [49,67,50], for high Ba–Sr granitoids from [24], and for low-Ti and high-Ti lamprophyres from [47].
Figure 6. Comparison of chondrite-normalized REE patterns between granitoids of the Dazeshan and their enclaves (a), Dazeshan granitoids and middle Early Cretaceous granitoids (132–122 Ma) (b), Dazeshan granitoids and late Early Cretaceous granitoids (118–110 Ma) (c), Dazeshan granitoids and high Ba–Sr granitoids (d), Dark microgranular enclaves and low-Ti (Lithospheric mantle-derived) lamprophyres (e), and Dark microgranular enclaves and high-Ti (Asthenospheric mantle-derived) lamprophyres (f). The published data for middle Early Cretaceous granitoids (132–122 Ma) are from [64,65,66], for Late Early Cretaceous granitoids (118–110 Ma) from [49,67,50], for high Ba–Sr granitoids from [24], and for low-Ti and high-Ti lamprophyres from [47].
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Figure 7. Comparison of primitive mantle-normalized spider diagrams between granitoids of the Dazeshan and their enclaves (a), Dazeshan granitoids and middle Early Cretaceous granitoids (132–122 Ma) (b), Dazeshan granitoids and late Early Cretaceous granitoids (118–110 Ma) (c), Dazeshan granitoids and high Ba–Sr granitoids (d), Dark microgranular enclaves and low-Ti (Lithospheric mantle-derived) lamprophyres (e), and Dark microgranular enclaves and high-Ti (Asthenospheric mantle-derived) lamprophyres (f). The published data for middle Early Cretaceous granitoids (132–122 Ma) are from [64,30,65,66], for Late Early Cretaceous granitoids (118–110 Ma) from [49,67,50], for high Ba–Sr granitoids from [24], and for low-Ti and high-Ti lamprophyres from [47].
Figure 7. Comparison of primitive mantle-normalized spider diagrams between granitoids of the Dazeshan and their enclaves (a), Dazeshan granitoids and middle Early Cretaceous granitoids (132–122 Ma) (b), Dazeshan granitoids and late Early Cretaceous granitoids (118–110 Ma) (c), Dazeshan granitoids and high Ba–Sr granitoids (d), Dark microgranular enclaves and low-Ti (Lithospheric mantle-derived) lamprophyres (e), and Dark microgranular enclaves and high-Ti (Asthenospheric mantle-derived) lamprophyres (f). The published data for middle Early Cretaceous granitoids (132–122 Ma) are from [64,30,65,66], for Late Early Cretaceous granitoids (118–110 Ma) from [49,67,50], for high Ba–Sr granitoids from [24], and for low-Ti and high-Ti lamprophyres from [47].
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Figure 8. (87Sr/86Sr)i vs. εNd(t) diagram for Dazeshan granitoids and their enclaves. Data sources: MORB [68]; Mafic dikes derived from lithospheric mantle (132–120 Ma) from [28,47,69]; Mafic rocks derived from asthenospheric mantle (107–78 Ma) from [34,70]; Neoarchaean-Neoproterozoic basement rocks in the Jiaobei Terrane from [71]; Neoproterozoic basement rocks in the Sulu Terrane from [38]; Triassic Shidao alkaline complex from [72]. CHUR: chondritic uniform reservoir; MORB: middle ocean ridge basalt; DM: depleted mantle.
Figure 8. (87Sr/86Sr)i vs. εNd(t) diagram for Dazeshan granitoids and their enclaves. Data sources: MORB [68]; Mafic dikes derived from lithospheric mantle (132–120 Ma) from [28,47,69]; Mafic rocks derived from asthenospheric mantle (107–78 Ma) from [34,70]; Neoarchaean-Neoproterozoic basement rocks in the Jiaobei Terrane from [71]; Neoproterozoic basement rocks in the Sulu Terrane from [38]; Triassic Shidao alkaline complex from [72]. CHUR: chondritic uniform reservoir; MORB: middle ocean ridge basalt; DM: depleted mantle.
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Figure 9. (a) Na-K-Ca and (b) Sr-Rb-Ba plots for the Dazeshan granitoids based on [16]. The published data for middle Early Cretaceous granitoids (132–122 Ma) [64,65,66,67] and Late Early Cretaceous granitoids (118–110 Ma) [49,50,68] are also shown in the Figures. Fields of low-Ba–Sr and high-Ba–Sr granitoids are from [76], and the field of adakite is from [17].
Figure 9. (a) Na-K-Ca and (b) Sr-Rb-Ba plots for the Dazeshan granitoids based on [16]. The published data for middle Early Cretaceous granitoids (132–122 Ma) [64,65,66,67] and Late Early Cretaceous granitoids (118–110 Ma) [49,50,68] are also shown in the Figures. Fields of low-Ba–Sr and high-Ba–Sr granitoids are from [76], and the field of adakite is from [17].
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Figure 10. Plots for the Dazeshan granitoids and their enclaves on the Greig diagram. Fields for liquid immiscibility are from [80,95].
Figure 10. Plots for the Dazeshan granitoids and their enclaves on the Greig diagram. Fields for liquid immiscibility are from [80,95].
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Figure 11. Ratios of REE elements (a) and trace elements (b) in dark enclaves to their corresponding host granitoids. Ranges for ratios of REE elements (a) and trace elements (b) in silicic liquid to those in mafic liquid are based on data from [80,89,93,94].
Figure 11. Ratios of REE elements (a) and trace elements (b) in dark enclaves to their corresponding host granitoids. Ranges for ratios of REE elements (a) and trace elements (b) in silicic liquid to those in mafic liquid are based on data from [80,89,93,94].
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Figure 12. Schematic tectonic model illustrating the generation of the high Ba-Sr Dazeshan granitoids and their dark enclaves (see text for details). Adapted with permission from [33,47,52]. MASH—melting, assimilation, storage, and homogenization; SCLM—subcontinental lithospheric mantle; SOB—Sulu orogenic belt; NCC—North China craton; YC—Yangtze craton; CC—continental crust; WQYF—Wulian-Qingdao-Yantai Fault; TF—Tan-Lu fault.
Figure 12. Schematic tectonic model illustrating the generation of the high Ba-Sr Dazeshan granitoids and their dark enclaves (see text for details). Adapted with permission from [33,47,52]. MASH—melting, assimilation, storage, and homogenization; SCLM—subcontinental lithospheric mantle; SOB—Sulu orogenic belt; NCC—North China craton; YC—Yangtze craton; CC—continental crust; WQYF—Wulian-Qingdao-Yantai Fault; TF—Tan-Lu fault.
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Table 1. LA-ICP-MS zircon U–Pb data of dark enclaves and host monzogranites of the Dazeshan pluton.
Table 1. LA-ICP-MS zircon U–Pb data of dark enclaves and host monzogranites of the Dazeshan pluton.
SpotConcentrations (ppm)Th/UU–Pb Isotopic RatiosAges (Ma)
PbThU207Pb/206Pb207Pb/235U206Pb/238U207Pb/206Pb207Pb/235U206Pb/238U
DZSD04B3-0172552920.90.0520.0040.1330.0110.0190.00024333172126101212
DZSD04B3-0281903240.60.0490.0030.130.0090.0190.00023167−4912481231
DZSD04B3-0362052590.80.0480.0030.1220.0090.0190.0002712214311781202
DZSD04B3-04112964490.70.0490.0030.1260.0070.0190.0002116712812061191
DZSD04B3-0562162450.90.0490.0030.1260.0080.0190.0002720013312171212
DZSD04B3-06103203850.80.0490.0030.1280.0070.0190.00025143−6412371222
DZSD04B3-07123124620.70.0490.0020.1240.0060.0180.000231329911951181
DZSD04B3-08102423970.60.0490.0020.1260.0070.0190.00023128−7912161201
DZSD04B3-0961522340.60.050.0040.130.0090.0190.0003117616312481232
DZSD04B3-10102614100.60.050.0030.1270.0080.0190.0002517614712271202
DZSD04B3-1172472720.90.0480.0040.1260.010.0190.0002710218512091212
DZSD04B3-1272672880.90.0460.0060.1150.0150.0180.000279296110141152
DZSD04B3-13112414440.50.0510.0120.1320.0290.0190.00074228456125261225
DZSD04B3-14231301750.70.0490.0090.6920.1190.1020.00131200302534716258
DZSD04B3-152613018591.50.050.0070.130.0190.0180.0002191315124171181
DZSD04B3-1681673420.50.0470.0050.1230.0130.0190.0002732222118121202
DZSD04B3-1761652720.60.0460.0040.1170.010.0190.000293318311291192
DZSD04B3-1873211700.50.0460.0040.1190.010.0190.00028301811491202
DZSD04B3-19382872661.10.0670.0030.9270.0350.10.0012483781666186157
DZSD04B3-20151182420.50.0560.0020.4160.0190.0550.00183435873531434511
DZSD04B3-2151162210.50.0530.0030.1330.0080.0190.000332414412771192
DZSD04B3-2261462660.50.050.0030.1270.0080.0190.0003118914512271192
DZSD04B3-23112784840.60.050.0020.1310.0050.0190.0002220910012551211
DZSD04B3-2461822600.70.0490.0030.1270.0070.0190.0003312812612161212
DZSD04B3-25563824990.80.0660.0020.7420.0190.0810.00087120049564115025
DZSD06B2-6-01201261291.00.0670.0021.030.0320.1130.0023835597191668813
DZSD06B2-6-0282053160.60.0530.0020.1390.0060.0190.0002734510213251222
DZSD06B2-6-0382623120.80.0490.0030.1260.0070.0190.0002513912812161202
DZSD06B2-6-04165276580.80.050.0020.1270.0040.0190.000181957512241181
DZSD06B2-6-0581823390.50.0470.0020.1220.0060.0190.000265010411751192
DZSD06B2-6-0661542390.60.050.0030.1250.0070.0190.0003618714612061192
DZSD06B2-6-0792173850.60.050.0030.1260.0060.0190.0003918713412061192
DZSD06B2-6-0871832820.60.0490.0030.1230.0070.0180.0003815413311861172
DZSD06B2-6-0951631870.90.0510.0040.1190.0090.0180.0004622017911481143
DZSD06B2-6-1081603920.40.0510.0030.1380.0070.020.0003522812213271252
DZSD06B2-6-1161282450.50.0520.0040.1330.0080.0190.0007828315612681235
DZSD06B2-6-1251641970.80.0490.0030.1270.0090.0190.0003515416812181182
DZSD06B2-6-1381823360.50.0470.0030.120.0070.0180.000275613311561182
DZSD06B2-6-14102914190.70.0510.0020.1340.0060.0190.0002725010612851222
DZSD06B2-6-1591552860.50.0460.0030.1170.0070.0190.00027614111371182
DZSD04B1-01453118850.050.0560.0030.2990.0140.0380.00054471100266112413
DZSD04B1-022213378031.70.0480.0020.1230.0050.0190.000271008911751182
DZSD04B1-0362412116522.50.1420.0630.1190.0370.0190.000442252852114341223
DZSD04B1-0431172110541.60.0530.0030.1420.0090.0200.0004933214713481263
DZSD04B1-0533190810551.80.0480.0050.1210.0130.0190.00082122231116121195
DZSD04B1-0641521710.90.0490.0070.1200.0170.0180.00035150315115151152
DZSD04B1-0752192071.10.0510.0080.1310.0200.0180.00036239315125181172
DZSD04B1-083015559461.60.0510.0130.1360.0360.0190.00022232513129321231
DZSD04B1-09139396401.50.0470.0070.1210.0180.0190.0003565324116161192
DZSD04B1-104881850.50.0510.0050.1260.0130.0190.00038243230121121192
DZSD04B1-1139185813621.40.0460.0020.1200.0060.0190.00022012211561201
Table 2. Rb-Sr and Sm-Nd isotopic results of host granitoids and dark enclaves from the Dazeshan pluton.
Table 2. Rb-Sr and Sm-Nd isotopic results of host granitoids and dark enclaves from the Dazeshan pluton.
SampleRock TypeRb
(ppm)
Sr
(ppm)
87Rb/86Sr87Sr/86Sr±2σ(87Sr/86Sr)iSm (ppm)Nd (ppm)147Sm/144Nd143Nd/144Nd±2σεNd(t)TDM2 (Ma)TDM (Ma)
DZSD04B1Monzo-granite1085930.527360540.7107140.0000190.7098146124.1730.30.0832018220.5114340.000018−21.75 2679 2000
DZSD04B2-11225940.5947191920.7107370.0000160.7097227353.9226.70.0887593710.5115350.000015−19.87 25271967
DZSD04B2-21376380.6217824450.7108380.0000160.7097775794.22280.0911158290.5115040.000009−20.51 2579 2042
DZSD04B31136380.5128570530.7106570.0000160.7097823473.75250.0906840.5115380.000021−19.84 2525 1993
DZSD05B11335900.6527369490.7108760.0000140.7097627883.3922.20.0923179460.5114680.000011−21.23 2637 2107
DZSD06B2-11276020.6108657810.7107910.0000140.7097491974.6634.90.0807234840.5115660.00001−19.14 2468 1813
DZSD06B2-21226320.5589607590.7107410.0000130.7097877193.8526.70.0871743820.5115370.000009−19.81 25221939
DZSD06B2-31066010.5107048250.7106380.0000210.7097670173.67250.0887494080.5115580.000009−19.42 2491 1937
DZSD06B2-41236320.5635424050.7107390.0000110.7097779054.5130.80.0885248570.5115420.00001−19.73 2516 1954
DZSD06B2-51316090.6228630540.7107770.0000160.7097147374.0226.60.0913658350.5115380.000008−19.85 2526 2005
DZSD06B2-6955230.5259694070.7106660.0000160.7097689844.3630.30.0869927920.5115290.00001−19.96 2534 1946
DZSD14B1-11085550.5634681080.7107990.0000180.7098380324.1429.40.0851319180.5115650.000013−19.23 2475 1876
DZSD14B1-21224510.7832886920.7106970.0000140.7093611383.2821.80.0909613210.51150.000018−20.59 2585 2044
DZSD14B1-394.44860.5624375310.7107420.0000160.7097827894.19280.0904680860.5115520.000017−19.56 2502 1973
DZSD14B1-41015640.5185382980.7107420.0000210.7098576573.97260.0923116620.5115240.000007−20.14 2549 2037
DZSD14B1-51055530.5497974680.7106770.0000160.7097393464.1631.20.0806080.5115780.000006−18.91 2449 1798
DZSD04B1(bt)enclaves2024541.2883506610.711740.0000140.7095427797.657.30.0801859690.5116140.000007−18.20 2392 1751
DZSD04B2-1(bt)1625350.8767985050.7110180.0000160.70952266213.280.10.0996278650.5114390.000014−21.91 26912280
DZSD04B2-2(bt)1914421.2512660630.7117920.0000110.7096580259.9972.80.0829609120.5116330.000011−17.87 2366 1766
DZSD05B1(bt)2163871.6161488370.7124820.0000170.70972573510.6092.60.0692044920.511470.000006−20.84 26051770
Note: εNd = [(143Nd/144Nd)S/(143Nd/144Nd)CHUR − 1] × 10000, fSm/Nd = (147Sm/144Nd)S/(147Sm/144Nd)CHUR − 1, tDM2 = (1/λSm)ln(1 + A), A = {(147Sm/144Nd)S − (147Sm/144Nd)DM − [(147Sm/144Nd)S − (147Sm/144Nd)C] (eλt − 1)}/[(147Sm/144Nd)C − (147Sm/144Nd)DM], (147Sm/144Nd)DM = 0.2136, (147Sm/144Nd)DM = 0.513151, (147Sm/144Nd)CHUR = 0.1967, (143Nd/144Nd)CHUR = 0.512638, (147Sm/144Nd)C = 0.118, t = crystallization age of zircon (120Ma), λSm = 6.54 × 10−12 year.
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Wang, Z.; Zhao, R.; Ye, T.; Wang, Y.; Wu, M.; Wang, X.; Zhang, R.; Li, M.; Liu, Y.; Qiao, J. Petrogenesis of Early Cretaceous High Ba-Sr Granitoids in the Jiaodong Peninsula, East China: Insights into Regional Tectonic Transition. Appl. Sci. 2023, 13, 1000. https://doi.org/10.3390/app13021000

AMA Style

Wang Z, Zhao R, Ye T, Wang Y, Wu M, Wang X, Zhang R, Li M, Liu Y, Qiao J. Petrogenesis of Early Cretaceous High Ba-Sr Granitoids in the Jiaodong Peninsula, East China: Insights into Regional Tectonic Transition. Applied Sciences. 2023; 13(2):1000. https://doi.org/10.3390/app13021000

Chicago/Turabian Style

Wang, Zhongliang, Rongxin Zhao, Tong Ye, Yu Wang, Mingchao Wu, Xuan Wang, Rifeng Zhang, Mingyun Li, Yabo Liu, and Jiahao Qiao. 2023. "Petrogenesis of Early Cretaceous High Ba-Sr Granitoids in the Jiaodong Peninsula, East China: Insights into Regional Tectonic Transition" Applied Sciences 13, no. 2: 1000. https://doi.org/10.3390/app13021000

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