- School of Geographic Science, Nantong University, Nantong, China
Abstract: The amalgamation of the Yangtze and the Cathaysia Block in Neoproterozoic time led to the formation of the South China Block (SCB) and generated the Jiangnan Orogen with the occurrences of juvenile magmatic rocks. After this orogeny, a typical collisional orogen formed during the early Paleozoic period in Southeast Asia which is mainly distributed in the Wuyi-Nanling-Yunkai area in the SCB. However, the transitional time from syn-collisional compression to post-collisional extension is debatable. Here, we present new data on zircon U-Pb zircon ages, Lu-Hf isotopes, and geochemistry for the Guzhang and Shadi granites from the Nanling area, South China. Both plutons have similar zircon 238U/206Pb ages of ca. 430 Ma. Petrographic and geochemical characteristics (e.g., FeOt/(FeOt+MgO) = 0.82–0.95) indicate that both granites are peraluminous A-type, with high Ga/Al ratios (2.43–2.91) as well as high concentrations of Zr, Nb, Ce, Y (sum values from 327 to 527 ppm), and formation temperature (820°C–845°C). Shadi granite exhibit high positive εHf(t) values (clustering within 0 to +6) while Guzhang granite show relatively lower εHf(t) values (−8.7 to −2.9). Their mildly negative to positive zircon εHf(t) values are higher than that of many coeval granites and can be derived from anhydrous melting of tonalitic genesis in the middle crustal depth, with the Shadi pluton having more orthometamorphite in the source. The ages and Hf isotopic compositions of inherited zircons (εHf(t = 960 Ma) = 9.2, εHf(t = 950 Ma) = 7.3) suggest that the Neoproterozoic juvenile magmatic rocks in the Jiangnan Orogen were a significant source for these granites. We interpret these A-type granites derived at the post-collisional stage. Their occurrence indicates that the geological setting of this Paleozoic orogen shifted from compression to extension no later than 430 Ma.
1 Introduction
A nearly 2000 km long and 450 km wide orogen formed in Southeast Asia during the Ordovician to Silurian periods (Figure 1; Charvet et al., 2010; Li et al., 2010; Zhao et al., 2022). This collisional belt was characterized by widely distributed regional metamorphic rocks (greenschist, amphibolites, and minor granulites) in the Wuyi-Nanling-Yukai area with ages ranging from 460 to 436 Ma (e.g., Shu et al., 2008; Charvet et al., 2010; Yu et al., 2014). The orogeny also caused angular unconformity between the Devonian and pre-Devonian strata. The origin of this early Paleozoic orogen was long timely debated from the early 1990s to the present (e.g., Ren et al., 1997; Lin et al., 2018; Wang et al., 2018). The main point of contention is whether the orogen formed with or without oceanic crust subduction. The lack of early Paleozoic ophiolites, magmatic volcanic rocks, subduction complexes, and high-pressure metamorphism was cited as evidence for intracontinental origin (Charvetet al., 2010; Li et al., 2010; Shu et al., 2014; Wang et al., 2013; Yao et al., 2012; Kong et al., 2021; Zhao et al., 2022). While the oceanic crust subduction model is supported by a few newly discovered arc-like rocks with ages from 445 to 430 Ma (Peng et al., 2006; Peng et al., 2016; Zhang et al., 2016; Lin et al., 2018). To our opinion, the lack of abundant volcanic rocks and detrital zircons with ages ranging from 520 to 460 Ma in the adjacent strata and river sands of South China (Xu et al., 2007) may further support the intra-continent model.
FIGURE 1. Age distribution map of early Paleozoic granitic rocks in South China Block. Most of the metamorphic and magmatic rocks are distributed in the WuYi-Nanling-Yukai area. The A-type granites (marked with ①∼④) are uncommon and have ages from 415 to 400 Ma. The Jiangshan-Shaoxing fault is thought to be the boundary between the Yangtze and the Cathaysia block at the Neoproterozoic time while the westward extension of the boundary is unclear(marked as the dotted lines in Figure 1A.
Despite this debate, the geological processes related to syn-collisional crustal thickening and post-collisional thinning were documented in this orogen. The time scale of the collisional events could be constrained by the ages of regional amphibolite-facies metamorphic rocks and gneissic S-type granites (e.g., 460–440 Ma, Li et al., 2010). While the approximate time when the region began to shift into an extensional geological setting is still under debate (e.g., Huang and Wang, 2019; Xin et al., 2020). Some previous studies suggested the hornblende bearing I-type granites and associated mafic rocks (442–430 Ma) were produced in an extensional setting caused by lithospheric delamination (e.g., Zhong et al., 2012; Zhang et al., 2015). For instance, Zhang et al. (2015) suggest an extensional tectonic regime has developed from the beginning of the Silurian (442 Ma) with the occurrence of Guiyang I-type granites and associated Dakang mafic-felsic intrusion. Others regarded the occurrence of the A-type granites (Figures 1, 400–415 Ma) as the mark of the extensional setting (Feng et al., 2014; Li et al., 2016b; Cai et al., 2017; Xin et al., 2020). The transitional time defined by the A-type granites (ca. 415 Ma) is incompatible with the timing defined by the I-type granites and the contemporaneous mafic rocks (ca. 435 Ma), which require urgent constraint.
In this study, we identified two new A-type granites with ages of 430 Ma in the Nanling region. This new finding, which is in agreement with the presence of I-type granites and contemporaneous mafic-felsic complex, suggests that the Wuyi-Nanling-Yunkai orogeny had changed from compressional setting to an extensional setting at least from 430 Ma.
2 Geological background and sample introduction
The South China Block has recorded two major orogenic events before the Carboniferous era: the Neoproterozoic Jiangnan orogeny and the Early Paleozoic Wuyi-Nanling-Yunkai orogeny (Zhao et al., 2022). The Jiangnan Orogen was formed at 1.0–0.82 Ga during the assemblage of the Yangtze and Cathaysia block (Yao et al., 2019) and is characterized by the occurrence of arc-related magmatic rocks with highly depleted Nd-Hf isotopes (Li et al., 2009). However, early Paleozoic mafic rocks in the Wuyi-Nanling-Yunkai orogeny have slightly enriched to moderately depleted Nd-Hf isotopes (Xu and Xu, 2017), and were suggested to be mainly derived from a lithospheric mantle that had been metasomatized by the Neoproterozoic subducted crustal materials (e.g., Wang et al., 2013). These rare mafic rocks have a total outcrop of ca. 50 Km2 (gabbros, with minor basalt and hornblende, Shu et al., 2020), with the ages varying from 443 to 400 Ma.
More than 200 Ordovician-Devonian granitic plutons have been found in the South China Block, with large proportions of S-, a few I- and minor A-type granites. These granitic rocks have zircon 238U/206Pb ages ranging from 464 to 381 Ma (e.g., Zhang et al., 2010; Huang et al., 2013; Cai et al., 2017) and made up the vast majority proportion of the magmatic rocks during the orogeny. The S- type granites have zircon 238U/206Pb ages from 464 to 401 Ma (e.g., Huang and Wang, 2019), and the I-type granites have zircon 238U/206Pb ages from 442 to 381 Ma (e.g., Zhao et al., 2013; Xu and Xu, 2015). Only four A-type granitic plutons have been reported, with zircon 238U/206Pb ages from 415 to 400 Ma (Feng et al., 2014; Li et al., 2016b; Cai et al., 2017; Xin et al., 2020).
The newly identified A-type granites, including two plutons named Guzhang and Shadi, are located in the middle part of the early Paleozoic Wuyi-Nanling-Yukai orogeny (Figure 2). The Guzhang granite has an outcrop of ca. 208 km2 and Shadi granite has an outcrop of ca. 54 Km2. The Guzhang and Shadi granitic pluton intruded into the Cambrian and Neoproterozoic basement rocks. The Cambrian rocks are mainly composed of quartz greywacke and carbonaceous slates and the Precambrian rocks are composed of tuffaceous sandstone. Hornfels is found in the granites and basement rocks contact zone.
FIGURE 2. Geological map of the two A-type granitic plutons in this study. Both plutons intruded into the Neoproterozoic to Cambrian strata and have fault contact with the younger wall rocks.
The Guzhang pluton is mainly porphyritic biotite granite with minor two mica granite (Figures 3A–F). The phenocrysts are composed of plagioclase and K-spar, with 2–4 cm in length (Figure 3). It contains K-spar (33%–44%), plagioclase (20%–25%), quartz (20%–25%), biotite (5%–9%) and muscovite (2%–4%). The K-Spars are plate-shaped, dominated by micro-plagioclases, followed by perthites (Figure 3E). Lattice twinning and striped twinning are developed in those feldspars. Plagioclases are characterized by polysynthetic twinning (Figure 3C). The perthites and interstitial biotites indicate that crystallization occurred under anhydrous and high-temperature conditions (Philpotts, 1990). The accessory minerals are mainly zircons, apatites, Fe-Ti oxides with minor fluorite, and tourmaline. The Shadi granite is mainly composed of fine to coarse-grain biotite granite with a porphyritic texture (Figures 3G–I). The phenocrysts are composed of coarse gain (0.5–2 cm) plagioclase, K-spar and minor quartz with middle to fine grain (<3 mm) plagioclase (25%–31%), K-spar (25%–30%), quartz (20%–25%), biotite (6%), muscovite (2%) as matrixes. The perthites and interstitial biotites are also developed in this pluton. The accessory minerals are mainly zircons, apatites, and Fe-Ti oxides. We collected 12 samples from Guzhang and Shadi pluton for whole rock analysis and five samples for the zircon U-Pb dating and Lu-Hf isotopic analysis.
FIGURE 3. Photos from the field and thin sections for samples collected at the Guzhang (A–F) and Shadi granites (G–L). The typical porphyritic structure can be seen in the hand specimen (B). Perthites and interstitial biotites are common in both plutons. Abbreviation: Bi= Biotite; Q = Quartz; Kf = K-feldspar; Pl = Plagioclase; Mu = Muscovite; Chl= chlorite.
3 Analytical methods
3.1 Zircon U-Pb dating
Zircon grains were isolated using density and magnetic separation techniques. Zircons were mounted into an epoxy resin disk and polished to expose their surfaces. After photographing in both reflected and transmitted light, CL (cathode luminescence) imaging was taken by a JSM6510 SEM attached to a Gatan CL detector. Zircon U-Pb isotopic analyses were carried out on the transparent zircons without fracture or mineral inclusion using a Thermo X2 ICP-MS housed at the Testing Center of Shandong Bureau of China Metallurgical Geology Bureau, Jinan, Shandong province. The mounted zircon grains were ablated using an attached Coherent Geolas Pro 193 nm laser ablation system with a spot diameter of 30 μm. Ablation occurred in intervals of ten sample zircons, directly preceded and followed by two 91,500 standard zircons and one artificial glass 610. The analyzed results of the 91,500 fall into the ranges of the long-term test values of the Lab, with the uncertainty of 1.5% (1 RSD) for most of the 206Pb/238U measurement and are listed in Supplementary Table S1. Detailed instrument conditions and data acquisition have been described by Li et al. (2016a). The ICPMSDataCal 8.0 (Liu et al., 2010) was used to select offline raw data, integrate background and analytical signals, and time drift correct and quantitative calibrate U-Pb isotopes. The common lead correction was made following the method of Anderson (2002). The age distributions are visually compared using probability density plots (PDPs; Ludwig, 2003). Weighted average age calculation was made using Isoplot 3.23 (Ludwig, 2003).
3.2 Whole rock major and trace element geochemistry
All samples were prepared by crushing them in an agate shatter box. Major elements were analyzed using an Axios 4.0 X-ray fluorescence spectrometer (XRF) at the Testing Center of Shandong Bureau of China Metallurgical Geology Bureau, Jinan, Shandong province, following the procedures described by Franzini et al. (1972), with analytical precision better than 1%. Rare earth elements and other trace elements from the rocks were analyzed using ICP-MS (Thermo Fisher icap Q) techniques at the Testing Center of Shandong Bureau of China Metallurgical Geology Bureau, Jinan, Shandong province. The precisions for most elements are better than 5% (1SE).
3.3 Zircon Lu-Hf isotopic composition
Zircons Hf isotope analyses were carried out using a Neptune Plus MC-ICP-MS equipped with a GeoLas Pro193 nm laser at MiDeR, Nanjing University. The diameter is 44 μm with a pulse rate of 10 Hz, and beam energy of 5 J/cm2. Only zircon grains with concordant ages and suitable sites for Hf analyses were analyzed. The zircon standard 91,500 was analyzed during the analytical session, which yielded a176Hf/177Hf ratio of 0.282310 ± 9 (N = 34). The calculation of εHf (t) value and TDM used the following parameters: λLu = 1.867 × 10−11 a−1 (176Lu/177Hf) CHUR = 0.0336 and (176Hf/177Hf) CHUR = 0.282785, (176Lu/177Hf) DM = 0.0384 and (176Hf/177Hf) DM = 0.28325 (Griffin et al., 2000). The average crustal 176Lu/177Hf value used for TDM calculations is 0.015 (Griffin et al., 2002).
4 Results
4.1 Zircon U-Pb ages and Lu-Hf isotopic composition
4.1.1 Guzhang granite
Zircons from the Guzhang pluton are euhedral, with long axis lengths from 100 to 200 μm, and aspect ratios from 1:2–1:4. These zircons have clear fine magmatic oscillation zones, which is a typical feature of zircon in the felsic rocks (Figures 4E, F e.g., Shu et al., 2011). Sixteen zircon grains were analyzed from sample 9653. Four of the results are discordant and one grain is inherited zircon. These zircons have low Th, U concentrations (<500 ppm), with Th/U ratios from 0.13 to 1.05, and are of magmatic origin (Hoskin and Schaltegger, 2003). Eleven zircon grains yield a weighted average 206Pb/238U ages 424 ± 6 Ma (Figure 4A, MSWD = 2.9, 2σ). The 206Pb/238U age of the inherited zircon is 950 ± 18 Ma. Most zircons from sample 9605 have Th/U ratios larger than 0.3, which indicates these zircons are of magmatic origin. Except for one inherited zircon have the 206Pb/238U ages of 654 ± 17 Ma, other zircons yield a concordant weight average 206Pb/238U ages of 435 ± 6 Ma (Figure 4B, n = 17, MSWD = 0.49, 2σ).
FIGURE 4. Zircon U-Pb dating Concordia diagrams (A-E) and representative cathode luminescence photos (F). The small red circle is the zircon U-Pb analysis position and the big blue circle is the position of Lu-Hf isotope analysis.
Zircon Hf isotopes from both samples of Guzhang pluton have similar values (Figure 5). The zircon εHf(t) values from sample 9605 are concentrated from −8.7 to −3.9 (n = 17), with a peak value close to −5. The TDM2 ages (two-stage model ages relative to the depleted mantle) are from 1.63 to 1.95 Ga. The inherited zircon from 9605 has εHf(t = 654 Ma) value of −0.2 ± 0.6. The zircon εHf(t) values from sample 9653 have more narrow ranges, varying from −6.7 to −3.0 (n = 15), with a peak value close to −4, corresponding to the TDM2 ages from 1.60 to 1.81 Ga. The inherited zircon from 9653 has εHf(t = 950 Ma) value of 7.3 ± 0.5.
FIGURE 5. Zircon Hf isotopic composition from Guzhang and Shadi plutons. The ranges of the εHf(t) values for other granitic rocks (B) are from Huang and Wang et al., 2018; A-type granites are from Xin et al., 2020. Because the mafic rocks generally lack zircons, the εHf(t) values of mafic rocks are recalculated from the data source in Shu et al., 2021 by assuming the Nd-Hf isotopes are coupled (εHf=1.36∗εNd+3; Vervoort et al., 1999). The Nd-Hf relationship of early Paleozoic magmatic rocks was discussed by Xia et al., 2014.
4.1.2 Shadi granite
Zircon samples 8953–1, 8953–4, and 8953–6 were analyzed from the Shadi pluton. The zircon grains in the Shadi granites from all samples are euhedral with clear fine magmatic oscillation zones. The grain sizes vary from 100 to 200 μm with an aspect ratio from 1:2 to 1:4. Most of the zircons have Th/U ratios from 0.2 to 0.6. which indicates they are of magmatic origin. We analyzed 16 grains with U-Pb and Lu-Hf isotopes for each sample. The concordant weighted average 206Pb/238U ages for those samples are 427 ± 6 Ma (Figure 4C, 8953–6, n = 15, MSWD = 0.3, 2σ), 431 ± 4 Ma (Figure 4D, 8953–4, n = 15, MSWD = 0.11, 2σ), and 432 ± 3 Ma (Figure 4E, 8953–1, n = 15, MSWD = 0.063, 2σ). Only one inherited zircon was found in sample 8953–6, with the 206Pb/238U ages of 960 ± 14 Ma.
Zircon Lu-Hf isotopes in the three samples have similar peak values (Figure 5). Except for one grain have εHf(t) of −12 ± 0.8, other zircons from sample 8953–1 have εHf(t) values ranging from −5.5–5.7 (n = 15), with a peak of 1, corresponding to the TDM2 ages of 1.03–1.75 Ga. Two zircons in 8953–4 have lower εHf(t) of −7.1 ± 0.8 and −7.5 ± 0.6, while other Zircons in 8953–4 have εHf(t) values concentrated from −0.9 to 5.2 (n = 13), with peak value close to 1, corresponding to the TDM2 ages of 1.06–1.45 Ga. All zircon in 8953–6 has εHf(t) values concentrated from −2.5 to 6.3 (n = 15), with a peak close to 2, corresponding to the TDM2 ages of 0.98–1.56 Ga. The inherited zircon from sample 8953–6 has εHf(t = 960 Ma) values of 9.2 ± 0.6.
4.2 Major element geochemistry
The Guzhang granite is characterized by high SiO2 (71.14–74.07 wt%), FeOt (2.35–4.37 wt%), K2O (3.90–4.64 wt%), Na2O (2.67–3.02 wt%), moderate P2O5 (0.14–0.24 wt%), Al2O3 (13.04–13.71 wt%) and low CaO (0.37–0.81 wt%), MgO (0.52–0.62 wt%) contents (Supplementary Table S1, Figure 6). It shows strongly peraluminous character, with obvious high ASI values which range from 1.21 to 1.38. Samples from the Guzhang granite were plotted in the calcic-alkalic ferroan A-type field due to the high FeOt/(FeOt + MgO) ratios (0.82–0.88) (Figure 7; Frost and Frost, 2011). The Shadi pluton has SiO2 contents that range from 66.76 to 75.07 wt%, with lower FeOt (1.32–3.44 wt%), CaO (0.44–0.54 wt%), moderate P2O5 (0.12–0.22 wt%) and higher K2O (4.30–6.14 wt%) and Na2O (2.92–5.02 wt%) contents. The Shadi granite has mildly high ASI values (1.12–1.22) and also belongs to the peraluminous series. It has FeOt/(FeOt+MgO) values varying from 0.85 to 0.95, slightly higher than the Guzhang granites. Both Guzhang and Shadi plutons have obvious high FeOt/(FeOt+MgO) values and low Cao and MgO contents compared with coeval granitic rocks in the orogeny at the same SiO2 (Figures 6A,B,D).
FIGURE 6. Harker diagrams for representative major (A-E) and trace elements (F-H) from the Shadi and Guzhang plutons.The coeval magmatic rock samples from the Nanling area are also plotted for comparison and the detailed data are listed in the appendix in Shu et al., 2021.
FIGURE 7. Compositional trends of melts from partial melting experiments on quartzofeldspathic rocks. (A) ASI [aluminium saturation index; Al/(Ca −1.67P+Na+K)] vs. SiO2; (B) Na2O+K2O-CaO vs. SiO2 (C) (FeOtotal)/(FeOtotal +MgO) vs. SiO2. Modified from Frost and Frost, 2011. The colored area in figure b and c is the same as marked in Figure A.
4.3 Trace elements and REEs
Samples from Guzhang have higher concentrations of high-field-strength elements (HFSEs, e.g., Nb, Zr, Figures 6F,G) when compared with other coeval granites in the Nanling area (Xu and Xu, 2015). Primitive mantle normalized spider diagrams exhibit strong enrichment in Rb, Th, U, and Nd as well as clear negative anomalies in Ba, Nb, Sr, P, Eu, and Ti. The Rare earth element (REE) abundances vary from 152 to 212 ppm with light REE enrichment, significant negative Eu anomalies, and flat-sloping heavy REE patterns (Figures 8A, B). Samples from the Shadi have similar trace element features with the Guzhang granite, which are featured by the enrichment of HFSEs and depletion of Ba, Nb, Sr, Eu, and Ti. The total REEs of Shadi granites have larger variations than that of Guzhang granites, from 67 to 254 ppm. It also shows strong negative Eu abnormally on the chondrite normalized REEs patterns (Figures 8C, D). The heavy depletion of Eu, Ba, and Sr in both plutons indicates that the feldspars played a significant role during the magma generation, either as residuals in the source or as fractionated minerals.
FIGURE 8. C1-Chondrite normalized REE patterns (A–C) and primitive mantle normalized alteration resistant trace element pattern (B–D) for the samples from the Guzhang and Shadi plutons. Chondrite and primitive mantle compositions are from Sun and McDonough (1989).
5 Discussions
5.1 Genesis type
The majority of granites can commonly be classified as I-, S-, or A-types based on mineral combinations and geochemical characteristics (Bonin, 2007). Chappell and white (1974) divided the granites in the Lachlan fold belt into I- and S-type. The I-type granites are characteristic of low SiO2 contents, ASI values (normally <1.1), depleted isotopes (e.g., Sr, Nd, Hf), and the appearance of hornblendes, derived from mainly meta-igneous rock sources. The S-type granites are featured by high ASI values (normally >1.1), enriched isotopes with the appearance of garnet and/or cordierite, and are suggested to be mainly derived from meta-sedimentary rocks. It is worth noting that the mineralogical and geochemical characteristics mentioned above are not solid standards for the classification of granite types. For example, aluminum-rich minerals such as primary garnet can also be found in weak peraluminous and even meta-aluminous granites (Chappell, 1999). The geochemical characteristics of A-type granites differ from those of I- and S-type granites (e.g., high contents of HFSEs and Ga/Al ratios), and the geochemical parameters used to define A-type granite are unambiguous. (Loiselle and wones, 1979; Eby, 1990; Creaser et al., 1991; Bonin, 2007).
Even the high ASI values and the existence of biotite and minor muscovite are similar to the future of some typical S-type granites (Bonin, 2007), the high formation temperatures, FeOtot/(FeOtot+MgO) ratios, and limited inherited zircons (3 inherited zircons of 76 grains) and other features that will be discussed next preclude the S-type origin. The most noticeable characteristics of Guzhang and Shadi plutons are as follows: 1) high FeOtot/(FeOtot+MgO) ratios and ASI values (Figures 6, 7); 2) low contents of Al2O3, CaO, MgO (Figure 6); 3) mildly negative to positive Zircon Hf isotopic composition (Figure 5B); 4) high HFSEs concentrations and Ga/Al ratios; 5) the occurrences of interstitial biotites and perthitic microcline; 6) lack of inherited zircons. The FeOt/(FeOt+MgO) ratios of samples from both plutons are plotted in the ferroan A-type granites field (Figure 7C, defined by 175 A-type granites worldwide; Frost et al., 2001) and are distinguishable compared with the magmatic rocks that formed during 460–400 Ma in Nanling area (Figure 6B). Most of the samples were plotted near or in the field of A-type granites on different chemical diagrams because of the high HFSEs concentrations and 10,000*Ga/Al ratios (Figure 9).
FIGURE 9. Chemical classification diagrams for granites: (A) (FeOt/MgO) vs. (Zr + Nb+ Ce + Y); (B) (K2O+ Na2O) vs 10,000 Ga/Al; (C) Nb vs. (Zr + Nb + Ce + Y); (D) Rh/Sr vs. (Zr + Ce + Th) (Whalen et al., 1987 and Cámera et al., 2017). FG: Fractionated granites; OGT: unfractionated M-, I- and, S-type granites.
Besides the distinct A-type granite geochemical features, these two plutons also have high Zr saturation temperatures. The Guzhang granite has whole rock Zr saturation temperatures from 820°C to 840°C (Supplementary Table S1, M[(Na + K + 2*Ca)/(Al*Si)]=1.1–1.2; Watson and Harrison, 2005) and four of six samples from the Shadi granite (M=1.2–1.4) have temperatures from 813°C to 845°C (Figure 10A). The other two low-temperature samples (ca. 750°C) from the Shadi pluton have the highest SiO2 and lowest Zr (68 and 80 ppm) and Ti contents, which may cause by fractional crystallization. The zircon Ti thermometry is also used to calculate the zircon crystallization temperature. A new correction of Ti in zircon temperature calculation was made by Schiller and Finger (2019), and they suggest the zircon temperatures in most A-type granites were underestimated. The zircons from Guzhang and Shadi granite have saturation temperatures from 700°C to 1000°C and 700°C–950°C, respectively (Figure 10B). Combined with the occurrences of interstitial biotites and perthitic microcline, it may be concluded that both plutons evolved under anhydrous conditions at high temperatures. All of the aforementioned characteristics suggest that these two granitic plutons are ferroan A-type.
FIGURE 10. Calculated temperatures for samples and zircons from the Guzhang and Shadi plutons. Figure (A) is the Zr saturation temperature calculated from whole rock geochemistry. Figure (B, C) are the temperatures calculated from the Ti concentrations in zircons.
5.2 Origin of the two peraluminous A-type granites
There is no consensus on the origin of the A-type granites, especially on the source (Bonin, 2007). Even Frost and Frost (2011) suggested using the term “Ferroan granites” instead of “A-type granites” for some reason, the term “A-type granite” is still more popular than the “Ferron granites” nowadays. The main petrogenetic models for the A-type granite include 1) Partial melting of lower crust rocks that had been granulitized during an earlier thermal event (Collins et al., 1982; Feng et al., 2014); 2) Direct differentiation from the mantle-derived basaltic magma (Frost and Frost, 2011; Girei et al., 2019; Jiang et al., 2022); 3) Partial melting of the quartzofeldspathic rocks (Patiño Douce, 1997; Bogaerts et al., 2006; Kong et al., 2018; Li et al., 2018a; Li et al., 2018b; Li et al., 2018c); 4) Magma mixing from anatectic granitic and mantle-derive mafic magmas (Dahlquist et al., 2010; Cámera et al., 2017).
The granulite model with pre-extraction of I-type granitic melt was argued by some scholars for such melts would have low Fe/Mg and (Na2O+K2O)/Al2O3 ratios that differ from typical A-type granites (e.g., Creaser et al., 1991; Frost and Frost, 2011; Jiang et al., 2022). However, some studies suggested that the early Paleozoic A-type granites in the Wuyi-Nanling-Yunkai orogen were derived from mainly granulitic rock sources, such as granulitic meta-igneous rocks (Cai et al., 2017), granulitic meta-sedimentary rocks (Feng et al., 2014) or granulite that had extracted S-type granitic magma (Xin et al., 2020). The main reason is due to the low water affinity of the granulite which seems as a suitable source for the anhydrous A-type magmas. We are not intended to connect the Guzhang and Shadi plutons with the granulite source, since it is not a necessary factor to generate the A-type granites (Creaser et al., 1991; Skjerlie and Johnston, 1993).
The Guzhang granite has negative zircon εHf(t) values (−8.7—−3.0) that are unlikely derived from a coeval mantle-derived mafic magma (Figure 5B). The Shadi granite has higher εHf(t) values that overlap with the ranges of coeval mafic rocks, which can be derived from the differentiation of the basaltic rocks isotopically (Figure 5B). However, A-type granites that derived from differentiation of the basaltic magma are generally metaluminous and commonly found in association with mafic intrusions (Mccurry et al., 2008). Both Guzhang and Shadi plutons are peraluminous and not found to be associated with mafic intrusion or mafic enclaves. Thus, they are not likely derived from the direct fractionation of mafic magmas. Besides, zircon εHf(t) values from both plutons have large ranges, up to 10 ε units. The large ranges in zircon εHf(t) are either caused by magma mixing (Griffin et al., 2002) or by disequilibrium melting during the crustal anataxis (Tong et al., 2021). The magma mixing model is not favored here because mafic magmas mostly have low ASI values (<0.8) and the magma produced by pure mixing can hardly achieve the strong peraluminous affinity of our samples, while source mixing is more plausible.
Partial melting of mainly quartzofeldspathic rocks during crustal anataxis is a possible way to generate the A-type granites (Frost and frost, 2011). For instance, dehydration melting of F-rich tonalitic gneiss at mid-crustal pressures can generate strong peraluminous A-type granites (Figure 7; Skjerlie and Johnston, 1993). The Guzhang granite has mildly negative εHf(t) values (−8.7—−3.0), which are higher than most coeval granitic plutons, especially the typical S-type granites (εHf(t) = −34.2—−0.2; n=963, median = −8.4; Xin et al., 2020) and also the Neoproterozoic basement rocks in the west Wuyishan area. (Figure 11). Thus, it is unlikely derived from a source that is dominated by old metasedimentary rock. Zircon from the Shadi pluton has positive εHf(t) values up to +6.3, indicating that it originated from the partial melting of more immature source rocks rather than sedimentary source rocks.
FIGURE 11. εHf(t) vs ages (Ma) diagrams. The Neoproterozoic data is from Li et al., 2009; Chen et al., 2009. The ranges of Neoproterozoic basement rocks in the west Wuyishan area are from Xin et al. (2020). Both plutons are not likely derived from the old basement rocks for the higher εHf(t) values. The Shadi granites can be mainly derived from a source similar to the Neoproterozoic juvenile tonalitic rocks in the eastern Jiangnan Orogen while the Guzhang granites have a mixed source with more old crustal materials.
The Neoproterozoic juvenile rocks in the Jiangnan Orogen, like the tonalitic to rhyolitic magmatic rocks from Shuangxiwu and Pingshui area, seem a good candidate as the source of these A-type granites (Chen et al., 2009; Li et al., 2009). Neoproterozoic inherited zircons with depleted Hf isotopic characteristics were found in the Shadi (εHf (t=960 Ma) = 9.2 ± 0.6) and the Guzhang pluton (εHf (t=950 Ma) = 7.3 ± 0.5), both of which occur within the ranges of zircons from the tonalitic rocks at the eastern Jiangnan Orogen (Figure 11; Li et al., 2009). Besides, the Beiwu volcanic rocks with tonalitic composition (See Supplementary Table S2 in Li et al., 2009) have major elements similar to the starting materials used in the dehydration melting experiment in Skjerlie and Johnston, 1993. Thus, the dehydration melting of source rocks that are similar to the juvenile tonalitic rocks from the east Jiangnan Orogen can generate peraluminous Shadi A-type granite, geochemically and isotopically. Therefore, we suggest these two peraluminous granitic plutons were most likely formed by the dehydration melting of Neoproterozoic juvenile tonalitic rocks with minor metasedimentary rocks at medium crust pressure, with the source of Guzhang granite containing more old metasedimentary rocks (Figure 12).
FIGURE 12. The schematic cartoons showing the tectonic evolution of SCB and the generation of the A-type granites in this study. The amalgamation of the Yangtze and the Cathaysia Block in Neoproterozoic time generated intermediate to felsic magmatic rocks with depleted Nd-Hf isotopic features (A). This amalgamation was followed by a post-orogenic extension which is recorded by A-type granites and other rift-related mafic rocks (B), Yao et al., 2019). However, after 760 Ma, the magmatism in SCB was limited (C). Some magmatic rocks and metamorphic rocks were identified in SCB with the ages from 470 to 445 Ma and regarded as products of the continental collisional stage (D). Large volumes of magmatic rocks were formed at the extensional stage (430–400 Ma) after the delamination of the thickened crust and upper lithospheric mantle (E).b
5.3 Tectonic implication
The orogeny of this early Paleozoic belt was first recognized by the mass distributions of the regional metamorphic rocks (greenschist, amphiboles, and minor granulites, Figure 1). Systematic geochronology studies of those metamorphic rocks were formed at 460–436 Ma (Yu et al., 2005; Yu et al., 2014; Li et al., 2010; Tong et al., 2021). The occurrence of high-pressure metamorphic rocks revealed crustal thickening events in the belt (Li et al., 2010; Yu et al., 2014; Tong et al., 2021). The crustal thickening events were mainly suggested to be triggered by continental collision (Charvet et al., 2010; Li et al., 2010; Yao et al., 2012; Wang et al., 2013; Shu et al., 2014; Kong et al., 2021; Zhao et al., 2022). The youngest metamorphic zircon U-Pb ages from the Yiyang granulite are at ca. 435 Ma (Yu et al., 2014) and this age may mark the end of the collision event since no metamorphic rocks with younger ages have been reported. However, the accurate transformational age of this belt from compression to extension is still debated.
A-type granites had long been recognized as derived at extensional settings (e.g., Collins et al., 1982; Forst and Forst, 2011). In collisional orogens, syn-collisional crustal thickening has been followed by delamination of substantial amounts of mantle lithosphere at the post-collisional stage (Davies and von Blanckenburg, 1995). The post-collisional extension provides a suitable environment for hot mafic magma upwelling and also the heat for melting the source rocks of A-type granites (Jiang et al., 2022). Thus, the formation ages of A-type granites are often suggested to be the time that the region changes into a strongly extensional geological background. A-type granites in SCB have previously been dated between 415 and 400 Ma, hence it was hypothesized that the Wuyi-Nanling-Yunkai orogeny transitioned from syn-orogenic crustal thickening to a post-orogenic thinning at 415 Ma. (e.g., Xin et al., 2020).
However, most studies considered the hornblende bearing I-type granites (e.g., Guiyang granite formed at 442 Ma, Zhang et al., 2015) and coeval mafic rocks (e.g., Chayuanshan high Mg basalts formed at 435 Ma, Yao et al., 2012) were produced in an extensional setting that caused by lithospheric delamination. Huang and Wang (2019) also suggested that the occurrence of massive high-K calc-alkaline I-type granites in the Xuefengshan area can exemplify the transitional period from compression to extension, with the ages of ca. 430 Ma. Besides, the gneissic S-type granites in the belt mainly have a peak age of 440 Ma, and massive S-type granites have a peak age of 430 Ma. Those massive S-type granites were also suggested to be derived during the orogenic collapse stage (Feng et al. (2014). The ages of Shadi and Guzhang A-type granites in this study are consistent with the conclusion from the S-, I- type granites and the coeval mafic rocks. Thus, we suggest that the setting of Wuyi-Nanling-Yunkai orogen had changed from compression to extensional at least at ca. 430 Ma, which is 15 Ma earlier than the previous conclusion from A-type granites.
6 Conclusion
1) We identified two new peraluminous granites in the Wuyi-Nanling-Yunkai orogen, South China. These two plutons have high FeOt/(FeOt + MgO), Ga/Al ratios, and HFSEs concentrations with low CaO and MgO contents as well as high formation temperature, and are fitted with the affinities of A-type granites.
2) LA-ICP-MS zircon U-Pb dating results indicate the Shadi granite and the Guzhang granite were formed at 430 ± 5 Ma. Both granites can be formed by partial melting of mainly Neoproterozoic juvenile meta-tonalitic rocks at medium crust pressure while the source of Guzhang granite contains more old crustal materials. The Neoproterozoic juvenile tonalitic rocks in Jiangnan Orogen might be a significant source for the A-type granites.
3) This new finding suggests the geological setting of the Nanling area in the Wuyi-Nanling-Yunkai orogeny changed from collision to post-collisional extension no later than 430 Ma.
Data Availability Statement
The original contributions presented in the study are included in the article/Supplementary Material, further inquiries can be directed to the corresponding author.
Author contributions
X-JS, writing-original draft preparation, WJ sampling, experiment, data calculation. DW, supervision, review. CC and HW, discussion, editing, language.
Funding
This work was supported by financial support from the National Natural Science Foundation of China (41802063).
Acknowledgments
We thank Dehong Du and Jiangwei Zhang for the Discussions.
Conflict of interest
The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.
Publisher’s note
All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.
Supplementary material
The Supplementary Material for this article can be found online at: https://www.frontiersin.org/articles/10.3389/feart.2023.1137157/full#supplementary-material
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Keywords: orogenic magmatism, A-type granite, early Paleozoic, Southeast Asia, geological setting
Citation: Shu X-J, Jiang W, Wang D, Cheng C and Wang H-Z (2023) Origin and implication of two newly identified peraluminous A-type granites in the early Paleozoic orogeny, Southeast Asia. Front. Earth Sci. 11:1137157. doi: 10.3389/feart.2023.1137157
Received: 04 January 2023; Accepted: 01 February 2023;
Published: 10 February 2023.
Edited by:
Hossein Azizi, University of Kurdistan, IranReviewed by:
Huan Li, Central South University, ChinaDan-Ping Yan, China University of Geosciences, China
Copyright © 2023 Shu, Jiang, Wang, Cheng and Wang. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
*Correspondence: Xu-Jie Shu, eGpzaHVAbnR1LmVkdS5jbg==