1. Introduction
Prydz Bay in East Antarctica is renowned for its role in deciphering the Earth’s tectonic evolution during the Precambrian. This region has experienced both the Grenvillian orogeny (~1000 Ma) tectono-thermal event and the Early Paleozoic Pan-African (~530 Ma) tectono-thermal event. There are varying opinions on the P-T trajectory of the metamorphic process, with some proposing that it comprises two distinct high-grade metamorphic events [1,2,3,4,5,6,7,8,9]. Two contradictory perspectives exist regarding the tectonic attributes of the two metamorphic events in the Prydz belt. The clockwise P-T trajectory of the tectonic belt suggests the occurrence of a Pan-African collisional orogenic process. The Prydz belt is directly linked to the ultimate convergence of the East Gondwana paleocontinent during the early Paleozoic [1,10,11,12,13,14,15,16,17,18,19,20,21]. The Prydz belt is a complex metamorphic belt that underwent several metamorphic stages, with the Grenville metamorphism being the most prominent. This metamorphism is linked to the collisional orogenic event that occurred during the formation of the Rodinia supercontinent. Similarly, Pan-African metamorphism is considered the result of the intracontinental adjustment effects of the East Gondwana collisional orogeny [6,22,23,24,25,26,27,28,29,30,31,32,33,34].
The Larsemann Hills experienced significant magmatic activity and intense crustal melting activity around 500 Ma, prompting a comprehensive investigation into their crustal evolution [35,36]. During Pan-African magmatic activity, a notable abundance of granitic rocks formed, exhibiting high differentiation and originating from the crystallization of residual magmas with increased volatility [37,38,39,40,41,42]. It is essential to emphasize that pegmatites can achieve complete crystallization and differentiation only under specific conditions [42]. This holds particular significance during petrogenesis and mineralization, aiding in the identification of material sources and the understanding of geotectonic evolution [43].
The Larsemann Hills are defined by the presence of numerous coarse-grained, light-colored pegmatite veins. These pegmatites were formed at different stages during the Larsemann Hills’ deformational history and are found either as flat bodies or as separate lenses that generally occupy structurally controlled positions, such as at fold hinges, in shear zones, and at boudin necks [2]. It is necessary to further strengthen the comprehensive correlation analysis among pegmatite veins, country rocks, and their tectonic context. Previous studies on the absolute age, and isotopic composition of Pan-African pegmatites are rare. This research focuses on Pan-African pegmatites in the Larsemann Hills, employing lithological and geochemical analyses. LA-(MC)-ICP-MS techniques are utilized for zircon dating, trace element analysis, and Lu-Hf isotope analysis. Through these studies, the pegmatite formation process can be effectively elucidated, shedding light on the nature of deep melting host rocks, clarifying the genesis of zircons in pegmatites, constraining the time of anatexis, and exploring the diagenetic relationship between the metamorphic evolution of Pan-African ultra-high-temperature rocks in the Larsemann Hills [7]. Additionally, examining the formation age and magmatic genesis of Pan-African pegmatites in the Larsemann Hills can provide a better understanding of the magmatic activity and structural features of Prydz Bay.
2. Geological Background
The Larsemann Hills, located in Prydz Bay, East Antarctica, constitute one of the three bedrock outcrops in the area (Figure 1). These hills are vital for the study of the late Precambrian high-grade metamorphic terrane of the region [44,45,46]. The terrain encompasses high amphibolite facies to granulite facies to psammitic and pelitic paragneiss, along with a small quantity of pyroxene-bearing mafic granulite and leucogranitic orthogneiss [6,41,46,47].
The Brattstrand paragneiss stands as the primary rock formation, comprising various metasedimentary units. Within these units, certain types are recognized for their high levels of boron (B), exemplified by tourmaline quartzite and a suite of borosilicate minerals like grandidierite, kornerupine, and tourmaline [3,49,50]. This paragneiss exhibits significant features of partial melting, resulting in the formation of diverse gneiss and migmatites that feature mixtures of sillimanite and cordierite [2,5,18,24,36,51]. The Søstrene orthogneiss, primarily composed of a mafic–felsic magmatic complex, is typically preserved in pelitic granulite in lens-, lentil-, and sausage-shaped forms. Following its peak in metamorphism, an actual occurrence of deep melting took place, leading to the formation of multiple pegmatites, migmatites, and garnet-containing granites. These occurrences were distributed among syenite granites and monzonitic granites [6,24,52] (Figure 1). The granite is syn- and post-tectonic, and the elongated rock aligns with the overall distribution of gneiss in the surrounding rock where it is emplaced [12,53].
The distribution of the different rock types has a NE–SE direction. Most of the sequence is represented by metamorphic lithotypes. The primary tectonic line in the Larsemann Hills follows a NEE–SWW direction, while the eastern Mirror peninsula aligns NNW–SSE, forming a complex compound syncline that wraps in a NEE direction [54]. Wang’s [55] research categorizes the deformation in the Larsemann Hills into four phases. The first phase of regional deformation (D1) occurred during the Grenvillian orogeny associated with the peak metamorphic event (M1). The second phase of deformation (D2) resulted in tightly closed asymmetric folds. The third phase of deformation (D3) exhibited significant tensor ruptures that cut through the asymmetric folds formed in D2. Subsequently, magma intruded along tensional fracture surfaces, creating granite veins. Finally, in the D4 stage, a set of nearly equidistant and densely arranged upright broken cleavages developed (Table 1).
3. Analytical Methods
3.1. Major and Trace Elements
The samples were subjected to dissolution in a mixture of HNO3 and HF. Major element analyses were performed using X-ray fluorescence (XRF), while the analysis of trace elements was performed utilizing a Perkin-Elmer Sciex Elan 6000 ICP-MS instrument [56]. All experiments were carried out at the laboratory of Hebei Regional Geology and Mineral Resources Survey and Research Institute, China (Langfang, China).
3.2. Zircon U-Pb Dating
The samples were crushed by conventional methods, and zircons were subsequently separated using a conventional flotation method. Zircon particles with bipyramidal–prismatic and transparent properties were handpicked under a binocular lens for further analysis. The chosen zircon grains were affixed to double-sided adhesive and, after undergoing the epoxy resin fixation, curing, and surface polishing process, were subjected to zircon micrography and cathodoluminescence photography. Cathodoluminescence (CL) imaging on the zircon grains was performed using a JEOL scanning electron microscope (SEM) equipped with a Gatan CL detector (Oxford, UK) at Nanjing Hongchuang Geological Exploration Technology Service Co., Ltd. in China (Nanjing, China). U-Pb zircon geochronology was carried out using laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) at Beijing Createch Test Technology Co., Ltd. in China (Beijing, China). Laser sampling utilized an ESINWR 193 nm laser ablation system, and ion signal intensity was determined using an Anlyitik Jena PQMS Elite ICP-MS instrument, 91500, and GJ-1 was used as the standard materials for calibration, with operating conditions consistent with Zong et al. [9]. All errors were reported within 1 standard deviation (σ). Offline raw data selection and integration of background and analyte signals, as well as time drift correction and quantitative calibration for U-Pb dating, were performed using ICPMSDataCal (V10. 0) [57]. Age calculations and concordance plots were generated using Isoplot /Ex_ver3 [58].
3.3. Zircon Lu-Hf Isotope Analysis
Laser ablation multi-collector inductively coupled plasma mass spectrometry (LA-MC-ICPMS) was employed for the in situ analysis of zircon Hf isotopes at the State Key Laboratory of Geological Processes and Mineral Resources, China University of Geosciences (Wuhan). The analyses were carried out using Neptune Plus MC-ICP-MS in combination with a GeoLas 2005 ArF-excimer laser ablation system (German Thermo Fisher Science, Dreieich, Germany).
4. Petrography and Mineralogy
Five samples were collected from various locations (Figure 1), including granitic pegmatite (Z1220-23-2) and plagioclase pegmatite (Z1218-6) from Broknes Peninsula, syenite pegmatite (Z1229-42-4) from Mirror Peninsula, plagioclase pegmatite (Z1230-45-2) from Manning Island, and granitic pegmatite (Z1231-50-1) from Stornes Peninsula.
The granitic pegmatite (Z1220-23-2) outcrop, with a gray-white appearance, spans tens of centimeters, displaying a penetrating invasion (Figure 2a). The primary rock-forming minerals include quartz (30%–35%), K-feldspar (20%–25%), plagioclase (20%–25%), biotite (~10%), and magnetite (~5%). K-feldspar displays a self-shaped and semi-self-shaped plate-column structure (Figure 2b), with Carlsbad twinning. In contrast, plagioclase exhibits a plate-columnar shape and polysynthetic twinning. The quartz structure is irregularly granular with wavy extinction. Biotite is distributed within the pores of other minerals, exhibiting a relatively high degree of self-shaping. The plagioclase pegmatite (Z1218-6) outcrop is a few tens of centimeters wide, is light yellow, and forms a vein of penetrating intrusion (Figure 2c), surrounded by semi-pelitic gneiss. The primary rock-forming minerals are plagioclase (70%–75%), quartz (20%–25%), microcline (5%–10%), garnet (~5%), and biotite (~2%). Feldspar and garnet appear as large crystals, typically exceeding 5 mm. Plagioclase shows obvious polysynthetic twinning, while microcline exhibits apparent tartan twinning. Additionally, small black mica particles are distributed in the interstices of other minerals as sheets (Figure 2d).
The syenite pegmatite (Z1229-42-4) is exposed over a width ranging from tens of centimeters to several meters. It exhibits a flesh-red color and forms a vein throughout the intrusion. The surrounding rock consists of pelitic gneiss (Figure 2e), characterized by coarse-grained minerals with varying granulometry mostly exceeding 3 mm, displaying a medium–coarse-grained texture and massive structure. The primary rock-forming minerals include K-feldspar (70%–75%), quartz (20%–25%), garnet (~10%), biotite (~5%), and sillimanite (~2%). K-feldspar is euhedral and semi-euhedral plate-columnar, with Carlsbad twinning. Notably, and a substantial number of fibrous sillimanite crystals develop in the contact zone between K-feldspar and garnet (Figure 2f).
The granitic pegmatite (Z1231-50-1) is exposed over a width of approximately 4 m, appearing grayish-white and predominantly lenticular in shape. It intrudes along the loose parts between pelitic gneiss layers (Figure 2g). Most minerals exhibit a highly crystalline structure, with uneven sizes, typically larger than 3 mm. Plagioclases display a medium-grained texture and an overall massive structure. The principal rock-forming minerals include microcline (60%–65%), quartz (20%–25%), plagioclase (20%–25%), biotite (~5%), and magnetite (~2%). Tartan twinning is observed in microcline, and plagioclase with polysynthetic twinning is abundant. Quartz occurs as irregular grains with obvious wavy extinction (Figure 2h).
The exposed width of the plagioclase pegmatite (Z1230-45-2) spans tens of meters, and the rock sample from the outcrop appears reddish due to weathering. Plagioclases, affected by weathering, take on a reddish color, which can be mistaken for K-feldspar in the field. These plagioclases are layered and intrude along the softer portions of the interlayer (Figure 2i), with psammitic gneiss as the enclosing rock. The minerals display a large geometric form, a uniform grain size, mostly 5 mm, and massive structures. The primary rock-forming minerals are plagioclase (60%–65%), microcline (20%–25%), quartz (15%–20%), biotite (~5%), garnet (~5%), and magnetite (~2%). The most representative mineral plagioclase is lamellar and columnar with a polysynthetic twin (Figure 2j).
5. Results
5.1. Major and Trace Elements
The samples Z1229-42-4 and Z1230-45-2 plot the intersection between the Shoshonite and high K (calc-alkaline) series’ fields (Table 2; Figure 3a). The remaining samples (Z1220-23-2, Z1218-6, and Z1231-50-1) fall into the Shoshonite series field. The aluminum saturation index (A/CNK) for all the samples falls within the range of the aluminum saturation series (Figure 3b). The results from the standard mineral calculations indicate the presence of standard corundum molecules (Table 2), classifying all pegmatites as peraluminous magmatic rocks.
The samples show a strong differentiation in the distribution of rare-earth elements (REEs), with clear differentiation between light and heavy REEs’ separation (Figure 4a). The plagioclase pegmatites, specifically Z1218-6 and Z1230-45-2, exhibit less-enriched light rare-earth elements (LREEs), with a notable positive Eu anomaly. The normalized values for the Eu anomaly are 3.94 and 6.90, respectively, determined by using the ratio of 2EuN/(SmN + GdN) [62] (Figure 4a). In the case of samples Z1220-23-2, Z1229-42-4, and Z1231-50-1, the chondrite-normalized REE patterns highlight a negative Eu anomaly. This suggests that the granitic melt underwent crystallization and separation, resulting in a highly evolved magmatic system. In the primitive mantle-normalized trace element plot, the high-field-strength elements (HFSE) such as Ba, Nb, Sr, P, and Ti are depleted, while elements like Rb, K, Th, and U, known as large-ion lithophile elements (LILE), appear to be more abundant (Figure 4b). This implies that the source material could be from ancient island arc material [62].
5.2. U-Pb Geochronology and Hf Isotope Systematics
5.2.1. Zircon U-Pb Ages
The zircons from the granitic pegmatite (Z1220-23-2) have well-defined shapes, appearing as either short or long columns with a length of approximately 50 μm along the length/width ratio, ranging from 1:1 to 3:1. Cathodoluminescence (CL) examination reveals internal oscillatory zoning in magmatic zircons, and some zircons contain slight core inclusions (e.g., 28 and 35) (Figure 5a). CL images do not show evidence of fluid action in the process and later stage of zircon crystallization [65]. Thirty U-Pb dating analyses were conducted on the zircon grains, including 11 white zircons with ages ranging from 615 to 1116 Ma, showing dispersed ages of 206Pb/238U. These zircons are considered inherited grains derived from the surrounding rocks during pegmatite crystallization. The inherited zircons experienced Pb losses after the Pan-African tectono-thermal events, resulting in their distribution in beads on the concordia diagram [6,24,33,66]. The newly formed magma zircons exhibit a distinct light gray color and show prominent growth zoning, with the weighted average age of 206Pb/238U at 517 ± 4 Ma (MSWD = 0.057, n = 9) (Figure 6a, Table 3).
The zircons found in the plagioclase pegmatite (Z1218-6) exhibit predominantly round or columnar shapes, with a length ranging from about 80 to 150 μm along the length/width ratio of 1:1–2:1. Cathodoluminescence (CL) images reveal a lack of developed zircon growth zones (Figure 5b). The color of the zircons is grayish black, and some zircons exhibit tiny cores. A total of 68 analyses were performed on the zircon grains. Among them, 24 zircons are distributed in a string of beads (Figure 6c), with individual 206Pb/238U ages ranging from 524 to 850 Ma. In CL imaging, these zircons generally appear dark, and the banding is not apparent, indicating that they are inherited grains derived from the surrounding rocks during pegmatite crystallization, while Pb loss is explained to a certain extent by the influence of the Pan-African events. According to the concordia diagram for 206Pb/238U and 207Pb/235U, the weighted average age of 206Pb/238U is determined to be 521 ± 4 Ma (MSWD = 1.4, n = 25) (Figure 6c,d, Table 3).
The zircons in the syenite pegmatite (Z1229-42-4) exhibit irregular and incomplete shapes, with diameters ranging from approximately 50 to 150 μm. Cathodoluminescence (CL) images reveal the development of oscillatory zoning in zircon particles (Figure 5c). Most zircons display darker cores and lighter edges. A total of 35 analyses were conducted on zircon grains, and 16 zircon ages exhibit a bead-like distribution (Figure 6e), with 206Pb/238U ages ranging from 535 to 988 Ma. The darker cores and the lack of apparent banding in CL imaging suggest the inherited nature of these grains was derived from the surrounding rocks during crystallization, with some Pb loss due to the influence of the Pan-African events. For the 206Pb/238U and 207Pb/235U ages’ concordia diagram, the weighted average age of 206Pb/238U is determined as 534 ± 7 Ma (MSWD = 0.63, n = 19) (Figure 6e,f, Table 3).
In the granitic pegmatite (Z1230-50-1), zircons are observed as granular or columnar, with particle sizes ranging from 100 to 200 μm and a length/width ratio of 1:1–3:1. Cathodoluminescence (CL) images show that some zircon grains exhibit a nucleus–edge structure, featuring a wide inherited nucleus and a slight accretive edge (Figure 5d). Most zircons are lighter, displaying pronounced oscillatory bands and darker edges. A total of 44 U-Pb measurements were conducted on zircon grains, and the 206Pb/238U and 207Pb/235U ratios exhibit good concordance (Figure 6g, Table 3). The weighted average age of the 206Pb/238U peak in the zircon core is 546 ± 6 Ma (MSWD = 0.076, n = 15) (Figure 6h). The 206Pb/238U age of the zircon accretive edge ranges from 463 to 534 Ma, indicating apparent traces of fluid action during later stages, likely representing the new metamorphic edge of pegmatite zircon after the transformation of subsequent thermal events.
Most of the zircons found in the plagioclase pegmatite (Z1230-45-2) exhibit a round shape, with sizes ranging from approximately 80 to 150 μm. Cathodoluminescence (CL) images reveal that the oscillating bands of zircons are not clearly apparent, and inclusions are developed in most zircon cores. The color of the core is lighter, while the color of neogenic zircons is darker. The images indicate signs of fluid alteration during and after the crystallization of zircons (Figure 5e). A total of 44 U-Pb measurements were performed on zircon grains. The concentrated age of new magmatic zircons without Pb loss is 562 ± 6 Ma (MSWD = 0.076, n = 20) (Figure 6i,j, Table 3). The zircon core exhibits a beaded age distribution, suggesting that the zircon core was influenced by the superposition of late tectonic-thermal events. This influence is primarily attributed to varying degrees of resetting from both the Pan-African tectonic-thermal events and Grenville tectonic-thermal events.
All the zircons of the five samples (ΣREE, ppm) exhibit LREE depletion and the left-dip characteristics of HREE enrichment (Figure 7a–e). The majority of surveyed sites have zircons that display obvious negative Eu anomalies and positive Ce anomalies, and most have test data with Th/U values between 0.1 and 1 (Table 4), indicative of magmatic zircon characteristics. In the zircon-type discrimination diagram, most zircons within the pegmatites fall within the range associated with magmatic zircons–alteration zircons (Figure 8a,b) [67].
5.2.2. Lu-Hf Isotopes in Zircon
In the sample Z1220-23-2, the εHf(t) values are negative and range from −15 to −1, with a corresponding tDM2 range of 2202–2453 Ma. In the case of Z1218-6, the εHf(t) ranges from −2.13 to 6.32, with its corresponding tDM2 falling between 1101 and 1619 Ma. Z1230-42-4 exhibits εHf(t) values from −0.46 to −16.52, and its corresponding tDM2 ranges from 1528 to 2534 Ma. For Z1230-50-1, the εHf(t) is negative (−7.46 to −11.67), and the corresponding tDM2 falls within the range of 1975–2211 Ma. Finally, in the case of Z1230-45-2, εHf(t) ranges from −9 to −3, and its corresponding tDM2 is within the range of 1738–2092 Ma (Figure 9 and Table 5).
6. Discussion
The nature of the Prydz Pan-African tectonic belt remains a subject of debate due to research limitations on the unified East Gondwana landmass. There are conflicting opinions among researchers, with some suggesting that it is a collisional orogenic belt [11,13,16,19,20,21]. Others express concerns about the lack of direct indicators for specific facies, such as ophiolites, island arc accretion complexes, and high-pressure metamorphic rocks [24,26,29,34].
Based on the trace element composition of Pan-African pegmatites in the Larsemann Hills (Figure 6, Table 1), it is evident that pegmatite samples from the D2–D4 stage are enriched in large-ion lithophile elements (LILE) and depleted in high-field-strength elements (HFSE). The scarcity of P and Ti reflects the separation and crystallization of apatite and Ti-rich minerals. The loss of Nb and Ta may be linked to the separation and crystallization of rutile, or it could be attributed to crustal material contamination in the source area. Samples Z1220-23-2, Z1229-42-4, and Z1231-50-1 exhibit moderate negative Eu anomalies, potentially connected to separate plagioclase crystallization. In contrast, samples Z1230-45-2 and Z1218-6, being plagioclase pegmatites, show varying degrees of positive Eu anomalies.
The pegmatites in the Larsemann Hills studied in this paper are characterized as peraluminous and contain minerals such as garnet that also exhibit peraluminous characteristics. A comprehensive analysis reveals that the residual phases in the pegmatites are plagioclase and garnet. Plagioclase becomes unstable when the pressure exceeds 1.5 GPa [69]. Therefore, the formation pressure of the pegmatites is inferred to be less than 1.5 GPa, corresponding to a magmatic depth of less than 40 km [70]. The results indicate that the five samples are classified as I- and S-type granites (Figure 10a) and fractionated I-, S-, and M-type granites (Figure 10b) [71], aligning with volcanic arc granites (VAG) and syn-collisional granites (syn-COLG) (Figure 11a). They are linearly projected near the boundary between volcanic arc granite (VAG) and syn-collisional granite (syn-COLG) (Figure 11b) [72].
Zircon, a key mineral for U–Pb geochronology, is a stable mineral [74,75], and its Lu-Hf isotopes are extensively used in geochemical studies to understand the origin of magma and specific magmatic processes. Previous studies have shown that the genesis of magmatic rocks has two modes: (1) the partial melting of preexisting crustal material, in which the εHf(t) value of the zircons in magmatic rocks is lower than that in chondrite; (2) new crustal material or partially melted mantle material, in which the zircon εHf(t) value of magmatic rocks is higher than that of chondrite [9]. This provides conclusive evidence for identifying source areas [76]. The tDM2 age of zircon can offer a more precise reflection of the average retention age of the source material [77].
These features indicate a magmatic origin for the investigated zircons based on their shape, CL images, REE distribution patterns, and Th/U ratios. According to the zircon U-Pb data of the analyzed samples, it can be inferred that the Pan-African pegmatites in the Larsemann Hills formed at least 519–562 Ma, predating the emplacement of Progress granite at 514–516 Ma [12]. The chronological order of the formation of geological units, as indicated by the zircon U-Pb ages in this study, is consistent with the field investigation results reported by [78] and Ren (personal communication). Therefore, it is unlikely that the genesis of the Larsemann Hills’ Pan-African pegmatites is the result of the differentiation and crystallization of Progress granitic magma, Lines 370–372, from the petrographic descriptions and field relations; some pegmatites contain sillimanite and contact with metapelites, indicating a possible origin as a result of partial melting of the metapelites. The 176Lu/177Hf ratios of all zircons are less than 0.002, indicating that zircons have accumulated less radiogenic Hf during the evolution process after rock body formation. Thus, the zircon 176Lu/177Hf ratio can be used to elucidate genetic information during rock body formation [79]. Additionally, the fLu/Hf values range from −1.00 to −0.94, smaller than the fLu/Hf values of silico-aluminous crust (−0.72) and the fLu/Hf values of mafic crust (−0.34) [76]. Therefore, the TDM2 age more clearly reflects the time when the source material was obtained from the depleted mantle.
In the granitic pegmatite (Z1220-23-2) and the plagioclase pegmatite (Z1218-6) of the D4 phase of the Larsemann Hills, the εHf(t) values of zircons in the granitic pegmatite (Z1220-23-2), which formed at ~517 Ma(D4-2), range from −15.27 to −11.39, indicating values lower than chondrite (Figure 9). The granitic pegmatite (Z1220-23-2) primarily originates from the reworked Brattstrand paragneiss [78], and its corresponding tDM2 is 2202 to 2453 Ma, suggesting a partial provenance relationship with the Paleoproterozoic crust. The εHf(t) values of the zircons in the plagioclase pegmatite (Z1218-6), formed at ~521 Ma(D4-2), range from −2.13 to 6.32. The positive εHf(t) values indicate the presence of juvenile zircons. Their corresponding tDM2 is 1101–1619Ma, indicating that the plagioclase pegmatite (Z1218-6) is derived from a magma formed by the mixing of Mesoproterozoic crust-derived magma and mantle-derived magma. The εHf(t) values of zircons from the ~534 Ma granitic pegmatite (Z1229-42-4), formed in the D3 stage, range from −16.52 to −0.46. Although all εHf (t) values are negative, there is extensive variation. The corresponding tDM2 is 1528–2534Ma, indicating that granitic pegmatite (Z1229-42-4) primarily results from the partial melting of Paleoproterozoic crustal material. In the granitic pegmatite (Z1230-50-1) formed at 562 ± 6 Ma (the D2 stage) in the Larsemann Hills, the zircon εHf(t) of the granitic pegmatite (Z1230-50-1) ranges from −11.67 to −7.52 (Figure 9). The corresponding tDM2 is 1975–2211 Ma, suggesting that the granitic pegmatite (Z1220-50-1) primarily results from the partial melting of Paleoproterozoic crustal material. In the plagioclase pegmatite (Z1230-45-2), formed at 546 ± 6 Ma(D2), the εHf(t) value of the zircons in the plagioclase pegmatite (Z1230-45-2) ranges from −9.20 to −3.43, indicating a lower value than that of chondrite in both the zircon U-Pb age and εHf(t) diagrams. The corresponding tDM2 is 1738–2084 Ma, suggesting that the plagioclase pegmatite (Z1230-45-2) primarily originates from the partial melting of Paleoproterozoic ancient crustal material. It is inferred that the D2–D4 pegmatites have multiple different source areas, with D2–D3 pegmatites mainly derived from Paleoproterozoic crustal material. The D4-stage pegmatite exhibits characteristics of both Paleo–Mesoproterozoic crustal material sources and mantle material sources. The D4-1 pegmatite (~521 Ma) suggests both Paleo–Mesoproterozoic crustal and mantle origin. This aligns with the formation age and structural attributes of the Pan-African post-collisional granite in Prydz Bay [12]. The D4-2 pegmatite (~517 Ma) originates from the crust layers.
Combining rock geochemical and zircon characteristics, the Pan-African pegmatites in the Larsemann Hills likely originated from the Pan-African high-grade tectonic mobile belt of the Gondwana paleocontinent (Figure 12a), forming the D2–4 stage pegmatites (562–517 Ma). This was followed by lithospheric thinning (Figure 12b). These results provide new insights into the origin of pegmatites in the D2–D4 stage and effectively confirm the presence of a critical Gondwana paleocontinental extension zone near Prydz Bay.
7. Conclusions
Based on petrography, U-Pb geochronology, Lu-Hf isotopes, and major and trace element data on the pegmatites from the Larsemann Hills, the following conclusions were obtained:
According to geological and geochronological data, the pegmatites in the Larsemann Hills formed during the Pan-African D2–D4 stage. The D2 pegmatite formed between 546 and 562 Ma, the D3 pegmatite around 534 Ma, and the D4 pegmatite between 517 and 521 Ma. These pegmatites were formed during the Pan-African tectono-thermal event in an environment marked by an extension. It is plausible that a prominent breakup zone may be situated near the Larsemann Hills.
The Pan-African-period pegmatites discovered in the Larsemann Hills have different sources of material. Pegmatites from the D2–D3 period are considered to primarily originate from Paleoproterozoic crustal materials. In contrast, pegmatites from the D4-1 stage (~521 Ma) have sources from both Paleo–Mesoproterozoic crustal material sources and mantle material sources. Pegmatites from the D4-2 stage (~517 Ma) have sources that originated from the crust layers.
Conceptualization, S.Z. and Y.C.; methodology, S.Z.; software, S.Z.; validation, Y.C. and L.R.; formal analysis, S.Z.; investigation, S.Z., H.Z., S.C. and W.W.; resources, Y.C.; datacuration, S.Z.; writing—original draft preparation, S.Z.; writing—review and editing, Y.C., L.R. and S.L.; visualization, S.Z.; supervision, Y.C.; project administration, Y.C.; funding acquisition, Y.C. All authors have read and agreed to the published version of the manuscript.
Data is contained within the article.
The authors declare no conflict of interest.
Footnotes
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Figure 1. The geological map of the Larsemann Hills, Prydz Bay, East Antarctica, and the sample locations show major lithological units [6,24,28,33,48]. Insert shows the position of the Larsemann Hills in Prydz Bay. Abbreviations: LH (Larsemann Hills), AIS (Amery Ice Shelf), VH (Vestfold Hills), RI (Rauer Islands), RG (Rauer Group), DG (Dalkoy granite), MKG (Munro Kerr granite), PG (Progress granite), LG (Landing granite), AG (Amanda granite).
Figure 2. Field photographs (a,c,e,g,i) show the relationships between pegmatite and their surrounding rocks; microphotographs (b,d,f,h,j) show the contact relationship between rock-forming minerals. The mineral abbreviations is: Qtz (quartz), Bi (biotite), Kfs (K-feldspar), Pl (plagioclase), Grt (garnet), Mgt (magnetite), Mc (microcline).
Figure 3. K2O-SiO2 ((a) solid line after Peccerillo and Taylor, 1976 [59]; dashed line after Middlemost, 1985 [60]) and A/CNK-A/NK ((b), A/NK = Al2O3/(Na2O + K2O), A/CNK = Al2O3/(CaO + Na2O + K2O) after Maniar and Piccoli, 1989 [61]) plots for pegmatites from Larsemann Hills.
Figure 4. Chondrite-normalized REE patterns ((a) normalization values after Sun and McDonough, 1989 [63]) and primitive mantle normalized trace element patterns ((b), normalization values after McDonough and Sun, 1995 [64]) for pegmatites from Larsemann Hills.
Figure 5. The CL images of representative zircons from the samples (a–e) (The red solid circles represent the U-Pb test points. The green solid circles represent the Hf test points.).
Figure 6. Zircon U–Pb concordia diagrams and age histograms of the (a,b) granitic pegmatite (Z1220-23-2), (c,d) plagioclase pegmatite (Z1218-6), (e,f) the syenite pegmatite (Z1229-42-4), (g,h) the plagioclase pegmatite (Z1230-45-2), and (i,j) the granitic pegmatite (Z1231-50-1).5.2.2. Trace Elements in Zircon.
Figure 7. Chondrite-normalized REE patterns (normalization values after Sun and McDonough, 1989 [63] and Hoskin, 2005 [68]) of the new magmatic zircons from the samples. (a) Z1220-23-2; (b) Z1218-6; (c) Z1229-42-4; (d) Z1230-50-1; (e) Z1230-45-2.
Figure 8. Discriminant diagrams of zircons for pegmatites in the Larsemann Hills in (a,b) [67].
Figure 10. 104 Ga/Al vs. Ce (a), Zr + Nb + Ce + Y vs. (K2O + Na2O)/CaO (b) classification diagrams [71] of Pan-African pegmatites in Larsemann Hills.
Figure 11. Discrimination diagrams of the tectonic environment of granitic pegmatites in the Larsemann Hills (a,b). Abbreviations: syn-collision granite (syn-COLG), volcanic arc granite (VAG), with plate granite (WPG), and normal and anomalous ocean ridge granite (ORG) (based on Pearce et al., 1984 [73]).
Figure 12. Simplified geological map of Prydz Bay in East Antarctica (a) (modified after Ren et al. [40]). Simplified evolution of Pan-African pegmatites in Prydz Bay (b).
Main geological events in the Larsemann Hills and adjacent areas of East Antarctica (after Wang, 2002 [
Pan-African period | D4: Further stretching on the basis of D3 |
D3: N–S stretching event | |
D2: WNW thrust event | |
Grenville period | D1-2: Act II of slow return stage |
Syntectonic perilla granite intrusion | |
D1-1: (S1 foliation of Bt-Sil-Qtz in Grt) | |
Metasedimentary rocks | |
Mafic–felsic composite gneiss |
Whole-rock major elements.
Sample | Z1220-23-2 | Z1229-42-4 | Z1231-50-1 | Z1230-45-2 | Z1218-6 |
---|---|---|---|---|---|
SiO2 | 56.33 | 74.70 | 70.96 | 72.14 | 64.46 |
Al2O3 | 22.38 | 12.59 | 16.00 | 15.40 | 19.06 |
TiO2 | 0.18 | 0.02 | 0.16 | 0.17 | 0.10 |
Fe2O3 | 4.56 | 0.42 | 0.33 | 0.19 | 0.06 |
FeO | 9.42 | 3.70 | 0.34 | 0.78 | 0.27 |
CaO | 0.24 | 0.53 | 1.03 | 1.38 | 0.62 |
MgO | 0.66 | 0.42 | 0.41 | 0.38 | 0.14 |
K2O | 4.17 | 5.27 | 6.53 | 5.56 | 12.01 |
Na2O | 0.73 | 1.28 | 3.36 | 3.17 | 2.61 |
MnO | 0.05 | 0.37 | 0.00 | 0.01 | 0.00 |
P2O5 | 0.14 | 0.07 | 0.12 | 0.06 | 0.09 |
LOI | 0.51 | 0.52 | 0.53 | 0.56 | 0.31 |
Total | 99.64 | 99.92 | 99.92 | 99.89 | 99.78 |
A/NK | 3.91 | 1.61 | 1.27 | 1.37 | 1.10 |
A/CNK | 3.85 | 1.47 | 1.13 | 1.13 | 1.05 |
Na2O + K2O | 4.90 | 6.55 | 9.89 | 8.73 | 14.62 |
K2O/Na2O | 5.70 | 4.13 | 1.94 | 1.75 | 4.60 |
Quartz | 29.27 | 42.60 | 24.08 | 28.79 | 1.92 |
Anorthite | 0.26 | 2.15 | 4.35 | 6.53 | 2.49 |
Albite | 6.26 | 10.87 | 28.69 | 27.06 | 22.22 |
K-feldspar | 24.94 | 31.34 | 38.85 | 33.09 | 71.37 |
Corundum | 16.75 | 4.02 | 1.83 | 1.79 | 0.86 |
Hypersthene | 15.13 | 8.19 | 1.13 | 1.98 | 0.64 |
Ilmenite | 0.35 | 0.04 | 0.31 | 0.33 | 0.20 |
Magnetite | 6.69 | 0.61 | 0.48 | 0.28 | 0.08 |
Apatite | 0.33 | 0.17 | 0.28 | 0.14 | 0.22 |
Li | 28.10 | 10.82 | 11.23 | 22.03 | 9.60 |
Be | 4.41 | 0.56 | 0.43 | 1.06 | 0.45 |
Sc | 1.17 | 7.09 | 4.22 | 1.50 | 1.22 |
V | 27.65 | 2.19 | 15.27 | 13.27 | 8.00 |
Cr | 4.01 | 6.80 | 6.61 | 6.24 | 4.33 |
Co | 34.30 | 5.14 | 2.66 | 2.56 | 0.86 |
Ni | 30.12 | 5.45 | 5.38 | 3.42 | 1.57 |
Cu | 6.07 | 4.20 | 9.68 | 3.83 | 7.41 |
Zn | 14.63 | 8.60 | 8.16 | 17.63 | 11.75 |
Ga | 15.92 | 14.39 | 15.65 | 16.16 | 17.51 |
Rb | 308.55 | 225.78 | 249.80 | 229.91 | 429.46 |
Sr | 20.30 | 78.86 | 118.08 | 142.36 | 202.40 |
Y | 1.91 | 21.72 | 18.73 | 2.78 | 1.65 |
Zr | 88.52 | 84.28 | 33.73 | 17.04 | 20.68 |
Nb | 6.61 | 2.01 | 2.96 | 4.67 | 2.76 |
Mo | 1.81 | 0.21 | 0.39 | 0.01 | 0.49 |
La | 21.80 | 177.72 | 75.21 | 18.29 | 13.64 |
Ce | 46.49 | 36.50 | 28.76 | 27.77 | 19.90 |
Pr | 5.37 | 29.73 | 16.19 | 2.69 | 1.87 |
Nd | 17.63 | 98.04 | 58.42 | 7.84 | 6.10 |
Sm | 3.39 | 21.65 | 12.45 | 1.09 | 1.07 |
Eu | 0.29 | 1.41 | 1.58 | 1.36 | 2.30 |
Gd | 2.33 | 18.29 | 9.35 | 1.03 | 0.97 |
Tb | 0.26 | 2.85 | 1.10 | 0.13 | 0.10 |
Dy | 0.86 | 20.62 | 4.76 | 0.62 | 0.41 |
Ho | 0.11 | 4.99 | 0.75 | 0.10 | 0.06 |
Er | 0.32 | 15.72 | 1.85 | 0.22 | 0.17 |
Tm | 0.05 | 2.83 | 0.23 | 0.03 | 0.03 |
Yb | 0.31 | 16.97 | 1.19 | 0.13 | 0.16 |
Lu | 0.05 | 2.01 | 0.14 | 0.02 | 0.02 |
Hf | 3.10 | 3.62 | 1.18 | 0.54 | 0.55 |
Ta | 0.45 | 0.11 | 0.16 | 0.20 | 0.13 |
Pb | 55.74 | 45.65 | 22.26 | 42.16 | 65.22 |
Th | 19.62 | 117.52 | 58.52 | 2.87 | 5.52 |
U | 2.46 | 14.85 | 2.07 | 0.61 | 0.61 |
ΣREE | 99.25 | 739.34 | 342.21 | 61.32 | 46.80 |
LREE/HREE | 22.21 | 7.77 | 16.68 | 25.91 | 23.40 |
LaN/YbN | 51.22 | 7.51 | 45.51 | 99.38 | 60.95 |
δEu | 0.31 | 0.22 | 0.45 | 3.94 | 6.90 |
LA-ICP-MS zircon U-Pb data of the samples.
Spots | Th | U | Th/U | 207Pb/206Pb | 207Pb/206Pb | 207Pb/235U | 207Pb/235U | 206Pb/238U | 206Pb/238U | 207Pb/206Pb | 207Pb/206Pb | 207Pb/235U | 207Pb/235U | 206Pb/238U | 206Pb/238U |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
ppm | ppm | Ratio | 1σ | Ratio | 1σ | Ratio | 1σ | Age (Ma) | 1σ | Age (Ma) | 1σ | Age (Ma) | 1σ | ||
Z1220-23-2 | |||||||||||||||
3 | 114.6 | 985.0 | 0.1164 | 0.0623 | 0.0019 | 0.6835 | 0.0259 | 0.0794 | 0.0016 | 687 | 65 | 529 | 16 | 492 | 10 |
4 | 91.8 | 438.7 | 0.2092 | 0.0586 | 0.0013 | 0.6752 | 0.0163 | 0.0837 | 0.0013 | 554 | 55 | 524 | 10 | 518 | 8 |
5 | 204.7 | 652.3 | 0.3138 | 0.0608 | 0.0019 | 0.6993 | 0.0230 | 0.0836 | 0.0015 | 632 | 69 | 538 | 14 | 517 | 9 |
7 | 119.5 | 449.2 | 0.2659 | 0.0562 | 0.0017 | 0.6412 | 0.0186 | 0.0829 | 0.0012 | 461 | 67 | 503 | 12 | 514 | 7 |
8 | 131.7 | 134.0 | 0.9827 | 0.0782 | 0.0022 | 1.7650 | 0.0530 | 0.1642 | 0.0034 | 1154 | 57 | 1033 | 19 | 980 | 19 |
9 | 52.9 | 110.1 | 0.4799 | 0.0779 | 0.0027 | 1.7552 | 0.0526 | 0.1653 | 0.0031 | 1146 | 69 | 1029 | 19 | 986 | 17 |
10 | 571.1 | 893.4 | 0.6393 | 0.0759 | 0.0019 | 1.8397 | 0.0510 | 0.1768 | 0.0041 | 1094 | 50 | 1060 | 18 | 1050 | 22 |
11 | 102.0 | 137.5 | 0.7414 | 0.0789 | 0.0023 | 2.0391 | 0.0554 | 0.1890 | 0.0037 | 1169 | 51 | 1129 | 19 | 1116 | 20 |
12 | 104.0 | 411.7 | 0.2527 | 0.0580 | 0.0014 | 0.6683 | 0.0176 | 0.0838 | 0.0015 | 528 | 56 | 520 | 11 | 519 | 9 |
14 | 123.3 | 450.9 | 0.2734 | 0.0571 | 0.0013 | 0.6766 | 0.0180 | 0.0859 | 0.0011 | 494 | 52 | 525 | 11 | 531 | 7 |
15 | 117.7 | 471.1 | 0.2498 | 0.0606 | 0.0015 | 0.7242 | 0.0213 | 0.0867 | 0.0014 | 633 | 56 | 553 | 13 | 536 | 8 |
16 | 243.3 | 593.9 | 0.4097 | 0.0595 | 0.0013 | 0.6983 | 0.0182 | 0.0855 | 0.0016 | 583 | 16 | 538 | 11 | 529 | 10 |
17 | 323.9 | 515.9 | 0.6279 | 0.0709 | 0.0014 | 1.2571 | 0.0362 | 0.1287 | 0.0030 | 955 | 36 | 827 | 16 | 780 | 17 |
19 | 192.3 | 503.6 | 0.3818 | 0.0579 | 0.0012 | 0.7114 | 0.0172 | 0.0891 | 0.0014 | 528 | 46 | 546 | 10 | 550 | 8 |
20 | 153.2 | 151.0 | 1.0148 | 0.0716 | 0.0017 | 1.5690 | 0.0547 | 0.1582 | 0.0037 | 976 | 47 | 958 | 22 | 947 | 21 |
21 | 133.3 | 469.6 | 0.2838 | 0.0577 | 0.0011 | 0.7014 | 0.0150 | 0.0883 | 0.0012 | 517 | 43 | 540 | 9 | 545 | 7 |
22 | 208.8 | 581.0 | 0.3593 | 0.0563 | 0.0013 | 0.6689 | 0.0170 | 0.0862 | 0.0012 | 465 | 55 | 520 | 10 | 533 | 7 |
23 | 20.9 | 158.5 | 0.1316 | 0.0711 | 0.0019 | 1.6118 | 0.0414 | 0.1647 | 0.0017 | 961 | 54 | 975 | 16 | 983 | 9 |
24 | 111.0 | 575.5 | 0.1928 | 0.0560 | 0.0012 | 0.6430 | 0.0128 | 0.0833 | 0.0008 | 454 | 46 | 504 | 8 | 516 | 5 |
26 | 137.6 | 477.4 | 0.2883 | 0.0546 | 0.0011 | 0.6296 | 0.0137 | 0.0838 | 0.0011 | 394 | 44 | 496 | 9 | 519 | 6 |
27 | 68.2 | 377.8 | 0.1806 | 0.0576 | 0.0013 | 0.6649 | 0.0157 | 0.0837 | 0.0010 | 517 | 44 | 518 | 10 | 518 | 6 |
28 | 135.8 | 477.6 | 0.2843 | 0.0552 | 0.0010 | 0.6380 | 0.0162 | 0.0836 | 0.0012 | 420 | 34 | 501 | 10 | 518 | 7 |
29 | 100.5 | 799.0 | 0.1258 | 0.0565 | 0.0010 | 0.6890 | 0.0163 | 0.0884 | 0.0014 | 472 | 39 | 532 | 10 | 546 | 8 |
30 | 89.9 | 124.1 | 0.7242 | 0.0646 | 0.0019 | 0.8886 | 0.0281 | 0.1002 | 0.0016 | 761 | 64 | 646 | 15 | 615 | 10 |
31 | 160.0 | 461.7 | 0.3465 | 0.0572 | 0.0013 | 0.6591 | 0.0150 | 0.0837 | 0.0010 | 502 | 50 | 514 | 9 | 518 | 6 |
32 | 114.4 | 135.5 | 0.8445 | 0.0615 | 0.0016 | 0.9371 | 0.0307 | 0.1105 | 0.0021 | 657 | 50 | 671 | 16 | 676 | 12 |
34 | 79.4 | 118.8 | 0.6682 | 0.0762 | 0.0019 | 1.4539 | 0.0381 | 0.1387 | 0.0021 | 1102 | 50 | 912 | 16 | 837 | 12 |
35 | 62.4 | 317.5 | 0.1965 | 0.0732 | 0.0019 | 1.8212 | 0.0579 | 0.1809 | 0.0037 | 1020 | 53 | 1053 | 21 | 1072 | 20 |
Z1218-6 | |||||||||||||||
1 | 185.8 | 346.9 | 0.5356 | 0.0596 | 0.0014 | 0.6575 | 0.0147 | 0.0799 | 0.0012 | 591 | 50 | 513 | 9 | 496 | 7 |
2 | 75.7 | 158.6 | 0.4772 | 0.0594 | 0.0016 | 0.6550 | 0.0184 | 0.0798 | 0.0010 | 589 | 59 | 512 | 11 | 495 | 6 |
3 | 146.8 | 240.5 | 0.6103 | 0.0578 | 0.0012 | 0.6746 | 0.0154 | 0.0845 | 0.0012 | 520 | 46 | 523 | 9 | 523 | 7 |
4 | 71.4 | 176.1 | 0.4052 | 0.0642 | 0.0017 | 0.8176 | 0.0209 | 0.0923 | 0.0012 | 750 | 52 | 607 | 12 | 569 | 7 |
6 | 15.7 | 37.7 | 0.4156 | 0.0640 | 0.0040 | 0.7480 | 0.0470 | 0.0848 | 0.0016 | 743 | 132 | 567 | 27 | 525 | 9 |
8 | 44.7 | 98.5 | 0.4541 | 0.0614 | 0.0019 | 0.6752 | 0.0228 | 0.0797 | 0.0011 | 654 | 67 | 524 | 14 | 494 | 7 |
9 | 158.8 | 245.5 | 0.6468 | 0.0586 | 0.0015 | 0.6888 | 0.0175 | 0.0855 | 0.0012 | 550 | 53 | 532 | 11 | 529 | 7 |
10 | 100.6 | 185.4 | 0.5428 | 0.0607 | 0.0012 | 0.7716 | 0.0154 | 0.0923 | 0.0013 | 628 | 75 | 581 | 9 | 569 | 7 |
11 | 33.8 | 56.3 | 0.6006 | 0.0609 | 0.0029 | 0.6962 | 0.0308 | 0.0835 | 0.0016 | 635 | 101 | 537 | 18 | 517 | 9 |
12 | 135.6 | 285.4 | 0.4753 | 0.0606 | 0.0013 | 0.7113 | 0.0191 | 0.0848 | 0.0013 | 633 | 72 | 545 | 11 | 525 | 8 |
13 | 11.9 | 26.1 | 0.4544 | 0.0568 | 0.0031 | 0.7019 | 0.0391 | 0.0896 | 0.0015 | 483 | 116 | 540 | 23 | 553 | 9 |
14 | 190.7 | 258.9 | 0.7364 | 0.0589 | 0.0015 | 0.7037 | 0.0194 | 0.0864 | 0.0011 | 565 | 54 | 541 | 12 | 534 | 7 |
15 | 124.5 | 180.5 | 0.6898 | 0.0577 | 0.0013 | 0.7077 | 0.0163 | 0.0891 | 0.0014 | 517 | 52 | 543 | 10 | 550 | 8 |
16 | 42.7 | 97.7 | 0.4370 | 0.0575 | 0.0020 | 0.6600 | 0.0263 | 0.0830 | 0.0013 | 509 | 78 | 515 | 16 | 514 | 8 |
18 | 25.4 | 50.5 | 0.5021 | 0.0557 | 0.0029 | 0.6297 | 0.0314 | 0.0824 | 0.0014 | 439 | 115 | 496 | 20 | 510 | 8 |
19 | 47.5 | 104.0 | 0.4563 | 0.0552 | 0.0023 | 0.6194 | 0.0254 | 0.0816 | 0.0015 | 420 | 93 | 490 | 16 | 505 | 9 |
20 | 55.2 | 116.5 | 0.4736 | 0.0606 | 0.0021 | 0.8114 | 0.0303 | 0.0968 | 0.0016 | 628 | 74 | 603 | 17 | 596 | 9 |
21 | 52.9 | 121.3 | 0.4359 | 0.0647 | 0.0021 | 0.9604 | 0.0362 | 0.1074 | 0.0027 | 765 | 67 | 683 | 19 | 658 | 16 |
22 | 13.7 | 31.1 | 0.4397 | 0.0553 | 0.0029 | 0.6325 | 0.0344 | 0.0833 | 0.0020 | 433 | 149 | 498 | 21 | 516 | 12 |
23 | 428.7 | 1393.1 | 0.3077 | 0.0649 | 0.0009 | 1.0037 | 0.0161 | 0.1119 | 0.0014 | 770 | 28 | 706 | 8 | 684 | 8 |
24 | 60.2 | 86.8 | 0.6931 | 0.0648 | 0.0025 | 0.7348 | 0.0292 | 0.0823 | 0.0013 | 769 | 86 | 559 | 17 | 510 | 8 |
25 | 77.2 | 135.3 | 0.5703 | 0.0592 | 0.0016 | 0.7116 | 0.0194 | 0.0872 | 0.0011 | 572 | 61 | 546 | 11 | 539 | 7 |
26 | 38.6 | 68.3 | 0.5655 | 0.0610 | 0.0026 | 0.7992 | 0.0331 | 0.0951 | 0.0014 | 639 | 91 | 596 | 19 | 586 | 8 |
28 | 151.9 | 259.7 | 0.5849 | 0.0711 | 0.0015 | 1.0851 | 0.0253 | 0.1104 | 0.0014 | 961 | 43 | 746 | 12 | 675 | 8 |
29 | 127.6 | 199.4 | 0.6396 | 0.0600 | 0.0016 | 0.7025 | 0.0211 | 0.0848 | 0.0013 | 611 | 58 | 540 | 13 | 525 | 8 |
32 | 12.2 | 26.2 | 0.4636 | 0.0597 | 0.0045 | 0.6509 | 0.0506 | 0.0790 | 0.0019 | 591 | 163 | 509 | 31 | 490 | 11 |
33 | 99.1 | 119.7 | 0.8280 | 0.0671 | 0.0021 | 0.9798 | 0.0370 | 0.1057 | 0.0024 | 843 | 65 | 694 | 19 | 648 | 14 |
34 | 31.5 | 66.2 | 0.4756 | 0.0714 | 0.0023 | 1.1113 | 0.0305 | 0.1133 | 0.0015 | 970 | 65 | 759 | 15 | 692 | 9 |
36 | 57.6 | 126.0 | 0.4575 | 0.0603 | 0.0020 | 0.7858 | 0.0252 | 0.0947 | 0.0016 | 617 | 70 | 589 | 14 | 583 | 9 |
38 | 136.9 | 278.8 | 0.4909 | 0.0579 | 0.0016 | 0.7381 | 0.0238 | 0.0920 | 0.0013 | 528 | 61 | 561 | 14 | 568 | 7 |
39 | 260.2 | 275.5 | 0.9442 | 0.0670 | 0.0016 | 1.0839 | 0.0248 | 0.1175 | 0.0013 | 835 | 51 | 746 | 12 | 716 | 7 |
40 | 16.2 | 35.7 | 0.4539 | 0.0540 | 0.0038 | 0.6004 | 0.0393 | 0.0819 | 0.0017 | 369 | 155 | 477 | 25 | 507 | 10 |
41 | 165.9 | 285.8 | 0.5804 | 0.0576 | 0.0015 | 0.6530 | 0.0201 | 0.0819 | 0.0012 | 522 | 59 | 510 | 12 | 508 | 7 |
42 | 59.4 | 80.5 | 0.7381 | 0.0632 | 0.0025 | 0.9055 | 0.0541 | 0.1021 | 0.0034 | 717 | 83 | 655 | 29 | 627 | 20 |
43 | 102.6 | 155.4 | 0.6602 | 0.0608 | 0.0017 | 0.7955 | 0.0292 | 0.0948 | 0.0024 | 632 | 66 | 594 | 16 | 584 | 14 |
44 | 58.5 | 101.0 | 0.5786 | 0.0586 | 0.0020 | 0.7366 | 0.0277 | 0.0911 | 0.0016 | 554 | 77 | 560 | 16 | 562 | 9 |
45 | 20.7 | 55.8 | 0.3717 | 0.0557 | 0.0028 | 0.6434 | 0.0314 | 0.0842 | 0.0012 | 439 | 111 | 504 | 19 | 521 | 7 |
47 | 152.8 | 233.4 | 0.6549 | 0.0591 | 0.0024 | 0.6889 | 0.0279 | 0.0847 | 0.0012 | 569 | 87 | 532 | 17 | 524 | 7 |
48 | 77.3 | 138.2 | 0.5590 | 0.0677 | 0.0028 | 0.9202 | 0.0365 | 0.0991 | 0.0018 | 861 | 86 | 662 | 19 | 609 | 11 |
49 | 81.9 | 180.2 | 0.4542 | 0.0672 | 0.0018 | 1.1317 | 0.0357 | 0.1221 | 0.0022 | 843 | 56 | 769 | 17 | 743 | 12 |
50 | 194.5 | 357.0 | 0.5448 | 0.0667 | 0.0012 | 1.3011 | 0.0426 | 0.1410 | 0.0034 | 829 | 44 | 846 | 19 | 850 | 19 |
51 | 96.2 | 270.7 | 0.3555 | 0.0638 | 0.0016 | 0.9577 | 0.0276 | 0.1087 | 0.0015 | 744 | 54 | 682 | 14 | 665 | 9 |
52 | 20.3 | 42.4 | 0.4781 | 0.0583 | 0.0039 | 0.6809 | 0.0417 | 0.0861 | 0.0016 | 543 | 146 | 527 | 25 | 532 | 9 |
53 | 101.8 | 147.4 | 0.6904 | 0.0598 | 0.0014 | 0.7410 | 0.0208 | 0.0898 | 0.0016 | 598 | 55 | 563 | 12 | 554 | 10 |
54 | 80.8 | 165.5 | 0.4884 | 0.0573 | 0.0018 | 0.6468 | 0.0195 | 0.0820 | 0.0012 | 506 | 69 | 507 | 12 | 508 | 7 |
55 | 170.0 | 262.6 | 0.6471 | 0.0596 | 0.0014 | 0.7369 | 0.0202 | 0.0895 | 0.0014 | 591 | 20 | 561 | 12 | 553 | 8 |
56 | 115.0 | 230.5 | 0.4989 | 0.0619 | 0.0013 | 0.8252 | 0.0188 | 0.0967 | 0.0014 | 672 | 42 | 611 | 10 | 595 | 8 |
57 | 123.9 | 159.8 | 0.7751 | 0.0591 | 0.0017 | 0.7218 | 0.0194 | 0.0890 | 0.0015 | 572 | 63 | 552 | 11 | 549 | 9 |
59 | 45.6 | 62.7 | 0.7274 | 0.0605 | 0.0028 | 0.7575 | 0.0381 | 0.0910 | 0.0019 | 620 | 102 | 573 | 22 | 561 | 11 |
60 | 72.4 | 87.4 | 0.8287 | 0.0595 | 0.0022 | 0.7304 | 0.0278 | 0.0891 | 0.0015 | 587 | 80 | 557 | 16 | 550 | 9 |
61 | 46.4 | 112.1 | 0.4141 | 0.0551 | 0.0020 | 0.6302 | 0.0223 | 0.0831 | 0.0012 | 417 | 81 | 496 | 14 | 514 | 7 |
62 | 109.7 | 211.3 | 0.5191 | 0.0563 | 0.0015 | 0.6338 | 0.0167 | 0.0816 | 0.0010 | 465 | 59 | 498 | 10 | 505 | 6 |
63 | 124.8 | 313.7 | 0.3978 | 0.0578 | 0.0015 | 0.6831 | 0.0191 | 0.0856 | 0.0012 | 524 | 62 | 529 | 12 | 530 | 7 |
64 | 130.8 | 209.2 | 0.6254 | 0.0626 | 0.0017 | 0.9466 | 0.0256 | 0.1097 | 0.0015 | 694 | 57 | 676 | 13 | 671 | 9 |
66 | 22.4 | 30.3 | 0.7403 | 0.0653 | 0.0043 | 0.8326 | 0.0553 | 0.0926 | 0.0018 | 783 | 139 | 615 | 31 | 571 | 11 |
67 | 156.8 | 244.6 | 0.6411 | 0.0585 | 0.0018 | 0.6510 | 0.0187 | 0.0812 | 0.0014 | 546 | 67 | 509 | 12 | 503 | 8 |
68 | 95.6 | 147.6 | 0.6481 | 0.0636 | 0.0025 | 0.9304 | 0.0377 | 0.1060 | 0.0013 | 728 | 83 | 668 | 20 | 649 | 7 |
70 | 136.0 | 275.9 | 0.4931 | 0.0612 | 0.0017 | 0.6954 | 0.0191 | 0.0825 | 0.0010 | 656 | 61 | 536 | 11 | 511 | 6 |
71 | 111.2 | 233.1 | 0.4770 | 0.0593 | 0.0021 | 0.6449 | 0.0203 | 0.0794 | 0.0012 | 576 | 78 | 505 | 13 | 493 | 7 |
72 | 55.7 | 126.7 | 0.4391 | 0.0573 | 0.0026 | 0.6474 | 0.0287 | 0.0823 | 0.0011 | 502 | 106 | 507 | 18 | 510 | 6 |
73 | 59.8 | 115.7 | 0.5173 | 0.0669 | 0.0023 | 1.0517 | 0.0360 | 0.1142 | 0.0017 | 835 | 72 | 730 | 18 | 697 | 10 |
75 | 45.2 | 109.3 | 0.4139 | 0.0561 | 0.0028 | 0.6338 | 0.0297 | 0.0824 | 0.0014 | 457 | 109 | 498 | 18 | 510 | 8 |
76 | 156.2 | 376.4 | 0.4149 | 0.0588 | 0.0014 | 0.6959 | 0.0181 | 0.0859 | 0.0012 | 567 | 52 | 536 | 11 | 531 | 7 |
77 | 75.0 | 128.8 | 0.5828 | 0.0649 | 0.0017 | 1.0205 | 0.0270 | 0.1142 | 0.0013 | 770 | 56 | 714 | 14 | 697 | 8 |
78 | 57.9 | 132.3 | 0.4374 | 0.0612 | 0.0022 | 0.6512 | 0.0206 | 0.0776 | 0.0012 | 656 | 76 | 509 | 13 | 482 | 7 |
79 | 62.2 | 147.5 | 0.4214 | 0.0595 | 0.0023 | 0.6760 | 0.0251 | 0.0826 | 0.0011 | 587 | 116 | 524 | 15 | 511 | 6 |
80 | 66.5 | 87.4 | 0.7607 | 0.0623 | 0.0025 | 0.8365 | 0.0343 | 0.0975 | 0.0012 | 683 | 87 | 617 | 19 | 600 | 7 |
81 | 29.4 | 71.4 | 0.4119 | 0.0636 | 0.0033 | 0.6520 | 0.0340 | 0.0747 | 0.0011 | 728 | 111 | 510 | 21 | 465 | 7 |
Z1230-42-4 | |||||||||||||||
1 | 95.3 | 609.7 | 0.1562 | 0.0620 | 0.0017 | 0.7070 | 0.0235 | 0.0834 | 0.0026 | 674 | 60 | 543 | 14 | 516 | 15 |
2 | 92.5 | 1488.9 | 0.0621 | 0.0652 | 0.0014 | 0.7392 | 0.0198 | 0.0823 | 0.0022 | 781 | 44 | 562 | 12 | 510 | 13 |
3 | 107.4 | 928.6 | 0.1156 | 0.0600 | 0.0016 | 0.7208 | 0.0222 | 0.0870 | 0.0017 | 606 | 57 | 551 | 13 | 538 | 10 |
5 | 81.9 | 717.2 | 0.1142 | 0.0652 | 0.0014 | 1.0492 | 0.0417 | 0.1161 | 0.0029 | 789 | 51 | 729 | 21 | 708 | 17 |
6 | 40.8 | 1388.0 | 0.0294 | 0.0724 | 0.0018 | 1.4369 | 0.0337 | 0.1441 | 0.0023 | 998 | 54 | 904 | 14 | 868 | 13 |
8 | 93.7 | 936.7 | 0.1001 | 0.0624 | 0.0011 | 0.9007 | 0.0205 | 0.1047 | 0.0018 | 687 | 37 | 652 | 11 | 642 | 11 |
9 | 146.0 | 671.0 | 0.2175 | 0.0591 | 0.0011 | 0.7180 | 0.0218 | 0.0878 | 0.0020 | 572 | 43 | 550 | 13 | 543 | 12 |
10 | 51.1 | 4929.3 | 0.0104 | 0.0714 | 0.0012 | 1.3557 | 0.0338 | 0.1374 | 0.0025 | 969 | 36 | 870 | 15 | 830 | 14 |
11 | 131.2 | 534.6 | 0.2454 | 0.0612 | 0.0016 | 0.8244 | 0.0233 | 0.0978 | 0.0017 | 656 | 57 | 610 | 13 | 602 | 10 |
13 | 25.7 | 2180.6 | 0.0118 | 0.0709 | 0.0013 | 1.2310 | 0.0401 | 0.1252 | 0.0031 | 955 | 39 | 815 | 18 | 761 | 18 |
14 | 41.9 | 2646.0 | 0.0158 | 0.0633 | 0.0012 | 0.9297 | 0.0255 | 0.1066 | 0.0026 | 717 | 44 | 667 | 13 | 653 | 15 |
16 | 51.0 | 2411.9 | 0.0212 | 0.0672 | 0.0010 | 1.0058 | 0.0193 | 0.1086 | 0.0021 | 844 | 31 | 707 | 10 | 665 | 12 |
19 | 25.1 | 774.8 | 0.0324 | 0.0660 | 0.0015 | 0.9405 | 0.0204 | 0.1036 | 0.0019 | 806 | 42 | 673 | 11 | 636 | 11 |
20 | 75.4 | 604.4 | 0.1248 | 0.0671 | 0.0017 | 0.8645 | 0.0265 | 0.0933 | 0.0021 | 840 | 56 | 633 | 14 | 575 | 13 |
21 | 114.0 | 1121.2 | 0.1016 | 0.0664 | 0.0023 | 0.9864 | 0.0393 | 0.1081 | 0.0032 | 817 | 70 | 697 | 20 | 662 | 18 |
22 | 9.3 | 1249.1 | 0.0075 | 0.0809 | 0.0018 | 1.8551 | 0.0713 | 0.1656 | 0.0054 | 1220 | 43 | 1065 | 25 | 988 | 30 |
25 | 95.2 | 872.9 | 0.1091 | 0.0632 | 0.0009 | 0.9464 | 0.0211 | 0.1084 | 0.0020 | 722 | 31 | 676 | 11 | 664 | 12 |
27 | 269.0 | 1076.3 | 0.2499 | 0.0591 | 0.0010 | 0.6908 | 0.0166 | 0.0844 | 0.0015 | 572 | 5 | 533 | 10 | 523 | 9 |
28 | 74.3 | 723.3 | 0.1028 | 0.0658 | 0.0020 | 0.7368 | 0.0248 | 0.0823 | 0.0028 | 798 | 58 | 561 | 15 | 510 | 17 |
29 | 8.5 | 1024.2 | 0.0083 | 0.0653 | 0.0023 | 0.7719 | 0.0342 | 0.0864 | 0.0036 | 787 | 73 | 581 | 20 | 534 | 21 |
30 | 175.9 | 925.9 | 0.1899 | 0.0574 | 0.0013 | 0.7322 | 0.0208 | 0.0930 | 0.0026 | 506 | 55 | 558 | 12 | 573 | 15 |
32 | 94.4 | 837.4 | 0.1127 | 0.0650 | 0.0026 | 0.8114 | 0.0460 | 0.0910 | 0.0045 | 772 | 83 | 603 | 26 | 561 | 27 |
33 | 68.5 | 707.4 | 0.0969 | 0.0582 | 0.0018 | 0.7370 | 0.0254 | 0.0934 | 0.0035 | 539 | 67 | 561 | 15 | 576 | 21 |
34 | 19.8 | 291.1 | 0.0681 | 0.0587 | 0.0018 | 0.6705 | 0.0212 | 0.0846 | 0.0032 | 567 | 73 | 521 | 13 | 524 | 19 |
35 | 84.6 | 740.8 | 0.1142 | 0.0610 | 0.0015 | 0.6821 | 0.0191 | 0.0816 | 0.0023 | 643 | 53 | 528 | 12 | 506 | 14 |
39 | 39.4 | 933.6 | 0.0422 | 0.0652 | 0.0013 | 0.7901 | 0.0189 | 0.0877 | 0.0016 | 789 | 47 | 591 | 11 | 542 | 10 |
40 | 21.6 | 255.5 | 0.0846 | 0.0573 | 0.0018 | 0.6406 | 0.0163 | 0.0820 | 0.0021 | 502 | 67 | 503 | 10 | 508 | 13 |
41 | 133.1 | 853.0 | 0.1561 | 0.0594 | 0.0013 | 0.7270 | 0.0184 | 0.0891 | 0.0023 | 583 | 48 | 555 | 11 | 550 | 13 |
42 | 384.4 | 1346.1 | 0.2855 | 0.0797 | 0.0032 | 1.6907 | 0.0774 | 0.1531 | 0.0031 | 1191 | 80 | 1005 | 29 | 918 | 17 |
44 | 52.8 | 645.7 | 0.0817 | 0.0593 | 0.0011 | 0.6766 | 0.0157 | 0.0825 | 0.0015 | 589 | 39 | 525 | 10 | 511 | 9 |
46 | 91.0 | 799.9 | 0.1138 | 0.0552 | 0.0010 | 0.6582 | 0.0147 | 0.0863 | 0.0015 | 420 | 36 | 514 | 9 | 534 | 9 |
47 | 87.1 | 875.0 | 0.0996 | 0.0593 | 0.0011 | 0.8239 | 0.0178 | 0.1006 | 0.0019 | 589 | 39 | 610 | 10 | 618 | 11 |
50 | 15.9 | 238.0 | 0.0666 | 0.0613 | 0.0017 | 0.6939 | 0.0191 | 0.0823 | 0.0015 | 650 | 61 | 535 | 11 | 510 | 9 |
52 | 42.6 | 557.2 | 0.0764 | 0.0605 | 0.0014 | 0.7218 | 0.0184 | 0.0866 | 0.0017 | 620 | 82 | 552 | 11 | 535 | 10 |
53 | 57.3 | 494.3 | 0.1159 | 0.0590 | 0.0012 | 0.7004 | 0.0159 | 0.0859 | 0.0014 | 569 | 44 | 539 | 9 | 531 | 8 |
Z1230-50-1 | |||||||||||||||
2 | 33.3 | 969.1 | 0.0344 | 0.0581 | 0.0008 | 0.7145 | 0.0161 | 0.0890 | 0.0017 | 532 | 30 | 547 | 10 | 550 | 10 |
3 | 773.3 | 191.2 | 4.0453 | 0.0623 | 0.0022 | 0.7724 | 0.0419 | 0.0884 | 0.0021 | 683 | 79 | 581 | 24 | 546 | 13 |
4 | 600.4 | 277.6 | 2.1626 | 0.0613 | 0.0016 | 0.7760 | 0.0232 | 0.0918 | 0.0017 | 650 | 56 | 583 | 13 | 566 | 10 |
5 | 522.2 | 258.8 | 2.0176 | 0.0573 | 0.0016 | 0.6956 | 0.0207 | 0.0879 | 0.0011 | 502 | 63 | 536 | 12 | 543 | 7 |
6 | 65.8 | 756.5 | 0.0870 | 0.0638 | 0.0012 | 0.7788 | 0.0212 | 0.0884 | 0.0020 | 744 | 38 | 585 | 12 | 546 | 12 |
7 | 455.3 | 305.3 | 1.4910 | 0.0626 | 0.0025 | 0.6432 | 0.0335 | 0.0744 | 0.0023 | 694 | 85 | 504 | 21 | 463 | 14 |
8 | 421.5 | 173.6 | 2.4276 | 0.0633 | 0.0023 | 0.6919 | 0.0293 | 0.0791 | 0.0015 | 717 | 76 | 534 | 18 | 491 | 9 |
9 | 29.8 | 1063.2 | 0.0280 | 0.0633 | 0.0014 | 0.7418 | 0.0187 | 0.0852 | 0.0017 | 717 | 46 | 563 | 11 | 527 | 10 |
10 | 432.1 | 145.6 | 2.9674 | 0.0618 | 0.0018 | 0.6973 | 0.0210 | 0.0821 | 0.0015 | 733 | 62 | 537 | 13 | 508 | 9 |
11 | 83.5 | 821.2 | 0.1017 | 0.0590 | 0.0011 | 0.7160 | 0.0240 | 0.0879 | 0.0024 | 565 | 41 | 548 | 14 | 543 | 14 |
12 | 21.5 | 1260.1 | 0.0171 | 0.0610 | 0.0024 | 0.6366 | 0.0295 | 0.0755 | 0.0016 | 639 | 83 | 500 | 18 | 469 | 10 |
13 | 205.7 | 190.4 | 1.0805 | 0.0655 | 0.0021 | 0.7751 | 0.0332 | 0.0853 | 0.0019 | 791 | 66 | 583 | 19 | 528 | 11 |
15 | 461.8 | 248.3 | 1.8597 | 0.0573 | 0.0017 | 0.7238 | 0.0275 | 0.0920 | 0.0025 | 502 | 65 | 553 | 16 | 568 | 15 |
16 | 16.6 | 685.5 | 0.0242 | 0.0594 | 0.0010 | 0.7019 | 0.0148 | 0.0859 | 0.0016 | 589 | 39 | 540 | 9 | 531 | 9 |
17 | 325.5 | 120.7 | 2.6973 | 0.0613 | 0.0024 | 0.7208 | 0.0274 | 0.0862 | 0.0017 | 650 | 83 | 551 | 16 | 533 | 10 |
18 | 334.2 | 561.5 | 0.5953 | 0.0635 | 0.0020 | 0.6752 | 0.0264 | 0.0771 | 0.0020 | 724 | 69 | 524 | 16 | 479 | 12 |
20 | 243.7 | 91.0 | 2.6771 | 0.0653 | 0.0026 | 0.8290 | 0.0335 | 0.0926 | 0.0021 | 783 | 85 | 613 | 19 | 571 | 12 |
21 | 222.5 | 102.6 | 2.1681 | 0.0555 | 0.0018 | 0.6738 | 0.0279 | 0.0880 | 0.0023 | 432 | 69 | 523 | 17 | 543 | 13 |
22 | 287.8 | 94.3 | 3.0503 | 0.0612 | 0.0022 | 0.7174 | 0.0282 | 0.0849 | 0.0013 | 656 | 76 | 549 | 17 | 525 | 8 |
23 | 35.2 | 900.8 | 0.0391 | 0.0628 | 0.0015 | 0.6880 | 0.0231 | 0.0795 | 0.0022 | 702 | 52 | 532 | 14 | 493 | 13 |
24 | 191.8 | 337.3 | 0.5686 | 0.0607 | 0.0021 | 0.7772 | 0.0309 | 0.0931 | 0.0020 | 628 | 76 | 584 | 18 | 574 | 12 |
26 | 434.6 | 148.7 | 2.9229 | 0.0589 | 0.0022 | 0.7183 | 0.0261 | 0.0892 | 0.0018 | 565 | 80 | 550 | 15 | 551 | 11 |
27 | 39.8 | 1033.5 | 0.0385 | 0.0585 | 0.0012 | 0.6668 | 0.0173 | 0.0829 | 0.0019 | 546 | 44 | 519 | 11 | 513 | 11 |
28 | 141.7 | 142.9 | 0.9912 | 0.0602 | 0.0030 | 0.6289 | 0.0266 | 0.0767 | 0.0017 | 613 | 107 | 495 | 17 | 476 | 10 |
29 | 953.5 | 386.4 | 2.4681 | 0.0658 | 0.0014 | 0.7952 | 0.0205 | 0.0878 | 0.0018 | 1200 | 51 | 594 | 12 | 542 | 11 |
30 | 160.5 | 261.0 | 0.6150 | 0.0619 | 0.0021 | 0.7563 | 0.0266 | 0.0892 | 0.0021 | 672 | 72 | 572 | 15 | 551 | 13 |
31 | 235.5 | 159.3 | 1.4788 | 0.0573 | 0.0017 | 0.6461 | 0.0212 | 0.0820 | 0.0019 | 506 | 65 | 506 | 13 | 508 | 11 |
33 | 273.4 | 199.8 | 1.3679 | 0.0571 | 0.0017 | 0.7111 | 0.0225 | 0.0906 | 0.0017 | 494 | 67 | 545 | 13 | 559 | 10 |
34 | 148.3 | 293.0 | 0.5062 | 0.0574 | 0.0015 | 0.7227 | 0.0263 | 0.0910 | 0.0022 | 506 | 57 | 552 | 16 | 561 | 13 |
35 | 319.2 | 108.2 | 2.9513 | 0.0647 | 0.0024 | 0.8896 | 0.0280 | 0.1020 | 0.0031 | 765 | 79 | 646 | 15 | 626 | 18 |
36 | 153.5 | 1062.0 | 0.1445 | 0.0616 | 0.0012 | 0.8003 | 0.0219 | 0.0942 | 0.0021 | 661 | 43 | 597 | 12 | 580 | 13 |
37 | 549.1 | 147.2 | 3.7311 | 0.0544 | 0.0023 | 0.6202 | 0.0247 | 0.0834 | 0.0015 | 387 | 96 | 490 | 15 | 516 | 9 |
38 | 42.4 | 1128.3 | 0.0376 | 0.0620 | 0.0023 | 0.7210 | 0.0348 | 0.0837 | 0.0019 | 674 | 78 | 551 | 21 | 518 | 11 |
39 | 425.8 | 119.2 | 3.5726 | 0.0630 | 0.0032 | 0.8078 | 0.0450 | 0.0926 | 0.0022 | 709 | 107 | 601 | 25 | 571 | 13 |
40 | 108.8 | 1002.6 | 0.1085 | 0.0643 | 0.0016 | 0.8029 | 0.0208 | 0.0903 | 0.0015 | 754 | 249 | 598 | 12 | 557 | 9 |
41 | 410.6 | 130.6 | 3.1444 | 0.0596 | 0.0020 | 0.7223 | 0.0274 | 0.0876 | 0.0018 | 591 | 70 | 552 | 16 | 541 | 11 |
42 | 380.0 | 277.8 | 1.3682 | 0.0576 | 0.0015 | 0.7019 | 0.0230 | 0.0882 | 0.0018 | 522 | 57 | 540 | 14 | 545 | 11 |
43 | 98.7 | 1048.1 | 0.0942 | 0.0629 | 0.0012 | 0.7722 | 0.0234 | 0.0887 | 0.0021 | 702 | 39 | 581 | 13 | 548 | 12 |
44 | 52.5 | 1179.3 | 0.0446 | 0.0632 | 0.0020 | 0.7604 | 0.0325 | 0.0864 | 0.0017 | 717 | 63 | 574 | 19 | 534 | 10 |
45 | 42.1 | 1078.4 | 0.0391 | 0.0582 | 0.0011 | 0.6793 | 0.0146 | 0.0844 | 0.0013 | 539 | 45 | 526 | 9 | 522 | 8 |
46 | 160.0 | 1000.8 | 0.1599 | 0.0575 | 0.0011 | 0.7237 | 0.0181 | 0.0909 | 0.0017 | 522 | 39 | 553 | 11 | 561 | 10 |
47 | 333.1 | 157.4 | 2.1168 | 0.0615 | 0.0027 | 0.7567 | 0.0382 | 0.0884 | 0.0020 | 657 | 92 | 572 | 22 | 546 | 12 |
48 | 244.2 | 99.2 | 2.4621 | 0.0556 | 0.0022 | 0.6813 | 0.0331 | 0.0888 | 0.0028 | 435 | 87 | 528 | 20 | 548 | 16 |
49 | 25.1 | 1035.9 | 0.0242 | 0.0598 | 0.0013 | 0.7271 | 0.0154 | 0.0884 | 0.0017 | 594 | 44 | 555 | 9 | 546 | 10 |
50 | 513.3 | 162.4 | 3.1598 | 0.0584 | 0.0019 | 0.6873 | 0.0258 | 0.0850 | 0.0017 | 546 | 72 | 531 | 16 | 526 | 10 |
Z1230-45-2 | |||||||||||||||
1 | 96.2 | 601.8 | 0.1598 | 0.0655 | 0.0023 | 0.8150 | 0.0383 | 0.0901 | 0.0033 | 791 | 70 | 605 | 21 | 556 | 20 |
2 | 36.2 | 2220.2 | 0.0163 | 0.0600 | 0.0014 | 0.7305 | 0.0185 | 0.0889 | 0.0022 | 611 | 48 | 557 | 11 | 549 | 13 |
3 | 195.3 | 1026.2 | 0.1903 | 0.0573 | 0.0012 | 0.6644 | 0.0149 | 0.0844 | 0.0016 | 502 | 46 | 517 | 9 | 523 | 10 |
5 | 287.3 | 478.5 | 0.6005 | 0.0678 | 0.0015 | 1.1851 | 0.0334 | 0.1273 | 0.0033 | 865 | 46 | 794 | 16 | 773 | 19 |
6 | 137.0 | 966.7 | 0.1417 | 0.0652 | 0.0025 | 0.8012 | 0.0258 | 0.0906 | 0.0023 | 789 | 80 | 598 | 15 | 559 | 13 |
9 | 55.3 | 1587.2 | 0.0348 | 0.0694 | 0.0024 | 1.0308 | 0.0478 | 0.1072 | 0.0027 | 909 | 76 | 719 | 24 | 656 | 16 |
11 | 19.2 | 1248.7 | 0.0154 | 0.0641 | 0.0035 | 0.8099 | 0.0602 | 0.0911 | 0.0036 | 744 | 112 | 602 | 34 | 562 | 21 |
12 | 481.6 | 842.8 | 0.5714 | 0.0689 | 0.0020 | 0.9402 | 0.0323 | 0.0992 | 0.0025 | 894 | 59 | 673 | 17 | 610 | 14 |
13 | 351.2 | 642.1 | 0.5470 | 0.0743 | 0.0028 | 1.3025 | 0.0385 | 0.1284 | 0.0053 | 1050 | 77 | 847 | 17 | 779 | 30 |
14 | 88.0 | 415.4 | 0.2118 | 0.0614 | 0.0016 | 0.8943 | 0.0237 | 0.1068 | 0.0027 | 654 | 56 | 649 | 13 | 654 | 16 |
15 | 73.9 | 351.3 | 0.2102 | 0.0565 | 0.0016 | 0.7473 | 0.0229 | 0.0970 | 0.0026 | 478 | 63 | 567 | 13 | 597 | 16 |
17 | 278.9 | 335.0 | 0.8327 | 0.0799 | 0.0031 | 1.7867 | 0.1192 | 0.1600 | 0.0059 | 1195 | 77 | 1041 | 43 | 957 | 33 |
18 | 101.0 | 1962.1 | 0.0515 | 0.0612 | 0.0014 | 0.7723 | 0.0224 | 0.0914 | 0.0021 | 648 | 48 | 581 | 13 | 564 | 13 |
19 | 138.3 | 382.8 | 0.3614 | 0.0611 | 0.0015 | 0.8144 | 0.0217 | 0.0967 | 0.0017 | 643 | 54 | 605 | 12 | 595 | 10 |
20 | 116.2 | 718.4 | 0.1617 | 0.0694 | 0.0016 | 1.0429 | 0.0297 | 0.1090 | 0.0025 | 910 | 52 | 725 | 15 | 667 | 15 |
21 | 345.0 | 545.8 | 0.6320 | 0.0645 | 0.0016 | 0.9699 | 0.0291 | 0.1089 | 0.0024 | 767 | 52 | 688 | 15 | 666 | 14 |
22 | 288.4 | 605.1 | 0.4766 | 0.0676 | 0.0015 | 1.1497 | 0.0332 | 0.1226 | 0.0024 | 857 | 46 | 777 | 16 | 746 | 14 |
23 | 45.5 | 3417.5 | 0.0133 | 0.0578 | 0.0010 | 0.7265 | 0.0197 | 0.0910 | 0.0024 | 520 | 42 | 555 | 12 | 561 | 14 |
24 | 33.9 | 3659.8 | 0.0093 | 0.0586 | 0.0011 | 0.7492 | 0.0200 | 0.0923 | 0.0021 | 554 | 36 | 568 | 12 | 569 | 12 |
25 | 81.5 | 421.4 | 0.1934 | 0.0638 | 0.0016 | 0.7767 | 0.0214 | 0.0883 | 0.0021 | 744 | 52 | 584 | 12 | 546 | 12 |
26 | 44.7 | 4226.8 | 0.0106 | 0.0596 | 0.0011 | 0.7864 | 0.0229 | 0.0952 | 0.0024 | 587 | 41 | 589 | 13 | 587 | 14 |
27 | 52.7 | 2809.1 | 0.0187 | 0.0613 | 0.0012 | 0.7803 | 0.0162 | 0.0927 | 0.0021 | 650 | 47 | 586 | 9 | 571 | 13 |
28 | 108.0 | 938.7 | 0.1150 | 0.0634 | 0.0014 | 0.7723 | 0.0209 | 0.0879 | 0.0016 | 724 | 46 | 581 | 12 | 543 | 9 |
29 | 96.7 | 220.4 | 0.4387 | 0.0589 | 0.0017 | 0.7525 | 0.0243 | 0.0925 | 0.0019 | 565 | 65 | 570 | 14 | 570 | 11 |
30 | 44.2 | 2711.2 | 0.0163 | 0.0632 | 0.0013 | 0.7625 | 0.0156 | 0.0874 | 0.0016 | 717 | 47 | 575 | 9 | 540 | 9 |
31 | 53.9 | 1525.3 | 0.0354 | 0.0578 | 0.0012 | 0.6945 | 0.0162 | 0.0869 | 0.0015 | 520 | 44 | 535 | 10 | 537 | 9 |
32 | 61.8 | 1216.0 | 0.0508 | 0.0582 | 0.0012 | 0.7072 | 0.0188 | 0.0877 | 0.0017 | 600 | 44 | 543 | 11 | 542 | 10 |
33 | 304.3 | 1711.8 | 0.1778 | 0.0706 | 0.0023 | 1.1169 | 0.0464 | 0.1139 | 0.0022 | 946 | 67 | 762 | 22 | 695 | 13 |
34 | 34.4 | 3714.3 | 0.0093 | 0.0579 | 0.0012 | 0.7686 | 0.0184 | 0.0962 | 0.0019 | 524 | 44 | 579 | 11 | 592 | 11 |
35 | 148.5 | 518.2 | 0.2865 | 0.0570 | 0.0013 | 0.6814 | 0.0188 | 0.0866 | 0.0018 | 500 | 52 | 528 | 11 | 536 | 11 |
36 | 164.1 | 603.4 | 0.2720 | 0.0590 | 0.0014 | 0.6986 | 0.0193 | 0.0857 | 0.0015 | 565 | 47 | 538 | 12 | 530 | 9 |
38 | 45.9 | 3938.2 | 0.0117 | 0.0623 | 0.0012 | 0.7650 | 0.0219 | 0.0887 | 0.0018 | 687 | 43 | 577 | 13 | 548 | 10 |
39 | 117.8 | 377.5 | 0.3122 | 0.0580 | 0.0012 | 0.7615 | 0.0270 | 0.0946 | 0.0024 | 532 | 46 | 575 | 16 | 583 | 14 |
40 | 71.2 | 6465.7 | 0.0110 | 0.0592 | 0.0011 | 0.8382 | 0.0185 | 0.1027 | 0.0019 | 576 | 8 | 618 | 10 | 630 | 11 |
42 | 286.6 | 584.7 | 0.4901 | 0.0680 | 0.0022 | 0.9720 | 0.0513 | 0.1025 | 0.0031 | 878 | 101 | 690 | 26 | 629 | 18 |
43 | 32.7 | 3076.5 | 0.0106 | 0.0622 | 0.0012 | 0.7830 | 0.0228 | 0.0916 | 0.0024 | 680 | 41 | 587 | 13 | 565 | 14 |
44 | 54.7 | 2697.7 | 0.0203 | 0.0624 | 0.0015 | 0.7664 | 0.0232 | 0.0894 | 0.0021 | 687 | 52 | 578 | 13 | 552 | 12 |
47 | 24.8 | 2720.1 | 0.0091 | 0.0639 | 0.0012 | 0.7982 | 0.0200 | 0.0910 | 0.0021 | 739 | 45 | 596 | 11 | 561 | 12 |
49 | 35.4 | 3761.1 | 0.0094 | 0.0592 | 0.0011 | 0.7589 | 0.0195 | 0.0933 | 0.0022 | 572 | 6 | 573 | 11 | 575 | 13 |
50 | 122.4 | 705.4 | 0.1735 | 0.0593 | 0.0012 | 0.7319 | 0.0174 | 0.0899 | 0.0019 | 589 | 10 | 558 | 10 | 555 | 11 |
52 | 45.0 | 2438.6 | 0.0185 | 0.0669 | 0.0014 | 0.8554 | 0.0273 | 0.0928 | 0.0025 | 835 | 43 | 628 | 15 | 572 | 14 |
53 | 124.0 | 539.7 | 0.2298 | 0.0663 | 0.0010 | 1.0573 | 0.0277 | 0.1155 | 0.0024 | 817 | 33 | 732 | 14 | 704 | 14 |
55 | 34.4 | 3303.4 | 0.0104 | 0.0585 | 0.0009 | 0.7315 | 0.0174 | 0.0906 | 0.0017 | 550 | 31 | 557 | 10 | 559 | 10 |
57 | 161.5 | 838.9 | 0.1925 | 0.0591 | 0.0010 | 0.6990 | 0.0179 | 0.0859 | 0.0019 | 569 | 37 | 538 | 11 | 531 | 12 |
Zircon trace and REE (×10−6) analysis results for the pegmatites.
Spots | Th | U | Th/U | La | Ce | Pr | Nd | Sm | Eu | Gd | Tb | Dy | Ho | Er | Tm | Yb | Lu | Y | Nb | Hf | Ta | ΣREE | LREE | HREE | LREE/HREE | δEu | δCe |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Z1220-23-2 | |||||||||||||||||||||||||||
4 | 91.8 | 438.7 | 0.2092 | 0.01 | 1.15 | 0.07 | 1.35 | 5.93 | 0.06 | 27.52 | 9.10 | 67.64 | 12.76 | 27.88 | 3.45 | 23.15 | 2.98 | 395.48 | 1.30 | 12,459.67 | 0.53 | 183.04 | 8.57 | 174.47 | 0.05 | 0.01 | 15.63 |
5 | 204.7 | 652.3 | 0.3138 | 0.17 | 2.87 | 0.31 | 4.67 | 11.60 | 0.21 | 46.34 | 14.69 | 118.68 | 27.62 | 85.47 | 15.07 | 125.12 | 19.43 | 871.32 | 2.29 | 11,319.99 | 0.93 | 472.26 | 19.83 | 452.43 | 0.04 | 0.03 | 3.08 |
7 | 119.5 | 449.2 | 0.2659 | 0.01 | 1.42 | 0.10 | 1.93 | 7.20 | 0.06 | 29.31 | 8.85 | 68.00 | 12.35 | 25.97 | 3.37 | 21.99 | 3.10 | 380.54 | 1.26 | 11,882.43 | 0.51 | 183.65 | 10.72 | 172.93 | 0.06 | 0.01 | |
12 | 104 | 411.7 | 0.2527 | 0.02 | 1.41 | 0.08 | 1.50 | 5.32 | 0.07 | 25.78 | 8.12 | 66.11 | 13.28 | 35.92 | 5.62 | 49.45 | 7.71 | 427.32 | 1.61 | 12,807.29 | 0.66 | 220.39 | 8.40 | 211.98 | 0.04 | 0.02 | 8.80 |
24 | 111 | 575.5 | 0.1928 | 0.02 | 1.43 | 0.08 | 1.66 | 6.93 | 0.10 | 35.44 | 12.11 | 95.80 | 18.14 | 41.82 | 5.13 | 31.26 | 3.80 | 592.94 | 1.77 | 13,645.61 | 0.89 | 253.72 | 10.22 | 243.50 | 0.04 | 0.02 | 8.98 |
26 | 137.6 | 477.4 | 0.2883 | 0.03 | 1.75 | 0.13 | 3.01 | 8.99 | 0.11 | 40.35 | 11.96 | 86.32 | 14.82 | 31.44 | 3.76 | 23.76 | 2.97 | 486.74 | 1.56 | 12,736.93 | 0.58 | 229.40 | 14.01 | 215.39 | 0.07 | 0.02 | 7.52 |
27 | 68.2 | 377.8 | 0.1806 | 0.01 | 0.88 | 0.05 | 0.92 | 3.39 | 0.02 | 16.90 | 5.51 | 45.30 | 8.90 | 21.33 | 2.90 | 18.43 | 2.44 | 286.98 | 1.22 | 13,837.74 | 0.53 | 126.98 | 5.26 | 121.71 | 0.04 | 0.01 | 8.95 |
28 | 135.8 | 477.6 | 0.2843 | 0.01 | 1.56 | 0.13 | 2.57 | 8.87 | 0.06 | 34.80 | 10.14 | 74.74 | 13.25 | 28.27 | 3.50 | 23.11 | 2.98 | 428.65 | 1.42 | 12,766.57 | 0.59 | 204.00 | 13.20 | 190.80 | 0.07 | 0.01 | 0.73 |
31 | 160 | 461.7 | 0.3465 | 0.02 | 1.86 | 0.17 | 3.32 | 11.28 | 0.12 | 41.35 | 11.68 | 81.62 | 14.04 | 29.66 | 3.82 | 23.93 | 3.29 | 458.63 | 1.39 | 13,047.11 | 0.52 | 226.16 | 16.77 | 209.39 | 0.08 | 0.02 | 8.82 |
Z1218-6 | |||||||||||||||||||||||||||
3 | 146.77 | 240.47 | 0.61 | 0.11 | 1.42 | 0.04 | 0.25 | 0.36 | 0.24 | 2.00 | 0.97 | 13.00 | 5.20 | 28.39 | 7.20 | 83.97 | 15.94 | 180.37 | 0.31 | 7853.54 | 0.16 | 159.10 | 2.42 | 156.68 | 0.02 | 0.86 | 5.18 |
6 | 15.67 | 37.70 | 0.42 | 0.03 | 2.57 | 0.02 | 0.40 | 0.94 | 0.18 | 5.45 | 2.23 | 29.49 | 11.62 | 57.72 | 13.26 | 135.69 | 22.87 | 395.34 | 0.41 | 10,255.56 | 0.33 | 282.47 | 4.14 | 278.33 | 0.01 | 0.24 | 25.96 |
9 | 158.82 | 245.53 | 0.65 | 0.05 | 2.07 | 0.02 | 0.25 | 0.40 | 0.15 | 2.94 | 1.21 | 17.27 | 7.10 | 36.98 | 8.98 | 100.76 | 19.27 | 241.55 | 0.49 | 8626.94 | 0.40 | 197.44 | 2.94 | 194.51 | 0.02 | 0.41 | 18.06 |
11 | 33.83 | 56.32 | 0.60 | 0.24 | 2.87 | 0.08 | 0.66 | 0.78 | 0.14 | 4.24 | 1.59 | 21.61 | 8.52 | 41.28 | 9.36 | 99.63 | 17.47 | 284.17 | 0.47 | 9814.07 | 0.41 | 208.47 | 4.77 | 203.70 | 0.02 | 0.23 | 4.92 |
12 | 135.65 | 285.36 | 0.48 | 0.75 | 3.27 | 0.47 | 2.55 | 1.03 | 0.12 | 1.98 | 0.60 | 9.33 | 4.31 | 24.96 | 6.67 | 83.69 | 18.05 | 144.99 | 0.34 | 9271.08 | 0.25 | 157.79 | 8.19 | 149.60 | 0.05 | 0.25 | 1.36 |
14 | 190.67 | 258.92 | 0.74 | 0.13 | 2.58 | 0.05 | 0.43 | 0.36 | 0.23 | 2.23 | 0.90 | 13.68 | 5.63 | 27.74 | 7.26 | 81.93 | 15.09 | 186.91 | 0.26 | 8413.33 | 0.35 | 158.23 | 3.77 | 154.46 | 0.02 | 0.78 | 8.09 |
16 | 42.72 | 97.74 | 0.44 | 0.01 | 2.14 | 0.02 | 0.26 | 0.47 | 0.19 | 3.23 | 1.26 | 16.95 | 7.07 | 35.78 | 9.18 | 101.17 | 19.35 | 233.79 | 0.52 | 10,150.70 | 0.62 | 197.09 | 3.10 | 193.99 | 0.02 | 0.46 | 30.05 |
18 | 25.35 | 50.49 | 0.50 | 0.12 | 2.30 | 0.03 | 0.37 | 0.59 | 0.14 | 4.30 | 1.62 | 22.02 | 9.75 | 47.57 | 11.66 | 124.94 | 22.50 | 320.94 | 0.50 | 11,534.19 | 0.64 | 247.91 | 3.55 | 244.37 | 0.01 | 0.26 | 9.92 |
22 | 13.69 | 31.14 | 0.44 | 0.01 | 2.70 | 0.04 | 0.46 | 1.17 | 0.22 | 8.16 | 2.80 | 39.33 | 15.76 | 71.50 | 15.25 | 153.99 | 25.82 | 490.56 | 1.00 | 10,439.30 | 0.83 | 337.20 | 4.58 | 332.61 | 0.01 | 0.22 | 96.23 |
25 | 77.16 | 135.30 | 0.57 | 0.13 | 1.88 | 0.04 | 0.29 | 0.37 | 0.17 | 2.65 | 0.77 | 10.44 | 4.32 | 21.78 | 5.39 | 58.63 | 10.66 | 141.18 | 0.31 | 9228.96 | 0.26 | 117.52 | 2.89 | 114.63 | 0.03 | 0.53 | 6.84 |
29 | 127.57 | 199.44 | 0.64 | 0.17 | 2.19 | 0.06 | 0.47 | 0.68 | 0.30 | 3.58 | 1.26 | 18.21 | 7.33 | 38.32 | 9.13 | 102.77 | 18.50 | 244.88 | 0.32 | 9840.19 | 0.13 | 202.97 | 3.87 | 199.10 | 0.02 | 0.59 | 5.35 |
30 | 12.16 | 26.23 | 0.46 | 0.09 | 1.70 | 0.04 | 0.52 | 0.64 | 0.28 | 2.43 | 1.00 | 12.89 | 5.23 | 27.10 | 6.84 | 77.78 | 14.55 | 185.68 | 0.25 | 9047.11 | 0.21 | 151.08 | 3.27 | 147.81 | 0.02 | 0.67 | 6.82 |
45 | 20.74 | 55.79 | 0.37 | 0.01 | 2.81 | 0.02 | 0.28 | 0.60 | 0.13 | 3.78 | 1.68 | 20.57 | 8.51 | 43.34 | 10.09 | 101.36 | 18.27 | 277.16 | 0.67 | 11,874.08 | 0.70 | 211.44 | 3.83 | 207.60 | 0.02 | 0.27 | |
47 | 152.85 | 233.39 | 0.65 | 0.17 | 1.71 | 0.05 | 0.39 | 0.49 | 0.32 | 3.31 | 1.34 | 19.20 | 7.81 | 41.40 | 10.18 | 111.93 | 21.70 | 258.06 | 0.32 | 10,556.61 | 0.34 | 219.99 | 3.13 | 216.86 | 0.01 | 0.77 | 4.38 |
52 | 20.27 | 42.40 | 0.48 | 0.17 | 2.60 | 0.04 | 0.58 | 0.57 | 0.16 | 3.53 | 1.24 | 16.00 | 6.61 | 31.99 | 7.16 | 74.79 | 13.30 | 215.07 | 0.32 | 10,043.36 | 0.33 | 158.74 | 4.12 | 154.62 | 0.03 | 0.35 | 7.80 |
61 | 46.44 | 112.15 | 0.41 | 0.01 | 1.66 | 0.00 | 0.10 | 0.29 | 0.07 | 2.35 | 0.93 | 13.03 | 5.74 | 30.22 | 7.27 | 80.66 | 15.59 | 189.64 | 0.58 | 10,171.51 | 0.69 | 157.95 | 2.15 | 155.80 | 0.01 | 0.28 | 13.30 |
63 | 124.80 | 313.72 | 0.40 | 0.01 | 0.37 | 0.00 | 0.08 | 0.01 | 0.11 | 0.87 | 0.39 | 6.24 | 3.07 | 17.60 | 4.99 | 59.22 | 12.63 | 104.65 | 0.23 | 8413.70 | 0.15 | 105.59 | 0.57 | 105.02 | 0.01 | 7.37 | |
70 | 136.03 | 275.86 | 0.49 | 0.00 | 0.53 | 0.04 | 0.11 | 0.13 | 0.16 | 0.98 | 0.62 | 8.39 | 3.70 | 21.27 | 5.89 | 73.05 | 15.15 | 128.90 | 0.27 | 10,934.09 | 1.07 | 130.01 | 0.97 | 129.04 | 0.01 | 1.36 | 13.20 |
72 | 55.65 | 126.74 | 0.44 | 0.03 | 2.41 | 0.03 | 0.20 | 0.49 | 0.24 | 3.53 | 1.46 | 20.94 | 8.74 | 43.62 | 11.80 | 126.13 | 25.31 | 291.27 | 0.56 | 10,539.55 | 0.77 | 244.92 | 3.39 | 241.53 | 0.01 | 0.57 | 21.06 |
75 | 45.24 | 109.30 | 0.41 | 0.01 | 2.32 | 0.00 | 0.21 | 0.50 | 0.22 | 3.72 | 1.23 | 18.09 | 7.30 | 38.51 | 9.86 | 106.69 | 21.22 | 245.95 | 0.63 | 10,715.34 | 0.80 | 209.89 | 3.26 | 206.62 | 0.02 | 0.48 | 16.04 |
76 | 156.15 | 376.39 | 0.41 | 0.01 | 0.42 | 0.00 | 0.04 | 0.16 | 0.06 | 1.28 | 0.53 | 8.29 | 3.96 | 22.51 | 6.14 | 73.72 | 16.23 | 130.49 | 0.13 | 9832.89 | 0.13 | 133.37 | 0.69 | 132.68 | 0.01 | 0.44 | 13.58 |
79 | 62.16 | 147.49 | 0.42 | 0.01 | 1.24 | 0.00 | 0.00 | 0.25 | 0.06 | 1.27 | 0.70 | 10.10 | 4.12 | 22.21 | 5.65 | 68.95 | 12.96 | 141.20 | 0.38 | 10,409.56 | 0.54 | 127.52 | 1.56 | 125.96 | 0.01 | 0.33 | 0.69 |
Z1229-42-4 | |||||||||||||||||||||||||||
1 | 95.26 | 609.69 | 0.16 | 0.18 | 1.97 | 0.19 | 1.46 | 2.04 | 0.35 | 7.80 | 2.95 | 32.40 | 7.76 | 23.05 | 3.43 | 25.25 | 2.96 | 252.29 | 1.64 | 14,910.14 | 0.36 | 111.82 | 6.20 | 105.61 | 0.06 | 0.27 | 2.60 |
3 | 107.40 | 928.63 | 0.12 | 0.23 | 2.61 | 0.25 | 2.27 | 5.05 | 0.73 | 23.57 | 6.29 | 45.58 | 9.98 | 27.72 | 5.10 | 40.12 | 5.48 | 300.34 | 0.47 | 14,425.48 | 0.36 | 174.99 | 11.15 | 163.85 | 0.07 | 0.21 | 2.69 |
9 | 145.96 | 670.98 | 0.22 | 0.01 | 1.15 | 0.07 | 1.44 | 3.86 | 0.13 | 15.93 | 6.05 | 63.68 | 14.95 | 43.80 | 6.19 | 40.54 | 4.53 | 492.09 | 1.82 | 13,612.56 | 0.47 | 202.34 | 6.67 | 195.67 | 0.03 | 0.05 | 9.21 |
27 | 268.98 | 1076.28 | 0.25 | 0.10 | 1.93 | 0.17 | 1.72 | 3.93 | 0.27 | 17.04 | 6.56 | 66.60 | 16.48 | 44.77 | 6.46 | 45.09 | 5.13 | 518.35 | 2.71 | 14,957.96 | 0.89 | 216.25 | 8.12 | 208.13 | 0.04 | 0.10 | 3.64 |
29 | 8.48 | 1024.15 | 0.01 | 0.62 | 8.64 | 0.49 | 2.70 | 1.95 | 1.00 | 9.23 | 4.84 | 89.91 | 41.33 | 245.53 | 75.97 | 977.27 | 172.67 | 1189.52 | 1.25 | 12,641.97 | 1.67 | 1632.14 | 15.40 | 1616.74 | 0.01 | 0.72 | 3.85 |
34 | 19.81 | 291.15 | 0.07 | 0.06 | 0.99 | 0.09 | 0.82 | 1.70 | 0.18 | 9.37 | 4.08 | 48.43 | 13.35 | 43.24 | 7.12 | 57.61 | 7.13 | 431.49 | 1.21 | 12,921.65 | 0.54 | 194.16 | 3.84 | 190.33 | 0.02 | 0.14 | 3.50 |
39 | 39.41 | 933.56 | 0.04 | 1.73 | 12.61 | 1.42 | 8.65 | 4.48 | 2.65 | 12.62 | 5.47 | 67.28 | 19.19 | 62.90 | 10.88 | 85.84 | 11.80 | 627.95 | 1.62 | 12,581.27 | 1.23 | 307.52 | 31.54 | 275.98 | 0.11 | 1.08 | 1.97 |
41 | 133.13 | 852.95 | 0.16 | 0.51 | 5.04 | 0.61 | 3.72 | 3.13 | 0.87 | 10.92 | 3.66 | 39.70 | 10.14 | 30.42 | 4.74 | 36.37 | 4.35 | 322.35 | 2.10 | 12,948.01 | 0.54 | 154.18 | 13.88 | 140.30 | 0.10 | 0.45 | 2.23 |
46 | 90.98 | 799.86 | 0.11 | 0.01 | 0.66 | 0.03 | 0.51 | 1.15 | 0.06 | 5.92 | 2.57 | 37.18 | 12.27 | 47.91 | 8.84 | 78.60 | 10.42 | 404.70 | 1.00 | 20,909.30 | 0.33 | 206.11 | 2.39 | 203.72 | 0.01 | 0.07 | |
52 | 42.56 | 557.24 | 0.08 | 0.04 | 0.78 | 0.04 | 0.37 | 1.06 | 0.11 | 4.58 | 2.12 | 25.45 | 7.63 | 29.70 | 6.48 | 45.22 | 11.36 | 252.04 | 1.18 | 21,894.37 | 0.27 | 134.95 | 2.40 | 132.55 | 0.02 | 0.16 | 4.85 |
53 | 57.29 | 494.30 | 0.12 | 0.01 | 0.61 | 0.03 | 0.46 | 1.78 | 0.06 | 7.51 | 3.54 | 41.11 | 11.64 | 37.91 | 7.03 | 61.92 | 9.82 | 386.07 | 1.12 | 26,511.66 | 0.42 | 183.42 | 2.93 | 180.49 | 0.02 | 0.05 | |
Z1230-50-1 | |||||||||||||||||||||||||||
2 | 33.30 | 969.08 | 0.03 | 0.80 | 6.79 | 0.39 | 2.22 | 2.23 | 0.50 | 14.14 | 7.27 | 90.31 | 23.87 | 72.38 | 11.87 | 94.27 | 13.96 | 741.31 | 1.49 | 12,742.33 | 1.24 | 340.98 | 12.93 | 328.05 | 0.04 | 0.27 | 2.99 |
3 | 773.27 | 191.15 | 4.05 | 0.42 | 78.96 | 1.76 | 21.27 | 19.54 | 4.60 | 37.65 | 7.52 | 56.27 | 13.96 | 49.45 | 9.35 | 77.96 | 11.76 | 408.52 | 1.32 | 9634.46 | 0.35 | 390.47 | 126.55 | 263.92 | 0.48 | 0.52 | 22.46 |
5 | 522.22 | 258.84 | 2.02 | 0.22 | 20.72 | 1.41 | 17.43 | 18.00 | 1.66 | 35.46 | 6.78 | 48.44 | 11.33 | 34.24 | 5.27 | 41.58 | 5.57 | 325.36 | 0.95 | 10,491.42 | 0.32 | 248.11 | 59.43 | 188.68 | 0.31 | 0.20 | 9.09 |
6 | 65.78 | 756.49 | 0.09 | 2.12 | 15.29 | 1.96 | 11.60 | 5.38 | 1.27 | 13.31 | 5.44 | 72.10 | 23.77 | 92.02 | 17.21 | 137.66 | 19.99 | 747.49 | 1.11 | 12,305.58 | 2.03 | 419.12 | 37.62 | 381.50 | 0.10 | 0.46 | 1.84 |
11 | 83.53 | 821.16 | 0.10 | 0.01 | 4.50 | 0.12 | 1.55 | 2.71 | 0.30 | 13.74 | 6.87 | 88.39 | 26.95 | 94.18 | 15.73 | 112.19 | 15.86 | 865.69 | 1.94 | 12,240.86 | 1.27 | 383.11 | 9.19 | 373.92 | 0.02 | 0.15 | 28.97 |
21 | 222.49 | 102.62 | 2.17 | 0.03 | 29.85 | 0.28 | 4.26 | 5.12 | 1.07 | 12.99 | 2.80 | 22.06 | 5.96 | 20.01 | 3.57 | 32.97 | 4.97 | 174.73 | 0.90 | 9904.65 | 0.33 | 145.93 | 40.60 | 105.33 | 0.39 | 0.40 | 84.18 |
26 | 434.65 | 148.70 | 2.92 | 0.23 | 24.22 | 1.33 | 17.39 | 16.51 | 3.68 | 41.03 | 8.45 | 64.12 | 16.31 | 51.58 | 8.93 | 72.25 | 10.98 | 437.18 | 1.53 | 8874.09 | 0.53 | 337.00 | 63.36 | 273.63 | 0.23 | 0.43 | 10.75 |
29 | 953.54 | 386.35 | 2.47 | 1.22 | 50.43 | 3.37 | 38.13 | 34.28 | 5.00 | 72.99 | 15.03 | 113.67 | 28.94 | 93.68 | 16.06 | 133.89 | 18.98 | 831.19 | 1.67 | 9442.87 | 0.59 | 625.68 | 132.43 | 493.25 | 0.27 | 0.31 | 6.09 |
30 | 160.55 | 261.05 | 0.62 | 0.01 | 7.05 | 0.17 | 2.58 | 4.67 | 0.45 | 15.89 | 3.80 | 30.70 | 7.57 | 22.66 | 3.73 | 27.82 | 3.67 | 241.71 | 1.03 | 11,693.20 | 0.56 | 130.76 | 14.92 | 115.84 | 0.13 | 0.16 | 63.21 |
41 | 410.59 | 130.58 | 3.14 | 0.28 | 44.53 | 1.38 | 19.48 | 17.39 | 3.41 | 34.73 | 6.42 | 50.80 | 13.45 | 43.36 | 7.81 | 62.23 | 9.40 | 370.72 | 0.91 | 8992.53 | 0.36 | 314.67 | 86.47 | 228.20 | 0.38 | 0.42 | 17.47 |
42 | 380.01 | 277.75 | 1.37 | 0.01 | 12.91 | 0.37 | 6.26 | 8.84 | 0.54 | 23.43 | 5.05 | 37.65 | 8.73 | 26.69 | 4.32 | 31.02 | 4.13 | 262.81 | 1.40 | 10,809.46 | 0.51 | 169.93 | 28.93 | 141.00 | 0.21 | 0.12 | 47.21 |
43 | 98.70 | 1048.06 | 0.09 | 1.26 | 15.93 | 0.63 | 3.64 | 3.07 | 0.76 | 11.48 | 4.66 | 58.06 | 18.34 | 75.76 | 15.69 | 143.76 | 22.83 | 550.80 | 2.43 | 11,817.06 | 1.84 | 375.87 | 25.29 | 350.58 | 0.07 | 0.39 | 4.37 |
47 | 333.09 | 157.35 | 2.12 | 0.29 | 19.50 | 1.14 | 14.65 | 13.21 | 2.41 | 28.22 | 6.36 | 50.78 | 13.06 | 43.89 | 7.80 | 66.44 | 9.88 | 365.80 | 1.90 | 8342.74 | 0.53 | 277.64 | 51.19 | 226.45 | 0.23 | 0.38 | 8.37 |
48 | 244.15 | 99.16 | 2.46 | 0.06 | 56.78 | 0.45 | 5.76 | 6.09 | 1.60 | 13.51 | 2.69 | 21.65 | 6.01 | 22.10 | 4.34 | 37.76 | 6.11 | 182.11 | 0.72 | 9189.56 | 0.23 | 184.92 | 70.75 | 114.17 | 0.62 | 0.54 | 86.80 |
49 | 25.11 | 1035.92 | 0.02 | 0.04 | 1.70 | 0.07 | 0.35 | 0.79 | 0.14 | 4.95 | 3.07 | 46.18 | 16.76 | 77.58 | 19.73 | 213.69 | 38.07 | 567.60 | 1.60 | 11,485.24 | 1.92 | 423.11 | 3.09 | 420.02 | 0.01 | 0.21 | 7.61 |
Z1230-45-2 | |||||||||||||||||||||||||||
1 | 96.20 | 601.80 | 0.16 | 0.78 | 8.53 | 0.91 | 6.66 | 4.40 | 1.79 | 13.38 | 4.90 | 46.60 | 15.20 | 64.38 | 14.09 | 142.74 | 23.52 | 65.19 | 1.99 | 11,780.76 | 1.37 | 347.89 | 23.08 | 324.81 | 0.07 | 0.71 | 2.48 |
2 | 36.20 | 2220.20 | 0.02 | 1.66 | 10.88 | 1.55 | 8.64 | 4.61 | 2.57 | 11.18 | 4.78 | 54.98 | 12.71 | 29.86 | 3.54 | 20.55 | 2.00 | 58.70 | 1.12 | 11,513.59 | 1.49 | 169.51 | 29.91 | 139.60 | 0.21 | 1.10 | 1.67 |
6 | 137.00 | 966.70 | 0.14 | 1.08 | 9.02 | 0.90 | 7.21 | 8.07 | 1.95 | 26.42 | 6.65 | 46.52 | 8.16 | 18.09 | 2.12 | 12.35 | 1.40 | 60.64 | 1.06 | 11,304.11 | 0.55 | 149.96 | 28.24 | 121.72 | 0.23 | 0.41 | 2.24 |
11 | 19.20 | 1248.70 | 0.02 | 1.03 | 9.59 | 0.53 | 3.04 | 2.11 | 0.81 | 4.17 | 2.08 | 27.68 | 10.51 | 46.66 | 10.27 | 82.51 | 13.26 | 64.04 | 1.29 | 12,620.83 | 1.47 | 214.23 | 17.10 | 197.13 | 0.09 | 0.83 | 3.18 |
18 | 101.00 | 1962.10 | 0.05 | 0.34 | 5.67 | 0.28 | 1.71 | 2.11 | 0.46 | 11.75 | 5.21 | 67.15 | 24.87 | 110.83 | 23.31 | 218.03 | 32.08 | 60.18 | 2.19 | 11,046.88 | 1.92 | 503.81 | 10.57 | 493.24 | 0.02 | 0.28 | 4.52 |
23 | 45.50 | 3417.50 | 0.01 | 0.02 | 0.69 | 0.01 | 0.28 | 1.02 | 0.12 | 8.44 | 5.66 | 90.46 | 33.91 | 143.26 | 27.33 | 216.99 | 28.76 | 60.37 | 1.88 | 12,523.64 | 2.45 | 556.98 | 2.16 | 554.82 | 0.00 | 0.12 | 9.16 |
24 | 33.90 | 3659.80 | 0.01 | 0.35 | 2.42 | 0.27 | 1.84 | 1.91 | 0.29 | 11.45 | 7.07 | 94.72 | 26.33 | 77.31 | 10.13 | 65.11 | 6.76 | 60.66 | 1.96 | 12,687.47 | 2.61 | 305.98 | 7.09 | 298.89 | 0.02 | 0.19 | 1.93 |
25 | 81.50 | 421.40 | 0.19 | 0.38 | 5.04 | 0.49 | 3.91 | 4.71 | 1.14 | 14.00 | 4.09 | 28.77 | 5.36 | 12.53 | 1.54 | 9.47 | 1.03 | 63.89 | 0.67 | 11,396.00 | 0.49 | 92.44 | 15.67 | 76.77 | 0.20 | 0.43 | 2.86 |
26 | 44.70 | 4226.80 | 0.01 | 4.54 | 22.90 | 3.22 | 15.69 | 6.19 | 7.71 | 15.27 | 7.64 | 123.30 | 48.93 | 224.05 | 50.05 | 457.94 | 74.07 | 60.21 | 2.52 | 12,297.49 | 2.79 | 1061.50 | 60.25 | 1001.25 | 0.06 | 2.43 | 1.47 |
27 | 52.70 | 2809.10 | 0.02 | 8.47 | 62.02 | 4.91 | 25.85 | 10.74 | 5.42 | 17.33 | 6.35 | 84.09 | 31.90 | 141.34 | 29.09 | 256.42 | 36.71 | 58.99 | 2.38 | 12,160.40 | 3.50 | 720.64 | 117.41 | 603.23 | 0.19 | 1.21 | 2.36 |
29 | 96.70 | 220.40 | 0.44 | 0.03 | 3.31 | 0.03 | 0.36 | 0.94 | 0.74 | 5.21 | 1.92 | 23.45 | 8.96 | 45.03 | 9.85 | 98.79 | 16.79 | 64.01 | 1.07 | 11,292.50 | 0.83 | 215.41 | 5.41 | 210.00 | 0.03 | 1.03 | 27.52 |
38 | 45.90 | 3938.20 | 0.01 | 4.99 | 37.03 | 3.75 | 19.71 | 8.54 | 5.11 | 17.58 | 7.22 | 100.66 | 40.54 | 191.88 | 41.11 | 361.65 | 49.91 | 59.25 | 2.55 | 11,784.48 | 3.97 | 889.69 | 79.14 | 810.55 | 0.10 | 1.28 | 2.10 |
39 | 117.80 | 377.50 | 0.31 | 0.03 | 2.09 | 0.06 | 1.57 | 2.94 | 0.10 | 11.32 | 2.85 | 20.49 | 3.81 | 7.91 | 0.94 | 5.05 | 0.53 | 65.16 | 0.83 | 12,162.60 | 0.55 | 59.69 | 6.79 | 52.90 | 0.13 | 0.05 | 11.98 |
43 | 32.70 | 3076.50 | 0.01 | 6.70 | 76.65 | 4.72 | 24.27 | 10.41 | 6.83 | 19.60 | 7.62 | 81.98 | 19.04 | 46.40 | 5.18 | 28.50 | 2.88 | 60.21 | 1.51 | 12,578.78 | 1.94 | 340.80 | 129.59 | 211.21 | 0.61 | 1.46 | 3.34 |
44 | 54.70 | 2697.70 | 0.02 | 7.54 | 75.55 | 5.90 | 30.34 | 13.10 | 7.23 | 18.19 | 6.41 | 80.41 | 25.82 | 98.31 | 18.45 | 159.73 | 21.17 | 59.46 | 1.52 | 12,907.12 | 1.88 | 568.15 | 139.66 | 428.49 | 0.33 | 1.43 | 2.78 |
47 | 24.80 | 2720.10 | 0.01 | 4.83 | 70.91 | 2.63 | 12.38 | 5.05 | 3.87 | 11.21 | 4.57 | 64.24 | 21.26 | 76.91 | 14.00 | 105.63 | 13.16 | 58.60 | 1.15 | 11,268.17 | 1.87 | 410.67 | 99.68 | 310.99 | 0.32 | 1.57 | 4.87 |
49 | 35.40 | 3761.10 | 0.01 | 0.01 | 0.29 | 0.00 | 0.14 | 0.83 | 0.04 | 8.39 | 4.61 | 81.76 | 35.19 | 165.35 | 35.80 | 296.12 | 39.17 | 60.33 | 1.91 | 12,739.59 | 3.23 | 667.67 | 1.30 | 666.37 | 0.00 | 0.05 | 0.93 |
50 | 122.40 | 705.40 | 0.17 | 0.01 | 1.52 | 0.06 | 0.97 | 2.89 | 0.09 | 16.29 | 5.30 | 42.68 | 7.99 | 15.72 | 1.77 | 9.26 | 1.08 | 64.32 | 1.17 | 11,328.30 | 0.97 | 105.63 | 5.53 | 100.10 | 0.06 | 0.04 | 32.72 |
52 | 45.00 | 2438.60 | 0.02 | 5.52 | 68.98 | 3.32 | 16.33 | 6.41 | 5.48 | 12.21 | 4.54 | 62.12 | 23.58 | 110.97 | 24.38 | 219.00 | 31.69 | 55.65 | 1.83 | 11,486.49 | 2.83 | 594.53 | 106.04 | 488.49 | 0.22 | 1.89 | 3.95 |
55 | 34.40 | 3303.40 | 0.01 | 0.30 | 2.58 | 0.30 | 1.63 | 1.65 | 0.59 | 7.07 | 4.70 | 75.92 | 31.84 | 143.46 | 30.89 | 256.87 | 34.93 | 60.12 | 1.80 | 12,740.00 | 3.13 | 592.72 | 7.04 | 585.68 | 0.01 | 0.53 | 2.12 |
Zircon Lu-Hf isotopic data of the samples.
Sample | 176Yb/177Hf | 2σ | 176Lu/177Hf | 2σ | 176Hf/177Hf | 2σ | Age (Ma) | εHf (t) | TDM1 (Ma) | TDM2 (Ma) | fLu/Hf |
---|---|---|---|---|---|---|---|---|---|---|---|
Z1220-23-2 | |||||||||||
4 | 0.001318 | 0.000015 | 0.000036 | 0.000001 | 0.282071 | 0.000014 | 518 | −13.4 | 1621 | 2326 | −1.00 |
12 | 0.008493 | 0.000140 | 0.000304 | 0.000002 | 0.282129 | 0.000031 | 519 | −11.39 | 1553 | 2202 | −0.99 |
14 | 0.002127 | 0.000070 | 0.000062 | 0.000002 | 0.282011 | 0.000038 | 531 | −15.27 | 1704 | 2453 | −1.00 |
19 | 0.001566 | 0.000012 | 0.000045 | 0.000001 | 0.282070 | 0.000015 | 550 | −12.72 | 1623 | 2309 | −1.00 |
27 | 0.001262 | 0.000010 | 0.000035 | 0.000000 | 0.282094 | 0.000012 | 518 | −12.58 | 1590 | 2276 | −1.00 |
31 | 0.001949 | 0.000068 | 0.000056 | 0.000002 | 0.282058 | 0.000016 | 518 | −13.86 | 1639 | 2355 | −1.00 |
Z1218-6 | |||||||||||
3 | 0.006438 | 0.000027 | 0.000273 | 0.000002 | 0.282511 | 0.000019 | 522 | 2.2 | 1028 | 1346 | −0.99 |
9 | 0.011279 | 0.000126 | 0.000466 | 0.000005 | 0.282498 | 0.000026 | 528 | 1.77 | 1052 | 1377 | −0.99 |
36 | 0.008736 | 0.000202 | 0.000374 | 0.000008 | 0.282415 | 0.000023 | 583 | 0.08 | 1164 | 1527 | −0.99 |
37 | 0.010024 | 0.000094 | 0.000430 | 0.000004 | 0.282470 | 0.000032 | 531 | 0.84 | 1090 | 1438 | −0.99 |
40 | 0.049057 | 0.000433 | 0.001851 | 0.000016 | 0.282433 | 0.000027 | 507 | −1.42 | 1184 | 1564 | −0.94 |
41 | 0.012529 | 0.000228 | 0.000534 | 0.000010 | 0.282627 | 0.000032 | 507 | 5.87 | 874 | 1101 | −0.98 |
44 | 0.008471 | 0.000075 | 0.000339 | 0.000003 | 0.282605 | 0.000025 | 561 | 6.32 | 900 | 1112 | −0.99 |
47 | 0.009077 | 0.000076 | 0.000397 | 0.000002 | 0.282390 | 0.000025 | 523 | −2.13 | 1198 | 1619 | −0.99 |
52 | 0.006321 | 0.000037 | 0.000242 | 0.000001 | 0.282493 | 0.000019 | 532 | 1.75 | 1052 | 1380 | −0.99 |
Z1230-42-4 | |||||||||||
1 | 0.015971 | 0.000678 | 0.000449 | 0.000019 | 0.282231 | 0.000018 | 516 | −7.92 | 1419 | 1981 | −0.99 |
3 | 0.003249 | 0.000154 | 0.000092 | 0.000005 | 0.281972 | 0.000015 | 537 | −16.52 | 1757 | 2534 | −1.00 |
9 | 0.002353 | 0.000029 | 0.000061 | 0.000001 | 0.282324 | 0.000022 | 542 | −3.94 | 1279 | 1750 | −1.00 |
27 | 0.005329 | 0.000286 | 0.000150 | 0.000009 | 0.281992 | 0.000020 | 522 | −16.18 | 1734 | 2503 | −1.00 |
34 | 0.008197 | 0.000586 | 0.000187 | 0.000011 | 0.282167 | 0.000038 | 523 | −9.96 | 1497 | 2114 | −0.99 |
39 | 0.002116 | 0.000023 | 0.000052 | 0.000001 | 0.282423 | 0.000015 | 541 | −0.46 | 1143 | 1528 | −1.00 |
41 | 0.003061 | 0.000069 | 0.000089 | 0.000002 | 0.282221 | 0.000020 | 550 | −7.41 | 1419 | 1973 | −1.00 |
46 | 0.005436 | 0.000141 | 0.000158 | 0.000004 | 0.282194 | 0.000026 | 533 | −8.78 | 1459 | 2046 | −1.00 |
50 | 0.002255 | 0.000041 | 0.000063 | 0.000001 | 0.282353 | 0.000026 | 509 | −3.65 | 1239 | 1705 | −1.00 |
52 | 0.015970 | 0.000362 | 0.000654 | 0.000013 | 0.282017 | 0.000015 | 535 | −15.18 | 1722 | 2450 | −0.98 |
Z1219-50-1 | |||||||||||
2 | 0.008867 | 0.000159 | 0.000311 | 0.000007 | 0.282166 | 0.000014 | 550 | −9.43 | 1504 | 2103 | −0.99 |
4 | 0.008980 | 0.000324 | 0.000289 | 0.000010 | 0.282177 | 0.000016 | 566 | −8.69 | 1487 | 2066 | −0.99 |
8 | 0.004610 | 0.000077 | 0.000148 | 0.000003 | 0.282152 | 0.000019 | 490 | −11.18 | 1516 | 2167 | −1.00 |
11 | 0.007078 | 0.000018 | 0.000211 | 0.000003 | 0.282179 | 0.000017 | 543 | −9.09 | 1481 | 2074 | −0.99 |
26 | 0.006352 | 0.000222 | 0.000212 | 0.000007 | 0.282219 | 0.000020 | 550 | −7.52 | 1426 | 1980 | −0.99 |
31 | 0.011156 | 0.000299 | 0.000383 | 0.000010 | 0.282130 | 0.000020 | 508 | −11.67 | 1556 | 2211 | −0.99 |
33 | 0.002440 | 0.000014 | 0.000080 | 0.000000 | 0.282189 | 0.000022 | 558 | −8.37 | 1463 | 2040 | −1.00 |
39 | 0.004478 | 0.000076 | 0.000148 | 0.000002 | 0.282148 | 0.000022 | 570 | −9.59 | 1521 | 2125 | −1.00 |
42 | 0.003002 | 0.000016 | 0.000095 | 0.000000 | 0.282149 | 0.000018 | 545 | −10.07 | 1518 | 2138 | −1.00 |
47 | 0.005546 | 0.000076 | 0.000174 | 0.000002 | 0.282222 | 0.000020 | 546 | −7.46 | 1421 | 1975 | −0.99 |
50 | 0.006224 | 0.000056 | 0.000196 | 0.000001 | 0.282185 | 0.000019 | 526 | −9.25 | 1472 | 2070 | −0.99 |
Z1230-45-2 | |||||||||||
2 | 0.001276 | 0.000013 | 0.000028 | 0.000000 | 0.282194 | 0.000014 | 549 | −8.35 | 1454 | 2033 | −1.00 |
16 | 0.042659 | 0.000347 | 0.001306 | 0.000018 | 0.282241 | 0.000024 | 597 | −6.16 | 1438 | 1930 | −0.96 |
24 | 0.007720 | 0.000462 | 0.000235 | 0.000016 | 0.282214 | 0.000014 | 569 | −7.31 | 1435 | 1981 | −0.99 |
29 | 0.008848 | 0.000371 | 0.000335 | 0.000014 | 0.282324 | 0.000013 | 570 | −3.43 | 1288 | 1738 | −0.99 |
47 | 0.004942 | 0.000119 | 0.000128 | 0.000003 | 0.282169 | 0.000020 | 561 | −9.01 | 1492 | 2084 | −1.00 |
55 | 0.014009 | 0.000141 | 0.000432 | 0.000005 | 0.282168 | 0.000024 | 559 | −9.2 | 1504 | 2092 | −0.99 |
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Abstract
Prydz Bay is an important part of the Pan-African high-grade tectonic mobile belt. The focus of this investigation, by applying zircon LA-ICP-MS U-Pb geochronology, zircon Lu-Hf isotope systematics, and whole-rock geochemistry, is on Pan-African pegmatites in the Larsemann Hills of Prydz Bay, East Antarctica, their association with country rocks, and the formation conditions. Based on the obtained results, it is concluded that the pegmatites exhibit elevated levels of silica and alkali and possess peraluminous features. These pegmatites originated during the late Neoproterozoic–Early Cambrian (Pan-African) event, specifically in the D2–D4 stages. The D2 stage occurred between 546 and 562 Ma, followed by D3-stage pegmatites around 534 Ma. The pegmatites from the D2–D3 stages are considered to originate from Paleoproterozoic crustal materials, while there are at least two phases of pegmatites in the D4 stage (~517 Ma and ~521 Ma). The D4-1 pegmatite (~521 Ma) suggested both Paleo–Mesoproterozoic crustal origin, perhaps connected to extension. The D4-2 pegmatite (~517 Ma) originated from the crust layers. In the Larsemann Hills, Pan-African pegmatites formed in a recurring regime of tension. Therefore, the obtained data elucidate that a Pan-African stretching process might have occurred in Prydz Bay.
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1 Polar Research Institute of China, Shanghai 200136, China;
2 Institute of Geology, Chinese Academy of Geological Sciences, Beijing 100044, China;