Canadian Journal of Earth Sciences
Zircon U-Pb Chronology, Geochemistry, and Petrogenesis of the High Nb-Ta Alkaline Rhyolites at the Tuohe Tree Farm, Northern Volcanic Belt, Great Xing’an Range, China
Journal: Canadian Journal of Earth Sciences
Manuscript ID cjes-2018-0332.R2
Manuscript Type: Article
Date Submitted by the 29-May-2019 Author:
Complete List of Authors: Sun, Guosheng; Jilin University Zhao, Tianxue; Jilin University, College of Earth Science Jin, Ruixiang; Jilin University Wang, Qinghai;Draft Jilin University Xingan Block, High Nb-Ta, Alkaline Rhyolite, Zircon U-Pb Chronology, Keyword: Geochemistry, Petrogenesis
Is the invited manuscript for consideration in a Special Not applicable (regular submission) Issue? :
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1 Zircon U-Pb Chronology, Geochemistry, and Petrogenesis of the High Nb-Ta
2 Alkaline Rhyolites at the Tuohe Tree Farm, Northern Volcanic Belt, Great Xing’an
3 Range, China
4 Guosheng Sun;Tianxue Zhao1;Ruixiang Jin;Qinghai Wang
5 College of Earth Science, Jilin University
6 Address of all authors: No.2199, Jianshe Street, Jilin University, Changchun, China
7 130061
Draft
1 Corresponding author (E-mail: [email protected]; Address: No.2199, Jianshe Street, Jilin University, China 130061; Fax: 0431-88502055; Tel: 15044096612) 1
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9 Abstract: We studied newly found high Nb-Ta alkaline rhyolites in the Northern
10 volcanic belt of the Great Xing’an Range, China. The LA-ICP-MS U-Pb weighted
11 mean age is 114.07±0.55 Ma, indicating that the rocks formed during the late Early
12 Cretaceous and were the product of the late eruption of a Mesozoic volcano. The
13 major element contents are characterized by high Si, rich K, low Fe, and poor Ca and
14 Mg. In the Total Alkaline–Silicon diagram, the sample points are in the alkaline
15 rhyolite region. Meanwhile, rare earth elements show obvious Ce/Ce* positive
16 anomalies and Eu/Eu* negative anomalies; in addition, trace elements are 17 characterized by high Nb, Ta, andDraft Yb and low Sr. The two stage Nd isotopic model
18 age T2DM of the depleted mantle is between 799–813 Ma, indicating that there
19 diagenetic material originated from the depleted mantle or partial melting of newly
20 formed young crustal materials. The source rocks melted at a relative shallow depth
21 (< 30 km), under lower pressure (< 0.5 Gpa) and high oxygen fugacity; moreover, the
22 residues in the source region were Ca-rich mafic plagioclase + amphibole +
23 orthopyroxene. In the Nb-Y-3Ga and Nb-Y-Ce diagrams, the sample points are in the
24 A1 type region. It can be concluded that the mantle-derived basaltic magma
25 underplated and supplied the heat sources for partial melting of the metamorphic
26 crustal rocks in an intraplate extensional tectonic environment related to a rift, mantle
27 plume, and hot spot.
28 KEYWORDS: Xingan Block, High Nb-Ta, Alkaline Rhyolite, Zircon U-Pb
29 Chronology, Geochemistry, Petrogenesis.
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30 Introduction
31 The Northern volcanic belt of the Great Xing’an Range is the superimposed part
32 of the ancient Asian oceanic tectonic domain, the Pacific domain, and the
33 Mongolia–Okhotsk oceanic domain(Wu et al. 2011; Xu et al. 2009; Zhou Jian-bo et
34 al. 2016). The area was subject to formation of the Xingan block metamorphic
35 basement during the Precambrian, closure of the paleo-Asian ocean and the
36 combination of several microcontinents during the Proterozoic (Zhang Xing-zhou et
37 al. 2006), and remote superposition and transformation caused by the closure of the
38 Mongolia–Okhotsk ocean and subduction of the paleo-Asian ocean plate (Ge 39 Wen-chun et al. 1999; Lin Qiang etDraft al. 1998; Ren Jisun et al. 1999; Shao Ji-an, Zhang 40 and Lu-qiao 1999; Wu et al. 2007; Zhao Guo-long et al. 1989). The area is widely
41 covered by Mesozoic mafic and felsic volcanic rocks. It is the largest Mesozoic
42 volcanic rock zone and an important metallogenetic belt of nonferrous metals as well
43 as rare and rare earth elements in China. Thus far, many controversies remain
44 regarding the dynamic background of the formation of the Great Xing’an Range
45 Mesozoic volcanic rock’s minerals and the nature of the magma source because of the
46 complex tectonic evolution and the superposition of multiple tectonic domains in the
47 study area (Chen Yan-jing et al. 2012; Fan et al. 2003; Ge Wen-chun et al. 1999; Lin
48 Qiang et al. 1998; Meng R 2003; Wang et al. 2007; Wu et al. 2011; Xu et al. 2009;
49 Zhang et al. 2008; Zhang et al. 2010; Zhao Yue et al. 1994). The origin of the
50 volcanic belt has been a high-profile issue and a focus of Chinese geologists.
51 During the 1:50,000 Mineral Geological Survey implemented over recent years,
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52 several widely distributed high Nb–Ta (alkaline) rhyolites were discovered in the
53 Great Xing’an Range, of which the Nb2O5 contents reach on average more than
54 0.03% with the highest content exceeding 0.06%. These values exceed the 0.02% of
55 industrial grade niobium tantalum ore deposits in China. The Nb and Ta contents in
56 the rhyolites are generally high and the rocks have not been superimposed or
57 reformed via later hydrothermal solutions. This shows that the Nb and Ta enrichment
58 was restricted by the nature of the source area and magmatic evolution. Recently, high
59 Nb-Ta alkaline rhyolite was discovered in the Baiyingaolao Formation in the northern
60 part of the Xingan block in the Great Xing’an Range. Many studies were completed 61 and are reported in this paper to provideDraft a constraint basis for the tectonic background 62 of the formation of the Great Xing’an Range volcanic rock belt and the nature of the
63 magmatic source through zircon U-Pb chronology and the geochemical characteristics
64 of the high Nb-Ta alkaline rhyolite.
65 Geological background and sample description
66 Geological background
67 The main volcanic belt in the Great Xing’an Range is west of the
68 Hegenshan–Heihe fault, east of the Xinlin–Xiguitu fault, and north of the
69 Xilamulun–Changchun paleo-Asian oceanic suture (Figure 1a), distributed in a NE
70 direction, the main part of which are the Great Xing’an Range w composed of
71 Mesozoic volcanic rocks. The Xingan block metamorphic basement is represented by
72 the Xinghua Ferry Group that formed from the Neoarchean to Proterozoic (Ge
73 Wen-chun et al. 2007; Şengör et al. 1993; Xu et al. 2009). It is composed of
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74 sillimanite-garnet bearing gneiss, felsic gneiss, amphibolite, graphite schist, and high
75 greenschist facies – high amphibolite facies metamorphic rocks (Chen Yan-jing et al.
76 2012; Zhao Yue et al. 1994). It underwent high-greenschist facies metamorphism and
77 high-breccia facies metamorphism (HBGMR, 1993). Proterozoic covers are mainly
78 distributed in the upper Heilongjiang depression in the northern Xingan block, but are
79 sporadically exposed in the western and south-central Xingan block;
80 Silurian–Devonian–early Carboniferous strata are continuously deposited marine
81 facies or shallow-marine facies and the late Carboniferous palaeogeographic pattern
82 includes continental sediments to the north and marine sediments to the south (Zhou 83 Jian-bo et al. 2016). The Jurassic rocksDraft in the Mesozoic – Cretaceous basic and acidic 84 lava and pyroclastic rocks are exposed widely in the Xingan block, including the
85 following groups from oldest to youngest: the Tamulangou (J2tm), Manketouebo
86 (J3mk), Manitu (J3mn), Baiyingaolao (K1b). and Meiletu groups (K1ml) according to
87 the lithology and eruption age. The Tamanguou Formation (J2tm) is the lowest part of
88 the Mesozoic Daxing 'anling volcanic belt of Middle Jurassic age. Its lithology is
89 mafic-intermediate volcanic rocks with normal sedimentary rocks. The Manketou
90 Obo formation (J3mk) is discordant from the Tamangou Formation (J2tm) of early
91 Late Jurassic age and its lithology is mainly acid volcanic lava and acidic volcanic
92 clastic lava. The Manitou Formation concordantly overlies the Manketou Obo
93 Formation (J3mk) of late Late Jurassic age. Its lithology is neutral (dacitic – andesitic)
94 volcanic lava and volcanic clastic lava. The Baiyingaolao Formation disconcordantly
95 overlies the Manitu Formation of early Early Cretaceous age. Its lithology is acidic
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96 lavas and acidic volcanic clastic lava with normal sedimentary rocks. The Meiletu
97 Formation (K1ml) disconcordantly overlies the Baiyingaolao Formation. It is mainly
98 composed of a set of intermediate-basic volcanic rocks, including fumarolic
99 amygdaloid or dense massive trachy andesite, basalt, etc. (Regional geology of Inner
100 Mongolia, 1991. According to lithologic characteristics and zircon U-Pb dating, the
101 high Nb-Ta alkaline rhyolite studied in this paper was found in early Cretaceous
102 stratum of the Baiyingaolao Formation in the northern part of the Xingan block; it is
103 the upper effusive facies lithologic member (Figure 1b).
104 Sample description 105 The high Nb-Ta alkaline rhyolitesDraft are exposed in the western Tuohe Tree Farm in 106 the Kyihe county of the Oroqen Autonomous Banner. East longitude 122°34′20″,
107 north latitude 50 ° 18 ′ 28 ″ .The rhyolites are belt-like and distributed in a NNW
108 direction in an area of 3 km2. They form a parallel unconformable contact with the
109 underlying late Jurassic andesite of the Manitu group to the west and south, cover the
110 early Cretaceous rhyolitic debris-crystal tuff of the Baiyingaolao Formation to the
111 north, and are covered by Quaternary rocks to the east (Figure 1).
112 The fresh surface of the alkaline rhyolite is grayish purple or gray white with
113 porphyritic, rhyolitic, and massive structure (Figure 2). Approximately 8% of the rock
114 is phenocrysts composed of sanidine, quartz, and minor biotite. The sanidine shows
115 euhedral-subhedral plating with micro cracks developed, mostly showing a
116 porphyritic or glomero-porphyritic texture, and biaxial crystals (2V = 63°). It is a type
117 of high temperature sanidine with a weak stripe structure visible and Cartesian double
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118 crystal or Manebach twins locally containing oligoclase; the diameter of the sanidine
119 is 1–2 mm and the content is 5%. The quartz shows xenomorphic granulation and a
120 diameter of 0.5–1 mm; its content is approximately 3%.
121 Biotite, pyrochlore, and ilmenite – magnetite occasionally occur in the alkaline
122 rhyolite. Biotite is flaky, brown, palm red and reddish brown; some biotite minerals
123 have darkened edges. The biotite shows parallel extinction, a group of perfect
124 cleavage, and is 0.1–0.5 mm in particle size. The pyrochlore is dark brown and
125 reddish brown, extremely convex, irregularly granular, and 0.1–0.5 mm in particle
126 size. The Nb - Ta mainly occurs in the pyrochlore (Fig. 2c) and titanomagnetite (Fig.
127 2d). Electron probe test results showDraft that the Nb2O5 content in the titanomagnetite 128 reaches 1.89%–2.28%. The matrix has a coarse-to-fine structure, a micro-embedded
129 crystal-containing structure, and a particle structure. Alkali feldspar microcrystals,
130 quartz, and dusty ilmenite are arranged in a semi-parallel arrangement.
131 Sample analysis methods
132 Analyses of major and trace elements were completed at the Jilin University Test
133 Center. The determination of major elements was as follows: first, we chose seven
134 fresh rock samples; second, we crushed them to less than 200 mesh using an agate
135 mortar; third, samples were melted into glass cake; finally, we determined major
136 elements using an XRF-1500X fluorescence spectrometer with an analytical precision
137 of approximately 1%. However, the determination of trace elements was as follows:
138 first, we weighed 40 mg samples and placed them into a Teflon tank; second, we
139 added HF and HNO3 and thoroughly dissolved them; third, we diluted the sample
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140 with 1% HNO3; finally, we determined the trace and rare earth elements using the
141 dual focus inductively coupled plasma mass spectrometer (ICP-MS) ELEMENT
142 produced by Finnigan-MAT company with an analytical precision greater than 5%.
143 The zircon particles in good crystal form and standard samples for dating were
144 separated using the conventional gravity and magnetic separation method and selected
145 using a binocular microscope. Then, they were immediately placed into a colorless
146 and transparent epoxy resin and turned into targets after solidification. Then, the
147 targets were polished until the central part of the zircon was exposed. The zircon
148 sample in good crystal form was chosen for cathodoluminescence (CL) photography 149 using the Mono CL3+ CathodoluminescenceDraft System produced by British Gatan 150 company. CL photography was completed at the Laboratory of Tianjin Institute of
151 Geology and Mineral Resources. Laser Ablation Inductively Coupled Plasma Mass
152 Spectrometry (LA-ICP-MS) zircon dating was completed at the Laser Plasma Mass
153 Spectrometry Laboratory at the China University of Geosciences (Beijing campus)
154 using the laser plasma mass spectrometer that was a combination of the 193=nm laser
155 denudation injection system (UP 193SS) produced by the American New Wave
156 company and the Aglient7500a type four-stage bar plasma mass spectrometer
157 produced by the American AGILENT Technology Co., Ltd. During the experiment,
158 the laser working frequency was 10 Hz; the beam diameter of the test point was 30
159 μm; the pre-ablation time was 5 s; the ablation time was 45 s; and high purity He gas
160 denudation material was used as the carrier gas stream (the flow rate was 0.88 L/min)
161 The isotopic ratio was used to normalize based on the standard zircon 91500 as the
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162 external standard. The blind samples included standard zircon TEMORA and Qinghu.
163 The age was calculated via the international standard program Isoplot. The zircon
164 U-Pb isotopic ratio was determined using ICP-MS and calculated via the Glitter
165 program. The elemental content in the zircon was determined based on the
166 international standard NIST610 which acted as the external standard and Si which
167 acted as the internal standard; the blind samples included NIST612 and NIST614. The
168 error of every single data point was 1σ, the weighted mean value error was 2σ, and
169 the average age was calculated using the 206Pb/238U age.
170 The Sr and Nd isotopic tests were completed at the laboratory of the Tianjin 171 Institute of Geology and Mineral Resources.Draft The samples were dissolved using mixed
172 acid (HF+HClO4) and attacked for more than 12 h under high-temperature conditions
173 in a closed Teflon dissolving device. Then, Sr, the output of the Isotope Concentration
174 (IC) process, was purified a second time. The purification of Nd was supported by the
175 Di-(2-ethylhexyl)phosphoric acid (HDEHP) color layer technology. The content and
176 isotopic ratio were all determined using Triton thermo-ionization mass spectrometry.
177 The level of the system blank of the whole process was stable at the following values:
178 Rb = 5.6×10-10 g, Sr = 3.8×10-10 g, Sm = 3.0×10-11 g, Nd = 5.4×10-11 g. During the
179 sample testing, the Nd-Sr isotopic ratios of the BCR-1 Nd standard samples and
180 NBS-607 Sr standard samples were as follows: 143Nd/144Nd = 0.512739±5 (±2σ)
181 and87Sr /86Sr = 1.200050±5 (±2σ), respectively. The Sr and Nd isotopic test data were
182 exponentially processed with mass fractionation correction in which the internal
183 standards are as follows: 88Sr /86Sr = 8.37521 and 146Nd/144Nd = 0.7219.
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184 Results
185 Zircon U-Pb dating and trace element characteristics
186 Twenty-nine zircon samples were selected from the alkaline rhyolite for LA-ICP-
187 MS U-Pb dating. The samples appeared pink brown, showing a
188 hypidiomorphic-euhedral short column texture, and the crystal form was mainly a
189 combination form composed of {100}+{110}+{111} and
190 {110}+{110}+{311}+{131}. The particle sizes were mostly between 0.1 and 0.25
191 mm, with a ratio of length to width between 1:1 and 3:1. It can be seen from the CL
192 photo (Figure 3) that the zircon show an oscillatory zoned structure of magmatic 193 origin whose Th/U ratio was betweenDraft 1.1 and 2.2 (Table 2). It also shows the typical 194 characteristics of magmatic crystallized zircon (Belousova et al. 2002; Koschek
195 1993). Zircon has a high rare earth element content and the total amount of rare earth
196 elements (∑REE) was 1912–3399 µg/g. The ratio of LR/HR was 0.09–0.21, implying
197 significant REE fractionation. In the chondrite-normalized partition diagram of rare
198 earth elements, the samples are inclining to left (Figure 4a), implying a significant
199 enrichment in heavy rare earth elements (HREEs). There are obvious Ce/Ce*
200 (Ce/Ce*=9-384) positive anomalies and Eu/Eu* (Eu/Eu*=0.26–0.29) negative
201 anomalies, consistent with the characteristics of REEs in crustal source magmatic
202 zircons (Hoskin and Schaltegger 2003). Strong Ce/Ce* positive anomalies suggest
203 that the high Nb-Ta alkaline rhyolite formed under an environment of higher oxygen
204 fugacity(Burnham and Berry 2012; Mass et al. 1992); the element Eu should occur
205 as Eu3+ when the magma has high oxygen fugacity and cannot be fractionated from
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206 other trivalent rare earth elements; thus, the Eu/Eu* negative anomaly is the
207 inheritance of the low Eu content in the magma. The zircon 206Pb/238U ages of 29
208 sample points are between 111 and 116 Ma (Table 2); in zircon U-Pb dating
209 harmonious graphs (Figure 4b), the data points are centrally distributed and on or
210 near the harmonious line. A weighted average 206Pb/238U age of 114.07±0.55 Ma
211 (MSWD = 0.63, n = 29) (Table 2, Figure 4b) shows that the eruption age of the
212 rhyolite is late Early Cretaceous.
213 Characteristics of major and trace elements
214 Major elements 215 The major element contents inDraft the high Nb-Ta alkaline rhyolite are characterized
216 by high Si, rich K, low Fe, and poor Ca and Mg. The SiO2 content in the rock is
217 between 72.35% and 73.22%, indicating that the rock is acidic; moreover, the Al2O3
218 content is 13.18%–13.60% and the aluminum saturation index A/CNK is 0.88–1.05,
219 indicating that the rock is quasi-aluminous. Total alkali (K2O+Na2O) content varies
220 between 9.39% and 11.43%, showing that the rock is obviously alkaline rich. The
221 K2O/Na2O ratio is 1.03–2.16 with an average of 1.52, implying that the rhyolite is
222 potassic; the FeOT contents (1.53%–2.35%) are low while the CaO (0.12%–0.18%),
223 TiO2 (0.19%), and MgO contents (0.04%–0.08%) are lower. In the SiO2-Na2O+K2O
224 silicon-alkali diagram (Figure 5a), the rhyolite samples are above the
225 alkaline-subalkaline boundary in the rhyolite region, indicating that are alkaline
226 rhyolite. In the discrimination diagram of A/CNK-A/NK aluminum saturation (Figure
227 5b), the sample points are in the peralkaline region, and in the SiO2- K2O diagram
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228 (Figure 5c), the sample points are in the shoshonite series region. There is standard
229 mineral quartz in the CIPW standard minerals calculations (22.56%–23.93%),
230 showing that the rock is silicon saturated or oversaturated. The K-feldspar contents
231 (Or) (32.72–46.35) and albite (Ab) (24.75–37.87) in the standard minerals are high
232 and anorthite (An) was not found, consistent with the characteristics of rich alkalinity
233 and poor Ca. Acmite (Ac) (2.92–3.15) and sodium silicate (Ns) (0.29–1.08) occurs,
234 but no alkaline minerals such as alkaline pyroxene or alkaline amphibole are found.
235 Trace elements
236 The total REE content in the rock (ΣREE) is high, from 86.87×10-6 to 161.72×10-6
237 (Table 3, Figure 6a). The LREE/HREEDraft ratio is 3.40–6.87 and the LaN/YbN ratio is 238 3.76–4.54; thus, there was moderate fractionation between LREE and HREE. The
239 ratios of LaN/SmN are 2.87–5.85; thus, there was significant LREE fractionation. The
240 total HREE content is high, 10 times higher than that of the standard chondrite; the
241 ratios of GdN/YbN (0.54–0.80) suggest the enrichment of HREEs and weak
242 fractionation (Figure 6a). The Sr/Y ratio (0.04–0.35) was also low, indicating that a
243 large number of garnet minerals that were primarily stable under the high-pressure
244 condition in the magma source area melted during a later period The diagenetic
245 pressure is low while the depth is very shallow (Evans and Hanson 1993; Hanson
246 1978); YbN (23.76) > HoN (21.95), showing a slight loss in medium rare earth
247 elements (MREEs) and suggesting that there was residual amphibole in the source
248 area. The Ce/Ce* ratio is between 1.05–1.31, a positive anomaly, indicating that the
249 rocks formed in a strong oxidizing environment or there was an inheritance of high Ce
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250 minerals in the source area. The strongly depleted Eu/Eu* ratio (0.39–0.44) and low
251 Ca content in the major elements imply that basic plagioclase rich in Ca was the main
252 residual in the source area.
253 It can be seen from the trace element spider diagrams (Figure 6b) that Rb, Nb, Ta,
254 Zr, Hf, Th, and U are quite enriched in the rocks, but Ba, Sr, P, and Ti are obviously
255 depleted. NbN and TaN, the primitive mantle standardization value of Nb and Ta in the
256 rocks, is 153.04–177.70 and 143.75–343.0, respectively, suggesting obvious
257 enrichment of Nb and Ta and indicating that the rocks are high Nb-Ta alkaline
258 rhyolites. The Nb2O5 + Ta2O5 content ranges from 0.026% to 0.031%, reaching and 259 exceeding the industrial grade of 0.02%Draft of niobium tantalum ore in China. The Nb/Ta 260 ratio of the rock is 7.2–14.9, lower than that of the primitive mantle (Nb/Ta=17.5)
261 (Jochum et al. 1997; Mc Donough and Sun 1995; Sun and Mc Donough 1989) and
262 falling in the Nb/Ta ratio range of continental crust (Nb/Ta=10–14). The Zr and Hf
263 contents in the rhyolite are high, among which, the Zr content is as high as 447.9×10-6
264 – 543.7×10-6, suggesting that zirconium-rich minerals such as zircon were
265 concentrated and melted in the source region. The contents of basic compatible
266 components such as Co (0.18×10-6–0.24×10-6), Ni (0.01×10-6–0.77×10-6), and Cr
267 (0.07×10-6–0.41×10-6) are low; the Sr content in the rock is 1.86×10-6–8.8×10-6, <
268 100×10-6, and the Yb content is 3.35×10-6 – 4.65×10-6, > 2×10-6, suggesting that the
269 rock is an 'extremely low Sr and high Yb' type (Zhang Qi et al. 2006) rhyolite. The
270 low Sr also suggests that there was plagioclase residual in the source area while the
271 high Yb implies that garnet is a molten phase in the source region. The Rb/Sr ratios
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272 (27.05–135.23>10) and Th/U ratios (4.57–7.77) of the rocks are all high, implying
273 that the source rocks of the alkaline rhyolite were continental crust materials.
274 Characteristics of Sr and Nd isotopes
275 We completed tests and analyses of the compositions of the Sr and Nd isotopes of
276 the four alkaline rhyolite samples in the study (Table 4). The results are as follows:
277 the ratio of Rb/Sr is 199.72–208.95 while the ratio of Sm/Nd is 0.12–0.16, indicating
278 that the alkaline rhyolite is characterized by high Rb/Sr and low Sm/Nd. ISr, the initial
279 ratio of the Sr isotope, is 0.70437–0.72621, while the εSr(t) value is -0.01–310.6.
280 Moreover, the ISr and εSr(t) values of the four samples vary greatly; among the four
281 samples, the εSr(t) values of three Draftsamples are all positive but one is negative. The ISr 282 values of one sample are 0.7040–0.7060 while those of the other three samples are far
143 144 283 greater than 0.7060. INd, the initial ratio of Nd/ Nd, is 0.512553–0.512590 and the
284 εNd(t) values are positive (1.2–1.9), the same as those of the continental crust derived
285 granite in the Xingmeng orogenic belt (Mass et al. 1992; Shao and Zhang 1999). The
286 characteristics of the Sr and Nd isotopes indicate that there was not only
287 mantle-derived materials but also crustal materials in the magmatic source area. The
288 two-stage Nd isotopic model age T2DM of the depleted mantle is between 799 and 813
289 Ma, similar to the model age of the granites in the Center Asia Orogenic Belt which is
290 dominantly between 600–800 Ma (Guo Zhi-jun et al. 2014; Hong Da-wei et al. 2000;
291 Zhao Zhen-hua et al. 2008). The T2DM value is much greater than the formation age of
292 the high Nb-Ta alkaline rhyolite, showing that the formation of the rocks is related to
293 partial melting of crustal materials. In a word, the source rocks of the high Nb-Ta
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294 alkaline rhyolite were crust composed of mantle materials, basalt, and sedimentary
295 clastic rocks.
296 Discussion
297 Diagenetic age, petrogenesis type, and tectonic setting
298 Diagenetic age
299 The Mesozoic volcanic rocks of the Great Xing’an Range include the Tamulangou
300 (J2tm), Manketouebo (J3mk), Manitu (J3mn), Baiyingaolao (K1b) and Meiletu groups
301 (K1ml) from oldest to youngest (GMBIM, 1996), formed during the period 122–173
302 Ma (Chen Zhi-guang et al. 2009; Meng En et al. 2011; Xu Mei-Jun et al. 2011; Xu 303 Wen-liang et al. 2008; Zhang Ji-hengDraft 2009; Zhang et al. 2010; Zhang et al. 2008). 304 The volcanic eruptions can be divided into three stages: early Late Jurassic (159–162
305 Ma), early Early Cretaceous (141–139 Ma), and late Early Cretaceous (123–127
306 Ma)(Gou Jun et al. 2010; Wang Jian-guo et al. 2013). "Regional Geological
307 Chronicles of the Inner Mongolia Autonomous Region" (1993(IMBGMR, 1991)and
308 "Lithostratigraphy of the Inner Mongolia Autonomous Region" (1996) (GMBIM,
309 1996) determined the formation age of the rocks in the Baiyingaolao Formation to be
310 Late Jurassic because detailed high-precision chronological data were not available at
311 that time. During recent years, zircon LA-ICP-MS U-Pb chronology study of the
312 Baiyingaolao Formation indicated that the formation age of the volcanic rocks in the
313 Baiyingaolao Formation is 125–144 Ma (Gou Jun et al. 2010; Huang Ming-da et al.
314 2016; Nie Li-jun et al. 2015; Si Qiu-liang et al. 2015; Wang Jian-guo et al. 2013;
315 Zhang Le-tong et al. 2015; Zhang Xiang-xin et al. 2016; Zhang Xue-bin et al. 2015),
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316 i.e. the Early Cretaceous. The high Nb-Ta alkaline rhyolite of the studied Tuohe Tree
317 Farm is in parallel unconformable contact with the underlying Late Jurassic rocks of
318 the Manitu group, covering the rhyolitic debris–crystal tuff and continuous sediments
319 of the upper part of the Baiyingaolao Formation. The magmatic zircon U-Pb age of
320 the rhyolite is 114.07±0.55 Ma, showing that the formation age of the alkaline
321 rhyolite is late Early Cretaceous. Compared to the formation age of the Baiyingaolao
322 Formation volcanic rocks in the Great Xing’an Range in previous studies (>122 Ma),
323 the alkaline rhyolite formed later (114 Ma) and was the product of late volcanic
324 eruptions of the volcanic rock belt in the Great Xing’an Range. 325 Petrogenetic type and tectonic settingDraft 326 Some researchers believe that after suturing of the north China plate and the
327 Siberian craton along the Xilamulun–Changchun suture from the late Late Permian to
328 early Early Triassic (Li Jin-yi et al. 2007; Liu Jian-feng et al. 2016; Wang Cheng-wen
329 et al. 2008), the Great Xing’an Range region had completed the transformation from
330 the paleo-Asian oceanic domain to the superposition of the circum-Pacific tectonic
331 domain and the Mongolia–Okhotsk oceanic tectonic domain during the
332 Mesozoic–Cenozoic (Ge Wen-chun et al. 1999; Lin Qiang et al. 1998; Ren Jisun et al.
333 1999; Shao Ji-an et al. 1999; Wu et al. 2007; Zhao Guo-long et al. 1989). However,
334 until now, direct evidence of subduction of the paleo-Pacific plate along the eastern
335 margin of the Eurasian plate during the early and middle Mesozoic has not been found
336 in eastern China and East Asia (Sao Ji-an et al. 2001). Zhao et al. (1994) and Xu et al.
337 (2013) suggested that it was mainly the Songliao Basin and its eastern region in
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338 Northeast Asia that were influenced by the Mesozoic circum–Pacific tectonic system,
339 while the western Songliao Basin such as the Xingan block and the north margin of
340 north China were mainly influenced by the Mongolia–Okhotsk oceanic tectonic
341 system. However, many controversies remain regarding the subduction direction and
342 closure time of the Mongolia–Okhotsk ocean (Chen Zhi-guang et al. 2010; Huang
343 Ming-da et al. 2016; Jiang Si-hong et al. 2010; Li Jin-yi et al. 2007;Liu Jian-feng et al.
344 2016; Nie Li-jun et al. 2015; Sao Ji-an et al. 2001; Wang Cheng-wen et al. 2008; Xu
345 Wen-liang et al. 2013; Zeng Wei-shun et al. 2014; Zhang Xiang-xin et al. 2016).
346 Some researchers believe that both the formation of the Triassic porphyry Cu-Mo 347 deposits in the Ergun block and Draft the formation of the Triassic granite in the north 348 segment of the Ergun block are related to the subduction of the Mongolia–Okhotsk
349 ocean to the south (Chen Zhi-guang et al. 2010; Jiang Si-hong et al. 2010; Wu et al.
350 2011; Zeng Wei-shun et al. 2014) and have speculated that the Mongolia–Okhotsk
351 ocean was closed during the Triassic (Jiang Si-hong et al. 2010) while others
352 suggested during the late Jurassic–early Cretaceous (Cogné M et al. 2005;
353 Kravchinsky et al. 2002; Metelkin et al. 2010; Parfenov et al. 2001; Pei et al. 2011;
354 Zonenshain et al. 1990).
355 Major elements of the high Nb-Ta alkaline rhyolite in the Tuohe Tree Farm are
356 characterized by rich Si and K and poor Ca and Mg while trace elements are quite
357 enriched in Rb, Th, Nb, Ta, Zr, Hf, Ga, and Y but depleted in Sr, Ba, Ti. and P. The
358 chondrite-normalized partition curve of the REEs varies as a 'V' type with obvious Eu
359 negative anomalies, with the same typical chemical composition as an A-type granite
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360 (Collins et al. 1982; Ge Wen-chun et al. 2005; Zhang Qi et al. 2012; Zhao Zheng-hua
361 et al. 1997). In the tectonic environment discriminated diagrams(Figure 7a,b,c), the
362 rock samples are in the intraplate granite region, indicating that the alkaline rhyolite
363 was formed in an intraplate extensional tectonic environment.The 10,000 Ga/Al ratio
364 is between 3.81–4.04, higher than the lower limit ratio of an A-type granite(i.e. 2.6).
365 In the rhyolite genesis discrimination diagram of 10,000 Ga/Al (Figure 8a, b, c, d), the
366 rock samples are all in the A-type granite region. In the Nb-Y-3Ga and Nb-Y-Ce
367 diagrams for discrimination of A1 and A2 tectonic settings (Eby 1992; Whalen et al.
368 1987), the sample points are all in the A1=type region (Figure 8e, f), indicating that 369 the alkaline rhyolite formed inDraft an intraplate extensional and not in a tensional 370 tectonic environment developed by post-collisional or post-orogenic continental crust
371 collapse. The eruption of the 'extremely low Sr, high Yb' A1 type alkaline rhyolite
372 implies that the Xingan block was in an intraplate non-orogenic period during the late
373 Early Cretaceous (114 Ma), indicating that the Mongolia–Okhotsk ocean closed
374 before the early Cretaceous. Based on this, it is speculated that the closing time of the
375 Mongolia–Okhotsk Ocean occurred during the Late Jurassic.
376 Nature of the magmatic source
377 The A-type granite formed under alkali rich, anhydrous, and non-orogenic
378 conditions (Loiselle M C and Wones D, 1979; Zhang Qi et al. 2012). The anhydrous,
379 high-viscosity A-type granitic magma and a small density difference between the
380 rock-forming minerals and granitic magma was not able to support large-scale
381 crystallization differentiation (Reid J B J et al. 1993; Zhang Qi et al. 1993); moreover,
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382 cumulates associated with the high Nb-Ta alkaline rhyolite and the synchronous
383 intermediate–basic igneous rocks were not found in the study area, indicating that the
384 rock was not formed via crystallization fractionation of mantle-derived magma. In the
385 La/Sm–La diagram (Figure 9a) to discriminate the magmatic process, the sample
386 points are distributed along the oblique line, showing that the diagenetic process was a
387 type of partial melting. Major elements in the rock are characterized by rich Si and K
388 and poor Ca and Mg while trace elements are quite enriched in Rb, Th, U, K, and Pb
389 but depleted in Ba, Sr, P, Ti, Co, Ni, and Cr The rock shows a Ce positive anomaly
390 and the εSr(t) value is between -18.21 and 102.94 All of these characteristics show 391 that the source rocks were alumina-richDraft ancient crust or originated from basic upper 392 crust (King et al. 1997; Wang Jian-guo et al. 2013). It is generally accepted that
393 aluminous A-type granite should form via partial melting of lower crust rich in Al
394 (Patino Douce 1997; Rajesh 2000), which is seemingly not consistent with the
395 geochemical characteristics of low Al content in alkaline rhyolite. However,
396 quasi-aluminous A-type granite can form via partial melting of lower crust rich in Al
397 because of the formation condition of alkaline A-type granite and the residues of the
398 Al-rich minerals in the source area. The residual phases of a partial melting
399 experiment on the A-type granite were mainly basic plagioclase rich in Ca +
400 orthopyroxene (Litvinovsky et al. 2000; Patino Douce 1997; Skjerlie and Johnston
401 1992; Turner Sand Rushmer T, 2010); this and the depletion of in the rock suggests
402 that there was residual amphibole in the source area. Ca-rich basic plagioclase and
403 amphibole are minerals rich in Al whose large-scale residues in the source area
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404 caused Al depletion in the magmatic lava and the formation of low-Al
405 quasi-aluminous A-type granite. Therefore, the source rock did not exclude the
406 Al-rich ancient crust.
407 Among the main characteristics of the alkaline rhyolite in the Tuohe Tree Farm is
408 the enrichment of Nb and Ta. In general, Nb and Ta mainly occur in Ca and Ti
409 minerals, such as rutile, sphene, perovskite, titanium (magnetic) iron ore, and allanite,
410 and secondarily exist in Fe and Mg minerals, such as pyroxene, amphibole and biotite
411 (Hong Da-wei et al. 2000). Because the rhyolite is poor in Ca, Ti, Fe, and Mg, the
412 source of Nb-Ta should be independent of Ca, Ti, Fe, and Mg minerals. The Nb 413 contents in the rocks increase as theDraft lithology changes from basic rock to acidic rock 414 and to alkaline rock, and among those rocks, the Ta content in acidic rock is the
415 highest; thus. it is difficult to explain why the Nb contents (99.57×10-6–85.7×10-6) and
416 Ta (5.75×10-6–13.72×10-6) are high in the alkaline rhyolite suing the reason of partial
417 melting of the volcanic rock. However, during the process of rock weathering, Nb, Ta,
418 and Zr tend to be enriched in hydrolytic sediments and terrigenous Nb, Ta, and Zr
419 placer can also form on river beds and coastlines. According to statistics,
420 approximately 24% of the world's Nb and Ta production originates from placer
421 deposits (Mou Bao-lei, 1999). It is speculated that continental or terrigenous
422 meta-sandstone or mudstone rich in Nb and Ta occurred in the Al-rich ancient crust.
423 Ce/Ce* positive anomalies in rock imply that the source rocks might be
424 terrigenous meta-sandstone or mudstone, not crustal or marine sediments. Volcanic
425 rocks typically show a Ce zero anomaly or weak negative anomalies. In marine
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426 sediments, sediments in the middle ridge regions of the ocean (Ce/Ce*=0.29) and in
427 basin areas (Ce/Ce*=0.55) show negative anomalies medium or above, except that the
428 oceanic ferromanganese crusts (nuclei) of colloidal genesis show an obvious Ce/Ce*
429 positive anomaly. The continental margins show Ce weak negative anomalies or
430 positive anomalies (0.90–1.30) (Murry et al. 1990; Zhao Zheng-hua and Zhou ling-li,
431 1997), indicating that Ce was relatively enriched in the continental or terrigenous
432 sediments. The rock is characterized by low Fe and Mn, showing that the Ce/Ce*
433 positive anomaly is not related to oceanic ferromanganese crusts (nuclei) and also
434 implying that the source rocks were not subducted oceanic crust but related to 435 terrigenous sediments. The Zr contentDraft (447.9×10-6–543.7×10-6) in the rocks is high, 436 implying that Zr and other Zr-rich minerals are enriched and melted in the source
437 region. The trace element analytical data (Table 1) show that the Ce content in the
438 zircon is relatively high and there are obvious positive Ce anomalies. To some extent,
439 the Ce positive anomaly in the rhyolite is an inheritance of the Ce positive anomaly in
T T 440 the zircon. In the SiO2-(FeO +MgO+TiO2) / FeO +MgO+TiO2 melting test diagram
441 to distinguish the nature of the source area (Patino Douce AE, 1999) (Figure 9b), the
442 sample points are at the intersection of the argillaceous rock trend line and basalt
443 trend line.
444 In addition, basic crustal materials are also involved in the magmatic source; INd,
445 the initial ratio of 143Nd/144Nd,is 0.512537–0.512539 and the εNd ( t ) value is
446 positive (1.9–2.0), while the εSr(t) value of a sample is -0.01. All of these results
447 imply that the source rock is from melting of basalt, a basic lower crust material
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448 derived from the mantle. Therefore, the source rocks of the high Nb-Ta alkaline
449 rhyolite should have originated from a magmatic source composed of Al-rich crustal
450 materials, basic crustal materials, and basalt. The two-stage Nd isotopic model age
451 T2DM of the depleted mantle is between 754–813 Ma, consistent with the
452 Neoproterozoic magmatic-thermal event of the Xingan block basement and the
453 formation age of the Khondalite in the Xingan block (Zeng Wei-shun et al. 2014;
454 Zhou Jian-bo et al. 2016). The Al-rich schist – gneisses and amphibolites of the
455 Xinghua ferry group in the Xingan block metamorphic basement are metamorphic
456 crustal rock (HBGMR, 1993; Wu et al. 2012; Zhou Jian-bo et al. 2016; Zhou et al. 457 2011a) whose formation age is betweenDraft 660–970 Ma (Miao Lai-cheng et al. 2003; 458 Zhou and Wilde 2013: Zhou et al. 2011b). Geochemical characteristics show that the
459 chemical composition characteristics of rare earth elements (Figure 10a) and trace
460 elements (Figure 10b) are similar to rhyolite. The chemical composition
461 characteristics and variation trend of the Al_rich schist_gneiss are closer to the
462 rhyolite(Figure10). The source rocks of the Al-rich schist–gneisses were mudstone
463 and sandstone, with Eu negative anomalies (δEu = 0.32–0.79) and Ce/Ce* positive
464 anomalies (0.90–1.30), indicating that the sedimentary environment of the Al rich
465 schist– gneisses was a metastable continental margin sedimentary environment. In
466 addition, the source rock of the amphibolites was weakly alkaline basalt (Dong Ce
467 and Zhou Jian-bo, 2012; Zhou Jian-bo et al. 2016). The metamorphic crustal rocks are
468 typical volcano sedimentary formations including sedimentary rocks composed of
469 metamorphic basic volcanic rocks and metamorphic terrigenous clastic rocks (Biao
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470 Shang-hu et al. 1999; Liu Xiao-guang, 2007; Sun Guang-rui et al. 2002; Wei-wei et al.
471 2016). The metamorphic crustal rocks composed of low alkaline basalt and
472 terrigenous clastic rocks in the Neoproterozoic Xinghua ferry group show
473 characteristics of mantle and crust material origin and their formation age and
474 geochemical characteristics are in accordance with those of the source rocks of the
475 high Nb-Ta alkaline rhyolite.
476 Physico-chemical conditions of the source area
477 The zircon saturation temperature of granitic magma can be calculated from the Zr
478 content and major elements in the rock by means of the following formula:
479 TZr=12900/[2.95+0.85M+ln(496000/ZrDraftmelt)] (Watson E B and Harrison T M ,1983), in 480 which 'T' is the absolute temperature, 'M' is the number of moles of
481 (Na+K+2Ca)/(Al×Si); Si+Al+Fe+Mg+Ca+Na+K+P = 1 (mole fraction) in the
482 calculation; and Zrmelt is the Zr content in the magma. The aforementioned formula
483 was used to calculate the zircon saturation temperature of six samples, which was
484 866℃–924℃ with an average of 881℃. The zircon saturation temperature can be a
485 good estimation of the magmatic emplacement temperature because zircon begins to
486 crystallize during the beginning of magma evolution and consequently the zircon
487 saturation temperature is near the magmatic liquidus. In addition, the zircon saturation
488 temperature can be approximated as the temperature of magma formation given the
489 approximate adiabatic rising and emplacement of granitic magma.
490 The poor Al, Ca, and Sr of the rock, and strong Eu/Eu* negative anomalies,
491 indicate that the residual phase of the magmatic source was plagioclase; the stability
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492 of plagioclase in the source area mainly depended on the pressure (Martin H et al.
493 2005), which was lower than 0.8 Gpa. The residue phase of basalt melting is
494 plagioclase + amphibole ± orthopyroxene ± ilmenite (no garnet)(Wu et al. 2002);
495 However, for the high Nb - Ta alkaline rhyolite in Tuohe Tree Farm, the pressure
496 under which the ‘very low Sr, high Yb’ A-type granitic magma formed might have
497 been much lower (<0.5 Gpa) (Zhang Qi et al. 2006). It is generally accepted that
498 A-type granite is low-oxygen-fugacity granite (Martin 2006; Reid et al. 1993; Wang
499 Yang et al. 2013); however, Anderson J L et al. (2005) and Dall' Agnol R et al. (2007)
500 argued that A-type granite can be completely formed under a condition of oxidation. 501 Obvious Ce/Ce* positive anomaliesDraft of zircon and rock indicate that the high Nb-Ta 502 alkaline rhyolite formed under a high-oxygen-fugacity condition. The alkaline
503 rhyolite at the Tuohe Tree Farm formed under conditions of low pressure (< 0.5 Gpa),
504 high temperature (>881℃), and high oxygen fugacity. It is speculated that the magma
505 source of the rhyolite was upper crust, a 'high level magma' formed from the melting
506 of upper crust.
507 Conclusion
508 (1) The weighted average of the zircon 206 Pb / 238 U age is 114.07 ±0.55 Ma,
509 indicating that rhyolites in the Tuohe Tree Farm formed during the end of Mesozoic
510 volcanic eruptions in the Great Xing’an Range, China.
511 (2) The major elements of rocks are rich in alkali and the trace elements are high in
512 Nb-Ta, low in Sr and high in Yb. Thus, the rhyolite in the Tuohe Tree Farm is
513 alkaline rhyolite with 'extremely low Sr, high Yb' and high Nb-Ta.
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514 (3) It is speculated from the petrochemical and Sr and Nd isotopic compositions, that
515 the magmatic source rock is metamorphic crust rock of the Xinghua ferry group in the
516 Xingan block metamorphic basement; the magma formation process was
517 characterized by the physical and chemical conditions of low pressure, high
518 temperature, and high oxygen fugacity.
519 (4) The magma formed following closure of the Mongolia–Okhotsk ocean in an
520 intraplate extensional tectonic environment related to a rift, mantle plume, and hot
521 spot, as the basaltic magma underplating supplied a heat source resulting in partial
522 melting of the metamorphic crustal rock of the Xinghua ferry group in the Xingan 523 block basement. Draft 524 References
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Table1 Rare Earth Element Test Data of Zircon ( × 10 - 6 ) and Its Parameters
Sample I01 I02 I03 I04 I05 I06 I07 I08 I09 I10 I11 I12 I13 I14 I15 I16 I17 I18 I19 I20 I21 I22 I23 I24 I25 I26 I27 I28 I29 La 0.04 0.09 0.04 0.05 0.05 0.05 0.05 0.01 15.18 0.04 0.03 0.02 0.03 7.03 0.00 0.02 0.68 1.54 0.30 0.03 0.06 0.09 8.58 0.43 0.22 0.01 0.03 0.04 0.03 Ce 420 352 205 314 342 420 269 180 320 171 401 375 203 281 308 316 179 289 151 390 412 262 473 263 276 289 253 401 162 Pr 0.43 0.47 0.51 0.42 0.40 0.73 0.78 0.21 5.35 0.21 0.35 0.30 0.38 2.60 0.32 0.31 0.51 0.92 0.32 0.31 0.49 0.30 5.48 0.52 0.73 0.40 0.40 0.42 0.30 Nd 7.69 7.52 8.64 7.38 6.29 7.37 12.22 4.25 27.81 4.03 7.74 6.77 6.24 17.25 6.83 6.25 6.87 11.24 4.35 7.67 9.34 6.08 32.08 8.07 9.30 6.61 6.70 7.98 5.47 Sm 21.39 19.70 18.15 18.36 17.63 20.99 24.42 11.01 25.11 10.91 21.37 19.67 13.51 21.99 16.26 16.42 13.61 21.56 10.38 20.15 22.72 15.19 29.38 17.37 20.87 16.88 16.61 20.53 12.90 Eu 5.44 4.78 4.68 4.66 4.53 5.54 6.06 2.87 5.54 2.79 5.39 4.70 3.59 5.10 4.00 4.30 3.58 5.51 2.87 5.16 5.59 3.89 6.35 4.21 4.87 4.44 4.07 5.05 3.33 Gd 110 102 93 99 92 115 124 60 103 55 105 98 76 101 88 86 72 104 56 101 115 77 120 85 100 89 80 103 65 Tb 39 36 33 35 33 39 44 23 37 21 37 34 28 37 30 32 27 38 22 35 41 30 40 31 37 33 29 37 25 Dy 440 402 382 400 374 427 496 267 417 252 415 382 324 415 347 368 310 437 269 402 460 346 447 367 420 385 340 408 293 Ho 156 142 136 144 133 148 175 100 148 92 145 133 Draft119 149 125 134 114 155 102 140 162 125 155 132 150 141 121 142 107 Er 645 586 574 601 554 587 719 424 618 397 591 542 501 616 513 561 477 638 435 566 664 524 620 554 611 578 507 578 457 Tm 124 112 111 116 107 110 137 84 119 80 112 102 98 120 100 109 94 124 86 107 127 103 116 107 118 111 99 108 89 Yb 1075 980 973 1019 931 943 1188 747 1042 703 956 884 854 1040 863 966 819 1072 763 921 1094 896 994 942 1018 981 867 921 805 Lu 185 168 169 175 160 161 203 131 181 123 162 150 150 181 147 168 142 187 135 157 186 157 169 165 177 171 150 156 138 Y 4596 4226 4095 4292 3959 4341 5020 2957 4372 2770 4295 3979 3532 4378 3733 3980 3326 4631 2980 4153 4892 3693 4595 3906 4422 4141 3649 4233 3218 ΣREE 3230 2911 2708 2934 2755 2985 3399 2033 3063 1912 2958 2731 2376 2993 2548 2768 2259 3084 2038 2852 3299 2545 3216 2677 2942 2807 2473 2888 2164 LREE 455 384 237 345 371 455 312 198 399 189 436 406 227 335 336 343 205 330 170 423 450 288 555 294 312 317 281 435 184 HREE 2774 2527 2470 2589 2384 2530 3087 1835 2664 1723 2522 2324 2149 2658 2212 2425 2054 2755 1869 2428 2849 2257 2661 2384 2630 2490 2192 2453 1979 LREE/ 0.16 0.15 0.10 0.13 0.16 0.18 0.10 0.11 0.15 0.11 0.17 0.17 0.11 0.13 0.15 0.14 0.10 0.12 0.09 0.17 0.16 0.13 0.21 0.12 0.12 0.13 0.13 0.18 0.09 HREE δEu 0.28 0.26 0.28 0.27 0.28 0.27 0.27 0.27 0.29 0.28 0.28 0.27 0.27 0.28 0.26 0.28 0.28 0.29 0.29 0.29 0.27 0.28 0.28 0.28 0.27 0.28 0.28 0.27 0.29 δCe 296 216 121 220 254 175 105 259 9 230 342 375 161 16 300 315 72 58 108 384 250 242 16 118 105 221 189 285 165
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Table 2 Zircon U–Pb analytical data for rich Nb-Ta rhyolite.
Pb Th U 207Pb/206Pb 207Pb/235U 206Pb/238U 207Pb/206Pb 207Pb/235U 206Pb/238U
Isotope Isotope Isotope Age Age Age
Point (×10-6) Th/U Ratio 1σ Ratio 1σ Ratio 1σ (Ma) 1σ (Ma) 1σ (Ma) 1σ
I-1 20 1221 707 1.73 0.048340.001840.11951 0.0049 0.017930.00048 116 50 115 4 115 3
I-2 17 1084 609 1.78 0.048290.001970.116760.005090.017530.00047 114 55 112 5 112 3
I-3 8 389 313 1.24 0.048320.002270.118970.005840.017850.00049 115 65 114 5 114 3
I-4 14 799 512 1.56 0.04838 0.0022 0.119850.005750.017960.00049 118 63 115 5 115 3
I-5 16 923 591 1.56 0.048330.002260.117740.005770.017670.00049 115 64 113 5 113 3
I-6 23 1594 759 2.10 0.04835 0.0021 0.11979 0.0055 0.017970.00049 116 59 115 5 115 3
I-7 11 564 396 1.42 0.048410.002370.120690.006170.018080.00049 119 69 116 6 116 3
I-8 8 344 307 1.12 0.048220.002520.120720.006540.01815 0.0005 110 74 116 6 116 3
I-9 11 515 403 1.28 0.048070.004480.118290.011010.017850.00056 103 148 114 10 114 4
I-10 8 315 300 1.05 0.048530.005770.119110.01419 0.0178 0.00054 125 210 114 13 114 3
I-11 21 1531 769 1.99 0.048360.002580.118330.006510.01774 0.0005 117 75 114 6 113 3
I-12 22 1563 753 2.08 0.04825 0.0016 0.115660.004240.017380.00046 112 42 111 4 111 3
I-13 8 382 322 1.19 0.048270.002560.119090.006530.01789 0.0005 113 75 114 6 114 3
I-14 10 508 389 1.30 0.048330.003720.120440.009390.018070.00051 115 122 115 9 115 3 I-15 17 1047 576 1.82 0.0483 0.00269Draft0.117960.006730.01771 0.0005 114 79 113 6 113 3 I-16 13 638 488 1.31 0.048360.002690.119350.00686 0.0179 0.00049 117 81 114 6 114 3
I-17 8 381 301 1.26 0.048150.003250.116970.008070.017620.00049 107 103 112 7 113 3
I-18 12 689 448 1.54 0.048220.002180.118380.00561 0.0178 0.00049 110 61 114 5 114 3
I-19 7 286 271 1.06 0.048220.003380.11928 0.0085 0.017940.00051 110 107 114 8 115 3
I-20 24 1667 812 2.05 0.048280.002030.119180.00534 0.0179 0.00048 113 57 114 5 114 3
I-21 20 1263 717 1.76 0.04829 0.0022 0.120610.005780.018110.00049 114 63 116 5 116 3
I-22 11 522 414 1.26 0.04815 0.002 0.12024 0.0053 0.018110.00049 107 55 115 5 116 3
I-23 26 1869 861 2.17 0.048280.001870.117830.00491 0.0177 0.00048 113 51 113 4 113 3
I-24 10 426 377 1.13 0.048370.003630.118590.009010.017780.00051 117 117 114 8 114 3
I-25 11 551 440 1.25 0.048070.003670.118020.009130.017810.00051 103 119 113 8 114 3
I-26 11 555 444 1.25 0.04832 0.0025 0.118210.006340.017740.00049 115 73 113 6 113 3
I-27 11 568 417 1.36 0.048370.002830.119260.007160.017880.00051 117 85 114 6 114 3
I-28 24 1653 791 2.09 0.048380.002080.118630.005410.017780.00049 118 58 114 5 114 3
I-29 7 316 272 1.16 0.0483 0.003260.118830.008150.017840.00051 114 101 114 7 114 3
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Table3 Contents of major elements(wt%) and trace elements(ppm) of rich Nb-Ta rhyolite
Sample I-1 I-2 I-3 I-4 I-5 I-6 I-7 Ave
SiO2 72.66 72.37 73.22 73.00 72.82 72.35 72.63 72.72
Al2O3 13.23 13.25 13.18 13.38 13.18 13.42 13.60 13.32
Fe2O3 1.70 1.66 1.37 1.49 1.67 1.62 1.86 1.62 FeO 0.09 0.09 0.37 0.19 0.14 0.14 0.68 0.24 CaO 0.17 0.17 0.17 0.16 0.18 0.18 0.12 0.16 MgO 0.07 0.06 0.08 0.04 0.07 0.06 0.06 0.06
K2O 7.80 7.78 5.51 5.61 6.97 7.43 4.81 6.56
Na2O 3.61 3.65 5.34 5.16 3.99 3.91 4.58 4.32
TiO2 0.18 0.17 0.18 0.18 0.17 0.17 0.19 0.18
P2O5 0.01 0.01 0.02 0.03 0.02 0.01 0.02 0.02 MnO 0.04 0.04 0.12 0.06 0.02 0.01 0.09 0.05 LOI 0.40 0.41 0.26 0.35 0.44 0.37 0.68 0.42 Total 99.97 99.67 99.82 99.64 99.65 99.68 99.32 99.68 TFeO 1.62 1.58 1.60 1.53 1.64 1.60 2.35 1.70 TFeO/(TFeO+MgO) 0.96 0.96 0.95 0.97 0.96 0.96 0.98 0.96 A/NK 0.92 0.92 0.89 0.92 0.93 0.93 1.07 0.94 A/CNK 0.90 0.90 0.88 0.90 0.91 0.91 1.05 0.92 La 21.16 23.33 21.19 19.51 15.27 26.8 24.38 21.66 Ce 44.89 50.46 52.94 45.64 32.59 56.76 82.66 52.28 Pr 4.69 5.06 4.10 4.64 3.53 4.95 4.65 4.52 Nd 15.26 16.43 12.48 15.26 12.24 16.02 16.38 14.87 Sm 3.38 3.58 2.34 3.38 3.08 3.11 4.14 3.29 Eu 0.51 0.50 0.32 0.46 0.41 0.4 0.58 0.45 Gd 3.58 3.67 2.18 3.61 3.41 3.63 4.87 3.56 Tb 0.83 0.84 Draft0.50 0.81 0.77 0.91 1.19 0.84 Dy 5.34 5.67 3.19 5.63 5.31 6.64 8.47 5.75 Ho 1.36 1.39 0.86 1.39 1.29 1.44 1.74 1.35 Er 3.98 4.05 2.51 4.12 3.73 4.48 5.19 4.01 Tm 0.64 0.66 0.45 0.65 0.59 0.75 0.85 0.66 Yb 4.27 4.50 3.35 4.65 4.04 5.12 5.78 4.53 Lu 0.69 0.68 0.56 0.71 0.62 0.74 0.84 0.69 ΣREE 110.57 120.81 106.96 110.46 86.87 131.75 161.72 118.45 LREE/HREE 4.35 4.63 6.87 4.12 3.40 4.56 4.59 4.65 LaN/YbN 3.56 3.72 4.54 3.01 2.71 3.76 3.03 3.47 δEu 0.44 0.42 0.43 0.40 0.39 0.36 0.39 0.40 δCe 1.06 1.09 1.31 1.14 1.05 1.21 1.9 1.25 Y 23.08 25.01 12.62 23.13 24.71 46.79 33.85 27.03 Be 3.16 3.19 7.59 7.34 4.28 3.96 7.05 5.22 Sc 2.50 2.56 2.77 2.84 2.68 2.04 2.24 2.52 V 0.24 0.21 0.08 0.08 0.16 5.03 1.56 1.05 Cr 0.29 0.41 0.07 0.34 0.16 5.29 5.7 1.75 Co 0.24 0.24 0.18 0.20 0.21 2.52 2.28 0.84 Ni 0.23 0.77 0.03 0.39 0.01 3.12 2.82 1.05 Cu 0.78 1.81 1.31 0.81 0.94 3.23 5.8 2.10 Zn 68.23 72.69 106.90 75.24 82.66 69.3 127 86.00 Ga 23.16 24.32 24.51 24.80 24.43 24.4 25.3 24.42 Rb 320.60 325.90 237.60 237.10 298.30 247 238 272.07 Sr 4.80 2.41 4.45 3.35 4.27 1.86 8.8 4.28 Ba 10.54 10.53 6.99 12.32 8.50 35.3 26.6 15.83 Nb 98.74 98.13 99.57 99.51 93.47 85.7 92.3 95.35 Ta 13.72 12.34 12.19 11.77 10.97 5.75 6.38 10.45 Zr 482.50 454.40 494.70 543.70 447.90 543 643 515.60 Hf 15.70 14.57 16.29 17.19 15.52 19.6 20.6 17.07 Th 18.90 20.96 20.00 21.17 16.21 15 21.6 19.12 U 3.87 3.91 3.80 4.05 3.18 3.28 2.78 3.55 Pb 17.25 17.74 26.19 38.73 21.48 28 50.2 28.51
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Table4 Sr-Nd isotopic results of rich Nb-Ta rhyolite.
87 86 87 86 147 144 143 /144 87 86 143 144 Rb/ Sr Sr/ Sr Sm/ Nd Nd Nd t/Ma εSr(0) εSr(t) fRb/Sr ( Sr/ Sr)ⅰ εNd(0) εNd(t) fSm/Nd TDM T2DM ( Nd/ Nd)
I -1 199.72 1.049779 0.1402 0.1401963 114 4901.05 310.16 2413.98 0.72621 0.61 1.4 -0.29 1005 799 0.512562ⅰ I -3 200.21 1.048341 0.1187 0.118676 114 4880.64 278.36 2413.96 0.72397 0.8 1.9 -0.40 758.0 754. 0.512590
I -4 211.58 1.047149 0.1402 0.140238 114 4863.72 -0.01 2557.41 0.70437 0.6 1.4 -0.29 1005 7990 0.512562 I -5 208.95 1.052516 0.1591 0.159132 114 4939.90 136.78 2525.56 0.71400 0.76 1.2 -0.19 1339 813 0.512553
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1 2 Fig.1 SimplifiedDraft geological map and Sampling position 3 4
5 6 Fig.2 Hand specimen photograph (a) 、photomicrograph of rich Nb-Ta rhyolite(b)、pyrochlore(c) and 7 titanomagnetite(d)
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8 9 Fig.3. CL images of zircons from rich Nb-Ta rhyolite 10 11 Draft
12 13 Fig.4 Zircon Chondrite-normalized REE distribution patterns (a) and LA–ICP-MS zircon U–Pb concordia 14 diagrams(b) of rich Nb-Ta rhyolite 15 16
17 18
19 Fig.5 Plots of SiO2 versus (SiO2 +K2O)(a)、Plots of A/CNK versus A/NK (b) and Plots of SiO2 versus K2O(c) for 20 rich Nb-Ta rhyolite
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21 22 Fig.6 Chondrite-normalized REE patterns (a) primitive mantle-normalized spidergram(b) of rich Nb-Ta 23 rhyolite 24 25
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26 27 Fig.7 Diagrams for discriminating tectonic setting of R1-R2(a)、Yb-Ta(b) and Hf-Rb/30-Ta×3(c) for rich Nb-Ta 28 rhyolite 29 30
31 32 Fig.8 Diagrams for genetic types(a、b、c、d) and Diagrams for discriminating tectonic setting(e、f) of rich Nb-Ta 33 rhyolite
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-6 36 Fig.9 Diagrams for La×10 versus La/Sm(a) and SiO2-(TFeO+MgO+TiO2) versus (TFeO+MgO+TiO2)(b) of rich 37 Nb-Ta rhyolite 38 39
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40 41 Fig.10 Diagrams for rare earth elements (a) and trace elements (b).
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