Journal Pre-proofs Zircons from the Tarim basement provide insights into its positions in Columbia and Rodinia supercontinents Peng Wang, Guochun Zhao, Qian Liu, Yigui Han, Jinlong Yao, Jianhua Li PII: DOI: Reference:
S0301-9268(19)30237-2 https://doi.org/10.1016/j.precamres.2020.105621 PRECAM 105621
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Precambrian Research
Received Date: Revised Date: Accepted Date:
18 April 2019 4 December 2019 8 January 2020
Please cite this article as: P. Wang, G. Zhao, Q. Liu, Y. Han, J. Yao, J. Li, Zircons from the Tarim basement provide insights into its positions in Columbia and Rodinia supercontinents, Precambrian Research (2020), doi: https:// doi.org/10.1016/j.precamres.2020.105621
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1
Zircons from the Tarim basement provide insights into its
2
positions in Columbia and Rodinia supercontinents
3 4
Peng Wang1, Guochun Zhao1, 2*, Qian Liu1, Yigui Han2, Jinlong Yao1, 2, Jianhua Li4
5 6
1
7
2 State
8
Department of Earth Sciences, The University of Hong Kong, Pokfulam Road, Hong Kong, China Key Laboratory of Continental Dynamics, Department of Geology, Northwest University, Northern Taibei
Street 229, Xi’an 710069, China
9
3
School of Earth Sciences and Engineering, Nanjing University, Nanjing 210093, China
10
4
Institute of Geomechanics, Chinese Academy of Geological Sciences, Beijing 100081, China
11 12
ABSTRACT
13
The positions of the Tarim Craton in two Precambrian supercontinents Columbia and
14
Rodinia still remains unknown or controversial due to the lack of geological and
15
paleomagnetic data as the craton is largely covered by desert in the central part and
16
sparse Precambrian basement rocks are scattered at its margins. In this contribution, we
17
attempt to use new in situ zircon U-Pb ages and Hf isotopic data, combined with
18
comprehensive compiled data from Precambrian basement rocks at its margins, to
19
provide new insights into positions in two pre-Pangean supercontinents. Available data
20
indicate that the northern margin of Tarim most likely developed as an active margin at
21
2.5-2.7 Ga, which collided with the southern margin of Siberia at 1.8-2.0 Ga, and then
22
drifted away at 0.9-1.5 Ga, without any record for Grenvillian events in the northern
23
margin of Tarim, which was an active margin in the Neoproterozoic (600-800 Ma). In
24
southern Tarim, Neoproterozoic magmatic rocks were closely related with the
25
evolution of Rodinia. The ~0.9 Ga Ma gneissic granites were formed in collisional
26
settings due to collision between the Southern Tarim and North India during the
27
assembly of Rodinia, which is supported by comparable zircon age spectra and Hf
28
isotopes from Neoproterozoic strata in two terrenes. The ~800 Ma granitic intrusions
29
and mafic dikes were generated in continental rifting settings associated with the
30
breakup of Rodinia. This model considers the Tarim Craton remaining as a single block
31
in the period from Columbia to Rodinia.
32
Keywords: Igneous rock, Detrital zircon, Columbia; Rodinia; Tarim Craton
33 34
1. Introduction
35 36
Positioning blocks in Precambrian supercontinents like Columbia and Rodinia is much
37
difficult due to limited Precambrian strata and reliable paleomagnetic data (Evans and
38
Mitchell 2011; Li et al., 2008; Zhao et al., 2004, 2018). This is particularly the case
39
with the Tarim Craton of China, and its positions in the two pre-Pangean
40
supercontinents remain unknown or controversial. The Tarim Craton is largely
41
occupied by desert in its central part, and only few Precambrian basements and
42
Paleozoic to Mesozoic strata sporadically outcrop along its margins. In addition to
43
limited Precambrian rocks, magmatic rocks in northern Tarim and southern Tarim have
44
similar ages but markedly different tectonic settings, and detrital zircons from
45
equivalent strata also show distinct age spectra. These discrepancies have also
46
significantly hindered us from relocating its positions in supercontinents (Xu et al.,
47
2013). Some models proposed that the Tarim Craton is composed of discrete terranes
48
and experienced complicated assembly and breakup (Wen, et al., 2017; Xu, et al., 2013;
49
Zhang, et al., 2019). Alternatively, other models considered the Tarim Craton as one
50
unified block in the pre-Pangean supercontinents (Li et al., 1996; Huang et al., 2005).
51
To date, a few studies have located the positions of the Tarim Craton in the Columbia
52
and Rodinia supercontinents, popularly quoting or agreeing with the view that the
53
northern Tarim Craton was connected to the Kimberley Block in NW Australia during
54
Paleoproterozoic to Early Cambrian time, as it was thought that two blocks have similar
55
Paleoproterozoic
56
Neoproterozoic sedimentary successions (Li et al., 1996; Turn, S.A., 2010; Zhao et al.,
57
2004). However, newest available geochronological dating has shown that no
58
Mesoproterozoic strata were developed in northern Tarim, except for only two small
59
Mesoproterozoic diabase exposed in this area (Table S1). Moreover, comprehensive
60
compiled data have revealed that Neoproterozoic strata in northern Tarim almost
61
certainly lack 1.1-1.7 Ga detrital zircons, remarkably distinct from those of strata in
62
NW Australia characterized by Grenville-age zircons (Cawood et a., 2015; He et al.,
63
2014). To locate the Tarim Craton in the the Columbia and Rodinia supercontinents, it
64
is fundamentally important to decrypt discrepancies in magmatic activities and age
65
spectra of detrital zircons between the northern Tarim and southern Tarim. In this
66
contribution, we decipher and compare tectonic settings of magmatic activities and
67
trace provenance of Proterozoic strata based on comprehensive zircon U-Pb ages and
68
Hf isotopic data. We infer that the Tarim Craton was possibly an integrated block at
69
least during Proterozoic time. While the northern Tarim Craton might have been
70
assembled on the southern Siberia within Columbia, the southern Tarim Craton was
71
connected with the northern Indian within Rodinia.
basement
rocks
and
weakly-metamorphosed
Meso-
to
72 73
2. Settings of the Tarim Craton
74 75
The Tarim Craton is bounded by the Tianshan Mountain to the north, the Kunlun
76
Mountain to the south and the Altyn Tagh mountain to the southeast (Fig. 1a). The
77
craton is largely occupied by desert in its central part, and only few Precambrian
78
basement rocks and Paleozoic to Mesozoic strata sporadically outcrop along its margins.
79
The basement rocks are mostly exposed along its margins and also identified in drill
80
cores in the central part (Xu et al., 2013). Until now, Archean rocks are predominantly
81
exposed in the Dunhuang area and the Altyn Tagh Mountain (Fig. 1a), and the oldest
82
rocks are ca. 3.7 Ga tonalitic gneisses (Ge et al., 2018). In northern Tarim, other well-
83
documented Precambrian rocks are mainly distributed in the Kuluketage and Aksu
84
areas (Fig. 1), and the oldest rocks are subduction-related ca. 2.7 Ga Korla complex in
85
the Kuluketage area (Ge et al., 2014). Igneous rocks are characterized by mafic-felsic
86
suites with ages from 2.7 Ga to 0.7 Ga in the Kuluketage area, and some Neoproterozoic
87
mafic to felsic rocks were identified in the Aksu area (Wu et al., 2018). In southern
88
Tarim, the oldest rocks are represented by ca. 2.4 Ga Heluositan complex (Ye et al.,
89
2016). Notably, the exposed Archean rocks along the margins of Tarim have distinct
90
two-stage Hf model ages (TDMC), which led some researchers to regard the Tarim
91
Craton as discrete terranes that amalgamated during Neoproterozoic time (Ye et al.,
92
2016). This inference has also been used to interpret time-equivalent magmatism and
93
strata formed in distinct settings along northern and southern margins (Xu et al., 2013;
94
Zhang et al., 2019). In the Kukuketage area, Neoproterozoic and Paleoproterozoic strata
95
are exposed, with the former consisting of glacial deposits, volcanic rocks, and marine
96
sediments, and the latter composed of sedimentary clastic and carbonate rocks (Long
97
et al., 2011). Localized Neoproterozoic blueschist-dominated strata are distributed in
98
the Aksu area. In southern Tarim, Precambrian igneous rocks are dominated by felsic
99
rocks and well-constrained Precambrian metasediments are Neoproterozoic schist-
100
dominated strata deposited in continental extensional settings (Wang et al., 2011) (Fig.
101
1a).
102 103
3. Methods
104 105
Cathodoluminescence images for the zircons were obtained with a MonoCL3 (Gatan,
106
Abingdon, UK) cathodoluminescence instrument attached to a scanning electron
107
microscope (JSM-6510A, JEOL, Tokyo) at Jinyu Technology, Chongqing, China.
108
Zircons were separated using heavy-liquid and magnetic techniques at Laboratory of
109
Geological Team of Heibei Province, China. All analytical jobs were conducted at
110
Nanjing FocuMS Technology Co. Ltd, China. Analytical procedures were summarized
111
in the following text.
112
Most of zircons analyzed have clear oscillatory zonings, using a Photon Machines
113
excimer 193-nm LA-ICPMS. A laser repetition rate of 7 Hz, energy of 6.71 J/cm2 were
114
used. Zircon 91500 and GJ-1 were used for U-Pb isotopic ratio correction (Jackson et
115
al., 2004). The raw data were processed offline with ICPMSDataCal. Concordia
116
diagrams and weighted mean calculations were made using Isoplot (version 3.0).
117
Zircons Hf isotope compositions were made on the same age domains previously
118
analyzed for U-Pb dating. And only zircons with good Concordia ages were analyzed.
119
Australian Scientific Instruments RESOlution LR laser-ablation system (Canberra,
120
Australian) and Nu Instruments Nu Plasma II MC-ICP-MS (Wrexham, Wales, UK)
121
were combined for the experiments. The 193 nm ArF excimer laser, homogenized by a
122
set of beam delivery systems, was focused on zircon surface with fluence of 3.5J/cm2.
123
Ablation protocol employed a spot diameter of 50 um at 8 Hz repetition rate for 40
124
seconds (equating to 320 pulses). Helium was applied as carrier gas to efficiently
125
transport aerosol to MC-ICP-MS. Standard zircons (including GJ-1, 91500, Plešovice,
126
Mud Tank, Penglai) were treated as quality control every five unknown samples.
127 128
4. Results
129 130
Five Neoproterozoic schists in the southern Hetian area and two Mesoproterozoic
131
quartzites in the southern Yutian area were collected for zircon U-Pb dating (Fig. 1a
132
and b). A total of 422 detrital zircon ages were obtained and 172 of them were chosen
133
for Lu-Hf isotopic analyses. Representative cathodoluminescence images of zircons
134
and corresponding
135
values are shown in Fig. 2. These prismatic zircons display narrow oscillatory zones
136
and high Th/U ratios (most > 0.2) and U/Yb ratios (most > 0.1), indicating a continental
137
magmatic origin (Grimes et al., 2007) (Fig. 3).
207Pb/206Pb
ages (>1.0 Ga),
206Pb/238U
ages (< 1.0 Ga) and εHf(t)
138
Zircons from five Neoproterozoic schists yielded similar U-Pb age patterns: one
139
prominent age population at 800 Ma and a small amount of other ages (Fig. 4). Five
140
samples restricted the maximum depositional age at 760-800 Ma (Fig. 4). Ninety-four
141
zircons from Mesoproterozoic quartzite 17WP55 defined a dominant age population at
142
1350 Ma and two subordinate peaks at 1250 Ma and 1600 Ma, with a maximum
143
depositional age at 998 Ma (Fig. 5). Ninety-nine zircons from Mesoproterozoic
144
quartzite 17WP47 yielded one prominent age population at 1500 Ma, one subordinate
145
age population at 1220 Ma and a maximum depositional age at 1023 Ma (Fig.5). A total
146
of 122 Lu-Hf isotopic analysis of zircons from five Neoproterozoic schists yielded εHf(t)
147
values ranging from -17 to 11. Ca. 800 Ma zircons are characterized by εHf(t) values
148
ranging from -15 to -5. In contrast, 55 zircons from two Mesoproterozoic quartzites
149
show mostly positive εHf(t) values (0 to 10).
150
151
5. Discussion
152 153
4.1 Igneous rocks
154
In northern Tarim, igneous rocks record the evolution of the Columbia supercontinent
155
from amalgamation to breakup (Fig. 6). The well-documented ~2.7 Ga rocks consist
156
mainly of orthogneiss (probably meta-volcanics) and amphibolite (meta-mafic rocks),
157
which are enriched in light rare elements (LREE) and Th, and depleted in Nb-Ta and
158
Ti, indicative of arc-related settings (Fig. 7) (Ge et al., 2014). In addition, these rocks
159
have heterogeneous zircon εHf(t) values ranging from -5 to10, suggesting materials from
160
both depleted mantle and ancient continental crust (Fig. 8) . Thus, it is inferred that the
161
~2.7 Ga rocks were formed in continental arc settings (Ge et al., 2014). Similarly, the
162
~2.5 Ga rocks include (meta-) gabbro, diorite, and granodiorite, in which the
163
granodiorites have significantly negative Nb-Ta-Ti anomalies, strongly fractionated
164
REE patterns, and mostly negative zircon εHf(t) values, defining typical continental arc
165
settings (Fig. 6) (Long et al., 2011). The 1.8-2.0 Ga intermediate-acidic meta-igneous
166
rocks were sourced from crust-dominated sources in collisional settings, as supported
167
by strongly negative εHf(t) values approaching -20 and strong depletions in Nb-P-Ti and
168
significant negative Eu anomalies (Wang, XD et al., 2018) (Fig. 8a). These collision-
169
related 1.8-2.0 Ga magmatism and the ~1.8 Ga regional high-grade metamorphism are
170
genetically related to the assembly of Columbia. The ~1.5 Ga meta-diabases show
171
geochemical features akin to within-plate basalts, such as no or slight Nb-Ta negative
172
anomalies, positive Eu anomalies, and enrichments in Zr and Ti elements (Wu et al.,
173
2014; Zhang J et al., 2018). These rocks have relatively homogenous zircon εHf(t)
174
values ranging from -4 to 2 (Fig. 8a), which were considered as derivation from
175
enriched continental lithospheric mantle within rifting settings corresponding to the
176
initial breakup of Columbia (Fig. 6) (Wu et al., 2014). In contrast to these
177
aforementioned consensus views about the tectonic settings of Meso-Paleoproterozoic
178
rocks, the tectonic settings of the Neoproterozoic igneous rocks (600-800Ma) have been
179
hotly disputed, with different authors proposing different settings from long-lasting
180
subduction to the breakup of Rodinia or mantle plume (Long, et al., 2011).
181
In southern Tarim, Neoproterozoic magmatic rocks are closely related with the
182
evolution of Rodinia (Fig. 6). The ~2.4 Ga granitic gneisses have negative zircon εHf(t)
183
values and are products of recycled Archean crust due to upwelling of hotter mantle in
184
extensional continental environments (Fig. 8a) (Ye et al., 2016). Unlike northern Tarim,
185
no collision-related rocks associated with the assemblage of Columbia have been
186
identified in southern Tarim, and instead minor 1.8-2.0 Ga A-type granites defined
187
intraplate settings based on geochemical data (Zhang et al., 2019). The ~1.4 Ga A-type
188
gneissic granites, with zircon εHf(t) values clustering around 0, are products of partial
189
melting of mafic lower crust and juvenile crust in extensional anorogenic settings
190
related to the breakup of the Columbia supercontinent (Ye et al., 2016). The ~0.9 Ga
191
gneissic granites, with variable zircon εHf(t) values ranging from -28 to 12, but an
192
average of 0, were originated from mixing sources and formed in collisional/ post-
193
collisional settings corresponding to the assembly of Rodinia (Wang et al., 2013). The
194
mafic dikes (~800 Ma), with εHf(t) negative zircon values ranging from -10 to -2, were
195
sourced from mafic lower crust in continental rifting settings, recording the initial
196
breakup of Rodinia (Zhang et al., 2018) (Fig. 6).
197
Although the northern and southern margins of Tarim record intense magmatism
198
during early Neoproterozoic time, two regimes show distinct rock assemblages with
199
different zircon εHf(t) values and geochemical characters, indicative of subduction and
200
continental rifting settings, respectively (Fig.6 and 8). In northern Tarim, the ca. 800
201
Ma intermediate-acidic rocks are enriched in LREEs and large-ion lithophile elements,
202
and depleted in Nb-Ta-Ti, and have negative zircon εHf(t) values (-30 to -10) (Fig. 7,
203
8a) (Ge et al., 2014). Similarly, the younger ca. 640 Ma rocks include granodiorites,
204
mafic dikes, rhyolites, and basalts, in which the felsic units show geochemical
205
similarities, such as depletions in Nb-Ta-Ti, but have relatively higher zircon εHf(t)
206
values (-10 to -2) (Ge et al., 2014). Their geochemical compositions of both ca. 800 and
207
ca. 640 magmatic rocks define arc settings, as also evidenced by the ca. 700 Ma
208
blueschists and ca. 640 glacial diamictites in the Aksu area in northern Tarim (Fig. 6)
209
(Nakajima et al., 1990). In particular, advancing and retreating subduction settings can
210
be inferred for the ca. 800 Ma and ca. 640 Ma magmatism, as indicated by switch of
211
zircon Hf isotopic compositions (Fig. 2a) (Collins et al., 2011). The later has increasing
212
zircon εHf(t) values indicating more contribution of mantle-derived juvenile materials
213
due to crustal extensional of overriding plate, which is typical of accretionary process
214
(Han et al., 2016). Comparatively, in southern Tarim, the ca. 800 Ma granites exhibit
215
strong intraplate affinities closely related to continental rifting settings, which are
216
consistent with the worldwide breakup of Rodinia (Zhang et al., 2018).
217
4.2 Proterozoic strata
218
New and compiled zircon U-Pb and Hf isotopic data characterize Proterozoic strata
219
along the northern and southern margins of the Tarim Craton. The complied data
220
mainly include Neo- and Paleoproterozoic strata exposed in the Kuluketage and the
221
Aksu areas in northern Tarim, and Neo- and Mesoproterozoic strata distributed in
222
southwestern Tarim. Data from southern Tarim show a continuous spectrum of ages
223
from ca. 3000 to ca. 600 Ma, with a dominant peak at ~800 Ma, and minor several
224
peaks at ~1200 Ma, ~1300 Ma, and ~1850 Ma (Fig. 9a). Comparatively, data from
225
northern Tarim are characterized by two dominant peaks at ~800 Ma and ~1900 Ma,
226
respectively (Fig. 9b). The ~800 Ma detrital zircons have various εHf(t) values (-20 to
227
10), clustering at -10, and the ~740 Ma zircons have more concentrated εHf(t) values
228
from -5 to 5 (Fig. 8). These values match well with those of zircons from time-
229
equivalent igneous rocks that are closely linked with advancing subduction and
230
retreating subduction settings, respectively (Fig. 8). It is worth noting that almost no
231
1.1-1.7 Ga detrital zircons identified in the Proterozoic strata (Fig. 8), together with
232
no traces of Grenville-age event recognized in northern Tarim, are similar to that of
233
the southern Siberia Craton (Fig. 9c) (Gladkochub et al., 2019). Given that the
234
northern Tarim was involved in collisional events associated with the assembly of
235
Columbia, it is inferred that the northern Tarim was probably linked to the southern
236
Siberia within Columbia, and that both were on the periphery of Rodinia or not
237
involved in Rodinia (Fig. 10a, b). This inference is also supported by their similar
238
age populations of Neoproterozoic strata in northern Tarim and southern Siberia (Fig.
239
9). The departure time of the northern Tarim from Siberia occurred during 0.9-1.5
240
Ga, constrained by the existence of ca. 0.9 Ma oceanic crust and ca.1.5 Ga diabase
241
sills/ dikes in northern Tarim, and ca. 1.5 Ga diabase dikes in southern Siberia (Ernst,
242
et al., 2000; Qu et al., 2011; Zhang J et al., 2018), but more work is needed to
243
constrain the accurate timing of detachment.
244
Unique to the Mesoproterozoic quartzites strata in southern Tarim are abundant 1.0
245
-1.7 Ga detrital zircons with mostly positive εHf(t) values (Fig. 8b). The
246
Mesoproterozoic quartzites, with a maximum depositional age of ~1.0 Ga, were
247
deposited in collisional settings associated with the assembly of Rodinia (Fig. 6). In
248
contrast, the ca. 800 Ma detrital zircons have mostly negative εHf(t) values (mostly -5
249
to -15), indicating crust-dominated magmatic sources in continental extensional
250
settings (Fig. 6) (Wang et al., 2011). Specifically, the continental extensional settings
251
possibly corresponded to the breakup of Rodinia during early Neoproterozoic time,
252
posterior to ca. 940 Ma collision-related granitic rocks in southern Tarim related to
253
the assembly of Rodinia (Zhao et al., 2018). In other worlds, the southern Tarim
254
might have collided with a terrane in Rodinia at ~940 Ma and subsequently begun to
255
drift away at ca. 800 Ma (Fig. 10c). The possible terrane is North India, as indicated
256
by similar age spectra of detrital zircons and well comparable Hf isotopic
257
compositions (Fig. 6b, 10) (Wang W et al., 2018). In addition, the detrital zircon age
258
distribution of the Neoproterozoic strata in southern Tarim is similar to that of Neo-
259
Mesoproterozoic strata in South China, implying adjacent positions in Rodinia
260
(Cawood et al., 2015). However, the age spectrum of the southern Tarim is different
261
from that of western Australia which has a prominent age population of ca. 1.2 Ga,
262
precluding that they had a common provenance within Rodinia (Fig. 8) (Li et al.,
263
1996).
264
Our new model considers the Tarim Carton as an integrated block and first links the
265
northern Tarim Craton with southern Siberia within Columbia and the southern Tarim
266
Craton with North India within Rodinia. Our result also provides new insights into
267
interpretation in the different igneous activities and provenance of strata in northern
268
and southern Tarim.
269 270 271
6. Conclusions
272
The northern Tarim possibly collided with the southern Siberia at 1.8-2.0 Ga within
273
Columbia, and drifted away at 0.9-1.5 Ga. No Grenvillian events have been found in
274
northern Tarim in the Neoproterozoic. The southern Tarim possibly collided with North
275
India during the assembly of Rodinia and drifted away at 800 Ma. This model considers
276
the Tarim Craton remaining as a single block in the period from Columbia to Rodinia.
277 278
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Acknowledgements
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This work was funded by the National Science Foundation of China (41730213 and
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41190075). We thank all members from the Nanjing FocuMS Technology Co. Ltd for
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the assistance in experimental analyses.
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Figure caption
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Fig. 1 a: Simplified map showing the Precambrian strata in the Tarim Craton. Insert
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map showing the Tarim Craton and adjacent Cratons. b: Geological map of the southern
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Hetian showing dating samples; c: Geological map of the southern Yutian showing
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dating samples.
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Fig. 2 Representative cathodoluminescence images of zircons and corresponding
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207Pb/206Pb
ages (>1.0 Ga), 206Pb/238U ages (< 1.0 Ga) and εHf(t) values.
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Fig. 3 a: Th vs. U; b: U/Yb vs. Y for zircons analyzed in this study (Grimes et al., 2007).
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Fig. 4 Detrital zircons U-Pb concordia diagrams, maximum depositional ages,
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histograms and normalized probability curves for Neoproterozoic schists in south
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Hetian.
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Fig. 5 Detrital zircons U-Pb concordia diagrams, maximus depositional ages
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histograms and normalized probability curves for detrital zircon ages for
431
Mesoproterozoic quartzite in south Yutian.
432 433
Fig. 6 Ages of rocks, rock assemblages, and corresponding tectonic settings for rocks
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from the northern Tarim and southern Tarim (data sources are in Supplementary
435
Information). Orthogneisses and amphibolite refer to rocks whose protolith are not
436
certain or complicated. The passive continental margin in southern Tarim at 1.1 Ga is
437
inferred from the age of assembly of Rodinia (1.1-0.9 Ga, Zhao et al., 2018), lack of
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arc-related Mesoproterozoic rocks, and ~1.0 Ga depositional age of the
439
Mesoproterozoic quartzite formed in collisional settings in this study.
440 441 442
Fig. 7 a and b: Tectonic discrimination diagrams for granitic samples from the Tarim
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Craton (after Pearce et 1984); c and d: A-type granite discrimination diagrams (after
444
Whalen et al., 1987); e and f: Average chondrite-normalized rare elements and
445
primitive-mantle-normalized trace elements diagrams (normalizing values are from
446
Sun and McDonough (1989)). In figure e, n indicates the number of values. (data
447
sources are in Supplementary Information)
448
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Fig. 8 Zircon Hf isotope compositions for igneous rocks and strata in the northern Tarim,
450
southern Tarim, and North India (data sources in Supplementary Information). Detrital
451
zircons from Neoproterozoic strata in North India and those from Neo-Mesoproterozoic
452
strata in southern Tarim show broadly similar zircon εHf(t) values. n-number of single-
453
grain zircon εHf(t) values.
454 455
Fig. 9 Histograms and normalized probability curves for detrital zircon ages for rocks
456
from North Tarim, South Tarim, South Siberia, North India, West Australia, and South
457
China (Data sources in Supplementary Information). Zircon ages > 1.0 were calculated
458
using 207Pb/206Pb and ages < 1.0 Ga were calculated using 206Pb/238U. Two downward
459
black arrows indicate approximate depositional ages of Neoproterozoic strata in Hetian
460
and Mesoproterozoic strata in Yutian (at 760 Ma and 1000 Ma, respectively, Fig. S3).
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n-number of single-grain zircon ages.
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Fig. 10 a: reconstruction of Columbia showing the position of Tarim Craton (modified
464
from Zhao et al., 2004); b: reconstruction of Rodina showing the position of Tarim
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Craton (after Cawood et al., 2015); c: Series of schematic evolution model for the Tarim
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Craton during Proterozoic. N-north, S-south.
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Table captions
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Table 1 Complied data of igneous rock in Tarim Craton.
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Table 2 Zircon U-Pb data for Neo-Mesoproterozoic strata in south Tarim in this study.
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Table 3 Hf data of zircons for Neo-Mesoproterozoic strata in south Tarim in this study.
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473 474
The authors declare no conflict of interest
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Northern Tarim possibly collided with southern Siberia at 1.8-2.0 Ga within Columbia, and drifted away at 0.9-1.5 Ga. Southern Tarim possibly collided with north India during the assembly of Rodinia and drifted away at 800 Ma. This model considers the Tarim Craton as a single block in the period from Columbia to Rodinia