Precambrian Research 259 (2015) 78–94
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Precambrian Research
jo urnal homepage: www.elsevier.com/locate/precamres
Proterozoic supercontinental restorations: Constraints from
provenance studies of Mesoproterozoic to Cambrian clastic rocks, eastern Siberian Craton
a,∗ b a c
Andrei Khudoley , Kevin Chamberlain , Victoria Ershova , James Sears ,
d c,e f a
Andrei Prokopiev , John MacLean , Galina Kazakova , Sergey Malyshev ,
f g h i
Anatoliy Molchanov , Kåre Kullerud , Jaime Toro , Elizabeth Miller ,
j,k a,l l
Roman Veselovskiy , Alexey Li , Don Chipley
a
Geological Department, St. Petersburg State University, 7/9 University Nab., St. Petersburg 199034, Russia
b
Department of Geology and Geophysics, University of Wyoming, 1000 E. University Ave., Dept. 3006, Laramie, WY 82071, USA
c
Department of Geosciences, University of Montana, Missoula, MT 59812, USA
d
Diamond and Precious Metal Geology Institute SB RAS, Lenin Avenue 39, Yakutsk 677980, Republic Sakha (Yakutia), Russia
e
Southern Utah University, 351 West University Boulevard, Cedar City, UT 84720, USA
f
All Russian Geological Research Institute (VSEGEI), Sredniy Prospect 74, St. Petersburg 199106, Russia
g
Department of Geology, Faculty of Science and Technology, University of Tromsø, 9037 Tromsø, Norway
h
Department of Geology & Geography, West Virginia University, Morgantown, WV, USA
i
Department of Geological and Environmental Sciences, Stanford University, Stanford, CA 94305, USA
j
Geological Department, Moscow State University, 1 Vorob’evy Gory, Moscow 119899, Russia
k
Schmidt Institute of Physics of the Earth RAS, B. Gruzinskaya 10, Moscow 123995, Russia
l
Department of Geological Sciences and Geological Engineering, Queen’s University, Kingston, Ontario K7L 3N6, Canada
a r t i c l e i n f o a b s t r a c t
Article history: The Mesoproterozoic–Neoproterozoic sedimentary succession of the eastern part of the Siberian Craton
Received 28 April 2014
consists of several unconformity-bounded, kilometer-scale siliciclastic-carbonate cycles. The overlying
Received in revised form
Lower Cambrian rocks are often compositionally similar to the uppermost units of the Neoproterozoic
26 September 2014
succession.
Accepted 1 October 2014
Twenty-nine samples were collected for U–Pb detrital zircon study and 27 samples were analyzed
Available online 14 October 2014
for whole-rock Sm–Nd isotopes. In total, 1491 detrital zircon grains were dated and 1148 grains were
selected for provenance interpretation. Samples from the Uchur and Aimchan groups only contain detri-
Keywords:
tal zircons of Paleoproterozoic and Archean age. Samples from the Kerpyl Group located on the Siberian
Eastern Siberian Craton
Craton contain Paleoproterozoic and Archean grains as well, but samples from the Kerpyl Group in the
Mesoproterozoic - Lower Cambrian
U–Pb detrital zircon geochronology Sette-Daban Ridge have significant numbers of Mesoproterozoic detrital zircons. Mesoproterozoic detri-
Sm–Nd isotopic study tal zircons predominate in samples from the Uy Group. In the northern part of the study area, samples
Provenance from the uppermost Neoproterozoic and Lower Cambrian strata contain numerous ca. 790–590 Ma detri-
Paleocontinent restoration
tal zircons, whereas in the southern part of the study area only Paleoproterozoic and Archean grains have
been found. The whole-rock Sm–Nd isotopic values of clastic rocks show that most samples have isotopic
signatures typical for the Siberian Craton basement, whereas some samples from the Kerpyl Group and
younger rock units have isotopic signatures typical of the Grenville Orogen.
Most of the Archean and Paleoproterozoic detrital zircons were eroded from the basement of the
Siberian Craton, although some ca. 2080–2030 Ma detrital zircons are likely to have a non-Siberian pro-
venance. However, rocks younger than ca. 1700 Ma are not known in the Siberian Craton basement and
all Mesoproterozoic and younger grains must therefore have a non-Siberian provenance.
The detrital zircon age distributions and whole-rock Nd isotopic signatures of many samples from
the Kerpyl Group and younger units are very close to those of the Grenville Orogen in North America,
∗
Corresponding author. Tel.: +7 9217573876.
E-mail address: [email protected] (A. Khudoley).
http://dx.doi.org/10.1016/j.precamres.2014.10.003
0301-9268/© 2014 Elsevier B.V. All rights reserved.
A. Khudoley et al. / Precambrian Research 259 (2015) 78–94 79
suggesting that erosion of the latter contributed to clastic deposition along the Siberian margin. Three pale-
ocontinental restorations proposed by Sears and Price (1978, 2003), Rainbird et al. (1998) and Pisarevsky
and Natapov (2003) are invoked to explain the occurrence of Grenville-age detrital zircons in the Siberian
sedimentary succession. The provenance of ca. 790–590 Ma detrital zircons is most likely to be located
within the Central Taimyr accretionary belt formed along the northern margin of the Siberian Craton in
the Neoproterozoic.
© 2014 Elsevier B.V. All rights reserved.
1. Introduction 2. Geologic setting and stratigraphy of Meso- to
Neoproterozoic rock units
The Siberian Craton is the largest structural unit of northeast
Asia, consisting of Archean to Paleoproterozoic basement and a The study area, located in eastern Siberia, occupies the east-
thick overlying Mesoproterozoic to Cenozoic sedimentary cover. It ern and central parts of the Siberian Craton and the foreland
is bordered by the Taimyr, Verkhoyansk, and Central Asian fold and of the adjacent Verkhoyansk Fold and Thrust Belt (Verkhoyansk
thrust belts to the north, east and south respectively, which display FTB), underlain by Archean and Paleoproterozoic crystalline base-
a series of extensional and compressional events related to the for- ment varying in age from ca. 3570 Ma to ca. 1700 Ma (e.g. Smelov
mation and break-up of paleocontinents from the Precambrian to et al., 2001, and references therein) (Fig. 1). Recent overviews
Mesozoic time. emphasize the distribution of ca. 2000–1850 Ma, 2600–2500 Ma
Since the study by Sears and Price (1978), many authors and 3100–2900 Ma rocks in the Siberian Craton basement that also
have discussed the relationship between the Siberia paleo- have Nd model ages (TDM) older than ca. 2100 Ma (Rosen et al.,
continent and other continents in the Precambrian. The most 2006; Smelov and Timofeev, 2007; Glebovitsky et al., 2008).
studied connection has been the one between Siberia and Lau- The Meso- to Neoproterozoic stratigraphy of the strata dis-
rentia, with differing reconstructions modeling a connection cussed here was established by Semikhatov and Serebryakov
between northern Laurentia and various parts of the Siberian (1983), and mainly followed by Shenfil (1991), and Melnikov et al.
Craton, including: northern Siberia (Hoffman, 1991; Pelechaty, (2005). This stratigraphy was significantly revised as isotopic dat-
1996), eastern Siberia (Condie and Rosen, 1994), southeast- ing of magmatic and carbonate rocks was carried out (see overview
ern Siberia (Frost et al., 1998), and southern Siberia (Rainbird in Khudoley et al., 2007, and references therein). In this paper
et al., 1998; Gallet et al., 2000; Pavlov et al., 2002; Didenko we mainly follow the correlations presented by Khudoley et al.
et al., 2003). In the reconstructions proposed by Sears and (2007) with the incorporation of new data discussed here. How-
Price (1978, 2003), western Laurentia was connected to east- ever, available isotopic studies are still scarce and often insufficient
ern Siberia, whereas some studies rule out a Laurentia–Siberia for reliable correlation; therefore the stratigraphic chart, proposed
connection (Smethurst et al., 1998). From 1999 to 2004 an inter- in this paper (Fig. 2) should be considered as a first-order approxi-
national team addressed the problems concerning reconstruction mation only.
of the late Mesoproterozoic–Neoproterozoic Rodinia superconti- According to Semikhatov and Serebryakov (1983), the most
nent with Siberia forming a promontory of the supercontinent complete Meso- and Neoproterozoic succession is located along
(Li et al., 2008) following ideas discussed earlier by Pisarevsky the southeastern margin of the Siberian Craton and correspond-
and Natapov (2003). However, just a few years later, new stud- ing parts of the Verkhoyansk FTB. The Meso- and Neoproterozoic
ies provided support for a southern Siberia–northern Laurentia succession here is divided into the following six widely recognized
connection (Evans and Mitchell, 2011; Metelkin et al., 2012) and units: the Uchur Group, Aimchan Group, Kerpyl Group, Lakhanda
an eastern Siberia–western Laurentia connection (MacLean et al., Group, Uy Group and Yudoma Group (Fig. 2). According to Rus-
2009; Sears, 2012). sian stratigraphic nomenclature the first five groups are Riphean,
These contrasting reconstructions result from a paucity of com- whereas the Yudoma Group is Vendian in age (e.g. Melnikov et al.,
parative geological data. At least three concurrent models of the 2005; Khudoley et al., 2007). The Uchur, Aimchan and Kerpyl groups
Siberian Craton basement age and composition are widely dis- are unconformity-bounded, kilometer-scale siliciclastic-carbonate
cussed (Rosen, 2003; Smelov and Timofeev, 2007; Glebovitsky transgressive cycles. Significant unconformities are documented at
et al., 2008), casting doubt on any restoration based on matching the base of the Yudoma Group and at the base of its upper unit
basement structures from different continents. Provenance stud- as well. Smaller-scale siliciclastic-carbonate transgressive cycles,
ies appear to be more useful, giving direct information on the mainly composed of carbonates occur in the Lakhanda and Yudoma
age of eroded rocks and constraining the relationship between groups. The Uy Group is clastic and its lower part contains sev-
uplifted crustal blocks and the potential source of clastics, but eral coarsening-upward cycles several hundred meters thick. Most
only a few provenance studies of Meso- and Neoproterozoic of these formations contain indicative sedimentary structures of a
rocks of Siberia have been published to date (Rainbird et al., shallow marine depositional environment and only the Uy Group
1998; Khudoley et al., 2001; MacLean et al., 2009; Chumakov contains evidence for deeper-water gravity-mass-flow sedimenta-
et al., 2011a, 2011b; Gladkochub et al., 2013; Letnikova et al., tion.
2013). Two distinct southern and northern areas are recognized, based
Since the early 2000s, many authors of this paper have been on variations in regional stratigraphy (Fig. 2). In the south, the Aim-
involved in a series of projects which included U–Pb detrital zircon chan and Uy groups are truncated westward across the platform
and whole-rock Sm–Nd dating of clastic Meso- and Neoproterozoic and, farther to the west, the Yudoma Group truncates the Kerpyl
rocks in the eastern and central parts of the Siberian Craton. The Group and unconformably rests on the Uchur Group or crystalline
main subject of this paper is to discuss these studies with an empha- basement. A recent U–Pb detrital zircon study of the lowermost
sis on their consequences for paleocontinental reconstruction. The clastic unit, previously described as a part of the lower Mesopro-
main focuses of this study are the Meso- to Neoproterozoic clas- terozoic succession and penetrated by Srednemarkhinsk 2250 Well
tic rocks that rim the Siberian Craton, but Lower Cambrian clastic in the central part of the Siberian Craton (Fig. 1), revealed that it
rocks were studied in a few locations as well. contains detrital zircon grains as young as 740 ± 5, 710 ± 4, and
80 A. Khudoley et al. / Precambrian Research 259 (2015) 78–94
Fig. 1. Distribution of the Mesoproterozoic to Neoproterozoic sedimentary basins in Siberian Craton and location of the sampled sections (after Shenfil, 1991; Surkov and
Grishin, 1997; Khudoley et al., 2007).
689 ± 3 Ma (Kochnev et al., 2013). Furthermore, basal conglomer- Mukun Group, has shown occurrence of detrital zircon grains as
ates are compositionally similar to the Neoproterozoic diamictites young as ca. 1000 Ma pointing to local occurrence of a Neoprotero-
from southern Siberia (Kochnev et al., 2013). If this lower clas- zoic clastic unit that has not previously been recognized (Fig. 2)
tic unit is indeed Neoproterozoic in age, the commonly accepted (Kuptsova et al., 2011).
widespread distribution of Mesoproterozoic rocks across central
Siberia (e.g. Melnikov et al., 2005) may be an overestimation, as 3. Provenance study
upper Neoproterozoic rocks correlated with the Yudoma Group
typically rest directly on crystalline basement. The basal diamictite 3.1. Sampling and analytical procedure
unit has not been reported along the eastern margin of the Siberian
Craton suggesting that deposition of the Yudoma Group and its cor- Within the study area, 29 samples for the U–Pb detrital zircon
relatives was time transgressive, commencing in different parts of study and 27 samples for the Sm–Nd whole-rock isotopic study
the Siberian Craton at different times. On the southeastern margin were collected (Online Attachment 1). U–Pb dating of detrital zir-
of the Siberian Craton, the Yudoma Group unconformably overlies cons is important for the understanding of the provenance history
the Ingili alkaline intrusion, which has yielded a U–Pb zircon age of of clastic sediments, as the age of individual grains can often be
±
654 7 Ma (Figs. 1 and 2) (Yarmolyuk et al., 2005). used to interpret the age of the source rock. Over the past 20 years,
In the northern part of Siberia, the stratigraphy of Meso- and detrital zircon geochronology has become the most powerful tool
Neoproterozoic rocks is more complicated reflecting deposition in for provenance study and also for the estimation of the maximum
mostly isolated sedimentary basins (Fig. 2). A recent carbon and depositional age of clastic rock units (e.g. Gehrels, 2012 and refer-
oxygen isotopic study by Khabarov and Izokh (2014) showed that ence therein). However, whilst zircons are numerous within felsic
the exposed section in the Kharaulakh Mountains (frontal ranges rocks, they are much rarer in mafic or ultramafic rocks. By con-
of the Verkhoyansk FTB) is not older than ca. 800 Ma. According trast, Sm–Nd isotopic ratios in clastic rocks are very sensitive to
to U–Pb baddeleyite dating the thick Sololy sill from the Olenek the presence of juvenile rocks in the source region (e.g. McLennan
±
uplift is as old as 1473 24 Ma (Wingate et al., 2009), suggesting et al., 2003, and references therein). We therefore used both U–Pb
that most of the succession is early Mesoproterozoic in age. The detrital zircon and Sm–Nd whole-rock isotopic studies to obtain
sedimentary succession in the Khastakh 930 Well has been corre- the most complete information on the age and composition of the
lated with that of the Olenek uplift in different ways (Grausman, provenance regions for the clastic sediments studied.
1995; Melnikov et al., 2005). Following the similarity in the detrital U–Pb detrital zircon ages were determined using different
zircon age distribution, discussed later in this paper, we provision- equipment (Online Attachment 1). Eight samples (X04-15-3, X04-
ally correlate the Khaipakh Formation of the Khastakh 930 Well 16-2, X04-23, X04-24, X04-33, X04-34, Mls-1, TT-3) were studied
(Grausman, 1995) with the Uktinsk Formation of the Kharaulakh using the SHRIMP-RG facility at Stanford University, 4 samples
Ridge (Fig. 2). The best exposed Meso- and Neoproterozoic section (309-322, 514-2, 571-3, 678) were studied using the SHRIMP-II
was documented along the margins of the Anabar Shield, where the facility at VSEGEI (St. Petersburg), and 7 samples (09AP117, Shein1,
upper part of the clastic succession (Mukun Group) was intruded Shein6, Shein9, Khast12, Khast19, Khast55) were studied using
±
by a sill dated as 1513 51 Ma (Sm–Nd isochron age, Veselovskiy Cameca IMS 1280 (NORDSIM, Stockholm). LA-ICP-MS equipment
±
et al., 2006) or 1493 34 Ma (U–Pb baddeleyite age, Khudoley et al., was used to study 10 samples (X04-15-3, X04-16-2, X04-18, X04-
±
2009). Overlying carbonates are cross-cut by a 1384 4 Ma mafic 19, X04-21, X04-23, X04-26, X04-33, C-3, TT-4) at Washington
dyke (U–Pb baddeleyite age, Ernst et al., 2000), pointing to an State University, 3 samples (07AP36, 07AP42, 07AP43) at Queen’s
early Mesoproterozoic age of the succession. However, the recent University, and 1 sample (99JT02) at Arizona Laser Chron Center.
U–Pb detrital zircon study of a clastic unit penetrated by wells in Most samples were studied using LA-ICP-MS and SHRIMP technolo-
the southeastern part of the Anabar Shield and interpreted as the gies, and in order to ensure consistency between data from the
A. Khudoley et al. / Precambrian Research 259 (2015) 78–94 81
Fig. 2. Meso-Neoproterozoic stratigraphic chart for the eastern Siberian Craton. Ages in italics are from this study. Data source for compiled sections: Rainbird et al. (1998),
Ovchinnikova et al. (2001), Ernst et al. (2000), Semikhatov et al. (2000, 2003), Melnikov et al. (2005), Yarmolyuk et al. (2005), Veselovskiy et al. (2006), Khudoley et al. (2007,
2009), Kochnev et al., 2013, Khabarov and Izokh (2014) and references therein. Local stratigraphic unit names: Uc – Uchur Group, Am – Aimchan Group, Kr – Kerpyl Group, Lh
– Lakhanda Group, Us – Uy Group, Jd – Yudoma Group, Uk – Uktinsk Formation, Es – Eseleekh Formation, Nl – Neleger Formation, St – Sirtchan Formation, Hr – Kharayutekh
Formation, Hp – Khaipakh Formation of the Khastakh 930 Well, nn – noname unit, Hb – Khorbusuonka Group, Mk – Mukun Group, Bl – Billyakh Group, Sr – Staraya Rechka
Formation.
two instruments, we analyzed thirty-six grains from four samples 1280. Following Gehrels (2012) we used a −10% to 30% discordance
(X04-15-3, X04-16-2, X04-23, X04-33) by both instruments. Mea- cutoff for zircons studied by LA-ICP-MS to preserve the relative
surements were taken from the same spots on twenty-six grains proportion of zircons with different ages. Grains with common Pb
and from different spots on ten grains. Two of the analyses did content above 5% and with 1 error >100 Ma were also filtered.
207 206 206 238
not yield interpretable results; the other thirty four Pb/ Pb Interpreted ages are based on the Pb/ U ratio for grains with
206 238 207 206
dates are equivalent within 2 error. Therefore, we assume that Pb/ U ages younger than 1000 Ma, and the Pb/ Pb ratio
206 238
there is little or no instrument bias between the datasets from the for grains with Pb/ U ages older than 1000 Ma. After filtering,
two instruments (MacLean, 2007). The analytical procedures, data 1148 grains were selected for interpretation and discussion. Two
tables and concordia plots for each sample are presented in files samples (07AP-42 and Shein6) each contained one dated zircon
combined in Online Attachment 2. in each sample that was obviously younger than the depositional
A total of 1491 detrital zircon grains were dated. Individual grain age (ca. 470 Ma and 425 Ma, respectively) and these were also
ages were filtered by discordance, with the filter being set at −5% excluded from the discussion. Sample 571-3 was collected from
to 10% discordance for zircons studied by SHRIMP or Cameca IMS the Mukun Group that is cut by dykes dated as 1384 ± 4 Ma (Ernst
82 A. Khudoley et al. / Precambrian Research 259 (2015) 78–94
Well successions, located in the internal parts of the Siberian Craton
(Fig. 4). The stratigraphy and facies changes of the Meso- and Neo-
proterozoic rocks of this area were discussed in detail by Khudoley
et al. (2001).
3.2.1. Lower Mesoproterozoic: Uchur Group
The easternmost succession located in the Sette-Daban Ridge
is represented by samples X04-24 and X04-26 (Figs. 2 and 4).
Sample PN-1 from Khudoley et al. (2001) is also included. Sam-
ples X04-24 and PN-1 are arkosic sandstones from the same
lowermost exposed unit and are from approximately the same
stratigraphic horizon. Sample X04-26 is a quartzose to subarkosic
sandstone with a dolomitic matrix and is from the upper part of
the Uchur Group. In total, 71 grains were used to produce the
probability plot. The detrital zircon age distribution is character-
ized by a significant, almost unimodal, Paleoproterozoic age peak
at 2060–2055 Ma, with only two Archean grains between 2900 and
2750 Ma and a few grains younger than 2000 Ma (Fig. 5A). Deposi-
tional age of the lower unit is constrained by the age of the youngest
detrital zircon grain at 1717 ± 32 Ma (2 , Khudoley et al., 2001),
whereas the youngest grain in the upper part of the Uchur Group
Fig. 3. Detrital zircon age probability plot and concordia plots for the sample Shein1.
±
A – concordia plot for all grains with the 32-point (gray ellipses) discordia identifying is 1521 31 Ma.
±
an upper intercept age at 2721 7 Ma, B – probability plot for grains that meet The succession located in the frontal ranges of the Verkhoyansk
concordance criteria,.
FTB is represented by a sample from the Ebeke-Khayata Ridge (X04-
33, Fig. 5B), whereas the succession located in the internal part
et al., 2000) and ca. 1500 Ma (Veselovskiy et al., 2006; Khudoley of the Siberian Craton is represented by a sample from the Uchur
et al., 2009). The youngest detrital zircon grain in sample 571-3 has Depression (309–322, Fig. 5C). Fifty-three and 26 grains respec-
207 206
±
been dated in two spots, yielding Pb/ Pb ages of 1341 41 Ma tively were used to produce the probability plots. Both samples
±
(spot 571-3.25.1, 4.7% discordance) and 1574 22 Ma (spot 571- are red arkosic to lithic sandstones. The detrital zircon population
3.25.2, 29.8% discordance). However, the grain has a high U content in X04-33 (platform margin) is very similar to that in the Sette-
(ca. 1600 ppm) and contains several fractures showing evidence of Daban Ridge succession displaying an almost unimodal distribution
alteration and, therefore, we did not use this grain for the maximum with a Palaeoproterozoic age peak at 2055–2050 Ma. In the Uchur
depositional age estimation. Depression, the detrital zircon population also has a prominent
Several samples with a high proportion of discordant grains Paleoproterozoic age peak but at 1980 Ma, with a few grains dated
have concordia plots with a clustered distribution. For example, at 2300–2200 Ma and 2850–2500 Ma.
the sample Shein1 contains 64 dated grains, but only 28 of them
met concordance criteria (Fig. 3A and B). However, the concor- 3.2.2. Middle Mesoproterozoic: Aimchan Group
dia diagram indicates broadly modern-day Pb loss for grains with Two samples from the Sette-Daban and Ebeke-Khayata ridges
207 206
Pb/ Pb age ranging from 2740 Ma to 2620 Ma. Although only were analyzed, X04-21 and X04-34 respectively. Both sam-
13 out of the 32 grains met the concordance criteria, the 32-point ples are quartz sandstones from the lowermost sandstone units
±
discordia identify an upper intercept age at 2721 7 Ma (Fig. 3A). above the unconformity between the Aimchan and Uchur groups
Although the probability plots contain only grains that met the (Figs. 2 and 4). Sample X04-21 has a dolomitic matrix. Fifty-seven
concordance criteria, a study of the clustered distribution of zircon grains were used to produce the probability plot for the Sette-
grains was also used to identify the provenance more precisely. Daban Ridge succession (X04-21). Paleoproterozoic detrital zircons
For the following discussion, we produced probability plots predominate with prominent peaks at 2050 Ma and 1980 Ma and a
combining together samples from the same area which sit within few Archean grains at 3250–2700 Ma (Fig. 6A). The three youngest
a similar part of the stratigraphy and have a similar detrital zir- grains have a weighted average age of 1696 ± 28 (2 ) Ma, which
con age distribution. Data from papers by Rainbird et al. (1998) and does not definitively constrain the depositional age. In the Ebeke-
Khudoley et al. (2001) were incorporated as well. Khayata Ridge succession, only 32 grains were used to produce
Sm and Nd isotopes were analyzed in the Institute of Geology the probability plot (X04-34, Fig. 6B). Both Paleoproterozoic and
and Geochronology of Precambrian of the Russian Academy of Sci- Archean grains are abundant in the detrital zircon population.
ences, St. Petersburg. The analytical procedure and data tables for Among the Paleoproterozoic grains, age probability peaks occur
these analyses are presented in Online Attachment 3. To enlarge at 2055 Ma, whereas Archean grains are distributed from 2950
the data set, data from Podkovyrov et al. (2007) and Kuptsova et al. to 2550 Ma with the most prominent age probability peak at
(2011) were incorporated as well. 2740–2735 Ma. In sample X04-34, 30 grains, including those with
high discordance, define a discordia that has an upper intercept
±
3.2. U–Pb detrital zircon data: Southern area with concordia at 2027 17 Ma.
In the southern area (Fig. 2) samples from the Sette-Daban Ridge, 3.2.3. Upper Mesoproterozoic: Kerpyl Group
Ebeyke-Khayata and Kyllakh ridges, Uchur Depression, and Shein The Sette-Daban Ridge succession, located within the Verkhoy-
1P Well were analyzed. Three successions with differing stratig- ansk FTB, is represented by sample X04-23. Data from sample TT-2,
raphy and structural setting are recognized: (1) the Sette-Daban previously reported by Khudoley et al. (2001) were also included.
succession, located within the Verkhoyansk FTB, (2) the Ebeke- Both samples are subarkosic sandstones and were taken from the
Khayata and Kyllakh successions, located in the frontal ranges of basal part of the succession just above the pre-Kerpyl unconformity
the Verkhoyansk FTB where deformed sedimentary cover of the (Figs. 2 and 4). In total, 115 grains have been used to produce the age
Siberian Craton is exposed, (3) the Uchur Depression and Shein 1P probability plot. Fifty-one grains (44% of the total population) are
A. Khudoley et al. / Precambrian Research 259 (2015) 78–94 83
Fig. 4. Correlation chart for the Mesoproterozoic and Neoproterozoic sedimentary units of the southern area showing location of samples for U–Pb detrital zircon dating and
facies and thickness changes of rock units. Uc – Uchur Group, Am – Aimchan Group, Kr – Kerpyl Group, Lh – Lakhanda Group, Us – Uy Group, Jd – Yudoma Group.
Data source: Semikhatov and Serebryakov (1983), Khudoley et al. (2001, 2007) and Melnikov et al. (2005).
Mesoproterozoic in age showing an age distribution with promi- 99JT02) were collected (Figs. 2 and 4). Data from sample MM-1,
nent peaks at 1200 Ma, 1495 Ma, and 1560–1555 Ma (Fig. 7A). Fifty previously reported by Rainbird et al. (1998), were also used in our
five grains (48%) are of Paleoproterozoic age, with the most promi- compilation. Sandstone composition varies from greywacke and
nent peak at 2035–2030 Ma and several subordinate peaks ranging lithic sandstone to arkose and subarkose. All studied samples are
from 1950 to 1820 Ma. Only 9 grains (8%) are Archean, ranging in quite immature in composition.
age from 2900 to 2550 Ma. The four youngest grains overlap in In total, 185 grains were used to produce the age probability plot.
age within 1 error and yield a weighted average age at 1120 ± 17 Mesoproterozoic grains predominate, comprising 71% of the whole