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International Geology ReviewPublication details, including instructions for authors and subscription information:http://www.tandfonline.com/loi/tigr20
Constraining the mid-crustal channel flow beneath theTibetan Plateau: data from the Nielaxiongbo gneissdome, SE TibetDan-Ping Yan a b , Mei-Fu Zhou b , Paul T. Robinson b c , Djordje Grujic c , John Malpas b ,Allen Kennedy d & Peter H. Reynolds ca The State Key Laboratory of Geological Processes and Mineral Resources and School ofEarth Sciences and Resources, China University of Geosciences, Beijing, 100083, PR Chinab Department of Earth Sciences, University of Hong Kong, Hong Kong, PR Chinac Department of Earth Sciences, Dalhousie University, Halifax, NS, Canadad SHRIMP Facility, John de Laeter CEMS, Curtin University, Bentley, 6103, Australia
Available online: 24 Jun 2011
To cite this article: Dan-Ping Yan, Mei-Fu Zhou, Paul T. Robinson, Djordje Grujic, John Malpas, Allen Kennedy & Peter H.Reynolds (2012): Constraining the mid-crustal channel flow beneath the Tibetan Plateau: data from the Nielaxiongbo gneissdome, SE Tibet, International Geology Review, 54:6, 615-632
To link to this article: http://dx.doi.org/10.1080/00206814.2010.548153
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International Geology ReviewVol. 54, No. 6, 20 April 2012, 615–632
Constraining the mid-crustal channel flow beneath the Tibetan Plateau: data from theNielaxiongbo gneiss dome, SE Tibet
Dan-Ping Yana,b∗, Mei-Fu Zhoub, Paul T. Robinsonb,c, Djordje Grujicc, John Malpasb,Allen Kennedyd and Peter H. Reynoldsc
aThe State Key Laboratory of Geological Processes and Mineral Resources and School of Earth Sciences and Resources, ChinaUniversity of Geosciences, Beijing 100083, PR China; bDepartment of Earth Sciences, University of Hong Kong, Hong Kong, PR
China; cDepartment of Earth Sciences, Dalhousie University, Halifax, NS, Canada; dSHRIMP Facility, John de Laeter CEMS, CurtinUniversity, Bentley 6103, Australia
(Accepted 8 November 2010)
Gneiss domes involving the South Tibetan Detachment System provide evidence for crustal extension simultaneous withshortening. The Nielaxiongbo gneiss dome is composed of a metamorphic complex of granitic gneiss, amphibolite, andmigmatite; a ductilely deformed middle crustal layer of staurolite- or garnet-bearing schist; and a cover sequence of weaklymetamorphosed Triassic and Lower Cretaceous strata. The middle crust ductilely deformed layer is separated from boththe basement complex and the cover sequence by lower and upper detachments, respectively, with a smaller detachmentfault occurring within the ductilely deformed layer. Leucogranites crosscut the basement complex, the lower detachment,and the middle crustal layer, but do not intrude the upper detachment or the cover sequence. Three deformational fabricsare recognized: a N–S compressional fabric (D1) in the cover sequence, a north- and south-directed extensional fabric (D2)in the upper detachment and lower tectonic units, and a deformation (D3) related to the leucogranite intrusion. SHRIMPzircon U–Pb dating yielded a metamorphic age of ∼514 million years for the amphibolite and a crystallization age of ∼20million years for the leucogranite. Hornblende from the amphibolite has an 40Ar/39Ar age of 18 ± 0.3 million years, whereasmuscovites from the schist and leucogranite yielded 40Ar/39Ar ages between 13.5 ± 0.2 and 13.0 ± 0.2 million years. Theseresults suggest that the basement was consolidated at ∼510 Ma and then exhumed during extension and silicic plutonism at∼20 Ma. Continuing exhumation led to cooling through the 500◦C Ar closure temperature in hornblende at ∼18 Ma to the350◦C Ar closure temperature in muscovite at ∼13 Ma. The middle crustal ductilely deformed layer within gneiss domesof southern Tibet defines a southward-extruding ductile channel, marked by leucogranites emplaced into migmatites andamphibolites. We propose a model involving thinned upper crust for the initial extension of the Tibetan Plateau in the earlyMiocene.
Keywords: Nielaxiongbo; SE Tibet; gneiss dome; mid-crustal channel flow; South Tibetan Detachment System; middlecrustal layer; leucogranite
1. Introduction
Gneiss domes occurring within the South Tibetan sedi-mentary sequence have similar structural geometries anddeformational successions (Burg et al. 1984; Chen et al.1990; Lee et al. 2000, 2004, 2006; Aoya et al. 2005, 2006;Quigley et al. 2006, 2008), whereas numerous models havebeen proposed to explain their genesis. For example, Burget al. (1984) proposed a thrusting model to explain the for-mation of these domes, whereas Yin (2006) favoured a latewedge extrusion model in which the domes were formedby passive–active roof faulting. Nevertheless, all modelsaccount for the Miocene–Oligocene leucogranites (Zhanget al. 2004; Watts and Harris 2005; Aoya et al. 2006), wellknown in the Greater Himalayan Sequence (GHS) (Le Fort1981; France-Lanord and Le Fort 1988; Inger and Harris
∗Corresponding author. Email: [email protected]
1993; Harrison et al. 1997; Grujic et al. 2002). On theother hand, identification of the South Tibetan DetachmentSystem (STDS; Burg et al. 1984; Burchfiel et al. 1992;Edwards et al. 1996; Hodges 2000; Lee et al. 2000, 2004;Searle and Godin 2003; Aoya et al. 2005; Quigley etal. 2006; Lee and Whitehouse 2007; Zhang et al. 2007)(Figure 1) has led some workers to interpret the domesas metamorphic core complexes (e.g. Chen et al. 1990; Liet al. 2003).
A change in shear direction from top-to-north in thenorthern side to top-to-south in southern side in therocks of South Tibet has been related to intrusion of theleucogranites (Aoya et al. 2005, 2006). A similar kine-matic inversion, which has also been observed elsewherein the Himalaya along the footwall of the STDS, suggests
ISSN 0020-6814 print/ISSN 1938-2839 online© 2012 Taylor & Francishttp://dx.doi.org/10.1080/00206814.2010.548153http://www.tandfonline.com
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90°E
86°E
29
°N
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88°E 90°E 92°E
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Figure 1. A schematic tectonic map showing the distribution of North Himalayan gneiss domes in South Tibet and the South TibetanDetachment System (after Burchfiel et al. 1992; Hodges 2000). The South Tibetan Detachment System is marked by the heavy ticked linesin the hanging wall. YZS, Yarlung Zangbo Suture; STDS, South Tibetan Detachment. MCT, Main Central thrust; MBT, Main BoundaryThrust; A–B, cross section in Figure 9.
southward extrusion of the GHS (e.g. Grujic et al. 1996).Protracted melting of the middle crust during convergenceat ∼26–10 Ma (Harris et al. 2004; Zhang et al. 2004) sup-ports the existence of a mid-crustal ductile channel flow(Godin et al. 2006; Bai et al. 2010) related to the for-mation of the GHS and the STDS (Grujic et al. 1996,2002; Searle and Szulc 2005; King et al. 2007). Thus,the proposed mid-crustal ductile channel flow model mayprovide a link between the metamorphism, ductile defor-mation, and concomitant leucogranite intrusion in the GHSand the STDS (Grujic et al. 1996, 2002; Beaumont et al.2001, 2004; Jamieson et al. 2002, 2004, 2006; Searle andSzulc 2005; Hollister and Grujic 2006; King et al. 2007).However, the different processes of such a channel flow andgeochronological constraints need further determining.
The Nielaxiongbo gneiss dome, the easternmost domein South Tibet, lies about 250 km east of the Kangmardome (Chen et al. 1990; Lee et al. 2000; Aoya et al.2006). It contains leucogranites similar to those elsewherein South Tibet and the Greater Himalayas (BGMRXAR1993; Zhang et al. 2007). Little is known about the timingand origin of the leucogranite in this complex and its rela-tionship to the middle crustal rocks due to a lack of detailedstructural, petrographic, and geochronological data.
To determine the character of the Nielaxiongbo gneissdome and its relationship to the STDS and possibleexistence of mid-crustal channel flow beneath southern
Tibet, we carried out a reconnaissance field investigationand collected samples from all the relevant zones of thedome (Figure 2). This article describes the geology of thegneiss dome and presents new SHRIMP zircon U–Pb and40Ar/39Ar dating results for this body. The principal objec-tives of this article are to provide better constraints onthe deformational/magmatic history of the Nielaxiongbogneiss dome and to elucidate the role of ductile deforma-tion and silicic magmatism in its formation. We furthercombine our data with those from other North Himalayangneiss domes to explain the origin of these enigmatic fea-tures. Our data support a link between uplift of the NorthHimalayan gneiss domes and mid-crustal ductile channelflow in South Tibet.
2. Geological background
Southern Tibet consists of two major tectonic units: theIndian subcontinent to the south and the Lhasa Block tothe north, separated by the Yarlung Zangbo suture zone(Girardeau et al. 1984; Hirn et al. 1984; Zhou et al. 1996;Aitchison et al. 2000; Yin 2000) (Figure 1). The nar-row, 2–10 km-wide Yarlung Zangbo suture zone is markedby various lenses of Cretaceous ophiolites and mélange,Cretaceous forearc sedimentary sequences, and Tertiarymolasse deposits, and consists of highly deformed green-schist, mica-quartz schist (Rowley 1996; Aitchison et al.
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91°54″E
50°60°
35°
65°
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40°
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45°
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″N2
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″N
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″N2
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″N
92°00″E 92°06″E 92°12″E
Basement complex + leucogranites
91°54″E 92°00″E 92°06″E
L2 (n = 46)
6587 m
L2 (n = 9)
10 m 2 m
2 m
4 km
2 m
(A) (B)
(C)
S2
S0
(D) (E) (F)
92°12″E
Figure 2. Geological map of the Nielaxiongbo gneiss dome (modified from TGSA 2002 and Zhang et al. 2007). Pz1, lower Palaeozoic;Pz2, upper Palaeozoic; T3, Upper Triassic; K1, Lower Cretaceous. Insets A and B, a lower hemisphere Wulff net showing the D2 min-eral lineations (the solid dots are from TGSA 2002, and open squares are our measurements). C-D indicates a section crosscutting theNielaxiongbo dome.
2000, 2003; Malpas et al. 2003; Geng et al. 2006). TheLhasa Block is composed mainly of Precambrian basementrocks, Palaeozoic and Mesozoic cover strata intruded byabundant Mesozoic and Cenozoic granitic plutons (Zhuet al. 2009) (Figure 1). The basement rocks are com-posed mainly of gneiss, amphibolite, and schist, along withsporadic marble and granulite lenses (Dong et al. 2009;Wang et al. 2009; Zhang et al. 2010). These metamor-phic rocks show evidence of extensive migmatization andpolyphase deformation with P–T conditions of ∼1.0 GPaand 750−850◦C (Wang et al. 2009). The sedimentary coverof the Lhasa Block consists of Devonian to Jurassic sedi-mentary rocks together with volcanic intercalations (Genget al. 2006).
The Indian subcontinent includes the Tethys-Himalayasand the GHS. Within the subcontinent, the STDSjuxtaposes the Cambrian–Eocene Tibetan sedimentary
sequence over the GHS, which are composed mainly ofamphibolite- to granulite-facies Proterozoic metasedimen-tary rocks, intruded locally by early Palaeozoic granites(Liu and Zhong 1997; Lee et al. 2000; Ding et al. 2001;Yin and Harrison, 2001; Geng et al. 2006; Goscombeet al. 2006; Zhang et al. 2010). Farther south, the GHSlies above the Main Central Thrust (MCT). The MainBoundary Thrust separates the Lesser Himalayas from theSub-Himalayas (Figure 1). A series of gneiss domes farthernorth form an E–W-trending belt within the Tibetan sedi-mentary sequence (Figure 1). Leucogranites are commonin these domes.
3. Nielaxiongbo gneiss dome
The Nielaxiongbo gneiss dome is a NW-striking, dome-like anticline, 22 km long and 10 km wide. It consists
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of a metamorphic complex (BGMRXAR 1993; TGSA2002; Zhang et al. 2007; Zhang and Guo 2007), a ductilelydeformed middle crustal layer, and the Tibetan sedimen-tary sequence that in this area comprises Upper Triassicand Lower Cretaceous sedimentary strata. The basementcomplex is composed of amphibolite-grade gneissesand locally migmatite, kyanite + staurolite + garnetgneiss, biotite + muscovite + plagioclase gneiss, andbiotite + plagioclase gneiss with well-developed folia-tion. The metamorphic grade of these rocks decreasesstructurally upward around the dome. A similar decreasein metamorphic grade outward from the dome is alsoobserved in middle crustal Palaeozoic rocks overlying thebasement sequence. These rocks pass outward from garnet-mica schist, locally containing staurolite, to mica-bearingquartzite to phyllite. The cover sedimentary sequenceof Upper Triassic and Lower Cretaceous age is a majorcomponent of the Tibetan sedimentary sequence (Figure 1)and is composed of terrigenous flysch (TGSA 2002). Alower detachment separates the basement complex fromthe middle crustal layer, and a major upper detachmentseparates the middle crustal layer from the cover sequence(Figure 2). In addition, minor normal faults within themiddle crustal layer thinned or selectively removed partsof the strata. Several leucogranite plutons and stocksintrude the basement complex, the lower detachment,and the middle crustal layer, but do not intrude the upperdetachment (Figure 2). These relationships are similar
to those described for the Kangmar, Kampa, and otherdomes in South Tibet (Chen et al. 1990; Lee et al. 2000;Watts and Harris 2005; Quigley et al. 2006). At least threedeformational stages (D1–D3) have been identified withinthe Nielaxiongbo gneiss dome.
3.1. N–S compressional top-to-south phase (D1)
The earliest deformational phase D1 is well developed inthe Tibetan sedimentary sequence and locally preserved inthe upper detachment fault and the middle crustal layer. Itis represented by numerous sub-horizontal brittle thrusts,which typically cut the Tibetan sedimentary sequence.Within the Tibetan sedimentary sequence, the deformedplane is the original bedding surface (S0). The folds in thepelitic and psammitic interbeds are sub-harmonic in pro-file with type 1B folds in competent sandstone beds andtype 1C or 2 folds in incompetent shale or siltstone beds(cf. Ramsay and Huber 1987) (Figures 2 and 3A). Thesandstone layers display a fan-shaped spaced cleavage (S1
foliation), whereas the slates have inverse fan-shaped axialplane slaty cleavages (S1 foliation) (inset C in Figure 2).In some cases, S1 is represented by crenulation cleavage(inset F in Figure 2) and spaced cleavage, which has S-Cfabrics indicating southward thrusting and displays a strongflattening strain (Figure 3C). S1 is sub-perpendicular to thebedding S0 on a regional scale. The axial planes of the foldsstrike E–W and dip steeply to north in the northern limb
Figure 3. Field and thin section photos of brittle-ductile deformation and metamorphic mineral assemblages in the upper detachmentfault. (A) Type 1C fold in Triassic interlayered sandstone and argillite, which indicate S0 and S1. Distance along the axial trace is ∼300 m;(B) Triassic sandstone with penetrative cleavage S1; and (C) spaced cleavage with S-C fabric in the foliated sandstone.
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and to south in the southern limb of the dome (Figures 2and 3A–3C), reflecting regional N–S compression.
In general, structural styles in the middle crustal layerare similar to those in the Tibetan sedimentary sequence(inset in Figure 2). The metamorphic mineral assemblage,which defines the foliation (S1), consists of muscovite/sericite + plagioclase + chlorite + quartz (Figure 3B),reflecting deformation under low greenschist-faciesconditions.
3.2. Extensional deformational phase (D2)
Deformational phase D2 includes brittle/brittle-ductiledeformation in the upper detachment fault and ductiledeformation in the middle crustal layer, the basementdetachment, and the basement complex.
The upper detachment fault zone contains breccia andphyllite with phyllitic foliation S2, which is sub-parallel tothe fault (Figure 2). The upper detachment fault crosscutsD1 folds and S1 foliation and thus belongs to the D2 defor-mation (Figure 4A). The metamorphic mineral assemblagealong S2 within this fault consists of muscovite/sericite + chlorite + plagioclase + quartz (Figure 4A),which indicates low to middle greenschist-faciesconditions related to this deformation.
The ductile deformation of the middle crustal layer andbasement detachment (D2) is manifested by the presenceof (1) mylonite (Figures 4 and 5); (2) a penetrative S2
foliation (Figure 4B–4D) defined by the axial planesof intrafolial folds; and (3) N–S-trending ductile shearbands of centimetre size with a consistent top-to-the-northsense of shear, S-C fabric, kinking, and fan-type splittingalong (001) of S1 biotite porphyroblasts, garnet ‘b’-typepressure shadows, and well-developed mineral lineations,which have a N–S trend (Figures 2A, 2B, and 2F, 4Cand 4D). Within the sequence, the upper Palaeozoicrocks are separated from those of the lower Palaeozoicby a minor detachment fault (TGSA 2002). The meta-morphic mineral assemblages consist of muscovite +plagioclase + biotite + garnet + quartz + hornblende ±staurolite (Figure 6A and 6B), indicating loweramphibolite-facies conditions that produced a garnet–staurolite belt along the lower detachment (TGSA2001). The assemblage of muscovite + plagioclase+ biotite + garnet + quartz (garnet belt) in lowerPalaeozoic sequence indicates upper greenschist-faciesmetamorphism and somewhat higher grade assemblages,consisting of hornblende + biotite + plagioclase +garnet + staurolite + quartz (staurolite belt), indicateupper greenschist- to lower amphibolite-facies meta-morphism (Figure 2; TGSA 2002). An assemblage ofmuscovite + plagioclase + biotite + quartz (Figure 4D) inthe upper Palaeozoic strata indicates middle greenschist-facies metamorphism. The ductile deformation of D2
indicates north-directed extensional tectonics at themiddle–upper crustal level.
Ductile deformation at the top of the basement com-plex, which produced a mylonitic foliation (S2) and ashallowly N- or S-dipping mineral lineation (L2) (Figure5A and 5B), is equivalent to the D2 deformation in themiddle crustal layer; however, S-C fabrics and garnet ‘b’-type pressure shadows indicate a top-to-the-south sense ofshear (Figure 5B). The metamorphic mineral assemblagealong the S2 foliation consists of kyanite + sillimanite +K-feldspar + muscovite + hornblende + staurolite + pla-gioclase ± biotite + quartz (Figure 5A and 5B), indicatingamphibolite-facies metamorphism. The local occurrence ofmigmatite indicates partial melting within the complex.
3.3. Deformational phase (D3) related to the intrusionof leucogranites
The leucogranites form two nested bodies of adamellitewith many peripheral dikes and sills. The Quzen body(Figure 5C) intrudes the basement complex, the lowerdetachment fault, and the middle crustal layer, that is, itcuts through the D1 and D2 fabrics but not the upperdetachment fault or cover sequence (Figure 2; Zhanget al. 2007). S3 crenulation and L3 mineral lineation,which define the D3 deformation, dip steeply outwardaround the dome (Figures 2, 4A, and 5B). Thus, D3 wasformed during final emplacement of the leucogranites. Theleucogranites are medium grained and consist essentiallyof plagioclase (An24–26), K-feldspar, muscovite, and quartz(Figure 5D). The Quzen body is intruded by the Renbuobody of fine-grained adamellite with an identical mineral-ogy, that is, plagioclase (An22–24), K-feldspar, and quartzwith minor muscovite, biotite, zircon, apatite, and rutile.The leucogranites crosscut the well-developed D2 folia-tion and L2 lineation in the country rocks. A few samplesof deformed leucogranite (M22 and M1) from the Quzenbody contain remnants of sillimanite (D2) along shearbands (S3) (Figure 2) with steeply outward-dipping minerallineation, indicating that the leucogranite was emplacedinto sillimanite-grade country rocks already at high temper-ature and that the ductile deformation pre-dated the mainemplacement of the plutons.
4. Analytical methods
4.1. SHRIMP dating of zircon
Using conventional heavy liquid and magnetic techniques,zircon grains were separated from two samples, an amphi-bolite (M13) from the basement complex and a leucogran-ite (M22) from the Quzen body that intrudes the basementcomplex (Figure 2). After separation, about 100 grainsof zircon were mounted for U–Pb isotope analysis atthe SHRIMP II lab at Curtin University of Technology,Australia. Analytical and data-reduction procedures aresimilar to those described by Compston et al. (1984). Pb/Uages are based on a value of 564 million years determined
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Figure 4. Field and thin section photos of ductile deformation and metamorphic mineral assemblages in the middle crustal layer.(A) S2 crenulations with axial plane foliation S3. Note that quartz-rich and mica-rich shear bands define the S1 foliation; (B)penetrative S2 foliation within garnet-bearing mylonite of the middle crustal layer; (C) S2 defined by the oriented growth of mus-covite + plagioclase + biotite + quartz (garnet belt) in the middle crustal layer; (D) in the middle crustal layer, the penetrative S2 foliationis defined by alignment of muscovite + plagioclase + biotite + quartz, and σ -type garnet porphyroblasts with pressure shadows; and (E)S1 biotite porphyroblast shows kinking and fan-type splitting along (001) within the penetrative S2 foliation indicating top-to-the-northshearing in the lower detachment shear zone.
by thermal ionization mass spectrometry U–Pb analysis ofthe standard zircon CZ3. Because the 207Pb/206Pb ages aresensitive to the common Pb correction, the 206Pb/238U ageis normally adopted for Phanerozoic samples (Compstonet al. 1984). Individual analyses (Table 1) are presentedas 1σ error boxes on concordia plots and uncertainties inmean ages are quoted at the 95% confidence level (2σ ).
4.2. 40Ar/39Ar dating
For 40Ar/39Ar dating, muscovite was separated from apegmatitic adamellite (M12B) of the Renbuo body, aleucogranite of the Quzen body (M1), and a garnet-mica
schist (M7). Hornblende was separated from an amphi-bolite (M4) of the middle crustal layer. Fresh portions ofeach sample were cut, crushed, and sieved to obtain min-eral grains of 0.2–2 mm diameter. These were washed indistilled water in an ultrasonic bath for 30 min and air dried.Muscovite and hornblende separates, greater than 99%purity, were handpicked under a binocular microscope.Samples were loaded into irradiation disks along with thehornblende MMhb-1 standard (520 ± 2 Ma; Samson andAlexander 1987). The disks were wrapped in aluminiumfoil and vacuum sealed in silica glass tubes. The packageswere then shielded with cadmium and irradiated for 54hours at the McMaster University nuclear reactor. Isotopicanalyses were carried out in the Argon Isotope Laboratory
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Figure 5. Field and thin section photos of the deformation and mineral assemblages in the GHS and leucogranite. (A) Migmatiteof the GHS; (B) gneiss from the core complex showing mylonite foliation (S2) and a metamorphic mineral assemblage of (silli-manite) + hornblende + plagioclase + muscovite + biotite + quartz + K-feldspar; (C) leucogranite intruded into the amphibolite; and (D)leucogranite of the Quzen body.
(A)
M13-747±1 Ma
M22-3 (G1)482±9 Ma
M22-3 (G1)20±0 Ma
M13-651347±7 Ma
(B)
Figure 6. Cathodoluminescence morphologies of zircon grains from (A) amphibolite (M13) and (B) leucogranite (M22) of theNielaxiongbo, showing metamorphic recrystallization and growth in the leucogranite magma.
at Dalhousie University, Canada, using a VG 3600 massspectrometer equipped with an internal tantalum resistancefurnace of the double-vacuum type. Details of the experi-mental procedures are as described in Muecke et al. (1988).All dates are reported using 5.543 × 10−10 a−1 as the totaldecay constant for 40K (Steiger and Jager 1977).
5. Analytical results
5.1. SHRIMP zircon U–Pb age
The amphibolite, M13, from the basement complex con-tains zircon grains with a variety of textures and morpholo-gies. The grains display highly complex internal structuresas shown in the cathodoluminescence images (Figure 6A),
which likely resulted from variable degrees of recrystalliza-tion. Some grains have thin overgrowths with intermediateto high U contents and low and variable Th/U ratios(<1–0.01) (Figure 7A). Many of the recrystallized grainscontain inclusions.
The SHRIMP analytical results for zircon from sampleM13 are given in Table 1 and are plotted on a concordia dia-gram (Figure 7B and 7C); 14 of 18 analyses cluster around500 million years on the concordia diagram, whereas theother 4 have much younger ages (Figure 7B). Two grainswith ages close to 500 million years (M13-5 and M13-6)have very low U contents and one (M13-16) yielded a dis-cordant analysis (Figure 7C). When these three anomalousanalyses are excluded, the remaining 11 form a coherent
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Tabl
e1.
SH
RIM
PU
–Pb
isot
opic
anal
yses
for
zirc
ons
from
the
leuc
ogra
nite
and
base
men
tcom
plex
ofN
iela
xion
gbo
dom
e.
Rat
ios
corr
ecte
dco
mm
onP
bA
ges
(Ma)
Spo
t
206P
b c(%
)
U
(ppm
)
Th
(ppm
)
Pb
(ppm
)T
h/U
%co
ncor
danc
e20
6P
b/23
8U
±%20
7P
b/23
5U
±%20
7P
b/20
6P
b±%
208P
b/23
2T
h±%
206
Pb/
238
U±
207P
b/23
5U
±20
7P
b/20
6P
b±
M22
(Quz
enad
amel
lite
ofle
ucog
rani
te)
M22
-10.
0038
8580
3916
524
0.02
660.
0032
766.
50E
−05
0.02
0961
0.00
1036
0.04
641
0.00
1991
0.00
0835
0.00
0749
210
211
3287
M22
-20.
0085
6786
1813
228
0.02
00.
0035
147.
80E
−05
0.02
2197
0.00
1311
0.04
5812
0.00
2384
0.00
1114
0.00
1134
231
221
063
M22
-30.
0006
2494
816
770
0.18
100
0.07
7685
0.00
1457
0.60
742
0.01
3352
0.05
6708
0.00
0531
0.02
3009
0.00
0643
482
948
28
480
21
M22
-50.
0060
2923
1421
60.
010
0.00
2794
5.80
E−0
50.
0167
270.
0023
410.
0434
20.
0058
97−0
.000
726
−0.0
0436
618
017
20
59
M22
-60.
0101
9335
4348
100.
010
0.00
2907
5.90
E−0
50.
0175
790.
0020
480.
0438
540.
0049
230.
0006
170.
0025
8319
018
20
47
M22
-70.
0033
2773
3514
720
0.02
00.
0030
345.
90E
−05
0.01
8983
0.00
0872
0.04
5385
0.00
1777
0.00
0386
0.00
0620
019
10
37
M22
-70.
1797
941
2956
190.
010
0.00
2849
8.80
E−0
50.
0116
740.
0079
440.
0297
230.
0200
9−0
.006
607
−0.0
1031
418
112
80
41
M22
-80
5339
9014
0.02
120.
0028
635.
50E
−05
0.01
9443
0.00
0508
0.04
9255
0.00
077
0.00
208
0.00
0125
180
201
160
36
M22
-90.
0067
5444
3262
110.
010
0.00
2761
5.60
E−0
50.
0166
240.
0020
540.
0436
750.
0052
16−0
.000
799
−0.0
0251
318
017
20
40
M22
-40.
0043
7868
8912
420
0.02
00.
0032
096.
20E
−05
0.02
012
0.00
1082
0.04
5475
0.00
2176
0.00
0669
0.00
0914
210
201
033
M13
(am
phib
olit
ein
base
men
tcom
plex
)
M13
-187
359
877
0.68
111
0.08
1301
0.00
1149
0.62
8769
0.01
076
0.05
6091
0.00
0451
504
749
57
456
18
M13
-311
0545
593
0.41
980.
0823
250.
0011
820.
6562
710.
0119
690.
0578
160.
0005
5451
07
512
752
321
M13
-472
937
463
0.51
111
0.08
2263
0.00
1163
0.63
6879
0.01
3763
0.05
615
0.00
0824
510
750
09
458
33
M13
-535
924
531
0.68
910.
0796
430.
0011
780.
6409
760.
0189
910.
0583
70.
0013
9449
47
503
1254
452
M13
-634
587
280.
2510
40.
0828
540.
0012
490.
6517
730.
0192
040.
0570
530.
0013
4151
37
510
1249
452
M13
-784
912
267
0.14
102
0.08
3083
0.00
1171
0.65
6325
0.01
2566
0.05
7294
0.00
0648
514
751
28
503
25
M13
-838
812
821
0.33
870.
0510
680.
0007
730.
3801
160.
0089
710.
0539
840.
0008
8132
15
327
737
037
M13
-975
650
169
0.66
118
0.08
3136
0.00
1179
0.63
7348
0.01
328
0.05
5601
0.00
0756
515
750
18
436
30
M13
-10
1889
149
148
0.08
101
0.08
412
0.00
119
0.66
8804
0.01
1436
0.05
7663
0.00
0462
521
752
07
517
18
M13
-11
2653
9020
80.
0398
0.08
5148
0.00
1185
0.68
411
0.01
0726
0.05
827
0.00
0331
527
752
96
540
12
M13
-12
9121
3163
0.00
324
0.00
7692
0.00
0106
0.05
3357
0.00
0916
0.05
0309
0.00
0435
491
531
209
20
M13
-13
942
615
870.
6510
40.
0850
80.
0011
810.
6734
960.
0121
70.
0574
130.
0005
7252
67
523
750
722
M13
-14
1176
851
109
0.72
106
0.08
3446
0.00
1163
0.65
4373
0.01
1898
0.05
6875
0.00
0572
517
751
17
487
22
M13
-15
1292
1630
0.01
320.
0249
260.
0003
620.
1957
10.
0056
110.
0569
450.
0013
0815
92
181
548
951
M13
-16
946
673
900.
7190
0.08
6004
0.00
1399
0.70
7874
0.01
7461
0.05
9695
0.00
0993
532
854
310
593
36
M13
-17
2378
716
0.00
331
0.00
7289
0.00
011
0.04
9306
0.00
2515
0.04
9061
0.00
2298
471
492
151
106
M13
-18
1594
1113
142
0.70
101
0.08
112
0.00
1117
0.63
9228
0.01
0734
0.05
7152
0.00
046
503
750
27
497
18
M13
-19
186
8115
0.44
970.
0796
570.
0013
410.
6309
220.
0380
140.
0574
450.
0032
0549
48
497
2450
912
3
Not
es:20
6P
b c(%
)in
dica
tes
perc
enta
geof
tota
l206P
bth
atis
non-
radi
ogen
ic.C
omm
onP
bco
rrec
ted
byas
sum
ing
206P
b/23
8U
-208P
b/23
2T
hag
e-co
ncor
danc
e.
Dow
nloa
ded
by [
Gua
ngzh
ou I
nstit
ute
of G
eoch
emis
try]
at 0
1:38
15
Mar
ch 2
012
International Geology Review 623
10000
0.12
0.10
0.08
100
100
200
300
400
500
200
300
Upper intercepts at206
Pb/238
U = 470 ± 92 Ma
50 Ma
400
500
0.06
0.04
0.02
0.00
0.10
0.08
0.06
0.04
0.02
0.0000.0 0.2 0.4 0.6 0.8
0.0 0.1 0.2 0.3 0.4
207Pb/
235U
206P
b/2
38U
206P
b/2
38
U
207Pb/
235U
0.5 0.6 0.7 0.8
(A)
(B)
(D)
1000M22
Amphibolite, M13
Leucogranite, M22
M13
100
10
11 10
TH/U=1
TH/U=0.1
TH/U=0.0
1
100
U (ppm)
Th (
ppm
)
1000 10000
0.10
0.09
0.08
0.070.5 0.6 0.7 0.8
206P
b/2
38U
207Pb/
235U
(C)Amphibolite, M13
550
450
514 ± 6 Ma
206Pb/
238U = 514 ± 6 Ma
207Pb/
235U = 511 ± 6 Ma
207Pb/
206U = 503 ± 1 3 Ma
N = 11
0.0045
0.0035
0.0025
0.00150.008 0.012 0.016 0.020 0.024 0.028
Lower intercepts at206
Pb/238
U = 20.3 ± 1.9 Ma
206P
b/2
38U
207Pb/
235U
(E)
26
30
22
18
14
10
Leucogranite, M22
N = 9
Figure 7. (A) Th versus U diagram for the analysed zircons from the Nielaxiongbo gneiss dome. (B and C) Concordia diagrams forthe zircon from the amphibolite (M13). (D and E) Concordia diagrams of zircon from the leucogranite (M22). For sample locations, seeFigure 2.
group with a mean 206Pb/238U age of 514 ± 6 millionyears, a mean 207Pb/235U age of 511 ± 6 million years,and a mean 207Pb/206Pb age of 503 ± 13 million years(Figure 7C). The chi-squared values for these ages are 1.2,2.0, and 2.2, respectively, indicating a small but significantscatter in the ages. The scatter suggests some geologicaldisturbance, consistent with the recrystallization of zirconsshown in the cathodoluminescence images (Figure 6A).The four grains with much younger ages (M13-8, -12, -15, -17) have very low Pb contents coupled with high Ucontents, suggesting some post-crystallization disturbanceof the U–Pb systematics.
Zircon grains from the leucogranite sample, M22(Table 1), show oscillatory zoning and are clearly magmaticin origin (Figure 6B). They have relatively low Th contentswith Th/U ratios of 0.18–0.01 (Figure 7A). When plottedon a concordia diagram (Figure 7D), one sample yielded adiscordant age with an upper intercept 206Pb/238U age of
470 ± 92 million years (Figure 7D). The other nine form asingle cluster on the diagram (Figure 7E), yielding a mean206Pb/238U age of 20.3 ± 1.9 million years (Figure 7E),which is considered to be the best estimate of the crystal-lization age for the leucogranite. The older grain is closein age to zircons from the basement amphibolite and isprobably a xenocryst captured during emplacement of theleucogranite.
5.2. 40Ar/39Ar analytical results
The 40Ar/39Ar data of muscovite and hornblende, cor-rected for interfering isotopes and mass discrimination, aresummarized in Table 2, and the apparent age spectra foreach sample are illustrated in Figure 8. All age errors arequoted at the 95% confidence level (2σ ). They includeerrors in the irradiation correction factors and the errorin the neutron fluence parameter but do not include the
Dow
nloa
ded
by [
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nstit
ute
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eoch
emis
try]
at 0
1:38
15
Mar
ch 2
012
624 D.-P. Yan et al.
Tabl
e2.
Res
ults
of40
Ar/
39A
rda
ting
ofth
ese
para
ted
mus
covi
tean
dam
phib
ole.
Sam
ple/
sepa
rate
T(◦
C)
39A
r(m
V)
39A
r(%
)A
ge(M
a)±
1σA
tm.c
ont.
(%)
37A
r/39
Ar
36A
r/40
Ar
39A
r/40
Ar
IIC
(%)
M1/
mus
covi
tea
600
14.8
0.4
8±
590
.70.
030.
0030
820.
0478
930.
1265
029
.80.
810
±3
87.7
00.
0029
770.
0485
380.
0270
043
.81.
27
±3
93.8
00.
0031
780.
0321
590.
0375
097
.22.
711
±1
74.9
00.
0025
40.
0873
490
775
169.
94.
712
±0
620
0.00
210.
1268
390
800
434.
212
.113
±0
340
0.00
1151
0.20
630
825
548.
615
.213
±0
14.9
00.
0005
070.
2650
730
850
427.
111
.913
±0
9.7
00.
0003
30.
2855
320
875
366.
610
.213
±0
11.2
00.
0003
80.
2814
210
900
258.
67.
212
±0
15.6
00.
0005
30.
2686
920
925
177.
34.
912
±0
15.7
00.
0005
350.
2709
030
950
151.
14.
212
±0
150
0.00
051
0.27
2986
097
514
2.6
3.9
12±
014
.20
0.00
0485
0.27
3949
010
0014
7.2
4.1
12±
013
.10
0.00
0446
0.27
7235
010
5027
1.6
7.5
13±
014
.10
0.00
0478
0.27
0901
011
0020
05.
513
±0
7.8
00.
0002
650.
2926
960
1250
60.2
1.6
12±
166
.60
0.00
2259
0.11
5017
014
5045
.51.
211
±2
84.4
00.
0028
630.
0583
950.
02M
7/m
usco
vite
b60
019
.60.
79
±3
75.5
0.08
0.00
2573
0.10
7679
0.29
650
311.
112
±2
61.7
0.06
0.00
2099
0.12
7233
0.17
700
39.4
1.4
10±
272
.20.
050.
0024
540.
1072
880.
1675
091
.23.
412
±0
54.4
0.02
0.00
1845
0.15
0456
0.06
775
246.
49.
212
±0
54.1
00.
0018
350.
1523
740.
0180
079
2.5
29.7
12±
035
00.
0011
870.
2084
660
825
386.
314
.512
±0
20.3
00.
0006
890.
2517
620
850
322.
112
.112
±0
20.1
00.
0006
810.
2534
220
875
222.
58.
312
±0
21.4
00.
0007
280.
2478
810
900
126.
64.
712
±0
26.8
00.
0009
110.
2365
70
925
74.9
2.8
12±
142
.90
0.00
1457
0.19
0072
0.01
950
52.8
1.9
12±
129
.20
0.00
0995
0.23
0051
0.02
975
47.6
1.7
12±
130
.80.
010.
0010
510.
2276
360.
0410
0048
.91.
812
±1
25.2
0.01
0.00
0859
0.23
7156
0.04
1050
68.7
2.5
12±
021
.90.
020.
0007
470.
2468
530.
0411
0051
.71.
913
±1
17.7
0.02
0.00
0606
0.25
7389
0.06
1250
29.4
1.1
13±
258
.20.
170.
0019
80.
1274
690.
414
508.
30.
30
±22
100.
40.
320.
0034
040.
0080
493.
89
Dow
nloa
ded
by [
Gua
ngzh
ou I
nstit
ute
of G
eoch
emis
try]
at 0
1:38
15
Mar
ch 2
012
International Geology Review 625
M12
B/m
usco
vite
c60
05.
70.
217
±32
96.8
0.16
0.00
3281
0.00
7244
0.29
650
8.7
0.3
5±
3599
.40.
030.
0033
680.
0039
430.
2270
021
.30.
90
±23
103.
20.
010.
0034
950.
0039
170
750
151.
56.
410
±1
84.8
00.
0028
720.
0584
880
775
411.
517
.512
±0
33.4
00.
0011
340.
2097
560
800
332.
414
.113
±0
8.9
00.
0003
030.
2854
570
825
332.
514
.113
±0
5.9
00.
0002
010.
2943
390
850
284.
812
.113
±0
50
0.00
017
0.29
6349
087
523
4.4
1013
±0
4.5
00.
0001
540.
2982
250
900
145.
46.
213
±0
9.6
00.
0003
260.
2824
620
925
83.5
3.5
13±
09.
20
0.00
0313
0.28
5742
095
056
2.3
13±
010
.50
0.00
036
0.28
1104
097
548
.62
12±
111
.10
0.00
038
0.28
245
010
0046
.51.
912
±1
11.5
00.
0003
940.
2827
960
1050
803.
412
±0
18.2
00.
0006
210.
2611
850
1100
76.1
3.2
13±
014
.20
0.00
0484
0.26
6207
012
5021
.10.
911
±3
78.6
00.
0026
720.
0796
850.
0114
503.
20.
10
±90
100.
60.
120.
0034
090.
0040
340.
59M
4/m
usco
vite
d65
04.
40.
843
±40
91.1
5.95
0.00
3091
0.00
8238
4.52
750
5.5
10
±24
102.
511
.02
0.00
348
0.01
3081
41.6
985
08.
81.
77
±13
96.7
15.1
50.
0032
830.
0179
4663
.990
010
.62
5±
895
16.1
60.
0032
360.
0383
4495
.88
950
7.5
1.4
7±
1192
.818
.81
0.00
3168
0.03
6481
73.9
897
517
.23.
311
±4
79.8
17.0
80.
0027
360.
0708
4646
.83
1000
44.6
8.7
15±
160
.117
.11
0.00
2073
0.10
3935
.13
1025
39.6
7.7
15±
152
.317
.93
0.00
1844
0.12
4987
37.5
210
507.
41.
412
±6
65.8
18.6
90.
0023
780.
1058
7547
.17
1075
12.8
2.4
13±
464
.718
.54
0.00
229
0.10
2652
43.3
611
0040
.97.
915
±2
54.8
17.9
70.
0019
170.
1173
4937
.13
1125
102
19.8
15±
053
.117
.78
0.00
183
0.12
5074
37.2
711
5087
.517
16±
144
.117
.52
0.00
1549
0.13
9233
34.6
311
7575
.214
.616
±1
38.6
16.7
90.
0013
860.
1496
4232
.71
1250
42.5
8.3
16±
149
.515
.95
0.00
1741
0.12
2174
30.7
413
502.
70.
558
±52
86.2
14.4
70.
0029
310.
0095
78.
4514
503
0.5
0±
103
100.
97.
250.
0034
220.
0032
5817
.42
Not
es:37
Ar/
39A
r,36
Ar/
40A
r,an
d39
Ar/
40A
rar
eco
rrec
ted
for
mas
ssp
ectr
omet
er.
IIC
(%),
inte
rfer
ing
isot
opes
corr
ecti
on.
a Tot
alga
sag
e=
12.8
±0.
2m
illi
onye
ars;
mea
nag
e(7
75–1
250◦
C)=
13±
0.1
mil
lion
year
s(2
σun
cert
aint
y);J
=0.
0023
±0.
0000
23.
bTo
talg
asag
e=
12.7
±0.
2m
illi
onye
ars;
mea
nag
e(7
50–1
250◦
C)=
13±
0.2
mil
lion
year
s(2
σun
cert
aint
y);J
=0.
0022
79±
2.27
9E–0
5.c T
otal
gas
age=
12.8
±0.
4m
illi
onye
ars;
mea
nag
e(7
75–1
100◦
C)=
13.5
±0.
2m
illi
onye
ars
(2σ
unce
rtai
nty)
;J=
0.00
2279
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20(A) (B)
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Figure 8. Age and 37Ar/39Ar spectra for muscovite and amphibole from the Nielaxiongbo gneiss dome. (A) M1 muscovite; (B) M7 mus-covite; (C) M12B muscovite; and (D) M4 amphibole. Half-heights of open rectangles indicate the 1σ relative (between-step) uncertainties.Plateau ages (with 2σ uncertainties) are indicated. For sample locations, see Figure 2.
Figure 9. Geological section A–B through the Bhutan Himalayas and Nielaxiongbo gneiss domes. The geology is based on the geologicalmap of Bhutan, INDEPTH geophysical data, Lee et al. (2000), BGMRXAR (1993), and our observations. The topography is from SRTM90 DEM data. The arrows indicate the flow direction of the middle crust ductilely deformed channel. For section locations, see Figure 1.Imposed on both sections are the contours, which indicate resistivity contours, after Unsworth et al. (2005, Figure 3). We suggest that thehigher contours may correspond to the active channel. The concentric dashed lines on the right-hand side indicate isotherms. The contoursin the eastern region are dashed because of the distance to the INDEPTH line (it has been shown that the resistivity varies along theorogen). MCT, Main Central thrust; YZS, Yarlung Zangbo Suture; MBT, Main Boundary Thrust; MFT, Main Frontal Thrust; MHT, MainHimalayan Thrust; KT, Kakhtang Thrust; STDS, South Tibetan Detachment; LHS, Lesser Himalayan Sequence; GHS, Greater HimalayanSequence; SK, Sakteng Klippe (remnants of the Tibetan sedimentary sequence soled by the STD); GBt, Gangdese Batholith; ILC, IndiaLithospheric Continent; IML, India Mantle Lithosphere.
uncertainty in the potassium decay constants. In this arti-cle, a plateau is defined as a sequence of three or moreconsecutive steps that are mutually indistinguishable at 1σ
and encompass at least 50% of the total 39Ar released.All three muscovite samples (M1 from leucogranite,
M12B from pegmatitic adamellite, and M7 from garnet-mica schist) (Table 2) yielded well-defined plateau agesat 13.0 ± 0.1, 13.5 ± 0.2, and 13.0 ± 0.2 million years,respectively (Figure 8). The hornblende sample from themiddle crustal layer (M4) also yielded a well-definedplateau age of 18 ± 0.3 million years.
6. Discussion
There are several major domes in South Tibet, includ-ing the Kangmar, Kampa, Mabja, and Malashan domes(Chen et al. 1990; Lee et al. 2004; Aoya et al. 2006;
Quigley et al. 2006), with the Nielaxiongbo dome beingthe easternmost one. These domes all have a similar struc-ture and are composed of a basement complex, a middlecrustal layer, and a sedimentary cover sequence, each unitbeing separated from one another by detachment faults.The Nielaxiongbo dome has ductilely deformed layer andabundant leucogranites, both of which may shed light on amiddle crustal ductile flow underneath the Tibetan Plateau.In particular, knowledge on the mechanism and timing ofuplift of the basement may provide important constraintson the evolution of such ductile flow.
6.1. Nature of the basement complex
The basement complex in the Nielaxiongbo gneiss domeconsists of amphibolites and granitic gneisses. Zirconsfrom an amphibolite (sample M13) yielded an average
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SHRIMP age of ∼514 million years. However, four grainsfrom this sample have much younger zircon ages of 47, 49,159, and 327 million years (Table 1), suggesting successivethermal disturbance. The youngest ages (47–49 millionyears) coincide approximately with the early stages of col-lision between the Indian and Eurasian plates (Himalayanorogeny) (Yin and Harrison, 2001; Thanh et al. 2010).
The early Palaeozoic age of the basement complex inthe Nielaxiongbo gneiss dome is similar to the ages of thegneiss from the Kangmar dome, which has a U–Pb zir-con age of 560 ± 4 million years (Scharer et al. 1986)and an Rb–Sr isochron age of 485 ± 6 million years(BGMRXAR 1993). Lee et al. (2000) reported similar U–Pb zircon ages of 508 million years for two orthogneissesin the Kangmar dome. Liu et al. (2006) also obtainedSHRIMP zircon U–Pb ages of 513 ± 10 and 502 ± 9million years for the Tanggaximu and Tongbashi plutons,respectively, both intruding basement rocks in the Yadongarea (Figure 1). The similar ages obtained from widely dis-tributed rocks indicate the existence of a common basementbeneath South Tibet.
We interpret these dates as marking the age of meta-morphism and magmatism in the basement rocks, sug-gesting consolidation of the basement during the earlyPalaeozoic. Thus, metamorphism and magmatism in theSouth Tibet basement rocks are thought to be related tothe Pan-African orogeny (Valdiya 1997; Liu et al. 2006),indicating an affinity with the Indian plate.
6.2. Exhumation of the basement complex associatedwith Neogene extension
In the Nielaxiongbo dome, E–W-striking deformationalfeatures, such as brittle thrust planes, the strike of type 1Cor 2 fold axial planes, and fan-shaped spaced crenulationcleavages fans (S1 foliation) (Figures 2, 3, and 4A), docu-ment early crustal shortening and thickening (D1). Previousstudies have dated the onset of crustal thickening at ∼50Ma; understanding in this process, however, remains lim-ited (Rowley 1998; Yin and Harrison 2001; Green et al.2008).
Ductile deformation (D2) produced foliation S2 andmineral lineation L2, S-C fabrics, press shadows withintrafolial folds, shear bands, and splitting of biotite por-phyroblasts (Figures 2, 4, and 5B), indicating top-to-the-north shear sense in the middle ductile crustal layer andshallower tectonic levels. In contrast, the basement com-plex, similar to that in the GHS, has features showingtop-to-the-south sense of shear.
Our 40Ar/39Ar ages obtained from the basement com-plex at Nielaxiongbo range from 18 ± 0.3 million yearsfor amphibole to 13.0 ± 0.2 million years for mus-covite (Figure 8). These ages suggest a cooling rate of30 ± 10◦C/million years through approximately 500◦C
to 350◦C (argon closure temperatures in amphibole andmuscovite, respectively), associated with exhumation of thebasement rocks. Based on K–Ar and 40Ar/39Ar apparentages, exhumation of the basement complex in Kangmaroccurred between 12.5 and 19 Ma (Debon et al. 1985),∼13 Ma (Chen et al. 1990), or 22 Ma (Liu 1984). Amore detailed 40Ar/39Ar thermochronological study of theKangmar dome yielded muscovite cooling ages of 15.24 ±0.05–12.23 ± 0.03 million years and biotite cooling agesof 17.04 ± 0.04–10.94 ± 0.03 million years (Lee et al.2000). The basement ages in Kangmar increase with depthand young northwards within a single structural level. NewU/Pb zircon ages from deformed migmatites and unde-formed granite in the core of the Mabja dome suggest thatextension, synchronous with peak metamorphism, beganat 35.0 ± 0.8 Ma, was ongoing at 23.1 ± 0.8 Ma andceased at 16.2 0.4 Ma (Lee et al. 2004, 2006; Lee andWhitehouse 2007). The young age corresponds with thetime of exhumation of the Himalayan metamorphic belt,which is dated at 16.8 Ma (Liu 1984). Thus, our new struc-tural and geochronological data from Nielaxiongbo andother works from Kangmar dome suggest that the ductiledeformation in the region began at or before ∼35 Ma in adeep tectonic level, resulting in southward ductile flow atthe mid-crustal tectonic level that continued from ∼23 Mato 13 Ma.
In the Nielaxiongbo gneiss dome, later brittle-ductiledeformation (D3) is characterized by spaced cleavage S3
and mineral lineation L3 (Figures 4A and 5B). These fab-rics are concentric to the leucogranite pluton, indicatingthat they were produced by intrusion of the leucogranite.The S3 foliation cuts the lower, but not the upper detach-ment, indicating that the lower detachment pre-dated theleucogranite intrusion.
These deformational features and their ages suggestthat development of D3 and intrusion of the leucogran-ites occurred immediately after, or partly synchronouswith, the north-directed ductile and brittle-ductile deforma-tion of the Tibetan sedimentary sequence and the south-ward ductile flow of the basement complex (GHS), whichformed D2. The metamorphic rocks of the dome, whichdecrease in metamorphic grade upward from migmatiteto kyanite + sillimanite + K-feldspar, to staurolite and gar-net + biotite assemblages, are similar to those at the top ofthe GHS (Waters et al. 2006).
6.3. Implications of silicic magmatism for themid-crustal ductile channel flow model
Leucogranites within the Nielaxiongbo gneiss dome havea zircon U–Pb age of ∼20 million years (M22 in Quzenadamellite), and muscovite, which develops along D2 fab-rics, has 40Ar/39Ar ages of 13 and 13.5 million years. Thisindicates that the leucogranites were emplaced at ∼20 Ma
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and cooled to ∼350◦C at 13.4–13 Ma. Thus, unroof-ing and cooling of the gneiss dome, which was triggeredby intrusion of the leucogranite, would have occurredslightly later than, or partly overlap with, the develop-ment of D2. The 40Ar/39Ar dates of ∼13 Ma constrainthe timing of top-to-the-north movement along the upperdetachment.
A deformed leucocratic dike swarm in the Mabja domeyielded a zircon U–Pb age of 23.1 + 0.8 million years,whereas a post-tectonic two-mica granite in the same bodyyielded a zircon U–Pb age of 14.2 + 0.2 million years and amonazite U–Pb age of 14.5 + 0.1 million years. The old ageis interpreted as the ongoing age for middle crustal ductileextension in the North Himalayan gneiss domes, whereasthe younger ages indicate that ductile deformation ceasedin the middle Miocene (Lee et al. 2006). The younger agesare similar to an age of 14.4 + 0.1 million years reportedby Zhang et al. (2004). It is concluded that emplacement ofthe leucogranite post-dated initiation of the D2 mid-crustalductile flow, indicating that the ductile flow triggered theintrusion of the leucogranite.
It is widely accepted that exhumation of the basementcomplexes in South Tibet was associated with extensionaltectonics and emplacement of granitic magmas (Maluski etal. 1988; Guillot et al. 1995; Harrison et al. 1997; Searleet al. 1997; Li et al. 2003). It is also generally acceptedthat these magmas formed by melting of crustal materi-als (Harris et al. 2004; Zhang et al. 2004). Leucogranites,which are widely distributed in the GHS and gneiss domes,have similar ages between ∼23 and ∼13 million yearsthroughout the region (Searle and Godin 2003; Godin etal. 2006; Quigley et al. 2006). Our SHRIMP U–Pb zir-con age of ∼20 million years for the leucogranite inNielaxiongbo is consistent within analytical errors with our40Ar/39Ar amphibole age for the local amphibolite, sug-gesting that exhumation of the Nielaxiongbo gneiss domewas associated with silicic plutonic activity.
The ductile deformation of the basement complex andthe middle crustal layer within the Nielaxiongbo, Kangmar,Kampa, Mabja, and Malashan domes, as well as similarbodies elsewhere in South Tibet and the Greater Himalayas,took place at mid-crustal levels between 24 and 12 mil-lion years and is probably partly a result of the ductilechannel flow in South Tibet (Chen et al. 1990; Edwardset al. 1996; Grujic et al. 1996, 2002; Hodges 2000, 2006;Beaumont et al. 2001, 2004, 2006; Li et al. 2003; Searleand Godin 2003; Godin et al. 2006; Yin 2006; Zhang et al.2007; Bai et al. 2010; Langille et al. 2010). The leucogran-ites could have been produced by melting of high-grademetamorphic basement rocks within the thickened crust(Le Fort et al. 1987; Inger and Harris 1993; Guillot andLe Fort 1995; Harris et al. 2004). The presence of par-tial melts (migmatites) or granitic magmas would havelubricated the boundaries of the ductile channel within themiddle crust, which may be represented by the extruded
palaeochannel of the Greater Himalayas (Grujic et al. 1996,2002; Beaumont et al. 2001, 2004, 2006; Godin et al. 2006;Hodges 2006). The metamorphic grade decreases upwardin both the gneiss domes and the GHS (Waters et al. 2006);a kinematic transition exists in South Tibet (Aoya et al.2005, 2006); and a kinematic inversion occurs elsewherein the GHS (Grujic et al. 1996). All of these features arecompatible with southward and upward extrusion of themid-crustal ductile channel flow.
6.4. An integrated model for the mid-crustal ductilechannel flow in South Tibet
Evidence for important normal faulting exists on the north-ern side of the Greater Himalayas (Burg and Chen 1984;Burchfiel et al. 1992; Edwards et al. 1996; Edwards andHarrison 1997; Wu et al. 1998), and the Kangmar dome hasbeen related to the same extensional event that producedthe STDS. The STDS and the gneiss domes in southernTibet suggest that shortening and extension were contem-poraneous at different tectonic levels within the Himalayanand South Tibetan crust (Chen et al. 1990; Burchfiel etal. 1992; Hodges et al. 1992, 1993). However, the extru-sion and channel flow hypothesis implies that the normalfaulting of the STDS resulted from southward flow andextrusion of the Greater Himalayas beneath the Tibetansedimentary sequence. The finite-element thermal mechan-ical model of Beaumont et al. (2001, 2004, 2006) andJamieson et al. (2002, 2004, 2006) provided test for thishypothesis, concluding that the formation of the NorthHimalayan gneiss domes was a response to flow dynam-ics in the weak mid-crustal channel rather than regionaltectonic extension or gravitational collapse of the TibetanPlateau. Relative N–S extension may have occurred inthe upper crust but is caused by shear stresses along theupper boundary of the southward-flowing middle crustalchannel (Beaumont et al. 2001, 2004). In addition, geo-dynamic models suggest that squeezing of the channelabove a crustal ramp can destabilize the upper crustaloverburden, facilitating the formation of a dome. Haucket al. (1998) and Yin (2006) have suggested that theNorth Himalayan domes are actually culminations alongthe North Himalayan antiform, which could be above aramp in the Main Himalayan Thrust.
The deformation and metamorphic gradients in theNielaxiongbo dome are most likely related to southwardand upward extrusion of the GHS. Although both themiddle crustal layer and the cover sequence have a north-ward kinematic sense, the contrast of deformational styleand metamorphic grade indicates a southward extrusionof the ductilely deformed middle crustal layer (the GHS)related to N–S extension of the cover sequence (Figure5B). Therefore, both the metamorphic gradient and theductile deformation are consistent with the tectonic modelinvolving southward extrusion between the MCT and the
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STDS (Grujic et al. 1996, 2002, 2006; Beaumont et al.2001, 2004, 2006; Godin et al. 2006).
Thus, we propose that the southward and locallyupward extrusion of the ductile channel flow in the middlecrust in South Tibet was responsible for the formation andexhumation of the gneiss domes in South Tibet (Figure 9).
The ductile channel flow in South Tibet occurs in themiddle crust where it includes at least amphibolite-faciesmetamorphic rocks plus migmatite and magmas producedby partial melting of the metamorphic rocks (Figure 9).Southward flow (D2) in this channel might have startedbetween the STDS and the MCT at ∼20 Ma or even ear-lier at 24–26 Ma (e.g. Godin et al. 2006; Hodges 2006; Leeand Whitehouse 2007), resulting in north-directed shear-ing along the STDS at shallow levels. The consequentemplacement of leucogranitic magmas (D3), which lubri-cated the boundary of the ductile channel flow, formedthe domes (Figure 9). Exhumation of the complex led tocooling through 500◦C and 300◦C between ca. 18 Ma and13 Ma and formed ductile deformation fabrics similar tothose in the Greater Himalayas (Hodges 2000). We suggestthat the upward movement of the ductile channel mighthave been due to continuous N–S shortening in the mid-dle and lower crusts of southern Tibet (Figures 1 and 9).Therefore, the extensional thinning of the upper crust ofthe Tibetan Plateau is marked by the doming and uplift ofductile channel in the STDS.
7. Conclusions
The Nielaxiongbo gneiss dome is composed of a GreaterHimalayan basement, a middle ductilely deformed crustallayer, and a sedimentary cover sequence, all separatedby detachment faults. Both the basement complex andthe middle crustal layer were intruded by leucogranites.The south-directed ductile deformation and associatedhigh-grade metamorphism, partial melting, and top-to-the-north shearing along the two strands of the STDSdefine mid-crust ductile channel flow. The basement rockswere exhumed during the Miocene involving temperaturesbetween approximately 500◦C and 350◦C at 18–13 Ma.Doming of the weak mid-crustal channel flow was probablyinitiated by the silicic plutonism at ∼20 Ma and associatedthinning of the upper crust of southern Tibet, which wascaused by the southward mid-crustal ductile channel flow.
AcknowledgementsThis study was supported by research grants from the NationalBasic Research Programme of China (2009CB421001), NationalScience Foundation of China (40872140, 40921062), the 111Project (B07011), and the National Science and EngineeringResearch Council of Canada. We are grateful to the geologicalteam of the Tibetan Geological Survey for assistance in the field,and we thank Keith Taylor for technical assistance in the ArgonIsotope Laboratory at Dalhousie University.
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