multiple tectonometamorphic imprints in the lower crust: first evidence of ca. 950 ma (zircon u-pb...
TRANSCRIPT
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Multiple tectonometamorphic imprints in the lower crust: rst evidenceof ca. 950Ma (zircon U-Pb SHRIMP) compressional reworking of UHT
aluminous granulites from the Eastern Ghats Belt, India
KAUSHIK DAS 1*, SANKAR BOSE 2, SUBRATA KARMAKAR 3,DANIEL J. DUNKLEY 4 and SOMNATH DASGUPTA5
1Department of Geology, Bengal Engineering and Science University, Howrah, India2Department of Geology, Presidency College, Kolkata, India
3Department of Geological Sciences, Jadavpur University, Kolkata, India4National Institute of Polar Research, Tokyo, Japan
5Indian Institute of Science Education and Research, Kolkata, India
Integrated structural, petrological and geochronological study on a suite of granulites from the central part of the Eastern Ghats Belt (EGB),India unveils polyphase tectonothermal evolution. We document (a) M1 ultrahigh temperature (UHT) metamorphism (10008C at6.58.5 kbar) on an anticlockwise PT trajectory simultaneously with early deformations D1D2 involving partial melting, (b) coolingdown to 8008C, 6 kbar that produced a variety of coronae/symplectites (M1R), (c) an unrelated compressional orogeny (D3) that produceddeep crustal shears and mylonitic foliation (S3m) at low angles to D1D2 structures and was associated with slight loading, and possible partialmelt extraction under granulite facies condition (M2 7 kbar, 8508C), and (d) localized retrogression (M3) in the presence of meltaccompanying D4 deformation. This is the rst record of the prograde PT path of the superimposed granulite facies metamorphism in theEGB. U-Pb SHRIMP data of zircon preserves an inherited grain domain of ca. 1700Ma (207Pb-206Pb age) that traces back the history of EGBwith a lineage of the Mesoproterozoic supercontinent, Columbia. The UHT metamorphosed (peakM1 at ca. 1000Ma) and subsequentlycooled crustal segment (M1R) was subjected to strong tectonothermal reworking (M2) along a clockwise PT path at 953 6Ma (concordiaage) that partially exhumed the rocks to mid-crustal levels. A later uid-induced retrogressive event vis-a`-vismelt crystallization occurred atca. 900Ma (207Pb-206Pb age). The post-peak evolution reveals striking similarities with those recorded in the rocks of the Rayner Complex ofeast Antarctica, thereby strengthening the notion of Indo-Antarctic correlation as part of Rodinia. Copyright# 2010 JohnWiley & Sons, Ltd.
Received 27 November 2009; accepted 29 March 2010
KEY WORDS deep crustal reworking; Eastern Ghats Belt; India; UHT aluminous granulites; zircon U-Pb SHRIMP ages
Supporting information (supplementary tables S2-S6) may be found in the online version of this paper.
1. INTRODUCTION
Many of the ultrahigh temperature (UHT, > 9008C, Harley,1998; Kelsey, 2008) metamorphosed terrains record a nearly
isobaric cooling retrograde PT trajectory (reviewed in
Harley, 1989, 1998, 2004; see also Santosh et al., 2007;
Santosh and Kusky, 2010; Liu et al., 2011). Two prominent
examples include the Archaean Napier Complex in east
Antarctica (Harley and Hensen, 1990; Harley, 2003) and the
Proterozoic Eastern Ghats Belt in India (Dasgupta and
Sengupta, 2003). Exhumation of these isobarically cooled
terranes occurred in response to unrelated later orogenic
events. In case of the Napier Complex, the Rayner orogeny
of broadly ca. 940910Ma age reworked the early
granulites, records of which are found in marginal shear
zones (Harley and Hensen, 1990; Kelly et al., 2000,
references therein). Limited radiometric dates on the Eastern
Ghats rocks show overprinting by ca. 1000950Ma orogeny
on the early UHT granulites during a second granulite
facies metamorphism characterized by near isothermal
decompression during retrogression (Grew and Manton,
1986; Shaw et al., 1997; Mezger and Cosca, 1999;
Dasgupta et al., 1994, 1995; Dasgupta and Sengupta,
2003). However, the prograde path of the second granulite
GEOLOGICAL JOURNAL
Geol. J. 46: 217239 (2011)
Published online 24 June 2010 in Wiley Online Library
(wileyonlinelibrary.com) DOI: 10.1002/gj.1246
*Correspondence to: K. Das, Department of Geology, Bengal Engineeringand Science University, Howrah 711103, India.E-mail: [email protected]
Copyright # 2010 John Wiley & Sons, Ltd.
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facies metamorphism in the Eastern Ghats and the nature of
deformation associated with re-working of granulites remain
undetermined. Knowledge on these aspects is a pre-requisite
in understanding the way the isobarically cooled lower crust
reacted in response to the later orogeny.
Recent studies reveal that the Eastern Ghats Belt (EGB) is
a collage of discrete crustal provinces with characteristic
petrological, structural and isotopic histories (Rickers et al.,
2001; Dobmeier and Raith, 2003; Bose and Das, 2007;
Chetty, in press). The present study is concentrated in the
central part of the Eastern Ghats Province (Dobmeier and
Raith, 2003) or Domain 2 (Rickers et al., 2001), where
metamorphic, magmatic and isotopic signatures are well
constrained (reviewed in Dasgupta and Sengupta, 2003;
Shaw et al., 1997; Mezger and Cosca, 1999; Simmat and
Raith, 2008, Bose et al., 2008). We present structural,
petrological and geochronological data on aluminous
granulites to constrain multiple structural and metamorphic
events. Our particular emphasis here is to characterize the
structural and petrological reworking of the early UHT
granulites of this belt.
2. GEOLOGICAL BACKGROUND
The EGB represents a Proterozoic orogenic belt that extends
over 1000 km from the Brahmani river valley in Orissa to
southeastern parts of Andhra Pradesh along the eastern coast
of the Indian peninsula (Figure 1). The tectonometamorphic
events in this regional terrain are distinct from those in the
Figure 1. Geological map of the study area (Panirangini) and adjoining areas. Note the isolated occurrences of aluminous granulites within leptynite andenderbite. The inset map shows the location of the study area (Panirangini) in the broad geological framework of the Eastern Ghats Belt of India.
Copyright # 2010 John Wiley & Sons, Ltd. Geol. J. 46: 217239 (2011)
218 k. das ET AL.
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surrounding cratonic zones and at the same time, there are
differences in evolutionary histories in different domains
inside the belt ranging in age from at least Meso- to
Neoproterozoic time. With all the complexity in the growth
history, this belt stands out to be crucial for reconstruction of
Proterozoic East Gondwana (Yoshida, 1995). Moreover,
recent studies have shown that the EGB preserves the
evidence for regional-scale anomalous extreme thermal
condition of metamorphism in excess of 10008C at lowercrustal pressure of 810 kbar (Dasgupta and Sengupta, 2003;
Harley, 2003). Such extreme metamorphic conditions are
inferred from reaction textures in diverse mineral assem-
blages of aluminous granulites and calc silicate granulites
exposed in different parts of this terrain (Bhowmik et al.,
1995; Bose et al., 2006, references therein).
The present study area is near Panirangini (N1881826, E8285428) in the Araku Valley in the Visakhapatnamdistrict of Andhra Pradesh, India (Figure 1). The major
lithological units in Panirangini and its adjoining
area are khondalite (garnet-sillimanite-quartz-perthite gneiss),
leptynite (plagioclase-garnet-perthite-quartz gneiss), enderbite
(orthopyroxene-plagioclase-perthite-quartz garnet gneiss),mac granulite (orthopyroxene-clinopyroxene-plagioclase-
garnet gneiss), calc-silicate granulite (scapolite-wollastonite-
garnet-plagioclase-quartz gneiss) and aluminous granulite
(sapphirine-cordierite-spinel-garnet-orthopyroxene-quartz-silli-
manite gneiss). The major part of the area is dominated by
khondalite. The unit is conformable with the associated
enderbite and leptynite. Aluminous granulite occurs as small
pods within leptynite and enderbite. Mac granulite occurs as
thick bands and/or lenses within leptynite, calc-silicate granulite
and enderbite. The gneissic foliation in leptynite is demarcated
by alternating garnet-biotite rich and quartzofeldspathic layers.
The general trend of this foliation is NNE that has been
deformed by later events (discussed later) giving rise to regional-
scale fold interference (Figure 2). The aluminous granulite near
Panirangini occurs as small podswithin sheared leptynitic gneiss
and shows two structural variations, (1)massive and the other (2)
foliated. The foliated variety shows alternating layers of quartzo-
feldspathic and mac-rich (orthopyroxene garnet) domain.This gneissic foliation in aluminous granulite and the associated
leptynitic gneiss is subvertical. Centimetre-thick quartz veins
show down-dip stretching lineation (rodding) on the foliation
plane. The massive variety is coarse-grained containing
orthopyroxene cordierite aggregate and occurs in the sameoutcrop as the foliated type. Two generations of quartzo-
feldspathic veins occur within the leptynitic gneiss and those lie
at low angle to the general foliation. Foliation-parallel elongated
Figure 2. Strike map of major foliation planes in the study area showing regional folding and other variation in different places. Note the presence of shear zoneand associated foliation near the study area.
Copyright # 2010 John Wiley & Sons, Ltd. Geol. J. 46: 217239 (2011)
multiple tectonometamorphic imprints in the lower crust, egb, india 219
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bodies of mac granulite occur within leptynite close to the
aluminous granulite exposed at Panirangini.
3. STRUCTURAL RELATIONSHIPS
The rocks of the study area were affected by four episodes of
deformation. Superposed deformation and concomitant
metamorphic imprints have also been identied from the
nearby Borra Caves area (Bhowmik, 1997). The earliest
recognizable planar fabric in mesoscopic scale is identied
in khondalite and leptynite. This fabric is dened by layers
of ferromagnesian minerals and quartz-feldspar that could
represent modied compositional banding or a transposed
gneissic fabric on compositional banding during the
earliest D1 deformation and is termed henceforth as S1.
3.1. D2 deformation
D2 caused transposition of S1 and parallelism of S2 that is the
dominant form surface in the area. Due to intense later
deformations, folds produced on S1 are rarely preserved as
rootless, isoclinal to tight intrafolial folds (F2) (Figure 3a)
in local low-strain domains. The dominant transposed S2gneissic fabric is dened by alternating ferromagnesian
Figure 3. (a) Rootless, isoclinal, intrafolial folds (F1) on compositional banding (S1) in quartzo-feldspathic gneiss. Note the feature in the centre of the photobelow the pencil. (b) Upright, plunging fold on gneissic fabric in quartzo-feldspathic gneiss. The black arrow shows the folded limb on plan, while the whitearrow is that on the transverse surface. (c) Microscopic fractures developed during D4 that healed up with biotite. (d) Crystal plastic deformation is evident inleptynites and aluminous granulites, undulose extinction in quartz and deformation twin lamellae in alkali feldspar (Kfs) clasts. (e) Porphyroblastic garnet (Grt)containing inclusion of biotite (Bt) and quartz (Qtz) in Association A. This garnet is overgrown by a dusty intergrowth of garnet, sillimanite and quartz(Grt SilQtz). (f) Spinel (Spl) and quartz (Qtz) inclusions in coarse garnet (Grt) that is also overgrown by the intergrowth of garnet, sillimanite, quartz and/orbiotite (GrtSilQtzBt). (g) A complex intergrowth of garnet (Grt), spinel (Spl) and ilmenite (Ilm) growing at the fringe of porphyroblastic garnet (Grt)associated with matrix quartz (Qtz). Note the presence of biotite (Bt) patches along the fractures of garnet. (h) BSE image showing a spongy intergrowth of
garnet (Grt), quartz (Qtz) and sillimanite (Sil) on cordierite (Crd).
Copyright # 2010 John Wiley & Sons, Ltd. Geol. J. 46: 217239 (2011)
220 k. das ET AL.
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(garnetiferous in favourable compositional bands) and
quartzo-feldspathic layers.
3.2. D3 deformation
D3 deformation formed small-scale shear zones accom-
panying regional-scale folding F3 on the dominant form
surface S2. F3 folds are NESW trending open, upright,
gently plunging on S2 and are pervasive to all the lithological
units of the area on regional- (Figure 2) and on mesoscopic-
scale (Figure 3b). Repetition of transposition produced a
composite S2/S3 gneissic fabric during this event. The S3 is
only identied at the low-strain zone, i.e. hinges of small-
scale parasitic folds of F3. Garnetiferous leucocratic layers,
presumably produced by partial melting (discussed later),
participated in F3 folding. D3 therefore postdates partial
melting. The geometries of F2 and F3 folds indicate that the
fold axes are at acute angles.
Localization of shear bands is conspicuous in leptynite that
overprints the dominant S2 gneissosity. Shearing produced a
CS fabric in this rock where C-surfaces (trending NESW)
are at acute angles with the pervasive S2 fabric showing a
sinistral sense on horizontal section. Apart from C-surfaces,
subsidiary shear bands develop at an angle that affects the
rock and drags the gneissic foliation resulting in small folds.
The F3 fold axes, developed on the transposed S2 with S3, are
accentuated producing sheath folds and are identied as eyed
folds on outcrop. Locally, a steeply dipping (608 westerly tosubvertical) mylonitic foliation (S3m) striking NESW is
developed in leptynite (Figure 2). The exposed foliation
planes have down-dip stretching lineation. The geometry of
folds and shear zone features illustrate bulk compression
along SENW that produced the F3 folds and small-scale
deep crustal compressional shearing. The horizontal com-
ponent of the oblique down-dip shear stress shows a sinistral
sense, i.e. the eastern part moved northeasterly and western
part moved southwesterly. Such deep crustal compressional
local shear planes characteristically have a steep dip (Ramsay,
1979).
3.3. D4 deformation
D4 deformation produced cross folding (F4) on F3 axial trace
(Figure 2). Regionally F3 folds are intersected by a NWSE
trending folds of the last deformation. The superposition
gave rise to non-plane folding and domal structure. D4 is
evident by the presence of microscopic to small-scale
fractures, healed up with biotite (Figure 3c).
4. TEXTURES AND MICROSTRUCTURES
The studied aluminous granulites have three distinct mineral
associations that developed in closely spaced domains in
outcrop scale. The mineral assemblages, key micro-structural
and textural features, mineralogical evolution with defor-
mation vis-a`-vis metamorphic events and brief mineral
chemical characteristics are summarized in Table 1.
Association A contains garnet porphyroblasts set in a ner
quartzo-feldspathic matrix. The association B is distinctly
migmatitic with alternating light and dark layers forming
composite S2/S3 gneissic fabric and a mylonitic foliation
(S3m). Evidences of crystal plastic deformation on a micro-
scale are widely preserved in this sheared variety of
aluminous granulite (Figure 3d). The association C is
developed as massive domains within the aluminous
granulite. Mineral abbreviations are after Kretz (1983).
Subscripts with minerals refer to both the mineral association
and sequence of development in each association.
In association A, garnet porphyroblasts (GrtA1) contain
inclusions of biotite (BtA1) (Figure 3e), spinel (SplA1),
quartz (Figure 3f) and ilmenite. It (GrtA2) occasionally
forms intergrowth with spinel (SplA2) and ilmenite (IlmA2)
(Figure 3g) sapphirine. Layers of GrtA1 in Association Ashow ductile deformation forming pinch-and-swell and
boudinage structure. Cordierite (Crd) is replaced by a
spongy symplectic intergrowth of garnet (GrtA3), quartz and
sillimanite (SilA3) along grain boundaries (Figure 3h). At
places, this symplectite overgrows GrtA1. This intergrown
assemblage after cordierite is possibly developed during the
high-strain event producing S3m fabric (D3).
The gneissic foliation in association B developed
during D1D2 and is characterized by quartz-perthite-
plagioclase-bearing leucosomes alternating with dark layers
comprising porphyroblastic orthopyroxene (OpxB1),
cordierite, spinel-magnetite solid solution (SplB1), quartz,
plagioclase, ilmenite and minor prismatic sillimanite (SilB1).
OpxB1, SplB1 and Crd grains are extremely stretched and
attened parallel to the foliation. Porphyroblastic OpxB1commonly shows pinch and swell and en-echelon micro-
structures. The features suggest that this assemblage
containing OpxB1 was stabilized prior to D3. The mylonitic
fabric (S3m), represented by ribbon quartz, is preserved in
high-strain areas wrapping local low-strain domains.
Dynamic recrystallization by grain boundary migration
(GBM) is shown by quartz and feldspar in quartzo-
feldspathic microdomains and also in OpxB1 and cordierite
grains (Figures 4a and b). Perthite occurs as asymmetric
grains with strings of intergrowth and quartz ribbons
sweep around these porphyroblasts resembling CS fabric
(Figure 4a) while plagioclase grains show bent twin
lamellae. Asymmetric mantle structure is shown by
recrystallized orthopyroxene grains around porphyroclasts
of the same OpxB1 (Figure 4c). OpxB1 often forms
aggregates and contains lamellae of spinel (SplB2) and
cordierite along the same crystallographic plane (Figure 4d).
OpxB1 also contains lamellae of garnet (GrtB2) along the
same crystallographic direction along with globules of
Copyright # 2010 John Wiley & Sons, Ltd. Geol. J. 46: 217239 (2011)
multiple tectonometamorphic imprints in the lower crust, egb, india 221
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Table
1.Summaryofmineralogy,texture,mineral
chem
istry,eldandmicrostructure
andPT-tconstraintsofthethreevarieties
ofaluminousgranulites
Mineral
association
Structural/micro-structural
characters
Key
texturalfeatures
D1D2(M
1)andPost
D2-interkinem
atic
(M1R)event
D3(M
2)event
Mineral
chem
istry
AssociationA
GrtCrdIlm
Spl
Rt
QtzPl
KfsSilBt
Spr
Migmatitic
withalternate
leucosomes
(Qtz,PlandKfs)
andmelanosome(G
rtA1,Crd,
IlmA1,Rt,PlandQtz);fabric
S1/S
2;ductiledeform
ation
inGrtA1.
Bt A
1,Spl A
1,Qtz
andIlmA1
inclusionin
GrtA1,exsolved
Hem
inIlmA1;intergrowth
ofGrtA2
Spl A
2IlmA2;GrtA3SilA3Qtz
symplectiteafterCrd;Grtreplaced
byBt.
M1:peakreached
through
Bt-meltingreactionsproducing
GrtA1CrdRt
melt
(1&
2);GrtA2Spl A
2IlmA2
SprafterOpxA1.
Crd
breakdownto
GrtA3SilA3
Qtz
(3)
GrtA1/GrtA2:Alm
50Prp
46Grs2,
GrtA3:Alm
60Prp
37Grs2Sps 1;Spl A
1
(XMg0.390.42),2.83.3wt%
ZnO,Spl A
2(X
Mg0.580.60),
2.12.4wt%
ZnO;Spr
(XMg0.770.80)close
to7:9:3;Crd
(XMg0.86);Bt A
1(X
Mg0.830.88),
5.2wt%
TiO
2,XF
0.29.
AssociationB
OpxCrdSpl SSIlm
QtzPl
KfsSilGrt
Gneissic
fabric
(transposedS1/S
2)with
alternateleuco-(Q
tz
Plag
Kfs)andmelanocratic
layers
(OpxB1,Crd,Spl,Ilm,Qtz,
Pl
Sil);mylonitic
foliation
(S3m);plastic
deform
ation
inOpxB1,Spl B1,Crd
and
Qtz
grains.
OpxB2S
ilB2coronaover
Spl B1
(Ilm);exsolved
Hem
inIlm,
lamellaeofSpl B2,Crd
and
GrtB2in
OpxB1;OpxB3SilB3
Qtz
intergrowth
afterCrd.
M1:peakthroughBtmelting
reactionproducingOpxB1
Spl B1Crdmelt(5);
Spl B2CrdGrtB2intergrowth
afterOpxB1(6&
7).
M1R:OpxB2SilB2afterSpl B1
Crd/Qtz
(8, 9, 10)
Crd
breakdownto
Opx
B3SilB3
Qtz
(11).
OpxB1(X
Mg0.630.66),9.7wt%
Al 2O3(core),OpxB2(X
Mg0.65)
7.87.4%
Al2O3;OpxB3(X
Mg0.63,
6.86.3wt%
Al 2O3)Spl B1
(XMg0.370.43)2.22.8wt%
ZnO,0.63.1wt%
Cr 2O3;Spl B2
(XMg0.38)1.4wt%
ZnO;
GrtB2:Alm
58Prp
40Grs1Sps 1
AssociationC
Opx,Crd,Spr,Pl,Kfs,
Sil
Qtz
Massive,isolatedclusters
inlow
strain
domains
wrapped
byS3m.
OpxC2S
ilC2double
coronaafter
Spr
Crd/Qtz;inclusionofSplin
Spr;OpxC3SilC3Qtz
intergrowth
afterCrd;OpxC1replacedbylate
Bt.
M1:peakthroughBtmelting
reactionproducingOpxC1
Crd
C1/Spl(13, 14);stability
ofSpr(15, 17),
M1R:coronal
OpxC2SilC2
(16, 18, 19)
Crd
breakdownto
OpxC3SilC3Qtz
Included
Spl(X
Mg
0.380.42)0.71.0wt%
ZnO;OpxC1/OpxC2
(XMg0.66)8.0wt%
Al 2O3at
core
to7.1wt%
atrim;OpxC3
(XMg0.66),6.26.9wt%
Al 2O3;
Spr(X
Mg0.740.76)close
to7:9:3
Deform
ation
D1D2
Post-D
2interkinem
atic
gap
D3
D4
Metamorphicevents
Progradeto
peakM
1M
1R
M2
M3Localized
retrogressionin
presence
ofmelt
PT
conditions
Progradepathfrom
high
T/lowPconditionsto
10008C
,6.58.5kbar
atthepeak
Coolinganddecompression
to
8008C
,6kbar
Loadingto7
8kbar,8508C
,possibly
accompaniedby
partial
meltextraction
5008008C
(poor
constraint)
PT-tpath
ACW
path
Coolingwithdecompression
CW
path
Unknown
Ageconnotationand
possiblecorrelation
ca.1000Ma
ca.950MaRayner
orogeny;assembly
ofRodinia
ca.900MaD3D4
ofRSEin
Rayner
Complex
Denotesreactionnumber
asdiscussed
intext.
Copyright # 2010 John Wiley & Sons, Ltd. Geol. J. 46: 217239 (2011)
222 k. das ET AL.
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quartz (Figure 4e). The intergrown lamellae of garnet can at
places, be traced continuously to the grain boundary.
Sillimanite (SilB3) forms a spongy (and sometimes skeletal)
intergrowth with granular orthopyroxene (OpxB3) and quartz
that replaces cordierite along the margins (Figure 4f). This
intergrowth commonly forms wispy trails and shows a
mylonitic fabric. Occasionally, cordierite grains are com-
pletely pseudomorphed by ne-grained intergrowth of
OpxB3, SilB3 and quartz (Figure 4g). This symplectic
intergrowth along with other polymineralic matrix grain
aggregates, form an oriented fabric (S3) that sweeps
asymmetrically around cordierite clasts (Figure 4f). This
indicates contemporaneous shear fabric development with
breakdown of cordierite. Extreme grain renement is
evident in quartz and feldspar grains. An oblique foliation
(as S-) is developed by the shape fabric of dynamically
recrystallized polymineralic matrix grains with attened,
recrystallized quartzose bands and ribbon quartz (C-).
OpxB1 clasts are attened with recrystallized asymmetric
trails giving s structure in unoriented section (Figure 4c).The ne-grained polymineralic matrix is the product of
dynamic recrystallization by the process of subgrain rotation
Figure 4. (a) Asymmetry in alkali feldspar clast and also bending of exsolution lamellae in alkali feldspar. (b) Orthopyroxene grains show evidences of dynamicrecrystallization. (c) Asymmetry in orthopyroxene grains is to be noted where recrystallized grain fabric wraps around it. (d) Orthopyroxene grains (Opx)containing lamellae of spinel (Spl) and cordierite along the same crystallographic plane. (e) BSE image showing orthopyroxene porphyroblast (Opx) containinglamellae of garnet (Grt) and globular quartz (Qtz) along a crystallographic plane. (f) BSE image showing symplectic intergrowths of Opx SilQtz form anoriented fabric that sweeps asymmetrically around cordierite clasts. (g) The same intergrowth of sillimanite (Sil), orthopyroxene (Opx) and quartz (Qtz)pseudomorphing cordierite (Crd) grain. (h) Bands of coarse recrystallized quartz forming ribbons engulfed within ne-grained polymineralic recrystallized
matrix with sharp boundaries.
Copyright # 2010 John Wiley & Sons, Ltd. Geol. J. 46: 217239 (2011)
multiple tectonometamorphic imprints in the lower crust, egb, india 223
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(SR). Small grains in the matrix show development of
subgrains (recovery stage). The rock contains discontinuous
and asymmetrically tapered-head bands of coarse quartz
either engulfed within or alternating with ne-grained
polymineralic recrystallized matrix with sharp boundaries.
Grain boundary area reduction (GBAR) is evident in these
bands with curved to straight grain boundary in polygonal
aggregates that are free from any intracrystalline defor-
mation (Figure 4h). These grains are therefore statically
recrystallized. Extensive recrystallization might have been
caused by the combined effects of subgrain rotation and
grain boundary migration with increase in temperature
(Hirth and Tullis, 1992; Passchier and Trouw, 1998). These
microstructural signatures collectively imply shear defor-
mation at high-T granulite-grade metamorphic conditions.
High temperature and presence of uid along grain
boundaries generally favour recovery and recrystallization,
while high strain rate promotes distortion (Passchier and
Trouw, 1998). Secondary grain growth due to GBAR and
development of strain-free monomineralic quartz ribbons
are indicative of high temperature, above 7008008C(Passchier and Trouw, 1998). OpxB1clasts, surrounded by
mantle of recrystallized grains (Figures 4b and Figure 4c),
also suggest granulite facies metamorphic condition in the
temperature range mentioned earlier (Passchier and Trouw,
1998).
Association C develops both Qtz-rich and Qtz-poor
microdomains. Isolated clusters of porphyroblastic ortho-
pyroxene and cordierite grains in low-strain domains impart
a massive look to the rock. The quartz-absent domain is
characterized by megacrystic orthopyroxene (OpxC1),
cordierite, sapphirine, plagioclase, perthite and also
dominance of sillimanite (SilC1). Sapphirine occurs in the
interstices of porphyroblastic cordierite and is separated
from the latter by a double corona of OpxC2 and SilC2(Figure 5a). The development of these coronal phases was
possibly pre-D3. Rare inclusions of spinel are present in
sapphirine that occurs at the contact of cordierite. On the
other hand, the quartz-bearing domain also contains
porphyroblastic orthopyroxene (OpxC1), cordierite, sapphir-
ine, plagioclase, perthite and sillimanite as major minerals.
Sapphirine (SprC1) is separated from quartz by a thick
corona of sillimanite (SilC2) and orthopyroxene (OpxC2)
(Figure 5b). In both the microdomains (quartz-present
and quartz-absent) cordierite shows breakdown to
OpxC3 SilC3 quartz intergrowth during D3 event similarto that described in Association B.
5. MINERAL CHEMISTRY
Representative samples of all the types were analysed by
electron microprobe (JEOL 733) at Hokkaido University,
Figure 5. (a) Xenoblastic sapphirine (Spr) is separated from cordierite(Crd) by a double corona of sillimanite (Sil) and orthopyroxene (Opx).Note the presence of relic spinel (Spl) in sapphirine and biotite (Bt) patcheson orthopyroxene. (b) BSE image of quartz-present microdomain wherematrix sapphirine grain (Spr) is separated from quartz by a thick corona ofsillimanite (Sil) and orthopyroxene (Opx). (c) Compositional plots ofsapphirine grains to show the extent of Tschermak substitution (alongthe line joining 2:2:1 and 7:9:3 compositions). Note that all the compo-
sitions plot close to the latter point.
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224 k. das ET AL.
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Japan. The instrument was operated at 15 kV accelerating
voltage and 20 nA specimen current. Synthetic and natural
standards are used. Raw data were processed by ZAF
correction scheme. Individual phase chemical data are
presented in the Supporting information (Supplementary
Tables 26), while a summary of the phase chemical
characteristics are given in Table 1.
In Association A, GrtA1 and GrtA2 have similar
compositions, while GrtA3 is more iron-rich (Alm60Prp37Grs2Sps1) (Supplementary Table 2). SplA1 has variable
composition (XMg 0.390.42) and contains 2.83.3 wt%ZnO. SplA2 is more magnesian (XMg 0.580.60) withlower Zn (2.12.4wt% ZnO). Sapphirine is magnesian
(XMg 0.770.80) and is close to the 7:9:3 composition(Figure 5c). Cordierite is magnesian (XMg 0.86) andhomogeneous in composition. IlmA1 contains 1015mol%
hematite and 47mol% geikielite components. Exsolved
hematite is titaniferous containing 16mol% ilmenite and
negligible geikielite components. Included BtA1 is magne-
sian (XMg 0.830.88) and contains 5.2 wt% TiO2. Thesegrains contain 2.5wt% F (XF 0.29) and negligible Cl. Latebiotite (XMg 0.0.830.91) is compositionally similar withrespect to XMg, but contains lower Ti (TiO2 2.14.2wt%)and higher F (2.93.9wt% F; XF 0.340.44).In Association B, orthopyroxene shows compositional
variations in different textural modes. OpxB1 (XMg 0.630.66) is highly aluminous and the alumina content decreases
from intergrowth-free core regions (maximum Al2O39.7wt%) to regions having intergrowth of SplB2 (Al2O38.0wt%) as well as near the rims (Al2O3 6.8wt%).However, XMg does not change appreciably ( 0.65). OpxB2is compositionally similar in XMg (0.65) but slightly less
aluminous than the core of OpxB1. Thick coronal grains
show decrease in alumina content from the core (7.8wt%) to
rim near SplB1 (7.4wt%). OpxB3 (XMg 0.63) contains 6.36.8wt% alumina. Spinel shows compositional variations in
different modes. SplB1 grains are compositionally more or
less homogeneous (XMg 0.370.43) with ZnO 2.22.8wt% and 0.63.1wt% Cr2O3. Magnetite content in
SplB1 ranges between 34mol%. SplB2 (XMg 0.38)contains 1.4wt% ZnO and is low in Cr2O3 content. All
these phases contain insignicant amount of TiO2 (Supple-
mentary Table 3). Ilmenite contains 1013mol% hematite
and 34mol% geikielite components. Exsolved hematite
contains maximum 17mol% ilmenite component. GrtB2 is
compositionally Alm58Prp40Grs1Sps1. Cordierite is homo-
geneous in composition (XMg 0.830.84). Sillimanitecontains 0.91.1wt% Fe2O3 (total). Plagioclase is
Ab74An26. Late biotite (XMg 0.740.78) contains 4.45.3wt% TiO2 and 2.4wt% of F (XF 0.29).Spinel included within sapphirine in Association C has
XMg 0.380.42 and is low in ZnO (0.71.0wt%) andCr2O3 (0.20.3wt%). SilC1 contains 1.0wt% Fe2O3 (total).
Cordierite (XMg 0.830.85) is again homogeneous. OpxC1shows compositional homogeneity in terms of FeMg
distributions (XMg 0.66), but exhibits Al-zoning fromcore (Al2O3 8.0wt%) to rim (Al2O3 7.1wt%). A thickcorona of OpxC2 shows a comparable composition as that
of OpxC1. Symplectic OpxC3 (XMg 0.66) contains 6.26.9wt% alumina. Sapphirine is magnesian with XMg 0.740.76 and mostly 7:9:3 in composition (Figure 5c). Recalcu-
lated composition shows variable amount of ferric iron
(Fe2O3 1.94.0wt%) and appreciably high XFe3 (Supple-mentary Table 4). Late biotite (XMg 0.760.78) contains5.5 wt% TiO2, 2.3 wt% F (XF 0.27) and insignicant Clcontent.
6. EVOLUTION OF MINERAL ASSEMBLAGES
The textural and compositional features in the aluminous
granulites presented earlier attest to several stages of mineral
reconstitution.
6.1. Association A
High modal abundance of garnet, quartz and Fe-Ti oxides in
this association implies a Fe-Ti-rich silica-saturated proto-
lith. The peak metamorphic stage, culminated during the D2event, is characterized by the presence of coarse garnet
(GrtA1) in this rock. Presence of biotite, spinel and quartz
inclusions in garnet (Figures 3e and f) and presence of
cordierite in close association suggest the following
KFMASH dehydration-melting reaction during D1D2event:
BtA1 SplA1 Qtz GrtA1 Crdmelt (1)
This reaction has a steep dP/dT slope and occurs in the
temperature range 8009008C under 5 kbar pressure in thehigh fO2 KFMASH grid (Dasgupta et al., 1995). In the low
fO2 grid, however, this reaction is encountered at slightly
lower PT condition of 7408C, < 4 kbar emanating fromthe [Opx,Spr] invariant point (Scrimgeour et al., 2001).
The presence of included ilmenite in GrtA, highly
titaniferous composition of BtA1 and development of
abundant rutile would indicate a more complicated multi-
variant reaction involving TiO2, such as
BtA1 SplA1 Qtz IlmA1 GrtA1 Rt Crdmelt (2)
The mesoperthite quartz plagioclase mat surroundinggarnet could indicate the former presence of melt. Owing to
the coarse grain size of the garnet porphyroblasts and the
presence of voluminous proportion of quartzo-feldspathic
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multiple tectonometamorphic imprints in the lower crust, egb, india 225
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minerals, we consider that a high degree of partial melting
occurred at elevated temperatures. Both the above two
reactions may involve K-feldspar, either as reactant or
product (Harley, 2008). Experimental data on dehydration
melting of biotite indicate that such reactions occur at
T> 8128C at 10 kbar (Vielzeuf and Holloway, 1988; Patinoand Patino Douce, 1991; Gardien et al., 1995; Pickering and
Johnston, 1998), with the volume of melt increasing with
temperature. Experimental data also show that XMgBt, TiO2
Bt
and FBt increase with temperature (Munoz, 1984; LeBreton
and Thompson, 1988; Peterson et al., 1991; Patino Douce,
1993; Skjerlie and Johnston, 1993; Dooley and Patino
Douce, 1996; Stevens et al., 1997; Pickering and Johnston,
1998). The included biotite in the present study area is
magnesian, titaniferous and uorine-rich, which attests to
very high metamorphic temperatures in the study area.
Coarse garnet occurs in this rock as another textural
variety (GrtA2) where it is intergrown with sapphirine, spinel
(SplA2) and ilmenite (IlmA2) needles (Figure 3g). This
intergrowth may be a breakdown product of anomalously
high aluminous orthopyroxene formed during the pre-peak
prograde stage (Das et al., 2006a).
Fine-grained aggregate of GrtA3 SilA3Qtz thatreplaces cordierite (Figure 3h) during the high-strain
event D3 suggesting the reaction
Crd GrtA3 SilA3 Qtz (3)
This reaction has at negative dP/dT slope and operates
due to loading. This could also ensue on melt loss and
reduction of H2O activity (Harley, 2008).
Late biotite was formed during M3D4 at the fringes of
garnet grains with invasion of hydrous uid via the reaction
GrtA1 SilA3 H2O Bt Qtz (4)
6.2. Association B
Abundance of spinel solid solution, plagioclase with quartz
and rare occurrence of prismatic sillimanite and FeTi
oxides in this association suggest a Fe-rich, Ti-poor and
silica-saturated protolith. The peak assemblage in this rock
is constituted of spinel (SplB1) quartz aluminous ortho-pyroxene (OpxB1) cordierite with minor rutile, monaziteand zircon. Textural data suggests that CrdQtzOpxB1SplB1 formed a stable assemblage during the peak stage.
Stabilization of this assemblage could be achieved by biotite
dehydration melting in a semipelitic bulk composition
during the D1D2 event, viz.
Bt Pl Qtz OpxB1 SplB1 Crdmelt (5)under high Tlow P conditions (Vielzeuf and Montel, 1994).
The intergrowth of spinel, cordierite and garnet in
orthopyroxene porphyroblasts in this association can be
explained by the reaction relations involving Tschermak
molecules present in the early-stabilized anomalously high
aluminous orthopyroxene (Bose et al., 2006). The occur-
rence of spinel and cordierite in some aluminous orthopyr-
oxene porphyroblasts can be represented in MAS system via
Mg-Tschermak breakdown reaction
Mg Ts Spl Crd (6)at low Phigh T conditions.
On the other hand, participation of garnet (Prp) in the
intergrowth requires involvement of Mg-Tschermak com-
bined with enstatite (En)
Mg Ts En Prp (7)
This reaction, modelled by Gasparik (1994) occurs due to
loading or heating.
The appearance of a double corona of OpxB2 SilB2separating SplB1 against cordierite porphyroblasts in local
quartz-free microdomain indicates the operation of FMAS
divariant reaction in the pre-D3 stage
SplB1 Crd OpxB2 SilB2 (8)
A similar double corona of OpxB2 SilB2 also appears onSplB1 separating it from quartz through another FMAS
divariant reaction
SplB1 Qtz OpxB2 SilB2 (9)
These two reactions operate in closely spaced micro-
domains, possibly during the same stage of metamorphic
crystallization. These divariant reactions emanate from the
FMAS univariant reaction
SplB1 Crd Qtz OpxB2 SilB2 (10)
Reaction (8) has a at positive dP/dT slope and operates
due to cooling with or without loading.
The unique textural feature of the studied rock is
the breakdown of cordierite to ne-grained orthopyroxene
(OpxB3), sillimanite (SilB3) and quartz (Figures 4f, Figure 4g).
This suggests the reaction during high-strain event D3
Crd Opx B3 SilB3 Qtz (11)
This reaction has a at dP/dT slope and operates due to
loading. However, this reaction will occur only due to
loading in a melt-present situation (Carrington and Watt,
1995).
Late biotite formed along the margins of orthopyroxene at
the last M3D4 event due to hydration in presence of melt/
alkali feldspar via the reaction
Opx Sil H2O Bt Qtz (12)
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226 k. das ET AL.
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6.3. Association C
As discussed earlier, this association has two microdomains
marked by the presence or absence of quartz. In the quartz-
absent microdomain, presence of sapphirine, and abundance
of sillimanite and cordierite, coupled with the magnesian
nature of all the FeMg phases clearly indicate a silica-
undersaturated high-magnesian-aluminous domainal bulk
composition. The early-stabilized phases in this assemblage
are aluminous orthopyroxene and cordierite with occasional
relict spinel grains (now enclosed in sapphirine). Such an
assemblage could form during D1D2 by partial melting of a
biotite-sillimanite-bearing protolith through the reactions
Bt SilC1 Qtz OpxC1 Splmelt (13)
Bt Spl Qtz OpxC1 CrdC1 melt (14)
K-feldspar can participate in such reactions either as
reactant or as product depending on the K2O/H2O ratio
between biotite and melt (Carrington andWatt, 1995). These
reactions occur in the pressure range of 67 kbar at a
temperature> 8508C (Das et al., 2001). Absence of quartzin this association possibly implies complete removal of
silica during the said melting reactions.
Appearance of sapphirine of 7:9:3 composition engulng
spinel close to cordierite grains (Figure 5a) suggests the
FMAS reaction
Spl CrdC1 Sil Spr (15)
This reaction occurred during D1D2 prograde meta-
morphism as it represents a part of the metamorphic peak
assemblage. The presence of a double corona of
OpxC2 SilC2 over sapphirine separating it from cordierite(Figure 5a) suggests the reaction
Spr CrdC1 OpxC2 SilC2 (16)
This reaction has a at positive dP/dT slope and operated
due to cooling in the pre-D3 stage.
In the quartz-present microdomain of this association, the
appearance of sapphirine from spinel can be explained by
FMAS reaction during D1D2 prograde metamorphism
Spl Qtz Sil Spr (17)
Textural evidence suggests that sapphirine and quartz in
this microdomain are separated by thick coronae of
sillimanite and orthopyroxene (Figure 5b). This indicates
cooling in the pre-D3 stage across the reaction
Spr Qtz OpxC2 SilC2 (18)
Reactions (17) and (18) emanate from the FMAS
univariant reaction
Spl Spr Qtz OpxC2 SilC2 (19)
Coarse cordierite grains show breakdown to the sym-
plectic intergrowth of OpxC3 SilC3Qtz through reaction(11) during D3 as observed in Association B.
Development of late biotite during M3D4 over orthopyr-
oxene can be explained by the reaction (12) as inferred for
Association B.
7. THERMOBARIC CONDITIONS OF
METAMORPHISM
Estimation of PT conditions of metamorphism in a
polymetamorphosd UHT terrane is plagued with two
major problems. One is related to down-temperature re-
equilibration of mineral composition (Harley, 1989; Frost
and Chacko, 1989; Pattison et al., 2003). The other
constraint lies in the identication of equilibrium mineral
compositions at each metamorphic stage.
First we estimate peak metamorphic temperatures from
fossil thermometers using the reintegrated composition of
peak phases. Reintegrated composition of mesoperthitic
feldspar gives a temperature close to 10008C isotherm in thediagram of Elkins and Grove (1990). The orthopyroxene
Al-isopleth diagram of Harley (2004) gives peak meta-
morphic temperatures close to 10008C for the assemblageOpxC1-Spr-Qtz. Intergrown sapphirine and spinel in
peak garnet (GrtA2 gives temperatures around 8608708Cfollowing the formulation of Das et al. (2006b). This lower
estimate is probably due to down-temperature resetting of
mineral compositions.
Coexistence of sapphirine and quartz during the peak
metamorphism in Association C clearly indicates tempera-
tures in excess of 10008C based on both petrogenetic grids inthe system KFMASH (Dasgupta et al., 1995; Das et al.,
2003; Kelsey et al., 2004) and PT pseudosections
calculated with the internally consistent dataset of Holland
and Powell (1998) (Kelsey et al., 2004). The pressure
condition during peak metamorphism is difcult to estimate,
as there is a discrepancy of 2.53 kbars between the twoapproaches that has been ascribed to variations in aH2O(Harley, 1998; Kelsey et al., 2004; Baldwin et al., 2005).
While the experimentally constrained petrogenetic grid in
the system KFMASH (Das et al., 2003) would indicate peak
pressures of 9 kbar for the mineral assemblages (spinel-sapphirine-garnet-quartz-orthopyroxene) developed at this
stage in different associations, the computed grid and
pseudosection of Kelsey et al. (2004) would indicate 6.57 kbar for the same set of assemblages. Moreover, the
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actual pressure estimate will be dependent on the Zn content
in spinel (Waters, 1991), thereby adding to further
uncertainty.
Given the above constraints, we estimate the peak
metamorphic conditions during the culmination of D1D2to be> 10008C and 79 kbars.Using the Al-isopleth diagram (Harley, 2004), we have
estimated temperatures in the range of 8008508C whereorthopyroxene equilibrated with cordierite, sillimanite and
quartz in all the three associations. Garnet (GrtB2) lamellae
in OpxB1 give a temperature 7308308C using garnet-orthopyroxene thermometer after Lee and Ganguly (1988) in
the pressure range of 79 kbar. This is obviously a reset
temperature as the same compositions give temperatures of
9309408C using the method of Pattison et al. (2003). Wehave used the composition of coexisting Spl-Crd to calculate
temperature using the formulations of Nichols et al. (1992),
which takes into consideration the gahnite component in
spinel. The estimated temperature ranges from 660 to 6908Cat assumed pressures of 78 kbars. The thermometric data
attests to signicant cooling, probably down to 8008C in thepre-D3 stage, but the pressure conditions during cooling
could not be pinpointed.
The appearance of orthopyroxene-sillimanite-quartz
intergrowth (both in Associations B and C) and of garnet-
sillimanite-quartz (in Association A) after cordierite may
imply a rise in pressure as these reactions have at dP/dT
slopes in the subsystem FMAS (Hensen, 1986). Therefore, it
is likely that the cooled granulites were subjected to loading
during D3. Using the orthopyroxene (OpxB3, C3)cordierite
barometric formulation of Bertrand et al. (1992), we obtain
pressures around 7.88.0 kbar at an assumed temperature of
8008C. The garnet (GrtA3)cordierite thermometer ofNichols et al. (1992), gives 7208C at 8 kbar. It is evidentfrom the above that minor loading of 1 kbar could havetaken place during D3. In the subsequent section, we will
explore an alternative explanation.
Garnet-biotite thermometry (after Ferry and Spear, 1978)
gives 4008C for late biotite (Bt2) patches on garnet occurringduring theM3D4 event. Since this formulation does not take
into account the Ti and F content in biotite, the estimate is
only a lower limit. An upper limit is obtained from the Ti
content of late biotite in this rock saturated with ilmenite and
quartz that plots above the 8008C isotherm (Henry et al.,2005).
8. PSEUDOSECTION AND PETROGENETIC GRID
CONSIDERATIONS
In this section we investigate further the PT conditions and
PT path of metamorphism using pseudosection modelling.
Such studies are complicated in the case of polymeta-
morphic granulites because re-metamorphism occurs in a
bulk composition that has changed substantially from that of
the protolith due to partial melting and melt loss during the
earlier event (White et al., 2001). Extraction of melt in
varying proportions is considered to be a key factor in the
preservation of peak granulite assemblages (White and
Powell, 2002; Kelsey et al., 2003). Drawing analogy, we can
argue that an indenite amount of melt was extracted from
the studied rocks as the peak UHT assemblages are
preserved. While the breakdown of cordierite to orthopyr-
oxene sillimanite quartz (Reaction 11) or to gar-net sillimanite quartz (Reaction 3) can be facilitatedby extraction of melt, preservation of all stages of textural
conversions (Figures 4f and g) show that melt loss was far
from complete. Formation of high F-bearing biotite
during D4 attests to limited melt-solid interaction signifying
presence of melt at even the last stage. At the same time,
maximum reaction progress (complete pseudomorphism)
can occur in domains of extensive melt loss. Since the
cordierite breakdown reactions occurred simultaneously
with D3 compression and shearing, melt extraction could
have been facilitated in domains by tectonic squeezing. This
would obviate the requirement of loading for cordierite to
break down. We have undertaken a PT pseudosection
approach to test whether loading is at all required to break
cordierite down.
Two general approaches have been followed to model the
protolith composition where possible melt loss occurred.
One approach is to use several hypothetical bulk compo-
sitions (White et al., 2001, 2007; Johnson and Brown, 2004),
primarily because the migmatites are themselves refractory
from which an unspecied amount of melt has been lost. A
more rigorous approach to resolve this problem is to use the
changed bulk rock composition using the theoretical
calculation matched with natural data (cf. Saha et al., 2008).
A second approach uses an effective bulk composition,
estimated through calculated mineral modes and mineral
compositions have been applied to compute PT pseudosec-
tion (Kelsey et al., 2003; Baldwin et al., 2005). In this work
we have followed the latter because of the difculty to
estimate the volume and composition of melt extracted from
the system. Even where leucosomes are present, as in the
case of Associations A and B, it is likely that part of these
could be of cumulate origin (e.g. Johnson and Brown, 2004).We have taken up two unique microdomains in the studied
rocks for phase relation modelling. These represent discrete
mineralogical domains with distinct domainal chemical
compositions. One is the intergrowth involving cordierite,
spinel, garnet and quartz in porphyroblastic orthopyroxene
(Figures 4d and e). The other one is the pseudomorphous
breakdown of cordierite porphyroblasts in the high-strain
zones to orthopyroxene, sillimanite and quartz
(Figures 4f and g). The bulk compositions for both the
microdomains have been calculated by the modal ratios of
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228 k. das ET AL.
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the phases present (using image analysis of microphoto-
graphs and BSE images) and their respective mineral
compositions. The recalculated bulk compositions in both
the cases can be represented in the simplied FMAS (FeO-
MgO-Al2O3-SiO2) system. Phase relations were modelled in
the FMAS system using THERMOCALC v.3.2.3 (Powell
and Holland, 1988), and the dataset of Holland and
Powell (1998, version 5.5 s, November 2003) with the
activity-composition model for sapphirine of Kelsey et al.
(2004).
The two pseudosections were constructed to characterize
the PT history of the near-peak metamorphic condition and
of the later high-strain event (D3). Porphyroblastic
aluminous orthopyroxene (zoned in terms of alumina from
core to rim) contains intergrown garnet, spinel and cordierite
along crystallographic orientations in the presence of quartz
in Association B. This assemblage is considered to have
developed at near-peak metamorphic condition. In the
earlier section, we explained the development of these
intergrowths in porphyroblastic orthopyroxene from break-
ing down of non-quadrilateral aluminous orthopyroxene. It
is, however, not possible to construct pseudosections with
ctive components, such as the Tschermak molecule in
orthopyroxene. Instead, we have modelled the reaction
orthopyroxene spinel quartz garnet cordierite (Spr,Sil) from the recalculated domainal bulk composition in the
FMAS system (compositional relationship is shown in
Figure 6a) to obtain the relative stability elds of the
different assemblages present in the intergrowths. The
pseudosection (Figure 6b) shows that the reaction has a
steep slope separating different divariant and trivariant
elds. On the low pressure side the stable trivariant
assemblage contains orthopyroxene, spinel and cordierite.
With increasing pressure the stable assemblages on the low
temperature side change to orthopyroxene-cordierite-garnet,
and subsequently to orthopyroxene-garnet-quartz through
intermediate divariant assemblages, e.g. orthopyroxene-
spinel-garnet-cordierite and orthopyroxene-cordierite-gar-
net-quartz. Although it is not possible to identify any
sequence of mineral development from Figures 4d and
Figure 4e, stabilization of quartz with garnet (Figure 4e)
may reect loading from an early-stabilized cordierite and
spinel (Figure 4d), as shown in Figure 6b. Loading near to
Figure 6. (a) Compositional plots of the phases in (AlFe3)2O3/totalFMAS vs. SiO2/total FMAS space (in atomic fraction). The tie-line ip andpiercing plane relations are elucidated in the text. Note the position ofcordierite (Crd) within the two compositional triangles, i.e. Opx-Sil-Qtz andGrt-Sil-Qtz. (b) PT pseudosection for the microdomain with recalculatedbulk composition of SiO2:Al2O3:MgO:FeO 46.55:10.25:25.28:17.91 (inmole ratio) made by THERMOCALC v3.2.3 (Powell and Holland, 1988).Internally consistent thermodynamic dataset of Holland and Powell (1998)is used. Activity-composition model of sapphirine is taken from Kelseyet al. (2004). Dashed isopleths are for y(Opx) and mixed dash-dot linerepresents isopleth for XFe of garnet, i.e. x(Grt). Note the probable PT pathshowing evolution in the near-peak metamorphic condition. (c) PT
pseudosection for the microdomain where cordierite is broken down toorthopyroxene-sillimanite-quartz assemblage in a later structuralevent, D3. Bulk composition recalculated as SiO2:Al2O3:MgO:FeO56.06:21.94:18.16:3.85 (in mole ratio). Note the disposition of differentvariance elds (v 2 and 3) and the isopleths [y(Opx) as dashed lines,x(Opx) as dotted lines and x(Crd) as thin continuous lines]. At 8508C, aslight pressure increase of 500 bars can induce this breakdown through thedivariant eld of orthopyroxene-cordierite-sillimanite-quartz at proper uidactivity. As discussed in the text, such breakdown can be aggravated further
by melt loss from the high-strained microdomains.
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multiple tectonometamorphic imprints in the lower crust, egb, india 229
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peak metamorphic conditions is also supported by the
garnet-spinel-sapphirine intergrowth in Association A (cf.
Das et al., 2006a). The postulated near-peak loading is
consistent with an anticlockwise PT path deduced from
adjacent areas (Sengupta et al., 1990; Bose et al., 2000).
Similar anticlockwise PT paths have also been reported
from other UHT terranes (e.g. Santosh et al., 2007). The
cooling segment of the PT path shown in Figure 6b is
construed from the Al-zoning in orthopyroxene as described
in the preceding section. Although the pseudosection is
constructed in the FMAS system, the presence of a small
amount of Fe3 in sapphirine, spinel and orthopyroxeneactually implies the relevant system be FMAS(O). At
elevated oxygen fugacity, the stability of phases like spinel
would enlarge and as a result grid topology would change
and even some of the peak assemblages would be enlarged
towards lower temperature (KFMASH system; Das et al.,
2003; Harley, 2008 and references therein).
The second pseudosection was constructed to model the
FMAS reaction orthopyroxene cordierite sillimanitesapphirine quartz (Grt, Spl) (compositional relationship isshown in Figure 6a) using the microdomainal bulk
composition in Association C (Figure 6c). Two divariant
assemblages, e.g. orthopyroxene-cordierite-sillimanite-
quartz on the lower temperature side and orthopyroxene-
cordierite-sapphirine-quartz on the high temperature side,
are associated with this univariant reaction. On the lower
temperature side, cordierite breaks down to orthopyroxene,
sillimanite and quartz with slight increase of pressure
0.5 kbar. In Association C this reaction occurredduring D3, subsequent to cooling down to 8008 C(reactions 16, 18). The above analysis suggests possible
minor loading of the cooled granulites at around 8508C(Figure 6c). As discussed earlier, breakdown of cordierite
could have been aided by extraction of melt with its
dissolved H2O along high-strain zones of the rock (tectonic
squeezing (?) during D3 event contemporaneous with the
development of S3m mylonitic foliation). Oxide total in all
analysed cordierite grains ranges between 9798wt%,
which implies the possible presence of uids. However,
in the absence of analytical data for H2O and CO2, we can
hardly quantify the nature of uid and its control over
cordierite stability in the studied rocks. It is therefore
difcult to specify whether cordierite breakdown is solely
caused by loading or melt extraction.
9. GEOCHRONOLOGY
We analysed zircon grains for U-Pb ages with an ion
microprobe to constrain major thermal imprints on the
assemblages. Additionally, we undertook EPMA chemical
dating of monazite included within orthopyroxene and
sapphirine porphyroblasts in Association C to constrain the
timing of M1 metamorphism. Monazite grains present
within cordierite grains were also analysed for
comparison.
9.1. Analytical methods
About 1 kg of the representative sample (Pan03) was
initially crushed, and zircon grains were concentrated using
water table and magnetic separation. Individual crystals
were selected and hand-picked under the optical microscope
for mounting. Analytical procedures adopted were the
same as those followed in Shiraishi et al. (2008). Spots
within the zircon crystals were selected using optical, BSE
and CL imaging (Figure 7), and were analysed on the
SHRIMP II at the National Institute of Polar Research,
Japan. Analytical data are presented in Supplementary
Table 5 and plotted in a TerraWasserburg diagram
(Figure 8a). Uncertainties quoted in the tables and in the
text for individual analyses (ratios and ages) as well as plots
are at 68% condence level (1s), whereas concordia and
mean age calculations were done at 95% condence level.
Concordia age calculation has been done using the program
SQUID (version1.02, Ludwig, 2001) which takes into
account the error in the standard. Plots are done by the
program ISOPLOT/EX (version 3.6, Ludwig, 2008). Back
Scatter Emission (BSE) and Cathodoluminescence (CL)
images of the analysed zircon grains reveal complex internal
structure with characteristic CL responses. While neoblastic
homogeneous to simple concentric zoned zircon shows
virtually no inheritance, other grains contain inherited
domains surrounded by overgrowth.
Monazite grains included within orthopyroxene or
associated with sapphirine were targeted for chemical
analysis. Those grains were analysed by the CAMECA-
SX100 electron microprobe at Indian Institute of Technol-
ogy, Kharagpur, India. The instrument was operated with
20 kV acceleration voltage and 200 nA beam current with
1mm beam diameter. Details of analytical procedure areafter Bhandari et al. (2011). Natural standards were used for
chemical analyses, while externally dated monazite standard
with an IDTIMS age of 2546Ma were used for age
calibration. During the entire analytical session, the above
standard gave an age of 2558 105Ma. Counting times forPb and Th were taken as 300 s and 200 s, respectively, while
those for other elements vary in the range 20100 s. Prior to
analysis, the target grains were mapped for U, Th, La and Ce,
so that different compositional domains could be identied.
Results of all the analyses are presented in Supplementary
Table 6. Calculation of weighted mean age is done by the
program ISOPLOT/EX (version 3.6, Ludwig, 2008).
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230 k. das ET AL.
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9.2. Results
Mounted zircon grains are oval to circular in shape with a
few elongated and euhedral in appearance. Grain size varies
from 100 to 200mm in length and 100150mm in width.Apart from a few neoblastic grains, most grains show core-
rim structure where the inner part is made of a thick
oscillatory-zoned domain with or without inherited cores.
Neoblastic grains are broadly homogeneous, some having
simple concentric zoning. Few apparently neoblastic grains
shows faint traces of hidden oscillatory/planar zoning at the
core region (Figure 7a). The outermost domain consists
of planar banded overgrowth with moderate CL response
(Figures 7b and c). Inherited cores in a few grains show
sector-zoning with brighter CL response compared to the
overgrowths (Figures 7d and h). The overgrowth domain is
5080mm thick and normally inclusion-free, but a fewbiotite akes were noticed in some grains. Some of these
grains show sector-zoning (Figures 7c and e), typically
found in zircon growing from anatectic melt (Vavra et al.,
1996; Schaltegger et al., 1999; Kelly et al., 2002; Kelly and
Harley, 2005). The oscillatory zoned domain is 50100mmin length often with abraded and angular outline. In a few
grains, the oscillatory zoned domain shows prominent
resorption (Figures 7f and i). In others, it is often blurred in
appearance and surrounded by a somewhat dark-CL domain
where faint traces of oscillatory zoning could be identied
(Figure 7g). Inclusions of biotite (both aky and sub-
rounded) and alkali feldspar are present within this domain.
The dark-CL domain surrounding the oscillatory zoned
domain shows evidence of recrystallization and resorption
presumably by a coupled dissolution reprecipitation process
(Geisler et al., 2007). The sharp contrast in CL responses and
Th/U ratios between the oscillatory zoned and the over-
growth domain suggest the former as inherited in origin.
Some of the oscillatory zoned zircon grains, however,
Figure 7. Cathodoluminescence (CL) images of analysed zircon grains showing internal structures and obtained ages. 207Pb-206Pb ages are shown inparentheses as quoted from Supplementary Table 5 with 1s uncertainty. Grain numbers are shown at the top left of each grain while spot numbers are labelled ineach spot. (a) Neoblastic grain, (b) Planar-zoned grain with detrital core, (c) Neoblastic grain with planar zoning, (d) Planar zoned overgrowth on multilayeredgrain with detrital core, (e) Sector zoned overgrowth on detrital core, (f) Planar zoned overgrowth on dark-CL core containing resorbed detrital core, (g)Oscillatory zoned grain showing faint traces of blurring of zoning towards the periphery, (h) and (i) Truncated bright-CL core surrounded by dark-CL
recrystallized zone.
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multiple tectonometamorphic imprints in the lower crust, egb, india 231
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preserve tiny relics of detrital core of rounded to irregular
outline.
Forty-four spots were analysed from 33 grains including
multiple spots from oscillatory zoned, recrystallized/
resorption and overgrowth domains. Spots from the
oscillatory zoned domain (four spots) show varying U
(2611176 ppm) and Th (133564 ppm) contents as
reected in a wide variety in the Th/U ratio (0.122.23).
Three spots give weakly discordant ages (36% discor-
dance) and show broadly similar Th/U ratio (0.120.37).207Pb-206Pb age spans ca. 16801710Ma with a weighted
mean of 1698 46Ma (95% conf., MSWD 2.7). Theother spot 33.1 shows a very strong reverse discordance,
even though the U content is below 300 ppm. An irregular
count of radiogenic Pb observed in this particular analysis
(and a few others as shown in Supplementary Table 5), could
be the major factor as noted in other studies (Compston,
1992; McFarlane et al., 2006). A large number of spots
were analysed from the dark-CL recrystallized/resorption
domain (n 20). This combined domain shows variable U(1702594 ppm), Th (43234 ppm) and Th/U ratios (0.06
0.95). Th/U ratios, however, lie in the much narrower range
of 0.060.29 except spot 1.1. Obtained ages are all
discordant (123%) in the range ca. 16001100Ma
(207Pb-206Pb age; Supplementary Table 5). Spot ages are
more concordant (14%) at the older age end and most
Figure 8. (a) TerraWasserburg diagram showing plots of data points. 24 data points from oscillatory zoned and recrystallized/resorption domains are used forcalculation of intercept ages. Three spots (out of four) from oscillatory zoned domain gives 207Pb-206Pb mean age of 1698 46Ma. A group of spots (n 7)from overgrowth and neoblastic grains denes a concordia age of 953 6Ma.Weighted average ofmean 207Pb-206Pb ages from a group of 6 data points from thesame domain denes an age of 902 17Ma. Reversely discordant data are not used for group age calculation. (b) and (c) Weighted average of mean ages of two
groups of data from overgrowth and neoblastic grain domain.
Copyright # 2010 John Wiley & Sons, Ltd. Geol. J. 46: 217239 (2011)
232 k. das ET AL.
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discordant (923%) at the midway. This observation and
internal structure convincingly prove that the recrystalliza-
tion/resorption domain developed due to disturbance of the
oscillatory zoned domain and obtained ages imply mixing of
two thermal events. When we combine all data from this
domain with data from the oscillatory zoned domain and plot
in the TerraWasserburg diagram, the mixing line shows
upper and lower intercepts of 1689 62Ma and934 57Ma, respectively (Figure 8a) with high scatter(MSWD 6.0). The upper intercept age is in the range ofcalculated mean age and signies the crystallization age of
oscillatory zoned domain, which we equate with the timing
of magmatism in the source region from which the sediment
was derived. This age is similar to that documented recently
from central part of EGB (Bose et al., 2008). The lower
intercept age broadly matches with ages from overgrowth
and neoblastic grain domains (discussed below).
Outer overgrowth and neoblastic grains show similar CL
characters and a narrow range of U (211585 ppm) and Th
(26142 ppm) contents. Th/U ratio mostly varies in the
range 0.20.4, while a few show lower (< 0.1) and highervalues (0.60.7). Analysed spots (n 20) give concordant toweakly discordant ages. A few grains show weak to
moderate reverse discordance as well due to irregular
radiogenic Pb count (discussed before). 207Pb-206Pb ages
spread in the range ca. 1020880Ma with a distinct
cluster near ca. 950Ma (Figure 8a). A concordant age of
953 6Ma (95% conf., MSWD 1.4) is obtained from agroup of seven spots. This is broadly similar to the mean207Pb-206Pb age of 949 10Ma (95% conf., MSWD 1.6;Figure 8b). These concordant and pooled ages imply that the
major growth of zircon took place at ca. 950Ma. Spots with207Pb-206Pb ages in the range ca. 9601020Ma (n 6) areweakly discordant (16%). It is noted that this age group is
shown by spots occurring at the central part of a neoblastic
grain with hidden cores (as spot 11.1) or inner part of the
overgrowth that partly overlaps with the oscillatory zoned
domain (spot 21.1). These spot ages are thus not used for
group age calculation. A group of six spots with similar CL
character and Th/U ratios give a younger mean age of
902 17Ma (95% conf., MSWD 1.9, Figure 8c). Thismay suggest partial modication of an older zircon by an
unrelated much younger event (Pan African?) during which
no new zircon growth took place. Alternatively, this age may
signify the nal crystallization of zircon from extracted melt
and associated hydration event (M3D4). In the absence of
new zircon growth during any event younger than 900Ma,
the latter possibility seems more reasonable. The three-fold
clustering of ages is very similar to geochronologic data
from similar rocks in the adjacent localities (Bose et al.,
2008) and possibly the entire central part of the EGB.
The Th/U ratio is an important criterion to distinguish zircon
produced by magmatic (Th/U> 0.1) and metamorphic (Th/U
< 0.1) process (Rubatto, 2002). Most of the analysed spots inthe present sample show a Th/U ratio in the range 0.50.1
(Figure 9a). Notably, spots from oscillatory zoned domain
are always showing Th/U > 0.1, while a few spots fromovergrowth domain show Th/U < 0.1. No clear correlationexists between Th/U ratio and spot age (Figure 9b). A simple
correlation of Th/U ratio and zircon forming process
(magmatic or metamorphic) is problematic because enrich-
ment and/or depletion of Th over U is a complex function of
multiple factors (as discussed by Harley et al., 2007). There are
examples of zircon of undisputed metamorphic origin where
Th/U ratio exceeds 0.1 that even reached up to > 1 (Hokadaand Harley, 2004; Kelly and Harley, 2005).
The timing of M1 metamorphism is difcult to determine
from mounted zircon grains since the textural contexts are
not properly understood. Texturally constrained monazite
grains, however, proved to be extremely useful for this
purpose. Monazite included within orthopyroxene and
associated with sapphirine grains (Figure 5c) are likely to
reect the timing of near-peak condition of M1 event since
the enclosing phases are demonstrably stabilized during the
peak (Figures 10a and b). A weighted average of U-Pb spot
Figure 9. (a) Plot of Th and U contents of all the spots from oscillatory-zoned, recrystallized and overgrowth/neoblastic grain domains. (b) Plot of
Th/U ratio and 207Pb-206Pb ages from all the analysed spots.
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multiple tectonometamorphic imprints in the lower crust, egb, india 233
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ages gives a mean of 987 11Ma, which is the best estimatefor this event (Figures 10c and d). This age broadly coincides
with a few spot ages from mounted zircon grains,
particularly those from the central part of neoblastic zircon.
Other textural varieties of monazite grains enclosed
within cordierite grains were also analysed for comparison.
Those yield spot ages close to 900Ma (grain 4 in
Supplementary Table 5), distinctly younger than the other
population. This ca. 900Ma monazite age broadly coincides
with a zircon U-Pb SHRIMP age for the overgrowth domain.
10. DISCUSSION AND CONCLUSIONS
Integrated structural, petrological and geochronological
study on a suite of aluminous granulites and associated
gneisses from the study area in the Eastern Ghats Belt attests
to polyphase tectonothermal evolution of the rocks. The
deformation history is presented schematically in Figure 11
depicting fold interference pattern arising out of three
deformational episodes. The isoclinally folded F2 has been
superposed by a broadly NWSE compression (D3) at low
angles to that of the D2 compression. This fold interference
produced upright gently plunging folds with NESW
trending axial trace. The D3 event also witnessed develop-
ment of localized shears accompanying F3. The nal
architecture of the fold interference is manifested by cross
folding at high angles during D4 producing a non-planar fold
and domal structure.
Aluminous granulites recorded polymetamorphic signa-
tures with an early counter-clockwise metamorphic evol-
ution (M1) culminating in UHT condition (> 10008C) at6.58.5 kbar, corresponding to a crustal depth of 2030 km.
The prograde path of M1 traversed from an initial high T-low
P condition, followed by loading contemporaneous with
D1D2 deformations. Since it is not possible to denitely
assign any mineral reaction specically to either D1 or D2,
we are constrained to amalgamate these together. Never-
theless, it is evident that extensive partial melting of the
protolith occurred during prograde metamorphism, followed
by limited melt segregation/extraction. Later thermal
relaxation of the crust was achieved by cooling (M1R)
down to 8008C, during the inter-kinematic gap D2D3. M2
Figure 10. Chemical age data from included monazite (Mnz) grains (a) associated with sapphirine (Spr) porphyroblasts and (b) included within orthopyroxene(Opx) from the studied samples. Note that both the sapphirine and the monazite grains are surrounded by same layer of sillimanite (Sil) corona. Spot ages are
plotted on the respective monazite BSE images. (c) Weighted mean age and (d) probability density plot for the analysed sample.
Copyright # 2010 John Wiley & Sons, Ltd. Geol. J. 46: 217239 (2011)
234 k. das ET AL.
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metamorphism was associated with a slight loading of the
cooled granulites, and was heralded by a compressive
event D3. D3 caused deep crustal shears accompanying
small- to regional-scale folds due to bulk SENW
compression. Crystal plastic deformation of ferromagnesian
minerals indicates shearing at elevated temperatures
under M2 granulite facies condition. It is likely that tectonic
squeezing during D3 caused partial melt extraction thereby
promoting mineral reactions. Since we identify D3 as a
distinct structural event superimposed on cooled granulites,
we propose that it is temporally unrelated to D1D2 and M1metamorphism. Regardless of the relative importance of
the two phenomena, viz. melt extraction and loading, in
promoting the mineral reactions during D3, we propose
that D3M2 is a distinctly separate tectonothermal event
superimposed on the cooled UHT granulites. Minor retro-
gression of the mineral assemblages occurred during D4 in
localized zones in the presence of melt. The tectonometa-
morphic history of the studied area is summarized in Table 1
and Figure 12.
Previous studies on the EGB granulites (summarized in
Dasgupta and Sengupta, 2003) also invoked granulite facies
re-metamorphism of isobarically cooled UHT metamor-
phosed rocks. While an anticlockwise PT trajectory has
been established for the UHT metamorphism (Sengupta
et al., 1990; Dasgupta et al., 1995), the PT path for the
second granulite metamorphism remained elusive. The
present study showed for the rst time a prograde history
Figure 12. The overall PT-t evolutionary history of the studied rockplotted on the FMAS grid to show the important stable mineral assemblages.The evolutionary path is drawn combining PT vectors from Figures 6b andc as well as geochronological data. The stability eld of SprOpxQtzand other UHT assemblages are drawn following the data of Kelsey et al.(2004). The post-M2 retrogressive segment is shown as a broken line
although there is no diagnostic textural feature present in the rock.
Figure 11. Schematic block diagram showing interference of folding developed by three episodes of deformation. Note the angular relationship between the F2and F3 fold axes and also the steeply dipping shear bands produced during the D3 event.
Copyright # 2010 John Wiley & Sons, Ltd. Geol. J. 46: 217239 (2011)
multiple tectonometamorphic imprints in the lower crust, egb, india 235
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(loading with/without heating) of the second granulite
metamorphism (M2 in this work synchronous to a high-
strain event triggering possible melt extraction). Available
geochronological data on the EGB rocks is inconclusive
with respect to the timing of M1 metamorphism (1.5 Ga,
Shaw et al., 1997; 1.11.2 Ga, Jarick, 2000, 1.11.25 Ga,
Simmat and Raith, 2008). A recent geochronological study
from the Ongole Domain of the southern part of EGB reveals
that the UHT metamorphism occurred at ca. 1.63 Ga
(Upadhyay et al., 2009). Data presented by Upadhyay et al.
(2009) further show that the timing of metamorphism in the
type Eastern Ghats Province within the EGB (of which the
present study area belongs) is much younger (ca. 1.2
0.5Ga). The monazite chemical age data presented in our
study suggest that the M1 event was much younger (ca.
1000Ma) than envisaged by previous monazite age data
(Simmat and Raith, 2008). Weakly to strongly discordant
ages from the oscillatory zoned domains in zircon with a
mean age of ca. 1700Ma probably record a magmatic event
in the source region (see Bose et al., 2008). The granulite-
grade overprint on the UHT M1 assemblages, which is
documented as M2 in the present study is considered to be of
younger age based on earlier isotopic data (1.00.95 Ga,
Grew and Manton, 1986; Shaw et al., 1997; Mezger and
Cosca, 1999; Simmat and Raith, 2008 and references
therein). SHRIMP U-Pb data from the present study yield a
concordant age of 953 6Ma, which tightly constrainsthe timing of M2 metamorphism. This event witnessed
growth of new zircon (neoblastic grains) as well as zircon
overgrowth on inherited zircon, possibly in the presence of
melt that has subsequently been extracted during the D3mevent. This sharply dened age of M2 event matches with the
thermal and structural events in the Rayner Complex
(ca. 940910Ma, Kelly et al., 2002; Harley, 2003; Halpin
et al., 2005, 2007). The UHT M1 metamorphism in the
central EGB is temporally unrelated to the crustal
development in the Rayner Complex. However, the timing
and deduced PT path of M2 overprint in the EGB is similar
to that in the Kemp Land and Oygarden areas of the Rayner
Complex (Harley, 2003; Kelly and Harley, 2005). Ayounger
pooled age of ca. 900Ma in the studied rock possibly
signies the M3D4 event when zircon grains nally
crystallized from the extracted melt. This is again similar
to the timing of zircon growth during the D3D4 events in
rocks from Oygarden area of the Rayner Complex (Kelly
et al., 2002). Moreover, a striking similarity between the D3structural characteristics in the present study area and D3D4structural reworking in the Oygarden area (Kelly et al.,
2000) reinforces the notion that the EGB and Rayner
Complex shared a common geologic history from ca.
950Ma to ca. 900Ma as parts of Rodinia.
The present study provides record of a prolonged
geological history spanning nearly 800Ma (ca. 1700
900Ma) in the EGB, which is far longer than what has been
conceived so far. Though the retrievable tectonometa-
morphic history ranges from ca. 1000Ma to ca. 900Ma, the
earliest ca. 1700Ma age domain from zircon is intriguing, as
similar ages are reported from southern and central parts of
the EGB in recent times (Bose et al., 2008). Moreover,
tectonothermal events of this age have been reported from
different crustal blocks of India (Sarkar et al., 1989, Buick
et al., 2006) as well as crustal blocks of Antarctica,
Australia, North China and Laurentia (Goodge et al., 2001).
This timeframe witnessed the growth of the supercontinent
Columbia (Rogers and Santosh, 2002, 2009; Zhao et al.,
2004; Santosh et al., 2009). Future research in the EGB
needs to be aimed at understanding the signicance of
the older ages. The EGB rocks, however, record a more
pervasive tectonothermal imprint during the assembly of
Rodinia.
ACKNOWLEDGEMENTS
Authors thank Dr Ichiro Ohnishi for the EPMA analyses data
of biotite in certain key microdomains. T. Kuwajima, H.
Nomura andM. Ikeda of Hokkaido University helped during
analysis. They also thank Dr N.C. Pant for monazite EMP
analysis. Insightful comments by Drs. S.K. Bhowmik and T.
Tsunogae helped to improve the quality of the manuscript.
Simon Harleys comments and suggestions on an earlier
version of this manuscript were very helpful during sub-
sequent revision. Editorial handling by M. Santosh is thank-
fully acknowledged. KD and SB acknowledge DST,
Government of India for a research grant. SK has been
supported by the CAS programme of Jadavpur University.
SB acknowledges the Japan Society for the Promotion of
Science (JSPS grant no. 07043) for working in Yokohama
National University in collaboration with the National Insti-
tute of Polar Research, Japan. SB was also supported by
FIST programme of DST of Government of India at
Presidency College. SDG acknowledges nancial support
from the DST, Government of India through J.C. Bose
Fellowship.
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