Magmatic and metamorphic imprints in 2.9 Ga chromitites from the Sittampundi Layered Complex, Tamil...
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Magmatic and metamorphic imprints in 2.9 Ga chromitites from the Sittam-pundi Layered Complex, Tamil Nadu, India
Upama Dutta, Uttam K. Bhui, Pulak Sengupta, Sanjoy Sanyal,D.Mukhopadhyay
PII: S0169-1368(11)00052-7DOI: doi: 10.1016/j.oregeorev.2011.05.004Reference: OREGEO 856
To appear in: Ore Geology Reviews
Received date: 28 December 2009Revised date: 12 May 2011Accepted date: 15 May 2011
Please cite this article as: Dutta, Upama, Bhui, Uttam K., Sengupta, Pulak, Sanyal,Sanjoy, D.Mukhopadhyay, Magmatic and metamorphic imprints in 2.9 Ga chromititesfrom the Sittampundi Layered Complex, Tamil Nadu, India, Ore Geology Reviews (2011),doi: 10.1016/j.oregeorev.2011.05.004
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Magmatic and metamorphic imprints in 2.9 Ga chromitites from the Sittampundi
Layered Complex, Tamil Nadu, India
Upama Dutta1, Uttam K. Bhui1, Pulak Sengupta1,**, Sanjoy Sanyal1, D.Mukhopadhyay2
1Department of Geological Sciences, Jadavpur University, Kolkata 700032, India
2Department of Geology, University of Calcutta, 29, Ballygunge Circular Road, Kolkata 700019, India
Abstract
The c.2.9 Ga old Sittampundi layered complex (SLC) of South India belongs to a special group of
deformed and metamorphosed Archaean rocks where chromitites are interlayered with anorthosite.
Detailed field studies have revealed that the SLC comprises of a sequence of magmatic rocks
consisting of clinopyroxenite, anorthosite and mafic rocks of tholeiitic composition. Minor BIF
(Banded Iron Formations) intercalated with the mafic rocks are the only sedimentary rock within the
SLC. Chromitite occurs as continuous to discontinuous bands (a few mm up to 6 m thick) within
clinopyroxenite and highly calcic anorthosite (An 99-100) but never in the enclosing mafic rocks.
Chromite occurs broadly in three textural types: (a) cumulus grains in chromitite layers; (b)
disseminated grains in clinopyroxenite and anorthosite; and (c) small grains included in clinopyroxene
and plagioclase. A suite of felsic magma intruded the SLC at c.2.51 Ga. Subsequently the entire rock
sequence underwent polyphase deformation and metamorphism at c.2.50-2.45 Ga (granulite facies) and
at 0.72–0.50 Ga (amphibolite facies). During the latter event, extensive alteration of clinopyroxene to
amphibole and chlorite, of plagioclase to clinozoisite and of chromite to Cr-poor green spinel took
place.
* Corresponding author. Tel.: +91 33 24152782. E-mail addresses: [email protected]
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Chromite compositions show large variations (Cr# = 26-60, Mg# = 4-45, Fe3+# = 2-24) depending
upon textural type and nature of the associated phases. The most conspicuous compositional variation
took place when chromite was metasomatically replaced by green spinel (Cr# = 3-21; Mg# 45-61)
during amphibolite facies metamorphism. On a Cr# vs. Mg# plot, pristine magmatic compositions of
chromite define an array that suggest increasing Cr# with concomitant decrease in Mg#, presumably
during magmatic fractionation. Highly calcic plagioclase in anorthosite and Fe-Al rich chromite in
chromitite in the SLC are consistent with a hydrous parental magma of tholeiitic composition. This
hydrous magma was generated in an oceanic arc environment and crystallized close to the surface of
the earth. In terms of mineralogy and field relations, chromitite-bearing rocks of the SLC show
remarkable similarity with the Archaean anorthosite-hosted chromitite deposits in layered magmatic
complexes at Fiskenaesset (Greenland) and Messina (South Africa) but contrasts sharply with the
chromitite deposits of Proterozoic and Phanerozoic age. A change in the style of arc magmatism
appears to be the controlling factor for marked change in chromite compositions across the Archaean-
Proterozoic boundary.
Keywords: Chromitite; Anorthosite; Archaean; Sittampundi layered complex; Arc magma.
1. Introduction
Studies in the past two decades have revealed that the Earth’s mantle has undergone significant
physical and chemical changes over geological time (reviewed in Rollinson, 2007). Episodic melting,
extraction of melts from the mantle and contamination of materials from the subducted slab to the
overlying mantle wedge are considered to be primarily responsible for chemical evolution of the mantle
(Rollinson, 2007). Because of slow mixing rates and slow rates of diffusion, mantle heterogeneities are
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preserved over a long time (≥1 Ga, Rollinson; 2007). This observation makes mantle-derived magmas a
potential tool for deciphering chemical evolution of the mantle. Anorthosite-bearing layered magmatic
complexes represent an important component of mantle-derived magmatic rocks that range in age from
Archaean to Phanerozoic (Ashwal, 1993). On the basis of form, structure and plagioclase composition,
Precambrian anorthosites are broadly divided into layered- and massif-types (reviewed in Ashwal,
1993). The Archaean layered anorthosite complexes are hosted in high-grade metamorphic terrains, and
are complexly deformed and metamorphosed along with their host rocks (Windley et al., 1981). Most
post-Archaean layered complexes (e.g., Bushveld complex, Stillwater complex), on the other hand,
occur as sill like bodies, and are mostly undeformed and unmetamorphosed (Hatton and von
Gruenewaldt, 1990; Ashwal, 1993; Stowe, 1994). Chromite, which is considered to be an important
petrogenetic indicator (Irvine, 1965, 1967), occurs in many of the Precambrian layered anorthosite
complexes (Hatton and von Gruenewaldt, 1990; Ashwal, 1993; Stowe, 1994; Rollinson et al., 2002).
Detailed petrological characterization of chromite deposits in Archaean layered complexes should,
therefore, provide invaluable information about the enigmatic mantle processes in early Earth history.
Existing information has indicated that chromite in Archaen layered complexes has distinct
compositions that contrast sharply with the chromite compositions in Proterozoic and Phanerozoic
rocks (Rollinson et al., 2002). Plagioclase in Archaen layered complexes is also highly calcic compared
to their younger counterpart (Ashwal, 1993). However, examples of Archaean layered complexes are
limited, and detailed information on chromite is hitherto available only from two complexes: 1)
Fiskenaesset, Greenland and 2) Messina, South Africa (Windley et al., 1981; Ashwal, 1993; Rollinson
et al., 2002).
Highly deformed and metamorphosed layered complexes of Bhavani (BLC) and Sittampundi (SLC)
of south India have been known for their anorthosite and chromitite for a long time (Subramanium,
1956; Ramadurai et al., 1975; Windley et al., 1981; Srikantappa et al., 2003). Recent geochronological
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studies have unequivocally demonstrated that both the layered complexes were formed within late
Archaean time (ca. 2.9-2.8 Ga; Bhaskar Rao et al., 1996; Ghosh et al., 2004). Detailed study on this
important Archaean chromite deposit in the light of recent advances of the subject is lacking and is the
subject of this communication. Here we present field relations, textural features and compositional
characteristics of chromite deposits from the SLC. Interpreting the petrological features of SLC and the
rocks of a wider area, an attempt has been made to (a) compute composition and depth of emplacement
of parental magma from which magmatic rocks of the SLC were formed (b) constrain the probable
tectonic setting where the SLC might have been emplaced, (c) asses the nature and extent of
compositional modifications of magmatic chromite during fluid-induced metamorphism and (d)
compare and contrast the geological history of the SLC with other well studied chromite deposits
associated with Achaean layered magmatic complexes.
2. Geological background
The granulite terrain of south India is considered to be a mosaic of crustal domains with distinctive
geological and geochronological characteristics (Braun and Kriegsman, 2003; Bhaskar Rao et al., 2003;
Ghosh et al., 2004). A number of crustal-scale shear zones are presumed to have divided the entire
granulite belt into three major domains (Fig. 1). The northernmost domain, the northern granulite
terrains (NGT), exposes an assemblage of mafic, ultramafic and volumetrically major felsic
orthogneisses that underwent a latest high-grade event at ca. 2.6-2.5 Ga whereas the southernmost
domain (Madurai Block or MB) shows a latest high-grade event at a much younger age (ca. 0.6-0.5 Ga;
Chetty, 1996; Braun and Kriegsman, 2003; Bhaskar Rao et al., 2003; Chetty et al., 2003; Ghosh et al.,
2004). The NGT and MB are separated by a roughly E-W trending belt. The rock associations in this
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belt show complex magmatic, metamorphic and deformational history over a protracted period from
2.9 Ga to 0.5 Ga (Braun and Kriegsman, 2003; Bhaskar Rao et al., 2003; Mukhopadhyay et al., 2003;
Ghosh et al., 2004, Raith et al., 2010). Several crustal-scale shear zones are believed to have affected
the rocks of this linear belt for which is often referred to as the Cauvery Shear System (CSS, Chetty,
1996; Fig. 1). The CSS that is dissected by ductile to brittle shears is believed to have a protracted
geological history with major reactivation at ca. 0.6-0.5 Ga (Meissner et al., 2002; Srikantappa et al.,
2003). An assemblage of mafic-ultramafic-anorthosite-felsic orthogneisses is the dominant rock
association of the CSS.
A number of layered magmatic complexes with or without economically viable chromite deposits
are located in the CSS, of which the layered complexes of Bhavani (BLC) and Sittampundi (SLC) have
been studied in some details (Fig. 1; Subramanium, 1956, Janardhan and Leake, 1975, Anbarasu et al.
2011, Bhaskar Rao et al., 1996, 2003; Ghosh et al., 2004). The first systematic study on the rocks of
SLC was done by Subramanium (1956). Existing geochronological data indicate that the layered
complexes were emplaced at c. 2.9 Ga (Subramanium, 1956; Bhaskar Rao et al., 1996; Ghosh et al.,
2004). A suite of felsic magmas now represented by enderbite and charnockite (felsic orthogneiss)
subsequently intruded the members of the SLC. The entire ensemble of mafic, ultramafic and felsic
rocks underwent deformation accompanied by high-grade metamorphism at ca. 2.450-2.45 Ga and by
amphibolite facies metamorphism during ca. 0.72-0.50Ga (Bhaskar Rao et al., 1996; Meissner et al.,
2002; Ghosh et al., 2004). Late Archaean and Neoproterozoic tectonothermal activities obliterated the
primary magmatic features of the layered complexes in most places although vestiges of rhythmic
interlayering among anorthosite, chromitite and clinopyroxenite are present and are considered to be of
magmatic origin (Subramanium, 1956). The BLC locally shows nearly complete magmatic stratigraphy
(see Fig. 2b). The sequence starts with a unit of olivine-rich ultramafic rocks e.g., harzburgite, wehrlite
and dunite (now extensively altered to serpentinite and magnesite) which is overlain successively by
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clinopyroxenite, leucogabbro / anorthosite and basaltic rocks (now garnetiferous mafic granulites) (Fig.
2b). Chromite occurs as thin layers and disseminated grains within the olivine-rich ultramafic rocks.
BIF is intercalated with the top mafic unit of the sequence in a few places (Fig. 2b). Extant geological
and geochronological information have shown that the late Archaean high-grade rock ensemble of the
CSS remained undisturbed for a protracted period until these rocks were polydeformed, intruded by
voluminous granitoids and were extensively retrogressed during the Pan-African tectonothermal events
(ca. 0.72-0.5 Ga: Bhaskar Rao et al., 2003; Ghosh et al., 2004). Proximal to the boundary with the MB,
the CSS exposes a packet of young supracrustal rocks (now represented by marble, calc-silicate rocks
and metapelites) having an average crustal residence age of 1.9 Ga (Fig. 1; Meissner et al., 2002).
Locally the metapelites contain blocks of granulite-grade BIF suggesting that the sediments were
deposited on the ca. 2.5 Ga granulite basement (Ghosh et al., 2004). These supracrustal rocks
underwent prograde metamorphism that culminated at 9±1 kbar and 700±50 °C on a clockwise P-T
trajectory (Meissner et al., 2002; Sengupta et al., 2009a). Geochronological data bracket the age of
metamorphism of these supracrustal rocks within ca. 0.61-0.52 Ga (Meissner et al., 2002; Raith and
Srikantappa, 2008).
3. The Sittampundi layered complex (SLC)
3.1. Magmatic and metamorphic events in the SLC and the enclosing rocks
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The generalized geological map of the SLC showing dispositions of the different lithologies is
presented in Fig. 2a. The rocks of this magmatic complex and the adjoining areas have been studied by
a number of authors (Subramanium, 1956; Ramadurai et al., 1975; Bhaskar Rao et al., 1996, 2003;
Mukhopadhyay et al., 2003; Ghosh et al., 2004; John et al., 2005; Shimpo et al., 2006; Sengupta et al.
2009 a, b, among others). The SLC comprises an intercalated sequence of clinopyroxenite, anorthosite
and a suite of mafic rocks now represented as mafic granulite with the mineralogy clinopyroxene +
plagioclase ± orthopyroxene ± garnet ± amphibole (Bhaskar Rao et al., 1996; Ghosh et al., 2004; our
unpublished data). Although dm to cm-thick chromitite layers are present in clinopyroxenite and
anorthosite, thick bands (up to 6 meter thick, Subramanium, 1956) of economic-grade chromite occur
only in clinopyroxenite (now extensively retrograded to amphibolite).
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Extant geochemical and Nd-isotope data indicate that the mafic–ultramafic rocks of the SLC are co-
genetic and show a fractionation trend akin to that of tholeiitic magma (Bhaskar Rao et al., 1996). A ca.
2.9 Ga emplacement age for the SLC has been established by whole-rock Sm-Nd isochron and U-Pb
dating of zircon (Bhaskar Rao et al., 1996; Ghosh et al., 2004). Vestiges of Banded Iron Formation
(BIF), which represent the sole sedimentary component in the magmatic sequence and are intimately
associated with the mafic rocks of the SLC, show cm to mm thick compositional layers alternatively
rich in magnetite + pyroxene and quartz (Fig. 3a, b). The compositional banding of BIF, that
presumably represent primary sedimentary layering can be traced laterally for several meters. Owing to
repeated folding actual number of BIF layers in the mafic host cannot be determined. The SLC is
surrounded by felsic orthogneiss (Fig. 2; ca. 2.51 Ga emplacement age; Ghosh et al., 2004), which
contains fragments of mafic-ultramafic rocks including xenoliths of dunite, harzburzite and wherlite
(Fig. 3c), and sends apophyses into the rocks of the magmatic complex. Field studies together with
extant geochronological data indicate that subsequent to the emplacement of felsic magma, the
ensemble of ca. 2.9-2.51 Ga rocks underwent polyphase deformation at ca. 2.50-2.45 Ga (granulite
facies) and at ca. 0.72-0.50 Ga (amphibolite facies) (Bhaskar Rao et al., 1996; Ghosh et al., 2004; Raith
et al., 1999). The high-grade metamorphism that produced garnet and orthopyroxene-bearing
leucosomes in felsic rocks and megacrystic garnet in mafic rocks and BIF were culminated at 9.5 ± 1
kbar and 800 ± 50 oC (Bhaskar Rao et al., 1996; our unpublished data). Recently, from one locality
near SLC, Sajeev et al. (2009) reported mafic rocks that shows ultra-high pressure metamorphism (>20
kbar) and interpreted it as slices of mantle rocks that exhumed during Neoproterozoic metamorphism.
During the Neoproterozoic (ca. 0.72-0.50 Ga) events voluminous granitoid batholiths intruded the high
grade Archaean rocks. Extensive retrogression of high-grade rocks particularly at the contact of these
granitoid batholiths transformed the granulites facies pyroxenes and feldspars to secondary minerals
principally amphibole, chlorite, epidote and biotite at distinctly lower P-T conditions (650 ± 50 °C, 6-7
kbar, Bhaskar Rao et al., 1996; Sengupta et al., 2009 a, b). Prismatic amphibole and megacrystic
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corundum (ruby) with coronitic green spinel having variable thickness (Fig. 3d) were developed in
anorthosite during this retrogressive event. Randomly oriented amphibole and chlorite grains and
preservation of delicate corona of green spinel around corundum suggest static condition at the time of
growth of these secondary minerals. ca. 540 Ma concordant U-Pb zircon date from one small granitoid
pluton fixes the age of emplacement of these granitoids (Ghosh et al., 2004). In most places, the
original magmatic relations among the rocks of the SLC are obscured due to superposed deformation
and polyphase metamorphism and hydration. Nevertheless, a generalized magmatic stratigraphy has
been developed integrating all the field features (Fig. 2b). Except for the presence of thick chromite
seams and lack of olivine-rich ultramafic rocks the magmatic stratigraphy and the age of emplacement
of the SLC bear striking resemblance with the BLC (Fig. 2b). However, the possibility that olivine-rich
rocks may occur beneath the exposed section of the SLC cannot be ruled out in view of the presence of
dunite and wehrlite xenoliths in the felsic gneiss whose protolith intruded the magmatic complex, and
might have sampled the lower part of the complex. Features such as (a) occurrence of chromite-bearing
ultramafic enclave in mafic rocks, and (b) presence of tongues of mafic rocks in anorthosite corroborate
the view that mafic rocks represent the uppermost part of the SLC. Intimate association of mafic rocks
with BIF which is presumed to have deposited as chemical sediments also corroborates this view.
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Chromite occurs in a number of forms in the SLC. In the most abundant mode, thin to thick chromitite
(up to 6 meter thick) seams are present within clinopyroxenite layers (Fig. 3e). These banded
sequences of chromitite and pyroxenite that can be traced laterally for a distance of more than
500 meters are presumed to be of magmatic origin. In another mode, mm to cm thick
chromitite layers occur within anorthosite (Fig. 3f, g). Intense post-crystallization deformation
affected the chromitite layers and its host clinopyroxenite and anorthosite. There is pinch and
swell and boudin structure in the competent chromitite layers (Fig. 3f). Intense Neoproterozoic
deformation also caused intricate folding of interlayered anorthosite and chromitite (Fig. 3g).
In places, green-spinel rich veins (confirmed by petrography) were found along the extension
direction of deformed chromite seams (Fig. 3d). Chromite layers are absent in the adjoining
mafic rocks.
3.2. Mutual relations between chromite and associated phases
Detailed petrographic study of anorthosite and clinopyroxenite are beyond the purview of this
communication. In the following sections, salient petrographic features of these rocks that have direct
relation on the formation and alteration of chromite will be described.
3.2.1. Chromite in thick chromitite layers and in host clinopyroxenite
In the thick chromitite layers, coarse chromite grains show a typical cumulus texture (Fig. 4a),
which is partially modified by superposed deformation. However this texture will be referred to as
cumulate texture. Commonly, volume of cumulus chromite exceeds 90 vol.%. Minor (<10 vol.%)
secondary amphibole and chlorite (Fig. 4a) occupy the interstitial spaces of coarse chromite grains.
Locally, inclusions of corroded clinopyroxene were found in secondary amphibole. Secondary chlorite
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grains replace secondary amphibole and rarely coexist with calcite. Cumulus chromite grains show
minor (≤2 vol.%, estimated from visual inspection and image analyses) crystallographically oriented
fine needles of rutile (Fig. 4b). Granular rutile grains locally surround cumulus chromite grains in a few
places (Fig. 4a). These features indicate that rutile was “exsolved” from and migrated out of the host
chromite grains during cooling (Subramanium, 1956, Mitra and Samanta, 1996). In the host
clinopyroxenite, small chromite grains are either included in the cumulus clinopyroxene (Fig. 4c) or
disseminated in the interstitial space formed by cumulus clinopyroxene grains. Alteration of
clinopyroxene to amphibole (Fig. 4c) is a common feature in these rocks.
3.2.2. Chromite in anorthosite
In thin chromitite layers in anorthosite, small grains of plagioclase and clinopyroxene that are in
different stages of alteration to amphibole and chlorite occur in the interstitial space formed by cumulus
chromite grains (Fig. 4d). The proportion of interstitial silicate minerals is distinctly higher (10-30 vol.
%) than in the thick chromitite layers in clinopyroxenite. In the host anorthosite, recrystallization of
magmatic plagioclase develops a polygonal grain mosaic (Fig. 4e). A few megacrystic plagioclase
grains that are set in polygonal matrix grains show impress of deformation manifested by kinked twin
lamellae, undulose extinction and formation of polygonal sub-grains. All these features suggest that the
grain size of magmatic plagioclase in anorthosite was much larger than what is seen now. Disseminated
chromite grains occur at the triple-point junctions of the polygonal plagioclase grains as well as
inclusions within clinopyroxene (Fig. 4f). Aggregates of the secondary minerals amphibole, chlorite,
calcite and clinozoisite partially replace polygonal grains of clinopyroxene, plagioclase and
disseminated chromite grains. Large stumpy grains of corundum (corundum 1) are embedded in a
matrix made up of polygonal plagioclase grains (Fig. 4g). These corundum grains developed coronitic
green spinel of variable thickness (Fig. 4g). Green spinel protrudes into the adjacent polygonal
plagioclase grains (Fig. 4g). The coronitic green spinel breaks down to an aggregate of granular
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corundum (corundum 2), magnetite and chlorite (Fig. 4g). Green spinel that occurs in veins in stretched
chromitite layers contains relics of chromite at the core of it and replaced the latter mineral to different
extent (Fig. 4h-i). Appel et al. (2002) described a similar feature from Greenland and attributed it to
melt-chromite interaction at a late stage of magmatic evolution. However, microstructural features
described before corroborate the view that replacement of chromite by green spinel in the SLC
occurred during or after regional deformation (see also below).
4. Mineral chemistry
4.1. Compositional variation of chromite in the SLC
Compositions of chromite from different textural types are presented in Fig. 5a, b and Table 1a.
Spot analyses of chromite show uniformly low TiO2 (≤0.43 wt.%) and Fe3+ (0.05 to 0.47 atom per
formula unit; a.p.f.u.) contents, irrespective of its association and textural type (Table 1a). The presence
of rutile as fine exsolution lamellae in as well as granules along the periphery of cumulus chromite
grains suggest that the primary (magmatic) chromite had higher TiO2 content than those represented by
spot analyses. Considering low volume of the exsolved rutile, TiO2 content of cumulus chromite never
exceeded 0.5 wt.%. Depending on the textural types, chromite grains marked variation on Cr#
(100×Cr/(Cr+Al)) vs. Mg# (100×Mg/(Mg+Fe2+)) plot (Fig. 5a). Cumulus chromite grains from
chromitite layers in clinopyroxenite and in anorthosite define an array, which is characterized by
reverse relation between Mg# and Cr# with larger range of the former compared to the latter (Fig. 5a).
No significant compositional variation was noted between core and rim compositions in individual
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cumulus chromite grains in the chromitite layers (Table 1a). Even when the cumulus chromite grains
coexist with volumetrically minor silicate grains, compositional profile in the former show only minor
change in terms of Mg#, Cr# and Fe3+# on few microns in the rim whereas the core regions have
virtually uniform compositions (Fig. 5b). All these features attest to the view that the primary
composition of cumulus chromite, particularly at the core region of these grains, did not change
significantly during subsolidus and metamorphic processes. Volumetrically minor and disseminated
chromite grains, on the other hand, show significant post-magmatic compositional modification. At the
contact with metamorphic amphibole, disseminated chromite grains show the highest Cr# and lowest
Mg# (Fig. 5a). This may be attributed to the loss of Al (relative to Cr) and Mg (relative to Fe2+) in
chromite due to exchange of elements between amphibole and chromite during amphibolite facies
metamorphism (Beeson and Jackson, 1969; Murck and Campbell, 1986; Kimball, 1990; Rollinson,
1995; Rollinson et al., 2002). The most conspicuous compositional variation was observed in chromite
grains that coexist with green spinel (Fig. 5a). Compositions of these chromite grains define a positive
array showing reverse relation between their Mg# and Cr# (Fig. 5a). This compositional trend is
steeper than the ‘magmatic crystallization’ trend defined by cumulus chromite, and the two trends meet
at Cr#~50 and Mg#~25 (Fig. 5a). This compositional variation trend that is associated with
replacement of chromite by green spinel is consistent with the coupled substitutions of the types
MgFe2+-1 and AlCr-1 (Fig. 5a).
This trend of compositional variation in the chromite in spinel-rich veins has marked resemblance
with the ‘replacement trend’ described by Rollinson et al. (2002) from the Fiskenaesset complex. The
authors attributed this ‘replacement trend’ to melt-chromite interaction during the late stage of
magmatic history of the layered complex of Fiskenaesset, Greenland. However, the following features
support that in the studied area replacement of chromite by green spinel occurred during amphibolite
facies metamorphism:
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a) Cumulus chromite grains were replaced by green spinel in the extensional fractures in the deformed
chromitite layers in anorthosite (Figs. 3d and 4i-h).
b) Corona of green spinel also formed around the stumpy corundum crystals that were set in the
recrystallized polygonal aggregates of plagioclase in anorthosite (Figs. 3d and 4g). Existing
petrological and geochronological information suggest that the deformation of anorthosite and
chromitite occurred during Pan-African (0.72-0.50 Ga) tectonothermal events (Bhaskar Rao et al.,
1996; Ghosh et al., 2004). Composition of coronitic green spinel over corundum 1 effectively lies along
the hercynite-pleonaste join (Mg#=45-61, Cr#=3-21) with insignificant Ti and Fe3+. Estimated
temperature of 650 ± 50 °C ( Bhaskar Rao et al., 1996; Srikantappa et al., 2003; Sengupta et al., 2009a,
b) during the Pan-African metamorphism in the area is suitable for coexistence of Al- and Cr-rich
spinels (Sack and Ghiorso, 1991).
4.2. Compositions of the associated phases
In clinopyroxenite and anorthosite, the clinopyroxene is diopside (Mg#=85 to 90, Table 1b).
Clinopyroxene (diopside) in clinopyroxenite is distinctly lower in Al2O3 (<0.56 wt.%) than the
clinopyroxene in anorthosite (0.76 to 6.67 wt.%, Table 1b). This difference in the Al2O3 content of
clinopyroxene possibly mimics the bulk Al2O3 content of rocks in which clinopyroxene grew. Cr2O3
(<0.62 wt.%) and TiO2 (0.03-1.09 wt.%) content of clinopyroxene are low (Table 1b). The CaSiO3
component of diopside ranges between 0.46-0.52 (Table 1b). Individual grains do not show any
significant compositional zoning. Irrespective of the mode of occurrence, plagioclase is almost end-
member anorthite (≥99 mol.%, Table 1c).
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Secondary amphibole shows marked compositional variation depending upon the associated
phases. Amphibole from the thick chromitite and clinopyroxenite is less aluminous (3.9-12.9 wt.%
Al2O3 and 0.65 to 2.15 Al a.p.f.u.) and slightly more magnesian (Mg#=82-91) compared to amphibole
in anorthosite (11.8-14.8 wt.% Al2O3; 2.00 to 2.52 Al a.p.f.u., Mg#=76-85, Table 1d). TiO2, Na2O and
Cr2O3 contents of amphibole varies in different association. TiO2 varies within the range 0.33-1.20 wt.
%; whereas Na2O and Cr2O3 varies in the range of 0.59-2.14 wt.% and 0.04-1.79-wt.%, respectively
(Table 1d). Amphibole in anorthosite has higher TiO2 and Na2O compared to amphibole in
clinopyroxenite and chromitite (Table 1d). According to the amphibole nomenclature of Leake et al.
(1997), the composition ranges from magnesio hornblende to pargasite to tschermakite (Table 1d).
Chlorite is the most magnesian phase in the rock (Mg#>90, Al2O3 ~20-22 wt.% Table 1e). Cr2O3
content of chlorite varies from 1.54 to 3.85 wt.%. The most Cr-rich chlorite grains are at physical
contact with chromite. This mineral contains insignificant TiO2.
Corundum contains 0.33-0.75 wt.% Fe2O3 and 0.05-0.12 wt.% Cr2O3 (Table 1f) whereas clinozoisite
contains ~5 mol.% pistacite molecule (Table 1f). Carbonate is almost pure CaCO3.
5. Physico-chemical conditions during crystallization of chromite in the SLC
5.1. Nature of the parental melt of the chromitite-bearing rocks of Sittampundi
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In the absence of chilled margin and the presence of high variant chromite-bearing assemblages
estimation of parental melt composition of the SLC is not very straightforward. Nevertheless, certain
mineral-chemical observations made in this study in combination with results of the existing
experimental studies shed some light on the composition of melt from which the chromitite-bearing
rocks of the studied area might have crystallized. This study has demonstrated that highly calcic
plagioclase (>An98), clinopyroxene and Fe-Al rich chromite were the liquidus phases in anorthosite
(clinopyroxene and Fe-Al chromite in case of clinopyroxenite). Compositions of the liquidus phases are
consistent with the view that the melt from which these minerals were formed was rich in Al, Fe and Cr
and poorer in silica, alkalis, Ti and Mg (Rollinson et al., 2010). Composition of chromite has long been
used as a proxy for the composition of the melt that deposited the chromite (Maurel and Maurel, 1982;
Kamenetsky et al., 2001). In the Cr# vs. Mg# plot, the chromites of SLC follow a trend with
progressive Fe and Cr enrichment (Fig. 5a). When the graphical methods of Kamenetsky et al. (2001)
are used, the most primitive compositions of chromite (having the highest Mg#) that represent core
compositions of cumulus chromite not in physical contact with any other Fe-Mg bearing minerals,
suggest that the parental melt contained up to 18 wt.% Al2O3 and low TiO2 (<0.6 wt.%) (Fig. 6)
Integration of small volume proportion of exsolved rutile lamellae with their host chromite composition
would marginally enhance the TiO2 content of the estimated melt composition. It is to be noted that the
most primitive chromite compositions of the SLC are aluminous that evolved to more Fe- and Cr- rich
composition presumably during crystal fractionation. The compositional array of the chromite in the
SLC follows the same trend that is defined by the anorthosite hosted chromites of the Fiskenaesset
complex of Greenland (Rollinson et al., 2010). REE pattern of the anorthosite and mafic granulites of
the SLC (Bhaskar Rao et al., 1996) and Fiskenaesset complex (Polat et al., 2009) are similar. In view of
similarity in terms of chromite chemistry and the REE pattern of enclosing mafic rocks and anorthosite
between the SLC and Fiskenaesset complex, it is presumed that both the complexes share a similar
petrogenetic history. This involved early fractionation of magnesian phases (olivine, orthopyroxene)
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from a tholeiitic parental magma that depleted the residual liquid in Mg and silica and enriched in Ca,
Cr, Al and Fe The evolved composition of the melt then triggered the precipitation of Fe-Al rich
chromite and highly calcic plagioclase (Polat et al., 2009; Rollinson et al., 2010). Presence of dunite,
wehlite and harzburzite xenoliths in younger felsic magma (protoliths of enderbite) further corroborates
this view.
5.2. Depth and crystallization history of chromitite in the SLC: significance of highly calcic
plagioclase
Lack of contact aureole and the presence of high variant primary mineral assemblage make
estimation of the depth of emplacement of chromitite seams difficult. Nevertheless, intimate
association of BIF with the mafic rocks suggests that SLC were emplaced at a relatively shallow depth.
Further insight about the depth of emplacement of the magmatic rocks can be achieved from the
stability of highly calcic plagioclase (>An98) in the anorthosite of the SLC.
Experimental studies have demonstrated that the KD Ca-Na (plag-melt) increase abruptly with a small
increase in H2O in the basaltic melt (Sisson and Grove, 1993; Berndt et al., 2005; Takagi et al., 2005;
Feig et al., 2006). Total pressure was shown to have little or no effect on this distribution coefficient
(Sisson and Grove, 1993). In view of these factors, the parental melts of the chromite-bearing
clinopyroxenite and anorthosite of the SLC are presumed to be hydrous. The highly calcic plagioclase
(>An90) that are reported by Takagi et al. (2005) and Arculus and Wills (1980) from hydrous arc basalts
justify our presumption. Recent experimental data of Feig et al. (2006) demonstrate the influence of
H2O on the crystallization sequence of a tholeiitic melt, a likely analogue of the parental melt of the
SLC. The phase diagrams of Feig et al. (2006) are shown in figure 7a-d. It is evident from Fig. 7a-b
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that clinopyroxene can crystallize before plagioclase at low pressure (≤2 kbar) if the melt has more than
3 wt.% H2O. For water saturated melt, clinopyroxene touches liquidus before plagioclase at pressure
close to only 1 kbar (Fig.7d). Enlargement of the stability field of clinopyroxene at higher H2O content
was also documented by Hamada and Fujii (2008). Olivine always crystallizes before clinopyroxene
irrespective of the H2O content of the melt at least up to 5 kbar (Fig. 7a-c). At ≥2 kbar, field of
orthopyroxene expands so much that this mineral will be a liquidus phase at all temperatures above
1100 °C (Fig. 7c). The absence of orthopyroxene in the anorthosite and chromitite-bearing pyroxenite
in the SLC, therefore, seems to be consistent with the fact that the parental magma(s) of the SLC was
emplaced at shallow depth (<2 kbar, corresponding to a maximum depth of ca. 6 km). Figures 7a-c also
demonstrate that amphibole does not appear as a liquidus phase unless H2O content of the melt exceeds
2 wt.% and temperature of crystallization is below 1000 °C. This then follows that hydrous basaltic
melt will crystallize amphibole if the crystallization temperature drops below 1000 oC. Textural
features in the chromitite-bearing rocks of the SLC indicate that amphiboles replaced clinopyroxene.
This evidence, however, does not completely rule out the possibility of crystallization of magmatic
amphibole in SLC. However, in the absence of any clue in support of magmatic amphibole, it is
presumed that higher crystallization temperature (>1000 oC) rather than H2O-undersaturation of the
parental melt was instrumental for non appearance of magmatic amphibole in the SLC.
On the basis of the foregoing analyses a generalized crystallizing sequence can be developed for the
SLC. A parental melt having the composition of hydrous tholeiitic magma crystallized combination of
dunite, wehrlite and hurzburgite. These early-crystallized rocks plausibly lie beneath the exposed level
and was sampled by the intruding felsic magma. Continued crystallization of the evolved melt
produced an alternate sequence of clinopyroxene- and chromite-rich layers at pressure <2 kbar. Since,
Mg is preferentially partitioned to clinopyroxene than the coexisting melt, crystallization of large
volumes of clinopyroxene (to form clinopyroxenite) would enrich the parental melt with Cr, Fe and Al
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which then triggered the crystallization of Fe-Al-rich chromite to form thick to thin chromite seams in
clinopyroxenite. Crystallization of Fe-Al-rich chromite, in turn, enriched the magma in Mg and paved
the way for crystallization of clinopyroxene. Continuation of this process can explain formation of
several layers of chromitite in clinopyroxenite. This process eventually enriched the residual melt with
Ca, Al and H2O from which anorthosite with highly calcic plagioclase was crystallized. Crystallization
of large volume of calcic plagioclase increased Cr concentration of the melt, which when reached a
critical value, deposited thin chromite seams in anorthosite. High PH2O of the evolved melt could also
help crystallization of chromite in the anorthosite (Matveev and Ballhaus, 2002). Temperatures during
the entire crystallization sequence were above 1000 °C in order to suppress crystallization of magmatic
amphibole.
6. Discussion
6.1. Tectonic setting of the SLC
The tectonic setting in which Archaean layered anorthosite with highly calcic plagioclase and Fe-Al
rich chromite have been studied in great detail for the occurrences of Greenland (Weaver et al., 1981;
Ashwal, 1993; Dymek and Owens, 2001; Polat et al., 2009; Rollinson et al., 2010). Although the
compositions of plagioclase and chromite are remarkably similar between the Fiskenaesset Complex of
Greenland and the SLC, absence of quality geochemical and isotopic data is the main impediment for
precise delineation of the tectonic setting in which the SLC was emplaced. Nevertheless a number of
features suggest that the SLC represents fragments of oceanic crust. These are:
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1. The rock ensemble of the SLC is enclosed by mafic-ultramafic rocks (now mafic granulites
with or without garnet). BIF constitutes the only sedimentary rocks in the complex. The
voluminous felsic rocks (enderbite) that occurs in wider areas are intrusive into the SLC and
their enclosing mafic-ultramafic rocks.
2. The pseudomagmatic stratigraphy developed for the SLC and its temporally equivalent BLC
(Fig. 2b) matches well with the ultramafic-mafic-chert/BIF association of many well-studied
ophiolites of Phanerozoic (Kusky et al., 2001) and Precambrian (Harper, 1984, 1986; Kusky et
al., 2001; Slabunov et al., 2003; Dilek and Polat, 2008) ages.
These observations corroborate the view that Archaean high-grade complexes with layered
anorthosite are remnants of the oceanic crust (Weaver et al., 1981; Polat et al., 2009). Presence of
highly calcic plagioclase in anorthosite indicates that the melts that deposited plagioclase and Fe-Al
rich chromites in the SLC were hydrous in nature. A number of studies have indicated that hydrous
basaltic magmas are generated in arc setting from Archaen to present day where these magmas
precipitate highly calcic plagioclase (>An90, Arculus and Wills, 1980; Takagi et al., 2005; Polat et al.,
2009). Furthermore, some primitive arc basalts also have chromites with low Mg# (<0.6) and low Cr#
(0.4-0.6), which overlaps with the compositions of chromites from SLC and Fiskenaesset Complex
Greenland (Grove et al., 2003; Righter et al., 2008; Rollinson et al., 2010).
On the basis of REE patterns and Nd-Sm isotope compositions, Bhaskar Rao et al. (1996) opined
that the mafic rocks and the chromitite-bearing rocks of the SLC are genetically linked. To put some
additional constraints on the tectonic setting, bulk compositions of some mafic rocks from SLC and the
adjoining BLC were analyzed with XRF (Table 2). Figure 8 shows some tectonic discriminant plots
that separate basalts from spreading centers (MORB), Island Arc (IAB) and within plate continental
flood basalts (WPB). In these diagrams, most compositions of basic rocks are plotted in the field of
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IAB with a data straddle the boundary between MORB and IAB (Fig. 8). Mafic rocks of the
Fiskenaesset Complex also show similar trend although more rigorous geochemical analyses were done
in this complex. The compositional plots of Fig. 8, together with the inferred high PH2O of the parental
liquids are consistent with parental liquid of the SLC being derived from Neoarchaean (c.2.9 Ga) upper
mantle that was metasomatized by subduction-derived components during formation of oceanic arc
system (Polat et al., 2009). However, compared to the compositions of chromites that are formed in
modern arc basalts, chromites from the Neoarchaean layered magmatic complexes of Fiskenaesset and
Sittampundi are distinctly aluminous at similar Mg# (Fig. 5a). This difference has been attributed to the
fact that Neoarchaean mantle wedge that occurred above the subducting oceanic plate was more
aluminous owing to percolation of Al-rich melt derived from melting of subducting oceanic crust (Polat
et al., 2009; Rollinson et al., 2010).
In summary, mineralogy of the chromitite-bearing rocks together with geochemical signatures of the
enclosing mafic rocks support the view that the magmatic rocks of the SLC were emplaced in an arc
setting and the rock ensemble presumably represents a fossil suprasubduction zone in Neoarchaean
time (Dielek and Polat 2008). Excluding ultramafic rocks of upper mantle affinity, the rock ensembles
of SLC and BLC and their reconstructed stratigraphy bear remarkable similarity with several ophiolite
complexes of of Archaean age (Harper, 1984, 1986; Kusky et al., 2001; Slabunov et al., 2003; Dilek
and Polat, 2008). The absence of upper mantle rocks in the SLC and BLC may be attributed either to a
lack of exposure of the lowermost parts of the magmatic sequence or to detachment at crustal level
rather than within the mantle, during emplacement (Harper, 1984, 1986). Absence of mantle xenoliths
in the younger felsic intrusive rocks (protoliths of felsic granulites) tends to support the second option.
A high thermal gradient in the oceanic lithosphere and/or a thicker oceanic crust in the Archaean time
may help decoupling of oceanic crust from its mantle root (Harper, 1984, 1986). Detailed geological,
geochemical and isotopic studies on the fragments of the Archaean layered magmatic complexes of the
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CSS will help unravel the enigmatic crust-mantle interactions and tectonic patterns during the early part
of the Earth’s history.
6.2. Comparison between the chromite deposits in the SLC and other layered complexes in Archaean
high-grade terrains
Archaean high-grade terrains expose polydeformed and polymetamorphosed middle to lower
continental crust (Windley et al., 1981; Ashwal, 1993; Harley et al., 1998). Only a few of these
Archaean terrains contain chromite-bearing mafic-ultramafic-anorthosite complexes (Windley et al.,
1981; Hatton and von Gruenewaldt, 1990; Ashwal, 1993; Harley et al., 1998; Rollinson et al., 2002;
Rollinson, 2008). Although superposed deformation and high-grade metamorphism obliterated, to a
great extent, the original magmatic stratigraphy and mineralogy of the chromite-bearing rocks, detail
studies on the layered magmatic complexes of Messina, S. Africa (Hor et al., 1975; Barton et al., 1979)
and Fiskenaesset, Greenland (Windley et al., 1981; Ashwal, 1993; Peck and Valley, 1996; Rollinson,
2008; Polat et al., 2009; Rollinson et al., 2010) provide a wealth of information about the magmatic
history and metamorphic reconstitution of the rocks of these complexes. In the following sections we
present similarity and contrast in terms of salient geological features among the three chromitite-
anorthosite occurrences (Fiskenaesset, Messina and the SLC) that are hosted in the Archaean high-
grade terrines.
Similar to the layered complexes of Fiskenaesset and Messina, the SLC shows a lower ultramafic
unit, which grades upward to leucogabbro to anorthosite to mafic rocks (Fig. 2b). Olivine-rich rocks
(dunite/harzburgite) that form the lower part of the magmatic sequences of Fiskenaesset complex and
Messina complex are also observed in BLC and their presence is inferred from the xenoliths in the
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younger felsic intrusive in the SLC. In all the four complexes, anorthosite and the co-genetic
pyroxenite are interlayered with chromitite seams and underwent polyphase deformation and upper
amphibolite to granulite-facies metamorphism (Windley and Smith, 1976; Windley et al., 1981;
Ashwal, 1993; Windley and Garde, 2009; Rollinson et al., 2010). In Fiskenaesset Complex and SLC,
anorthosite and chromite-bearing rocks are enclosed by mafic rocks of ocean floor affinity and were
subsequently intruded by voluminous felsic rocks of TTG affinity. Emplacement of Messina complex
within a sequence BIF, quartzite and pelite supports its continental affinity (Windley et al., 1981).
Highly calcic plagioclase (XAn>0.8) and Fe-Al-rich chromitite are the unique features of the
magmatic complexes of Messina, Fiskenaesset and SLC (Windley et al., 1981; this study).
Tschermakitic amphibole, which is considered as “primary’ magmatic mineral in the Fiskenaesset
complex (Rollinson et al., 2010), has metamorphic origin in the SLC.
Figure 5a shows that chromite compositions from Neoarchaen layered complexes of Fiskenaesset
and Sittampundi define an array showing decreasing Mg# and increasing Cr#. This array of chromite
compositions contrasts with the compositions of chromite from other occurrences that show distinctly
higher Cr# and Mg# than the layered anorthosite hosted chromitite (Fig. 5a).
Detail petrological, geochemical and stable isotopic data show that layered anorthosite of
Fiskenaesset Complex, Greenland was emplaced at or close to the oceanic surface (Weaver et al., 1981;
Windley et al., 1981; Peck and Valley, 1996; Rollinson et al., 2010). Shallow level intrusion
presumably in a stable shelf region is also considered for Messina complex from their intercalated
rocks (Windley et al., 1981). Geological features of SLC indicate that like the other two Neoarchaean
magmatic complexes, SLC were also emplaced at or close to the sea surface.
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In summary, chromite-bearing rocks of Achaean high-grade terrains share a number of geological
features that contrast sharply with their younger counterparts. Anorthosite with highly calcic
plagioclase and chromite with Fe-Al rich compositions that are key to the features of Neoarchaean
anorthosite hosted chromitite deposits are attributed to hydrous and aluminous nature of the parental
melt compositions from which these magmatic complexes were formed. Dwindling of these hydrous
magmas in the post Archaean may be related to a number of factors such as desiccation of mantle
through repeated discharge of hydrous magmas during the Archaean, dominance of slab dehydration in
place of slab melting at reduced geothermal gradient in the post Archaean time and melting of mantle
wedge in place of slab melting during post Archaean era (Rollinson, 2007; Rollinson et al., 2010).
Acknowledgements
We are thankful to the Department of Science and Technology (DST), New Delhi, India, DAAD-DST PPP
and CAS, Department of Geological Sciences, Jadavpur for financial assistance. Most of the analyses were done
during the stay of P.S., U.K.B. and U.D.in the Mineralogisch-Petrologisch Institute, Bonn as a part of the DST-
DAAD PPP programme. We are indebted to Professor M.M. and Prof. C. Ballhaus, Directors, Mineralogisch
Petrologisches Institut, Bonn, Germany, for extending the analytical facilities of the institute. D.M.
acknowledges support from Senior Scientist Project from the Indian National Science Academy. The final draft
of this manuscript was prepared when P.S. was visiting the Mineralogy and Geology Department of University
of Cologne, Germany as a AvH Fellow. P.S. thanks Prof. C. Muenker and Prof. R. Kleinschrodt of Mineralogy
and Geology Department, University of Cologne for many stimulating discussions. We thank Profs. H.
Rollinson and P. Page for their critical but extremely useful comments on an earlier draft of the manuscript. This
manuscript is greatly benefitted from the erudite comments from the journal reviewers Prof. H. Rollinson, Prof.
B.F. Windley, Prof. G. Grieco and Associate Editor Prof. S. Rowins. We thank Prof. N.J. Cook for through
editorial corrections and additional comments that improved the clarity of the manuscript.
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Figure captions
Fig. 1. Generalized geological map of Cauvery Shear System (CSS) modified after the geological quadrangle
map of Tamil Nadu (Geological Survey of India, 1995). Different shear zones in CSS and adjoining areas are
shown in the inset. DC: Granite-greenstone belt of Dharwar Craton, FL: Fermore line separating DC from the
South Indian granulite terrane, NGT: Northern Granulite Terrane, CSS: Cauvery Shear System (Chetty,
1996), MSZ: Moyar shear zone, BSZ: Bhavani shear zone, MBASZ: Moyar-Bhavani Attur shear zone,
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PCSZ: Palghat-Cauvery shear zone, MB: Madurai Block, KKPTSZ, Karur-Kumbum-Panivu-Trichur shear
zone (Ghosh et al., 2004), ACSZ: Achankovil shear zone, KKB: Kerala khondalite belt, BLC: Bhavani
layered complex, SLC: Sittampundi layered complex.
Fig. 2. (a) Detailed lithological map of the studied area showing the sample locations. (b) Schematic
stratigraphic sections of the layered complexes of (i) Bhavani (BLC) and (ii) Sittampundi (SLC). Mafic rocks
now represented by mafic granulites with or without garnet. These granulites are partly altered to
amphibolites. Thickness of units is not to scale. See text for detail.
Fig. 3. Field photos showing lithological relationships among different rock units in and around the SLC. (a)
Alternation of thin layers rich in magnetite and silica in the Banded Iron Formation (BIF). (b) Sharp contact
between BIF and the enclosing garnetiferous mafic granulites (GMG). Note the tight folding of magnetite-
rich layers within BIF. (c) Dunite xenolith within felsic (enderbitic) gneiss. Note the swerving of foliation of
the host gneiss around the dunite xenolith. (d) Corundum (ruby) with coronitic green spinel in anorthite-rich
layers close to chromitite layer. Note the occurrence of thin green spinel-rich veins in chromitite at high angle
to the compositional layers. (e) Alternate layering of clinopyroxenite and chromitite. (f) Deformed chromitite
layers within anorthosite. Note the pinch and swell structure and boudinage in viscous chromitite layer. (g)
Folds defined by alternate layers of anorthosite and chromite-bearing pyroxenite/chromitite.
Fig. 4. Photomicrographs showing textural relationship among minerals within chromitite, clinopyroxenite and
anorthosite. (a) Cumulus chromite (Chr) with interstitial amphibole (Hbl) and chlorite (Chl). Note the
presence of rutile (Rt) along the grain boundary of chromite. Thick chromitite layer in clinopyroxenite. BSE
image. (b) Cumulus chromite (Chr) with fine exsolved lamellae of rutile (Rt). Thick chromitite layer in
clinopyroxenite. BSE image. (c) Cumulus clinopyroxene (Cpx) grains partially altered to amphibole (Hbl)
along the grain boundary. Chromite-bearing clinopyroxenite.Length of the photo 1.72 mm. polarized light (d)
Chlorite (Chl) grains replace cumulus chromite (Chr) and retrograde amphibole (Hbl) in anorthosite. BSE
image. (e) Recrystalized and polygonal aggregates consisting of plagioclase (Pl) and clinopyroxene (Cpx)
grains. Anorthosite. Length of the photo = 1.72 mm. crossed polars. (f) Chromite (Chr) inclusion within
clinopyroxene (Cpx) in anorthosite. Note the development of clinozoisite (Czo) over clinopyroxene and
plagioclase grain. Length of the photo = 1.72 mm. crossed polars. (g) Green spinel (Spl) rims coarse
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corundum (Crn 1) against plagioclase (Pl). The green spinel (Spl) breaks down to aggregates of granular
corundum (Crn 2), magnetite (Mag, highly reflecting) and chlorite (Chl). BSE image. (h) Vein of green spinel
(Spl) in chromitite at high angle to the compositional layering (see Fig. 3d). Note the relics of chromite (dark)
within green spinel (Spl). Length of the photo = 1.72 mm. polarized light (i) Irregular veins of green spinel
(shades of gray) replacing chromite (bright). Reflectivity increases with Cr2O3 content of spinel. Also note the
plagioclase (Pl) in the interstitial space. Anorthosite. BSE image. Abbreviations after Kretz (1983).
Fig. 5a. Comparison of chromite compositions of the studied area (symbols) with the compositions of chromite
from other Archaean and younger deposits. 1 = Picrites, 2 = Komatiites, 3 = MORB (Rollinson et al., 2002);
4 = Layered complexes (Windley et al., 1981); 5-6= Chromite in Archaean chromitite associated with
ultramafic rocks. Nuasahi and Sukinda massifs, Singhbhum, India (Mondal et al., 2006); Arrows with “M”
and “R” indicate the magmatic crystallization trends of the magmatic crystallization and replacement of
chromite from Ujaragssuit nunat area, west Greenland (Rollinson et al., 2002). Compositional spread of
‘magmatic’ and metasomatically altered chromite from the studied area. ● = chromite from thick chromitite
in clinopyroxenite, ■ = chromite from thin chromitite in anorthosite, ○ = Disseminated chromite within
anorthosite, ∆ = small chromite grains included in clinopyroxene, anorthosite, ▲ = compositional variation
of chromite due to replacement by green spinel. Light and deep shaded regions represent cluster of chromite
compositions (core) from Fiskenaesset Complex, Greenlan and the chromite compositions (core) from the
modern arc basalts respectively (Rollinson et al., 2010). Note that the composition of cumulus chromite from
the SLC and Greenland show similar magmatic differentiation trend. See text.
Fig. 5b. Variation of Cr#(Cr/Cr+Al), Mg# (Mg/Mg+Fe2+) and Fe3+# (Fe3+ + Al+Cr) from rim to core of a
cumulus chromite in a thick chromitite layer in clinopyroxenite. Note that barring first few microns on the
rim, the composition of chromite remain virtually constant (see text).
Fig. 6 (a)-(b). Al2O3 and TiO2 contents of parental melt calculated from the chromite compositions of the studied
area following the procedure of Kamenetsky et al. (2001). The solid lines represent the best fit lines through
all the data of Kamenetsky et al. (2001). Symbols are same as in figure 5.
Fig. 7 (a)–(d). Experimentally determined stability field of some magmatic minerals in hydrous basaltic melts
(after Feig et al., 2006). Note the enlargement of the stability field of clinopyroxene (Cpx) with increasing
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H2O content of the melt. Filled circles represent crossover point of crystallization of clinopyroxene (Cpx) and
plagioclase (Pl). See text.
Fig. 8. Tectonic discrimination diagram for mafic rocks (a) Cr vs. Y discrimination diagram for basalt (after
Pearce, 1982). (b) Ti vs. Zr discrimination diagram of Pearce (1982). (c) V-Ti discrimination diagram of
Shervais (1982). (d) Zr/Y vs. Zr discrimination diagram of Pearce and Norry (1979). IAB= island-arc basalt;
MORB= mid-ocean ridge basalt; WPB= within-plate basalt; IAT= island-arc t
Appendix A
Analytical details. Chemical compositions of the minerals were determined with a CAMECA CAMEBAX
MICROBEAM electron microprobe at the University of Bonn, Germany. The instrument was operated at 15 kV
accelerating voltage, 2 microns beam diameter and 15 nA current. Natural mineral standard were used and the
raw data were corrected by PAP procedure (Pouchou and Pichoir, 1984). Details of the analytical procedures are
described in Raith et al. (2010). Detection limit for the electron microproble analyses are different for different
elements depending on several factors. Considering all the factors, detection limit of the measured
concentrations has been set at 0.02 wt%. Mineral abbreviations are according to Kretz (1983).
The samples of mafic rocks were analyzed for their major and trace element composition (i.e., bulk chemical
analysis) by PHILIPS X-RAY FLUORESCENCE at University of Bonn, Germany. Details of the analytical
procedures and the analytical precision are described in Prame (1997). Following Prame (1997), trace element
concentrations that measure 2 ppm or less are excluded from Table-2.
Backscattered electron images were obtained from the JEOL JSA 6490 Electron Microprobe at the
Department of Geology and Geophysics, Indian Institute of Technology, Khargapur, West Bengal.