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, APRIL 2012, 63, 2, 97—106 doi: 10.2478/v10096-012-0008-4
Petrology of plagiogranite from Sjenica, Dinaridic Ophiolite
Belt (southwestern Serbia)
DRAGAN MILOVANOVIĆ
1
, DANICA SREĆKOVIĆ-BATOĆANIN
1
, MARIJA SAVIĆ
1
and DANA POPOVIC
2
1
University of Belgrade, Faculty of Mining and Geology, Department of Petrology and Geochemistry, Djusina 7, 11 000 Belgrade, Serbia;
danicabat@yahoo.com
2
Geological Institute of Serbia, Rovinjska 12, 11 000 Belgrade, Serbia
(Manuscript received September 7, 2010; accepted in revised form September 30, 2011)
Abstract: The Sjenica plagiogranite occurs in the southern part of the Dinaridic Ophiolite Belt, 5 km northwest of
Sjenica. The main minerals are albite with strongly altered biotite (replaced with chlorite), with occasional amphibole
(magnesio hornblende to tschermakite) and quartz. An enclave of fine-grained granitic rocks with garnet grains was
noted too. Secondary minerals are calcite and chlorite (daphnite). Major, trace and REE geochemistry coupled with
field observations support a model by which the Sjenica plagiogranite could be formed by fractional crystallization of
mantle origin mafic magma in a supra-subduction zone setting. Occurrences of calcite and chlorite nests in the Sjenica
plagiogranites revealed that these rocks underwent hydrothermal alteration due to intensive sea water circulation in a
sub-sea-floor environment.
Key words: Serbia, Dinaridic Ophiolite Belt, geochemistry, petrology, ophiolite, plagiogranite.
Introduction
Occurrences of plagiogranites within ophiolitic complexes
are of particular interest because of their extreme composi-
tion and controversial origin. Ophiolitic sequences are con-
sidered incomplete without plagiogranites.
In Serbia plagiogranites occur in the Dinaridic Ophiolite
Belt and in the Vardar Zone (Karamata & Krstić 1996). In the
Dinaridic Ophiolite Belt plagiogranites were noted at numer-
ous localities (Karamata 1958; Pamić & Olujić 1969; Pamić &
Tojerkauf 1970; Lugović et al. 1991; Majer & Garašić 2001),
while in the Vardar Zone they are less abundant (Milovanović
1980; Jović 1984). Both, the Dinaridic Ophiolite Belt and the
Vardar Zone, are parts of the Alpine-Mediterranean mountain
belt which belongs to a main suture zone between Eurasia and
Gondwanaland after their collision during the Late Jurassic/
Early Cretaceous (Karamata 2006). These two differ in origin,
structure and age and can be traced continually nearly 700 km,
from the Southern Alps in the north to the Hellenides in the
south. Different reconstructions of the Mesozoic ophiolite
evolution in the Balkan Peninsula during the last few years
have aroused the questions about the existence of one or more
oceanic basins, their size, emplacement etc. One suggestion is
that Tethys ophiolites were developed in two or more ocean
basins, separated by rifted micro-continents (Pamić 1999;
Karamata et al. 2000; Pamić et al. 2002; Robertson 2002;
Stampfli & Borel 2002; Karamata 2004). During the Meso-
zoic, the Drina-Ivanjica-Pelagonide micro-continent separated
the Vardar Ocean in the east from the Dinaridic Ocean in the
west (Robertson & Karamata 1994). An alternative suggestion
is that Tethys ophiolites were generated from a single ocean
basin (e.g. Dercourt et al. 1986, 1993; Dal Piaz et al. 1995;
Bortolotti et al. 2004).
The aim of this paper is to define petrographic and
geochemical features of the Sjenica plagiogranites which oc-
cur in the southern part of the Dinaridic Ophiolite Belt. This
part of the Eastern Mediterranean region has been investigated
by numerous workers. The most important studies are those
made by Karamata who has studied the Sjenica plagio-
granites and initiated a new approach to interpretation of
Mesozoic evolution in this region (1958, 2004).
Geological setting
The Sjenica plagiogranite occurs in the southern part of
the Dinaridic Ophiolite Belt, which represents remnants of
the Tethys and its marginal seas. The Sjenica plagiogranite
occurs 5 km northwest of Sjenica (Coordinates: E 7146381,
N 4793606; Fig. 1). The largest area is covered by ophiolite
mélange (J
2,3
) composed of chert, sandstone, claystone, lime-
stone, diabase, gabbro, serpentinite and plagiogranite blocks
(lenses) bonded with the sandy-silty matrix. Triassic rocks com-
prise widespread Middle Triassic limestone and dolomites with
chert concretions and Upper Triassic banked to massive, highly
karstified dolomitic limestone and dolomites, reaching in thick-
ness up to 300 m. Lower Jurassic, Liassic limestone (J
1
) is light
reddish, oolitic in places. The youngest unit in this area
is Miocene in age and corresponds to freshwater sediments with
lignite layers and less abundant marly and dolomitic limestone
(Fig. 2). Plagiogranites occur as lenses, about 50 m in length
and 20 m in thickness, enclosed in the ophiolitic mélange,
with irregular and jagged contacts. Field relations between
plagiogranites and surrounding rocks could not be established
due to intensive faulting. The present variably dismembered
state is related to obduction and post-obduction tectonics.
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Methods and techniques
On the basis of careful petrographic study of 30 samples, a
representative suite of 5 samples was selected for geochemical
analysis. The major element oxide, trace and REE element
contents of these rock samples were analy-
sed at the ACME analytical laboratory in
Vancouver (Canada). The major and trace
elements were determined from fused
LiBO
2
discs by ICP-OES and ICP-MS, re-
spectively, using 5 g of sample powder.
Rare Earth elements were analysed by in-
ductively coupled plasma-mass spectrome-
try (ICP-MS). The composition of minerals
in selected samples was determined using a
CAMECA SX 100 electron microprobe at
the Department of Mineralogy and Petro-
graphy, University of Hamburg, Germany.
Operating conditions were 20 kV acceler-
ating voltage and 20 nA beam current with
20 s and 2 s counts for peak and back-
ground respectively.
Petrography and mineral chemistry
The Sjenica plagiogranite is holocrystal-
line, medium- to coarse-grained (average
grain size 2 mm), homogeneous and unfoli-
ated (Fig. 3). The overall texture is hypidio-
morphic granular. These rocks show slight
variations in the proportions of mafic and
felsic minerals across the outcrop. Plagio-
granites are mainly composed of plagioclase
(albite) and quartz (Fig. 4). Vermicular
quartz-plagioclase intergrowths that were
interpreted as a primary magmatic feature
by Coleman & Donato (1979), have been
observed occasionally. Quartz comprises up
to 30 % of the mode. In samples with am-
phibole the quantity of quartz decreases to
about 20—25 %.
Albite is present as euhedral, twinned
crystals, up to 5 mm in size, with minor
sericitization. Plagiogranites contain 40 to
50 % modal albite. Twelve plagioclase
grains were analysed. According to the ob-
tained data, presented on Table 1 they corre-
spond to almost pure albite ranging in
composition between Ab (92.1—98.7 %).
Mafic minerals are chlorite, strongly al-
tered biotite (?) and occasional amphibole.
Chlorite occurs in veins, as irregular patches,
interstitial accumulations (nests between al-
bite and quartz grains) or as pseudomorphs
after primary biotite. Chlorite is present in
abundances from 5 % to 10 %. Microprobe
analyses of chlorite were performed on
twelve chlorite grains (Table 2). The ob-
tained X
Fe
values (Fe/Fe + Mg) range from 0.807 to 0.848.
Chlorites are dominantly daphnite (Holland & Powell 1998).
Amphiboles occur locally in the eastern part of the out-
crop. They are randomly oriented, typically exhibiting pris-
matic and acicular shapes. This mineral is partially altered
Fig. 1. The terranes in the central part of the Balkan Peninsula along with the position
of the Sjenica plagiogranite: ESCB – The composite terrane of the Carpatho-Bal-
kanides; SMCT – The Serbian-Macedonian Composite Terrane; VZCT – The Vard-
ar Zone Composite Terrane; KB – The Kopaonik Block; JBT – Jadar Block
Terrane; DIT – The Drina-Ivanjica Terrane; DOB – The Dinaridic Ophiolite Belt;
EBDT – The East Bosnian-Durmitor Terrane; CBMT – The Central Bosnia Mts Ter-
rane; DHCT – The Dalmatian-Herzegovinian Composite Terrane (after Karamata 2004).
Fig. 2. Geological map of the Sjenica area with the occurrence of the plagiogranite
(black arrow). Basic Geological Map, Sheet Bijelo Polje, 1 : 100,000 (Živaljević et al.
1982). Legend: T
2
1
– Middle Triassic limestone with cherts; T
3
– Upper Triassic lime-
stone; J
1
– Liassic reddish limestone; J
2,3
– Ophiolitic mélange;
– Basaltic pillow
lavas; Se – Serpentinite; M
2
– Miocene clastic sediments;
– Plagiogranite (on the
Basic Geological Map signed as granodiorite and quartzmonzonite).
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Fig. 4. Microphotograph of the Sjenica plagiogranite (N+ . Abbre-
viations: Ab – albite, Chl – chlorite, Q – Quartz.
into chlorite and iron oxides. Pale green pleochroism has
been observed. Amphibole grains correspond to Ca amphi-
bole according to the nomenclature of Leake (1997), more
precisely to magnesio hornblende or to tschermakite (Ta-
ble 3, Fig. 5). The presence of two groups of amphiboles
could be either a result of different conditions during crystal-
lization or the result of their different alteration degree. The
abundances of amphibole is below 10 %.
Fig. 5. Composition of amphiboles from the Sjenica plagiogranites
plotted on the diagram of Leake (1997).
Secondary calcite occurs locally, building nests with chlo-
rite, usually in intergranular spaces between albite and
quartz grains. Calcite forms up to 3 % vol. of rock. Accessory
minerals are apatite, zircon and magnetite.
In the eastern part of the outcrop (Fig. 6) we have found
within the plagiogranite an enclave approximately 10 cm in
diameter of fine-grained garnet-bearing granite (which also
contains albite, chlorite and quartz).
Fig. 3. The Sjenica plagiogranite outcrop, with detail of rock sample.
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Table 1: Chemical composition of albite.
Table 2: Chemical composition of chlorite.
Table 3: Chemical composition of amphibole ( – core of grains).
Sample
1
2
3
4
5
6
7
8
9
10
11
12
SiO
2
66.95 66.83 66.96 66.81 67.32 67.48 66.42 67.21 66.78 66.86 66.03 66.32
Al
2
O
3
20.61 20.97 20.42 20.92 20.77 19.97 21.09 20.32 20.87 20.91 22.11 20.78
CaO
0.35 0.11 0.12 0.41 0.12 0.16 0.21 0.21 0.35 0.43 0.16 0.26
Na
2
O
10.95 10.94 10.99 10.87 11.22 11.35 10.87 11.23 10.99 10.95 10.31 10.98
K
2
O
0.00 0.64 0.59 0.61 0.15 0.22 0.94 0.21 0.52 0.61 1.21 0.73
Total
98.86 99.49 99.08 99.62 99.58 99.18 99.53 99.18 99.51 99.76 99.82 99.07
Calculated on 32 O
Si
11.81 11.76 11.83 11.75 11.81 11.89 11.71 11.84 11.75 11.74 11.60 11.74
Al
4.28 4.34 4.25 4.33 4.29 4.14 4.38 4.22 4.33 4.33 4.58 4.33
Ca
0.07 0.02 0.02 0.08 0.02 0.03 0.04 0.04 0.07 0.08 0.03 0.05
Na
3.75 3.73 3.76 3.71 3.81 3.88 3.72 3.84 3.75 3.73 3.51 3.77
K
0.00 0.14 0.13 0.14 0.03 0.05 0.21 0.05 0.12 0.14 0.27 0.17
An
1.8 0.6 0.5 2.0 0.6 0.8 1.0 1.0 1.8 2.0 0.8 1.2
Ab
98.2 95.9 96.2 94.4 98.7 98.0 93.7 97.7 95.2 94.4 92.1 94.5
Or
0.0 3.5 3.3 3.6 0.7 1.2 5.3 1.3 3.0 3.6 7.1 4.3
Sample
1
2
3
4
5
6
7
8
9
10
11
12
SiO
2
23.58 23.33 25.31 25.24 24.63 23.43 23.54 23.26 23.29 24.51 25.14 24.36
Al2O
3
20.29 20.91 19.09 19.98 19.20 19.86 20.02 20.83 20.31 19.70 18.98 19.08
FeO
tot
37.06 38.32 37.22 37.40 37.98 38.74 38.88 38.09 38.55 38.38 37.79 39.26
MnO
1.03
1.05
0.82
0.86
0.95
1.04
0.97
1.09
1.07
0.89
0.85
1.05
MgO
4.98
3.92
4.62
4.62
4.43
4.18
4.16
4.18
4.03
4.33
4.48
3.95
Total
86.94
87.53
87.06
88.10
87.19
87.25
87.57
87.45
87.25
87.81
87.24
87.70
Calculated on 28 O
Si
5.39
5.34
5.76
5.67
5.61
5.39
5.40
5.32
5.36
5.57
5.71
5.59
Al
5.42
5.63
5.11
5.28
5.15
5.38
5.41
5.61
5.50
5.27
5.08
5.15
Fe
7.08
7.33
7.08
7.02
7.23
7.46
7.46
7.29
7.42
7.30
7.18
7.53
Mn
0.20
0.20
0.16
0.16
0.18
0.20
0.19
0.21
0.21
0.17
0.16
0.20
Mg
1.70
1.34
1.57
1.55
1.50
1.43
1.42
1.43
1.38
1.47
1.52
1.35
Sample
1
2
3
4
5
6
7
8
9
10
SiO
2
49.72 50.04 41.93 42.15 42.63 42.01 41.83 48.96 49.52 48.46
TiO
2
0.03 0.87 3.63 3.46 3.26 3.31 3.40 0.97 0.88 1.06
Al
2
O
3
4.57 4.14 12.06 12.03 11.34 11.75 11.92 4.94 4.16 5.02
FeO
tot
18.69 17.63 13.63 13.51 13.41 13.71 13.46 17.72 17.45 17.80
Cr
2
O
3
0.03 0.07 0.03 0.02 0.03 0.06 0.05 0.07 0.09 0.14
MnO
0.64 0.27 0.23 0.00 0.23 0.26 0.00 0.23 0.27 0.31
MgO
11.29 13.27 13.27 13.29 13.31 13.27 13.29 12.88 13.16 12.69
CaO
11.30 10.01 10.89 10.90 10.89 10.90 10.91 10.16 9.74 10.11
Na
2
O
0.61 0.98 2.49 2.49 2.38 2.46 2.51 1.10 0.96 1.13
K
2
O
0.20 0.20 0.11 0.13 0.10 0.11 0.11 0.29 0.19 0.28
Total
97.08
97.48
98.27
97.98
97.58
97.84
97.48
97.32
96.42
97.00
Calculated on 23 O (13-CNK)
Si
7.332
7.198
6.039
6.085
6.177
6.078
6.074
7.090
7.185
7.051
Ti
0.003
0.094
0.393
0.376
0.355
0.360
0.371
0.106
0.096
0.116
Al
0.794
0.701
2.045
2.046
1.936
2.002
2.038
0.842
0.711
0.860
Cr
0.003
0.008
0.003
0.002
0.003
0.007
0.006
0.008
0.010
0.016
Fe
3+
0.748
1.312
1.010
0.937
0.927
1.025
0.945
1.244
1.382
1.267
Fe
2+
1.557
0.809
0.631
0.694
0.698
0.634
0.690
0.902
0.735
0.899
Mn
0.080
0.033
0.028
0.000
0.028
0.032
0.000
0.028
0.033
0.038
Mg
2.482
2.845
2.849
2.860
2.875
2.862
2.877
2.780
2.847
2.753
Ca
1.785
1.543
1.680
1.686
1.691
1.690
1.697
1.576
1.514
1.576
Na
0.174
0.273
0.696
0.697
0.668
0.690
0.707
0.309
0.270
0.319
K
0.038
0.037
0.020
0.024
0.018
0.020
0.020
0.054
0.035
0.052
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Fig. 6. Enclave of fine-grained plagiogranite with garnet porphyroblasts (?), black arrow. Microphotograph is N II.
Table 4: Chemical compositions of garnets.
Sample
1
2
3
4
5
6
SiO
2
36.36 36.38 36.46 36.11 36.79 36.50
TiO
2
0.28 0.29 0.25 0.27 0.25 0.25
Al
2
O
3
21.28 20.96 21.05 20.83 20.79 20.86
FeO
tot
34.48 34.20 34.80 34.37 34.13 34.25
Cr
2
O
3
0.05 0.06 0.08 0.00 0.06 0.07
MnO
2.16 2.35 2.15 2.37 2.36 2.00
MgO
3.71 3.78 3.76 3.46 3.46 3.75
CaO
1.69 1.83 1.71 1.93 1.78 1.71
Total
100.01
99.85
100.21
99.34
99.62
99.39
Calculated on 12 O
Si
2.925
2.925 2.921 2.923 2.969 2.947
Ti
0.017
0.075
0.015 0.016 0.015 0.015
Al
1.997
1.984
1.986 1.986 1.977 1.984
Cr
0.003
0.004
0.005 0.000 0.004 0.004
Fe
2.320
2.299
2.331 2.327 2.304 2.313
Mn
0.147
0.160
0.146 0.163 0.161 0.137
Mg
0.445
0.453
0.449 0.418 0.416 0.451
Ca
0.146
0.158
0.147 0.167 0.154 0.148
Almandine 68.500 67.183
68.208 68.174 67.780 68.216
Andradite
6.016
6.469
5.965 7.128 2.961 5.218
Grossulare
0.000
0.000
0.000 0.000 3.566 0.880
Pyrope
18.997 19.291 19.248 17.779 18.335 19.491
Spessartine
6.284
6.814
6.253 6.919 7.106 5.906
Uvarovite
0.204
0.244
0.326 0.000 0.253 0.289
The garnet is almandine rich, but it must be noted that the
high amount of Fe
3+
probably implies subsequent alteration
processes (Table 4). Almandine component ranges from 67.2
to 68.5 %, pyrope from 17.8 to 19.5 %. Spessartine and an-
dradite contents are about 6 %, whereas amounts of uvaro-
vite and grossular components are insignificant. No
compositional zoning was detected.
Classification and nomenclature
Coleman & Peterman (1975) proposed the term “oceanic
plagiogranite” for rocks consisting of quartz and plagioclase
(An10—60), typically characterized by a granophyric inter-
growth with less than 10 % ferromagnesian minerals. This
term encompasses rocks that range from diorite through
trondhjemite to albite granite, which are all associated with
ophiolites. On the basis of a wt. % K
2
O vs. SiO
2
discrimina-
tion diagram (Coleman & Peterman 1975; Coleman & Donato
1979; Maniar & Piccoli 1989), the Sjenica plagiogranites can
be considered as oceanic plagiogranites, except the sample
with amphibole (Fig. 7). Plagiogranites from the Milatkoviće
village near Novi Pazar which display similar geochemical
features with the oceanic plagiogranites from the Troodos
ophiolite massif were plotted on the same diagram
(Milovanović 1980). For the purpose of geochemical charac-
terization, CaO, Na
2
O and K
2
O have been plotted in the CNK
ternary diagram of Glikson (1979) and the CIPW-normative
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Fig. 9. Classification and nomenclature of the Sjenica plagiogranite
according to the normative An—Ab—Or diagram (after Barker 1979).
An, Ab and Or ternary diagram of Barker (1979). In both
diagrams, samples of the investigated rocks fall in the
trondhjemite field (Figs. 8 and 9). The exception is the sam-
ple with amphibole, which is near the boundary of
trondhjemite and tonalite fields on figure 8.
One rock (sample 5, with amphibole) within a representa-
tive suite of 5 selected samples has a bulk chemical composi-
tion that is intermediate between the plagiogranites and the
enclosing gabbroic rocks. This sample has a relatively high
MgO content (6.14 %) and a lower SiO
2
content (55.89 %)
with respect to the plagiogranites. The other four samples of
plagiogranites from Sjenica show low TiO
2
, K
2
O, P
2
O
5
, Rb
and Ba and high Na
2
O contents (Table 5).
Geochemistry
REE data (Table 5) and their distribution patterns show
that the plagiogranites are enriched by twenty to one hun-
dred times compared with the relative average chondrite val-
ue (Fig. 10). They all show similar patterns with a slight
LREE enrichment and a small negative Eu anomaly. The lat-
ter indicates plagioclase involvement during either a frac-
tionation or melting process (Floyd et al. 1998).
On a multi-element spider diagram normalized to primi-
tive mantle the Sjenica plagiogranites show enrichments of
Rb, Ba, K, Th, Sr, depletions of Eu, Ti, P and Sr and flat
HREE patterns (Fig. 11). When taken together these data
suggest that the plagiogranites may have been generated by
low-pressure fractionation in which plagioclase and pyro-
xene were important differentiation phases and garnet and
hornblende were not involved (Drummond & Defant 1990).
Discussion
Usually suggested models for plagiogranite genesis in
ophiolite complexes are:
fractional crystallization of a parental MORB melt at shal-
low depths in oceanic crust. This model has been supported by
a number of authors on Alpine and Apennine ophiolites (e.g.
Coleman & Peterman 1975; Engel & Fisher 1975; Coleman
1977; Saunders et al. 1979; Dixon & Rutherford 1979;
Kontinen 1987; Borsi et al. 1996; Montanini et al. 2006);
partial melting of gabbroic rocks under hydrous condi-
tions in tectonically active areas of midocean ridge systems
(Gerlach et al. 1981; Pedersen & Malpas 1984; Koepke et al.
2004, 2007). The role of water-rich fluid, either of magmatic
origin (e.g. Maeda et al. 2002) or sea-water derived (e.g.
Gregory & Taylor 1981), is suggested by the presence of
amphibole in these leucocratic rocks;
liquid immiscibility (Dixon & Rutherford 1979);
special type of anatexis proceeding at the roof zone of
axial magma chambers under fast spreading ridges (e.g.
Michael & Schilling 1989).
Plagiogranites of Sjenica display similar values in the ele-
mental abundances with respect to ORG (ocean ridge granites;
Pearce et al. 1984). ORG-normalized patterns are character-
Fig. 8. Plot of the Sjenica plagiogranite ( – full symbols for pla-
giogranites with chlorite; – empty symbol for plagiogranite with
amphibole) and Milatkovice plagiogranite ( ) on K
2
O (%) vs. SiO
2
(%) binary diagram. Field boundaries are after Coleman &
Peterman (1975).
Fig. 7. Classification and nomenclature of the Sjenica plagiogranite
according to CNK diagram (Glikson et al. 1979).
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Table 5: Chemical composition of the Sjenica plagiogranites (1—4 –
plagiogranites with chlorite; plagiogranite with amphibole).
Fig. 10. REE patterns of plagiogranites (normalized values from
Sun & McDonough 1989).
Fig. 11. Primitive mantle normalized multielement spider diagram
of the Sjenica plagiogranite. Normalizing values from Sun &
McDonough (1989).
ized by high content of LILE elements (K
2
O, Rb, Ba and Th)
and Ta negative anomalies (Fig. 12). Such geochemical fea-
tures can be attributed to an arc or suprasubduction zone
ophiolitic plagiogranites or variable mobilizations of the LILE
elements during metamorphism, crustal involvement and/or
hydrothermal alteration (ocean floor metamorphism).
On the N-MORB-normalized trace-element variation dia-
gram the Sjenica plagiogranites are characterized by some
large ion lithophile element (LILE) enrichments and relative
depletion in HFSE (Fig. 13).
Amphibole-bearing plagiogranites, which are present in
minor abundances, could form at fluid pressure of 200 MPa,
and at depths greater than 6 km (Dixon & Rutherford 1979).
The enclave with garnet appears to have originated by low
to moderate degree partial melting of hydrated basaltic/gab-
broic rocks in oceanic crust. The essential conditions for the
stability of garnet varies over a temperature range of 800—
1000 °C and within a pressure range of 0.9—1.4 GPa (Vielzeuf
& Schmidt 2001) which correspond to a depth < 30 km. The
garnet could not be regarded as a major residual phase as no
significant LREE/HREE fractionation was noted.
The major, trace and REE geochemistry and field relations
indicate that plagiogranites were formed through a complex
process of fractional crystallization of mantle origin mafic mag-
ma that derived under high degrees of partial melting in the
presence of water introduced by subduction (?). The chemistry
of the Sjenica plagiogranites cannot be explained without a sub-
duction processes (Moores et al. 1984). The enrichment of Rb,
Ba, Sr, Th and LREE values and the presence of Nb anomalies
are consistent with variable mobilization of the LILE elements
Sample
1
2
3
4
5
SiO
2
67.06 66.44 62.90 61.82 55.89
TiO
2
0.37 0.37 0.46 0.59 1.05
Al
2
O
3
14.96 15.88 15.95 16.06 14.48
FeO
tot
5.17 5.75 6.13 8.71 8.76
MnO
0.13 0.16 0.17 0.23 0.20
MgO
0.53 0.71 0.73 1.23 6.14
CaO
1.52 1.38 3.08 2.02 3.84
Na
2
O
6.41 6.15 6.46 5.73 5.61
K
2
O
0.61 0.93 0.76 0.84 0.15
P
2
O
5
0.16 0.15 0.20 0.25 0.11
LOI
2.38 2.09 3.26 2.71 3.31
Total
99.30 100.01 100.10 100.19 99.54
Trace elements (ppm)
Ba
124 115 121 106 103
Rb
18
28
34
30
4
Sr
146
187
184
231
88
Ga
22
22
18
21
9
Ta
0.6
0.3
0.3
0.4
0.4
Nb
17
10
12
12
10
Hf
8.8
9
5
8
4.7
Zr
326 340 380 398 191
Y
68
51
42
45
34
Th
8
8
7
7
4
U
1.3
0
0
0
0.8
Cr
41
171
39
71
291
Ni
80
36
115
94
120
Co
22
25
27
29
32
Sc
22
20
23
21
34
V
29
52
84
125
209
Cu
25
28
37
82
85
Pb
12
11
12
12
2
Zn
89
92
93
115
124
REE elements (ppm)
La
25.5
22
18
21
15.2
Ce
61.8
53
41
37
34.1
Pr
7.5
6
8
4
4.1
Nd
33.7
21
26
33
17.7
Sm
8.9
7
5
9
4.5
Eu
2.2
2
1
2
1.3
Gd
10.1
8
9
6
5.3
Tb
2 2 2 1 1
Dy
11.7
9
11
6
6
Ho
2.4
1
1
1
1.2
Er
7.9
5
7
4
3.8
Tm
1.2
1
1
1
0.6
Yb
7.4
8
5
4
3.5
Lu
1.1
1
1
1
0.53
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in an arc or supra-subduction zone (SSZ). It is increasingly ac-
cepted that many ophiolites have been formed by spreading
above subduction zones, the so-called supra-subduction zone
ophiolites (Pearce et al. 1984; Shervais 2001). Supra-subduc-
tion type ophiolites typically formed during short-lived periods
( < 5 Ma) of regional plate re-organization, in narrow rifted ba-
sins where melts were contaminated by partial melting of neigh-
bouring lower crust (Hall 1984; Dilek et al. 1999).
Occurrences of calcite and chlorite nests in the Sjenica
plagiogranites revealed that these rocks were affected by hy-
drothermal alteration due to intensive sea water circulation
in a sub-sea-floor environment (Spooner & Fyfe 1973;
Lecuyer et al. 1990). Hydrothermal alteration in the oceanic
environment is known to often induce strong chemical mobi-
lization in ophiolites and ocean ridge rocks (Alt 1995, 1999).
The high Na
2
O and low K
2
O contents in plagiogranites are
due to exchange with sea water that gained access to the
magma chamber or to late magmatic vapour-phase transport
and removal of K
2
O (Coleman & Donato 1979; Sinton &
Byerly 1980). The availability of Na during these processes
was probably responsible for the enlargement of the stability
field of albite. Sea water infiltration into the lower crust oc-
curred along listric shear zones under low fluid/rock ratios
during the initial stages of deformation and metamorphism.
These relations clearly show that successive episodes of hy-
drothermal alteration of fossil oceanic crust in the Dinaridic
Ophiolite Belt were entirely intra-oceanic in origin.
Conclusion
The Sjenica plagiogranites correspond to remnants of an
oceanic basement evolved in the Dinaridic Ophiolite Belt, and
so in an intra-oceanic environment. The absence of LT/HP
metamorphism suggests that ocean basins in which the
Dinaridic ophiolites have been formed were mainly bordered
by passive margins.
The Sjenica plagiogranites, a part of the East Mediterra-
nean ophiolites are fragments of the oceanic lithosphere
probably related to a process of fractional crystallization of
mantle origin mafic magma in the so-called supra-subduc-
tion zone. The SSZ type ORG affinity of the Sjenica pla-
giogranite is substantiated by a low content of HFSE relative
to high abundance of LILE. The mineral composition and
chemistry of plagiogranites were additionally changed due to
interaction with sea water during sub-sea-floor metamor-
phism. However, a complete understanding of these ophio-
lite emplacements remains elusive including the occurrence
of garnet that requires further investigation.
Acknowledgments: We are grateful to colleagues at the De-
partment of Mineralogy and Petrography, University of
Hamburg for enabling chemical analyses of minerals for this
manuscript. We thank reviewers for their very helpful and
much appreciated comments and suggestions for improve-
ment of the manuscript. This research has been supported by
the Serbian Ministry of Science, Project No. 176019.
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