GEOLOGICA CARPATHICA, 52, 2, BRATISLAVA, APRIL 2001
79—90
WHOLE-ROCK CHEMISTRY AND GENETIC TYPOLOGY
OF THE WEST-CARPATHIAN VARISCAN GRANITES
IGOR BROSKA and PAVEL UHER
Geological Institute, Slovak Academy of Sciences, Dúbravská cesta 9, 842 26 Bratislava, Slovak Republic
(Manuscript received June 9, 2000; accepted in revised form March 15, 2001)
Abstract: The geochemistry of 166 new whole-rock analyses from West-Carpathian Variscan granitic rocks are pre-
sented on the basis of their division into four principal groups: S-, I-, A- and specialized S-type (S
S
). The contribution
shows some discrimination diagrams which are useful for the recognition of these principal granite groups and also give
a possible outline of the geodynamic scenario of their origin. All studied groups belong to mainly crustal aluminic (S
S
-,
S-type) and aluminocafemic (I-, A-, partly S-type) associations, mantle-derived cafemic dioritic rocks are rare. Gener-
ally, the S- and I-type groups show predominantly Na
2
O/K
2
O ratio > 1, whereas A- and S
S
-type granites usually exhibit
Na
2
O/K
2
O < 1. I-types are more Si-poor and Fe, P-rich than other groups, however, a part of the S
S
-type group belongs
to the P-rich evolved granites (>0.2 wt. % P
2
O
5
) and the A-types are generally very poor in P. The Zr vs. SiO
2
diagram
clearly discriminates Zr and Si-rich hypersolvus A-type from other groups, similarly the A-types show the highest Zr/Hf-
ratio and Y contents (>20 ppm). Ba-Sr and Sr-Rb diagrams successfully divide plagioclase-rich I-type from S-, A-type
and especially from K,Na-feldspar-rich S
S
-type. The newly modified Rb-Ba-Sr diagram reliably discriminates the groups:
poorly (I, S), mildly (S, A, rarely I) and strongly evolved granites (S
S
, rarely S and A) were recognized. REE rock/
chondrite normalized diagram discriminate all groups: REE-rich I-type without Eu-anomaly, from REE-rich A-type with
negative Eu-anomaly and REE-poor S- and especially S
S
-type with pronounced negative Eu-anomaly. In this sense of the
geotectonic position, the S- and I-type can be considered as orogenic granites, in contrast, the A-type and S
S
-type
granites are post-orogenic members.
Key words: Western Carpathians, geochemistry, granitic rocks, S-, I-, A-, S
S
- types.
Introduction
New analytical data, for the most part unpublished have been
gathered in chemical laboratories at Ottawa University, Cana-
da and in Memorial St. John’s University, Canada. These data
permit a new study of the chemical variability of granitic rocks
in the Western Carpathians. A subset of the samples which
were analysed and published previously (mainly “ZK” series,
Cambel & Walzel 1982; “BP” series, Uher et al. 1994) were
re-analysed. Consequently, this set is the first complete large
database of major and trace elements of all principal genetic
types of West Carpathian Variscan granitic rocks.
Geochemical studies of the West-Carpathian granites until
now, usually did not take into account variations between the
genetic groups of the granites but they were based mainly on
the investigation of granitic groups according to the IUGS
classification and composition variations between granites,
granodiorites and tonalites. The West-Carpathian Variscan
granitic rocks were considered as genetically more-or-less co-
herent group which shows primary differentiation caused
mainly by fractional crystallization. Tonalite, granodiorite to
granite sequences were regarded as common differentiation
trend characterized by the decreasing of compatible elements,
such as P, Zr, Hf, Cr, Ni, Co, V, and by the increasing of in-
compatible elements, such as Rb, Sn (e.g. Cambel & Vili-
novičová 1981; Cambel & Vilinovič 1987; Jacko & Petrík
1987; Hovorka & Petrík 1992; Kohút & Janák 1994). Occa-
sionally, besides the crystal fractionation, wall-rock assimila-
tion has been emphasized (Jacko & Petrík 1987). In the past,
the granite rock-forming minerals (feldspars, micas) were
studied in detail (e.g. Macek et al. 1979, 1982; Petrík 1980,
1982b; Vilinovičová 1989). Later geochemical granite subdi-
vision into I- and S-types were realized (Klomínský et al.
1981; Cambel & Petrík 1982; Cambel et al. 1985), the subdivi-
sion of the Ve ká Fatra granites into two separate independent
groups on the basis of bulk rock compositions was proposed
(Kohút 1992).
Using the fundamental mineralogical criteria, especially ac-
cessory mineral assemblages, zircon typology and allanite-
monazite dichotomy, together with geochemical and isotopic
data led to a subdivision of the West-Carpathian granites, into
monazite-ilmenite and allanite-magnetite group (Broska &
Uher 1991; Broska & Gregor 1992; Petrík & Broska 1994).
Later, the identification of post-orogenic A-type granites
mainly on the basis of zircon typology and trace-element
chemistry (Uher & Gregor 1992; Uher & Broska 1996) shed a
new light on the understanding of granite development in the
Western Carpathians. It resulted to the division of the West-
Carpathian granites into S-, I-, A-type groups (Petrík et al.
1994).
The aim of this paper is to characterize Variscan West-Car-
pathian granites on the basis of 166 new analyses in terms of
recently used genetic classification, based on S, I, A typology
(Chappell & White 1974; Whalen et al. 1987), except the De-
vonian metagranites (orthogneisses), which were not included
into the sample set. For this purpose, we subdivided studied
set of West-Carpathian granite analyses into the four geochem-
ical groups: (1) S-type granites, meso-Variscan (2) I-type,
80 BROSKA and UHER
meso- + late-Variscan, (3) A-type, post-Variscan and (4) post-
Variscan specialized rare-element S-type granites (S
S
-type).
Despite plotting of numerous discrimination diagrams of
granitic rocks, we present only the most distinctive ones in or-
der to demonstrate the chemical variability of the granite
groups. The contribution also illustrates an outline of the pos-
sible geotectonic scenario of the West-Carpathian Variscan
granites in sense of their time and spatial relationship.
Occurrences of the West-Carpathian
Variscan granitic rocks
Variscan magmatic activity is manifested by intrusions of
several granitoid plutons, separated tectonically in the princi-
pal West-Carpathian Alpine superunits: Tatric, Veporic and
Gemeric (Plašienka et al. 1997) Fig. 1. The granites often oc-
cur as sheet-like bodies (Kohút & Janák 1994) or laccoliths
(Lexa & Bezák 1996) and they are emplaced into metapelites
to metapsammites of amphibolite facies, locally contact ther-
mal metamorphism caused by granitoid intrusions occurs (e.g.
Krist et al. 1992). The protolith of the granites was represent-
ed mostly by the metapelites, metagreywackes or older meta-
granites (Petrík 2000). The inhomogeneties in Sm/Nd system
are interpreted as the evidence of contamination and/or mag-
ma mixing (Kohút et al. 1996, 1999a) and a Proterozoic recy-
cling component in granite protoliths is supposed (Kohút et
al. 1995, 1999a). At the present tectonic position, relatively
large granitic plutons crop out in the Tatric and Veporic Su-
perunits, in contrast to small and mostly hidden granitic bod-
ies in the Gemeric Superunit. The Velence granites in the
Trans-Danubian Superunit (Hungary), occur to the N of the
Balaton lineament and belong to the Western Carpathians
(cf. Plašienka et al. 1997). U-Pb and Rb-Sr isotope dating of
the West-Carpathian granitic rocks reveal a relatively wide
time span of their origin, around 150 Ma (e.g. Cambel et al.
1990; Petrík & Kohút 1997; Petrík 2000; Uher & Broska
2000; Poller et al. 2000).
Typology of the West-Carpathian
Variscan granitic rocks
S-type granites
They represent peraluminous biotite and two-mica granites
to granodiorites locally accompanied by numerous pegmatites.
They are characterized by the dominance of monazite-(Ce)
Fig. 1. Schematized geological map of the distribution of Variscan West-Carpathian granites. Explanations: MK – Malé Karpaty Mts, T –
Tribeč Mts, PI – Považský Inovec Mts, SMM Suchý and Malá Magura Mts, MF – Malá Fatra Mts, VF – Ve ká Fatra Mts, NT – Nízke
Tatry Mts, VT – Vysoké Tatry Mts, V – Velence Mts (Hungary).
WHOLE-ROCK CHEMISTRY AND GENETIC TYPOLOGY OF VARISCAN GRANITES 81
over allanite-(Ce) or absence of allanite accompanied with xe-
notime-(Y). The allanite-monazite dichotomy or antagonism
has been observed in the West-Carpathian granitic rocks for
over three decades (e.g. Hovorka & Hvož ara 1965; Chovan &
Határ 1978; Hvož ara 1979; etc.), and together with zircon ty-
pology, and presence of almandine and ilmenite, it became one
of the basic criteria for the genetic subdivision of the West-
Carpathian granites into the S- and I-type granite groups (Bros-
ka & Uher 1991; Broska & Gregor 1992; Petrík & Broska
1994). Zircon typology of the S-type granites (mainly S
1-2
,
S
6-7
, L
1-2
, G
1
subtypes) indicates low-temperature crustal alu-
minous character of the granites according to the Pupin (1980)
classification. Apatite locally show a dusky brown (smoky) co-
lour due to minute carbon-bearing inclusions, which indicates
low fO
2
conditions of crystallization (Broska et al. 1992).
These features are typical for peraluminous granitic rocks
which represent the most abundant granite type in the Western
Carpathians. They have been formed probably by biotite and/
or muscovite dehydration melting of upper crustal quartzo-
feldspathic rocks, such as greywackes, due to crustal thicken-
ing and prograde metamorphism during Carboniferous colli-
sion (Petrík et al. 1994). In accordance with isotopic dating
(e.g. Cambel et al. 1990; Krá et al. 1997), the monazite-(il-
menite)-bearing granites formed during the Meso-Variscan,
Lower Carboniferous period with the culmination of formation
at about 350 Ma.
I-type granites
I-type, allanite-bearing granites are metaluminous to slightly
peraluminous biotite (leuco)tonalites to granodiorites, rarely
biotite to muscovite-biotite granites, locally with pink K-feld-
spar phenocrysts. Except of allanite-(Ce), the typical primary
accessory mineral assemblage is represented by magnetite and
titanite. Zircon typology (mainly S
12
, S
16
subtypes) indicates a
medium-temperature crustal to crustal-mantle character. The
U-Pb zircon and Rb-Sr wall-rock dating show a wide age span
of I-type group granite formation, from meso-Variscan, Late
Devonian—Early Carboniferous (~370—340 Ma) to late-
Variscan, Late Carboniferous (~310—290 Ma) – Broska et al.
(1990), Bibikova et al. (1990), Cambel et al. (1990), Michalko
et al. (1998). On the basis of recent data, their origin is con-
nected with lower crustal continental melting with a contribu-
tion of infracrustal or mantle material (Petrík et al. 1994; Ko-
hút et al. 1999). Locally abundant microgranular mafic
enclaves in these granites, which are products of mixing of
melts, as well as the bulk chemistry is evidence for such pro-
cesses (Broska & Petrík 1993).
A-type granites
The recognition of the zircon typology with dominant high-
temperature and high-alkaline P- and D- zircon subtypes in
granites was the first impulse for the determination of these
post-orogenic A-type granites (Uher & Gregor 1992; Uher et
al. 1994). They form small intrusions of biotite leucogranites
to granite porphyries with hypersolvus, transsolvus to subsol-
vus textures (Uher & Broska 1996). The accessory mineral as-
semblage includes allanite-(Ce), magnetite or ilmenite, rarely
monazite-(Ce) (Uher & Broska 1996). U-Pb isotopic geochro-
nology of zircon showed the Permian to Triassic age of the A-
type granites (Uher & Pushkarev 1994; Putiš et al. 2000).
Specialized S-type granites
Specialized tin-bearing biotite-muscovite to muscovite
leucogranites, and rare granite porphyries from the Gemeric
Superunit (the Spiš-Gemer type) are the most evolved S-type
granites in the Western Carpathians. Locally greisen and albi-
tite cupolas with disseminated rare element Li, Sn, Nb, Ta, W,
F mineralization occur (Malachovský 1992 in Grecula 1995).
Accessory minerals of the Spiš-Gemer granites comprise tour-
maline (schorl to foitite), almandine, topaz, zircon, apatite, lo-
cally also rare monazite-(Ce), cassiterite, wolframite and Nb-
Ta phases (e.g. Faryad & Dianiška 1993). Zircon of S
8
subtype predominate. The character of zircon typology is dis-
tinct and distinguished these granites from the rest of the
West-Carpathian granites (Jakabská & Rozložník 1989; Bros-
ka & Uher 1991). The granites show Permian Rb-Sr WR and
mineral ages and they are characterized by very high initial Sr
isotope ratios, I
Sr
above 0.720 (Kovách et al. 1986; Cambel et
al. 1990). The Permian age was also constrained by monazite
probe dating (Finger & Broska 1999) and single-grain isotopic
dating of zircon (Poller et al. 2000).
Analytical methods
All 166 analyzed samples were obtained from the crushed
homogenized rocks of 3—12 kg in weight. Major elements and
Rb, V, Cr, Co, Ni, Zn, Sr, Ba, Th and U of the rocks were de-
termined by XRF at Ottawa University (Canada), and REE, Y,
Nb, Ta, Zr and Hf by ICP-MS in Memorial University of
Newfoundland (Canada). The analytical procedure of ICP-MS
was as follows: (1) sintering of a 0.2 g sample aliquot with so-
dium peroxide, (2) dissolution of the sinter cake, separation
and dissolution of REE hydroxide-bearing precipitate, (3)
analysis by ICP-MS using the method of internal standardiza-
tion to correct for matrix and drift effects. Natural rocks and
pure quartz reagent (blank) were used as reference standards.
For detailed information on the ICP-MS method see Jenner et
al. (1990) and Longerich et al. (1990).
Results
Major element geochemistry
Representative chemical analyses of the major elements of
all four geochemical granite groups are presented in Table 1,
statistical parameters are shown in the Table 2. The complete
data used for the construction of diagrams are available as
Table 3 on request in the Editorial Office or from the au-
thors.
The chemical analogue of the modal IUGS classification
by Streckeisen & Le Maitre (1979) using the Mielke & Win-
kler mesonormative calculation (1979), shows the preva-
82 BROSKA and UHER
lence of tonalites and granodiorites in the I-type granite
group, the S-type type of granitic rocks are granites, grano-
diorites, rarely tonalites and the A- as well as the S
S
-type be-
long to feldspar granites and syeno- as well as monzo-granites
(Fig. 2).
Another rock classification diagram expressing the balance
between characteristic peraluminous minerals (e.g. micas, gar-
nets) and metaluminous Al-poor, Ca-rich minerals (e.g. horn-
blende, epidote, titanite) after Debon & Le Fort (1983) shows
the distinct peraluminous character of practically all studied
West-Carpathian rocks except part of the subaluminous and
metaluminous I-type tonalites and diorites. The diagram re-
veals their dominantly crustal origin, with aluminic to alumi-
nocafemic associations (Fig. 3). Cafemic association (field IV)
is represented almost only by amphibole-biotite-bearing dior-
ites as well as microgranular mafic enclaves of tonalite-diorite
composition in I-type granites, which indicate their mantle ori-
gin (cf. Debon & Le Fort 1983). Amphibole-bearing tonalites
are very rare in this region, and the majority of granitic rocks
belong to biotite and two-mica types. S-type and specialized
S-type granites are plotted in field I (Ms>Bt), which is in ac-
cordance with the petrographic data. Biotite-bearing A-type
leucogranites (~4—5 vol. % Bt) and especially biotite-rich I-
type granites (~5—10 vol. % Bt) lie in the Bt>Ms (II) and Bt
(III) fields (Fig. 3).
A Na
2
O/K
2
O vs. SiO
2
diagram is plotted in Fig. 4. The
prevalence of Na
2
O over K
2
O is dominant for the S- and I-type
granites as was described earlier (e.g. Hovorka & Petrík 1992),
on the contrary, the A-type and S
S
-type granites show the
prevalence of K
2
O. The I-type granitic group shows a regular
trend of decreasing Na
2
O/K
2
O vs. SiO
2
content, whereas the
S-types exhibit distinctly scattered Na
2
O/K
2
O values and the
A- and S
S
-type granites are almost invariably below the value
of 1 (Fig. 4). Locally, high albite content, especially in the S-
type, cause the shift of Na
2
O/K
2
O ratio over 3. Other litho-
phile elements, as Mg, Ti and Mn do not discriminate the
West-Carpathian granite types distinctly.
The iron content is slightly higher in the A-type granites
than in the I- and S-type granites, whereas the specialized S-
type granites show generally low iron (Fig. 5).
Decreasing of P
2
O
5
content during the differentiation pro-
cess, caused mainly by apatite fractionation, is well docu-
mented for the I- and A-type granites while P
2
O
5
vs. SiO
2
distribution in both S- and S
S
-type granites show large irreg-
ularities (Fig. 6). The P
2
O
5
content in S-type decreases with
SiO
2
only in early less fractionated members (<70 % SiO
2
),
whereas the more fractionated and peraluminous granites
(>70 % SiO
2
) reveal scattered to increased content of P
2
O
5
(Fig. 6). The A-type granites form a distinct group with the
lowermost P
2
O
5
and apatite contents in comparison to the I-
and S-type granites.
Trace element geochemistry
Although zirconium and hafnium systematically decrease
with increasing of SiO
2
, there are a significant differences in
the distribution of these elements for A-type granites in com-
parison to the other granite groups (Fig. 7). The Hf vs. Zr dia-
gram shows a high positive correlation (R = 0.98, Fig. 8), how-
Fig. 3. A-B multicationic diagram (Debon & Le Fort 1983) of the
Variscan West-Carpathian granitic rocks.
Fig. 2. Mesonormative Q’-ANOR diagram of the Variscan West-
Carpathian granitic rocks. Explanations: aG – alkali-feldspar
granite; sG – syenogranite; mG – monzogranite; Grnd – gra-
nodiorite; T– tonalite; D – diorite (without BMF-8).
Fig. 4. Na
2
O/K
2
O vs. SiO
2
plot of the Variscan West-Carpathian
granitic rocks documenting the discrimination of the A-type gran-
ites. Na
2
O/K
2
O ratio below 1 is characteristic for the post-orogenic
granites.
ever, the diagram reveals a different trend for the A-type in
comparison with the rest of granite groups due to the higher
Zr/Hf ratio.
WHOLE-ROCK CHEMISTRY AND GENETIC TYPOLOGY OF VARISCAN GRANITES 83
Binary Ba vs. Rb and Sr vs. Rb and the ternary Rb-Ba-Sr
diagram (modified after El Bouseily & Sokkary 1975) clear-
ly discriminate relatively poorly evolved I- and S-type group
from mildly to highly evolved S-, A- and especially S
S
-type
granite groups (Figs. 9—11).
Chondrite-normalized rare earth element data show distinct
differences among S-, I- and A-type granites. The average pat-
terns of the normalized values show the highest value of the
REE and especially HREE for the A-type group (Fig. 12). The
HREE enrichment of the A-type group is documented also by
high yttrium concentrations – more than 20 ppm (Fig. 13).
The higher contents of the LREE are characteristic of the I-
types in comparison with both S-types, nevertheless the HREE
average content is almost identical for both granite groups
(Fig. 12). The similar slope of the rock/chondrite normalized
plot indicate similar differentiation tendencies of the S- and I-
type granites: Ce
N
/Yb
N
is 11.4 and 16.7, respectively. On the
contrary, the S
S
- and A-type granite groups clearly reveal
HREE enrichment: Ce
N
/Yb
N
is 2.8 and 5.6, respectively. The
more pronounced Eu-negative anomaly is typical of special-
ized S-type granites (Eu/Eu* = 0.2) and for the A-type (Eu/
Eu* = 0.4), on the other hand it is only 0.6 for the S-type
group, and the I-type group has an insignificant Eu-anomaly
(Eu/Eu* = 0.8).
Discussion
Geochemistry
The results show differences between all four groups of
Variscan West-Carpathian granitic rocks. The mesonorma-
tive Q’-ANOR diagram (Fig. 2) is generally concordant with
older modal and mesonormative diagrams (Petrík 1982a),
however, studied differentiated I-type granites lie mainly in
granodiorite and monzogranite fields, whereas common to-
nalite compositions were described by Petrík (1982a). The
multicationic A-B diagram (Debon & Le Fort 1983) reveals
generally aluminous crustal±alumino-cafemic character of
all granite groups, although with some tendency of I-type to
metaluminous mainly mantle domain which is typical of am-
phibole-bearing dioritic rocks and enclaves (Fig. 2). These
results are in accordance with mainly crustal character of S-,
A- and especially S
S
-type groups and with some mantle con-
tribution in the origin of the I-type group (Petrík et al. 1994;
Uher & Broska 1996; Petrík & Kohút 1997).
The exclusive character of the A-type group is documented
in Na
2
O/K
2
O vs. SiO
2
and FeO vs. SiO
2
plots (Figs. 4, 5)
which reflects presence of the K-feldspar and annite-rich bi-
Fig. 5. FeO
tot
vs. SiO
2
plot of the Variscan West-Carpathian granit-
ic rocks.
Fig. 6. P
2
O
5
vs. SiO
2
plot of the Variscan West-Carpathian granitic
rocks.
Fig. 7. Zr vs. SiO
2
plot of the Variscan West-Carpathian granitic
rocks.
Fig. 8. Hf vs. Zr plot of the Variscan West-Carpathian granitic
rocks.
84 BROSKA and UHER
dominate over Na
2
O is evident also for the S
S
-type group,
whereas, S- and especially I-type group are sodium-rich (Fig.
4). Consequently, the older meso- and late-Variscan granites
are mainly plagioclase-bearing rocks, whereas the post-
Variscan A- and S
S
-type exhibit K-feldspar dominance.
The very low P
2
O
5
contents in the A-type group (Tables 1—
3, Fig. 6) is comparable with other anorogenic granites
world-wide (cf. Whalen et al. 1987), and it should be one of
the typical feature of A-type granites, reflected in low
amount of apatite in these Ca, P-poor rocks. Low P contents
in the A-type granites could be explained by formation from
melt-depleted lower crust after main granite production dur-
ing Variscan orogeny. The I-type group shows negative cor-
relation between P
2
O
5
vs. SiO
2
due to apatite preferential
precipitation in the early differentiation members. On the
contrary, scattered P
2
O
5
contents is the consequence of the
higher P
2
O
5
solubility with increasing A/CNK in late frac-
tionated members (Pichavant et al. 1992). Moreover, positive
correlation between P
2
O
5
and SiO
2
in more evolved mem-
bers of S- and especially S
S
-type groups (>70 wt. % SiO
2
) is
connected with incompatible behaviour of P in strongly pera-
luminous, alkali- and fluid-rich magmas which resulted in
enrichment of P and its entry into alkali feldspar structure in
fractionated alkali-rich leucogranites (e.g. Pichavant et al.
1992; London 1992, 1998; Breiter 1998). Such a trend is
characteristic especially for phosphorus-rich rare-element
peraluminous granites of the Spiš-Gemer type (S
S
-group)
where K-feldspar contains up to 0.5 wt. % P
2
O
5
(Broska et
al. in prep.).
The content and behaviour of trace elements during differ-
entiation processes clearly characterize the differences be-
tween the S-, I- and A-type granitic rocks. Of special impor-
tance are the findings on the compatibility or incompatibility
of trace elements during differentiation. Some elements, such
as Sr, Sc, V, Zr, Cr and Co behave compatibly in all granite
types. Low Th and U content are not suitable for discrimina-
tion purposes as was formerly proposed by Yates et al.
(1982). On the contrary, Zr is a very useful element for gran-
ite discriminations. The Zr vs. SiO
2
diagram (Fig. 7) strongly
discriminates some of the A-type group from each other:
high and irregular distribution of Zr (Tables 1—3) is another
characteristic feature of alkali granites (e.g. Whalen et al.
1987). Very strong positive Hf vs. Zr correlation (Fig. 8) in-
dicates the close and exclusive relationship between zirconi-
um and hafnium in granitic magmas which resulted in crys-
tallization of zircon as an essential Zr, Hf-bearing phase in
all studied groups of granitic rocks. Different Zr/Hf ratio in
hypersolvus A-type group in comparison to the other granites
is probably related to contrasting solubility of Zr and Hf in
(per)alkaline Al-poor F-rich A-type magmas in comparison
to peraluminous H
2
O-rich S- and I-type granites. This is also
reflected in higher Zr/Hf ratios in zircon from post-orogenic
and anorogenic granite suites (Pupin 1992) and is also docu-
mented for zircon of West Carpathian A-type group (Uher &
Broska 1996).
The geochemical separation among granite types is strong-
ly apparent in the distribution of Rb, Sr and Ba, which are
concentrated mainly in the feldspars and micas. The highest
contents of Rb show specialized S- and A-type groups due to
Fig. 10. Sr vs. Rb plot of the Variscan West-Carpathian granitic
rocks.
Fig. 11. Rb-Ba-Sr ternary discrimination diagram of the Variscan
West-Carpathian granitic rocks. Explanations: 1 – poorly evolved
granites, 2 – mildly evolved granites, 3 – highly evolved granites.
Fig. 9. Ba vs. Rb plot of the Variscan West-Carpathian granitic
rocks. Note: The Turčok type represents anomalous A-type granite
with low Rb content (Gemeric Superunit).
otite in the granite group (Uher & Broska 1996). These
geochemical features are generally prominent in A-type
granites (Whalen et al. 1987). The tendency of K
2
O to pre-
WHOLE-ROCK CHEMISTRY AND GENETIC TYPOLOGY OF VARISCAN GRANITES 85
their higher level of fractionaction and K-feldspar enrich-
ment. On the contrary, less evolved, plagioclase-rich I- and
S-type granites exhibit the highest Ba and Sr but the lowest
Rb contents (Tables 1—3, Figs. 9—11). A general Rb-Sr-Ba
differentiated trend toward the specialized granites described
by El Bouseily & Sokkary (1975) is evident also in the West-
Carpathian granitic suites (Fig. 11). However, in our opinion,
fields such as “anomalous or normal granites, granodiorites
etc.” in the diagram of El Bouseily & Sokkary (1975) do not
discriminate the natural granite types properly and they are
inadequatly defined, in addition some of the West-Car-
pathian granites s.s. plot in the granodiorite field or vice ver-
sa. Therefore, we propose new categories for this ternary Rb-
Ba-Sr diagram according to their degree of differentiation:
poorly-evolved, mildly-evolved, to highly evolved granites
(Fig. 11). Such modification of the diagram allow us to use
Rb, Sr and Ba as the important discrimination parameters for
the classification of the West-Carpathian Variscan granite
suites and could be more generally useful.
REE,Y-distribution as well as the presence or absence of a
negative Eu-anomaly also discriminate all four geochemical
groups of the West Carpathian granites (Tables 1—3, Figs. 12,
13). Again, the A-type group strongly differs from each other
with high Y contents, generally over 20 ppm (Fig. 13). The Y
and HREE enrichment in the A-type granites is due to the high
content of zircon and locally also the presence of xenotime-
(Y) and garnet (Uher & Broska 1996). The bulk REE distribu-
tion is controlled by essential REE-bearing phases, such as al-
lanite-(Ce), monazite-(Ce) and xenotime-(Y), however a
contribution of almandine and zircon for bounding of HREE
and Y as well as apatite for LREE-fixing is also important
(e.g. Wark & Miller 1993). The wider range of the rare earth
elements abundance for the S-, but also for A-type granite, in
comparison with I-type is also a significant feature of the bulk-
rock chemistry of the West-Carpathian granites. Although the
I-type granite set also comprises differentiated dykes, the rare
earth elements pattern range is narrower mainly in the LREE
part of the diagram and max/min REE values are around 10, in
contrast to max/min REE values for the S-types of around 100
due to their more heterogeneous nature. We can only speculate
that such a difference in pattern is a result of the composition-
ally different precursor of I-type granites as well as their rapid
ascent and differentiation.
Fig. 13. Y vs. SiO
2
plot of the Variscan West-Carpathian granitic
rocks.
Fig. 12. Averages of the chondrite normalized REE patterns of the
Variscan West-Carpathian granitic rocks.
Fig. 14. Simplified geodynamic evolution of the principal granitic
groups in the Western Carpathians.
86 BROSKA and UHER
Table 1: Representative chemical analyses of the basic group of the West-Carpathian Variscan granites. Main elements (in wt. %), trace ele-
ments V to U (in ppm) are analysed by XRF, REE’s, Zr, Hf, Nb and Ta (in ppm) by ICP-MS. (Abr. tr. = trace content). Explanations: MK –
Malé Karpaty Mts, T – Tribeč Mts, PI – Považský Inovec Mts, MF – Malá Fatra Mts, SGR – Slovenské rudohorie Mts (Gemeric Supe-
runit), Vepor – Slovenské rudohorie Mts (Veporic Superunit), V – Velence Mts (Trans-Danubian Superunit, Hungary), PKB – Pieniny
Klippen Belt (pebbles).
Sample
ZK-48
T-87
Z-4/89
I-3
BMF-1
ZK-13
GZ-1
GZ-15
T-88
T-60/86
VG-54
ZK-118
BP-1
BP-35
VG-86
VE-4
type
S
S
S
S
S
Ss
Ss
Ss
I
I
I
I
A
A
A
A
Mts.
MK
T
Z
PI
MF
SGR
SGR
SGR
T
T
Vepor
Vepor
PKB
PKB
Vepor
V
SiO
2
69.67
71.37
72.95
73.44
68.26
74.05
71.21
72.85
64.63
74.30
64.57
65.55
74.49
71.85
70.72
76.87
TiO
2
0.40
0.37
0.19
0.21
0.34
0.11
0.04
0.21
0.79
0.12
0.80
0.78
0.15
0.27
0.33
0.05
Al
2
O
3
15.64
14.87
14.62
14.00
16.71
14.65
16.14
14.89
16.30
13.87
16.34
16.26
13.18
14.09
15.00
12.59
FeO
to t
1.96
2.31
1.59
1.75
2.49
1.15
1.53
1.32
4.40
1.12
4.29
4.06
1.86
2.10
2.48
0.63
MnO
0.05
0.05
0.04
0.03
0.04
0.02
0.02
0.02
0.07
0.02
0.07
0.05
0.03
0.02
0.06
0.01
MgO
0.85
0.87
0.36
0.36
0.71
1.60
0.24
0.91
1.77
0.25
1.62
1.56
0.09
0.82
0.99
0.04
CaO
2.61
1.73
1.19
1.18
2.81
0.34
0.30
0.26
3.55
0.89
3.59
3.24
0.36
1.25
0.26
0.50
Na
2
O
3.88
3.54
4.21
3.27
5.09
0.27
5.92
3.41
4.22
4.26
4.36
4.22
3.73
5.63
2.09
2.96
K
2
O
3.10
3.02
3.18
4.39
1.89
4.46
1.25
3.19
2.34
4.00
2.54
2.16
5.16
1.54
5.28
5.37
P
2
O
5
0.13
0.18
0.12
0.10
0.06
0.23
0.21
0.15
0.28
0.12
0.29
0.34
0.03
0.07
0.16
0.02
LOI
0.80
1.30
0.80
0.70
1.30
2.90
1.00
1.50
1.30
0.70
1.70
2.30
0.60
2.40
1.80
0.90
TOTAL
99.09
99.61
99.25
99.43
99.70
99.78
97.85
98.72
99.65
99.65
100.17
100.52
99.68
100.04
99.17
99.94
V
34
44
17
16
25
8
3
17
93
10
82
84
10
7
32
7
Cr
15
16
4
9
16
22
tr.
1
20
1
18
24
5
16
8
5
Co
4
15
1
2
2
33
8
6
11
tr.
7
6
7
2
5
1
Ni
tr.
4
tr.
tr.
tr.
5
5
6
5
tr.
4
3
tr.
3
9
2
Zn
58
60
50
53
60
19
78
24
77
20
89
76
73
25
18
17
Rb
119
92
101
138
54
400
173
300
72
113
67
59
209
79
233
277
Sr
289
482
261
203
498
15
30
13
852
193
860
850
24
65
42
32
Zr
170
143
98
111
154
62
33
133
240
60
237
268
247
422
129
64
Hf
5
4
2
3
4
2
1
3
5
2
6
6
5
9
3
2
Nb
11
9
8
12
7
14
4
10
13
8
18
14
14
16
10
10
Ta
0.75
0.84
0.46
0.77
0.34
5.46
2.38
1.19
0.59
0.85
1.35
0.53
1.07
1.18
1.22
1.56
Ba
830
854
844
988
327
117
42
150
1105
602
1263
1144
499
358
347
97
Th
12
9
7
13
9
9
15
21
10
9
9
12
19
20
14
30
U
1
4
3
2
3
5
3
4
5
0
4
9
1
2
2
4
Y
14.07
11.62
10.96
9.09
6.94
17.73
8.12
26.82
15.18
11.1
23.01
11.31
28.23
44.68
30.33
30.57
La
32.32
25.52
25.38
36.04
28.52
13.97
2.84
13.33
43.66
17.73
52.52
61.97
48.96
64.45
17.38
14.74
Ce
64.45
49.94
50.97
75.34
59.14
26.49
6.82
25.83
87.9
36.15
116.75
124.77
104.96
131.49
36.95
30.2
Pr
7.35
5.64
5.86
8.63
6.79
3.11
0.92
3.68
10.21
4.37
14.12
14.15
12.08
15.75
4.41
3.99
Nd
27.21
21.15
22.56
31.69
25.91
11.56
3.17
14.48
38.47
16.35
55.61
50.58
45.86
60.47
16.96
14.89
Sm
5.0
3.8
4.32
6.48
4.79
2.87
1.27
3.86
6.45
3.45
10.27
8.24
8.77
11.77
4.51
3.89
Eu
1.08
1.1
0.7
0.93
1.03
0.45
0.02
0.3
1.58
0.6
2.38
1.87
0.68
1.64
0.59
0.19
Gd
3.97
2.84
3.21
4.73
3.19
2.9
1.28
4.46
4.61
2.79
7.27
5.18
7.42
9.98
4.89
3.83
Tb
0.52
0.4
0.43
0.53
0.37
0.56
0.3
0.79
0.6
0.4
0.92
0.61
1.02
1.56
0.84
0.68
Dy
2.85
2.28
2.25
2.41
1.72
3.5
1.73
5.22
3.11
2.27
4.71
2.89
6.05
9.25
5.19
4.69
Ho
0.51
0.43
0.39
0.32
0.26
0.58
0.24
0.99
0.57
0.42
0.84
0.46
1.13
1.79
1.04
1.02
Er
1.38
1.11
0.97
0.69
0.6
1.45
0.62
2.88
1.49
1.13
2.42
1.09
3.16
5.0
3.04
3.27
Tm
0.19
0.15
0.13
0.09
0.09
0.2
0.09
0.45
0.21
0.16
0.36
0.13
0.45
0.74
0.46
0.52
Yb
1.26
0.95
0.83
0.42
0.62
1.17
0.55
2.99
1.27
1.05
2.19
0.94
2.83
4.69
2.83
3.9
Lu
0.19
0.14
0.13
0.07
0.1
0.15
0.06
0.43
0.19
0.14
0.32
0.14
0.43
0.68
0.4
0.63
An explanation of the Eu-anomaly is found mainly in the
different oxygen fugacity or water activity of the primary
melts. In concordance with Puchelt & Emmermann (1976),
Williams (1997), Sha & Chappel (2000), we regard the nega-
tive anomaly as an indicator of lower fO
2
provided that the
whole rock was not depleted in europium. The negative Eu-
anomaly originated under reducing conditions, when europi-
um occurs only in the divalent state and it is incorporated
into plagioclase. Lower fO
2
or water activity in the melts in
comparison with I-type granites was actually assumed for S-
type groups also on the basis of Fe
2+
-rich accessory mineral
paragenesis (presence of almandine and ilmenite, absence of
magnetite, allanite and titanite). Biotite composition indicat-
ed the I-type granitoids originated in relatively oxidized and
water-rich conditions (about 5—6 wt. % of water), on con-
trary, the S-type granites crystallized from a relatively re-
duced magma with low water content (2—3 wt. % ) (Petrík &
Broska 1994; Petrík & Kohút 1997). The oxidized conditions
in the I-type melt provided the trivalent state of Eu and it ex-
plains, why europium was not able to fractionate with feld-
spars in these granites.
Geodynamic scenario of granite origin
The compositional variations and differences among the
granitic groups of the Western Carpathians reflected their
genesis including the geotectonic position and source rocks.
The geotectonic position of the S and I-type granites was
WHOLE-ROCK CHEMISTRY AND GENETIC TYPOLOGY OF VARISCAN GRANITES 87
Table 2: Average and ranges of granitic rock compositions (distribution see in the Fig. 1). Note: 6 diorite analyses are not presented.
S-type n = 78
spec. S-type n = 22
I-type n = 29
A-type n = 30
Sample
av.
st. dev.
max.
min.
av.
st. dev.
max.
min.
av.
st. dev.
max.
min.
av.
st. dev.
max.
min.
SiO
2
71.84
2.89
77.45
63.02
72.04
2.83
75.93
65.30
67.82
3.60
74.30
62.51
72.86
2.45
78.93
68.65
TiO
2
0.26
0.19
0.89
0.02
0.17
0.17
0.73
0.04
0.57
0.32
1.25
0.09
0.24
0.10
0.46
0.05
Al
2
O
3
14.90
0.99
18.48
12.84
14.78
1.67
19.18
13.07
15.35
1.18
18.85
13.50
13.77
0.88
15.69
12.45
Fe
tot
1.96
1.16
6.50
0.43
1.63
0.75
3.99
0.82
3.37
1.34
5.79
1.12
2.27
0.92
3.99
0.46
MnO
0.04
0.04
0.23
0.00
0.04
0.07
0.37
0.01
0.06
0.02
0.10
0.02
0.05
0.10
0.59
0.00
MgO
1.02
3.38
30.00
0.06
4.42
19.34
91.00
0.05
1.32
0.65
2.98
0.19
0.43
0.29
1.00
0.02
CaO
1.38
0.90
3.03
0.14
0.38
0.35
1.88
0.14
2.40
1.12
3.79
0.30
0.74
0.51
2.20
0.04
Na
2
O
3.94
0.79
5.51
0.27
3.42
1.33
5.92
0.13
3.98
0.67
6.83
3.03
3.92
1.09
7.99
2.96
K
2
O
3.17
1.08
5.31
0.90
4.23
1.48
5.87
0.37
3.20
1.14
7.07
1.94
4.18
1.35
5.37
0.10
P
2
O
5
0.15
0.07
0.57
0.04
0.18
0.06
0.33
0.06
0.24
0.11
0.45
0.07
0.07
0.04
0.19
0.01
V
26.0
22.4
97
1.0
10.0
10.0
41
1.0
63.1
33.9
125
10.0
14.9
11.2
43
tr.
Cr
14.0
23.5
184
tr.
8.6
7.1
22
1.0
21.5
10.3
53
1.0
15.2
19.5
108
2.0
Co
6.5
6.5
30
tr.
8.6
9.5
40
tr.
10.0
7.8
34
1.0
5.5
7.6
33
1.0
Ni
6.1
12.9
83
tr.
6.2
5.7
29
1.0
5.7
5.0
27
tr.
4.4
6.4
33
tr.
Zn
43.6
27.2
139
2.0
37.7
16.1
78
14.0
66.2
27.7
114
15.0
49.9
23.3
110
9.0
Rb
103.0
39.2
233
24.0
400.7
179.3
868
173.0
86.1
23.6
159
58.0
185.4
65.9
277
6.0
Sr
300.5
219.0
1056
10.0
24.8
15.4
82
7.0
599.2
242.8
906
81.0
74.8
65.4
344
10.0
Zr
113.1
60.6
272
18.0
82.8
47.5
214
26.0
185.6
79.1
309
46.0
241.7
132.2
649
64.0
Nb
8.1
2.9
18
1.0
11.2
4.0
18
1.0
11.1
4.4
21
5.0
15.1
3.8
26
9.0
Ba
693.4
399.0
2469
32.0
120.7
84.0
310
29.0
1100
365.2
2146
455.0
479.1
312.6
1294
29.0
Nd
22.7
12.5
53
tr.
12.4
10.2
41
0.0
37.8
17.8
85
5.0
38.6
17.9
84
3.0
Th
8.2
6.2
42
tr.
19.2
17.7
95
8.0
11.2
6.3
35
4.0
19.4
7.5
52
10.0
U
2.5
1.7
8
tr.
20.5
62.2
298
2.0
4.1
2.9
14
tr.
3.4
2.2
8
tr.
Y
12.00
6.05
31.07
3.91
20.27
7.20
30.77
8.12
14.70
7.95
37.02
2.79
38.90
27.81
157.59
15.34
Nb
8.00
3.52
21.96
1.22
14.30
4.29
22.32
6.69
10.88
5.14
25.40
3.56
16.41
5.61
32.74
2.86
La
23.34
12.99
70.91
0.84
9.37
6.26
25.35
2.60
40.90
18.92
86.91
12.96
38.28
20.27
78.84
4.81
Ce
48.00
25.60
126.98
1.58
22.06
14.39
55.55
6.82
84.58
39.84
179.40
22.90
81.00
42.15
175.60
9.10
Pr
5.52
2.87
13.09
0.18
2.64
1.58
6.77
0.88
9.45
4.90
19.32
1.09
9.69
5.25
21.33
1.87
Nd
20.73
10.63
47.55
0.50
9.96
6.04
26.04
3.17
37.02
17.84
70.73
10.46
37.30
20.65
84.29
8.54
Sm
4.03
1.78
8.66
0.19
2.81
1.27
6.14
1.27
6.43
3.01
13.56
2.34
8.12
5.05
26.57
2.66
Eu
0.80
0.35
1.87
0.02
0.19
0.17
0.68
0.02
1.43
0.68
3.19
0.46
0.97
0.63
2.92
0.03
Gd
3.15
1.36
7.52
0.19
2.90
1.15
5.64
1.28
4.53
2.20
10.36
1.57
7.58
5.69
32.46
2.36
Tb
0.45
0.19
1.18
0.07
0.59
0.18
0.94
0.30
0.58
0.29
1.42
0.14
1.21
0.92
5.26
0.42
Dy
2.44
1.15
6.56
0.67
3.87
1.23
5.76
1.73
3.04
1.57
7.57
0.62
7.49
5.38
30.48
2.87
Ho
0.44
0.22
1.22
0.13
0.71
0.28
1.14
0.24
0.55
0.29
1.40
0.10
1.49
1.07
5.97
0.54
Er
1.16
0.63
3.41
0.31
2.04
0.93
3.41
0.62
1.47
0.84
3.81
0.30
4.33
2.91
15.91
1.55
Tm
0.16
0.09
0.52
0.02
0.31
0.15
0.54
0.09
0.21
0.13
0.55
0.05
0.63
0.37
1.81
0.23
Yb
1.00
0.57
3.42
0.04
2.02
1.02
3.38
0.55
1.31
0.80
3.51
0.36
4.17
2.23
11.82
1.56
Lu
0.15
0.08
0.51
0.05
0.28
0.16
0.51
0.06
0.19
0.11
0.50
0.07
0.63
0.33
1.76
0.21
Hf
2.99
1.38
6.46
0.48
2.00
0.83
4.74
1.21
4.69
1.80
7.42
1.46
5.27
2.23
11.60
1.85
Ta
0.73
0.43
2.03
0.10
2.67
1.24
5.46
1.19
0.74
0.38
1.50
0.23
1.33
0.45
3.06
0.57
Th
8.35
6.06
42.36
0.56
10.72
2.72
18.64
7.21
11.69
6.01
35.04
3.79
17.59
7.55
51.03
6.16
firstly discussed by Petrík et al. (1994), and the A-type gran-
ites by Uher & Broska (1996). In addition, we propose a
modified outline of the genesis of all four principal Variscan
granitic groups in the Western Carpathians, subdivided ac-
cording to the presented mineralogical and geochemical cri-
teria (Fig. 14). Early Carboniferous continental collision,
which in generally operated in the European Variscides
(Matte 1986; Finger & Steyrer 1990; von Raumer & Neubau-
er 1993; Stampfli 1996 among others), led to crustal thicken-
ing along thrusting planes, formation of the Variscan nappes
and partial melting of the lower crust in the zone of contrac-
tion of the lithospheric slab. After subduction of oceanic
crust along destructive active plate margins (Stampfli 1996),
the lower density of the continental crust, which is buoyant
and remains on the upper surface of the lithosphere, led to
thickening of the collided continents and crust (Fig. 14A).
Emplacement of the S-type granite, which originated mainly
from the metagreywacke protoliths (Petrík 2000) as well as
granites with transitional features between the S- and I-type
group probably from the amphibolite-bearing lower crust
(Kohút et al. 1999b), occurred in the extension zones, which
occur locally in the framework of the continental collision
(Schaltegger 1997) or in the upper part of the flexures of the
lithosphere plate (Fig. 14A) (c.f. Coward 1994). A local ex-
tension zone is indicated for example by the presence of lac-
colith (Lexa & Bezák 1996) but also by the sheet-like shape
of the emplaced plutons (Kohút & Janák 1994). However, the
numerous pegmatites accompanying the S-type granites in
the Western Carpathians show the general collisional (com-
pression) conditions. On the other hand, post-collisional tec-
tonics associated with the gravitational instability of thicken-
ing lithosphere started the process of thinning of the
lithosphere and extensional regime, which resulted in the
production of the I-type granites with lesser pegmatite for-
88 BROSKA and UHER
mation in the region. The origin of the I-type granites show
the distinct influence of the mantle or infracrustal contribu-
tion and process of their melting was triggered by heating of
the crust due to the underplated mafic lithospheric mantle
melt (Fig. 14B) which was primarily activated by previous
detaching of the oceanic slab and its injection into the mantle
(Fig. 14A). Uplift into a vertical tectonic extensional fault
system is followed by formation of larger batholiths (Hutton
1987) in the middle crust which is observed mainly in the
Veporic Superunit. The thermal influence of the huge cham-
bers of I-type granite melts in the middle crust also caused
the partial melting of the middle crust and origin of a new
generation of the S-type granite (Hraško et al. 2000). The S-
and I-type granite can be regarded as orogenic granites. In
contrast, the A-type granites which were formed in the Pan-
gaea continent (Late Paleozoic to Mesozoic supercontinent
– see e.g. Johansson 2000) belong already to post-orogenic
granite suites which are typically distributed in European
Variscan terrain along the strike-slip lineaments and faults in
the crust (Bonin 1990) (Fig. 14C). The process of A-type
granites formation is associated with melting of granitic
sources (Petrík 2000) and emplaced during extension and
transtension regime. The specialized S-type granites (S
S
-
type), which occurred in the same period as the A-type gran-
ites, were probably melted from the muscovite metapelites
(Petrík 2000) in the middle crust and during continuation of
the thermal event caused by underplated mafic melts, which,
through deep rifts to the mantle, also formed numerous vol-
canic extrusions in the Permian or Permian—Triassic age
(Fig. 14C). The rifting process, which opened the Meliata-
Hallstadt ocean in Triassic, could have been a thermal source
for melting of the middle crust.
Conclusions
The results presented generally support the subdivision of
the Variscan West-Carpathian granites into four genetic
geochemical groups based on older mineralogical, geochemi-
cal and isotope data.
The S-type group exhibits typical features of orogen-related
crustal granites with a relatively wide span of fractionation
level. The I-type group represents relatively poorly evolved
rocks enriched in compatible elements such as Ba, Sr, Zr and
REE’s with a possible contribution of mantle material during
their origin. The A-type group represents a specific post-oro-
genic hot and dry granite with a relatively high fractionation
level rich in compatible (REE, Y, Zr) as well as alkali elements
(K, Rb). The S
S
-type group belongs to the highly-evolved B,
Sn peraluminous and P-enriched suite with rare-element spe-
cialization (high Si, K, Ta, Sn, F, Rb, Nb). The different char-
acter of these principal granite groups in the Western Car-
pathians is reflected in their geotectonic positions. The S- and
I-type granites as representatives of the orogenic granites are
directly connected with collisional and extensional regime
during/after continent collission with a various contribution of
mantle lithospheric melt especially in the post-collisional tec-
tonics. On the other hand, the A- and S
S
granite types formed
in post-orogenic conditions.
Finally, the major and trace-element geochemistry together
with the accessory mineral paragenesis clearly document a
complex and long history of Variscan granite origin in the
West-Carpathian area from early-orogenic to post-orogenic
stages and it could contribute to the understanding of such
evolution in analogous orogenic belts.
Acknowledgements: The work was supported by NSERC Re-
search Grant and a Major Installation Grant to P. Černý, Univ. of
Manitoba, Winnipeg, Canada, during Post-Doctoral Fellowship
of P. U. in Canada. The evaluation of the samples was financed
by VEGA Grant #7074. The authors thank to M. Kohút and I.
Petrík for providing some samples for fruitful discussion which
improved the early version of the manuscript. We are also
grateful to D. Plašienka and W.E. Stephens for their comments
and to L. Zahradník for his assistance with PC. The paper is a
contribution to the UNESCO “International Geological Correla-
tion Project #373” headed by R. Seltmann.
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