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, JUNE 2014, 65, 3, 177—194 doi: 10.2478/geoca-2014-0012
Introduction
The Periadriatic-Balaton Lineament (PABL) is a major dextral
shear zone in the Alpine-Carpathian orogeny that is dividing
the Eastern and the Southern Alps in the west, as well as the
ALCAPA (Alp-Carpathian-Pannonian) and Zagorje-Mid-
Transdanubian Units along its eastern section (Fig. 1). The
structurally deformed zone of the PABL was a principal chan-
nel of magma and fluid flow in various geotectonic situations,
from the Mesozoic onwards. The formation of Cretaceous
lamprophyric magmatism (Eisenkappel, Velence Mts), Paleo-
gene and Neogene intermediate magmatism (Recsk, Velence
Mts), diorite intrusions and stratovolcanoes (Zala Basin volca-
nics in the Pannonian Basin; Adamello, Berger plutons;
Pohorje intrusions in the Alps; Fig. 1) as well as various types
of mineralization (Cu-porphyry, epithermal, lead-zinc epige-
Triassic fluid mobilization and epigenetic lead-zinc sulphide
mineralization in the Transdanubian Shear Zone
(Pannonian Basin, Hungary)
ZSOLT BENKÓ
1
, FERENC MOLNÁR
1
, MARC LESPINASSE
2
, KJELL BILLSTRÖM
3
,
ZOLTÁN PÉCSKAY
4
and TIBOR NÉMETH
1,5
1
Department of Mineralogy, Eötvös Loránd University, Budapest, Hungary; zsoltbenkoo@gmail.com; ferenc.molnar@gtk.fi
2
University of Lorraine, UMR GeoRessources 7359, CNRS-CREGU BP 239, Bd des Aiguillettes, 54506 Vandoeuvre les Nancy Cedex,
France; marc.lespinasse@univ-lorraine.fr
3
Laboratory of Isotope Geology, Swedish Natural History Museum, Stockholm, Sweden; kjell.billstrom@nrm.se
4
Institute of Nuclear Research, Hungarian Academy of Sciences, Debrecen, Hungary; zoltan.pecskay@gmail.com
5
Institute for Geochemical Research, Hungarian Academy of Sciences, Budapest, Hungary; ntibi@geochem.hu
(Manuscript received November 28, 2013; accepted in revised form March 11, 2014)
Abstract: A combined fluid inclusion, fluid inclusion plane, lead isotope and K/Ar radiometric age dating work has been
carried out on two lead-zinc mineralizations situated along the Periadriatic-Balaton Lineament in the central part of the
Pannonian Basin, in order to reveal their age and genetics as well as temporal-spatial relationships to other lead-zinc-
fluorite mineralization in the Alp-Carpathian region. According to fluid inclusion studies, the formation of the quartz-
fluorite-galena-sphalerite veins in the Velence Mts is the result of mixing of low (0—12 NaCl equiv. wt. %) and high
salinity (10—26 CaCl
2
equiv. wt. %) brines. Well-crystallized (R3-type) illite associated with the mineralized hydrother-
mal veins indicates that the maximum temperature of the hydrothermal fluids could have been around 250 °C. K/Ar
radiometric ages of illite, separated from the hydrothermal veins provided ages of 209—232 Ma, supporting the Mid- to
Late-Triassic age of the hydrothermal fluid flow. Fluid inclusion plane studies have revealed that hydrothermal circulation
was regional in the granite, but more intensive around the mineralized zones. Lead isotope signatures of hydrothermal
veins in the Velence Mts (
206
Pb/
204
Pb = 18.278—18.363,
207
Pb/
204
Pb = 15.622—15.690 and
208
Pb/
204
Pb = 38.439—38.587)
and in Szabadbattyán (
206
Pb/
204
Pb = 18.286—18.348,
207
Pb/
204
Pb = 15.667—15.736 and
208
Pb/
204
Pb = 38.552—38.781) form
a tight cluster indicating similar, upper crustal source of the lead in the two mineralizations. The nature of mineralizing
fluids, age of the fluid flow, as well as lead isotopic signatures of ore minerals point towards a genetic link between
epigenetic carbonate-hosted stratiform-stratabound Alpine-type lead-zinc-fluorite deposits in the Southern and Eastern
Alps and the studied deposits in the Velence Mts and at Szabadbattyán. In spite of the differences in host rocks and the
depth of the ore precipitation, it is suggested that the studied deposits along the Periadriatic-Balaton Lineament in the
Pannonian Basin and in the Alps belong to the same regional scale fluid flow system, which developed during the advanced
stage of the opening of the Neo-Tethys Ocean. The common origin and ore formation process is more evident considering
results of large-scale palinspastic reconstructions. These suggest, that the studied deposits in the central part of the Pannonian
Basin were located in a zone between the Eastern and Southern Alps until the Early Paleogene and were emplaced to their
current location due to northeastward escape of large crustal blocks from the Alpine collision zone.
Key words: Triassic, Velence Mts, Szabadbattyán, Periadriatic-Balaton Lineament System, lead isotopes, fluid inclu-
sions, Alpine-type epigenetic lead-zinc mineralization.
netic at Recsk and in the Velence Mts) is clearly or apparently
controlled by the repeated reactivation of this fault system.
Along the eastern segment of the PABL, in the central part
of the Pannonian Basin two Paleozoic, allochthonous com-
plexes, the Szabadbattyán Block and the Velence Mts crop
out. The western part of the Velence Mts is built up of early
Permian monzogranite, which is the host of vein-type fluo-
rite-galena-sphalerite-calcite mineralization (hereinafter base-
metal-fluorite veins). The near-by (30 km) Szabadbattyán
Block is composed of structurally deformed Paleozoic
metasedimentary rocks and Triassic andesitic intrusions. The
Devonian limestone at Szabadbattyán is host of vein-, and
metasomatic-type Pb mineralization.
The age and origin of both mineralizations have been con-
troversial for a long time (Velence Mts: Jantsky 1957; Kas-
zanitzky 1958; Horvát Ódor 1984; Molnár 1996, 2004,
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Fig. 1. Geological overview map of the Alp-Carpathian region compiled after Kovács et al. (2007) and Köppel (1983). Abbreviations: Faults:
PABL – Periadriatic Balaton Lineament System. Epigenetic lead-zinc deposits along the PABL: Sal – Salafossa, Blei – Bleiberg. Paleo-
gene plutons and volcanites: A – Adamello Pluton, B – Bergell Pluton, ZB – Zala Basin, R – Recsk. Carboniferous to Permian granite
intrusions along the PAL: a – Bressanone Pluton, b – Eisenkappel Pluton, c – Buzsák, d – Ságvár, Ka – Karawanken Mts. Tectonic
units: ZMTU – Zagorje—Mid Transdanubian Unit.
Table 1: Summary of magmatic and hydrothermal processes and their characteristics in the Velence Mts and Szabadbattyán Block.
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TRIASSIC FLUID MOBILIZATION AND EPIGENETIC SULPHIDE MINERALIZATION (HUNGARY)
Szabadbattyán: Kiss 1951; Földvári 1952; Kiss 2003), due to
their allochthonous, exotic positions along the PABL.
In order to shed further light on the timing, nature of ore-
forming processes and paleogeographical relations of the
mineralizations in the two Paleozoic units we have adopted a
multi-method approach. Fluid inclusion microthermometry
as well as a new method, called Fluid Inclusion Plane (FIP)
technique have been performed to extend the existing know-
ledge about the nature of ore-forming fluids and enable a dis-
cussion on the depth of ore formation. Lead isotope data
were collected in order to elucidate the timing and the origin
of the Pb components in the ore. Furthermore, we have car-
ried out K/Ar radiometric age determinations on hydrother-
mal clay mineral assemblages and a rock forming mineral
surrounding the veins for a better determination of age con-
straints of ore formation.
Regional geology and hydrothermal processes
The Velence Mts are located along the southern part of the
Alcapa Megaunit and the northern side of the PABL (Fig. 1).
The Alcapa Megaunit is composed of the metamorphosed
Proterozoic to Mesozoic blocks of the Eastern Alps, the Paleo-
zoic low-grade metamorphic and Mesozoic carbonaceous se-
quences of the Transdanubian Mountain Range (TMR), the
Bükk Mts, as well as the crystalline blocks of the Inner West-
ern Carpathians (Fig. 1). By the Oligocene—Early Miocene,
the Alcapa Megaunit escaped northeastward from the Alpine
collision zone (Kázmér & Kovács 1985; Csontos et al. 1992;
Fodor et al. 1998; Haas et al. 2000). The total 350—400 km
present day offset can be attributed to the Paleogene to Mid-
Late Miocene extension, lateral extrusion and counter-clock-
wise rotation of the Alcapa Megaunit (Tari 1996; Csontos &
Fig. 2. Geology of the Velence Mts, modified after Dudko (1999) with sample localities of the current study.
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Vörös 2004). Along the PABL, Paleozoic and Paleogene
units can be regarded as allochthonous blocks in a tectonic
mega-mélange between the Alcapa and Zagorje-Mid-Trans-
danubian Unit (Fig. 1).
The Velence Mts consist of two major units: the western unit
is a Permian monzogranite intrusion; the eastern unit is an Early
Oligocene intrusive-volcanic complex of intermediate composi-
tion (Fig. 2). The granite intrusion can be further divided into
two blocks. The boundary between the eastern and the western
part of the granite intrusion is the Pákozd Line which is a post-
Triassic normal fault (Benkó 2008). The complete sequence of
magmatic and hydrothermal events and p-T conditions of the
different processes are summarized in Table 1.
The Permian granite is an A-type, peraluminous biotitic
monzogranite (Uher & Broska 1994, 1996; Broska & Uher
2000; Finger et al. 2003), which intruded into an early Paleo-
zoic anchimetamorphic slate at 274—290 Ma (Balogh et al.
1983; Buda 1985; Buda et al. 2004). The results of mineral-
ogical and fluid inclusion studies by Molnár (1997) suggested
that the superimposing quartz-molybdenite-pyrite-grey ore
stockwork mineralization along the contact of the granite
and the shale was linked to the post-magmatic hydrothermal
system of the granite.
The N—S and NE—SW striking base-metal-fluorite veins
occur in the western part of the granite body of the Velence
Mts (Fig. 2). These veins are surrounded by argillic alter-
ation (illite, kaolinite, smectite) envelopes (Nemecz 1973;
Benkó 2008). Galena and sphalerite are co-genetic phases,
whereas fluorite is partially co-genetic, and partly younger
than other ore minerals. Characteristic ore textures are co-
cade and brecciated (Jantsky 1957). According to sulphur
isotope studies (Benkó 2008) the maximum temperature of
ore formation was around 230—250 °C.
By the time of the Late Cretaceous, the granite was intruded
by monchiquite-spessartite dykes (Horváth & Ódor 1984).
These dykes were K/Ar dated at 77.6 ± 30 Ma (Balogh et al.
1983). The dykes are not altered and they did not generate
hydrothermal alteration in the granite host.
In the eastern part of the Velence Mts, a hydrothermally
altered and eroded andesitic stratovolcanic structure (dated
by the K/Ar method at 28—30 Ma; Bajnóczi 2003) crops out
and this unit is underlain by diorite intrusions (Fig. 2). The
Paleogene calc-alkaline igneous rocks are characterized by
medium- to high-K content and they are regarded as results
of syn- to post-syncollisional magmatism, which occurred
by the collision of the Apulian Microplate (of African origin)
and the European Plate (Darida-Tichy 1987; von Blancken-
burg 1995; Benedek 2002; Benedek et al. 2004).
In the Paleogene Volcanic Unit of the Velence Mts, Cu-por-
phyry and minor skarn mineralization is spatially linked to
the diorite intrusion whereas alteration zones typical for
high-sulphidation type epithermal systems are known in the
outcrops of the stratovolcano (Molnár 1996, 2004; Bajnóczi
et al. 2002; Bajnóczi 2003).
The hydrothermal system of the Paleogene age has also in-
teracted with the Permian granite intrusion in the eastern part
of the Velence Mts, east of the Pákozd Line (Molnár 2004;
Benkó & Molnár 2004; Benkó et al. 2012). Secondary fluid
inclusions that are attributed to the Paleogene fluid circula-
tion in the old granite can easily be recognized in rock form-
ing quartz, because the Paleogene fluid circulation took place
under low pressure (max. 150—200 bar) boiling conditions
resulting in common occurrences of vapour phase-rich and
liquid phase-rich (sometimes halite bearing) fluid inclusions.
The Szabadbattyán Block is a thrusted unit composed of
metamorphosed slate, phyllite, and carbonate nappes (Fig. 3).
Igneous activity is marked by the presence of Carboniferous
granite porphyry dykes, whereas andesite dykes of Triassic
age (K/Ar data from Balogh et al. 1983 and Bagdaszarjan
1989) intrude the Polgárdi Limestone Formation (Table 1).
The epigenetic base-metal mineralization occurs in fractures
and as roughly bedding—parallel metasomatic-replacement
bodies in the Polgárdi Limestone Formation. The major ore
mineral is galena. Bournonite, sphalerite, chalcopyrite, tetra-
hedrite and native silver are the most common minerals asso-
ciated with galena (Szakáll & Molnár 2003).
Fig. 3. Section of the Szabadbattyán area (Fülöp 1990).
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TRIASSIC FLUID MOBILIZATION AND EPIGENETIC SULPHIDE MINERALIZATION (HUNGARY)
Sampling and analytical methods
There are no outcrops of the discussed mineralizations
therefore no detailed field work has been carried out on these
formations. Mineralized samples were collected from the
historical Mineralogical Collection of the Eötvös Loránd
University, Budapest. Sample localities of rock samples are
summarized in Fig. 2.
Fluid inclusion studies have been carried out on quartz,
fluorite and sphalerite from the base-metal-fluorite veins in
the Velence Mts. For comparison, we also analysed second-
ary fluid inclusions in rock forming quartz from unaltered
granite and from the alteration halo of the hydrothermal
veins. To establish the relationships between argillic alter-
ation zones and fluid inclusion assemblages responsible for
their formation, the FIP method was applied. In order to de-
termine the extension of the hydrothermal fluid flow, and the
rock volume affected by the hydrothermal system, fluid in-
clusion thermometry and FIP studies have been carried out
on the inclusions of the rock forming quartz crystals. Details
of the FIP method have been published in Lespinasse &
Pecher (1986), Lespinasse & Cathelineau (1990), Lespinasse
et al. (2005). Briefly, FIP are Type III extensional microfrac-
tures that form always perpendicular on the minimum stress
axes of the stress field in rock forming quartz crystals of gra-
nitic rocks. If the age of the fluid circulation and hence the
age of the FIPs is known one can determine the minimum
stress axes of the stress field during fluid flow and mineral-
ization. Another advantage of the method is that FIP density
(number of FIP per unit surface, expressed in 1/mm
—2
and
cumulative length per unit surface expressed in mm/mm
2
) in
the rock forming quartz crystals displays a systematic in-
creasing trend towards the alteration zones (e.g. argillic al-
teration zones, vein swarms; Benkó et al. 2008). Using this
approach, secondary fluid inclusions in magmatic quartz
crystals of granite can be directly related to certain alteration
zones (e.g. argillic alteration) that do not contain hydrother-
mal minerals with primary fluid inclusions. Fluid inclusion
assemblages and FIP density were analysed by the computer
code AnIma (Lespinasse et al. 2005), developed at the Uni-
versity of Lorraine, Nancy, France.
Fluid inclusion microthermometric studies were carried
out on a Chaixmeca heating—freezing stage. The studies have
yielded reproducible temperatures within ± 0.1 °C (below
0 °C) and ± 1 °C (above 0 °C), respectively. The equipment
was standardized with synthetic fluid inclusions (H
2
O—CO
2
and pure water) of known microthermometric properties (i.e.
triple point temperature for pure CO
2
at —56.6 °C, melting
temperature of ice at 0 °C). Thin sections used for fluid in-
clusion petrography and microthermometry were double pol-
ished 100—150 µm thick. Characteristic isochors were
calculated using the equations of Zhang & Frantz (1987).
The salinities of the aqueous fluid inclusions were calculated
using the experimental equation of states of Oakes et al.
(1990) and Bodnar (1993).
K/Ar radiometric age determinations were carried out at
the Institute of Nuclear Research of the Hungarian Academy
of Sciences. Details of the analytical methods can be found
in Balogh (1985). Clay mineral phases were collected from
alteration selvages of base-metal-fluorite veins cutting the
granite and from NE—SW trending clay mineral filled veins.
Purity and composition of the mineral fractions were con-
trolled by X-ray powder diffraction (XRPD). After careful
separation and mild crushing, the samples were suspended in
water glass columns for 200 minutes. Following Stoke’s law
we then extracted the portion of the suspension which con-
tained the < 2 µm size clay mineral fraction. This fraction
has the greatest surface area/volume ratio and hence is the
most susceptible to diffusion of radiogenic Ar. Nevertheless,
several authors presented meaningful K/Ar age data also
from < 0.2 µm and < 0.1 µm size fractions (e.g. Zhao et al.
1997; Zwingmann et al. 2010), especially from sedimentary-
diagenetic environments and from shallow fault gauges.
The mineral composition of the clay fraction was deter-
mined on the separated, randomly oriented powder samples
by semi-quantitative phase analysis. Three aliquots of each
sample were separated for diagnostic treatments. Clay miner-
als were identified by XRD diagrams obtained from parallel-
oriented specimens. Diagnostic treatments were carried out for
the identification and characterization of the clay minerals.
Samples were treated by ethylene-glycol at 60 °C overnight
for the detection of swelling clay minerals and mixed layer
clay minerals. Magnesium saturation followed by glycerol
solvation at 95 °C overnight was used to distinguish smectite
and vermiculite. Layer charge of swelling clay minerals was
estimated by potassium saturation. Chlorite-kaolinite dis-
tinction is based on heating of the samples at 350 and 550 °C
for 2 hours. The tetrahedral or octahedral origin of layer
charge was determined by the Greene-Kelly test (Greene-
Kelly 1953). XRPD measurements were carried out using a
Philips PW 1710 diffractometer with CuK
α radiation at 45 kV
and 35 mA in the lab of the Institute for Geological and Geo-
chemical Research of the Hungarian Academy of Sciences.
Lead isotope measurements were performed on pure galena,
calcite and fluorite crystals collected from the base-metal-
fluorite veins. Minerals were separated by hand picking under
stereomicroscope. The analytical part followed routines adapted
at the Swedish Museum of Natural History, Stockholm
(DeIgnacio et al. 2006). After dissolution in acids and subse-
quent ion exchange routines, clean lead separates were yielded.
The isotopic analyses were carried out using a Micromass
Isoprobe ICP-mass spectrometer in the Swedish Museum of
Natural History, Stockholm. Mass bias corrections were ac-
counted for by using an internal Tl normalization, and NBS
981 were run repeatedly to secure data accuracy. Typically,
the precision (2
σ error) of Pb runs is ±0.10 % or better.
Results
Fluid inclusion petrography and microthermometry
Relatively large (10—20 µm) two phase, liquid—vapour fluid
inclusions ratios were detected along the growth zones and
in isolated clouds in hydrothermal quartz, in fluorite and in
sphalerite crystals in the base-metal-fluorite veins (Fig. 4a,b).
The phase ratio between vapour and liquid phases is around
0.1 in the samples from west of the Pákozd Line and around
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0.2 in the samples from east of the Pákozd Line in the
hydrothermal quartz. Fluid inclusion data are listed in the
Appendix (as a Supplement in the electronical version;
www.geologicacarpathica.com).
Two phase liquid-vapour primary fluid inclusions in fluorite
from the base-metal-fluorite veins homogenized into liquid
phase at temperatures of 90—130 °C in the western block of
the granite (e.g. west of the Pákozd Line, Fig. 5a). Consider-
ing the eutectic melting temperatures of ice at around —21 °C,
their compositions can be modelled in the NaCl—H
2
O sys-
tem. Melting temperatures of ice are distributed between
—5.1 °C and —9.8 °C corresponding to 8—13 NaCl equiv.
wt. % salinities.
Fig. 4. a – Base-metal-fluorite
vein with cocade texture from the
Velence Mts. The brecciated and
altered (illite-kaolinite-smectite)
granite is cemented by quartz
(white with concentric zonation)
and sphalerite (brown). The white
circle indicates the place of fluid
inclusion studies; b – Primary
two phase (L + V; liquid-vapor)
fluid inclusions along growth
zones in sphalerite; c – Second-
ary, two-phase (liquid-vapour)
fluid inclusions in rock forming
quartz crystals of the granite.
The vapour/liquid ratio is 0.2.
Fluid inclusions are aligned along
fluid inclusion planes; d – Sec-
ondary, two—phase (liquid—va-
pour) fluid inclusions in rock
forming quartz crystals of the
granite. The vapour/liquid ratio
is 0.1; e – NE—SW trending
argillic alteration zone in the
western block of the granite. The
central part of the alteration zone
is greenish due to the smectite
whereas the rim is rather white
because of the higher relative
amount of illite; f – FIP in rock
forming quartz in unaltered gran-
ite. FIP are short and the number
of FIP in a certain area is low;
g – FIP in quartz crystals in al-
tered granite. FIP are long and
the number of FIP is high.
Two phase liquid—vapour primary fluid inclusions in
sphalerite homogenized at 80—160 °C in the western unit of
the granite (Fig. 5d). Due to their very low eutectic and ice
melting temperatures, partly below —60 °C and below
—21 °C, respectively, their compositions cannot be modelled
in the NaCl—H
2
O system. Because of difficulties with the re-
producible observations of hydrohalite melting, the fluid
composition has been modelled in the CaCl
2
—H
2
O system.
Melting of ice took place from —14.8 to —24.5 °C, and the cal-
culated salinities are between 18 and 23 CaCl
2
equiv. wt. %.
Primary, two-phase fluid inclusions in the hydrothermal
quartz homogenize at 80—130 °C west of the Pákozd Line
and 170—220 °C east of the Pákozd line (Fig. 5d). Eutectic
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TRIASSIC FLUID MOBILIZATION AND EPIGENETIC SULPHIDE MINERALIZATION (HUNGARY)
melting in these inclusions started below —50 °C. Therefore
salinities of these inclusions were calculated in CaCl
2
equiv.
wt. %. Final melting temperatures in the inclusions west and
east of the Pákozd Line varied from —6.2 °C to —26.4 °C and
from —4.3 °C to —21.7 °C, respectively. These final melting
temperatures correspond to salinities from 10—25 CaCl
2
wt. %
and 7—21 CaCl
2
wt. %.
Fig. 5. Homogenization temperature distribution diagram of the measured fluid inclusions in fluorite, sphalerite, hydrothermal quartz, as
well as in the rock forming quartz crystals of the granite from the Velence Mts. a—b—c – fluid composition is modelled in the NaCl—H
2
O
system; d—e—f – fluid composition is modelled by CaCl
2
—H
2
O system. c. – concentration.
Secondary fluid inclusions with similar phase ratios also
occur in the rock forming quartz of the granite. Independently
of the distance from the alteration zones, these inclusions are
regionally present in the granite. However, density of FIP is
high in the close vicinity of the veins (53.2—125.1 1/mm
2
and
11.3—26.0 mm/mm
2
; Fig. 4e,f) and decreases to the less
altered granite (23.9—51.9 1/mm
2
and 4.5—6.9 mm/mm
2
;
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Table 2; Fig. 4, e.g). The orientation of the fluid inclusion
planes is always parallel to the strike of the base-metal-fluo-
rite veins (NE—SW; Benkó 2008).
One group of secondary fluid inclusions in rock-forming
quartz of fresh and argillic altered granite is characterized by
eutectic melting temperatures at around —21 °C. The salini-
ties calculated from the melting temperatures of the ice (—0.2
to —8.6 °C) are in the range of 0.3—12 NaCl equiv. wt. %.
Homogenization of these inclusions took place into liquid
phase at 70—230 °C and 170—260 °C in the western and east-
ern blocks of the granite, respectively. The median of the ho-
mogenization temperatures is around 130 °C in inclusions
west of the Pákozd Line and around 210 °C east of the
Pákozd Line (Fig. 5b,c).
Another group of secondary fluid inclusions in rock—form-
ing quartz of fresh and argillic altered granite displayed eu-
tectic melting temperatures from —49 to —56 °C with melting
temperatures of the ice between —32.3 °C and —13.6 °C.
These fluid inclusions were also modelled in the CaCl
2
—H
2
O
system thus calculated salinities are between 9.9 and
25.8 CaCl
2
equiv. wt. %. Homogenization temperatures are
50—180 °C and 160 °C —260 °C east and west of the Pákozd
Line, respectively. The median of the homogenization tem-
peratures varies similarly to the low salinity secondary fluid
inclusions. In the western and eastern block the median is
around 135 °C and around 220 °C, respectively (Fig. 5e,f).
Lead isotope data
Lead isotope analyses have been carried out on galena
(n = 4), fluorite (n = 4) and calcite (n = 2) from the base-metal-
fluorite veins of the Velence Mts and from vein filling galena
(n = 4) from the Polgárdi Limestone Formation of the Sza-
badbattyán Block (Figs. 2 and 3). In the Velence Mts, the
Table 3: Lead isotope data of the lead-zinc mineralization in the Velence Mts and at Szabadbattyán. S—K – Stacey & Kramers (1975)
model age; C—R – Cummings & Richards (1975) model age.
Sample number
Analysed
mineral
Area
206
Pb/
204
Pb
207
Pb/
204
Pb
208
Pb/
204
Pb µ
value
S-K model
age (Ma)
C-R model
age (Ma)
BE50301
galena Velence
Mountains
18.288 15.679 38.587 10.06 412
310
BE50806
galena Velence
Mountains
18.278 15.653 38.506
9.95 369
310
BE303030
galena Velence
Mountains
18.305 15.622 38.439
9.80 286
300
BE51339
galena Velence
Mountains
18.268 15.645 38.481
9.91 360
330
BE51041
galena Velence
Mountains
18.363 15.690 38.599
BE51659
galena Velence
Mountains
18.318 15.660 38.466
BE50691
galena Velence
Mountains
18.313 15.654 38.443
BE
51045
fluorite
Velence
Mountains
18.438 15.657 38.703
BE
50691
fluorite
Velence
Mountains
18.511 15.697 38.547
BE
50301
fluorite
Velence
Mountains
18.325 15.660 38.499
BE
51041
fluorite
Velence
Mountains
18.457 15.665 38.770
M06
calcite Velence
Mountains
18.366 16.658 38.545
M30
calcite Velence
Mountains
18.351 15.663 38.494
BE50269
galena Szabadbattyán
18.286 15.667 38.552 10.01 390
310
BE51654
galena Szabadbattyán
18.339 15.710 38.694 10.19 435
290
BE51664
galena Szabadbattyán
18.348 15.736 38.781 10.30 477
280
BE50300
galena Szabadbattyán
18.293 15.679 38.588 10.06 408
310
accuracy: ± 0.10 %
Locality
Rock type and type of
hydrothermal alteration
Selected mineral
fraction
K-content (%)
40
Ar rad/g(cm
3
/g)
40
Ar rad
(%)
K/Ar age
(million year)
Pákozd, Big quarry
granite, argillic alteration
illite, kaolinite,
smectite
5.010 4.5827x10
–5
90.20 221.2±6.7
Pákozd, “Pegmatite quarry” granite, argillic alteration
illite, kaolinite,
smectite
4.214 3.6442x10
–5
89.30 209.8±3.7
Székesfehérvár, Kisfalud
quarry, next to the aplite
vein
granite, argillic alteration
illite, kaolinite,
smectite
3.185 2.8262x10
–5
75.00 214.6±6.7
Székesfehérvár, Kisfalud
quarry
granite, argillic alteration
illite, kaolinite,
smectite
3.260 3.038x10
–5
97.30 232.3±5.1
Sukoró, Rigó-hill
granite, no alteration
orthoclase
9.747
8.9088x10
–5
89.60 220.9±6.7
Table 4: K-Ar radiometric ages of hydrothermal and rock forming minerals from the Velence Mts and Szabadbattyán.
FIP density
Locality
Number of
FIP/unit area
Summa lenght
of FIP/unit area
1
77.2
11.8
2
125.1
26
3
73.9
13.7
Center of illite-
kaolinite-smectite
alteration zones
4
53.2
11.3
5
38.9
6.13
6
23.9
4.5
7
31.2
6.9
Out of alteration
zones
8
51.9
6.26
Table 2: Fluid inclusion plane density data, measured in the rock
forming quartz crystals of the Velence Mts granite.
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lead isotope data obtained for galena are as follows:
206
Pb/
204
Pb = 18.278—18.363,
207
Pb/
204
Pb = 15.622—15.690
and
208
Pb/
204
Pb=38.439—38.587 (Table 3). Lead isotope ratios
for galena from the Szabadbattyán Block are slightly higher:
206
Pb/
204
Pb = 18.286—18.348,
207
Pb/
204
Pb = 15.667—15.736 and
208
Pb/
204
Pb = 38.552—38.781. However, these data are margin-
ally different to those from the Velence Mts only, taking the
analytical uncertainties into consideration. The results for cal-
cite and fluorite from the base-metal-fluorite veins of the Ve-
lence Mts are close to, but typically slightly more evolved
than those for galena of the same veins (Table 3).
Thus, the isotope data from the two areas form a tight clus-
ter and, besides, one can note a tendency towards a linear ar-
ray (Table 3).
When treated together, the galena data from the two areas
yield µ values of 9.8—10.3 (Table 3), following the S-K model
(Stacey & Kramers 1975). This is higher than the average
crustal value (µ
2
= 9.74), and a dominant upper crustal
source for ore lead is also indicated by the plumbotectonic
model of Zartman & Doe (1981). Model ages, based on the
206
Pb/
204
Pb and
207
Pb/
204
Pb data for the combined galena
data set are quite consistent at around 300 Ma when the
Cumming & Richards (1975) model is applied, whereas S-K
model ages vary considerably (286—477 Ma).
XRPD results and clay mineralogy
Fig. 6. Radiometric age dates measured on different mineral fractions in the Velence Mts and at the
Szabadbattyán Block.
XRPD analyses were carried
out on the clay mineral assem-
blage of the argillic alteration
halo of the granite-hosted hydro-
thermal base-metal-fluorite veins
in the Velence Mts. Argillic alter-
ation zones without base metal
mineralization along NE—SW
trending faults were also studied.
The colour of alteration zones
changes from the fresh granite
towards the central part of the
alteration zones: the central
parts are more greenish, while
the lateral parts of the alteration
are dominated by white clay
minerals (Fig. 4a). According to
the XRPD studies the green co-
loured clay is dioctahedral
smectite with calcium and/or
magnesium in the interlayer
space. The basal reflection is
shifted from 15 Å to 12.6 Å af-
ter potassium saturation, indicat-
ing the low-layer charge of the
smectite. The Greene-Kelly test
indicates that this charge arises
from isomorphic substitution in
the octahedral sheet (Greene-
Kelly 1953). These results show
that the smectite is a low charged
montmorillonite. Besides mont-
morillonite, illite/montmorillonite, white coloured mixed layer
clay mineral containing 15—20 % illite, pure illite and kaolin-
ite are also present. Illite crystallinity has been checked by
combined XRPD and IR spectroscopic analyses (Benkó 2008)
and both methods have indicated a well—crystallized R3-type
illite based on the classification scheme of Środoń (1984).
K—Ar radiometric ages
K/Ar ages for illite (n = 4) are between 209.8 and
232.3 Ma, with individual errors in the order of ± 10 Ma, or
less. One K-feldspar from the relatively fresh granite (sam-
ple 6620) yielded an age of 220.9 Ma, which is comparable
to the ages of the illite (Table 4, Fig. 6).
Discussion
Our studies suggest that petrographic, fluid inclusion and
isotope data do not support old genetic models stressing that
base-metal-fluorite mineralization in the Velence Mts can be
related to the formation of the granite.
Nature of the ore-forming fluids
The petrography of fluid inclusions in the Velence Mts
suggest trapping from a homogeneous parental fluid, there-
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fore the measured homogenization temperatures are only
minimum estimates of the trapping conditions. True trapping
temperatures and pressures can be obtained only by pressure
correction using an independent thermometer.
Field evidence combined by the XRPD results indicates that
illite (white) was the first phase to form due to fluid/rock in-
teraction, followed by kaolinite (white) and smectite (green)
as gradual opening of the faults proceeds. In hydrothermal
systems clay mineral assemblages are useful for temperature
estimation (Reyes 1990; Hedenquist & Lowenstern 1994; Parry
& Jasumback 2002). Pure illite forms above 220—250 °C,
while kaolinite and smectite form below 180 (200) °C. Conse-
quently, it may be suggested that mineralization in the Ve-
lence Mts started at temperatures above 250 °C, resulting in
illite alteration, and with gradual cooling of the fluids below
200 °C there was a formation of kaolinite and smectite. Sul-
phur isotope analyses on syngenetic galena-sphalerite mineral
pairs also provided temperatures around 230—250 °C (Benkó
2008), which support the view that the maximum temperature
of the hydrothermal system could be around 250 °C.
Fluid inclusions with NaCl—H
2
O and CaCl
2
—H
2
O model
compositions are simultaneously present as primary objects in
the hydrothermal quartz and fluorite in the Velence Mts and as
secondary inclusions in the rock-forming quartz of the granite.
In spite of the compositional differences, their homogeniza-
tion temperature distributions in all outcrops are the same and
the number of their FIP increases towards the alteration
zones. If we assume that these inclusions relate to the cool-
Fig. 7. Temperature—pressure conditions of fluid inclusion entrapment in the Triassic and Alpine hydrothermal systems of the Velence Mts.
Isochors were calculated on the basis of equations of Zhang & Frantz (1987). c. – concentration.
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TRIASSIC FLUID MOBILIZATION AND EPIGENETIC SULPHIDE MINERALIZATION (HUNGARY)
ing of the granite which crystallized at 2 kbar (Buda 1993;
Fig. 7), the isochores for the low homogenization temperature
(Th ~ 90—120 °C) inclusions should have crossed the 2 kbar
isobar at 150—220 °C. This low temperature at 6—8 km, ac-
cording to the 2 kbar pressure, assumes a very low geothermal
gradient (20 °C/km). In the case of a cooling granite body,
a higher temperature than the average (35 °C/km) geothermal
gradient is expected. Therefore the observed fluid inclusion
features is difficult to relate to the postmagmatic-hydrothermal
system of the granite as it was suggested by Jantsky (1957).
The estimated geothermal gradient during the Triassic was
45 °C/km (Schuster et al. 1999). Intersecting the Triassic
(45 °C/km) geotherm calculated for hydrostatic and lithostatic
conditions with the isochors of the fluid inclusions from the
eastern block of the granite, the obtained pressures are be-
tween 400 and 1200 bars. Intersecting the isochors of the
higher homogenization temperature group (eastern block;
210—220 °C) with the 250 °C isotherm (which is the assumed
maximum temperature for illite crystallization; Reyes 1990;
Hedenquist & Lowenstern 1994; Parry & Jasumback 2002),
results in pressures around 400 bar (Fig. 7). This pressure is
lower than the estimated pressure at the time of the formation
of the granite, higher than the pressure range for the Paleogene
hydrothermal system (30—280 bar, Molnár 1996; Fig. 7) and
equivalent to the pressure calculated by the interception of the
isochors and the Triassic (hydrostatic) geotherms (Fig. 7).
Therefore it is assumed that the pressure conditions during the
fluid circulation could be near-hydrostatic. Differences in ho-
mogenization temperatures between the eastern and the west-
ern block of the granite can be explained by post-hydrothermal
tectonic activity of the Pákozd Line (Benkó 2008).
In petrography the fluid inclusion assemblages associated
with the Paleogene intrusive-volcanic activity in the eastern
part of the Velence Mts are significantly different from the fluid
inclusion assemblages in the western part of the granite (e.g.
boiling of low-, and high-salinity fluids with temperatures be-
tween 250 °C and 450 °C; Molnár 2004; Fig. 7), therefore we
proceed to explore the possibility that all of the studied fluid
inclusion populations are linked to a third fluid flow event in-
dependent from those in the Paleogene and Permian.
Fluid inclusion data for Alpine-type epigenetic lead-zinc
ore deposits hosted by Triassic carbonate rocks along the
PABL in the Drau Range (Mežica, Bleiberg) are similar to
our results for the mineralization of the Velence Mts (Fig. 8).
The Alpine-type epigenetic Pb-Zn ore deposit is a subtype of
the carbonate hosted stratabound Pb-Zn mineralizations. The
mineralization is epigenetic, hosted by Ladinian—Carnian
limestones in the Eastern and Southern Alps. The ores have
simple mineralogy, containing galena, sphalerite, pyrite and
marcasite. Zeeh et al. (1998) reported that the temperature of
the hydrothermal fluids of the first ore phase ranged between
122 °C and 159 °C (Phase I; Fig. 9). In their study, the salin-
ity of the early ore forming fluids was 8—12 NaCl equiv.
wt. % in sphalerite and 15—19 NaCl equiv. wt. % in saddle
dolomite. The salinity of the late hydrothermal phase was
higher as indicated by the data from fluorite (18—21 NaCl
equiv. wt. %). A similar mixing of low- and high salinity
fluids during ore formation in the Velence Mts was first
suggested by Molnár (1996). Maintaining the concept of a
mixing model including two types of fluids we postulate
that fluid mixing may have played a significant role in ore
formation.
Fig. 8. Comparison of fluid inclusion data for
two Alpine-type epigenetic lead-zinc deposits in
the Drau Range (Bleiberg, Mežica; Kuhlemann et
al. 2001) and the Pb-Zn mineralization of the Ve-
lence Mts.
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Sources of Pb in the veins
The lead isotope ratios in the base-metal-fluorite
veins of the Velence Mts and the Szabadbattyán
Block essentially overlap (Fig. 9a,b) with the data for
galena from Alpine-type epigenetic Pb-Zn mineral-
izations along the PABL (Bleiberg, Mežica, Salafossa,
Raibl, Gorno (Figs. 1 and 11). Köppel & Schroll
(1988) proved the importance of early Paleozoic
high-grade metamorphic crystalline basement rocks
(gneiss, amphibolite, micaschist) as sources of metals
in the Alpine-type lead-zinc deposits. High-grade
metamorphic rocks are not known in the currently
studied areas, but pebbles of such rocks were docu-
mented in a late Variscan molass formation, located
close to the reconstructed pre-tectonic site (cf. the
Carboniferous conglomerate in Fig. 10c).
It is therefore possible that the metals in the investi-
gated deposits of the Pannonian Basin were also de-
rived from a range of rocks, including spatially
associated magmatic rocks (the host rock granite in the
Velence Mts and the andesite dykes at Szabadbattyán),
the underlying sedimentary rocks and the deeply situ-
ated metamorphic basement. Interestingly, despite the
difference in host rock character (Permian granite and
Devonian limestone, respectively), the ore lead signa-
tures at the Velence Mts and at the Szabadbattyán
Block are more or less identical (Fig. 9a,b). This sug-
gests that the host limestone in the Szabadbattyán
Block did not act as a major source of lead, and it is
more likely that a range of deep-seated rocks provided
the metals.
Radiometric age constraints and age correlations
with adjoining areas
The age of the host granite in the Velence Mts is
280—290 Ma (Buda 1985) as is indicated by the K/Ar,
Rb—Sr data for rock-forming biotite. The K/Ar block-
ing temperature of pure illite is around 250 °C (Clauer
& Chaudhuri 1995). Hence, it seems plausible that
the measured K/Ar age data from pure illite from the
argillic alteration zones around the base-metal-fluo-
rite veins of the Velence Mts represent the true age of
the hydrothermal circulation. As the obtained K/Ar
160 °C in Triassic times. Evidently, the inferred Triassic hy-
drothermal alteration was not related in age to the Carbonif-
erous, magmatism (host granite), Cretaceous lamprophyre
dykes or to the Paleogene magmatic activity in the eastern-
most part of the Velence Mts. Therefore, we can rule out any
hypothesis (Jantsky 1957; Kaszanitky 1958; Horváth &
Ódor 1984) assuming that either of these magmatic events
acted as the heat source for the mineralizing fluids.
Triassic magmatic activity in the Velence Mts is not known,
but age data for andesite dikes from the Szabadbattyán Block
(Balogh et al. 1983; Bagdaszarjan 1989; Dunkl 1991) are
equivalent to the obtained K/Ar ages for illite in the Velence
Mts. This is exemplified by a 210 ± 4 Ma K/Ar age of whole
rock samples of one andesite dyke from Szabadbattyán
Fig. 9. Lead isotope evolution diagrams (a –
207
Pb/
204
Pb—
206
Pb—
204
Pb,
b –
208
Pb/
204
Pb—
206
Pb/
204
Pb) with growth curves according to Zartman &
Doe (1981) (Z—D) and Stacey & Kramers (1975). The shaded boxes repre-
sent whole rock Pb isotope data of the three main tectonic units of the Alps
(Köppel & Schroll 1988). The field bordered by dashed line represents lead
isotope data from galena of Alpine-type Pb-Zn deposits along the PABL
(Köppel 1983). Data points represent lead isotope data from the Velence
Mts and the Szabadbattyán Block measured in galena and fluorite.
ages of 210—230 Ma almost overlap within analytical error,
it is possible to establish a Mid-Late Triassic ore-forming
event (Fig. 6). K/Ar data for the orthoclase from the western
part of the granite body at Velence Mts also provide support
for a Mid-Late Triassic thermal event. This is based on the
fact that the blocking temperature of K-feldspar is around
160 °C (Harrison et al. 1979), and therefore the K/Ar ages of
feldspars either represent the time of cooling of the rock be-
low 160 °C (Faure 1977; Richards & Noble 1998) or the
post-emplacement history involving other events when the
temperature of the rock passed the 160 °C isograd for the last
time. Following this, we anticipate that the 221 Ma age of
the rock forming fresh orthoclase represents a re-set age
which is due to a regional heating of the granite body above
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TRIASSIC FLUID MOBILIZATION AND EPIGENETIC SULPHIDE MINERALIZATION (HUNGARY)
(Bagdaszarjan 1989), whereas Balogh et al. (1983), obtained
213 ± 13 Ma for another dyke. Dunkl (1991) established a
214 ± 5 Ma age for titanite from those andesite dykes by the
fission track method (Fig. 6). This age agreement between the
two mineralized study areas suggests that a presently not iden-
tified Triassic magmatic event might have been the driving
force for hydrothermal alteration in the Velence Mts. This
view is consistent with an active Triassic magmatism along
the eastern segment of the PABL (Ferrara & Innocenti 1974).
There is evidence that it also extended into the Southern Alps.
The eastern part of the Neo-Tethys region is characterized by
slightly older magmatism (Haas 2004). Pamić (1984) reported
Ladinian magmatic ages in the 216—250 Ma range in the
Karawanken, by using a range of isotopic methods (U—Pb,
Rb—Sr and K/Ar data), which may be related to the rift phase
of the Dinaric part of the Neo-Tethys Ocean. Castellarin et al.
(1988) documented Ladinian bimodal magmatites from the
Southern Alps. However, on the basis of geochemical data,
they emphasized an orogenic origin of the magmas.
It is not the aim of this paper to discuss whether the Ladin-
ian magmatic rocks in both the Alpine region and along the
PABL have a rift or an orogenic origin. Still, as a general
theory (cf. Haas 2004), we prefer the rift origin and we con-
nect the Ladinian hydrothermal circulation in the Velence
Mts and the Szabadbattyán region to the contemporaneous
rift events in the Neo-Tethys Ocean.
Model of formation of lead-zinc deposits in the Pannonian
Basin and their possible genetic link to the Alpine-type epi-
genetic mineralizations
Comparison of the studied deposit and the Alpine deposits
is summarized in Table 5.
There are striking similarities between the granite-hosted
deposit in the Velence Mts and certain deposits (Meziča,
Bleiberg, Salafossa, Gorno, etc.) in the Alps along the PABL
(Fig. 10a,b, Table 5), especially regarding fluid inclusion
and lead isotope signatures. However, the host rock of the
Table 5: Comparison of geochemical, fluid inclusion and mineralogical characteristics of the studied (Szabadbattyán and Velence Mts) and
other base-metal and fluorite mineralizations along the PABL (Bolzao granodiorite, Alpine-type epigenetic lead-zinc mineralizations).
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Fig. 10.
a
–
Regional
geology
of
the
SE
part
of
the
Alcapa
Megaunit
and
the
eastern
part
of
the
Eastern
and
Southern
Alps
after
Kázmér
&
Kovács
(1985).
The
Alcapa
Megaunit
escaped
during
the
Late
Paleogene—Early
Neogene
from
the
collision
zone
of
the
Eastern
Alps
and
Southern
Alps
along
the
dextral
PABL;
b
–
Pb-Zn
deposits
along
the
PABL
in
the
eastern
segment
of
the
Eastern
Alps
(Bauer
1985);
c
–
Pb—Zn
in
deposits
along
the
PABL
in
the
Pannonian
basin
(Sza
badbattyán
Block
and
Velence
Mts
after
Dudko
1999).
The
similar
geology
in
the
broader
vicinity
of
the
Pb—Zn
deposits
suggests
that
these
deposits
could
be
spa
tially
in
contact
prior
to
the
escape
of
the
Alcapa
Megaunit
fr
om
the
Alpine
collision
zone.
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TRIASSIC FLUID MOBILIZATION AND EPIGENETIC SULPHIDE MINERALIZATION (HUNGARY)
Alpine-type epigenetic lead-zinc deposits in the Alps is
mainly Triassic limestone (e.g. Raibl beds) and the ores oc-
cur as stratabound bodies, whereas mineralization in the Ve-
lence Mts is characteristically vein-type, hosted by granite.
Mineralization in the Alpine deposits often occurs as matrix
of tectonic breccias, but also forms fissure filling, karst fill-
ing or fault-related epigenetic ore bodies (Brigo et al. 1977).
This suggests that the diagenetic process and the carbonate
host rock are not truly decisive factors for governing ore
deposition, and mineralization can occur in very different
forms and in different type of rocks.
Also, the timing aspect is important when a potential ge-
netic link is tested between different ores. Observations pre-
sented in this paper argue for an epigenetic, Mid-,
Late-Triassic ore-forming event in the Velence Mts and the
Szabadbattyán Block (209—232 Ma). Epigenetic lead-zinc
deposits north of the PABL occur in the Late—Triassic (Car-
nian – 228—216 Ma; Brigo et al. 1977).
Another candidate for comparison along the PABL is the
Brixen (Bolzano) granodiorite (Fig. 1), which is the host of
vein type quartz-fluorite mineralization. Age, geochemical,
and genetic similarities of the two host crystalline formations
have been established by Buda et al. (2004). Age, texture
and fluid inclusion properties of the two mineralizations in
the Velence Mts and in the Szabadbattyán Block also show
several striking similarities (Table 5). On the basis of the
characteristics of the Bolzano mineralization, Hein et al.
(1990) connected the formation of the quartz-fluorite veins
to a large-scale fluid flow system and excluded the possible
role of magmatism as a driving force of fluid flow. In his
model, fluorine originated from the sedimentary basement
rocks. Based on the fluorine anomalies in the carbonate-
hosted lead-zinc deposits along the PABL, he proposed a ge-
netic link between the granite hosted quartz-fluorite veins
and the lead-zinc deposits. Regarding the large distance be-
tween Bolzano granite and the studied deposits ( ~ 600 km
along the PABL) it is not necessarily stated that the two crys-
talline formations formed an identical unit. However, if the
Velence Mts are interpreted as a tectonic megamelange
along the PABL the former spatial relationship of the two
rock units cannot be excluded.
In our model a rift related regional fluid flow was initiated
by the time of the Mid Triassic. The heat source of the fluid
convection could be the attenuated and heated continental
crust but locally magma intrusions may also have played a
significant role. Ca-rich, high-salinity formational fluids mi-
grating in the basement metamorphic and sedimentary rocks
leached base metals. Mixing with low-salinity fluids and
cooling decreased their transfer capacity and base metals
precipitated in some tectonic zones (Fig. 11). Consequently,
base-metal veins in the Velence Mts represent the relatively
deep channels of the fluid flow, whereas epigenetic deposits
in the Alps are the uppermost, discharge part of a similar hy-
drothermal system.
The spatial relationship between the different levels of the
hydrothermal convection system is not obvious at first sight.
However several authors (Géczy 1984; Dulai 1990; Vörös
1993; Csontos 1995; Haas et al. 1995; Ebner et al. 1998;
Márton & Fodor 2003) proved that the Transdanubian
Mountain Range escaped 450—500 km east from the Alpine
collision zone during the Late Paleogene—Early Neogene. Ac-
cordingly, in the Triassic, in its original position the Velence
Fig. 11. Proposed genetic model of lead-zinc mineralization in the Velence Mts and its possible connection to the Alpine-type epigenetic
lead-zinc mineralization, without scale. Base-metal-fluorite mineralization in the Velence Mts represents a deep conduit part of the hydro-
thermal system. During ascent and cooling of hydrothermal fluids, fissure filling and brecciated lead-zinc ore formed in Triassic limestones
along the PABL. Carbonate hosted Alpine-type epigenetic lead-zinc deposits formed at the discharge site of the convection system. Due to
the different tectonic histories during the Alpine orogeny epoch, shallow levels of the system are preserved in the Alps, whereas the deeper
part of the system is exposed in the central part of the Pannonian Basin.
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Mts formed the basement of the carbonaceous sedimentary
formations that are now the host of the stratiform-stra-
tabound epigenetic deposits. Due to the intense orogenic
processes during the Alpine orogeny in the Creatceous some
parts of the system were lifted up more intensively and eroded
(Velence Mts, Szabadbattyán on the southern flank of the
syncline of the Transdanubian Mountain Range) while other
parts were not exhumed and eroded (Alpine-type epigenetic
lead-zinc deposits).
Later, as a result of the eastward extrusion of the Alcapa
Megaunit from the Alpine collision zone, the two levels of
the former hydrothermal system were farther displaced.
Carbonaceous rocks similar to the host of the Alpine depos-
its far north from the PABL are widely known in the Trans-
danubian Mountain Range. Except for a few indications, no
mineralization has been found yet in these rocks. This implies
that the PABL as a major fluid flow channel had a particular
role in the formation of the various lead-zinc deposits.
Summary and conclusions
Clay mineralogy, K/Ar radiometric ages, lead isotope and
fluid inclusion studies have been carried out on the vein type
and metasomatic base-metal-fluorite mineralization of the
Paleozoic basement units of the Pannonian Basin in the Ve-
lence Mts and the Szabadbattyán Block in order to establish
a model for their origin.
The maximum temperature of the hydrothermal fluid
flow was around 250 °C according to the clay mineral stud-
ies. The fluids then gradually cooled during the hydrother-
mal fluid flow to below 200 °C. Formation of the
base-metal-fluorite mineralization is the result of the mixing
of low salinity (0—12 NaCl equiv. wt. %) and high salinity
(10—26 CaCl
2
equiv. wt. %) formational brines. Our studies
on fluid inclusions and clay gangue minerals indicate that
the temperature (130—240 °C) and pressure conditions
(400—500 bar) during ore formation were different from the
magmatic—postmagmatic system for the Permian granite
intrusion (550—690 °C; 2 kbar) and the Paleogene fluid
flow (240—480 °C; 30—280 bars).
Lead isotope data (Velence Mts:
206
Pb/
204
Pb=18.278—18.363,
207
Pb/
204
Pb=15.622—15.690 and
208
Pb/
204
Pb = 38.439—38.587
and Szabadbattyán:
206
Pb/
204
Pb = 18.286—18.348,
207
Pb/
204
Pb = 15.667—15.736
and
208
Pb/
204
Pb=38.552—38.781)
demonstrate a common isotope pattern for the two studied
mineralizations and the obtained results are also in concor-
dance with data for Alpine-type epigenetic lead-zinc depos-
its. Magmatic rocks and basement metamorphic rocks,
carrying an upper crustal signature, probably supplied a ma-
jor part of the lead contained in the ores.
K/Ar radiometric age dating (208—232 Ma) suggests a
Mid- to Late-Triassic age of the mineralization and related
regional heating of the granite. Thus our results give no sup-
port to earlier hypotheses, including ore formation related to
Carboniferous, Cretaceous and Paleogene magmatism.
Several lines of presented evidence suggest a genetic rela-
tionship between the two studied mineralization of the Pan-
nonian Basin and other, Alpine-type epigenetic lead-zinc
deposits along the PABL, in the Southern and Eastern Alps.
A tectonic reconstruction suggests a direct spatial relationship
to the deposits along the PABL in the Southern and Eastern
Alps. We propose that the two described mineralizations in
the Pannonian basin are deep feeder channels of a regional
fluid flow system that occasionally discharged to form shal-
low epigenetic Pb—Zn mineralizations. The latter are now
eroded away, if they were ever present in the study areas.
Acknowledgments: The measurements were supported by
the Synthesys (SE-TAF-3772) program of the EU. The au-
thors are particularly grateful to the editor Pavel Uher and
the reviewers, Peter Koděra and Sándor Szakáll for their de-
tailed review of the manuscript. Their suggestions and con-
structive criticism of the earlier manuscript resulted in major
improvements to the final article.
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ELECTRONIC SUPPLEMENT — BENKÓ et al.: TRIASSIC FLUID MOBILIZATION AND EPIGENETIC LEAD-ZINC SULPHIDE
MINERALIZATION IN THE TRANSDANUBIAN SHEAR ZONE (PANNONIAN BASIN, HUNGARY)
Appendix A
Fluid inclusion data. A — Low salinity fluid inclusions modelled in the NaCl+H
2
O binary system.
Block
Locality
Host
mineral
Host rock
alteration
Fluid inclusion
classifiacation
Th (°C)
Te (°C)
Tm (°C)
Salinity
(CaCl
2
equiv. wt. %)
Secondary
192
–48
–15.8
18.3
Secondary
199
–47
–16.0
18.4
Secondary
243
Secondary
246
–47
–16.0
18.4
Secondary
214
–48
–16.0
18.4
Secondary
226
–16.8
18.9
Secondary
213
–15.6
18.2
Secondary
239
–15.6
18.2
Secondary
228
–8.8
13.2
Secondary
229
Secondary
226
Secondary
218
–13.0
16.5
Secondary
212
–48
–14.0
17.2
Secondary
235
Secondary
185
–10.4
14.5
Secondary
229
–15.0
17.8
P
á
k
o
zd
L
in
e
E
Secondary
204
Secondary
142
–50.2
–11.4
15.3
Secondary
98
–48
–16.0
18.4
Secondary
200
–17.0
19.0
Secondary
151
–41
–12.8
16.4
Secondary
120
–45
–20.3
20.8
Secondary
151
–51
–19.8
20.6
Secondary
170
–51
–11.1
15.1
Secondary
144
–15.6
18.2
Secondary
138
–50
–25.0
23.1
Secondary
98
–45
–31.0
25.5
R
ig
ó
H
il
l
Secondary
157
–57
–33.0
26.2
Secondary
160
–60
–28.0
24.3
Secondary
205
–15.1
17.9
Secondary
128
–56.6
–17.4
19.3
Secondary
167
–56
–20.0
20.7
Secondary
167
–56.6
–23.3
22.3
Secondary
191
–53
–18.0
19.6
Secondary
184
–55
–21.4
21.4
Secondary
214
–57.2
–22.2
21.8
Secondary
164
–51
–19.0
20.2
Secondary
197
–57
–17.5
19.3
Secondary
217
–53.7
–18.1
19.7
Secondary
203
–18.3
19.8
S
o
ro
m
p
ó
V
a
ll
ey
N
o
a
lt
er
a
ti
o
n
Secondary
211
–52
–17.6
19.4
Secondary
137
–64.5
–28.4
24.5
Secondary
200
–64
–28.1
24.4
Secondary
155
–66
–20.6
21.0
Secondary
158
–17.8
19.5
Secondary
–66
–17.4
19.3
Secondary
157
–57
–17.0
19.0
Secondary
–58.8
–16.9
19.0
Secondary
133
–27
–16.6
18.8
Secondary
159
–60
–15.2
18.0
Secondary
103
–65
–14.9
17.8
Secondary
162
–65
–14.0
17.2
Secondary
146
–57
–13.3
16.7
Secondary
140
Secondary
157
Secondary
152
Secondary
172
E
a
st
er
n
Z
se
ll
ér
ek
p
a
st
u
ra
le
G
ra
n
it
e,
r
o
ck
f
o
rm
in
g
q
u
a
rt
z
Il
li
te
-k
a
o
li
n
it
e-
sm
ec
ti
te
a
lt
er
a
ti
o
n
a
n
d
q
u
a
rt
z
v
ei
n
s
Secondary
196
ii
ELECTRONIC SUPPLEMENT — BENKÓ et al.: TRIASSIC FLUID MOBILIZATION AND EPIGENETIC LEAD-ZINC SULPHIDE
MINERALIZATION IN THE TRANSDANUBIAN SHEAR ZONE (PANNONIAN BASIN, HUNGARY)
Appendix B
Fluid inclusion data. B — High salinity fluid inclusions modeled in the CaCl
2
+H
2
O binary system.
Block
Locality
Host
mineral
Host rock
alteration
Fluid inclusion
classifiacation
Th (°C)
Te (°C)
Tm (°C)
Salinity
(CaCl
2
equiv. wt. %)
Secondary
113
Secondary
139
–51.2
–22.7
22.0
Secondary
163
–21.7
21.5
Secondary
166
–29.0
24.7
Secondary
134
–28.7
24.6
Secondary
112
Secondary
113
Secondary
116
Secondary
50
Secondary
108
Secondary
139
Secondary
134
Secondary
103
–20.9
21.1
Secondary
113
–16.9
19.0
Secondary
98
–23.0
22.2
Secondary
118
–20.2
20.8
Secondary
88
–14.9
17.8
Secondary
114
Secondary
135
–9.4
13.7
Secondary
118
–8.7
13.1
Secondary
150
–21.9
21.6
Secondary
119
–16.0
18.4
Secondary
134
0.0
Secondary
132
–16.0
18.4
Secondary
74
–15.0
17.8
P
á
tk
a
S
o
u
th
N
o
a
lt
er
a
ti
o
n
Secondary
101
–14.0
17.2
Secondary
92
–33
–25.0
23.1
Secondary
92
Secondary
115
–10.4
14.5
Secondary
119
–23.7
22.5
Secondary
87
Secondary
123
–50
–26.5
23.7
Secondary
119
–48
–27.0
23.9
Secondary
88
–48
Secondary
90
–15.0
17.8
Secondary
97
Secondary
99
–47.6
–10.5
14.6
Secondary
90
Secondary
75
Secondary
93
Secondary
81
–57
–30.5
25.3
Secondary
82
–56.1
–25.0
23.1
Secondary
133
–14.0
17.2
Secondary
137
Secondary
118
–13.0
16.5
Secondary
–24.5
22.9
S
zé
k
es
fe
h
ér
v
á
r,
l
a
k
e
Secondary
–20.2
20.8
Secondary
289
–16.0
18.4
Secondary
296
–5.8
10.0
Secondary
282
–16.5
18.7
Secondary
78
–13.9
17.12
Secondary
113
Secondary
116
–47
–13.0
16.5
B
ir
k
a
ta
n
y
a
G
ra
n
it
e,
r
o
ck
f
o
rm
in
g
q
u
a
rt
z
Secondary
62
–14.7
17.64
Primary
105
–53.6
–17.0
19.03
Primary
105
–53.1
–16.9
18.97
Primary
112
Primary
109
–53
–16.7
18.86
Primary
106
–50.7
–17.3
19.2
Primary
109
–50.4
–15.8
18.32
Primary
93
–50.2
–16.8
18.92
Primary
98
–56.6
–20.9
21.14
Primary
84
–48.6
–19.0
20.15
Primary
81
–48.7
–22.1
21.73
Primary
85
–49.5
–20.8
21.09
Primary
99
–51.7
–18.8
20.04
Primary
96
–57.5
–17.0
19.03
Primary
74
–55.1
–23.0
22.16
P
á
tk
a
,
S
z
zv
á
r
m
in
e
S
p
h
a
le
ri
te
Primary
87
–54
–16.4
18.68
Secondary
138
–70
–24.7
22.94
Secondary
159
–67
–25.4
23.23
Secondary
204
–67
–26.0
23.51
Primary
83
–20
–19.0
20.15
Primary
90
–25.0
23.08
Primary
90
–19.8
20.57
Secondary
121
–23.2
22.26
Secondary
175
–69
–26.7
23.81
Secondary
166
–72
–24.6
22.9
Primary
183
–78.5
–24.6
22.9
Primary
78
–50.6
–16.1
18.5
Primary
84
–56
–14.9
17.76
Primary
80
–61.8
–15.7
18.26
Primary
98
Primary
139
Primary
126
Primary
72
–51
Primary
81
–14.0
17.18
Primary
81
–17.0
19.03
We
st
er
n
P
á
k
o
zd
b
lo
ck
H
y
d
ro
th
er
m
a
l
q
u
a
rt
z
Il
li
te
-k
a
o
li
n
it
e-
sm
ec
ti
te
a
lt
er
a
ti
o
n
a
n
d
q
u
a
rt
z
v
ei
n
s
Primary
89
–13.7
16.98