www.geologicacarpathica.sk
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, FEBRUARY 2013, 64, 1, 39—62 doi: 10.2478/geoca-2013-0003
Introduction
In spite of numerous previous works devoted to the terminal
Triassic sedimentary and biotic evolution, precise dating and
event successions during the Rhaetian transgression have re-
mained little known since the establishment of the “Avicula
contorta Schichten” by Winkler (1859). We selected the Kar-
dolína section situated on a steep western slope of the Mt
Pálenica (NNE of the Tatranská Kotlina village) in the Belian-
ske Tatry Mts (GPS coordinate 49°14
’997”N: 20°18’894”E,
Figs. 1 and 2) as the most continuous section of the Rhaetian
Fatra Formation in the former Zliechov Basin (Fatric Unit),
the upper part of which has been studied by Michalík et al.
(2007). The sedimentary record was analysed by sedimento-
logical, biostratigraphical, geochemical and magnetic suscep-
Paleoenvironments during the Rhaetian transgression and
the colonization history of marine biota in the Fatric Unit
(Western Carpathians)
JOZEF MICHALÍK
1
, OTÍLIA LINTNEROVÁ
2
, PATRYCJA WÓJCIK-TABOL
3
,
ANDRZEJ GAŹDZICKI
4
, JACEK GRABOWSKI
5
, MARIÁN GOLEJ
1
, VLADIMÍR ŠIMO
1
and
BARBARA ZAHRADNÍKOVÁ
6
1
Geological Institute, Slovak Academy of Sciences, Dúbravská cesta 9, P.O.Box 106, 840 05 Bratislava, Slovak Republic;
geolmich@savba.sk; geolmgol@savba.sk; geolsimo@savba.sk
2
Department of Geology and Mineral Deposits, Faculty of Natural Sciences, Comenius University, Mlynská dolina G1, 842 15 Bratislava,
Slovak Republic; lintnerova@fns.uniba.sk
3
Department of Geological Sciences, Jagiellonian University, Oleandry Str. 2a (room 109), 30-063 Kraków, Poland
4
Institute of Paleobiology, Polish Academy of Sciences, Twarda 51/55, 00-818 Warszawa, Poland; gazdzick@twarda.pan.pl
5
Polish Geological Institute, National Research Institute, Rakowiecka 4, 00-975 Warszawa, Poland; jacek.grabowski@pgi.gov.pl
6
Slovak National Museum, Natural Science Museum, Vajanského nábrežie 2, P.O.Box 13, 810 06 Bratislava, Slovak Republic;
barbara.zahradnikova@snm.sk
(Manuscript received May 23, 2012; accepted in revised form September 18, 2012)
Abstract: Terminal Triassic environmental changes are characterized by an integrated study of lithology, litho- and
cyclostratigraphy, paleontology, mineralogy, geochemistry and rock magnetism in the Tatra Mts. The Carpathian Keuper
sequence was deposited in an arid environment with only seasonal rivers, temporal lakes and swamps with scarce
vegetation. Combination of a wide range of
18
O values (—0.7 to + 2.7) with negative
13
C values documents dolomite
precipitation either from brackish or hypersaline lake water, or its derivation from pore water comparably to the Recent
Coorong B-dolostone. Negative
13
C values indicate microbial C productivity. Rhaetian transgressive deposits with
restricted Rhaetavicula fauna accumulated in nearshore swamps and lagoons. Associations of foraminifers, bivalves
and sharks in the Zliechov Basin were controlled by physical factors. Bivalve mollusc biostromes were repetitively
destroyed by storms, and temporary firm bottoms were colonized by oysters and burrowers. Subsequent black shale
deposition recorded input of eolian dust. Bottom colonization by pachyodont bivalves, brachiopod and corals started
much later, during highstand conditions. Facies evolution also revealed by geochemical data, C and O isotope curves
reflect eustatic and climatic changes and help reconstruct the evolution of Rhaetian marine carbonate ramp. The Fatra
Formation consists of 100 kyr eccentricity and 40 kyr obliquity cycles; much finer rhythmicity may record monsoon-
like climatic fluctuations. Fluvial and eolian events were indicated by analysis of grain size and content of clastic
quartz, concentrations of foraminiferal (Agathammina) tests in thin laminae indicates marine ingression events. Mag-
netic susceptibility (MS) variations reflect the distribution of authigenic and detrital constituents in the sequence. In-
creasing trend of MS correlates with the regressive Carpathian Keuper sequence and culminates within the bottom part
of the Fatra Formation. Decreasing trend of MS is observed upwards the transgressive deposits of the Fatra Formation.
Key words: uppermost Triassic, Western Tethys, Slovakia, sedimentology, sequence stratigraphy, geochemistry, marine
fauna.
tibility methods. Detailed study of cyclostratigraphy enabled
us to assess periodicity estimate, duration of sedimentary cy-
cles, and climate proxies. Preservation of primary magnetic
record is promising for future detailed study of magneto-
stratigraphy.
Geological setting
Terrigenous Carpathian Keuper was deposited during the
Carnian and Norian on extensive lowlands adjacent to North
Tethyan shelves. Limanowski (1903) interpreted its environ-
ment as a continental domain. Turnau-Morawska (1953) re-
garded variegated shales, sandstones and dolostones as marine
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Fig. 2. Rocky outcrop above the Kardolína gamekeeper’s cottage on
the western slope of Mt Pálenica. Right corner: contact of the Car-
pathian Keuper with the Fatra Formation.
sediments with fluvial intercalations. Borza (1959) postulated
a primary character of Keuper dolostones. Gaździcki et al.
(1979) recognized three informal members in the sequence:
the basal member with clastic intercalations, the middle one
Fig. 1. Location of the Kardolína section on the slope of Mt Len-
dacká Pálenica near Tatranská Kotlina in the Belianske Tatry Mts.
with prevalence of variegated claystones and the upper mem-
ber, that consists of claystone/dolostone alternation. They
stressed the terrigenous nature of the palynoflora in the clay-
stones (Gliscopollis/Classopollis assemblage), whereas the
dolostone intercalations yielded more diversified associa-
tions of pollen, spores and marine acritarchs. Al-Juboury &
Ďurovič (1992, 1996) supposed hypersaline conditions of
the Keuper dolomite formation. Rychliński (2008) and Jaglarz
(2010) distinguished several depositional environments:
mudflats, fluvial, sabkha, and flat marine, evolving under
fluctuating wet – semi-arid and arid climate.
During the latest Triassic, dry emerged plains were inun-
dated by shallow sea flooding the opening tensional depres-
sions (Michalík 1993). Transgression was not a short and
uniform event. Instead, sea reached different parts of the area
in several pulses (Gaździcki & Iwanow 1983). Bioclastic,
shelly, and oolitic limestones, marlstones, dolostones and
marls were laid down in salt marshes, littoral banks, carbon-
ate ramps, up to deeper neritic slope of the almost 300 km
long and 100 km wide tensional semi-closed shallow marine
basin (the Fatric Zone of the central Western Carpathians;
Michalík 1977; Michalík et al. 2007). The carbonate ramp
faced a deeper, dysoxic basin.
The new biotope created by the Rhaetian marine transgres-
sion was colonized by pioneer organisms (foraminifers, bi-
valves and fish). The Kardolína section is more suitable for
detailed study of this process than other less complete sections
in the Fatric Unit (Michalík 1977, 1979, 1982; Michalík et al.
2007). Benthic associations were dominated by bivalves
Placunopsis alpina (Winkler) and Rhaetavicula contorta
(Portlock), gastropods, and foraminifers Agathammina austro-
alpina Kristan-Tollmann & Tollmann (Michalík & Jendrejá-
ková 1978; Michalík 1978a). Upper Triassic bivalve faunas
have been studied by Allasinaz (1972), Kollárová-Andrusovová
& Kochanová (1973), Hallam (1981), Golebiowski (1991),
Ivimey-Cook et al. (1999) and Hautmann (2001). Fish re-
mains (single shark and actinopterygian teeth and scales)
were reported by Gaździcki (1974), Duffin & Gaździcki
(1977), Michalík (1977, 1979), and by Gaździcki et al.
(1979). More mature communities were represented by bra-
chiopods Rhaetina gregaria (Suess), Zugmayerella uncinata
(Schafhäutl), Austrirhynchia cornigera (Suess) – (Michalík
1975, 1978b, 1980); foraminifers Aulotortus friedli (Kristan-
Tollmann), Glomospirella pokornyi (Salaj), Triasina hantkeni
Majzon – (Gaździcki 1983); and/or by corals Retiophyllia
paraclathrata Roniewicz, Rhaetiastraea tatrica Roniewicz,
etc. – (Roniewicz & Michalík 1998); sponges, algae and hy-
drozoans inhabiting the carbonate ramp. However, evolution
of any true reef bio-constructions was prevented by storms
and sea-level fluctuations (Michalík 1980, 1982). The pa-
lynofacies characterized by Ricciisporites tuberculatus Lund-
blad was dominated by terrestrial components and by a high
amount of phytoclasts. Its marine fraction dominated by the
dinoflagellate cyst Rhaetogonyaulax rhaetica Sarjeant points
to a very shallow marine depositional environment (Götz in
Michalík et al. 2007). Microflora from the upper part of the
Fatra Formation resembles associations of the Ricciisporites
tuberculatus Zone of the Polish zonation and of the Ricci-
isporites—Polydiisporites Zone of the SE North Sea Basin,
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both indicating middle to late Rhaetian age (Ruckwied &
Götz 2009).
Material and methods
In the well exposed, 122 m thick Kardolína section, we
concentrated on its lower part (69 m, Fig. 3), where 42 dolo-
stone and 103 limestone layers were distinguished and num-
bered. Basal beds of the Fatra Formation were designated as
the “zero interval” (however, later, it was proved that the up-
permost layers of the Carpathian Keuper bear signs of marine
origin and the Bed —5 consists of first limestone biomicrite).
Samples were taken by the bed by bed method, but thicker
layers were sampled more densely. The Carpathian Keuper se-
quence was numbered downwards, thus in opposite order to
the Fatra Formation, but with a “minus” mark.
From each sample, a thin section has been made for micro-
scopic study. Allochem contents were evaluated from per-
centages obtained under an optical microscope both with use
of estimation tables (Bacelle & Bosellini 1965; Schäfer
1969; Soudant 1972; Michalík et al. 2007), and of the
NICON NIS-Elements BR System for screen analysis. Mi-
crite, sparite, bioclast and lithic clast contents, as well as the
average size of clastic quartz grains were measured (Fig. 4).
Micrite and sparite were compared as antagonistic elements
(as the Reijmer 1968) in Fig. 5.
Total abundance of major oxides, several trace elements,
and REE were analysed in the ACME Analytical Laborato-
ries, Ltd in Vancouver, Canada, in 12 samples. REE were
normalized to the Post-Archaean Australian Shale = PAAS
(Taylor & McLennan 1985). The Eu/Eu* ratios (Eu anomaly
values) were calculated using Eu
PAAS
/Sm
PAAS
Gd
PAAS
)
0.5
ratio. The inter-elemental relationship has been evaluated us-
ing the Pearson’s Correlation Factor.
The total organic carbon content (TOC) and total inorganic
carbon content (TIC) was measured on C-MAT 5500
Ströhlein device in the laboratory of the Geological Institute
of the Slovak Academy of Sciences in Banská Bystrica. TIC
content was re-calculated on the content of CaCO
3
in 35 se-
lected samples.
O and C isotope ratios were analysed in 65 samples in CO
2
after the standard dissolution of samples in 100% phosphoric
acid on the Finigan MAT-2 Mass Spectrometer in the labora-
tories of both the Czech Geological Institute in Prague and the
Institute of Paleobiology of the Polish Academy of Sciences
in Warsaw. The results are presented in standard delta nota-
tion ( ) in permil (‰) relative to the Vienna International Iso-
topic Standard (VPDB) with 0.01‰ accuracy.
The carbon isotope ratio of C
org
was analysed after carbon-
ate dissolution in 8 samples enriched to TOC. The
13
C mea-
surements were performed in the Czech Geological Survey
Laboratory in Prague by flash combustion in a Fisons 1108
Elemental Analyzer coupled with Mat 251 Isotope Ratio Mass
Spectrometer in a continuous flow regime. The sample size
was adjusted to contain a sufficient amount of C
org
to obtain
external reproducibility of 0.15 ‰ for
13
C
org
for all types of
samples with NBS22 as the reference material. Isotope data
are reported in the usual delta ( ) notation relative to VPDB.
Foraminiferal tests were studied in thin sections by optical
microscope. Bivalve molluscs were prepared mechanically by
vibro-tool, they were coated with ammonium chloride prior to
photographying. Shark teeth were collected mainly from the
upper part of Beds 2.2 and 2.3, single fish teeth and vertebrae
from insoluble residue after dissolving samples 2.3, 3.4, 13/14
and 14 in diluted acetic acid. Descriptive terminology of
Chondrichthyes is based on Cappetta (1987) and fish termi-
nology is based on Swift & Martill (1999). The shark and fish
teeth are housed in the Natural Science Museum in Bratislava.
Tooth photographs were taken by JSM-6390 (JEOL) scanning
electron microscope in the Banská Bystrica Department of the
SAS Geological Institute and in the State Geological Institute
of Dionýz Štúr in Bratislava.
Magnetic susceptibility (MS) and rock magnetic studies
were performed in the Paleomagnetic Laboratory of the Polish
Geological Institute—National Research Institute in Warsaw.
MS was measured in 143 samples using KLY-2 kappabridge
(AGICO Brno, frequency 0.92 kHz), and normalized for
mass. Rock magnetic experiments on pilot collection of 22
specimens included measurements of MS in low (0.47 kHz)
and high (4.7 kHz) frequency using a Bartington MS2 sus-
ceptibility meter (to evaluate the contribution of the very fine
magnetic fraction close to superparamagnetic state), isother-
mal remanent magnetization (IRM) applied in the field of IT,
Fig. 3. Lower part of the Fatra Formation in the Kardolína section
formed by the “tempestite cycle” (Beds 3 to 10). Right lower cor-
ner: the Bed 4 with loadcasts on the base.
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Fig. 4. Quartz grain size (left column, average size denoted by thick line) and percentage content of quartz grains (right column). Each
point was obtained by averaging of 200 measurements in a particular thin section with the use of the NIS system. Right column: Magnetic
susceptibility of the Kardolína section sequence and interpretation of sedimentary environment. Lithological signs same as in Fig. 5.
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Fig. 5. Lithological composition of the uppermost three cycles of the Carpathian Keuper and the lowermost seven cycles of the Fatra Forma-
tion in the Kardolína section. Left: Lithological log shows numbering of beds in negative numbers down from the Fatra Formation base in the
Carpathian Keuper, but in positive numbers upwards in the Fatra Formation proper. Micrite content (in percent) increases to the left from the
zero axis, antagonistic sparite representation increases to the right. Bioclasts content indicated by asterisks: their content is positively related to
sparite in the lower part of the sequence, but inversely in the upper part, indicating autochthonous occurrence of benthic organisms.
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and then antiparallel in the 100 mT field, by means of
MMPM1 pulse magnetizer. S-ratio, calculated as a ratio of
IRM intensities applied in both fields was indicative for rela-
tive proportions of low and high coercivity minerals.
Results
Lithology and fossils
The Carpathian Keuper
Two of the three informal members recognized by
Michalík (1977) in the Carpathian Keuper sequence, namely
the “lower clastics” and the “main claystone” are covered
below the scree (Rychliński 2008). The thirty meters thick
sequence of mixed terrigenous, lacustrine, fluvial and eolian
variegated greenish and violet-red dolomitic claystones with
occasional intercalations of pale greenish-grey clayey dolos-
tone, exposed in the Kardolína section, represents the upper-
most part of the Carpathian Keuper (“upper dolomite
member” of Michalík, l.c.). Bedding planes of rusty weather-
ing pale greenish-grey dolomicrite layers (20 to 130 cm
thick) sometimes bear ripple marks. Interbeds of yellow-, vio-
let-, or dark grey claystone may attain thickness of 20 to
160 cm, but sometimes they are only few centimeters thick.
“Unit I” is typical of thinning- and fining upwards ar-
chitecture (65 to 20 cm). Grey biomicrite with raised CaCO
3
content (Beds —43 to —41) contains dispersed quartz grains
(0.005 to 0.2 mm in diameter; Fig. 4) and numerous ostracod
tests (3 to 10 %; Fig. 5). Higher up (in Beds —40 to —38) the
dolomicrosparite content increases (to 9 %), and fragments
of plants become abundant. Dolostone layers are followed
by a 330 cm thick brown claystone interval.
Dolomicrite layers (14 to 65 cm thick) of the “unit II”
of lumpy texture contain dispersed tiny dolomite crystal nu-
clei becoming abundant upwards, where dolomicrosparite
and even dolosparite prevails. Claystone interbeds are 2 to
60 cm thick. Grey claystone lense in basal part (interbed be-
tween Beds —35 and —34) contains rich and relatively large
carbonized fragments of plants.
“Unit III” forms an eminent rock step of thick (20 to
130 cm) dolostone layers. Dolomicrosparite on the base
(Bed —23) contains small plant fragments. Dolomicrite beds
(Beds —22 to —16) are of lumpy structure, with an admixture of
eolian quartz silt (0.02 mm), larger quartz grains (0.04 to
0.05 mm) are rare, tiny plant fragments occur occasionally.
Dolomicrosparite beds (Beds —15 to —11) contain sparry crys-
tallites, dolomicrite occurs in irregular nests and lumps. Lumps,
pellets, phytoclasts and tiny shell fragments occur in dolomi-
crite in the upper part (Beds —10 to —6). Biodetritus (ostracods,
foraminifers, bivalve shell fragments, fish teeth and scales) be-
come frequent in the uppermost layers (Beds —7 and —6).
The Fatra Formation
The Fatra Formation attains a thickness of 96 m here, in
contrast to other places where it does not exceed 25 to 53
meters. Michalík (1978), Michalík et al. (1979), Gaździcki et
al. (1979) divided the sequence into two biostromal members,
separated from each other by a “barren interval”, from the un-
derlying Carpathian Keuper by “basal beds”, and from the
overlying Kopieniec Formation by “transitional beds”. How-
ever, detailed study of the Kardolína section shows that the ar-
chitecture of the Fatra Formation is much more complex.
Transgressional “unit IV” (Figs. 4—5): Each of five
palustrine (shallowing upwards) cycles (Beds —5 to 2.3;
Fig. 5) starts with grey dolostone or even with dark organo-
detrital limestone and intercalation of dark brown to black-
grey shale. The sequence was reduced by condensation and
resedimentation (pale dolostone clasts dispersed in clayey
matrix, dark crusts, erosion on bed surfaces).
Dark to black-grey argillites (70—120 cm thick) contain
small pieces of carbonized wood, ooids, bone fragments,
shark teeth, linguloid brachiopods, bivalves and black inter-
layers of laminated bituminous argillitic lime dolostone.
Wavy (flaser) and parallel lamination appears in dolostone
intercalations in the middle of black shales. Black ferrugi-
nous/phosphate crusts enriched by dispersed tiny rock clasts,
fish teeth and bone fragments occur on upper bedding
planes.
Fine clastic laminae in Beds —4, —3 and in the “zero beds”
(0.1 to 0.8) contain numerous foraminiferal tests (Agatham-
mina austroalpina Kristan-Tollmann & Tollmann; Figs. 4
and 6a—b; 15 to 60 in one thin section), indicating deposition
in a low-energy environment, most likely on tidal flats.
U-shaped spreiten-burrows (with diameter of 35 to
40 mm) of Rhizocorallium jenense Zenker, parallel or ob-
lique to bedding plane occur on the base of the dark marl-
stones of Bed 0.2 (Fig. 6c). Their limbs are more-or-less
parallel. The tube ornamented by scratchy bioglyphes is
5 mm wide, its length is greater than 150 mm. Spreite lamel-
lae of coarser sediment with rounded litho- and bioclasts (1 to
2 mm) usually attain diameters of > 1 : 5 .
The oldest bivalve molluscs (Modiolus minutus Lamarck)
appear in the Bed —3.2. Higher levels of the “zero beds” (0.3
and 0.4) contain more diverse bivalve fauna: Bakevellia
praecursor (Quenstedt), Isocyprina ewaldi (Bornemann),
Modiolus minutus, Neoschizodus? sp., Pleuromya? sp.
The yellowish weathering fine-organodetrital limestone
layer (Bed 1) contains a lot of broken shells correlatable with
water turbulence, rather than with micrite content. Clastic
quartz grains are rare and rather small, bearing signs of
wind- not of riverine transport. Biodetrital limestone is fol-
lowed by brown claystone intercalated by dolostone layers
with bone-bed type surfaces. Condensation occurs near the
top of individual layers, sometimes connected with enrich-
ment of phosphatic matter, fine breccia and teeth and bone
fragments (“bonebeds” 2.1 and 2.2; Fig. 7).
A shark tooth of Hybodus minor Agassiz and another 23
teeth belonging to Lissodus minimus Agassiz were collected
in Beds 0.4 and 2.1. The symmetrical tooth of the first species
is 1.5 mm high. High, upright central cusp flanked by up to
four pairs of lateral cusplets with fairly wide base is lingually
inclined in lateral view. Fairly coarse vertical ridges descend
cusps from apices, occasionally bifurcate basally. Lateral cut-
ting edges of cusps are sharp. Shallow root lingually projects
in so-called “lingual torus”, roughly semicircular in basal
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Fig. 6. a – Foraminifer Agathammina microfacies (the best preserved specimens are arrowed), Kardolína section, Fatra Formation base
(Bed 0.3). b – Agathammina austroalpina Kristan-Tollmann & Tollmann, 1964, layer 0.4. c – Rhizocorallium jenense, Bed 0.2. d – spreite
lamellae bordered with U-tube. e –scratches inside the U-tube.
view and perforated by numerous vascular foramina. Labial
face attains less than one-fifth of total tooth height.
Teeth of Lissodus minimus are up to 4 mm long. Low crown
with stubby central cusp is flanked by up to five pairs of very
low lateral cusplets and ornamented by series of often bifurcat-
ing vertical ridges descending from cusp apices on labial and
lingual faces. Longitudinal ridge surrounds tooth along surface
of crown shoulder. Lateral margins of crown extend well be-
yond crown/root junction. Distinctive peg-like expansion of
central cusp is situated low down on labial side. Pressure scar
resulting from tooth to tooth contact in the jaw often developed
in corresponding position on lingual side of central cusp. Root
is of approximately same height as crown and projects slightly
lingually from crown undersurface. Its upper face on labial side
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Fig. 7. Shark and fish teeth and vertebrae from bonebeds in transitional cycles of the Fatra Formation in the Kardolína section. A – Hybodus
minor Agassiz, 1837; B – molariform tooth of Sargodon tomicus Plieninger, 1847; C – fish vertebra; D – Lissodus minimus Agassiz, 1839;
E – fish vertebra; F1, 2 – incisiform tooth of Sargodon tomicus Plieninger, 1847; G – vertebral spine?; H, I – Severnichthys acuminatus
(Agassiz, 1835), H – tooth of “Saurichthys longidens” type; I – tooth of “Birgeria acuminata” type.
Fig. 8. Rhaetian bivalves from basal part of the Fatra Formation, Kardolína section. White scale bars = 1 cm. A, B – Placunopsis? alpina
(Winkler, 1859). Two left valves with xenomorphic sculpture. Specimen on the left side was originally attached to the closed ventral margin of
another, probably “pectinid” species, Bed 8; B – Left valve (coll. 5.1/94), Bed 5.1v; C – Bakevellia praecursor (Quenstedt, 1856). Internal
mould of right valve, Bed 2.3; D, G – Rhaetavicula contorta (Portlock, 1843), D – right valve, G – left valve, Bed 2.3; E – Palaeocardita
austriaca (von Hauer, 1853), right valve, Bed 8; F – Gervillaria inflata (Schafhäutl, 1851), right valve, Bed 5.1 (coll. 5.1/72); H – Elegan-
tinia emmrichi (Winkler, 1859), right valve, Bed 5.1 (coll. No. 5.1/61); I, J – Entolium (Entolium) aff. lunare (Roemer, 1839), I – External
mould of the dorsal part of right valve. Byssal notch is developed below the anterior auricle, J – left valve, 10; K – Propeamussium (Par-
vamussium) schafhaeutli (Winkler, 1859), left valve. Impressions of internal radial ribs are visible in the central part of the discus, Bed 10;
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L – Plicatula archiaci (Stoppani, 1861), left valve, Bed 5.1v (coll. 5.1/94); M – “Permophorus” elongatus (Moore, 1861). Internal mould of
the left valve, Bed 5.1v; N – Atreta “intusstriata”. Right valve cemented on the surface in the umbonal part of the Propeamussium (Parva-
mussium) schafhaeutli (Winkler, 1859), left valve, Bed 10; O – Nuculana (Nuculana) deffneri (Oppel, 1856), left valve, Bed 5.1 (coll. 5.1/3);
P – Botulopis faba (Winkler, 1859), right valve, Bed 5.1.
Continued from the previous page
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is very shallow, bearing a longitudinal row of tiny vascular fo-
ramina. Labial face of root is concave, containing much larger,
randomly distributed foramina in its lower portion.
Fish are represented by four molariform and incisiform
teeth of Sargodon tomicus Plieninger (Fig. 7) and conical
teeth of Severnichthys acuminatus (Agassiz), a “primitive”
basal actinopterygians. Two tooth types are recognized within
the latter species, each of which has previously been assigned
to a separate taxon: “Birgeria acuminatus” type (4 teeth) and
“Saurichthys longidens” type (2 teeth).
Tempestite “unit V”. This four and half meters thick
limestone sequence (Beds 3—7) consists of bedded (10—
30 cm) grey biomicrites to calcarenites with wavy bedding
planes. They contain frequent mollusc and brachiopod
shells, sometimes with distorted geopetal fillings. Loadcasts
and erosional marks on the layer bases, and gradation of
clasts occur frequently, indicating origin in distal tempestite
lobes laid on a soft marly bottom. Intensive storm activity
seems to be a typical feature of the environment during sedi-
mentation of this cycle.
Between loadcasts, deformed tubular bodies with typical
Y-shaped structure and ramification attributable to Thalassi-
noides sp. occur. These traces were produced by crustaceans
(Bromley 1996) indicating omission surfaces due to sudden
erosive events (Mikuláš 2006).
Foraminiferal diversity increases upwards (Aulotortus friedli,
Aulotortus, Frondicularia, Planinvoluta, Ophthalmidium,
Nodosaria). They are accompanied by other marine organ-
isms (Aciculella, Theelia, solenoporaceans, ostracods). The
first brachiopods appear in Bed 5.4.
The preservation of originally aragonite shells (recrystal-
lized or as internal or composite moulds) of four bivalve as-
sociations recognized within this cycle proves that the fossil
record was not depleted and it represents the original compo-
sition.
a. The Rhaetavicula contorta association (Bed 2.3; Figs. 8,
9, 11c) characterized by dominance of epifaunal byssate-
(46 %), semi-infaunal byssate- (30 %) and cementing bivalve
types (18 %) is composed of suspension feeders. Pectenids
like Propeamussium (Parvamussium) schafhaeutli (Stur) and
Chlamys mayeri (Winkler) were present among these first bi-
valve colonizers. Right valves of Rhaetavicula contorta (Port-
lock) occur rarely (Fig. 8; similarly to statements of Pflücker
& Rico 1868; Cox 1961; Ivimey-Cook et al. 1999). Relatively
small shell size and lack of infaunal molluscs points to nutri-
ent-poor and dysoxic substrate, their preservation (left and
right valves together, no fragmentation but post-mortem disar-
ticulation only) indicates low water energy above a soft but
stable substrate. A possible epifaunal character of these ani-
mals attached to sea plants can be considered, too.
The mixed Rhaetavicula contorta and “Placunopsis” alpina
association (Bed 4; Fig. 8; 34 % of byssate epifauna, 25 % of
byssate semi-infauna) reflects diversification within a quiet,
nutrient poor environment on a firm and stable substrate in a
carbonate regime. Increase of cementing bivalves (“Pla-
cunopsis” alpina: up to 30 %) could have been associated
with a firmer substrate (abundant bioclasts, shell fragments).
b. The tempestite coquina of 5.1 Bed contains accumula-
tions of large dissarticulated convex down (both right and left)
Gervillaria inflata (Schafhäutl) and “Permophorus” elongates
(Moore) valves with soft body imprints (Figs. 8—10, 11b). The
association is composed of byssate semi-infauna (50 %), shal-
low infauna, mobile- (34 %), or byssate epifauna (14 %),
which, with the exception of one detritus eater (Nuculana sp.),
were suspension feeders. This fact indicates a firm and stable
substrate in a high energy environment, supplied with food in
suspension. Despite reworking and mixing, right and left
valve ratio does not indicate any significant sorting (Fig. 9).
Shell accumulation of the “Corbula” alpina association domi-
nated by shallow infaunal suspension feeders (93 %) occur at
the base of Bed 7b (Figs. 9, 10). The composition of this
storm shell accumulation is identical to that of soft-bottom
bivalve association of the underlying marlstone. Lack of
epifauna could be associated with the scarcity of attachment
opportunities. On the upper bedding plane of this bed, clusters
of Rhaetavicula contorta, rarely of Modiolus minutus occur.
Shallow infaunal suspension feeders are dominant (96 %) in
the association from the Bed 9.3 (Fig. 11). This 1.5 cm thick
accumulation resembles that of the Bed 7b. However, while
the former association occurs on the tempestite base, the latter
one is situated in the upper part of the bed as a result of ero-
sion of fine mud by bottom currents. Convex-up and down
and also articulated shells occur. The underlying marlstone
contains the same species composition which indicates condi-
tions similar to Bed 7b.
c. Sorting due to storm activity formed temporary firm sub-
strate for cementing larvae of “Placunopsis” alpina, of large
Plicatula sp. and of attached Atreta intusstriata forming shell
accumulation (Figs. 8—11a). Epifaunal cementing bivalves are
dominant (65 %) in this association (Beds 5.1v, and 8b;
Fig. 9), followed by epifaunal byssate (30 %) and semi-infau-
nal byssate bivalves (10 %). In spite of some redeposition, bi-
valve composition indicates a firm and stable substrate. The
“Placunopsis” alpina shells are exclusively left upper valves.
While Triassic “Placunopsis” shells cemented to the substrate
(Seilacher 1954; Hölder 1990; Hautmann 2001), Jurassic
forms attributed to different taxa were byssus-attached (Todd
& Palmer 2002). Secondary texture patterns (Fig. 8a,b) devel-
oped on left valves copying the surface of the substrate of their
right valves. However, the texture resembles radially ribbed
bivalves, which are not common in the association (although
Paleocardita austriaca could be one possible candidate).
d. The Propeamussium (Parvamussium) schafhaeutli and
Entolium sp. association (Bed 10; Fig. 9) is dominated
(42 %) by epifaunal byssate pectinid bivalves (Entolium sp.
and Chlamys mayeri). Epifaunal free-lying/vagile morpho-
type is represented by radially ornamented left valves of
Propeamussium (Parvamussium) schafhaeutli (32 %) only.
No right (smooth and thin-shelled) valves were found, al-
though both equally smooth and thin valves of Entolium sp.
are common. Microstructure of both species shows aragonite
shell mineralogy. Long exposure before their burial could be
indicated by common cementing of Atreta richthofeni on both
outer and inner surfaces. Hence, less resistant right valves
were broken and dissolved. The association lived on a stable
detrital substrate with medium water energy near the maxi-
mum storm wave base. Protected shelters under empty bivalve
shells were often inhabited by ostracod populations (Fig. 12).
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Fig. 9. Histograms showing percentual representation of species in bivalve assemblages from individual beds in basal part of the Fatra For-
mation, Kardolína section.
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“Unit VI” – eolianites. Thick limestone layers (Beds 8
and 9) form the base of the sixth, 12 m thick unit. It is formed
by dark brown aleuritic marl with intercalations of dark grey
fine detrital argillaceous limestone (fining and thinning up-
wards cycle). Abundant quartz grains attaining diameters of
0.02 to 0.03 mm indicate eolian transport. Burrows of infaunal
organisms occur in the uppermost parts of the layers.
Fig. 10. Rhaetian bivalves from basal part of the Fatra Formation, Kardolína section. White scale bars = 1 cm. A – “Permophorus” elongatus
(Moore, 1861). Storm accumulation of shells, Bed 5.1 (coll. No. 5.1/2); B – “Chlamys” mayeri (Winkler, 1861), left valve, Bed 8; C – Ger-
villaria inflata (Schafhäutl, 1851). Stormy shell accumulation on the lower bedding plane, Bed 5.1; D – Corbula alpina Winkler, 1859. Shell
accumulation on the lower bedding plane, Bed 7; E – Protocardia rhaetica (Merian, 1853). Moulds of the right (upper left corner of photo)
and left valves (in the middle of the photo), Bed 7.
Two types of isolated fish teeth from Beds 13/14 and 14 be-
long to Sargodon tomicus Plieninger, 1847. The molariform
type is characterized by a hemispherical crown up to 4 mm in
diameter, circular to oval in occlusal view, often heavily worn.
Wearing reveals characteristic pattern of underlying dentine,
consisting of radial network of large cavities with finely
branching canaliculi at their ends. Molariform teeth were
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Fig. 11. Graphic reconstructions of three Rhaetian bivalve assem-
blages from the lowermost part of the Fatra Formation, Kardolína
section. a – “Placunopsis” alpina assemblage, Bed 5.1v; b – Rhae-
tavicula contorta assemblage, Beds 2.3 and 4; c – “Corbula” alpina
assemblage, Bed 5.1.
Fig. 12. Valve of Placunopsis alpina with cluster of ostracods im-
mediately inside. Scale bar is equal to 10 mm.
arranged in longitudinal rows on both upper and lower jaws,
with the smallest teeth in front and at sides of dentitional pave-
ment. Incisiform teeth up to 14 mm long comprise chisel-like
crown surmounting a deep root. Lingual face of crown is di-
vided into two by a wear facet in centre produced by func-
tional ante-mortem contact abrasion. As in all bifid crowns,
highest cusp is located closest to midline of mouth. Incisiform
teeth were used to pluck bivalves from the substrate, and the
battery of molariform teeth provided an effective mill for
breaking their shells (Swift & Martill 1999). Teeth of Birgeria
acuminata (Agassiz) were found between Beds 13 and 14.
“Unit VII”. The seventh unit is about 10 m thick; it
starts with sandy organodetrital limestone (Beds 15 and 16)
with nodular appearance (flaser texture). Intercalations of
black marls are rich in coprolites, fish teeth, pectenids and
other bivalve shells, and crinoids. Layer 19 contains large
megalontid bivalve shells. Higher up, the clay content in-
creases.
“Unit VIII”. Thick-bedded limestones (Beds 20—24)
contain debris of corals transported down the submarine
slope. Other organic fragments (bivalve shells, crinoids, oss-
icles) are less frequent. Intercalations of grey marl with bra-
chiopods Rhaetina gregaria (Suess) in situ appear in the
upper part of this unit.
“Unit IX”. The ninth unit starts with detrital lime-
stone. Thick algal dololaminite layer (Bed 29) preserved fine
record of dolostone rhythms. Marls increase in the higher
part of the thinning upwards cycle.
“Unit X”. The tenth unit consists of thick-bedded fine
organodetrital limestones of slope facies. This lithology
records the start of a general deepening of the basin.
Magnetic susceptibility and rock magnetic properties
MS values are moderately high for carbonate rocks, mostly
in the range between 5 and 20 10
—8
m
3
/kg, with a single
maximum above 30 10
—8
m
3
/kg (Fig. 4). An increasing trend
was observed from the bottom (Carpathian Keuper facies) up
to the middle part of the section, with maximum values in
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the lower part of the Fatra Formation, at the bottom of the
VI-th cycle (Fig. 4), followed by a decreasing trend in the up-
per part of the Fatra Formation. All pilot samples studied re-
vealed significant MS frequency dependence (Fig. 13a) which
accounts for contribution of ultrafine magnetic particles, close
to superparamagnetic to single domain state to MS (Forster et
al. 1994; Grabowski et al. 2009). As there is also a very good
correlation between MS and IRM intensity acquired in the 1 T
field (Fig. 13b), it is necessary to conclude, that MS is based
mostly on ferromagnetic minerals. Magnetite seems to be the
most important magnetic, as inferred from predominantly low
coercivities – samples are almost saturated in the field of
300 mT (Fig. 13c) and maximum unblocking temperatures of
low and medium coercivity fraction (0.1 T and 0.4 T respec-
tively; Fig. 13d) between 500 and 550 °C. Subordinate
amounts of hematite occur as well, as is indicated by slightly
increasing IRM intensity above 500 mT (Fig. 13c), and max-
imum unblocking temperatures around 650 °C for the high
coercivity (1.4 T) fraction (Fig. 13d).
Geochemistry
Major elements
Total rock analyses of 12 samples were performed (Ta-
ble 1) in order to obtain a more precise idea of the origin of
the source material and to determine chemical changes po-
tentially forced by hydrological, climatic and other factors.
The chemical composition of the samples is given mainly by
the proportion of carbonate (represented by CaO, MgO) and
silicates (represented by SiO
2
, Al
2
O
3
; Table 1). The dolomite
non-carbonate content is higher (approximately 20 to 30 %)
than in limestones (approximately 5 to 15 %; Fig. 16). Sam-
ples —34, —3.2 and 14 can be designated as argillites, as their
carbonate content is low ( < 5 to about 30 %; Fig. 6).
The composition of major elements in argillites is close to
the Post-Archean Australian Shale (PAAS) composition and
could indicate that (weathered) felsic rocks were the proba-
ble source of our sediments (German et al. 1991; Condie
1993; Bau & Dulski 1996). These characteristics are in line
with the mineral composition of samples analysed. Illite with
only very low content of smectite dominates in the clay size
fraction of samples 32, —3.2, 14, 19G. The clay composition
of samples both from the Carpathian Keuper or from the
Fatra Formation is almost identical (Biroň in the Środoń et
al. 2006, or in Michalík et al. 2010).
In spite of relatively low values, P
2
O
5
, MnO, and S
tot
con-
tents are higher in the Fatra Formation limestone than in the
Carpathian Keuper dolostone: they document a shift in sedi-
mentary and diagenetic conditions associated with marine
transgression. P
2
O
5
enrichment was probably related to in-
creased bioproductivity in the marine basin indicated by
bonebed occurrence.
Trace elements and REE
Low silicate admixture complicates the interpretation of
large ion lithophile elements (LILE: Rb, Cs, Ba), with the ex-
ception of Sr. The LILE substituting K are accumulated in the
phyllosilicates in both parts of the sequence. High Sr content
in carbonate (495—861 ppm) in comparison with the argillites
(135—228 ppm) and high correlation of Sr vs. Ca (r > 0.9) doc-
uments Ca vs. Sr substitution, typical of biogenic aragonite or
of a phase precipitated from evaporated marine water or brine
(Rosen et al. 1989; Garcia del Cura et al. 2001; Korte et al.
2005). Carpathian Keuper dolostones are enriched in Sr but
more depleted in total sulphur (S
tot
~
~ 0.02 %) than limestones
(0.02 to 0.55 %) of the Fatra Formation (Table 1). In accor-
dance with the facies scheme presented, it is possible that do-
lomite comes from the sulphate-free fluvial/lacustrine waters
(Warren 2000; Garcia del Cura et al. 2001 and their references).
However, low S content could result from diagenetic leaching
of sulphate. By analogy, higher S
tot
content and pyrite grains
observed in thin sections of limestone document a marine-water
environment. Framboidal aggregates represent a typical dia-
genetic pattern of pyrite: they indicate more O-depleted dia-
genetic conditions than those of limestone accumulation. Low
C
org
content was connected with balanced productivity and, lo-
cally, with higher input of terrestrial organic debris, as indicated
by the quality of the organic matter and by C-isotope analyses.
The compositional pattern between the incompatible ele-
ments Th and Y and the compatible Sc, Cr, V and Ni indicates
that the sediment is more likely to have originated from a fel-
sic than from a mafic source (Fig. 14; Table 1). Incompati-
bility of Th and Y results in their higher concentration in well
differentiated felsic rocks (Condie 1993; Cullers 2000). The
Th/Sc ratios are generally similar to the ratio reported for the
PAAS (0.91). The Y/Ni ratios of sediment studied are higher
than these of the PAAS (0.49). In spite of high Cr/Th and Cr/V
ratios (PAAS = 7.53; 0.73 respectively), the samples are closer
to the felsic source and point to local enrichment of Cr-miner-
als rather than to origin from a mafic source. This conclusion
fits with the interpretation of major elements and with mineral
composition.
The total rare earth elements (TREE) contents in the argillite
samples are similar to those of PAAS (Condie 1993; Cullers
2000). The samples —32 and 14 display flat PAAS-normalized
REE pattern with little depletion of heavy REE (HREE;
Fig. 15). The sample —3.2 (IV-th cycle) reveals weak HREE
enrichment expressed by ratios Gd
N
/Yb
N
= 0.8 and La
N
/
Yb
N
=0.69. All three samples show weak negative Eu anomaly
(Eu/Eu* = 0.82, 0.77 and 0.94; Table 1) whereas Ce/Ce* ratios
are close to unity and record very weak negative Ce anomaly.
Dolostones of the Carpathian Keuper are depleted of REE
relative to PAAS (0.2 to 0.4) and show slight positive Eu
anomaly (Fig. 15; Table 1). Fatra Formation limestones are
depleted relatively to PAAS but the elements from Sm to Ho
(middle – MREE; Ounis et al. 2008) relatively increased to
0.5—0.6 content of PAAS. The Eu values reach PAAS level and
show positive Eu anomaly. Increased content of the MREE doc-
uments different fractionation of REE in the Fatra Formation
limestones in comparison with the Carpathian Keuper dolos-
tones and can be interpreted in line with sedimentary evolution.
C and O isotopes
The results of C-isotopic analyses indicate two individual
terrestrial vs. marine sources of organic matter. Less negative
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Fig. 13. Rock magnetism and its correlation with geochemistry: a – Diagram of frequency dependence of magnetic susceptibility: difference
between low frequency MS (
lf
) and high frequency MS (
hf
) plotted as a function of
lf.
b – Correlation between volume magnetic suscepti-
bility (k) and intensity of isothermal remanent magnetization acquired in the field of 1 T (IRM
1 T
). c – Stepwise acquisition of IRM, sample 13.
d – Thermal demagnetization of 3 axes IRM acquired in the fields of 0.1 T, 0.4 T and 1.4 T. e – Correlation between mass normalized MS ( )
and Al
2
O
3
content, Fatra Formation. f – Correlation between mass normalized MS ( ) and Al
2
O
3
content, Carpathian Keuper.
values (—24.63 to —24.45 ‰ VPBD) occur in Beds —34/1, —34/2
and 19G, 19F with higher content of plant debris, in contrast
with more negative ones (—27.27 to —25.64 ‰ VPDB) coming
from the Beds —5 to +13 containing organic matter with more
marine character (Fig. 16, see palm tree marks).
The C and O isotope data demonstrated in plots (Figs. 16, 17)
document different character of two carbonate production sys-
tems represented by Carpathian Keuper dolostones and Fatra
Formation limestones in the Kardolína section. The values of
both carbon and oxygen isotopic ratios achieved relatively
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Element Unit
Beds
25.1 19.1 14
10.3 5.5 2.3A 0.8 –3.2 –22
–15
–23
–34
SiO
2
%
3.43 5.51 53.35 8.61 9.19 11.90 6.60 56.1 17.07 14.47 20.90 62.54
Al
2
O
3
%
0.87 0.97 13.30 1.32 2.26 2.84 1.70 16.67 5.36 5.95 3.63 15.58
Fe
2
O
3
%
1.12 1.97 4.92 2.07 2.34 2.70 0.45 4.72 2.05 2.05 2.71 1.80
MgO
%
1.42 1.63 1.98 1.05 1.66 1.52 1.30 1.97 9.37 14.34 16.09 3.07
CaO
%
51.02 49.39 9.44 47.76 45.42 43.51 48.39 4.01 28.26 23.22 21.51 2.28
Na
2
O
%
0.07 0.11 0.7 0.17 0.15 0.06 0.4 0.18 0.12 0.18 0.06 0.43
K
2
O
%
0.1 0.14 2.41 0.15 0.39 0.31 0.22 4.10 1.35 1.81 0.23 4.37
TiO
2
%
0.04 0.04 0.74 0.07 0.12 0.11 0.07 0.94 0.27 0.23 0.13 1.01
P
2
O
5
%
0.01 0.08 0.06 0.19 0.11 0.08 0.02 0.12 0.02 0.04 0.03 0.12
MnO
%
0.04 0.08 0.04 0.14 0.09 0.17 0.05 0.08 0.05 0.05 0.08 0.02
S
tot
%
0.21 0.55 0.02 0.41 0.30 0.13 0.03 0.02 0.02 0.07 0.02 0.00
LOI
%
41.8 40
12.9 38.4 37.7 36.7 40.7 10.9 35.8 37.3 34.3 8.60
Ba
ppm
8
13
165
15
28
52
20
259
214
108
45
218
Co
ppm
0.8 3.5 9.5 2.7 4.2 2.0 <0.2 38.8 2.6 3.7 5.9 6.4
Cs
ppm
0.2 0.4 7.3 0.3 0.9 0.7 0.4 8.5 2.4 3.5 0.4 7.2
Cr
ppm
< d.l.
< d.l. 108.8
< d.l. 95.2 13.6 20.4 142.8 40.8 40.8 27.2 122.4
Hf
ppm
0.2 0.3 8.3 0.4 1.0 0.4 0.3 9.6 1.3 1.1 0.7 9.5
Nb
ppm
0.7 0.9 15.9 1.4 2.4 2.1 1.6 22.3 5.6 4.7 2.5 20.7
Ni
ppm
5.4 9.5 26.9 7.1 9.5 9.4 1.5 106.4 11.9 12.1 32.7 14.7
Rb
ppm
3.8 5.7 109.1 5.7 15.5 12.7 7.3 180.8 57.2 77.5 9.4 174
Sc
ppm
0.9 2
12
2
3
3
2
16
6
6
3
15
Sr
ppm
711
530
229
689
532
494
582
119
861
430
547
136
Th
ppm
0.6 2.1 12.1 1.6 2.4 2.2 1.1 17.7 4.3 3.9 2.3 18.4
U
ppm
1.3 0.7 2.5 1.7 1.4 0.9 3.2 12
1
1.5 1.4 9
V
ppm
11
16
111
22
21
23
17
127
33
41
25
104
Zr
ppm
6.9 13.8 298.9 15.9 34
16.2 11.1 354.1 51.8 36.3 23.3 320.1
Y
ppm
3.8 11.6 27.4 11
13.9 14.9 5.2 24.5 10.7 9.7 5.3 25.3
TREE
ppm
23.36 61.72 190.65 61.12 88.73 71.78 24.84 155.21 67.88 56.09 35.42 211.64
La
ppm
4.7 12.1 39.2 11.4 17.1 13.3 5.0 29.9 12.6 10.8 6.9 38.7
Ce
ppm
9.7 22.9 81.5 24.0 33.4 26.5 9.8 64.4 28.7 22.8 14.7 91.5
Pr
ppm
1.15 3.07 9.15 3.06 4.47 3.37 1.22 7.67 3.38 2.73 1.75 10.91
Nd
ppm
4.6 13.3 35.1 13.4 20.0 15.4 4.8 29.5 13.2 10.8 7.0 43.1
Sm
ppm
0.78 2.53 6.00 2.35 3.76 3.49 0.93 5.21 2.52 2.09 1.25 7.57
Eu
ppm
0.26 0.62 1.11 0.84 1.18 0.90 0.23 0.79 0.56 0.46 0.28 1.15
Gd
ppm
0.75 2.49 5.00 2.26 3.54 3.24 0.92 4.29 2.24 1.88 1.12 5.66
Tb
ppm
0.12 0.38 0.85 0.33 0.47 0.47 0.15 0.77 0.34 0.31 0.17 0.88
Dy
ppm
0.61 2.04 4.89 1.57 2.31 2.28 0.79 4.61 1.78 1.68 0.95 4.66
Ho
ppm
0.11 0.37 1.04 0.30 0.41 0.43 0.15 0.99 0.37 0.34 0.18 0.96
Er
ppm
0.29 0.92 3.06 0.83 0.98 1.17 0.4 2.92 1.00 1.02 0.51 2.80
Tm
ppm
0.04 0.13 0.46 0.10 0.14 0.16 0.06 0.48 0.15 0.15 0.08 0.45
Yb
ppm
0.22 0.77 2.85 0.59 0.85 0.94 0.34 3.2 0.9 0.89 0.46 2.85
Lu
ppm
0.03 0.10 0.44 0.09 0.12 0.13 0.05 0.48 0.14 0.14 0.07 0.45
LaN/YbN
1.57 1.15 1.01 1.43 1.48 1.04 1.08 0.68 1.03 0.89 1.10 1.00
Gd N/YbN
2.03 1.93 1.05 2.28 2.48 2.05 1.61 0.80 1.48 1.26 1.45 1.18
EuN/EuN*
1.58 1.15 0.94 1.67 1.51 1.25 1.16 0.78 1.10 1.08 1.10 0.82
CeN/CeN*
0.96 0.86 0.99 0.93 0.88 0.91 0.91 0.98 1.01 0.96 0.97 1.02
LOI (Lost of Ignition)
Eu/Eu* Eu-anomaly
Ce/Ce* Ce-anomaly
N-normalised to PASS
Table 1
wide ranges:
13
C from —5.04 to +2.63 ‰ VPDB,
18
O from
—7.03 to +2.49 ‰ VPDB associated both with facies and with
environmental variability of the sequence.
The
18
O vs.
13
C variation chart documents the polymodal
type of the data set but two main limestones and dolostones
subgroups are distinctly separated (Fig. 17). The position of
other points in the chart indicates more complex processes,
mainly in the “transitional beds”. The low
18
O vs.
13
C data
covariance of the whole set and/or separated subgroups docu-
ments quite well preserved isotopic records of the carbonate
beds and detects a transgression regime of sedimentation.
Discussion
REE distribution during transgression
The typical seawater REE pattern shows HREE enrich-
ment, often also with negative Ce anomaly (Hannigan &
Sholkovitz 2001; Haley et al. 2004; Ounis et al. 2008). The
REE (III) – carbonate ion complexes are the dominant dis-
solved REE species in seawater: their ability to form carbon-
ate complexes increases from light REE (LREE) to heavy
REE (HREE). Increased REE accumulation could be more ef-
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Fig. 14. Felsic/mafic sources of clastic material.
fective in the occurrence of biogenic apatite (like bonebed ap-
atite) where Eu
2+
or trivalent REE ions substitute Ca
2+
. The
REE released from iron oxides, from particulated organic mat-
ter (POC) and potentially from other active surfaces (clays)
served as alternative source of REE in the carbonates precipi-
tated (Haley et al. 2004; Shield & Webb 2004). Observed
changes in REE content (or pattern; Table 1, Fig. 15) indicated
a restoration of marine water composition during the trans-
gression. However, the REE distribution in sediments could
change due to fluctuation of redox and pH condition. Different
dissolved species can be introduced or removed from the sea-
water and cause variation in the water and sediments (Ounis et
al. 2008; Sheldon & Tabor 2009). The distribution of REE can
also indicate weathering process, because their leaching be-
haviour varies according the regional humidity and increased
acidity, as documented in paleosoils (Sheldon & Tabor 2009).
Eu and Ce anomalies in REE distribution pattern commonly
identify redox proxies, because Eu
2+
separates from other
REE
3+
under reducing condition and Ce
4+
divides into oxide
under oxidizing conditions (Cao et al. 2012).
The different REE distribution patterns in the sample set
studied indicate variability of the siliclastic source or unstable
Fig. 15. REE contents in argillites, limestones and dolomites of the Kardolína section.
transport by wind and water flow during Carpathian Keuper
dolostone and Fatra Formation limestone sedimentation. Eu
enrichment in other REE indicates more reductive conditions
during biogenic limestone precipitation or during early di-
agenesis, as relative increase of C
org
contents (Fig. 16) indi-
cates. However, biogenic carbonates are also enriched in
phosphate, in which REE accumulated. The “bell-shaped”
MREE-pattern could indicate that weathering of biogenic
phosphates in freshwater could mobilize MREE and relatively
increase its content in the limestone rock (Hannigan &
Sholkovitz 2001; Ounis et al. 2008). Local bone-beds oc-
curred in the basal part (Beds 0.4, 2.1, 2.2; Fig. 5) of the
Fatra Formation.
Carbon isotope distribution during transgression
Negative
13
C values in the Carpathian Keuper sequence
(Beds —43 to 0) and also in the first two sedimentary cycles
(IV/V) of the Fatra Formation (Beds + 1 to + 7: —3.25 to
—0.59 ‰; Fig. 16) fluctuate between —0.05 and —5.0 ‰, but
mostly in the range from —2 to —5 ‰. Later, in the sixth cycle,
13
C values continually increase to positive
13
C range (from
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Fig. 16. Contents of organic carbon (TOC) and
18
O and
13
C curves in the lowermost part of the Kardolína section.
—0.05 to + 1.22 ‰). These three cycles locate a span of tempo-
ral sedimentation and indicate continuing carbonate produc-
tion and accumulation within marine transgression. Increased
13
C (from 1.84 to 2.69 ‰) value fall into the typical interval
of marine limestone documented earlier (Michalík et al. 2007)
in the higher part of the Kardolína section. Positive
13
C val-
ues in limestone could indicate balanced marine conditions,
where “biological pump” supported effective carbonate pro-
duction without increase of accumulation and/or burial of or-
ganic carbon as documented by low content of total organic
matter in the samples (Fig. 16).
Negative
13
C values in dolomite generally document C en-
richment by light
12
C isotope in comparison with common
marine carbonates. Such isotopically light C could have been
produced by specific production or by biotic extinction in the
water column or by release from methane buried in sediment.
Negative C-isotope event could indicate regional or global cli-
mate change as documented in the T/J boundary beds else-
where (Pálfy et al. 2001, 2007; Ward et al. 2007; Michalík et
al. 2007, 2010; Preto et al. 2010). As
13
C negative values are
associated with dolostones, they must have been connected
with dolomite precipitation (Masaryk & Lintnerová 1997;
Warren 2000; Garcia del Cura et al. 2001; Berra et al. 2010).
Carpathian Keuper
18
O values fall in the range —7.03 to
+ 2.49 ‰ and are associated with facies differences (Fig. 17).
Negative to positive
18
O values in the range —1 to + 3 ‰ are
typical of massive dolostones of the third cycle. Samples
with more negative values in the interval from —3 to —1 ‰
are discontinually located in certain parts of the cycle and
probably indicate climatic/hydrologic changes and copy os-
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cillation pattern in sediments. However, as the cyclostratig-
raphy study indicates, the isotope sample set is too small to
verify this dependence.
Sharp negative
18
O excursions occur in the basal part of
the dolostone sequence (Beds —43 to —40: from —5.02 to —4.74)
and in the first cycle of the Fatra Formation (from —7.05 to
+ 2.03). In both parts, mixture of calcite/dolomite mineralogy
occurs. These
18
O changes can be either connected with
sedimentary facies, or they reflect composition of lake/basi-
nal water. Local climatic/hydrological changes controlled
the amount of fresh or meteoric water input to the Carpathian
Keuper’s brackish lake and decreased
18
O values. The
18
O
pattern of the Beds —4 to + 2 (cycle IV) indicates more com-
plex process induced by marine transgression, where short
saline to freshwater floods occurred.
Although post-sedimentary alteration of this part cannot
be entirely excluded, continual increase to more positive
13
C values documents continual restoration of marine ramp
and does not indicate any important diagenetic substitution
of carbonate phases.
Limestone
18
O values are relatively similar to each other
and fall in the range from —4.33 to —6.23 ‰, as a common fea-
ture of uppermost Triassic marine limestones (Michalík et al.
2007). A more positive
18
O excursion (—0.66 ‰) in Bed 29
was associated with early diagenetic dolomitization of algal
mats (Fig. 16). It reflected a salinity increase rather than fresh-
water influx. This supposition is underlined by slight response
of
13
C values to this episodic dolomitization.
Dolomitization model
As mentioned above,
18
O and
13
C variation (Fig. 17)
simply indicates heterogeneity of the sample set. In compari-
son with diagenetic marine dolostone (Smith & Dorobek
1993; Warren 2000; Wacey et al. 2007), dolostone data fall
into unusual area of the plot because of negative
13
C (—4 to
—3 ‰ VPDB) and more positive
18
O (in range from —1.5 to
+ 1.0). Relatively positive
18
O data indicate either freshwa-
ter or saline reservoir waters (or dolomite-forming fluids)
and negative
13
C values reflect input or generation of car-
phates and producers of CO
2
enriched to light
12
C. However,
study of the Coorong dolostone did not confirm regular oc-
currence of isotopically light C (Wacey et al. 2007). Nega-
tive
13
C values also occur in soil carbonates where the
influence of meteoric waters which are in chemical equilibri-
um with atmospheric CO
2
(—7 ‰ PDB) cannot be excluded
at all (Warren 2000). Model with equilibrated soil-water or
water-atmospheric CO
2
could be alternatively applied to the
isotope composition of limestone/dolomite mixed mineralogy
(—43 to —41 or —6 to —1) where negative
13
C (—4 to —3 ‰)
values are attached to negative
18
O (—4 to —5 ‰). A similar
mixed marine-meteoric model of the Carnian to Norian Keu-
per dolostone generation was presented by Rychliński (2008)
and Jaglarz (2010). A relatively high content of Sr in carbon-
ates came more probably from brine water. This interpretation
is in line with the facies character of the Carpathian Keuper
dolostones as climatically induced sediments.
Cyclostratigraphic remarks
The thickness of the Fatra Formation sequence in the
Kardolína section (107 meters) is three times greater than in
other sections. This gives a reason to suppose that the se-
quence is more complete, formed by a more rapid sedimentary
rate (60 mm/kyr) on a gentle submarine slope. 18 sedimentary
cycles were distinguished in the Fatra Formation, which are
attributable to short eccentricity (100 kyr) cycles, taking into
consideration the 2 Myr duration of the Rhaetian; and three
cycles have been discerned in the uppermost part of the Car-
pathian Keuper. The dominance of eccentricity cycles was
stated during the Late Permian (cf. Legler & Scheider 2008);
or during the Late Triassic/Early Jurassic (Haas et al. 2010).
Both the geometry and lithological composition of the majori-
ty of the Fatra Formation cycles indicate a shallowing upward
trend: however, this phenomenon was often combined with
the effect of freshwater influx bringing coarse sedimentary
particles (Fig. 18) in conditions of raised humidity trend at the
end of the Triassic (Ahlberg et al. 2002; Preto et al. 2010).
Fine lamination preserved in the “zero interval” of the
transitional (IV) cycle between the Carpathian Keuper and
Fig. 17. Grouping of C and O isotopes in carbonates of the Kardolína section compared
with typical composition of the Coorong dolomite.
bon enriched to light C, probable iso-
topically fractionated in biogenic/meta-
bolic process (Pálfy et al. 2001). If we
accept the sedimentary and microfacies
character of the dolostone studied, then
the C and O isotope and Sr contents in-
dicate that Keuper fine-crystalline dolo-
mite precipitated from brine or from
pore water and can be compared with
type B of the Coorong dolostone (Rosen
et al. 1989; Warren 2000; Garcia del
Cura et al. 2001; Wacey et al. 2007).
Brine with optimal Mg/Ca ratio can be
generated by microbial processes in
specific climate and hydrology. The life
activity of S reducing (SRB) and photo-
synthesizing bacteria was frequently
discussed as a source of organic matter
(Bechtel et al. 2007), consumers of sul-
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Fig. 18. Schematic illustration of cyclostratigraphic division of the Carpathian Keuper sequence in the Kardolína section based on bed
thickness.
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the Fatra Formation deserves special attention. Beds 0.3, 0.4,
0.5, 0.6 and 0.9 consist of argillite to marly mudstone. Detri-
tal quartz forms 0.4 to 2.3 mm thick laminae. Individual
laminae are arranged in a regular pattern (Fig. 19): two
thicker bands are usually followed by seven thinner ones.
Considering the average sedimentary rate, influx events
bringing quartz detritus must have repeated in rhythms of ap-
proximately 20 years (solar Hale cycles?).
The close-up view on the dololaminite in Bed 29 (Fig. 19)
is even more surprising. Laminae are well preserved, show-
ing details of a fine stratification pattern. Several laminae
show stromatolitic character of former algal mats. Planar
laminae are very thin (0.2 to 0.8 mm), in bundles of 7 to 9
( = Hale rhythm?). In closer view, series of thinner laminae
are visible between them, in groups of 5.
Magnetic susceptibility
According to Ellwood et al. (2000) and Crick et al. (2001),
the MS record in most marine rocks is of detrital origin and re-
lated to the influx of lithogenic fraction to a basin, controlled
by both: climate variations (e.g. humidity) and eustatic sea-
level changes. MS highs and lows are related to regressive and
transgressive intervals, respectively. The model seems to work
in rather open marine environments (Whalen & Day 2010).
However, in the carbonate platform settings an inverse corre-
lation might also be observed (Da Silva et al. 2009). In the
Kardolína section the lowest sea-level is postulated at the tran-
sition interval between the Carpathian Keuper and Fatra For-
mation. It corresponds well to MS trends observed in the
Kardolína section. The Carpathian Keuper with increasing MS
trend would correspond to the regressive interval, while step-
wise decrease of MS in the Fatra Formation might be inter-
preted as a transgressive trend. This interpretation alone would
be not sufficient because it might be possible that the decreas-
ing MS trend is related to dilution of ferromagnetic particles in
carbonate matrix, and thus to a possibly higher sedimentation
rate. However, as the same trend is also inferred from sedi-
mentological analysis (see above) and MS correlates quite
well with some sedimentological features, like quartz grain
size (Fig. 4), it might be accepted as a quite likely model.
The primary nature of the MS record might also be tested,
correlating the MS values with Al
2
O
3
. Al is regarded as a
predominantly lithogenic element which might be used as a
proxy for fine detrital clay input into the basin (Calvert &
Pedersen 1993; Śliwiński et al. 2010). The correlation graphs
Fig. 19. Lamination in Beds 0.3, 0.4, 0.5, 0.6, 0.9 and 29, in the Kardolína section. Scale bars are 10 mm long.
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(see Fig. 13e—f) reveal a moderate positive correlation be-
tween MS and Al content – this might be treated as prelimi-
nary confirmation that MS contains a significant detrital
component. However, both MS and geochemical data were
available from only 9 samples. Moreover, it seems that MS
carriers are different in the Fatra Formation and Carpathian
Keuper: the MS correlates with Al
2
O
3
within a lithostrati-
graphic unit, but when the entire dataset is considered (Fatra
Formation+Carpathian Keuper) – the correlation is not sig-
nificant! It cannot be excluded that a part of the SP magne-
tite is of authigenic origin and not directly related to other
erosion – derived components (Jackson 1993; Grabowski et
al. 2009; Devleeschouwer et al. 2010).
Paleocommunities
The lowermost sedimentary cycles contain sporadic fos-
sils, mostly plant fragments and ostracods, inhabiting tempo-
ral water reservoirs. The third cycle represents swampy
environments which contained much more diverse mixed
marine and brackish organisms: foraminifers (Agathammina),
bivalve molluscs (Rhaetavicula community), linguloid bra-
chiopods, sharks, fish, amphibians (?) and burrowing ani-
mals producing Rhizocorallium burrows.
The fifth cycle recorded stabilization of marine environ-
ments (and communities, cf. Michalík & Jendrejáková 1978;
Gaździcki 1983) affected by storm activity. Inhabitants of
shallow lagoons (Corbula and Gervillaria community) were
periodically washed out by stormy turbulent waters from the
soft bottom, killed and their broken shells were accumulated
in tempestite layers. Shell accumulations formed temporary
firm ground for an oyster (Placunopsis) community. During
continuing deepening and accumulation of fine mud, the
bottom was inhabited by an infaunal Propeamussium and
Entolium community.
Fine quartz dust transported by eolian activity accumulated
in a marine bay. Deteriorating oxygenation enabled deposition
of shaly beds rich in coprolites, crinoid ossicles, pectinid bi-
valves and fish teeth. Megalodon limestone indicates settle-
ment of pachyodont bivalves during shallowing events.
Conclusions
The Kardolína section yields an almost complete record of
the Rhaetian marine transgression into the Zliechov Basin. A
comprehensive study of mineralogy, lithology, lithostratig-
raphy, cyclostratigraphy, fossils, geochemistry including C
and O stable isotopes and rock magnetism has provided de-
tailed information about environmental changes at the end of
the Triassic.
The sequence consists of distinct cycles of 100 kyr eccen-
tricity and 40 kyr obliquity character, but some laminated
layers also bear signs of much finer rhythmicity, including
repetition in 100, 20 and even in 4(?) year cycles of events.
Rhythmically repeating detrital laminae were formed by al-
ternation of climatic parameters (monsoon-like periods).
Analysis of clastic quartz grain size and content shows that
both fluvial input and eolian activity were involved in their or-
igin. On the other side, high concentrations of foraminifers
(Agathammina) in some of these laminae indicates rather in-
tensification of marine influence.
The sequence stratigraphic and cyclostratigraphic division
fits well with magnetic susceptibility which reflects the dis-
tribution of authigenic and detrital constituents in the rock
sequence. The good preservation of the primary magnetic
record is promising from the point of view of magnetostrati-
graphic study which will be performed in the near future.
The integrated geochemical data are consistent with the
character and time span of sedimentary facies evolution. C
and O isotope curves responded selectively to changes of
eustacy and climate and tightly followed restoration of ma-
rine carbonate ramp during the Rhaetian.
A wide range of
18
O values (—7.0 to + 2.7) by itself is not
anomalous in the Triassic carbonates but combination of these
data with negative
13
C values resulted in an unusual distri-
bution of dolostone data in the plot (Fig. 15, Table 1). It
documents either dolomite precipitation from brackish or hy-
persaline lake water or its derivation from pore water compa-
rable to the Recent Coorong B dolostone. Less positive
18
O
values indicate level of diagenetic/thermal fractionation of the
oxygen isotope. Negative C values indicate water enrichment
to light C (HCO
3
—
) induced by microbial productivity.
Stabilization of benthic communities in the Fatra Formation
basin was not straightforward since it was strictly controlled
by physical environmental factors. Although foraminifers, bi-
valves and sharks appeared shortly after the start of the trans-
gression, bivalve mollusc biostromes were repetitively
destroyed by storms and temporary firm bottoms were colo-
nized by oysters and burrowers. Bottom colonization by
pachyodont bivalves, brachiopods and corals was possible
much later, in highstand conditions.
Acknowledgments: The authors acknowledge help from
three reviewers, namely Prof. József Pálfy for valuable dis-
cussion, inspiring comments and thorough corrections, but
also Prof. Ján Soták and Dr. Tomasz Rychliński who sub-
stantially contributed to the scientific level of the manu-
script. Field works could not have been done without the
painstaking help of our young co-workers, namely Jakub
Rantuch, Martin Závacký, Štefan Szalma, Mgr. Zuzana
Weissová, Dr. Peter Ledvák, Dr. Martina Martincová, Mgr.
Peter Klepsatel, Mgr. Ján Čatloš, and Mgr. Hanna Nizin-
kiewicz. We always met with friendly support from the Tatra
National Park State Forests administration and its Research
Station in Tatranská Lomnica (Dr. Stanislav Pavlarčík), and
from the Spišská Belá municipality, as well. Field research
was also supported by direction and workers of the Aca-
demia Hotel in Stará Lesná, where we always had our home
base. Thanks for financial support go to 0065/12 VEGA
Project. SEM photographs were provided by Dr. I. Holický
(State Geological Institute of Dionýz Štúr, Bratislava) and
by Mgr. N. Halašiová (Geological Institute SAS, Banská
Bystrica). MS and rock magnetic experiments were performed
within a Project No. 61.2301.0902.00.0 of the PGI-NRI, as a
part of the IGCP 580 Project. Isotope analyses were done
mostly by Dr. K. Małkowski (Polish Academy of Sciences,
Warszawa).
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