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, DECEMBER 2014, 65, 6, 433—450 doi: 10.1515/geoca-2015-0004
Introduction
The Skole Nappe is the most external nappe of the Eastern
Outer Carpathians in their Polish segment (Fig. 1A,B). It
comprises a 3.0—3.8 km thick series of the Lower Creta-
ceous—Neogene flysch sediments (Poprawa & Nemčok 1998).
The Lower Cretaceous strata are represented by silty and
clayey turbidites, classified to the Bełwin Mudstones (Hau-
terivian) and Spas Shales (Hauterivian—Albian). They contain
sandy turbidite intercalations of the Kuźmina Sandstones
(Fig. 2 – Koszarski & Ślączka 1973; Kotlarczyk 1978; Gucik
1987; Gucik et al. 1991; Gedl 1999). This series is interpreted
as deposits of post-rift thermal subsidence in the Skole Basin,
which was a part of the external basins of the Outer Car-
pathian domain (Książkiewicz 1962; Oszczypko 2004),
formed along the European margin in Late Jurassic—Early
Cretaceous times (Oszczypko 2006).
The younger succession (Cenomanian in age) contains a
series of deep-water hemipelagic non-calcareous shales with
calcareous (biogenic) and siliciclastic turbidites. These have
been determined as the Barnasiówka Radiolarian Shale For-
mation (BRSF – Bąk et al. 2001, 2007b,c – Fig. 2). Bio-
genic-rich-turbidites precede the laminated organic-rich
shales and mudstones, which were deposited in the latest
Cenomanian in response to progressive eustatic sea-level
rise and expansion of the oxygen minimum zone in the Outer
Carpathian basins (Bąk K. 2006, 2007a—c). These organic-
rich facies record an oceanic anoxic event (OAE-2), docu-
mented by carbon isotope data (Bąk K. 2007b). Such facies
also occur in other Outer Carpathian basins in the same
stratigraphic position representing a Bonarelli-equivalent ho-
rizon (cf. Bąk K. 2007d; Bąk M. 2011).
The OAE-2 sediments are replaced in the Skole Nappe by
a ferro-manganese carbonate layer. This layer is a chronoho-
rizon in the Outer Carpathian sediments corresponding to the
uppermost Cenomanian—lowermost Turonian (Bąk K. 2007d).
Its occurrence was related to the extremely low sedimenta-
tion rate in the basin and an increase in deep-water circula-
tion, causing basin oxygenation. This layer forms the base of
red non-calcareous shales of the Turonian age (Variegated
shales – Fig. 2), which have been deposited mostly under
well-oxygenated conditions and contain numerous biogenic
particles (Bąk K. 2006, 2007a—c; Okoński et al. 2014).
The above-mentioned Cenomanian succession, classified
as the BRSF, reflects the diverse environmental conditions
in the Skole Basin, recorded by various facies. The present
paper deals with the reconstruction of environmental condi-
tions during the period preceding OAE-2, recorded as the
Environmental conditions in a Carpathian deep sea basin
during the period preceding Oceanic Anoxic Event 2 – a case
study from the Skole Nappe
KRZYSZTOF BĄK
1
, MARTA BĄK
2
, ZBIGNIEW GÓRNY
3
and ANNA WOLSKA
2
1
Institute of Geography, Pedagogical University of Cracow, Podchorążych 2, 30-084 Kraków, Poland; kbak@up.krakow.pl
2
Faculty of Geology, Geophysics and Environmental Protection, AGH University of Science and Technology, Mickiewicza 30,
30-059 Kraków, Poland; martabak@agh.edu.pl; a.wolska@gmail.com
3
Institute of Geological Sciences, Jagiellonian University, Oleandry 2a, 30-063 Kraków, Poland;
zbigniew.gorny@uj.edu.pl
(Manuscript received March 13, 2014; accepted in revised form October 7, 2014)
Abstract: Hemipelagic green clayey shales and thin muddy turbidites accumulated in a deep sea environment below the
CCD in the Skole Basin, a part of the Outer Carpathian realm, during the Middle Cenomanian. The hemipelagites
contain numerous radiolarians, associated with deep-water agglutinated foraminifera. These sediments accumulated
under mesotrophic conditions with limited oxygen concentration. Short-term periodic anoxia also occurred during that
time. Muddy turbidity currents caused deposition of siliciclastic and biogenic material, including calcareous foramini-
fers and numerous sponge spicules. The preservation and diversity of the spicules suggests that they originate from
disarticulation of moderately diversified sponge assemblages, which lived predominantly in the neritic-bathyal zone.
Analyses of radiolarian ecological groups and pellets reflect the water column properties during the sedimentation of
green shales. At that time, surface and also intermediate waters were oxygenated enough and sufficiently rich in nutri-
ents to enable plankton production. Numerous, uncompacted pellets with nearly pristine radiolarian skeletons inside
show that pelletization was the main factor of radiolarian flux into the deep basin floor. Partly dissolved skeletons
indicate that waters in the Skole Basin were undersaturated in relation to silica content. Oxygen content might have been
depleted in the deeper part of the water column causing periodic anoxic conditions which prevent rapid bacterial degra-
dation of the pellets during their fall to the sea floor.
Key words: Cenomanian Upper Cretaceous, Polish Outer Carpathians Skole Nappe, environment, Radiolaria,
Foraminifera, sponge spicules, pellets.
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Fig. 1. Location of the study area. A – Outer Carpathians against the background of a simplified geological map of the Alpine orogens and
their foreland: I.C. – Inner Carpathians, C.F. – Carpathian Foredeep, PKB – Pieniny Klippen Belt, TESZ Zone – Trans-European Su-
ture Zone; B, C – Location of the study area in the Polish part of the Carpathians (B), with sketch topographic map of the surroundings of
Rybotycze village Przemyśl Foothills (C – after Bryndal 2011); D, E – Geological sketch map of the Trójca creek near the Kanasin Hill
(D – after Gucik et al. 1991) with location of the studied section and outcrops (E).
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Fig. 2. Lithostratigraphy of the Lower mid-Cretaceous deposits in the Skole Nappe, Polish Outer Carpathians (after Koszarski & Ślączka
1973; Kotlarczyk 1978; Gucik 1987; Gucik et al. 1991; Bąk 2007a,b).
Fig. 3. Lithological log of the Trójca section (Skole Nappe, Polish Outer Carpathians) plotted against radiolarian composition foraminiferal
datum events. Number of specimens: r (rare) – 1—5, f (frequent) – 6—10, c (common) – 11—20, a (abundant) – more than 20.
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green radiolarian shales with muddy turbidites. Here, we
document the micropaleontological record and discuss the
detected paleoenvironmental features of the Skole Basin.
Geological setting
The studied section is located in the inner part of the Skole
Nappe (Poland), within one of the tectonic scales, on both
banks of the Trójca creek (Przemyśl Foothills), near Rybotycze
village, about 30 km south of Przemyśl (Fig. 1B—E). In this
area, the outcrops of the lower part of the BRSF are limited to
several sections, 0.5—4.5 m thick. Two of them (Fig. 1E) have
been studied and the results are presented in this paper. The
contact between the BRSF and the underlying Spas Shales is
tectonic at this locality. The upper and middle parts of the
BRSF containing the organic-rich sediments of OAE-2
(Bonarelli-equivalent level – Fig. 2) and the Turonian red
non-calcareous shales overlying the BRSF are not exposed
here. The BRSF is in tectonic contact with the Turonian sili-
ceous marls here.
Material and methods
A total of 14 samples were collected from the Trójca com-
posite section, with an average sample interval of 30 cm
(Fig. 3). Microfossils were extracted by repeated heating and
drying of rock samples in a sodium carbonate solution. Resi-
dues were dried, washed through sieves with mesh in diame-
ters of 63 µm. Foraminiferal and radiolarian specimens and
sponge spicules were manually picked from the fraction
0.063—1.5 mm. Microfacies and pellet analyses were carried
out in thin sections.
The microfossil slides and the residual rock samples are
housed in the Department of Geology and Geotourism, Fac-
ulty of Geology, Geosciences and Environmental Protection,
AGH University of Science and Technology (collection of
Marta Bąk).
Results
The studied section contains green non-calcareous clayey
shales, a few black clayey shale layers (several millimeters
thick) which are partly intercalated with green and grey, thin,
muddy turbidites (up to 5 cm thick), which contain siliciclas-
tic and calcareous (biogenic) particles. Among the siliciclastic
material, silt-sized quartz grains dominate, and are associated
with rare micas (Fig. 4J,K), glauconite (Fig. 4M,N) and Fe-Mn
oxides. Redeposited in turbidity currents biogenic particles in-
clude siliceous sponge spicules, calcareous benthic and plank-
tonic foraminifers, and fragmented otoliths (Fig. 4C,D,F,G).
Biogenic material from non-calcareous hemipelagic clayey
shale consists mainly of radiolarian skeletons (Fig. 3) and
agglutinated foraminiferal tests. Fish teeth (Fig. 4A,B) were
also found sporadically.
Radiolarian assemblages
Radiolaria occur in most of the studied samples of the
Trójca section. They are frequent (Fig. 3) but poorly to mod-
erately preserved. Most of the radiolarian skeletons are re-
crystallized or replaced by pyrite and Fe-oxides, resulting in
destruction of external and internal wall structures. With
such poor preservation, only 20 % of the skeletons were rec-
ognized and classified. Identifiable forms were found in
samples Ryb-1, Ryb-3 and Ryb-9 (Fig. 5). As a general ten-
dency, green hemipelagic shales contain higher numbers of
better preserved radiolarians, while in dark-grey and black
shales, the radiolarians are usually present as pyritized
moulds (Fig. 4I).
Eight radiolarian families, nine genera and twelve species
have been recognized in the studied material, according to
Fig. 4. Organic and mineral components from lower part of the Barnsiówka Radiolarian Shale Formation in the Trójca section (Skole
Nappe, Polish Outer Carpathians). A, B – fish teeth (A – Ryb-10), B – Ryb-1); C, D, F – otoliths (Ryb-1); E – pyritized foraminiferal
tube (Ryb-2); G, H – otoliths (Ryb-1); I – Pyritized skeletons of radiolarians; J – Muscovite grains (Ryb-1); K – Biotite grain (Ryb-2);
L – ?Magnetite grain (Ryb-1); M, N – Glauconite grains (Ryb-6).
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Fig. 5. Radiolarians from lower part of the Barnsiówka Radiolarian Shale Formation in the Trójca section (Skole Nappe, Polish Outer Car-
pathians). A, B – Praeconocaryomma lipmanae Pessagno (Ryb-3); C, D – Gongylothorax siphonofer Dumitrică (Ryb-9); E – Dactylio-
sphaera maxima (Pessagno) (Ryb-9); F—H – Holocryptocanium barbui Dumitrică (Ryb-9), specimens represent different stages of
preservation; I – Secondary infield moulds after Holocryptocanium barbui Dumitrică (Ryb-6); J—L – Holocryptocanium tuberculatum
Dumitrică (Ryb-9); M, N – Pseudoeucyrtis spinosa (Squinabol) (Ryb-9); O – Squinabollum fossile (Squinabol) (Ryb-9); S – Xitus
mclaughlini Pessagno (Ryb-9); T, X – Stichomitra communis Squinabol (Ryb-9); P—R – Thanarla veneta (Squinabol) (Ryb-9);
U, V – Pseudodictyomitra pseudomacrocephala (Squinabol) (Ryb-9); W – Xitus spicularius (Aliev) (Ryb-9); Y – Stichomitra stocki
(Campbell & Clark) (Ryb-9).
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radiolarian classification proposed by De Wever et al. (2001)
and adopted to Carpathian settings by Bąk M. (2011). In the
whole section, cryptothoracic and cryptocephalic nasselari-
ans are the main components of radiolarian assemblages.
The species from the family Williriedellidae prevail, with
most common Holocryptocanium barbui Dumitrică –
(Fig. 5F—I), which is a dominate taxon in the mid- to late
Cenomanian in Western Tethyan settings (Bąk M. 2011), as-
sociated with specimens of Holocryptocanium tuberculatum
Dumitrică – (Fig. 5J—L). These two species may consist
even 70—100 % of the whole radiolarian assemblage. Other
nassellarian species belong to families such as: Xitidae
(Xitus spicularius (Aliev) – (Fig. 5W), Xitus mclaughlini
(Pessagno) – Fig. 5S), Eucyrtidiidae (Stichomitra stocki
(Campbell & Clark) – Fig. 5Y), Stichomitra communis
Squinabol – (Fig. 5T,X), Pseudoeucyrtis spinosa (Squina-
bol) – Fig. 5M,N), Syringocapsidae (Squinabollum fossile
(Squinabol) – Fig. 5O), Pseudodictyomitridae (Pseudodic-
tyomitra pseudomacrocephala (Squinabol) – Fig. 5U,V),
Archaeodictyomitridae (Thanarla veneta (Squinabol) –
Fig. 5P—R) and, Sethocapsidae (Gongylothorax siphonofer
Dumitrică – Fig. 5C,D).
Spumellarians are less common and less diversified. Spe-
cies recognized in the assemblages belong to two families:
Conocaryommidae (Praeconocaryomma lipmanae Pessagno
– Fig. 5A,B) and Dactyliosphaeridae (Dactyliosphaera
maxima (Pessagno) – Fig. 5E).
Foraminiferal assemblages
The studied section is dominated by deep-water aggluti-
nated foraminifera (DWAF – Table 1), moderately diversi-
fied. The Fischer alpha index ranges between 2.2 and 7.7
(calculated using the PAST software version 3.01; Hammer
Table 1: Foraminifera from the Middle Cenomanian sediments in the Trójca section, Skole Nappe, Outer Carpathians. Numbers of deter-
mined specimens are indicated.
Ry
b-14
Ry
b-12
Ry
b-11
Ry
b-10
Ry
b-8
Ry
b-7
Ry
b-6
Ry
b-5
Ry
b-4
Ry
b-3
Ry
b-2
Ry
b-1
Agglutinated
Ammodiscus cretaceous
(Reuss)
6 1
3 2 . . . 3 . . . .
Ammodiscus sp.
1
. . 2 . . 6
. . 2
. 1
Bulbobaculites problematicus
(Neagu)
17 1 . . 35 . 2 17 . . . 2
Caudammina ovula (Grzybowski)
1 2 . . 1 . . 1 1 . . .
Gerochammina stanislawi
Neagu
1 1 1 . 1 . 2 1 . . . 4
Gerochammina lenis
(Grzybowski)
11 2 6 . 9 . 14
11 1 2 . 2
Gerochammina obesa
Neagu
4 3 2 . 4 . 3 5 1 3 . .
Glomospira irregularis (Grzybowski)
1
.
.
1
1
.
2
4
.
.
.
.
Haplophragmoides sp.
. . . . . . . . . . . 1
Hyperammina sp.
1 1 . . . . . . 1 . . .
Psammosphaera sp.
. . 1 . 1
1 . . . . . .
Pseudonodosinella parvula
(Huss)
. . . . . . 2 . . . . .
Pseudonodosinella troyeri (Tappan)
15 6 4 . 29 . 50 13 . . . 1
Recurvoides contortus
Erland
. . . . 2 . . . . . . .
Recurvoides imperfectus
(Hanzlikova)
. . 2 . . . . . . . . .
Recurvoides sp.
15
21
5
9
11
.
8
20
32
12
.
5
Reophax sp.
. . . 1 . . . . . . . .
Repmanina charoides (Jones & Parker)
1
1
1
.
11
.
6
1
.
.
.
2
Rhabdammina sp.
. . . . . . . 1 1 1 . 2
Rhizammina sp.
2 2 1 1 4 . 3 6 . 3 . .
Rothina silesica
. 1 . . . . 2 . . . . .
Saccammina grzybowskii (Schubert)
1 . . 1 . . . . . . . .
Saccammina placenta
(Grzybowski)
2 . . . . 1 . 1 . . . 1
Thalm. meandertornata Neagu & Tocorjescu
5
4
2
4
6
.
17
9
.
.
.
.
Trochammina sp.
12 4 1 5 8 . 10
20
14 . . 5
Calcareous benthic
Berthelina baltica
Brotzen
. . . . . . . . . . 2 5
Berthelina cenomanica
(Brotzen)
. . . . . . . . . . 1 4
Globulina Prisca
Reuss
. . . . . . . . . . . 1
Pleurostomella sp.
. . . . . . . . . . 1 1
Valvulineria lenticularia
(Reuss)
. . . . . . . . . . 2 9
Planktonic
Hedbergella delrioensis
Casey
. . . . . . . . . . 85
97
Hedbergella planispira
(Tappan)
. . . . . . . . . . 6 3
Globigerinelloides ultramicra Subbotina
. . . . . . . . . . 7
12
Praeglobotruncana cf. delrioensis Plummer
. . . . . . . . . . . 2
Rotalipora (Th.) cf. appenninica
Renz
. . . . . . . . . . . 2
Rotalipora (Th.) sp.
. . . . . . . . . . . 2
Whiteinella archaeocretacea
Pessagno
. . . . . . . . . . 3 .
Whiteinella baltica Douglas & Rankin
.
.
.
.
.
.
.
.
.
.
2
.
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Fig. 6. Agglutinated foraminifers from lower part of the Barnasiówka Radiolarian Shale Formation in the Trójca section (Skole Nappe, Polish
Outer Carpathians). A – Rhizammina sp. (Ryb-5); B – Psammosiphonella discreta (Brady) (Ryb-1); C – Kalamopsis grzybowskii
(Dylążanka) (Ryb-12); D – Ammodiscus cretaceous (Reuss) (Ryb-11); E – Caudammina ovula (Grzybowski) (Ryb-1); F – Repmanina
charoides (Jones & Parker) (Ryb-8); G – Glomospira irregularis (Grzybowski) (Ryb-8); H – Saccammina placenta (Grzybowski) (Ryb-1);
I – Saccammina grzybowskii (Schubert) (Ryb-10); J, K – Pseudonodosinella troyeri (Tappan) (Ryb-6); L, M – Bulbobaculites prob-
lematicus (Neagu) (Ryb-6); N, O – Haplophragmoides kirki Wickenden (Ryb-6); P – Trochammina sp.: A – (Ryb-14); Q – Trochammina
sp.: B – (Ryb-5); R, S – Thalmannammina meandertornata Neagu & Tocorjescu (Ryb-5); T – Recurvoides sp. (Ryb-10); U – Gerocham-
mina cf. stanislawi Neagu (Ryb-12); V—X – Gerochammina lenis (Grzybowski) (V – Ryb-6, W – Ryb-8, X – Ryb-11); Y – Spiroplecti-
nella dentata (Alth) (Ryb-1).
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Fig. 7. Planktonic foraminifers from lower part of the Barnasiówka Radiolarian Shale Formation in the Trójca section (Skole Nappe, Polish
Outer Carpathians). A—C – Globigerinelloides ultramicra Subbotina (Ryb-1); D, E – Hedbergella delrioensis Carsey (Ryb-2); F, G – Ro-
talipora sp. (Ryb-1); H, I – Whiteinella baltica Douglas & Rankin (Ryb-2); J, K – Rotalipora (Th) cf. appenninica Renz (Ryb-1);
L, M – Praeglobotruncana cf. delrioensis (Plummer) (Ryb-1); N—P – Whiteinella archaeocretacea Pessagno (Ryb-2).
et al. 2001 – Fig. 3). Most of them represent flysch-type mi-
crofauna, known from Cretaceous and Paleogene bathyal—
abyssal turbiditic environments (e.g. Morgiel & Olszewska
1982; Kuhnt & Kaminski 1989; Kuhnt et al. 1990, 1992;
Bąk 2004; Kaminski & Gradstein 2005). Tubular specimens
belonging to a few genera (Rhizammina – Fig. 6A), Rhab-
dammina, Psammosiphonella – (Fig. 6B) and Kalamop-
sis – (Fig. 6C) are rare. The most frequent among them are
tiny rhizamminids (Table 1). The most abundant agglutinated
foraminifera, each with frequency exceeding 20 %, belong to
Bulbobaculites problematicus (Neagu) – (Fig. 6L,M),
Pseudonodosinella troyeri (Tappan) – (Fig. 6J,K) and gero-
chamminids – (Fig. 6U—X). Recurvoides – (Fig. 6T) and
Thalmannammina – (Fig. 6R,S) are also abundant through-
out the studied sections. However, their frequency is difficult
to measure, because many of them are not transparent and are
partly filled with pyrite. Some samples also contain numerous
completely pyritized large moulds of Recurvoides (Thalman-
nammina)-type shapes. Less frequent in the studied sections
are Ammodiscus – (Fig. 6D), Saccammina – (Fig. 6H,I),
Caudammina – (Fig. 6E), Repmanina – (Fig. 6F), Glomo-
spira – (Fig. 6G), Haplophragmoides – (Fig. 6N,O), and
Spiroplectinella – (Fig. 6Y). The total frequency of these
taxa is around 10 % in individual samples. Similarly, small
trochamminids (Fig. 6P,Q) comprise nearly 10 % of the total
number of specimens in the samples.
Calcareous benthic foraminifera have been recorded in
only two samples occurring together with sponge spicules
and planktonic foraminifera (Table 1). This suggests that
they constitute redeposited assemblages, transported by tur-
bidity currents. Only five species have been recognized that
belong to Valvulineria lenticula (Reuss), Berthelina ceno-
manica (Brotzen), Berthelina baltica Brotzen, Globulina
prisca Reuss and Pleurostomella sp. All these taxa are well
known from the Upper Cretaceous epicontinental seas that
surrounded the northern basins of the Western Tethys (e.g.
Gawor-Biedowa 1972; Heller 1975; Pożaryska & Wytwicka
1983; Peryt 1983; Hradecka 1993; Dubicka & Peryt 2012).
Numerous planktonic foraminifera are found in the topmost
part of the studied section (samples Ryb-1 and Ryb-2 – Fig. 3)
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with numerous forms belonging to Globigerinelloides ultra-
micra Subbotina – (Fig. 7A—C) and Hedbergella delrioensis
Carsey – (Fig. 7D,E). Their dimensions do not exceed
150 µm – most of them are 80—120 µm in diameter. More-
over, rare and small (not longer than 200 µm) specimens of
Whiteinella baltica Douglas & Rankin – (Fig. 7H,I),
Whiteinella archaeocretacea Pessagno – (Fig. 7N—P),
Praeglobotruncana delrioensis Plummer – (Fig. 7L,M) and
Rotalipora (Th.) appenninica Renz – (Fig. 7J,K) have been
recorded from these sediments.
Sponge spicules
Loose sponge spicules have been found in six samples
(Fig. 3) but the most numerous and diversified spicules oc-
cur in a turbidite siltstone—claystone layer (Ryb-9). All of
them belong to sponges classified as Demospongiae
(Fig. 8G—Z) and Hexactinellidae (Fig. 8A—F). Practically all
the spicules are broken and strongly disintegrated. The spi-
cules represent choanosomal and dermal assemblages which
derived from various sponge species (Fig. 8). Spicules of
Demospongiae are the most common. They consist of 64 %
of the whole assemblages and prevail over the spicules clas-
sified to Hexactinellidae (21 %). Various types of oxea,
which may belong to both sponge groups, consist of 15 % of
the spicule assemblages.
Hexactinellidae spicules are represented only by hexac-
tines and pentactines (Fig. 8A—F). The hexactines are most
probably choanosomal spicules. Some fused spines present
in the studied material suggest that they were a part of solid
skeletons of Hexactinosa (Schrammen).
Demospongiae are represented mostly as loose and usually
strongly articulated tetraxial and monaxial spicules. The
most common spicules belong to the Lithistida. These are a
different type of desmas (Fig. 8G—O), which were a part of
choanosomal skeletons, as well as different types of ectoso-
mal phyllotriaenes (Fig. 8U—V). Tetraclone desmas and
phyllotriaenes are characteristic of lithistid sponges of the
family Theonellidae Lendenfeld (Pisera & Levi 2002a,b).
The most common choanosomal desmas are rhizoclones
(Fig. 8G—K). Fossil rhizoclones are usually assigned to the
suborder Rhizomorina Zittel (Pisera 1997, 2002). The pres-
ence of various types of triaenes with long rhabdomes may
indicate the presence of species from the group of Astro-
phorida Sollas (Fig. 8R—T).
In addition to macroscleres, the microscleres are also
present in the material studied, represented by sterrasters
(Fig. 8Q). They are undoubtedly derived from species of the
family Geodiidae. A more precise assignment is not possi-
ble, because the shape and sculpture of singular forms have
no taxonomic value (Uriz 2002). Some of the oxeas found in
the material studied may also belong to geodiid sponges.
Pellets
Pellets are a common component of the green shales suc-
cession in the BRSF. Analysis of thin-sections shows that
pellets are one of the main constituents of silt and clay frac-
tions (Fig. 9). They vary in size and shape, which suggests
their production was caused by both micro- and mesozoo-
plankton. Most common are elliptical forms with the longer
axis up to 300 µm. (Fig. 9A). Semi-spherical pellets have
diameters up to 500 µm. Longitudinal forms extend along
the longer axis over 1 mm. Pellets contain large amounts of
undigested or partially digested material, which consists of
complete or crushed radiolarian skeletons (Fig. 9A—D), as
well as planktonic foraminiferal tests (Fig. 9B). Some pellets
contain homogenous material (Fig. 9A) which might have
been several times digested by different consumers during
their journeys through the water column.
Radiolarian biostratigraphy
There are no precise radiolarian age markers in the assem-
blage investigated, however, the radiolarian species occur-
ring in the studied section, and the general quantitative
composition of radiolarian assemblages, allow us to make
some observations about the stratigraphy. The general pic-
ture of nassellarian distribution in the Western Tethys is one
of high abundance in the middle and upper Cenomanian de-
posits below the onset of OAE-2 (Bąk M. 2011). This feature
of radiolarian assemblages has been recognized in the Um-
bria-Marche and the Carpathian basins. In the Outer Car-
pathian sediments, the most abundant are representatives of
the family Williriedellidae (e.g. Dumitrică 1975; Bąk M.
2000, 2004, 2011). The same trends have been observed here
in the sediments of the Skole Nappe.
The co-occurrence of two abundant radiolarian species –
Holocryptocanium barbui Dumitrică and H. tuberculatum
Dumitrică with the presence of Gongylothorax siphonofer
Dumitrică indicate a middle to late Cenomanian age (Fig. 3),
based on correlation with the H. barbui—H. tuberculatum ra-
diolarian assemblage reported by Dumitrică (1975) from the
Romanian Carpathians and with comparison to previous data
obtained from the Polish Outer Carpathians and the Pieniny
Klippen Belt (Bąk M. 1993a,b, 1996a,b, 1999, 2000, 2004;
Bąk M. & Bąk K. 1999).
On the other side, the studied sediments do not contain
radiolarian species such as Alievium superbum (Squinabol),
Crucella cachensis Pessagno, Praeconocaryomma universa
Pessagno, Dictyomitra napaensis Pessagno, Cavaspongia
antelopensis Pessagno, Patellula ecliptica O’Dogherty and P.
andrusovi Ožvoldová, which are common in the uppermost
Cenomanian of the Outer and Inner Carpathian sections (e.g.
Górka 1995; Bąk M. 1996a,b, 2000, 2004, 2011; Bąk K. &
Bąk M. 2013). Fortunately, Cenomanian species as Tanarla
veneta (Squinabol) and Xitus mclaughlini (Pessagno), which
finally became extinct at the top of the uppermost Cenoma-
nian organic-rich facies of OAE-2, are present here (Fig. 3).
To refine the age assignment, an important observation is
that these sediments lack a very characteristic radiolarian
zonal marker – Hemicryptocapsa prepolyhedra Dumitrică
– which commonly occurs in the Carpathians (Bąk M.
1996b, 2000, 2004, 2011). The first appearance of this spe-
cies defines the lower boundary of the Hemicryptocapsa pre-
polyhedra Interval Radiolarian Zone in the Western Tethyan
sediments (Bąk M. 1999, 2011). It has been dated in the Polish
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Fig. 8. Sponge spicules from lower part of the Barnasiówka Radiolarian Shale Formation in the Trójca section (Skole Nappe, Polish Outer
Carpathians). A—F – Hexactines of Hexactinosa (Ryb-9); G—K – Rhizoclone desmas of Lithistida (Ryb-9); M—O – Tetraclone desmas
of Lithistida (Ryb-9); P – Strongyloxeas of “soft” demosponge (Ryb-9); Q – Sterrasters of geodiidid (Astrophorida) (Ryb-9);
R—T – Plagiodichotriaenes of “soft” Demospongae, most probably Astrophorida; U—V – Ectosomal phyllotriaenes of theonellid (Ryb-9);
W—X – Choanosomal calthrops of Astrophorida (Ryb-9); Y—Z – Criccalthrops (Ryb-9).
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Outer Carpathians to 1.0 Ma before the onset of OAE-2 (Bąk
M. 2011). The Middle/Upper Cenomanian boundary lies
within this radiolarian zone (Bąk M. 2011).
Another important species for stratigraphy is Stichomitra
stocki (Campbell & Clark), the first appearance of which is
known in the Carpathian basins earlier than H. prepolyhedra
but after the Mid-Cenomanian Event (MCE sensu Jenkyns et
al. 1994; Jarvis et al. 2006 – see discussion in Bąk M. 2011).
To summarize, all the presented data indicate that sedi-
mentation of the studied sediments began during the middle
Cenomanian (after the Mid-Cenomanian Event) and finished
earlier than 1.0 Ma before the onset of Oceanic Anoxic
Event 2, namely near the middle—upper Cenomanian bound-
ary taking into account the chronostratigraphy by Ogg &
Hinnov (2012).
Foraminiferal biostratigraphy
Planktonic foraminiferal assemblages are present only in
redeposited sediments of the topmost part of the studied sec-
tions. The Cenomanian rotaliporid index species are absent
in these assemblages. Relative age interpretation can be
made on the basis of sporadic forms belonging to the
whiteinellids and rotaliporids (Fig. 3). The FOs of whiteinel-
lids is noted from the Tethyan realm from the middle Cen-
omanian (Robaszynski & Caron 1995). On the other hand,
the last appearance of rotaliporids was diachronous in the
Tethys, related to the oxygen content in the water column. It
took place near the base of OAE-2, corresponding to the lat-
est Cenomanian.
The agglutinated assemblages from the whole studied suc-
cession contain numerous specimens of Bulbobaculites
problematicus (Neagu) – (Fig. 3), an index species in
benthic zonations of the Carpathian basins (e.g. Geroch &
Nowak 1984; Olszewska 1997; Bąk K. & Bąk M. 2013). Its
FO was precisely documented in the Pieniny Klippen Belt,
where it corresponds to the Rotalipora reicheli Zone (middle
Cenomanian) – (Bąk K. et al. 1995; Bąk K. 1998, 2000).
In conclusion, the datum events of foraminiferal species
show that the studied sediments represent the interval after
the first appearance of whiteinellids and B. problematicus
Fig. 9. Microfacies from black organic-rich mudstone layer of the Barnasiówka Radiolarian Shale Formation in the Trójca section (Skole
Nappe, Polish Outer Carpathians). A – Bioturbated organic-rich shale with different type of pellets. Elliptical forms (ep) prevail over lon-
gitudinal (lp). Small, rounded radiolarians (r), (probably williriedellids) are incorporated into the pellets or they are attached to pellet sur-
face; B – Flattened pellets with sharp boundaries in organic-rich shale. Pellets contain different organic particles such as fish bones (f),
agglutinated foraminifera (af) and radiolarians (r); C—D – Close up of pellet with microcrystal of quartz filled in moulds after complete (r)
and/or broken (rb) radiolarian skeletons. Most of the skeletons are spherical, resembling williriedellids.
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(Neagu) (Middle Cenomanian) and before the final extinc-
tion of the rotaliporids (uppermost Cenomanian). These data
confirm the radiolarian stratigraphy in the sense of determin-
ing the lower boundary of the studied succession. The upper
biostratigraphical limit is here less precise than that based on
the radiolarian biostratigraphy.
Environmental conditions at the floor
The lack of calcareous foraminifers in the hemipelagic lay-
ers indicates that the sedimentation of the deposits studied in
the Skole Basin took place below the calcium compensation
depth. The green claystone layers contain numerous radiolari-
ans with siliceous- and organic-walled benthic (agglutinated)
foraminifers typical of the Cretaceous bathyal and abyssal en-
vironments. Planktonic and calcareous benthic foraminifera
are redeposited and occur only in clay- and silt-sized turbid-
ites, where they are associated with siliceous sponge spicules.
The characteristic feature of these sediments is their green
colour (from pale-green in hemipelagic layers to dark-green
in turbiditic layers), which dominate among the clayey and
muddy shales, excluding a few very thin dark-grey and black
layers. The dominance of green colouration is characteristic
of the Upper Albian—Cenomanian deep-water hemipelagic
sediments in all the Outer Carpathian tectonic and facies
zones (e.g. Książkiewicz 1962). These sediments significantly
differ in colour from the Lower Cretaceous hemipelagic strata
and the latest Cenomanian OAE-2 hemipelagic sediments,
which possess dark-grey and black colouration. Because of
the lack of chemical studies of these sediments, the interpre-
tation of this fact is not discussed here. However, from the
general point of view, using the published micropaleontolog-
ical data related to the increase in diversity of deep-water
benthic foraminiferal assemblages from the Aptian to Cen-
omanian in the Carpathian sediments (cf. Geroch & Nowak
1984; Kuhnt et al. 1992; Olszewska & Malata 2006), the
change of sediment colour from black to green would be re-
lated to the increase in the oxygen content of deep water and
in the uppermost part of the sediment column in relation to
the pre-Cenomanian time period.
Such a conclusion also derives from features of the studied
benthic microfossils. The DWAF assemblages are low to
moderately diversified. The Fisher alpha index, as a measure
of species diversity ranges from 2.2 to 7.7. These values of
diversity are comparable to the values of the Early Creta-
ceous assemblages from deep-water oxygen-depleted envi-
ronments of the Tethyan realm (e.g. Geroch & Koszarski
1988; Decker & Rögl 1988; Kuhnt 1995) and significantly
lower than the values in Late Cretaceous (Turonian—Maas-
trichtian) assemblages from oxygenated deep sea basins of
the same area (e.g. Kuhnt & Kaminski 1989; Bąk K. 2000;
Kaminski et al. 2008; Kaminski et al. 2011).
Environmental interpretation of the sea floor is also possi-
ble using paleoecological interpretation of benthic foramin-
ifera by means of morphogroup analysis. The morphogroup
concept refers to grouping of similar shapes and growth pat-
terns of foraminiferal tests using the idea that species with
the same test shape have the same preferred life habitats,
which can be related to feeding strategies, and that morpho-
groups distribution and abundance can reflect changes in se-
lected environmental parameters (e.g. Jones & Charnock
1985; Nagy 1992; Nagy et al. 1995; Kaminski et al. 1995;
Peryt et al. 1997; Preece et al. 1999; Van Den Akker et al.
2000; Peryt et al. 2004; Bąk K. 2004; Kaminski & Gradstein
2005; Kender et al. 2008a,b; Cetean et al. 2011; Murray et
al. 2011; Mancin et al. 2013).
Fig. 10. Percentage content of foraminiferal genera in lower part of
the Barnasiówka Radiolarian Shale Formation in the Trójca section
(Skole Nappe, Polish Outer Carpathians). Tubular taxa have not been
included here due to their uncertain number, related to fragmentation
of the tests during fossilization and washing processes. Morphogroup
numbers (M2a to M4b) after Kaminski & Gradstein (2005).
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The assemblages studied are dominated by elongate subcy-
lindrical and elongate tapered forms including Pseudono-
dosinella, Gerochammina, and Bulbobaculites. They comprise
nearly 60 % of the total number of foraminiferal assemblages
(Fig. 10). Using the definition of agglutinated foraminiferal
morphogroups, with interpreted life habitat and feeding
strategy, presented by Kaminski & Gradstein (2005), these
forms, representing morphogroups M4a and M4b, are inter-
preted as deep infauna living as active deposit feeders. The
deep infaunal forms are associated here with surficial epifau-
nal taxa, represented by rounded trochospiral, streptospiral,
and planoconvex trochospiral forms (morphogroup M2b
sensu Kaminski & Gradstein 2005) including Recurvoides,
Thalmannammina and Trochammina. This morphogroup
consists of nearly 30 % of the total number of foraminiferal
tests (Fig. 10). The tubular taxa (mostly tiny rhizamminids)
which are suspension feeders are rare in the sediments studied
(Table 1), reaching a few percent in total numbers of fora-
minifers. Such a composition of the morphogroups points to
distinct dominance of deep infaunal taxa, however, without
conspicuous domination by particular species.
As observed in modern deep-water environments (e.g. Joris-
sen et al. 1995; Kaminski et al. 1995; Gooday & Rathburn
1999; De Rijk et al. 2000; Gooday et al. 2000; Wollenburg
& Kuhnt 2000; Szarek et al. 2007; Murray et al. 2011), two
main factors control the structure of benthic foraminiferal as-
semblages: organic carbon flux to the sea floor, and the oxy-
gen concentration in the bottom waters and in the uppermost
part of the sediment. In deep sea basins, water depth is another
factor affecting the benthic foraminiferal assemblages. The
depth of the basin floor influences the reduction flux of or-
ganic matter from surface plankton production, which could
be several times lower if compared with marginal marine set-
tings (cf. Szarek et al. 2007; Murray et al. 2011). On the other
hand, the supply of organic matter can be occasionally en-
hanced in deep sea environments due to terrigenous fluxes,
associated with turbidity currents. Both sources of organic
matter on the deep sea floor of the Skole Basin are interpreted
here, based on observation of microfacies (Fig. 9). From one
side, green clayey shales contain numerous pellets, which
could be one of the main sources of organic matter to the sea
floor. At the same time, numerous flakes of organic matter
are dispersed in muddy and silty turbiditic material (Fig. 9D).
The occurrence of relatively numerous flakes of organic
matter in the green clayey shales points to another conclu-
sion, related to the oxygen content at the sediment—water in-
terface. The low oxygen concentration that is here suggested
for the studied sediments, could favour the preservation of
organic matter. From another point of view, dysoxic condi-
tions could be the main factor which limited the number of
epifaunal forms within the foraminiferal assemblages thereby
providing an opportunity for exploitation of the sea floor by
deep infauna, composed of low-oxygen tolerant taxa. Similar
conditions occur recently in abyssal zones of the Sulu Sea, a
semi-enclosed, meso-to-oligotrophic basin in the western
equatorial Pacic, characterized by warm (ca. 10 °C) and oxy-
gen-depleted (dysoxic; <1 ml/l O
2
) deep-waters (Szarek et
al. 2007). In such conditions, foraminiferal assemblages con-
sisted mainly of shallow infaunal agglutinated forms, with
dominant species belonging to Lagenammina difugiformis
(Brady), Ammoscalaria tenuimargo (Brady), Ammobaculites
paradoxus Clark and various Reophax species. A compari-
son of the morphogroup composition from the sediments
studied (characterized by dominance of deep infaunal forms)
with the TROX ecological model by Jorissen et al. (1995)
explaining benthic foraminiferal microhabitat preferences,
also suggests a mesotrophic environment with limited oxygen
concentration for the Skole Basin floor during the prevailing
time periods of the middle Cenomanian. Nevertheless, short-
termed periodic anoxia also occurred during that time, as
documented by the occurrence of several very thin (2—5 mm)
black organic-rich layers.
Concluding, the dysaerobic bottom water conditions with
a moderate rate of organic matter flux from surface plankton
production and from turbidity currents with short-term an-
oxia characterized the deepest part of the Skole Basin during
the Middle Cenomanian.
Source area of sponge spicules from turbidite
layers
Turbidite layers contain a rich assemblage of siliceous
sponge spicules. The assemblage indicates that the sponge
fauna was dominated by lithistid demosponges represented
by Theonellidae and rhizomorinids. Demosponges from
family Geodiidae (Astrophorida) are also common. Hexacti-
nellidae spicules are rare; only spicules derived from order
Hexactinosa were recognized.
Bathymetric reconstructions for the studied sediments,
based on sponges are imprecise because these organisms of-
ten have very wide bathymetric ranges. However, the studied
assemblage is neither characteristic of very shallow nor very
deep marine environments. Modern lithistid sponges prefer a
deep water environment from one hundred to several hun-
dred meters depth (Vacelet 1988; Maldonado 1992; Pisera
1997). Species from the family Geodiidae are known to have
wide bathymetric ranges from intertidal to bathyal depths,
however, they are more specific to the bathyal zone (Uriz
2002). In contrast, theonellids might occur mainly at shal-
low-water depths (Vacelet 1988). The presence of hexacti-
nellid sponges indicate deep environments (Reid 1968)
excluding the submarine caves and fjords where they could
thrive at shallower depths (Vacelet 1988; Vacelet et al. 1994).
Among hexactinellids, species from the order Hexactinosa,
from which spicules are present in the turbiditic layers, are
known to have settled environments deeper than 100 meters,
preferring a stable environment with low water turbulence
(Mehl 1992).
Most of the lithistids and species of the Hexactinosa group
formed rigid skeletons, which could be attached to a hard
substrate. However, some species from the family Geodi-
idae, could have been adapted to a soft substrate (Uriz 2002;
Pisera 2004).
The presented data show that the spicules from the studied
material came from disarticulation of moderately diversified
solid sponge assemblages, which lived mainly in the deeper
parts of the shelves and on the upper parts of the slopes (ner-
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itic—bathyal zones), generally, below the storm wave base
(100 m or more). However, some of them could have origi-
nated from shallow shelves. The poor state of preservation of
spicules and well sorted spicule material may indicate that
spicules were transported over a long distance, including not
only transport by turbidity currents, but also by bottom cur-
rents on the shelves.
Water properties based on radiolarians and pellets
analyses
The majority of radiolarians are indicators of nutrient-rich
surface waters, such as in upwelling areas (Casey 1977; De
Wever et al. 2001). Present day studies in the Equatorial Pa-
cific region show that total radiolarian standing stocks in-
crease in such regions, responding to a general increases in
nutrients, chlorophyll-a, and diatom occurrence during La
Niña periods (Yamashita et al. 2002). Studies of the equato-
rial region, Southern Ocean, and the Namibia upwelling re-
gime show that radiolarians are most abundant in the upper
50—150 m of the water column within the mixed layer, but
also occur below it (Abelmann & Gowing 1996, 1997). In-
tense radiolarian flux subsequently results in the accumula-
tion of a large number of radiolarian individuals in
sediments, which enhances the organic carbon flux and in-
creases primary productivity (Wang et al. 2000; Chen et al.
2003). The lowest abundances occur in nutrient-poor sub-
tropical regions and close to the Subtropical Front (Abel-
mann & Gowing 1996).
Although radiolarian assemblages in the studied deposits
are strongly influenced by sedimentary and diagenetic pro-
cesses, some features of the living assemblages can be recog-
nized. The numerous radiolarians represent two ecological
supergroups, “B” and “E”, distinguished for the Cenoma-
nian—Turonian assemblages in the Tethyan realm (Bąk M.
2011). Forms assembled in supergroup “B”, which are the
most common, have been interpreted as living in the deeper
part of the water column. Among supergroup “B”, most spe-
cies belong to group “B3”, whose dominant taxon – Holo-
cryptocanium barbui Dumitrică – was widely tolerant with
respect to nutrient surplus in the water column, and could
live in the wide vertical range below the mixed surface layer.
Group “B2”, which is represented in the studied material by
Squinabollum fossile (Squinabol), assembled specimens that
lived in waters with an increasing amount of phosphorus,
characteristic for the eutrophic zone. Other species (Xitus
mclaughlini (Pessagno) and Thanarla veneta (Squinabol))
belong to the “B5” group, which comprises forms that lived
in oxygen depleted waters and/or close above the oxic/anoxic
interface. The “B6” group is represented here by Pseudo-
eucyrtis spinosa (Squinabol), which lived below the mixed
layer in waters moderately rich in nutrients.
Radiolarian assemblages that belong to supergroup “E”
are interpreted as an association living in surface waters,
mostly in the mixed layer (Bąk M. 2011). Among these radio-
larian sets, Xitus spicularius (Aliev), Stichomitra communis
Squinabol, and Holocryptocanium tuberculatum Dumitrică
(“E3” group), and Pseudodictyomitra pseudomacrocephala
(Squinabol) (“E4” group) were surface dwellers that lived in
very shallow waters, and possibly tolerated a wide range of
water temperatures and salinity. Species from group “E3”
(Xitus spicularius (Aliev), Stichomitra communis Squinabol,
Holocryptocanium tuberculatum Dumitrică) have been inter-
preted as living also in the surface mixed layer but with in-
creasing phosphorus content. They were more opportunistic
and more widely vertically distributed. These species pos-
sess skeleton shapes predestinated to a bacterivorous type of
feeding (Bąk M. 2011).
The radiolarian ecological groups presented above show
that the surface and intermediate waters were well enough
oxygenated and sufficiently rich in nutrients to enable plank-
ton production, however, oxygen content might have been
depleted in the deeper water column or waters may have
been seasonally anoxic as indicated by the occurrence of
species from group “B5”.
Another indicator of water properties might be pellets,
which occur in hemipelagic clayey shales. These pellets are
homogenous inside or contain undigested or secondary di-
gested radiolarian skeletons and foraminiferal tests. The ra-
diolarian skeletons are present in various types of pellets in
different positions. Usually small, rounded skeletons (most
probably forms belonging to williriedellids) are located in-
side pellets or they are attached to the pellets periphery. This
fact suggests that pellets are the main conveyor of radiolarian
skeletons from the water column into sea-floor sediment. In
this way, pellets could be the main source of siliceous skele-
ton flux from the upper water column, as previously suggested
for the Carpathian deposits (Bąk M. 2011). Thus sediments
enriched in siliceous skeletons might be a function not only
of the proliferation of silica-secreting biota, but also their
consumption by larger zooplankton. Pellets came from un-
known primary radiolarian consumers. Where such pellets
are large (Fig. 9A,C), they might have been derived from the
epipelagic zone and have sunk fast enough to avoid re-pro-
cessing by other zooplankton. Crushed and strongly pro-
cessed skeletons occurring inside pellets might be examples
of re-ingestion by other zooplankton (Fig. 9D).
The studied pellets do not possess an organic membrane,
which usually surrounds their modern counterparts. In this
study, boundaries with surrounded material represent two
types: sharp or with boundaries weakly visible. Sharp
boundaries suggest that pellets might have retained a chiti-
nous membrane much longer, during sinking, than pellets
whose outer boundaries are difficult to determine (Fig. 9A).
Analogous pellets, most probably deriving from copepod
grazing activity, are the main components of the green clay-
stones from the younger part of the BRSF (not studied here),
and green claystones from the Variegated Shale in the Silesian
and Subsilesian units of the Outer Carpathians (Bąk M. 2011).
One of the important factors for the contribution of pellets
to transport of particles is the mineralization of pellet material
during sinking. Non-mineralized pellets can be rapidly de-
graded by bacterial activity on the sea floor (Hansen et al.
1996) and destroyed. This process is much faster at higher
water temperatures and during higher rates of biogenic pellet
accumulation (Hansen et al. 1996). The degradation processes
lower the particulate organic carbon value without changing
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the biogenic silica flux (Dagg et al. 2003), however, released
skeletons are more sensitive to dissolution in water under
saturated with respect to silica. Pellets in the material inves-
tigated possess their original intact and not compacted
shapes. In the case of such pellets, the degradation processes
must be arrested before final bacterial decomposition. Such
preservation of pellets would suggest the presence of water-
column anoxia which prevented secondary digesting and
rapid disintegration by microbial and faunal activity.
Water saturation with respect to silica
The radiolarian content and preservation of skeletons may
approach the saturation of sea water with respect to silica.
Similar processes are observed in modern counterparts,
which are sensitive to dissolution during settling through the
water column and within the bottom sediment (Takahashi &
Honjo 1983) because modern sea water is Si-under saturated
from the surface layer to the bottom. In such conditions, the
pelletization process is very important for the radiolarian
flux and their further preservation within the sediment.
The radiolarians in the hemipelagites of the middle Cen-
omanian sediments of the Skole Unit are characterized by
the dominance of thick-walled, siliceous skeletons, resistant
to dissolution and skeletons replaced by pyrite or ferrous ox-
ides. Most of the radiolarian skeletons that occur in the
whole studied succession are partly dissolved. Moreover, a
part of the planktonic foraminifers together with radiolarians
have been transported in pellets, as observed in thin sections
of the sediment. Complete, undigested pellets contain better
preserved skeletons, while crushed and partly dissolved
radiolarian skeletons are visible in thin sections as surrounded
by the remnants of disintegrated remains of the pellet. This
suggests that more complete and better preserved skeletons
were protected by fecal mass, while partly dissolved skeletons
have been temporary exposed to aggressive waters undersatu-
rated in respect to silica. This means that the number of radio-
larian individuals is a function of production vs. resistance in
the upper part of the Si-undersaturated water column.
Conclusions
Hemipelagic green clayey shales with associated thin
muddy and clayey turbidites, such as the lower part of the
Barnasiówka Radiolarian Shale Formation, were accumulated
in a deep sea environment, below the CCD. The radiolarians
and foraminifers from these sediments show that their sedi-
mentation took place during the middle Cenomanian and
continued at least until the middle—late Cenomanian bound-
ary, namely near 1.0 Ma before the onset of OAE-2. Conse-
quently, these sediments reflect a record of environmental
conditions in the Skole Basin during the period between two
oceanic anoxic events, the Mid-Cenomanian and the latest
Cenomanian (OAE-2).
The taxonomic composition and low to moderate diversity
of benthic foraminifers (deep-water agglutinated foramin-
ifera) from hemipelagic shales suggests mesotrophic condi-
tions with limited oxygen concentration for the Skole Basin
floor during the prevailing time periods of the middle Cen-
omanian. Additionally, short-term periodic anoxia also oc-
curred during that time, as documented by the occurrence of
several very thin black organic-rich layers. Comparison of
the DWAF assemblages, dominated by infaunal taxa, with
their modern counterparts, and using the TROX ecological
model, enabled us to assess the rate of organic matter fluxes
from surface plankton production as moderate, but the flux
was periodically enhanced by turbidity currents.
Muddy turbidity currents transported to the seafloor silici-
clastic and biogenic material, including calcareous foramini-
fers and numerous sponge spicules. The composition of the
spicules, dominated by spicules of demosponges (lithistids),
suggests that they originated from the disarticulation of
moderately diversified solid sponge assemblages, which
lived mainly in the neritic—bathyal zone, but, some of them
could have come from shallower parts of the shelves. Their
poor state of preservation and high rate of disintegration in-
dicate that spicules were transported over a long distance, in-
cluding transport by bottom currents on the shelves.
Analysis of radiolarian assemblages in the studied sedi-
ments, in comparison to ecological groups distinguished for
the Cenomanian—Turonian taxa in the Tethyan realm (Bąk
M. 2011) allowed us to interpret the conditions in the water
column. The investigated taxa live in a surface mixed layer
with increasing phosphorus content and also in intermediate
waters, well-enough oxygenated and sufficiently rich in nu-
trients to enable plankton production. However, the oxygen
content might have been depleted in deeper parts of the wa-
ter column by periodic anoxia, as indicated by the occur-
rence of species that lived in oxygen depleted waters and/or
close above the oxic/anoxic interface.
The studied hemipelagic green shales contain numerous
undigested radiolarian skeletons inside pellets. This fact sug-
gests that pellets are the main conveyor of radiolarian skele-
tons from the water column into the sea-floor sediment. The
occurrence of numerous uncompacted pellets with well-pre-
served radiolarians inside them also indicates water anoxia
which impeded the rapid bacterial degradation of the pellets.
Acknowledgments: This paper was supported by Funds of
the Pedagogical University of Kraków and AGH University of
Science and Technology awarded to K. Bąk (DS-UP-WGB-4n)
and to M. Bąk (DS-AGH WGGiOŚ-KGOiG No.11.11.140.173).
Michael A. Kaminski (King Fahd University of Petroleum and
Minerals, Saudi Arabia), Špela Goričan (Slovenian Academy
of Science and Arts) and Claudia Cetean (Babe -Bolyai Uni-
versity, Romania) are thanked for comments on the manu-
script and improving the English.
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