www.geologicacarpathica.com
GEOLOGICA CARPATHICA
, JUNE 2016, 67, 3, 223–238
doi: 10.1515/geoca-2016-0015
Calcareous nannofossils of the Jurassic/Cretaceous boundary
strata in the Puerto Escaño section (southern Spain)
— biostratigraphy and palaeoecology
ANDREA SVOBODOVÁ
1,2
and MARTIN KOŠŤÁK
2
1
Institute of Geology, The Czech Academy of Sciences, v.v.i., Rozvojová 269, 165 00 Prague 6 - Lysolaje; asvobodova@gli.cas.cz
2
Institute of Geology and Palaeontology, Faculty of Science, Charles University in Prague, Albertov 6, 128 43 Prague 2;
andrea.svobodova@natur.cuni.cz, martin.kostak@natur.cuni.cz
(Manuscript received July 14, 2015; accepted in revised form March 10, 2016)
Abstract: We obtained material from the Puerto Escaño section (southern Spain) to study the Jurassic/Cretaceous
(J/K) boundary interval. The same samples had already been processed for magnetostratigraphic studies and biostrati-
graphic zonation based on calpionellids and ammonites (Pruner et al. 2010), but not for calcareous nannofossils. The aim
of this study was to process the samples using micropalaeontological analysis and to compare and calibrate results for
calcareous nannofossils with existing magnetostratigraphic and other biostratigraphic data. The calcareous nannofossil
assemblage was dominated by the genera Watznaueria, Cyclagelosphaera, Nannoconus, Conusphaera and Polycostella.
Several nannofossil bioevents were recorded on the basis of the distribution of stratigraphically important taxa, including
zonal and subzonal markers. Based on the lowest occurrences (LO) of M. chiastius, N. globulus minor, N. wintereri,
N. steinmanii minor, N. steinmannii steinmannii, N. kamptneri minor and N. kampteri kamptneri, two nannofossil
subzones (NJT 15b, NJT 17a) and two nannofossil zones (NJT 16, NK-1) were recognized. The paper introduces new
palaeoecological data based on geochemical analysis and macrofauna occurrences.
Key words: Jurassic/Cretaceous boundary, southern Spain, Tethys, biostratigraphy, calcareous nannofossils,
palaeoecology.
Introduction
The existence of two different temperate Realms in the
Northern hemisphere (the Tethyan and the Boreal) during the
J/K boundary interval was associated with the occurrence of
different biotic elements in the two Realms due to their spe-
cific climatic and palaeoceanographic conditions (Zakharov
et al. 2014). Also from this point of view, the J/K boundary
is the last System boundary remaining to be defined. For the
clarification and precise determination of the J/K boundary
strata, several markers have been suggested as keys for the
correlation — namely calpionellids, calcareous nannofossils,
magnetostratigraphy (base M18r, M19.1n, M19n.1r), ammo-
nites, palynomorphs, geochemistry (Wimbledon et al. 2011).
One of the possible markers of the J/K boundary interval is
based on the Calpionella alpina ‘acme zone’. This marker
was identified in the Puerto Escaño section approximately in
the middle part of the M19n magnetozone (Pruner et al.
2010) and it is partly re-interpreted here. The Jurassic/Creta-
ceous (J/K) boundary interval is currently one of the most
studied, because no appropriate stratotype for the base of the
Cretaceous has yet been defined despite an extensive re-
search effort (e.g., Hoedemaeker et al. 1998; Houša et al.
1999, 2004; Lakova et al. 1999; Oszczypko et al. 2004; Mi-
chalík et al. 2009; Reháková et al. 2009; Channell et al.
2010; Grabowski et al. 2010; Lukeneder et al. 2010; Mi-
chalík & Reháková 2011; Wimbledon et al. 2011, 2013;
Wimbledon 2014).
Globally, plankton assemblages with rock-forming poten-
tial developed during this time interval. The remarkable
radiation of the some groups, especially nannoconids and
calpionellids, significantly increases their biostratigraphical
value. Moreover, the richness of different fossil groups (am-
monites, calcareous nannofossils, calpionellids) offers the
opportunity to compare and calibrate different biozonations
and bioevents, improving the knowledge of Jurassic and Cre-
taceous biochronology (Marino et al. 2004). This study is fo -
cused on calcareous nannofossil biostratigraphy, an essential
component of standard multidisciplinary J/K boundary re-
search.
According to Pruner et al. (2010), the lithological succes-
sion of the Puerto Escaño section in southern Spain shows
relatively continuous sedimentation with minor incidence of
hiatuses, conditions favourable for study of palaeomagnetic
polarity. They also reported rich fossil assemblages of
calpionellids and ammonites; calpionellids, in particular,
were very well preserved, highly diversified, and with a full
record of their evolution.
The ammonite fauna of this section has been evaluated by
Olóriz (1978); Olóriz & Tavera (1989, 1990); Tavera et al.
(1994); Olóriz et al. (1995, 2004). Lithology, development
and associated ichnofabric assemblages were investigated by
Caracuel (1996); Caracuel et al. (2000). The first relevant
geochemical data (stable isotopes) from this section, cali-
brated by bio- and magnetostratigraphy were given by Žák
et al. (2011).
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The aim of this paper is to describe the Late Jurassic– Early
Cretaceous calcareous nannofossil assemblage from Puerto
Escaño, and to discuss its biostratigraphy and possible
palaeoecological affinities. We compare these calcareous
nannofossil results with the magnetostratigraphic and bio-
stratigraphic (ammonites, calpionellids) data of Pruner et al.
(2010) to define the J/K boundary interval.
Geological setting
The section at Puerto Escaño, in the province of Córdoba,
south-eastern Spain (Fig. 1) is located in the External
Subbetic, which was positioned during the Late Jurassic and
Early Cretaceous in a more distal, rather epioceanic environ-
ment, located in the S-E Iberian subplate palaeomargin (Co-
imbra et al. 2014a). Generally, the Subbetic Zone is a
complex tectonostratigraphic unit which, palaeogeographi-
cally, was part of the pelagic domain of the southern passive
margin of the Iberian Plate. Palaeoenvironmental characteris-
tics, based on geochemistry of carbonates, were recently
provided by Coimbra et al. (2014a,b) and Coimbra et al.
(2015).
According to Pruner et al. (2010), the Upper Jurassic to
lowermost Cretaceous deposits in the studied section (spe-
cifically GA-7, UTM 30SUG44859) consist of upper Am-
monitico Rosso and related facies, ranging from well-bedded
limestones to clayey nodular limestone horizons reflecting
deposition on a distal, epioceanic swell. The section studied is
dominated by wackestone showing microfacies with
variable contents of radiolarians, calcareous dinoflagellates,
planktonic crinoids, planktonic and benthic foraminifers,
calpionellids, ostracods, cephalopods, echinoderms (plates
and spines), sponge spicules and pelagic bivalves, among
others. Macroscopic fossil remains are mostly ammonites,
and less abundant components are belemnites, brachiopods
and echinoids. Their occurrence is concentrated into several
limited horizons (beds — see below). Tavera et al. (1994)
also reported relatively abundant calcareous nannofossils
from this section.
Fig. 1. Location of the studied section (A). The position of section GA-7 at Puerto Escaño with roads in the surroundings (B). Black area
represents the Betic Cordillera. Maps modified from Pruner et al. 2010.
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Material and methods
Calcareous nannofossils
We used the same rock material as in the previous study by
Pruner et al. (2010) for calcareous nannofossil analysis.
These were unused, very small fragments from samples in
the same stratigraphic interval (an 8.1m-thick part of the sec-
tion straddling the upper Tithonian and lower Berriasian),
and numbering. These remnants provided enough material
for detailed micropalaeontological analysis of the nannofos-
sils. Samples numbered from No. 5 to No. 42 (Fig. 2) were
chosen from throughout the profile (Fig. 2).
Calcareous nannofossils were analysed in 51 smear slides
prepared using the standard techniques described by Švábe-
nická (2001), under an Olympus BX51 light microscope
using an immersion objective with a magnification of 100×.
Digital images of nannofossil specimens were taken with an
Olympus DP70 digital camera. At least 200 specimens were
counted on each slide, to obtain relative abundances and
semiquantitative information about nannofossil species di-
versity. Each slide was then scanned for identification of
scarce, but biostratigraphically important, species.
The set of smear slides is stored at the Institute of Geology
and Palaeontology (Chlupáč´s museum of Earth history),
Faculty of Sciences, Charles University in Prague as item
(IGP/2015/PE001).
Preservation of calcareous nannofossils was characterized
using the abbreviations described by Bown (1992):
VP (very poor)=extreme etching
P (poor)=etching and overgrowth; obscured, damaged, or
destroyed central area structures
M (moderate)=moderate etching or overgrowth.
The scale for the estimate of nannofossil total abundance
was modified after Casellato (2010):
A (abundant): >11 specimens per field of view
C (common): 1–10 specimens per field of view
F (few): 1 specimen every 1–5 fields of view
R (rare): 1 specimen every 6 or more fields of view.
The individual abundances for each species per sample
were counted according to the classification proposed by
Bown (1992):
R (rare)=1–2 specimens
F (few)=3–10 specimens
C (common)=11–100 specimens
A (abundant)=more than 100 specimens (out of 200 specimens).
A full list of the calcareous nannofossil taxa found in this
study is given in alphabetical order in Appendix A. The listed
calcareous nannofossils are indexed according to Perch-
Nielsen (1985) and Bown & Cooper (1998). Biostratigraphic
data were interpreted with reference to the nannofossil zona-
tion of Casellato (2010), commonly used for the Upper Ju-
rassic and the Lower Cretaceous in the Tethyan/
Mediterranean area.
Macrofossil record and geochemistry
The abundance of the macrofossils, also including the
benthic assemblage is based on a simple quantitative analy-
sis, calculating the number of specimens recorded in a
1m-wide unit of the bed. An abundance exceeding 5–10
specimens or fragments per unit is considered herein to be
significantly high (in relation to other beds within the pro-
file, where almost no benthic fauna has been recorded).
Higher belemnite abundance (≥3–4 per unit) should be con-
sidered as a bio-event and it is reported in the “Palaeoecolo-
gy” chapter.
Stable isotope curves have been published by Žák et al.
(2011) and they are reduced herein into a single column
(δ
18
O — Fig. 3) as δ
13
C values (varying from 1.14 to 1.53 ‰
V-PDB): they show no significant expressions suitable for
palaeoecological interpretations (see below).
We have used additional AAS geochemical methods as
a tool for recognizing possible terrigeneous (siliciclastic
SiO
2
and Al
2
O
3
) input within the Puerto Escaño section. All
analysis (concentrated to oxide and element detections) was
carried out using a VARIAN (type SpectrAA 280 FS) instru-
ment at the Faculty of Science, Charles University in Prague
(Laboratories of the Geological Institutes).
Results
In the samples studied, calcareous nannofossils were rare
to abundant and very poorly to moderately well preserved. In
total, 35 calcareous nannofossil taxa were identified (Fig. 2).
The most common component of the assemblage is the genus
Watznaueria, forming nearly 58 % of the nannofossils, in-
cluding W. barnesiae (Fig. 4/1), W. manivitiae (Fig. 4/2), W.
communis (Fig. 4/3), W. fossacincta (Fig. 4/4) and W. britan
nica (Fig. 4/5). W. barnesiae was present in all samples and
ranged from 38 % to 59 % of the total assemblage. The
highest abundance of this species was recorded in bed 19.
The percentages of W. manivitiae ranged from 3 % to 17 %
of the total assemblage and the highest abundances were re-
corded from beds 11 to 22. W. britannica formed approxi-
mately 2 % of the total assemblage, while W. fossacincta and
W. communis occurred only sporadically, representing ~0.5
% of the genus Watznaueria.
The second most common genus is Cyclagelosphaera spp.
(~27 % of all identified nannofossils), particularly C. margerelii
(Fig. 4/6), C. deflandrei (Fig. 4/7) and C. argoensis (Fig. 4/8).
Other abundant genera are: Conusphaera spp. (~7 %) repre-
sented by C. mexicana mexicana (Fig. 4/19, 20) and C. mexi
cana minor, Nannoconus spp. (~4 %) represented by
Nannoconus sp. (Fig. 5/1), N. infans, N. erbae (Fig. 5/2, 3),
N. puer (Fig. 5/4, 5), N. globulus minor (Fig. 5/6–9),
N. globulus globulus (Fig. 5/10–13), N. wintereri (Fig. 5/14–17),
N. steinmannii minor, N. steinmannii steinmannii (Fig. 5/18–21),
N. kamptneri minor, and N. kamptneri kamptneri (Fig. 5/22,
23), and finally Polycostella beckmannii (Fig. 4/22, 23), rep-
resenting more than 2 % of the total nannofossil assemblage.
Three nannoliths - Conusphaera spp., Nannoconus spp. and
Polycostella sp. showed the most significant fluctuations in
the nannofossil assemblage, as shown in previous studies
(e.g., Tremolada et al. 2006a). The percentage representation
and peaks in abundance of these most abundant genera
across the studied profile are presented in Fig. 6.
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Fig. 2. Lithology, magnetostratigraphy, biostratigraphy (calpionellid, ammonite and calcareous nannofossil zonation) and vertical distribu-
tion of nannofossil species of the Puerto Escaño section. Open circles indicate uncertain species identification. Biozonal (ammonite, calpionel-
lid) and magnetozonal data after Pruner et al. 2010 (modified). Nannofossil zones follow Casellato (2010). The expected J/K boundary
interval is marked in grey. CNZ — calcareous nannofossil zonation; CZ — calpionellid zonation; CAAZ — Calpionella alpina “acme zone”;
?CPAZ — Crassicollaria parvula “acme zone”; PZ — Praetintinnopsella Zone;
*
— beds studied for calcareous nannofossils (this work).
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Fig. 3. Puerto Escaño section (after Pruner et al. 2010) — magnetostratigraphy, lithology, benthic organisms occurrence, belemnite rela-
tively abundant horizons, geochemical analysis of the bulk rock samples (ratio of oxides CaO, SiO
2
and Al
2
O
3
) and the stable isotpe signals
of the δO
18
curve (after Žák et al. 2011) in relation to the calcareous nannofossil (this paper), calpionellid and ammonite Zones (Pruner et
al. 2010). CNZ — calcareous nannofossil zonation; CZ — calpionellid zonation.
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Fig. 4. Calcareous nannofossils from the Puerto Escaño section. Cross polarized light; scale bar represents 5 µm. 1 — Watznaueria bar
nesiae; sample 25-1 t. 2 — W. manivitiae; sample 25-2 b. 3 — Watznaueria communis; sample 23-3. 4 — W. fossacincta; sample 41.
5 — W. britannica; sample 24 b. 6 — Cyclagelosphaera margerelii; sample 25-1 t. 7 — C. deflandrei; sample 24 b. 8 — C. argoensis;
sample 30. 9, 10 — Cruciellipsis cuvillieri; 9 — sample 25-2 t, 10 — sample 28. 11–13 — Diazomatolithus lehmanii; 11 — sample
26-2, 12 — sample 41, 13 — sample 39. 14, 15 — Hexalithus noeliae; sample 13. 16 — Microstaurus chiastius; sample 25-2 t.
17 — Zeugrhabdotus embergeri; sample 40. 18 — Z. cooperi; sample 41. 19, 20 — Conusphaera mexicana mexicana; 19 — sample 22 b,
20 — sample 26-3 b. 21 — Pentalith; sample 25-2 t. 22, 23 — Polycostella beckmannii; sample 11. 24 — Lithraphidites carniolensis;
sample 26-3 t.
Discussion
Biostratigraphy
Generally, calcareous nannoflora represent an important
source of biostratigraphic data for the Mesozoic and Cenozoic
ages. Indeed, in some multiproxy studies, the most signifi-
cant stratigraphic data were obtained by the analysis of cal-
careous nannofossils (e.g. Halásová et al. 2012).
Despite the relatively poor preservation of the calcareous
nannofossils in our material, several biostratigraphic events
have been defined. The lowest occurrence (LO) of M. chias
Other nannoliths represented by Faviconus multicolumna
tus, Assipetra infracretacea, Hexalithus noeliae (Fig. 4/14,
15), Lithraphidites carniolensis (Fig. 4/24) and an unidenti-
fied pentalith (one specimen, Fig. 4/21) occurred less fre-
quently, as did other members of the coccolithophorids such as
Zeugrhabdotus embergeri (Fig. 4/17), Z. cooperi (Fig. 4/18),
Z. erectus, Rhagodiscus asper, Diazomatolithus lehmanii
(Fig. 4/11–13), Cruciellipsis cuvillieri (Fig. 4/9, 10), Dis
corhabdus ignotus, Microstaurus chiastius (Fig. 4/16) and
Biscutum constans. The preservation and total abundance of
calcareous nannofossils and the individual abundances for
each species are summarized in Fig. 7.
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Fig. 5. Calcareous nannofossils from the Puerto Escaño section. XPL — cross polarized light, PPL — plane polarized light. Scale bar repre-
sents 5 µm. 1 — Nannoconus sp., cross section; sample 25-2 b, XPL. 2, 3 — N. erbae; 2 — sample 23-3, XPL; 3 — sample 23-3, PPL
(the same specimen). 4, 5 — N. puer; 4 — sample 25-2 b, XPL; 5 — sample 25-2 b, PPL (the same specimen). 6–9 — N. globulus minor;
6 — sample 25-1 b, XPL; 7 — sample 25-1 b, PPL (the same specimen); 8 — sample 25-1 t, XPL; 9 — sample 25-1 t, PPL (the same spec-
imen); 10–13 — N. globulus globulus; 10 — sample 25-1 t, XPL; 11 — sample 25-1 t, PPL (the same specimen); 12 — sample 30, XPL;
13 — sample 30, PPL (the same specimen). 14 –17 — N. wintereri; 14 — sample 35, XPL; 15 — sample 35, PPL (the same specimen);
16 — sample 40, XPL; 17 — sample 40, PPL (the same specimen). 18–21 — N. steinmannii steinmannii; 18 — sample 35, XPL; 19 — sam-
ple 35, PPL (the same specimen); 20 — sample 35, XPL; 21 — sample 35, PPL (the same specimen). 22, 23 — Nannoconus kamptneri
kamptneri; 22 — sample 35, XPL; 23 — sample 35, PPL (the same specimen). 24 — Faviconus multicolumnatus; sample 13.
the NJT 17b Subzone, that continues to the LO of N. stein
mannii minor sensu Casellato (2010). Unfortunately, this
bioevent has not been identified in the studied section and
the LO of N. steinmannii minor has been observed in the
middle parts of the Calpionella Zone and the Jacobi Zone
and corresponds to the LOs of N. steinmannii steinmannii,
N. kamptneri minor and N. kamptneri kamptneri (Figs. 6, 7),
that indicates the beginning of the NK-1 Zone (sensu Bra-
lower et al. 1989). In the interval between the LO of N. win
tereri and the LOs of N. steinmannii minor, N. steinmannii
steinmannii, N. kamptneri minor and N. kamptneri kampt
neri, the Calpionella alpina ‘acme zone’ and the beginning
tius indicating the beginning of the NJT 16 Zone sensu
Casellato (2010) was recorded in the middle part of the
M20n magnetozone, at the end of the Chitinoidella Zone and
in the middle part of the Transitorius Zone (Tavera et al.
1994). The LO of N. globulus minor is found in the middle
part of the M19r magnetozone and indicates the beginning of
the NJT 17 Zone sensu Casellato (2010). The LOs of
N. globulus globulus and C. cuvillieri were recorded in the
lower part of the M19n magnetozone, in the middle part of
the Crassicolaria Zone and at the beginning of the Jacobi
Zone. In the upper part of the Crassicolaria Zone, the LO of
N. wintereri was observed. This indicates the beginning of
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Fig. 6. Lithology, magnetostratigraphy and biostratigraphy (calcareous nannofossil zonation). Includes representation of selected nanno-
fossil genera in the Puerto Escaño section as a percentage and the main recorded bioevents. Lithology and magnetozonal data after Pruner
et al. 2010 (modified). Nannofossil zones follow Casellato (2010). * — beds studied for calcareous nannofossils (this work); LO — lowest
occurrence.
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of the Calpionella Zone were observed (Pruner et al. 2010).
It should be noted, that the LO of N. kamptneri minor usually
appears a little above the LO of N. steinmannii minor, but in
this paper it occurs together with the LOs of N. steinmannii
steinmannii and N. kamptneri kampteri in bed 35. This anoma-
ly can be explained by the very poor preservation and ex-
treme etching of calcareous nannofossils between beds 32
and 34 (Fig. 7). Moreover, the appearance of these four spe-
cies together suggests the presence of a hiatus.
In the previous study by Tavera et al. (1994), the zonal
scheme proposed by Bralower et al. (1989) was used. How-
ever, the zonation of Bralower et al. (1989) and specifically
the definition of subzones NJK-A, NJK-B and NJK-C is
based on the lowest occurrences of species with relatively
delicate structures (Umbria granulosa granulosa and Rote
lapillus laffittei) which may disappear from the association
as a result of preservational effects (Tavera et al. 1994). The
material studied in Tavera et al. (1994) was also not well pre-
served and U. granulosa and R. laffittei taxa have not been
recorded. Indeed, only the NJK-D subzone based on the LO
of N. steinmannii minor was determined. This subzone is cor-
related with the lowermost Berriasian (Tavera et al. 1994),
corresponding to the NKT Zone sensu Casellato (2010). In
comparison, two additional nannofossil subzones (NJT 15b,
NJT 17a) and two nannofossil zones (NJT 16, NK-1) were
recognized in this study. Moreover, the time interval of the
NJT 17 and NKT Zones sensu Casellato (2010) has been ob-
served.
Correlation of the main bioevents with magnetostrati-
graphic data (Pruner et al. 2010) is given in Fig. 8, where the
comparison with other studied sections of the J/K boundary
is shown. The LO of N. wintereri has been recorded in the
M19n magnetozone in Puerto Escaño, as well as in Le Chouet,
Brodno, Foza and Torre de’ Bussi sections. In Fiume Bosso,
this bioevent has been observed in M18r and in Barlya sec-
tion in M17r magnetozone. Similarly, the LO of N. steinman
nii minor within the M19n magnetozone has been recorded in
Puerto Escaño, as well as in Le Chouet, Lokut and Torre
de’ Bussi sections. This bioevent has been recorded in M17n
zone in Foza and Fiume Bosso and in M18r in Barlya sec-
tion. The LO of N. steinmannii steinmannii in M19n magne-
tozone was observed only in Puerto Escaño section, then in
M17r zone in Foza and Fiume Bosso sections.
Palaeoecological interpretations
This chapter is divided into four major parts: the calcareous
nannofossils palaeoecology, macrofossil record, new addi-
tional geochemical data and remarks on the key Bed 28 (J/K
boundary sensu Pruner et al. 2010).
Remarks on selected Late Jurassic calcareous nannofossils
In some cases, calcareous nannofossils provide only spo-
radic information about the palaeoecological conditions of
a depositional area. But there is also evidence reported from
the literature that calcareous nannoplankton may give impor-
tant information regarding the trophic levels of the superfi-
cial oceanic water, about the water temperature or salinity
(e.g., Erba 1992; Tremolada et al. 2006b; Aguado et al.
2008, Mattioli et al. 2008). Some palaeoecological aspects
can also be presented from our study.
Generally, the most dominant genera in studied material
are Watznaueria, Cyclagelosphaera, Nannoconus, Conus
phaera and Polycostella (see chapter Results). This compo-
sition of calcareous nannofossil assemblages across J/K
boundary interval is typical for “low latitudes“ sections and
has been already observed in previous studies (e.g. Tavera et
al. 1994; Bornemann et al. 2003; Tremolada et al. 2006a;
Michalík et al. 2009; Lukeneder et al. 2010).
The most common taxon recorded is Watznaueria
barnesiae, representing 48 % of the entire taphocoenosis. This
species is not susceptible to dissolution and is resistant to dia-
genetic alteration (Hill 1975; Thierstein 1980; Roth 1981;
Roth & Bowdler 1981; Roth & Krumbach 1986). Roth &
Krumbach (1986) described assemblages containing more
than 40 % of W. barnesiae as heavily altered by diagenesis.
However, the genus Watznaueria is generally considered to
be the robust and most successful Mesozoic coccolitho-
phore, in terms of abundance, across the widest range of en-
vironments. By some authors Watznaueria is considered to
be an opportunistic, r-strategist taxa (e.g., Tremolada et al.
2006a; Lees et al. 2006; Tantawy et al. 2009; Colombié et al.
2014; Suchéras-Marx et al. 2015). It is ubiquitous and domi-
nant through most of the Mesozoic, further illustrating its
wide palaeoecological tolerance. In the fossil record, W. bar
nesiae displays a eurytopic, ecologically robust form, and
was one of the first species to settle new habitats. In an eco-
logical sense, it is similar to a recent species, Emiliania hux
leyi. Together with Cyclagelosphaera, these two genera are
stratigraphically long-ranging (Jurassic–earliest Palaeocene)
and morphologically conservative, characteristics of gene-
ralist rather than specialist taxa (e.g., Mutterlose & Wise
1990; Street & Bown 2000; Melinte & Mutterlose 2001;
Bown & Concheyro 2004; Lees et al. 2004). Both are con-
sidered to be cosmopolitan taxa and Lees et al. (2006) sug-
gest, that C. margerelii lived in a higher trophic position
than W. barnesiae and was more r-selected, possibly with
more extreme nutrification affinities.
Species such as Biscutum constans, Discorhabdus ignotus,
Diazomatolithus lehmanii and Zeugrhabdotus erectus oc-
curred only sporadically in our samples. These species indi cate
eutrophic environments and preferred higher nutrient
levels in the oceanic surface water (Roth 1981; Roth &
Bowdler 1981; Roth & Krumbach 1986; Bornemann et al.
2003; Tremolada et al. 2006a,b). Dominance of B. constans
and Zeugrhabdotus spp. is usually considered indicative of
upwelling of cold water rich in nutrients (e.g., Mutterlose &
Kessels 2000; Lees et al. 2005; Hardas & Mutterlose 2007;
Lowery et al. 2014). Higher abundances of the taxa B. con
stans (~11 % of the total assemblage) and Z. erectus (~33 %
of the total assemblage) have been associated with the oc-
currence of black shales and phosphorite deposition (Kessels
et al. 2003). However, these species show very low abun-
dances in our samples — only one specimen of each species
(Fig. 7). It can be explained by high susceptibility to dissolu-
tion of these small coccoliths such as Z. erectus, B. constans
232
SVOBODOVÁ and KOŠŤÁK
GEOLOGICA CARPATHICA
, 2016, 67, 3, 223–238
Fig. 7. Age, calcareous nannofossil zonation and calcareous nannofossil range chart of the Puerto Escaño section, including information on
preservation, total abundance and relative abundance of each taxon. Question marks indicate uncertain species identification of heavily dis-
solved specimens or of nannofossils that occutred only as fragments. Uncertain occurrence was often associated with beds where preserva-
tion was very poor (marked by grey colour) (b=bottom, m=middle, t=top of the bed).
Both situations are probably connected with controlling
factors, namely shallowing but rather the presence of higher
nutrient flux. Shallowing should be excluded, maybe excep-
ting that in Beds 10–17 (i.e. lower and middle part of the
Transitorius ammonite Zone, Fig. 3), where siliciclastic and
Al
2
O
3
influx (with some signs of cyclicity) has been detected
(Fig. 3), but this phenomenon could also be connected with
periods with higher run-off. Probably, the sequences with
abundant benthos represent the result of larger nutrient flux
and subsequent biological productivity. In this context, the
co-occurrence of Biscutum constans, Discorhabdus ignotus,
Diazomatolithus lehmanii and Zeugrhabdotus erectus with
abundant benthic organisms (Fig. 3) — namely eutrophic
communities, should indicate some correlation. This should
also support the results of Bornemann et al. (2003) and
Tremolada et al. (2006a,b), who suggested these nannofossil
taxa were dependent on a eutrophic environment. However,
we assume that more relevant data are needed. We could not
confirm the hypothesis of Mutterlose & Kessels (2000), Lees
et al. (2005), Hardas & Mutterlose (2007), Lowery et al.
(2014) and others relative to the oxygen stable isotope curve,
as no marked cooling (related to upwelling of cold waters) is
recorded in the δ
18
O
values (Fig. 3). Nevertheless, we agree
with the conclusion that these taxa represent rather eutrophic
organisms.
Benthic assemblages with skeleton remains occur in Bed
complex 10–17 (in the middle part of the Transitorius
Zone), 22–25 (corresponding approximately to the Duran-
gites ammonite Zone), 28 (“Saccocoma Bed”, suggested
J/K boundary), 33 (lower part of the standard Calpionella
Zone) and 36 (i.e. the middle part of the Calpionella Zone)
(Fig. 3).
Higher abundances of belemnites (active nektonic ani-
mals) have been recorded in beds 14A, 21, 23, 33B–C, and
42. Their occurrences partly correlate with the benthos
presence — namely with more eutrophic conditions (see
above). It has been suggested that higher belemnite abun-
dances (predominantly hibolithids and pseudobelids) are de-
pendent on the transgressive/regressive tracts (Mitchell
2005; Wiese et al. 2009), however, the sea-level oscillations
in the epioceanic development of the Puerto Escaño se-
quence (Olóriz et al. 2004) seems to be under the analytical
limits and further investigations are needed. In this respect,
the winnowing effect, concentrating macrofossil records,
cannot be excluded. On the other hand, the presence of these
remains only in several horizons suggests that their original
habitat, in terms of the environment, lithology and geochemi-
cal record in other beds, in which they are missing, is fully
comparable.
Additional geochemical data
New geochemical data are based on the AAS silicate analy-
sis (see above), which detects especially oxides and element
and D. ignotus (Hill 1975; Thierstein 1980; Roth 1981,
1983; Roth & Krumbach 1986), because a diagenetic over-
print may imply a decrease in their relative abundance
(Giraud 2009; Giraud et al. 2013).
Irregular occurrence of Rhagodiscus asper and Lithraphi
dites carniolensis began in bed 26, which corresponds to the
NJT 17a nannofossil subzone, close below the J/K boundary
interval. Erba (1987) and Erba et al. (1992) interpreted these
species as thermophilous warm-water taxa indicating warm
surface water that was poor in nutrients. In this context, there
is also increased abundance of Nannoconus spp. in this part
of the section (Fig. 6). Nannoconids have been characterized
as typical Tethyan taxa of warm, low-latitude, carbonate-
shelf environments. Similar to Watznaueria are considered
to be r-selected taxa, moreover robust and not susceptible to
dissolution (Street & Bown 2000; Melinte & Mutterlose
2001; Bown & Concheyro 2004; Tremolada et al. 2006b).
These extinct ‘incertae sedis’ nannofossils are often inter-
preted as living in the lower photic zone (e.g., Erba 1994;
Bornemann et al. 2003; Herrle 2003; Barbarin et al. 2012).
The ecological affinities of other abundantly represented
species, Conusphaera and Polycostella, are unknown, except
considering Conusphaera to be a warm water taxon (e.g.,
Melinte & Mutterlose 2001; Mutterlose et al. 2005). However,
Bornemann et al. (2003) proposed for them an ecological
setting similar to that of Nannoconus, due to some similari-
ties in the skeletons of these taxa.
Macrofossil abundance
The ammonite fauna has been studied in great details by
numerous authors (Olóriz & Tavera 1989; Tavera et al.
1994; Pruner et al. 2010; etc.) and the belemnite record (sta-
ble isotopes) has partly been investigated by Žák et al.
(2011). However, the presence and abundance of the macro-
fauna, predominantly benthic filter feeders and substrate
feeders (i.e. brachiopods, echinoids, less abundant bivalves,
echinoderms, sponges) is of great interest. Their presence/
absence is shown in Fig. 3. The constant sedimentation rate
(i.e. 1–5 mm/ky; 2.87 mm/ky with standard deviation
1.17 mm/ky for the whole section; Pruner et al. 2010) as well
as palaeocological conditions — namely a very low variation
of geochemical content in carbonates (also supported by the
stable isotope data; Žák et al. 2011, Fig. 3) within the lime-
stone beds through the whole section do not suggest any rapid
changes either in sedimentology (and bathymetry, not ex-
ceeding the CCD — supported by almost continuous ammo-
nite record) or in taphonomy. Skeletons of all the above
mentioned benthic groups as well as belemnites are com-
posed predominantly by calcite. Thus, we assume very low
fluctuations within the preservation potential of these fossils.
So, the basic scheme for benthic assemblage distribution
should be introduced based on simple fact — namely on rela-
tively abundant/absent.
233
CALCAREOUS NANNOFOSSILS OF THE J/K PUERTO ESCAÑO SECTION (S SPAIN)
GEOLOGICA CARPATHICA
, 2016, 67, 3, 223–238
SAMPLE
PRESER
VA
TION
TOT
AL
ABUNDANCE
Assipetra infracr
etacea
Biscutum constans
Conusphaera m. mexicana
Conusphaera mexicana minor
Cruciellipsis cuvillieri
Cyclagelosphaera ar
goensis
Cyclagelosphaera deflandr
ei
Cyclagelosphaera mar
ger
elii
Diazomatolithus lehmanii
Discor
habdus ignotus
Faviconus multicolumnatus
Hexalithus noeliae
Lithraphidites carniolensis
Micr
ostaurus chiastius
Nannoconus sp.
Nannoconus erbae
Nannoconus globulus globulus
Nannoconus globulus minor
Nannoconus infans
Nannoconus k. kamptneri
Nannoconus kamptneri minor
Nannoconus puer
Nannoconus steinmannii minor
Nannoconus s. steinmannii
Nannoconus winter
er
ei
Pentalith
Polycostella beckmannii
Rhagodiscus asper
W
atznaueria barnesiae
W
atznaueria britannica
W
atznaueria communis
W
atznaueria fossacincta
W
atznaueria manivitae
Zeugr
habdotus cooperi
Zeugr
habdotus ember
geri
Zeugr
habdotus er
ectus
CALCAREOUS NANNO
-
FOSSILS ZONA
TION
ST
AGE
42
P C - - R - - - C C R - - - - - F - - R - - R - R - - - - - C F - R C - F -
NK-1
LOWER BERRIASIAN
BERRIASIAN
41
P C - - R - - - C C R - - - R - F - R F - - - - F - R - - - C F - R C R - -
40
P C - - F - - - C C - - - - R - C - F F - - - - F - F - - R C F - F C - R -
39
P C - - F - - - C C R - - - R - F - R F - - R - - - F - - - C F - - C - R -
38 t
VP F - F - - - C C - - - - - - C - - R - - - - - - R - - - A R - - C - - -
38 b
VP R - - F - - - C C - - - - - - C - R - - - R - - - R - - - A - - - C - R -
37
VP C - - C R - - C C - - - - R - C - R R - - - - - - R - - - A R - - C - R -
36
P C - - C R - - C C - - - - R - C - R R - - F - F R - - - - C F - - F - R -
35
M A - - R R - - C C F - - - - - C - F R - R F - C F R - - R C F - - F R R -
34
VP C - - F - - - C C - - - - - - F ?R - ?R - - - - - - R - - - A R - R C - - -
NJT
17 / NKT
J/K
33B
P C R - C F - - C F - - - - - - F - R - - - - - - - - - - - C R - R C - R -
33A
VP C - - C F - - C C - - - - - - C - - R - - - - - - - - - - C R - - C - R -
32 t
P C R - C R - - C C - - - R R - F - R R - - - - - - - - - - C F - R C - - -
32 m VP R - - R R - - C C R - - - - - F - ?R - - - - - - - - - R - A R - R C - - -
32 b
VP C - - F F - - C C - - - - - - C ?R R R - - - R ?R - F - - - A R - - F - - -
31
P C - - F F - - C C - - - - R - F - R R - - - R - - R - - - C R - R C R - -
30
M C - - F F - R C C - - - - - - C R R F - - - R - - R - - R C R - R C R - -
29
VP C R - C C - - C C R - - - - - F - - R - - - - - - R - - - C R - F C - - -
28
P F - - C C R - C C - - - - - - F - - R - - - - - - - - - - C F - - C - - -
27
P C - - C C - - C C R - - - - - F - R R - - - R - - R - - - C F R - C - - -
26-3 t P C - - F F - - C C
- - - R - F - - R - - - - - - - - - R C F - - C - R -
NJT
17a
UPPER TITHONIAN
T I
T H O N I
A
N
26-3 b P C - - C C - - C C - - - - - - F - R R - - - - - - - - - - C F - - C - R -
26-2
P F - - C C - - C C R - - - ?R - F - R R - - - - - - - - ?R - C - - - C - - -
26-1
P C - - C C - - C C - - - - - - F - - - - - - - - - - - - - C F - R C - R -
25-2 t M C - - C F R - C C - - - - - R - - R R - - - - - - - ?R - - C F - - C - - -
25-2 b M C - - F F - - C C R - - - - - F - - R R - - R - - - - - - C F - - C - - -
25-1 t P C - - C F - - C C - R - - - - - - R R - - - - - - - - - - C R - - C - R -
25-1 b P C R - C F - - C C - - - - - - - - - R - - - R - - - - - - C R - - C - - -
24 t
VP C - - R F - - C C - - - - - - R - - - - - - - - - - - R - A R - - C - - -
24 b
P C - - F F - - C C R - - - - - - R - R - - - - - - - - ?R - C R R R C - - -
23-3 VP F - - F F - - C C - - - - - - - R - R ?R - - - - - - - - - A F R - C - - -
23-2
P C - - F C - - C C - - - - - - - - ?R ?R - - - - - - - - - - C F - - C - - -
NJT
16
MIDDLE TITHONIAN
23-1
P C - - F F - - C C R - - - - - R - - - - - - - - - - - F - C F - - C - R -
22 t
P C R - C F - - C C R - - - - - R - ?R ?R - - - - - - - - R - C R - - C - - -
22 m M C R - C F - - C C - - - - - R R - - ?R ?R - - - - - - - F - C F - - C - - -
22 b
P F R - F F - - C C - - - - - - R - - - - - - - - - - - F - C R - R C - - -
21
P F - R R F - - C C R - - - - R ?R - - - - - - - - - - - F - C F - R C - - -
20 t
P F R - R R - - C C R - - - - - - - - - - - - - - - - - F - A F - - C - - R
20 b
P F R - R F - - C C - - - - - R - - - - ?R - - - - - - - F - A R - R C - - -
19
VP R R - - - - - C C R - - - - - - - - - - - - - - - - - C - A R - R C - - -
18
VP F R - - ?R - - C C ?R - - - - R R - - - - - - - - - - - C - A R - - C - - -
17
P C F - R - - - C C - - - - - ?R - - - - - - - - - - - - F - A F - - C - - -
16
VP C F - R - - - C C - - - - - - - - - - - - - - - - - - C - A R - F C - - -
15
VP C F - - - - - C C R - - - - R - - - - - - - - - - - - C - A R - R C - - -
14
VP C F - - - - - C C R - - R - R ?R - - - - - - - - - - - C - A F - - C - - -
13
M A R - F R - - C C - R R R - - - - - - - - - - - - - - C - A F - R C - - -
11/12 VP C R - - R - - C C R - - - - - - - - - - - - - - - - - C - A F - R C - - -
11
P F F - - R - - C C R - - ?R - R - - - - - - - - - - - - C - A F - - C - - -
10
VP C - - - - - - C C - - - - - - - - - - - - - - - - - - C - A F - R C - - -
NJT
15
15b
9
P C R - - - - - C C - - - - - - - - - - - - - - - - - - C - A F - - C - R -
8
P A R - - R - - C C - - - - - - - - - - - - - - - - - - C - A F - F C - - -
234
SVOBODOVÁ and KOŠŤÁK
GEOLOGICA CARPATHICA
, 2016, 67, 3, 223–238
Fig.
8.
Correlatio
n
of
selected
sequences
showing
the
M20–M17
interval;
W
imbledon
et
al.
(2013),
modified.
Revised
from
W
imbledon
et
al.
(201
1).
Brodno
columns
based
on
data
in
Houša
et
al.
(2007)*
and
Michalík
et
al.
(2009)**.
Data
1–4
in
Tethys
(base
of
B.
jacobi
Subzone,
base
of
Alpina
Subzone,
top
of
M19n.2n, and
base
of
Ferasini
Subzone)
and
their
approximate
posi
-
tions at Nordvik (column after Houša et al. 2007).
The Barlya column is based on data provided by Platon
Tchoumatchenco
(unpublished magnetozones by B. Galbrun). Lókút after Grabowski
et al. (2010).
The lowest occurences (LOs) of biostratigrafically significant calcareous nannofossils in the Puerto Escaño section (this work) are indicated in red.
235
CALCAREOUS NANNOFOSSILS OF THE J/K PUERTO ESCAÑO SECTION (S SPAIN)
GEOLOGICA CARPATHICA
, 2016, 67, 3, 223–238
components of the sediment. Three major events representing
marked inputs of terrigeneous material were detected at the
levels of the beds 8, 30-31 and 40-41 (Fig. 3). Positive curve
excursions of oxides SiO
2
and Al
2
O
3
are accompanied by
marked increases (however, at the lower concentrations) of
FeO, K
2
O, TiO
2
and Na
2
O, as well as marked increases of
U
238
, Th
232
, Pb
208
and other rare elements (unpublished
data), clearly documenting a terrigeneous input. A positive
(however, not so straightforward) correlation between the in-
crease of calcareous nannoplankton diversity and the terrige-
neous input is indicated in the beds 13, 29-31 and 40-41, but
less marked in the in beds 22 and 35 levels. Higher terrige-
neous input should be evidence of weathering and/or the re-
gression trend. In the studied profile, we should recognize
three major sequences with higher terrigeneous input —
namely bed 8 (and overlying beds 9-14A), beds 29-31 and
the upper part of bed 40 into the lower part of bed 41. The al-
most identical chemical composition of oxides and element
content probably proves the same source area. However, its
position within the Subbetic Basin margin is unknown.
The stable isotope data were precisely analysed by Žák et
al. (2011). The δ
18
O curve (Fig. 3), shows minor positive ex-
cursions in beds 8, 12, 23, 27-32, 34 and 40 levels, and the
major negative peak has been recorded in bed 26-3 (Fig. 3).
Only the peak in the Bed 12 corresponds to the higher abun-
dance of Polycostella sp. (Fig. 6) and the positive excursion
at level 34 corresponds to abundance increase of Conus
phaera spp. In this respect, we cannot estimate any signifi-
cant correlation between the calcareous nannofossil diversity
development and the temperature changes, as only limited
variations in the δ
18
O curve have been recorded.
Remarks on the key Bed 28
Bed 28 (J/K boundary sensu Tavera et al. 1994; see also
Pruner et al. 2010) contains a large accumulation of smaller
globular (spherical) Calpionella alpina (Pruner et al. 2010).
Bed 28 (“Saccocoma Bed” herein, Fig. 3) also contains ex-
tremely large, calcitic skeletal debris of Saccocoma skele-
tons, and thus, the reworking of smaller calpionellids cannot
be excluded. However, there is no sign of siliciclastic input
in this horizon, and the highest ratio between Ca-oxide and
minimum SiO
2
and Al
2
O
3
input is recorded in this bed
(Fig. 3). The opposite trend is visible in the overlying beds,
beds 29-31, where the marked decrease of Ca-oxide and in-
crease of siliciclastics input (represented by SiO
2
), as well as
an increase of Al
2
O
3
seems to prove a run-off increase due to
an acceleration of weathering and/or rather a regressive se-
quence. The regression hypothesis should be supported by
the presence of a marked increase in crassicollarian abun-
dance (C. parvula — parvula Acme zone, “CPAZ” sensu
Pruner et al. 2010), suggested to have been reworked from
older upper Tithonian limestones and incorporated into the
micrite matrix of the Alpina Subzone (Wimbledon et al.
2013). We agree with this interpretation and we preliminari-
ly suggest the section studied represents a regressive se-
quence (beds 29-31). A similar trend is recorded in the
uppermost part of bed 40 and especially in the lower part of
bed 41, where decrease of Ca-oxide and increase of SiO
2
and
Al
2
O
3
(as a product of the laterite weathering) input have
been detected (Fig. 3).
Conclusions
We have studied the calcareous nannofossils from the
GA-7 section at Puerto Escaño. Consistent with the results of
Tavera et al. (1994), the dominant genera in the calcareous
nannofossil associations of the section are Watznaueria spp.,
Cyclagelosphaera spp., Nannoconus spp. and Conusphaera
spp. and Polycostella sp.
We have applied the nannofossil zonation of Casellato
(2010), and recognized several nannofossil LOs (Figs. 6, 7):
Microstaurus chiastius, N. globulus minor, N. globulus globu
lus and Cruciellipsis cuvillieri, N. wintereri and finally
N. steinmannii minor, N. steinmannii steinmannii, N. kampt
neri minor and N. kamptneri kampteri. Moreover, the com-
position of the nannofossil assemblage indicated a warm,
carbonate-shelf environment with oligotrophic conditions.
The J/K boundary transition has been approximated with
the LO of N. wintereri to the LOs of N. steinmannii minor,
N. steinmannii steinmannii, N. kamptneri minor and N. kampt
neri kamptneri. This interval is located between beds 27 and
35. Consistent with Pruner et al. (2010), the J/K boundary
lies in approximately the upper middle part of the M19n
magnetozone and includes the Calpionella alpina ‘acme
zone’ (Fig. 2).
The co-occurrence of taxa Biscutum constans, Discorhab
dus ignotus, Diazomatolithus lehmanii and Zeugrhabdotus
erectus with abundant benthic organisms should confirm
their preferences for higher nutrient levels.
The diversity of calcareous nannofossils at higher levels
partly corresponds to the levels with terrigeneous input, well
documented by geochemical methods.
Here we suggest that the increase in abundance of Crassi
collaria parvula (i.e. — Parvula Acme zone, “CPAZ” sensu
Pruner et al. 2010) is the result of reworking from older up-
per Tithonian deposits, in relation to the regressive sequence
between beds 29-31.
Acknowledgements: The authors thanks the Institute of
Geology of the Czech Academy of Sciences for financial
support (Research Plan RV067985831), the Grant Agency of
the Czech Republic (Grant No. GACR 16-09979S), the
Project 7AMB14SK201 supported by the Ministry of Educa-
tion of the Czech Republic and PRVOUK P44. Ladislav Str-
nad (Laboratories of the Geological Institutes, Prague) is
greatly acknowledged for geochemical analysis. We are in-
debted to William Wimbledon (University of Bristol) for lin-
guistic corrections and valuable comments. We are grateful
to the journal reviewers Kristalina Stoykova and an anony-
mous reviewer, for insightful comments on an earlier draft.
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Appendix A — Taxonomic index in alphabetical order