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Ammonite biostratigraphy of the uppermost Hauterivian in the Betic Cordillera (SE Spain)

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A detailed analysis of the stratigraphic distribution of ammonites from fourteen sections in the External Zones of the Betic Cordillera has enabled us to identify accurately the sequence of bioevents that take place throughout the uppermost Hauterivian and to propose a more precise biostratigraphic scheme for this interval. Thus, we have divided the two currently admitted zones (the Crioceratites balearis Zone and the Pseudothurmannia angulicostata auct. Zone) into several subzones. Four subzones can be recognised within the Cr. balearis Zone. The base of each subzone is defined by the first occurrence of one of four successive species belonging to the same Crioceratites lineage. These species are: Cr. balearis, Cr. binelli, Cr. krenkeli and Cr. angulicostatus. The Ps. ohmi Zone (which replaces the classical Ps. angulicostata Zone) can be divided into three subzones characterised by three successive species of the genus Pseudothurmannia: Ps. ohmi, Ps mortilleti (here considered as a senior synonym of Ps. catulloi) and Ps. picteti. According to the current definition, the first occurrence of Taveraidiscus hugii (OOSTER) marks the lower boundary of the Barremian stage. This event fits into a major faunal-renewal episode that begins in the upper part of the Ps. picteti Subzone.
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Ammonite biostratigraphy of the uppermost Hauterivian
in the Betic Cordillera (SE Spain)
Biostratigraphie d’ammonites de l’Hauterivien terminal
dans la Cordillère Bétique (sud-est de l’Espagne)
Miguel Company *, José Sandoval, José M.Tavera
Departamento de Estratigrafía y Paleontología, Facultad de Ciencias, Universidad de Granada, 18002 Granada, Spain
Received 2 October 2002; accepted 23 December 2002
Abstract
A detailed analysis of the stratigraphic distribution of ammonites from fourteen sections in the External Zones of the Betic Cordillera has
enabled us to identify accurately the sequence of bioevents that take place throughout the uppermost Hauterivian and to propose a more precise
biostratigraphic scheme for this interval. Thus, we have divided the two currently admitted zones (the Crioceratites balearis Zone and the
Pseudothurmannia angulicostata auct. Zone) into several subzones. Four subzones can be recognised within the Cr. balearis Zone. The base
of each subzone is defined by the first occurrence of one of four successive species belonging to the same Crioceratites lineage. These species
are: Cr. balearis, Cr. binelli, Cr. krenkeli and Cr. angulicostatus. The Ps. ohmi Zone (which replaces the classical Ps. angulicostata Zone) can
be divided into three subzones characterised by three successive species of the genus Pseudothurmannia: Ps. ohmi, Ps mortilleti (here
considered as a senior synonym of Ps. catulloi) and Ps. picteti. According to the current definition, the first occurrence of Taveraidiscus hugii
(OOSTER) marks the lower boundary of the Barremian stage. This event fits into a major faunal-renewal episode that begins in the upper part
of the Ps. picteti Subzone.
© 2003 Éditions scientifiques et médicales Elsevier SAS. All rights reserved.
Résumé
L’analyse détaillée de la distribution stratigraphique des ammonites dans quatorze coupes localisées dans les Zones Externes de la
Cordillère Bétique nous a permis d’identifier avec précision la séquence des bioévénements qui ont eu lieu durant l’Hauterivien sommital et
de proposer un schéma zonal précis pour cet intervalle. Ainsi, nous avons divisé les deux zones actuellement admises (Zone à Crioceratites
balearis et Zone à Pseudothurmannia angulicostata auct.) en plusieurs sous-zones. Quatre sous-zones ont pu être reconnues dans la Zone à Cr.
balearis. La base de chaque sous-zone est définie par la première apparition de l’une des quatre successives espèces appartenant à la même
lignée crioceratitique. Ces espèces sont : Cr. balearis, Cr. binelli, Cr. krenkeli et Cr. angulicostatus. La Zone à Ps. ohmi (qui vient remplacer
la Zone classique à Ps. angulicostata) peut être subdivisée en trois sous-zones caractérisées par trois espèces successives du genre
Pseudothurmannia : Ps. ohmi, Ps. mortilleti (considérée ici comme synonyme de Ps. catulloi)etPs. picteti. D’après la définition
actuellement admise, la première apparition de Taveraidiscus hugii (OOSTER) marque la limite inférieure de l’étage Barremien. Cet
événement coïncide avec un épisode de renouvellement faunique important qui débute dans la partie supérieure de la sous-zone àPs. picteti.
© 2003 Éditions scientifiques et médicales Elsevier SAS. All rights reserved.
Keywords: Ammonoids; Upper Hauterivian; Zonation; Mediterranean Province
Mots clés : Ammonites ; Hauterivien supérieur ; Zonation ; Province Méditerranéenne
* Corresponding author.
E-mail address: mcompany@ugr.es (M. Company).
Geobios 36 (2003) 685–694
www.elsevier.com/locate/geobio
© 2003 Éditions scientifiques et médicales Elsevier SAS. All rights reserved.
doi:10.1016/j.geobios.2002.12.001
1. Introduction
In the current standard zonation for the Mediterranean
region (Hoedemaeker and Rawson, 2000), the uppermost
Hauterivian interval is represented by the Crioceratites bale-
aris Zone and the Pseudothurmannia angulicostata auct.
Zone. These two units, introduced by Busnardo (1984) in his
zonation for the Lower Cretaceous of southeastern France,
were adopted by the Lower Cretaceous Cephalopod Team in
its first zonal scale formulated at the Digne Workshop (Hoe-
demaeker and Bulot, 1990). The Ps. angulicostata auct.
Zone was later, at the proposal of Ph. Hoedemaeker during
the Mula Workshop (Hoedemaeker and Company, 1993),
divided into two subzones: a lower Ps. ohmi Subzone and an
upper Ps. catulloi. This disposition has been retained un-
changed in the zonations subsequently proposed by the
working group.
The excessive simplicity of this scheme contrasts with the
high resolution attained by some of the zonations recently
proposed for other Lower Cretaceous intervals (see Klein
and Hoedemaeker, 1999). To solve this deficiency, more
detailed analyses of the ammonite distribution in the upper-
most Hauterivian were needed in order to identify accurately
the sequence of bioevents and to enable the construction of a
more precise zonation for this interval. To this end, we
undertook bed-by-bed sampling of several sections located
in different palaeogeographic domains of the Betic Cordil-
lera (Fig. 1). These sections are:
Barranco de la Aguzadera (La Guardia, Jaén): sections
X.G and X.G1.
Ermita de Cuadros (Bedmar, Jaén): section X.EC.
Río Argos (Caravaca, Murcia): sections X.Ag1 (= sec-
tion A in Hoedemaeker, 1995)(Fig. 2), X.Ag4 and
X.Ag5.
Barranco de Cavila (Caravaca, Murcia): section X.Kv3.
Arroyo de Gilico (Cehegín, Murcia): section X.V1
(Fig. 3).
Cerro del Tornajo (Lorca, Murcia): sections X.Tj1 and
X.Tj2.
Sierra del Cid (Petrer, Alicante): sections X.A1 and
X.A2.
Barranco de la Querola (Cocentaina, Alicante): section
X.Q.
Cantera de l’Almuxic (Oliva,Valencia): section X.O.
More than 5000 identifiable ammonites were collected
from the interval studied in these sections. The analysis of
species distribution has enabled us to divide the two classic
zones into several subzones (Fig. 4). Thus, we have recogn-
ised four subzones in the Cr. balearis Zone and three sub-
zones in the Ps. ohmi Zone (= Ps. angulicostata auct. Zone).
All of these are interval subzones, the lower boundary of
which is defined by the first occurrence of the index species,
the upper boundary coinciding with the base of the next unit.
Although the zonal scheme presented here is proposed only
for the Betic Cordillera, its constituent units can be easily
Fig. 1.Geographical and geological location of the studied sections.
Fig. 1. Localisation géographique et géologique des coupes étudiées.
686 M. Company et al. / Geobios 36 (2003) 685–694
Fig. 2.Río Argos-1 section (X.Ag1). Lithological succession and ammonite distribution.
Fig. 2. Coupe de Río Argos 1 (X.Ag1). Succession lithologique et distribution des ammonites.
687M. Company et al. / Geobios 36 (2003) 685–694
recognised in many other parts of the Mediterranean area. A
preview of these results was presented by Aguado et al.
(2001).
2. Zonation
2.1. Crioceratites balearis Zone
This unit was introduced, without formal definition, by
Busnardo (1984) and later defined by Hoedemaeker and
Leereveld (1995) as the biostratigraphic interval between the
first occurrence of Cr. balearis (NOLAN) and the first occur-
rence of Ps. ohmi (WINKLER). Four subzones, defined by
the consecutive appearances of four different chronospecies
belonging to the same Crioceratites lineage, can be recogn-
ised within this zone. These species are: Cr. balearis
(Fig. 5(1–3)), Cr. binelli (ASTIER) (Fig. 5(4)), Cr. krenkeli
(SARKAR) (Fig. 5(6–8)) and Cr. angulicostatus
(D’ORBIGNY) (Fig. 5(9–10)). They correspond to four suc-
cessive steps in what appears to be an evolutionary trend
Fig. 3.Arroyo Gilico section (X.V1). Lithological succession and ammonite distribution.
Fig. 3. Coupe de Arroyo Gilico (X.V1). Succession lithologique et distribution des ammonites.
688 M. Company et al. / Geobios 36 (2003) 685–694
towards a stronger ornamentation and a clearer differentia-
tion between main and intermediate ribs in the middle onto-
genetic stages. In addition to these forms, we have found
specimens attributable to Cr. majoricensis (NOLAN)
(Fig. 5(5)), which probably represent morphotypes of the
same lineage showing a more prolonged trituberculate stage
(trituberculate ribs can be present in the innermost whorls of
all members of the group).
Together with the genus Crioceratites, the faunal assem-
blage from this zone is composed mainly of long-ranging
species such as Plesiospitidiscus subdiffıcilis (KARAK-
ASCH) (Fig. 6(3)), Abrytusites neumayri (HAUG), Neolis-
soceras subgrasianum (DRUSHCHITS), Lytoceras subfim-
briatum (D’ORBIGNY), Phylloceras thetys (D’ORBI-
GNY), Phyllopachyceras infundibulum (D’ORBIGNY) and
Phyllopachyceras winkleri (UHLIG).
2.1.1. Cr. balearis Subzone
Cr. balearis is the first member of the lineage. Its orna-
mentation in the middle stages consists of uniform and dense
ribs lacking distinct umbilical tubercles. The fauna in this
interval is scarce and shows low diversity. The last specimens
of Discoidellia couratieri VERMEULEN occur at the base
of this subzone, whereas the first Paraspiticeras appear in its
upper part.
2.1.2. Cr. binelli Subzone
The next species of the group, Cr. binelli, differs from Cr.
balearis in the appearance of rib bundles rising from well-
defined umbilical bullae. The faunal assemblages from this
subzone are still poorly diversified and numerically domi-
nated by the index species and Pl. ligatus.
2.1.3. Cr. krenkeli Subzone
Cr. krenkeli shows a clear differentiation between main
and intermediate ribs from quite early ontogenetic stages. In
this subzone, the fauna is more abundant and diversified than
in the previous ones. Discoidellia vermeuleni CECCA,
FARAONI and MARINI and the first representatives of the
genus Anahamulina, attributable to An. jourdani (ASTIER
sensu OOSTER), appear together with the index species at
the base of this interval.
2.1.4. Cr. angulicostatus Subzone
As is well known (Sarkar, 1955; Hoedemaeker, 1995), the
species Ammonites angulicostatus D’ORBIGNY has been
Fig. 4.Proposed zonation and ranges of the most significant ammonite species.
Fig. 4. Zonation proposée et distribution stratigraphique des principales espèces d’ammonites.
689M. Company et al. / Geobios 36 (2003) 685–694
690 M. Company et al. / Geobios 36 (2003) 685–694
misinterpreted by most authors. After having analysed a cast
of the holotype, we are convinced, in agreement with Hoede-
maeker (1995), that this taxon should be placed among the
Crioceratites species. Cr. angulicostatus would then be the
last member of the lineage that begins with Cr. balearis and
the ancestor of the forms currently included in the genus
Pseudothurmannia (see taxonomic note below).
The first Emericiceras and Acrioceras, respectively repre-
sented by Em. thiollierei (ASTIER) and Ac. meriani
(OOSTER) (Fig. 5(11)), also appear in this subzone. These
two nominal species may be no more than the two antidimor-
phs of a single biological species.
This stratigraphic interval is very unevenly represented in
the sections studied (compare Figs. 2 and 3), probably be-
cause of the slumps, which frequently affect the sediments of
that age.
2.2. Pseudothurmannia ohmi Zone
We use this unit in the sense of Hoedemaeker and Leerev-
eld (1995), who introduced it as a substitute for the ancient
Ps. angulicostata Zone. According to their interpretation, the
Ps. ohmi Zone would correspond to the interval comprised
between the first occurrence of the index species and the
lower boundary of the Barremian stage. This interval is
characterised by the development of the genus Pseudothur-
mannia. It can be divided into three subzones defined by the
consecutive appearances of Ps. ohmi (WINKLER) (Fig. 6(1,
2)), Ps. mortilleti (PICTET and DE LORIOL) (Fig. 6(4)) and
Ps. picteti (SARKAR) (Fig. 6(6, 7)). These three species also
represent three successive stages of an evolutionary trend
towards a more involute coiling.
Together with the Pseudothurmannia species, which are
by far the main components, the faunal assemblages from
this zone are composed of heteromorphs, desmoceratids,
phylloceratids and other minor groups. Contrary to the data
presented by some authors (Vašícˇek, 1995; Hoedemaeker,
1995; Avram and Melinte, 1998), we have not found Crio-
ceratites of the balearis-binelli group coexisting with
Pseudothurmannia. In this respect, our observations coin-
cide with those of Vermeulen (1980), Braga et al. (1982),
Autran (1993) and Ropolo (1995). These discrepancies may
be due to differences in taxonomic interpretations.
2.2.1. Pseudothurmannia ohmi Subzone
The base of this subzone, as already defined by Hoede-
maeker and Leereveld (1995), coincides with the first occur-
rence of the index species. Ps. ohmi is the first and more
evolute species of the genus Pseudothurmannia. It differs
from its ancestor, Cr. angulicostatus, in having the whorls
always in touch and having definitely lost the initial trituber-
culate stage. The fauna from this subzone is very abundant
and composed, in addition to the index species, of taxa
already present in lower levels.
2.2.2. Pseudothurmannia mortilleti Subzone
The lower boundary of this subzone is defined by the first
occurrence of Ps. mortilleti, here considered a senior syn-
onym of Ps. catulloi (PARONA). An important faunal re-
newal, already pointed out by Hoedemaeker (1995), takes
place around this boundary. Besides the index species, Ps.
pseudomalbosi(SARASIN and SCHÖNDELMAYER)(here
considered a senior synonym of Ps. sarasini SARKAR)
(Fig. 6(5)), Anahamulina subcylindrica (D’ORBIGNY)
(Fig. 6(9)), “Barremites” uhligi (HAUG sensu SARASIN
and SCHÖNDELMAYER), Discoidellia favrei (OOSTER)
and Lytoceras densifimbriatum UHLIG also appear at this
level. At the same time, D. vermeuleni and other long-
ranging taxa such as Nl. subgrasianum, L. subfimbriatum
and Ph. winkleri disappear.
This faunal turnover coincides with the start of an organic-
rich interval that, because of its sedimentologic and palaeon-
tologic characteristics, can be considered the equivalent of
the Faraoni Level, recognised in a similar stratigraphic posi-
tion in central and northern Italy and southeastern France
(Cecca et al., 1994; Cecca et al., 1996; Baudin et al., 1999).
2.2.3. Pseudothurmannia picteti Subzone
The base of this subzone is defined by the appearance of
Ps. picteti, the youngest and more involute species of the
genus Pseudothurmannia. Apart from the index species,
which is restricted to the lower part of the subzone, the fauna
from this interval is not well characterised. Small and hardly
interpretable heteromorphs are frequent, among which we
have identified Paraspinoceras morloti (OOSTER)
(Fig. 6(8)), a probable senior synonym of Par. evolutus
(FALLOT and TERMIER). The first true Barremites, attrib-
Fig. 5.1. Crioceratites balearis (NOLAN), X.Ag1.131.7, Cr. balearis Subzone. 2. Crioceratites balearis (NOLAN), X.G.6.10, Cr. balearis Subzone. 3.
Crioceratites balearis (NOLAN), X.G.6.4, Cr. balearis Subzone. 4. Crioceratites binelli (ASTIER), X.EC.3.1, Cr. binelli Subzone. 5. Crioceratites
majoricensis (NOLAN), X.EC.4.1, Cr. binelli Subzone. 6. Crioceratites krenkeli (SARKAR), X.G1.2.1, Cr. krenkeli Subzone. 7. Crioceratites krenkeli
(SARKAR), X.G1.(5-7).1, Cr. krenkeli Subzone. 8. Crioceratites krenkeli (SARKAR), X.G1.6.1, Cr. krenkeli Subzone. 9. Crioceratites angulicostatus
(D’ORBIGNY), X.V1.-2.65, Cr. angulicostatus Subzone. 10. Crioceratites angulicostatus (D’ORBIGNY), X.V1.-4.15, Cr. angulicostatus Subzone. 11.
Acrioceras meriani (OOSTER), X.Ag1.145.30, Ps. ohmi Subzone. (All specimens natural size).
Fig. 5. 1. Crioceratites balearis (NOLAN), X.Ag1.131.7, Sous-Zone à Cr. balearis.2. Crioceratites balearis (NOLAN), X.G.6.10, Sous-Zone à Cr. balearis.
3. Crioceratites balearis (NOLAN), X.G.6.4, Sous-Zone à Cr. balearis.4. Crioceratites binelli (ASTIER), X.EC.3.1, Sous-Zone à Cr. binelli.5. Crioceratites
majoricensis (NOLAN), X.EC.4.1, Sous-Zone à Cr. binelli.6. Crioceratites krenkeli (SARKAR), X.G1.2.1, Sous-Zone à Cr. krenkeli. 7. Crioceratites krenkeli
(SARKAR), X.G1.(5-7).1, Sous-Zone à Cr. krenkeli.8. Crioceratites krenkeli (SARKAR), X.G1.6.1, Sous-Zone à Cr. krenkeli.9. Crioceratites angulicostatus
(D’ORBIGNY), X.V1.-2.65, Sous-Zone à Cr. angulicostatus.10. Crioceratites angulicostatus (D’ORBIGNY), X.V1.-4.15, Sous-Zone à Cr. angulicostatus.
11. Acrioceras meriani (OOSTER), X.Ag1.145.30, Sous-Zone à Ps. ohmi. (Tous les échantillons sont figurés en grandeur naturelle).
691M. Company et al. / Geobios 36 (2003) 685–694
692 M. Company et al. / Geobios 36 (2003) 685–694
utable to B. dimboviciorensis BRESKOVSKI, also appear in
this interval. The forms described by Cecca et al. (1998) as B.
primitivus,coming from the Faraoni Level,are interpreted by
us as a variety of Ps. subdiffıcilis.
2.3. Hauterivian/Barremian boundary
According to the current definition (Rawson, 1996), the
first occurrence of Taveraidiscus hugii (OOSTER)
(Fig. 6(10)) marks the lower boundary of the Barremian
stage. This event forms a part of a major faunal renewal that
begins in the upper part of the Ps. picteti Subzone. Other
species such as T. intermedius (D’ORBIGNY) (Fig. 6(11))–
here considered a senior synonym of T. vandeckii (OOSTER)
and T. kiliani (PAQUIER) – “Barremites” boutini
(MATHERON), Silesites sp., Psilotissotia mazuca (CO-
QUAND), Arnaudiella malladae (NICKLÈS) and Hamulin-
ites munieri (NICKLÈS) also appear around this level.
Hoedemaeker (1995) argued that the Haute
rivian/Barremianboundary should be drawn at the base of his
Ps. catulloi Subzone, equivalent to the base of our Ps. mor-
tilleti Subzone. This author considered this level to separate
an assemblage of reputedly Hauterivian ammonites from an
assemblage composed mostly of Barremian species. Never-
theless, some of the taxa, which, according to Hoedemaeker,
would appear in the Ps. catulloi Subzone, are actually
present in lower levels.This is the case of Ab. neumayri and
the genera Paraspiticeras, Emericiceras and Acrioceras.
Moreover, Ps. subdiffıcilis is still present throughout the Ps.
mortilleti Subzone, being substituted by B. dimboviciorensis
in the Ps. picteti Subzone. It is also worth mentioning that the
assemblages from the Ps. mortilleti Subzone are composed
for the most part of specimens of Pseudothurmannia (63% of
the whole) and Plesiospitidiscus and other long-ranging taxa
inherited from lower levels (12%), giving these assemblages
a marked Hauterivian look.
3. Taxonomic note
On establishing the genus Pseudothurmannia,Spath
(1923) designated Am. angulicostatus D’ORBIGNY (in Pic-
tet, 1863: Pl. 1bis, Fig. 1) as “genotype”. Sarkar (1955)
however, showed that Pictet’s specimen could not be conspe-
cific with Am. angulicostatus D’ORBIGNY and separated it
as a new species Ps. picteti SARKAR. Moreover, as shown
above, the species of d’Orbigny is closer to Crioceratites
species than to the forms currently included in the genus
Pseudothurmannia. We believe that Article 70.3 of the
I.C.Z.N. is applicable to this case. According to it, and in
order to maintain the usage, we designate Ps. picteti
SARKAR as type species of the genus Pseudothurmannia.
Acknowledgements
We are very grateful to our colleagues Ph. Hoedemaeker
(Nationaal Natuurhistorisch Museum, Leiden), G. Schairer
(BayerischeStaatssammlung für Paläontologie, Munich)and
D. Decrouez (Muséum d’histoire naturelle, Geneva) for hav-
ing provided us with casts of the holotypes of Cr. angulicos-
tatus, Ps. ohmi and Ps. picteti. Critical comments of F.
Atrops and P.F. Rawson are also gratefully appreciated. This
work has been co-financed by Project BTE 2001-3020
(Spanish Ministry of Science and Technology) and Research
Group RNM-178 (Junta de Andalucía).
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694 M. Company et al. / Geobios 36 (2003) 685–694
... In a given basin where multiple sections have been studied, it is possible to assess and minimize the uncertainties linked to the quality of preservation of the paleontological record provided the lithological changes can be correlated. This is the case for the Vocontian Basin and the Subbetic Domain, where remarkable bundles have been correlated through the basin (Cotillon, 1971;Company et al., 2003;Gréselle and Pittet, 2010;Martinez et al., 2020a;Kenjo et al., 2021;Aguado et al., 2022;Figs. 6-8). ...
... In the Hauterivian Stage, the Tethyan and Andean Ammonite zonation are available in Bulot et al. (1992), Reboulet and Atrops (1999), Hoedemaeker and Leereveld (1995), Company et al. (2003Company et al. ( , 2005, Martinez et al. (2012), Aguado et al. (2014) and Aguirre-Urreta et al. (2017 and calcareous nannofossil data are from Thierstein (1973), Gardin (2008), Hoedemaeker and Leereveld (1995), Company et al. (2003) and Aguado et al. (2014). Correlation between the Andean and Tethyan Ammonite zones is necessary to anchor the astrochronology of the Tethyan areas (where the stage boundaries are defined) to the Andean radio-astrochronology (where U-Pb ages are available; Aguirre-Urreta et al., 2017). ...
... In the Hauterivian Stage, the Tethyan and Andean Ammonite zonation are available in Bulot et al. (1992), Reboulet and Atrops (1999), Hoedemaeker and Leereveld (1995), Company et al. (2003Company et al. ( , 2005, Martinez et al. (2012), Aguado et al. (2014) and Aguirre-Urreta et al. (2017 and calcareous nannofossil data are from Thierstein (1973), Gardin (2008), Hoedemaeker and Leereveld (1995), Company et al. (2003) and Aguado et al. (2014). Correlation between the Andean and Tethyan Ammonite zones is necessary to anchor the astrochronology of the Tethyan areas (where the stage boundaries are defined) to the Andean radio-astrochronology (where U-Pb ages are available; Aguirre-Urreta et al., 2017). ...
... They were notably the consequence of humid-arid cycles forced by insolation cycles . High amount of macro-and microfossils allow the Tethyan ammonite and calcareous nannofossil zones and subzones to be precisely bounded (Hoedemaeker and Leereveld, 1995;Company et al., 2003; Aguado Barrier et al., 2018). B, Picture of the Barranco Cavila section in the Sartousiana Zone with interpretations of the 100-kyr eccentricity cycles (labelled "e" in the figure). ...
... The quality of the record of the Milankovitch cycles in the Subbetic Domain represents an opportunity to provide much more precise constraint on the duration of the Barremian Stage that can be integrated in a broader stratigraphic scheme. Notably, strata in the Subbetic Domain can be correlated sometimes bed-to-bed with other sections in the Subbetic Domain (Company et al., 2003;Aguado et al., 2014a) and with the Vocontian Basin (Hoedemaeker and Herngreen, 2003). We here performed spectral analyses on high-resolution magnetic susceptibility and CaCO 3 content curves in two sections of the Subbetic Domain to identify the record of the Milankovitch cycles and precise the duration of the Barremian Stage and its biostratigraphic subdivisions. ...
... Arroyo Gilico is a 75-m thick section, which stratigraphically ranges from the uppermost Hauterivian to the lowermost upper Barremian. Data on ammonite, calcareous nannofossil and planktic foraminifera biostratigraphy and isotope stratigraphy of this section have been published in several previous papers (Company et al., 2003;Aguado et al., 2008;Aguado et al., 2014a;Premoli Silva et al., 2018). Barranco de Cavila is a 70-m thick section covering the upper Barremian and the lowermost Aptian. ...
Article
The ages and durations of the stages in the Early Cretaceous commonly show discrepancies of several million years when the Geologic Time Scale (2020) from the International Commission of Stratigraphy (ICS) and recently published radio-astrochronologic data are compared. Here, we provide an astronomical time scale for the Barremian Stage and its subdivisions based on spectral analyses performed on magnetic susceptibility and calcium carbonate content series in two sections studied located in the Subbetic Domain of southeastern Spain. The sections are tied to Tethyan ammonite and calcareous nannofossil zones, allowing detailed correlations with other sections in the Subbetic Domain and other basins in the Tethyan Realm. Eccentricity cycles are observed throughout the series and can be correlated with the eccentricity cycles observed in other sections in the Subbetic Domain, showing that the results are reproducible. Based on the number of 405-kyr eccentricity cycles in the study interval, and considering uncertainties linked to variations in the sedimentation rates within an eccentricity cycle, the duration of the Barremian Stage is calculated at 4.58 -0.29 +0.15 Myr. From the astronomical time scale proposed here, together with recently published radio-astrochronological studies, the base of the Barremian Stage is dated at 125.98 ± 0.21 Ma and the top at 121.40 ± 0.34 Ma. The age of the Barremian/Aptian boundary differs from the ICS Geologic Time Scale 2020 by 3.6 Myr, but fits with the age of the base of magnetochron M0r recently deduced from a synthesis of radiochronologic data. The episodes of environmental change of the late Hauterivian–Barremian show an average pacing of 2.2 Myr, suggesting an orbital control on the expansion of oceanic anoxic conditions in the Tethys.
... OCCURRENCE: According to , B. binelli occurs in the Upper Hauterivian in the balearis Zone in France, Spain, Hungary, Romania, and in Crimea (Ukraine), with the addition of Slovakia and the Eastern Alps. Company et al. (2003) cites the occurrence of B. binelli in the lower part of the balearis Zone in Spain, whereas Leroy et al. (2017) -as a horizon in the middle part of the balearis Zone. According to Reboulet et al. (2018), the occurrence is in the binelli Subzone (lower part of the balearis Zone ...
Article
Butkov Quarry provides the best exposed stratigraphic sequence of marly limestones with Early Cretaceous ammonites in the Manín Nappe of the Central Western Carpathians. The presented paper deals with the sporadically occurring zonal ammonites, or ammonites of guiding character, from the Lower Valanginian to Upper Hauterivian. Sixteen species are taxonomically elaborated here in detail. More attention is given to the basic taxonomy of the Subfamily Crioceratitinae Gill, 1871. The species described here, like most of the previously published species from Butkov Quarry, are representatives of the Mediterranean bioprovince and are close to the ammonite association from the Vocontian Basin.
... According to Company et al. (1995) Paraspiticeras and Hamulinites are long-ranging taxa which first appeared in the Pseudothurmannia angulicostata Zone (now the Pseudothurmannia ohmi Zone) in the Betic Cordillera, but later the first Paraspiticeras were recorded from a lower level e the upper part of the Balearites balearis Subzone (Company et al., 2003). This suggests a possible correlation of the base of the bituberculatum Zone with this level (Fig. 13). ...
Article
The Paraspiticeras groeberi Zone is one of the five ammonoid biozones previously recognized in the Agua de la Mula Member of the Agrio Formation of late Hauterivian age in the Neuquén Basin of west-central Argentina. However, the ammonoid faunas of this zone and the beds immediately below, corresponding to the upper levels of the current Crioceratites diamantensis Zone, remain poorly known. Extensive collections now allow us to recognize a diverse endemic ammonoid fauna. After an exhaustive taxonomic and stratigraphic review, the Paraemericiceras argentinense and Paraspiticeras bituberculatum Zones are proposed to replace the P. groeberi Zone and the original index species is now placed in Vutacuracrioceras gen. nov. Vutacuracrioceras groeberi first appears with the earliest Paraemericiceras argentinense gen. et sp. nov. and extends through both zones. It is joined in the Paraspiticeras bituberculatum Zone by the index species and Paraspiticeras sp. aff. P. precrassispinum, Australopseudothurmannia flexuosa gen. et sp. nov. and Hamulinites sp. Based on this new biostratigraphic scheme, the late Hauterivian in the Neuquén Basin is represented now by six ammonoids zones that can be correlated provisionally with the European standard of the West Mediterranean Province of the Tethyan Realm
... The upper part of this unit is made up of clayey limestone beds with two grey laminated limestone beds capped by a marlstone bed. Dothurmannia mortilleti subzone has been recognized in this third double calcareous bar (Company et al. 2003) and within the F-OAE. ...
Article
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Within the Valanginian–Hauterivian series of the northern Tethyan margin, two organic-rich laminated black shale intervals corresponding to the Valanginian Weissert and the late Hauterivian Faraoni oceanic anoxic events (W-OAE and F-OAE, respectively) are well documented. However, in Tunisia as part of the southern Tethyan margin, despite several biostratigraphic and structural studies awarded to this period, geochemical characterization based mainly on wireline logs data was undertaken. Here, we aimed to confirm the extension of these Valanginian–Hauterivian organic-rich deposits throughout a bulk and biomolecular geochemical (Rock–Eval pyrolysis and gas chromatography–mass spectrometry analysis) study carried out on selected surface outcrops in northern Tunisia. To that end, three hemi-pelagic sections belonging to the Tunisian backbone (Jebel Zaghouan), the Tunisian trough (Jebel Oust) and the diapiric zone (Jebel Boulahouajeb) have been chosen and analysed with highly interest to their organic matter (OM) contents and biomolecular composition. Rock–Eval pyrolysis shows that Jebel Oust section presents total organic carbon (TOC) contents ranging from 0.18 to 0.57 wt% with an average of 0.38 wt% and low hydrogen index (HI) values ranging from 15 to 74 mg HC/g TOC indicating a type IV OM. Its hydrocarbon generation potential (HGP) is very low where the average value is around 0.19 mg HC/g rock, while Jebel Zaghouan section reveals TOC values reaching up to 0.56 wt% with a low HGP up to 1.01 mg HC/g rock and high maturity levels attested by Tmax values ranging from 449 to 460 °C. Jebel Boulahouajeb section shows low TOC values ranging from 0.22 to 0.69 wt% with an average of 0.35 wt%. Its HGP is very low with a maximum value of 1.67 mg HC/g rock and presents marginally mature to mature stage where Tmax values ranging from 438 to 450 °C with an average of 443 °C. This maturity distribution was guided by the basin architecture marked by the presence of subsiding zones in local faulted blocks and palaeohighs occupied by Triassic salt domes and horsts. Molecular biomarker analyses from the Valanginian–Hauterivian Boulahouajeb and Jebel Zaghouan facies indicated a mainly marine origin of the OM and a suboxic depositional environment in a normal marine water column. Throughout this study, we confirm the installation, in the southern Tethyan margin (northern Tunisia), of dysoxic depositional conditions during the early Valanginian and late Hauterivian times corresponding to the Weissert and Faraoni events, respectively. However, these depositional environments were not favourable for preservation of high quantities of OM. This was mainly controlled by the presence of an oxygen minimum zone generally disturbed by detrital discharges. Additionally, the results highlight the important interplay of the basin architecture, the various faults developed with an extensional tectonic regime during the Valanginian–Hauterivian period, the warm climate conditions and the eustatic sea-level variations where transgressive systems tracts coincide with black shales deposited majorly under dysoxic conditions.
... emericii. The ammonites are typical for the HauterivianeBarremian of the Tethys (Dimitrova, 1967;Obata et al., 1982;Company et al., 2003) and inoceramids are characteristic in the Hauterivian and Barremian (Anderson, 1938;Pergament, 1965;Pokhialainen, 1994). Thus, the Primanka Formation is considered as HauterivianeBarremian. ...
Article
Upper Mesozoic (Upper Jurassic and Cretaceous) rocks are widely distributed in Sikhote-Alin (Russian Far East) and northeastern China. In Sikhote-Alin, the Upper Jurassic and Lower Cretaceous rocks are represented mainly by marine deposits, whereas the Upper Cretaceous rocks are mainly volcanic and non-marine sedimentary-volcanic. In northeastern China, the upper Mesozoic rocks are, on the contrary, mainly non-marine. Fully marine Upper Jurassic – Valanginian deposits are restricted to the northeastern Heilongjiang Province near the border with Russia. Barremian-Albian non-marine deposits alternating with marine ones also occur in this region. They contain marine and non-marine fauna and, therefore, represent an important object for non-marine and marine correlation. On the rest of the territory of northeastern China, upper Mesozoic rocks are represented by non-marine sedimentary and volcanogenic deposits. The complex geological structure of the region as well as different types of sedimentary basins cause difficulties in correlation between the upper Mesozoic rocks of Sikhote-Alin and northeastern China. Despite the long history of investigations, their correlation schemes are still rare. Creation of a correlation scheme between Sikhote-Alin and northeastern China should be based on revision of published stratigraphic data on both regions. This article is the first in a series of articles devoted to the upper Mesozoic stratigraphy of Sikhote-Alin and northeastern China. In the present article the Upper Jurassic – Hauterivian stratigraphy of Sikhote-Alin and northeastern China is reviewed. The Upper Jurassic – Hauterivian deposits of Sikhote-Alin and northeastern China contain abundant Buchia and rarer ammonites. Based on stratigraphic distribution of buchiid assemblages, the correlation scheme for Kimmeridgian – Valanginian (possibly lowermost Hauterivian) strata of northeastern China and Sikhote-Alin is proposed. The succession of Jurassic-Cretaceous buchiid assemblages of Sikhote-Alin and northeastern China is similar to those of the other regions, e.g., Northern Siberia (Arctic Realm) and California (North Pacific Realm).
Article
Full-text available
The 7th meeting of the IUGS Lower Cretaceous Ammonite Working Group the ‘Kilian Group (KG)’ was held in Warsaw, Poland, in 21st August 2022. Need of major changes for the Jurassic/Cretaceous transition, namely to the uppermost Tithonian and lower Berriasian, and for the upper Aptian and Albian schemes is a long–known issue, which are finally conceptualized and hereby introduced into the Standard Mediterranean Ammonite Zonation (SMAZ, Western Tethys). Besides, refinements were added to the Valanginian and Hauterivian stages, discussion on some zonal indices and units are also provided. The KG highlights again the exclusive use of interval zones and subzones. Most important changes of the uppermost Tithonian–Berriasian stages are the followings: i) use of two folded Berriasian is agreed, to be in better accordance with ammonite turnovers and microfossil framework; ii) uppermost Tithonian Lopeziceras chaperi, top–uppermost Tithonian to lowermost Berriasian Praedalmasiceras progenitor and lower Berriasian Pseudosubplanites grandis Zones are accepted to be introduced into the SMAZ, these three zones to cover the former ‘Berriasella’ jacobi Zone auctorum which is formally abandoned; iii) lower Berriasian Delphinella delphinensis Subzone is accepted as a reliable marker level of the upper Praedalmasiceras progenitor Zone; iv) Strambergella jacobi Zone is established and discussed. Tirnovella occitanica Zone and Tirnovella subalpina Subzone are discussed. Modifications on the Valanginian zonation are the followings: i) Neocomites premolicus Subzone is re–defined, ii) Neolissoceras (Vergoliceras) salinarium Subzone is introduced; iii) Neocomites neocomiensiformis Zone is divided into two subzones, the lower N. neocomiensiformis and the upper Busnardoites campylotoxus Subzones. Modifications on the Hauterivian stage are the followings: i) all horizons are deleted; ii) Olcostephanus (Olcostephanus) variegatus Subzone is introduced; iii) Balearites angulicostatus Subzone is introduced; iv) all subzonal index–species of the B. balearis Zone are assigned to genus Balearites; v) Pseudothurmannia mortilleti is considered as a senior synonym of P. catulloi, therefore its nominal subzone also changed its name to mortilleti. No change in the Barremian scheme, however the base of Toxancyloceras vandenheckii Subzone and Zone is defined by the first appearance of the genus Toxancyloceras. Most important changes of the upper Aptian zonation are the followings: i) Nolaniceras nolani and Hypacanthoplites jacobi zones are retained from the SMAZ; ii) re–introduction of Diadochoceras nodosocostatum Zone is given. For the Aptian–Albian transition interval, introduction of ‘Hypacanthoplites’ elegans Zone is accepted, where the Aptian/Albian boundary lies within. Most important zonal changes of the Albian stage are: i) the Leymeriella−based succession is abandoned from the SMAZ and replaced by the cosmopolitan Douvilleiceras−based succession; ii) Douvilleiceras leightonense Zone is introduced; iii) middle Albian Hoplites dentatus, Euhoplites loricatus, Euhoplites lautus zones and Hoplites spathi Subzone are retained from the SMAZ and restricted to the Boreal ammonite scheme; iv) Lyelliceras lyelli Subzone arisen to zonal rank defining the basal middle Albian; v) Oxytropidoceras (Oxytropidoceras) roissyanum Zone is introduced; vi) upper Albian zonation based on the phyletic lineage of Mortoniceratids is kept, however generic names of the indices are modified to Pervinquieria; vii) Pervinquieria pricei Zone is divided into three subzones of Hysteroceras varicosum, H. binum and H. choffati from the oldest to youngest; viii) Pervinquieria inflata Zone is divided into two subzones of Hysteroceras bucklandi and Cantabrigites spp. The KG tributes to our recently deceased ammonitologist colleagues in the Supplement, a discussion on the future work is provided. The next Kilian Group meeting will be held in Hannover, prior to the first day of the 12th International Symposium on the Cretaceous System.
Article
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A detailed study of calcareous nannofossil assemblages from twelve uppermost lower Barremian–lower Aptian sections in the Subbetic domain of the Betic Cordillera was performed. Seven new nannofossil species (Crucibiscutum bastetanum, Crucibiscutum gracile, Chiastozygus lamprostauros, Cyclagelosphaera platyaspis, Lithraphidites aichmoides, Lithraphidites pugio, and Rhagodiscus sicutclipeus) are described, one species is emended (Lithraphidites magnus) and the taxonomic concept of the marker species Hayesites irregularis is discussed and clarified. The detailed stratigraphic ranges of the new species, together with those of other relevant taxa, are determined and correlated to standard ammonite biostratigraphy. Age estimates of biostratigraphically relevant calcareous nannofossil biohorizons are calculated using astrochronologically tuned cyclostratigraphic data. Five new calcareous nannofossil subzones are proposed which enhance upper Barremian biostratigraphic resolution at a regional scale and are directly correlated with respect to the standard Tethyan ammonite zonation. Two of the new species described here are used as biostratigraphic markers for the newly proposed subzones. The duration of each subzone is provided through astrochronological calibration. This study allows the refinement of the calcareous nannofossil zonation for the Mediterranean–Atlantic province of the Tethyan domain. The implications of these new results are discussed regarding the extant definition and use of the Barremian/Aptian boundary. The morpho-evolutionary trends of selected nannofossil groups are reviewed in relation to the latest Barremian–Aptian paleogeographic changes, showing these were a prominent factor controlling calcareous nannoplankton evolution and biogeographical distribution in the west European-Atlantic region.
Article
The lower part of the Lower Cretaceous Bolos Sandstone Formation as exposed in the Barranco de la Muela section (Sierra de la Muela Range, southeastern Spain) yields two species of ornamented nautiloids, Cymatoceras neocomiense and Eucymatoceras plicatum. These have been collected together with other cephalopods (ammonoids, belemnites) and different invertebrates (corals, brachiopods, bivalves, gastropods, echinoids). This fossil assemblage includes numerous large macroconchs of the ammonite Pseudothurmannia mortilleti, here considered as a senior synonym of P. catulloi, index species of the homonymous subzone of the upper Hauterivian “Pseudothurmannia ohmi” Zone. On this basis, the here reported findings constitute the first biostratigraphically well-constrained records of C. neocomiense and E. plicatum, namely in the Pseudothurmannia catulloi Subzone. The presence of these two ornamented and relatively depressed nautiloids in fine sandstone levels interbedded with sandy marls of the Bolos Formation, together with the palaeoecological characteristics of the associated fauna suggest a nearshore to inner-middle shelf, shallow to moderately deep palaeoenvironment with mixed siliciclastic-carbonate sedimentation, and high to moderate energy.
Article
Hemihoplitidae evolution is well documented in the north-west Tethyan margin at the lower upper Barremian. In this context, the genus Lenicostites gen. nov. (L. rusticus), with ‘hemihoplitid-like’ morphology, is unexpected because of its age older than the earliest Hemihoplites and its evolutionary stasis that contrasts with the rapid changes of the Hemihoplitidae. Data show no connection between Hemihoplitidae and Lenicostitidae fam. nov. and the resemblance is homeomorphy. The numerous reported occurrences of Hemihoplitinae over the world are reviewed. Their critical revision shows that some of them are contradictory with the evolutionary history of the group. The ‘hemihoplitid-like’ morphology is iterative in several taxa without any phyletic links (homeomorphy). Reasons could be linked to the morphospace occupation in the zone of maximum equilibrium between different constraints (a Pareto-optimal solution), making such morphology effortless to reproduce. The Austral Homeomorphitinae subfam. nov. (with Homeomorphites aguirreurretae gen. nov. et sp. nov.) are assigned to the Neocomitidae. A phyletic link between Shasticrioceras and Antarcticoceras is suggested (Shasticrioceratidae fam. nov.). Until proven otherwise, there is no Hemihoplitinae outside the north and west margins of the Tethys (including the Essaouira Basin). Homeomorphy between Hemihoplitinae and Lenicostitidae fam. nov. is explored and convergence seems the most convincing hypothesis. The further appearance of Camereiceras (Hemihoplitinae) could establish favorable conditions for interspecific competition, and the disappearance of Lenicostites gen. nov. could be interpreted as a complete competitive replacement. In this hypothesis Lenicostites gen. nov. is a victim of the Gause Principle as it lost the Red Queen race.
Article
Full-text available
Inter-regional correlation in the Barremian is impossible because of strong biotic differentiation between realms coupled with a lack of obvious non-biostratigraphic markers to provide good boundaries. Thus we have chosen the best of the limited options available to define boundaries within the Tethyan Realm. We recommend that the base of the Barremian be placed at the base of the Spitidiscus hugii ammonite Zone in the Rio Argos section, SE Spain. Supplementary information will be compiled to fully document this choice before formal submission via the Cretaceous Subcommission to the Commission on Stratigraphy. The base of the Upper Barremian should be defined by the first appearance of the ammonite Ancyloceras vandenheckei in one of the Subbetic sections in SE Spain, probably section X.KV (Barrano de Cavila, Caravaca). Other sections in the region require further documentation before the final recommendation can be made.
Article
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This report is the synthesis of the discussions held during the 2nd W orkshop of the Lower Cretaceous Cephalopod Team of IGCP-Project 262: Tethyan Cretaceous Correlation (Mula, SE Spain, July 2-5, 1992). It presents a new proposition of zonal scheme fór the Lower Cretaceous of the M editerranean Region and justifications about the choice of the index-species fór somé biostratigraphical units. RESUMEN Se presentan las conclusiones dél " 2nd W orkshop of the Lower Cretaceous Cephalopod Team of IGCP-Project 262: Tethyan Cretaceous Correlation " , celebrado en M ula (SE de Espana) durante los días 2 al 5 de julio de 1992. Se incluye la propuesta de un nuevo esquem a zonal basado en am m onites para el Cretácico Inferior dél ámbito mediterráneo, así como notas aclaratorias sobre la elección de las especies índice de algunas unidades bioestratigráficas.