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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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