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Introduction
The location of Cuba within the Caribbean plate, offers a good
point of reference to compare and establish links between the
geological and biological processes in the Eastern and West-
Calpionellid distribution and microfacies across the Jurassic/
Cretaceous boundary in western Cuba (Sierra de los Órganos)
RAFAEL LÓPEZ-MARTÍNEZ
1,
, RICARDO BARRAGÁN
1
, DANIELA REHÁKOVÁ
2
and
JORGE LUIS COBIELLA-REGUERA
3
1
Instituto de Geología, Universidad Nacional Autónoma de México, Ciudad Universitaria, Delegación Coyoacán, C.P. 04510, México
D.F., México; rafaelopez83@hotmail.com
2
Comenius University, Faculty of Natural Sciences, Department of Geology and Paleontology, Mlynská dolina G, 842 15 Bratislava,
Slovak Republic; rehakova@fns.uniba.sk
3
Departamento de Geología, Universidad de Pinar del Río, Martí # 270, Pinar del Río, C.P. 20100, Cuba
(Manuscript received May 21, 2012; accepted in revised form December 11, 2012)
Abstract: A detailed bed-by-bed sampled stratigraphic section of the Guasasa Formation in the Rancho San Vicente
area of the “Sierra de los Órganos”, western Cuba, provides well-supported evidence about facies and calpionellid
distribution across the Jurassic/Cretaceous boundary. These new data allowed the definition of an updated and sound
calpionellid biozonation scheme for the section. In this scheme, the drowning event of a carbonate platform displayed
by the facies of the San Vicente Member, the lowermost unit of the section, is dated as Late Tithonian, Boneti Subzone.
The Jurassic/Cretaceous boundary was recognized within the facies of the overlying El Americano Member on the basis
of the acme of Calpionella alpina Lorenz. The boundary is placed nearly six meters above the contact between the San
Vicente and the El Americano Members, in a facies linked to a sea-level drop. The recorded calpionellid bioevents
should allow correlations of the Cuban biozonation scheme herein proposed, with other previously published schemes
from distant areas of the Tethyan Domain.
Key words: Jurassic/Cretaceous boundary, Cuba, calpionellid biostratigraphy, microfacies, drowned platform, storm
deposits.
tributed to the topic, especially Furrazola-Bermúdez &
Kreisel (1973), who recognized the presence and stratigraphic
distribution of the Crassicollaria and Calpionella Zones in
some sections of western Cuba, and reported a new species
of Chitinoidella. However, in their study, they did not pro-
Fig. 1. Map showing the location of the Rancho San Vicente stratigraphic section and the main tec-
tonic units and structures of western Cuba. Modified from Cobiella-Reguera & Olóriz (2009).
ern Tethys during the Mesozoic,
particularly those at the Juras-
sic—Cretaceous interval. Sev-
eral good successions of the
Tithonian/Berriasian boundary
interval of western Cuba are
well-exposed in the Pinar del
Río Province. They are essen-
tially recorded on the Guasasa
Formation, a typical unit of the
San Vicente stratigraphic sec-
tion at “Sierra de los Órganos”
orogenic belt (Fig. 1).
Pioneering works on the def-
inition of the Jurassic/Creta-
ceous boundary in western
Cuba on the basis of ammo-
nites, calpionellids and other
microfossils were focused on
stratigraphic sections across the
“Sierra de los Órganos”. The
first
contribution
was
by
Brönnimann in 1954. Since
then, several authors have con-
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duce sound data to establish the Jurassic/Cretaceous bound-
ary in Cuba by means of calpionellids. Later, Pop (1976)
analysed three sections in the “Sierra de los Órganos” belt
defining calpionellid zones and concluded that the Jurassic/
Cretaceous boundary in this area could be established at the
base of the Calpionella Zone. Pszczółkowski (1978) subdi-
vided the Guasasa Formation into four members, namely in
stratigraphic order: San Vicente, El Americano, Tumbadero
and Tumbitas. That author placed the contact between the
San Vicente and El Americano Members as coincident with
the Kimmeridgian/Tithonian boundary, whereas the contact
between the El Americano and Tumbadero Members was con-
ceived as coincident with the Tithonian/Berriasian boundary.
Myczyński & Pszczółkowski (1990) kept the El Americano/
Tumbadero contact as coincident to the Tithonian/Berriasian
boundary on the basis of ammonites and microfossils. How-
ever, Fernández-Carmona (1998) in his unpublished Doctoral
Thesis placed the Tithonian/Berriasian boundary within the
uppermost strata of the El Americano Member. Afterwards,
Pszczółkowski & Myczyński (2003) pursued and accepted
that idea for some sections in western Cuba.
Pszczółkowski et al. (2005) identified calpionellid and
radiolarian zones in western Cuba and correlated them with
ammonite zones from the western Tethys. The last relevant
contribution to this topic in western Cuba is by Pszczółkowski
& Myczyński (2010), who analysed calpionellid and ammo-
nite assemblages, but no differences in age of the members of
the Guasasa Formation, neither the stratigraphic position of
the Jurassic/Cretaceous boundary within the unit were reported.
The present contribution focuses on calpionellid bio-
stratigraphy from the San Vicente to Tumbadero Members
within the Guasasa Formation in the San Vicente Section of
the “Sierra de los Órganos”. In order to specify the age of the
limits between its members, and to establish a reliable posi-
tion of the Tithonian/Berriasian boundary within the unit,
this work was based on a high resolution sampling.
Regional geological setting
According to Iturralde-Vinent (1997), the stratigraphy of
Cuba can be differentiated into two main domains associated
with different geological histories: the foldbelt (Early—Middle
Jurassic to Late Eocene) and the neoautochthonous. The
foldbelt is composed of elements detached from several old
tectonic plates, while the neoautochthonous was formed in
the North America Passive Margin after the accretionary
process that led to the formation of the foldbelt.
The nappe pile of the Guaniguanico Cordillera (Hatten
1967; Khudoley & Meyerhoff 1971; Piotrowska 1978;
Pszczółkowski 1978, 1994) is a great lens-shaped antiform
with five main tectonic sheets, each one with its own strati-
graphic sections (Cobiella-Reguera 2008). Pszczółkowski &
Myczyński (2010) referred to this nappe pile as the “Guani-
guanico megaunit” in which the Sierra de los Órganos occu-
pies the lowest structural position, whereas the Sierra del
Rosario unit contains the uppermost nappes (Fig. 1).
In previous works the Mesozoic paleomargin sections in
the Guaniguanico Cordillera were considered as exotic crustal
blocks or terranes (Iturralde-Vinent 1997; Pszczółkowski
1999) detached from the Maya Block. In the opinion of other
authors, a good correlation between the Mesozoic sections in
the southeastern Gulf of Mexico and western Cuba sheds
new light on the idea of an original juxtaposition between
both domains (Moretti et al. 2003; Cobiella-Reguera &
Olóriz 2009). However, Saura et al. (2008) considered west-
ern Cuban facies as a distal expression of the development of
the Bahamas-Florida margin.
Lithostratigraphy
The rock sequences of the Jurassic-Cretaceous boundary
transition in western Cuba are exposed in the “Sierra de los
Órganos”, and recognized within the facies of the Guasasa
Formation (Pszczółkowski 1978, 1999). This unit defined by
Herrera (1961) was subdivided by Pszczółkowski (1978)
into four members, which are named in stratigraphic order as
San Vicente, El Americano, Tumbadero and Tumbitas
(Fig. 2). Pszczółkowski & Myczyński (2010), correlated the
members with ammonites and calpionellid biostratigraphy as
shown on Fig. 3. In the section we studied, the upper part of
the San Vicente, the whole El Americano and Tumbadero and
the lowermost part of the Tumbitas Members are recorded.
San Vicente Member
This unit is of Kimmeridgian—Early Tithonian age accord-
ing to Pszczółkowski & Myczyński (2010), and is mainly
composed by massive thick-bedded shallow-water carbon-
ates. A diagnostic feature of this unit is represented by par-
tially dolomitized limestones at the top. The fossils recorded
within this unit, mainly consist of Nerinea sp., Textulariidae
(Pszczółkowski 1978), miliolids, and scarce calcareous di-
nocysts (Fernández-Carmona 1998).
El Americano Member
It is composed of thin-bedded limestones with shaly inter-
beds. The fossil record includes calpionellids and ammonites
in the topmost Tithonian and in the Berriasian (Fernández-
Carmona 1998; Pszczółkowski et al. 2005).
Tumbadero Member
It is represented by thin-bedded limestones of Middle—
Late Berriasian age with very thin cherty beds and lenses. A
rich association of radiolarians and calpionellids indicates
the pelagic origin of the limestones of this member
(Pszczółkowski & Myczyński 2003).
Tumbitas Member
It is mainly composed of thick-bedded, light microgranular
limestones, with a few clay interbeds. The field diagnostic cri-
teria to discriminate the Tumbadero and the Tumbitas Mem-
bers are the disappearance of the cherty lenses and the light
colour of the limestones. The stratigraphic section studied in
this work includes only a small lower part of this member.
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Materials and methods
The present research focuses on the stratigraphic interval
from the topmost part of the San Vicente to the topmost part of
the Tumbadero Members. The sampling was done on a bed-
by-bed basis, including inter-layers. The samples RSV A—M
correspond to the San Vicente Member, RSV 1—95 to the
El Americano Member, and RSV 95—145 to the Tumbadero
Member (see Fig. 9 for detailed samples position).
Biostratigraphic results
Early Tithonian Semiradiata dinocyst Zone (Samples
RSV A—M)
These samples at the top of the San Vicente Member corre-
spond to the lower part of the studied section (Fig. 9). In thin
section the rocks are characterized as poorly sorted and washed
wackestones (occasionally non-fossiliferous mudstones) of in-
traclasts, peloids and pellets, alternating with peloidal pack-
stones (Fig. 4A). The main skeletal particles are benthic
foraminifers, favreinids, gastropods, green algae, ostracods
and scarce bryozoans. Some samples are partially dolomitized
with euhedral dolomitic crystals; bioturbation is abundant prin-
cipally due to incrustation. The rock displays cloudy structure
in thin section due to microbial activity. Biostratigraphic indi-
cators are very scarce and the age of the member was deter-
mined only by the presence of a few Cadosina semiradiata
semiradiata Wanner (Fig. 4B) which could determine the Early
Tithonian Semiradiata dinocyst Zone sensu Reháková (2000a).
Late Tithonian
Chitinoidella Zone
Boneti Subzone (Samples RSV 1—5)
These rock samples from the very base of the El Americano
Member (Fig. 9) consist of saccocomid mudstones to pack-
stones with less abundant filaments, glauconitic grains, few
gastropods and echinoids (Fig. 4C—F). This interval is charac-
terized by the presence of Chitinoidella along with other gen-
era displaying microgranular calcitic walls looking dark under
a transmitted light microscope. The Chitinoidella Zone is di-
vided into two subzones namely from bottom to top as Dobeni
and Boneti Grandesso (1977), Borza (1984). In the analysed
section only chitinoidellids of Boneti Subzone were found.
Specimens of Chitinoidellidae are scarce, being represented
only by a few poorly preserved specimens of Chitinoidella
boneti Doben (Fig. 4G), Longicollaria sp. (Fig. 4H), Daciella
sp. (Fig. 4I) and Daciella danubica Pop (Fig. 4J). The state
of preservation prevents observation of diagnostic features
of most of the specimens of this family. The matrix is always
microsparitic and masks other possible markers.
Nonetheless, this assemblage and the presence of Chiti-
noidella boneti Doben, provide a good point to identify the
Boneti Subzone sensu Borza (1984). The absence of the un-
derlying Dobeni Subzone is explained by paleoecological
reasons due to the shallow-water conditions prevailing be-
fore the drowning of the San Vicente carbonated bank.
Fig. 2. Correlation of Upper Jurassic and Berriasian lithostrati-
graphic units between the main tectonic domains of western Cuba.
Modified from Cobiella-Reguera & Olóriz (2009).
Fig. 3. Calpionellid and ammonite biostratigraphy of the Rancho San
Vicente section according to Pszczółkowski & Myczyński (2010).
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Fig. 4. Photomicrographs of thin-sections of the San Vicente and the lower part of the El Americano Members. A – Poorly sorted peloid
packstone—wackestone with micro-sparitic matrix. San Vicente Member, sample RSV-B; B – Cadosina semiradiata semiradiata Wanner.
Sample RSV-A; C – Glauconitic grains from the base of the El Americano Member. Sample RSV-1.2; D—F – Differently orientated sections
of Saccocoma sp. Sample RSV-5; G – Chitinoidella boneti Doben. Sample RSV-2; H – Longicollaria sp. Sample RSV-3; I – Daciella sp.
Sample RSV-5; J – Daciella danubica Pop. Sample RSV-4.
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The Boneti Subzone has been recorded with a similar as-
semblage from Cuba (Kreisel & Furrrazola-Bermúdez 1971;
Furrrazola-Bermúdez & Kreisel 1973), Mexico (Lugo 1975),
Western Balkanides (Bakalova 1977; Lakova 1993), Western
Carpathians (Borza 1984; Reháková & Michalík 1997),
Northwestern Anatolia (Altiner & Özkan 1991) and Eastern
Alps (Reháková 2002).
Late Tithonian
Crassicollaria Zone (Samples RSV 6—22)
An abrupt change in the facies occurs in this part of the
section still within the base of the El Americano Member
(Fig. 9). The Saccocoma packstones are replaced by wacke-
stones with sponges, radiolarians, calpionellids, filaments
and scarce resedimented gastropods and bryozoans
(Fig. 5A,B). In addition intercalations of grainstones to rud-
stones appear. The calcareous dinocysts are scarce and repre-
sented by Stomiosphaerina proxima Rěhánek (Fig. 5C,D).
The calpionellid association consists of the Crassicollaria and
Tintinnopsella and is represented by Crassicollaria colomi
Doben (Fig. 5E), Crassicollaria parvula Remane (Fig. 5F),
Crassicollaria massutiniana (Colom) (Fig. 5G), Crassicol-
laria brevis Remane (Fig. 5H), Crassicollaria intermedia
Durand-Delga (Fig. 5I), Tintinnopsella remanei (Borza)
(Fig. 5J), and small Tintinnopsella carpathica (Murgeanu &
Filipescu) (Fig. 5K). The Calpionella is scarce and recorded
only in the topmost part of the zone. The large forms such as
Calpionella grandalpina Nagy and Calpionella elliptalpina
Nagy were not found.
This interval is characterized by the taphonomic and sedi-
mentary condensation. The evidence of this condensation is
expressed by the mixture of different subzones of Crassicol-
laria Zone and glauconitic grains. This condensation prevents
the subdivision of Crassicollaria Zone in the studied section.
The topmost part of this interval is marked by storm de-
posits characterized by grainstones of peloids and resedi-
mented shallow-water fossils similar to those illustrated in
Fig. 6 (A,B).
Early Berriasian
Calpionella Zone
Alpina Subzone (Samples RSV 23—38)
The acme of small spherical forms of Calpionella alpina
Lorenz (Fig. 6C—E) marks a change in the assemblage com-
position and defines the base of the Calpionella Zone, its Al-
pina Subzone (sensu Remane 1986; Lakova 1994; Olóriz et
al. 1995; Pop 1996; Reháková & Michalík 1997; Houša et al.
1999; Boughdiri et al. 2006; Andreini et al. 2007; Wimbledon
et al. 2011; Michalík & Reháková 2011 and others) (Fig. 9).
The lower part of this zone is recognized as coincident with
the Tithonian/Berriasian boundary.
Another change is the abrupt decrease in the abundance of
Crassicollaria. Only a few scarce Crassicollaria parvula
Remane cross the Jurassic/Cretaceous boundary.
Microfacies show an evident relationship of this subzone
with storm deposits. These deposits began in the Crassicol-
laria
Zone and are very frequent in the lower part of the
Calpionella Zone.
The presence of these storm deposits and the considerable
amounts of resedimented fossils in the Jurassic/Cretaceous
boundary interval may be a response to a sea-level fall dur-
ing this period, with the consequent influence of the shallower
water conditions.
Thus, the Jurassic/Cretaceous boundary is placed within
the sample number 23, about 6 meters above the base of the
El Americano Member (Fig. 9).
Ferasini Subzone (Samples RSV 38—51)
Upwards within the El Americano Member, the base of the
Ferasini Subzone is characterized by the First Occurrence
(FO) of Remaniella ferasini Catalano (Fig. 6F,G) (Pop 1994,
1996; Reháková & Michalík 1997) (Fig. 9). This biostrati-
graphic unit has also been referred to as the Remaniella Sub-
zone (Olóriz et al. 1995).
Remaniella is scarce and very poorly preserved in the facies
studied. Due to the absence of collars only a few specimens
were identified. Nonetheless, the shape of the lorica of many
specimens resembles the type of the remaniellids. Calpionella
alpina Lorenz is frequent and dominates the assemblage. Tin-
tinnopsella carpathica (Murgeanu & Filipescu) (Fig. 6H) is
also frequent; there are also scarce Crassicollaria parvula.
The microfacies of this interval are radiolarian and calpio-
nellid mudstones to wackestones. The matrix is microsparitic
and dolomitized in some parts and, as a consequence, the col-
lars of the Remaniella are persistently damaged (Fig. 6I).
Abundant spores of Globochaete alpina Lombard were ob-
served (Fig. 6J). Dark organic matter and pyrite are present
in all intervals.
Elliptica Subzone (Samples RSV 52—83)
The FO of Calpionella elliptica Cadish (Fig. 7A) defines
the base of the Elliptica Subzone (Catalano & Liguori 1971;
Reháková & Michalík 1997) and is recognized herein to-
wards the top of the El Americano Member (Fig. 9). Calpio-
nella alpina Lorenz still dominates over other species.
Tintinnopsella carpathica (Murgeanu & Filipescu) is abun-
dant but always subordinated to Calpionella alpina Lorenz.
Remaniella is represented by two species: Remaniella ferasini
(Catalano) (Fig. 6F,G) and Remaniella duranddelgai Pop
(Fig. 7B). The occurrence of calpionellids joined by the collar
(Fig. 7C,D) is very common in this level. This phenomenon
was described by Borza (1969) and Colom (1988) and inter-
preted as the form of calpionellid reproduction.
The microfacies of this interval are less variable compared
to the preceding. The rocks represent mudstones and wacke-
stones with radiolarians and calpionellids and abundant
Globochaete alpina Lombard, frequent incursions of resedi-
mented ostracods, pelecypod fragments and abundant biotur-
bation (Fig. 7E). The rocks commonly contain dark organic
matter and the matrix is microsparitic as a rule. This type of
preservation makes calpionellids hardly determinable. A re-
duced number of specimens of Remaniella are preserved with
collars. The majority of specimens are with damaged or no
collar. A frequent recrystallization of the lorica made it impos-
sible to distinguish between different species.
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Fig. 5. Photomicrographs of microfacies and calpionellids of the Crassicollaria Zone. A, B – Main components of the Crassicollaria Zone.
Wackestones—packstones of sponge spicules, radiolarians and calpionellids. Sample RSV-6; C, D – Stomiosphaerina proxima Řehánek. Sam-
ple RSV-10; E – Crassicollaria colomi Doben. Sample RSV-11; F – Crassicollaria parvula Remane. Sample RSV-7; G – Crassicollaria
massutiniana (Colom). Sample RSV-7; H – Crassicollaria brevis Remane. Sample RSV-6; I – Crassicollaria intermedia Durand-Delga.
Sample RSV-7; J – Tintinnopsella remanei (Borza). Sample RSV-7; K – Tintinnopsella carpathica (Murgeanu & Filipescu). Sample RSV-15.
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Fig. 6. Microfacies and calpionellids of the Late Tithonian and Early Berriasian. A, B – Storm deposits in the Crassicollaria Zone. Picture
A shows grainstone of peloids with imbrications. Sample RSV-9; Picture B shows an upper part of the storm deposit with ostracod valves
concave down. Sample RSV-9; C—E – Calpionella alpina Lorenz. Tithonian/Berriasian boundary. Sample RSV-23; F, G – Remaniella
ferasini Catalano. Base of the Ferasini Subzone. Sample RSV-43; H – Tintinnopsella carpathica (Murgeanu & Filipescu). Sample RSV-46;
I, J – Characteristic facies of the Ferasini Subzone. J – Mudstone—wackestone of calpionellids, radiolarian and sponge spicules. The ma-
trix is microsparitic and the calpionellid collars are preserved only in a few specimens. Sample RSV-51; K – Frequent Globochaete alpina
Lombard in the Ferasini Subzone. Sample RSV-51.
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Fig. 7. Microfacies and calpionellids of the Elliptica—Oblonga Subzones. A – Calpionella elliptica Cadish. Sample RSV-62; B – Remaniella
duranddelgai Pop. Sample RSV-72; C, D – Calpionellids joined by the collar. Reproduction form according to Borza (1969). Sample
RSV-72; E – Microfacies of the Elliptica Subzone. Mudstone—wackestone of calpionellids, radiolarians and resedimented material. Sample
RSV-72; F – Calpionellopsis simplex (Colom). Sample RSV-84; G – Calpionellopsis oblonga (Cadish). Sample RSV-84; H – Tin-
tinnopsella longa (Colom). Sample RSV-87; I, J – Aberrant?, deformed calpionellids in the Oblonga Subzone. Sample RSV-120;
K – Tintinnopsella subacuta (Colom). Sample RSV-120.
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Late Berriasian
Calpionellopsis Zone (Samples RSV 84—141)
An important change in the calpionellid assemblage is
marked with the FO of the Calpionellopsis which defines the
base of the Calpionellopsis Zone. In the section studied, this
change takes place at the topmost part of the El Americano
Member, and the biozone spans into the whole overlying
Tumbadero Member (Fig. 9). The FO of the Calpionellopsis
which is normally represented by Calpionellopsis simplex
(Colom) (Fig. 7F) in the section studied is concurrent with the
appearance of Calpionellopsis oblonga (Cadish) (Fig. 7G).
Towards the top of the biozone, Calpionella alpina Lorenz
and Calpionella elliptica Cadish become scarce. On the other
hand, Tintinnopsella carpathica (Murgeanu & Filipescu) is
very common throughout, and the FO of Tintinnopsella longa
(Colom) (Fig. 7H) is in the middle part of the zone, and the
species is always scarce.
It is worth noting the appearance of many aberrant forms
within this interval similar to those reported by Reháková
(2000b) for the Calpionellopsis Zone (Fig. 7I,J). The most
diversified calpionellid assemblage is recorded in this inter-
val, and is represented by Tintinnopsella subacuta (Colom)
(Fig. 7K), Tintinnopsella longa Colom (Fig. 7H), Tintinnop-
sella carpathica (Murgeanu & Filipescu) (Fig. 5K), Am-
phorellina lanceolata Colom (Fig. 8A), Calpionella minuta
Houša (Fig. 8B), Lorenziella plicata Le Hégarat & Remane
(Fig. 8C), Remaniella duranddelgai Pop (Fig. 7B), Remaniella
filipescui Pop (Fig. 8D) and Remaniella cadischiana (Colom)
(Fig. 8E).
In the course of the Calpionellopsis Zone, an interesting
radiolarian and sponges event occurs. The abundance of ra-
diolarians, sponges and organic matter increases consider-
ably. This event affects preservation of the calpionellids. The
radiolarian and sponges beds are much silicified, dolo-
mitized and the organic matter is oxidized (Fig. 8F,G). This
event may be attributable to upwelling currents.
Murgeanui Subzone (Sample RSV-141)
One specimen of Praecalpionellites murgeanui Pop
(Fig. 8H) was found in the upper part of this interval (sample
RSV-141). This index species indicates the presence of the
Murgeanui Subzone. No microfacies change is visible in this
horizon.
Early Valanginian
Calpionellites Zone, Darderi Subzone
(Samples RSV 142—145)
In an overlaying biomicrite limestone (wackestone) con-
taining rare calcified radiolarians and calpionellids, loricas
of Calpionellites darderi (Colom) (see Fig. 8I) were identi-
fied. This index marker characterizes the Early Valanginian
Darderi Subzone of the Calpionellites Zone.
Discussion
Detailed bed-by-bed sampling in the Rancho San Vicente
section of “Sierra de los Órganos” in western Cuba allows
the recognition of a precise calpionellids and facies distribu-
tion (Fig. 9).
Lower Tithonian shallow-water carbonated bank San Vi-
cente Member lacks biostratigraphical markers which makes
the definition of the stratigraphic range of facies very diffi-
cult. Thus, it was dated by superposition and partially by the
occurrence of the Early Tithonian Semiradiata Zone underly-
ing the Chitinoidella-bearing limestones. The facies of this
member are considered in the present work as representing a
shallow-water bank without terrigenous influence, but addi-
tional work is necessary to define more precisely the dynamics
of this carbonated bank. The topmost part of the San Vicente
Member is dated as Early Tithonian (Semiradiata Zone). In
previous works (Pszczółkowski 1978, 1999), the contact be-
tween the San Vicente and the El Americano Members was
dated as Kimmeridgian—Tithonian.
The age from Pszczółkowski (1978, 1999) is coincident
with Goldhammer & Johnson’s (2001) second order trans-
gression in the Kimmeridgian/Tithonian in the whole Gulf
of Mexico province and Proto-Caribbean. Nonetheless, in
more detailed work it is possible to find a diachronism in the
apparition of the pelagic conditions. This diachronism re-
veals that the San Vicente carbonated bank prevailed for a
time after the initiation of the global sea-level rise. The glo-
bal sea-level rise started in the Kimmeridgian/Tithonian and
the complete drowning of the San Vicente bank occurred in
the Upper Tithonian. According to Rosales et al. (1992) an
anoxic event took place in the Kimmeridgian/Tithonian in
the Gulf of Mexico marked by the formation of facies en-
riched in organic matter. However, the San Vicente section
does not show a clear anoxic facies. In contrast to the asser-
tions by Pszczółkowski & Myczyński (2010), the presence
of only juvenile and the scarcity or lack of adult gastropods
are interpreted herein as rather due to taphonomic processes,
similar to the interpretations by Fernández-López & Meléndez
(1995), than as a consequence of low oxygenation levels.
The position of the San Vicente section in more oxygenated
waters is a reasonable explanation of a longer permanence of
the carbonated bank. Nonetheless, we do not have enough
evidence to reject the drowning of the San Vicente carbonate
bank as a result of sea-level rise and the action of the regional
anoxic event on the aforementioned drowning of the carbon-
ate platform.
The pelagic facies represented by the lower part of the
El Americano Member are mainly composed by Saccocoma-
bearing limestones with clear signals of sedimentary and
taphonomic condensation (mixture of calpionellid biozones
and presence of glauconite). Similar Saccocoma facies al-
though Kimmeridgian in age were described by Reháková
(2000b). According to Matyszkiewicz (1997) and Keupp &
Matyszkiewicz (1997), the saccocomids were very abundant
in the late transgressive system tract and probably within the
high-stand deposits of the northern Tethys during the Late
Oxfordian/Early Kimmeridgian and the latest Kimmerid-
gian/Early Tithonian. Saccocoma is recorded in the United
States (Brönnimann 1954), Europe (Pisera & Dzik 1979),
Mexico (Aguilera-Franco & Franco-Navarrete 1995), North-
ern Africa (Matyszkiewicz 1997), Asia (Hess 2002), Cuba
(Brodacki 2006) and Argentina (Kietzmann & Palma 2009).
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Fig. 8. Continuation of the microfacies and calpionellids of the Oblonga, Murgeanui and Darderi Subzones. A – Amphorellina lanceolata
Colom. Sample RSV-120; B – Calpionella minuta Houša. Sample RSV-89; C – Lorenziella plicata Le Hégarat & Remane. Sample RSV-90;
D – Remaniella filipescui Pop. Sample RSV-142; E – Remaniella cadischiana (Colom). Sample RSV-139; F, G – Radiolarian event.
Picture F displays the facies in polarized light. Sample RSV-106; H – Praecalpionellites murgeanui Pop. Sample RSV-141; I – Calpio-
nellites darderi (Colom). Sample RSV-142.
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Fig. 9.
Stratigraphic
column
displaying
a
detailed
microfacies
distrib
ution
and
calpionellid
biostratigraphy
of
the
San
Vicente
secti
on.
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In all those areas, these facies span from the Kimmeridgian
through to the Tithonian.
The recognition of this type of facies in Cuba is important
due to its stratigraphical coincidence with coeval strata from
Mexico and Argentina. In the three areas (Cuba, Mexico and
Argentina), this type of deposits started its record during ear-
liest Late Tithonian and may be the result of a connection be-
tween the Tethys and the Pacific Ocean during the sea-level
rise. This fact is difficult to discern due to the absence of re-
ports of Saccocoma facies in other parts between Mexico and
Argentina, which may be due to the scarcity of works on the
topic in those areas. It is evident that the sea-level rise identi-
fied here within the Chitinoidella Zone could be correlated
with the same sea-level rise expressed by Reháková (2000b).
The Jurassic/Cretaceous boundary was easily identified be-
cause of the dominance of Calpionella alpina Lorenz in the
assemblage in the bed number RSV-23, about six meters
above the base of the El Americano Member. Frequent storm
deposits in the top part of the Crassicollaria Zone closely re-
lated to the Jurassic/Cretaceous boundary could be attribut-
able to a response to a global sea-level drop. This sea-level
drop may be correlated with the limit between third order cy-
cles 1.3 and 1.4 in the super cycle LZB1 of the Sea-level curve
sensu Haq et al. (1988).
It is worth mentioning that previous works (i.e.
Pszczółkowski & Myczyński 2010) interpreted the Jurassic-
Cretaceous transition as a long-term subsidence that masked
the global Tithonian/Berriasian sea-level drop in outcrops of
the area. Nonetheless, the abundance of shallow-water fos-
sils (gastropods, pelecypods), reworked materials and abun-
dant storm deposits across this boundary documented in the
present research, clearly reflect a sea-level drop after the sea-
level rise recorded in the Boneti Subzone and which drowned
the San Vicente carbonate bank.
Interesting bioevents occur in the transition between the
Elliptica Subzone and the Calpionellopsis Zone. This transi-
tion should be represented by the FO of the Calpionellopsis
simplex (Colom), however, the first specimens of the Calpio-
nellopsis in the section are identified as Calpionellopsis ob-
longa (Cadish).
The transition through Elliptica-Oblonga Subzones oc-
curred without an apparent sedimentary break in the section
and, therefore, it is difficult to associate the absence of the
Simplex Subzone to a sedimentary gap. To assess this prob-
lem we considered two options. The first refers to the possi-
bility of a very thin Simplex Subzone, and as a consequence,
its loss by sampling effect. This explanation is hard to assume
due to the intensity of the sampling but there is a possibility to
consider a sedimentary condensation. The second assumption
is a possible confusion between Calpionellopsis simplex and
Calpionellopsis oblonga, due to the bad preservation. This ex-
planation is hard to assume as well, due to the differences in
the morphology of the lorica between the two taxa, even in ob-
lique sections and without preserved collars. Remane (1985)
explained that this confusion is only possible in the D2—D3
passage where transitional forms occur. An appropriate expla-
nation of this phenomenon is out of the scope of the present
work, and perhaps a regional detailed composite section will be
necessary to unravel this biostratigraphic interval in the future.
Another important change in microfacies and fossil assem-
blage occurs in the Oblonga Subzone. Within this unit, radio-
larians and organic matter become very abundant (Fig. 8F,G).
The facies of this interval are darker and display frequent sili-
ceous nodules.
The increase of radiolarians and organic matter is attribut-
able in the present work to upwelling currents. This interpre-
tation is supported by the abundance of sponge spicules and
by the fact that all siliceous nodules found in the studied sec-
tion were diagenetic. It is interesting to note that aberrant
calpionellids (Fig. 7I,J) are only present within this interval
of the radiolarian facies. There may be a relationship be-
tween the nutrification associated with the upwelling system
and these aberrant calpionellids, but more detailed work is
necessary to prove this assertion.
Conclusion
The high resolution sampling of an outcrop of the Guasasa
Formation in the Rancho San Vicente section of the “Sierra de
los Órganos” provided new and well-supported data about fa-
cies and calpionellid distribution across the Jurassic/Creta-
ceous boundary in western Cuba. The drowning event of the
San Vicente carbonate bank, a major regional paleogeographic
element on the facies studied, occurred during the earliest Late
Tithonian, Boneti Subzone, and led to deposition of the pelagic
facies of the El Americano Member. Thus, the stratigraphic
contact between the San Vicente and the El Americano Mem-
bers, the two lowest units of the Guasasa Formation, is Early/
Late Tithonian and not Kimmeridgian/Tithonian as consid-
ered in previous works. The sea-level rise associated with this
drowning event was probably the cause of the dispersion of
Saccocoma sp. into different paleogeographic domains, in-
cluding the Neuquen Basin. The Jurassic/Cretaceous bound-
ary in the studied section is identified at sample number 23,
six meters above the contact between the San Vicente and the
El Americano Members and not in the topmost part of the
latter unit as previously assumed. The facies of this bound-
ary are linked to the global sea-level drop recognized for that
age, indicated in the facies of this study by a concomitant shal-
low-water influence and storm deposits. The top of the strati-
graphic section corresponds to the Early Valanginian Darderi
Subzone of the Calpionellites Zone. Finally, the distribution
of calpionellids through the section allows good correlation
of the Jurassic/Cretaceous Cuban facies with European sec-
tions of the same period. Even though small differences were
found between the two areas, they can be attributed to spe-
cial local sedimentary conditions such as condensation and
to bad preservation of some specimens.
Acknowledgments: This research was possible due to the fi-
nancing of the Projects PAPIIT IN 108709 and IN 109912-3
from the Dirección General de Asuntos del Personal
Académico, Universidad Nacional Autónoma de México. The
research was also supported by the Grant Agencies for Sciences
of Slovakia (Project APVV 0644-10; VEGA 2/0068/11 and
VEGA 2/0042/12) and by the Project “Evolución geodinámica
(paleogeográfica) de Cuba occidental y central entre el Jurásico
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Tardío y el Plioceno”, from the University of Pinar del Río,
Cuba. The paper is a contribution to the activity of the Berria-
sian Working Group of the international Subcomission on
Cretaceous Stratigraphy.
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