major lithostratigraphic units in land-outcrops of north-central mexico
TRANSCRIPT
Major lithostratigraphic units in land-outcrops of north-central Mexico
and the subsurface along the northern rim of Gulf of Mexico Basin
(Upper Jurassic–lowermost Cretaceous): a proposal for correlation
of tectono-eustatic sequences
Federico Oloriza,*, Ana Bertha Villasenorb, Celestina Gonzalez-Arreolab
aDepartamento de Estratigrafıa y Paleontologıa, Facultad de Ciencias, Universidad de Granada, 18002, Granada, SpainbDepartamento de Paleontologıa, Instituto de Geologıa, Universidad Nacional Autonoma de Mexico, Ciudad Universitaria, 04510, Mexico, D.F., Mexico
Received 1 May 2001; accepted 1 July 2001
Abstract
The stratigraphic and geodynamic interpretation of Upper Jurassic lithostratigraphic units is revised in north-central Mexico and the
northern rim of the Gulf of Mexico Basin through updated ammonite and calpionellid biochronostratigraphy. Significant events in the
geodynamic evolution in these areas are evaluated and interpreted in terms of tectono-eustatic sequences (TES) of third and second orders.
3rd-TES-I and 2nd-TES-II/III in Mexico and 3rd-TES-I, 3rd-TES-II, and 3rd-TES-III at the northern rim of the Gulf of Mexico show the
main traits of the Upper Jurassic Supercycle in these regions, allowing the identification of a combined ‘Atlantic-Tethyan cachet’ in the
course of structuring/configuration of the Gulf of Mexico Basin during the Late Jurassic. The easy identification of 3rd-TES-I in north-central
Mexico and at the northern rim of the Gulf of Mexico Basin shows no significant difference in geodynamic history during the Oxfordian,
which contrasts with the increasing difference from the Kimmeridgian to the Early-Middle Berriasian. Shared trends in stratigraphic
architecture with the European margin of the North Atlantic Basin, as well as with epicontinental shelves surrounding Iberia and other
Tethyan areas, are interpreted to show phases of the geodynamic evolution in the central North Atlantic Basin, traces of which are
recognizable also in western Africa.
q 2003 Elsevier Ltd. All rights reserved.
Keywords: Stratigraphy; Biostratigraphy; Correlation; Tectono-eustasy; Upper Jurassic; Lowermost cretaceous; North-central Mexico; Northern gulf rim
1. Introduction
The present consensus is that Jurassic geologic evolution
of Mexican areas, other than Pacific ones, was closely
related to that of the central North Atlantic Basin (‘Atlantic
Tethys’ or southern North Atlantic Basin in Lancelot, 1980).
However, the beginning of Jurassic marine deposition in
Mexico has been related to a transgression from the Pacific
(Salvador, 1987, 1991), recognized by the occurrence of
Sinemurian and Pliesbachian ammonites. This resulted from
a major eustatic rise, which is evident across/through the
North Atlantic Basin (Jansa, 1986) and identified in
southern central Mexico at the Huayacocotla Basin,
Tenango de Doria and Xochicoatlan, and Mazatepec
(Erben, 1956; Schmidt-Effing, 1980; Imlay, 1984; Schlatter
and Scmidt-Effing, 1984; Lopez-Ramos, 1985), as well as in
Sonora in northeastern Mexico (Burckhardt, 1930; Imlay,
1952, 1980; Roldan-Quintana and Rangin, 1978; Dowlen
and Castill, 1981; Buitron and Gonzalez-Leon, 1982;
Stinnesbeck et al., 1993 in Calmus and Sosson, 1995;
Calmus et al., 1997; Linares et al., 1997).
1.1. Tectono-eustasy during the Late Jurassic
in the southeastern North American plate
The overall transgressive trend of Jurassic deposition in
Mexico was punctuated by tectono-eustatic interactions that
determined relative sea-level fluctuations; one of the more
significant also affected the Gulf of Mexico Basin and the
Caribbean areas (see below). Emery and Uchupi (1984)
suggested that sea-floor spreading in the Gulf of Mexico
0895-9811/03/$ - see front matter q 2003 Elsevier Ltd. All rights reserved.
doi:10.1016/S0895-9811(03)00049-X
Journal of South American Earth Sciences 16 (2003) 119–142
www.elsevier.com/locate/jsames
* Corresponding author. Fax: þ34-958-248528.
E-mail address: [email protected] (F. Oloriz).
Basin began during the Callovian or Early Oxfordian.
Salvador and Green (1980); Salvador (1987) argued for a
Callovian-Early Oxfordian tectonic phase that ended in the
separation of the Yucatan block from the main North
American Plate; this preceded a significant increase in
distance from the South American Plate during the post-
Oxfordian Late Jurassic. In southwestern Mexico, the
Middle Jurassic deformation event identified by Centeno-
Garcıa et al. (1998) could be mainly Callovian in age. In
Cuba, the second magmatic episode (Cobiella-Reguera,
1996) was an event coeval with the beginning of spreading
in the Gulf area; the Kimmeridgian drift envisaged by
Alvarez Castro et al. (1998) is also in accordance with a
post-Oxfordian increasing separation of the North and South
American Plates.
All the above points to the early-Late Jurassic context in
which marked changes in the paleogeography of the
ancestral Gulf of Mexico were interpreted by Salvador
(1991). In related areas such as western Cuba, the
interpretation of geological features as evidence for the
beginning of a passive margin in the southeastern North
American Plate (Cobiella-Reguera, 1996) also implies
coeval events. In such a context, a trailing-plate-margin
situation determined the tectono-sedimentary context of
epicontinental shelves in the southern North American Plate
(Scott, 1984) and net back-stepping platform margins
(Winker and Buffler, 1988) combined with low carbonate
production during post-Oxfordian times (Michalzik and
Schumann, 1994).
1.2. Lithostratigraphy
The Callovian-Oxfordian was a time of major transgres-
sion affecting central Atlantic margins (Lancelot et al.,
1977; Lancelot, 1980; Lancelot and Winterer, 1980), with
local/regional variations (Winterer and Hinz, 1984). There
is broad consensus on the transgressive features of the lower
Upper Jurassic in Mexico and the Gulf Coast Rim (USA),
although lithologic correlations vary. In fact, depositional
conditions in closely related regions fluctuated in time,
commonly resulting in a pattern of lithofacies recurrence.
Moreover, environmental availability for the presence of
time-marker organisms fluctuated. Since sedimentation was
often forced by tectonics, correlations and interpretations of
sedimentary environments have often been somewhat
controversial in north-central Mexico. Controversial points
are deposition depths and major lithofacies relationships
(e.g. the Zuloaga, La Caja and La Casita Formations, and
lateral equivalents; see Longoria, 1984). In addition,
informal nomenclature concerning lithostratigraphic units
in Mexico, and, to a lesser extent, in southern USA (see
below), raises doubts about the precision of stratigraphic
interpretations. Thus, Humphrey (1956) in Longoria, 1984;
Humphrey and Dıaz, (1956) in Bracken, 1984) introduced
the Zuloaga Group to include the Zuloaga and Minas Viejas
Formations, and the La Casita Group for the overlying
Upper Jurassic strata, i.e. those rocks between his Zuloaga
and Durango Groups in NE Mexico (fide Lopez-Ramos,
1985). Rather informally, several authors have used the
terms ‘Zuloaga’ and/or ‘La Casita’ Groups (e.g. Bracken,
1984; Cabral in Moran Zenteno, 1984; Wilson et al., 1984;
Wilson, 1990; Lopez-Ramos, 1985; Gotte and Michalzik,
1992). Since these terms were used in general descriptions,
usually with low precision in their lithostratigraphic
subdivison, we will refer to these terms as the ‘Zuloaga
Group’ and ‘La Casita Group’. On the whole, the most
widely accepted models suggest the correlation between the
‘Zuloaga Group’ and ‘La Casita Group’ in Mexico with the
Louark and Cotton Valley Groups at the northern rim of the
Gulf of Mexico Basin, respectively.
The analysis presented here updates that of Oloriz et al.
(1990), and is based on field data obtained by the authors in
a research program focused on biostratigraphic and
lithostratigraphic revision of Upper Jurassic and lowermost
Cretaceous type-sections in Mexico. This is complemented
with re-interpretation and correlation of available infor-
mation from subsurface core-sections in the northern rim of
the Gulf of Mexico Basin. The results are then compared
with information from European regions, especially Iberia,
and DSDP sites in eastern North America and western
Africa (Fig. 1) that include haul-dredged material.
2. Revised Biochronostratigraphy: the Zuloaga–La
Casita ‘Groups’ (north-central Mexico) and the
Louark - Cotton Valley Groups (northern rim of Gulf
of Mexico Basin)
The biochronostratigraphic revision is based on the
Upper Jurassic and lowermost Cretaceous standard ammo-
nite scale in Europe (Cariou et al., 1991; Geyssant and Enay,
1991; Hantzpergue et al., 1991), and recommendations for
calpionellid biochronostratigraphy made by the Tithonian
Working Group Meeting in Summeg 1984 (Remane et al.,
1986). This latter was complemented, with only minor
changes, following Tavera et al. (1994) in the precise
interpretation of the calpionellid A/B Zone boundary and its
correlation with the Tithonian/Berriasian boundary based on
ammonites, and Oloriz et al. (1995), who provided the most
precise and westernmost reported calpionellid biostratigra-
phy known from the West-Tethys. Myczynski et al. (1998);
Oloriz et al. (1999) provided the correlation charts used
below for the Oxfordian to the Berriasian stages.
Since our analysis is based on biochronostratigraphic
control, it is restricted to deposits containing age-significant
biota. This limitation prevents an accurate biochronostrati-
graphic re-evaluation of terrigenous and evaporitic deposits
at the base of the Upper Jurassic sections both in northern-
central Mexico and in the northern rim of the Gulf of
Mexico Basin.
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142120
Fig. 1. (A): Location of the areas studied in the southern North American Plate (vertical and horizontal ruling for north-central Mexico and the northern rim of the
Gulf of Mexico Basin, respectively). (B): Present-day isochron map of the ocean basins, mainly Atlantic, with location of the areas depicted on the left (adapted
from Scotese et al., 1988). (C): Late Jurassic paleogeography, mainly Late Kimmeridgian–Early Tithonian, with location of areas cited in text. Numerical time
scale following Odin (1992), adapted to biochronostratigraphy from Marques et al. (1991). Paleogeography and site/area locations inspired on Enay (1972);
Salvador and Green (1980); Lancelot and Winterer (1980), Ogg et al. (1983), Azema and Jaffrezo (1984), Imlay (1984), Tucholke and Jansa (1986, see Jansa,
1986); Ziegler (1988); Salvador (1991); Rowley (1992), Fourcade et al. (1993a,b), and Enay and Cariou (1997). See text for the source of data from the Aaiun Basin
(CORC 15-1); Algarve and Prebetic shelves (ALG-PB); Cat Gap (DSDP site 100); Cuba (C); the Blake-Bahama Basin (DSDP sites 391c and 534); the
Haha/Essaouira Basin (Ha); the Iberian Range (Ib); Kachchh (K); the lower continental rise hills between New York and Bermuda (DSDP site 105); the Lusitanian
Basin (Ls); the Moroccan Basin (DSDP sites 416, 370); the Mazagan escarpment area (V30-RD38; DSDP sites 544, 545, 547B); the north-central Mexico
(Mexican Altiplano, MxA); the NewfoundlandBasin (NfB); the North-Sea Basin (NSB); the Northeastern Alps (NA); the northern rim of the Gulf of Mexico Basin
(nrGMx); North-West European shelves (NW-Es); the Cape Verde Basin (DSDP site 367); the Rif-Tell Basin (R-TB); the Scotian Basin (ScB); the Subbetic (SB);
the Trento Plateau (TP); Transdanubian (TrD); West Arctic Canadian Islands from the Amerasian Basin (wACI-AB); and the West-Iberia foreland (WIbf).
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142 121
2.1. North-Central Mexico
The occurrence of ammonites and calpionellids in land-
outcrops from north-central Mexico (Fig. 1, vertical ruling
on the upper left; Fig. 2) makes it possible to establish
reliable biochronostratigraphy using bed-by-bed analysis,
and the revision of older (last-decade) data by Oloriz
(1992); Oloriz et al. (1990, 1998b, 1999); Adatte et al.
(1992, 1994a-c); Callomon (1992); Gonzalez-Arreola et al.
(1992); Stinnesbeck et al. (1993); Myczynski et al. (1998);
Oloriz and Villasenor (1999), and Villasenor et al. (2000).
Among the lateral equivalents of the Zuloaga and La Casita
‘Groups’, lithology and biostratigraphy are better known for
the Santiago, Taman, lower Malone and Pimienta For-
mations (e.g. Cantu-Chapa, 1967, 1976, 1984, 1998; see
Lopez-Ramos, 1985 for an overview). However, infor-
mation from sections sampled bed-by-bed is not available
and, therefore, correlations can be made only in general
terms. Hence, we focus on biochronostratigraphy based on
data recovered from Zuloaga carbonates and La Caja-La
Casita deposits, while commenting on their lateral equiva-
lents when appropriate.
2.1.1. The lower ‘Zuloaga Group’
Ammonites from the lower part of the ‘Zuloaga Group’
indicate mainly the Middle Oxfordian (Imlay, 1984), middle
rather than upper Plicatilis Zone (Myczynski et al., 1998).
The rarity of Late Callovian–Early Oxfordian ammonites in
wide areas of Mexico (Callomon, 1992; Westermann, 1992;
Cantu-Chapa, 1998) agrees with discontinuous deposition
(hiatuses) during the latest Middle to the beginning of the
Late Jurassic. Thus, unfavorable habitats for ammonoids
and other time-marker organisms are assumed to span a
major part of the Early to early-Middle Oxfordian. Wide-
spread continental to marine-marginal and shallow-marine
sediments (La Joya Formation and lateral equivalents)
represent this stratigraphic interval, hampering precise
placing of the lower boundary of the ‘Zuloaga Group’.
In the Tampico-Misantla area (eastern Sierra Madre), the
partly lateral equivalent of the Zuloaga carbonates is the
lower Santiago Formation. It deserves special attention
since Bathonian to Oxfordian ammonites (Lopez-Ramos,
1985; Cantu-Chapa, 1998) have been gathered from this
brownish to dark-gray siltstone and silty-limestone rhyth-
mite. The oldest ammonites recovered from the Oxfordian
at Taman (San Luıs Potosı; Cantu-Chapa, 1984) have been
reinterpreted biostratigraphically by Myczynski et al.
(1998), who concluded that their age is Middle Oxfordian,
probably middle to late Plicatilis Chron. Thus, on the basis
of current knowledge, the oldest Oxfordian ammonite
assemblages in the Santiago Formation and Zuloaga
carbonates are coeval. Further research in the lower
Santiago Formation is needed to clarify if discontinuous
ammonite assemblages of the Bathonian, Callovian and
Oxfordian are evidence of sampling failure, hiatal depo-
sition and/or ecologically restricted living conditions for
Fig. 2. Correlation chart for the Upper Jurassic Supercycle in north-central Mexico and the northern rim of the Gulf of Mexico Basin. Geological Groups and
Formations (capitals); Members and informal units (others labellings); intercalation of Buckner-type deposits (‘B’). Early (E), Middle (M) and Late (L).
Biochronostratigraphy according to European standards for ammonites and calpionellids (see text). Unconclusive biochronostratigraphic boundary (broken
lines). Hiatuses (vertical ruling). Black for unnamed and poorly known (inconclusively dated) basinal-equivalent deposits. Second-order Supercycles and long-
term global eustatic curve adapted from Haq et al. (1987, 1988) (arrows). Relative sea-level curve for the region, especially for north-central Mexico (thin line).
Transgression (T) and Regression (R). Upper Jurassic Cycles in the northern Gulf Coast (J3.1, J3.2) according to Emery and Uchupi (1984). Tectono-eustatic
sequences/supersequences (TES-I, II, III). Ammonites: Berriasellidae (B), Dichotomosphinctes (DI), Durangites (DU), Gregoryceras (GR), microconchiate
Hybonoticeras (Hy), Idoceras (I), Mazapilites (MZ), Nebrodites (N), Praeataxioceras (PRX), Procraspedites (PRO), Salinites (S), Schneidia (SCHN),
Spiticeratinae (SP), Virgataxioceras-like ammonites under study (V). calpionellids (U).
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142122
ammonoids of the Tampico-Misantla area (eastern Sierra
Madre), irrespective of the apparently homogeneous
lithologic succession.
2.1.2. The boundary between the Zuloaga and La Casita
‘Groups’
The boundary between the ‘Groups’ Zuloaga (Zuloaga
Limestone ¼ Zuloaga Formation, and lateral equivalents)
and La Casita ( ¼ La Caja and La Casita Formations; other
assumed lateral equivalents are not considered here because
of the poorly known biostratigraphy) is usually interpreted
to be close to the Oxfordian/Kimmeridgian boundary,
without precise paleontological revision of existing data.
Some authors have placed the upper boundary of the
Zuloaga Formation (Zuloaga Limestone) within the Kim-
meridgian for some areas of the Mexican Altiplano
(Lopez-Ramos, 1985), northeastern Mexico (Salvador,
1991), and the Eastern Sierra Madre (Gotte and Michalzik,
1992; Michalzik and Schumann, 1994). These latter authors
suggested an Early Kimmeridgian age, but they did not
provide precise ammonite data. Gotte and Michalzik (1992)
referred to several studies, among which Weidie and
Wolleben (1969) gave the most accurate data on ammonite
biohorizons. These latter authors stated, however, that the
oldest Kimmeridgian haploceratids and perisphinctids from
the La Casita Formation s.str. were collected 8–9 m above
the contact with the Zuloaga limestone ( ¼ Zuloaga
Formation) in the Sierra de los Muertos, Nuevo Leon.
Callomon (1992) dated the youngest Oxfordian ammo-
nites in Mexico as Late Oxfordian, within the Bimammatum
Chron. Oloriz (1992); Oloriz et al. (1992) re-interpreted data
on latest Oxfordian ammonites in Mexico, and Myczynski
et al. (1998) concluded that the youngest ammonites
collected from the Zuloaga Formation (within the ‘Zuloaga
Group’) were lower Planula Zone, uppermost Oxfordian
according to the standard ammonite biochronostratigraphy
in Europe, or lowermost Kimmeridgian according to recent
proposals for revision of the Oxfordian/Kimmeridgian
boundary (Wierzbowski, 1991; Atrops et al., 1993; Oloriz
et al., 1994; Matyja and Wierzbowski, 1995), which is
slightly younger than that interpreted by Callomon (1992).
Villasenor (1991); Callomon (1992); Oloriz (1992); Oloriz
et al. (1992) interpreted the oldest ammonites from the La
Casita and La Caja Formations as Early Kimmeridgian,
Platynota Chron (except its lower part), but they have
recently been re-interpreted as late Platynota-earliest
Hypselocyclum Chrons (Villasenor et al., 2000).
Thus, new ammonite data and interpretations reduce
uncertainty about the age of the boundary between the
Zuloaga and La Casita Formations (and therefore between
the Zuloaga and La Casita ‘Groups’), supporting a latest
Oxfordian-earliest Kimmeridgian ( ¼ Early Kimmeridgian
according to some authors) interval including this boundary.
However, the lowermost occurrence of ammonites in the La
Casita and La Caja Formations changes locally, as may be
confirmed by comparing the data in Contreras et al. (1988);
Villasenor (1991); Oloriz et al. (1999); Villasenor et al.
(2000). The latest Oxfordian–earliest Kimmeridgian guide-
fossils are unknown (extremely rare?), both in the Zuloaga
and La Casita Formations (and therefore in the Zuloaga and
La Casita ‘Groups’). Therefore, the boundary between the
Zuloaga Formation ( ¼ Zuloaga Limestone), and/or lateral
equivalents, and the La Casita-La Caja Formations may
include hiatuses (Verma and Westermann, 1973; Emery and
Uchupi, 1984; Oloriz et al., 1999) that are related to local
supratidal or restricted marine conditions unfavorable for
the occurrence of age-significant biota.
A lateral equivalent of the upper Zuloaga carbonates
(Zuloaga Formation) is the dark-gray siltstone and silty-
limestone rhythmite of the upper Santiago Formation
recognized from the eastern Sierra Madre in the Tampico-
Misantla area. The most recent biostratigraphic revision of
ammonite assemblages from the upper Santiago Formation
was made by Myczynski et al. (1998), who correlated them
with those known from the Zuloaga carbonates. However,
Cantu-Chapa (1984) recognized the progressive transition
from dark-gray siltstones and silty-limestones with no
calcareous concretions in the upper Santiago Formation to
dark-gray limestones of the Taman Formation. Since the
youngest ammonites (Praeataxioceras) in the Santiago
Formation are Late, not latest, Oxfordian, and the oldest
ones (Schneidia Assemblage) in the Taman Formation) are
Early, (not earliest) Kimmeridgian (European standard
biochronostratigraphy), no continuous ammonite record is
known within a stratigraphic interval with gradual change in
lithofacies. In conclusion, further research is necessary to
establish whether the discontinuities of the ammonite
assemblages indicate incomplete sampling, stratigraphic
gaps or poor ecologic conditions for horizons between
Praeataxioceras (the Zona con Discosphinctes in Cantu-
Chapa, 1969, 1979, 1984) in the Santiago Formation and the
Schneidia Assemblage (the Zona con Ataxioceras in
Cantu-Chapa, 1969, 1979, 1984) in the Taman Formation.
2.1.3. The upper boundary of the ‘La Casita Group’
On the assumption that the upper boundary of this
‘Group’ is the top of the La Casita Formation and its
envisaged lateral equivalents, this boundary was commonly
placed at the Tithonian/Berriasian (Jurassic/Cretaceous)
boundary, on the basis of informal interpretations of both
the Tithonian and Berriasian stages in Mexico. This
informality became evident when calpionellids were
considered (Cantu-Chapa, 1980, 1989; Longoria, 1984,
among others). However, Ortuno Arzate and Delfaud (1988)
placed the top of the La Casita deposits in Chihuahua within
the Lower Cretaceous.
The interpretation of ammonite and calpionellid data
made by Oloriz and Tavera (1989); Tavera et al. (1994);
Oloriz et al. (1995), as well as the results of recent studies in
north-central Mexico (Adatte et al. 1992, 1994a–c; Gonza-
lez-Arreola et al. 1992; Oloriz et al. 1992, 1996, 1999;
Michalzik and Schumann, 1994; Villasenor et al. 2000),
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142 123
agree with the recommendations of the Tithonian Working
Group Meeting (Remane et al., 1986) and with the updated
Tithonian Standard biochronostratigraphy in Europe (Geys-
sant and Enay, 1991; see minor changes to calpionellid-
ammonite correlation in Oloriz et al., 1999). The above data
and interpretations place the uppermost horizons of La
Casita-La Caja Formations and their lateral equivalents in the
Early to early-Middle Berriasian. Recent studies by Blauser
and McNulty (1980); Gonzalez-Arreola et al. (1992); Adatte
et al. (1994a–c), and Michalzik and Schumann (1994)
provide the evidence for regional condensations and/or
hiatuses close to the boundary between the La Casita deposits
and the overlying Taraises Formation. Eguiluz and Aranda
(1984); Michalzik and Schumann (1994), interpreted a
comparatively restricted record of La Casita-type deposits
as extending into the Valanginian.
A lateral equivalent of the La Casita deposits is the so-
called Jurassic Pimienta Formation, the upper part of which
contains Himalayites, Kossmatia, Salinites, Proniceras,
Durangites and Corongoceras(Lopez-Ramos, 1985).
Assumed correlative deposits have yielded Paradontoceras
sp. aff. callistoides, Paradontoceras sp., Protancyloceras
hondense, Proniceras lerense and Protacanthodiscus sp.
(Cantu-Chapa, 1967, 1984). These two ammonite assem-
blages indicate Early Berriasian age, not Late Tithonian as
interpreted by these authors. This age re-interpretation agrees
with the content in calpionellids (Calpionella alpina,
Calpionella elliptica, Tintinnopsella longa) and the calcar-
eous nannofossils (Nannoconus steinmanii) reported by
Cantu-Chapa (1967), as well as with the record of
Calpionella elliptica and Tintinnopsella oblonga indicated
by Lopez-Ramos (1985). Current consensus on ammonite
and calpionellid biochronostratigraphy (see above) supports
our age interpretation.
2.2. Northern rim of Gulf of Mexico Basin
2.2.1. Smackover carbonates
In southeastern USA (Fig. 1, horizontal ruling on the
upper left; Fig. 2), Imlay and Herman (1984); Young and
Oloriz (1993) studied and illustrated ammonites from the
Smackover Formation.
In Louisiana and Texas, Imlay and Herman (1984)
indicated a Middle–Late Oxfordian age for ammonites from
the Smackover Formation. Their material from the middle
Smackover Formation yielded Dichotomosphinctes and so-
called Discosphinctes. Ammonites interpreted by these
authors as Ataxioceras and Idoceras (the latter recorded
from Smackover by Imlay and Herman, 1984, in fig. 5) are
known from the upper Smackover Formation, where they
occur in an upper assemblage containing the ammonites
cited as Discosphinctes by Imlay and Herman (1984). More
precisely, they (Imlay and Herman (1984), fig. 5) reported
Ataxioceras and Idoceras from shales and mudstones in the
upper Smackover Formation, below a probable lateral
equivalent of the Buckner deposits at the Philips Kendrick
no. 1 well (Louisiana). Imlay and Herman (1984) dated the
upper Smackover Formation as Late Oxfordian on the basis
of the supposed Discosphinctes. Oloriz et al. (1990)
discussed the use of Discosphinctes (and coeval assumed
Ataxioceras) by Imlay and Herman (1984), and concluded
that the upper assemblage of these ammonites could be
interpreted as Praeataxioceras, a genus known from the
Upper Oxfordian (Bimammatum and Planula Zones) mainly
in Submediterranean Europe. Myczynski et al. (1998)
interpreted the assemblage with Praeataxioceras, Euaspi-
doceras and Subnebrodites or Enayites as characteristic for
the youngest Oxfordian deposits in southern USA, including
the Cotton Valley Oilfield.
The upper Smackover ‘Idoceras-Ataxioceras assem-
blage’ has been re-interpreted, from data in Imlay and
Herman (1984), as the Passendorferiinae-Praeataxioceras
assemblage and compared with the uppermost Oxfordian
ammonite-bearing deposits in southern USA by Myczynski
et al. (1998). The traditional interpretation of Late
Oxfordian Idoceras from Sonora (Beauvais and Stump,
1976) has been proven wrong (Linares et al., 1997).
Furthermore, the presence of the Ataxioceras Assemblage
(in Cantu-Chapa, 1969) indicates the Lower Kimmeridgian
Platynota Zone in Mexico (Villasenor, 1991; Callomon,
1992; Oloriz, 1992; Oloriz et al., 1992), which has been
recently reinterpreted as the Schneidia Assemblage char-
acterizing the uppermost Platynota–lowermost Hypselocy-
clum Zone (Villasenor et al., 2000). Thus, the base of the
Kimmeridgian has not been recognized in Mexico from
ammonite occurrences, nor has Burckhardt (1930) record of
Sutneria platynota from Huayacocotla been confirmed.
Moreover, true Idoceras have been correctly dated as
Kimmeridgian in Mexico from Burckhardt (1906), with
only minor differences in age interpretation within the Early
and Middle Kimmeridgian (three-fold division).
In Louisiana, Young and Oloriz (1993) noted a relatively
continuous record of ammonites in the Smackover Limestone
from the A.J. Hodges no. 1 Pardee-Calloway borehole at the
Cotton Valley Oilfield. The presence of Middle Oxfordian
Gregoryceras (first report from North America) was
documented in horizons 100 m below the top of the
Smackover Limestone, and probable Late Oxfordian Praea-
taxioceras, Orthosphinctes and Euaspidoceras were reported
in horizons above the level containing Gregoryceras.
In conclusion, the revised biochronostratigraphy of the
Smackover Formation, yielding Perisphinctes (Dichotomo-
sphinctes) and Gregoryceras below, and Orthosphinctes
(Praeataxioceras) and Subnebrodites or Enayites
(¼ ?‘Idoceras’ in Imlay and Herman, 1984) near the top,
places the stratigraphic interval here analyzed in the
Middle-Upper Oxfordian (Young and Oloriz, 1993; Myc-
zynski et al., 1998), except for the uppermost Oxfordian
(considered as lowermost Kimmeridgian in recent propo-
sals; see above). Unfortunately, no ammonites were
recovered in cores of the uppermost Smackover Limestone
at Webster Parish, Louisiana (Young and Oloriz, 1993).
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142124
2.2.2. The Pre-Bossier deposits
In the cores studied by Imlay and Herman (1984), the
Smackover Formation is overlain by the unfossiliferous
Buckner deposits, making it difficult to improve the
biostratigraphic interpretation of the topmost Smackover
Fm. In the core sections studied by Imlay and Herman
(1984) between the Buckner and the base of the Bossier
Formation, which was considered to be Lower Kimmer-
idgian, lies what they referred to as the Gilmer Limestone.
Imlay and Herman (1984) suggested that the Oxfordian/
Kimmeridgian boundary could lie within their Gilmer
Limestone (now recognized as equivalent to, or a member
of, the upper part of the Haynesville Formation, and usually
referred to as the Cotton Valley Limestone; G. Wahlman
pers. comm. to FO, 1998; A. Salvador suggested to FO this
term should be avoided because it refers to strata that do not
belong to the Cotton Valley Group). True Idoceras
recovered by Imlay and Herman (1984) from the upper
part of their Gilmer Limestone indicate a late-Early to early-
Middle Kimmeridgian age. Based on ammonites, Young
and Oloriz (1993) recognized in Louisiana the Lower, but
not lowest, Kimmeridgian (upper Hypselocyclum-Divisum
Zones?) in the lower part of correlative shales from the
Haynesville Formation (which yielded no ammonites in
cores from its base). Thus, the precise biostratigraphy of the
base of Gilmer and Haynesville deposits in Louisiana
remains unknown. The youngest ammonite horizon in the
assumed equivalent ‘Cotton Valley Limestone’ (term
applied by G. Wahlman for core Amoco No. 1 Jimmy Hill
Gas Unit, East Texas; pers comm. to FO, 1998) contains
rare Virgataxioceras-like ammonites and therefore is close
to the Kimmeridgian/Tithonian boundary (Oloriz, in prep.).
2.2.3. The Cotton Valley Group
According to Imlay and Herman (1984), the lower part of
the overlying Bossier Formation contains Lower Kimmer-
idgian ammonites. The assumed correlations in the area
(discussed below) and data of Young and Oloriz (1993), as
well as unpublished records of Virgataxioceras-like ammo-
nites (Oloriz, in prep.) from the equivalent ‘Cotton Valley
Limestone’ (the Gilmer Member of the Haynesville
Formation), indicate that the base of the Bossier deposits,
i.e. the base of the Cotton Valley Group, is diachronous.
Ammonites recorded by Imlay and Herman (1984) from the
upper Bossier Formation are Berriasian (Salinites, ?Proni-
ceras, and probably Substeueroceras and ?Durangites),
while the youngest ammonites (Madeira, ‘Leopoldia’ ¼
Karakaschiceras, ‘Neocomites’) from the upper Schuler
Formation are of Valanginian age.
2.3. Concluding remarks on biochronostratigraphy
Middle Oxfordian ammonites typically mark the oldest
identified biohorizons in the Zuloaga and Smackover
deposits. The top of these two shallow carbonate-shelf
systems cannot be accurately dated, but the youngest
ammonites collected indicate Late, but not latest, Oxfordian
(early Planula Chron ¼ earliest Kimmeridgian in recent
proposals in Europe). The Oxfordian/Kimmeridgian bound-
ary has not been identified biostratigraphically in northern-
central Mexico or at the Gulf Coast Rim. The next
ammonite datum is Early Kimmeridgian, identified from
siliciclastic and limy deposits in both regions (late
Platynota-earliest Hypselocyclum Chron in north-central
Mexico and probable early Divisum Chron in the northern
rim of the Gulf of Mexico Basin). No precise biochronos-
tratigraphy could be established for the top of the La Casita
deposits and the Cotton Valley Group, but their upper parts
include Berriasian deposits.
3. Biochronostratigraphic correlation of the Zuloaga
and La Casita ‘Groups’ (north-central Mexico) with theLouark and Cotton Valley Groups (northern rim of Gulf
of Mexico Basin)
Updated biochronostratigraphy provides the basis for our
correlations, and so our interpretations concern mainly
deposits yielding guide-fossils. On the other hand, dia-
chrony usually occurs in shallower epicontinental environ-
ments with complex lithofacies patterns, as documented by
subsurface data from the northern rim of the Gulf of Mexico
Basin (e.g. Smackover Formation in Bradford, 1984;
Smackover-Buckner complex in Ferns and York, 1984;
Smackover-Buckner sequence in Vinet, 1984; Smackover-
Buckner in Montgomery, 1996; Gilmer Member in Moore
1984, fig. 11 non fig. 2; and Bossier Formation in McGraw,
1984, among others). Therefore, we have limited our study
to subtidal successions, and excluded innermost shelf sites,
i.e., very proximal and nearshore or tidal-supratidal
environments showing deposits poor or lacking in biostrati-
graphic data, such as those represented by the lower
‘Zuloaga Group’ and the lower Louark Group.
3.1. Northern-Central Mexico
3.1.1. The Zuloaga Group–carbonate section: Zuloaga
Formation (locally referred to as Zuloaga Limestone)
In Mexico, the Zuloaga Formation and ammonite-
yielding lateral equivalents range in age from the Middle
to the Late Oxfordian, i.e. middle-late Plicatilis to earliest
Bimammatum–early Planula Chron (Fig. 2) of the Medi-
terranean and Submediterranean ammonite standard bio-
chronostratigraphy (Cariou et al., 1991). Local records of
Lower Oxfordian deposits are dubious, but cannot be ruled
out. The discontinuous lower part of the Upper Jurassic
section is assumed to be Early, or more probably, Early to
early-Middle Oxfordian. This accords with the total range of
stratigraphic gaps and discontinuous records, at least in
terms of ammonite biochronostratigraphy identified else-
where in Tethyan regions that are epioceanic-oceanic
(Sequeiros, 1974; Sarti, 1988; Fozy, 1993a,b; Oloriz et al.,
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142 125
1998a; Channell et al., 1990; Caracuel et al., 2000; and
references therein) or epicontinental (Wildi, 1983; Wilson,
1988; Bernardes and Corrochano, 1992; Atrops and Benest,
1994; Enay and Mangold, 1994; Aurell et al., 1994, 2000;
Krishna and Ojha, 1996; Kamoun et al., 1999; Gygi, 2000;
Pena dos Reis et al., 2000; and references therein), and even
correlates with northern European shelves (Fortwengler and
Marchand, 1994) and western Arctic Canadian islands of the
Amerasian Basin (Harrison et al., 2000). Thus, early to
middle-Late Jurassic transgressions over continental, mar-
ginal to shallow marine deposits of the La Joya Formation
and its lateral equivalents expanded widely in Mexico,
scattering components of the Tethyan biota. The Middle
Oxfordian peak transgression (‘Atlantic Transgression’ in
Lancelot and Winterer, 1980) has been used as a reference
event for correlation between western and eastern margins
of the central North Atlantic (Lancelot et al., 1977; Lancelot
and Winterer, 1980), as well as to identify the beginning of
the Upper Jurassic Supercycle in Iberia and other Tethyan
areas. Therefore, this transgressive event, which marks the
beginning of the ‘maturation’ of the Atlantic into a real
ocean (Lancelot and Winterer, 1980), is valuable for long-
distance correlations, including Mexico.
The missing record of ammonites from the top of the
Zuloaga Formation (thus from the top of the ‘Zuloaga
Group’), and from transitional deposits between the
Santiago and Taman Formations, corresponds to
the regressive trend that Salvador (1991) placed close to
the Oxfordian/Kimmeridgian boundary (Fig. 2). Factors
determining this trend of shallowing and shoaling (local
emersion/erosion included) would have forced ammonites
to move from previously colonized areas, thereby regionally
counteracting high-sea-level conditions at a global scale, as
proposed by Haq et al. (1987, 1988). Active salt tectonics in
the area, including faulting, has been attributed by Salvador
(1991) to these times.
3.1.2. The La Casita Group–the more or less
ammonite-rich La Casita and La Caja Formations
The record of ammonites from the base of the La Casita
Group is known from horizons close to the base of the La
Casita and La Caja Formations (Fig. 2), as well as from the
lower Taman Formation. The oldest record of ammonites in
the La Casita and La Caja Formations is diachronous within
the Lower Kimmeridgian section, ranging between the
upper Platynota-lowermost Hypselocyclum and the upper
Hypselocyclum–lower Divisum Zones (Oloriz et al., 1999;
Villasenor et al., 2000). The duration of the interval
involved in the turnover between Zuloaga carbonates and
La Casita-La Caja deposits is hard to estimate with
precision. The rather abrupt change from carbonate ramp
(Zuloaga) to siliciclastic shelf (La Casita) depositional
conditions has been related to tectonic reactivation with
change in the subsidence regime (Michalzik and Schumann,
1994). This event forced erosion and deposition that had no
Oxfordian equivalents in the area. Several events were more
or less coeval: subduction pulses in NW Mexico (Araujo
Mendieta and Estavillo Gonzalez, 1987); the beginning of a
rift phase in northern Mexico (Ortuno Arzate and Delfaud,
1988); and active faulting and salt movements (Salvador,
1991). Therefore, the shifts in lithofacies from Zuloaga to
La Casita Groups reflect regional, tectonically driven sea-
level changes. This interpretation agrees with the regional
tectonics as interpreted by Araujo Mendieta et al. (1982);
Araujo Mendieta and Estavillo Gonzalez (1987); Ortuno
Arzate and Delfaud (1988); Oloriz et al. (1990); Salvador
(1991); Michalzik and Schumann (1994).
Biostratigraphic data from the top of the La Casita Group
(tops of the La Casita and La Caja Formations), and from
the top of the so-called Jurassic Pimienta Formation, need
improvement. A significative number of assignations to
Late Tithonian age (Imlay, 1943; Cantu-Chapa, 1967, 1984,
1989; Longoria 1984; Lopez-Ramos, 1985; Contreras et al.,
1988; Addate et al., 1992, 1994a–c; Stinnesbeck et al., 1993
to a lesser degree) might be corrected for Berriasian (Oloriz
and Tavera, 1989; Addate et al., 1992, 1994a–c; Gonzalez-
Arreola et al., 1992; Oloriz et al., 1999; Stinnesbeck et al.,
1993; Villasenor et al., 2000), and thus the placing of the
Jurassic/Cretaceous boundary at the top of the La Casita
deposits was incorrect (Fig. 2). Hiatuses and/or unfavorable
environmental conditions for time-marker biota during the
Early Cretaceous have been envisaged (Imlay, 1936;
Gonzalez-Arreola et al., 1992; Addate et al., 1994a–b;
Oloriz et al., 1999), but information is incomplete at present.
However, it is worth noting that Ortuno Arzate and Delfaud
(1988) identified the top of the La Casita deposits with the
boundary between their megasequences I and II, referring to
the rift series in the Chihuahua Basin and representing a part
of their Tethyan phase in the geodynamic evolution.
3.2. Northern rim of the Gulf of Mexico Basin
In contrast to the general agreement on the composition
of the Zuloaga and La Casita Groups in Mexico (But see
Gotte and Michalzik, 1992), some controversy exists
concerning the interpretation of lithologic units comprising
the Louark and Cotton Valley Groups, at the northern rim of
the Gulf of Mexico Basin, as a result of limited subsurface
data (Salvador, 1991). Therefore, the age interpretation of
these stratigraphic sequences depends largely on the
acquisition of new subsurface data and on regional
correlation based on reliable data from surface outcrops in
Mexico, where biochronostratigraphy is becoming more and
more accurate.
3.2.1. The Louark Group
In accordance with the above treatment of Mexican data,
we exclude the mainly terrigenous or evaporitic deposits
underlying the oldest horizons identified biostratigraphi-
cally in Upper Jurassic carbonate facies. However, it is
significant for wide-regional stratigraphy and correlation to
note that, elsewhere in the world, ammonitiferous sections
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142126
commonly contain fossils with a more or less complex
taphonomic history, which is related to regionally discon-
tinuous deposition, at about the Middle-Upper Jurassic
boundary. In the Gulf of Mexico Basin the interpretation of
equivalent unfossiliferous deposits is controversial (Salva-
dor, 1991). This was a time of major paleogeographic
changes, including spreading in the Gulf (Emery and
Uchupi, 1984) with the break-up and separation of the
Yucatan block or platform, as interpreted by Salvador and
Green (1980); Salvador (1987) respectively. In southeastern
Mexico, this presumably forced discontinuous deposition in
the context of syn-rift tectonics interpreted by Michaud and
Fourcade (1989).
On the basis of ammonite biochronostratigraphy, we
identify one of the ‘datum planes’ by the occurrence of
Dichotomosphinctes and Gregoryceras (Middle Oxfordian
in age) in the lower Smackover Formation. Accordingly, the
base of the Smackover carbonates at the northern rim of
the Gulf of Mexico Basin correlates with the base of the
Zuloaga carbonate facies in Mexico (Fig. 2).
No diagnostic fossils other than those indicating Late
Oxfordian (not the latest) have been reported from the upper
(not the topmost) Smackover Formation and its lateral
equivalents. As at the top of the Zuloaga Formation, no
latest Oxfordian ammonites have been reported from the top
of the Smackover carbonates; the known ammonites (see
above, and Myczynski et al., 1998) permit biochronostrati-
graphic correlation between horizons containing the young-
est Oxfordian ammonites in the Zuloaga and Smackover
carbonates. This coincidence points to coeval damaging of
ammonite habitats during shallowing trends, both in Mexico
and in the northern rim of the Gulf of Mexico Basin (Fig. 2).
The time for restricted or even supratidal facies of the
post-Smackover–pre-Bossier, and pre-Bossier-type depos-
its, is considered as mainly latest Oxfordian–Early (not
earliest) Kimmeridgian (Standard European ammonite
biochronostratigraphy, Cariou et al., 1991; Hantzpergue
et al., 1991) by their stratigraphic position (Salvador, 1991)
and our biochronostratigraphic interpretation of the oldest
ammonites reported from the Haynesville Formation.
Salvador (1991) correlated Buckner evaporitic deposits
[Buckner Formation or Buckner Member of the Haynesville
Formation (Moore, 1984); Harwood and Fontana, 1984
among others] with the evaporites and red beds of the lower
Olvido Formation in Mexico. Therefore, Buckner and lower
Olvido deposits should correspond to the stratigraphic
interval lacking ammonites. This interval expands between
the youngest ammonitiferous horizon in the Zuloaga
Formation and that containing the oldest ammonites in the
lowermost La Casita-La Caja deposits in Mexico, and
between the Smackover and the base of the Haynesville
Formation or equivalents in the northern rim of the Gulf of
Mexico Basin (Fig. 2). We assume that, during this time
interval, significant changes in sedimentation and ecology
(at least for ammonites) occurred in relation to major
geodynamic processes in the area, such as: initial separation
of the North and South American Plates (Salvador and
Green, 1980); displacement of the Yucatan platform (Burke,
1988); spreading center in North America jumping south-
ward from the Gulf of Mexico Basin to the area between
Yucatan and northern South America (Ross and Scotese,
1988); abrupt changes in the thickness of Buckner and lower
Olvido evaporites, probably resulting from salt movement
forced by contemporaneous faulting (Salvador, 1991).
The overlying lower part of the Haynesville Formation,
conformed by terrigenous and evaporitic deposits, is
tentatively correlated with the lower La Caja and La Casita
Formations, which usually yield no ammonites in north-
central Mexico. Thus, these terrigenous and evaporitic
deposits would correlate with deposits below beds with
Idoceras in the La Caja and La Casita (and the Taman)
Formations, which locally carry the Early Kimmeridgian
Schneidia Assemblage of late Platynota-earliest Hypselo-
cyclum age (Villasenor et al., 2000) (Fig. 2).
Lower Bossier-type deposits and lateral equivalents
including carbonate packages (named Gilmer or Haynes-
ville Limestone, more or less informally) overlie the lower
Haynesville Formation, which in turn overlies Buckner
evaporites. As previously discussed, ammonite records
indicate an Early, but not earliest, Kimmeridgian age for
these deposits (Imlay and Herman, 1984; Young and Oloriz,
1993), and their correlation with the stratigraphic interval
with Idoceras in the lower “La Casita Group” in Mexico
(lower La Casita and La Caja Formations) (Fig. 2).
Upper Bossier-type deposits are correlated with mainly
carbonate deposits. This could better fit a more formal
definition of the Gilmer Limestone and correspond to the
upper Haynesville Formation and the so-called Cotton
Valley Limestone. Lithostratigraphic terminology is con-
fused, as recognized by Salvador (1991), referring to the
Gilmer Limestone (a member of the Haynesville Formation
in Moore, 1984) as either equivalent to both the Haynesville
Limestone (see Forgotson and Forgotson, 1976 for defi-
nition and correlation) and the Cotton Valley Lime that
marks the top of the Louark Group, or as underlying the
Cotton Valley Group, as interpreted by Todd and Mitchum
(1977); Benson and Mancini (1984); Bracken (1984); Cregg
and Ahr (1984); Faucette and Ahr (1984); Imlay and
Herman (1984); Moore (1984); Montgomery (1996).
Published ammonites from this stratigraphic interval (e.g.
Taramelliceras, Nebrodites, Procraspedites and ‘Virgato-
sphinctes’), which correlates with the upper Bossier-type
deposits, together with unpublished ataxioceratids from the
Cotton Valley Limestone (informal term, see p.7) in a
subsurface borehole in Leon County, Texas (Oloriz, in
prep), indicate the latest Kimmeridgian rather than earliest
Tithonian for the youngest horizons in the Louark Group
(Fig. 2). These data correlate with occurrences of atax-
ioceratid ammonites in the La Casita and La Caja
Formations in Mexico (Oloriz et al., 1993; Oloriz and
Villasenor, 1999; Villasenor et al., 2000) and indicate
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142 127
diachrony for the earliest Bossier-type deposition in the
northern rim of the Gulf of Mexico Basin.
3.2.2. The Cotton Valley Group
Above the Haynesville carbonates, shale-dominated
deposits, becoming coarser-grained and terrigenous land-
ward, serve to identify the Bossier Formation s.str.
(overlying Bossier-type deposits) and the Schuler For-
mation, respectively, as well as the base of the Cotton
Valley Group, which lies on older Louark Group deposits
basinward. Overlying the carbonate packages of the
Haynesville Formation, the lowermost part of the Bossier
Formation ranges in age from the middle-late Early
Kimmeridgian to the latest Kimmeridgian; the earliest
Tithonian was an age of widespread terrigenous influx in the
northern Gulf coast. Durangites, Salinites, Spiticeratinae
and Berriasellidae in higher horizons of the Bossier
Formation indicate Early Berriasian, whereas the oldest
record of Durangites may indicate the Late Tithonian.
The age of the top of the Cotton Valley Group, as usually
placed, has been dated by calpionellids from the reefal
Knowles Limestone as the Middle Berriasian-Valanginian
(Scott, 1984). Ammonites cited by Imlay and Herman
(1984) did not come from the top of the Bossier Formation
and, therefore, indicate earlier ages within the Berriasian
and the latest Tithonian. As noted previously, further
research is needed to determine hiatuses within the upper
Cotton Valley Group; some of them could be of crucial
importance for updated correlation (Fig. 2).
4. A proposal for tectono-eustatic sequences
Recent interpretations of the Smackover Formation and
related units (Buckner deposits, and Gilmer carbonates and
siliciclastics) in the north-western rim of the Gulf of Mexico
Basin have been made in terms of ‘major sequences’
(Moore and Druckman, 1991; Heydari et al., 1997; among
others). Though the duration of these sequences is variable,
it belongs to the lower range of the excessively wide and
variable one assumed for third-order depositional sequences
(Haq et al., 1987; 1988; Vail et al., 1984; Vail and Eisner,
1989; Miall, 1991; Ponsot and Vail, 1991; Kendall et al.,
1995). The sequence architecture that we interpret for Upper
Jurassic deposits in north-central Mexico and the northern
rim of the Gulf of Mexico Basin resulted from higher-
hierarchy interactions between tectonics and eustasy. Thus,
we are concerned with the high range of third-order cycles
(4–6 Ma) and with a wider range corresponding to a set of
them (to slightly over 10 Ma). Hence, we interpret this
sequence architecture in terms of high-third-order Tectono-
Eustatic Sequences (3rd-TES) and a low-second-order
Tectono-Eustatic Supersequence (2nd-TES), following the
mean duration assumed by Mitchum (1977). Goldhammer
(1998) interpreted four major second-order supersequences
(,15 Ma approx.) for the Middle Jurassic-Lower
Cretaceous onshore in the Gulf of Mexico at the East
Texas Salt Basin, each of which exhibited subordinate third-
order sequences (1–3 Ma), but he did not give precise data
about third-order sequences. Thus, the sequences and
supersequences interpreted by Goldhammer (1998) are
hard to correlate with those that we interpret.
On the basis of ammonite biochronostratigraphy, com-
plemented with calpionellid data, we assume that major
stratigraphic features defining the Mexican Zuloaga and La
Casita “Groups”, as previously considered, can be corre-
lated with those identified in coeval deposits from the
northern rim of the Gulf of Mexico Basin. We interpret
these sedimentary packages in terms of Tectono-Eustatic
Sequences (TES) (Fig. 2). The new data we present here
update our earlier hypotheses on subsurface Groups in the
northern rim of the Gulf of Mexico Basin (Oloriz et al.,
1990).
The above controversial or rather intricate lithostrati-
graphic terminology for the northern rim of the Gulf of
Mexico Basin results from the complex pattern of facies
relationships in shallow environments in the area. Salvador
(1991) gave complete and essentially correct correlation
charts of lithostratigraphic units. Depositional models by
Moore (1984); Montgomery (1996) show the distal margin
of the carbonate shelf to be a carbonate barrier, before
‘Bossier-time’, in which the Smackover Formation and the
Gilmer Limestone, or lateral equivalents, are identified only
where ‘Buckner-deposition’ developed. In Moore’s (1984)
model, the Gilmer Limestone is a diachronous facies,
including all deposits of the Louark Group above the
Smackover Formation, i.e., the Haynesville Formation. In
contrast to the usual interpretations, Gotte and Michalzik
(1992) correlated the Gilmer Member of the Haynesville
Formation at the top of the Louark Group with the Zuloaga
Limestone, which caps the Zuloaga Group in Mexico.
In the following analysis, we only refer to shelf areas,
excluding nearshore sites and those basinward from the
outer margin that show long-term homogeneous lithofacies
(black in Fig. 2).
4.1. 3rd-TES-I
The base of this sequence (3rd-TES-I) cannot be
established accurately. Its lower part is recognizable by
the occurrence of Middle Oxfordian ammonites, indicating
the oldest identified biohorizons in the Zuloaga and
Smackover carbonates (see above; Fig. 2), and lateral
equivalents. This datum plane indicates the end of the
Callovian-Early Oxfordian phase of the geodynamic
evolution in Mexico and the Gulf of Mexico Basin, and
the initial Late Jurassic flooding (shallow open-sea waters)
following the late Middle Jurassic major paleoceanographic
changes interpreted by Jansa (1986) in the central North
Atlantic. Hanisch (1983) recognized these events through an
erosional unconformity in the North Sea Graben (Tampen
Spur). The base of 3rd-TES-I is coeval with, and related to,
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142128
a major event in plate reorganization of the Atlantic-
Tethyan domain (e.g. Ziegler, 1988) forcing wide regional
and commonly composite (coalesced) unconformities in this
domain, especially well known from the Mediterranean
Tethys and surrounding areas. From north to south, this
event is recognized in the west-Canadian Arctic (Harrison
et al., 2000), in the NW Atlantic at Jameson Land (East
Greenland), and throughout the eastern North Atlantic
margin, from the southern end of the Viking Graben in the
NE Atlantic (Hanisch, 1983) to more southern areas in
the eastern central North Atlantic, such as the Celtic Sea, the
Bay of Biscay and the Lusitanian Basin, as well as in the
Betic Cordillera (southern Spain) and the Iberian Range
(eastern Iberia) at the western Tethys (e.g. Sequeiros, 1974;
Ziegler, 1988; Aurell et al., 2000; Bernardes and Corro-
chano, 1992; Caracuel et al., 2000). Marques et al. (1991)
recognized the composite character of the discontinuity at
the base of the Upper Jurassic (DIII) in southern and western
Iberia, and Aurell et al. (2000) gave data on associated
hiatuses in eastern Iberia. The discontinuity involves at least
3–4 Ma of discontinuous (hiatal) deposition according to
the cycle-chart proposed by Haq et al. (1987, 1988), and has
been interpreted as a composite unconformity related to the
major tectonic pulse, named by Marques et al. (1991) the
Callovian-Oxfordian Crisis.
At the same time, Mexican areas belonging to the
southern North American Plate were indirectly affected by
geodynamic events (Fig. 2) determining the plate’s break-
up, including the separation of the Yucatan shelf system and
the syn-rift tectonics undergone by the Gulf of Mexico
Basin (Salvador and Green, 1980; Emery and Uchupi, 1984;
Salvador, 1987; Michaud and Fourcade, 1989). Centeno--
Garcıa et al. (1998) estimated 158 ^ 4 Ma (U/Pb) for
volcanism in northern Zacatecas, and 156–152 Ma for the
pre-deformational event associated, which indicates a
mainly Callovian geodynamic activity ending close to the
Callovian/Oxfordian boundary. Emery and Uchupi (1984)
envisioned a tectonic event of Middle-Late Jurassic
boundary age in Cuba, and proposed the existence of a
seaway between Florida and Cuba connecting the Proto-
Gulf of Mexico with the central North Atlantic (see also
Jansa, 1986). The age of this marine connection could be
Oxfordian (Cobiella-Reguera pers. comm.,1998; Cobiella
and Oloriz this issue). Moreover, at the southern margin of
the North American Plate cropping out in northwestern
Cuba, Cobiella-Reguera (1995, 1996) has documented
significant intrusions of mafic tholeitic rocks of Oxfordian
age overlain by Middle Oxfordian carbonates, i.e. the
interpreted episode of magmatism related to the beginning
of a passive-margin situation under tensional conditions and
the turnover of terrigenous deposits by Middle Oxfordian
carbonates in the area. As demonstrated in Mexico and in
the northern rim of the Gulf of Mexico Basin, the oldest
ammonite assemblages in these transgressive deposits in
Cuba indicate Middle Oxfordian (middle-late Plicatilis
Chron) age (Myczynski et al., 1998), which essentially
correlates with the base of sequence J1 in the western
Lusitanian Basin (Bernardes and Corrochano, 1992). In
southern areas of the eastern Atlantic margin, this
transgression has been recognized in the western Morocco
Mazagan escarpment area, the Haha Basin, Cape Rhir and
the Aaiun Basin, as well as in Nova Scotia on the western
Atlantic margin (Renz et al., 1975; Lancelot et al., 1977;
Lancelot and Winterer, 1980; Steiger and Jansa, 1984). In
the latter area, a Mid-Oxfordian abrupt transgression is
recognizable from Nova Scotia to the Gulf Coast (Lancelot
and Winterer, 1980). Thus, it is possible to recognize an
‘isochronous’ event at the western and eastern margins of
the central North Atlantic Basin.
The upper boundary of the 3rd-TES-I is placed close to
the Oxfordian/Kimmeridgian boundary (Fig. 2) overlain by
deposits belonging to the 3rd-TES-II (northern rim of the
Gulf of Mexico Basin) and the 2nd-TES-II/III (north-central
Mexico). Although the Middle and Late Oxfordian
corresponded to a transgressive period over the long term
(Haq et al., 1987, 1988), it included short-term fluctuations
in relative sea-level. One of these short-term fluctuations
occurred during the youngest Oxfordian and earliest
Kimmeridgian (close to the Planula-Platynota Chron
boundary, standard ammonite biochronostratigraphy in
Europe), or during the Early Kimmeridgian according to
recent reinterpretations of this stage. It has been recognized
in the Iberian Subplate and related areas (see Marques et al.,
1991 for regional updating of the global curve in Haq et al.,
1987, 1988). On this basis, shallowing trends during the
Late Oxfordian in Mexico and the Gulf of Mexico Basin
(slightly earlier in Cuba?) are interpreted as resulting from
significant and widespread interactions between tectonics
and eustasy, which are envisaged to be related to
environmental conditions determining the upper boundary
of 3rd-TES-I. Thus, the 3rd-TES-I is recognizable in north-
central Mexico and in the northern rim of the Gulf of
Mexico Basin. Future research in Cuba will determine the
significance of this tectono-eustatic sequence in the
Caribbean.
4.2. 3rd-TES-II
In this region, the base of the 3rd-TES-II sequence is
placed at the base of (within?) Buckner deposits and lateral
equivalents, and essentially correlates with the top of
Smackover carbonates (Fig. 2). Alternatively, it could be
placed between Buckner and Haynesville evaporites, but
emersion at the top of Smackover carbonates (Moore and
Druckman, 1991) during assumed high sea-levels over the
long term (Haq et al., 1987, 1988) does not favor this
hypothesis. The top of the shallow carbonate shelf systems
in the northern rim of the Gulf of Mexico Basin (Smackover
carbonates) and in north-central Mexico (Zuloaga carbon-
ates) cannot be accurately dated, but the youngest
ammonites identified indicate the Late, not latest, Oxfor-
dian. Therefore, and taking into consideration the oldest
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142 129
ammonites known from the overlying deposits, the base of
the 3rd-TES-II should be close to the Oxfordian/Kimmer-
idgian boundary, and related to a major compressional event
along western Mexico (U/Pb: 145 Ma in Centeno-Garcıa
et al., 1998), a widespread tectonic pulse involving plate
readjustment identified in Mexico (Araujo Mendieta et al.,
1982; Araujo Mendieta and Estavillo Gonzalez, 1987;
Ortuno Arzate and Delfaud, 1988; Salvador, 1991), in the
Gulf of Mexico Basin (Salvador and Green, 1980; Burke,
1988; Ross and Scotese, 1988; Salvador, 1991), in the North
Atlantic [down-faulting in the eastern Greenland margin
(Emery and Uchupi, 1984), and tectonic pulses related to the
better-developed erosional unconformity in the northern
North Sea (Hallet, 1981 in Hanisch (1983), Rawson and
Riley (1982)] and in northwestern Europe (Rawson and
Riley, 1982). Marques et al. (1991); Salas and Casas (1993)
reported coeval changes in the rate of subsidence in the
West-Tethyan epicontinental areas surrounding Iberia, and
Pena dos Reis et al. (2000) in the Lusitanian Basin in
western Iberia. Unfortunately, accurate data on the Oxfor-
dian/Kimmeridgian boundary in Cuba are unavailable, but
the significant impoverishment in ammonites during the
youngest Oxfordian slightly precedes and then shares the
same trend with Mexico and the Gulf of Mexico Basin.
Therefore, ammonite-poor deposits in the region could be
related to ecological damage resulting from tectonically
induced low relative sea levels, as suggested by Myczynski
et al. (1998).
The base of 3rd-TES-II in the northern rim of the Gulf
of Mexico Basin does not coincide with the base of the
Cotton Valley Group (Fig. 2), the lower (but not
lowermost) horizons of which yielded Idoceras in the
lower Bossier or Bossier-type shales. Thus, the base of
the Bossier or Bossier-type deposits analyzed belongs to
the Lower Kimmeridgian, above the Platynota Zone.
Terrigenous-evaporite deposits (upper Buckner and Hay-
nesville evaporites included) between Bossier, or Bossier-
type, and Smackover deposits could embrace the strati-
graphic interval from horizons close to the Oxfordian/
Kimmeridgian boundary (the Planula-Platynota Chron
boundary, Standard Ammonite Biochronostratigraphy in
Europe) to the late Platynota-earliest Hypselocyclum
Chron (Early Kimmeridgian) included. The youngest
ammonite biohorizon recognized locally in the Cotton
Valley Limestone of the Haynesville Formation (Amoco
No. 1 Jimmy Hill Gas Unit, East Texas) is close to the
Kimmeridgian-Tithonian boundary (see above), and its
recognition within assumed carbonate equivalents in the
Haynesville Formation (Gilmer and/or Haynesville Lime-
stone) remains to be made.
According to our biochronostratigraphic interpretation,
local unconformities at the base and top of the Haynes-
ville Formation at the Gulf Rim Coast (Forgotson and
Forgotson, 1976; Todd and Mitchum, 1977) resulted from
eustatic and tectonic pulses, respectively. Thus, the
unconformity at the base of the Haynesville Formation
could correspond to the sequence boundary between third-
order cycles 4.4 and 4.5 in Marques et al. (1991), with
Haynesville evaporites being lowstand deposits of the 4.5
cycle. This interpretation agrees with evidence from the
oldest ammonites known from Haynesville carbonates,
and lateral equivalent Bossier or Bossier-type shales,
indicating transgressive deposition over evaporites during
the late-Early Kimmeridgian Divisum Chron. In contrast,
the unconformity at the top of the Haynesville Formation
occurred during deposition of the transgressive system
tract of cycle 4.6 in Marques et al. (1991) and a rising sea
level over the long term, thus showing the influence of
tectonic pulses.
Goldhammer (1998) placed his SS1/SS2 supersequence
boundary at the East Texas Salt Basin within the Buckner
deposits, estimating an age of 144 Ma. Although this
regional stratigraphic datum essentially coincides with the
base of our 3rd-TES-II, the age-interpretation made by
Goldhammer (1998) indicates the correlation of the SS1/
SS2 supersequence boundary with the Platynota/Hypselo-
cyclum Zone boundary in Marques et al. (1991). Therefore,
the SS1/SS2 supersequence boundary recognized by Gold-
hammer (1998) correlates with the sequence boundary
between eustatic cycles 4.4 and 4.5 in Marques et al. (1991),
which we interpret as coinciding with the base of
Haynesville evaporites. Hence, only a minor stratigraphic
difference exists between the SS1/SS2 supersequence
boundary interpreted by Goldhammer (1998) and the base
of our 3rd-TES-II, both these levels being dated as
belonging to the same age. However, distinguishing
between evaporites belonging to the upper Buckner (low-
stand system tract of SS1) and the Haynesville (transgres-
sive system tract of SS2) Formations could be difficult
within the sequence-stratigraphic interpretation made by
Goldhammer (1998). As commented above, we interpret
evaporite deposits from the upper Buckner and the lower
Haynesville Formations to be uppermost highstand system
tract and lowstand deposits, respectively. Concerning the
boundary between the Louark and the Cotton Valley
Groups, the irregular topography recognized by Gold-
hammer (1998) at the top of the Haynesville Formation
agrees with our interpretation of tectonic pulses during
rising sea levels.
The 3rd-TES-II spans a major part of the Kimmeridgian,
as confirmed by ammonites (Fig. 2), this being a time of
active structuring in the area, as deduced from patterns of
facies relationships far more complex than in the Oxfordian
(see Salvador, 1991, for overview). Hence, Kimmeridgian
instability followed the major geodynamic event that
occurred during the latest Oxfordian-earliest Kimmeridgian
(see below). Like the 3rd-TES-I, the 3rd-TES-II in the
northern rim of the Gulf of Mexico Basin developed during
long-term sea-level rising (Haq et al., 1987, 1988). At
present, the 3rd-TES-II in the northern rim of the Gulf of
Mexico Basin is not clearly recognized in Mexico, but its
stratigraphic interval broadly correlates with the drifting
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142130
period envisaged in the central Cuba Las Villas Domain by
Alvarez Castro et al. (1998).
4.3. 2nd-TES-II/III
The lower boundary of this supersequence (2nd-TES-
II/III) in north-central Mexico is placed at the top of the
Zuloaga Formation (top of the Zuloaga Limestone), and
correlated with the Lower Olvido Formation (or with a
poorly known horizon within it). The base of this super-
sequence is correlated with the base of the 3rd-TES-II in the
northern rim of the Gulf of Mexico Basin (Fig. 2). In
contrast, the upper boundary of this supersequence in north
central Mexico does not correlate with the top of the 3rd-
TES-II in the northern rim of the Gulf of Mexico Basin. In
fact, 2nd-TES-II/III in north-central Mexico is interpreted as
embracing the longer stratigraphic interval represented by
the “La Casita Group” (slightly longer than 10 Ma) and,
therefore, its upper boundary is assumed to correlate with
the top of the Cotton Valley Group (see below). The future
subdivision of the 2nd-TES-II/III in north-central Mexico is
envisaged according to preliminary data pointing to a Late
Kimmeridgian-earliest Tithonian low relative sea level
identified in San Luis Potosı (Oloriz et al., 1996). At
present, the 2nd-TES-II/III spans from the Early, though not
earliest, Kimmeridgian to a still poorly identified Berriasian
age (Fig. 2). According to preliminary biochronostrati-
graphic data, it may locally range into the Early Valangi-
nian.
4.4. 3rd-TES-III
The 3rd-TES-III is recognizable only in the northern rim
of the Gulf of Mexico Basin (Fig. 2). Its base is defined by
the youngest level at which the Louark Group (Haynesville
Formation) is overlain by the Cotton Valley Group, and
earliest Tithonian in age (the time of definitive influx of
terrigenous sediments into the area). As previously stated,
the unconformity related to the base of the 3rd-TES-III
(Dinkins, 1968; Forgotson and Forgotson, 1976; Todd and
Mitchum, 1977) was tectonically forced, a possibility not
discarded by Salvador (1991) and compatible with data in
Goldhammer (1998). The upper boundary, which corre-
sponds with the top of the Cotton Valley Group, determines
an important discontinuity (sequence boundary) within the
Berriasian (Todd and Mitchum 1977), according to
nannoplankton data. However, a major discontinuity at the
top of the Cotton Valley Group is not recorded seismically
in some areas of Texas (McGowen and Harris 1984), and
Valanginian-Hauterivian ammonites were recorded by
Imlay and Herman (1984) from the upper part of the Cotton
Valley Group in the Humble-Benevides No. 1 well in Webb
County, Texas. When present, the discontinuity at the top of
the Cotton Valley Group is undoubtedly Early Neocomian
in age (Fig. 2), but Berriasian-Valanginian hiatuses remain
to be dated accurately.
The upper boundaries of the 3rd-TES-III (mainly a
Tithonian to Early Berriasian sequence) in the northern rim
of the Gulf of Mexico Basin and the 2nd-TES-II/III (mainly
a Kimmeridgian to Early Berriasian supersequence) in
north-central Mexico are delimited by the lower boundary
of the Lower Cretaceous TESs, which are beyond the scope
of the present study. However, the lowermost boundary (the
real bottom) for TESs in the Lower Cretaceous is assumed
to be intra-Berriasian, although finer biochronostratigraphy
is necessary for the top of the “La Casita Group” and the
Cotton Valley Group (preliminary interpretation in Fig. 2).
As noted above, the interpretation of a Tethyan phase in
the geodynamic evolution of the Chihuahua Basin (Ortuno
Arzate and Delfaud, 1988) is relevant, especially as the
result of the identification of a megasequence boundary at
the top of the La Casita deposits. The interpretation by
Emery and Uchupi (1984) of the top of the uppermost cycle
(top of the Cotton Valley Group) in the Jurassic Supercycle
identified in eastern Texas is compatible with this
hypothesis.
Unconformities capping the uppermost Jurassic in
Atlantic areas have usually been referred to as the ‘Late
Cimmerian unconformity’. In fact, the latter has been
related to a major rifting pulse associated with an abrupt
sea-level fall (Ziegler, 1977; Vail et al., 1977) affecting the
North Atlantic rift system and related areas during the Late
Jurassic/Early Cretaceous transition (Ziegler, 1988 among
others). However, based on available biostratigraphic data,
we agree with Rawson and Riley (1982) that the term ‘Late
Cimmerian unconformity’ is an oversimplification. Data
from the Upper Jurassic of the NE Atlantic (North Sea)
given by Hanisch (1983) are of special relevance, showing
two major regional unconformities in the area, the better
developed being registered at the base of the Kimmeridgian
and the younger within the Berriasian. The age interpret-
ation for the latter agrees with the updated interpretation of
calpionellids reported by Jansa et al. (1980), partly
improved by Jansa (1981); Jansa et al. (1982). The updated
interpretation is based on ammonite-calpionellid correlation
in Tavera et al. (1994), and the most complete and updated
calpionellid biostratigraphy from the westernmost west-
Tethys (Oloriz et al., 1995). This, in turn, shows higher
potential for correlation of related tectonic disturbances and
hiatuses between the Canadian Atlantic Shelf and the North
Sea in the NE Atlantic.
The 3rd-TES-III in the northern rim of the Gulf of
Mexico Basin, as well as the Tithonian-Berriasian part of
the 2nd-TEM-II/III in north-central Mexico, developed
during a long-term sea-level low, before the eustatic sea-
level rise during the Late Berriasian (Haq et al., 1987, 1988;
Marques et al., 1991). Terrigenous deposition with shallow-
ing and coarse-upward sequences (Salvador, 1991) is
consistent with such an eustatic context, but see Gold-
hammer (1998) for the East Texas Salt Basin. However, the
abrupt ending of the uppermost carbonates in the Louark
Group used to place the boundary between the 3rd-TES-II
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142 131
and 3rd-TES-III in the northern rim of the Gulf of Mexico
Basin, together with evidence for tectonic pulses in Mexico
(Oloriz et al., 1996, 1998c, 1999), indicate interactions
between tectonics and eustasy. In areas where these tectono-
eustatic events severely affected deposition (northern rim of
the Gulf of Mexico Basin), the recognition of the 3rd-TES-
III in the Upper Jurassic is strengthened. In contrast, where
the influence of tectono-eustatic interactions was more
restricted, or less known, (north-central Mexico) further
research is necessary to interpret stratigraphic sequences
and their meaning on the basis of updated ammonite
biochronostratigraphy and correlation.
Gotte and Michalzik (1992) inferred the existence of
two megasequences in Mexico and the northern rim of
the Gulf of Mexico Basin, referring to tectonic control at
least for their lower megasequence. This megasequence
embraced a “Zuloaga Group” composed of the La Joya,
Minas Viejas and Zuloaga Formations in the Eastern
Sierra Madre (its correlative in the northern rim of the
Gulf being the Louark Group as reinterpreted by Gotte
and Michalzik, 1992). However, this megasequence is
rather difficult to correlate, since it includes lower
terrigenous and evaporite units lacking biostratigraphic
control for reliable stratigraphic interpretation (cf. Moran
Zenteno, 1984; Longoria, 1984; Meyer and Ward, 1984;
Moore, 1984; Lopez-Ramos, 1985; Salvador, 1991).
Moreover, the upper boundary of the lower megase-
quence proposed by Gotte and Michalzik (1992), which
includes their “Zuloaga Group” and their correlative
Louark Group, should be latest Kimmeridgian-earliest
Tithonian in age, according to recent data from the
Haynesville carbonates. However, this hypothesis is
untenable for the Zuloaga Limestone and lateral equiva-
lents in Mexico. In addition, the top of the upper
megasequence in Gotte and Michalzik (1992), which
includes the La Casita deposits and the assumed
correlative Cotton Valley Group, represents neither the
top of the Tithonian nor, therefore, the Jurassic/Cretac-
eous (Tithonian/Berriasian) boundary.
5. Discussion
The lithostratigraphic units analyzed (Mexican “Groups”
in land outcrops and formal subsurface Groups in the
northern rim of the Gulf of Mexico Basin) and the tectono-
eustatic sequences and supersequences interpreted are not
correlative. The Mexican Zuloaga and La Casita “Groups”
comprise the Mexican 3rd-TES-I (mainly Middle-Late
Oxfordian) and 2nd-TES-II/III (mainly Kimmeridgian to
partly Berriasian). In contrast, the Louark and Cotton Valley
Groups cannot be correlated with the 3rd-TES-I (mainly
Middle-Late Oxfordian), 3rd-TES-II (mainly Kimmerid-
gian) and 3rd-TES-III (mainly Tithonian-Early Berriasian)
interpreted in the northern rim of the Gulf of Mexico Basin.
The lack of correlation between these major
lithostratigraphic units in north-central Mexico and the
Gulf of Mexico Basin indicates differential responses to
geodynamic evolution in these regions.
The Oxfordian 3rd-TES-I embraces the interpreted
“Zuloaga Group”, including lower Olvido deposits in
north-central Mexico. In the northern rim of the Gulf of
Mexico Basin this sequence is represented by Smackover
carbonates and, probably, a lower part of Buckner evaporites,
the extent of which is difficult to specify (Fig. 2). The
correlation of the Buckner Member with the lower part of the
Mexican Olvido Formation (Imlay, 1942, 1945, 1952;
Wilson et al., 1984) has been tentatively interpreted as
ranging from Late Oxfordian to Early Kimmeridgian (Imlay,
1942, 1945, 1953; Wilson et al. 1984). Salvador (1991)
correlated Buckner evaporites with the terrigenous-evapori-
tic deposits of the lower Olvido Formation, and considered
the upper carbonate Olvido as roughly equivalent to the
upper part of the Haynesville Formation ( ¼ Gilmer Lime-
stone and its informal equivalent termed Cotton Valley
Limestone), a correlation also admitted by Goldhammer
(1998) for the East Texas Salt Basin. Gotte and Michalzik
(1992) proposed the correlation of the Lower Olvido with the
Minas Viejas Formation and interpreted the upper Olvido
limestones as a time marker and lateral equivalent to the
Gilmer Limestone.
On the basis of our data and revision of ammonites, we
agree with the correlation of Olvido evaporites (lower
Olvido) with Buckner deposits. However, we cannot support
the complete correlation proposed by Salvador (1991), given
the tectonic context that we envisage, since it could have
resulted in a period of instability and shallow-water
environments, hampering the precise correlation of shifting
lithofacies without biochronostratigraphic control. This is
especially true for the correlation of the Upper Olvido with
the entire Haynesville carbonate interval, an interpretation
not supported by current paleontological data but assumed by
A. Salvador based on electric logs (pers. comm. to FO,1998).
Goldhammer (1998) also interpreted the Upper Olvido and
the entire Haynesville carbonate intervals as correlative,
based on sequence stratigraphy and composite accommo-
dation models. However, the only paleontological support
for interpreting the uppermost Olvido deposits could perhaps
be the indirect interpretation made by Imlay (1943), who
interpreted the Olvido Formation as Lower Kimmeridgian,
below horizons with Idoceras balderum. Imlay’s (1943)
interpretation has been supported by subsurface data in the
Burgos Basin (NE Mexico) showing Olvido deposits below
La Casita horizons with Idoceras (Cantu-Chapa, 1998). The
undefined top for Olvido deposits in Fig. 2 reflects the
inconclusive stratigraphy available, especially if the typical
diachrony at the top of the Haynesville Formation is taken
into account.
Despite the difficulty in the precise identification of a
sequence boundary within or between terrigenous-evapor-
ite successions, especially in a context of tectono-eustatic
interactions (see above), the easy correlation of
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142132
the 3rd-TES-I in north-central Mexico and the northern rim
of the Gulf of Mexico Basin points to a time of minor
differentiation in geodynamic evolution during the Middle
and Late Oxfordian in these regions.
According to our biochronostratigraphic correlation of
American and European margins of the North Atlantic
Basin (Fig. 1), the 3rd-TES-I (Fig. 2) spans a clearly
evidenced Middle-Late Oxfordian (earliest Kimmeridgian?)
tectono-eustatic cycle in the central North Atlantic. Data
available from western Africa recovered from the Moroccan
to the Senegal Basins agree with this interpretation. The
Atlantic transgression during the early-Middle Oxfordian,
used to place the lower boundary of the 3rd-TES-I, is well
documented in southwestern Morocco, the Essaouira and
Aaiun-Tarfaya Basins, and at Cape Rhir in the Western
High Atlas (Lancelot and Winterer, 1980). More reliable
data have been obtained from the Mazagan escarpment area
and DSDP site 367 in the Cape Verde Basin (Renz et al.,
1975; Lancelot et al., 1977; Jansa et al., 1977; Renz, 1977).
In the Mazagan escarpment, Renz et al. (1975) dated the
lower yellow-brown limestone at the dredge haul V30-
RD38 as Middle Oxfordian, and later confirmed this age in
close highs (DSDP sites 544A and 545) of the Mazagan
escarpment area (Renz, 1984). Southwards, in the Cape
Verde Basin (DSDP site 367), the radiometric age of basalts
(Jansa et al., 1977) correlates with the stratigraphic location
interpreted for the lower boundary of the 3rd TES-I
discussed. On the assumption of the similarity in deposi-
tional conditions between the central North Atlantic and
western Tethys (Bernoulli, 1972; Lancelot et al., 1977;
Jansa et al., 1984), and the age of common changes in
lithofacies in the epicontinental Upper Oxfordian from
southern Spain (Prebetic), shifts between ammonitico rosso
type facies and gray mudstones containing Oxfordian-
Kimmeridgian aptychi at DSDP site 367 (implicitly
interpreted as close to the Oxfordian/Kimmeridgian bound-
ary by Renz, 1977) could be reinterpreted as Late
Oxfordian, at least that recorded from sample 35. Thus, it
could be correlative with the upper boundary of the 3rd-
TES-I. This interpretation agrees with the Late Oxfordian-
earliest Kimmeridgian age interpreted by Renz et al. (1975)
for ammonites recovered from the white limestone over-
lying the Middle Oxfordian yellow-brown limestone at the
Mazagan escarpment (West Morocco), thus assuming,
implicitly, a Late Oxfordian shift in lithofacies at dredge
haul V30-RD38.
The aforementioned stratigraphic interval, embracing the
3rd-TES-I in north-central Mexico and in the northern rim
of the Gulf of Mexico Basin, correlates with the part of the
S1 supersequence in the South Iberian paleomargin
(Marques et al., 1991) between its base and the top of the
tectono-eustatic sequence KI. In eastern Iberia the correla-
tives are the majority of sequence J8 in Salas and Casas
(1993), except its hiatal lowermost part, and the J3.3 and
J3.4 sequences of Aurell et al. (2000). In western Iberia, this
stratigraphic interval basically correlates with sequences J1
and J2 in the western Lusitanian Basin (Bernardes and
Corrochano, 1992) and with the tectono-sedimentary stage
interpreted by Pena dos Reis et al. (2000) in relation with
the onset of rifting (rift initiation) throughout the Lusitanian
Basin.
In the central Cuba Las Villas Domain, drifting began
during the Early Kimmeridgian (Alvarez Castro et al., 1998)
after the turnover from ammonite-rich to ammonite-barren
deposits during Late, not latest, Oxfordian. Thus, with
minor uncertainty, it is possible to identify a structuring
phase affecting the Mexico-Caribbean region, the central
North Atlantic Basin and northwestern Tethys epicontinen-
tal shelves, i.e. a tectonic event undergone by the central
North Atlantic, according to the stratigraphic imprint on
areas close to the western and eastern margins of the basin.
After the latest Oxfordian-earliest Kimmeridgian tec-
tonic phase, fine-grained terrigenous sedimentation over-
whelmingly dominated in the north-central Mexico and
basinward sites in the northern rim of the Gulf of Mexico
Basin, resulting in a renewed phase of sedimentation
interpreted as the 2nd-TES-II/III and 3rd-TES-II in these
areas, respectively. However, a more restricted carbonate
deposition persisted in the northern rim of the Gulf, with
episodic terrigenous inputs during the Kimmeridgian. This
pattern is evidenced by diachronous boundaries between
Louark carbonates and Bossier (or Bossier-type) shales,
thus determining the diachronous boundary between the
Louark and the Cotton Valley Groups. Relatively homo-
geneous deposition in the “La Casita Group” during the
Kimmeridgian and earliest Tithonian contrasts with the
intricate pattern of facies characteristic of the Kimmeridgian
part of the Louark Group. This demonstrates the differences
in geodynamic evolution, such as greater basin stability in
north-central Mexico, than in the northern rim of the Gulf of
Mexico Basin, which progressively and episodically
deepened.
The sharp decrease in carbonate deposition close to the
Oxfordian/Kimmeridgian boundary, together with the
dominance of terrigenous sedimentation during the Kim-
meridgian, indicates tectonic influence: a tilting that caused
rejuvenation, changes in depositional conditions; and
ecological stress during high but fluctuating relative sea
levels in Mexico (clastics of the “La Casita Group”).
McGowen and Harris (1984) related the terrigenous input in
the southeastern USA to a tilt-reversal phase affecting the
rift margins along the northern rim of the Gulf of Mexico
Basin, which was probably coeval with the beginning of
differential subsidence of the central Gulf as suggested by
Salvador (1987). According to our biochronostratigraphic
interpretation, the tilt-reversal phase began during the Early
Kimmeridgian, then continued episodically during the
Kimmeridgian, and ended close to the Kimmeridgian/
Tithonian boundary. The Kimmeridgian/Tithonian bound-
ary is correlated with the sequence boundary between 3rd-
TES-II and 3rd-TES-III in the northern rim of the Gulf of
Mexico Basin. This might correlate with the change from
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142 133
green-gray interbedded calcareous claystones and lime-
stones to the grayish-red calcareous claystones of the Cat
Gap Formation at DSDP site 534 (dated by Habib and
Drugg, 1983), which could be related to a hiatus according
to Ogg et al. (1983). The ages interpreted for the boundaries
of the 3rd-TES-II in the northern rim of the Gulf of Mexico
Basin correlate with the main events of shallowing and
deepening in the Guaniguanico Cordillera (Myczynski,
1994), which span the period for drifting in central Cuba as
suggested by Alvarez Castro et al. (1998).
In north-central Mexico, Kimmeridgian to Early Berria-
sian deposits of the La Casita Group show the 2nd-TES-
II/III. Relatively homogeneous deposition, indicating inter-
actions between tectonics and eustasy, makes it difficult to
identify shorter stratigraphic intervals. However, deposi-
tional events in the Middle (three-fold division) Kimmer-
idgian (Oloriz et al., 1988, 1998b,c) and the Late
Kimmeridgian to Early, or Early-Middle, Tithonian (Oloriz
et al., 1996, 1999) could be informative and will be
investigated on the basis of improved ammonite
biochronostratigraphy.
Biochronostratigraphic data from eastern Mexico, closer
to the western rim of the Gulf of Mexico Basin, show the
turnover between the Taman and Pimienta Formations
occurring early, but diachronically, during the Tithonian
(Cantu-Chapa, 1967, 1984). This fact indicates changing
geodynamic history in intermediate areas between the Gulf
of Mexico Basin and north-central Mexico.
In northern Chihuahua and southwestern Texas, Cantu-
Chapa (1976) recognized an Early Kimmeridgian transgres-
sion followed by increased drowning during the Tithonian
and then regression during the Late Tithonian, which in fact
is Early Berriasian. Combined biochronostratigraphic and
lithologic data given by Cantu-Chapa (1976) are valuable,
but too limited for a conclusive interpretation. Despite this
shortcoming, Cantu-Chapa’s (1976) data demonstrate the
late-Early Kimmeridgian age for the widely known record
of Idoceras in Mexico related to the progressive homogen-
ization in depositional conditions following a southeastern-
northwestern trend, from Sierra de Almagre to Sierra de
Chorreras and Placer de Guadalupe, during the Late
Kimmeridgian and Tithonian. The lack of data about
depositional discontinuities and/or precise changes in
lithofacies, impedes the identification and/or correlation of
stratigraphic intervals between the initial transgression and
final regression recognized by Cantu-Chapa (1998). The
base and top of this Late Jurassic-earliest Cretaceous marine
flooding in northern Chihuahua and SW Texas correlate
with the 2nd-TES-II/III that we propose for north-central
Mexico, especially in areas where it was slightly delayed (in
terms of ammonite biochronostratigraphy) during the Early
Kimmeridgian. In addition, the beginning of the Tithonian
drowning interpreted by Cantu-Chapa (1998) could be
roughly correlative with the 3rd-TES-II/TES-III boundary
proposed for the northern rim of the Gulf of Mexico Basin.
The duration of the drowning would then be equivalent to
the time-span interpreted for 3rd-TES-III. Thus, in a strictly
transitional area between these two major regions, evidence
exists to support our interpretations.
For the Tethys–North Atlantic Rift System, Late
Jurassic-earliest Cretaceous data indicate significant phases
of individualization during this time-interval of clear
separation between Europe and the North American Plate,
as stated by Rehault and Mauffret (1979). Updated
biochronostratigraphy supports a Middle Oxfordian age
for the lower boundary of the Zuloaga and the Louark Group
analyzed, while tops of the La Casita Group and the Cotton
Valley Group are commonly placed within the Berriasian,
and locally within the Early Valanginian. Between these
age-limits the second and fourth Upper Jurassic cycles have
been identified within the Upper Jurassic Supercycle in the
Gulf of Mexico Basin, and have been interpreted as natural
divisions of the Drift Supersequence (Emery and Uchupi,
1984). In addition, this Late Jurassic-earliest Cretaceous
interval represents one of the significant events in the
Mesozoic evolution of the North Atlantic, determining
the second sequence bounded by major unconformities in
the Lusitanian Basin (Wilson, 1988). These unconformities
correlate with the base of J1 and the top of J6 sequences in
the succession of lower-order depositional sequences
identified by Bernardes and Corrochano (1992) in the
western Lusitanian Basin. The Upper Jurassic Supercycle
proposed by Emery and Uchupi (1984) embraces cycles and
the respective second and third megasequences (Lopez-
Garrido and Garcıa-Hernandez, 1988) within the so-called
Jurassic Cycle in the Prebetic Zone of southern Iberia
(Garcıa-Hernandez and Lopez-Garrido, 1988). The uncon-
formity-related lower boundary assumed by Emery and
Uchupi (1984) for the Upper Jurassic Supercycle in the Gulf
of Mexico correlates with the beginning of the second-phase
of rifting in west Iberia (Mougenot et al., 1979; Rehault and
Mauffret, 1979). This unconformity is known from the west-
Canadian Arctic Amerasian Basin (Harrison et al., 2000)
and is widely recognized in the North Atlantic Basin (Todd
and Mitchum, 1977), especially on the European margin
(Ziegler, 1988), as well as in westernmost Tethyan southern
Europe (Ramalho, 1985; Marques et al., 1991). Emery and
Uchupi (1984) established a ‘Valanginian/earliest Cretac-
eous’ age for the top of the Upper Jurassic Supercycle in
eastern Texas and the Gulf of Mexico. According to
available updated biochronostratigraphy, the age of this
boundary appears to be intra-Berriassian and, therefore,
correlative with unconformities in epicontinental shelves
surrounding Iberia.
In western Iberia, earliest Cretaceous unconformities
were related to local emersion and erosion capping the Late
Jurassic carbonate platform bordering the western Iberia
foreland and its marginal uplifted blocks. This extended
westwards to form part of a great carbonate-shelf system
reaching the conjugate Canadian protomargin, according to
Comas et al. (1988). Data about Anchyspirocyclina
lusitanica provided by these authors support this
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142134
interpretation, showing close correlation with the upper part
of the third cycle and the widespread emersion recognized
by Garcıa-Hernandez and Lopez-Garrido (1988) at
the Portlandian/Berriasian boundary in the Prebetic Zone
(southern Spain). This interpretation agrees with the placing
of the top of J6 sequence by Bernardes and Corrochano
(1992) and with evidence for distensive pulses during the
Late Tithonian/Berriasian transition (Pena dos Reis et al.,
2000) within the so-called Upper Jurassic-Berriasian Cycle
identified on land outcrops from the Lusitanian Basin
(western Iberia). Northwestwards, there is evidence
(Groupe Galice et al., 1979; Sibuet and Ryan, 1979)
indicating a Late Jurassic-Early Cretaceous tectonic episode
responsible for major trends in the configuration of the
continental margin in the Galicia Bank and the Vigo
Seamount areas (northwestern Iberia), involving rotating
fault activity in both the Iberian and the Armorican margins.
Groupe Galice et al. (1979) interpreted important epeiro-
genic movements at the end of the Jurassic in the northern
part of the Portuguese Basin. These movements forced a
marked regression with deposition of red sandstones, which
correlates with widespread continental deposition in
Western Europe. In eastern Iberia, Aurell et al. (2000)
have reported a widespread discontinuity at the end of the
Berriasian, preceded by a more restricted one at the
Tithonian/Berriasian boundary, but biostratigraphic data
are scant, as is usual in very shallow environments. Salas
and Casas (1993) interpreted a regional unconformity
capping the so-called Jurassic Supersequence in eastern
Iberia, and an intra-Berriasian unconformity bounding their
‘Jurassic’ sequences J10 and J11. Paleomargin instability
(calciturbidites) during the widespread latest Jurassic-
Neocomian regression in northwestern Africa (DSDP sites
370 and 416) is correlative on the basis of updated
biochronostratigraphy, mainly the calpionellids reported
by Vincent et al. (1980a,b).
Between the Middle Oxfordian and the Early-Middle
Berriasian, Marques et al. (1991) recognized four major
events of interaction between tectonics and eustasy
affecting the Iberian Subplate: (1) The Callovian-Oxfor-
dian Crisis, which led to coalesced unconformities
embracing more than two low-third-order eustatic cycles
at the Middle-Upper Jurassic transition; (2) The Final-
Oxfordian Crisis, which played a significant role in the re-
structuring of epicontinental shelves surrounding Iberia
close to the Oxfordian/Kimmeridgian boundary, and
brought about a low-third-order tectono-eustatic sequence
(KI) in the South Iberian paleomargin (in relation to a
tectonic pulse also recognized in eastern and western
epicontinental shelves in Iberia and northwestern Africa);
(3) The Middle Kimmeridgian Event, related to a slow but
persistent uplift of epicontinental shelves favoring the
typical growth of carbonate shelves during more than 3
third-order eustatic cycles; and (4) The Early-Middle
Berriasian Crisis, a wide regional event commonly
identified through an unconformity within Cycle 1.4
in the Supercycle LZB-1 proposed by Haq et al. (1987,
1988) and revised by Marques et al. (1991) for
southern Iberia.
According to the interpretation of the Tithonian/Berria-
sian boundary in southern Spain by Tavera et al. (1994) and
the most accurate calpionellid biostratigraphy known from
the westernmost west-Tethys at the Sierra Norte (Mallorca
Island, eastern Spain; Oloriz et al., 1995), the following
geologic traits recognized in Atlantic margins other than
Iberian ones, and geologically related areas, correlate with
the Early-Middle Berriasian Crisis interpreted by Marques
et al. (1991): (1) early phases of seafloor spreading in the
Amerasian Basin, as dated by Rowley and Lottes (1988) and
correlated with the best interim evaluation for the Jurassic
time-scale considered by Odin (1992) and the European
ammonite biochronostratigraphic standard scale for the
Tithonian (Geyssant and Enay, 1991); (2) tectonic disturb-
ances, hiatuses and related unconformities reported for the
Scotian and East Newfoundland Basins (Jansa et al., 1980,
1982; Jansa, 1981); (3) the bottom of the white chalky
limestone in the Atlantic margin of North America at the
DSDP site 105 (lower continental rise hills between New
York and Bermuda; Lehman, 1972), DSDP site 391c
(Blake-Bahama Basin; Wind, 1978), and DSDP site 534
(Blake-Bahama Basin; Habib and Drugg, 1983; Roth 1983;
Roth et al., 1983), though Remane (1983) interpreted an
apparently older age for the bottom of the Blake-Bahama
Formation, considering the basal Berriasian as indicated by
the upper part of the Calpionellid Zone B. Remane’s (1983)
interpretation resulted in an excessively extended Tithonian
stage in Hole 543A; (4) increased subsidence of Atlantic
margins in the Florida-Bahamas and Yucatan shelves,
affecting northern Cuba (Myczynski and Pszczokowski,
1994); (5) the third episode of magmatism in western Cuba
(Cobiella-Reguera, 1996), but see Cobiella-Reguera and
Oloriz (in progress); (6) the oceanic crust (ophiolites) in the
central Cuba Las Villas province (Llanes Castro and Garcıa
Delgado, 1998); (7) distal turbidite deposition in the
Moroccan Basin at DSDP site 416 (Vincent et al., 1980a,
b); (8) the Berriasian unconformity at the Mazagan
escarpment (DSDP site 547B) with associated deposits
containing Remaniella ferasini (Azema and Jaffrezo, 1984),
although the related hiatus was interpreted to be post-
Berriasian by Jansa et al. (1984). Note that Remaniella
cadishiana (FAD placed at the mid-Zone B ¼ middle-Early
Berriasian in Mallorca according to Oloriz et al., 1995) was
the first record of calpionellids reported by Vincent et al.
(1980b) from calciturbidites at DSDP site 416; and finally
(9) the significant shift in lithofacies within the Cape Verde
Basin (DSDP site 367; Jansa et al., 1977), and probably that
recognized by Arthur et al. (1979) in drill hole CORC 15-1
at the Aaiun Basin, onshore southwestern Morocco (former
Spanish Sahara). Thus, these data point to a rather
isochronous tectono-eustatic pulse in the central North
Atlantic and geodynamically related areas, which correlates
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142 135
with tectonic events known from distant northern regions
such as the Canadian Arctic.
In north-central Mexico and the northern rim of the Gulf
of Mexico Basin (and western Cuba in terms of ammonite
paleobiogeography according to Myczynski, 1994), the
Middle Oxfordian-Berriasian/Lower Valanginian strati-
graphic interval identified is broadly coeval with the
Supercycles LZA-4 þ LZB-1 þ lowermost LZB-2 of Haq
et al. (1987, 1988) in the western Tethys. A long-term rising
sea level during the lower LZA-4 (Early-early Middle
Oxfordian–Early Kimmeridgian) was tectonically punctu-
ated in Mexico and the ancestral Gulf of Mexico region
during the youngest Oxfordian to the Early Kimmeridgian
up to the late Platynota or earliest Hypselocyclum Chron.
Active faulting, salt movement, and supratidal conditions in
the northern rim of the Gulf of Mexico Basin (Buckner
deposits), are assumed to be coeval with the general erosion
and/or non-deposition together with local shallow subtidal-
supratidal evaporite deposition in Mexico. These events
ended the Late Jurassic carbonate-shelf deposition phase
(Zuloaga and mainly lower Olvido deposits). The hiatus that
Medd (in Ogg et al., 1983) envisaged and related to the
beginning of the lower green-gray interbedded calcareous
claystone and limestone of the Cat Gap Formation at DSDP
site 534 (Habib and Drugg, 1983), and the better-expressed
unconformity identified by Hanisch (1983) at the base of the
Kimmeridgian in the northern North Sea, could be useful for
correlation.
The end of the tilt-reversal phase in the ancestral Gulf
area caused the exclusiveness of the terrigenous deposition
during the Tithonian and Berriasian, which characterizes the
Cotton Valley Group before Early-Middle Berriasian
transgressive pulses favoring reefal growth (Knowles
Limestone). The tectonic imprint during the latest Jur-
assic-earliest Cretaceous in the area is clearly shown by the
regressive trend recognized by Salvador (1991) for Cotton
Valley deposits, the context of increasing accommodation
interpreted by Goldhammer (1998) at the East Texas Salt
Basin, and the assumed global sea-level fall over the long
term (Haq et al., 1987, 1988; Marques et al., 1991). In the
absence of precise ammonite biochronostratigraphy, calpio-
nellid data together with a careful analysis of depositional
features of the Knowles facies should improve the
interpretation of depositional history during the Berriasian.
According to the above interpretation, the geodynamic
structuring of the ancestral Gulf of Mexico during the Late
Jurassic, as recorded in its northern rim, was causally related
to that occurring in north-central Mexico, although partly
diachronous. The combined “Atlantic-Tethyan cachet” of
this structuring is recognized through shared trends with
some northwestern margins of the Tethys. Hence, an Upper
Jurassic Supercycle can be recognized, including latest
Oxfordian-earliest Kimmeridgian tectonic pulses within the
Late Mesozoic Break-up Phase of plate reorganization, as
interpreted by Ziegler (1988) for the North Atlantic and
Tethys. Reliable data from the Iberian Plate have been
provided by Garcıa-Hernandez and Lopez-Garrido (1988);
Lopez-Garrido and Garcıa-Hernandez (1988); Wilson
(1988); Marques et al. (1991); Bernandes and Corrochano
(1992); Salas and Casas (1993); Aurell et al. (2000); Pena
dos Reis et al. (2000). Salas and Casas (1993) emphasized
the close correlation between the course of geodynamic
evolution in the North Atlantic and Iberia during the Late
Jurassic and the Early Cretaceous. In a wider regional
context, Lemoine (1983) recognized ‘good agreement’ (lit.
translation) between the evolution of the central North
Atlantic and the Ligurian Tethys, which he interpreted as
following nearly the same timing for transition from rifting
to drifting.
In the Mexican-Gulf-Caribbean region, very shallow
waters and local supratidal conditions prevailed, probably as
a consequence of the differential uplift induced by
progressive separation of the North and South American
Plate during the Oxfordian (3rd-TES-I), reaching substantial
separation from latest Oxfordian-earliest Kimmeridgian
onwards. The episodic deepening of the central Gulf region,
with a final Jurassic phase close to the Kimmeridgian/-
Tithonian boundary, marked a significant difference in the
geologic evolution between the northern rim of the Gulf of
Mexico Basin (and probably western Cuba) and north
central Mexico. This resulted in the possibility for
recognition of the 3rd-TES-II and, therefore, the overlying
3rd-TES-III in the northern rim of the Gulf of Mexico Basin
before the significant fluctuations in relative sea level,
which marked the end of the latter sequence during the
Berriasian.
In the regional cycle chart proposed by Todd and
Mitchum (1977) for the Texas Gulf Coast (slightly adapted
by Emery and Uchupi, 1984), the lower boundary of J3.1
might be placed within the Middle Oxfordian (probably
intra-Plicatilis Zone). The boundary between cycles J3.1
and J3.2 is reinterpreted as close to the Kimmeridgian/
Tithonian boundary, assuming local variation. Available but
inconclusive biochronostratigraphic data indicate diachron-
ism of the upper boundary of the J3.2 cycle related to
differential topography and subsidence in this region. A
detailed study of the uppermost beds of the J3.2 cycle and
the lowermost beds of the K1.2 cycle is needed. The
reinterpreted J3.2 cycle fits well with the 3rd-TES-III
interpreted in the area (doubts persist for its comparatively
poorly-known upper part; see Fig. 2), but the J3.1 cycle
cannot be correlated at the scale we used. The recognition of
three TESs in the northern rim of the Gulf of Mexico Basin
could be consistent with a subdivision of the Kimmeridgian-
Berriasian 2nd-TES-II/III in north central Mexico (prelimi-
nary data in Oloriz et al., 1999).
More research based on updated ammonite and calpio-
nellid biochronostratigraphy is necessary to understand the
preserved features of the geo-biological evolution in
Mexico and the Gulf of Mexico Basin during the Late
Jurassic-earliest Cretaceous. This evolution determined the
Upper Jurassic Supercycle, also identified in the Iberian
F. Oloriz et al. / Journal of South American Earth Sciences 16 (2003) 119–142136
Subplate, showing significant geologic traits within a
suitable stratigraphic framework for understanding of the
Late Jurassic evolution of the central North Atlantic.
We agree with previous authors who argue for an
Atlantic–Western Tethys System during the Late Jurassic,
emphasizing that ‘synchronism’ could be higher than
suspected, at least in terms of current ammonite and
calpionellid biochronostratigraphy, which is not contra-
dicted by autocyclic factors forcing local deviations.
We envision the future subdivision of Mexican TESs into
lower-order sequences, especially within widely distributed
Kimmeridgian-Tithonian deposits containing time-marker
fossils enabling differentiation between eustatically and
tectonically driven sedimentation. A similar treatment could
be applied, more locally, to Oxfordian deposits. In such a
context, improved stratigraphy in the northern rim of the
Gulf of Mexico Basin, Mexico and Cuba will provide new
insights into the geological, and then geobiological,
evolution in the Mexico-Caribbean area and its relation to
the development of the central North Atlantic Basin and the
Atlantic-Pacific connection.
Acknowledgements
This research was made under financial support from
DGAPA (UNAM, Mexico), Project PB97-0803 DGICYT
(Spain) and the EMMI Group (RNM 0178 Junta de
Andalucıa, Spain). This paper benefited from insightful
comments and suggestions made by A. Salvador (University
of Texas at Austin, USA) and L. Jansa (Geological Survey
of Canada; Bedford Institute of Oceanography, Dartmouth,
Nova Scotia) on an early draft of the manuscript. Final
revision by Jansa and G.E.G. Westermann (McMaster
University, Canada), as well as editorial suggestions are
acknowledged. We are indebted to Houston BP-Amoco for
permission to advance ammonite data from core-sections in
East Texas.
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