Barra Honda (Upper Paleocene--Lower Eocene) and El Viejo (Campanian-Maastrichtian) carbonate platforms in the Tempisque area (Guanacaste, Costa Rica).
En la zona de Palo Verde (Fig. 5) las facies tipicas de Barra Honda pasan a facies de alta energia, caracterizadas por la presencia de macroforaminiferos del Paleoceno Superior-Eoceno Inferior Ranikothalia catenula, Neodiscocyclina barkeri asociados a Ethelia alba.
En el cerro Espiritu Santo se observa la transgresion de la plataforma de Barra Honda sobre lutitas siliceas alteradas y cubiertas por un posible paleosuelo, estas lutitas descansan sobre basaltos. Las primeras capaz de plataforma contienen cantos rodados y perforados tipicos de la zona costera.
En el extremo sur de los afloramientos de Barra Honda, cerca de Pochote observamos una secuencia que documenta el retrabajo de clastos del Cretacico terminal en un ambiente de mar abierto, estan caracterizados por abundantes foraminiferos planctonicos del Paleoceno Superior (Morozovella velascoensis) y Pentacrinites sp. (crinoideo de plataforma abierta). La secuencia pasa gradualmente a facies tipicas de Barra Honda hacia el techo. Calizas de plataforma somero datados del Eoceno Inferior--Medio afloran como pequenos monticulos en la region de la Laguna Jicote, en el noroeste de la zona estudiada. Se caracterizan por una microfacies rica en algas rojas (Coralinaceas) y macroforaminiferos (Discocyclina, Eoconuloides Wellsi, Amphistegina). Por ahora no podemos interpretar el origen de estos afloramientos. La plataforma Barra Honda sobreyace discordantemente a las formaciones deformadas del Cretacico Superior-Paleoceno. tanto al oeste del rio Tempisque, como en la zona de Palo Verde. Al este del rio Tempisque, en la zona del cerro Naranjo, el contacto basal de Barra Honda se caracteriza por la deformacion semiplastica intensa de las formaciones detriticas subyacentes, las cuales pueden ser tan jovenes como el Eoceno Medio. El emplazamiento de Barra Honda sobre estas formaciones puede ser atribuido a una compactacion de las formaciones detriticas y un asentamiento de las calizas, aunque tambien puede ser un resultado de una situacion transcompresiva, a lo largo de las fallas longitudinales que han sido senaladas a lo largo del Tempisque.
ABSTRACT: In this preliminary paper we report on age, microfacies, microfossils and structural setting of platform limestones, that crop out in the Rio Tempisque arca (Guanacaste, Costa Rica). The limestones can be attributed to two distinct carbonate platform systems: 1. The El Viejo Platform, dated as late Campanian--Maastrichtian, which is represented by slope facies in the Cerros Ballena and Cebollin (near Filadelfia, Peninsula de Nicoya). 2. The Barra Honda Platform, of Upper Paleocene--Lower Eocene age, that extends from the classical outcrops at Cerro Barra Honda in the South, to the Palo Verde region in the North.
At Cerro Cebollin, carbonate-rich turbitites and mass flow deposits test unconformably on basalts of the Nieoya Complex s. str. Pelagic limestone clasts with planktonic foraminifera, and abundant rudist fragments document a late Campanian--Maastrichtian age of the sequence. Basalt and serpentinite lithoclasts witness erosion of an oceanic basement, such as the Santa Elena Ultramafic Unit. The Cerro Cebollin sequence is interpreted as a slope deposit that received abundant material form shallow carbonate platforms of the El Viejo Formation that crops out in the northern Nicoya and Santa Elena Peninsulas.
At Cerro Barra Honda, Cerro Quebrada Honda and other classical outcrops of the Barra Honda Formation microfacies range from restricted to open marine. Most facies contain Ethelia alba a Squamariacean algae reported for the first time from Central America. Restricted micritic facies from Lomas las Pozas contain Thalmannita madrugaensis, a Rotaliid foraminifer, so far only known from the Paleocene of Cuba. In the Palo Verde arca to the North, typical Barra Honda facies pass into high energy, open platform facies characterized by abundant red algae and larger foraminifera ranging from Late Paleocene to Early Eocene. Planktonic foraminifera such as Morozovella velascoensis allow to restrict the base of Barra Honda to the latest Paleocene.
In general, the Barra Honda Platform rests unconformably on deformed Late Cretaceous-Paleocene deep-water sediments. Its basal onsett is transgressive over subaerially altered rocks (Espiritu Santo) or progradational over open marine Late Paleocene sediments (Pochote). Reworked Late Cretaceous lithoclasts testify for lithification and (tectonic) exposure of the underlying rocks.
To the East of the Tempisque River, in the area of the Cerro Naranjo the emplacement of Barra Honda over intensely deformed detrital formations as young as middle Eocene may be attributed to gravity tectonics and/or a transpressive setting along longitudinal strike-slip faults that have been postulated along the Tempisque River.
The paleotectonics of Southern Central America are characterized by an assemblage of terranes, essentially of oceanic origin, that have been juxtaposed during the last 60 my along the East Pacific convergent plate margin. Carbonate platforms in such a setting are in general ephemerous, small scaled features, and their existente is often recorded only as resediments in deeper water sequences. In turn, the age, size, facies and the substrate of such platforms provide valuable information on the tectonic and/or magmatic events that rose oceanic basement or volcanic edifices into the photic zone.
Recent paleomagnetic data (Di Marco et al., 1995) suggest that the Santa Elena Peninsula and most of the outer Nicoya Peninsula are allochtonous relative to the Chorotega Terrane, which constituted the western edge of the Caribbean Plate during the Late Cretaceous-Paleocene. Their allochtony is also corroborated by fundamental differences in age, lithology and tectonic structure between both units (Baumgartner, 1984; Baumgartner et al., 1984). Di Marco et al. (1995) indicated that the docking must have taken place during the Middle or Late Paleocene. This event certainly caused uplift in the studied area permitting the installation of a carbonate platform, such as Barra Honda.
Our study mainly focuses on the limestones outcropping in the Tempisque Basin (Fig. 1). This area is around 1000 kilometers square, located at the lower basin of the Tempisque River, near its mouth into the Nicoya Gulf. Geologically, this area is in a transpressive shear zone, originated by northwest right lateral faulting, which tectonically has controlled the area during the Tertiary.
[FIGURA 1 OMITIR]
The Barra Honda Formation (Dengo, 1962), micritic limestones of predominantly restricted platform origin (Mora, 1981), have not been dated directly nor correlated correctly with other facies in the area. Sprechmann et al. (1987) and Calvo 0987, 1998) correlated the Barra Honda limestones with the platform sequence of the El Viejo Formation (Schmidt-Effing, 1975), deposited during the Late Cretaceous. Neither Sprechmann et al. (1987) nor Calvo (1987, 1998) provided solid facts that would assess a Cretaceous depositional age for the Barra Honda limestones, generally considered devoid of age-diagnostic fossils. Calvo (1987) assumed that the rudist facies characteristic of the El Viejo Formation was marginal to the restricted Barra Honda facies without providing any evidence of the lateral continuity between the two formations. Rivier (1983) suggested a Miocene depositional age for the Barra Honda limestones, evoking mainly structural considerations.
Only few data exist considering the limestones outcropping in the Palo Verde region. Calvo and Bolz (1991) described an Upper Paleocene-Lower Eocene transgressive sequence in the Cerro Espiritu Santo. Di Marco et al. (1995) mentions small Discocyclina, characteristic of a Paleocene-Early Eocene age, in micritic limestones of the Cerro Guayacan.
We present here an attempt to group the limestones of the Tempisque area and to propose a coherent depositional history in a rapidly evolving active margin environment. We report on new fossil associations and a new paleoenvironmental interpretation of the Late Cretaceous-Early Eocene limestones of the area. Detailed field mapping allowed us to clarify the extension of the Barra Honda Platform. P. Denyer and P.O. Baumgartner carried out reconnaissance field work for this study in 1996. S. Jaccard and M. Munster did detailed mapping, sedimentological and structural analysis of every limestone outcrop of the area during 1999. C. Baumgartner-Mora, is responsible for micropaleontology and microfacies interpretation in this study.
THE CAMPANIAN--MAASTRICHTIAN EL VIEJO PLATFORM
Geologic setting of the Cerro Matapalo region
The Cerro Matapalo region (Fig. 2-3) lies about 20 km SE from Filadelfia. The major part of the outcrops is constituted by oceanic basalts, which we believe are part of the Nicoya Terrane basement. These basalts are unconformably overlain by a sequence of siliceous of calcareous hemipelagites and distal turbidites belonging to the Sabana Grande Formation (Campanian, Dengo, 1962). A Late Santonian-Early Campanian tectonic event that lead to the obduction of the Santa Elena Orogenic Complex and created an important, mostly submarine, relief (Azema & Tournon, 1980, Di Marco et al., 1995) that was subject to intense erosion. In the following, we report on redeposited limestones and volcan-oclastic turbidites that crop out in the Cerro Cebollin and Cerro Ballena.
[FIGURAS 2-3 OMITIR]
Cerros Cebollin and Ballena
Cerro Cebollin and Cerro Ballena (Fig. 4) the basaltic basement is stratigraphically overlain by coarse-grained rudist-beating mass-flow sequences (Fig. 5). The bivalves are almost intact, attesting a short transport distante, and are often biocorroded. Rocks also contain number of larger benthic foraminifera: Sulcoperculina globosa, Sulcoperculina vermunti, Pseudorbitoides rutteni. Asterorbis, Nummuloculina, Proporocyclina (Pl. 1) and various red and green algae, attesting a Campanian-Maastrichtian depositional age. The basaltic basement is locally overlain by fine-grained basaltic material resulting from the alteration of the pillow-lavas. The approximately 20 m-thick rudist-beating mass-flow deposits are followed by pebbly-mudstone layers.
[FIGURAS 4-5 OMITIR]
The uppermost part of the sequence is constituted by a succession of thin marly layers representing a minimum thickness of 40 m. The proportion between detritic and carbonated fractions varies from one bed to another. They contain lots of pelagic and volcanic lithoclasts, occasionally larger than 10 mm. The pelagic clasts (Pl. 1-1) are rich in large benthic and planktonic foraminifera such as Globotruncanita elevata (Pl. 2-2), which also are present in the matrix, suggesting a Late Campanian-Maastrichtian depositional age. The igneous lithoclasts include serpentinite fragments. The surveyed rocks also contain rudists (Pl. 1-3), echinoderms, and different types of algae (Solenoporacea, Corallinacea). Bioclasts are generally broken and perforated indicating their reworking in the photic zone. This thick turbiditic sequence is followed by other coarse-grained rudist-bearing mass-flow deposits, similar to those cropping out at the bottom of the sequence.
These deposits provide valuable clues concerning the regional paleogeographic interpretation during the Late Cretaceous. Rudists must have originated from the carbonate platform constituting the El Viejo Formation (Schmidt-Effing, 1975). This platform expanded directly on the Santa Elena Orogenic Complex during the Late Cretaceous (Late Campanian-Maastrichtian) (Azema & Tournon, 1980). This Complex formed the structurally most elevated part on the Terrane. Igneous lithoclasts, mainly serpentinite, reflect the alteration of this ophiolitic complex. The reworked carbonate facies closely resemble those exposed in the El Viejo Formation, but are distinct from Late Cretaceous facies overlying the Tortugal Ultramafic Suite (Alvarado et al., 1997). Therefore, we interpret the studied sequences at Cerro Cebollin as slope facies of the El Viejo Platform. The thickness of these turbiditic sequences clearly indicates that this platform was well-developed and that part of the underlying ophiolitic basement was exposed to erosion, suggesting that the Complex underwent a significant uplift during this period.
The location of the fault and the overthrust (Fig. 4) affecting the basalts as well as the detritic series in the Cerro Cebollin is based on stratigraphic observations. The overthrust has a decametric vertical throw. The southern, nothwest--southeast trending fault probably underwent a significant dextral strike-slip motion. The overthrust marks the contact between the turbiditic series and the basalts on the eastern hillside of the Cerro Cebollin. It seems to have an hectometric relative displacement. These structures could be related to the dextral transverse fault system affecting the Tempisque Basin (Fig. 1).
THE PALEOCENE--EOCENE BARRA HONDA PLATFORM
Geological setting of the Palo Verde Region
The Palo Verde Region (Fig. 2-6) includes the area between the Rio Tempisque and the Rio Bebedero, in the north-east of the Tempisque Basin. Scattered hills are systematically crowned by limestone outcrops that overlie the Sabana Grande turbiditic Formation. Most of the studied area is part of the Palo Verde National Park.
[FIGURA 6 OMITIR]
All limestone in this area appear to be of Paleocene-Early Eocene age (see below), but are of a wide variety of microfacies. We divided this area into three major parts: the Cerro Espiritu Santo, the Cerro Alto Viejo and Cerros la Cueva del Tigre area, and the southern part, to which the Cerros Guayacan and Fila Catalina belong.
The Cerro Espiritu Santo (Fig. 7) is the only place where there is clearly no tectonic discontinuity between the limestones and the underlying detrital sediments. An outcrop near the top of the hill (coord.: 388.1/263.1) shows the evidence of a Late Paleocene-earliest Eocene transgression of the Barra Honda carbonate platform on deeply altered Sabana Grande-type sediments (Fig. 8).
[FIGURAS 7-8 OMITIR]
The western base of the Cerro Espiritu Santo consists of basalts, overlain by 40-80 m of Sabana Grande turbidites (Fig. 7). At the top of the sequence, the detritic layers are very altered and are covered by a thin centimetric brownish layer interpreted as a paleosoil (see also Di Marco et al., 1995). The first calcareous elements appear on top of this layer (Fig. 8), as well rounded, encrusted and bored limestone cobbles (Di Marco et al. 1995), showing a typical beach environment. These consist of mudstones and wackestones containing red algae and gastropods. The encrustation is made by Melobesiae (encrusting red algae) and a Squamariacean algae, Ethelia alba, also present in the matrix (see discussion below).
One meter higher in the sequence, the facies vary laterally and are distributed as lenses. We found some Discocyclina-grainstones and some oolithic- and Amphisteginid and Ranikothalia limestones, in which cross-beddings could be observed.
All these facies are characteristic of a shallow-water, high-energy environment representing the platform edge. Thus, the Cerro Espiritu Santo is the relic of the transgression and setting up of a limestone platform during the Late Paleocene-Early Eocene.
Cerro Alto Viejo and Cerros La Cueva del Tigre
Along the crest of the Cerros Alto Viejo and La Cueva del Tigre, we observed many, different facies, each of which crops out as a single coherent block of about 10 m width and has no continuity with the others. There are large foraminifera-packstones and wackestones, sedimentary calcareous microbreccias, Miliolidae-and red algal-wackestones, and even a Lower Paleocene pelagic lime-mudstone. In various blocks of different faeies we found Morozovella velascoensis (Pl. 3-2), which is restricted to the Upper Paleocene.
The variety of the facies as well as their incoherent juxtaposition cannot yet be explained in a satisfactory way. The facies that represent distinct paleoenvironments could have become juxtaposed by dismembering of the platform due to compaction of the underlying soft sediments, probably during earthquakes. This interpretation is supported by the presence of siliceous veins proceeding from the underlying detrital sediments, which often penetrate the limestone blocks. However, because of similar age ranges of the different facies we think that they belong to the same platform.
South-eastern outcrops (Cerro Guayacan, Fila Catalina and related outcrops)
The variety of facies of the south-eastern outcrops (Fig. 6) is much less important than the in the Cerros Alto Viejo and La Cueva del Tigre. They are mostly red algal- and echinoderm-wackestones, with abundant micrite. At the site called Mirador La Roca (coord.: 390.5/258.5), we found lots of well developed rodoliths, as well as Discocyclinids (Neodiscocyclina barkeri) from the Upper Paleocene-Lower Eocene (Caudri, 1975).
[FIGURA 6 OMITIR]
Remarks on Ethelia
Many limestones are rich in the Squamariacean alga Ethelia alba (Pfender 1936), (Pl. 2-5 Pl. 3-1) that grew encrusting rhodoliths and any other hard bioclastic substrate is typical of Paleocene algal platforms. Although its total range is given as Barremian to Eocene (Massieux and Denizot 1964, Praturlon 1966), most illustrated specimens come from Paleocene limestones of Southern Europe and the Middle East, in America it was reported from the Lower-Eocene of Venezuela (Pfender & Schneegans, 1949). We report Ethelia alba for the first time from Costa Rica (and probably from Central America). It is characteristic of the various Barra Honda facies. It has not been observed in any Late Cretaceous facies assemblage of Costa Rica. Ethelia alba is found as crusts in situ made of multiple thalli (Pl. 2-5) in moderate to high energy open platform facies, but also as fragments in micritic, restricted platform facies. Apparently, individual thalli got easily stripped off the crusts and transported by storms into the more protected areas of the platform.
Synthesis of the Palo Verde Region
Our structural, sedimentological and micropaleontological analysis of the Palo Verde region demonstrates that a variety of facies in these different areas share the same Paleocene to Early Eocene age. Every sample is typified by the presence of Ethelia alba. We found this algae in "living position" at the Espiritu Santo (Pl. 2-5), together with Ranikothalia catenula sensu Caudri 1990 (Pl. 3-4). We propose that there is only one platform in the whole region. Its transgressive base is evidenced in the Espiritu Santo section (Fig. 8). The Cerro Alto Viejo and Cerros La Cueva del Tigre crest could be the remnant of a collapsed rim of the platform, setting blocks of different facies side by side.
[FIGURA 8 OMITIR]
The limestones of the Bajo Tempisque are the classical Barra Honda outcrops lying west of the Rio Tempisque, as well as those around Puerto Nispero and Pena Blanca, east of the river. In this region they rest on the Campanian-Paleocene Rivas Formation. Until now no direct dating has been performed in this area, because of the lack of adequate micropaleontological data.
The predominant facies are white algal-and echinoderm-rich wackestones, whose matricial contents can be variable. In some places the rock is made of pure micrite, and can be strongly recristallized. Miliolids, gastropods, as well as ostracods are quite common. The Squamariacean alga Ethelia alba (Pl. 3-1) is also present in quite every sample and is sometimes more than two centimeters large.
The facies variations are at a very small scale (metric to decametric), and seem to be erratic. They range from a restricted to an open platform shallow-water environment. The platform had probably a complex, small scale paleogeography with a network of current channels, small ponds and numerous algal patch reefs.
On the Cerro Coralillo, we found besides numerous Miliolids, Alveolinids such as Praealveolina (Pl. 3-3). At Lomas las Pozas we discovered Morozovella sp. from the Upper Paleocene-Lower Eocene. At the same locality we also found Thalmannita madrugaensis (Cushman and Bermudez) a rotalijd that is so far known only from the Paleocene of Cuba (Bermudez, 1978).
North of Puerto Nispero (coord.: 401.1/244.3), Aguilar & Denyer (in press) described a Paleogene coral reef with m-sized coral colonies in living position scleractinia: Euphyllia nov. sp., unique in the whole Tempisque Basin.
At Pochote (coord.: 395.6/236.6) (Fig. 2), south of the Cerros Copal, we studied a sequence which shows the reworking of pelagic Cretaceous limestones in an Upper Paleocene-Lower Eocene foreslope matrix at its base, and grades upsection into typical Barra Honda facies (Fig. 9). The serie begins with a polymict breccia, containing pelagic limestones and Barra Honda-type red algae white packstone clasts. The matrix consists of an encrinitic packstone, containing many different planctonic foraminifera and red algae. It disappears slowly near the middle of the serie. We found some Morozovella sp. and a Pseudohastigerina in it. Ethelia alba (Pl. 3-1) is present in both the matrix and the platform clasts. The pelagic lithoclasts are the largest and the most abundant at the base; higher in the sequence, they become smaller and finally disappear, meanwhile the opposite happens to the platform type clasts. At the top of the serie, only platform clasts remain and there is no more open-marine influence.
[FIGURA 9 OMITIR]
The angular pelagic clasts (Pl. 2-1) contain planktonic foraminifera from the Upper Cretaceous (Globotruncana ventricosa, Pl. 2-2) and some of them are bored by bivalves. These limestones have probably been uplifted and lithified before being eroded, bored and redeposited. There are also autochthonous resedimented clasts (intraclasts) derived from the surrounding rock itself. All this is in agreement with a fore-slope environment, which collects fragments of a platform in an open-marine environment. Fracturing of slightly indurated platform sediments could have occurred during earthquakes or related events. Fragments were transported by submarine currents downslope.
The Pochote outcrop seems to be the remnant of the Upper Paleocene-Lower Eocene progradation of the Barra Honda Platform, which probably appeared after the uplift that exposed Upper Cretaceous pelagic limestones to erosion. Although the Pochote outcrops are not directly connected to a major limestone body, its geographic position, sedimentology and age matches correctly with the Barra Honda Platform history.
The wackestones outcropping near the Lomas el Jicote (Fig. 3) rest unconformably on the Sabana Grande turbiditic series. These limestones contain a number of age-diagnostic Discocyclinids (Pl. 3-5), such as Neodiscocyclina bullbrooki (Caudri) and Amphisteginids as Eoconuloides cf. wellsi (Pl. 3-6) indicating an Early-Middle Eocene depositional age. The samples are matrix-supported and contain numerous echinoderm fragments and various red algae types. Their emplacement history is still enigmatic. Their morphology and structural position privilege an olistolithic deposition. These limestones only cover a restricted area and might represent the top of the Barra Honda Platform. This speculative hypothesis may only be confirmed by further work.
Cerros Cebollin and Ballena
Because of its Late Cretaceous age and facies associations, the carbonate-rich slope deposits at Cerros Cebollin and Ballena cannot be slope facies of the Paleocene Barra Honda Platform as sugested by Calvo (1987, 1998). For instance, Ethelia alba, omnipresent in the Barra Honda Limestones has not been found at Cebollin and Ballena. On the other hand, the redeposited matrerial compares very well with rocks attributed to the El Viejo Formation, exposed in Northern Nicoya and Santa Elena. Baumgartner et al. (1984) described a sequence with very similar, but more proximal facies in the southeastern cliffs of Bahia Santa Elena, that is overlain by Late Campanian-Maastrichtian pelagic and then turbiditic sediments.
Relationship of the Barra Honda Platform with underlying rocks
In general, west of the Tempisque River, and in the Palo Verde area the Barra Honda Limestones unconformably overlie Campanian to Paleocene pelagic-hemipelagic and turbiditic formations commonly attributed to the Sabana Grande and Rivas Formations, respectively (Dengo, 1962). The basal onset of the formation is clearly transgressive over deeply altered, probably subaerially exposed Rivas at Cerro Espiritu Santo, the northernmost outcrops of Barra Honda. At the southern edge of Barra Honda outcrops, near Pochote, the onset of the formation is regressive or progradational over open marine Late Paleocene calcarenites. Reworked and bored Late Cretaceous lithoclasts are very common in the basal outcrops of Barra Honda. They testify for lithification and (tectonic) exposure of the underlying formations, prior to the sedimentary onset of Barra Honda. Hence, the Barra Honda Platform can be considered as a mesoautochthonous (i. e. formed between two tectonic events) sequence that unconformably overlies the deformed Sabana Grande and Rivas Formations. Calvo (1987, 1998), Sprechmann et al. (1987, 1994) assumed a Late Cretaceous age for Barra Honda and implied a tectonic or gravitative emplacement of the whole platform over the underlying rocks. We cannot confirm a general allocthony of Barra Honda. However, where basal contents ale exposed they are generally tectonized and the underlying poorly lithified detrital rocks are squeezed into the fractured and karstified limestones. These observations apply for the southernmost outcrops, east of the Tempisque River and for the Quarry at Cerro Calera, East of the town Nicoya (Fig. 2) where we saw striation and deformation at the base of the limestones. It seems obvious that the contact between limestones and turbidites has undergone relative displacement: small scale overthrust indications (shear zones in the detrital sediments, small decametric overthrusts) can be observed quite often.
We also found some tectonic breccias, which lie mostly at the base of the limestones, but which can also sometimes be intraformational. On the eastern side of the Tempisque, micropaleontologic dating seems to indicate an Eocene age for the detrital sediments forming the substrate of Barra Honda (Rivier 1981), implying a tectonic emplacement of the older limestones over younger detrital sediments. However, the sediments which directly underlie the limestones have not been dated and the precise tectonic relationship between the two units has to be examined.
If the sediments underlying the limestones were of Paleocene age, Barra Honda would follow stratigraphically. If the underlying sediments were Eocene in age, we would consider an eastward post-Eocene overthrust of the Barra Honda Platform over these sediments. This could have occurred in the context of the transpressive shear zone shown in figure 1.
We can divide the limestones of the Tempisque Basin in two clearly distinct carbonate platform systems:
1-- The El Viejo Platform, dated as late Campanian-Maastrichtian by abundant rudistids and larger benthic and planctonic foraminifera. It is represented in the Cerros Ballena and Cebollin. The turbidites and mass flow deposits at this locality are interpreted as slope deposits that received abundant material from shallow carbonate platforms of the El Viejo Formation that crops out in the northern Nicoya and Santa Elena Peninsulas. Therefore, this area can be attributed to the Nicoya Terrane as defined by Di Marco et al. (1995).
2-- The Barra Honda Platform, dated as Upper Paleocene-Lower Eocene by larger benthic, and planctonic foraminifera. The observation of Morozovella velascoensis allows restriction at least of the base of the Barra Honda Platform to the latest Paleocene (P4 to lowermost P6). Today, the platform extends from the classical outcrops at Cerro Barra Honda in the South, to the Palo Verde region in the North. At Cerro Espiritu Santo, the latest Paleocene landward transgression of the platform is exposed. At Pochote in the South, we observed evidence of seaward progradation of the platform over open marine carbonates during the latest Paleocene. Small scaled lateral facies changes between moderate- to high energy and restricted microfacies suggest a relatively small platform covered by numerous algal patch reefs that are separated by current-swept channels. The common feature of these microfacies is the presence of red algae and Ethelia alba, a Squamariacean algae that seems to have grown in the high energy paleoenvironment and was transported as fragments into the restricted platform environment. We believe that the docking of the Nicoya Terrane during the Late Paleocene could have caused the necessary uplift to create a shallow substrate for the initiation of the Barra Honda Platform deposition.
We are very thankful to Lucas Hottinger who verified our micropaleontological determinations and to make valuable suggestions to the age and facies interpretation given in this work.
The field work of P.O.B. and P. D. was carried out in the frame of Projects No. 2000-039545.93 and 2000-49401.96 of the Swiss National Science Foundation. Without this financial support, field work in Costa Rica would have been impossible.
We gratefully acknowledge the Ministerio del Ambiente y Energia (MINAE) of Costa Rica (Mr. Javier Guevarra), who extended permits for research and collection of samples in the Palo Verde and Barra Honda National Parks. We acknowledge the logistical support provided by The Escuela Centroamericana de Geologia and the project 113-90-071 of the Universidad de Costa Rica.
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(Recibido 14/4/2000; Aceptado 31/8/00)
Samuel Jaccard (1), Marc Munster (1), Peter O. Baumgartner (1), Claudia Baumgartner-Mora (1) and Percy Denyer (2)
(1) Institut de Geologie, Universite de Lausanne, BFSH2, CH-1015 Lausanne, Switzerland Peter.Baumgartner@igp.unil.ch
(2) Escuela Centroamericana de Geologia, Univ. Costa Rica, Apdo. 214-2060 UCR, Costa Rica
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|Author:||Jaccard, Samuel; Munster, Marc; Baumgartner, Peter O.; Baumgartner-Mora, Claudia; Denyer, Percy|
|Publication:||Revista Geologica de America Central|
|Date:||Jun 1, 2001|
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