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Revista mexicana de ciencias geológicas

versão On-line ISSN 2007-2902versão impressa ISSN 1026-8774

Rev. mex. cienc. geol vol.30 no.3 Ciudad de México Dez. 2013

 

Carbon and oxygen isotopic variations in early Albian limestone facies of the Mural Formation, Pitaycachi section, northeastern Sonora, Mexico

 

Variaciones isotópicas de carbón y oxígeno en facies de caliza de la Formación Mural del Albiano temprano, sección Pitayachi, noreste de Sonora, México

 

Jayagopal Madhavaraju1*, Alcides N. Sial2, Carlos M. González-León1, and Ramasamy Nagarajan3

 

1 Estación Regional del Noroeste, Instituto de Geología, Universidad Nacional Autónoma de México, Av. L. D. Colosio s/n, esq. con Madrid, campus Universidad de Sonora, Hermosillo, Sonora 83000, México. *mj@geologia.unam.mx, jmadhavaraju@yahoo.com.

2 Nucleo de Estudos Geoquímicos e Laboratório de Isótopos Estáveis (NEG - LABISE) Departmento de Geologia, Universidade Federal de Pernambuco Caixa Posta 7852, 50670-000 Recife, PE, Brazil.

3 Department of Applied Geology, School of Engineering and Science, Curtin University, CDT 250, 98009, Miri, Sarawak, Malaysia.

 

Manuscript received: July 27, 2012
Corrected manuscript received: September 20, 2013
Manuscript accepted: September 23, 2013

 

ABSTRACT

We used petrofacies analysis and stable isotope data to interpret the isotopic variations in the marine carbonate succession of the Early Cretaceous Mural Formation of northeastern Sonora (Pitaycachi section), Mexico. The petrographic study reveals a range of lithofacies from bioclastic mudstones to boundstones. Allochems consist of corals, algae, rudists, echinoids, sponge spicules, radiolarians, foraminifera and calpionellids. Samples analyzedfor stable isotope are significantly depleted with δ18O values of -15.19‰ to -6.32‰ and exhibit positive δ13C values ranging from 2.91‰ to 4.39‰. The lack of correlation between δ13C and δ18O values also supports a primary marine origin for the δ13C values of limestones from the Pitaycachi section. In the δ13C profile, the Cánova Member shows an upward increasing trend from 3.09‰ to 4.36‰ interpreted to indicate an increase in the rate of marine organic production and/or organic burial in the basin during early Albian time. The abrupt increase in carbon isotope values in the lower part of the section correlates with OAE1b. The shape of the C-isotope curve of the present study is similar to other C-isotope curves from Mexico and other continents (e.g., Vacontian basin, France) indicating that OAE1b may have been global in extent.

Key words: stable isotopes, petrography, oceanic anoxic events, Pitaycachi section, Mural Formation, Sonora.

 

RESUMEN

En este trabajo se analizan las variaciones isotópicas en la sucesión marina carbonatada de la Formación Mural (Cretácico Inferior) que aflora en la sección Pitaycachi, noreste de Sonora, México, a partir de datos petrográficos y de isótopos estables. Las petrofacies de esta sucesión varían de "mudstone" bioclásticas a "boundstone", y los aloquímicos son corales, algas, rudistas, equinodermos, espículas de esponjas, radiolarios, foraminíferos y calpionélidos. Las calizas de la sucesión analizada por isótopos estables presentan valores bajos de δ18O que varían entre -15.19‰ y -6.32‰ y valores positivos de δ13C entre 2.91‰ y 4.39‰. La falta de correlación entre los valores de δ13C y δ18O indica un origen marino primario para los valores de δ13C de las calizas de la sección de Pitaycachi. El perfil de δ13C del miembro Canova de la sección estudiada muestra un incremento hacia su parte superior, que va de 3.09‰ a 4.36‰, interpretándose como un aumento en la tasa de producción de materia orgánica y/o secuestro de ella en la cuenca durante el Albiano temprano. El abrupto incremento de los valores de isótopos de carbón en la parte inferior de la sección se correlaciona con OAE1b y la forma de su curva es similar a otras reportadas de México y de otros continentes (e.g., la cuenca Vacontian en Francia), sugiriendo que OAE1b pudo haber sido un evento global.

Palabras clave: isótopos estables, petrografía, eventos anóxicos oceánicos, sección Pitaycachi, Formación Mural, Sonora.

 

INTRODUCTION

The carbon cycle was influenced by a series of oceanic anoxic events during the Cretaceous period and simultaneous phases of platform destruction, which are marked by several high-amplitude positive carbon isotopic excursions that have been documented globally (Jenkyns, 1995; Weissert et al., 1998; Erba et al., 1999; Veizer et al., 1999; Herrle et al., 2004; Weissert and Erba, 2004; Wissler et al., 2004). An increase in atmospheric CO2 is thought to have stimulated a global "green house" climate, which enhanced the sedimentary preservation of organic matter (increased burial) and leading to distinct Oceanic Anoxic Events (OAEs) (Schlanger and Jenkyns, 1976; Barron and Washington, 1982). Carbon isotope records are generally used to establish the global organic carbon budget during the OAEs. The significant positive carbon isotope shift that corresponds to OAE2 (Scholle and Arthur, 1980) suggests that the volume of organic carbon (Corg) buried was a sizable part of the global carbon budget. Isotopic studies on the shallow marine carbonates of Lower Cretaceous age have revealed evidence for paleo-oceanographic (Kumar et al., 2002; Madhavaraju et al., 2004; Sial et al., 2001; Marquillas et al., 2007; Nagarajan et al., 2008; Armstrong-Altrin et al., 2009), climatic and biotic changes (Deshpande et al., 2003; Préat et al., 2010;), in addition to global scale tectonic events (Gröcke et al., 2005; Maheshwari et al., 2005; Amodio et al., 2008).

The sudden increase in carbon isotope values is noticed above the early Aptian (OAE1a) and remains high into Albian. The carbon isotopic variations for the Aptian-Albian interval are somewhat complex (Pratt and King, 1986) and their relationship with dysoxic/anoxic conditions (OAE1b) is less understood. In general, OAE1b includes multiple anoxic events (Jacob event, Kilian event, Paquier event and Leenhardt event) and it is also called as OAE 1b set (Fôllmi et al., 2006). The Albian time was characterized by a global sea level rise and geodynamic activity expressed by elevated production of oceanic crust leading to an increased rate of CO2 degassing (Caldeira and Rampino, 1991; Larson, 1991). Major inconsistencies exist in the chronostratigraphic correlation of the carbon isotope record in the Lower Cretaceous strata of Mexico (Scholle and Arthur, 1980) and Europe (Weissert and Lini, 1991; Leckie et al., 2002; Herrle et al., 2004). Information related to the mid-Cretaceous global events is largely derived from the Tethyan sections exposed in France and Italy (Arthur and Premoli Silva, 1982; Premoli Silva et al., 1989; Coccioni et al., 1992; Herrle et al., 2004), whereas information on the Lower Cretaceous events exposed in Mexico is sparse (Scholle and Arthur, 1980; Bralower et al., 1999).

Lower Cretaceous clastic and carbonate sediments of the Bisbee Group are well exposed in Sonora, northwestern Mexico. Numerous studies (stratigraphic, palaeontological, geochemical and tectonic) have been carried out on the Mural Formation (upper Aptian-lower Albian) (Bilodeau and Lindberg, 1983; Jacques-Ayala, 1995; Lawton et al., 2004; González-León et al., 2008; Madhavaraju et al., 2010; Madhavaraju and González-León, 2012). However, very few published studies incorporate stable isotope data from the carbonate within the succession. Madhavaraju et al. (2013) carried out the carbon, oxygen and strontium isotope studies on the limestones collected from the proximal part of the Bisbee basin (Cerro Pima section) to understand the palaeoceanographic changes that occurred during the Lower Cretaceous epoch. Here we present carbon and oxygen isotope data from the more distal carbonate facies of the Bisbee basin exposed in the Cerro El Caloso-Pitaycachi section (Figure 1). The section reveals an overall shallowing-upward trend, from deep shelfal deposition in the lower part (Cánova Member) to shallow marine conditions in the upper part (El Caloso Member). Lower order shallowing-upward cycles are recognized within this overall regressive section. The objectives of the present study are: a) to provide an isotopic record of the Lower Cretaceous limestones in the distal part of the Bisbee basin; b) to assess the degree of diagenetic alteration of the isotopic signals; c) to determine the presence/absence of OAEs in the Cerro El Caloso-Pitaycachi section and: d) to compare the isotope stratigraphy of this section with that of the Cerro Pima section in western Sonora (Madhavaraju et al., 2013).

 

GEOLOGY AND STRATIGRAPHY

Early Cretaceous sediments of the Bisbee Group are well exposed in the northern Sonora, Mexico, and show similar stratigraphic characteristics with Bisbee Group sediments exposed in southern Arizona and New Mexico, USA (Ransome, 1904; Cantú-Chapa, 1976; Bilodeau and Lindberg, 1983; Mack et al., 1986; Dickinson et al., 1989; Jacques-Ayala, 1995; Lawton et al., 2004). The Bisbee Group is composed predominantly of sedimentary rocks with lesser amounts of volcanic deposits of Late Jurassic to Early Cretaceous age (Lawton et al., 2004). In the type area (southeastern Arizona), the Bisbee Group is divided into the Glance Conglomerate, Morita Formation, Mural Formation and Cintura Formation. The Glance Conglomerate consists of cobble- to boulder-conglomerate intercalated with volcanic flows and tuffs (Bilodeau et al., 1987). The Morita and Cintura Formations are dominated by fluvial siltstone, arkose and feldspathic arenite (Dickinson et al., 1986; Klute, 1991). The Mural Formation however, consists of clastic and carbonate sediments that record a major marine transgression in the region of Sonora and Arizona during Aptian-Albian time (Scott, 1987).

The sedimentary sequence of the Mural Formation is well exposed in a 260 km transect from Sierra El Chanate (westernmost part) to Cerro El Caloso-Pitaycachi (northeastern most outcrops) in northern Sonora (Figure 1) (González-León et al., 2008). The interpreted depositional environments of the Mural Formation vary from restricted shelf with deltaic and fluvial influence in the west to open shelf with coral rudist buildups and offshore shelf environments in the east (González-León et al., 2008). A distinct lateral facies change occurs between these regions, and separate members of the Mural Formation have been recognized by Warzeski (1983, 1987) at the Sierra Anibácachi and Cerro Caloso-Cabullona localities. Warzeski (1983, 1987) recognized various members of the upper Mural Formation at the Cerro Caloso locality, namely Canova, El Caloso, La Aguja and Agua Prieta members. Outcrops of the Mural Formation at Cerro El Caloso-Pitaycahi (Figure 2) are located 30 km east of the Cerro Caloso-Cabullona but the base of the section is not exposed. The lowest exposed part below the Cánova Member consists of interbedded, green to light gray shale and siltstone with trigonids, and has been correlated with the Tuape Shale Member of this formation, which crops out to the west in northern Sonora. The ammonite Douvilleiceras sp. juv. cf. rex (Scott) is found in the shales of this member suggesting a latest late Aptian to early Albian age (González-León et al., 2008). The Cánova member is 190 m thick and is composed of dark to light gray, thin to thick, massive to nodular limestone. The Cánova member includes Lower Albian calpionellids Colomiella recta and Calpionellopsella maldonadoi, pelagic foraminifera, notably Globigerina (formery Hedbergella) washitensis, sand and silt-size fragments of the pelagic crinoids Saccocoma sp., and also larger foraminifera such as Orbitolina (Warzeski, 1983).

The El Caloso member is composed of an incomplete 26 m-thick sequence that represents the lower part of this member (Warzeski, 1983 report a total thickness of 80 m for this member in Cerro Caloso-Cabullona). The El Caloso Member contains corals, algae, rudists, mollusks and larger foraminifera (e.g., orbitolinids). The facies associations and faunal assemblages of the Cánova Member indicate a moderately deep to deep shelf basin, in contrast of their shallow lateral correlatives of the Los Coyotes and Cerro La Puerta members that crop out in the western part of the basin in northern Sonora. Similarly, the El Caloso member is correlative with the Cerro La Espina Member (González-León et al., 2008), which represents a shallowing marine setting comprised of large patch reefs and carbonate bank complexes, following deposition of the deeper water Cánova Member.

 

METHODOLOGY

Twenty five thin sections were prepared for the petrographic study. Twenty one limestone samples from the Cerro El Coloso-Pitaycachi section were selected for stable isotope analysis (Figure 2). The carbon and oxygen isotope composition was analyzed using a SIRA II mass spectrometer at the Stable Isotope Laboratory (LABISE) of the Federal University of Pernambuco, Brazil. For carbon and oxygen isotope measurements, the limestone samples were treated with H3PO4 in a vacuum at 25 °C for one day and the resulting CO2 gas analyzed according to the method described by Craig (1957). The evolved CO2 gas was analyzed using the reference gas BSC (Borborema Skarn Calcite), which calibrated against NBS-18, NBS-19 and NBS-20 has a value of -11.28 ± 0.004‰ PDB for δ18O and -8.58 ± 0.02‰ PDB for δ13C. The results are reported in the per mil notation (‰) in relation to the international VPDB scale.

 

RESULTS

Petrography

Petrographic description of the carbonate samples follows the classification schemes of Dunham (1962) and the extended classification of Embry and Klovan (1971). Four major lithotypes have been identified in the Cánova and El Caloso members: i) mudstone, ii) wackestone, iii) packstone and iv) grainstone. These major lithotypes and their sub-types are discussed as follows:

 

Mudstone

The Calpionellid foraminiferal mudstone occurs in the lower and middle part of the Cánova Member and contains calpionellid, foraminifera and radiolarian grains (Figure 3a). A few sponge spicules and echinoid plates are also present in the micritic matrix. The limestone exhibits small scale veins that are filled with sparry calcite cement. Pore spaces are commonly filled with sparry and poikilotopic calcite cement.

 

Wackestone

Limestone beds of the lower part of the Cánova Member are characterized by the Calpionellid wackestone (Figure 3b). It contains predominantly calpionellids along with some foraminifera and echinoids, and minor radiolarian within the micritic matrix. The original opaline silica of the radiolarian tests have been replaced by calcite. In addition, the pore spaces present on the surface of the radiolarian test were partly replaced by micritic mud. The limestone also exhibits numerous irregular microstylolite seams. The Echinoid foraminiferal wackestone is present in the upper part of the Cánova Member and is characterized by echinoid and foraminiferal bioclasts within a micritic matrix (Figure 3c). Minor radiolarians and sponge spicules are found in the matrix. Also present are ferruginized intraclasts derived from the older sequence. It contains fine-grained, subangular quartz grains. Most of the quartz grains are monocrystalline, however some exhibit a polycrystalline type. Microcracks within this lithofacies are generally filled by calcite cement.

The middle part of the Cánova Member is characterized by the Foraminiferal molluscan wackestone, which consists of foraminifera, radiolaria and mollusks within the micritic matrix (Figures 3d, 3e). It also contains many fine- to medium-grained, subangular quartz and feldspar grains. In addition, this lithofacies contains both U and V-shaped calpionellids (Figures 3f, 3g). Many foraminiferal chambers are filled with microsparite and sparry calcite cement. Most of the quartz grains are monocrystalline with a few polycrystalline grains also present. Few echinoid spines are also seen in the micritic matrix. The limestone exhibits numerous stylolites (Figure 3h) in the foraminiferal molluscan wackestone. The lower part of the Cánova Member also contains the Echinoidal foraminiferal molluscan wackestone, which exhibits calpionellid, radiolarian, foraminifera and molluscan fragments. Echinoid plates and spines are also common in this lithofacies (Figure 4a).

 

Packstone

The Coral foraminiferal molluscan packstone is present in the upper part of the Cánova Member. It contains rudist, algae, coral, foraminifera and molluscan grains. Both planktonic and benthic foraminifera are present. Echinoid plates and spines, and some quartz grains are observed in the micritic matrix. Many foraminiferal grains are coated with a micritic layer (Figure 4b). Because of the micritic envelope, the internal structure of the shell fragments has remained intact. This lithofacies also exhibits small-scale stylolitic seams and small- to medium-scale veins filled with sparry calcite and blocky cement (Figure 4c).

 

Grainstone

The Rudist foraminiferal coral grainstone, found in the upper part of the El Caloso Member, contains rudist, foraminifera and coral framework grains (Figure 4d). Many rudist and foraminiferal grains are coated with micrite and this layer prevents the removal of the shell fragments partly or completely from this lithofacies. The limestone shows a few larger foraminifera (e.g., Mesoorbitolina). The primary intergranular porosity is filled by coarse sparry calcite cement. The Foraminiferal algal coral molluscan grainstone that is also found in the upper El Caloso Member, has a framework consisting of algae, coral, foraminifera and molluscan grains with few echinoid fragments (Figure 4e). It is also characterized by numerous, fine- to medium-grained, subangular quartz and feldspar grains. The limestone contains distinctive, large oyster shell fragments that display well defined internal layering (Figure 4f). Most of the bio-clasts in this lithofacies have thin micritic coating.

 

Boundstone

The Coral boundstone has a framework comprised of molluscan and coral grains. The cross section of the corals show a cerioid growth pattern characterized by corallite which are touching each other (Figure 4g). The organic framework resulted from the complete filling of the interspaces between corallite by binding and encrusting organisms (Figure 4h). The large pore spaces between organic frameworks were partly filled with isopa-chous calcite cement and cavity-filling sparry calcite cement. This lithofacies also exhibits small-scale stylolites seams.

 

Stable isotope results

δ13C and δ18O values of the Cánova and El Caloso members are displayed in Table 1. The carbon isotope composition of Cánova Member ranges from 2.9‰ to 4.39‰ whereas the El Caloso member ranges from 3.11‰ to 3.64‰. Overall, limestones of the Cánova and El Caloso members show positive carbon isotope values. The Cánova Member samples show significant variation in oxygen isotope composition with values ranging from -12.23‰ to -6.32‰. The El Caloso member shows even lower oxygen isotope values that range from -15.19‰ to -12.15‰.

 

DISCUSSION

Lithostratigraphy and age of the Mural Formation

Most of the limestones from the Cánova Member consist of fine-grained carbonates (micrite) whereas the El Caloso Member is composed of both fine-grained (mic-rites) and coarse-grained carbonates (abundant bioclastic grains and coarse cements). The limestones from the lower and middle part of the Cánova Member exhibit numerous bedding-parallel, large amplitude stylolites, whereas the El Caloso Member shows a few small-scale stylolites (Figure 5a). The pressure solution effects are more prevalent in the Cánova Member and the stylolites contain numerous dark coloured insoluble materials (stylocumulate) along the pressure solution surfaces. The dark stylocumulate mainly consists of clay and pyrite. In addition, the limestone from the lower part of the Cánova Member (4-21-05-10 sample, Table 1) displays a nodular fabric that also formed due to pressure solution. The densely packed carbonate nodules are subangular with the contact between nodules often defined by dark stylolitic seams (Figure 5b).

The limestones of the Cánova Member contain a range of calpionellids. Warzeski (1987) identified Colomiella recta and Calpionellopsella maldonadoi in the Cánova Member and assigned it to the lower Albian Colomiella Zone. The Colomiella tunisiana and Colomiella recta are common in the Cánova Member and the occurrence of these species suggest placement in the Colomiella zone of Trejo (1975) (Scott, 1987). Trejo (1975) placed the Aptian-Albian boundary at the base of the Colomiella recta zone. Longoria (1984) proposed a detailed zonal scheme for the Cretaceous rocks exposed in the Gulf of Mexico region based on the distribution of calpionellids, nannoconids and planktonic foraminifera. He placed the Colomiella zone between K12 and K14 based on the first and last appearance of the taxa. He assigned a late Aptian - early Albian age for the Colomiella zone in agreement with Trejo (1975).

In the present study, we have identified Colomiella recta and Calpionellopsella maldonadoi species from the Cánova Member of Cerro El Caloso-Pitaycachi section. The calpionellids completely disappear in the middle part of the Canova Member (absent from sample 4-21-05-18 onwards). The common and distinctive larger foraminifera present in the Canova Member is Orbitolina texana (Roemer). The presence of Orbitolina texana (Figure 5c) in the Canova Member suggests that it is approximately equivalent to the lower Albian Glen Rose Formation, Texas, USA (Scott, 1987). In addition, Globigerina (= Favusella) Washitensis Carsey, Globigerina planispira Tappan and Globigerina (= Hedbergella) delrioensis Carsey was identified near the base of the Canova Member in Sonora (Scott, 1987). The limestones from the El Caloso Member show rudist, coral, algal and molluscan fragments and also exhibit few larger foraminifera (e.g., Orbitolina). The presence of Calomiella recta and Calpionellopsella maldonadoi in the Canova Member also suggest an early Albian age.

Precise identification of the Aptian/Albian boundary in this section is somewhat difficult due to lack of direct age constraints. The available foraminifera and calpionel-lids suggest an early Albian age for the Canova Member. The Douvilleiceras sp. juv. cf. rex (Scott) found below the Canova Member suggest that its age ranges between late Aptian to early Albian (Gonzalez-Leon et al., 2008). In addition, the first occurrence of the Calpionellids Colomiella recta and Calpionellopsella maldonadoi occurs at the base of the Canova Member equivalent to the lower Albian Colomiella Zone (Trejo, 1975).

 

Identification of primary carbon isotope values

In general, marine limestones are composed of a variety of skeletal and non-skeletal grains with a certain amount of matrix material, and diagenetic processes that readily alter the primary isotopic signatures (Allan and Matthews, 1982; Veizer, 1983; Marshall, 1992; Kaufman and Knoll, 1995; Madhavaraju et al., 2004; Armstrong-Altrin et al., 2011). However, data from the Canova and El Caloso members show very poor correlation between δ13C and δ18O values (r= -0.38, n=21; lack of statistically significant correlation; Verma, 2005, Figure 6) indicating a lack of diagenetic influence on the carbon isotopic signatures. Considering lack of correlation between δ13C and δ18O, we suggest that limestones from the Pitaycachi section exhibit primary carbon isotope values and can be used as a direct proxy for the composition of seawater in the Bisbee basin during Aptian-Albian time.

 

Carbon and oxygen isotopic variations

The δ18O values -in the study samples vary between -15.19‰ and -6.32‰ (Figure 7), displaying a significant decreasing upwards trend. The lower part of the Canova Member shows comparatively heavier oxygen isotope values than the upper part and the El Caloso Member is even more 18O depleted, with values ranging from -15.19 to -12.15‰. Marine limestones that have been affected by diagenesis often show more negative δ18O values (Land, 1970; Allan and Matthews, 1977) because cementation and/ or re-crystallization frequently takes place in fluids depleted in 18O with respect to seawater (e.g., meteoric water), or at elevated temperatures due to deep burials. Nevertheless, the carbon isotopes are less prone to diagenetic alterations than oxygen isotopes (Hudson, 1977; Anderson and Arthur, 1983; Banner and Hanson, 1990; Marshall, 1992; Frank et al., 1999).

The carbon isotope composition of bulk carbonate shows positive δ13C values throughout the study section (Figure 7). In the carbon isotope profile, the δ13C value is close to 3.4‰ at the base of the section and 3.3‰ the top. The middle part of the section shows a sudden increase from 3.09‰ to 4.36‰, followed by a plateau in values, followed by a fall, rise and consistent downward trend. Such carbon isotope shifts are significant in terms of paleoceanography. According to Berger and Vincent (1986), the excess removal of 1‰ of the oceanic reservoir of organic carbon produces 0.2‰ of positive shift. The positive isotopic excursion observed in the middle part of the Pitaycachi section has amplitude of 1.3‰, which indicates a significant change in the carbon fluxes in the distal part of the basin during this interval. This positive δ13C excursion may indicate the increasing impact of primary production in the photic zone, with associated organic burial rates exceeding those of its oxidative mineralization of organic matter (Kump and Arthur, 1999). Variations in the δ13C signatures of shallow marine carbonates are widely used to interpret the primary variations in seawater δ13C during the Early Cretaceous (Jenkyns, 1995; Vahrenkamp, 1996; Grotsch et al., 1998). Carbon isotope values obtained from fine grained carbonate rocks are generally considered as appropriate proxies for seawater δ13C because the carbon isotopic composition is more resistant to post-depositional alteration than δ18O (Banner and Hanson, 1990). The limestones of the Canova Member are fine grained (micritic) whereas those in the El Caloso Member are both fine and coarse grained. The δ13C records of the Pitaycachi section suggest that the δ13C values measured are considered to represent original seawater composition (mainly above 0 and below +3‰; Föllmi et al., 1994). So, the carbon isotope data of bulk rocks from the Canova and El Caloso members will be compared with the published values of late Aptian - early Albian age in order to evaluate the reliability of δ13C values as a proxy for the δ13C of seawater.

A number of published studies state that carbon isotope geochemistry is considered a useful tool for the interpretation of the stratigraphy of pelagic sequences (Scholle and Arthur, 1980; Schlanger et al., 1987) as well as their shallow water counterparts (Jenkyns, 1995; Adabi, 1997; Ferreri et al., 1997; Heldt et al., 2008) and may also be used for global chronostratigraphic correlation where the age constraints are poor. The δ13C values (2.91 to 4.39‰) of the analyzed samples are slightly higher than the published values thought to be typical of Albian seawater (mainly above 0 and below +3‰; Föllmi et al., 1994; Menegatti et al., 1998; Bralower et al., 1999; Herrle et al., 2004; Wissler et al., 2004; Föllmi et al., 2006). Although there are differences in magnitude and absolute values, the shape of the carbon isotope curve of the Cerro El Caloso-Pitaycachi section is more or less identical to those recorded in mid-Cretaceous carbonates and marlstones from Italy, Mexico, Switzerland and France (Bellanca et al., 1996; Bralower et al., 1999; Strasser et al., 2001; Herrle et al., 2003, 2004).

The carbon isotopic variations observed in the Albian interval of the Pitaycachi section (δ13Ccarb variations are ~2 per mil) are lower than the shallow water limestones of the Mural Formation in the (Cerro Pimas Section (δ13Ccarb variations are ~4 per mil). However, the magnitude of variation in δ13Ccarb values of the Pitaycachi section is similar to other Tethyan and Mexican sections (Vocontian basin, France: δ13Ccarb variations are ~2 per mil, after Herrle et al., 2004; Mazagan Plateau: δ13Ccarb variations are ~2 per mil, after Herrle et al., 2004; Peregrina canyon, Mexico: δ13Ccarb variations are ~2 per mil, after Scholle and Arthur, 1980).

As the Pitaycachi section was deposited in the distal part of the basin, we have compared our results with the shallow water equivalent facies (Cerro Pimas section) in order to understand the lateral variations in the isotopic shift. The deep water Canova Member is correlatable with the shallow facies equivalent of the Los Coyotes and Cerro La Puerta members, while the El Caloso Member is correlated with the Cerro La Espina Member (Gonzalez-Leon et al., 2008). The limestones from the Los Coyotes and Cerro La Espina members are well developed in the Cerro Pimas section and the carbon isotope curve for this section has been studied by Madhavaraju et al. (2013). The carbon isotope curve in the Cerro Pimas section (-2.5 to +2.2‰ VPDB) shows fluctuations with larger amplitude than observed in the C-isotopic curve of the Pitaycachi section (+2.91 to +4.39‰ VPDB). It suggests that the shallow water settings are comparatively less stable in their isotopic composition than the open marine settings and that numerous factors, including changes in productivity, may magnify changes of the global oceanic carbon reservoir (Jenkyns, 1995; Vahrenkamp, 1996; Wissler et al., 2004). Overall, the carbon isotope curve of the Pitaycachi section is comparable to that of the Cerro Pimas section of the Mural Formation. We also compared the carbon isotope curve of the Pitaycachi section with those of Scholle and Arthur (1980) and Herrle et al. (2004) curves to understand the similarities between them (Figure 8). Based on the published isotope curves, we have identified three comparable segments (C12, C13 and C14) of Bralower et al. (1999) isotope curve and two identical segments (Al2 and Al5) of Herrle et al. (2004) curve.

In the Pitaycachi section, the commencement of OAElb is coincident with a sharp positive δ13C excursion followed by a decrease in δ13C values. The present study suggests that the global OAE1b is also present in the distal part of the Bisbee basin recorded in the Pitaycachi section. Although, as correlated, the Pitaycachi section has a significant positive excursion above OAElb (Paquier event), which suggests that the Bisbee basin might have been experienced multiple anoxic events (OAE 1b set) during the early Albian time. The observed OAE1b in this section may be comparable to Paquier event. Further, the detailed and high-resolution isotopic study in this section will provide further clue regarding the presence of other anoxic event particularly Leenhardt event.

 

CONCLUSIONS

The limestones of Canova Member mainly consist of micrite whereas the El Caloso member contains both mic-rite and coarse grained carbonate (more sparry calcite and blocky cements). The presence of the calpionellid species Calomiella recta and Calpionellopsella maldonadoi, and larger foraminifera like Orbitolina texana in the Canova Member suggest an early Albian age. The limestones show more negative δ18O values (-15.19‰ to -6.32‰) where as δ13C values show significant positive values (2.91‰ to 4.39‰). The lack of correlation between δ18O and δ13C values suggests that the limestones were not subjected to significant post-depositional modification and preserve their primary carbon isotope signatures. The carbon isotope curve of the present study shares three comparable segments (C12, C13 and C14) with that published by Bralower et al. (1999), and two identical segments (Al2 and Al5) with the Herrle et al. (2004) curve. The onset of OAE1b is paralleled by a significant increase in δ13C values in the Pitaycachi section, and is followed by a negative excursion. The general patterns of δ13C values excursions in the study section can be correlated with other Mexican and Tethyan sections.

 

ACKNOWLEDGEMENTS

This work was supported by Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de Mexico (UNAM) through Programa de Apoyo para la Superación del Personal Académico de la UNAM. We would like to thank Dr. Jonathan Kiddings and Dr. J.S. Armstrong-Altrin for their useful comments and suggestions which improved the quality of this paper. We thank Mr. Pablo Peñaflor, Estación Regional del Noroeste, Instituto de Geología, Universidad Nacional Autónoma de México for powdering of limestone samples for isotope analyses. We also thank Mrs. Adriana Aimée Orcí Romero for preparing thin sections for the petrographic study.

 

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