Abstract
The main goal of the paper is the reconstruction of a Middle Triassic buildup cropping out in the central part of the Southern Apennines. Middle Triassic reefs of the western Tethys realm are well known in the Northern and Southern Alps. In contrast, few studies of the Anisian–Ladinian carbonate platforms of the southern Apennines are available, due to the diagenetic alteration and tectonic disruption that hinder their paleoenvironmental and stratigraphic reconstruction. In an attempt to fill this gap, and to improve the knowledge on the Anisian–Ladinian carbonates of central Mediterranean area, this research is focused on a carbonate buildup cropping out in the “La Cerchiara” area, Sasso di Castalda (Basilicata, Southern Italy). The buildup, affected by intense tectonic deformation associated with the development of the Apennine thrust and fold belt, was studied using a statistical evaluation of the quantitative microfacies data. The research enabled a reconstruction of the original stratigraphic relationships of the various buildup fragments. A positive linear regression between the sample positions vs the percentage of autochthonous carbonates indicates an increase of the autochthons carbonate toward the top of the succession. The allochthonous fabrics (packstone/wackestone) at the base of the section (Unit IIIa) pass gradually upward into autochthonous (boundstones) facies (Units IIIb, I), consisting of microbialites (clotted peloidal micrite, microbial-derived laminae, and aphanitic micrite), microproblematica and cyanobacterial crusts, with few encrusting skeletal organisms. Statistical data suggest that units IIIa, IIIb, and I are in stratigraphic order while unit II appears to have been moved by tectonic dislocation from its original position at the base of the succession. The absence of metazoan reef framework, and the richness of micro-encrusters, autochthonous micrite and synsedimentary cements, suggest a mud-mound style of growth for the carbonate bodies of the Southern Apennine during the Anisian.
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Introduction
Mass extinction at the P/T boundary caused a sharp decrease in carbonate production, inducing a stasis in reef development (Sheehan 1985; Stanley 1988; Flügel 1994; Webb 1996; Enos et al. 2006; Minzoni et al. 2015). Therefore, Early Triassic carbonates were essentially characterized by a higher amount of microbialites than the end-Permian metazoan reefs (Sheehan and Fagerstrom 1988; Baud et al. 1997, 2007; Lehrmann 1999; Pruss et al. 2006; Brayard et al. 2011; Kershaw et al. 2012; Heindel et al. 2018; Martindale et al. 2019). Following this phase, during the Middle Triassic, the establishment of suitable carbonate environments, together with the recurrence of reefal skeletal organisms, allowed reefs to re-flourish (Flügel 1982, 2002; Velledits 1999, 2008; Velledits et al. 2011). During early-middle Anisian, the slow restoration of the carbonate producers led to the formation of buildups in which the contribution of skeletal organisms was minor in comparison with the microbial bio-induced component, which was indispensable for their growth.
Triassic reefs have been widely studied in the Dolomites, where, from Anisian through Carnian times, low-relief terrigenous-carbonate ramps, rich in loose micritic mud, evolved into isolated high-relief carbonate buildup, dominated by automicrite and syndepositional cements (Biddle 1981; Gaetani et al. 1981; Brandner et al. 1991; Harris 1993, 1994; Blendinger 1994, 1996; Keim and Schlager 1999, 2001; Emmerich et al. 2005; Russo 2005; Stefani et al. 2010; Marangon et al. 2011; Guido et al. 2016, 2018, 2019). Anisian buildups generally lack primary metazoan framework and evidence of strong syndepositional cementation (Bosellini and Rossi 1974; Cros 1974), whereas late Anisian–early Ladinian buildups are dominated by autochthonous micrite, calcimicrobes, microproblematica, and synsedimentary cements (Bechstädt and Brandner 1970; Brandner and Resch 1981; Gaetani et al. 1981; Brandner et al. 1991, 2007, 2012; Russo 2005; Seeling et al. 2005; Brandner and Keim 2011). Late Ladinian and Carnian platforms, developed after a Ladinian volcanic event, consist mainly of micrites, cements and subordinately skeletons (Bosellini 1984; Blendinger 1994; Russo 2005; Stefani et al. 2010). Automicrites make up the main constituent of the late Ladinian–Carnian carbonates, accounting for the 50% of the rock volume, whereas cements amount to 20%, and skeletal remains to less than the 10% (Russo 2005; Stefani et al. 2010). Metazoan skeletons are subordinate comparing to microproblematica and microbial-induced carbonates. During the Carnian, small calcareous bioconstructions, interpreted as patch reefs, show similarity with modern bioconstructions, constituted of a primary calcified demosponge and scleractinians skeletal framework (Russo 2005; Stefani et al. 2010). Taxonomic diversity increased greatly, and the skeletal components exceed 50% of the rock volume (Russo 2005; Stefani et al. 2010).
Western Tethyan Anisian–Ladinian reefs are well known from the Northern and Southern Alps and from Hungary (Flügel 2002; Velledits et al. 2011), whereas only very few studies have been focused on the Middle Triassic reefs exposed in the Southern Apennines and in general in Central Mediterranean area. In the study area, paleontological, sedimentological and structural studies were addressed to the characterization of the Monte Facito Formation cropping out in Basilicata, but they have not adequately defined the geometry, structure and paleoenvironmental evolution of the carbonate bodies, due to the late dolomitization, intense tectonic deformation, and faulting (Scandone 1967; Donzelli and Crescenti 1970; Wood 1981; Ciarapica et al. 1986, 1990a; b, c; Panzanelli Fratoni et al. 1987; Miconnet 1988; Rettori et al. 1988; Martini et al. 1989; Ciarapica 1990; Panzanelli Fratoni 1991; Marsella et al. 1993; Ciarapica and Passeri 2000; Palladino 2015; Palladino et al. 2019).
Rare exposures of not-dolomitized carbonate bodies provide unique opportunity for studying the Middle Triassic buildups, in the central Mediterranean area. Among them, the carbonate units exposed at “La Cerchiara” (Basilicata, Southern Apennines; Figs. 1 and 2) provide a key contribution to the reconstruction of the type, paleoecology and paleoenvironmental evolution of the Anisian-(?)Ladinian buildups of this area. Characterization of their microfacies through quantitative analyses has allowed us to: (a) reveal the main constituents involved in the buildup growth; (b) distinguish the roles of metazoan vs microbialites in the carbonate production; (c) evaluate the depositional textures (autochthonous vs allochthonous); (d) correlate the microfacies variation with the depositional geometries; (e) reconstruct the paleoenvironment evolution of the buildup; and (f) compare the buildup with coeval carbonate platforms of the Tethys realm.
Geological setting
The “La Cerchiara” succession (40.509317° N, 15.694757° E), located in the area of Sasso di Castalda (Basilicata) (Figs. 1 and 2), is one of the most representative outcrop of the Early-Middle Triassic Monte Facito Formation (Scandone 1967; Wood 1981; Ciarapica et al. 1990a, b, c; Palladino 2015; Palladino et al. 2019). The Monte Facito Formation is a composite stratigraphic unit, consisting of isolated platform limestone slabs, fine- to medium-grained siliciclastic rocks, and radiolarites, which accumulated during the opening of the Lagonegro basin (Patacca and Scandone 2007). According to several authors (Finetti et al. 1996; Ciarapica and Passeri 2002; Stampfli and Borel 2002), the development of this basinal area was connected to the evolution of the late Permian–Early Triassic Ionian Sea, representing the northeastern prolongation of the Neo-Tethyan Oceanic domain. Other authors argue that the Lagonegro was an independent basin, not connected to the Tethys (Scotese and Schettino 2017; van Hinsbergen et al. 2020). Due to later tectonic processes, the original basement that hosted the sedimentation of the Monte Facito Formation is unknown (Patacca and Scandone 2007). For this reason, the determination of its original position above a possible continental or oceanic crust represents an unsolved problem in the geology of the Southern Apennines (Argnani 2013).
The Monte Facito Formation lies at the stratigraphical base of the Lagonegro Basin succession, which also includes the Calcari con Selce (Late Triassic), Scisti Silicei (Late Triassic-Jurassic), Galestri (Cretaceous) and Flysch Rosso (Cretaceous-Oligocene) formations (Scandone 1967, 1972; Donzelli and Crescenti 1970; Wood 1981; Ciarapica et al. 1988, 1990c; Miconnet 1988; Martini et al. 1989; Panzanelli Fratoni 1991; Marsella et al. 1993; Ciarapica and Passeri 2000; Passeri and Ciarapica 2010).
After deposition, the Lagonegro Basin succession has been affected by intense contractional deformation during the Miocene building of the Southern Apennines thrust and fold belt. This process led to the detachment of the Monte Facito Formation from its original basement, along a low-angle regional thrust surface, which is responsible for the general doubling of the Lagonegro Basin units, identified, respectively, as Lagonegro Unit I, located at the footwall of the thrust, and Lagonegro Unit II, at its hanging wall (Scandone 1972). During Early Pleistocene, the tectonic regime in the Apennine chain changed from contractional to extensional, as testified by the presence of strike-slip and normal faults, crosscutting pre-existing thrusts and folds (Bucci et al. 2014).
The Monte Facito Formation is commonly defined as a chaotic complex and it is often considered as a sedimentary mélange (Wood 1981; Marsella et al. 1993; Patacca and Scandone 2007; Palladino 2015; Palladino et al. 2019). The main evidence for this interpretation is the frequent presence of carbonate olistoliths and disrupted strata within a clayey and silty matrix (Ciarapica and Passeri 2000; Passeri and Ciarapica 2010). According to Palladino (2015), emplacement of sedimentary mélange followed the formation of carbonate build-ups of Early Ladinian age. Mélange deposits are thought to record diffuse land-sliding phenomena connected to the initial continental break-up of the Adria plate and to the opening of the Lagonegro Basin, starting from the Ladinian (Marsella et al. 1993; Patacca and Scandone 2007). More recent studies demonstrated that the current configuration of the Monte Facito Formation has been produced by a more complex evolution, resulting from a contractional tectonic overprint on an already chaotic Middle Triassic sedimentary mélange (Palladino et al. 2019).
The “La Cerchiara” succession
The “La Cerchiara” outcrops are roughly E–W oriented and expose an about 1400 m thick succession consisting of carbonate units alternating with basinal shales, followed by paraconglomerates and deep-water deposits (shales and radiolarian cherts) (Fig. 3). The studied section starts with shallow-water carbonates, organized in tens of meters-thick units separated by laminated deep-water yellow and red shales (Fig. 4). This first interval, known in the geological literature as the “Lame succession” (Ciarapica and Passeri 2000), shows an average thickness of 300 m and represents the main topic of our research. The age of the carbonate sequence has been doubtfully attributed to late Anisian–early Ladinian, on the basis of the algae, foraminifers, conodonts and calcareous sponge association (Scandone 1967; Panzanelli Fratoni et al. 1987; Miconnet 1988; Rettori et al. 1988; Martini et al. 1989; Ciarapica 1990; Ciarapica et al. 1990a, b, c; Panzanelli Fratoni 1991; Marsella et al. 1993; Ciarapica and Passeri 2000). The exact chronostratigraphic attribution is however not clearly defined, due to the contradictory data reported by various authors. The uncertainty mainly derives from the absence of accurate biostratigraphic markers and from the significant fragmentation of the carbonate bodies. In particular, the eastern build-up body (Unit I, see Fig. 3) was tentatively dated to the Anisian–Lower Ladinian transition (Illirian–Fassanian) for the presence of the conodont Paragondolella alpina szaboi (Ciarapica and Passeri 2000), whereas the western one (Units IIIa and IIIb, see Fig. 3) was attributed to a generic Ladinian for the presence of the foraminifers Lamelliconus procerus and Lamelliconus ex gr. ventroplanus which excludes a reference to Anisian (Ciarapica and Passeri 2000).
Although uncertainties remain, the abundance of microbialites, calcimicrobe crusts and microproblematica, very similar to the typical Anisian carbonate succession of the Southern Alps (Gaetani et al. 1981; Gaetani and Gorza 1989), suggests referring the studied carbonate units with the latter ones. The succession continues eastward with about 100 m brown shales, alternating with turbiditic sandstones and conglomerates, dated as late Ladinian (Ciarapica and Passeri 2000). The remaining portion of the succession, about 300–400 m thick, mainly consists of shales and radiolarites, comprising olistoliths, breccias and slide deposits (late Ladinian). The final part of the succession consists of alternating pelagic limestones and shales that characterize the transition toward the overlying “Calcari con Selce” Formation.
Our study is focused on quantitative microfacies characterization of the carbonate units in the “La Cerchiara” succession (Figs. 2, 3, and 4). The limestones were affected here by an initial phase of diagenetic recrystallization, but not affected by dolomitization that hampers the microfacies study of some of the carbonates outcropping in the region. Tectonic overprint is outlined by large-scale folding of the carbonate units, showing steeply dipping upright and locally overturned beds. This deformation challenges reliable geometric, stratigraphic and paleoenvironmental reconstructions. The complex tectonic setting led previous authors to formulate opposing interpretations of the younging direction of the “La Cerchiara” succession. Based on field observations, Scandone (1967) and Wood (1981) inferred an eastward younging, whereas Ciarapica and Passeri (2000) proposed westward younging, as suggested by paleontological data. More recently, support for eastward younging of the “La Cerchiara” succession was provided by Palladino (2015) on the basis of sedimentological criteria.
The base of the succession coincides with a normal fault that forms the western boundary of the carbonate succession (Fig. 2). The four carbonate intervals, here identified as Units, have been termed “Lame” by Ciarapica and Passeri (2000), who provided also the age estimates, based on foraminifera and conodonts content. The base of the succession consists of two superimposed planar-bedded carbonate bodies, 110 and 64 m thick, here identified as Unit IIIa and Unit IIIb (Figs. 3 and 4). Foraminifera content suggests a generic Ladinian for this carbonate body. These two Units, interpreted by Ciarapica and Passeri (2000) as a tectonic duplication of the same carbonate unit, are separated by a 10 m thick red shale interval. The succession continues upward with 20 m of red shales, characterized by a poor paleontological content, similar to the interval occurring between Unit IIIa and IIIb. The subsequent Unit II, attributed to a generic Ladinian, consists of a thin carbonate body (6 m thick) that pinches out northward and is separated from Unit I by 20 m of yellowish shales, dubiously dated to Fassanian?- early Longobardian? using conodonts content. Unit I, representing the uppermost carbonate body of the studied section, is 42 m thick and it is attributed to an Illirian–Fassanian according to conodonts content (Figs. 3 and 4).
Methods and studied materials
The four carbonate Units (I, II, IIIa and IIIB) were sampled in detail for microfacies analyses as follows: 30 samples from Unit III, 3 samples from the Unit II, and 8 samples from the Unit I (Figs. 3 and 4). Two thin sections, one perpendicular and one parallel to the bedding plane, were prepared from each sample. Microfacies characterization was performed with an optical microscope (Zeiss Axioplan Imaging II) under plane and cross-polarized light. Quantitative analyses of the microfacies were performed by point counting 24 polished thin sections. A grid with a 0.5 mm count step was used to count 400 points for each thin section, following the grain counting methodology described in Flügel (2010). The percentage of the various components was automatically obtained using a Counter AC-15 apparatus.
Epifluorescence observations were used to detect the distribution of the organic matter, with incident light emitted by a Hg high-pressure vapor bulb attached to Axioplan Imaging II microscope (Zeiss), equipped with high-performance wide bandpass filters (BP 436/10 nm/LP 470 nm, no. 488 006, for green light; and BP 450–490 nm/LP 515 nm, no. 488009, for yellow light).
Micro/nano-morphological studies were carried out with an FEI-Philips ESEM-FEG Quanta 200F Scanning Electron Microscope (SEM) on freshly broken samples, polished surfaces, or thin sections. In the last two cases, the observed surfaces were prepared with 0.25 micron diamond-impregnated grinding paper, then gently etched (0.05% HCl, 1 min). The samples were then carbon- or gold-coated (ca. 250 Å coating thickness). SEM working conditions were as follows: accelerating voltage of 15 kV, working distance between 10 and 15 mm.
Mineralogical and chemical analyses were obtained using an Electron Probe Microanalyzer (EPMA), JEOL- JXA 8230 on polished surfaces or thin sections, prepared with the same procedure as for SEM observations, but without the carbon or gold coating. EPMA working conditions were as follows: voltage 15 keV, Probe current 10 nA, Working Distance 11 mm, Take-off angle 40°, Live Time 50 s.
Results and analyses
Field observations
The carbonate Unit interval of “La Cerchiara” succession consists of carbonates and shales (Fig. 2). The carbonates are organized in four irregular-shaped bodies (Units), with thicknesses of the strata from tens of centimeters up to few meters (Figs. 3 and 4). They show bedding from planar, as in Unit IIIa and Unit II, to massive, as in Unit IIIb and I. The carbonates are light gray in color and show very finely crystalline matrix. Only larger grains, representing fragments of dasycladacean algae and intraclasts, are generally visible. Millimetric- to centimetric-sized cavities commonly occur, which are occluded by generations of isopachous and sparry cements. These cavities often contain yellowish material interpreted as fine-grained dolomite by Ciarapica and Passeri (2000).
Thin-section analyses
Carbonate components
The microfacies of the carbonate Units consist of boundstones and subordinately packstones, wackestones and grainstones. The boundstones are composed of encrusting organisms (calcimicrobs, foraminifers and microproblematica), green algae (Dasycladales) and calcisponges (Sphinctozoa). A high amount of autochthonous micrite is also present. It occurs as very fine-grained laminations, varying in size from few microns to tens of microns. The laminae generally encrust lithoclasts of reworked boundstone, skeletal fragments and detrital intervals. Clotted peloidal and aphanitic (structureless) textures are also widespread. Several generations of isopachous cements are present. They have a cloudy aspect, due to the presence of organic matter. Skeletal fragments of echinoderms and mollusks are less abundant. Homogeneous matrix containing small bioclasts and lithoclasts is encountered as detrital micrite. The amount and the relative texture of these components are variable in the different carbonate Units. Generally, the carbonates are affected by diagenesis, which sometimes make difficult to interpret the original microfacies.
Micrite types
The micrite is encountered mainly as microsparite as a consequence of the recrystallization processes which affected by the studied carbonates. Despite the diagenetic alteration, it was still possible to recognize two micrite types (Fig. 5a–d). They were discriminated by means of their depositional fabrics. Micrite organized in wrinkled laminations (Fig. 6a, b), pelodail clots (Fig. 6c), and structureless (aphanitic) (Fig. 5c), was attributed to autochthonous micrite derived from microbial metabolic activities. Micrite showing homogeneous and compact texture, which include fine bioclasts and lithoclasts, was attributed to allochthonous micrite. Autochthonous micrite, with finely crystalline light and dark wavy-wrinkled laminations, forms crusts that developed on various substrates (skeletal grains, intraclasts) (Fig. 6a, b). The growth patterns of these irregular crusts do not reflect physical depositional processes, notably transport and deposition. They are related to biological origin (microbial-mediated deposition) and syndepositional cementation (Fig. 5a, b). The bright epifluorescence of the autochthonous micrite suggests organic matter trapped among the finely calcite crystals (Fig. 5b, d). The presence of amorphous carbonaceous material among the fine crystals of autochthonous micrite, confirms the presence of organic matter and the bio-induced nature of this component. Organic matter remains were observed on both etched thin section surfaces and freshly broken fragments, do not treated with acids, excluding an artifact nature for their origin (Fig. 7a, c, d). Laminations occasionally form micro-columnar structures (Figs. 5a and 6b). Dark and light laminae differ in crystals size; the former are made of microcrystalline calcite (< 5 µm), the latter of microsparry calcite (> 10 µm) (Fig. 8). EPMA microanalysis revealed that the dark laminae are composed of low Mg-calcite, with average Ca and Mg contents of 99 and 1 wt%, respectively, whereas the light laminae show low Mg-calcite with average Ca and Mg content of 98 and 2 wt%, respectively.
Clotted peloidal micrite is often associated with calcimicrobes (Fig. 9a, b), microproblematica (Tubiphytes sp., Baccanella floriformis and Microtubus communis) (Fig. 9c–e), sponges (Olangocoelia otti) (Fig. 9f) and agglutinated polychaeta (Terebella) (Fig. 10c). The organic matter remains, revealed by UV epifluorescence, testify the bio-induced nature of this type of micrite. It is composed of low Mg-calcite, showing a crystal size < 2 μm, with average Ca and Mg contents of 98.6 and 1.4 wt%, respectively. Occasional autochthonous aphanitic micrite, often associated with Baccanella floriformis, is composed of low Mg-calcite, similar in composition to the peloidal micrite.
The allochthonous micrite has a homogeneous texture (Fig. 7b) and low content of organic matter, as indicated by the weak epifluorescence. Siliciclastic grains and clay minerals are dispersed within the bioturbated allochthonous micrite. This micrite type is abundant in Unit IIIa and II, and less frequent in Unit IIIb and Unit I.
Microfacies of the carbonate units
Unit IIIa
Detrital carbonates dominate Unit IIIa. Allochthonous micrite is abundant and the texture varies from mud (wackestones, Fig. 10a, b) to grain supported (packstones, Fig. 10c). Rare boundstones are present as cyanobacterial crusts, stabilizing medium-fine debris fractions (Fig. 10d). Lithoclasts, which are the main granular components (Fig. 10b), most likely originated as reworked boundstone, and are mainly composed of microproblematica (Tubiphytes sp., Baccanella floriformis), calcimicrobes (Girvanella sp.), and automicrite. The densely packed allochthonous micrite matrix shows mottles of bioturbation, engulfs small bioclasts and intraclasts (Fig. 10a), and is rich in green algae (Teutloporella herculea, Teutloporella nodosa), agglutinated foraminifers (Fig. 10c), and fragments of thin-shelled bivalves (Fig. 10a).
Unit IIIb
The Unit IIIb shows a great abundance of autochthonous micrite (Fig. 11a–d), microproblematica (Fig. 11a), and cyanobacterial crusts (Fig. 11c). The micrite shows mainly peloidal to clotted peloidal textures (Fig. 11d). Aphanitic texture (Fig. 11a, b) and laminae with antigravitative structures (Fig. 11c) are also present. The Unit is dominated by boundstones carbonates, and the main skeletal components are represented by microproblematica (Tubiphytes sp., Baccanella floriformis and Microtubus communis) and calcimicrobes (i.e., Girvanella) (Fig. 11a–d). Autochthonous micrite with columnar micromorphology are common (Fig. 11c). Isopachous early cements, up to several millimeters in thickness, and late druse cement, filling residual microcavities, are also present (Fig. 11b).
Unit II
Unit II is dominated by packstones (Fig. 12), similar in composition to those of Unit IIIa, and it is rich in grains derived from reworked boundstones (Fig. 12a–d). Sample LC33 is a mudstone/wackestone with traces of bioturbations and fine skeletal grains. Thin-shelled bivalves are frequently present, in association with occasional fragments of calcisponges (Olangocoelia otti), gastropods and polychaets (Fig. 12c). Only one sample (LC32) shows abundant clasts of reworked boundstone rich in autochthonous micrite, microproblematica and cyanobacterial crusts, similar to those in Unit IIIb (Fig. 12b).
Unit I
Unit I is mainly characterized by boundstones and rare packstones (Fig. 6a–f). The high amount of autochthonous micrite shows peloidal to clotted peloidal texture (Fig. 6e). The main boundstone constituents are microproblematica (Baccanella floriformis, Microtubus communis and Tubiphytes sp.), calcisponges (Olangocoelia otti), and calcimicrobes (Girvanella) (Fig. 6a–d). Subordinate skeletons include dasycladacean algae (Diplopora annulata, Teutloporella herculea, Teutloporella nodosa) and agglutinated polychaets (Terebella). Inter-skeletal cavities are lined by isopachous polyphase millimeter- to centimeter-thick cements (Fig. 6f) that have a cloudy aspect due to the presence of organic matter, evidenced by UV epifluorescence observations (Fig. 5e, f).
Geopetal allochthonous micrite and sparry calcite fill microcavities of the microbial boundstones (Fig. 6f). They prove the in situ deposition of these microfacies and reveal the original growth polarity of the buildup, in agreement with the eastward younging direction indicated by field evidence.
Early cements
Early cements, mainly associated with autochthonous micrite, cyanobacterial crusts and microproblematica, had a significant role in stabilizing the boundstones. They occur in Unit IIIb (Fig. 7b) and appear abundant in Unit I (Fig. 6f). These cements were observed in polished hand specimens as fibrous calcite bands of various thickness (from millimeter to centimeter) and appearance (cloudy and whitish). Cements occlude the primary porosity of the microbialite/microproblematica framework. Lithoclasts of reworked boundstone sometimes provided the substrate for the growth of the isopachous cements. These cements are characterized by alternation of cloudy and whitish bands showing epifluorescence, indicating that the organic matter is mainly concentrated in the cloudy bands (Fig. 5e, f).
Quantitative analyses of the microfacies
Quantitative analyses of the carbonate components were performed by point counting (Table 1 and 2). The microfacies were grouped into: (1) autochthonous carbonates, mainly formed of cyanobacterial crusts, microproblematica, microbial micrite, and boundstone sponges; (2) detrital carbonates, formed of bioclasts, intraclasts, lithoclasts, and allochthonous micrite. Isopachous (early) and drusy (late) cements were counted separately, both showing a weak and barely significant increase moving up-section.
The data show a general increase, from Unit III to Unit I, in autochthonous relative to detrital carbonates components (Fig. 13).
In the autochthonous carbonates (Units IIIb and I), with typical boundstone facies, the peloidal micrite (40–63%) is the main constituent among bio-induced autochthonous micrite, followed by laminated microfabrics (1–4%), and aphanitic micrite (0.5–2%). Cyanobacterial crusts are present throughout the succession, constituting from 2 to 8% of the total microfacies of the autochthonous carbonates. Similarly, microproblematica constitutes from 1 to 6% of the total rock volume.
Utilizing the sample positions as independent variable and the quantitative amount of autochthonous carbonates as dependent variable, it is possible to recognize a discrete positive linear regression (y = 0.002x + 0.129) with a correlation coefficient R2 = 0.60 (Fig. 14a). This is consistent with a linear increase of the autochthons carbonate toward the top of the succession. The sample positions vs detrital carbonates shows a negative linear regression (y = − 0.0026x + 0.8124) (R2 = 0.66), confirming a linear decrease of detrital carbonates toward the top of the succession (Fig. 14b). If we assume that Unit II was positioned at the base of the sequence before the tectonic events, the coefficients R2 increase considerably (0.75 and 0.74, respectively) (Fig. 14c, d), strengthening the hypothesis of the unit displacement after its origination.
Interpretation and discussion
Microfacies evolution and paleoenvironmental reconstruction
The well-preserved carbonate bodies of the “La Cerchiara” succession allow us to propose a model for the paleoenvironment reconstruction of a Middle Triassic buildup of Southern Apennines (Italy). We suggest that the quantitative variations in microfacies, depositional textures, cement abundances and micrites type, indicate a depositional evolution from lower to upper slope facies. The wackestones and packstones of Unit IIIa, originally consisting of loose detrital sediments, correspond to distal-slope facies, supplied by a bio-constructed margin located, probably, to the east of the study area (Fig. 15). The few boundstone horizons are formed by fine detrital grains, encrusted and stabilized by microbial laminae, forming bindstone fabric.
Unit IIIb and Unit I represent the upper slope/margin of the buildup, deposited into a shallower environment. This is suggested by the increase in boundstones, rich in autochthonous micrite, cyanobacterial crusts, microproblematica and early cements.
Ciarapica and Passeri (2000), considering their paleontological content, interpreted the two carbonate units of Unit IIIa and Unit IIIb as coeval parts of the same carbonate body, superposed one upon each other by a tectonic contact. Our microfacies data suggest that these carbonate bodies record different depositional environments. Specifically, Unit IIIa was deposited on a distal slope and Unit IIIb in an upper slope environment. Unit I represents the marginal extension of the bioconstruction (Fig. 15). The thin Unit II, cropping out between Unit IIIb and I, records a sharp change in depositional facies, from upper slope autochthonous micrite to allochthonous/detrital micrite of the distal-slope basin (Fig. 15). This abrupt change can be explained either by tectonic displacement of the thin Unit II, from the base of the succession to its current position between the Unit IIIB and I, or by an abrupt variation in paleoenvironmental conditions. The correlation coefficients R2 (0.60 for autochthonous carbonate and 0.66 for detrital carbonates) increase moving the Unit II at the base of the succession (0.75 for autochthonous carbonate and 0.76 for detrital carbonates). These data strengthen the hypostasis of a tectonic displacement of Unit II.
Thus, the quantitative microfacies analysis indicates the development of a single carbonate system, in which the facies pass eastward from a distal slope to a proximal margin facies. In our interpretation, the carbonate units at “La Cerchiara” derive from a unitary buildup succession. This is in agreement with the models proposed by Miconnet (1988) and Palladino et al. (2019), in which the Monte Facito Formation would consist of different part of a series of platform units, partly re-sedimented into siliciclastic basinal sediments of Ladinian age and later disrupted by tectonic deformation.
Depositional relationships between the carbonate units
The basal and lateral relations of the carbonate bodies are not visible. In addition, while the western part of the outcrop (Unit IIIa) is organized in more or less planar beds, the eastern part (Unit IIIb and Unit I) has a massive appearance, with variable lateral thickness. However, the variations in the carbonate constituents, revealed by the quantitative microfacies analyses, reflect the primary depositional relationships. The lower beds (Unit IIIa) are mainly characterized by detrital microfacies, while the upper massive bodies (Unit IIIb and Unit I) mainly consist of syndepositional cemented autochthonous boundstones. Micrite type varies along the section: allochthonous micrite prevails in the lower interval and tends to decrease in abundance towards the upper interval, where it is progressively substituted by autochthonous micrite. The variation from allochthonous to autochthonous micrite and the sindepositional cementation of the boundstone facies could reflect a change in the growth morphology of the buildup, even though this is presently obscured by the tectonic deformation. A similar trend occurs in an upper Anisian platform of the Dolomites (Sasso Bianco section, Formazione di Contrin) (Guido et al. 2016). Here, the succession records a change from loose detrital micrite, which dominates the lower carbonate bank, to syndepositional lithified micrite in the upper buildup (Guido et al. 2016). This variation is associated to a change in the depositional geometry, i.e. the steepening up of the slope. Similar relationships between carbonate sediments and depositional slope geometries have been documented by numerous studies (Kirkby 1987; Kenter 1990; Adams et al. 1998, 2002; Keim and Schlager 1999; Adams and Schlager 2000; Marangon et al. 2011). Schlager and Reijmer (2009) showed how different types of micrite affect the depositional geometry of slopes. Loose sedimentary particles precipitate as mud can readily be re-suspended during storms and exported to form low-angle slopes. On the contrary, in situ precipitation induced by microbial activity can form autochthonous early cemented micrite that stabilizes sediment on steep slopes.
Comparison with coeval Anisian–Ladinian carbonate buildups
The absence of metazoan reefal communities, forming a primary skeletal framework, and the dominance of micro-encrusters, microbialites and synsedimentary cements, are characteristics of early-middle Anisian period in the western Tethyan buildups of the Dolomites (Bosellini and Rossi 1974; Cros 1974; Gaetani et al. 1981; Bosellini 1984; Fois and Gaetani 1984; Gaetani and Gorza 1989; Brandner et al. 1991, 2012; Senowbari-Daryan et al. 1993; Blendinger 1994; Harris 1994, 1996; Russo et al. 1997, 2000; Keim and Schlager 1999, 2001; Emmerich et al. 2005; Russo 2005; Schlager and Keim 2009; Stefani et al. 2010; Marangon et al. 2011; Tosti et al. 2011, 2012, 2014; Guido et al. 2016, 2019). Synsedimentary autochthonous micrite, Tubiphytes and cement crusts have also been recorded in middle Anisian buildups of the northern and western Tethys (Okay et al. 1994; Grădinaru 1995, 2000; Săndulescu 1995; Banks and Robinson 1997; Török 1998; Szulc 2002; Hips 2007; Popa et al. 2014; Hips et al. 2015; Martindale et al. 2019). Similar evolution, from lower to upper slope facies, was also detected in Anisian platforms of the eastern Tethys (Enos et al. 1997, 2006; Kershaw et al. 1999, 2002, 2007, 2012; Lehrmann 1999; Payne et al. 2006, 2011; Lehrmann et al. 2007; Cao and Zheng 2009; Chen et al. 2009; Feng et al. 2010).
Fois and Gaetani (1984) described the recovery of rich and well-preserved Anisian reef-building communities in the Italian Dolomites. They recognized three growth stages of reefs, after the Permian–Triassic crisis. Although less rich and not so well preserved, the carbonate Units of the “La Cerchiara” succession are similar to the mounds described by Fois and Gaetani (1984). Nevertheless, it is clear that both communities lacked primary skeletal framework, although this was, to some extent, substituted by autochthonous micrite, encrusting algae, microproblematica and porifera. Some organisms are present in Anisian sediments of both both “La Cerchiara” and the Dolomite, e.g., calcareous algae (Diplopora annulata, Teutloporella herculea, Teutloporella nodosa, Physoporella sp.), Tubiphytes, Olangocoelia otti and cyanobacteria. The abundance of early cements in the “La Cerchiara” carbonates together with the minor abundance of organisms, represents a significant difference, in comparison with Anisian facies of the Dolomites described by Fois and Gaetani (1984). The studied units show similarity also with middle Anisian carbonates cropping out in south-eastern Romania (Popa et al. 2014), that consist of microbialitic boundstones, allochthonous micrite, and Tubiphytes, reinforced by large volumes of marine cements. The studied microfacies, of the central Mediterranean area, are comparable in term of amount of autochthonous micrite, with those of the Middle Triassic Hungarian reefs, but in these latter microbialites play a mutual role with sponges in formation of typical mud-mound deposit (Török 1998; Schlager 2003; Hips 2007; Hips et al. 2015; Martindale et al. 2019).
The widespread presence of microbialites and the lack of skeletal framework suggests a “mud mound” growth model for the Anisian “La Cerchiara” buildup. Microbialites are known to have significantly contributed to “reef”-like structures, in the past as well as in the present (e.g. Wood 1999, 2001; Saint-Martin et al. 2000; Olivier et al. 2004; Nose et al. 2006; Westphal et al. 2010; Sánchez-Beristain and Reitner 2019) and their role in building “mud mound”-like structures has long been recognized (Reitner and Neuweiler 1995; Dupraz and Strasser 2002; Chan et al. 2014). They can reach significant abundances (more than 50%) in ancient frameworks, particularly after major extinction events (Zhuravlev 1996; Turner et al. 2000; Shapiro 2004; Delecat and Reitner 2005; Ezaki et al. 2008; Zamagni et al. 2009; Tunis et al. 2011; Astibia et al. 2012; Kershaw et al. 2012; Wahlman et al. 2013; Kershaw 2017).
Conclusion
Before reworking, the carbonate units of the “La Cerchiara” succession belong to a single buildup, characterized by the absence of a skeletal framework, with high abundances of micro-encrusters, microbialites and early cements. The microfacies quantitative study of the carbonate units revealed a linear trend from detrital to autochthonous carbonate. The positive linear regression of the sample positions vs quantitative amount of autochthonous constituents moving toward the top of the succession, and the negative linear regression of sample positions vs detrital constituents in the same direction support this hypothesis.
The microfacies change is also in agreement with the inferred depositional geometries of the carbonate buildup. The change from the sub-horizontal beds of Unit IIIa to the massive beds of Units IIIb and I strengthens the model of a transition from distal-slope allochthonous sediments to upper slope/margin syndepositionally cemented and bio-constructed deposits. Statistical data suggest that units IIIa, IIIb and I are in stratigraphic order while unit II appears to have been moved by tectonic dislocation from its original position at the base of the succession. The richness in micro-encrusters, autochthonous micrite, and synsedimentary cements, together with the absence of metazoan reef communities forming a primary framework, suggests strong similarities with microbial-mound platform facies of similar early-middle Anisian age developed in the western Tethys.
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Acknowledgements
The authors wish to express their gratitude to Robert Riding for constructive comments and suggestions. Dr Mariano Davoli, University of Calabria, is thanked for help for technical support during SEM and EPMA data acquisition. This research was financially supported by MIUR (ex 60% 2019 A. Guido, University of Calabria). Data available on request from the authors.
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Guido, A., Palladino, G., Sposato, M. et al. Reconstruction of tectonically disrupted carbonates through quantitative microfacies analyses: an example from the Middle Triassic of Southern Italy. Facies 67, 22 (2021). https://doi.org/10.1007/s10347-021-00631-2
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DOI: https://doi.org/10.1007/s10347-021-00631-2