From Clastics to Carbonates and Black Shales: Deciphering Sedimentary Continuity and Discontinuity in the Devonian Landscape of the Volga-Ural Petroleum Province

1. Introduction

The Devonian succession of the central part of the Volga-Ural petroleum province (Figure 1), situated at depths of 1500-2000 metres, consists of three predominant types of marine sediments: clastic, carbonate, and black shale. The clastic and carbonate sediments, recognised as oil and gas bearing, contain over 900 oil plays (Muslimov, 2008). Black shales are commonly considered as oil source rocks due to their significant content of sapropelic organic matter (Strakhov, 1938; Stupakova et al., 2015, 2017; Liang et al., 2020; Kabanov et al., 2023a,b).

Detailed lithological and biostratigraphic analyses of the Devonian strata in the central part of the Volga-Ural province were completed by the end of the 20th century. The outcomes of these studies have been generalised in regional stratigraphic schemes (Decision…, 1990; Resolutions…, 2008; Fortunatova et al., 2018) and are summarised in specialised publications (Menning et al., 2006; Zonal stratigraphy…, 2006).

Recent studies have concentrated on examining the sedimentological and facies characteristics of Devonian sediments to develop detailed sedimentary models. These models have been developed separately for clastic sediments (Fortunatova et al., 2013; Loscheva et al., 2017; Silantiev et al., 2022), carbonate sediments (Fortunatova et al., 2016; Yousef et al., 2023), and black shales (Stupakova et al., 2015, 2017; Liang et al., 2020). In most cases, the authors examine only a certain stratigraphic interval of interest, not always using new stratigraphic schemes and data.

This study compares the regional Devonian conodont zonation of the Volga-Ural province (Aristov, 1988; Ovnatanova and Kononova, 2008; Nazarova and Kononova, 2015, 2020) with the standard conodont zones (Ziegler, 1962, 1969, 1971; Ziegler and Sandberg, 1984; 1990; Sandberg and Ziegler, 1996) and the global conodont zonation outlined in the modern Chronostratigraphic Chart (Becker et al., 2020). This comparative analysis clarifies the overall continuity of the Devonian succession in the central part of the Volga-Ural province and helps determine the duration of regional stratigraphic subdivisions (Regional Stages) in terms of absolute age.

We further analysed three predominant types of sedimentation observed in various settings of study area during the Devonian period (Aliev et al., 1978; Gubareva, 2003; Fortunatova et al., 2018): (1) condensed and non-condensed depressions, (2) slopes of depressions, and (3) shallow water environments situated within tectonic arches or local biohermal uplifts. Using the chronostratigraphic framework and available data on the rates of modern and ancient sediment accumulation, we demonstrate the duration of sediment deposition of different types in various settings of the basin. As expected, the completeness of the sedimentary record increases in the transition from shallow to deep-water environments, while the number of discontinuities in the stratigraphic succession is maximal in shallow-water settings. Evidently, these patterns are crucial for well log correlation and geological modelling.

Therefore, this study aims to ascertain the completeness of the Devonian sedimentary sequences within diverse marine environments in the central region of the Volga-Ural province. The research involved (1) the analysis of current biostratigraphic and chronostratigraphic data; (2) the examination of the three predominant types of sedimentation present in the study area during the Devonian period.

2. Geological Settings

In the central region of the Volga-Ural petroleum province, the Devonian succession is stratified into three series: Lower, Middle, and Upper, encompassing a total thickness of 500–1500 metres. The Lower Devonian (Emsian) exhibits a local distribution, in contrast to the Middle and Upper Devonian formations, which cover the whole area (Aliev et al., 1978; Gubareva, 2003; Muslimov, 2008).

The Devonian sediment accumulation occurred in an equatorial marine basin located on the passive margin of the East European Platform. This passive margin constituted a wide (500–1000 km in cross-section) continental shelf, gently dipping towards the continental slope's bend and exchanging water with the Ural Palaeoocean (Figure 1). The complicated geomorphology of the basin floor facilitated sometimes subsequent but more often simultaneous accumulation of clastic, carbonate, and organic-rich black shale sediments.

During the Late Devonian (Frasnian), some island arcs of the Ural Palaeoocean accreted to the eastern margin of Laurussia, leading to a decrease of the ocean size. This collision between the island arcs and the continental margin resulted in the fracturing of the East European Platform's basement, giving rise to a complex network of broad sags (or basinal low-plains) and narrow depressions across the shelf. This network, now known as the Kama-Kinel depression system, significantly influenced the basin's architecture (Figure 2). The basinal low-plains and depressions separated areas of shallow-water environments from each other. The gentle and steep slopes of depressions were conducive to the formation of biohermal reef-like carbonates.

In the central part of the Volga-Urals petroleum province, the Devonian system forms the basal layers of the sedimentary cover, lying unconformably atop either the Riphean-Vendian rocks of the avlacogenes or the platform's crystalline basement. The oldest strata of the Devonian succession, distributed in the east and southwest of the province, consist of variegated sandstones, mudstones, and siltstones, with occasional interbeds of dolomites and limestones. Palynological data have determined the Early Devonian (Emsian) age of these rocks.

The Eifelian sequence, developed in depressions or basinal low-plains, features alternating layers of carbonate and black shale sediments, with an overall thickness ranging from 130 to 175 meters. The carbonate strata consist of dark grey and black, clayey, bituminous limestones, enriched with fossils such as corals, ostracods, brachiopods, tentaculitids, and bivalves. The accompanying black shale layers encompass clayey shales, mudstones, and calcareous mudstones. On the depression slopes, the Eifelian deposits are characterized by intercalated clastic, carbonate, and black shale sediments, with a reduced total thickness of 50 to 125 meters. In the shallow water settings of tectonic arches, the Eifelian deposits are sporadically distributed and exclusively clastic, comprising sandy-clayey rocks with abundant charred plant remains, and exhibit a thickness of 2 to 45 meters.

The Givetian deposits, formed within depressions or basinal low-plains, are predominantly composed of dark coloured carbonate-clayey rocks, namely limestones and mudstones, with a total thickness reaching up to 1000 metres. The upper part of the Stage, the Pashyian and the lower part of the Timanian, consists mainly of clastic sediments, specifically siltstones and silty mudstones, interspersed with occasional limestone interbeds. The limestones contain organic remnants, including ostracods, brachiopods and crinoids, with a less frequent presence of corals and trilobites.

On the slopes of depressions, the Givetian deposits, up to 350 metres thick, are composed of clastic sediments with intervals of black shales, sandstones, siltstones, and mudstones enriched with siderite, pyrite, charred plant detritus, and spores. Carbonate interbeds contain crinoids, brachiopods, and ostracods. In shallow water environments, where the total thickness does not exceed 170 metres, the Givetian also consists of clastic sediments, including sandstones with interlayers of siltstones and mudstones. The mudstone interbeds contain lingulids, scolecodonts, fish scales, and plant detritus.

The Fransian deposits are widespread in the studied area. The lower part of the sequence (upper Timanian) is composed of interbedded clastic and carbonate rocks, while the overlying part of the sequence is composed of carbonate and black shale sediments.

In both condensed and non-condensed depressions, the geological section initiates with upper Timanian carbonate rocks, which are overlaid by black shales. The latter consist of bituminous or clay-siliceous carbonate shales with silicite interbeds, exhibiting a relict radiolarian structure. In non-condensed depressions, the thickness reaches up to 250 metres, whereas in the condensed depressions of the southeast of the province it increases to 1100 metres. The encountered fauna comprises sponge spicules, tentaculitids, lingulids, Buchiola bivalves, and algal fragments. Additionally, the rocks feature sapropelite interlayers with an organic carbon content of up to 30% (Fortunatova et al., 2018).

On the slopes of depressions, the Frasnian geological section primarily consists of carbonate sediments, including bioclastic limestones interspersed with marls, dolomites, and mudstones, hosting brachiopods and crinoids (with a total thickness of up to 650 metres). In the middle part of the section (Sargaevian), the slopes feature an intercalation of bioclastic carbonate sediments and black shales, characterized by dark coloured bituminous limestones, marls, mudstones, and shales. The bituminous rocks predominantly contain fauna typical of black shales, while the organogenic limestones are marked by stromatopores, ostracods, tentaculitids, and brachiopods. The upper part of the section comprises light coloured organogenic and bioclastic limestones, enriched with corals, foraminifers, brachiopods, and ostracods.

Shallow-water sediments of the Frasnian stage, with a total thickness ranging from 60 to 300 metres, are predominantly found outside the Kama-Kinel trough system and its slopes. These sediments are transgressively deposited over the underlying strata, characterized by a minimal thickness and often a mottled colouration, with an increased presence of sandy material in the lower part of the sequence. In shallow-water settings, the upper half of the Frasnian sedimentary sequence is typically composed of limestones, which frequently undergo dolomitisation.

Famennian deposits in non-condensed depressions, with a thickness of 50 to 70 metres, comprise black shale sediments. These sediments include interlayers of dark grey and black, thinly laminated, bituminous, and silicified limestones, interspersed with marls and mudstones. Fossils include foraminifers, sponge spicules, ostracods, and brachiopods. On the depression slopes, where deposits reach a thickness of 200 to 500 metres, carbonate sediments predominate. These sediments include clayey and organogenic limestones, occasionally with dark grey bituminous intervals and dolomite interlayers. The associated fauna is diverse, encompassing foraminifers, ostracods, serpulids, brachiopods, gastropods, bivalves, bryozoans, crinoids, and charred plant detritus. In the shallow water environments of tectonic arches, particularly the South Tatar arch, Famennian sediments, which are 200 to 350 metres thick, are widespread. These sediments consist of grey to light-grey irregularly dolomitised, sometimes silicified, organogenic-detrital limestones with thin clay interlayers and limestone breccia at the base.

3. Materials and Methods

The results and discussion in this paper are based on data from the study of sedimentological, faunistic, and ichnological characteristics of the Devonian sediments. These sediments were accessed through more than 60 wells across various locations in the central part of the Volga-Ural province. The total thickness of the core intervals studied exceeds 600 metres. Some of the findings, particularly on the clastic interval of the Givetian, which include detailed well logs, rock descriptions, and ichnofossil illustrations have been published recently (Silantiev et al., 2022; Miftakhutdinova, 2023). In-depth analysis of the well cores was conducted directly at the core storage facility, where highly representative rock samples were selected for closer examination. These samples were polished and scanned to provide a detailed study of sedimentological and ichnological features. The collection of core samples is housed at the Geological Museum of Kazan Federal University, under collection number 44.

Sedimentological analysis aimed to reconstruct the environments in which the sediments were formed, utilising the sedimentological characteristics of the rocks and their variations across the section. Detailed examinations of the core layers, conducted at the core storage facility with precision up to 1 cm, covered lithology, colour, lamination patterns, sediment sorting, and the nature of rhythmic interbedding, including boundaries with adjacent layers. The assessment also focused on the burial and preservation of faunal remains, identification of biogenic structures disrupting rock laminations, and observation of any secondary changes in the rocks.

Ichnofacies analysis entailed the identification and taxonomic classification of trace fossils indicative of organism activity in the rocks, determining ichnotaxa combinations within assemblages, and categorising these ichnoassemblages into specific ichnofacies.

Ichnofabric analysis was utilised to assess bioturbation intensity – quantifying the disruption in the rock's primary lamination due to living organisms' activity on the sediment. This reworking intensity was evaluated using a qualitative Ichnofabric Index scale, as devised by M. Droser and D. Bottjer (1986).

Biofacies analysis involved estimating the relative oxygen content and hydrodynamic conditions, based on the interplay between fossils and their surrounding rocks. This approach integrated findings from sedimentological, paleontological, ichnofacial, and ichnofabric analyses to offer a comprehensive environmental interpretation.

The assessment of oxygen levels in palaeoenvironments utilised a range of indicators, including the nature of textures and ichnotextures (highlighting the intensity of bioturbation), the presence of biota (especially groups differing in their resistance to oxygen reduction), and, when available, specific geochemical criteria such as the ratio of organic carbon to sulphur, sulphur isotopes, and trace element concentrations.

The evaluation of oxygen levels in organic-rich black shale sediments was conducted using the oxygen-restricted biofacies (ORB) determination method, as outlined by Wignall, Hallam (1991), Wignall (1994), and Flugel (2010). This method relies on assessing the abundance of fossil species, lamination, and ichnofabric in the rocks, offering insights into the sedimentary environment's oxygenation.

The interpretation of hydrodynamic conditions was based on an analysis of lithological, sedimentological, and palaeontological characteristics, including the identification of lithotypes of rocks, examination of lamination patterns, evaluation sediment sorting, understanding the burial nature of benthic fauna, studying ichnofossil assemblages, and determining the character and intensity of bioturbation.

Biostratigraphic and biofacial analyses of the fossils were conducted based on data presented in comprehensive publications (Aliev et al., 1978; Gubareva, 2003; Fortunatova et al., 2018 and others). These data were correlated with regional conodont zones of the Volga-Ural province, established for different facial settings (Aristov, 1988; Ovnatanova and Kononova, 2008; Nazarova and Kononova, 2015, 2020), representing the most reliable stratigraphic framework for Devonian of studied area. Regional conodont zones were compared with standard (Ziegler, 1962, 1969, 1971; Ziegler, Sandberg, 1984; 1990; Sandberg, Ziegler, 1996) and global conodont zones (Becker et al., 2020). This comparison served as the basis for correlating Regional stages of the Volga-Ural province with the contemporary Chronostratigraphic Chart.

The sedimentation rates were assessed by adopting the minimal accumulation rates observed in contemporary environments for both clastic and carbonate sedimentation processes. The rate for clastic sedimentation was established at 0.2 mm/year, corresponding to the minimal rate identified in the Gulf of Maine along the North American Atlantic coastline (Kukal, 1971). With such a rate and assuming continuous sedimentation, a minimum of 200 metres of sediment would accumulate over one million years. The rate for carbonate sedimentation was determined to be 0.03 mm/year, reflecting the minimal rate of carbonate mud accumulation recorded in the modern Gulf of Mexico and Caribbean Sea (Emiliani, 1966). At this rate, approximately 30 metres of sediment would accumulate over one million years with ongoing sedimentation. For organic-rich black shale sediments, the rate was set at 0.1 mm/year (or 10 cm/1000 years), aligning with the rate for modern sapropelic sediment accumulation in the Black Sea, as determined using 14C radioisotope datings (Staffers et al., 1978). At this rate, 100 metres of sediment would accumulate over one million years, excluding sediment compaction effects.

The assessment of the sediment compaction ratio was conducted based on an analysis of literary and empirical data. The compaction ratio for clastic and carbonate sediments, which can reach values of 1:2 (Shinn, Robbin, 1983; Croizé et al., 2013), was not considered in this work, specifically in the compiling of Figure 4, was not taken into account, because of the great variety of limestones presented in the succession and, apparently, possessing different compaction capacity. Quantitative data on the compaction of ancient organic-rich sediments have not yet to be found. Most studies indicate significant compaction ratio (at least 1:4) (Littke and Zieger, 2020).

Observations on the compaction of modern organic-rich sediments indicate that compaction occurs very rapidly (within the first 100–500 years after deposition) and under minimal pressures from overlying sediments (3–10 metres); compaction intensifies with an increase in organic matter content. For instance, organic-rich sediments (≥5% organic matter) in the Mississippi Delta, situated at depths of around 10 metres, have already experienced a fourfold compaction (Keogh et al., 2021). The compaction ratio calculated for modern sapropelic sediments in the Black Sea is 1:6 (i.e., 1 metre of primary sediment compacts to a 16.7 cm layer) (Staffers et al., 1978). It is noteworthy that these findings pertain to modern sediments that have not undergone diagenesis, a process that would further increase the degree of compaction in rocks.

The data on the compaction ratio of peat, an organic sediment from continental settings, exhibit a wide range of values. During the transformation of peat into coal, the compaction ratio can vary from 1:3 to 1:60 (Winston, 1986), indicating that the thickness of the primary sediment, composed of organic matter and water, can be reduced by 3 to 60 times. In the latter case, from 1 metre of primary peat, only a 1.67 cm thick coal seam would be preserved in the geological record. For this article, a compaction ratio of 1:10 is adopted for organic-rich black shale sediments, meaning for every metre of primary sediment, an average of 10 cm of preserved rock remains.

4. Results

4.1. Regional Conodont Zonation as Evidence of Stratigraphic Completeness of the Devonian Succession

The stratigraphic completeness of the Devonian succession in the central part of the Volga-Urals petroleum province is substantiated by the continuous conodont zonation traced from the lockelianus Zone of the Eifelian to the Devonian-Carboniferous boundary (Figure 3).

The Eifelian and Givetian conodont zonation is most comprehensively developed in the Voronezh Anteclise, located in the south-western part of the province. The initial conodont zonal schemes (Aristov, 1985) and the taxonomic composition of the conodont assemblages have been significantly refined in recent years (Kononova, Kim, 2005; Nazarova, Kononova, 2016, 2020). These updated schemes are applied to the central part of the Volga-Ural petroleum province (Figure 3), where Eifelian deposits are unevenly distributed and infrequently penetrated by wells. According to conodont zonation, the Mosolovian and Chernoyarian Regional Stages correspond to the interval of the kockelianus, eiflius, and ensensis Zones of the Global Scale, which matches the upper part of the Eifelian (Figure x3). The Vorobyovian and Ardatovian Regional Stages are correlated with the hemiansatus, timorensis, rhenanus-varcus Zones of the Global Scale, indicative of the lower and middle parts of the Givetian. The Mullinian, Pashyian and lower Timanian

Regional Stages, predominantly represented by clastic sediments, poses a challenge for correlation with the Global Scale due to the absence of representative conodont assemblages. The duration of this interval is estimated at approximately 3 Ma and can be correlated with the interval of conodont zonation from the ansatus Zone to the dengleri Zone, representing the upper Givetian in the International Chronostratigraphic Chart (Becker et al., 2020).

The Frasnian conodont zonation of the Volga-Ural petroleum province was elaborated separately for shallow-water and open, deeper-water settings (Khalymbadzha, Chernysheva? 1969a,b; Khalymbadzha, 1982, 2001; Ovnatanova and Kononova, 2008) (Figure 3). Conodont assemblages include species used in modern global zonation (Becker et al., 2020), which makes the comparison more reliable. Notably, species like Ancyrodella pristina Khalymbadzha and Chernysheva, 1970, pivotal for identifying the lowest Frasnian global zone, was originally established in the central part of the Volga-Ural province (Khalymbadzha and Chernysheva, 1970).

The Famennian zonation within the province aligns with the accepted Standard conodont zonation (Ziegler and Sandberg, 1984, 1990) and continues to be applied both in the central areas of the Volga-Ural province and in North-eastern European Russia (Ovnatanova et al., 2017).

In summary, almost all conodont zones (or their analogues) from the Standard (Ziegler, 1962a, 1969, 1971; Ziegler and Sandberg, 1984, 1990) and Global conodont zonations (Becker et al., 2020) have been identified in the Devonian of the central part of the Volga-Ural province. Correlation of Regional Stages with conodont zonation, and the latter with the International Chronostratigraphic Chart, enables estimate of the duration and sediment accumulation rate of distinct stratigraphic units in different depositional environments (Figure 3 and Figure 4).

Figure 3. Middle and Late Devonian conodont zonations: Global, Standard or classical, and regional for the east of the East European Platform. Conodont zonations, denoted with numbers (1) to (5), have been compiled from following sources: (1) Ovnatanova and Kononova, 2008; (2) Sandberg and Ziegler, 1996; (3) Wittekindt, 1966; Bultynck, 1975; (4) Aristov, 1988; (5) Nazarova and Kononova, 2016, 2020. Regional Stages are given according to (Decision…, 1990; Fortunatova et al., 2018); red font indicates global or standard conodont zones traceable in the central part of the Volga-Ural petroleum Province.

Figure 3. Middle and Late Devonian conodont zonations: Global, Standard or classical, and regional for the east of the East European Platform. Conodont zonations, denoted with numbers (1) to (5), have been compiled from following sources: (1) Ovnatanova and Kononova, 2008; (2) Sandberg and Ziegler, 1996; (3) Wittekindt, 1966; Bultynck, 1975; (4) Aristov, 1988; (5) Nazarova and Kononova, 2016, 2020. Regional Stages are given according to (Decision…, 1990; Fortunatova et al., 2018); red font indicates global or standard conodont zones traceable in the central part of the Volga-Ural petroleum Province.

Figure 4. Main types of Devonian sedimentation (clastic, carbonate and black shale) and duration of sediment accumulation in the predominant environments of the Volga-Ural petroleum province, compared with global sequence of events and sea level history (highlighting major transgression/regression cycles). The data on sedimentation are updated from Kabanov and Jiang, 2020; Kabanov et al., 2023 a, b; while the global events and sea level history compiled from Becker et al., 2020 (GTS 2020). Thickness indications: black font in parentheses – condensed and uncondensed depressions; blue font in oblique brackets – slopes of depressions; brown font – shallow waters (tectonic arches).

Figure 4. Main types of Devonian sedimentation (clastic, carbonate and black shale) and duration of sediment accumulation in the predominant environments of the Volga-Ural petroleum province, compared with global sequence of events and sea level history (highlighting major transgression/regression cycles). The data on sedimentation are updated from Kabanov and Jiang, 2020; Kabanov et al., 2023 a, b; while the global events and sea level history compiled from Becker et al., 2020 (GTS 2020). Thickness indications: black font in parentheses – condensed and uncondensed depressions; blue font in oblique brackets – slopes of depressions; brown font – shallow waters (tectonic arches).

4.2. Main Sedimentation Types and Their Distribution Patterns

In the central part of the Volga-Ural province, the Devonian sequences display considerable variation in sediment composition, faunal assemblages, thickness, and completeness. Based on these features, three predominant sedimentary types can be identified: clastic, carbonate, and black shale (Figure 4). The first two types have contributed to the deposition of carbonate and clastic reservoirs. The third type, which is characterised by a high content of organic matter, is traditionally considered a source rock.

Classic sediments are distributed from the Middle Devonian (Emsian) to the early Frasnian and are represented by well-sorted sandstones and siltstones interbedded with mudstones. The thicknesses range from the first hundreds of metres in depressions (and basinal low-plains) to the first tens of metres in uplifted areas of the seabed (including tectonic arches) representing shallow water environments. Marine fossils are rare; meanwhile, a diverse assemblage of ichnofossils including Chondrites, Spirophyton, Scolicia, Planolites, Palaeophycus, Zoophycos and Skolithos indicates the marine origin of these sediments (Silantiev et al., 2022, Miftakhutdinova, 2023). The Paschyian Regional Stage represents the time during which clastic sedimentation completely covered the entire studied area, displacing all other types of sedimentation.

Carbonate shallow-water oxic sediments include isolated carbonate buildups (reefs, banks and broader platforms) and off-reef carbonate and mud covers. Isolated carbonate buildups (up to 600 m thick) consist of biogenic limestones, oolitic, microbial, containing a relatively rich assemblage of fossils: calcareous algae, foraminifers, stromatopores, corals, crinoids, and conodonts. Sediments of this type were formed predominantly along the slopes of intrashelf trough net of the Kama-Kinel system (Figure x2). Off-reef carbonate and mud covers are composed of bioturbated limestones and mudstones with a diverse benthic fauna and average values of sediment thickness. In some cases, stratigraphic incompleteness and breaks in sedimentation are observed.

The Eifelian and Givetian accumulation of carbonate sediments occurred predominantly in depressions, on their slopes, and in basinal low-plains, where this type of sedimentation frequently coincided with the accumulation of deep-water organic rich black shales. This is recorded in the geological succession by the alternation of carbonate and black shale facies (Figure 4). At the end of the Givetian (Pashyian Regional Stage), carbonate sedimentation in the studied area completely terminated. Steady accumulation of carbonate sediments was recovered and stabilised in the studied area in the early Frasnian and continued until the global regression in the Early Visean (Silantiev et al., 2023). Transgression in the Early Frasnian for the first time extended carbonate sedimentation to shallow water environments located on tectonic arches.

In shallow water environments, carbonate sedimentation was often interrupted, resulting in the erosion of already accumulated sediments. In particular, calculations for the Frasnian indicate that carbonate sediments deposited in shallow water environments represent less than 60% of the duration of this time interval, while most of the geological time corresponds to discontinuities in sedimentation. The Famennian is characterised by the most stable carbonate sedimentation, distributed both on the slopes of depressions and on shallow water environments of tectonic arches, the differences between which are gradually erasing (Figure 4).

Black shale sediments, believed to have originated in photic-zone euxinic conditions (Kabanov et al. 2023a, b), consist of dark-coloured carbonate-clay or siliceous-clay-carbonate rocks with a high organic matter content. When these sediments have a considerable thickness (several hundred metres), they are usually interpreted as having been accumulated in non-condensed (compensated) depressions. In contrast, when the thickness is relatively minimal (several tens of metres), they are thought to have been deposited in condensed (uncompensated) depressions.

Black shale sediments are characterised by a low diversity of benthic fauna, represented by a few species of ostracods from the family Entomozoidae, a single species of bivalves, and both inarticulated and articulated brachiopods. In contrast, the diversity of planktonic and nektonic organisms is increasing. The plankton is represented by numerous radiolarians, pteropods, and tentaculitids (predominantly dacryoconarids), while the remains of actively swimming nektonic organisms are represented by trilobites, scolecodonts, cephalopods, conodonts, and fish.

The sedimentation of black shales began in the central part of the Volga-Ural province in the late Eifelian. Sediments of this type were accumulated predominantly in depressions or basinal low-plains and, as mentioned above, were adjacent to carbonate sediments. At the end of the Givetian (Pashyian Regional Stage) black shale sedimentation, as well as carbonate sedimentation, completely ceased in the studied area.

Reactivation of black shale sedimentation commenced in the Early Frasnian. From this period, the steady accumulation of black shales enveloped the axial zones of the Kama-Kinel trough system, persisting almost without interruption until the onset of the Carboniferous (Mississippian, Tournai). The most widespread and well-known black shales were accumulated during the Middle Frasnian (Semilukian). In the literature by Russian geologists, Middle Frasnian black shales are referred to as "Domanic sediments" or "Domanic facies", names derived from the Domanic Formation and Domanic River of Pechora Basin (Strakhov, 1938). The Middle Devonian-Mississippian organic-rich black shales located above and below the Middle Frasnian are designated as "domanikoids" or "domanikites" (Figure 4).

4.3. Rate and Duration of Sediment Accumulation

The Chronostratigraphic chart of the Middle and Upper Devonian, which includes global, standard, and regional conodont zonations (Figure 3), estimates that the Devonian strata deposited in the central part of the Volga-Ural region accumulated over a period of 35 million years, from the late Emsian to the late Famennian.

Section 3, Materials and Methods, provides an explanation of the sedimentation rates and compaction ratio used in this paper. The clastic sedimentation rate is assumed to be 0.2 mm/yr (1 Ma = 200 m of sediment), the carbonate sedimentation rate is assumed to be 0.03 mm/yr (1 Ma = 30 m of sediment), and the accumulation rate of organic-rich black shales is assumed to be 0.1 mm/yr (1 Ma = 100 m of sediment). The compaction ratio of 1:10 (i.e. 1 metre of primary sediment compacted to 10 cm of rock) was only considered for organic-rich black shale sediments.

Figure 4, specifically its "Main types of environments" column, shows the duration of accumulation of different sediment types (clastic, carbonate, black shale) in various sedimentary environments for each Regional Stage. The duration of accumulation is expressed through the vertical size of the symbols corresponding to each sediment type. The vertical size is calculated based on actual sediment thickness and assumed accumulation rates.

Below is an example of this column for organic rich black shale sediments that accumulated in non-condensed depressions during the Semilukovian Regional Stage (Middle Frasnian) (Figure 4). The Semilukovian in these sections averages 30 m. The compaction ratio of 1:10, which we adopted for black shales, increases this value by 10 times, i.e. up to 300 m of primary sapropelic sediment. The estimated duration for the accumulation of 300 metres of primary sapropelic sediment at an assumed rate of 0.1 mm/year (1 million years = 100 m) is 3 million years. Therefore, the vertical size of the icon in the column 'Main Types of Environments' indicating the accumulation of 30 metres of Semilukovian black shales (already compacted) corresponds to 3 Ma on the Chronostratigraphic Chart. Therefore, it appears that during the 3 Ma of the Semilukovian regional stage, there was a continuous accumulation of Semilukovian black shales in non-condensed depressions in the studied area.

Below we present a summary of our analysis regarding the duration of sediment accumulation across various sediment types.

The clastic sediments, which have the highest accumulation rate, are characterised by the maximum discontinuity and irregularity in the chronostratigraphic record (Figure 4). Despite of the total duration of clastic sedimentation in the studied area of 16 Ma, the duration of accumulation of individual intervals (or geological bodies) of clastic sediments varies from 100 Ka in shallow water environments to 1 Ma in depressions. In all cases, both in shallow water and in depressions, the accumulations of clastic sediments appear to be discrete events separated from each other by discontinuities. In the works of many researchers, the origin of clastic sediments was associated with continental alluvial processes (Danilova, 2008; Loscheva et al., 2017). Meanwhile, recent studies (Silantiev et al., 2022, Miftakhutdinova, 2023) have confirmed the marine origin of these sediments and linked them to transgressive episodes of the Devonian marine basin.

Carbonate sedimentation in the studied area extended over approximately 36 million years, from the Late Emsian to the Late Famennian. Before the Frasnian, periods of carbonate sedimentation were relatively brief, not exceeding 1 Ma, and were often interrupted by shorter episodes (200–300 Ka) of organic-rich black shale accumulation. A notable shift to prolonged and stable carbonate sedimentation commenced in the early Frasnian, initially affecting the slopes of depressions for up to 5 Ma. Subsequently, this sedimentation process expanded into the shallow water environments of tectonic arcs, lasting for up to 12 Ma during the Famennian.

Black shales accumulated in the studied area for about 29 Ma – from the Late Eifelian (Mosolovian Regional Stage) until the end of the Famennian (Figure 4). During the Eifelian and Givetian, the accumulation of black shales represented short (200–300 Ka) episodes alternating with episodes of carbonate sedimentation, and was confined to depressions, their slopes, and basinal low-plains (see e.g., Mosolovian).

During the Late Eifelian, Givetian and Early Frasnian, the accumulation of certain black shale intervals correlates well with the Devonian global anoxic events (Gradstein et al., 2020). For example, the accumulation of Chernoyarian black shales correlates with the Late Eifelian Kacak event, the accumulation of Mullinian black shales can be linked to the Givetian Taghanic event, and a short episode of black shale accumulation in the Timanian (Early Frasnian) is associated with the Frasnes event (Figure 4). The last two episodes of black shale accumulation are noteworthy for two reasons: (1) they are recorded not only in depressions, but also on their slopes, in shallower settings; (2) intervals of black shale accumulation are spatially closer to clastic sediments rather than carbonate ones, as observed in the Eifelian and Upper Devonian. It should be noted that the above observations require further confirmation based on the biostratigraphy and radioisotopic dating. In the middle-late Frasnian and Famennian, such comparisons are obscured.

Prolonged and stable sedimentation of black shales has been observed since the early Frasnian, with the formation of the Kama-Kinel trough system. Since that time, the sedimentation of black shales has occupied the deepest (axial) settings of depressions and no longer formed frequent alternations with carbonate sedimentation, which has spread to the slopes of depressions and shallow-water environments.

4.4. Accumulation of Sediments in Different Environments

During the Middle and Late Devonian periods, the central part of the Volga-Ural province included three predominant types of environments: (1) non-condensed depressions, (2) slopes of depressions, and (3) shallow waters of tectonic arches. These environments were filled with various types of sediments at different intervals throughout the Devonian history.

Condensed and non-condensed depressions contain the most complete sequences of sediments. In the Eifelian, these sequences are represented by alternating carbonate and black shale sediments; in the Givetian, thick layers of clastic rocks are added to them. In the Late Devonian, and more specifically from the beginning of the Middle Frasnian, these deep-water environments were occupied by the accumulation of organic-rich black shale sediments. Some regional hiatuses recorded in the sequences of depressions correspond well to global regressive events, particularly at the Eifelian-Givetian boundary, in the late Givetian (at the base of the Mullinian), and at the Frasnian-Famennian boundary (Figure 4).

Slopes of depressions throughout the Eifelian and Givetian represented environments in which sediments of all three main types were accumulated: clastic, carbonate and black shale. On the one hand, this may indicate the complex geomorphological surface of the slopes, and on the other hand, it may indicate the conventional nature of the designation of this type of settings (indirect confirmation of the latter assumption is provided by the close values of thicknesses of slope and shallow facies). Only since the Frasnian, the slopes of depressions have become well separated from other environments, which is emphasised by the predominance of carbonate sedimentation on them.

Shallow waters of tectonic arches are distinguished from other environments by the maximum incompleteness of the geological record. During the Middle Devonian, these environments were the scene of short-term (100 Ka) transgressive episodes of clastic sedimentation (Figure 4). It should be noted, that in Figure 4, each stratigraphic subdivision (Regional Stage) corresponds to only one episode of clastic accumulation; however, in reality, there may be multiple such episodes. Secondly, the position of these episodes on the chronostratigraphic scale is shown only conditionally. At present, we lack the tools to solve these problems: to determine the number of episodes of clastic sediment accumulation and their precise ages. Therefore, all correlations involving clastic intervals of the succession are approximate.

5. Discussion

Fortunatova et al. (2016, 2018) considered the Upper Devonian sequences of the Volga-Urals Petroleum Province and provided a regional conodont zonation for the Fransian and Famennian according to Ovnatanova and Kononova (2008), comparing it with the standard conodont zonation according to Gradstein (2004). We have used this comparison in this paper, extending the zonation to the Middle Devonian and adding a modern chronostratigraphic framework (Becker et al., 2020), which enables to estimate the duration of conodont zones and regional stages.

The designation of three predominant types of environments in the Middle-Late Devonian basin of the central part of the Volga-Urals Province: (1) condensed and non-condensed depressions, (2) slopes of depressions, and (3) shallow waters of tectonic arches (Aliev et al., 1978; Mkrtchyan, 1980) is supported by most contemporary researchers (Gatovsky et al., 2015; Fortunatova et al., 2016, 2018; Liang et al. 2015, 2020; Stupakova et al., 2015, 2017; Kabanov and Jiang, 2020; Kabanov et al., 2023a, b).

Many of the cited works consider essentially the Upper Devonian, i.e. the interval of the territory's evolution when the Kama-Kinel trough system was already formed, which intensified the difference in sedimentary settings (Figure 2). In this regard, most of the researches (Fortunatova et al., 2016, 2018; Liang et al. 2015, 2020; Stupakova et al., 2015, 2017; Kabanov and Jiang, 2020; Kabanov et al., 2023a, b) limit the time of black shale sedimentation to the interval from the Middle Frasnian of the Late Devonian to the Tournaisian of the Early Carboniferous (Mississippian). In this paper, we point out that these sediments, which are considered as source rocks, were formed in the studied area in both the Late and Middle Devonian. Particularly, in the Middle Devonian, they were accumulated for at least 8 Ma and could have been deposited both in the axial zones of the depressions and on their slopes (Figure 4).

Gorozhanina et al. (2019) suggest that the present narrow configuration of depressions in the Kama-Kinel trough system bounding the uplifted areas of tectonic arches appeared after the accumulation of the Devonian sediments and is related to tectonic (and neotectonic) movements. These authors consider the Late Devonian sedimentary setting as an extensive basinal low-plain with gentle shelf including shallow settings (about 20-50 m deep), deep settings (50-100 m deep), and depression settings (100-150 m deep). Our Middle Devonian data generally support this view, indicating that the accumulation of the main different types of sediments at that time occurred in approximately the same (or close) settings of the basin (see, e.g., Mosolovian, Vorobyovian, Mullinian, Figure 4).

Below we briefly discuss some contradictions in the views on the accumulation settings of the Devonian black shale sediments. For example, Stupakova et al. (2015, 2017; Karpushin, Stupakova et al., 2022) suggest that the accumulation of the Devonian organic-rich black shale sediments took place in relatively deep-water environments (100–300 m depth) predominantly under normal gas regime conditions. The absence of sulphide contamination of bottom waters is justified by these authors by the wide distribution of sessile benthic invertebrates (bivalves, articulated brachiopods) and nektonic cephalopods (goniatites) sensitive to oxygen deficiency. Simultaneously, the same authors point out that geochemical data indicate periodic episodes of hydrogen sulphide contamination, as derivatives of isorenieratene, a biomarker of sulphide contamination of the photic layer, were found in a number of samples (Stupakova et al., 2017).

A similar opinion is expressed in a recent study by Liang et al. (2020), which defines the depositional environment of black shales as "the basin with normal salinity, normal oxygen regime and a depth of about 100 m..." (Liang et al., 2020, p. 8). Interestingly, in a previous paper by the same first author (Liang et al., 2015, p. 54), the Devonian organic-rich sediment accumulation setting was associated with a stagnant hydrodynamic regime and hydrogen sulphide contamination of bottom waters.

Many authors attribute the formation of sediments enriched in organic matter to the maximum level of basin flooding; and the formation of carbonate sediments, on the contrary, to basin regression (Stupakova et al., 2017; Chupakhina et al., 2022; Karpushin, Stupakova et al., 2022; Zavyalova, Karpushin, and Stupakova, 2023).

Gatovsky et al. (2015) considering Middle Frasnian organic rich black shales noted that these sediments are oversaturated with organic matter, and this circumstance could be the reason for the complete absence of the oxidative zone of diagenesis and the development of benthic anoxic conditions. The authors attribute the accumulation of organic rich sediments to the periods of high planktonic bioproductivity, which resulted in the accumulation of thin interlayers of horizontally laminated sapropelic muds. Note that Wignall (1994) discusses the absence of true horizontal lamination in organic-rich sediments in detail. In turn, we note that the thickness of the primary Devonian sapropelic sediments could exceed hundreds of metres. The thickness of the first few tens of metres now documented in the geological record is the result of compaction of the primary sediment and an average tenfold reduction in its thickness.

In this paper, we accept the viewpoint of P. Kabanov et al. (Kabanov, Jiang, 2020; Kabanov et al., 2023a, b), who attributed the origin of organic-rich sediments to photic-zone euxinic conditions in the Devonian "greenhouse" shelf seas. Kabanov et al (2023a, b) hypothesised that variations in the concentration of hydrogen sulphide in the water column significantly impacted the facies structure of carbonate platforms and inter-platform anoxic troughs (Kabanov et al 2023a). They identified slowed water circulation, euxinic upwelling, and increased eutrophication from rising river runoff as the main factors forming the stratified water column with a fluctuating chemocline (oxic-anoxic water layer boundary).

Photic zone euxinia means that the water in the photic zone (the upper layer of the basin where light sufficient for photosynthesis penetrates) is oxygen-deficient or completely oxygen-free, but at the same time saturated with hydrogen sulphide (H₂S). Under normal conditions, the photic zone is oxygenated (~5 to ~14 mg/l depending on temperature, salinity and pressure) due to the photosynthetic activity of phytoplankton, which use sunlight to produce oxygen. However, under euxinic conditions, even in this illuminated zone, anoxic (oxygen-deficient or oxygen-free) conditions prevail, resulting in the accumulation of hydrogen sulphide. This situation may result from an excessive input of organic matter, consuming substantial oxygen during accumulation, or from slowed water circulation, preventing oxygen influx from other water layers. Euxinic conditions in the photic zone seriously affect the ecosystem, as most photosynthetic organisms and many other marine animals cannot survive in anoxic and hydrogen sulphide conditions. Such conditions transform the structure of the marine ecosystem, resulting in diminished biodiversity and altered food chains. Evidently, these are the alterations observed in Devonian organic-rich black shales.

Kabanov et al. (2023a, b) emphasised that the extensive zones of minimal oxygen content in the Devonian 'greenhouse' ocean supported stratification (layering) of the water column of shelf seas, i.e. conditions in which heavier, salty and oxygen-poor water remained at depth, whereas lighter and oxygen-rich water stayed at the surface; stratification prevented mixing of water layers and oxygen exchange. This circumstance explains the formation of thick anoxic (oxygen-poor) sediments in oceanographically open conditions, especially in the basin of the Volga-Urals Province, which was open to the Ural Palaeoocean.

The shallowness of hydrogen sulphide episodes in the water column is confirmed by the wide distribution of Chlorobi biomarkers in Devonian organic-rich sediments (Kabanov et al., 2023a, b). Chlorobi biomarkers represent a group of photosynthetic bacteria that inhabit the photic zone but perform photosynthesis under anoxic (oxygen-free) conditions, using sulfide as an electron donor instead of water. The presence of Chlorobi biomarkers in the Devonian organic-rich sediments suggests that hydrogen sulphide episodes were not restricted to deep waters, but also occurred at relatively shallow depths.

The shallow water chemocline in the extended oxygen minimum zone fluctuated with high frequency and probably suppressed the spatial expansion of carbonate accumulation, thus controlling the distribution of shallow and deep water facies (Kabanov et al. (2023a, b). These frequent changes in conditions may have prevented the expansion of carbonate sediments such as reefs or bioherms, which normally form under more stable and predictable conditions. As a result, such variable conditions influenced the general architecture of the seafloor, forming characteristic alternations of uplifts and depressions.

In general, the hypothesis proposed by Kabanov et al. (2023a; 2023b) aligns well with models of sapropel accumulation in modern environments, particularly in the Mediterranean Sea. These models include two processes: (1) reduced or absent ventilation of the deep water due to stratification of the water column, leading to anoxic conditions at the seafloor and consequently to preservation and accumulation of organic matter; (2) enhanced primary production due to increased nutrient availability in the surface water (Emeis et al., 2000a, 2000b; Rohling, 1994; Warning and Brumsack, 2000).

The Middle Devonian clastic sediments of the central part of the Volga-Ural province attract the attention of many researchers due to their high oil and gas content (Muslimov, 2008; Danilova, 2008). There are opinions about the formation of these sediments in continental alluvial and deltaic environments (Danilova, 2008; Loscheva et al., 2017, etc.). The detailed reviews of the composition and origin of these sediments considered in recent publications have proved their marine nature (Fortunatova et al., 2013; Silantiev et al., 2022).

We adhere to the viewpoint (Silantiev et al., 2022; Miftakhutdinova, 2023) that clayey-siltstone beds were formed in the conditions of the Cruziana Ichnofacies, localised between the levels of weak and storm waves. Sandy packs could have been formed in the Skolithos Ichnofacies, represented, most often, by well-sorted sands that had been constantly moved and subjected to sudden erosion or redeposition (Mikulash and Dronov, 2006; Bromley, 1996). Accumulation of clastic sediments of both clay-siltstone and sandy types occurred during marine transgressions, whereas regression of the sea led to erosion and destruction of the already formed sediments.

Figure 2 highlights a hiatus in the accumulation of black shale and carbonate sediments in the Late Givetian (Pashyian and lower Timanian); precisely during the deposition of the best and most widespread clastic reservoirs. This hiatus requires further study and clarification. Attention should be focused on the Pashyian mudstones, which represent a marker bed in the middle of the sequence (Danilova, 2008). Recent data (Silantiev et al., 2022) indicate that these mudstones contain remains of soft-bodied fauna, impressions of conodonts and internal moulds of myospores. This fossil assemblage and its preservation indicate unusual anaerobic (<0.2 ml/l O₂, normally no O₂) or dysaerobic (1.0–0.2 ml/l O₂) conditions for the formation of these mudstones. Finds of soft tissues of lingulids favour dysaerobic conditions. Lingulid burrows of reduced length (5–10 mm instead of 50–70 mm) were also found here (Miftakhutdinova, 2023), indicating that the primary sediment was compacted.

6. Conclusions

Examining the sediment accumulation across various environments leads to the following conclusions.

1. Depressions and basinal low-plains exhibited nearly continuous accumulation of organic-rich black shales, alternating with carbonate sediments in the Eifelian and Givetian. This accumulation of source rocks spanned from the end of the Eifelian (Mosolovian; 388 Ma) to the end of the Famennian (359.3 Ma), covering approximately 29 Ma (Figure x2).

2. Environments on the slopes of depressions often experienced discontinuities in sedimentation, particularly during the Givetian. Notably, in the Eifelian (Mosolovian), Givetian (Mullinian and lower Timanian), and Lower Frasnian (Sargaevian), these settings accumulated organic-rich black shales. This might be attributed to significant organic matter formation under photic-zone euxinic conditions in basins of varying depths.

3. Shallow water environments were marked by the thinnest sediment layers and the longest sedimentation hiatuses. These hiatuses likely represent periods of prolonged sorting of sandy and silty sediments, typical of the Middle Devonian clastic reservoirs in the study area.

4. Since the beginning of the Famennian, the distinctions between the slopes of depressions and shallow water environments have diminished, indicating a restructuring of the basin floor outside the axial zones of the Kama-Kinel trough system.

5. The results imply that correlating Devonian sequences in the central part of the Volga-Ural petroleum province should consider the accumulation rates of various sediment types and the incompleteness of the geological record in different environments.