- 1Institute of Geophysics, I. Javakhishvili Tbilisi State University, Tbilisi, Georgia
- 2Department of Engineering and Geology, “G. d’Annunzio” University of Chieti-Pescara, Chieti, Italy
- 3PACE Geoscience, Chieti, Italy
- 4Institute for Geological and Geochemical Research, Research Centre for Astronomy and Earth Sciences, ELKH, Budapest, Hungary
- 5CSFK, MTA Centre of Excellence, Budapest, Hungary
- 6A. Janelidze Institute of Geology, I. Javakhishvili Tbilisi State University, Tbilisi, Georgia
- 7Faculty of Mining and Geology, Georgian Technical University, Tbilisi, Georgia
The Rioni foreland fold-and-thrust belt is part of the Greater Caucasus pro-wedge and is one of the most important examples of the collision-driven far-field deformation of the Arabia-Eurasia convergence zone. Here we show the deformation structural style of the Rioni foreland fold-and-thrust belt based on seismic reflection profiles and regional balanced cross-section. The main style of deformation within the Rioni foreland fold-and-thrust belt is represented by a set of fault-propagation folds, duplexes, and triangle zone. The regional balanced cross-section shows that fault-propagation folds above the upper detachment level can develop by piggyback and break-back thrust sequences. Formation of fault-bend fold duplex structures above the lower detachment is related to piggyback thrust sequences. A balanced section restoration of compressional structures across the Rioni foreland fold-and-thrust belt provides a minimum estimate of shortening of −40%, equivalent −42.78 km. The synclines within the Rioni foreland fold-and-thrust belt are filled by the Middle Miocene-Pleistocene shallow marine and continental syn-tectonic sediments, forming a series of typical thrust-top basins. Fault-propagation folds and duplex structures formed the main structure of the thrust-top basin. The evolution of the thrust-top basins was mainly controlled by the kinematics of thrust sequences. Using end-member modes of thrust sequences, the thrust-top basins are divided into: 1) Type I-piggyback basin, 2) Type II-break-back basin, and 3) Type III—formation of thrust-top basin characterized by bi-vergent geometry and related to combined, piggyback and piggyback back thrust sequences.
Introduction
An understanding of the structural architecture of the foreland fold-and-thrust belts is important in the application of this knowledge to the compressional deformation history of orogens. In a foreland basin system, the frontal part of the orogenic wedge sediments is deformed into a series of fault-related folds and associated thrust-top basins (e.g., DeCelles and Giles, 1996; Roure, 2008). The timing of thrust-top basins sedimentation in the foreland basin is important because it is one of the indicators for the timing of shortening, and uplift of the orogens; syn-tectonic deposition within the basin records the upward stratigraphic evolution during the deformation (e.g., Ori and Friend, 1984; Turner, 1988; Suppe et al., 1992; Butler and Grasso, 1993; DeCelles and Giles, 1996; Suriano et al., 2015; Chanvry et al., 2018; Heydarzadeh et al., 2020).
The Rioni foreland fold-and-thrust belt (RFFTB) is one of the most important examples of the collision-driven far-field deformation of the Arabia-Eurasia convergence zone (Figure 1A). The RFFTB is a part of the Greater Caucasus pro-wedge (Alania et al., 2021a) and is one of the main hydrothermal provinces of west Georgia (Melikadze et al., 2014). During the last several years the understanding of the structure and kinematic evolution of the RFFTB has changed to a great extent. These studies have investigated this region focusing on 1) the tectonic development of the RFFTB (e.g., Banks et al., 1997; Vakhania, 2008a; Vakhania, 2008b; Adamia et al., 2010; Forte et al., 2014; Cowgill et al., 2016; Tibaldi et al., 2018; Alania et al., 2021a; Trexler et al., 2022), 2) the deformation style of the RFFTB (e.g., Banks et al., 1997; Cowgill et al., 2016; Tibaldi et al., 2017a; Tibaldi et al., 2017b; Tari et al., 2018; Tibaldi et al., 2018), 3) the timing of deformation of the RFFTB (e.g., Banks et al., 1997; Cowgill et al., 2016; Tari et al., 2018; Trexler et al., 2020; Alania et al., 2021a), and 4) the active structures of the RFFTB (e.g., Tsereteli et al., 2016; Adamia et al., 2017; Tibaldi et al., 2017a; Tibaldi et al., 2017b; Tibaldi et al., 2020; Trexler et al., 2020).
FIGURE 1. (A) Tectonic map of Arabia-Eurasia collision zone (modified from Sosson et al., 2016). (B) Tectonic map of the Caucasus (modified from Sobornov, 1996; Adamia et al., 2011a; Sosson et al., 2016; Adamia et al., 2020; Alania et al., 2021a, Alania et al., 2021b; Mosar et al., 2022). Abbreviations: GC-Greater Caucasus, LC-Lesser Caucasus, RFFTB-Rioni foreland fold-and-thrust belt, RFB-Rioni foreland basin; IUZ-Imereti uplift zone; ATFTB-Achara-Trialeti fold-and-thrust belt; KFFTB-Kura foreland fold-and-thrust belt; KFB-Kura foreland basin; NCFFTB-North Caucasus foreland fold-and-thrust belt; DWFTB-Deepwater fold-and-thrust belt; KB-Kuban Basin; TB-Terek Basin; AFB-Araks foreland basin.
Although previous studies have achieved an understanding of the role of detachments in the formation of the series of fault-related folds in the thin-skinned RFFTB, they are mainly dependent on boreholes data and field outcrops studies. Therefore, the deformation structural styles of this foreland fold-and-thrust belt have still remained controversial.
The main goals of this study are 1) to determine the deformation structural style, 2) to calculate the shortening by comparing the regional balanced and restored cross-sections, and 3) to determine the types of thrust-top basins using thrust sequences models. For these purposes, regional balanced and restored cross-sections were constructed across the Rioni foreland fold-and-thrust belt, based on surface and sub-surface data (seismic profiles and well data).
Geological setting
The Rioni foreland basin system is located between the Lesser Caucasus (LC) and the Greater Caucasus (GC) orogens (Figures 1A,B, 2). Deformation of the Rioni double flexural foreland basin (Banks et al., 1997) was controlled by the action of two opposing orogenic fronts, the LC retro-wedge to the south and the GC pro-wedge to the north (Alania et al., 2021a). The tectonic evolution of LC and GC is the result of the Arabia-Eurasia collision during Alpine times, which led to the inversion of back-arc basins and the formation of two orogens with the Rioni and Kura foreland basins in between (Figure 1B) (e.g., Adamia et al., 1981; Sobornov, 1996; Banks et al., 1997; Mosar et al., 2010; Nemcok et al., 2013; Cowgill et al., 2016; Sosson et al., 2016; Tari et al., 2018; Alania et al., 2021a; Alania et al., 2021b; Alania et al., 2021c; Corrado et al., 2021; Gusmeo et al., 2021; Gusmeo et al., 2022; Tari et al., 2021; Cowgill et al., 2022; Mosar et al., 2022). The Rioni and Kura foreland basins in turn are divided from each other by the Imereti Uplift Zone (IUZ) (Figure 1B).
FIGURE 2. Geological map of RFFTB and surrounding area (modified from Janelidze and Kandelaki, 1956; Vakhania, 2008a, Vakhania, 2008b; Adamia et al., 2020). Abbreviations: RFFTB, Rioni foreland fold-and-thrust belt; SSGC, Southern Slope of Greater Caucasus; CSA, Chaladidi-Sagvamischao anticline; KVA, Kvaloni anticline; KA, Khobi anticline; SA-Senaki anticline; NOA, Nokhalakhevi anticline; TSA, Tsaishi anticline; SHA, Sashurgaio anticline; ZUA, Zugdidi anticline; STA, Satanjo anticline; SBA, Saberios anticline; SAA, Sarakoni anticline.
Foreland basin sedimentation in the Rioni Basin, as well as in the Kura foreland basin is regarded to have started during the Oligocene to Early Miocene, consistent with the onset of rapid subsidence from the south by LC and from the north by GC (Alania et al., 2017; Alania et al., 2021a). North and central parts of the Rioni foreland basin during the Middle Miocene-Pleistocene time were deformed and shortening is concentrated at the outer part of the GC pro-wedge (Alania et al., 2021a). A similar picture can be observed in the Kura foreland fold-and-thrust belt (KFFTB), where compressional deformation began in the Middle Miocene (Alania et al., 2017; Corrado et al., 2021; Gusmeo et al., 2021).
The RFFTB sedimentary infill (more than 7 km) consists of pre-and syn-orogenic sequences. The simplified geological evolution of the studied area is summarized in a tectonostratigraphic chart (Figure 3). The pre-Mesozoic basement of the RFFTB exposed in the IUZ (Figure 1B) comprises Hercynian granitic metamorphic rocks in its core, overlain by Devonian to Carboniferous phyllites (Adamia et al., 2011a). The basement of the RFFTB is in general tilting towards the north and the associated orogenic flexure of the foreland region (Banks et al., 1997). Most of the pre-Mesozoic basement is intruded by granitoid and covered with volcanogenic rocks of the Middle Jurassic age (Adamia et al., 2011a).
FIGURE 3. Tectonostratigraphic chart of the Rioni basin and surrounding area (modified from Adamia et al., 2010; Adamia et al., 2011a, Adamia et al., 2011b; Vincent et al., 2016, Tari et al., 2018; Alania et al., 2021a).
The pre-orogenic sequences consist of Jurassic-Late Eocene shallow and deep marine deposits (e.g., Tari et al., 2018). According to Vincent et al. (2016) within the GC back-arc basin are distinguished three main phases of extension: 1) the first phase started in the Sinemurian (Early Jurassic); 2) a main phase of extension took place from the Aalenian to the Bajocian (Middle Jurassic); and 3) a thermal-sagging phase from the Bathonian (Middle Jurassic) to the Eocene. The Early Jurassic sandstones and shales (about 1500 m thick) are exposed north and south of RFFTB. Middle Jurassic is represented by Bajocian debris flow deposits and turbidities with rare intercalations of calk-alkaline andesite-basalts and the Bathonian freshwater-lacustrine coal-bearing sandy-argillaceous rocks; thickness is about 2500 m. Late Jurassic is represented by evaporites, clastic rocks, and basalts (about 500 m thick). Early Cretaceous turbidities, dolomites, limestones, and marls, with conglomerates at the base, transgressively rest on Late Jurassic rocks; thickness is about 350–400 m (e.g., Adamia et al., 2011a; Adamia et al., 2011b). The Late Aptian, Albian, and Cenomanian sequence is dominated by siliciclastic rocks. Late Cretaceous, Paleocene, and Eocene deposits are mainly built up by mixed carbonate-siliciclastic-volcaniclastic rocks; their thickness in some places exceeds 2000m (e.g., Adamia et al., 2011a).
The syn-orogenic sequences are composed of the foreland basin (Oligocene-Early Miocene) and syn-tectonic strata (Alania et al., 2021a). The Oligocene-Neogene stratigraphy of the RFFTB is dominated by siliciclastic sequences. The Oligocene-Early Miocene is represented mainly by the alternation of shales and sandstones and is underlain unconformably by the marl-dominated Eocene sequence; their thickness is about 800–900 m (Mayer et al., 2018; Sachsenhofer et al., 2018; Tari et al., 2018). Syn-tectonic strata of Middle-Late Miocene, Pliocene, and Pleistocene are represented by shallow marine and continental, predominantly terrigenous clastic rocks. The thickness of the syn-tectonic strata is about 1,500–2000 m (e.g., Adamia et al., 2010; Tari et al., 2018; Alania et al., 2021a). The Holocene is represented by undifferentiated continental strata and river-bed alluvial deposits (e.g., Adamia et al., 2010).
The RFFTB underwent from the Middle Miocene—Pleistocene N- to S-directed shortening (Banks et al., 1997; Tibaldi et al., 2017a; Tibaldi et al., 2017b; Tari et al., 2018; Alania et al., 2021a). The characteristic structural styles are represented by fault-related folds detached along the basal thrust which soles within the Late Jurassic evaporates and are dominated by a thin-skinned tectonic style (Banks et al., 1997; Adamia et al., 2010; Forte et al., 2014; Cowgill et al., 2016; Adamia et al., 2017; Tibaldi et al., 2017a; Tibaldi et al., 2017b; Tari et al., 2018; Alania et al., 2021a). The RFFTB system consists of several major anticlines, which from south to north are the Chaladidi-Sagvamichao, Kvaloni, Khobi, Tsaishi, Senaki, Nokalakevi, Sashurgaio, Zugdidi, Satanjo, Saberios, and Sarakoni anticlines. South of the Tsaishi anticline, the Chaladidi-Sagvamichao, Kvaloni, and Khobi anticlines have no evident expression at the surface and it has been imaged by seismic and boreholes data (Vakhania, 2008a; Vakhania, 2008b; Tari et al., 2018). The Tsaishi anticline is the fold with the deepest level of exhumation in the study area, and as a result, the Late Cretaceous limestones crop out in its core (e.g., Banks et al., 1997; Tibaldi et al., 2017a; Tibaldi et al., 2017b; Tari et al., 2018). Curve-shaped thrusts are developed north of the frontal folds of the RFFTB (Figure 2). According to Tibaldi et al. (2018), the structural development of the arcuate thrust system within RFFTB is related to oblique, asymmetric indentation of an upper crustal block moving to the SSW.
Recent GPS and earthquake data indicate that the RFFTB is still tectonically active and the earthquakes focal mechanisms are mainly thrust faults (e.g., Adamia et al., 2004; Tsereteli et al., 2016, Adamia et al., 2017; Sokhadze et al., 2018; Tibaldi et al., 2020, Tibaldi et al., 2021).
Data and methods
The database consists of published and unpublished data as well as field observations. The surface geological information is obtained from 1:100,000 and 1:200,000 geological maps (Janelidze and Kandelaki, 1956; Adamia et al., 2020) of the study area (Figure 2) and relevant papers (Banks et al., 1997; Adamia et al., 2010; Adamia et al., 2017; Tibaldi et al., 2017a; Tibaldi et al., 2017b; Tari et al., 2018; Adamia et al., 2020; Alania et al., 2021a). Fault-related folding and wedge thrust folding theories (Medwedeff, 1990; Suppe and Medwedeff, 1990; Shaw et al., 2005; Jabbour et al., 2012; Brandes and Tanner, 2014) were used in the interpretation of 2D depth-migrated seismic reflection profiles (R-15, R-16) (Figures 4A, 5A) and construction of the regional balanced and restored cross-sections (A-AI) across RFFTB (Figures 6A,B). The balanced cross-section is approximately parallel to the thrust transport direction and has a total length of 64 km. Interpretation of 2D seismic reflection profiles and constraints on balanced cross-section geometry comprise structural information (position of stratigraphic contacts, faults, thrusts, dips) and thicknesses of lithostratigraphic units. For interpretation of 2D depth-migrated seismic profiles, construction of regional balanced and restored cross-sections and forward kinematic modeling was used the Move 2018.2 software (2018–2019 academic licenses from Midland Valley). Balancing and restorations were performed using Move structural modeling software based on bed length and thickness conservation and the built-in flexural-slip algorithm for the sedimentary cover. Two kinematic algorithms were used during the construction of the forward kinematic model: 1) fault-propagation fold, and 2) fault-bend fold.
FIGURE 4. (A) Uninterpreted and (B) interpreted seismic reflection profiles R-15. Location is shown in Figure 2.
FIGURE 5. (A) Uninterpreted and (B) interpreted seismic reflection profiles R-16. Location is shown in Figure 2.
FIGURE 6. (A) Balanced—A-AI and (B) restored cross-sections. Location is shown in Figures 1, 2. Abbreviations: T1-T7—Thrusts; D1, D2, Detachments; CSA, Chaladidi-Sagvamischao anticline; SB, Sagvamichao basin; KVA, Kvaloni anticline; TB, Teklati basin; KA, Khobi anticline; KB, Khobi basin; NOA, Nokhalakhevi anticline; NOB, Nokhalakevi Basin; TSA, Tsaishi anticline; NB, Narazeni basin; SHA, Sashurgaio anticline; DZB, Dikhazungi basin; SAA, Sarakoni anticline; TSB-Tsalenjikha basin.
Results
We obtained four 2D depth-migrated seismic profiles (R-15, and R-16) through the Tsaishi, Kvaloni, and Khobi anticlines (Figures 4, 5) and cover the central part of the RFFTB (Figure 2). Strata boundaries on seismic profiles are constrained by geologic maps and well data. The geometry of faults within the central part of the RFFTB can be interpreted through direct fault-plane reflection and truncation of seismic reflections. The seismic profile R-15 (Figures 4A,B) clearly illustrate the geometry of the Tsaishi anticline. Interpreted seismic profile show that the Tsaishi anticline is a south-vergent fault-propagation fold whose front limb is broken by thrust faults. The backlimb of the Tsaishi anticline is complicated by backthrusts (Figure 4B). The top section is represented by Tertiary, Cretaceous, and Late Jurassic strata. The Base of the section is marked by the upper detachment, which correlates to the evaporates of the Late Jurassic. The lower section is represented by duplexes and is composed of Early-Middle Jurassic rocks (Figure 4B).
The seismic reflection profile R-16 (Figures 5A,B) revealed the geometry of Kvaloni and Khobi anticlines and show that these anticlines are north-vergent fault-propagation folds. Duplexes made-up by Middle Jurassic rocks are developed under the Khobi anticline (Figure 5B). The growth strata geometry within the seismic profile is well imaged and shows onlaps and fanning limb dips of Khobi fold. Growth strata above Kvaloni and Khobi folds show evidence of crestal erosion during the fold growth (Figure 5B). Seismic reflection profile R-16 imaging onlaps within the growth sequences (Figure 5B). Pliocene strata above the onlapping growth units of the forelimb of the Khobi anticline reflect a later phase of structural growth involving a component of limb rotation (Figure 5B).
On the R-16 seismic profile, the formation sequence of the Khobi and Kvaloni anticlines is fairly well-observed. Taking into account the geometry of separate horizons of Upper Miocene growth strata we suppose that initially, the Khobi anticline was formed (Figure 5B). On the back and forelimb of the Kvaloni anticline, lower horizons of Late Miocene growth-strata beds are onlapping the pre-growth beds (Figure 5B). In the forelimb, folded growth strata are observed as well (Figure 5B). In contrast to the Khobi anticline, the Late Miocene growth strata structures in the backlimb of the Kvaloni anticline are represented by younger horizons (Figure 5B). These are the data which allow us to link the anticlines formation with the break-back thrust sequence.
In the cross-section construction, balancing, and restoration, some assumptions were made. One of the general problems in constructing a balanced cross-section is ‘‘filling space’’ between a known detachment horizon at depth and the structural elevation of the sedimentary rocks exposed at the surface (e.g., Woodward et al., 1989). Although there are no duplexes exposed at the surface of the RFFTB, the balanced cross-sections suggest that Early-Middle Jurassic rocks could be duplexed in the subsurface. These duplexes fill space between the master detachment and the rocks exposed at the surface. The duplexes also account for the folding of higher-level detachment horizons as shown in the seismic profile and balanced cross-section (Figure 4B, 6A). The balanced cross-section show that the anticlines are developed above the location of the upper detachment level and that the thrust faults are the main control of the fault-propagation folding that formed the anticlines. The anticlines are mainly represented by south-vergent and north-vergent fault-propagation folds (Figure 6A). The balanced cross-section shows that the south-vergent duplexes are developed above the lower detachment level. The flat upper detachment is deformed by deeply rooted duplexes, associated with prominent fault-bend folds (Figure 6A). The frontal part of the RFFTB is represented by Chaladidi-Sagvamichao, Kvaloni, and Khobi anticlines. Chaladidi-Sagvamichao, Kvaloni, Khobi, Nokalakevi, Tsaishi, Sashurgaio, and Surakoni anticlines are interpreted as fault-propagation folds.
Seismic profile R-15 (Figure 4B) reveals the occurrence of normal faults within sedimentary strata. These faults are inherited from the Middle Jurassic-Middle Eocene and related to phases of extension. Most of them were not drawn in the balanced cross-section (Figure 6A) since they had no influence on the mechanics of the foreland fold-and-thrust belt.
Discussion
The discussion focuses on two topics: 1) deformation structural style and 2) defining the types of thrust-top basins in the RFFTB developed using the end-member modes of thrust sequences (e.g., Boyer and Elliott, 1982; Butler, 1982; Butler, 1987; Morley, 1988; McClay, 1992; Storti et al., 2000).
The regional balanced cross-section (Figure 6A) shows the general styles of deformations along the RFFTB and interpreted structural geometries which significantly differ from prior transects (e.g., Banks et al., 1997; Cowgill et al., 2016; Tari et al., 2018). Previous studies within the RFFTB indicate that compressional structures developed above the main detachment level and structures are represented by ramp anticlines or fault-related folds (Banks et al., 1997; Cowgill et al., 2016; Trexler et al., 2022). The main style of deformation within the RFFTB is represented by a set of growth fault-propagation folds, duplexes, and triangle zone (Figure 6A). The balanced cross-section (Figure 6A) reveals that the structure between the Khobi and Tsaishi anticlines is characterized by a ramp-dominated triangle zone and is represented by south-vergent duplexes and north-and south-vergent thrusts. The formation of these structure zone is similar to the classical model of triangle zone - Type-II (e.g., MacKay et al., 1996; Hagke and Malz, 2018).
The thin-skinned RFFTB is characterized by two major detachment levels. Two detachment levels that join on the termination of the duplexes developed under the Tsaishi anticline are well-observed on the interpreted seismic profile R-15 (Figure 4B). A balanced section restoration of compressional structures across the profile (A-AI) provides a minimum estimate of shortening of -40%, equivalent -42.78 km (Figures 6A,B). Unfortunately, the estimation of the shortening value of the RFFTB was not carried out in previous studies. The shortening value was detected only for the Tsaishi anticline—5.3 km (Trexler et al., 2022).
The synclines within the RFFTB are filled by the Middle Miocene-Pleistocene shallow marine and continental syn-tectonic sediments, forming a series of typical thrust-top basins (e.g., Turner, 1988; Turner, 1990) associated with fault-propagation folds (Figure 6A). Thrust-top basins (or piggyback, wedge-top) are special among sedimentary basins in that they experience contraction during sedimentation and are a common feature in foreland basins systems worldwide (Turner, 1988; Butler and Grasso, 1993; DeCelles and Giles, 1996). The terms “thrust-top”, “piggyback” or “wedge-top” basins were used for basins developed on active thrust sheets (Ori and Friend, 1984; Turner, 1988; Butler and Grasso, 1993; DeCelles and Giles, 1996). These terms that are used today in the geological literature often lead to misunderstandings. Our study area is not an exception. For instance, the Odishi piggyback basin (Banks et al., 1997), as well as the Rioni wedge-top basin (Forte et al., 2014), was distinguished and studied within the RFFTB.
One of the critical issues in the analysis of fold-and-thrust belts is the timing of thrusting. Several models have been proposed to explain deformation. These are: 1) a piggyback thrust sequence or a foreland-directed thrusting, where displacement is transferred onto a new thrust initiated in the footwall of the previously active thrust (Boyer and Elliott, 1982; Butler, 1982); 2) a break-back thrust sequence or a hinterland-directed thrusting, where new thrusts originate in the hangingwalls of older thrusts (Butler, 1987); 3) In-sequence thrusting, where a thrust sequence has formed progressively in one direction, which can either be a piggyback or a break-back sequence (McClay, 1992); 4) Out-of-sequence thrusting, where the sequence of thrusting does not conform with either a progressive piggyback or break-back sequence (Morley, 1988; McClay, 1992); and 5) Synchronous thrusting, where two or more thrusts accumulate displacement at the same time (Boyer, 1992; Storti et al., 2000). According to Storti et al. (2000), several of the above thrust sequence modes can act at the same time. The balanced cross-section (Figure 6A) shows that the sequence of thrusting in the RFFTB occurs mainly in two ways: a piggyback sequence (foreland-directed) and a break-back sequence (hinterland-directed). Fault-propagation folds and duplex structures formed the main structure of the RFFTB. The south-and north vergent fault-propagation folds are forming the thrust-top basins. The regional balanced cross-section (Figure 6A) shows that fault-propagation folds above the upper detachment level can develop by piggyback and break-back thrust sequences. The formation of fault-bend fold duplex structures above the lower detachment is related to piggyback thrust sequences and is interpreted as a blind duplex (Figure 6A). The rejuvenation of thrust-top basins in the north-south direction is observed on the balanced cross-section (Figure 6A). Seven thrust-top basins have been defined within the study area. Chronologically, the oldest is the Tsalenjikha thrust-top basin, the formation of which began in the middle Miocene, and the youngest is the Sagvamichao basin (Pliocene-Pleistocene) (Figure 6A).
According to the definition of the piggyback basin (or thrust-top) by Ori and Friend (1984), it is formed and filled while being carried piggyback thrust sequence on active thrust sheets. Accordingly, we considered it appropriate to name the thrust-top basins related to break-back thrust sequences break-back basins. Using end-member modes of thrust sequences (e.g., Butler, 1982; Butler, 1987; McClay, 1992) we can define three types of thrust-top basin: 1) Type I-piggyback basin—the evolution of thrust-top basins was mainly controlled by the piggyback thrust sequence; 2) Type II-break-back basin (Teklati basin)—the evolution of thrust-top basins was controlled by the break-back thrust sequence; and 3) Type III (Sagvamichao, Tsalenjikha basins)—formation of thrust-top basin is related to combined, piggyback and piggyback back thrust sequences and has bi-vergent geometry (Figure 6A). The majority of basins represent Type I (piggyback basin) and are developed between the growth fault-propagation folds (Narazeni, Nokalakhevi, and Dikhazungi basins). The Teklati basin represents the Type II (break-back basin) and is developed between the fault-propagation folds of Kvaloni and Khobi. The Sagvamichao and Tsalenjikha basins are characterized by bi-vergent geometry and are attributed to Type III (Figure 6A). The Sagvamichao basin is located between the south- and north-vergent growth fault-propagation folds. The geometry of the northern part of the wide Tsalenjikha thrust-top basin developed between the Sarakoni anticline and frontal monocline zone of the GC Southern Slope was controlled by duplex staking kinematics (Figures 6A, 7). The similar picture is typical for the Jaca basin in the South Pyrenean thrust-top basin (e.g., Turner, 1988). Since the Miocene the basin depocenters migration from the North to the South took place synchronously with the duplexes formation (Figure 7).
FIGURE 7. Kinematic models of sequential development of Tsalenjikha thrust-top basin. (A) Present-day structure. (B) Deformation during Pliocene. (C) Deformation during the late Miocene. (D) Wedge-related deformation during Middle Miocene and early late Miocene. (E) Restored cross-section.
Kinematic models of sequential development of frontal folds of the RFFTB demonstrate that the formation of Chaladidi-Sagvamichao, Kvaloni, and Khobi anticline during Late Miocene-Pleistocene is related to combined thrust sequences (Figure 8).
FIGURE 8. Kinematic models of sequential development of frontal folds of the RFFTB. (A) Present-day structure. (B) Deformation during early Pliocene. (C) Deformation during the late Miocene.
According to Banks et al. (1997), the timing of the onset of Cenozoic deformation in the RFFTB is in the Late Miocene. Based on fission-track data, the exhumation process in the western GC started at the end of the Oligocene and reached its peak in the Pliocene-Pleistocene (Vincent et al., 2007; Avdeev and Niemi, 2011; Vincent et al., 2011). The geometry of syn-orogenic sedimentation, associated with footwall synclines and the sedimentary infill of thrust-top basins, provides information on the thrusting activity within the RFFTB (Figures 7, 8). From the Miocene times onward, the compressional deformation within pro-wedge foreland basin and the onset of Middle Miocene syn-tectonic sedimentation took place (Alania et al., 2021a). Within the RFFTB are distinguished three major changes in basin-fill dynamics: 1) marine/regressive stage (Middle Miocene-Early Pliocene), 2) marine/transgressive stage (Late Pliocene), and 3) marine-continental/transgressive-regressive cycle (Pleistocene-Holocene) (Jones and Simmons, 1997). Unfortunately, the study area lacks any detailed sedimentological studies of syntectonic strata, although the basin-fill dynamics could be reconstructed taking into account basin geometry and depositional conditions.
The tectonic model across the western GC (Figure 9) demonstrates that the retro-wedge and the Terek foreland basin developed on the upper plate, whereas the pro-wedge and the Rioni foreland basin developed on the lower, subducting plate. According to Alania et al. (2021a), the build-up of the GC orogen is related to a two-phase compressive deformation: 1) an early, symmetric inversion during the Oligocene-Early Miocene, and 2) the formation of an asymmetric, double-wedge structure during the Middle Miocene-Pleistocene. Building of structures of the RFFTB was governed by the GC basement crustal-scale duplexes propagation along detachment horizons within the cover-generating thin-skinned structures made up of pre- (Jurassic, Cretaceous, Paleogene) and syn-orogenic (Miocene-Pleistocene) sequences (Figure 9).
FIGURE 9. Tectonic model of the western GC orogen (modified from Alania et al., 2021a).
The RFFTB is an excellent example of the formation of thrust-top basins related to piggyback, and break-back thrust sequences. Future integrated up-to-date sedimentological and thermochronological studies are fairly essential in order to strengthen the proposed structural model.
Conclusion
In this paper, we introduce the study results of the deformation structural style of the RFFTB using a seismic reflection profiles and a regional balanced cross-section. Our conclusions are summarized as follows:
• The main style of deformation within the thin-skinned RFFTB is represented by a set of growth fault-propagation folds, triangle zone, duplexes, and a series of thrust-top basins. The RFFTB is characterized by two major detachment levels. Fault-propagation folds above the upper detachments level can develop by piggyback and break-back thrust sequences. Duplex structures above the lower detachment can develop by piggyback thrust sequences.
• The amount of shortening obtained for this part of the regional balanced cross-section is 40% (−42.78 km).
• Within the RFFTB, a series of thrust-top basins developed. Fault-propagation folds and duplex structures formed the main structure of the thrust-top basins. The evolution of the thrust-top basins was mainly controlled by the kinematics of thrust sequences and competing growth fault-propagation folds. Using end-member modes of thrust sequences, the thrust-top basins are divided into: 1) Type I-piggyback basin, 2) Type II-break-back basin, and 3) Type III—formation of thrust-top basin characterized by bi-vergent geometry and related to combined, piggyback and piggyback back thrust sequences.
• Building of compressional structures of the RFFTB was governed by the GC basement crustal-scale duplexes propagation along detachment horizons within the cover-generating thin-skinned structures.
Data availability statement
The original contributions presented in the study are included in the article/Supplementary Material, further inquiries can be directed to the corresponding author.
Author contributions
VA: Conceptualization, Data acquisition, Data curation, Investigation, Methodology, Resources, Supervision, Validation, Visualization, Writing—original draft, editing. GM: Data curation, Investigation, Supervision, Methodology, Validation, Writing—original draft. PP: Methodology, Investigation, Validation, Writing—review and editing. IF: Investigation, Resources, Writing—review and editing. TB: Resources, Validation, Writing—review and editing. OE: Data curation, Investigation, Resources, Validation. AG: Investigation, Resources, Validation. AR: Investigation, Resources, Validation.
Funding
The work was supported by the Shota Rustaveli National Science Foundation of Georgia (Study of geothermal potential of Georgia by hydrogeochemical and isotope methods, FNF-18-19173).
Acknowledgments
We are very grateful to the Georgian State Agency of Oil and Gas for providing the seismic profiles for our interpretation. Many thanks to the Associate Editor, Prof. Antonio Pedrera, and two reviewers for their constructive comments and helpful suggestions.
Conflict of interest
The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.
Publisher’s note
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Keywords: Greater Caucasus orogen, rioni foreland fold-and-thrust belt, seismic reflection profile, balanced and reconstructed cross-sections, fault-propagation fold, duplex, thrust sequence, thrust-top basin
Citation: Alania V, Melikadze G, Pace P, Fórizs I, Beridze T, Enukidze O, Giorgadze A and Razmadze A (2022) Deformation structural style of the rioni foreland fold-and-thrust belt, western greater caucasus: Insight from the balanced cross-section. Front. Earth Sci. 10:968386. doi: 10.3389/feart.2022.968386
Received: 13 June 2022; Accepted: 13 September 2022;
Published: 05 October 2022.
Edited by:
Antonio Pedrera, Instituto Geológico y Minero de España (IGME), SpainReviewed by:
Esther Izquierdo Llavall, Instituto Geológico y Minero de España (IGME), SpainJosé Francisco Mescua, CONICET Argentine Institute of Nivology, Glaciology, and Environmental Sciences (IANIGLA), Argentina
Copyright © 2022 Alania, Melikadze, Pace, Fórizs, Beridze, Enukidze, Giorgadze and Razmadze. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
*Correspondence: Victor Alania, dmljdG9yLmFsYW5pYUB0c3UuZ2U=