The Miocene record of the Betic Cordillera uplift in Los Guájares valley (Granada province, S Spain)

The Los Guájares valley is located about 35 km south of Granada in the Internal Zones of the Betic Cordillera. The Miocene deposits in this area consist of six sedimentary units separated by unconformities, which are exposed in small and laterally discontinuous outcrops overlying metamorphic rocks of the Alpujárride Complex. The lowest unit comprises upper Serravallian marls with planktonic foraminifera filling neptunian dykes and covering Triassic dolomitic marbles of the Alpujárride Complex. These marls reflect deep marine deposition on the Betic basement under a local extensional regime. Uplift of the region led to emergence and deposition of continental red alluvial-fan conglomerates and foothill breccias. The overlying unit, a shoreline conglomerate with small oyster banks, indicates relative sea-level rise. Shallow-marine conditions continued during the deposition of the following unit, early Tortonian in age, which consists of calcareous sandstones with hermatypic corals. Small patch reefs developed in the overlying unit composed of sandy limestones with corals (Porites, Tarbellastraea, Thegioastraea) and oysters, and sandy limestones with coralline algae in the most distal areas. The coral reefs in Los Guájares and some coral heads in Albuñuelas, a near locality, are the only record of early Tortonian coral buildups in the Mediterranean. The last marine unit comprises lower Tortonian conglomerates, sandstones and siltstones accumulated in the front of a small delta. Oyster banks and concentrations of Turritelines suggest high nutrient levels in the delta-front paleoenvironments. The Los Guájares valley area emerged afterwards, following the onset of a compressional geodynamic regime in the central Betic Cordillera and since the early Tortonian only small bodies of foothill and alluvial-fan deposits formed in a predominantly erosional context.


Introduction
The Miocene sedimentary rocks that appear in small outcrops in the Internal Zones of the Betic Cordillera have been poorly studied, and the knowledge on their origin and relationships with adjacent larger basins, such as the Granada Basin is limited.This is the case of the Miocene deposits in the Los Guájares valley (Granada), which have only been reported in studies on the regional geology of the area.These works comprise the sheet 1041 (Dúrcal) of the MAGNA geological map from the late 1970s (Avidad et al., 1978), and a paper by Estévez et al. (1985), where the authors include a lithological map and a brief description of the stratigraphy of the Neogene to Quaternary cover on the metamorphic basement.The latter work points out the complex stratigraphy of the Miocene materials, which are faulted and folded and crop out in small, dispersed exposures.The described lithological succession reflects drastic changes in the depositional environments, which record the uplift history of this part of the Betic mountains in the Middle and early Late Miocene.Lower and Middle Miocene deposits in the Internal Zones of the Betic Cordillera generally occur in highly tectonized, scattered outcrops at the base of the sedimentary fillings of the Neogene intermontane basins (González-Donoso, 1978;Hodgson, 2002;Rodríguez-Fernández, 1982;Rondeel, 1965).Limited lateral and vertical exposures, unconformities and facies heterogeneity make difficult correlation and paleoenvironmental interpretation of the successive sedimentary units even if the age of some of them was constrained with planktonic foraminifer and nannoplankton biostratigraphy, strontium isotope stratigraphy and fission track thermochronology (González-Donoso, 1978;Hodgson, 2002;Johnson et al., 1998;Rodríguez-Fernández, 1982;Rondeel, 1965).This prevents an accurate reconstruction of the paleogeographical evolution of the region in a key period of exhumation and emergence of the cordillera.
The scarcity of data on coral reefs of early Tortonian age all over the Mediterranean region (Perrin & Bosellini, 2012) made worth a detailed study of the structure and composition of the coral reefs in Los Guájares valley reported by Estévez et al. (1985).
The primary aim of this work is to analyze the sedimentological features and fossil content of the successive lithostratigraphic units that can be distinguished in the Miocene rocks in the Los Guájares valley.Specific purposes are: (a) to establish a precise age of the largest possible number of units and correlate them with materials deposited in the Granada Basin, the nearest basin with a relatively well-developed and well-known Miocene sedimentary record; (b) to interpret the depositional paleoenvironments of each unit, as well as the sedimentary evolution of the area; and (c) to characterize the coral reefs in the area in the context of coral-reef decline in the Mediterranean region.

Geographical and geological context
The study area is located in the Los Guájares valley, an area of approximately 90 km 2 , about 35 km south of Granada, in southern Spain (Fig. 1).The Miocene deposits crop out between the villages of Guájar-Faragüit and Guájar-Alto, and cover about 5 km 2 (Fig. 2).The area belongs to the Internal Zones of the Betic Cordillera, the westernmost segment of the European Alpine belt.The cordillera can be divided into three main domains: (1) the External Zones that represent the Mesozoic to Middle Miocene southern continental margin of the Iberian Massif (García-Hernández et al., 1980;Vera, 1988); (2) the Campo de Gibraltar or Flysch Units that comprise a series of allochthonous, Cretaceous to Middle Miocene units (e.g., Sanz de Galdeano & Vera, 1992); and (3) the Internal Zones, mainly made up of metamorphic rocks (Fallot, 1948).The latter domain includes three stacked tectonic complexes, which in ascending order are: the Nevado-Filábride Complex (Paleozoic or older) (Gómez-Pugnaire et al., 2000, 2004), the Alpujárride Complex (Paleozoic to Mesozoic metasediments) (Delgado et al., 1981), and the Maláguide Complex, with a non-metamorphic Mesozoic to Cenozoic cover overlying a pre-Permian basement (Lonergan, 1993;Martín-Martín, 1996).The Miocene sedimentary rocks of the Los Guájares valley overlie rocks of the Alpujárride Complex, concentrating in grabens delimited by normal faults (Fig. 2).In the Los Guájares area, the Alpujárride Complex includes two units, the so-called Los Guájares and La Herradura nappes.These units, Paleozoic to Triassic in age, basically consist of graphitic schists, quartzites, calcschists and calcitic-dolomitic marbles (Avidad et al., 1978) (Fig. 2).

Methods
Twelve stratigraphic sections were logged in dispersed exposures along roads and in ravines in the Miocene outcrops in Los Guájares valley (Figs. 3,4).The lithological, sedimentological and paleontological characteristics, geometry and thickness variations of the sedimentary bodies, and significant stratigraphic surfaces were observed at the outcrops and the main distinguished units were mapped at 1:20,000 scale (Fig. 2).Macrofossils were collected for identification in the laboratory.Twenty-six thin sections were prepared from rock samples for petrographic analysis and identification of biogenic components in the laboratory.Calcimetry was performed on four samples to determine their calcium carbonate content.To extract foraminifera for biostratigraphic dating and paleoenvironmental interpretation, 16 samples of fine-grained sediments were washed using sieves of 0.25, 0.125 and 0.065 mm and then dried in an oven at 40ºC.The residue in the 0.125 mm fraction was the one examined.The extracted foraminifera were examined under an optical microscope Leica MZ12 and under a SEM Quanta 650 FEG (Thermofisher-FEI).

Lithostratigraphic units and paleontological content
In the twelve stratigraphic sections logged (Figs. 2,3,4), six units were identified based on lithology, fossil content and boundary surfaces (Fig. 5).From the lowest to the youngest these are:

Unit 1
This is the basal unit, directly overlying the dolomitic marbles of the Alpujárride Complex.It is laterally very discontinuous, appearing on the basement in numerous outcrops in the Haza Llana area and disappearing completely towards the south (Fig. 2).In Sect. 2 (Fig. 3), the unit is made up of whitish marls with heterometric angular clasts of the basement, up to 30 cm in size.The marls occur as a lens-shaped body approximately 2 m wide and 1 m thick, and do not contain fossils.In Sect.3, about 450 m south of Sect. 2 (Figs. 2, 3), well-lithified whitish marls fill in neptunian dikes in the basement marbles (Fig. 6A) and pass vertically to a more continuous bed of friable marls about 1 m thick.The fillings of the neptunian dykes are wackestones with angular marble fragments and abundant planktonic foraminifera (Fig. 6B), in contrast with the overlying marls, which contain altered specimens.
The identified planktonic foraminifera are Globigerina

Unit 2
In the Haza Llana area (Sects. 1,2,3 and 4,Figs. 2,3), this unit appears as a horizontally bedded, reddish conglomerate overlying an erosion surface.The conglomerate, up to 4 m thick, is highly heterometric, matrixsupported and without fossils.The clasts are mostly subrounded cobbles of dolomitic marbles.Locally, alternations of reddish and grey conglomerates, and sandstones can be observed.To the south, the unit abruptly changes along a direct fault plane (Figs. 2, 5) to a strongly lithified, clast-supported breccia, with a red terrigenous matrix (Fig. 6C).This breccia is structureless, up to 15 m in thickness, highly heterometric, with pebbles to boulders up to 100 cm in size and without fossils.The clasts are Fig. 2 Geological map of the study area.The location of logged sections (Figs. 3, 4) is indicated by numbers 1 to 12. Units 2 and 3, and 4 and 5, respectively, are mapped together due to their small extension carbonate fragments from the basement (dolomitic marbles and calcschists), except southeast of Sect.12 (Figs.2,  4), where the clast-supported breccia contains numerous angular clasts made up almost exclusively of schists because it lies directly on top of graphite schists.Poorly developed paleosols and rough horizontal stratification can be observed.Larger blocks (20-40 cm) appear concentrated in some beds.The unit overlies a karst surface carved on the basement in Sect.9 (Figs.2, 4).

Unit 3
It overlies an erosion surface on Unit 2 and consists of a thin, up to 1.5 m thick, laterally discontinuous matrix-supported breccia changing upwards to conglomerate with a greyish matrix.The breccia is structureless and heterometric.Clasts are carbonate and quartzite fragments from the Alpujárride basement.The predominantly angular clasts at the base change to more rounded at the top.The clast size varies from pebble to cobble (up to 20 cm).Carbonate clasts bored by bivalves (Gastrochaenolites isp.) and small specimens of Chlamys sp. can be observed.Small oysters  6 and 9 (Figs. 2,3,4).These patches are built by Ostrea edulis Linné and Magallana gryphoides (Schlotheim).The oysters are fragmented at the base whilst some valves are almost complete, up to 20 cm in size, towards the top.

Unit 4
This is a mixed terrigenous-carbonate unit, which is characterized by complex lateral facies changes.In Sects. 4,5,6 and 11 (Figs. 2,3,4), the unit is up to 2 m thick, and thins and disappears laterally.In Sect. 6 (Figs. 2,3), this unit overlies an erosion surface, adapting to a series of paleosteps carved on the underlying Unit 3. Unit 4 comprises a granule to pebble conglomerate at the base that passes upwards to reddish or yellowish fine-grained calcareous sandstone (21% of CaCO 3 content), with dispersed fragments of crustose coralline algae, such as Lithophyllum sp. and Neogoniolithon sp., and fragments of the coral Porites sp.The sandstone laterally includes larger fragments of branching colonies of Porites sp. that give a nodular aspect to the rock.In Sect.6 (Figs. 2, 3), isolated head-shaped colonies of Tarbellastraea sp., approximately 30-40 cm wide and 30 cm thick, can be observed in life position attached on top of the paleosteps, although they are also found embedded within the sandy matrix.The calcareous sandstone is rich in internal molds of bivalves of the order Lucinida, such as Lucina gracilis (Nyst), and some unidentified specimens of the order Nuculanida.There are also shells of calcitic bivalves, such as Pecten sp., Chlamys sp. and Spondylus sp., and some small specimens of O. edulis.In Sects.6 and 9 (Figs.2, 3, 4), the calcareous sandstone passes laterally southwards to siltstones (Fig. 5), which contain very scarce foraminifera (they represent less than 1% of the residue).Among planktonic foraminifera, Catapsydrax unicavus Bolli, Loeblich & Tappan, Globigerina bulloides (d'Orbigny), Paragloborotalia continuosa (Blow), Globigerinita glutinata (Egger), and Orbulina suturalis Brönnimann have been identified.Benthic foraminifera are extremely rare, mostly represented by a few specimens of Cibicides, Elphidium, and Nonion.This facies appears in several outcrops with limited lateral continuity.

Unit 5
In Sects.5, 6 and 11, it consists of sandy limestones (52% of carbonate content) overlying an erosion surface cutting Units 3 and 4 (Figs.2, 3, 4).They are terrigenous wackestones/packstones with Porites and Tarbellastraea colonies.Abundant branching and nodular colonies of Porites sp.intergrown with and encrusted by coralline algae (Lithophyllum sp., Neogoniolithon sp., and Spongites sp.) give a nodular aspect to the rock.The sandy reddish matrix is generally fine-grained, although locally it passes to patches with greenish colors richer in terrigenous grains of medium to coarse size.Together with the branching colonies of Porites sp., there are isolated heads of Tarbellastraea sp. in life position.Porites is more abundant than Tarbellastraea.Well-preserved isolated specimens of O. edulis and whole clypeasteroid echinoids can also be found.At some sites, such as Sect.6 (Figs. 2, 3), small coral patches overlie the sandy nodular limestones, forming bodies that range between 1 and 1.5 m in thickness and 15-20 m in width.They consist of head-shaped colonies of Porites sp. and Tarbellastraea sp., and coralline algae, which appear both encrusting corals and as small nodules dispersed in the wackestone matrix (Fig. 7A, B).Lithophyllum gr.racemus, Lithophyllum gr.nitorum, Neogoniolithon sp., and Spongites sp. were identified in the patches.
At the base of Sect.7 (Figs.2, 4), the unit consists of a bioherm structure, formed by colonies of Tarbellastraea abditaxis Chevalier in life position, locally encrusted by coralline algae (Lithophyllum sp., Lithophyllum gr.nitorum, Neogoniolithon sp., and Spongites sp.).These coralline algae also appear as nodules in the wackestone matrix.This bioherm is covered by a thin bed of yellowish siltstone, 30-40 cm thick, which in turn is overlain by a 2 m thick package of packstone rich in O. edulis.
In Sect. 10 (Figs. 2, 4, 8A), fine-to coarse-grained calcareous sandstones (30% to 38% of carbonate content) occur at the base of the unit.They are dark due to fragments of dolostone and schists from the basement, and contain larger benthic foraminifera, such as Borelis sp., gastropods and In outcrops in the Haza Llana area (Fig. 2), this unit consists of nodular sandy limestones, up to 2 m thick, which at Sect. 4 (Figs.2, 3) are capped by a conglomerate of subangular pebbles of dolomitic marble and quartzite, with a packstone matrix with larger benthic foraminifera (Nummulitidae), bivalves and coralline algae as the main bioclastic components.

Unit 6
This is the most extensive and thickest unit, up to 70 m, and consists of alternating conglomerates, sandstones and siltstones.This unit is present in all study sections, except in Sects. 2 and 3 (Figs.2, 3, 4).At the base of Sect. 8 (Figs. 2,4), massive granule to pebble conglomerates, up to 5 m thick, are followed by flat, roughly bedded sandstones and siltstones.Above them, amalgamated channelized deposits, 40-50 cm thick, show fining upward sequences from fine-grained conglomerates to medium/fine sandstones or silty sandstones.These are overlain by horizontal beds of sandstones and silty sandstones, 25-30 cm thick, with occasional bioturbation at the top.Locally, current ripples, 10-15 cm high, and smaller wave ripples appear at the top of the beds.A lobe-shaped morphology of sandstone bodies can be observed at the outcrop scale.Synsedimentary normal faults oriented N120-150E with decimeter-scale throws are common in these beds.These deposits are overlain by a new succession of amalgamated channelized bodies, with fining upward sequences from granule conglomerates to sandstones and silty sandstones, and flat-bedded sandstones.
In the upper part of Sect.8, clast-supported conglomerates appear in a large channel with erosive base, up to 4-5 m thick and tens of meters wide, which comprises several amalgamated smaller channels with fining-upward sequences, from conglomerate to medium sandstones.Clasts are made of quartzites (mostly), marbles and schists from the Alpujárride basement, mainly from granule (in the matrix) to cobble size (up to 15-20 cm).The axe of this large channel is oriented N25ºE.The succession continues with subhorizontal beds of sandstones and silty sandstones.
Oyster banks formed by large specimens of Ostrea edulis and Magallana gryphoides generally occur on top of siltstone and clay beds, although in the upper part of the section they appear within sandstone (Fig. 4).Some of these banks extend laterally for more than 7 m and are up to 50-60 cm thick.Articulated specimens of O. edulis are up to 26 cm long, and 18 cm wide, whereas.M. gryphoides can reach up to 25 cm in length, and 12 cm in width.Locally, buried Pinna sp.appears preserved in life position in silty sandstones.As commented in Unit 4, foraminifera are rare (less than 1% of the residue) and planktonic forms are much scarcer than benthic ones in the siltstones.Among the benthic foraminifera, the species At the top of Unit 6 (Fig. 4), a laterally continuous rudstone bed rich in siliciclastic grains with abundant O. edulis and M. gryphoides of large size (up to 30 cm) is followed by two rudstone beds, 30 and 70 cm thick, respectively, with a high carbonate content (about 70% CaCO 3 ).Both beds are rich in internal molds of Turritellines and clasts of quartzite and marble (Fig. 9).A small rudstone bed, 20 cm thick, with O. edulis and M. gryphoides, separates the two lower Turritelline beds from a third one of similar characteristics at the top.
This unit also outcrops in isolated patches distributed throughout the valley.In Haza Llana, these patches unconformably overlie all the underlying units (Figs. 2, 3).They consist of massive sandstones and matrix-supported pebble conglomerates with large O. edulis and clypeasteroids.In Sect.6 (Figs. 2, 3), sandstones and fine-grained conglomerates appear at the base, and are followed by strongly cemented sandstone beds, 30-50 cm thick, and large oysters (Fig. 2).In the southern outcrop, in Sect.12 (Figs.2, 4), the unit consists of a thick package of siltstones and clays (20-30 m) at the base, followed by sandstones and siltstones, in turn overlain by channelized bodies, decimeters in thickness, of granule to pebble conglomerates intercalated in sandstones.The conglomerates are composed of mainly quartzite clasts in a silty matrix.

Unit 1
The abundance of planktonic foraminifera in the whitish marls in Sect. 3 (Figs. 2,3,6B) indicates a pelagic marine environment (Fig. 10A).Benthic foraminifer assemblages point to deep-water conditions.The pelagic marls filled in the open fractures (neptunian dykes, Fig. 6A) in the basement, engulfing heterometric, angular clasts derived from the fractured dolomitic marbles with little transport (Fig. 6B).After filling the fractures, the marls draped the seafloor as evidenced by marl beds in Sect. 3 (Figs.2, 3).Their original thickness and lateral extension cannot be assessed due to subsequent erosion events.Marls of the same age, however, crop out in Hoya de las Bolinas, Zaza ravine (Estévez et al., 1985) and the Ízbor valley (González-Donoso, 1978) (Fig. 1B), suggesting they extended on the Betic basement in a large area.

Unit 2
The subrounded cobbles in a fine-grained matrix in subhorizontal beds with erosional bases indicate that the red facies of Unit 2 in the Haza Llana area (Fig. 2) correspond to alluvial fan deposits (Fig. 10B).Specifically, they are proximal fan facies where cobbles were transported by turbulent, high-energy and short-lived high-density currents (Colombo, 2010).The alternations of conglomerates and sandstones indicate changes in flow composition during fan progradation.
The heterometric cobble to boulder breccia, with a reddish matrix without fossils of Unit 2 in the rest of the outcrops (Figs. 2, 6C) corresponds to continental foothill deposits (Fig. 10B).This breccia of angular clasts indicates an original steep slope at the foot of an Alpujárride paleo-relief (Estévez et al., 1985).It is difficult to establish whether the breccias were more proximal than the alluvial fan facies, since the morphology of basement greatly conditioned the type of deposit.A steep relief would give rise to foothill breccias, whereas a relief with water outflows would promote alluvial fans.Both facies are similar to the Quaternary deposits in the Los Guájares valley and other Betic areas with an Alpujárride bedrock.

Unit 3
Marine bivalves, such as Chlamys sp. and bivalve perforations in large angular boulders in the highly heterometric breccia indicate that this is a subtidal deposit formed at a rocky shore with clasts derived by rock fall from the basement with little transport or reworking (Gupta & Allen, 1999) (Fig. 10C).The increase of clast roundness and better sorting of clasts towards the top suggests longer reworking/transport of clasts and a transgressive pattern within the unit.These deposits closely resemble the conglomerates and breccias with perforations found in the Miocene from Sierra Arana-Mencal in the Guadix Basin Fig. 10 Paleoenvironmental evolution of the Los Guajáres valley area.A In the late Serravallian the area was a deep-water pelagic setting.Marls filled in neptunian dykes an extended on the Betic basement.B Due to regional uplift the area emerged.Alluvial fans and foothill breccias covered a locally karstified surface.C Tectonic restructuring and relative sea-level rise caused partial flooding of the area and formation of near-shore breccias and conglomerates with small oyster banks.D In the early Tortonian continued sea-level rise led to shallow-water marine conditions and accumulation of calcareous sandstones with corals and siltstones in deeper settings.E Similar environmental conditions prevailed after a tectonic instability that caused an erosive unconformity.Conglomerates, sandy limestones and coral patches formed in the proximal areas, whereas sandy limestones with coralline algae (rhodoliths) prevailed in the more distal southern areas.F The marine sedimentation in the Los Guájares valley ended in the early Tortonian with delta deposits with abundant oyster concentrations.Delta-front sediments show a proximal-distal facies trend from north to south (Soria, 1994) and the conglomerates formed at a rocky shoreline of Alpujárride dolostones in the Late Miocene in Sierra de Gádor (Sola et al., 2022) (Fig. 1A).Oysters settled on the conglomerates forming small banks, which were partly reworked by waves.

Unit 4
The coralline algae Lithophyllum sp. and Neogoniolithon sp.(Aguirre et al., 2017;Braga, 2017;Braga et al., 2010), and the hermatypic corals Porites and Tarbellastraea suggest that calcareous sandstones were deposited in shallow subtidal environments (Fig. 10D).These coral genera formed reef structures of diverse dimensions, from meters to tens of meters in width, and decimeters to meters in thickness, in shallow paleoenvironments with terrigenous influx during the Late Miocene in the Neogene Betic basins (Braga et al., 1990;Martín et al., 1989;Santisteban & Taberner, 1983).In addition, the depositional setting was of low/moderate energy due to the presence of abundant micritic matrix.Hermatypic corals are typical of warm waters, in which lowest mean temperatures are higher than 16 °C (Veron, 1995).Applying the "energy hypothesis" of Fraser and Currie (1996), the genus richness during the Tortonian suggests minimum sea-surface temperatures of about 18 °C in the Mediterranean (Bosellini & Perrin, 2008;Rosen, 1999).In Unit 4, the small size of colonies points to a stressed environment with frequent disturbances limiting the coral growth (Bauman et al., 2013;Vermeij et al., 2007).These calcareous sandstones change laterally to silts formed in lowerenergy, deeper settings, as already pointed out by Estévez et al. (1985).

Unit 5
Unit 5 has biogenic components similar to those of Unit 4. It also accumulated in shallow-water settings in which zooxanthellate corals grew under the influence of terrigenous sedimentation in a generally low-energy environment as evidenced by the common occurrence of fine-grained sediment among the coral colonies and patches (Figs. 4, 8A,  10E).The presence of Hyotissa hyotis in Sect. 10 (Figs. 2,  4) is typical of warm-water reef environments and this species mainly inhabits shallow settings (Freneix et al., 1988).The occurrence of planktonic foraminifera suggests that the environment was open to the ocean.
The conglomerate of subangular pebbles with a packstone matrix in Sect. 4 in the Haza Llana area (Figs. 2, 3) can be interpreted as a more proximal and higher-energy facies than those outcropping around Guájar-Faragüit.The mixture of bioclastic components and reworked rock fragments derived from the Alpujárride suggest that the conglomerate formed in a rocky shore at the basin margin (Betzler et al., 1997;Sola et al., 2022).In contrast, the branching coralline alga Lithothamnion and the foralgaliths composed of encrusting foraminifera and Lithothamnion and Mesophyllum in the sandy limestones at the southern outcrops (Sect.12, Figs. 2,  4, 7C) indicate more distal paleoenvironments, several tens of meters deep (Aguirre et al., 2017;Bosence, 1991;Braga, 2017;Prager & Ginsburg, 1989).

Unit 6
Sediments in Unit 6 show lithologies, structures and fossil components characteristic of a fine-grained, fluvial dominated delta (Fig. 10F).Numerous channels occur at various levels within the unit, displaying fining-upward sequences from gravel to silt.The ripples that appear at some levels indicate a moderate influence of wave action.The facies association of this deltaic system indicates a delta front area, with a combination of channels and sand lobes with small interdistributary bays where silts predominated (Rodríguez-López & Arche, 2010).The banks of M. gryphoides that occur in the silty beds throughout the unit can be associated with interdistributary areas (Aguirre, 1998;Demarcq & Demarcq, 1989, 1990;Littlewood & Donovan, 1988;Martinius, 1991;Stenzel, 1971) where they lived attached to one another to counteract the adverse conditions presented by this type of environment (Herb & Geister, 1984).O. edulis and M. gryphoides are euryhaline bivalves that live in shallow marine environments (less than 20-30 m depth) and in hypersaline to brackish waters.The great abundance of oysters and the large size they reach in this unit would indicate a high productivity in the environment (Wood, 1993).The dense concentrations of Turritellinae (Fig. 9) at the top of the unit are also indicative of high nutrient content, usually showing an abundance of phytoplankton (Allmon & Knight, 1993;Allmon, 1988Allmon, , 1992)).The river was probably the nutrient source for the environment.The generally finegrained nature of the sediments and the high nutrient levels indicated by the fossil assemblages suggest that the fluvial system feeding the delta was perennial.
Facies distribution in the valley gives some indication of proximal/distal patterns.The predominance of sands and silts with small channels at Sect. 12 (Figs.2, 4) suggests that the deposits in the southern outcrop are the most distal ones.
6 Age of the stratigraphic units Estévez et al. (1985) were not able to obtain planktonic foraminifera from the samples collected in the Los Guájares valley.In the samples of Unit 1 in the Haza Llana area (Figs. 2, 3), the planktonic foraminifera are very scarce, including Globigerina spp., Globigerinita glutinata, Paragloborotalia mayeri, P. continuosa, P. siakensis, and Orbulina suturalis (Fig. 11A-C).This species assemblage ranges from the late Langhian to the earliest Tortonian (Wade et al., 2011;Young et al., 2017).Whitish marls, similar to those of Unit 1 from the Haza Llana area (Fig. 2), crop out in the nearby Zaza ravine, about 4 km to the NE, by the road connecting Los Guájares with Pinos del Valle (Fig. 1B).Estévez et al. (1985) indicated that the age of these marls was inconclusive as they found two groups of species of different age, which appear in similar state of preservation: one indicating a basal Serravallian and another pointing to a middle Serravallian age.However, they favored a basal Serravallian age, as the most consistent and simplest hypothesis (Estévez et al., 1985).
We collected a sample of whitish marls in the Zaza ravine to test their age and the possible correlation with the whitish marls of Unit 1.This sample is rich in planktonic foraminifera, with the following assemblage: Paraglobrotalia siakensis (very abundant), P. mayeri (very abundant), Globorotalia menardii, G. praemenardii, G. scitula, Dentoglobigerina altispira, Sphaeroidinellopsis spp., Orbulina universa, O. suturalis, Trilobatus trilobus, Globigerinoides obliquus, and Globigerina bulloides (Fig. 11D-I).The last appearance of G. praemenardii and the first occurrence of G. menardii occurred between 11.97 and 13.41 Ma, late Serravallian (Young et al., 2017), postdating the age attributed by Estévez et al. (1985).Three marl samples, stratigraphically located between the metamorphic basement and reddish conglomerates equivalent to Unit 2, were also collected at the base of the Miocene succession in the Ízbor valley (Fig. 1B) that was previously studied by González-Donoso (1978).The sampling locality is 8 km to the northeast of the Haza Llana outcrops, now at the exit 167 of the motorway A-44.Specimens of P. mayeri, P. siakensis, Globorotalia praescitula-scitula, G. praemenardii, G. menardii, and Fohsella fohsi were identified in these marls.This assemblage also indicates a late Serravallian age.
The planktonic foraminifera found in the silts of Unit 4 (Catapsydrax unicavus, Globigerina bulloides, Globigerinita glutinata, Orbulina suturalis, and Paragloborotalia continuosa) (Fig. 11L, M) indicate a wide age range, from the middle Langhian (first occurrence of O. suturalis) to the earliest Tortonian (last occurrence of C. unicavus) (Wade et al., 2011;Young et al., 2017).Taking into consideration the stratigraphic position of Unit 4, well above the late Serravallian marls of Unit 1, it seems reasonable to assume an earliest Tortonian age for this unit.

Sedimentary and paleogeographic evolution
The Miocene deposits in the Los Guájares valley reflect dramatic changes in depositional environments from deep marine to continental, which reveal a series of tectonic movements of the region, also recorded by the unconformities separating the distinguished units.Following the exhumation of the Alpujárride Complex after burial highpressure metamorphism (Azañón et al., 1998), in the late Serravallian the Los Guájares Nappe was exposed at the sea floor in a deep pelagic environment.The marls of Unit 1 filled in open fractures in the basement, which indicate a local extensional context, compatible with the extensional context that has been described in the entire Betic basement in the Serravallian (Comas et al., 1992;Galindo-Zaldívar et al., 2019;Martínez-Martos et al., 2017).Marls of Unit 1 extended over the Alpujárride basement from Los Guájares valley to the Zaza ravine and Hoya de las Bolinas (Fig. 1B).Similar marls rich in planktonic foraminifera of Serravallian age were described by González-Donoso (1978) overlying Alpujárride schists in the Ízbor valley (Fig. 1B).These marls were interpreted as coastal lagoon deposits by Rustichelli et al. (2013) due to the occurrence of gypsum in them.Nonetheless, the gypsum in the marls is secondary gypsum filling fractures and it is probably derived from the Alpujárride basement.In addition, the marls contain abundant planktonic foraminifera, indicating that they are pelagic sediments similar to those in Unit 1.
The exposure of at least part of the Alpujárride basement on the sea floor, however, took place earlier in the Early Miocene (early Burdigalian).In the southern part of the Granada Basin, near Murchas (Fig. 1), the Alpujárride basement is overlain by pelagic sediments older than those of the Los Guájares valley.Gonzalez-Donoso (1978) and Rodríguez-Fernández (1982) described lower Burdigalian marls overlying a breccia of clasts derived from the underlying Alpujárride basement.A similar succession of breccia of basement clasts and marls rich in early Burdigalian planktonic foraminifera was described as the Alamillos Formation by Rodríguez-Fernández (1982) at the base of the Neogene deposits in the Guadix Basin (Fig. 1A).Pascual-Molina (1997) reported pelagic deposits late Burdigalian-early Langhian in age on the Betic basement at the northwestern margin of Sierra Alhamilla and open-marine sediments rich in middle-Burdigalian planktonic foraminifera overlie Maláguide and Alpujárride rocks north of Sierra Cabrera and south of Sierra de Almagro at the margins of the Sorbas and Vera basins, respectively (Hodgson, 2002;Rondeel, 1965;Völk, 1967) (Fig. 1A).
The Los Guájares area was submerged again and became a shallow-water marine setting during deposition of Units 3 to 6.There were areas in the Betic basement that continued to rise, such as the antecedent reliefs of the present-day Sierra de la Tórtola or the Sierra Nevada nucleus (Braga et al., 2003) (Fig. 1A), while other areas such as the present-day Los Guájares valley were flooded by a relative sealevel rise.The grey breccias and conglomerates of Unit 3 formed at a rocky shoreline witnessing the initial steps of the flooding.
Further relative sea-level rise led to the establishment of a shallow marine environment with terrigenous influx from emergent reliefs in the early Tortonian during accumulation of Units 4 and 5, in which coral reefs thrived building small structures.Tectonic instability generated an erosive unconformity between Units 4 and 5 but the depositional paleoenvironment did not substantially change from one unit to the other.Some synsedimentary normal faults can be observed cutting deposits of these two units, which probably contributed to the creation of accommodation and reflect the extensional tectonics that generated the compartmentalization of the region mentioned above.Shallow-water deposits including small coral patches early Tortonian in age also occur in the southern part of the Granada Basin, near Albuñuelas (Juncal, Rivas et al., 1999) (Fig. 1B).These corals grew on conglomerates fed from the antecedent relief of the Sierra de la Tórtola, located to the north (Fig. 1A).
The nearshore, shallow-water marine conditions continued with the installation of a delta system in the area, mainly recorded by delta front deposits.The total thickness of the deposits, about 70 m, suggests a moderate subsidence to keep accommodation to similar delta-front facies during all the succession of Unit 6.The change from a carbonate-dominated setting to a terrigenous system might indicate higher sediment input due to increased uplift rate of the emergent source uplands.The presumably perennial nature of the fluvial system suggests a period of more humid climatic conditions at the southern slopes of the antecedent relief of Sierra de la Tórtola-Sierra Nevada (Fig. 1A) during the early Tortonian.This interpretation, however, is not supported by the early Tortonian pollen records in the southern Iberian Peninsula, which indicate a vegetation dominated by herbs and shrubs characteristic of relatively arid scrublands (Jiménez-Moreno et al., 2010).The occurrence of coeval fine-grained siliciclastic deposits rich in Turritellinae and oyster banks, immediately south of Sierra de la Tórtola (Rivas et al., 1999) (Fig. 1), suggests a certain areal extension of shallow-marine environments with high nutrient levels.
The complete and permanent emersion of the area took place since the early Tortonian, with intense deformation by folding and faulting that affected the Miocene rocks (Avidad et al., 1978;Estévez et al., 1985;Sanz de Galdeano & López-Garrido, 2000).The most common faults are roughly NW-SE normal faults, which also occur at the transition from the Granada Basin to Sierra Nevada (Fig. 1), facilitating an ENE-WSW extension and the relative subsidence of the basin and uplift of the mountain range (Galindo-Zaldívar et al., 2019).The end of marine sedimentation and emergence of Los Guájares is coeval with the individualization of the Granada Basin under a geodynamic regime determined by NNW-SSE to N-S compression.Sierra Nevada, Sierra de la Tórtola and the Betic basement to the south (Fig. 1A) were folded forming large E-W antiforms (Avidad et al., 1978;Galindo-Zaldívar et al., 2019;Sanz de Galdeano & Alfaro, 2004).
Shallow-marine sedimentation continued to the north and east of Los Guájares valley, with deposition of terrigenous rudstones to packstones, unconformably overlying the Betic basement and older Miocene deposits (Avidad et al., 1978;Braga et al., 1996;Estévez et al., 1985;González-Donoso, 1978;Rodríguez-Fernández, 1982;Rustichelli et al., 2013).These limestones extend southward to the Ízbor valley section (Fig. 1B) and probably are the remnants of the connection of the Granada Basin with the Mediterranean Sea during the Tortonian.Overlying these limestones, upper Tortonian coral reefs and delta systems were the last marine deposits in the Granada Basin before its isolation from the open sea by the end of the Tortonian (Braga et al., 1990;Dabrio et al., 1982;Galindo-Zaldívar et al., 2019;García-Alix et al., 2008).
Quaternary deposits are scattered throughout the valley and surrounding areas at the foot of the reliefs.

Coral reefs in the context of the western Mediterranean
The isolated small coral colonies and the coral colonies building the small coral patches in Units 4 and 5 mainly belong to Tarbellastraea and Porites.Only one colony of Thegioastraea was found.Coral heads of Tarbellastraea and Porites intensely bored by bivalves were also reported in lower Tortonian deposits in the vicinity of Albuñuelas (Juncal, Rivas et al., 1999), about 10 km NW of the Los Guájares reefs (Fig. 1B).These are the only coral reefs confidently dated as early Tortonian known in the Betic Cordillera.The genus richness in these reefs is lower than the one in older Langhian reefs in the Granada Basin, in which 8 genera were reported (Braga et al., 1996), and lower than the richness in late Tortonian reefs, which comprise 7 genera in the Almanzora Corridor (Martín et al., 1989) (Fig. 1A).Both assemblages include the three genera found in Los Guájares.The lower genus richness of coral reefs in the early Tortonian is probably due to a sampling bias caused by the limited extension of outcrops with reefs from this age, although unfavorable conditions for reef development cannot be ruled out.In this regard, in the entire Mediterranean region, zooxanthellate corals of early Tortonian (and Serravallian?) age have only been reported in detritic facies in the Rhône Valley.They consist of isolated colonies of Tarbellastraea and Montastraea that did not build reefs (Chevalier & Demarq, 1964;Perrin & Bosellini, 2012).By contrast, upper Tortonian reefs have been described in tens of localities all over the Mediterranean (Perrin & Bosellini, 2012).This scarcity of records and the very low diversity in the known localities might be an artifact due to the difficulty of assigning a precise age to Upper Miocene shallow-water carbonates.It might be possible that some early Tortonian coral reefs or zooxanthellate-coral sites were considered late Tortonian in age just because these structures and fossils are more common in the latter interval.However, the very low number of records suggests a true rarity of zooxanthellate corals during the early Tortonian in the Mediterranean region.The global conditions in the early Tortonian were not favorable for coral reef development as the sea level fell more than 30 m in that interval and global temperatures were 3-4 °C cooler than in times before the Middle Miocene Climatic Transition (Miller et al., 2020;Perrin & Bosellini, 2012).This cooling is also reflected in the pollen records of the southern Iberian Peninsula with a decrease in thermophilus plants (Jiménez-Moreno et al., 2010).In the case of the Mediterranean, these unfavorable circumstances affected a zooxanthellate coral fauna already isolated from the Indo-Pacific and consequently with a limited genetic pool (Perrin & Bosellini, 2012, 2013).

Conclusions
Miocene rocks occur in the Los Guájares valley, about 35 km south of Granada, in small and tectonized outcrops on metamorphic rocks of the Alpujárride Complex of the Internal Zones of the Betic Cordillera.Six sedimentary units separated by unconformities were distinguished by mapping and logging the Miocene deposits.The lowest unit consists of upper Serravallian marls with planktonic foraminifera filling neptunian dykes and draping the Alpujárride dolomitic marbles.They are deep pelagic deposits formed on the basement under an extensional regime.The overlying red conglomerates and breccias indicate continental deposition after emersion of the region.These materials are roughly coeval of other continental deposits that extend over the Betic basement in the central and eastern sectors of the cordillera.Relative sea-level rise and marine flooding of the area are evidenced by grey conglomerates with marine fossils in the following unit.Shallow marine conditions continued during deposition of the next two units in the early Tortonian, as indicated by coralline algae, zooxanthellate corals and small coral reefs included in sandstones and sandy limestones.The last marine Miocene rocks are delta front deposits early Tortonian in age.The lithology and facies distribution suggest a proximal-distal gradient from north to south.The abundance of oyster banks and concentrations of Turritellines point to a paleoenvironment with high nutrient levels.
The Los Guájares area emerged after the early Tortonian.Basement and Miocene deposits were folded and faulted under NNW-SSE to N-S compression and erosion processes prevailed in the valley.
The coral patches in Los Guájares, together with the nearby coral heads in Albuñuelas are the only documented early Tortonian coral reefs in the Mediterranean region.
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Fig. 1 A
Fig. 1 A Simplified geological map of the Betic Cordillera and situation of the study area (Los Guájares valley, red square) in the Internal Zones.B Access roads to the Los Guájares valley and adjacent villages (yellow).Localities mentioned in the text marked with red stars

Fig. 5
Fig. 5 Idealized stratigraphic scheme of the Miocene rocks in the Los Guájares valley

Fig. 9 A
Fig. 9 A Rudstone with internal molds of Turritellines and clasts of quartzite and dolostone at the top of Unit 6 at Sect. 8. Scale in centimeters.B Thin-section micrograph of A with Turritellines and quartzite and dolostone clasts (sample GUA-TUR)