Introduction

Cretaceous strata are very well exposed around Khur, in the northern part of the Yazd Block, Central Iran. After early mapping surveys (Aistov et al. 1984), the Cretaceous succession was the subject of a joint Iranian–German research initiative in the last decade (see summary in Wilmsen et al. 2015), and the integrated stratigraphy, depositional environments, and geodynamic significance of individual formations and major unconformities were detailed in several publications (Wilmsen et al. 2013, 2018a, b, 2020). During a field survey in 2012, a dinosaur trampling site was discovered within the upper Campanian–Maastrichtian Farrokhi Formation and it was revisited and restudied in 2018. The aim of the current short note is the first report and scientific description of the site that supplements the sparse Mesozoic record of dinosaur tracksites from Iran (see Lapparent and Davoudzadeh 1972; Lapparent and Nowgol Sadat 1975; Ataabadi et al. 2005; Abbassi 2006; Kellner et al. 2012; Abbassi and Madanipour 2014; Abbassi et al. 2015, 2018), representing the youngest hitherto known occurrence. With our report, we also hope to stimulate further research on that topic in the area north of Khur where, in the future, additional and better-preserved tracks may emerge from the Farrokhi Formation.

Geological setting and stratigraphy

The study area is located in the north-western part of the Central-East Iranian Microcontinent (CEIM; Takin 1972), occupying a structural key position in the complicated plate tectonic puzzle of the Middle East and consisting of three structural units, the Lut, Tabas, and Yazd blocks, respectively (Fig. 1a). The CEIM, Northwest Iran, the Alborz Mountains, and the Binalud Mountains form the Iran Plate that, as an element of the ribbon-like Cimmerian terrane assemblage, split off from the northern margin of Gondwana towards the end of the Palaeozoic Era (Late Permian; e.g. Stampfli and Borel 2002; Shamanian and Hattori 2021). The northward-directed drift of the Cimmerian terranes opened the Neotethys, and their collision with the southern margin of Eurasia (Turan Plate) closed the Palaeotethys Ocean during the Late Triassic (e.g. Berberian and King 1981; Sengör et al. 1988; Saidi et al. 1997; Wilmsen et al. 2009). After its welding to Eurasia, the Iran Plate remained a tectonically highly mobile area in Jurassic times (e.g. Fürsich et al. 2003; Seyed-Emami et al. 2004; Taheri et al. 2009; Salehi et al. 2018; Wilmsen et al. 2021). During the Early Cretaceous, strongly subsiding marginal oceans formed around the CEIM (Tirrul et al. 1983; Babazadeh and De Wever 2004; Nasrabady et al. 2011; Kazemi et al. 2019; Pirnia et al. 2020), probably in response to counterclockwise vertical-axis rotation of the microplate (e.g. Soffel et al. 1996; Alavi et al. 1997; Besse et al. 1998; Cifelli et al. 2013; Mattei et al. 2015; Wilmsen et al. 2021) and the break-up of deep-seated faults along its margins. The convergence of Arabia and Eurasia led to the closure of the narrow oceanic basins fringing the CEIM during the latest Cretaceous to Paleogene (e.g. Omrani et al. 2013; Delavari et al. 2014; Kazemi et al. 2019 ).

Fig. 1
figure 1

modified from Aistov et al. 1984)

Structural and geological setting and lithostratigraphic framework of the Maastrichtian dinosaur tracksite in the Farrokhi Formation of Central Iran. a Main structural units and sutures of Iran; the small rectangle shows the study area near Khur in the northern part of the Yazd Block (compare to c). b Lithostratigraphy of the area around Khur, simplified after Aistov et al. (1984) and Wilmsen et al. (2015). c Location of the dinosaur tracksite (asterisk), ca. 10 km northwest of Khur at the southern flank of Kuh-e-Azizabad (geological base map

Full size image

The Cretaceous succession in the Khur area, northern Yazd Block, attains a thickness of up to 5 km and has been subdivided into two large-scale transgressive–regressive megacycles based on a major late Turonian–early Coniacian tectonic event (Wilmsen et al. 2015). The resulting tectonic unconformity is regionally expressed by a coarse-grained and in places very thick conglomerate at the base of the Haftoman Formation, associated with block-faulting and deep-cutting erosion. The widespread and uniform carbonate facies of the overlying Coniacian–upper Campanian Haftoman Formation (Fig. 1b) reflects the establishment of a large-scale epeiric carbonate platform and an intermittent decline of tectonic instability (Wilmsen et al. 2018a). In the late Campanian, marls of the lower Farrokhi Formation onlap a subaerial surface at the top of the Haftoman Formation north of Khur, while the platform persisted in the southern part of the study area (Fig. 1b). Renewed northward progradation of the platform in the latest Campanian resulted in an intercalation of a middle limestone tongue of the Farrokhi Formation in the area north of Khur, capped by another subaerial surface. Maastrichtian marls and thin-bedded, fine-grained limestones of the upper Farrokhi Formation onlap the subaerial surface and indicate somewhat deeper marine conditions across the study area towards the end of the Cretaceous Period (Wilmsen et al. 2012). With a basal conglomerate, Paleocene carbonates of the Chupanan Formation rest unconformably on the Cretaceous succession (Fig. 1b).

The Farrokhi Formation has broadly been dated as Campanian–Maastrichtian by Aistov et al. (1984). Allameh and Nejad (2017) reproduced an early Campanian to late Maastrichtian age in the type area based on planktic foraminifers but obviously included the upper Haftoman Formation into their analysis. Correspondingly, Wilmsen et al. (2018a) showed that north of Farrokhi, the eponymous formation starts above an unconformity at the top Haftoman Formation in the mid-late Campanian. Based on planktic foraminifers, the overlying lower marl member of the Farrokhi Formation is late Campanian to earliest Maastrichtian in age, including the Globotruncana aegyptiaca and Gansserina gannsseri zones (Elyasi, 2017). No age data are available for the middle limestone member of the Farrokhi Formation, but the overlying upper marl member has a latest early to late Maastrichtian age based on a diverse assemblage of planktic and benthic foraminifers (Elyasi 2017). Thus, a late early Maastrichtian age can be assigned to the tracksite at the top of the middle limestone member of the Farrokhi Formation (ca. 70 Ma according to the new GTS 2020; Gale et al. 2020).

Materials and methods

Two field surveys were conducted in 2012 and 2018, applying standard palaeontological and sedimentological field methods (e.g. Goldring 1999; Stow 2005; Tucker 2011). Field-based grain-size and component analyses using a hand-lens were detailed later by microfacies analysis of thin-sections that have been prepared from characteristic lithofacies identified in the field, using a Leica M125 stereomicroscope with a Leica DFC 420 digital camera capturing images in the optical pathway. The classification of carbonate rocks follows Dunham (1962). Taphonomic observations at the tracksite were accompanied by a detailed photo-documentation as well as measurements and descriptions of individual tracks, following the terminology of Leonardi (1987). The track-bearing surface was traced along-strike for about 2 km towards the southeast. Thin-sections are stored in the palaeozoological collections of the Museum für Mineralogie und Geologie (MMG), Senckenberg Naturhistorische Sammlungen Dresden (SNSD), repository MMG: AsK.

Results

Section and microfacies

The tracksite is located ca. 10 km northwest of Khur, north of the road to Farrokhi and south of a low-lying, E–W-trending mountainous elevation known as Kuh-e-Azizabad (co-ordinates: N 33.850600, E 55.031030; Fig. 1c). The exposed stratigraphic succession starts with thick-bedded limestones of the middle Farrokhi Formation (Figs. 1b and 2a). Along an iron-stained emersion surface, the limestones are unconformably overlain by marls and thin-bedded limestone of the upper Farrokhi Formation (Figs. 2a. b and 3). The succession is concluded by the thick-bedded, brown carbonates of the Paleocene Chupanan Formation, which rest along a major erosional unconformity on the Farrokhi Formation (Fig. 2a).

Fig. 2
figure 2

Field and microfacies aspects of the Maastrichtian dinosaur tracksite in the Farrokhi Formation of Central Iran. a Panoramic view of the stratigraphic succession at Kuh-e-Azizabad: middle limestone member of the Farrokhi Formation overlain by soft-weathering marls and thin-bedded limestones of the upper Farrokhi Formation, followed by the brown, thick-bedded carbonates of the Paleogene Chupanan Formation; the level of the tracksite is arrowed. b Detailed view of the track-bearing surface; note the patchy red staining of the surface and the superposition with thin-bedded grey marls and limestones of the upper member of the Farrokhi Formation. c Well-sorted intra- and bioclastic packstone of the uppermost bed of the middle limestone member of the Farrokhi Formation in which the tracks are imprinted (sample 181016–3). d The transgressive strata of the upper marl member of the Farrokhi Formation sealing the track-bearing surface are composed of fine-grained skeletal wackestone with small benthic foraminifera and ostracods (sample 181016–4)

Full size image
Fig. 3
figure 3

Detailed stratigraphic log of the Maastrichtian tracksite interval observed at the boundary from the middle to the upper member of the Farrokhi Formation of Central Iran

Full size image

The contact between the middle and the upper member of the Farrokhi Formation is marked by an irregular surface with a relief of up to 20 cm and patchily distributed ferruginous pigmentation (Figs. 2b and 3). At this level, the footprints were observed. The underlying beige-brown limestones are well-sorted bio- and intraclastic packstones containing intraclasts, bahamite peloids, small shell fragments of bivalves and echinoderms, as well as small agglutinating and miliolid foraminifers (Fig. 2c). The thin-bedded limestones and marls of the lowermost part of the upper member of the Farrokhi Formation that are sealing the relief at the top of the middle member are slightly silty, fine-grained bioturbated wackestones with small benthic foraminifers, ostracods, and microbioclasts (Fig. 2d). On elevated parts of the contact surface, bivalve borings were observed (Fig. 3).

At the described site, a small ephemeral creek provided clean exposures of the contact surface between the middle and the upper member of the Farrokhi Formation. We followed the track level for about 2 km along-strike at the southern flank of Kuh-e-Azizabad but could not find a better exposure. Only some indifferent impressions were observed at places, showing that tracks potentially have a wider distribution on the surface.

Tracksite and track description

The tracksite comprises a surface of approximately 20 m2 (10 × 2 m), which is riddled with predominantly irregular, indifferent depressions 10 to 50 cm in diameter (Fig. 4a). The depressions, identified as tracks, are between 7 and 14 cm deep and commonly have steep margins with raised rims. In some cases, individual imprints are superimposed, forming composite, laterally coalescing depressions (Fig. 4a, b). According to lateral and vertical relationships as well as to the different fabrics of the impressions, two generations of imprints can be identified. The first generation is impressed into beige-brown carbonates and shows very irregular shapes and outlines, including the formation of sub-parallel bulges and overhanging margins (Fig. 4b, c). No cracking of the substrate or iron-staining has been observed with these imprints. The second generation is associated with a ferruginous staining and a conspicuous cracking pattern (Fig. 4e–i). The sloping margins of, and raised bulges between, individual impressions are cracked and partly elevated by having been squeezed-up (Fig. 4h, i), forming a polygonal shard pattern. In several cases, elongated cracks trace the outline of individual impressions, but short cracks also extend in a radial fashion. Better preserved individual footprints include a tridactyl impression more than 50 cm wide (Fig. 4d), sub-circular to oval imprints with differentiated terminations on one side (Fig. 4e, f) and a deeply indented acute termination superimposed onto a sub-circular track (Fig. 4g).

Fig. 4
figure 4

Photo-documentation of the Maastrichtian dinosaur tracksite in the Farrokhi Formation of Central Iran. a General view of the central part of the exposed track layer; note steep margins and elevated bulges (length of hammer: 33 cm). b Trampled surface without cracks (first generation of tracks); note partly overhanging walls and the absence of the iron-staining (28-cm-long hammer gives scale). c Detail of b: subparallel bulges testify the non-lithified, muddy nature of the substrate when these tracks were produced (length of hammer: 28 cm). d Tridactyl imprint more than 50 cm in width (length of hammer: 33 cm). e Sub-circular footprint with a one-sided terminal differentiation towards the top of the image (digit traces?); lens cap 55 mm in diameter. f Another sub-circular footprint with a one-sided differentiation (top of image); note the concentric crack pattern around the imprint (lens cap 55 mm in diameter). g Potential claw imprint; note the cracking of the hardened upper surface when the soft substrate below has been indented (lens cap 55 mm in diameter). h Composite impression with cracked margins and bulges (length of pencil sharpener: 25 mm). i Detail of a cracked bulge; note sub-parallel nature of cracks (length of pencil sharpener: 25 mm)

Full size image

Discussion

There is only a very sparse Mesozoic record of dinosaur tracks from Iran (Lapparent and Davoudzadeh 1972; Lapparent and Nowgol Sadat 1975; Ataabadi et al. 2005; Abbassi 2006; Kellner et al. 2012; Abbassi and Madanipour 2014; Abbassi et al. 2015, 2018). The bulk of the records is from the Lower and Middle Jurassic Ab-Haji Subgroup of the Shemshak Group of northern and Central Iran, and the uppermost Jurassic Ravar Formation of the Kerman area. The only Cretaceous reports so far are rather small sauropod and stegosaur footprints from Aptian strata of the Tirgan Formation of the Koppeh Dagh Basin in northeastern Iran (Abbassi et al. 2018).

The general appearance of the surface suggests that it represents a kind of “trampled dinosaur parade”. Such kind of indifferent dinosaur-induced bioturbation produced by individuals clattering around has been termed “dinoturbation” (Dodson et al. 1980; see also Thulborn 1990; Lockley 1991). According to the relative degree of trampling, a moderate dinoturbation index can be assigned to the Farrokhi site (cf. Lockley and Conrad 1989). The imprints can be classified as natural moulds (i.e. concave epireliefs sensu Leonardi 1987) with footprints bordered by a raised rim of displaced sediment (see Leonardi 1987; Thulborn 1990). The two generations described above were probably made at different times based on the different modes of preservation of the footprints. The first (earlier) generation was imprinted into a soft substrate (fine-grained carbonate sand with micritic matrix) that was squeezed out under the load of the trampling animal. Due to its consistency, the substrate was deformed without rupturing. The existence of overhanging walls suggests that the traces were preserved as undertracks and the created relief was immediately filled with overlying, still softer sediment. Details of the imprinting feet could not be preserved because the sediment was too soft (see also Sarjeant and Leonardi 1987). The second (later) generation was made some time afterwards when the layer had become superficially hardened. When loaded, the hardened surface failed and the trackmakers sunk into the still plastic layer below. However, again the substrate did not have the ideal consistency to preserve any details of the footprints, as below the few centimetres-thick hardened layer, the sediment was still soft. As a result, a rather irregular morphology was created, bordered by raised rims of displaced sediment covered by a cracked, mosaic-like layer. It is also possible that the cementation took place not right at the top surface but some centimetres below. The iron-staining was most likely formed under persistent subaerial exposure under (semi-)arid conditions and accompanied by further lithification of the surface. Similar climatic conditions have been proved for the underlying platform carbonates of the Coniacian–Campanian Haftoman Formation by the occurrence of intercalated red beds, gypsum nodules, and iron-stained karst surfaces (Wilmsen et al. 2018a).

The small sauropod and stegosaur footprints reported from Aptian strata of the Tirgan Formation of the Koppeh Dagh (NE Iran) were produced under subaerial conditions in an intertidal environment (Abbassi et al. 2018) and several other Mesozoic dinosaur tracksites have been reported from inter- to supratidal settings (e.g. Marty et al. 2003, 2018; Marty 2008; Razzolini et al. 2016); the same conditions apply for the footprints in the Maastrichtian Farrokhi Formation. Putting all available data together, a genetic model for the formation of the surface yielding the tracksite can be developed (Fig. 5): progressive shallowing towards the top of the middle member of the Farrokhi Formation during the late early Maastrichtian caused extremely shallow conditions and a first trampling of the soft, water-saturated sediments occurred (first generation of imprints; Fig. 5a). Subaerial exposure resulted in a subsequent initial hardening of the surface (Fig. 5b) or of a sediment layer some centimetres below the surface. At this stage, a second generation of footprints was imprinted, characterised by the conspicuous cracking patterns around the tracks (Fig. 5c). Further lithification of the layer during a subsequent prolonged emersion period produced a true hardground that became iron-stained under the prevailing (semi-)arid climate (Fig. 5d). This composite surface was bored by bivalves during the following late Maastrichtian transgression (Fig. 5e) and draped by fine-grained calcareous offshore sediments of the upper marl member of the Farrokhi Formation when accommodation was created during progressive deepening (Fig. 5f). An alternative interpretation for the differential preservation of the footprints may be that the two types of footprints are contemporaneous and the substrate consistency changed laterally (e.g. by the persistence of small ponds on the developing emersion surface). In this case, stages a and c in Fig. 5 need to be merged into one time slice.

Fig. 5
figure 5

Genetic model for the development of the Maastrichtian dinosaur tracksite found in the Farrokhi Formation of Central Iran from older below (a) to younger above (f) (not to scale; the successive trampling is shown in opposite directions for better differentiation of the two track generations). a First generation of tracks produced under very shallow conditions in a soft, fine-grained carbonate sand with micritic matrix (uppermost part of the middle limestone member of the Farrokhi Formation). b Emersion and initial hardening of the trampled surface following continuous relative sea-level fall. c Second generation of tracks imprinted into superficially hardened sediment that was still plastic underneath; conspicuous cracking pattern developed around imprints. d Subsequent long-term exposure of the surface caused subaerial lithification of the strata. e During the following late Maastrichtian transgression, the hardground was patchily bored by bivalves. f Further deepening during the late Maastrichtian transgression created accommodation and the composite surface was sealed by fine-grained, calcareous offshore sediments of the upper marl member of the Farrokhi Formation

Full size image

Based on the poor preservation of the footprints, mainly related to the unfavourable substrate conditions (cf. Sarjeant and Leonardi 1987; Marchetti et al. 2019), we can neither comment on the trackmakers nor on the ichnotaxonomic affinity of the traces. We have several round to oval footprints (Figs. 4e, f and 6a–c), one tridactyl form (Figs. 4d and 6e), a possible claw trace (Fig. 4g), and composite tracks resulting from repeated trampling of the surface (Figs. 4a, h and 6f–h); the numerous round to faintly oval imprints may be related to quadrupedal trackmakers, most likely sauropods, but no detailed conclusions are possible based on the poor to very poor morphological preservation of the tracks (cf. Marchetti et al. 2019). Consequently, the track surface in the Farrokhi Formation provides only a general indication of the passage of dinosaurs in an inter- to supratidal environment but very little information can be obtained about the potential trackmakers. Nevertheless, the occurrence enhances our knowledge on the preservation of dinoturbation in different kinds of substrates. Furthermore, the young, foraminifer-calibrated late early Maastrichtian age at the top of the middle limestone member of the Farrokhi Formation (cf. Elyasi 2017; ca. 70 Ma according to the new GTS 2020; Gale et al. 2020) places the tracksite in the evolutionary twilight close to dinosaur extinction at the end of the Cretaceous Period. The site is among the youngest dinosaur tracksites worldwide (e.g. Difley and Ekdale, 2002; Vremir and Codrea, 2002; Vila et al., 2013; Flaig et al., 2018; Meyer et al., 2021) and is by far the youngest record from Iran (see references above). Furthermore, there are only a few Cretaceous dinosaur tracksites known from the Middle East at all (e.g. Avnimelech 1962; Schulp et al. 2008; Gèze et al. 2016; Klein et al. 2020) that are all significantly older, and it thus appears that the discovery from the Farrokhi Formation of Central Iran is also the youngest record in the entire Middle East.

Fig. 6
figure 6

Outlines of different tracks observed. a–d Sub-circular to faintly oval imprints (possible sauropod tracks) with (d) showing a superimposed potential claw imprint. e Tridactyl imprint. f–h Composite tracks resulting from repeated trampling of the substrate

Full size image

Conclusions

A Maastrichtian dinosaur tracksite from northwest of Khur is reported from the Farrokhi Formation of Central Iran. It has been found at the junction of the middle to the upper member of the Farrokhi Formation and it was associated with subaerial exposure in a tidal flat environment. Biostratigraphic data indicate a late early Maastrichtian age for the tracks. The largely indeterminate footprints represent natural moulds (= concave epireliefs) bordered by raised rims of displaced sediment. Two generations of footprints were imprinted under extremely shallow to subaerial conditions related to an episode of sea-level fall, firstly into a soft fine-grained carbonate sand and, at a later stage, into a partially cemented substrate that was underlain by still plastic sediment. Evidence of partial lithification is a conspicuous cracking pattern around the footprints. Further lithification of the track-bearing surface was followed by formation of an iron-stained hardground. Finally, the dinoturbated horizon was sealed by the upper member of the Farrokhi Formation during the following late Maastrichtian transgression. Unfortunately, no anatomical details of the foot morphologies of the producers were recorded due to the unfavourable substrate conditions, and we thus can neither comment on the actual trackmakers nor on the ichnotaxonomic affinity of the traces. Nevertheless, the surface documents a kind of trampled dinosaur parade, representing a fine case of dinoturbation. Moreover, it is the youngest record (ca. 70 Ma) of dinosaur locomotion traces from Iran and, to the best of our knowledge, from the entire Middle East.