Article number: 22.3.56
Copyright Paleontological Society, September 2019
Submission: 29 Jukly 2018.. Acceptance: 12 August 2019.
A fish fauna newly discovered in the middle Eocene marine sediments cropping out near the village of Luna de Sus, Romania, completes the fossil record of the Eastern European region. Teeth belonging to 15 species of Chondrichthyes and two species of Actinopterygii are herein recorded from the lowermost Bartonian deposits. These Paleogene fish document a marine tropical environment of medium deep waters in the northwestern area of the Transylvanian Basin. The vertical distributions of extant equivalent taxa allow a sea depth estimation of 100 to 200 m. The warm climate is documented by both the present faunal assemblage and previous palynological studies. It is important to note the presence of the scarcely known and poorly understood pycnodont species Phacodus punctatus and of the oldest representative of Labridae from this Carpathian area. The diversity of the fauna was found to be average compared to some areas from Western Europe or North Africa, but it falls within the regional diversity range of the Eastern European localities.
Nicolae Trif. Department of Geology, Faculty of Biology-Geology, Babeş-Bolyai University, 1 Kogălniceanu St., 400084, Cluj-Napoca, Romania and Brukenthal National Museum, Natural History Museum, Sibiu, Romania, 1 Cetății St., Sibiu, 550160, Romania.
Vlad Codrea. Department of Geology, Faculty of Biology-Geology, Babeş-Bolyai University, 1 Kogălniceanu St., 400084, Cluj-Napoca, Romania.
Viorel Arghiuș. Environmental Sciences Department, Faculty of Environmental Sciences and Engineering, Babeş-Bolyai University, 30 Fântânele St., 400294, Cluj-Napoca, Romania.
Keywords: sharks; bony fish; Eocene; Căpuș Formation; Tethys Sea
Final citation: Trif, Nicolae, Codrea, Vlad, and Arghiuș, Viorel. 2019. A fish fauna from the lowermost Bartonian of the Transylvanian Basin, Romania. Palaeontologia Electronica 22.3.56. 1-29. https://doi.org/10.26879/909
Copyright: September 2019 Paleontological Society.
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Eocene-age fish teeth in the Transylvanian Basin were first described in the 1850s by Neugeboren (1850, 1851), who listed material belonging to 65 species of sharks from the southern side of this sedimentary basin. Almost half a century later, Koch (1894) reported a few new occurrences of Eocene fish teeth (again, mostly sharks) originating from the northwestern side of the basin. It is likely that in Koch's list, both middle and upper Eocene strata were represented, but the actual stratigraphy could not be confidently determined from this work. This same author appended these data to a larger subsequent list that includes the former Austro-Hungarian Empire (Koch, 1900). Following these researchers, only a handful of geologists focused on this topic, surveying mostly the northwestern area of the basin. The first one was Fuchs (1963, 1966), who described some fragmentary Myliobatis teeth from the Priabonian of Cluj-Napoca surroundings. The diversity of the Eocene fish fauna only started to be revealed a couple of decades later (Șuraru et al., 1980; Șuraru and Șuraru, 1987), but these studies focused exclusively on the same geological age. The list of Priabonian species has been supplemented again in the final decade of the last century (Dica et al., 1996; Codrea et al., 1997). The first definite mention of the middle Eocene fish fauna was at the beginning of the twenty-first century in an unpublished Ph.D. thesis (Dica, 2006). From the type locality of the Căpuș Formation (Căpușul Mic), Jaekelotodus sp., Striatolamia macrota (Agassiz, 1843), Myliobatis sp., Aetobatus irregularis (Agassiz, 1843) and Pycnodontidae indet. have been illustrated and described.
Recent surveys of the middle Eocene deposits of the Luna de Sus locality revealed a rich assemblage of fish teeth, a rostral and a dermal spine, and a tail sting. Luna de Sus is situated on the northwestern side of the Paleogene Transylvanian Basin, central Romania, at about 10 km westward from the city of Cluj-Napoca (Figure 1). This paper is the first to describe this locality for fossil fishes in Romania.
According to the paleogeographic reconstructions of the Tethys Sea (Meulenkamp and Sissingh, 2003), during the late Lutetian, the north-western area of the recent Transylvanian Depression was part of a Paleogene sedimentary basin covered by a shallow sea spreading over the thrusting nappes of the Apuseni Mountains landmass. To the east, this sea was in connection with the Eastern Carpathians Paleogene Flysh trough (i.e., the outer “Moldavides”, sensu Săndulescu, 1984). The Căpuş Formation (Popescu, 1978) of middle Eocene age is exposed in the northwestern area of the Transylvanian Basin (Gilău sedimentary area; Rusu, 1987).
The sedimentology illustrates a paleoenvironment of an inner continental shelf of an open sea with a tidal regime (Rusu et al., 2004). The formation consists mainly of marls bearing several important mollusk biohorizons with regional distributions useful for correlating these deposits. Its basal segment represents the level with Pycnodonte brogniartii Bronn, 1831, while the top bears the level with Nummulites perforatus Montfort, 1808 (Figure 2.1). The latest geological study shows that the age of the formation is Lutetian-Bartonian, but only its basal portion is Lutetian, with the remaining portion belonging to the Bartonian (Rusu et al., 2004).
The outcrop is situated on a very steep ravine, a right tributary of the Feneș Creek, on the southern side of the village of Luna de Sus. Its left bank is covered by a landslide; therefore, the main interest is restricted to only a few meters on the right bank of the ravine. The nearest equivalent outcrops situated at 650 m south-west, 400 m east and 80 m north of the gully did not reveal any fish fauna.
The Luna de Sus lithostratigraphic log is over 10 m thick, including: 7 m of marls bearing a basal Pycnodonte brongniarti lumachelle; 0.1 m marl with Sokolovia eszterhazyi Pávay, 1871, lumachelle; 0.17 m calcareous sandstone with some microconglomerate elements. The last two layers are where the fish remains were found. Above these layers there is a very thin (0.07 m) layer of quartz microconglomerate followed by 1 m of clayey shale and 2.4 m of marls bearing lumachelle of Nummulites perforatus. The outcrop exposes rocks of a geological age very close to the lowermost Bartonian, just above the Lutetian/Bartonian boundary (Figure 2.2).
MATERIAL AND METHODS
The specimens were collected during 20 short field excursions, from March 2009 to September 2017. The photographs were taken with a Nikon D80 camera mounted on a Nikon SMZ 1000 binocular microscope and with a Nikon D700 camera and a 105 mm Sigma lens. The described material is stored at the Faculty of Environmental Science and Engineering, Babeș-Bolyai University, Cluj Napoca, Romania (abbreviated hereinafter, FES). The single exception is the VT459 specimen donated to the Babeş-Bolyai University Paleontology-Stratigraphy Museum in Cluj Napoca (abbreviated hereinafter, BBUPSM). The taxonomic identification of the described material included a comparison with the high-resolution images of the holotype and paratypes of Macrorhizodus nolfi Zhelezko, 1999, from the Darwin State Museum, Moscow (DSM) and of the holotype of Phacodus punctatus Dixon, 1850, from the Natural History Museum, London (NHM). The systematic paleontology part follows Cappetta (2012) and Last et al. (2016a). The use of the name Otodus Agassiz, 1843, follows Cappetta (2012), and it includes Carcharocles as a subgenus. The terminology follows Deynat (1998), Cappetta (2012) and Hovestadt and Hovestadt-Euler (2013).
During the field excursions about 175 kg of sediment (sandstone) was collected. The high iron content of the sandstone made it somewhat inert to the acetic acid reaction that was used to dissolve the rock. Therefore, the process of disaggregation has been tedious and time consuming. A 0.5 mm mesh sieve was used to sieve the resulting sediment. The disaggregation of the sandstone samples together with the direct field collecting yielded ca. 75 fish teeth, rostral and dermal spines and a tail sting.
Class CHONDRICHTHYES Huxley, 1880
Subclass ELASMOBRANCHII Bonaparte, 1838
Order HETERODONTIFORMES Berg, 1937
Family HETERODONTIDAE Gray, 1851
Genus HETERODONTUS Blainville, 1816
Material. Two teeth (FES 045 and 098).
Description. Both teeth are small. Only the specimen FES 045 is complete, with a length and width of 8.1 by 3.2 mm. The teeth are labio-lingually compressed and mesio-distally elongated. A reticulated ornamentation is present on the labial side. The reticulation becomes smaller and finer towards the labial edge. The lingual face has an ornamentation of weak parallel ridges perpendicular to the mesial-distal direction. A longitudinal main ridge is present on the same direction, interrupted by a large central bump (in FES 098), or by a central massive functional wear facet (in FES 045). In occlusal view, the specimen FES 045 has a general sigmoid shape, with a rounded end in the mesial direction and an angled, pointed one distally. The crown overhangs the root in all directions. The root is low and flat. We cannot observe any marginal lingual or labial foramina because of some strongly cemented sediment adherent to the root.
Remarks. There are several Eocene species of Heterodontus: H. pineti Case, 1981 (Priabonian, Georgia, USA), H. vincenti Leriche, 1905 (Lutetian, Belgium) and H. wardenesis Casier, 1966 (Ypresian, England). Unfortunately, the preservation status of the fossils at our disposal does not allow us an assignation below the genus level.
Order CARCHARHINIFORMES Compagno, 1977
Family CARCHARHINIDAE Jordan and Evermann, 1896
Subfamily CARCHARININAE Jordan and Evermann, 1896
Genus RHIZOPRIONODON Whitley, 1929
Rhizoprionodon ganntourensis Arambourg, 1952
Material. Two teeth (FES 076 and 082).
Description. The teeth are small, their height around 2.5 mm and their width of almost 4 mm. The cusp is strongly bent distally. No cusplets are present, but the tooth exposes a distinct distal heel. The mesial side is elongated and slightly convex. The labial base of the enamel is quasi rectilinear, while on the lingual side it is slightly arched. The root foramen is small, oval and shifted distally.
Remarks. The teeth of this genus are characterized by a distinct gynadric heterodonty (Cappetta, 2012). In males, the central part of the cusp is thicker, and the mesial cutting edge is less convex. Our specimens are strongly compressed in the labial-lingual direction, and the central part of the cusp is strongly bent towards the rear. We interpret our specimens as belonging to females. According to Cappetta (1987), the teeth of this genus are very similar to the ones found in the Scoliodon and Loxodon genera. No progress has been made so far in the last quarter century to settle this issue, and the data remain the same in the more recent works (Cappetta, 2012).
Only a single Eocene species is known, Rhizoprionodon ganntourensis. The species is also present in the middle Eocene (Lutetian) of Morocco (Arambourg, 1952), Uzbekistan (Case et al., 1996), Togo (Cappetta and Traverse, 1988), the upper Eocene of France (Cappetta and Nolf, 1981), as well as the Eocene (Ciobanu, 2002) and the upper Eocene (Priabonian) of Romania (Dica, 2006).
Subfamily GALEOCERDINAE Whitley, 1929
Genus GALEOCERDO Müller and Henle, 1838
Galeocerdo cf. eaglesomei White, 1955
Material. Two incomplete teeth (FES 043 and 044).
Description. The teeth are broad but also high, with a triangular crown that bears a central distinct cusp inclined distally. FES 043 is 15 mm wide and 12 mm tall, while FES 044 is 15 mm wide and 10 mm tall. The mesial cutting edge is slightly convex in one specimen and completely straight in the other one, and it has numerous serrations that get smaller towards the apex of the crown. The distal cutting edge is almost straight, with serrations increasing towards the middle. No nutritive groove can be observed on the lingual surface of the root, but this could be due to its poor state of preservation. Both mesial and distal cutting edges of the main cusp are irregularly serrated. The serration of the main cusp covers two thirds of its length. The root is only partially preserved on both specimens. Specimen FES 044 probably had a very lateral position towards the commissure. It is interesting to note the possible formation of a possible secondary serration in specimen FES 043 (Figure 4.1').
Remarks. At least three Eocene species of Galeocerdo are known from the Eocene: G. latidens Agassiz, 1843, G. aegyptiacus Stromer, 1905 and G. eaglesomei White, 1955. Another possible species, named Galeocerdo sp., from the Fayoum Depression of Egypt, has also been described (Case and Cappetta, 1990).
We found Galeocerdo eaglesomei to be the species most similar to our material, with a comparable serration that extends closer to the tip of the cusp. The tall root is a morphological element also found in our material. The size of the tooth and the presence of the serration on the main cusp differentiate our fossils from the species G. latidens. Galeocerdo aegyptiacus from the Eocene of the Fayoum Depression (Egypt) differs from our material in being smaller in the basal-apical direction and with a more convex mesial edge. Galeocerdo sp. is similar to our specimens, but it has a smaller serration on the lateral heels. This unnamed species is considered to be distinct from G. latidens, G. eaglesomei and G. aegyptiacus (Underwood et al., 2011). Due to the fragmentary status of the fossils we have at our disposal, we keep our assignment to Galeocerdo cf. eaglesomei.
The species Galeocerdo eaglesomei can also be encountered in the middle Eocene of Texas (Westgate, 1989), Alabama (Maisch et al., 2014), the upper Eocene of Mexico (Gonzales Barba, 2003), the Eocene of Nigeria (White, 1955) and Egypt (Underwood et al., 2011).
Ciobanu (2002) documented Galeocerdo (as G. latidens) from the Eocene of Turnu Roșu, Romania.
Genus PHYSOGALEUS Cappetta, 1980
Physogaleus secundus Winkler, 1876
Material. Three lateral teeth (FES 050, 051, 052) and one antero-lateral tooth (FES053).
Description. The lateral teeth measure only 6 to 8 mm mesio-distally and 4 to 5 mm in the apical-basal direction. The main cusp is inclined distally and has a triangular shape. The mesial side of each tooth is long, almost straight, slightly convex with two very irregular cusplets. The distal edge is shorter and continues with two strong and triangular cusplets that are bent distally more than the main cusp. The teeth are labio-lingually compressed. On the lingual face the enameloid covers about half of the root height and forms a straight crown-root contact, while on the labial side the contact has an arched shape. The lingual side of the root has a deep central furrow while the labial side has only some dispersed foramens.
The antero-lateral tooth measures 6.5 mm mesio-distally and 5.5 mm in the apical-basal direction. The main cusp is narrower than that of the lateral teeth. The mesial edge is straight but incomplete at its base. The distal edge is shorter than the mesial one but the distal cusplets are smaller and not as well outlined as they are in the lateral teeth. The root has a much more pronounced lingual protuberance than that of the lateral teeth and the central furrow is very deep.
Remarks. Four Eocene species of Physogaleus are known: P. tertius Winkler, 1874, P. latecuspidatus Müller, 1992, P. secundus Winkler, 1876 and P. americanus Case, 1994. The species P. latecuspidatus is easily differentiated from P. secundus by a wider main cusp, especially towards the tip of the crown, hence its very illustrative name. Physogaleus americanus is a much smaller species with teeth of around 3.0 mm and with a distinct cusp on the mesial side. Physogaleus tertius lacks cusplets in the lateral teeth; it only has a wavy lateral edge that Case (1994 p. 121) considered an “unerupted ridge”. We acknowledge another poorly known species, P. rosehillensis Case and Borodin, 2000, described from a single tooth. Taking into account the limited description and the poor material, we will not consider P. rosehillensis further, as it lacks sufficient differentiating characters.
The morphology of our specimens is very similar to one of the specimens figured by Cappetta (2012, fig. 297), except for the labio-lingual compression, which is more pronounced in our teeth. We feel confident to assign our specimens to Physogaleus secundus.
Physogaleus secundus is common in the Eocene of Europe and Africa. The species is also found in the lower-middle Eocene of Denmark (Carlsen and Cuny, 2014), the Lutetian of Belgium (Eckhaut and De Schutter, 2009), the Ypresian of Morocco (Noubhani and Cappetta, 1997) and the Eocene of Romania (Ciobanu, 2002; Dica, 2006).
Genus ABDOUNIA Cappetta, 1980
Description. The teeth measure only 7.4 mm (FES 057) and 4.5 mm (FES 056) high in the apical-basal direction. The main cusp is triangular with a straight contact between the crown and the root on the labial side. The lingual side is convex. The lateral tooth has some very faint folds at the base of the crown, on the labial side. The cusplets on both teeth are triangular, divergent and not separated by the crown on the labial side.
Remarks. Based on the described morphology we assign our material to Abdounia sp. as it resembles closely the description of the genus in Cappetta (2012, p. 308). The scarce material and the imperfect preservation of the specimens prevent us from assigning a species. The genus Abdounia is common in the Eocene of Africa, Europe and Americas with at least seven valid species.
Order LAMNIFORMES Berg, 1958
Family LAMNIDAE Müller and Henle, 1838
Genus MACRORHIZODUS Glikman, 1964
Macrorhizodus praecursor (Leriche, 1905)
Material. Two teeth (FES no 041 and 042).
Description. The morphology of the specimens indicates a lateral position. The specimen FES 041 is 49 mm high and 49 mm wide while specimen FES 040 is 40 mm high and 41 mm wide. Both teeth have a triangular crown that is inclined slightly distally. The base of the crown is continued by a heel on both sides. The heels are raised on both sides of the tooth forming an almost straight cusplet. The contact of the crown with the root follows a straight line. The root lobes are slightly asymmetrical; the distal lobe has a sub-rectangular outline, and the mesial lobe is pointed and a little bit elongated. The specimen FES 041 has a visible central foramen on the lingual face of the root.
Remarks. Two species and a subspecies of Macrorhizodus are presumed to be present in the Eocene: M. praecursor (Leriche, 1905), M. praecursor americanus (Leriche, 1942) and M. nolfi Zhelezko in Zhelezko and Kozlov, 1999. The differences are based on the outline of the crown, the outline of the root lobes and the presence of so-called heel bumps (or vestigial cusplets), respectively.
Malyshkina and Ward (2016) consider that the presence of high lateral cusplets (or heels) separates the species Macrorhizodus nolfi from M. praecursor, but they note that the characteristics that separate the two species are unclear. Compared with M. praecursor (illustrated by Cappetta, 2012, figure 207 A-P), M. nolfi (as figured in Zhelezko and Kozlov, 1999, pl. 28, figs. 3a, 3b, 4a, 4b) has fully formed lateral cusplets.
Observations using high-resolution images of these cusplets of the holotype (no. KP OF 15478/41 DSM) and of the paratype (KP OF 15478/43 DSM) indicate that these cusplets are high and triangular. We also observed that the cusplets are positioned towards the margin in M. praecursor and are closer to the main cusp in M. nolfi. The root in M. nolfi is clearly higher than in the specimen of Macrorhizodus praecursor figured by Leriche (1906, pl. 16, figs. 12 and 12a), but similar to the specimen of M. praecursor figured by Cappetta (2012). Ignored for a long time, the existence of the sub-species M. praecursor americanus has been re-evaluated in recent decades and is mentioned only rarely in the literature. However, we consider the differences between M. praecursor and M. praecursor americanus to be too subtle and rather unclear. Cappetta (2012) regards M. praecursor americanus as valid and specific to Priabonian. We assign our specimens to Macrorhizodus praecursor due to the low development of the lateral heels and have decided not to assign the material to the sub-species level.
Family MITSUKURINIDAE Jordan, 1898
Genus STRIATOLAMIA Glikman, 1964
Striatolamia macrota (Agassiz, 1843)
Figure 5.5-7', 10-11
Material. Three anterior teeth (FES 068, 069, 070) and five lateral teeth (FES 058, 059, 067, 091, 103).
Description. The anterior teeth measure up to 46 mm apico-basally and up to 21 mm mesio-distally. The teeth are straight or trend slightly distally. The labial face is strongly convex in the lower third of the tooth, while the upper two thirds is flat. The lingual side is strongly convex and has faint vertical striations mostly in the lower half of the crown. The cutting edges are sharp and continuous but do not reach the base of the crown. One pair of very short but sharp lateral cusplets is present in two of the teeth. The cusplets do not reach the crown and are more pronounced on the labial side. The root lobes are long and pointed, with the exception of one specimen, whose distal lobe is more flattened. The lingual furrow is barely visible.
The lateral teeth have a main cusp with a distal inclination. The mesial edge is slightly convex in the upper third and has a distal cutting edge that is slightly concave in the lower third. The lingual face of the crown is flat and smooth while the labial face is slightly convex. The lingual face is ornamented with very weak, parallel striations. These striations extend only as far as the middle part of the crown in the apical-basal direction. In some specimens the striations are completely absent. The root lobes are rounded with the mesial lobe being the longest. The cusplets are well differentiated from the main cusp and have a rounded-triangular shape.
Remarks. Two species of Striatolamia are known, S. striata Winkler, 1876 and S. macrota Agassiz, 1843. S. striata is known only from the Paleocene (Müller, 1992; Dutheil, 1992; Smith et al., 1999; Moreau and Mathis, 2000), and it appears restricted to this age (Cappetta, 2012). Striatolamia macrota is very common in Ypresian, Lutetian (Cappetta, 2012) and Bartonian (Zhelezko and Kozlov, 1999). The characters we described and the geological age clearly indicate that these teeth are from Striatolamia macrota. The same features, including the faint striations of the adult specimens, have been reported by Zhelezko and Kozlov (1999) and Cunningham (2000).
Family OTODONTIDAE Glickman, 1964
|Genus OTODUS Agassiz 1843 (sensu Cappetta, 2012)
Otodus (Carcharocles) sp.
Material. One fragmented tooth (FES 071).
Description. The root measures 51 mm wide and both lobes are rounded. A single strong, wide and unevenly serrated cusplet is present on either side of the central cusp.
Remarks. The morphology agrees with that of Otodus (Carcharocles) auriculatus, a large shark from the middle Eocene, but the species could not be positively determined due to the lack of a main cusp.
Family ODONTASPIDIDAE Müller and Henle, 1839
Genus HYPOTODUS Jaekel, 1895
Hypotodus verticalis Agassiz, 1843
Material. One tooth (FES 061).
Description. The tooth has a triangular cusp with a broad base and smooth labial and lingual sides. The lingual side is convex, while the labial one is flat and has a medial vertical ridge. In distal view the crown is almost straight. Only one pair of cusplets is present on the sides of the crown from which they are separated by a rounded notch. The root lobes are moderately long and have pointed ends. The distal lobe is shorter than the mesial one. The lingual protuberance of the root is sharply outlined and bears a central, pronounced furrow.
Remarks. Although somewhat similar in general morphology, Hypotodus clearly differs from Jaekelotodus by lacking the enameloid that covers the upper part of the root lobes. Also, the labial side of Hypotodus is convex to a certain extent, while the labial side of Jaekelotodus is flat and has a clear basal depression.
The validity of this genus has been widely disputed. Over the years, authors such as Casier (1946), Gurr (1962), Herman (1977) and Ward (1988) misleadingly illustrated teeth belonging to other taxa but which they attributed to Hypotodus. Their opinions often changed the allocation of its sole species H. verticalis, from Hypotodus to other genera, hence invalidating the genus. Hypotodus has since been re-considered as valid, as enough characters have been found, and this made it possible to distinguish it from other genera (for further discussion on this subject see Cappetta and Nolf, 2005, p. 244-246).
Genus JAEKELOTODUS Menner, 1928
Jaekelotodus robustus (Leriche, 1921)
Material. Three anterior teeth (FES 062, 063, 064) and two lateral teeth (FES 060, 093).
Description. The teeth have a well-developed triangular crown that is slightly inclined distally. Both faces of the crown are smooth. The lingual face is strongly convex while the labial one is flat. At the base of the labial face is a central depression. On this same side the enameloid descends from the central depression and covers the upper portions of the root lobes. On the lingual side, the contact between the crown and the root is marked by a well defined neck. The sharp cutting edge reaches the base. A sharp cusplet occurs on either side of the crown and each cusplet is inclined towards the main cusp. In the mesial or distal view it is observed that the cusplets are not following the same plan as the main cutting edge, but instead are lingually inclined. In specimen FES 063 it is observed the tendency towards the formation of a secondary pair of cusplets partially separated from the main pair. This tendancy is also observed for the mesial cusplet of FES 093.
Remarks. At least two Eocene species of Jaekelotodus are known, J. trigonalis and J. robustus. However, Cappetta (2012) lists also J. londonensis Zhelezko, 1994 and an impressive number of subspecies for J. trigonalis, all from Kazakhstan.
Teeth of Jaekelotodus are easily distinguished from those of other genera of the same age by the stout triangular crown with the central labial depression and the medium sized, hook-shaped cusplets. The teeth of J. robustus can be recognized based on their single pair of lateral cusplets that are shorter compared to J. trigonalis and J. londonensis. Also, the root of J. robustus teeth has a furrow that is more pronounced than that of J. trigonalis (Cappetta and Nolf, 2005).
Superorder BATOMORPHII Cappetta, 1980
Order MYLIOBATIFORMES Compagno, 1973
Superfamily MILIOBATOIDEA Compagno, 1973
Family MYLIOBATIDAE Bonaparte, 1838
Subfamily MYLIOBATINAE Bonaparte, 1835
Genus MYLIOBATIS Cuvier, 1816
cf. Myliobatis sp.
Material. One almost complete dental plate (FES 074).
Description. The specimen measures 32.1 mm labial-lingualy and has a maximum width of 29 mm. The width-to-length ratio of the medial teeth is 5.3:1, while for the lateral ones it is 0.8:1 for the inner row and 0.6:1 for the outer row. A slight curvature is present in the labio-lingual direction. The eight medial teeth are the widest teeth in the plate and are slightly arched in occlusal view. All the teeth are hexagonal. The medial teeth are framed by two lateral roaws on each side. Longitudinal striations occur on the occlusal surface. The root is partially filled with sediment but is no more than 2 mm high and of a polyaulacorhize type. The root laminae are irregularly shaped, and the grooves between them are wider than the laminae.
Remarks. The genus is described by Bigelow and Schroeder (1948) and Cappetta (2012) as having a dental plate consisting of seven rows of teeth, the medial file being the widest, and each tooth being hexagonal shaped.
The number of fossil Myliobatis species is amazingly high. For instance, there are forty-five species described for the Eocene (Hovestadt and Hovestadt-Euler, 2013). However, Cappetta (1987) listed only six valid species from the entire Paleocene and later reduced this number to only five (Cappetta, 2012). We note that an extensive comparative study by Hovestadt and Hovestadt-Euler (2013) of the dental morphology of the extant representatives of the Myliobatinae subfamily showed that teeth morphological variation is very high even within the same species. For example, several species of Myliobatis show variation in the number of rows and in the width/length ratios. Also there is strong evidence that tooth morphology is correlated with dietary preference or prey availability within a given species (Hovestadt and Hovestadt-Euler, 2013, p. 22). As the specimen only partially fulfills the genus diagnostic characters, we assigned the specimen to cf. Myliobatis sp.
Family AETOBATIDAE Agassiz, 1958
Genus AETOBATUS Blainville, 1816
cf. Aetobatus sp.
Material. Two fragmentary upper teeth (FES 072, 073).
Description. The teeth are medium-sized (37 mm width and 9 mm length for the figured specimen), laterally arched and with a wavy outline, smooth occlusal surface and roots divided longitudinally by ridges and grooves, which continue from underside towards backside.
Remarks. The antero-posterior arched, wavy or M-shaped teeth from the Myliobatinae that have a posterior displaced root are typically assigned to Aetobatus. As with the genus Myliobatis, the lack of data regarding the variability of tooth morphology in extant genera and the poor knowledge of genera such as Aetomylaeus led to erroneous assignations.
Myliobatinae indet. 1
Material. One fragmented dental plate (VT459 BBUPSM).
Description. The fragment measures 28 mm labial-lingually and has a maximum width of 46 mm. Only a single tooth is complete. The width:length ratio of the complete medial teeth is 5:1. Only a small fragment of a lateral tooth is present. The root is heavily worn and the laminae are razed. Interestingly, the root contains deep grooves between the teeth.
Remarks. Similar deep grooves are present on a fragment assigned by Dica (2006) to Myliobatis sp. 1; this fragment was from the same formation, but a different locality (Căpușul Mic).
Myliobatinae indet. 2
Material. One tail sting (FES 048).
Description. The specimen is a fragment of a tail sting. The dorsal side is smooth. The ventral side has a longitudinal ridge along its entire length. The distal quarter of the sting exposes serrations on both sides. The exact shape of these serrations could not be determined due to the poor state of preservation.
Remarks. Since the tail stings of rays lack diagnostic characteristics according to Hovestadt and Hovestadt-Euler (2013), it could not be determined below the subfamily level.
Superfamily DASYATOIDEA Whitley, 1940
Family DASYATIDAE Jordan, 1888
Genus DASYATIS Rafinesque, 1810
Dasyatis cf. jaekeli (Leriche, 1905)
Material. One tooth (FES 095).
Description. The tooth is 1.8 mm wide and 1.4 mm high. Both occlusal and labial surfaces are covered by a network of alveoli and crests, while the lingual face is smooth. The tooth is deeply worn in the mesial direction of the occlusal face. The general shape of the occlusal surface is hexagonal. On lateral profile, one can notice a depression of the lingual side. The root is short and it has two lobes with triangular ends. The central foramen is barely visible between the root lobes.
Remarks. Tooth morphology of the genus is highly variable, and it is complicated by the gynatric heterodonty, as breeding males have cuspidate teeth and non-breeding males and all females have rounded ones (Kajiura and Tricas, 1996; Cappetta, 2012). The above described characters likely indicate a female tooth or a non-breeding male belonging to Dasyatis. It differs slightly from D. jaekeli, based on illustrations and descriptions from Leriche, (1905), Case (1994) and Ciobanu (2002), as it has a shallower lingual depression and the central occlusal ridge is less obvious. For this reason we treat the specimen here in an open nomenclature.
Order RHINOPRISTIFORMES Naylor et al., 2012
Family RHINOBATIDAE Müller and Henle, 1838
Genus RHINOBATOS Linck, 1790
Rhinobatos cf. steurbauti Cappetta and Nolf, 1981
Material. Two teeth (FES 096, 097).
Description. The teeth are very small. The widest crown measures 1.3 mm. The teeth have a general globular shape with a very weakly marked transversal ridge on the occlusal surface. A central, elongated uvula is visible lingually. A pair of lateral uvulae is present on the sides of the central uvula. The lateral uvulae are shorter than the central one and do not diverge. All uvulae have a rounded basal end. The root is missing in both teeth.
Remarks. Two species of Rhinobatos are known from the Eocene: R. bruxelliensis Jaekel, 1894 and R. steurbauti Cappetta and Nolf, 1981. Rhinobatos bruxelliensis has pointed and more divergent uvulae while R. steurbauti has uvulae that are rounded and less or non-divergent (Cappetta and Nolf, 1981, p. 96). Based on these differences, we assign the specimens to R. cf. steurbauti. Rhinobatos steurbauti is rarely reported but is present in the middle Eocene of France (Cappetta and Nolf, 1981), England (Bone et al., 1991) and Uzbekistan (Case et al., 1996).
Family PRISTIDAE Bonaparte, 1838
Genus PRISTIS Linck, 1790
Material. One incomplete rostral spine (FES 003).
Description. The rostral spine measures 48.0 mm in apical-basal direction, 12.0 mm in anterior-posterior direction and 4 to 6 mm dorsal-ventrally. The spine is dorso-ventrally compressed with a rounded anterior margin, and with a shallow longitudinal groove along the posterior margin. Both apical and basal ends of the spine are broken. The apical surface has asymmetrical margins along the longitudinal groove.
Remarks. Similar to the Myliobatidae, numerous of fossil pristids have been described in the last few centuries. Many of these species were described from isolated rostral spines. Twenty-six species belonging to four genera (Propristis Dames, 1883; Mesopristis Farres, 2003; Pristis Linck, 1790; and Anoxypristis White and Moy-Thomas, 1941) have been described from the Eocene. Propristis has a unique morphology, with rostral spines nearly as long as high (Cappetta 2012, p. 396). The newest genus, Mesopristis, was set in synonymy with Anoxypristis by Cappetta (2012), but without explanation. However, the rostral spines of Mesopristis lack a posterior groove. Anoxypristis can be excluded for the same reason. Pristis is the only genus that has a posterior longitudinal groove. Within the respective genus there are numerous Eocene species but the species cannot be determined from the material at hand. Observation on extant material belonging to Pristis, made by one of us (NT), indicate a high degree of variability in rostral spine length along with the width and depth of the posterior groove on the same specimen. Considering the above-mentioned facts the specimen, can be assigned with confidence to Pristis sp.
Order cf. RAJIFORMES Berg, 1940
Family, genus et species indet.
Material. Two dermal spine bases (FES 046, 088).
Description. These generally oval dermal spines have a truncated cone shape in lateral view. A shallow concavity and some very fine radial striations are present at the center of the dorsal side, as are some obvious concentric growth lines. The basal surface is slightly convex.
Remarks. The assignation of these thorn bases is challenging, as both Rajiformes and Myliobatiformes include numerous families where these dermal thorns are present (Deynat, 1998). Moreover, the local taphonomy may have reduced through abrasion some of the finer surface details. It is debatable if these thorns should be allocated to Rajiformes. Extant species show that thorn morphology can be variable on the same individual depending on the part of the body they occur (Gravendeel et al., 2002). Nevertheless, we found that several Rajidae genera have similarly shaped dermal denticles. In addition, we note that very similar fossil material from the upper Eocene of Germany has also been assigned to Rajiformes, based on comparison with extant material (Hillmer and Mundlos, 1981).
Superorder BATOMORPHII Cappetta, 1980
Material. Two dermal spine bases (FES 086, 087).
Description. These two specimens differ greatly from the above-described material. Specimen FES 086 has a pentagonal outline in dorsal view and a truncated cone shape from a lateral view. A deep concavity is present at the center of the dorsal side. Striations and growth lines were absent, unlike the cf. Rajiformes specimens. The base is completely flat. Specimen FES 087 (Figure 7.22-24) also differs from the cf. Rajiformes specimens and specimen FES 086 (Figure 7.19-21) by having a rounded outline and a torus-shaped lateral outline. The basal face is convex. This specimen has a concavity in the central raised portion of the dorsal surface.
Remarks. Specimen FES 087 is reminiscent of a pearl-shaped tubercle as defined by Deynat (1998, p.158).
Order PYCNODONTIFORMES Berg, 1940
Family incertae sedis
Genus PHACODUS Dixon, 1850
Phacodus cf. punctatus Dixon, 1850
Material. Twenty-nine teeth (FES 012 - 040).
Description. The teeth are generally oval or round and measure 4 to 11 mm along the long axis. The oral surface is covered by fine pits (Figure 8.18') that penetrate the enamel deeply. The basal side of the crown has a deep oval-shaped depression. In some specimens, the edges of the teeth show differently-sized and geometrically-shaped protrusions (Figure 8.15-16, 8.19).
Remarks. The generally oval or round shape and the presence of the fine pits that cover the entire occlusal surface of the tooth are characteristic traits of the monotypic Phacodus punctatus. The presence of Phacodus in the Paleogene is unusual. Until recently, Phacodus was known only from the Cretaceous (Dixon, 1850; Santos and Figueiredo, 1988; Hooks et al., 2013). In Romania, a single occurrence of Phacodus after the K/T boundary was known only from specimens found a few years ago in the upper Eocene of Turnu Roşu (Ciobanu and Trif, 2014). A Phacodus tooth has also been found at Căpuşul Mic (Căpuş Fm.), but it was referred only as Pycnodontidae indet. (Dica, 2006, plate 15, figure 2).
The species is based on a fragmentary associated dentition (holotype NHM PV OR 25829), representing possibly a splenial fragment, found in the Cenomanian of the UK. For a long time the species and the genus were rejected, the holotype specimen being considered just a very worn and fragmentary pycnodont (Woodward, 1888, 1895). However, the genus and species were finally accepted as valid by Woodward (1909), who had previously rejected them. Since then the genus has been studied only rarely. Arambourg (1952) found a vomer and two fragmentary splenials in the Maastrichtian of Morocco (Ouled Abdoun). Based on this material, he erected a new variety, Phacodus punctatus var. africanus, due to a slight difference in the outline of the central teeth and in the smaller size of the lateral teeth. Santos and Figuiredo (1988) described Phacodus sergipensis almost three years later, from the Turonian of Brazil. The difference between this new species and P. punctatus, based mainly on two additional lateral rows, was rejected by other authors (e.g., Hooks et al., 2013) who argued that the variation of the lateral number of rows in pycnodonts had been noted in other species too. While we have assigned our Romanian teeth to Phacodus cf. punctatus, micro-morphology and future research may lead us to a new conclusion.
Order PERCIFORMES Bleeker, 1859
Suborder LABROIDEI Bleeker, 1859
Family LABRIDAE Cuvier, 1817
Material. One upper pharyngeal tooth plate (FES 057).
Description. A fragmented pharyngeal plate was collected having numerous rounded teeth with diameters of 0.25 to 2.5 mm. The teeth are longest at the center of the plate and decrease towards the edges. The central teeth have a rough, irregular surface while the lateral ones have a completely smooth exterior. The teeth are arranged in regular, almost parallel rows. Together, they form a compact grinding surface. Note the considerable thickness of the plate in occlusal-basal direction, at 14.0 mm. The plate is triangular in transversal section, including the grinding surface.
Remarks. Although some authors consider Labridae tooth plates non-diagnostic (e.g., Long, 1992), others, such as Dica (2002), consider the morphology and the arrangement of the teeth on the pharyngeal plates to be indicative characters on the genus level. An example of this is the lower pharyngeal plate of Lachnolaimus multidens from the Priabonian of Romania (Dica, 2002, fig. 3). The figured specimen compares well with the previously described lower pharyngeal plate of L. multidens from the Miocene of the Vienna Basin (Münster, 1846, figs. 5a-c). However, we consider that the assignment of other upper pharyngeal plates from Transylvania to species level, as L. multidens (Dica, 2002, pl. 1, fig. 4; Ciobanu, 2013, figs. 1-6) is only arbitrary as the lower plate is missing.
The assignment of our specimen to Labridae is however valid, based on similar fossil upper dentitions (Münster, 1846; Wainwright, 1987).
The Labridae family is known from Eocene, primarily from associated skeletons from Monte Bolca (Bannikov and Carnevale, 2010), but isolated pharyngeal triturating plates from Eocene Labridae have also been reported (Bellwood et al., 2019).
The fish assemblage from Luna de Sus includes at least 17 species from as many genera; these fish belong to 12 families and seven orders. Seven of these genera (Physogaleus, Abdounia, Macrorhizodus, Striatolamia, Otodus, Jaekelotodus, Hypotodus) are extinct as is the entire order of Pycnodontiformes. One genus (Heterodontus) and four species (Galeocerdo cf. eaglesomei, Jaekelotodus robustus, Hypotodus verticalis and Rhinobatos cf. steurbauti) are new for Romania. This locality represents the second Cenozoic occurrence of the pycnodontiform Phacodus cf. punctatus in Romania and Europe. The first reported occurrence was the one from the upper Eocene of Turnu Roșu (Ciobanu and Trif, 2014). The Labridae material reported here represents the oldest record of this family in Romania.
The relative abundance of teeth and dermal spines at this level puts it in contrast with other layers from the same locality. Only a single other layer contains fish teeth, namely the Nummulites perforatus lumachelle, from where a single fish tooth of Striatolamia macrota has been recovered.
The general state of preservation of the teeth is good, as evidenced by their sharp cutting edges, fine lateral cusplets and mostly intact roots. This mode of preservation indicates that the remains were transported only minimally before final burial; therefore, we consider the specimens to be autochthonous or parautochthonous. All the teeth have a reddish-brown color specific to the fossils of the iron oxide-rich Căpuș Formation (Stoicovici and Mureșan, 1964a, 1964b).
The environment of sharks, rays and bony fishes from the locality of Luna de Sus can be reconstructed with some degree of approximation, considering the habitat preferences of extant relatives. Heterodontus is found in a wide range of depths, from intertidal to 275 m (Bass et al., 1975; Compagno, 2002). Rhizoprionodon is found both inshore and offshore, and at depths from less than 1 m to about 200 m, with some species reaching 500 m depth (Compagno, 1984). A transition towards a shallower reef habitat has been encountered in some species (Sorenson et al., 2014). Galeocerdo inhabits a wide range of depths and habitats, from intertidal to over 200 m depth, but spends most of its time in less than 50 m of water (Compagno, 1984; Vaudo et al., 2014). Aetobatus is benthopelagic and typically occurs nearshore, in 1 to 60 m depth (Mundy, 2005; White and Last, 2016). Myliobatis is also benthopelagic and is confined mostly to warm waters and shallow depths to 80 m (Love et al., 2005; Ebert and Stehmann, 2013). Dasyatis is demersal (to 40 m depth), with most species preferring shallow water. Many Dasyatis species are found inshore, in lagoons and river-mouths (Struhsaker, 1969; Ebert and Stehmann, 2013). Rhinobatos lives in shallow inshore estuarine to marine waters, to 100 m, but with some species living as deep as 180 m (Ebert and Stehmann, 2013). Extant Rhinobatidae live in warm-temperate to tropical waters, but a few species occur in deeper, cooler water offshore (Last and Compagno, 1999). Representatives of Pristis prefer shallow coastal waters and estuaries, typically in less than 10 m depth, but adults may be found in the 100 m depth or more (Poulakis and Seitz, 2004; Simpfendorfer, 2005; Ebert and Stehmann, 2013). Immature individuals are dependent on shallow habitats, living especially around the river-mouths (Simpfendorfer, 2005; Last et al., 2016b). Some extant Pristis species have a preference for freshwater habitats for nurseries (Peverell, 2005). The range for extant Pristidae is circumtropical (Nelson et al., 2016) and presumably the climate preference of the fossil Pristis was the same. Labrids are generally shallow-water fishes, though exceptionally, some species of Bodianus and Decodon occur in deep water at 200 m or more (Smith and Heemstra, 1986). Most Labridae live in association with structure such as coral reefs or rocky substrate in depths to 40 m (Allen et al., 2003).
The presence of Phacodus cf. punctatus in the Eocene of Luna is very unusual, as it is the only pycnodont found in northwestern Transylvania. Little is known about the ecological conditions of this fish. Taking into consideration the associated fauna from other Transylvanian occurrences (Ciobanu, 2002; Ciobanu and Trif, 2014), the warm, moderately deep waters are also among its environmental preferences. The pycnodonts are very rare in the northwestern portion of the Transylvanian Basin as compared to their occurrence in Turnu Roșu on the southern side of the basin. The pycnodont teeth are well represented in all three formations from Turnu Roșu (spanning the Ypresian-Priabonian interval). The presence of a high number of teeth from this single species in Luna de Sus indicates a well established population of pycnodonts in an unspecified ecological niche that allowed them to flourish among higher rank predators such as sharks.
The habitat preferences of modern relatives of studied fishes (Figure 9) indicate a moderate water depth of less than 200 m (more likely less than 100 m, as inferred by the preferred depth) in a warm sea.
The knowledge of the middle Eocene fish (documented by teeth) is still limited on the regional level of Eastern Europe. We compared the occurrences of taxa from Luna de Sus with those from elsewhere in the region and with those from other better-known localities. For this comparison we only took into consideration the Chondrichthyes, given their numeric dominance at Luna de Sus. We assessed the faunal diversity at this site with that of 13 sites from the European part of Russia, Hungary, Ukraine, Denmark, Germany, Belgium, France, Egypt, and Morocco (Figure 10). The data covers the early Lutetian through the late Bartonian (Table 1).
We note a few genera that are probably more adaptable and migratory and which are common throughout the entire Tethys Sea and North-East Atlantic coast, such as Striatolamia, Macrorhizodus and the small Carcharhiniformes Abdounia and Physogaleus (Dutheil, 1990; Udovichenko, 2006; Eeckhaut and De Schutter, 2009; Udovichenko, 2009; Timircev and Popov, 2011; Diedrich, 2012). The absence of Otodus from many sites of the close-by region (Kocsis, 2002; Udovichenko, 2006; Udovichenko, 2009; Malyshkina et al., 2013; Leder, 2013) is surprising, considering that this predator is present in many localities of North-East Atlantic coast and North Africa (Dutheil, 1990; Eeckhaut and De Schutter, 2009; Underwood et al., 2011; Adnet et al., 2010; Diedrich, 2012; Carlsen and Cuny, 2014). It is good to note that diversity on the genus level in the North Sea Basin, Paris Basin and in the south of the Tethys Sea is significantly higher than in Eastern Europe. The presence of Pristidae and small Carcharhinidae in southwestern Morocco and in the Midawara Formation of Egypt (Adnet et al., 2010), where tropical conditions were well established, also indicates the existence of a warm habitat for Luna de Sus. Another evidence to support this hypothesis is the lack of deep, cold-water taxa such as Centrophorus, Chlamydoselachus, Coupatezia, Echinorhinus and Hexanchiformes that are present in other sites (Dutheil, 1990; Eeckhaut and De Schutter, 2009; Malyshkina et al., 2013; Carlsen and Cuny, 2014) that indicates a shallow depth and warmer conditions in Luna de Sus.
The climate reconstructions based on palynology (Petrescu and Balintoni, 2003) confirms a warm climate. This is supported further by reconstructions using oxygen and carbon isotopes measured on Nummulites perforatus collected at the same locality of Luna de Sus, on “Pavel Brook”. For the interval involving the fish fauna, a mean paleotemperature is calculated at 26 °C, while for the levels immediately above this interval a slightly cooler tendency was recorded, calculated at 23-24 °C (Bartholdy et al., 2000).
The richness of the middle Eocene fish fauna of the Luna de Sus in the northwestern portion of the Transylvanian Basin is significant, with at least 17 species belonging to as many (17) genera. The vast majority of the teeth found here belongs to Chondrichthyes and apparently originate from large-to-medium-sized fish, but this could be a consequence of the sampling bias. As revealed by the teeth taphonomy, the layer of sediments the teeth were recovered from most likely accumulated under low energy depositional conditions, and we therefore consider these fossils to be either autochthonous or parautochthonous. The faunal analysis of the northeast Atlantic coast and of the Tethys Sea reveals in part a common elasmobranch fauna with a variable number of common genera. These common genera are mostly lamniforms (Hypotodus, Jaekelotodus, Macrorhizodus, Otodus, Striatolamia) that were opportunistic predators of more open water or at least with broader habitat preferences.
Four species and one genus are reported here for the first time from the Eocene deposits of Romania. Aside from them, one of the most important occurrences in these deposits is Phacodus cf. punctatus. This second report in the northwestern Transylvanian Basin confirms its survival of the K/Pg boundary.
We thank both anonymous reviewers for their critical reading of the manuscript and for their valuable suggestions. The authors are very grateful to J. Seitz for not only reviewing the English language but also for the suggestions and references he sent. The authors also would like to thank A. Fuciu for the help in translation of the early version of the manuscript. The manuscript greatly benefited from the discussions with P. de Schutter and T. Malyshkina.
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