Phylogenetic relationships

Ceratosauria traditionally consists of Ceratosaurus and all taxa closer to it than to Neornithes19. However, taxonomy within Ceratosauria has been complicated. Abelisaurs were formally known as Abelisauroidea (=Ceratosauroidea), that comprises Carnotaurus, Noasaurus and all their most recent common ancestors and all descendants (see below for further discussion). Ceratosauroidea are included in the clade called Averostra which comprises the taxa related to Ceratosauria and all derived theropods20. Approximately 32 Ceratosauroidea genera are currently known with most of the taxa originating from the Late Cretaceous (Table S1).

Ceratosauroidea is traditionally divided into two main branches: the Noasauridae and the Abelisauridae21 (but see also the last paragraph for new definitions). This classification has been followed in the recent phylogenetic analyses which have revealed more resolution of the relationships within the clades3,5,14,15,22. The relationships between of the two large groups is still being debated; however there are new hypotheses of relationships amongst the noasaurids improving the resolution within the family14. In the case of abelisaurids, two main branches divide the South American (called Brachyrostra)22 from the European/Indian/Madagascan taxa (previously called Majungasaurinae)5. Recent phylogenetic analyses recovered a new clade included in Brachyrostra that comprises the Santonian-Maastrichtian abelisaurids from South America: the Furileusaura13,15,23. Nevertheless the relationships amongst furileusaurians are still debated13.

The recent analyses of Wang et al.14 expanded the matrix for phylogenetic relationships of ceratosaurs (744 characters) with dense taxon sampling (198 taxa) including a broad outgroup which better allow to polarize homology statements at the node Ceratosauria. The new hypothesis of Wang et al.14 suggests Elaphrosaurus bambergi and Limusaurus inextricabilis as sister taxa as recovered by Rauhut and Carrano24. However, in a novel result Wang et al.14 find that Berberosaurus basal within Abelisauridae (=new Etrigansauria, see below), and Ceratosauridae is now composed of Eoabelisaurus plus Ceratosaurus and Genyodectes serus. According to Wang et al.14, Ceratosaurus is united within non-noasaurid ceratosauroids by the following features: (1) fusion of the quadratojugal and quadrate; (2) posterior extent of the posteroventral process of the dentary directly ventral to the posterodorsal process; (3) parapophyses distinctly below the level of the diapophyses in posterior dorsal vertebrae; (4) contact of the pubis and ischial obturator process and (5) transverse infrapopliteal ridge between the medial and lateral femoral condyles. Additionally, Dahalokely tokana is recovered as a majungasaurini instead of within Noasauridae as proposed by Farke and Sertich25 and Tortosa et al.5 or within Brachyrostra as suggested by Delcourt13 and Filippi et al.15. This new hypothesis suggests that the origin of ceratosauroids and its two main branches are older than previously thought, with and African origin, decreasing the length of previous ghost linages.

Nevertheless, the inclusion of Ceratosauridae in Abelisauridae as proposed by Wang et al.14 has important taxonomic implications and some clade definitions must to be done. According to the International Code of Zoological Nomenclature (ICZN)26, the family name Ceratosauridae has priority over Abelisauridae because the first was coined in 1884 by Marsh6 and the second was coined in 1985 by Bonaparte and Novas27. Additionally, according to the Principle of Coordination of ICZN26 “a name established for a taxon at any rank in the family group is deemed to have been simultaneously established for nominal taxa at all other ranks in the family group”. It means that once Ceratosauridae is nested in Abelisauroidea, the superfamily Ceratosauroidea is the synonym senior to Abelisauroidea and the synonym junior must be replaced. The definition of Ceratosauroidea here follows the suggestion of Wilson et al.28 for Abelisauroidea: the clade is composed by Carnotaurus, Noasaurus and all their most recent common ancestors and all descendants (also including Ceratosauridae). If the phylogenetic hypothesis of Wang et al.14 is correct, I propose a new clade to include Ceratosauridae and Abelisauridae as well as new definitions for these two families (Table 1):

Table 1 The proposed set of definitions for the ceratosaurian clades. Full size table

Also, it is worth noting that the subfamily Majungasaurinae5 in the topology of Wang et al.14 should be considered a tribe and called Majungasaurini because is inserted in the subfamily Carnotaurinae. This taxonomic change helps to clarify the relationships among Ceratosauroidea and satisfies the nomenclature requirements (Fig. 1). Therefore, in the present contribution I will follow the Wang et al.14 phylogenetic results. All the phylogenetic definitions used here are in the Supplementary Materials.

Figure 1 The hypothetical phylogenetic relationships of ceratosaurs based on current topologies. The main source is from Wang et al.15. The phylogenetic position of Chenanisaurus is from Longrich et al.24 and the Ligabueino, Austrocheirus, Majungasaurinae and Brachyrostra are from Filippi et al.16. Full size image

The origin of Ceratosauroidea is subject of debate concerning the time of the basal-most taxa. Although its origin has been recovered to the Early/Late Cretaceous (Aptian/Cenomanian, between 126–93.9 My)3,5,15,25, some authors suggest it could be earlier, originating in the Early Pliensbachian/Toarcian, between 191–174 My (Early Jurassic)14,29 or Aalenian/Bajacian (Middle Jurassic)12. These differences hinge on the position of Berberosaurus liassicus (Pliensbachian/Toarcian), a ceratosaurian from Morocco known by a partial postcranial skeleton29 and the position of Eoabelisaurus mefi (Aalenian/Bajacian) a medium-sized etrigansaurian from Argentina known by an almost complete skeleton12. Depending on the position of these taxa, the origin of Ceratosauroidea is younger or older. In some analyses, Berberosaurus is considered as a basal ceratosaurian12,13, a neoceratosaurian5, a basal abelisauroid29 or sister-taxa of cornisauria14. The topology of Eoabelisaurus is also controversial, falling out as basal within Ceratosauroidea5,13, Abelisauridae12 or within Ceratosauridae14.

Ceratosaur anatomy

Ceratosauroidea probably has most disparity (morphological variety) of any major theropod group30. They could be omnivorous/herbivorous such as in Limusaurus14, have horns as in Ceratosaurus, Carnotaurus and Majungasaurus crenatissimus or have extreme reduced forelimbs as in Majungasaurus, Aucasaurus garridoi and Carnotaurus31. However, the body plans of the main branches (Noasauridae and Etrigansauria) remain respectively similar within each group (Fig. 2).

Figure 2 The anatomy of ceratosaurs, showing the variety of cranial morphology in the group. Right lateral side of the skulls of (A) Ceratosaurus (USNM 4735), (B) Skorpiovenator (MMCH-PV 48) and (C) Carnotaurus (MACN-CH 894) (scale bar: 10 cm). Left maxilla of (D) Noasaurus (PVL 4061; Fundación Miguel Lillo, Tucumán, Argentina); reconstruction of the skull of (E) Masiakasaurus and left lateral side of the skull of (F) Limusaurus (IVPP 20093 V; Institute of Vertebrate Paleontology and Paleoanthropology, Beijin, China) (scales bar: 5 cm). Full size image

Noasaurids tends to be smaller and more gracile than etrigansaurians1 with a long neck, small heads, and larger forearms32,33,34. Although the morphology of noasaurids differs substantially from those etrigansaurians, the ilium of Noasaurinae (subfamily included in Noasauridae) is as low as in Carnotaurinae (subfamily included in Abelisauridae) despite the fact that these two groups are not closely related. The skull of noasaurids are long and low compared to those of abelisaurids17,33. Interestingly, even among noasaurids the morphology of the skull varies substantially. The skull of Limusaurus becomes toothless through ontogeny, likely to meet a change in diet (see below)14, whereas the skull of Masiakasaurus knopfleri presents strong procumbent dentitions which probably indicate additional divergence from the typical theropod diet35. The forearms of noasaurids are poorly known, but as in other ceratosauroids the humerus, radius and ulna are more reduced distally than proximally suggesting that the reduction may have occurred in a modular fashion, from the distal to proximal across the phylogeny12. However, the humeri of noasaurids are slenderer than those of abelisaurids (Fig. 3A).

Figure 3 Limbs elements and skin impression of ceratosaurs. (A) Pectoral and forelimb of Deltadromeus (SGM-Din 2; Ministère de l'Énergie et des Mines, Rabat, Morocco); (B) forelimb of Carnotaurus (MACN-CH 894); (C) distal articulated tibia, fibula, astragalus and calcaneum of Eoabelisaurus (MPEF-Pv 3990; Museo Paleontológico ‘Egidio Feruglio’, Trelew, Argentina); (D) articulated tibia, fibula, astragalus and calcaneum of Xenotarsosaurus (UNPSJB PV 194/1; Universidad Nacional de la Patagonia ‘San Juan Bosco’, Chubut, Argentina) and (E) caudal skin impression of Carnotaurus (MACN-CH 894). Scale bar: 5 cm. Abbreviations: a, astragalus; c, coracoid; ca, calcaneum; cn, cnemial crest; dc, deltopectoral crest; f, fibula; he, humeral head; mc, metacarpals; r, radio; rb, rib; sc, scapula; sk, skin impression; t, tibia; u, ulna. Full size image

The body plan of etrigansaurians strongly differs from other theropods, and their morphology is more thoroughly known than that of noasaurids1,4. Whereas the noasaurids have long skulls, the etrigansaurians have strong and deep skulls, especially those of Brachyrostra which also showed encroachment of the postorbital into the orbit, just beneath the eye22. The skull of abelisaurids became shorter and more rugose in more derived taxa. Ceratosaurus, Eoabelisaurus, and possibly Genyodectes have longer skulls compared to those of abelisaurids. The skull’s shortening and deepening started in abelisaurid basal forms, such as the Aptian-Albian Kryptops palaios and the Cenomanian Rugops primus, both from Niger36,37, and reached its extremity in the Carnotaurinae taxa. The skull of Carnotaurus is exaggeratedly short and deep compared with those other taxa of the same clade. The skull of Abelisaurus was largely reconstructed in the snout as well as in the posterior area1,3,38, and taphonomic distortion has modified the proportions and several contacts between elements are missing such as the jugal articulations3,38. Therefore, as previously suggested38, Abelisaurus should have had a shorter skull than was previously reconstructed and frequently reproduced resembling those of Carnotaurinae (e.g. Majungasaurus) instead of Ceratosaurus (as suggested by Bonaparte and Novas27).

Regarding the basal abelisaurids, Kryptops was diagnosed based on a left maxilla, several partial vertebrae and ribs and an articulated pelvic girdle and sacrum36. However, as noted by Novas et al.4 and Carrano et al.39, the pelvic gridle and sacrum of Kryptops were found “eroded and free of the rock some 15 meters distant” and have more shared features with tetanurans than abelisaurids. The vertebral non-sacral remains also share features with ceratosaurians as well as tetanurans36. The maxilla is also incomplete and with only a general diagnosis possible (e.g. external texture on the maxilla, which is composed of short linear grooves that are also shared with Majungasaurus and Rugops). The only autapomorphy is a secondary wall in the anteroventral corner of the antorbital fossa obscuring it and that has a scalloped and fluted dorsal margin36. Therefore, as the holotype of Kryptops is a miscellany of materials belonging to different groups with just one autapomorphy supporting the species, this taxon might have been considered as nomen dubium rather than a valid taxon. The postcranial skeleton probably has a phylogenetic relationship with carcharodontosaurids instead of abelisaurids as suggested by Novas et al.4 and Carrano et al.39.

Abelisaurids has strongly reduced forearms without grasping ability40 (Fig. 3B). According to Agnolin and Chiarelli40, abelisaurs probably also lacked forearm mobility. However, recent analyses on Majungasaurus musculature suggest that, although much reduced, abelisaurids did not lose full mobility of the forelimb, and may have used it for intraspecific display41. Some taxa such as Aucasaurus, Majungasaurus and Carnotaurus may have lost the ungual of the digits I and IV31,40,42 whereas the ceratosaurid Eoabelisaurus has strongly reduced the manual unguals12. The digit IV is fused to the metacarpal in Majungasaurus and Aucasaurus precluding mobility. Extreme reduction also reduced autonomy of all digits due to the extreme reduction, although the hemispherical humeral head and distal radius and ulna suggests that the shoulder and the wrist had a large range of motion38,41. However, as pointed by Gianechini et al.38 the range of motion of the humerus should have been higher in lateromedially (i.e. abduction-adduction) than in anteroposteriorly (i.e. flexion-extension) because the development of the dorsal and ventral rim of the glenoid fossa reduced anteroposteriorly movements. Also, is worth noting that the large scapulocoracoids and reduced forelimbs in ceratosauroids might be related to a close developmental association between scapular blade and the axial skeleton, holding the shoulder girdle to the axial skeleton and for mobility of the girdle and the ribcage38,41,43. Those muscles attached to the neck could have had an important role in feeding as in extant crocodiles (e.g. muscle levator scapulae which is an effective abductor of the neck and hence the head)41,44.

The hindlimbs of ceratosaurs are different in the two main branches. In noasaurids, the hindlimbs are more slender than the etrigansaurians; however this is due to the overall size of individuals of the groups1. Abelisaurids’ hindlimbs and caudal vertebrae suggest that these taxa, specially the brachyrostrans, may have had powerful cursorial abilities. The tibia have well developed dorsal anterior projection (cnemial crest) onto which the main knee extensor muscles are inserted (i.e. iliotibiales)45. The large size of the cnemial crest and its dorsal inclination suggest that some ankle extensors and digital flexors muscles were large, increasing their force-producing capability. Additionally, the dorsal inclination of the transverse processes in the caudal vertebrae suggests that the muscle caudofemoralis longus, the main femur extensor, may have been larger than in other theropods contributing to the cursorial ability10. Also, the presence of accessory articulations in caudal vertebrae (hyposphene-hypantrum) apart of the inclined transverse processes, increases the tail rigidity10,46 and may have enhanced overall speed and acceleration10. However, acceleration might have been more impressive than top speed. When preserved, feet of some abelisaurids are short (e.g. Majungasaurus47), indicating low tangential velocity at the ankle. The type of Carnotaurus lacks feet and the distal portion of the epipodials, even though it is often reconstructed as having gracile legs and feet17.

Etrigansaurian soft tissue

The etrigansaurians also are well known by their rugosities and projections from the skull elements3. Carcharodontosaurid theropods have rugosities in lateral skull bones as well, but the morphology is different48 and leads to misinterpretations of the group49. Although abelisaurids have strong rugose skulls, the textures are variable throughout the skull48. The texturization of the skull happened independently from the projections. For example, the skull of Ceratosaurus is diagnosed by having a rounded midline horn core on the fused nasals3 and horn cores forming a dorsal crest on the lacrimals50, although the skull is otherwise smooth48. On the other hand, the skull of Skorpiovenator bustingorryi is strongly texturized but without any projections22. The skull roof in abelisaurids is thick but this feature varies among the species48. Both majungasaurini Majungasaurus and Rajasaurus normandensis have a single medial horn formed by the frontal and frontal/nasal, respectively28,48, whereas the brachyrostran Carnotaurus has two frontal horns laterally oriented17, Aucasaurus has the lateral margins of frontal elevated in the orbital region, and Viavenator exxoni has almost flattened frontals51. The flattened frontals of Ekrixinatosaurus novasi52 and probably of Skorpiovenator suggest the basal position of these two taxa in relation to Furileusaura as proposed by Filippi et al.15.

The rugosities in abelisaurids resulted from a mineralization processes with specializations in the overlying dermis, such that the mineralized tissue includes the irregular surface texture representing mineralization of the bone’s periosteum, overlying dermal fibers or combination of the two, characterizing the metaplastic ossification48. The sculpture of lateral bones (e.g. maxilla, jugal, quadratojugal, dentary) presents a higher percentage of tangential vascular canals and grooves, whereas the dorsal roofing elements (e.g. frontal, dorsal postorbital and lacrimal, nasal, nasal process of the premaxilla) tend to have more projecting, tuberculate and/or cauliflower-like texture that combine with the vascular canals and grooves (Figs 4 and 5A,B)48. Sampson and Witmer48 have suggested that abelisaurids might have had more robust skulls than other theropods due to the high skull’s mineralization. Following the results of Hieronymus et al.53 for inference of soft tissues in Centrosaurine and Carr et al.54 for Tyrannosauridae, it is possible to assess the superficial cranial soft tissues of abelisaurids. These tissues show a hierarchy of textures which became more complex towards the phylogeny.

Figure 4 Skin structures inferred for abelisaurids. Dorsal surface of the skull of (A) Rugops (MNN IGU1), (C) Carnotaurus (MACN-CH 894) and dorsal surface of the fused nasal of (B) Abelisaurus (MPCA 11908). Scales bar: 5 cm. Full size image

Figure 5 Details of the skin structures inferred for abelisaurids. Right side of the skull of (A) Carnotaurus (MACN-CH 894) and left side of the skull of (B) Majungasaurus (FMNH PR 2100 – cast), both in dorsolateral view. Right side of the nasal of (C) Rugops (MNN IGU1) and left side of the nasal of Abelisaurus (MPCA 11908), both in dorsolateral view. Detail of the right frontal horn of (E) Carnotaurus (MACN-CH 894) and left side of nasal horn of (F) Ceratosaurus (USNM 4735). Arrowhead pointing rostrally without scale. Full size image

The basal abelisaurid Rugops has the dorsal surface of nasals with a row of seven pits, visible sutures between then and hummocky rugose surface which is also present in the dorsal surface of frontal, prefrontal lacrimal and maxilla (Figs 4A and 5C). These features are correlated with overlying scales as observed in living crocodiles and reptiles53. On the other hand, the anterior-most snout has a different texture compared to other categories of soft tissue. The nasal articulation processes of premaxilla and the anterior processes of nasal, show a papillate texture indicating the presence of armour-like dermis as suggested by Hieronymus et al.53. The presence of these tissues suggests that Rugops had, at least two categories of tissues covering the surface of the skull. Interestingly, the type of Rugops could be a subadult individual due to its small size, incomplete fusion between the nasals and the presence of the fenestra between the prefrontal, frontal, postorbital and lacrimal3. As the rugosities tend to increase during ontogeny18, the armour-like dermis could reach a larger surface if Rugops grew up and developed more papillate texture.

Abelisaurus, as other abelisaurids, have a lateral cranium surface (e.g. maxilla) with dense tangentially arranged grooves suggesting it was covered by large scales or scutes, as suggested by Sampson and Witmer48 and Hieronymus et al.53 (Figs 4B and 5D). However, the nasal of Abelisaurus differs from that of Rugops being extremely rugose with bones lobules across its surface. This texture is associated with armour-like dermis53, as seen in the anterior snout of Rugops (Fig. 5C)

The dorsal surface of carnotaurine skulls (nasal, frontal, dorsal lacrimal and dorsal postorbital) have coarse pitting and grooving on bone surfaces suggesting that these were covered by cornified tissue, being an osteological correlate with the cornified cover seen on muskoxen, centrosaurine dinosaurs53, and tyrannosaurids54 (Figs 4C and 5A,B). However, it is improbable that abelisaurids had projections higher than the frontal horns. This category of tissue increased the toughness of the head roof, which also might have had an important ecological function as discussed below.

The horns of Carnotaurus and Ceratosaurus would have been more extended than the preserved fossil and covered with cornified sheath, indicated by neurovascular grooves, depressed lip and less rugosity than the other bones surfaces as suggested by the results of Hieronymus et al.53 (Fig. 5E and F). Although the horn cores of Carnotaurus are more rugose than those of Ceratosaurus, ventral to the depressed lip the frontals are markedly lesser rugose. The single horn of Majungasaurus and Rajasaurus do not have the depressed lip seen in Carnotaurus and Ceratosaurus, suggesting that they were covered by cornified tissue without dorsal extension.

The only preserved soft tissues so far belongs to Carnotaurus and correspond to the anterior cervical region associated with cervical ribs, the shoulder region, thorax and tail17. The skin impressions present conical protuberances and there is no evidence for filaments or feathers (Fig. 3E). So far, the tubular filaments and feathers are only known in tetanuran theropods55,56.

Regarding the bone histology, some analyses also shed some light to the development of ceratosaurs as well as palaeoenvironment14,57,58,59. For example, the robustness of Masiakasaurus, once believed as different morphs (robust and gracile)60, might be considered to be developmental feature instead of dimorphism57, as also shown in allometric analyses1. Additionally, the slow growth of the same species can be related to the low resources of Maevarano Formation57,61.

Ceratosaur ontogeny

Ontogenetic traits are difficult to interpret in fossils, sometimes leading to misunderstanding in taxonomy3,62,63. In the case of abelisaurs, just a few species are known from certain ontogenetic series, such as Limusaurus, Ceratosaurus and Majungasaurus3,14,18. Also, there are some specimens of Masiakasaurus of different sizes33 with inference on ontogeny from bone histological analyses57.

The ontogenetic series of Ceratosaurus is still unclear. Madsen and Welles50 described two different species of Ceratosaurus (C. magnicornis and C. dentisulcatus) based on cranial and post-cranial associated elements. Nevertheless, Rauhut64 suggests that the diagnosis of these species are subjective and there might have been just one species of Ceratosaurus in Morrison Formation. Carrano and Sampson3, following Rauhut64, also argued that these two species have size-based diagnosis suggesting that they might be different ontogenetic specimens from Ceratosaurus. Although there are other materials attributed to Ceratosaurus3, no study was conducted to discuss the ontogenetic traits so far.

The series of Limusaurus shows at least 78 ontogenetic modifications through the growth from the analyses of 19 specimens14. Delcourt30 reported the loss of teeth in mature individuals, while most juveniles had toothed jaws, the skull also becomes longer through ontogeny. In a parallel and broader study, Wang et al.14 also reported several changes including the formation of a beak after birth. The amount of modifications in Limusaurus ontogeny and the presence of gastroliths in the abdominal region also suggest that this species change ontogenetically dietary preferences from omnivory to herbivory14,32.

The ontogeny of Majungasaurus was assessed by Ratsimbaholison et al.18 using mainly landmark-based approaches in the skull and in some isolated cranial elements (premaxilla, maxilla, lacrimal, postorbital, jugal, quadrate, dentary and surangular). The authors suggested that the ontogenetic changes include: the skull becomes deeper, the orbit becomes smaller, the sutures among the bones become more complex, and the texture of lateral bones increase18. In this study, the postcranial elements were not assessed.

Histological analyses suggest that Masiakasaurus57 and small abelisaurid theropods58 had a cyclical growth strategy as well as slowdown growing. However, in larger taxa, such as Aucasaurus, the growth rate tend to be higher than in smaller forms58.

Apart from these studies, some inferences about ontogenetic stages were made based on fusion of bones. For example the types of Xenotarsosaurus bonapartei, Eoabelisaurus, and Aucasaurus are considered mature individuals because they have a fused tibia and astragalus12,42 (Fig. 3C and D), whereas the type of Rugops has been suggested as being an immature individua based on the fusion of the cranial elements3 (see above). The type of Pycnonemosaurus nevesi, despite being considered the largest abelisaurid so far1, is considered a subadult specimen13 based on the presence of caudal vertebrae with unfused arches and centra as well as tibia. However, determining the maturity of a specimen based only on the fusion of arches with centrum is not safe because these elements are size-independent65.

Ceratosaur behaviour

Ceratosaur behaviour can be inferred from several studies on anatomy4,40,48 and biomechanics8,9,66. Also, the new information on soft tissue presented here (see above), suggest a behavioural pattern in abelisaurids as discussed below.

Gregarious behaviour is difficult to deduce; however small species found associated in the same assemblage localities, such as Masiakasaurus33 and Limusaurus14, suggest that they might have lived together. In the case of Majungasaurus, several specimens were found associated, but some materials (ribs, chevron, neural spines, transverse processes and neural arches) have teeth marks made by its conspecifics suggesting that this species had cannibalistic behaviour61. This behaviour can be explained by the resource scarcity in the Maevarano Formation during the Late Cretaceous that was semi-arid61.

Going through the new information of soft tissues of abelisaurids shown here (above), it is possible to infer that this clade might have had some intraspecific headbutting matches behaviour at least in carnotaurine taxa (as suggested for Carnotaurus8 and Majungasaurus67). The presence of cornified cover on the skull, that was inferred for Carnotaurus and Majungasaurus, has been related to headbutting behaviour in extant taxa (e.g. Ovibos moschatus, Syncerus caffer and Buceros vigil) as well as extinct (e.g. Pachyrhinosaurus, Achelousaurus horneri53 and Stegoceras validum68). Nevertheless, differing from those that engage in violent headbutting and have deep cancellous bone68 (which carnotaurine lack), the carnotaurine might have used the head in low-motion headbutting and shoving matches at low speeds (as marine iguana Amblyrhynchus cristatus69) or engaged giraffe-like strikes to each other’s neck and flanks67. The giraffe-like strikes have been proposed for Majungasaurus67 due to the presence of tall, rugose nasals, struts within sinuses and a unicorn-like projection of the frontals48,67, although stresses. Also, the mechanical analyses of Carnotaurus skull performed by Mazzetta et al.9 support the low-motion headbutting in this taxa. Furthermore, the presence of well-developed occipital region (e.g. nuchal crest)48 associated with large epipophysis and neural spines in the cervical vertebra increasing the neck musculature70,71 strongly suggest that the cervicocephalic complex (head and neck) withstood high stress. Indeed, the well-developed epipophyses indicate a good leverage for intervertebral dorsiflexion by the muscle tranversospinalis cervicis and the origin of a strong muscle complexus, a head dorsoflexior72. As similar features on neck and skull are spread throughout the carnotaurine abelisaurs, all the taxa belonging to this clade may have had similar behaviour in territoriality or mating matches for instance. It is worth noting that cranio-facial biting was reported for non-avian theropods73,74,75. This behaviour could have had several possible reasons, including territoriality, courtship/mating, play, predation/cannibalism, intrapack dominance and subadult dispersal74. In the case of carnotaurine, the headbutting and/or giraffe-like strikes could also have been added to the behavioural repertoire for any reasons above.

The low-motion headbutting behaviour also may have been present or began in more basal taxa such as Rugops and Abelisaurus in parallel with the development of scales and armour-like dermis on the dorsal cranium (e.g. nasal). For example, the dorsal surface of marine iguana skull has hummocky rugosities53 as in Rugops, suggesting that this structure associated with armour-like dermis might have allowed the abelisaurid a similar behaviour (i.e. low-motion headbutting).This hypothesis of low-motion headbutting developing through the phylogeny in abelisaurids can be tested if a species with similar skull showed Rugops hummocky rugosities plus well-developed cervical epipophyses and neural spine and if it was found in Early Cretaceous beds (e.g. Aptian). If the headbutting was not developed in this taxon, certainly the development of armour-like dermis and later cornified cover on the skull in more derived abelisaurids might have allowed for this behaviour. It is worth noting that the giraffe-like strikes seem to be more complex than the iguana-like low-motion headbutting because the first requires more complex development of the skull, as seen in Majungasaurus67, than in Rugops. Therefore, carnotaurine could potentially have adopted both combat styles. The possibilities of these behaviours in abelisaurids are testable with quantitative biomechanical methods8,9,67 and could be assessed in the future.

Biomechanical studies on the skull of abelisaurids have suggested that they had cranial mechanical advantage similar to allosaurs (e.g. Allosaurus fragilis and Carcharodontosaurus saharicus)66 and similar bite force (e.g. Carnotaurus: 3,341 Newtons9; Allosaurus: 3,573 Newtons76). These results mean that these two groups had high efficient mechanical advantage, but a bite force not as strong as that of Tyrannosaurus9,66.

According to the analyses of Therrien et al.77, carnotaurines (e.g. Majungasaurus and Carnotaurus) might have been ambush predators attacking large prey. Additionally, Sampson and Witmer48 have suggested that Majungasaurus, and possibly other carnotaurines, were “adapted for a mode of predation that entailed relatively few, penetrating bites accompanied by powerful neck retraction, as well as bite-and-hold behaviour”. This predatory behaviour is consistent with results on skull biomechanics9,66 as well as neck analyses69,70.

The development of advantageous features (e.g. large muscles for cursorial abilities)10 plus the increase the body size towards the phylogeny1 granted abelisaurids the opportunity to succeed the carcharodontosaurids as main predators in the Southern Hemisphere after their extinction in Turonian49,78. Interestingly, these two groups share dentary22,49 and skull advantage mechanics66 that might have helped the extinction of carcharodontosaurids through ecological interactions1 when this group was becoming rare in the Cenomanian, possibly due to climate changes (i.e. changing in the mean temperatures and floral compositions)79. Therefore, it is reasonable to suggest that the latest abelisaurids (carnotaurine) were tyrannoasaurid counterparts since the former were dominant in Southern Hemisphere3 and the latter in Northern Hemisphere2.

Ceratosaur biogeography

The new phylogenetic analyses presented by Wang et al.14 suggest that Ceratosauroidea was present in North America (Ceratosaurus) and Asia (Limusaurus, also suggested by Rauhut and Carrano24), instead just in South America, Europe, Africa, India and Madagascar4,5. However, Ceratosauroidea originated in Africa29 and the taxonomic diversity spread during the Middle Jurassic to North America, Europe, Asia, Africa, South America and Madagascar (Fig. 1). Australia and Antarctica do not have ceratosaur remains so far4, nevertheless it is possible that this group was present there and future discoveries can change this scenario.

The division of the mains branches of Ceratosauroidea (Noasauridae and Etrigansauria) happened in the Early Jurassic14,29 just after the origin of this group. The latest ceratosaurs, from the Aptian36, were restricted to Southern Hemisphere and Europe5. However, during the Barremian to Santonian Gondwana remained isolated from Laurasia when the fauna could acquire a wide geographic distribution across the southern landmass; relating to Europe in Campanian-Maastrichtian rather than Asiamerica4,80. The presence of the European majungasaurini Arcovenator escotae corroborates this biogeographic hypothesis5 whereas the European noasaurid Genusaurus sisteronis from Aptian14,81 would have to be considered a relic from the early origin of noasaurids.

It seems the abelisaurids body size increases along the phylogeny1; however, the new phylogenetic analyses presented by Wang et al.14 suggest a large abelisaur (i.e. Abelisaurus) in the base of the clade. Also, there is a new evidence that abelisaurids reached medium/large sizes (between 5.6 and 7.6 m long, based on a partial tibia) from Berriasian-Valanginian of South America82. Nevertheless, the largest species were restricted to South America and Africa so far1,23,83. This is because insular environments, such as Late Cretaceous of Europe5 and Madagascar, supports smaller fauna than continental landmass. Finally, the ability to live in semi-arid palaeoenvironment with low resources, such as those of Majungasaurus and Pycnonemosaurus61,84, and the high disparity of the group facilitated the evolutionary success of ceratosaurs during this time (Fig. 6).