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A new Cretaceous thyreophoran from Patagonia supports a South American lineage of armoured dinosaurs | Scientific Reports

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Abstract

The early evolution of thyreophoran dinosaurs is thought to have occurred primarily in northern continents since most evidence comes from the Lower and Middle Jurassic of Europe and North America. The diversification into stegosaurs and ankylosaurs is obscured by a patchy fossil record comprising only a handful of fragmentary fossils, most with uncertain phylogenetic affinities. Here we report the discovery of a new armoured dinosaur from the early Late Cretaceous of Argentina, recovered phylogenetically using various datasets either as a basal thyreophoran or a stem ankylosaur, closely related to Scelidosaurus. It bears unusual anatomical features showing that several traits traditionally associated with the heavy Cretaceous thyreophorans did not occur universally. Jakapil kaniukura gen. et sp. nov. is the first definitive thyreophoran species from the Argentinian Patagonia. Unlike most thyreophorans, it seems to show a bipedal stance, as in Scutellosaurus. Jakapil also shows that early thyreophorans had a much broader geographic distribution than previously thought. It is a member of an ancient basal thyreophoran lineage that survived until the Late Cretaceous in South America.

Introduction

Thyreophora is a clade of ornithischian dinosaurs characterized by the presence of dermal bone armour on their backs1. Although most thyreophorans are grouped within Eurypoda (Ankylosauria + Stegosauria), basal thyreophorans show unresolved phylogenetic placements. Traditionally, they have been recovered as non-eurypodan thyreophorans2,3,4,5. Alternatively, new research suggests them as non-ankylosaurian ankylosauromorphs6 (also suggested by Refs.7,8). The most representative of these forms are Scutellosaurus, Emausaurus and Scelidosaurus, from the Lower Jurassic of the USA, Germany and England, respectively. Scutellosaurus is a small (1.5–2 m body length) and slender thyreophoran with a bipedal life style9 whereas the larger Scelidosaurus (4.5 m body length) is thought to be facultatively bipedal10 (body length has not been confidently estimated for Emausaurus). Both Scutellosaurus and Scelidosaurus represent part of the early locomotor diversity of early ornithischians, with obligate quadrupedality evolving in later and larger ankylosaurs and stegosaurs9.

The fossil record of Thyreophora is mainly known from the northern hemisphere, and its presence in the Gondwanan continents remains poorly known, with only a few ankylosaurian or stegosaurian species, and several indeterminate materials4,11,12,13,14,15.

We present here a new thyreophoran genus and species from the Late Cretaceous of South America. The remains were found near the locality of Cerro Policía within the ‘La Buitrera Paleontological Area’ (LBPA), close to the E. Ramos Mexía Dam, in North Patagonia, Río Negro Province, Argentina. The outcrops exposed in the LBPA represent the upper section of the Candeleros Formation (Cenomanian). They are interpreted as aeolian accumulations of the Kokorkom Desert (a ~ 826 km2 paleoerg16), with shifts between arid and semi-arid climatic conditions17. Most fossils in the LBPA were found between beds of migrating dunes. The new specimen was found as a close association of elements in a small area (~ 1.5 m × 1 m), isolated from any other individual, as generally occurs in the Candeleros Formation in the LBPA. The remains were found disarticulated, and with a slight southwestern-northeastern orientation due to dune transport.

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The LBPA comprises a few localities such as La Buitrera, Cerro Policía, La Escondida and El Pueblito. This rich fossiliferous site produces three-dimensional, largely undeformed fossil vertebrates, including theropod dinosaurs18, uruguaysuchid crocodyliforms19, eilenodontine sphenodontians20, limbed snakes21, lizards22, chelid turtles23, dryolestoid mammals24, dipnoans16 and undescribed pterosaurs. Fragmentary sauropod skeletons and dinosaur tracks have also been recorded16. This new thyreophoran discovery from the LBPA provides new information about the structure of the early Late Cretaceous North Patagonian communities and the role of the still poorly known ornithischian component. In addition, this specimen provides new information about the early diversification and distribution of this cosmopolitan group.

Institutional abbreviations

AMNH, American Museum of Natural History, New York, USA; BRSMG: Bristol City Museum, Bristol, England; NHMUK: Natural History Museum, London, England; MNA: Museum of Northern Arizona, Flagstaff, USA; MPCA-PV: Colección de Paleovertebrados, Museo Provincial Carlos Ameghino, Cipolletti, Argentina; ZMNH: Zhejiang Museum of Natural History, Hangzhou, China.

Systematic paleontology

Dinosauria—Owen, 184225,

Ornithischia—Seeley, 188726,

Thyreophora—Nopcsa, 191527,

Jakapil kaniukura gen. et sp. nov. (Figs. 1, 2, 3, 4, Suppl. Figs. 2, 3).

Figure 1

Holotype of Jakapil kaniukura (MPCA-PV-630), skull bones. (a) Skull bones in right lateral view (dashed contours based on Scelidosaurus10); (b) basisphenoid in left lateral view. af anterior foramen, btp basipterygoid process, bt basal tubera, cp cultriform process, df double foramen, ene external naris edge, jf jugal facet of the maxilla, Mx maxilla, mxe maxillary emargination, Pmx premaxilla, vc Vidian canal, vp ventral process.

Figure 2
figure 2

Holotype of Jakapil kaniukura (MPCA-PV-630), lower jaw bones. (a) left mandible in lateral view; (b) left mandible in lateral view, interpreted bone contours; (c) left mandible in medial view; (d) left mandible in medial view, interpreted bone contours; (e) right surangular in lateral view (mirrored); (f) transversal section of the posterior half of the left mandible, cranial view; (g) articular bone in occlusal view; (h) predentary bone in occlusal view. A angular, af adductor fossa, Ar articular, Ar (gl) glenoid fossa of the articular, ce coronoid eminence, D dentary, de dentary emargination, dfo dentary foramen, dmp dorsomedial process of the articular, dr dentary rugosities, hi subhorizontal inflection (dashed line), imf internal mandibular fenestra, lp lateral process of the predentary, mc Meckelian canal, Pa prearticular, Pd predentary, rp retroarticular process, S surangular, saf surangular facet for the glenoid articulation, safo surangular foramen (canal), Sp splenial, st surangular tubercle, sy mandibular symphysis, vmc ventral mandibular crest.

Figure 3
figure 3

Holotype of Jakapil kaniukura (MPCA-PV-630), teeth. Maxillary teeth in labial (a,b) and lingual (c,d); (d) highlight the wear facet) views; dentary teeth in lingual (e,gj); (h,j) highlight the wear facets) and labial (f) views. dwf dentary tooth wear facet, me prominent mesial edge, mwf maxillary tooth wear facet.

Figure 4
figure 4

Holotype of Jakapil kaniukura (MPCA-PV-630), postcranial bones. Speculative silhouette showing preserved elements (a); osteoderm distribution is speculative and partial to show non-osteodermal elements); dorsal vertebra elements in dorsal (b), right lateral (c) and anterior (d,e) views; sacral vertebra in left lateral view (f); mid-caudal vertebra in left lateral view (g); fragment of the mid-shaft of a dorsal rib in posterior view (the enlarged, broken posterior edge is highlighted (h); expanded distal ends of two dorsal ribs (i); left scapula in lateral view (j); right scapula in lateral view (k); right coracoid in lateral view (l); left and right humeri in anterior view (m); probable right ulna in lateral view (n); metacarpals, non-ungual and ungual phalanx in dorsal views (o); left femur elements in anterior view (p); proximal end of the right fibula in lateral view (q); distal end of the left tibia in anterior view (r); ischial elements in side view (s); cervical osteoderms in dorsal view (t), flat scutes in dorsal view (u), spine-like osteoderm in side view (v) and ossicle in dorsal view (w). ac acromial crest, aco asymmetrical cervical osteoderm, alp anterolateral process, ap acromial process, at anterior trochanter, bb basal bone, ebr expanded broken rib edge, di diapophysis, dpc deltopectoral crest, ft fourth trochanter, gl glenoid, mc metacarpals, nc neural canal, ncs neurocentral suture, ph non-ungual phalanx, pp pubic peduncle, poz postzygapophyses, rug marginal rugosities, sb scapular blade, sc scute, tp transverse process, uph ungual phalanx.

Etymology

The genus, Jakapil (Ja-Kapïl: shield bearer), comes from the ‘gananah iahish’, Puelchean or northern Tehuelchean language. The specific epithet, comprising kaniu (crest) and kura (stone), refers to the diagnostic ventral crest of the mandible, and comes from the Mapudungun language. These languages, currently spoken by more than 200,000 people, have been combined as a tribute to both of the coexisting native populations of North Patagonia, South America.

Holotype

MPCA-PV-630 is a partial skeleton of a subadult individual (see Supplementary Information) that preserves fragments of some cranial bones (premaxilla, maxilla and basisphenoid), approximately 15 partial teeth and fragments, a nearly complete left lower jaw plus an isolated surangular, 12 partial vertebral elements, a complete dorsal rib and fifteen rib fragments, a partial coracoid, a nearly complete left scapula, a partial right scapula, two partial humeri, a possible partial right ulna, a complete and a partial metacarpal bone, three ischial and two femoral fragments, the distal end of a right tibia, the proximal end of a right fibula, three pedal phalanges, and more than forty osteoderms.

Referred specimens

MPCA-PV-371, two partial conical osteoderms.

Locality and horizon

Upper beds of the Candeleros Formation, early Late Cretaceous (Cenomanian, ~ 94–97 My, see16, and references therein), locality of Cerro Policía, Río Negro Province, North Patagonia, Argentina (Suppl. Fig. 1).

Diagnosis

Jakapil differs from all other thyreophorans in having: a large, ventral crest on the posterior half of the lower jaw, which is composed of the dentary, the angular and the splenial (medially hidden by the crest); a dorsomedially directed process in the short retroarticular process; leaf-shaped tooth crowns with a prominent mesial edge on their labial surface; maxillary and dentary tooth crowns differ from each other in their apical contour, the former being pointed and strongly asymmetrical, and the latter slightly curved distally with a more rounded and less asymmetrical contour; elongated (articular surface almost or completely beyond the posterior centrum face) and slender (width of less than a half postzygapophyses length) postzygapophyses in dorsal vertebrae; a strongly reduced humerus relative to the femur (proximal humeral width smaller than distal femoral width, see Supplementary Information), with a deep proximal fossa distally delimited by a curved ridge; a very large fibula relative to the femur (anteroposterior length of the proximal end almost comparable to the distal width of the femur); flattened and thin disk-like postcranial osteoderms.

Summarized description

A detailed description of the holotype is provided in the Supplementary Information. Jakapil is a small thyreophoran dinosaur (the subadult holotype is estimated to have been less than 1.5 m in body length and to have weighed 4.5–7 kg; see Supplementary Information, femoral description), with several novelties for a thyreophoran dinosaur.

A short skull is suggested by the size of the skull and jaw bones, and the reduced number of dentary tooth positions (eleven), compared with most non-ankylosaurid thyreophorans28,29. The antorbital and mandibular fenestrae seem absent, as in ankylosaurs29 (Fig. 1a; the mandibular fenestra is also absent in Scelidosaurus10). Dentary and maxillary emarginations are present, as usual in ornithischians30 (Fig. 1a). The block-like basisphenoid is strongly similar to that of Scelidosaurus10, with Vidian canals opened posterodorsally to the basipterygoid processes, the basipterygoid processes lateroventrally projected (unlike the anteriorly directed processes of stegosaurs28 and ankylosaurs29), and a strong cultriform process (as in Lesothosaurus31, Thescelosaurus32 and probably Scelidosaurus10; Fig. 1b).

Jakapil also bears the first predentary bone (Fig. 2a–d) with a plesiomorphic shape in a thyreophoran. It is subtriangular and quite similar to that of Lesothosaurus31, and externally it is ornamented by sulci and foramina, suggesting the presence of a keratinous beak. A beak is also supported in the edentulous and subtly ornamented preserved part of the premaxilla, as in derived thyreophorans28,29. The posterior half of the short lower jaw (Fig. 2a–f) is strongly dorsoventrally expanded, resembling the general shape of the heterodontosaurid33 and basal ceratopsian jaws34. This expansion is composed of a well-developed coronoid eminence (Fig. 2a–d, ce; similar to that in the stegosaur Huayangosaurus35 and most ankylosaurs36) and a large ventral crest at the dentary-angular contact that is unique among thyreophorans (Fig. 2a–d,f, vmc; resembling that of some ceratopsians, see SI). The dentary symphysis is slightly spout-shaped, as in most ornithischians37. Anteriorly, the dentary oral margin is subhorizontal in lateral view (Fig. 2a–d, D), unlike the strongly downturned line of most thyreophorans30,37. There is no evidence of a mandibular osteoderm as occurs in Scelidosaurus and ankylosaurs10. A surangular tubercle (Fig. 2a, st) adjacent to the glenoid fossa seems anteriorly continued by a subtly developed subhorizontal inflection of the anterior lamina (Fig. 2e, hi), in the position of the surangular ridge (synapomorphy of Thyreophora37), though the first is poorly developed. The glenoid fossa is roughly aligned with the tooth row in lateral view (Fig. 2a–d). The short retroarticular process bears a dorsomedially directed process resembling that of several theropods (Fig. 2g, dmp; see Discussion). This process is absent in all other thyreophorans 9,10,35,36.

The tooth crowns are leaf-shaped as in basal ornithischian and thyreophorans10,28,29,38 (Fig. 3). The tooth crowns are swollen labially at their base and lack both cingulum and ornamentation, unlike those of derived eurypodans28,29, heterodontosaurids33 and most neornithischians30,32. The mesial edge of the labial surface in the maxillary and dentary tooth crowns is prominent as in Scelidosaurus10, and ends distally in a denticle-like structure in Jakapil (Fig. 3, me). This prominent edge delimits anteriorly the wear facets of the dentary teeth. A striking difference with respect to most thyreophorans is that the maxillary and dentary tooth crowns are quite different (see Supplementary Information). The maxillary teeth (Fig. 3a–d) show seven/eight mesial and four distal denticles, a vertical apical denticle, and a straighter mesial denticle row (resembling those of non-ankylosaurid and non-stegosaurid thyreophorans10,35,36). The dentary teeth (Fig. 3e–j) bear seven mesial and five/six distal denticles, and a distally curved apical-most denticle. Also, the mesial denticle row is lingually recurved, as in Huayangosaurus35. Large, high-angled wear facets are present (Fig. 3d,h,j; dwf and mwf).

The axial elements are similar to those of Scelidosaurus39 (Fig. 4). The posterior articular surface of an isolated cervical centrum is flattened and seems almost as wide as high. A large foramen is placed just posteroventral to the parapophysis. The dorsal centra are cylindrical and elongated, with subcircular articular surfaces, and are biconcave (Fig. 4c,e). The neural arch is low but the neural canal is larger (Fig. 4d,e, nc). A dorsal neurocentral suture is visible (Fig. 4c, ncs). The diapophyses are laterodorsally directed almost 40° from the horizontal (Fig. 4d, di), at a lower angle than in stegosaurs28 and most ankylosaurs29, unlike the horizontal processes of basal ornithischians38. The postzygapophyses are medially fused in a slender (width of less than a half postzygapophyses length) and strongly elongated posteriorly structure (Fig. 4b, poz; more than in some ankylosaurs, such as Euoplocephalus and Polacanthus; see40,41). An isolated mid-caudal vertebra shows an equidimensional centrum in lateral view, with concave, oval articular surfaces (Fig. 4g). Transverse processes are very small and button-like (Fig. 4g, tp). Postzygapophyses are medially fused and do not extend beyond the centrum edge (Fig. 4g, poz). Proximally, the cross-section of the dorsal ribs is T-shaped. The low curvature of the shaft suggests a wide torso, as occurs in Emausaurus42, Scelidosaurus39, and ankylosaurs29. Some rib fragments with expanded (though broken) posterior edges suggest the presence of intercostal bones (Fig. 4h, ebr), as in Scelidosaurus39, Huayangosaurus43,44, some ankylosaurids45 (and references therein) and some basal ornithopods46. Some ribs are distally expanded (Fig. 4i) like the anterior dorsal ribs of Scelidosaurus39 and Huayangosaurus43.

Girdle and limb bones (see also Suppl. Figs. 2, 3) are mostly broken and with boreholes (probably due to bioerosion) at their ends. The scapular blade (Fig. 4j, sb) is elongated and parallel-sided, without distal expansion, an overall shape that resembles that of several theropods47, contrasting the distally expanded condition in most ornithischians30. A straight and parallel sided scapular blade is common in ankylosaurids29,40. The proximal scapular plate with a high acromial process (Fig. 4j,k, ap) is stegosaurian-like, and the lateral acromial crest (Fig. 4j,k, ac) is developed as in Huayangosaurus43. A low distinct ridge rises posterior to the glenoid fossa and represents the insertion site for the muscle triceps longus caudalis, as occur in ankylosaurids 40. The incomplete coracoid (Fig. 4l) is much shorter than the scapula, unlike that of ankylosaurs29,40, which bear a large coracoid. The coracoid and the scapula are not fused. The partial humeri (Fig. 3m) are strongly reduced in size, with overall limb proportions resembling those of basal ornithischians3,38 and several theropods47. A possible proximal end of the ulna (Fig. 4n) resembles that of other basal ornithischians, though more strongly laterally compressed. The anterolateral process is present (Fig. 4n, alp), and the olecranon process seems absent or poorly developed, as in Scutellosaurus9 and Scelidosaurus39. The ischia are poorly preserved (Fig. 4s). The pubic peduncle is separated from the iliac articulation, unlike the continuous cup-shaped structure of most ankylosaurs29. The shaft of the ischium is straight and parallel-edged, as in Scutellosaurus9 and Scelidosaurus39, and distally tapers as in stegosaurs28. The preserved femoral pieces (Fig. 4p) resemble those of basal ornithischians38,39. The bases of both the broken anterior and fourth trochanters (Fig. 4p, at, ft) are large, suggesting large elements; the fourth trochanter is proximally placed on the femoral shaft (near the height of the base of the anterior trochanter); and the distal end of the femur is slightly curved posteriorly. The proximal end of the right fibula (Fig. 4q) is much larger than that of all other thyreophorans (compared with both the femoral and tibial distal ends) and bears a large anterior curved crest. The block-like non-ungual phalanges and a bluntly pointed hoof-like ungual (Fig. 4o, ph, uph) are similar to those of Scelidosaurus39.

At least five osteoderm types are preserved in the holotype of Jakapil. The cervical elements are composed of an external, low-crested scute (Fig. 4t, sc) over a fused, smooth bone base (Fig. 4t, bb), as in Scelidosaurus48 and several ankylosaurs2,49. A probable cervical element is also composed of a concave base of smooth bone fused to a high, asymmetrical osteoderm (Fig. 4t, aco). The bases of these dermal elements present strong rugosities at one edge, suggesting a sutural contact between (Fig. 4t, rug), as in Scelidosaurus48 and some ankylosaurs (such as Pinacosaurus and Scolosaurus40,49,50). Scute-like post-cervical osteoderms (Fig. 4u) are strongly flattened, disk-shaped, and suboval with a very low crest, resembling those of few ankylosaurs such as Gastonia and Gargoyleosaurus51 (‘body osteoderms’ sensu Kinneer et al.52; see also49). Only one scute shows a high triangular cross-section like those of Scelidosaurus48. Also present are a few conical, spike-like osteoderms with deep concave bases (Fig. 4v), and many flat, disk-shaped, minute (7–10 mm) ossicles without crests (Fig. 4w).

Phylogeny

The phylogenetic analysis using the matrix of Soto-Acuña et al.5 recovers Jakapil within Thyreophora, as the sister taxon of Ankylosauria (Fig. 5). The branch support for the basal thyreophorans is considerably lower than that obtained by Soto-Acuña et al.5, although the support of Stegosauria and some less inclusive eurypodan clades is slightly better (ceratopsians and pachycephalosaurs also show a lower support). The Jakapil autapomorphies in this analysis are: ventrally orientated basipterygoid processes (char. 134; shared with Agilisaurus, Hypsilophodon, Zalmoxes, Tenontosaurus, Dryosaurus, Liaoceratops, Yamaceratops, Leptoceratops, Bagaceratops and Protoceratops); lateral orientation of the basipterygoid process articular facet (char. 136; shared with Homalocephale, Prenocephale, Stegoceras and Yinlong); a straight dentary tooth row in lateral view (char. 166; shared with the ornithischians Lesothosaurus, Eocursor, Scutellosaurus, Pinacosaurus, Euoplocephalus, heterodontosaurids and neornithischians); the presence of a ventral flange on the dentary (char. 170; shared with Psittacosaurus, Yamaceratops and Protoceratops); a well-developed coronoid process (char. 174; shared with heterodontosaurids and neornithischians); a surangular length of more than 50% the mandibular length (char. 183; shared with Stegoceras, Psittacosaurus, Yinlong, Chaoyangsaurus and Hualianceratops); less than 15 dentary teeth (char. 204; shared with heterodontosaurids, Gasparinisaura, Hypsilophodon, Wannanosaurus, Tenontosaurus, Dryosaurus and ceratopsians); apicobasally tall and blade-like cheek teeth crowns (char. 205; shared with Laquintasaura, Psittacosaurus, Yinlong, Chaoyangsaurus and Hualianceratops). Alternative phylogenetic analyses using the data matrices of Maidment et al.4, Norman6 and Wiersma and Irmis8 recover Jakapil as the sister taxon of Eurypoda (Stegosauria + Ankylosauria) and as a basal ankylosaur, respectively (see Supplementary Information). Being recovered either as an ankylosauromorph or a stem-eurypodan, Jakapil is closely related to Scelidosaurus in all analyses. Detailed phylogenetic results and discussion are provided in the Supplementary Information.

Figure 5
figure 5

Time-calibrated strict consensus of 26,784 most parsimonious trees (L = 1267) with the Soto-Acuña et al.5 matrix. CI 0.359, RI: 0.708. Branch supports are figured (Bremer/bootstrap). Record ages references are listed in the Supplementary Information (Suppl. Fig. 4).

A novel thyreophoran anatomy

The discovery of Jakapil in the Cenomanian of Argentina shows a completely new thyreophoran lineage for the Southern Hemisphere. The new taxon shares many features with basal ornithischians and thyreophorans (even with ankylosaurids, see Supplementary Information), but also bears several novelties. The relatively short mandible of Jakapil (Fig. 2a–d), with a large adductor fossa, extensively ornamented surangular, and a well-developed coronoid eminence (even higher than that of Scelidosaurus), resembles that of heterodontosaurids33 and basal ceratopsians34, suggesting a quite strong bite for a thyreophoran36,53. The wear facets of Jakapil (Fig. 3, dwf, mwf) indicate dental occlusion; they are larger than those of most basal thyreophorans and stegosaurs, resembling those of the adult lectotype of Scelidosaurus10, ankylosaurs, ceratopsids and hadrosaurids36,54. Scelidosaurus shows a patched arrangement of wear along the tooth rows10. In Jakapil, the wear on functional cheek teeth is large and high angled, and seems largely distributed along the tooth rows, from the anteriormost teeth backward, as in heterodontosaurids and cerapodans33,54. On the whole, it is probable that Jakapil had a masticatory system that was more efficient than the early thyreophorans in processing vegetation. The en echelon arrangement of tooth crowns suggests a mainly orthal motion for chewing, as in most thyreophorans6,36,53 (and references therein). In Scelidosaurus and other thyreophorans, the ventrally curved tooth row allows a ‘scissor’ effect of the anteriormost teeth10. By contrast, the straight, narrow snout of Jakapil suggests a different feeding strategy, not cutting leaves but selecting elements that require harder processing36. Thus, Jakapil expands the record of herbivorous vertebrates from the Kokorkom paleodesert, complementing this trophic level that contains the lepidosaur Priosphenodon20.

The predentary bone is the first known for a basal thyreophoran. Despite the variably complete lower jaws in Scutellosaurus9, Emausaurus42, Scelidosaurus10, “Tatisaurus55 and “Bienosaurus56, a predentary bone is absent. Norman10 suggested that this may be cartilaginous in Scelidosaurus. The presence of an ossified predentary bone in Jakapil contrasts with that hypothesis. Its plesiomorphic morphology mainly resembles that of the basal ornithischian Lesothosaurus31. It also shows some similarities with the predentary of stegosaurs35 and is very unlike the broad predentary of ankylosaurs29, suggesting a more selective food strategy36. Several features of the predentary, such as the large ventral process, are shared with some basal ceratopsians34. However, this process is usually very robust and proportionally larger that the lateral processes in basal ceratopsians when comparing with Jakapil.

The presence of a dorsomedial process in the articular (Fig. 2c,d,g, dmp) is a new component in a thyreophoran jaw. Some ankylosaurids bear a medial shelf of the glenoid formed by a medial expansion of the articular36. In Jakapil, the glenoid fossa is not medially extended, and the pointed dorsomedial process arises from the retroarticular process. A rather similar process is present in various coelurosaurian theropods, such as dromaeosaurids57, Tyrannosaurus58, Gobipteryx, and ornithurine birds59. In Neornithes, the dorsomedial process of the articular is more anteriorly placed, medial to the mandibular articulation (F. J. R., pers. obs. based on specimens in the Fundación Azara collection: Bubo, Guira, Pterocnemia and Eudromia; see also60), and receives the pterygoid adductor musculature61. In living crocodilians and lepidosaurs, the pterygoid musculature is usually attached to the posteroventral edge of the mandible (also inferred for non-avian dinosaurs61). However, the presence of a medial process in Jakapil may suggest a new placement of the pterygoid musculature, as in birds. If this were the case, the free ventral crest of the mandible (Fig. 2a–d,f, vmc) could have had an exhibition function, rather than being used as an enlarged musculature attachment. In fact, the rugged texture across the mandibular edge resembles an ornamentation element (as in Scelidosaurus10 and Pinacosaurus29; and references therein) with no obvious muscular scar. Otherwise, the crest may represent an enlargement of the surface for musculature insertion, increasing the efficiency of the chewing process (see above).

The armour of Jakapil is also peculiar. Almost all the recovered osteoderms are extremely low, unlike those of basal thyreophorans (Fig. 4r,s,u). The Morphotype A osteoderms of Scutellosaurus62 are very low and bear a central keel, being roughly similar to the disk-shaped osteoderms of Jakapil (Fig. 4s; although the keel of the osteoderms in the latter is smoother). Larger scutes in Jakapil show twice the radial extension of those of Scutellosaurus. Some ankylosaurs, such as Gastonia52 and Gargoyleosaurus51, bear depressed plate-like osteoderms (with or without a low, sharp keel) resembling those of Jakapil. In Scelidosaurus, the osteoderms develop a strong keel48, much higher than that seen in the Jakapil osteoderms. By contrast, large, high-keeled osteoderms and spikes are rare in Jakapil.

The above-mentioned features appear to be novelties, probably due to the poorly known record of thyreophorans in the Southern Hemisphere4,11,12,13,14,15. Moreover, the mixture of plesiomorphic, stegosaurian and ankylosaurian characters of Jakapil may also suggest a basal phylogenetic placement (outside Eurypoda) for this taxon (contra6). In addition, the incorporation of Jakapil into the data matrices of Soto-Acuña et al.5, Norman6, Maidment et al.4, and Wiersma and Irmis8 generates a general decrease in branch support. This demonstrates that the early diversification of thyreophorans is still poorly understood due to their poor Lower-Middle Jurassic fossil record and the scarcity of Gondwanan material4,11, and may explain the ambiguous phylogenetic placement of Jakapil and the early thyreophorans2,4,6.

Bipedalism in armoured dinosaurs

Regarding locomotion, the evolutionary trends observed in thyreophorans are associated with the transition between small, bipedal species and large or graviportal quadrupedal forms, observed in Ankylosauria and Stegosauria1. The transitional state has been attributed to the facultative quadruped Scelidosaurus39. In Jakapil, the relative dimensions of the forelimb, hind limb, and cranial remains (Fig. 4a) bear a greater resemblance to those of the bipedal theropods47, basal ornithischians38 and heterodontosaurids33 than thyreophorans. Moreover, the elongated, non-expanded scapular blade and the strong reduction in the humeri resemble those of specific theropod clades (e.g., abelisaurids47), and unlike the shorter, distally expanded scapular blade of the fully quadrupedal ornithischians and sauropods.

A comparison of the limb elements of some thyreophorans (Suppl. Fig. 4) shows the strong reduction in size of the humerus in Jakapil. Considering a reconstruction of the elements based on Scelidosaurus (the nearest taxon to Jakapil in all phylogenetic analyses), Scutellosaurus (a basal form) and Jinyunpelta (an ankylosaur), the reduction in size is evident. Despite the incompleteness of the material, we quantified this reduction comparing the proximal humeral (PHW) and the distal femoral widths (DFW; the distal end of the femur in Jakapil was measured in the only well-preserved transversal section, although this is not the most distal). The proximal humeral width/distal femoral width ratio (HFR) is lower in the basal taxa (Jakapil, Scutellosaurus and Scelidosaurus) with respect to the ankylosaurs Jinyunpelta and Euoplocephalus, showing a widening of the humerus in the quadrupedal taxa reaching a comparable width (ratio ~ 1). Such widening in the proximal humeral end is evident in the lack of fit of the Jakapil bones in the Jinyunpelta proportions, also suggesting limb proportions more similar to those of basal forms. Moreover, the incomplete distal end of the femur in Jakapil allows even smaller values of the HFR ratio (and of the humerus size). Also, a shortening of the humerus relative to the femur is present in the obligate quadrupedal Ankylosauria. Regardless of the unknown humeral length, the lack of a robust humerus in Jakapil allows us to reject a fully quadrupedal stance like that of the heavily built ankylosaurs.

In summary, the overall limb dimensions and estimations (with forelimb and olecranon process both reduced63), and the femoral anatomical similarities to the basal ornithischians and thyreophorans39 (e.g., large trochanters and a non-columnar element) suggest a bipedal stance in the specimen. However, the incompleteness of the remains demands caution to define the stance of Jakapil. To make more complex the scenery, Jakapil still retains quadruped-associated features, such as a probable anterolateral process in the ulna, and stout metacarpals63 (and references therein). More complete material is needed to make accurate quantitative comparisons with other taxa and clarify its stance.

Paleobiogeography of early thyreophorans

The Early Jurassic thyreophoran record consists of basal forms known from several continents showing a Pangean distribution. These comprise Scutellosaurus (Hettangian-Toarcian of the USA9), Scelidosaurus (Sinemurian of the UK; see 6,10), Emausaurus (Toarcian of Germany42), ‘Lusitanosaurus’ (Sinemurian of Portugal1), ‘Bienosaurus’, ‘Tatisaurus’ (both from the Hettangian-Sinemurian of China; see55,56) and Yuxisaurus (late Sinemurian-Toarcian64). Some recent papers recover the unarmoured ornithischians Lesothosaurus (Hettangian-Sinemurian of South Africa and Lesotho; see3,31) and Laquintasaura (Hettangian of Venezuela; see3,4,65) as Gondwanan basal members of Thyreophora. However, alternative studies show their phylogenetic position as controversial3,6,65, so they cannot be confidently assigned to Thyreophora.

The extensive distribution of armoured basal thyreophorans (excluding both Lesothosaurus and Laquintasaura) across the northern landmasses during the Early Jurassic shows a rapid diversification after the origin of the clade. However, basal thyreophoran remains from Gondwana known from the Middle Jurassic of Niger66, along with problematic material from the Lower Jurassic (Sinemurian-Pliensbachian) of India (see55,67 and references therein), suggest a more extensive distribution for the early thyreophorans. In addition, the early distribution of stegosaurs and ankylosaurs shows a similar pattern. The presence of the Middle Jurassic basal stegosaur Isaberrysaura from the Bajocian of Argentina68,4 and the stegosaurid Adratiklit from the Bathonian-Callovian of Morocco4 depict a distribution of the early stegosaurs that extends into southern landmasses. The Middle Jurassic thyreophoran fossil record also includes the stegosaur Loricatosaurus from the Callovian of England and France, the ankylosaurs Sarcolestes and ‘Cryptosaurus’ from the Callovian of England, the ankylosaur Spicomellus from the Bathonian-Callovian of Morocco15, the ankylosaur ‘Tianchisaurus’ from the Callovian of China, and indeterminate remains from Europe and Asia (see4,67 and references therein). On the whole, the Pangean distribution of early thyreophorans across the Early-Middle Jurassic makes it difficult to recognize a source area for Thyreophora and the most inclusive clades within it.

In this context, Jakapil not only increases the poor Gondwanan record of thyreophorans, but also establishes a theoretical framework for Gondwanan basal thyreophoran evolution and distribution (Fig. 5). Whether Jakapil is recovered as an ankylosaur or a non-eurypodan thyreophoran, it is closely related to Scelidosaurus (see Supplementary Information). The presence of a basal thyreophoran in the early Late Cretaceous of South America shows that an ancient Gondwanan lineage of early thyreophorans evolved independently from those of the Northern Hemisphere, whose relationships have to be traced during the Early-Middle Jurassic Pangean rupture and the consequent isolation of Gondwana and later South America. Accordingly, early Gondwanan thyreophorans survived a long time after the Pangean breakup, whereas the northern early thyreophorans seem to have gone extinct by the Middle Jurassic. The persistence of a Gondwanan lineage of thyreophorans finds support in new thyreophoran remains recovered from the Lower Cretaceous rocks of the Bajada Colorada Formation (Berriasian-Hauterivian), also from the Argentinian Patagonia (Neuquén Province). These remains are composed of a diversity of osteoderms, showing either a mixture of thyreophorans at the site, or a new, still poorly understood lineage69.

A new lineage of Gondwanan thyreophorans was recently proposed by Soto-Acuña et al.5, Parankylosauria. This clade includes Antarctopelta (Campanian-Maastrichthian of Antarctica), Stegouros (Campanian-Maastrichthian of South America), and the traditionally basal ankylosaur Kunbarrasaurus (Albian-Cenomanian of Australia)5. Despite their extensive Gondwanan distribution during the Cretaceous, anatomical differences with Jakapil are remarkable. Parankylosaurs show ankylosaurian features, like broad ornamented skulls, depressed caudal vertebrae, similar limb proportions, and a columnar femur with both reduced anterior and fourth trochanters (among others), which contrast with the mixture of features of Jakapil. Even more, ankylosaurian features present in Jakapil were recognized as convergent with ankylosaurids within Euankylosauria (e.g., a straight dentary tooth row in lateral view, a small diastema on the dentary, a shallow symphysis, scapular blade shape; see Supplementary Information) rather than with parankylosaurs. Therefore, a close phylogenetic relation between them is unlikely. Until more records contribute to the understanding of Gondwanan thyreophorans, both Jakapil and parankylosaurs belong to two different lineages. This shows that Gondwanan thyreophorans were a diverse clade with morphologically disparity.

On the other hand, further work will help to fill the extensive gap between the early thyreophorans and the Cretaceous remains from South America. Recent research is reflected in an increase in the thyreophoran fossil record from South America, with all its implications for thyreophoran evolution11,12,13,14,69,70; and this paper). The discovery of Jakapil not only supports the presence of a new Gondwanan lineage of early thyreophoran dinosaurs that persisted in Gondwana for a long time, but has also brought to light the importance of the Gondwanan fossil record in the study of the origin and evolution of dinosaurs (and other clades).

Methods

Morphological datasets

We used the dataset of Soto-Acuña et al.5, that comprises a broad sample of ornithischians suitable to test the phylogenetic position of Jakapil, a specimen with a complex mixture of features complete enough to include both several outgroups (non-thyreophoran ornithischians) and also both groups of thyreophorans. The dataset consists of 75 taxa and 383 morphological characters (see character list in Soto-Acuña et al.5 and references therein). Marasuchus was fixed as the outermost outgroup taxon. All characters were unweighted. Characters 2, 23, 31, 39, 125, 163, 196, 203, 204, 222, 227, 238, 243, 247, 268, 292, 296, 302, 306, 320 and 361 were treated as additive. Memory space was made for 1,500,000 trees.

Phylogenetic analyses

Phylogenetic analyses of the morphological matrix were carried out in TNT v1.5 (see Supplementary Information). A Traditional search was applied with 10,000 replicates of Wagner trees under the tree bisection reconnection (TBR) algorithm, saving 10 trees per replication. Trees saved in memory were resampled with an additional round of TBR. The support for each node in the trees was assessed in TNT. Bremer values were also recorded with Traditional searches until 22 suboptimal trees. Bootstrap analysis was carried out using 10,000 pseudoreplicates with a Traditional search, and Absolute frequencies. Consistency and retention indexes (from the archive STATS.RUN), character mapping, and moving taxon positions over the consensus to test parsimony, were carried out in TNT. The detailed phylogenetic methods are provided in the Supplementary Information.

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Acknowledgements

The authors thank to Mariluan family for kindly allowing us the access to the fossiliferous locality of Cerro Policía and to the Secretaría de Cultura of the Río Negro Province for allowing the respective permits; to the Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Agencia Nacional de Promoción de la Investigación, el Desarrollo Tecnológico y la Innovación (projects PICT 2014-0564 and PICT 2018-04598), the Fundación Azara-Universidad Maimónides, the Spanish Ministerio de Ciencia, Innovación e Universidades and the European Regional Development Fund (projects CGL2017-85038-P and PID2021-122612OB-I00), and the Gobierno Vasco/EJ (research group IT1418-19) for the funding. F. J. R. thanks to I. Díaz-Martínez, A. Martinelli, L. Leahey, R. Molnar, A. Vargas Milne, S. Soto Acuña, and M. Baron for digital material; to L. Pazo and J. Kaluza for the material preparation; to the members of the Area de Paleontología of the Fundación Azara, especially F. Garberoglio, L. Fernández Dumont and J. P. Garderes, for all the helping; to R. Ponti for the thin sectioning, and I. Cerda for his advice on histological aspects; to S. Bogan, S. M. Álvarez and J. Meluso for facilitate the access to the Fundación Azara collections. S. A. acknowledges J. Kaluza for identifying key materials. Thanks to R. Glasgow for reviewing the English text of the manuscript. Special thanks to the reviewers Susannah Maidment, Victoria Arbour, and an anonymous reviewer, whose comments strongly improved the manuscript.

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F.J.R. undertook the anatomical description, phylogenetic analyses, discussion, and produced the figures. All authors contributed to the interpretation of the results and discussions. S.A. led the project.

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Facundo J. Riguetti.

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Riguetti, F.J., Apesteguía, S. & Pereda-Suberbiola, X. A new Cretaceous thyreophoran from Patagonia supports a South American lineage of armoured dinosaurs.
Sci Rep 12, 11621 (2022). https://doi.org/10.1038/s41598-022-15535-6

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  • Received: 04 December 2021
  • Accepted: 24 June 2022
  • Published: 11 August 2022
  • DOI: https://doi.org/10.1038/s41598-022-15535-6

 

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Pine beetles adapting to a changing climate, finds study – BC News – Castanet.net

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Exposure to increased levels of carbon dioxide in the atmosphere accelerates the reproductive cycle of mountain pine beetles, a new study has found.

The findings, published in the journal Global Change Biology, show the beetle’s typical 40-day brooding period accelerated to 30 days when they were exposed to higher levels of carbon dioxide (CO2), the driving force behind human-caused climate change.

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Rashaduz Zaman, lead author and a PhD candidate in forest biology and management at the University of Alberta, said the results show that as the climate changes, insects like the mountain pine beetle are adapting at a time trees are becoming more vulnerable to things like drought.

“The prediction is the beetle can bounce back and attack more,” Zaman said.

Since the early 1990s, the mountain pine beetle has attacked about 18 million hectares of forest, including half of the total volume of commercial lodgepole pine in British Columbia, according to Natural Resources Canada.

Warmer winters and drier summers allowed the beetle to extend well beyond its traditional range in the boreal forests of B.C. But it remained unclear how the beetle will be affected by climate change and the rising concentrations of ozone and carbon dioxide that come with it.

Beetles learned to adapt in a simulated future climate

Climate change has pushed CO2 concentrations past 421 parts per million, substantially higher than the pre-industrial level of 280 parts per million, and less than half the 1,000 parts per million that could be achieved at some point this century.

To simulate those conditions, the University of Alberta researchers introduced male and female pairs into freshly cut lodgepole pine logs, which were placed in a controlled climate chamber.

Next, they manipulated the environment by changing levels of CO2, ozone and relative humidity between 33 per cent and 66 per cent. The researchers also introduced three species of fungus that have a symbiotic relationship with the beetles. After a month or so, the logs were returned to ambient conditions to allow the beetles’ broods to emerge.

mountain-pine-beetle-range-change
The historic range (before 2000) and expanded range (after 2000) of the mountain pine beetle in Canada. NRCan

The researchers found the lower the humidity, the more the fungi grew and the more the beetles reproduced. High CO2 concentrations were also found to speed up the growth of larvae.

But when it came to ozone — another gas whose atmospheric concentration is expected to rise over the coming decades — increased concentrations were initially found to have a negative impact on mountain pine beetle reproduction and brood fitness. ?

?In the wild, a mountain pine beetle will attack a tree by making a hole in it. Once inside, it releases pheromones to attract other beetles, while releasing fungi that blocks a tree’s own toxic defences and inhibits arboreal mechanisms for transporting water and nutrients.

In the lab, the spike in ozone gas was originally found to degrade the pheromones beetles rely on for finding a mate. At first, it seemed the gas may have evened the odds and pushed back against the effects of CO2. But over the next three to four months, the following beetle generations started to adapt.

“When we tested the ozone, the first generation that came out, they were smaller and lower weight. By the third generation, they developed resistance,” said Zaman.

Expect more outbreaks

The results could have significant results for places like British Columbia, where mountain pine beetle infestations have already wiped out millions of hectares of forest in recent decades.

Zaman said climate modelling suggests more drought in B.C.’s future, something expected to weaken pine trees and make them more susceptible to infestation.

He said years of above-average wildfire may have helped halt the beetle’s advance, but over the long-term, Zaman and his colleagues forecast the mountain pine beetle will be able to adapt to a new forest regime and once again cause “significant ecological and economic consequences.”

“B.C. has been a hot spot for the pine beetle,” Zaman said. “We expect more outbreaks.”

If there’s any good news, the scientist said more studies still need to be done to confirm what they found.

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Record breaker! Milky Way's most monstrous stellar-mass black hole is sleeping giant lurking close to Earth (Video) – Space.com

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The Milky Way has a big newfound black hole, and it lurks close to Earth! This sleeping giant was discovered with the European space telescope Gaia, which tracks the motion of billions of stars in our galaxy. 

Stellar-mass black holes are created when a large star runs out of fuel and collapses. The new discovery is a landmark, representing the first time that a big black hole with such an origin has been found close to Earth.

The stellar-mass black hole, designated Gaia-BH3, is 33 times more massive than our  sun. The previous most massive black hole of this class found in the Milky Way was a black hole in an X-ray binary in the Cygnus constellation (Cyg X-1), whose mass is estimated to be around 20 times that of the sun. The average stellar-mass black hole in the Milky Way is about 10 times heftier than the sun.

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Gaia-BH3 is located just 2,000 light years from Earth, making it the second-closest black hole to our planet ever discovered. The closest black hole to Earth is Gaia-BH1 (also discovered by Gaia), which is 1,560 light-years away. Gaia-BH1 has a mass around 9.6 times that of the sun, making it considerably smaller than this newly discovered black hole. 

Related: New view of the supermassive black hole at the heart of the Milky Way hints at an exciting hidden feature (image)

“Finding Gaia BH3 is like the moment in the film ‘The Matrix’ where Neo starts to ‘see’ the matrix,” George Seabrook, a scientist at Mullard Space Science Laboratory at University College London and a member of Gaia’s Black Hole Task Force, said in a statement sent to Space.com. “In our case, ‘the matrix’ is our galaxy’s population of dormant stellar black holes, which were hidden from us before Gaia detected them.”

Seabroke added that Gaia BH3 is an important clue to this population, because it is the most massive stellar black hole found in our galaxy. 

Of course, Gaia-BH3 is a small fry compared to the supermassive black hole that dominates the heart of the Milky Way, Sagittarius A* (Sgr A*), which has a mass 4.2 million times that of the sun. Supermassive black holes like Sgr A* aren’t created by the deaths of massive stars but rather by mergers of progressively larger and larger black holes.

A diagram showing the location of the three black holes discovered by Gaia (Image credit: ESA/Gaia Collaboration)

Sleeping giant black hole caused stellar companion to throw a wobbly

All black holes are marked by an outer boundary called an event horizon, at which point the black hole’s escape velocity exceeds the speed of light. That means an event horizon is a one-way light-trapping surface beyond which no information can escape. 

As a result, black holes don’t emit or reflect light, meaning they can only be “seen” when they are surrounded by material that they gradually feed on. Sometimes, this means a black hole in a binary system pulling material from a companion star, which forms a disk of gas and dust around it.

The tremendous gravitational influence of black holes generates intense tidal forces in this surrounding matter, causing it to glow brightly with material that is destroyed and consumed, also emitting X-rays. Additionally, the material the black hole doesn’t feast on can be channeled to its poles and blasted out as near-light speed jets, which are accompanied by the emission of light.

All of these light emissions can allow astronomers to spot black holes. The question is, how can “dormant” black holes that aren’t feeding on gas and dust around them be detected? For instance, what if a stellar-mass black hole has a companion star, but the two are too widely separated for the black hole to snatch stellar matter from its binary partner? 

In cases like this, the black hole and its companion star orbit a point that represents the system’s center of mass. This is also the case when a star is orbited by a light companion, such as another star or even a planet.

Orbiting the center of mass results in a wobble in the motion of the star, which is visible to astronomers. Because Gaia is adept at precisely measuring the motion of stars, it is the ideal instrument to see this wobble.

Gaia’s Black Hole Task Force set about looking for odd wobbles that couldn’t be accounted for by the presence of another star or a planet and that indicated a heavier companion, possibly a black hole. 

The region around the black hole Gaia-BH3. (Image credit: ESO/Digitized Sky Survey 2. Acknowledgement: D. De Martin.)

Homing in on an old giant star in the constellation Aquila, located 1,926 light-years from Earth, the team found a wobble in the star’s path. That wobble suggests that the star is locked in orbital motion with a dormant black hole of exceptionally high mass. The two are separated by a distance that ranges from the distance between the sun and Neptune at their widest and our star and Jupiter at their closest.

“It’s a real unicorn,” lead researcher Pasquale Panuzzo of CNRS, Observatoire de Paris in France, said in a statement. “This is the kind of discovery you make once in your research life. So far, black holes this big have only ever been detected in distant galaxies by the LIGO-Virgo-KAGRA collaboration, thanks to observations of gravitational waves.”

Related: What are gravitational waves?

Three stellar-mass black holes in our galaxy: (left) Gaia BH1, (middle) Cygnus X-1, and (right) Gaia BH3, whose masses are 10, 21, and 33 times that of the sun, respectively. Gaia BH3 is the most massive stellar black hole found to date in the Milky Way. (Image credit: ESO/M. Kornmesser)

Thanks to the sensitivity of Gaia, the Black Hole Task Force was also able to put constraints on the mass of Gaia-BH3, finding it to possess 33 solar masses. 

“Gaia-BH3 is the very first black hole for which we could measure the mass so accurately,” said Tsevi Mazeh, a scientist and Gaia collaboration member at Tel Aviv University. “At 30 times that of our sun, the object’s mass is typical of the estimates we have for the masses of the very distant black holes observed by gravitational wave experiments. Gaia’s measurements provide the first undisputable proof that [stellar-mass] black holes this heavy do exist.”

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However, the Gaia-BH3 system is bound to be of great interest to scientists for more than just its proximity to Earth and the mass of its black hole.

The star in this system is a sub-giant star that is around five times as large as the sun with 15 times its brightness, though it is cooler and less dense than our star. The Gaia-BH3 companion star is mainly composed of hydrogen and helium, the universe’s two lightest elements, lacking heavier elements, which astronomers (somewhat confusingly) call “metals.”

The fact that this star is “metal-poor” suggests that the star that collapsed and died to create Gaia-BH3 also lacked heavier elements. Metal-poor stars are expected to shed more mass than their more metal-rich counterparts during their lives, so scientists have questioned if they can maintain enough mass to birth black holes. Gaia-BH3 represents the first hint that metal-poor stars can indeed do so. 

“Gaia’s next data release is expected to contain many more, which should help us to ‘see’ more of ‘the matrix’ and to understand how dormant stellar black holes form,” Seabroke concluded. 

The team’s research was published today (April 16) in the journal Astronomy & Astrophysics.

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Nasa confirms metal chunk that crashed into Florida home was space junk

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A heavy chunk of metal that crashed through the roof of a Florida home is, in fact, space junk, Nasa has confirmed.

The federal space agency said that a cylinder slab that tore through a house in Naples, Florida, last month was debris from a cargo pallet released from the international space station in 2021, according to a Nasa blogpost.

The determination was made after the agency collected the debris from the Florida home and analyzed it at the Kennedy Space Center.

“Based on the examination, the agency determined the debris to be a stanchion from the Nasa flight support equipment used to mount the batteries on the cargo pallet,” the agency said.

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The pallet, which contained ageing nickel hydride batteries, was released after new lithium-ion batteries were installed in the space station.

The debris was supposed to be destroyed in the Earth’s atmosphere. Instead, a piece of metal crashed through a Florida home, NBC News reported.

The debris weighs 1.6lb and measures about 4in by 1.6in.

Homeowner Alejandro Otero described the experience to WINK News, which first reported the story.

“It was a tremendous sound. It almost hit my son. He was two rooms over and heard it all,” Otero said to WINK.

“Something ripped through the house and then made a big hole on the floor and on the ceiling.”

The scientific journal Ars Technica previously speculated that the metal was probably space station debris. Nasa finally confirmed the origin of the chunk on Monday.

The space agency added that it would investigate how the debris managed to survive its re-entry into Earth’s atmosphere and “update modeling and analysis”.

It is unclear if Nasa will cover the cost of damages to Otero’s home.

In comments posted to X shortly after the incident, Otero said that Nasa had not responded to messages he left with the agency.

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