Argentavis is an extinction genus of Teratornithidae known from three sites in the Epecuén and Andalhualá Formations in central and northwestern Argentina dating to the Miocene (Huayquerian). The type species, A. magnificens, is sometimes called the giant teratorn. Argentavis was among the largest flying to ever exist, holding the record for heaviest flying bird, although it was surpassed in wingspan after the 2014 description of Pelagornis sandersi, which is estimated to have possessed wings some 20% longer than those of Argentavis. Argentavis at Fossilworks.org Ancient American bird was glider. BBC, 2007-JUL-02. Retrieved 2008-JAN-14
Kenneth Campbell Jr. and Eduardo Tonni would go on to describe MLP 65-VII-29-49 in a 1980 paper and designated it as the Holotype of the new taxon Argentavis magnificens. The generic name Argentavis comes from the Latin “argentum”, meaning silver, and “avis”, meaning bird, and was used in reference to Argentina, the country where the remains of the animal were found. The specific name magnificens comes from the same word in Latin, meaning magnificent. They note that all the material has been severely fractured, although most of the material except for the skull was not severely crushed. This fracturing, among other sustained damages, meant that most of the postcranial skeleton lacked its diagnostic portions. However, the skull and quadrate provided strong enough evidence of Argentavis' relation to Teratornis, and permitted Campbell and Tonni to describe it as a Teratornithidae. This made it the third described genus in this family and the first from outside North America.
Campbell would go on to describe three additional specimens of Argentavis in a 1995 paper. All three were found during a survey of museum collections in Argentina in 1983. The first specimen, an uncatalogued Ungual, was found in the collections of the Museo Municipal de Ciencias Naturales in Mar del Plata. The specimen was collected from the genus’ type horizon, the Cerro Azul Formation of Argentina, in March of 1982 by Galilio Scaglia. However, it was found roughly 60km west of the type locality at a site near Carhué. The specimen was referred to Argentavis based on the development of the attachment site of the flexor muscle and a prominent groove running along the lateral and medial surface of the bone along with its size, being roughly 1.5x the size of the largest ungual phalanges of Teratornis merriami recovered from the La Brea Tar Pits. Marcos Cenizo and colleagues would revisit this element in 2012 and refer it to the family Phorusrhacidae instead, based on the fact that the provided characters were too poor to confirm an assignment to Argentavis. Cenizo and colleagues also mention a previously unreported proximal fragment of an ungual phalanx which was found associated with the holotype during further study. This element lacked both distinctive features of Campbell's 1995 element and possessed numerous others, confirming that it does not belong to A. magnificens.
The other specimens were found in the Andalhualá Formation of the Valle de Santa María, approximately 1200 km northwest of Argentavis' type locality. Two radioisotope dates were given for this formation in a 1979 publication by Marshall and colleagues, giving dates of 6.02 and 6.68 mya. This confirmed and refined the earlier Huayquerian (8-5 mya) estimate given by Campbell and Tonni in 1980. Both of these specimens are housed in the collections of the Paleontología Vertebrados Lillo in San Miguel de Tucumán. The first, a left coracoid (PVL 4600), was collected by G. Bossi in March of 1983. The second specimen, a tibiotarsus, was recovered by L. Peirano in October of 1939. These specimens were said to be smaller than the equivalent material in the holotype specimen and to have been in slightly better condition, although few new osteological characters could be differentiated.
Teratornithidae was included in a phylogenetic analysis that was published by Steven Emslie in 1988, reproduced below. The analysis was conducted using cranial characters of various taxa within the order Ciconiiformes, the storks, with a specific focus on Vulturidae (Cathartidae, New World vultures). This analysis included Teratornis as a representative of Teratornithidae, and found the group to be just outside of Vulturidae. Based off of the fact that this analysis found more shared characters distinguishing Vulturidae and Teratornithidae from other Ciconiiformes than ones specific to either group, indicating a close relation, Emslie suggested that Brodkorb's 1964 placement of teratornithids as a subfamily within Vulturidae might be more correct than retaining the familial rank, as Campbell and Tonni have done. Currently, Teratornithidae is still at the familial rank.
Said quadrate has a number of key differences that allowed distinction from Teratornis. The quadratojugal socket is positioned farther back, and the surface for mandibular articulation extends more anterioventrally, but not as far forwards proportionally. The articulation with the anteromedial portion is also much larger proportionally, lying at a lesser angle when compared to the horizontal. The site of articulation for the squamosal bone is hemispheric, and the articulation of the pterygoid is positioned more laterally. The shaft of the coracoid is laterally compressed near the humerus, with the anterior-glenoid facet nearly flat. Medially to the glenoid facet, the shaft is convex. The glenoid facet itself is concave when viewed from the side, with the deepest point just lower than the midline. In posterior view its nearly vertical, and lined up with the coracoidal fenestra, which lies much closer to the procoracoid. The procoracoid is reduced, with the ventral ridge leading from it to the internal distal angle being small, but distinct.
Argentavis
The tibiotarsus differs from that of Teratornis by being slightly curved when viewed from the front, although this might be due in part to breakage, and in having an underdeveloped fibular crest. The proximal end of the tendinal groove is more symmetrical, and closer to the center of the shaft, and the internal ligamental prominence is longer, more prominent, and lies proximally to the position observed in T. merriami.
The initial description by Campbell and Tonni in 1980 tentatively estimated the body mass of Argentavis at , while the 1983 paper by the same authors estimated its body mass at approximately . Subsequent studies have suggested a lower body mass estimate between . Argentavis still retains the title of the heaviest known flying bird by a considerable margin, with the aforementioned P. sandersi being estimated to have weighed no more than . Since A. magnificens is known to have lived in terrestrial environments, another good point of comparison is the Andean condor, the largest extant flighted land bird both in average wingspan and weight, with the former spanning up to with an average of around , and the latter reaching a maximum of up to . New World vultures such as the condor are thought to be the closest living relatives to Argentavis and other teratorns. Average weights are much lower in both the wandering albatross and Andean condor than in Argentavis, at approximately and , respectively.
As a rule of thumb, a wing loading of 25 kg/m2 is considered the limit for avian flight. A number of estimates related to wing loading have been produced for Argentavis, most notably the wing area, estimated at , and the wing loading, estimated at 84.6 N/m2 (1.77 lb/ft2), or about 8.64 kg/m2. The heaviest extant flying birds are known to weigh up to a maximum of (there are several contenders, among which are the European great bustard and the African kori bustard). An individual mute swan, which may have lost the power of flight due to extreme weight, was found to have weighed .
Although its legs were strong enough to provide it with a running or jumping start, the wings were simply too long to flap effectively until the bird had gained some vertical distance, meaning that, especially for takeoff, Argentavis would have depended on the wind. Argentavis may have used mountain slopes and headwinds to take off, and probably could manage to do so even from gently sloped terrain with little effort. It may have flown and lived much like the modern Andean condor, scanning large areas of land for carrion. It is probable that it utilised thermal currents to stay aloft, and it has been estimated that the minimal velocity for A. magnificens is about or . The climate of the Andean foothills in Argentina during the late Miocene was warmer and drier than today, which would have further aided the bird in staying aloft atop thermal updrafts.
Classification
Description
Size
Paleobiology
Life history
Flight
Predatory behavior
Further reading
External links
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