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Osteology of the Wide-Hipped Titanosaurian Sauropod Dinosaur Savannasaurus Elliottorum from the Upper Cretaceous Winton Formation of Queensland, Australia

Poropat, S; Mannion, P; Upchurch, P; Tischler, T; Sloan, T; Sinapius, G; Elliott, J; (2020) Osteology of the Wide-Hipped Titanosaurian Sauropod Dinosaur Savannasaurus Elliottorum from the Upper Cretaceous Winton Formation of Queensland, Australia. Journal of Vertebrate Paleontology , 40 (3) , Article e1786836. 10.1080/02724634.2020.1786836. Green open access

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Abstract

The titanosaurian sauropod dinosaur Savannasaurus elliottorum is represented by a partial postcranial skeleton from the lower Upper Cretaceous (Cenomanian–lowermost Turonian) Winton Formation of Queensland, northeast Australia. Here, we present a detailed description of this specimen, as well as an emended diagnosis for this titanosaur. Savannasaurus elliottorum displays numerous character states that are generally regarded as plesiomorphic for Titanosauria, as well as several traits that are often regarded as apomorphic of that clade or a less inclusive subset thereof. Several features of Savannasaurus support a close relationship with the coeval Diamantinasaurus matildae, and this clade appears to occupy an early-branching position within Titanosauria. Relative to body size, the thoracic and abdominal breadth of Savannasaurus is greater than that seen in giant titanosaurs such as the contemporaneous South American lognkosaurians; however, this relative breadth is not quite as extreme as that of the small-bodied latest Cretaceous saltasaurines, or Opisthocoelicaudia skarzynskii. The possible advantages engendered by the barrel-shaped thorax, robust limbs, wide-gauge gait, and lack of hyposphene-hypantrum articulations are explored, and it is hypothesized that these traits were positively selected by the wet, temperate floodplain environment in which Savannasaurus lived. Greater stability and flexibility might have reduced the risk of bogging, and/or facilitated more expedient self-extraction from muddy waterholes. Similar environmental pressures acting upon other titanosaurian taxa or clades elsewhere might have led to the repeated independent development, or accentuation, of the bauplan regarded as ‘typical’ for the clade Titanosauria. This would explain the many observed convergences between Savannasaurus and Diamantinasaurus, and Saltasauridae.

Type: Article
Title: Osteology of the Wide-Hipped Titanosaurian Sauropod Dinosaur Savannasaurus Elliottorum from the Upper Cretaceous Winton Formation of Queensland, Australia
Open access status: An open access version is available from UCL Discovery
DOI: 10.1080/02724634.2020.1786836
Publisher version: https://doi.org/10.1080/02724634.2020.1786836
Language: English
Additional information: This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Earth Sciences
URI: https://discovery.ucl.ac.uk/id/eprint/10098670
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