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      Extinction and dawn of the modern world in the Carnian (Late Triassic)

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          Abstract

          The roots of modern-style ecosystems go back to the Carnian (ca. 233 Ma), a time of global climate change and extinction.

          Abstract

          The Carnian Pluvial Episode (Late Triassic) was a time of global environmental changes and possibly substantial coeval volcanism. The extent of the biological turnover in marine and terrestrial ecosystems is not well understood. Here, we present a meta-analysis of fossil data that suggests a substantial reduction in generic and species richness and the disappearance of 33% of marine genera. This crisis triggered major radiations. In the sea, the rise of the first scleractinian reefs and rock-forming calcareous nannofossils points to substantial changes in ocean chemistry. On land, there were major diversifications and originations of conifers, insects, dinosaurs, crocodiles, lizards, turtles, and mammals. Although there is uncertainty on the precise age of some of the recorded biological changes, these observations indicate that the Carnian Pluvial Episode was linked to a major extinction event and might have been the trigger of the spectacular radiation of many key groups that dominate modern ecosystems.

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          PHANEROZOIC BIODIVERSITY MASS EXTINCTIONS

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            A basal dinosaur from the dawn of the dinosaur era in southwestern Pangaea.

            Upper Triassic rocks in northwestern Argentina preserve the most complete record of dinosaurs before their rise to dominance in the Early Jurassic. Here, we describe a previously unidentified basal theropod, reassess its contemporary Eoraptor as a basal sauropodomorph, divide the faunal record of the Ischigualasto Formation with biozones, and bracket the formation with (40)Ar/(39)Ar ages. Some 230 million years ago in the Late Triassic (mid Carnian), the earliest dinosaurs were the dominant terrestrial carnivores and small herbivores in southwestern Pangaea. The extinction of nondinosaurian herbivores is sequential and is not linked to an increase in dinosaurian diversity, which weakens the predominant scenario for dinosaurian ascendancy as opportunistic replacement.
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              The origin and early evolution of dinosaurs.

              The oldest unequivocal records of Dinosauria were unearthed from Late Triassic rocks (approximately 230 Ma) accumulated over extensional rift basins in southwestern Pangea. The better known of these are Herrerasaurus ischigualastensis, Pisanosaurus mertii, Eoraptor lunensis, and Panphagia protos from the Ischigualasto Formation, Argentina, and Staurikosaurus pricei and Saturnalia tupiniquim from the Santa Maria Formation, Brazil. No uncontroversial dinosaur body fossils are known from older strata, but the Middle Triassic origin of the lineage may be inferred from both the footprint record and its sister-group relation to Ladinian basal dinosauromorphs. These include the typical Marasuchus lilloensis, more basal forms such as Lagerpeton and Dromomeron, as well as silesaurids: a possibly monophyletic group composed of Mid-Late Triassic forms that may represent immediate sister taxa to dinosaurs. The first phylogenetic definition to fit the current understanding of Dinosauria as a node-based taxon solely composed of mutually exclusive Saurischia and Ornithischia was given as "all descendants of the most recent common ancestor of birds and Triceratops". Recent cladistic analyses of early dinosaurs agree that Pisanosaurus mertii is a basal ornithischian; that Herrerasaurus ischigualastensis and Staurikosaurus pricei belong in a monophyletic Herrerasauridae; that herrerasaurids, Eoraptor lunensis, and Guaibasaurus candelariensis are saurischians; that Saurischia includes two main groups, Sauropodomorpha and Theropoda; and that Saturnalia tupiniquim is a basal member of the sauropodomorph lineage. On the contrary, several aspects of basal dinosaur phylogeny remain controversial, including the position of herrerasaurids, E. lunensis, and G. candelariensis as basal theropods or basal saurischians, and the affinity and/or validity of more fragmentary taxa such as Agnosphitys cromhallensis, Alwalkeria maleriensis, Chindesaurus bryansmalli, Saltopus elginensis, and Spondylosoma absconditum. The identification of dinosaur apomorphies is jeopardized by the incompleteness of skeletal remains attributed to most basal dinosauromorphs, the skulls and forelimbs of which are particularly poorly known. Nonetheless, Dinosauria can be diagnosed by a suite of derived traits, most of which are related to the anatomy of the pelvic girdle and limb. Some of these are connected to the acquisition of a fully erect bipedal gait, which has been traditionally suggested to represent a key adaptation that allowed, or even promoted, dinosaur radiation during Late Triassic times. Yet, contrary to the classical "competitive" models, dinosaurs did not gradually replace other terrestrial tetrapods over the Late Triassic. In fact, the radiation of the group comprises at least three landmark moments, separated by controversial (Carnian-Norian, Triassic-Jurassic) extinction events. These are mainly characterized by early diversification in Carnian times, a Norian increase in diversity and (especially) abundance, and the occupation of new niches from the Early Jurassic onwards. Dinosaurs arose from fully bipedal ancestors, the diet of which may have been carnivorous or omnivorous. Whereas the oldest dinosaurs were geographically restricted to south Pangea, including rare ornithischians and more abundant basal members of the saurischian lineage, the group achieved a nearly global distribution by the latest Triassic, especially with the radiation of saurischian groups such as "prosauropods" and coelophysoids.
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                Author and article information

                Journal
                Sci Adv
                Sci Adv
                SciAdv
                advances
                Science Advances
                American Association for the Advancement of Science
                2375-2548
                September 2020
                16 September 2020
                : 6
                : 38
                : eaba0099
                Affiliations
                [1 ]School of Earth and Environments, University of Leeds, Leeds, LS2 9JT, UK.
                [2 ]State Key Laboratory of Biogeology and Environmental Geology, School of Earth Sciences, China University of Geosciences Wuhan, Wuhan, China.
                [3 ]MUSE–Science Museum, 38122 Trento, Italy.
                [4 ]School of Earth Sciences, University of Bristol, Bristol BS8 1RJ, UK.
                [5 ]GeoZentrum Nordbayern, Universität Erlangen-Nürnberg, 91054 Erlangen, Germany.
                [6 ]Department of Palaeontology, University of Vienna, 1090 Wien, Austria.
                [7 ]Department of Geosciences, University of Padova, 35131 Padova, Italy.
                [8 ]Department of Physics and Earth Sciences, University of Ferrara, 44100 Ferrara, Italy.
                [9 ]School of Natural and Built Environment, Queen’s University Belfast, Belfast, BT7 1NN, Northern Ireland, UK.
                [10 ]Museum of Nature South Tyrol, 39100 Bozen/Bolzano, Italy.
                [11 ]Department of Earth and Environmental Sciences, Paleontology & Geobiology, Ludwig-Maximilians-Universität München, 80333 München, Germany.
                [12 ]SNSB-Bayerische Staatssammlung für Paläontologie und Geologie, 80333 München, Germany.
                [13 ]Institute of Geosciences and Earth Resources (IGG-CNR), 35131 Padova, Italy.
                [14 ]Leibniz Centre for Tropical Marine Research (ZMT), 28359 Bremen, Germany.
                [15 ]Department of Physics and Earth Sciences, Jacobs University Bremen, 28759 Bremen, Germany.
                [16 ]Department of Geobiology, University of Göttingen, 37077 Göttingen, Germany.
                Author notes
                [* ]Corresponding author. Email: jacopo.dalcorso@ 123456gmail.com (J.D.C.); mike.benton@ 123456bristol.ac.uk (M.J.B.)
                Author information
                http://orcid.org/0000-0002-2500-4097
                http://orcid.org/0000-0003-4032-2082
                http://orcid.org/0000-0002-2721-3626
                http://orcid.org/0000-0002-0199-9923
                http://orcid.org/0000-0001-8757-328X
                http://orcid.org/0000-0001-7683-2880
                http://orcid.org/0000-0001-6072-501X
                http://orcid.org/0000-0002-0300-0175
                http://orcid.org/0000-0002-7162-0130
                http://orcid.org/0000-0001-8095-8056
                http://orcid.org/0000-0002-9266-8344
                http://orcid.org/0000-0001-5426-4667
                http://orcid.org/0000-0003-0093-2759
                http://orcid.org/0000-0003-0144-6867
                http://orcid.org/0000-0003-0074-9129
                http://orcid.org/0000-0002-4323-1824
                Article
                aba0099
                10.1126/sciadv.aba0099
                7494334
                767cb0f5-1a1b-48de-b24f-a60014c151fe
                Copyright © 2020 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution License 4.0 (CC BY).

                This is an open-access article distributed under the terms of the Creative Commons Attribution license, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

                History
                : 28 October 2019
                : 31 July 2020
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