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One of the key faunal transitions in Earth history occurred after the Permo-Triassic mass extinction (ca. 252.2 Ma), when the previously obscure archosauromorphs (which include crocodylians, dinosaurs, and birds) become the dominant terrestrial vertebrates. Here, we place all known middle Permian–early Late Triassic archosauromorph species into an explicit phylogenetic context, and quantify biodiversity change through this interval. Our results indicate the following sequence of diversification: a morphologically conservative and globally distributed post-extinction ‘disaster fauna’; a major but cryptic and poorly sampled phylogenetic diversification with significantly elevated evolutionary rates; and a marked increase in species counts, abundance, and disparity contemporaneous with global ecosystem stabilisation some 5 million years after the extinction. This multiphase event transformed global ecosystems, with far-reaching consequences for Mesozoic and modern faunas.
Ezcurra and Butler Supplementary Data 1 Character listEzcurra and Butler Supplementary Data 2 Raw MatrixEzcurra and Butler Supplementary Data 3 Occurence and temporal dataEzcurra and Butler Supplementary Data 4 Matrix for phenotypic ratesEzcurra and Butler Supplementary Data 5 MPTsEzcurra and Butler Supplementary Data 6 Script to calculate phylogenetic diversity4
Archosauromorpha, Diapsida, morphological disparity, biotic crisis
Archosauromorpha, Diapsida, morphological disparity, biotic crisis
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