| Literature DB >> 35345430 |
Chenyang Cai1,2, Erik Tihelka1,2, Mattia Giacomelli3, John F Lawrence4, Adam Ślipiński4, Robin Kundrata5, Shûhei Yamamoto6, Margaret K Thayer7, Alfred F Newton7, Richard A B Leschen8, Matthew L Gimmel9, Liang Lü10, Michael S Engel11,12, Patrice Bouchard11, Diying Huang1, Davide Pisani2,3, Philip C J Donoghue2.
Abstract
Beetles constitute the most biodiverse animal order with over 380 000 described species and possibly several million more yet unnamed. Recent phylogenomic studies have arrived at considerably incongruent topologies and widely varying estimates of divergence dates for major beetle clades. Here, we use a dataset of 68 single-copy nuclear protein-coding (NPC) genes sampling 129 out of the 193 recognized extant families as well as the first comprehensive set of fully justified fossil calibrations to recover a refined timescale of beetle evolution. Using phylogenetic methods that counter the effects of compositional and rate heterogeneity, we recover a topology congruent with morphological studies, which we use, combined with other recent phylogenomic studies, to propose several formal changes in the classification of Coleoptera: Scirtiformia and Scirtoidea sensu nov., Clambiformia ser. nov. and Clamboidea sensu nov., Rhinorhipiformia ser. nov., Byrrhoidea sensu nov., Dryopoidea stat. res., Nosodendriformia ser. nov. and Staphyliniformia sensu nov., and Erotyloidea stat. nov., Nitiduloidea stat. nov. and Cucujoidea sensu nov., alongside changes below the superfamily level. Our divergence time analyses recovered a late Carboniferous origin of Coleoptera, a late Palaeozoic origin of all modern beetle suborders and a Triassic-Jurassic origin of most extant families, while fundamental divergences within beetle phylogeny did not coincide with the hypothesis of a Cretaceous Terrestrial Revolution.Entities:
Keywords: CAT-GTR; Coleoptera; classification; diversification; phylogenomics; substitution modelling
Year: 2022 PMID: 35345430 PMCID: PMC8941382 DOI: 10.1098/rsos.211771
Source DB: PubMed Journal: R Soc Open Sci ISSN: 2054-5703 Impact factor: 3.653
Figure 1A full phylogeny of beetles displaying the systematic position of all sampled taxa analysed under the site-heterogeneous CAT-GTR + G4 model. Branch lengths have been omitted for clarity. Newly proposed taxonomic changes are followed. Support values are shown as BPP. Black numbered nodes indicate calibrations, see electronic supplementary material for full list of calibrations.
Figure 2Timescale of beetle evolution displayed as a family-level tree adapted from figure 1. Ages were estimated based on 57 calibrated nodes, integrating the results of analyses using IR and AC molecular clock models in MCMCtree. Newly proposed taxonomic changes are followed. Abbreviations: Arch., Archostemata; Bostrichif., Bostrichiformia; Carbonif., Carboniferous; Clambif., Clambiformia ser. nov.; Laem., Laemophloeidae; Myxo., Myxophaga; Neo., Neogene; Nosodendrif., Nosodendriformia ser. nov., Rhinorhipif., Rhinorhipiformia ser. nov.; Trogoss. + Thym., Trogossitidae + Thymalidae; Q., Quaternary.
Figure 3Proposed classification of Coleoptera showing the relationships of the suborders, series and superfamilies of beetles. Asterisks denote well-supported nodes with BPP ≥ 0.95.
Divergence dates (95% CI of the posterior distribution of age estimates, in Ma) of the crown groups of beetle suborders and series from IR and AC molecular clock analyses with uniform prior distributions.
| clade | IR | AC |
|---|---|---|
| Coleoptera | 321–306 | 322–318 |
| Adephaga | 287–259 | 288–266 |
| Archostemata – Myxophaga | 286–236 | 314–285 |
| Polyphaga | 301–288 | 307–286 |
| Scirtiformia | 177–77 | 227–90 |
| Clambiformia | 254–202 | 286–239 |
| Rhinorhipiformia | 287–271 | 283–264 |
| Elateriformia | 269–246 | 268–249 |
| Nosodendriformia | 276–258 | 271–253 |
| Staphyliniformia | 258–241 | 257–238 |
| Bostrichiformia | 237–203 | 250–228 |
| Cucujiformia | 249–231 | 233–220 |
Figure 495% CIs for the divergence of selected major beetle clades in the present and previous studies.