| Literature DB >> 31767921 |
Christian Kehlmaier1, Eva Graciá2, Patrick D Campbell3, Margaretha D Hofmeyr4, Silke Schweiger5, Albert Martínez-Silvestre6, Walter Joyce7, Uwe Fritz8.
Abstract
The five extinct giant tortoises of the genus Cylindraspis belong to the most iconic species of the enigmatic fauna of the Mascarene Islands that went largely extinct after the discovery of the islands. To resolve the phylogeny and biogeography of Cylindraspis, we analysed a data set of 45 mitogenomes that includes all lineages of extant tortoises and eight near-complete sequences of all Mascarene species extracted from historic and subfossil material. Cylindraspis is an ancient lineage that diverged as early as the late Eocene. Diversification of Cylindraspis commenced in the mid-Oligocene, long before the formation of the Mascarene Islands. This rejects any notion suggesting that the group either arrived from nearby or distant continents over the course of the last millions of years or had even been translocated to the islands by humans. Instead, Cylindraspis likely originated on now submerged islands of the Réunion Hotspot and utilized these to island hop to reach the Mascarenes. The final diversification took place both before and after the arrival on the Mascarenes. With Cylindraspis a deeply divergent clade of tortoises became extinct that evolved long before the dodo or the Rodrigues solitaire, two other charismatic species of the lost Mascarene fauna.Entities:
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Year: 2019 PMID: 31767921 PMCID: PMC6877638 DOI: 10.1038/s41598-019-54019-y
Source DB: PubMed Journal: Sci Rep ISSN: 2045-2322 Impact factor: 4.379
Figure 1Fossil-calibrated time tree for Cylindraspis and all extant tortoise genera, rooted with Chrysemys picta based on 15,510 bp of the mitochondrial genome. Cylindraspis species in boldface with collection acronyms identifying individual specimens (NHM[UK] = Natural History Museum, London; NMW = Natural History Museum, Vienna). Dagger symbols denote extinct taxa. Geographic distributions of the five major testudinine clades (1–5) on the right. For nodes, inferred mean ages and 95% Highest Posterior Density intervals are shown. The red circles indicate fossil-based constraints: (A) Hadrianus majusculus Hay, 1904, 50.3–100.5 Ma; (B) Cheirogaster maurini Bergounioux, 1935 and Gigantochersina ammon (Andrews, 1904), 33.9–66.0 Ma; (C) Cheirogaster maurini Bergounioux, 1935, 33.9–47.8 Ma; (D) Chelonoidis hesternus (Auffenberg, 1971), 11.8–33.9 Ma. For details of calibration, see Supplementary Information. Inset: lateral view of the historic shell of Cylindraspis vosmaeri in the Natural History Museum, Vienna (NMW 1461); photo: Silke Schweiger.
Figure 2Paleogeographic reconstruction of the western Indian Ocean Basin highlighting changes from the late Eocene (45 Ma) to the present. The grey line connotes the approximate position of the equator; black arrows, prevalent surface currents; red and blue arrows, alternative colonization routes. Our model favours the red pathway, but the blue is more consistent with currents. It remains unclear whether the Seychelles Plateau was used as a stepping stone. Arrows are added to multiple time intervals to highlight ambiguity in regard to timing. The dispersal shown for the present took place much earlier. For Mauritius and Rodrigues multiple colonization events occurred. In addition to the persistent presence of anticlockwise gyres in the Mozambique Channel and the Indian Ocean, we posit the presence of an enclosed clockwise gyre in the Arabian Sea prior to tectonic movement of India north of the equator. In the Eocene sporadic surface current changes allowed overseas dispersal from northeast Mozambique and Tanzania to northern Madagascar[39]. Abbreviations: C – Chagos Plateau, MA – Mauritius, MD – Maldives Ridge, N – Nazareth Bank, RE – Réunion, RO – Rodrigues, SE – Seychelles Plateau, SM – Saya de Malha Bank. All maps were redrawn from Scotese[41] using Photoshop CC 19.1.0 and then assembled and labelled using Illustrator 22.0.1.