Title
Mystacodon selenensis, the earliest known toothed mysticete (Cetacea, mammalia) from the late eocene of peru: Anatomy, phylogeny, and feeding adaptations
Date Issued
01 January 2019
Access level
open access
Resource Type
journal article
Author(s)
de Muizon C.
Bianucci G.
Lambert O.
Sorbonne Université
Publisher(s)
Museum National d'Histoire Naturelle
Abstract
Mystacodon selenensis Lambert, Martínez-Cáceres, Bianucci, Di Celma, Salas-Gismondi, Steurbaut, Urbina & Muizon, 2017 is a toothed mysticete that represents the earliest member of the suborder in the current state of knowledge. Its holotype is a relatively complete skeleton from the upper Eocene (early Priabonian, c. 36.4 Ma) Yumaque Member of the Paracas Formation from the southern coast of Peru. The thorough description of this specimen is presented here and reveals numerous similarities with the contemporaneous basilosaurids including the retention of an innominate that originally articulated to the unpreserved hind limb. However, several characters of M. selenensis clearly relate this taxon to the mysticetes, such as the large palate with a dorsoventrally flattened rostrum, the posterior extension of the palate with an infraorbital plate of the maxilla, the shortening of the premaxillary part of the rostrum, the zygomatic process of the squamosal being closely apposed to the postorbital process of the frontal, and the humeral head being oriented more proximally than posteriorly. A parsimony analysis retrieves Mystacodon as the earliest diverging branch of the Mysticeti with no close phylogenetic relationship with Llanocetus the second oldest known mysticete (c. 34.2 Ma). The dental formula of M. selenensis is that of basilosaurids (I 3/3, C 1/1, P 4/4, M 2/3). The anterior teeth (incisors and canine) are distinctly proportionally smaller than in basilosaurids, whereas the cheek teeth are very close in relative length, but are relatively larger than in most other toothed mysticetes (except Coronodon). The large cheek teeth of Mystacodon suggest a raptorial feeding strategy, probably assisted with some degree of suction, as indicated by the large size of the palate. The anterior teeth of the holotype display a subhorizontal apical wear facet and the cheek teeth a moderately sloping wear surface, differing from the subvertical attrition facets of basilosaurids. This pattern suggests an efficient dental abrasion resulting from feeding upon abrasive food items or/and from the ingestion of sediment during prey capture, which could indicate some degree of bottom feeding. On the forelimb, the size and orientation of the acromion, the great length of the deltopectoral crest, the massiveness of the olecranon of the ulna, and the strong radial anterior process indicate powerful shoulder movements, which suggest an active use of the forelimb when foraging for food on the sea floor. The robustness of digits and the pachyosteosclerosis of ribs with pestle-like distal end corroborate such a scenario. Mystacodon selenensis represents a first step in the evolutionary history of feeding adaptations of early mysticetes; the latter are likely to have experimented an abundant set of feeding strategies and were probably very eclectic in prey choice and capture before hyperspecialized filter feeding became widespread in the suborder.
Start page
401
End page
499
Volume
41
Issue
11
Language
English
OCDE Knowledge area
Geociencias, Multidisciplinar Ecología
Scopus EID
2-s2.0-85070109099
Source
Geodiversitas
ISSN of the container
12809659
Sponsor(s)
The holotype of Mystacodon selenensis was discovered by M. Urbina, who collected the skull and mandible. The field expedition, during which the postcranial skeleton of the holotype of Mystacodon selenensis has been collected, was funded by the Muséum national d’Histoire naturelle, Paris (Action Transversale “Biodiversité actuelle et fossile” 2010). Geological and stratigraphical field investigations were supported by a grant of the Italian Ministero dell’Is-truzione dell’Università e della Ricerca (PRIN Project 2012YSBMK). We thank R. Salas-Gismondi, M. Urbina, W. Aguirre, E. Díaz, and R. Varas-Malca for their help during the fieldwork campaign of November 2010, when the postcranial skeleton was collected, W. Aguirre for the careful preparation of MUSM 1917, R. Salas-Gismondi and R. Varas-Malca for giving access to the MUSM collection, and C. Di Celma, K. Gariboldi, E. Malinverno, and E. Steurbaut for their help in defining the geological context of Playa Media Luna and the chronostratigraphic age of the level where the holotype of M. selenensis was found. Special thanks are due to R. E. Fordyce and F. G. Marx for sending us photographs of the holotype of Llanocetus denticrenatus, F. G. Marx for providing extensive access to his photographs of other fossil and extant mysticetes as well as for fruitful discussions on several aspects of the manuscript, J. H. Geisler for providing photographs of Coronodon havensteini, M. D. Uhen for providing many photographs of Dorudon atrox, P. D. Gingerich for providing photographs of Basilosaurus and Rodhocetus, and V. de Buffrénil and R. Salas-Gismondi for fruitful discussions. A. Gennari prepared the life reconstruction of M. selen-ensis. We are indebted to C. Buell for giving permission to reproduce the reconstructions of Aetiocetus, Caperea, Eomysticetus, Eubalaena, Janjucetus, Physeter, and Tursiops of Figure 52 and to F. G. Marx for providing them; warm thanks also to A. Gennari (and J. Geisler for Coronodon) for his permission to use the reconstructions of Balaenoptera, Coronodon, Cynthiacetus, Piscobalaena, and Squalodon reproduced in Figure 52. Our special thanks to the reviewers R. W. Boessenecker and T. Kimura for their constructive comments, which greatly improved our manuscript. Thin sections illustrated on Figure 40 have been processed by S. Morel (CR2P – CNRS, MNHN Sorbonne Université).
Sources of information: Directorio de Producción Científica Scopus