Abderitid marsupials from the Miocene of Patagonia: An assessment of form,function, and evolution

Citation
Er. Dumont et al., Abderitid marsupials from the Miocene of Patagonia: An assessment of form,function, and evolution, J PALEONTOL, 74(6), 2000, pp. 1161-1172
Citations number
74
Categorie Soggetti
Earth Sciences
Journal title
JOURNAL OF PALEONTOLOGY
ISSN journal
00223360 → ACNP
Volume
74
Issue
6
Year of publication
2000
Pages
1161 - 1172
Database
ISI
SICI code
0022-3360(200011)74:6<1161:AMFTMO>2.0.ZU;2-S
Abstract
Abderitid marsupials are common in vertebrate-bearing deposits from the mid dle Miocene of Argentine Patagonia. Recent collections from the inland Pint uras Formation and slightly younger coastal Santa Cruz Formation have drama tically increased the number of abderitid specimens. These new collections permit a re-assessment of abderitid taxonomy as well as an investigation of the dietary habits of these unique small mammals. The vast majority of new specimens represent Abderites meridionalis; Pithiculites minimus is rare. Patterns of macrowear on the double-bladed, plagiaulacoid shearing complex suggest that abderitids used these teeth to prepare a variety of resistant food items as do modem marsupials with double-bladed shearing systems. Data summarizing molar-shearing morphology and body size further suggest that A . meridionalis was a frugivore. The diet of the small P. minimus is equivoc al, although it may represent a mixed feeder (frugivore/faunivore). A compa rison of relative species richness and dietary adaptation between abderitid s and palaeothentids (a closely related caenolestoid family that lacks the highly specialized shearing complex of abderitids) reveals distinct evoluti onary patterns within the two lineages. Abderitids exhibit low species dive rsity. In contrast, palaeothentids are represented by 17 species, lack high ly specialized shearing mechanisms, and typically exhibit molar morphologie s that range from frugivory to faunivory and include mixed feeders. Both te mporal and geographic variation are introduced as possible factors affectin g differences in the relative abundance of abderitids and palaeothentids in the Pinturas and Santa Cruz Formations.