Morrison Formation, Late Jurassic)

Morrison Formation, Late Jurassic)

Palaeogeography, Palaeoclimatology, Palaeoecology 237 (2006) 147–159 www.elsevier.com/locate/palaeo Paleoecology of the Quarry 9 vertebrate assemblage from Como Bluff, Wyoming (Morrison Formation, Late Jurassic) Matthew T. Carrano a,*, Jorge Velez-Juarbe b a Department of Paleobiology, National Museum of Natural History, Smithsonian Institution, P.O. Box 37012, Washington, DC 20013-7012, USA b Department of Geology, University of Puerto Rico, Mayaguez Campus, P.O. Box 9017, Mayaguez, Puerto Rico 00681 Received 9 May 2005; received in revised form 16 November 2005; accepted 18 November 2005 Abstract Quarry 9 is among the richest microvertebrate localities in the Morrison Formation, having thus far produced the remains of dozens of Late Jurassic taxa. Because this lenticular claystone deposit records such a high diversity of contemporaneous species, it provides an exceptionally detailed view of their paleoecology and local paleoenvironment. In this study, we reexamined the entire Quarry 9 collection, totaling more than 3700 specimens, and developed a revised faunal list that was used to determine taxonomic and ecological diversities. Comprehensive abundance data were collected as well, revealing significant discrepancies between the most diverse and most abundant groups. Amphibious taxa (crocodilians and turtles) were very abundant, and seemed to fill an important ecological role as bconnectorsQ between the terrestrial and aquatic food webs. In contrast, small terrestrial taxa (small theropods, mammals, and small reptiles) were very diverse, highlighting their central placement within the terrestrial food web. Lithologically and sedimentologically, the deposition of Quarry 9 occurred in a low-energy pond or swamp, an interpretation supported by the available taphonomic data. D 2005 Elsevier B.V. All rights reserved. Keywords: Dinosaurs; Paleoenvironment; Taphonomy; Food web; Mammals 1. Introduction dinosaurs, crocodylians, mammals, and other verte- brates. Indeed, Morrison dinosaurs and mammals are The Morrison Formation is one of the richest dino- among the best-known members of their respective saur-bearing strata in the world (e.g., Dodson et al., clades known from any Late Jurassic formation any- 1980a,b, 1983; Foster, 2003), and as such has provided where in the world. a wealth of data on Late Jurassic dinosaur morphology, The paleoecology of this environment was complex evolution, and paleoecology. The wide-ranging Morri- (Dodson et al., 1980a,b; Foster, 2003; Engelmann et al., son depositional paleoenvironment largely represents 2004), and in some ways remains puzzling. In part this semi-arid fluvio-lacustrine floodplains (Dodson et al., is due to the overwhelming bias of most Morrison sites 1980a,b; Demko and Parrish, 1998; Turner and Peter- toward very large animals, especially sauropods (whose son, 2004) that were host to a diverse assemblage of diversity testifies to how well-sampled these large her- bivores are in the formation) (cf. Turner and Peterson, * Corresponding author. 1999; Foster, 2003). Smaller vertebrates, including E-mail addresses: [email protected] (M.T. Carrano), amphibians, lepidosaurs, and fishes, have received [email protected] (J. Velez-Juarbe). less attention due to their relative infrequence, probably 0031-0182/$ - see front matter D 2005 Elsevier B.V. All rights reserved. doi:10.1016/j.palaeo.2005.11.018 148 M.T. Carrano, J. Velez-Juarbe / Palaeogeography, Palaeoclimatology, Palaeoecology 237 (2006) 147–159 resulting in an underestimation of their diversity. This is and McIntosh, 1999). The locality soon yielded many unfortunate because such taxa can be important indica- important specimens of Late Jurassic mammals (Marsh, tors of temperature, salinity, and other environmental 1880, 1887) and other small vertebrates (Simpson, factors; indeed, these smaller vertebrates are largely 1926a). Since then, most work has focused on the di- restricted to the wetter facies of the Morrison (Foster, verse mammalian assemblage (e.g., Simpson, 1925a,b,c, 2003; Engelmann et al., 2004). Such taxa bring the 1927, 1928; Prothero, 1981; Martin, 1999), which repre- added possibility of inferring biological data from po- sents the majority of mammalian diversity—and most of tentially similar extant relatives. the specimens—known from Jurassic North America Most information on Morrison microvertebrates (Prothero, 1981). The remaining Quarry 9 fauna comes from a limited number of sites, including Nine- includes dinosaurs, fishes, rhynchocephalians (Gilmore, mile Hill (Trujillo, 1999; Foster and Trujillo, 2000), 1909; Simpson, 1926b) and other lepidosaurs (Prothero Dinosaur National Monument (Chure et al., 1989; Hen- and Estes, 1980), as well as amphibians (Evans and rici, 1998; Chure and Evans, 1998; Evans and Chure, Milner, 1993), crocodylians (Ostrom, 1971), and tur- 1999; Evans et al., 2005), the Little Houston Quarries tles. Because it has received less study, the non-mam- (Martin and Foster, 1998; Foster, 2001), and Quarry 9, malian vertebrate material likely conceals additional at Como Bluff (Simpson, 1926a,b; Prothero, 1981; data on the lower-level diversity of these groups. Ostrom and McIntosh, 1999). Thankfully, more recent Only Simpson (1926a) attempted a paleoecological dinosaur quarry work has also focused on collecting reconstruction of the Quarry 9 assemblage, outlining associated microvertebrate remains, although study is hypothetical food chains of the aquatic and terrestrial still in progress for many such sites, especially in the components. His work was largely qualitative and fo- Fruita Paleontological Area (e.g., Kirkland et al., 1990; cused on taxonomic diversity, ignoring important data Small and Carpenter, 1997). In the context of more from relative taxonomic abundances. To this date, no general Morrison Formation sampling (e.g., Turner study has obtained complete abundance data from the and Peterson, 1999), microvertebrate localities probably Quarry 9 assemblage. This is problematic in mammal- account for less than 10% of all sites, although this is rich assemblages, because mammalian fossils tend to be only a qualitative assessment. This is in contrast with more closely studied (resulting in finer taxonomic res- (e.g.) the microvertebrate-rich Judith River and Hell olution) and more specifically identified (resulting in Creek Formations of the Late Cretaceous. more accurate counts of individuals) than taxa from Within the Morrison, Quarry 9 contains the richest other clades. and best-known microvertebrate sample to date. William In this paper, we present the results of a reanalysis of Reed discovered the site in 1879 while working for O.C. the Quarry 9 assemblage. We examined the entire Marsh along the Como Bluff anticline (Fig. 1; Ostrom collection from the original Quarry 9 site, with the Fig. 1. (A) Map of Wyoming showing the location of Como Bluff and the Quarry 9 site, Albany County. (B) Topographic map showing a portion of the Aurora Lake quadrangle and the approximate location of Quarry 9. M.T. Carrano, J. Velez-Juarbe / Palaeogeography, Palaeoclimatology, Palaeoecology 237 (2006) 147–159 149 goal of identifying as many individual specimens as assignment (Kielan-Jaworowska et al., 2004). We possible and thereby generating comprehensive diver- obtained both numbers of taxa and numbers of speci- sity estimates. In addition, we collected data on taphon- mens. We tallied both specific and generic diversity in omy and depositional environment, based on specimens order to minimize the inflating effects of the highly and existing blocks of matrix from the original excava- detailed methodology for identifying fossil mammalian tion. Ecological data were inferred directly from organ- taxa when compared to the quite general methods ismal morphology and indirectly based on extant applied to other fossil taxa. relatives of Jurassic taxa. These data were synthesized Many isolated theropod teeth are present in the to produce a new paleoecological reconstruction of the collection. We were able to identify some of these Quarry 9 paleoenvironment. teeth based on comparisons with in situ specimens of Ceratosaurus nasicornis (USNM 4734) and Allosaurus 2. Materials and methods fragilis (USNM 4735). We divided the remaining spe- cimens into three morphological groups based on ser- Como Bluff and Como Ridge are topographic fea- ration pattern (e.g., Currie et al., 1990; Fiorillo and tures that straddle the boundary between Carbon and Currie, 1994). Tooth type A had serrations along the Albany counties, Wyoming just north of US Route 30/ entire mesial carina; type B had serrations on the apical 287. Quarry 9 itself occurs in the SW 1/4 of section 12, portion of the mesial carina; type C lacked serrations on T22N, R77W (Fig. 1; Ostrom and McIntosh, 1999), the mesial carina. All three types retained serrations along the northern face of Como Ridge and toward its along the entire distal carina. Next, we measured the eastern end. The primary fossil collections were made fore-aft base length (FABL) and the number of serra- by Yale University crews between 1879 and 1889, tions per millimeter along the distal edge. By plotting followed by the American Museum of Natural History FABL versus serration density, we were able to identify in 1897. These collections were made prior to the morphometric bclustersQ that likely represented discrete advent of screenwashing techniques in vertebrate pale- theropod taxa. ontology, and were obtained through surface collection We used raw specimen counts to calculate

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