| 2003 Seattle Annual Meeting (November 2–5, 2003) | |
| Paper No. 167-16 | |
| Presentation Time: 5:15 PM-5:30 PM | |||||||||||||||||||||||||||||||||||
GENERIC RICHNESS OF NON-AVIALAN DINOSAURIA | |||||||||||||||||||||||||||||||||||
|
FASTOVSKY, David E.1, HUANG, Yifan2, HSU, Jason C.2, WEISHAMPEL, David B.3, MARTIN-MACNAUGHTON, Jamie4, and SHEEHAN, Peter5, (1) Department of Geosciences, Univ of Rhode Island, 9 East Alumni Ave, Kingston, RI 02881, defastov@uri.edu, (2) Department of Statistics, The Ohio State Univ, Columbus, OH 43210, (3) Cell Biology & Anatomy, The Johns Hopkins Univ School of Medicine, 725 N. Wolfe St, Baltimore, MD 21205, (4) Department of Geological Sciences, Brown Univ, Providence, RI 02912, (5) Milwakee Public Museum, Milwaukee, WI We have revisited the question of Mesozoic non-avialian dinosaur richness using a new global compilation of dinosaur genera from the second edition of The Dinosauria (in press). Considering body fossils only, this consists of 556 different genera distributed by stage among the Late Triassic (37), Early Jurassic (33), Middle Jurassic (38); Late Jurassic (64); Early Cretaceous (143); and Late Cretaceous (241). At this level of resolution, dinosaur generic richness unambiguously and dramatically increases throughout their tenure on Earth. Within the Late Cretaceous, the number of different dinosaur genera increases, reaching a peak in the Campanian (59), but decreasing (39) in the Maastrichtian. Because the database is constructed on published records of dinosaur taxa, 39% of all genera have more than one entry. This suggests an approach allowing comparison by rarefaction: the published records are treated as repeats in a counting experiment. Because rarefaction always adjusts downward to the smallest sample, we used Cenomanian (n=48) and rarified samples from the Turonian, Coniacian, Santonian, Campanian, and Maastrichtian.
When this is done the estimated diversity in the Maastrichtian becomes statistically indistinguishable from estimated diversity in the Campanian. The counts show no obvious relationship to length of time, suggesting that some aspect of real diversity is reflected in these numbers. | |||||||||||||||||||||||||||||||||||
|
2003 Seattle Annual Meeting (November 2–5, 2003)
| |||||||||||||||||||||||||||||||||||
| Session No. 167 Paleontology/Paleobotany III: Diversity Dynamics, Extinction, and Origination Washington State Convention and Trade Center: 400 1:30 PM-5:30 PM, Tuesday, November 4, 2003 Geological Society of America Abstracts with Programs, Vol. 35, No. 6, September 2003, p. 418 | |||||||||||||||||||||||||||||||||||
© Copyright 2003 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions. | |||||||||||||||||||||||||||||||||||