DOI: 10.1126/science.1189866 , 178-a (2010); 330Science et al.Nicholas D. Pyenson, Whales" Cenozoic Drivers of the Evolution of Modern Comment on "Climate, Critters, and Cetaceans: This copy is for your personal, non-commercial use only. . clicking herecolleagues, clients, or customers by , you can order high-quality copies for yourIf you wish to distribute this article to others . herefollowing the guidelines can be obtained byPermission to republish or repurpose articles or portions of articles (this information is current as of October 7, 2010 ): The following resources related to this article are available online at www.sciencemag.org http://www.sciencemag.org/cgi/content/full/330/6001/178-a version of this article at: including high-resolution figures, can be found in the onlineUpdated information and services, http://www.sciencemag.org/cgi/content/full/330/6001/178-a#otherarticles , 7 of which can be accessed for free: cites 13 articlesThis article http://www.sciencemag.org/cgi/content/full/330/6001/178-a#otherarticles 1 articles hosted by HighWire Press; see: cited byThis article has been http://www.sciencemag.org/cgi/collection/tech_comment Technical Comments http://www.sciencemag.org/cgi/collection/paleo Paleontology : subject collectionsThis article appears in the following registered trademark of AAAS. is aScience2010 by the American Association for the Advancement of Science; all rights reserved. The title CopyrightAmerican Association for the Advancement of Science, 1200 New York Avenue NW, Washington, DC 20005. (print ISSN 0036-8075; online ISSN 1095-9203) is published weekly, except the last week in December, by theScience o n O ct ob er 7 , 2 01 0 w w w .s ci en ce m ag .o rg D ow nl oa de d fro m Comment on ?Climate, Critters, and Cetaceans: Cenozoic Drivers of the Evolution of Modern Whales? Nicholas D. Pyenson,1,2*? Randall B. Irmis,3,4 Jere H. Lipps5 Marx and Uhen (Reports, 19 February 2010, p. 993) suggested that correlated diversity changes in the fossil record of whales and diatoms reflects secular evolutionary signals of underlying ecological drivers. We question the meaning of this association and outline avenues for more complete testing of correlations between productivity and marine consumers through geologic time. Given the densely sampled micropaleon-tological record and the comparativelysparse fossil record of cetaceans, we were surprised to see the strong correlation between diatom and cetacean richness patterns through time presented byMarx andUhen (1).We applaud their test of broad-scale evolutionary patterns with paleobiological occurrence data but note several concerns. First, the authors mischaracterize the structure ofmarine foodwebs in equating total global species richness of primary producers with consumer taxonomic richness, abundance, and body size. Ecologists continue to debate the relationships among species richness (the number of species), composition (identity of those species), and productivity (2, 3). Although the large spatial scale of marine systems prevents controlled field experiments, decades of observational research have demonstrated the co-occurrence of large- sized diatom productivity with the presence of large consumers (including cetaceans) in nutrient- rich, upwelling waters (4). Close trophic linkages between diatoms and cetaceans only occur for filter-feeding cetaceans in specific regions (e.g., the Southern Ocean), which have lower cetacean richness than temperate and tropical ecosystems (5), despite higher abundances. In upwelling systems that occur across temperate and tropical latitudinal gradients, both cetacean abundance and richness are high (5), whereas diatom richness is low despite having high abundances, because of the dominance of large-sized diatoms (3). This heterogeneous diatom distribution across the oceans confounds any interpretation of increased productivity as reflected by correlated rises in producer and secondary consumer richness in the fossil record, from the standpoint of global diver- sity metrics. Moreover, these associations are complicated by secondary consumer feeding spe- cializations (e.g., lunge-feeding or hypercarnivory), which have demonstrably changed in extant cetacean lineages since the Oligocene [e.g., 6, 7]. High secondary productivity likely affects the evolution of body size for some cetacean species (8), but a positive relationship between body size and species richness is not supported by global extant cetacean data (5, 9). Because questions about marine macroecology and its fossil record are similarly limited by an inability to directly investigate large-scale ecological phenomena, drawing the necessary comparisons between pro- ductivity and consumers requires an understanding of the relationship between productivity and spe- cies richness. Recent analytical advancements have improved our understanding of secular trends in the diatom fossil record (10), but the evolutionary consequences of these trends for the global richness of primary and secondary consumers are unclear because such global analyses include nanoplankton and smaller diatoms, which are too small and insufficiently abundant to substantially impact cetacean trophic ecology. Second, the record of fossil cetacean richness yields peaks driven by unusually abundant col- lections from a small number of mostly Northern Hemisphere assemblages. This overwhelming bias in the crown cetacean fossil record, and a defi- ciency in reported sampling for rock units older than ~23 million years (11), hamper our ability to test hypotheses about the origin of neocetes or their possible linkage with the formation of the Antarctic Circumpolar Current in the Southern Hemisphere. The cetacean fossil record lacks widespread, fine-scale geochronological calibra- tion, and even the richest and best-known assem- blages are time-averaged, which overinflates certain measures of diversity (12). To surmount these issues, we advocate more robust comparisons of marine producer and con- sumer diversity (measured by both abundance and richness), using well-sampled local-regional as- semblages, as terrestrial paleoecologists have done [e.g., 13)]. Such studies, considered in tandem with global data sets, would better resolve whether correlated diversity patterns from disparate trophic levels truly indicate ecological drivers at geologic time scales. References and Notes 1. F. G. Marx, M. D. Uhen, Science 327, 993 (2010). 2. B. J. Cardinale, D. M. Bennett, C. E. Nelson, K. Gross, Ecology 90, 1227 (2009). 3. B. Worm, J. E. Duffy, Trends Ecol. Evol. 18, 628 (2003). 4. J. H. Ryther, Science 166, 72 (1969). 5. J. Schipper et al., Science 322, 225 (2008). 6. T. A. Dem?r?, M. R. McGowen, A. Berta, J. Gatesy, Syst. Biol. 57, 15 (2008). 7. O. Lambert et al., Nature 466, 105 (2010). 8. D. A. Croll et al., Mar. Ecol. Prog. Ser. 289, 117 (2005). 9. G. J. Slater, S. A. Price, F. Santini, M. E. Alfaro, Proc. Biol. Sci. 277, 3097 (2010). 10. D. L. Rabosky, U. Sorhannus, Nature 457, 183 (2009). 11. M. D. Uhen, N. D. Pyenson, Palaeo. Electron. 10, 11A (2007). 12. N. D. Pyenson et al., Geology 37, 519 (2009). 13. J. C. Barry et al., Paleobiology 28 (suppl.), 1 (2002). 14. This work was supported by funds from the Natural Sciences and Engineering Research Council of Canada and the Smithsonian Institution (both to N.D.P.), University of Utah (to R.B.I.), and the Committee on Research, University of California, Berkeley (to J.H.L.). 18 March 2010; accepted 8 September 2010 10.1126/science.1189866 TECHNICALCOMMENT 1Department of Zoology, 6270 University Boulevard, Uni- versity of British Columbia, Vancouver, BC V6T 1Z4, Canada. 2Departments of Mammalogy and Paleontology, Burke Mu- seum of Natural History and Culture, Seattle, WA 98195, USA. 3Utah Museum of Natural History, 1390 East Presidents Circle, Salt Lake City, UT 84112?0050, USA. 4Department of Geology and Geophysics, University of Utah, Salt Lake City, UT 84112? 0102, USA. 5Museum of Paleontology and Department of Integrative Biology, University of California, Berkeley, CA 94720? 4780, USA. *Present address: Department of Paleobiology, National Mu- seum of Natural History, Smithsonian Institution, Washington, DC 20013, USA. ?To whom correspondence should be addressed. E-mail: pyensonn@si.edu 8 OCTOBER 2010 VOL 330 SCIENCE www.sciencemag.org178-a o n O ct ob er 7 , 2 01 0 w w w .s ci en ce m ag .o rg D ow nl oa de d fro m