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Published June 25, 2019 | Supplemental Material + Published
Journal Article Open

Climatic shifts drove major contractions in avian latitudinal distributions throughout the Cenozoic

Abstract

Many higher level avian clades are restricted to Earth's lower latitudes, leading to historical biogeographic reconstructions favoring a Gondwanan origin of crown birds and numerous deep subclades. However, several such "tropical-restricted" clades (TRCs) are represented by stem-lineage fossils well outside the ranges of their closest living relatives, often on northern continents. To assess the drivers of these geographic disjunctions, we combined ecological niche modeling, paleoclimate models, and the early Cenozoic fossil record to examine the influence of climatic change on avian geographic distributions over the last ∼56 million years. By modeling the distribution of suitable habitable area through time, we illustrate that most Paleogene fossil-bearing localities would have been suitable for occupancy by extant TRC representatives when their stem-lineage fossils were deposited. Potentially suitable habitat for these TRCs is inferred to have become progressively restricted toward the tropics throughout the Cenozoic, culminating in relatively narrow circumtropical distributions in the present day. Our results are consistent with coarse-scale niche conservatism at the clade level and support a scenario whereby climate change over geological timescales has largely dictated the geographic distributions of many major avian clades. The distinctive modern bias toward high avian diversity at tropical latitudes for most hierarchical taxonomic levels may therefore represent a relatively recent phenomenon, overprinting a complex biogeographic history of dramatic geographic range shifts driven by Earth's changing climate, variable persistence, and intercontinental dispersal. Earth's current climatic trajectory portends a return to a megathermal state, which may dramatically influence the geographic distributions of many range-restricted extant clades.

Additional Information

© 2019 National Academy of Sciences. Published under the PNAS license. Edited by Nils Chr. Stenseth, University of Oslo, Oslo, Norway, and approved May 7, 2019 (received for review March 8, 2019). We thank Michelle Casey (Towson University) for advice on paleo-plate rotation models. E.E.S. was supported by a Division of Earth Sciences National Science Foundation Postdoctoral Fellowship and Leverhulme Grant DGR01020. A.F. and D.J.L. were funded by United Kingdom National Environmental Research Council Grants NE/K014757/1, NE/I005722/1, NE/I005714/1, and NE/P013805/1. E.E.S. and D.J.F. contributed equally to this work. Author contributions: E.E.S. and D.J.F. designed research; E.E.S. and D.J.F. performed research; A.F., D.J.L., and N.S. contributed new reagents/analytic tools; E.E.S. and K.V.P. analyzed data; and E.E.S. and D.J.F. wrote the paper. The authors declare no conflict of interest. This article is a PNAS Direct Submission. Data deposition: Data from this study have been deposited on the online data archive Zenodo (DOI: 10.5281/zenodo.2658119). This article contains supporting information online at www.pnas.org/lookup/suppl/doi:10.1073/pnas.1903866116/-/DCSupplemental.

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Supplemental Material - pnas.1903866116.sapp.pdf

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Additional details

Created:
August 22, 2023
Modified:
October 23, 2023