Skip to main content
Article
A Molecular Phylogeny for Bats Illuminates Biogeography and the Fossil Record
Science
  • Emma C. Teeling, National Cancer Institute at Frederick; University College Dublin - Ireland
  • Mark S. Springer, University of California - Riverside
  • Ole Madsen, University of Nijmegen - Netherlands
  • Paul Bates, Centre for Systematics and Biodiversity Research - United Kingdom
  • Stephen J. O'Brien, National Cancer Institute at Frederick
  • William J. Murphy, National Cancer Institute at Frederick; Texas A&M University - College Station
Document Type
Article
Publication Date
1-28-2005
Abstract

Bats make up more than 20% of extant mammals, yet their evolutionary history is largely unknown because of a limited fossil record and conflicting or incomplete phylogenies. Here, we present a highly resolved molecular phylogeny for all extant bat families. Our results support the hypothesis that megabats are nested among four major microbat lineages, which originated in the early Eocene [52 to 50 million years ago (Mya)], coincident with a significant global rise in temperature, increase in plant diversity and abundance, and the zenith of Tertiary insect diversity. Our data suggest that bats originated in Laurasia, possibly in North America, and that three of the major microbat lineages are Laurasian in origin, whereas the fourth is Gondwanan. Combining principles of ghost lineage analysis with molecular divergence dates, we estimate that the bat fossil record underestimates (unrepresented basal branch length, UBBL) first occurrences by, on average, 73% and that the sum of missing fossil history is 61%.

Comments

©2005 American Association for the Advancement of Science

Additional Comments
National Cancer Institute contract #: N01-CO-12400; Darwin Initiative grant #: 162-11-09
ORCID ID
0000-0001-7353-8301
ResearcherID
N-1726-2015
Citation Information
Emma C. Teeling, Mark S. Springer, Ole Madsen, Paul Bates, et al.. "A Molecular Phylogeny for Bats Illuminates Biogeography and the Fossil Record" Science Vol. 307 Iss. 5709 (2005) p. 580 - 584 ISSN: 0036-8075
Available at: http://works.bepress.com/stephen-obrien/23/