4.2 Article Proceedings Paper

Evolution in the slow lane:: molecular rates of evolution in sexual and asexual ostracods (Crustacea: Ostracoda)

Journal

BIOLOGICAL JOURNAL OF THE LINNEAN SOCIETY
Volume 79, Issue 1, Pages 93-100

Publisher

OXFORD UNIV PRESS
DOI: 10.1046/j.1095-8312.2003.00186.x

Keywords

accumulation of mutations; Cypridoidea; Darwinula stevensoni; Darwinuloidea; intraspecific diversity; mitochondrial COI genes; nuclear ITS region; substitution rate; superfamilies

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Parthenogenetic lineages within non-marine ostracods can occur either in mixed (with sexual and asexual females) or exclusively asexual taxa. The former mode of reproduction is associated with a high intraspecific diversity at all levels (genetic, morphological, ecological) and, at least in the Cypridoidea, with geographical parthenogenesis. Obligate asexuality is restricted to the Darwinuloidea, the strongest candidate for an ancient asexual animal group after the bdelloid rotifers, and is characterized by low diversity. We have compared rates of molecular evolution for the nuclear ITS1 region and the mitochondrial COT gene amongst the three major lineages of non-marine ostracods with sexual, mixed and asexual reproduction. Absolute rates of molecular evolution are low for both regions in the darwinulids. The slow-down of evolution in ITS1 that has been observed for Darwinula stevensoni (Brady & Robertson) apparently does not occur in other darwinulid species. ITS1 evolves more slowly than COT within non-marine ostracod families, including the darwinulids, but not between superfamilies. The ancient asexuals might have a higher relative substitution rate in ITS1, as would be expected from hypotheses that predict the accumulation of mutations in asexuals. However, the speed-up of ITS could also be ancient, for example through the stochastic loss of most lineages within the superfamily after the Permian-Triassic mass extinction. In this case, the difference in rate would have occurred independently from any effects of asexual reproduction. (C) 2003 The Linnean Society of London.

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