Phylogenomic analysis of echinoderm class relationships supports Asterozoa

Author:

Telford Maximilian J.1,Lowe Christopher J.2,Cameron Christopher B.3,Ortega-Martinez Olga4,Aronowicz Jochanan5,Oliveri Paola1,Copley Richard R.67

Affiliation:

1. Department of Genetics, Evolution and Environment, University College London, Darwin Building, Gower Street, London WC1E 6BT, UK

2. Hopkins Marine Station, Department of Biology, Stanford University, 120 Oceanview Boulevard, Pacific Grove, CA 93950, USA

3. Départment de Sciences Biologiques, Université de Montréal, Pavillion Marie-Victorin, C.P. 6128, Succ. Centre-ville, Montréal, Québec, Canada H3C 3J7

4. Department of Biological and Environmental Sciences, Sven Lovén Centre for Marine Sciences, University of Gothenburg, Kristineberg 566, Fiskebäckskil 451 78, Sweden

5. Department of Organismal Biology and Anatomy, University of Chicago, Chicago, IL 60650, USA

6. CNRS, Laboratoire de Biologie du Développement de Villefranche-sur-mer (LBDV), Observatoire Océanographique, Villefranche-sur-mer 06230, France

7. Sorbonne Universites, UPMC Univ Paris 06, Laboratoire de Biologie du Developpement de Villefranche-sur-mer, Observatoire Oceanographique, Villefranche-sur-mer 06230, France

Abstract

While some aspects of the phylogeny of the five living echinoderm classes are clear, the position of the ophiuroids (brittlestars) relative to asteroids (starfish), echinoids (sea urchins) and holothurians (sea cucumbers) is controversial. Ophiuroids have a pluteus-type larva in common with echinoids giving some support to an ophiuroid/echinoid/holothurian clade named Cryptosyringida. Most molecular phylogenetic studies, however, support an ophiuroid/asteroid clade (Asterozoa) implying either convergent evolution of the pluteus or reversals to an auricularia-type larva in asteroids and holothurians. A recent study of 10 genes from four of the five echinoderm classes used ‘phylogenetic signal dissection’ to separate alignment positions into subsets of (i) suboptimal, heterogeneously evolving sites (invariant plus rapidly changing) and (ii) the remaining optimal, homogeneously evolving sites. Along with most previous molecular phylogenetic studies, their set of heterogeneous sites, expected to be more prone to systematic error, support Asterozoa. The homogeneous sites, in contrast, support an ophiuroid/echinoid grouping, consistent with the cryptosyringid clade, leading them to posit homology of the ophiopluteus and echinopluteus. Our new dataset comprises 219 genes from all echinoderm classes; analyses using probabilistic Bayesian phylogenetic methods strongly support Asterozoa. The most reliable, slowly evolving quartile of genes also gives highest support for Asterozoa; this support diminishes in second and third quartiles and the fastest changing quartile places the ophiuroids close to the root. Using phylogenetic signal dissection, we find heterogenous sites support an unlikely grouping of Ophiuroidea + Holothuria while homogeneous sites again strongly support Asterozoa. Our large and taxonomically complete dataset finds no support for the cryptosyringid hypothesis; in showing strong support for the Asterozoa, our preferred topology leaves the question of homology of pluteus larvae open.

Publisher

The Royal Society

Subject

General Agricultural and Biological Sciences,General Environmental Science,General Immunology and Microbiology,General Biochemistry, Genetics and Molecular Biology,General Medicine

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