A reference genome for ecological restoration of the sunflower sea star, Pycnopodia helianthoides (2024)

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Volume 115 Issue 1 January 2024
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Lauren M Schiebelhut

Life & Environmental Sciences, University of California

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Merced, CA

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United States

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Melissa B DeBiasse

Life & Environmental Sciences, University of California

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Merced, CA

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United States

Department of Biology, Radford University

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Radford, VA

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United States

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Lars Gabriel

Institute for Mathematics and Computer Science & Center for Functional Genomics of Microbes, University of Greifswald

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Greifswald

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Germany

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Katharina J Hoff

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Michael N Dawson

Life & Environmental Sciences, University of California

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Merced, CA

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United States

Corresponding author: Life & Environmental Sciences, University of California, Merced, CA, United States. Email: mdawson@ucmerced.edu

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Journal of Heredity, Volume 115, Issue 1, January 2024, Pages 86–93, https://doi.org/10.1093/jhered/esad054

Published:

20 September 2023

Article history

Received:

10 June 2023

Revision received:

29 July 2023

Published:

20 September 2023

Accepted:

29 September 2023

Corrected and typeset:

27 October 2023

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    Lauren M Schiebelhut, Melissa B DeBiasse, Lars Gabriel, Katharina J Hoff, Michael N Dawson, A reference genome for ecological restoration of the sunflower sea star, Pycnopodia helianthoides, Journal of Heredity, Volume 115, Issue 1, January 2024, Pages 86–93, https://doi.org/10.1093/jhered/esad054

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Abstract

Wildlife diseases, such as the sea star wasting (SSW) epizootic that outbroke in the mid-2010s, appear to be associated with acute and/or chronic abiotic environmental change; dissociating the effects of different drivers can be difficult. The sunflower sea star, Pycnopodia helianthoides, was the species most severely impacted during the SSW outbreak, which overlapped with periods of anomalous atmospheric and oceanographic conditions, and there is not yet a consensus on the cause(s). Genomic data may reveal underlying molecular signatures that implicate a subset of factors and, thus, clarify past events while also setting the scene for effective restoration efforts. To advance this goal, we used Pacific Biosciences HiFi long sequencing reads and Dovetail Omni-C proximity reads to generate a highly contiguous genome assembly that was then annotated using RNA-seq-informed gene prediction. The genome assembly is 484 Mb long, with contig N50 of 1.9 Mb, scaffold N50 of 21.8 Mb, BUSCO completeness score of 96.1%, and 22 major scaffolds consistent with prior evidence that sea star genomes comprise 22 autosomes. These statistics generally fall between those of other recently assembled chromosome-scale assemblies for two species in the distantly related asteroid genus Pisaster. These novel genomic resources for P. helianthoides will underwrite population genomic, comparative genomic, and phylogenomic analyses—as well as their integration across scales—of SSW and environmental stressors.

Asteroidea, climate change, conservation, kelp forest, ocean health, sea star wasting

© The Author(s) 2023. Published by Oxford University Press on behalf of The American Genetic Association. All rights reserved. For permissions, please e-mail: journals.permissions@oup.com

This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/pages/standard-publication-reuse-rights)

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Genome Resources

Corresponding Editor: Rachel Meyer

Rachel Meyer

Corresponding Editor

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