A chromosome-level reference genome for the giant pink sea star, Pisaster brevispinus, a species severely impacted by wasting

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

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.

A chromosome-level genome assembly of a deep-sea starfish (Zoroaster cf. ophiactis)

Understanding of adaptation and evolution of organisms in the deep sea requires more genomic resources. Zoroaster cf. ophiactis is a sea star in the family Zoroasteridae occurring exclusively in the deep sea. In this study, a chromosome-level genome assembly for Z. cf. ophiactis was generated by combining Nanopore long-read, Illumina short-read, and Hi-C sequencing data. The final assembly was 1,002.0 Mb in length, with a contig N50 of 376 Kb and a scaffold N50 of 40.4 Mb, and included 22 pseudo-chromosomes, covering 92.3% of the assembly. Completeness analysis evaluated with BUSCO revealed that 95.91% of the metazoan conserved genes were complete. Additionally, 39,426 protein-coding genes were annotated for this assembly. This chromosome-level genome assembly represents the first high-quality genome for the deep-sea Asteroidea, and will provide a valuable resource for future studies on evolution and adaptation of deep-sea echinoderms.