Remarks: Using the mtORF marker, Johnston et al. (2022 b) found that P. tuahiniensis sp. nov. is most abundant at depths around 10 m and greater on the fore reefs of Mo’orea, whereas co-occurring species have distinctly different relative abundance patterns across depth. Among these co-occurring species are P. meandrina Dana 1846 and P. verrucosa (Ellis and Solander 1786). Johnston et al. (2022 a) recognized P. verrucosa as a single lineage at Mo’orea (and includes mtORF haplotypes 3 a, 3 b, 3 e, 3 f, and 3 h; haplotype identification following Pinzón et al. (2013 )). Along with P. tuahiniensis sp. nov., these species are the most abundant species on the fore reefs of Mo’orea. The Great Barrier Reef is the type locality for P. verrucosa (Ellis and Solander 1786) and Schmidt-Roach et al. (2014) associated mtORF haplotypes 3 b, 3 d, 3 f, and 3 g to this species. Oury et al. (2023), however, resolved three different lineages associated with mtORF haplotype 3, with GSH 13 a containing haplotypes 3 c, 3 e, 3 g, 3 j, GSH 13 b containing haplotype 3 a, and GSH 13 c containing haplotypes 3 b, 3 d, 3 f, 3 h, 3 i. They conclude that GSH 13 a is restricted to the Red Sea, Arabian Gulf, and Western Indian Ocean (WIO) but that GSH 13 b and GSH 13 c are widespread based on the geographic distribution of the corresponding mtORF haplotypes reported in prior literature, despite in their study only sampling GSH 13 b from the WIO and GSH 13 c mostly from the Tropical South Pacific. While there may be some geographic segregation between mtORF 3 haplotypes found by Oury et al. (2023), the mtORF haplotypes recovered at Mo’orea were found to be a single genomic lineage (Johnston et al. 2022 a) and include those mtORF haplotypes used to identify P. verrucosa from its type locality, therefore we identify all mtORF 3 haplotypes at Mo’orea as P. verrucosa. Likewise, Oury et al. (2023) found two distinct lineages (GSH 9 a and GSH 9 b) associated with the mtORF haplotype 1 a + PocHistone lineage (genetic identification following Johnston et al. (2018 )) used to identify P. meandrina. GSH 9 a is found in both the Pacific and Indian Oceans, and encompasses the type locality, Hawai‘i, for P. meandrina Dana 1846. GSH 9 b is restricted to the Western Indian Ocean. We thus conclude that GSH 9 a, and what we call haplotype 1 a P. meandrina is P. meandrina Dana 1846, while GSH 9 b may be a regional endemic that needs further identification. The gross in situ colony appearance of P. tuahiniensis sp. nov. cannot easily be differentiated from that of P. meandrina or P. verrucosa at Mo’orea (Figure 2). The coralla of both P. tuahiniensis sp. nov. and P. meandrina are generally small, compact, and hemispherical, with branches that are flattened and meander towards the tips (Figure 1 – 3). Pocillopora grandis Dana 1846 also has branches that are flattened and meandering, but these branches can be paddle-like and are typically more robust than those of P. meandrina, P. tuahiniensis sp. nov., and P. verrucosa (Ellis and Solander 1786) (Figure 3 d). The branches of P. verrucosa typically do not meander and may be both flattened and cylindrical with swollen appearing branch tips (Figures 2 d, 3 b – 3 c). Both P. tuahiniensis sp. nov., P. meandrina, and P. grandis have neatly arranged verrucae that are equal in size (Figures 1 – 3), but the verrucae of P. tuahiniensis sp. nov. tend to have a more jagged, crown-like appearance (Figure 1 d – 1 e) in contrast to the rounded verrucae of P. meandrina, P. verrucosa, and P. grandis (Figure 3 b – f). The verrucae of P. verrucosa are verrucose and equally distributed, but in contrast to P. meandrina, P. grandis, and P. tuahiniensis sp. nov., they are irregular in size, shape, and height (Schmidt-Roach et al. 2014) (Figure 3 b – 3 c). The spinulae of P. tuahiniensis sp. nov. are much reduced, if present, and columellae are short and wide (Figures 1 e, 1 f, and 3 a). Columellae of P. meandrina are oval-convex to styloid and rarely obsolete (Schmidt-Roach et al. 2014). Pocillopora grandis can be differentiated from P. meandrina by its styliform columellae that may contain 1 – 3 stylae. The corallites of P. verrucosa are characterized as having many long, slender spinulae and absent to styloid columellae (Schmidt-Roach et al. 2014) (Figure 3 b). Mitochondrial and nuclear genomic data reveal that P. tuahiniensis sp. nov. is a unique species, sister to P. verrucosa, and in a clade different from that of P. meandrina (Johnston et al. 2022 a). By sequencing the mtORF region, P. tuahiniensis sp. nov. can be easily distinguished from other Pocillopora species. In French Polynesia, both P. tuahiniensis sp. nov. and P. verrucosa host the algal symbiont, Cladocopium pacificum Turnham, Sampayo, and LaJeunesse 2021, but P. tuahiniensis sp. nov. tends to host a population of C. pacificum that is genetically different from that hosted by P. verrucosa (Johnston et al. 2022 a).
Johnston, Erika C., Burgess, Scott C. (2023): Pocillopora tuahiniensis: a new species of scleractinian coral (Scleractinia Pocilloporidae) from French Polynesia. Zootaxa 5369 (1): 117-124, DOI: 10.11646/zootaxa.5369.1.5, URL: https://www.mapress.com/zt/article/download/zootaxa.5369.1.5/52231