Hemicyclopora hexaspinae, Harmelin & Rosso, 2023
publication ID |
https://doi.org/ 10.5252/zoosystema2023v45a10 |
publication LSID |
urn:lsid:zoobank.org:pub:370E4D0A-FF10-4CAC-AF9F-A1A866FC1BEB |
DOI |
https://doi.org/10.5281/zenodo.8056985 |
persistent identifier |
https://treatment.plazi.org/id/E749E551-2748-4D15-BD80-A92CB661B657 |
taxon LSID |
lsid:zoobank.org:act:E749E551-2748-4D15-BD80-A92CB661B657 |
treatment provided by |
Felipe |
scientific name |
Hemicyclopora hexaspinae |
status |
sp. nov. |
Hemicyclopora hexaspinae n. sp.
( Figs 10 View FIG D-F; 11A-G; 12A-E; Tables 1 View TABLE ; 2 View TABLE ; 4 View TABLE )
urn:lsid:zoobank.org:act:E749E551-2748-4D15-BD80-A92CB661B657
Hemicyclopora discrepans – Harmelin 1997: 144, table 2.
Hemicyclopora multispinata – Di Geronimo et al. 1990: table 1.
TYPE LOCALITY. — France, La Ciotat, 3PP Cave.
TYPE MATERIAL. — Holotype. Mediterranean, France • 1 colony, c. 20 zooids (5 ovicells) + ancestrula; La Ciotat , 3PP Cave, 25 m depth from entrance; 73°09’47.9”N, 5°35’59.8”E; 20 m depth; 15.I.1993; Div.; JGH leg.; MNHN-IB-2017-771 . GoogleMaps
Paratypes. Mediterranean , France • 1 coated colony, c. 23 autozooids (4 ovicells); La Ciotat, 3PP Cave, 40 m from entrance; 73°09’47.9”N, 5°35’59.8”E; 21 m depth; 28.XI.1991; Div.; JGH leg.; MNHN-IB-2017-772 GoogleMaps • 1 coated colony, c. 30 autozooids (1 ovicell); Marseille, ‘ Calanques’ Coast, Cape Morgiou Cave ; 73°12’05.8”N, 05°27’08.11”E; 27 m depth; 26.IX.1967; Div.; JGH leg.; MNHN-IB-2017-773 GoogleMaps .
Italy • 1 ovicellate colony with ancestrula; Ustica Island , Apollo Bank; c. 38°7’N, 13°1’E; 60 m depth; VI.1986; Dre; AR leg.; PMC. B32.12.12.2020 GoogleMaps .
OTHER MATERIAL EXAMINED. — Mediterranean, France • 1 colony; Marseilles , ‘ Calanques’ Coast , Eissadon Cave; 73°12’07”N, 5°29’24.2”E; 5 m depth; 17.VI.1992; Div.; JGH leg.; MNHN GoogleMaps • c. 13 colonies (12 sampled spots); La Ciotat , 3PP Cave; 19-25 m depth; same site as for holotype; from XI.1991 to XI.1994; Div.; JGH leg.; MNHN. Italy • 7 colonies + fragments; S Tyrrhenian Sea, Ustica Island , Apollo Bank, same data as for paratype PMC. B32.12.12.2020; PMC Rosso-Collection I. H. B. 91a GoogleMaps • 4 colonies; W Ionian Sea, SE Sicily, Catania, off Acitrezza Marine Protected Area , 110 m depth (2 col.); Ciclopi survey; VII.2000; Stn 8I; 95 m depth (1 col.) & Stn 9G; 63 m depth (1 col.); coarse DC with Würmian biogenic remains; Dre; AR leg.; PMC Rosso-Collection I. H. B. 91b. Atlantic Ocean, western approach of Gibraltar Strait • 1 small colony on shell; R / V Cryos; Balgim Expedition; Stn DR 42; 35°54.5’N, 6°13.3’W; 133-137 m depth; 2. VI.1984; Dre ; JGH leg.; MNHN GoogleMaps • 2 small colonies; R / V Cryos; Balgim Expedition; Stn DW 43; 35°54.1’N, 6°14.5’W; 150 m depth; 2. VI.1984; Dre ; JGH leg.; MNHN GoogleMaps • 1 small colony on shell; R / V Cryos, Balgim Expedition; Stn DR 49; 35°53.0’N, 6°32.8’W; 518-524 m depth; MNHN GoogleMaps .
ETYMOLOGY. — From Latin hexa (six) and spinae (spines), in apposition, for the typical number of oral spines of this species in both ovicellate and non-ovicellate autozooids.
DIAGNOSIS. — Autozooids bulged, frontal shield finely granular with usually small to medium-sized marginal pores. Orifice terminal, condyles prominent with blunt tips, proximal edge more or less concave, without suboral umbo. Oral spines six in both non-ovicellate and ovicellate autozooids with the proximal pair arched inwardly and the distal ones outwardly. Ovicell presumably semicleithral, attached to the distal wall of the maternal zooid, produced by a small, basal kenozooid, narrower than autozooids; endooecium finely granular, without proximal thickening. Ancestrula with an extended cryptocyst and a narrow proximal gymnocyst, and 10-11 spines, four of them edging the cryptocyst.
DESCRIPTION
Colony encrusting, unilaminar, small (in most cases, less than 30 zooids). Autozooids relatively small ( Table 1 View TABLE ), longer than wide (L/W: 1.31), relatively poorly calcified, cystid with maximum thickness at orifice level; frontal shield markedly bulging, finely granular ( Figs 11A, D View FIG ; 12B View FIG ); marginal pores very small and poorly visible in specimens from caves (about 5-7 µm; Fig. 11 View FIG A-C) or larger in colonies from open soft bottoms (20-25 µm; Figs 11D, E View FIG ; 12B View FIG ); disto-lateral and distal walls subvertical, with numerous small basal pore chambers ( Fig. 11 View FIG A-D). Orifice distal, slightly broader than long; proximal edge (= poster) slightly concave or nearly straight, without proximal umbo or thickened rim; condyles triangular, slightly curved proximally, located just above the poster corners ( Figs 10D, E View FIG ; 11A, F View FIG ). Six oral spines in both non-ovicellate and ovicellate autozooids, exceptionally seven in non-ovicellate zooids (about 2% in available samples from Mediterranean caves), relatively short, with an open tip, articulated on thick, barrel-shaped bases ( Figs 10D View FIG ; 11 View FIG E- G); in both non-ovicellate and ovicellate zooids, spines of the proximal pair arched inwardly while spines of the distal pair arched outwardly ( Fig. 11 View FIG A-G). Ovicells kenozooidal, present at the colony margin ( Fig. 11 View FIG A-E), attached to the distal wall of the maternal zooid and on a tiny kenozooidal base, ovoid, significantly narrower than the maximum width of the maternal autozooid, presumably semicleithral ( Fig. 11C View FIG ); endooecium finely granular, imperforate, a small, triangular labellum sporadically present, with smooth surface suggesting a gymnocystal origin (outer fold of the ooecium floor?). Ancestrula with typical structure, opesia with a concave proximal border rimmed by a narrow band of smooth calcification, cryptocyst particularly extensive, and gymnocyst wide laterally but drastically narrowing proximally, four spines bordering the distal half of the cryptocyst and six, exceptionally seven, opesial spines; one autozooid budded distally ( Figs 10F View FIG ; 12B, D View FIG ). The ancestrula or an autozooid can occasionally produce a tubule from a lateral pore chamber, at the extremity of which an autozooid may be budded ( Fig. 12 View FIG C-E).
REMARKS
Morphological features
The most obvious distinctive features of H. hexaspinae n. sp. are: 1) the number of oral spines, six in both ovicellate and non-ovicellate zooids, which are articulated on particularly large, barrel-shaped bases; 2) the distinctly terminal orifice, with a strait or slightly concave proximal edge, without a proximal umbo; 3) the very convex frontal shield of autozooids; 4) the downcurved, triangular shape of the condyles; 5) the comparably small, nearly isodiametrical ovicells produced by a tiny basal kenozooid; and 6) the ancestrula with a broad cryptocyst and a very narrow proximal gymnocyst. The small size of colonies with a high frequency of ovicells and the predominantly peripheral position of the latter are also typical. Samples from the large, dark 3PP cave attest to these features: the number of autozooids of 17 collected colonies ranged from three to 30 (mean = 13 ± 6 AZ, but many zoecia were empty), with a high proportion of ovicellate ones (71%). The occurrence of ovicells is predominant at the colony margin (74%). This peripheral location may indicate a growth stop of the colony due to insufficient energy allocation after reproduction, a condition observed in dark caves when food inputs are sporadic ( Harmelin 1997). Specimens from soft bottoms in the open sea differ from those from dark caves essentially in the larger size of their marginal pores. This difference might be related to the dynamics of growth in these two environments, which is very slow in dark caves with poor exchanges with the open sea ( Harmelin 2000, see below). The semicleithral type of the ovicell closure was identified by A. Ostrovsky (personal communication to JGH, 18.X.2022) from a SEM picture ( Fig. 11C View FIG ) showing an ovicell partially closed by the ooecial vesicule and a sclerite.
Taxonomic issues
Hemicyclopora hexaspinae n. sp. differs from Mediterranean congeners particularly in the number of oral spines, shape of the orifice, and type of ovicells ( Table 2 View TABLE ). This species has several characters in common with H. discrepans ( Table 2 View TABLE ): a bulged frontal shield with a granular texture, absence of a thickening or umbo proximally to the orifice and on the ovicell, protuberant triangular condyles, poster concave or straight, oral spines with very thick bases, distal wall subvertical, ovicell apparently terminal but associated with a small basal kenozooid. However, H. hexaspinae n. sp. differs clearly from H. discrepans in having constantly six spines instead of eight in non-ovicellate zooids, and an ancestrula with the proximal gymnocyst poorly developed and the cryptocyst area widely extended proximally ( Figs 10F View FIG ; 12A View FIG ). Among other Recent Hemicyclopora species, the boreal H. emucronata ( Smitt, 1872) , also has six oral spines in both ovicellate and non-ovicellate zooids ( Smitt 1872: fig. 27; Kluge 1962: fig. 270). However, available SEM pictures of Smitt’s type and of a specimen from Spitsbergen (Kuklinski et al., website Atlas of Arctic Bryozoa, accessed on 30.IX.2020) show that H. emucronata clearly differs from H. hexaspinae n. sp. The former has zooids with a flatter frontal shield, the ovicell endooecium is continuous with the frontal shield of the distal zooid, and the ancestrula has a different structure.
HABITAT DISTRIBUTION
The available material of H. hexaspinae n. sp. was collected in two habitats which are quite opposite in terms of environmental conditions and type of substrates: walls of dark parts of shallow submarine caves vs biogenic remains at the surface of relatively deep soft bottoms (60-150 m) in the open sea. In underwater caves from the Marseille area, H. hexaspinae n. sp. was present with tiny, frequently ovicellate colonies (“spot colonies”, Bishop 1989; Okamura et al. 2001). However, in dark caves with low energy inputs from the outside, the occurrence of ovicells in tiny colonies is not a sign of early fertility and high offspring production, such as in r-selected species (e.g. Pianka 1970) from productive environments. On the contrary, in dark caves, the growth of bryozoan colonies is limited to a very low yearly production of zooids. This feature is revealed by the external aspect of zooids, which are more or less blackened by deposits of Mn and Fe oxides that increase over time ( Allouc & Harmelin 2001), a common phenomenon in aphotic habitats. This is exemplified by a tiny colony from 3PP Cave composed of the ancestrula and three autozooids ( Fig. 12D, E View FIG ), each budded very sporadically as shown by the increasing darkening of the frontal wall and spines from the third, youngest, zooid to the ancestrula. Such populations and colony features are signs of an adaptive strategy for life in highly cryptic and oligotrophic habitats where energy inputs from the outside are very limited and sporadic ( Harmelin 2000; Okamura et al. 2001). Another peculiarity of the occurrence of H. hexaspinae n. sp. in cryptic habitat is its uneven distribution among caves clustered in the same area. Along the coast from Marseille to La Ciotat, despite the great frequency of this habitat (mostly karstic cavities), specimens were recorded in only three caves. Most of them were collected in the vast 3PP Cave, but none in the similarly large Trémies Cave, close to the former (linear distance: <8 km), despite extensive sampling of its dark parts (e.g. Harmelin 1969, 1986). Differences in the inner thermal regime of these two caves might be the cause of this uneven distribution. In 3PP Cave, because of a descending profile ( Harmelin 1997), yearly fluctuations are reduced (12.8- 14.5°C) and close to those of the homothermic deep-sea. In contrast, in the Trémies Cave, due to a karstic origin, the inner ascending profile leads to the trapping of warm water bodies in the upper dark parts ( Harmelin 1969). However, H. hexaspinae n. sp. was also present in two other shallow caves (Cape Morgiou, Eissadon) where the inner thermal regime fluctuates as in the open sea at the same depth. The punctuated distribution of H. hexaspinae n. sp. in caves of the Provence region suggests that connectivity between caves is very low and recruitment is mostly autochthonous. In the same region, H. hexaspinae n. sp. was never recorded in deep-water samples (100-300 m, rock fragments, dead shells, coral skeletons) from the shelf and the neighbouring Cassidaigne Canyon ( Harmelin 1976, table III and unpublished data). In southern Italy, small living and dead colonies of H. hexaspinae n. sp. were found on the outer shelf, in thanatocoenoses occurring at the surface of detritic biogenic bottoms (Ionian Sea, eastern Sicily), and also at the top of the Apollo Bank where rocky outcrops with Laminaria rodriguezii Bornet, 1888 alternate with coarse detritic sand. Living colonies were mostly colonising small rhodoliths, fragments of coralline algae, dead branches of erect bryozoans [e.g. Adeonella calveti Canu & Bassler, 1930 and Smittina cervicornis (Pallas, 1766) ] and shells.
GEOGRAPHICAL DISTRIBUTION
Obviously, the small size of colonies of H. hexaspinae n. sp., the types of substrates on which they grow, and their scattered condition increase considerably the stochasticity of records. Therefore, its actual geographical distribution is poorly known. Most records were from the western Mediterranean Sea, in Provence, in the southern Tyrrhenian Sea, and in the western Ionian Sea (Sicily). This species has also been collected in the NE Atlantic, close to the western entrance of the Gibraltar Strait ( Table 4 View TABLE ). This occurrence in the Gulf of Cadiz, down to 524 m depth, may suggest a possible influence of the Mediterranean outflow water (e.g. Bashmachnikov et al. 2015) on the composition of the bottom fauna.
MNHN |
Museum National d'Histoire Naturelle |
R |
Departamento de Geologia, Universidad de Chile |
V |
Royal British Columbia Museum - Herbarium |
VI |
Mykotektet, National Veterinary Institute |
No known copyright restrictions apply. See Agosti, D., Egloff, W., 2009. Taxonomic information exchange and copyright: the Plazi approach. BMC Research Notes 2009, 2:53 for further explanation.
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Hemicyclopora hexaspinae
Harmelin, Jean-Georges & Rosso, Antonietta 2023 |
Hemicyclopora discrepans
HARMELIN J. - G. 1997: 144 |