Bebryce inermis, Namin & Van Ofwegen, 2010
publication ID |
https://doi.org/ 10.5252/z2010n3a9 |
persistent identifier |
https://treatment.plazi.org/id/177787D3-FFBE-A611-FCA3-FD650C21B025 |
treatment provided by |
Felipe |
scientific name |
Bebryce inermis |
status |
sp. nov. |
Bebryce inermis View in CoL n. sp.
( Figs 1 View FIG ; 2A, B View FIG ; 3-7 View FIG View FIG View FIG View FIG View FIG )
TYPE MATERIAL. — Holotype: Oman. 23°31’38.92”N, 58°44’23.32”E, coll. K. Samimi Namin, 1.XII.2007, 1 colony ( MNHN). GoogleMaps
Paratypes: Oman. 23°31’48.88”N, 58°43’40.89”E, coll. K. Samimi Namin, XI.2007, 1 colony ( RMNH Coel. 38923). — 23°31’23.73”N, 58°44’50.58”E, coll. K. Samimi Namin, 30.XI.2007, 3 colonies ( RMNH Coel. 38924). — 23°31’48.88”N, 58°43’40.89”E, coll. K. Samimi Namin, 19.V.2009, 4 colonies ( RMNH Coel. 38925). — Daymaniyat islands, 23°50’20.85”N, 57°58’11.19”E, coll.K.SamimiNamin, 5 colonies ( RMNH Coel. 39556). — Bandar Al-Khiran, 23°31’38.92”N, 58°44’23.32”E, 3 colonies ( RMNH Coel. 39557). — Daymaniyat islands, 23°51’42.96”N, 58°07’10.15”E, coll. K. Samimi Namin, 27.V.2009, 4 colonies ( RMNH Coel. 39558). — 23°32’1.80”N, 58°42’54.06”E, coll.K.Samimi Namin, 8.VI.2009, 1 colony ( RMNH Coel. 39559).
ETYMOLOGY. — Latin “inermis”, unarmed, without weapons, defenceless, toothless, without a sting, refers to the calyx margin spindles without split antler-like projection.
DESCRIPTION
The holotype is fan-shaped without anastomoses. The colony is 6.5 cm high and 7 cm wide, the main stem is about 2 mm wide and branching starts at the base of the main stem ( Fig. 2A View FIG ). Polyps are situated all around the branches with prominent calyces about 1 mm high. Some parts of the colony, mostly at the base, are covered with an encrusting sponge.
Polyps are retracted and have 3-6 spindles per point. These spindles are up to 0.35 mm long and have spines or a spiny leaf at their distal end ( Fig. 4A View FIG ). Th e collaret has 2 or 3 rows of bent spindles, up to 0.40 mm long ( Fig. 4B View FIG ). Tentacles have bow-shaped spindles up to 0.07 mm long, and a few small rods, up to 0.05 mm long.
At the margin of the calyces spindles are present, up to 0.12 mm long, with an unilateral projection ( Fig. 4C View FIG ).
The surface layer sclerites are rosettes, up to 0.05 mm long, with warty, rounded, or bristle-like projections ( Fig. 4 View FIG D-F).
In the subsurface layer a few rosettes occur, up to 0.12 mm long ( Fig. 5A View FIG ). Most sclerites are stellate plates, up to 0.18 mm long ( Fig. 5B View FIG ). Furthermore, several less developed sclerites are also present ( Fig. 5C View FIG ).
Colour
Live colonies were brown-yellowish in colour with yellow polyps ( Fig. 3 View FIG ); preserved it is brown, sclerites colourless.
VARIABILITY
Several paratypes have a bushy colony shape ( Fig.2B View FIG ). Also the sclerites differ between colonies, in about half of the paratypes the stellate plates with long rays are few in number; also the number of rosettes with bristle-like projections is much smaller in these specimens ( Figs 6 View FIG ; 7 View FIG ). Very little is known about sclerite characters to use for identification of Bebryce species. At present we consider these observed differences to represent intra-specific variation rather than describing two related species.
HABITAT
Most of the specimens can be seen in dark places such as cracks and caverns on underwater cliffs and walls, often hanging down. We observed all collected specimens to be overgrown by sponges on some parts of the colony.
REMARKS
For comparison with B. studeri we used the material described by Grasshoff (1999): ORSTOM HG
200, New Caledonia, S lagon, Îlot Canard, stn 136, 23 m depth; material stored in the MNHN (under MNHN-Oct.0000-0569). Bebryce studeri differs from B. inermis n. sp. in having different calyx margin spindles, with a split projection ( Fig. 8C View FIG ), almost antler-like. Additionally, it lacks poorly developed subsurface sclerites ( Fig. 9 View FIG ). For further comparison we also present polyp sclerites and rosettes of B. studeri ( Fig. 8A, B, D, E View FIG ).
For comparison with B. stellata we used RMNH material from the type locality Ambon, collected during the 1996 LIPI-NNM Fauna Malesiana Maluku Expedition. Bebryce stellata differs from B. inermis n. sp. and B. studeri in having many ellipsoids in the subsurface layer.
Two colonies of RMNH Coel.39558 have several small colonies of an unknown Astrogorgia Verrill, 1868 species attached to the branches.
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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