Calvetopora, Berning & Harmelin & Bader & Cibio, 2017
publication ID |
https://doi.org/ 10.5852/ejt.2017.347 |
publication LSID |
lsid:zoobank.org:pub:41385EAB-F391-468D-89CA-F7A574F820AB |
DOI |
https://doi.org/10.5281/zenodo.3850655 |
persistent identifier |
https://treatment.plazi.org/id/546F87A1-FF95-FFBD-09B3-9629363EFDF1 |
treatment provided by |
Carolina |
scientific name |
Calvetopora |
status |
|
Calvetopora sp.
Fig. 15 View Fig A–B, Table 15
Material examined
GREAT METEOR BANK: 1 small and bioeroded colony fragment free of a substrate, mounted on stub and sputter-coated, Stn 22 ( OLL 2016/155); 2 small and bioeroded colony fragments free of a substrate, mounted on stub and sputter-coated, Stn 22 ( OLL 2016/156); 1 small colony fragment free of a substrate, mounted on stub and sputter-coated, Stn 20, ( OLL 2016/157); 3 small and bioeroded colony fragments free of a substrate, mounted on stub and sputter-coated, Stn 22 ( OLL 2016/158).
Remarks
The examined specimens are very closely related to C. otapostasis gen. et sp. nov., yet differ in having smaller zooids, orifices and avicularia. Moreover, the orifice margin bears six (rarely five) spines, and the avicularia are more laterally directed ( Fig. 15B View Fig ). The available material, which comprises only a few small and bioeroded fragments lacking ovicells, and which were found in sediment samples, is insufficient in order to unambiguously determine whether it belongs to C. otapostasis gen. et sp. nov. or should rather be ascribed to another new species. Considering the geographic distance between Atlantis Smt and the Great Meteor Bank, however, we here treat C. otapostasis gen. et sp. nov. and Calvetopora sp. as distinct species. The specimens were found on the Great Meteor Bank at depths between 403 and 476 m.
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.
Kingdom |
|
Phylum |
|
Class |
|
Order |
|
Family |