Zaphrentites cf. parallela (Carruthers, 1910)

El-Desouky, Heba, Herbig, Hans-Georg & Kora, Mahmoud, 2023, Kasimovian (late Pennsylvanian) cornute rugose corals from Egypt: taxonomy, facies and palaeogeography of a cool-water fauna from northern Gondwana, Swiss Journal of Palaeontology (32) 142 (1), pp. 1-39 : 21-24

publication ID

https://doi.org/ 10.1186/s13358-023-00296-0

persistent identifier

https://treatment.plazi.org/id/49386916-7F0D-FFEF-FC91-F9D3FE86FB68

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Felipe

scientific name

Zaphrentites cf. parallela (Carruthers, 1910)
status

 

Zaphrentites cf. parallela (Carruthers, 1910) .

( Fig. 11A View Fig 1–A View Fig 3 View Fig , B 1–B View Fig 4 View Fig , 12D View Fig ).

cf. 1910 Zaphrentis parallela Carruthers. - p. 533, Pl. 37, Fig. 4 View Fig .

cf. 2014 Zaphrentites parallela (Carruthers) .- Denayer and Hoşgör, p. 350, Fig. 4 View Fig : 6a–d, 14 (cum syn.).

Material: Tree corallites (RAh 109, RAh 111 and RAh 118); collected from the basal shales of the lower member of the Aheimer Formation. Nine transverse thin-sections are available.

Description: External characters: Straight, conical corallites, about 1.5 cm long, slightly curved in the immature stage. Calyx is largely eroded, apex not preserved. Septal furrows and delicate growth lines are distinctly marked on the external wall ( Fig. 11B View Fig 1 View Fig ). An attachment scar is visible in one corallite near the apical part.

Internal characters: In the earliest ontogenetic preserved stage ( Fig. 11A View Fig 1 View Fig ), septa are very thick, reaching the corallite axis. Tere are 16 septa at a corallite diameter of about 3 mm; of them the counter septum is the thickest. At diameter of 3.7 mm ( Fig. 11B View Fig 2 View Fig ), major septa are still thick, they join in the centre forming a thick stereocolumn; a parallel sided cardinal fossula can be recognised. In the subsequent early mature growth stage at a diameter of 5 mm, there are 20 major septa ( Fig. 11A View Fig 2 View Fig ). Minor septa are absent. Te axial ends of major septa join to form an axial stereocolumn slightly staggered towards the counter quadrants. Septa of the counter quadrants are radially arranged, the counter septum is slightly thicker and has the same length as the adjacent septa. Tose in the cardinal quadrants are grouped pinnately around a long parallel sided cardinal fossula. Te thin cardinal septum is straight, long and reaches beyond the corallite axis to join the stereocolumn at the upper end of the cardinal fossula in the counter quadrants. It further thins towards the axis. Further mature, at a diameter of 6.5 mm, there are 21 septa ( Fig. 11B View Fig 3 View Fig ); the cardinal septum becomes slightly shorter.

Te uppermost mature transverse section near the calice floor ( Fig. 11A View Fig 3 View Fig , B 4 View Fig ) is slightly deformed due to compaction and some of the septa are broken. In this stage there are maximum 26 septa in 8.6 mm ( Fig. 11B View Fig 4 View Fig ). Axial ends of the major septa in cardinal quadrants are bent to sides with the two pericardinal septa, curved most distinctly. Such septal morphology makes the cardinal fossula opens towards the free axial area. Te cardinal fossula is slightly deformed. Te cardinal septum is short, and the counter is slightly longer and thicker than the adjacent septa. All major septa are thick at the base, join at their rhopaloid ends around the well-developed cardinal fossula, which invades the counterpart, being longer than the radius of the corallite. Pseudoalar fossulae are not markedly developed. Minor septa are absent from the corallite lumen, they are visible in the stereoplasm of the wall.

Discussion: According to the septal arrangement and the axial stereocolumn, the current species clearly belongs to the genus Zaphrentites . It is closely similar to Z. parallela (Carruthers, 1910) in the septal arrangement and more or less in the shape of the cardinal fossula, with the cardinal septum withdrawn in late stages. However, our specimens reach larger n:d ratios ( Fig. 12D View Fig ) in the last mature stage near the calice (26:8.6 vs. 20:5.6). Z. delanouei ( Milne-Edwards and Haime, 1851) and Z. crassus Hudson, 1944 are both larger and have more septa than the herein described species. It is quite similar to Z. parallela of Denayer and Hoşgör (2014) from the Lower Carboniferous of Turkey. It differs in the n:d ratio of the last mature stage (21:8.5) and in general counts more septa at the same diameter.

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