Celeroliroceras celere Korn & Ghaderi, 2025, gen. et sp. nov.

Celeroliroceras celere gen. et sp. nov. urn:lsid:zoobank.org:act: B1A2F8FC-0603-4F60-A7BA-5E5735C44FF2 Fig. 43; Table 25 Liroceras sp. – Gliwa et al. 2020: text-fig. 17g. Diagnosis Species of Celeroliroceras gen. nov. with thinly globular, subinvolute to involute conch (ww/dm ~ 0.85–0.90; uw/dm ~ 0.15), weakly to moderately depressed whorl profile (ww/wh ~1.40–1.60) and extraordinarily high coiling rate (WER ~3.60) between a conch diameter of 30 and 60 mm. Whorl profile with broadly arched venter and flanks, broadly rounded umbilical margin and convex umbilical wall and small imprint zone (IZR ~0.15). Shell surface smooths. Suture line nearly straight. Etymology From the Latin ‘ celere ’ (adjective, n.)=‘fast’; because of the conch geometry with the extraordinarily high coiling rate. Type material Holotype IRAN – West Azerbaijan • Aras Valley; Araxoceras Beds of the Julfa Formation (early Wuchiapingian); 2011; Korn et al. leg.; illustrated in Fig. 43; MB.C.29352. Description Holotype MB.C.29352 is fully septate with a conch diameter of 57 mm (Fig. 43A). It is slightly deformed but relatively well preserved, allowing the study of conch geometry, suture line and, with limitations, ornamentation. The remarkable conch geometry is mainly caused by the extraordinarily high coiling rate (WER =3.60). The conch is globular and involute (ww/dm =0.88; uw/dm=0.14) and the ww/wh ration amounts 1.60. The whorl profile is crescent-shaped with a convex umbilical wall and a rounded umbilical margin from which the flanks converge strongly towards the broadly rounded venter (Fig. 43B). The whorl overlap zone is very small (IZR = 0.15). It appears that the whorl width increases faster than the whorl height on the last volution; the ww/wh ratio increases from 1.43 to 1.60 during the last half volution. There are some shell remains attached to the phragmocone; these are almost smooth with no traces of ornamentation. The suture line is almost straight, but has a very flat and very wide external lobe (Fig. 43C). Remarks Celeroliroceras celere gen. et sp. nov. is very different from all other Late Permian nautiloids. It is clearly separable from the co-occurring Liroceras choopani sp. nov. by its extraordinarily high coiling rate (WER= 3.60 in contrast to 2.30 in L. choopani) and the much smaller whorl overlap rate.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2025-09-24
DOI
https://doi.org/10.5281/zenodo.17234959
Primary Topic
Social Sciences and Governance
Type
article
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article

Celeroliroceras celere Korn & Ghaderi, 2025, gen. et sp. nov.

Zenodo (CERN European Organization for Nuclear Research)
Social Sciences and Governance
article

Celeroliroceras celere Korn & Ghaderi, 2025, gen. et sp. nov.

article en

Abstract

Celeroliroceras celere gen. et sp. nov. urn:lsid:zoobank.org:act: B1A2F8FC-0603-4F60-A7BA-5E5735C44FF2 Fig. 43; Table 25 Liroceras sp. – Gliwa et al. 2020: text-fig. 17g. Diagnosis Species of Celeroliroceras gen. nov. with thinly globular, subinvolute to involute conch (ww/dm ~ 0.85–0.90; uw/dm ~ 0.15), weakly to moderately depressed whorl profile (ww/wh ~1.40–1.60) and extraordinarily high coiling rate (WER ~3.60) between a conch diameter of 30 and 60 mm. Whorl profile with broadly arched venter and flanks, broadly rounded umbilical margin and convex umbilical wall and small imprint zone (IZR ~0.15). Shell surface smooths. Suture line nearly straight. Etymology From the Latin ‘ celere ’ (adjective, n.)=‘fast’; because of the conch geometry with the extraordinarily high coiling rate. Type material Holotype IRAN – West Azerbaijan • Aras Valley; Araxoceras Beds of the Julfa Formation (early Wuchiapingian); 2011; Korn et al. leg.; illustrated in Fig. 43; MB.C.29352. Description Holotype MB.C.29352 is fully septate with a conch diameter of 57 mm (Fig. 43A). It is slightly deformed but relatively well preserved, allowing the study of conch geometry, suture line and, with limitations, ornamentation. The remarkable conch geometry is mainly caused by the extraordinarily high coiling rate (WER =3.60). The conch is globular and involute (ww/dm =0.88; uw/dm=0.14) and the ww/wh ration amounts 1.60. The whorl profile is crescent-shaped with a convex umbilical wall and a rounded umbilical margin from which the flanks converge strongly towards the broadly rounded venter (Fig. 43B). The whorl overlap zone is very small (IZR = 0.15). It appears that the whorl width increases faster than the whorl height on the last volution; the ww/wh ratio increases from 1.43 to 1.60 during the last half volution. There are some shell remains attached to the phragmocone; these are almost smooth with no traces of ornamentation. The suture line is almost straight, but has a very flat and very wide external lobe (Fig. 43C). Remarks Celeroliroceras celere gen. et sp. nov. is very different from all other Late Permian nautiloids. It is clearly separable from the co-occurring Liroceras choopani sp. nov. by its extraordinarily high coiling rate (WER= 3.60 in contrast to 2.30 in L. choopani) and the much smaller whorl overlap rate.

Zenodo (CERN European Organization for Nuclear Research)
Museum für Naturkunde (DE), Ferdowsi University of Mashhad (IR)
Openalex Percentile: Top 38%
Social Sciences and Governance
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