Holopodidae Zittel 1879

Family Holopodidae Zittel, 1879 Remarks. Sieverts-Doreck (1951) believed that some ossicles and deformed Eugeniacrinus cups figured by Remeš (1902: pl. 19, figs. 11 a–c, 12–15) from the Štramberk Tithonian could belong to an Upper Jurassic species of Cyathidium. However, the figure is too imprecise to confirm an attribution to Holopodidae. The mere inclusion of Cyathidium depressum in a long list of cyrtocrinids cited from Lower Cretaceous Štramberk-type limestones (Salamon & Gorzelak 2010: 871) cannot be taken into account without a critical analysis of the material concerned. Moreover, the attribution to C. senessei (Valette in Lambert & Valette, 1934) of a very poorly preserved axillary from the Santonian of Poland by Salamon and Gorzelak (2011: 311, fig. 2C, D) is highly questionable. Here, we consider that the appearance of Holopodidae prior to the Cenomanian has not been demonstrated. It appears that the H/Wd ratio of IBrax is the best quantitative character to discriminate between the two genera in the family (> 0.7 in Holopus, <0.7 in Cyathidium) (Fig. 7). Stratigraphic distribution. Upper Cenomanian–Recent.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2024-11-28
DOI
https://doi.org/10.5281/zenodo.14248385
Primary Topic
Subterranean biodiversity and taxonomy
Type
article
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article

Holopodidae Zittel 1879

Zenodo (CERN European Organization for Nuclear Research)
Subterranean biodiversity and taxonomy
article

Holopodidae Zittel 1879

article en

Abstract

Family Holopodidae Zittel, 1879 Remarks. Sieverts-Doreck (1951) believed that some ossicles and deformed Eugeniacrinus cups figured by Remeš (1902: pl. 19, figs. 11 a–c, 12–15) from the Štramberk Tithonian could belong to an Upper Jurassic species of Cyathidium. However, the figure is too imprecise to confirm an attribution to Holopodidae. The mere inclusion of Cyathidium depressum in a long list of cyrtocrinids cited from Lower Cretaceous Štramberk-type limestones (Salamon & Gorzelak 2010: 871) cannot be taken into account without a critical analysis of the material concerned. Moreover, the attribution to C. senessei (Valette in Lambert & Valette, 1934) of a very poorly preserved axillary from the Santonian of Poland by Salamon and Gorzelak (2011: 311, fig. 2C, D) is highly questionable. Here, we consider that the appearance of Holopodidae prior to the Cenomanian has not been demonstrated. It appears that the H/Wd ratio of IBrax is the best quantitative character to discriminate between the two genera in the family (> 0.7 in Holopus, <0.7 in Cyathidium) (Fig. 7). Stratigraphic distribution. Upper Cenomanian–Recent.

Zenodo (CERN European Organization for Nuclear Research)
Centre National de la Recherche Scientifique (FR), École Pratique des Hautes Études (FR), Institut de Systématique, Évolution, Biodiversité (FR)
Openalex Percentile: Top 40%
Subterranean biodiversity and taxonomy
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