Hostname: page-component-74656f9884-j7cmm Total loading time: 0 Render date: 2026-11-07T06:47:27.702Z Has data issue: false hasContentIssue false

A new limulid genus from the Strelovec Formation (Middle Triassic, Anisian) of northern Slovenia

Published online by Cambridge University Press:  07 May 2019

Russell D. C. Bicknell*
Affiliation:
Palaeoscience Research Centre, School of Environmental and Rural Science, University of New England, Armidale, 2351, Australia
Jure Žalohar
Affiliation:
T-TECTO, Koroška cesta 12, SI-4000 Kranj, Slovenia
Primož Miklavc
Affiliation:
Department of Geology, Faculty of Natural Sciences and Engineering, University of Ljubljana, Aškerčeva ceta 12, SI-1000 Ljubljana, Slovenia
Bogomir Celarc
Affiliation:
Geological Survey of Slovenia, Dimičeva ulica 14, SI–1000 Ljubljana, Slovenia
Matija Križnar
Affiliation:
Slovenian Museum of Natural History, Prešernova 20, SI-1000 Ljubljana, Slovenia
Tomaž Hitij
Affiliation:
Dental School, Faculty of Medicine, University of Ljubljana, Hrvatski trg 6, SI-1000 Ljubljana, Slovenia
*
*Author for correspondence: Russell D. C. Bicknell, Email: rdcbicknell@gmail.com
Rights & Permissions [Opens in a new window]

Abstract

Horseshoe crabs are an archetypal chelicerate group with a fossil record extending back to Early Ordovician time. Although extensively studied, the group generally has a low diversity across the Phanerozoic Eonothem. Here, we expand the known diversity of true horseshoe crabs (Xiphosurida) by the description of a new taxon from the Middle Triassic Strelovec Formation of the Slovenian Alps. The mostly complete fossil is preserved as an external mould and assigned to the family Limulidae Zittel, 1881 as Sloveniolimulus rudkini, n. gen., n. sp. The use of landmark and semilandmark geometric morphometrics is explored to corroborate the systematic palaeontology and suggests that the new genus and species are valid. We also provide the first quantitative evidence for the extensive diversity of Triassic horseshoe crabs. We suggest that Triassic horseshoe crabs likely filled many ecological niches left vacant after the end-Permian extinction.

Information

Type
Original Article
Copyright
© Cambridge University Press 2019 
Figure 0

Fig. 1. Abundance of xiphosurid genera since the Triassic Period. Maximum abundance and diversity arose during the Triassic Period and decreased dramatically afterwards. The plot does not include Carcinoscorpius rotundicauda (Latreille, 1802), as the genus does not have a fossil species. Data from Dunlop et al. (2018).

Figure 1

Fig. 2. Stratigraphic column of the Križevnik mountain area. Modified from Celarc et al. (2012).

Figure 2

Fig. 3. Map of the Kamnik-Savinja Alps. Slatinski Plaz location is indicated with an asterisk.

Figure 3

Fig. 4. Slatinski Plaz Section (S1). The xiphosurid fossil was found near the base of Unit 2. Modified with permission after Miklavc et al. (2016).

Figure 4

Fig. 5. Sloveniolimulus rudkini holotype (PMSL T-993). (a) Complete specimen. Pustule (‘dumb-bell’) structures evident across entire specimen. (b) Close-up of cardiac lobe (white arrows) and cephalothoracic-thoracetron hinge (black arrow). (c) Close-up of left side of thoracetron. Thoracetronic border defined by pustules and possible distal section of a gill operculum (white arrow). (d) Close-up of left genal spine and cephalothorax. Indentation in genal spine (white arrow) and ophthalmic ridge (black arrow) noted. Ophthalmic ridge defined by pustules. (e) Close-up of right genal spine. Genal spine indentation (white arrow) slightly less pronounced than on left side. Specimen was coated with ammonium chloride.

Figure 5

Fig. 6. Silicon cast of Sloveniolimulus rudkini holotype (PMSL T-993.C) used to highlight genal spine deflection. (a) Complete cast, showing more clearly the putative walking trace at the posterior end of the specimen. (b) Close-up of left genal spine, showing deflection at distal section of spine (white arrow). (c) Close-up of right genal spine, showing less-pronounced deflection at distal section of spine (white arrow). Specimen was coated with ammonium chloride. Images were reflected to mirror the holotype.

Figure 6

Fig. 7. Carboniferous–Recent xiphosurids in PCA space. Austrolimulids fall in very positive PC1 space, reflecting their extreme cephalothoracic morphologies. Limulids and paleolimulids occupy a similar PC space. Sloveniolimulus rudkini falls into the extremes of shape space occupied by Limulidae and Paleolimulidae. (a) Austrolimulus fletcheri (AM F 38274, holotype). Note the large genal spines and splay. Courtesy of Josh White; Australian Museum specimen. (b) Tachypleus gadeai (MGSB 19195, holotype). Note termination of genal spines about cephalothorax-thoracetron hinge. Courtesy of Pedro Adserà; Museu Geologic del Seminari de Barcelona specimen. (c) Victalimulus mcqueeni (MV P22410B, holotype). A less extreme fossil morphology compared with A. fletcheri. Courtesy of Frank C. Holmes; Museums Victoria specimen.

Figure 7

Fig. 8. PCA plots detailing morphospace occupied by genera and the morphospace explored across the seven time-bins. (a) Xiphosurid genera bound by convex hulls. Sloveniolimulus rudkini falls outside of the Paleolimulus cluster, excluding the new species from Paleolimulidae. (b) Taxa colour-coded for time-bin and bound by convex hulls. Triassic taxa cover largest PC space, followed by Carboniferous and Jurassic taxa.

Figure 8

Fig. 9. Reconstruction of Sloveniolimulus rudkini and its possible prey. (a) Reconstruction of the studied PMSL T-993. Courtesy of Elissa Martin. (b–d) Examples of potential prey items found in the Slatinski Plaz Section: (b) Bivalve species Modiolus sp.; (c) small ammonoid; and (d) juvenile decapod crustacean Aeger sp.

Supplementary material: File

Bicknell et al. supplementary material

Bicknell et al. supplementary material 1

Download Bicknell et al. supplementary material(File)
File 20.2 KB
Supplementary material: File

Bicknell et al. supplementary material

Bicknell et al. supplementary material 2

Download Bicknell et al. supplementary material(File)
File 288 Bytes
Supplementary material: File

Bicknell et al. supplementary material

Bicknell et al. supplementary material 3

Download Bicknell et al. supplementary material(File)
File 27.7 KB