Surface Microornamentation of Demosponge Sterraster Spicules, Phylogenetic and Paleontological Implications

Type Article
Date 2020-12
Language English
Author(s) Cárdenas Paco1
Affiliation(s) 1 : Pharmacognosy, Department of Pharmaceutical Biosciences, Uppsala University, Uppsala, Sweden
Source Frontiers In Marine Science (2296-7745) (Frontiers Media SA), 2020-12 , Vol. 7 , P. 613610 (27p.)
DOI 10.3389/fmars.2020.613610
WOS© Times Cited 4
Keyword(s) Porifera, systematics, Geodia, Placospongia, Rhaxella, microfossils, sterrasters, selenasters

Siliceous spicules in demosponges exist in a variety of shapes, some of which look like minute spheres of glass. They are called “sterrasters” when they belong to the Geodiidae family (Tetractinellida order) and “selenasters” when they belong to the Placospongiidae family (Clionaida order). Today, the Geodiidae represent a highly diverse sponge family with more than 340 species, occurring in shallow to deep waters worldwide, except for the Antarctic. The molecular phylogeny of Geodiidae is currently difficult to interpret because we are lacking morphological characters to support most of its clades. To fill this knowledge gap, the surface microornamentations of sterrasters were compared in different genera. Observations with scanning electron microscopy revealed four types of surfaces, which remarkably matched some of the Geodiidae genera: type I characteristic of Geodia, type II characteristic of Pachymatisma, Caminus, and some Erylus; type III characteristic of other Erylus; type IV characteristic of Caminella. Two subtypes were identified in Geodia species: warty vs. smooth rosettes. These different microornamentations were mapped on new Geodiidae COI (Folmer fragment) and 28S (C1–D2) phylogenetic trees. The monophyly of the Geodiidae was once again challenged, thereby suggesting that sterrasters have evolved independently at least three times: in the Geodiinae, in the Erylinae and in Caminella. Surface microornamentations were used to review the fossil record of sterrasters and selenasters through the paleontology literature and examination of fossils. It was concluded that “rhaxes” in the literature may represent mixes of sterrasters and selenasters: while Rhaxella spicules may belong to the Placospongiidae, Rhaxelloides spicules belong to the Geodiidae. The putative Geodiidae fossil genera, Geoditesia, and Geodiopsis, are reallocated to Tetractinellida incertae sedis. Isolated Miocene-Pliocene fossil sterrasters Hataina (Huang, 1967), Silicosphaera (Hughes, 1985) and Conciliaspongia (Robinson and Haslett, 1995) become junior synonyms of Geodia (Lamarck, 1815). Overall, the fossil record suggested that Geodiidae was present at least since the Middle Jurassic (163–166 Mya), while Geodia sterrasters were present since the Santonian/Campanian boundary, Late Cretaceous (83.6 Mya).

Full Text
File Pages Size Access
Publisher's official version 27 15 MB Open access
Data_Sheet_1 95 KB Open access
Data_Sheet_2 76 KB Open access
Image_1 1 404 KB Open access
Table_1 66 KB Open access
Top of the page