Pileolosphaera
publication ID |
https://doi.org/10.1080/00318884.2023.2172841 |
DOI |
https://doi.org/10.5281/zenodo.15537843 |
persistent identifier |
https://treatment.plazi.org/id/03ED093D-5016-FFEA-FFAB-7850FC24FEC3 |
treatment provided by |
Felipe |
scientific name |
Pileolosphaera |
status |
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The extant nannolith-bearing species Pileolosphaera longistirpes K.J.S. Meier, Kinkel & Jer.R. Young , which is the type species of the genus Pileolosphaera , is composed of about six to eight circular shield-like nannoliths. The nannoliths are formed exclusively of V-units ( Meier et al. 2014) showing on the coccosphere, radially oriented calcite axes under light microscopy ( Meier et al. 2014). The nannoliths possess three radial segments with a central triradiate process. Light microscopy observations indicate that all three elements are formed of crystal units with their c-axes vertical relative to the nannolith, and therefore, radial relative to the coccosphere ( Meier et al. 2014). Pileolosphaera shares with Ericiolus the key features of triradiate symmetry and radial growth of the elements from the centre, rather than around a rim. There are, however, notable differences between the two taxa: 1) Pileolosphaera coccospheres have far fewer nannoliths than those of Ericiolus (6–8 vs 30–70); and 2) the Pileolosphaera nannoliths are considerably larger than those of Ericiolus (3.0–4.0 μ m vs 0.2–1.3 μ m). Despite these quantitative differences, Pileolosphaera nannoliths are structurally the closest extant forms to Ericiolus , and affinity between the two genera remains likely.
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