Distinguishing features:
Parent taxon (Arkhangelskiellaceae): Arkhangelskielids with shields predominantly formed of R-units, thus bright in cross-polarised light; V-units often form dark outer rim.
This taxon: R-units cover the distal surface, so coccolith appears bright, unicyclic, in LM (although darker towards outer edge); central-area has perforate plate with axial sutures. 4 tiers visible in side view.
Daughter taxa (time control age-window is: 0-800Ma) | ||||
Arkhangelskiella maastrichtiensis Large to very large (>10µm) with a broad rim (>1.5µm) | ||||
Arkhangelskiella cymbiformis Large (8-10µm), with a narrow rim (<1.5µm) | ||||
Arkhangelskiella confusa Small to medium sized (4-8µm), with a <1.5µm thick rim | ||||
Arkhangelskiella specillata Like A. cymbiformis but with >5 perforations per quadrant (Verbeek 1977) | ||||
Arkhangelskiella sp. Specimens not identified to species level |
Taxonomy:
Farinacci & Howe catalog pages: Arkhangelskiella + + + + *
Distinguishing features:
Parent taxon (Arkhangelskiellaceae): Arkhangelskielids with shields predominantly formed of R-units, thus bright in cross-polarised light; V-units often form dark outer rim.
This taxon: R-units cover the distal surface, so coccolith appears bright, unicyclic, in LM (although darker towards outer edge); central-area has perforate plate with axial sutures. 4 tiers visible in side view.
The most common genus and a characteristic component of Maastrichtian nannofossil assemblages. The central area structure is described in detail by Moshkovitz and Osmond (1989).
Morphology:
Ditinction from Broinsoinia:
- in LM the entire cocclith rim is brightly birefringent (vs there being a distinct dark outer cycle in Broinsoinia)
- in SEM in distal view, a single cycle of elements, typically with clear sutures, covers the distal surface (vs inner and outer cycles in Broinsonia).
- in SEM in side view, four tiers of elements are visible (vs 3 in Broinsonia).
- in SEM in proximal view, they are essentially identical.
LITHS: placolith, elliptical, CA: plate, pores, closed, CROSS-POLARS: rim-unicyclic, R-prominent, |
Lith size: 5->20µm; Data source notes: size range of included species |
Geological Range:
Last occurrence (top): at top of Maastrichtian Stage (100% up, 66Ma, in Danian stage). Data source: Total of ranges of the species in this database
First occurrence (base): within Campanian Stage (72.17-83.65Ma, base in Campanian stage). Data source: Total of ranges of species in this database
Plot of occurrence data:
Burnett, J. A. (1998). Upper Cretaceous. In, Bown, P. R. (ed.) Calcareous Nannofossil Biostratigraphy. British Micropalaeontological Society Publication Series . 132-199. gs O Linnert, C. & Mutterlose, J. (2009a). Biometry of the Late Cretaceous Arkhangelskiella group: ecophenotypes controlled by nutrient flux. Cretaceous Research. 30: 1193-1204. gs Moshkovitz, S. & Osmond, K. (1989). The optical properties and microcrystallography of Arkhangelskiellaceae and some other calcareous nannofossils of the Late Cretaceous. In, Crux, J. A. & van Heck, S. E. (eds) Nannofossils and their applications: Proceedings of the 2nd INA Conference, London 1987. British Micropalaeontological Society Publication Series . 76-97. gs O Vekshina, V. N. (1959). Coccolithophoridae of the Maastrichtian deposits of the West Siberian lowlands. Trudyi Instituta Geologii i Geogiziki, Sibiriskoe Otlodelenie, Akademiya Nauk SSSR (Nauka) Moscow. 2: 56-81. gsReferences:
Arkhangelskiella compiled by Jeremy R. Young, Paul R. Bown, Jacqueline A. Lees viewed: 10-9-2024
Short stable page link: https://mikrotax.org/Nannotax3/index.php?id=10035 Go to Archive.is to create a permanent copy of this page - citation notes |
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