The additional apertures of this taxon may be circular, oval or keyhole-shaped and are usually symmetrically arranged along the equatorial plane. It is likely that they developed by invagination of the margins of a typical Hantkenina-type aperture (Bermúdez, 1937; Bandy, 1949; Barnard, 1954; Banner and Blow, 1959; Ramsay, 1962; Blow and Banner, 1962; Dieni and Proto Decima, 1964). Specimens with apertures transitional in morphology between Hantkenina and Cribrohantkenina demonstrate that the evolution involved several steps and processes: broadening of the high-arched triradiate aperture (as seen in H. nanggulanensis); crenulation and invagination of the imperforate margin; and restriction of the primary aperture, creating isolated areal opening(s) in the imperforate surround.
The precise stratigraphic range of Cribrohantkenina in the uppermost Eocene is difficult to establish in many sites because of common dissolution events associated with the Eocene/Oligocene climatic transition (e.g., Shackleton and Kennett, 1975; Zachos and others, 1996). Rare complete specimens, or more commonly fragments of the characteristic aperture system, have been found ranging up to the Eocene/ Oligocene boundary at Torre Cardela, Fuente Caldera, and Molino de Cobo, Spain; Massignano, Italy; Tanzania (PNP, unpublished data); and ODP Site 707, Indian Ocean (Martinez-Gallego and Molina, 1975; Molina, 1986; Molina and others, 1988; Coccioni, 1988; Nocchi and others, 1988; Coxall, 2000) confirming that this genus existed in parallel with Hantkenina until their apparently simultaneous extinction at the boundary. Van Eijden (1995, p. 240) figured an interesting specimen with Cribrohantkenina-like areal apertures from Zone E12. This specimen has the morphology of H. compressa, and is relatively small and compressed in comparison to the forms found in the upper Eocene. No other occurrences of Cribrohantkenina have been recorded below Zone E14, hence Van Eijden’s specimen is considered a probable teratoid Hantkenina.
An important feature of our Cribrohantkenina taxonomy is the synonomy of Cribrohantkenina lazzarii (Pericoli) with C. inflata. Cribrohantkenina lazzarii has been commonly recorded from the uppermost Eocene of Italy and Spain. It is described as differing from C. inflata in having a more polygonal peripheral outline, more compact coiling (Pericoli, 1958) and a higher stratigraphic range, extending above the last occurrence of C. inflata to the Eocene/Oligocene boundary (Dieni and Proto Decima, 1964; Coccioni, 1988; Gonzalvo and Molina, 1992). The holotype of C. lazzarii has been examined under SEM for the first time in this work. Micrograph images reveal that the holotype is crushed and very poorly preserved (Pl.8.3, Figs. 15-16), hampering recognition of the cribrate aperture and exaggerating the polygonal morphology. In our investigations of uppermost Eocene assemblages (including DSDP Site 522, ODP Sites 707, Tanzania, Torre Cardela, and Massignano) we were unable to stratigraphically or morphologically distinguish the C. lazzarii morphotype from C. inflata at any location. Furthermore we have found inflated forms of the C. inflata-type ranging up to the Eocene/Oligocene boundary at Massignano, Tanzania and in the Spanish sections. In agreement with Coccioni (1988) and Gonzalvo and Molina (1992) we recognize that some forms of Cribrohantkenina have more polygonal chambers and an angular peripheral outline. However, we observe that this feature is also characteristic of earlier stages of ontogeny in all specimens of Cribrohantkenina and that loss of the final globular chamber through breakage (which is common in upper Eocene foraminiferal assemblages from the Tethyan region) changes the overall aspect of the shell considerably by emphasizing the pre-adult polygonal form. [Coxall & Pearson 2006]
Catalog entries: Hantkenina inflata, Hantkenina (Cribrohantkenina) bermudezi, Hantkenina danvillensis, Hantkenina lazzarii
Type images:Distinguishing features:
Parent taxon (Cribrohantkenina): Final chambers with tubulospines and areal apertures
This taxon: Hantkeninids with one of more areal apertures in addition to the primary aperture in the final adult chamber(s). Often very large (tests can be >1.0 mm).
Morphology:
Wall type:
Character matrix
test outline: | Lobate | chamber arrangement: | Planispiral | edge view: | Hourglass | aperture: | Equatorial |
sp chamber shape: | Inflated | coiling axis: | N/A | periphery: | Tubulospines | aperture border: | Thin lip |
umb chbr shape: | Inflated | umbilicus: | Wide | periph margin shape: | Broadly rounded | accessory apertures: | - |
spiral sutures: | Moderately depressed | umb depth: | Shallow | wall texture: | Smooth | shell porosity: | Finely Perforate: 1-2.5µm |
umbilical or test sutures: | Moderately depressed | final-whorl chambers: | 5-6 | N.B. These characters are used for advanced search. N/A - not applicable |
Geographic distribution
Aze et al. 2011 summary: Low to middle latitudes; based on Coxall & Pearson (2006)
Isotope paleobiology
Aze et al. 2011 ecogroup 2 - Open ocean mixed-layer tropical/subtropical, without symbionts. Based on _13C lighter than species with symbionts; also with relatively light _18O. Sources cited by Aze et al. 2011 (appendix S3): Wade & Pearson (2008)
Phylogenetic relations
specimens to become smaller and less inflated in the latest Eocene (cf. the C. lazzarii concept). [Coxall & Pearson 2006]
Most likely ancestor: Hantkenina nanggulanensis - at confidence level 4 (out of 5). Data source: Coxall & Pearson (2006), fig 8.1.
Geological Range:
Notes: Upper Eocene. Upper Zone E14 to the Eocene/Oligocene boundary. [Coxall & Pearson 2006]
Last occurrence (top): at top of E16 zone (100% up, 33.9Ma, in Priabonian stage). Data source: Coxall & Pearson (2006), fig. 8.1
First occurrence (base): in upper part of E14 zone (80% up, 36.3Ma, in Priabonian stage). Data source: Coxall & Pearson (2006), fig. 8.1
Plot of occurrence data:
Primary source for this page: Coxall & Pearson 2006 - Eocene Atlas, chap. 8, p. 226
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Cribrohantkenina inflata compiled by the pforams@mikrotax project team viewed: 20-9-2024
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