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Cerithium jekeliusi
Taxonomy
Cerithium jekeliusi was named by Svagrovsky (1971) [DISTRIBUTION: Middle Miocene; Paratethys.]. It is not a trace fossil.
Sister species lacking formal opinion data
C. abbassi, C. abictiforme, C. alternatum, C. angyostoma, C. armoricense, C. austriacum, C. binodulasum, C. boulei, C. bronni, C. calcivelatum, C. caloosaensis, C. dubium, C. georgianum, C. gonzagae, C. guinacium, C. heeri, C. hernandoensis, C. isidis, C. krauskopfi, C. leei, C. libycum, C. manzourensis, C. mazureki, C. mogharens, C. obsoletum, C. pachecoi, C. percostatum, C. periphractum, C. pirabicum, C. praecursor, C. roedereri, C. septemplicatum, C. simpsonense, C. struckmanii, C. vertagus, C. kobunense, C. cyprinum, C. kavasiense, C. koroniense, C. gilyandense
Synonymy list
Year | Name and author |
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1971 | Cerithium jekeliusi Svagrovsky |
2002 | Cerithium jekeliusi Harzhauser and Kowalke p. 70 |
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If no rank is listed, the taxon is considered an unranked clade in modern classifications. Ranks may be repeated or presented in the wrong order because authors working on different parts of the classification may disagree about how to rank taxa.
†Cerithium jekeliusi Svagrovsky 1971
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Diagnosis
Reference | Diagnosis | |
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M. Harzhauser and T. Kowalke 2002 | The stout, medium-sized, juvenile shell consists of six flattened whorls and measures 1.8 mm in height and 1 mm in width. A fragment of an adult shell indicates a size of up to 10 mm in height and 6 mm in width of fully grown specimens. The protoconch comprises two rounded whorls, which appear to be smooth. It measures 0.2 mm in height and 0.23 mm in maximum dimneter. The first whorl measures 0.05-0,06 mm in the width of the initial cap and 0.15-0.16 mm in maximum diameter. The transition to the teleoconch is indicated by a strong sinusigera notch, which extends over 0.12 mm. The sinusigera is thickened in its adapical portion and thin and broken off in its abapical portion. The teleoconch whorls are characterised by two rows of widely spaced nodes close to the sutures. These nodes are the blunt terminations of very weak axial ribs. The surface is covered by fine spiral grooves. |