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Late Cretaceous ammonites from the Bou Angueur syncline (Middle ...

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1841 Ammonites catillus SowERBY - n'ORBIGNY, p. 325; Plate 97, figs. 1-2.<br />

1850 Ammonites Geslinianus n'ORBIGNY - n'ORBIGNY, p. 146.<br />

1962 Metoicoceras geslinianum (n'ORBIGNY) - }EFFERIES, Plate 77, fig. 19.<br />

1998b Metoicoceras geslinianum (n'ORBIGNY) - LEHMANN, p. 28; Plate 3, fig. 3 (and synonymy).<br />

1999 Metoicoceras geslinianum (n'ORBIGNY) - LEHMANN, Plate 4, fig. 3.<br />

2004 Metoicoceras geslinianum (n'ORBIGNY) - BARROSO-BARCENILA, p. 96; Plate 1, fig. 5 a-c; Plate 2, fig. 1.<br />

2005 Metoicoceras geslinianum (n'ORBIGNY) - GALE, KENNEDY, VorGT & WALASZCZYK, text-fig. 9F & G; text-fig. 12C.<br />

2005 Metoicoceras geslinianum (n'ORBIGNY) - MEISTER & ABDALLAH, p. 128; Plate 8, fig. 1 (and synonymy).<br />

Material: GSUB C2558<br />

Description: The present specimen shows a compressed whorl section, with faint ribs, outer<br />

ventrolateral clavi and inner ventrolateral bullae. Its early whorls (wh 30 mm) occasionally bears umbilical bullae.<br />

Discussion: This species is very variable in morphology; for a full systematic account see WRIGHT &<br />

KENNEDY (1981), KENNEDY (1988) and KENNEDY & }UIGNET (1994b). A multivariate analysis based on coiling,<br />

dimensions and ornament, has been applied by REYMENT & KENNEDY (2000) to check <strong>the</strong> traditional taxonomy.<br />

This indicates that quantitative procedures reproduce traditional methods to a conspicuous degree, with <strong>the</strong> added<br />

advantage of objective repeatability. Fur<strong>the</strong>rmore, doubtful phylogenetic relationships have been resolved and<br />

new information on dimorphism has been obtained.<br />

0 cc u r re n c e: Metoicoceras geslinianum is <strong>the</strong> index fossil of <strong>the</strong> middle late Cenomanian M. geslinianum Zone. There are records<br />

<strong>from</strong> <strong>the</strong> United States, Mexico, Brazil, Colombia, Morocco, Nigeria, Angola, Spain, France, Germany, and England (e. g. LEHMANN 1998b)<br />

as well as <strong>from</strong> Tunisia (MEISTER & ABDALLAH 2005).<br />

Genus Spathites KuMMEL & DECKER, 1954<br />

Subgenus Spathites Ueanrogericeras) WIEDMANN, 1960<br />

Spathites Ueanrogericeras) reveliereanus (CouRTILLER 1860)<br />

(Plate 1, figs. C-E)<br />

1860 Ammonites revelieranus - CouRTILLER, p. 249; Plate 2, figs. 5-8.<br />

1980 Spathites Ueanrogericeras) reveliereanus (CouRTILLER) - KENNEDY et al., p. 826; Plate 105, figs. 1-12; Plate 106, figs. 1-2; text-figs. 3-<br />

6 (and synonymy).<br />

2007 Spathites Ueanrogericeras) reveliereanus (CouRTILLER) - BARROSO-BARCENILLA, p. 138; Plate 4, fig. g; Plate 5, figs. a-d; text-figs. 6ab<br />

(and synonymy)<br />

Material: GSUB C2556<br />

Description: GSUB C2556 is a phragmocone with a maximum diameter of about 110 mm. There are<br />

very strong umbilical bullae that give rise to very feeble flat folds on <strong>the</strong> flank and inner and outer ventrolateral<br />

clavi. On <strong>the</strong> intitial part of <strong>the</strong> ultimate whorl, <strong>the</strong> outer ventrolateral clavi are as big as <strong>the</strong> inner ventrolateral<br />

clavi, however, <strong>the</strong> outer ones quickly become larger and are about as big as <strong>the</strong> umbilical bullae at <strong>the</strong> end of <strong>the</strong><br />

ultimate whorl. There are 12 inner ventrolateral clavi, but only 8 umbilical bullae. On <strong>the</strong> venter a depression<br />

forms a discontinous ridge. The ventrolateral shoulder is well-rounded. The coiling is involute, <strong>the</strong> umbilicus<br />

small (about 20% of <strong>the</strong> diameterf).<br />

Discussion: GSUB C2556 falls into <strong>the</strong> broad variation of Spathites Ueanrogericeras) reveliereanus<br />

(CouRTILLER 1860), <strong>the</strong> sulcate venter is characteristic (KENNEDY et al. 1980; RoBASZYNSKI et al. 1982; WIESE<br />

1997). GSUB C2556 shows continuously strong inner ventrolateral clavi at a diameter of around 100 mm,<br />

corresponding to that figured by THOMEL (1992: Plate 118, figs. 3-4; Plate 119, fig. 1) and RoMAN (1912: Plate 1,<br />

fig. 1 & la).<br />

GSUB C2556 resembles equally sized representatives of <strong>the</strong> probable successor of Spathites, Mammites<br />

nodosoides (ScHLUTER 1871), in its tuberculation, but differs by <strong>the</strong> depression on <strong>the</strong> venter, a feature also<br />

occurring in Spathites (S.) chispaensis KuMMEL & DECKER , 1954. Spathites (S.) chispaensis differs <strong>from</strong> our material<br />

by an almost angular ventrolateral shoulder as well as <strong>the</strong> lack of ornament at this growth stage, typical for <strong>the</strong><br />

subgenus Spathites. In contrast to <strong>the</strong> present material, <strong>the</strong> ventral ridge is much more prominent and deeper in<br />

Spathites (S.) rioensis PowELL, 1963, and Spathites (S.) puercoensis (HERRICK & ]oHNSON 1900) also <strong>from</strong> North<br />

America that are, additionally, more closely tuberculated and stronger ornamented than GSUB C2556 (CoBBAN<br />

& HooK 1979; HooK & CoBBAN 1982; CoBBAN 1988; KENNEDY & CoBBAN 1988).

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