Created 2023/04/26
Updated 2024/10/12

Hoplites (Hoplites) paronai  Spath, 1925

profile
venter
section
Hoplites (Hoplites) paronai  CP-217
Measurements D mm H/D T/D O/D H/T
CP-709 figured 55.3 0.47 0.540.260.88
CP-217 69.3 0.43 0.520.290.83
Holotype 73 0.43 0.570.320.75
Age Origin
Dentatus nodule bed (bed 1)
Lower Gault, Middle Albian
Folkestone
Kent, England
Var.dentatusspathiparonai
H/T 1.21-1.32 0.92-1.02 0.67-0.83
T/D 0.32-0.40 0.49 0.52-0.70

Description. Read the entry for Hoplites (Hoplites) dentatus first. This ammonite, in black phosphate with one side not prepared, is completely septate and displays whorls that overlap by 50%, with a thick, depressed hexagonal section. The umbilicus is deep. Its raised wall, sloping at 70°, transitions to the flank via a rounded margin. Thirteen radial primary ribs originate from this wall and rise to form, shortly after the umbilical margin, very tall, radially pinched tubercles. Pairs of forward-curving ribs arise from these tubercles. The moderately raised terminations of ribs reach a 45° angle to the siphonal line. They alternate on each side and define a deep and straight groove with a flared U-shaped section.

Remarks. The last table lists, in increasing thickness, the Hoplites species with U-shaped sulcus from the lower dentatus zone, based on the specimens from Spath (1925). They are currently considered variants of H. dentatus, which has anteriority (Amédro, 1992; Courville & Lebrun, 2010; Amédro et al., 2014). Our specimen corresponds to Hoplites (Hoplites) paronai, the thickest and least frequent variant. It generally displays a wider umbilicus than the other variants. The reader can see two other specimens: one on www.ammonites.org and one in Jaffré (2007, p. 79). Our ammonite has ribs that project further forward, and their ventral terminations begin to rise on the last half-whorl.