Symmetrosulcus dockeryi, Lin & Nolf & Steurbaut, 2022
publication ID |
https://doi.org/ 10.5852/ejt.2022.814.1745 |
publication LSID |
lsid:zoobank.org:pub:74226488-DE8B-4A64-B1D4-A24C15AE79F6 |
DOI |
https://doi.org/10.5281/zenodo.7035278 |
persistent identifier |
https://treatment.plazi.org/id/124FFDA6-FA7C-442E-AC9E-88BE08F77445 |
taxon LSID |
lsid:zoobank.org:act:124FFDA6-FA7C-442E-AC9E-88BE08F77445 |
treatment provided by |
Felipe |
scientific name |
Symmetrosulcus dockeryi |
status |
sp. nov. |
Symmetrosulcus dockeryi sp. nov.
urn:lsid:zoobank.org:act:124FFDA6-FA7C-442E-AC9E-88BE08F77445
Fig. 18G–K View Fig
Diagnosis
OL/OH = 1.47–1.57, OsL/CaL = 1.43–1.73. Elliptic otoliths with angled posterior rim. Ventral rim deepest in the middle. Sulcus wide, oblong, but narrow. Ostium longer than cauda, each filled with a colliculum.
Etymology
The species is named in honor of David T. Dockery III (Mississippi Bureau of Geology) who provided major support during our field work.
Material examined
Holotype UNITED STATES OF AMERICA • Left otolith; Texas, Wall Farm 1; Weches Formation ; Fig. 18G View Fig ; IRSNB P 10090 .
Paratypes UNITED STATES OF AMERICA • 191 otoliths of which four are figured: Fig. 18H–K View Fig ; same collection data as for holotpye; IRSNB P 10091–10094 .
Type locality and horizon
United States of America, Wall Farm 1 (Texas), Weches Formation.
Dimensions of the holotype
Length = 3.16 mm; height = 2.11 mm; thickness = 0.93 mm.
Description
This species is characterized by elliptical otoliths with blunt, but well-marked antero- and postero-dorsal angles. The rim between those two angles is almost horizontal, but may be very slightly undulated in the smaller individuals ( Fig. 18I View Fig ). The posterior portion of the otoliths forms a tapering triangle. The ventral rim is smoothly curved with its deepest part in the middle of the otolith, providing it a regular rounded appearance. The anterior part of the otolith is slightly oblique and largely blunt at its lower, most prominent part. All the margins are smooth. The otoliths are moderately thick, with both the inner and outer faces convex. The thickness may be slightly more considerable near the posterior end, which is the case in the holotype ( Fig. 18G View Fig ). A straight sulcus occupies nearly the entire length of the inner face and is located in the central zone, but does not open to the margins of the otolith. There is a clear division into ostial and caudal parts, each fully filled by a colliculum. The cauda is about twice as long as the ostium. The cristae are clearly marked, but not ridge-like. They are almost horizontal, but the crista inferior may be slightly constricted at the collum, which is well visible in the holotype ( Fig. 18G View Fig ).
Comparison
The otoliths of this species can be distinguished from the co-occurring related species, S. meyeri ( Koken, 1888) , S. stintoni (Dante & Frizzell, 1965) , “ N. ” rotundus ( Müller, 1999), and “ N. ” virginicus Müller, 1999, by the combination of the following features: a more rectangular outline, a nearly flat dorsal rim, a more vertical anterior rim, a less extended posterior rim, and a dorsal area of similar width as the ventral one. See below for a detailed discussion on other ophidiid otoliths.
Stratigraphic and geographic distribution
Lutetian: Weches Formation, Texas; “lower” Lisbon Formation, Alabama. Bartonian: Cook Mountain Formation, Mississippi.
No known copyright restrictions apply. See Agosti, D., Egloff, W., 2009. Taxonomic information exchange and copyright: the Plazi approach. BMC Research Notes 2009, 2:53 for further explanation.