Eckhartiopsis parva E.M.FRIIS, P.R.CRANE et K.R.PEDERSEN, 2019
publication ID |
https://doi.org/ 10.2478/if-2019-0013 |
persistent identifier |
https://treatment.plazi.org/id/0396DC10-BF31-C23D-CD8D-B351E3001A30 |
treatment provided by |
Diego |
scientific name |
Eckhartiopsis parva E.M.FRIIS, P.R.CRANE et K.R.PEDERSEN |
status |
sp. nov. |
Eckhartiopsis parva E.M.FRIIS, P.R.CRANE et K.R.PEDERSEN sp. nov.
Text-fig. 40a–h View Text-fig
H o l o t y p e. Designated here. S170217 (Torres Vedras sample 39; figured Text-fig. 40a–h View Text-fig ).
P l a n t F o s s i l N a m e s R e g i s t r y N u m b e r.
PFN000476 (for new species).
R e p o s i t o r y. Palaeobotanical Collections , Department of Palaeobiology, the Swedish Museum of Natural History, Stockholm, Sweden .
E t y m o l o g y. From Latin: parvus for small referring to small size of the pollen grains.
T y p e l o c a l i t y. Torres Vedras (NE of Forte de
Forca; 39°06′13″ N, 9°14′47″ W).
T y p e s t r a t u m a n d a g e. Lower member of the Almargem Formation; Early Cretaceous (late Barremianearly Aptian).
D i a g n o s i s. As for the genus.
D i s t i n g u i s h i n g f e a t u r e s. Eckhartiopsis parva is distinguished from Eckhartia as represented in the Torres Vedras mesofossil flora ( Eckhartia brevicolumella , Eckhartia longicolumella , Eckhartia sp. ) by the broader anthers and the heteropolarity of the reticulum, in which the reticulum on the proximal surface is coarser than the reticulum on distal surface. Pollen grains of Eckhartiopsis also lack the distinct psilate region at the ends of the colpi that is characteristic of Eckhartia pollen. Nevertheless, Eckhartia and Eckhartiopsis have similar tooth-shaped orbicules and it is possible that they are systematically closely related.
D i m e n s i o n s. Length of anthers: about 0.53 mm; width of anthers: 0.25 mm. Length of pollen grains: 14– 15 µm.
D e s c r i p t i o n a n d r e m a r k s.Thespeciesisbased on a single well-preserved anther. The anther is dithecate and tetrasporangiate, about 0.53 mm long and 0.25 mm wide ( Text-fig. 40a View Text-fig ).
Pollen grains are about 14–15 µm in equatorial diameter and monocolpate. The exine is semitectate-reticulate, heterobrochate and columellate ( Text-fig. 40b–g View Text-fig ). The reticulum is coarser on the proximal face than on the distal face ( Text-fig. 40c–e View Text-fig ). Larger lumina on the proximal face are up to about 1.5 µm in diameter ( Text-fig. 40c View Text-fig ). Lumina on the distal face are smaller, and only slightly smaller along the colpus margin ( Text-fig. 40e, f View Text-fig ). Muri are about 0.2 µm wide with a rounded or flattened profile. Columellae are long, about 0.5 µm tall and typically widely spaced (Textfig. 40c, h). The foot layer is about 0.4 µm thick ( Text-fig. 40h View Text-fig ). The endexine is granular, apparently very restricted, and developed only under the aperture ( Text-fig. 40h View Text-fig ). The reticulum loosens easily from the foot layer sometimes leaving the main body of the grain naked ( Text-fig. 40g View Text-fig ). Orbicules are densely scattered on the inner surface of the anther wall and over the surface of the pollen grains (Textfig. 40b, e). They are tooth-like with pointed protrusions.
A f f i n i t y a n d o t h e r o c c u r r e n c e s. Eckhartiopsis parva is currently not known from any other mesofossil flora in Portugal.
R |
Departamento de Geologia, Universidad de Chile |
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