Eckhartia brevicolumella 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-BF36-C23A-CDF9-B7C8E3F91F35 |
treatment provided by |
Diego |
scientific name |
Eckhartia brevicolumella E.M.FRIIS, P.R.CRANE et K.R.PEDERSEN |
status |
sp. nov. |
Eckhartia brevicolumella E.M.FRIIS, P.R.CRANE et K.R.PEDERSEN sp. nov.
Text-fig. 37a–g View Text-fig
H o l o t y p e. Designated here. S136760 (Torres Vedras sample 44; figured Text-fig. 37c, g 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.
PFN000472 (for new species).
P a r a t y p e s. Designated here. S136661, S136662, S136751, S136752, S136673, S136765, S137920, S137921, S148021, S149204 (Torres Vedras sample 44).
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: brevis for short and columella referring to short columellae supporting the muri.
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 with the following additions: Anthers elongate. Reticulum coarse. Columellae short, densely spaced or sometimes laterally merged.
D i s t i n g u i s h i n g f e a t u r e s. Eckhartia brevicolumella is distinct from E. longicolumella (below) mainly in having much longer stamens, pollen grains with larger and fewer lumina and shorter, more densely spaced columellae. The coarse reticulum of the pollen grains also distinguishes Eckhartia brevicolumella from E. intermedia (below) although these two taxa both have similar short and densely spaced columellae.
D i m e n s i o n s. Length of anthers: about 1.2 mm; width of anthers: 0.12–0.16 mm. Length of pollen grains: 16–17 µm.
D e s c r i p t i o n a n d r e m a r k s. Eckhartia brevicolumella is based on many isolated stamens with pollen grains in situ. It was first illustrated by Friis et al. (2010a), but not formally described and named. The anthers are very long and narrow, about 1.2 mm long and 0.12–0.16 mm wide, dithecate and tetrasporangiate ( Text-fig. 37a, b View Text-fig ). The anther wall is usually well preserved and pollen grains are only visible in cracks or fragmented specimens. Pollen grains are about 16–17 µm in equatorial diameter and monocolpate. The exine is semitectate-reticulate, heterobrochate and columellate ( Text-fig. 37c, d, f, g View Text-fig ). The reticulum over most of the pollen grain is coarse with lumina of two sizes, with the larger lumina up to about 1.8 µm in diameter (Textfig. 37g). Towards the colpus margin, and especially around the end of the colpus, the lumina become very small and the colpus margin is psilate ( Text-fig. 37f, g View Text-fig ). Muri are about 0.2 µm wide with rounded or flattened profiles. Columellae are short, about 0.2 µm long, usually densely spaced, and sometimes fused into a short plates ( Text-fig. 37g View Text-fig ). Orbicules are densely spaced on the inner surface of the anther wall ( Text-fig. 37e View Text-fig ) and scattered over the surface of the pollen grains ( Text-fig. 37g View Text-fig ). They are about 1.8 µm long, irregular in shape with a solid rounded base bearing densely spaced rod-like protrusions that give the individual orbicules the appearance of a tooth with crown and roots (Textfig. 37e, g).
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.Thepollen grains show similarities to grains adhering to the stigmatic surface of Vedresia elliptica ( Text-fig. 49c View Text-fig ) and they may have been produced by the same kind of plant. Eckhartia brevicolumella has so far not been observed in any other mesofossil flora from Portugal.
R |
Departamento de Geologia, Universidad de Chile |
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