◄ Carnets Geol. 24 (7) ►
Outline:
[1. Introduction]
[2. Material and methods]
[3. The original description ...]
[4. Comparison with other assemblages of microspheres]
[5. Systematics]
[6. Conclusion]
[Bibliographic references] and ...
[Plate]
2 impasse Charles Martel, F-29217 Plougonvelin (France)
D pt. STU, Fac. Sci. Tech., UBO, 6 avenue Le Gorgeu, CS 93837, F-29238 Brest (France)
Published online in final form (pdf) on May 8, 2024
DOI
10.2110/carnets.2024.2407
[Editors:
Mikhail Rogov, Michel Moullade; language editor: Phil Salvador; technical editor: Bruno Granier]
In the literature, numerous accounts exist of microspheres scattered in the pelagic environments of the Tethys realm at the Jurassic-Cretaceous transition. These microspheres are commonly associated with genera such as Cadosina, Colomisphaera, or Stomiosphaera, and attributed to calcareous dinocysts. On the other hand, there are few records of the microsphere, initially described as Cadosina minuta Borza, 1980, which are arranged in small clusters, likely comprising six cells. This distinctive grouping and its architecture preclude attribution to the calcareous dinocysts. A new genus and a new species (as Octahedronoides tethysianus n.gen., n.sp.) are introduced to define these clusters of leiospheres, which are here reascribed to the acritarchs.
calcispheres;
leiospheres;
dinocysts;
acritarchs;
Berriasian
Granier B.R.C. (2024).- Octahedronoides tethysianus n.gen., n.sp., enigmatic clusters of microspheres at the Jurassic-Cretaceous transition.- Carnets Geol., Madrid, vol. 24, no. 7, p. 127-133.
Octahedronoides tethysianus n.gen., n.sp., des amas nigmatiques de microsph res la transition Jurassique-Cr tac .- Dans la litt rature, on trouve de nombreuses r f rences des microsph res dispers es dans les environnements p lagiques du domaine t thysien la transition Jurassique-Cr tac . Ces microsph res sont commun ment associ es des genres tels que Cadosina, Colomisphaera ou Stomiosphaera, et attribu es aux dinocystes calcaires. Toutefois, il est peu fait mention de microsph res, initialement d crites comme Cadosina minuta Borza, 1980, qui sont dispos es en petits amas, probablement constitu s de six cellules. Ce type distinctif de regroupement et son architecture singuli re excluent leur attribution aux dinocystes calcaires. Un nouveau genre (Octahedronoides n.gen.) et une nouvelle esp ce (Octahedronoides tethysianus n.gen., n.sp.) sont introduits pour d finir ces agr gats de l iosph res, qui sont ici r attribu s aux acritarches.
calcisph res ;
l iosph res ;
dinokystes ;
acritarches ;
Berriasien
During the revision of the
geology of Busot (Alicante, Spain: Granier et al.,
1995, nearing
completion; Ferr & Granier,
2000), numerous calcispheres
were found in thin sections alongside late Berriasian calpionellids. Amongst the
smallest microspheres, some identified as Cadosina minuta Borza,
1980, are commonly found in clusters (Pl. 1 
,
figs. A-BI). Borza
(1980) described this species as having an "unilocular spherical
shell" 28 to 32 m in diameter "with a thin micritic wall"
(translated from the original German diagnosis: "Geh use einkammerig,
kugelf rmig, Gehausewand d nn, von Mikrit-Kalzit gebildet"). He also noted
"that the specimens mostly occur in clusters and only rarely
occur individually" (translated from the original German description: "Es
ist auff llig dass
die Exemplare zumeist in Gruppen auftreten und nur
selten einzeln vorkommen"), which is not the case in our thin sections,
where one counts more solitary occurrences than combined duos, triplets, and
quartets. According to Pszcz łkowski and Myczyński
(2004), the "Status of Cadosina minuta Borza is not clear, as
these microfossils differ from the typical representatives of the genus Cadosina
(Wanner, 1940), by their thin and indistinct test wall in many specimens
and common occurrence in groups composed of 2-6 specimens". The author
fully supports this last opinion because most of these grouped arrangements
cannot be accidental. In any case, there are compelling reasons to investigate
these so-called cadosinas, supposedly representing calcareous dinoflagellate
cysts.
All photomicrographs were taken using a digital MU900 AmScope camera mounted on a Leitz Diaplan microscope. The material analyzed below comes from the author's collection, which is now fully registered in the collections of the 'Mus um d'Histoire naturelle de Gen ve' (Switzerland). There his thin sections are ascribed the following registration numbers: MHNG-GEPI-2024-10032: Busot (East) 1994 no. 2, MHNG-GEPI-2024-10060: Busot (Calvario) 1993 no. D (BR2660), MHNG-GEPI-2024-10065: Busot (Calvario) 2010 no. 4H (BR2759)[*], MHNG-GEPI-2024-10069: Busot (Calvario) 2010 no. 8 (BR2763), and MHNG-GEPI-2024-1007069: Busot (Calvario) 2010 no. 9 (BR2764).
Wanner (1940) regarded Cadosina, his new genus, with Cadosina fusca his new species, as an unilocular foraminifer. He describes them as "single-chambered foraminifera with spherical or ovoid shell of porcelain-like structure. Shell provided with a true aperture. Calcareous substance of the shell appears opaque, milky white under ordinary transmitted light, and in cross-polarized light without axial cross" (translated from the original German "Diagnose": "Einkammerige Foraminiferen mit kugeligem oder ovoidem Geh use von porzellanartiger Struktur. Geh use mit einer echten M ndung versehen. Die Kalksubstanz des Geh uses im gew hnlichen auffallenden Lichte opak, milchwei , im durchfallenden polarisierten Lichte bei gekreuzten Nicols ohne Achsenkreuz"). Later most authors will regard all cadosinas as calcareous dinocysts (e.g., Reh kov & Michalik, 1996; Lakova et al., 1999; Ivanova & Keupp, 1999; Reh kov , 2000a, 2000b).
Borza (1980) gave the following description of Cadosina minuta, his new species: "Unilocular shell, spherical or sometimes slightly oval, formed by microcrystalline calcite. In transmitted light, it is dark, rarely faintly brownish, sometimes difficult to distinguish from the micritic matrix. In reflected light, it is milky white. No opening has been observed. The shell is filled with sparite. It is noticeable that the specimens mostly occur in groups and only rarely occur individually" (translated from the original German "Beschreibung: Geh use einkammerig, kugelf rmig, manchmal schwach oval, von Mikrit-Kalzit gebildet. In Durchlicht ist sie dunkel, selten schwachbr unlich, manchmal schwer von der mikritischen Grundmasse unterscheidbar. In Auflicht ist sie milchig-weiss. Eine M ndung ist nicht beobachtet worden. Die Kammer ist von kristallischen Kalzit ausgef llt. Es ist auff llig dass die Exemplare zumeist in Gruppen auftreten und nur selten cinzeln vorkommen.").
From the above description, a few points deserve a clarification:
1)
According to Borza (1980), "In transmitted light", the
shell "is dark, rarely faintly brownish, sometimes difficult to distinguish
from the micritic matrix" (translated from the original German description)
with a "2-3 m thickness of the wall"
(translated
from the original German "Abmessungen": "Dicke der Wand
2-3 m "). Considering the thickness of the petrographic slide on the thin
section, which averages around 20 m, and considering the larger dimension of
the spheres, which never exceeds 30 m, the microsphere outlines are blurred.
Consequently, it is not possible to provide a reasonable estimate of the wall
thickness.
Therefore, it is suggested here that the wall mostly consists of a thin organic
lining and that the microcrystals on both sides of it do not necessarily
represent a shell. Subsequently, individual spheres should not be considered as
cadosinas, i.e., calcispheres, but as leiospheres.
2)
Contrary to Borza (1980), who never observed any opening, a single
section out of many studied from Busot material (Pl. 1 ,
fig. A) shows what
appears to be an unusual appendix open at its tip in a two-dimensional view.
This structure or break in the wall could be related to an excystment phase.
3)
As already mentioned by Borza (1980), "the specimens mostly
occur in groups and only rarely occur individually" (translated from the original German description).
However, scattered specimens
are quite common. Pszcz łkowski and Myczyński
(2004) also reported the peculiar nature of these "groups composed of 2-6
specimens" of representatives of Cadosina (Wanner,
1940).
Actually, groups of
microspheres appear in decreasing order of abundance as pairs (abundant),
triplets (common), and quartets (rare). In contrast, groups with higher number
of microspheres appear somewhat disorganized, as if they were composed of
distinct clusters. Accordingly, it is suggested here that the most likely
geometrical assemblage is
6 microspheres set in an octahedron (Fig. 1 ). As a matter of
fact, this
structure, with 12 edges, 8 faces, 2 axial planes and one equatorial plane best
corresponds to the counting results of pairs (edges), triplets (faces), and
quartets (planes).
|
|
Figure 1:
Possible arrangement of the microspheres as an octahedron. |
4) Just as 'a bicycle wheel or a pair of them is not a bicycle' and vice versa, a structured assemblage made up of several microspheres should not be identified by the name of a single microsphere, i.e., as a Cadosina sp. For this reason, a new genus is introduced here to name these peculiar assemblages.
5) The holotype of Cadosina minuta Borza, 1980, does not fit in the definition of the new genus. Therefore, a discrete holotype is selected from the Spanish material, and a new species is introduced here as well.
Clusters of microspheres found in Busot can be compared with:
a) Groups of cysts, i.e., pluricysts, of the Dasycladales, e.g., Terquemella, Frederica, etc. (see the review in Maksoud et al., 2021), including Russoella Barattolo, 1983, with its few cystic cavities. It is worth remembering that Dasycladales are marine benthic algae;
b) Polysphaera camerounensis Lambert & Villain, 1996, an incertae sedis tentatively ascribed to the Calcisphaerulidae sensu Villain or Thoracosphaeraceae, a family of the Class Dinophyceae. This phytoplanktonic option is more consistent with a pelagic setting at Busot. However, there are very few colonial Dinoflagellates, among which Gymnodinium catenatum H.W. Graham, 1943, which forms long-chained colonies rather than small packed clusters. Unlike the aforementioned taxa, the Busot microspheres are not embedded in a common 'shell';
c) Modern green algae of the family Scenedesmaceae Oltmanns, 1904, consist of colonies, also known as coenobia, where each one acts as a single organism. They exhibit various architectures with a variable number of cells embedded in the same mucilage. For instance, the number of cells is 4 in Tetrastrum R. Chodat, 1895, commonly 4 or 8 in Scenedesmus Meyen, 1829, and 4, 8, 16, 32, or 64 in Coelastrum N geli, 1849, and Hariotina P.-A. Dangeard, 1889. These numbers are part of geometric progressions starting from 4 and with common ratio of 2. They do not fit with the clusters of 6 cells characteristic of the Busot microfossils. Finally, very few fossil records of representatives of this family have been documented (e.g., Scenedesmus sp. by Fleming, 1989, in uppermost Cretaceous non-marine sediments).
c) Acritarchs are predominantly known from the Precambrian; there are fewer records from the Paleozoic (e.g., Cambrian in Kov ř et al., 2023, or Harvey, 2023), the Mesozoic (e.g., Jurassic in Sarjeant, 1976; Cretaceous in Habib & Knapp, 1982, or Schrank, 2003), or the Cenozoic (e.g., Oligocene in Fechner, 1996). Palynological preparations from the Middle Cambrian of the Czech Republic (Kov ř et al., 2023) yield five acritarch genera, namely Adara (Fombella, 1977), Cymatiosphaera Wetzel, 1933, Eliasum Fombella, 1977, Synsphaeridium Eisenack, 1965, and Timofeevia Vanguestaine, 1978, which have been found to form monogeneric clusters. Because these clusters consist of a highly variable number of specimens, ranging from two to more than 100 hystrichospheres, they differ markedly in size and organization. They may appear as "massive, densely packed accumulations", "specimens arranged in 'filament-like' rows", or "clusters of loosely aggregated specimens"; no common pattern of organization was observed. Similarly, palynological preparations from the Lower Cambrian of the Canada have been found to yield "strut-form" (...), "ring-form (Kahfia-like)" (...), and "plate-form (including Tapetisphaerites-like) colonies" (Harvey, 2023). However, even though it is the best option in terms of structural convergence, none of these arrangements match with those of the clusters of microspheres observed in Busot thin sections. Today, additional rock samples are required to implement palynological investigative techniques. The Busot microspheres are not concatenated. They are not in direct contact with each other either, but commonly leave a space of approximately half a microsphere diameter. However, there likely existed strong, albeit invisible, links between them. It is presumed that these leiospheres were originally encased in a non-fossilized substance, likely a mucilage, which kept them together during the early stages of fossilization.
Group: Acritarcha Evitt, 1963
Genus: Octahedronoides n.gen.
Etymology: From the supposed architecture of a cluster of six new microspheres.
Type species: Octahedronoides tethysianus n.gen., n.sp.
Diagnosis: Loose but orderly arranged (in rhombohedral- or tetragonal-sphenoidal manner) colonies of a few leiospheres, never arranged in filaments, nor in struts, rings, or plates.
Species: Octahedronoides tethysianus n.gen., n.sp.
(Pl. 1 ,
figs. C-BI)
Synonymy:
? 1980 Cadosina minuta n.sp., Borza, p. 263-264, Pl. (Taf.) I, figs. 1-4 [holotype: Pl. (Taf.) 1, fig. 1]
1980 Cadosina minuta n.sp., Borza, p. 263-264, Pl. (Taf.) I, figs. 5-12
1992 Cadosina minuta, Bucur, Fig. 2.h
1994 Cadosina minuta, Va icek et al., Pl. 8, fig. 4
1999 Cadosina minuta, Lakova et al., Pl. III, fig. 16
2000a Cadosina minuta, Reh kov , Pl. II, fig. 15
2000b Cadosina minuta, Reh kov , Pl. IV, fig. 8
2003 Cadosina minuta, Pszcz łkowski, Fig. 13.9-10
2004 "Cadosina" minuta, Pszcz łkowski & Myczyński, p. 152, Fig. 8.8
2007 Cadosina minuta, Lukeneder & Reh kov , Fig. 6.F
2011 Cadosina minuta, Reh kov , Pl. 9, fig. 18
2017 Cadosina minuta, Ivanova & Kietzmann, Fig. 7.21-24
2020 Cadosina minuta, Petrova, Fig. 5.w-y
Etymology: The new specific epiteth refers to the Tethys Ocean (with the superfluous qualifier tethysianus), not to the goddess Tethys (with the qualifier tethyanus, see discussion in Granier, 2022).
Locality: Busot, Alicante, Spain (Granier et al., 1995, nearing completion; Ferr & Granier, 2000).
Paleoenvironmental setting: The microfacies of the thin sections correspond to bioclastic wackestones, slightly silty (quartz), with a mixture of hemipelagic and reworked shallow-water material. They indicate sedimentation occurring on a paleoslope, i.e., on the transitional zone between the Prebetic platform and the Subbetic basin.
Holotype: The quartet in Plate 1 , fig. AG, MHNG-GEPI-2024-10065: Busot (Calvario)
2010 no. 4H (BR2759).
Additional studied material
(paratypes): Plate 1 ,
figs. C, H-X, Z-AD, AF, AH-BI, MHNG-GEPI-2024-10065: Busot
(Calvario) 2010 no. 4H (BR2759).
Stratigraphic horizon: Calpionellopsis Zone (zone D), upper Berriasian; lower part of the "Minuta zone", upper Berriasian-lower Valanginian.
Diagnosis: Aggregates
of at least two spherical to ovoid unilocular microspheres
with a diameter rarely exceeding 30 m, commonly 25 m. In
thin sections, microspheres appear in decreasing order of abundance as pairs (abundant),
triplets (common), and quartets (rare). Accordingly, it is suggested here
that the most likely geometrical assemblage is 6
microspheres set in an octahedron (Fig. 1 ), i.e., a structure
exhibiting 12 edges, 8 faces, 2 axial planes, and one equatorial plane. The
largest dimension of a colony may reach 80 m.
Stratigraphic range: The species is known from the lower Berriasian Elliptica Subzone of the Calpionella Zone (Borza, 1980; Michal k et al., 1990; Řeh nek, 1992) to the lower Valanginian Calpionellites Zone (Borza, 1980; Reh kov , 2000a, 2000b). Řeh nek (1992) created a 'Minuta zone' based on its total range whereas Reh kov (2000a) introduced a 'Minuta acme zone' that should be restricted to the upper part of the lower Valanginian. Considering the observed abundance of this microfossil in sample MHNG-GEPI-2024-10065: Busot (Calvario) 2010 no. 4H (BR2759), dated as late Berriasian by calpionellid biostratigraphy, it is suggested to abandon the acme zone and only refer to the newly renamed 'Tethysianus zone', a total range zone (instead of the former 'Minuta zone').
Octahedronoides tethysianus n.gen., n.sp., are planktonic organisms forming small colonies, a feature which excludes their ascription to the calcareous dinocysts, but justifies their transfer to the acritarchs. More rock samples should be collected because palynological techniques of investigation need to be implemented to definitively validate the reascription of these assemblages of organic-walled microspheres.
The two last field campaigns in SE Spain (in September 2010 and April 2024) were made possible thanks to a grant from the Association 'Carnets de G ologie'. The author would like to acknowledge the various contributions from several colleagues, namely the late Roque Aguado Merlo (1961-2023), Jos Miguel Andreu Rodes, Mohamed Benzaggagh, Joachim Blau, Eric B ker, the late Robert Busnardo (1926 2018), the late Bernard Clavel (1938-2018), Antonio Est vez Rubio, Bruno Ferr , Bernard C. Lambert, Eric Monteil, St phane Reboulet, Emmanuel Robert, and Aur lien Virgone for their contribution to a better understanding the stratigraphy in the Busot village, Alicante (Spain). The author is grateful to Daria K. Ivanova (Sofia), Joachim Blau (Frankfurt am Main), Malcolm Hart (Plymouth), and Tom Harvey (Leicester) for their comments, which helped improve the manuscript. Thanks are also due to Phil Salvador who kindly checked the final version of the English text.
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Plate
1:
? Cadosina minuta Borza, 1980
(A-B), and Octahedronoides
tethysianus n.gen., n.sp. (C-BI). Most photomicrographs are from thin section
MHNG-GEPI-2024-10065:
Busot (Calvario) 2010 no. 4H (BR2759), except for: a) figs. D,
F, Y from thin section Busot (Calvario) 2010, no. 8; b) fig. E from thin
section Busot (East) 1994, no. 2; c) fig. G from thin section Busot (Calvario)
1993, no. D60; and d) fig. AE from thin section Busot (Calvario) 2010,
no. 9. Scale bar (on fig. J)
= 100 m. |
|
[*] Microspheres are particularly abundant in this sample.
