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Home All issues Volume 191 (2020) BSGF - Earth Sci. Bull., 191 (2020) 39 Full HTML
Special Issue L'Ambre
BSGF - Earth Sci. Bull.
https://doi.org/10.1051/bsgf/2020039
2 Material and methods
3 Plant remains ...
4 Amber characteristics
BSGF - Earth Sciences Bulletin 2020, 191, 39
Amber- and plant-bearing deposits from the Cenomanian of Neau (Mayenne, France)
Le site à ambre et plantes du Cénomanien de Neau (Mayenne, France)
Didier Néraudeau1*, Jean-Paul Saint Martin2, Simona Saint Martin2, Laurent Jeanneau1, Jean-David Moreau3, Marc Philippe4, France Polette1,5, Damien Gendry1, John Brunet6 and Jérôme Tréguier7
1 Université de Rennes, UMR 6118, Géosciences Rennes, Campus de Beaulieu, avenue du Général Leclerc, 35042 Rennes, France
2 Centre de Recherche en Paléontologie − Paris, UMR 7207, Muséum national d'Histoire naturelle, Sorbonne Université, CNRS, 8, rue Buffon, 75005 Paris, France
3 Université de Bourgogne Franche-Comté, UMR 6282, Biogéosciences, 6, boulevard Gabriel, 21000 Dijon, France
4 Université de Lyon I and LEHNA, UMR 5023, 69622 Villeurbanne, France
5 Department of Geology, University of Namur, ILEE, Institute of Life, Earth and Environment, 61, rue de Bruxelles, 5000 Namur, Belgium
6 5, rue de Bellevue, 35220 Marpiré, France
7 Musée des Sciences, 21, rue du Douanier Rousseau, 53000 Laval, France
* Corresponding author: didier.neraudeau@univ-rennes1.fr
A new Cenomanian amber- and plant-bearing deposit has been discovered at Neau, in the Mayenne department (France). The Cenomanian fossiliferous lignites are located in karst filling in a substratum of Cambrian limestones. The amber corresponds mainly to tiny millimetric grains, devoid of arthropod inclusions, but rich in microorganisms, especially the sheated bacteria Leptotrichites resinatus, and containing pollen grains (Classopollis) and wood fibers (Araucariacae or Cheirolepidiaceae). The lignites provide abundant conifer and ginkgoale cuticle fragments (Frenelopsis, Eretmophyllum) and a lot of palynomorphs (e.g. Gleicheniidites senonicus, Cyathidites, Deltoidospora, Appendicisporites and Cicatricosisporites). The chemical signature of the amber suggests it was produced by conifers of the extinct family Cheirolepidiaceae. According to the palynological assemblage, the age of the lignites is upper lower Cenomanian or lower mid Cenomanian. The deposit environment corresponded to the upstream portion of a mangrove or the most inner part of a lagoon.
Un nouveau site à ambre et plantes du Cénomanien a été découvert à Neau, en Mayenne (France). Les lignites fossilifères cénomaniens sont localisés dans des remplissages de karsts développés dans des calcaires du Cambrien. L'ambre se présente essentiellement sous forme de grains millimétriques, dépouvus d'inclusions d'arthropode, mais riches en microorganismes, notamment en bactéries gainées de type Leptotrichites resinatus, et contenant des grains de pollen (Classopollis) et des fibres de bois (Araucariacae ou Cheirolepidiaceae). Les lignites fournissent d'abondants fragments de cuticules de conifères et de ginkgoales (Frenelopsis, Eretmophyllum) et une grande quantité de palynomorphes (e.g. Gleicheniidites senonicus, Cyathidites, Deltoidospora, Appendicisporites et Cicatricosisporites). La signature chimique de l'ambre suggère qu'il a été produit par des conifères de la famille éteinte des Cheirolépidiacées. D'après l'assemblage palynologique, l'âge des lignites est Cénomanien inférieur tardif ou Cénomanien moyen basal. L'environnement de dépôt correspondait à la partie amont d'une mangrove ou la partie la plus interne d'un lagon.
Key words: Palynology / Gymnosperm cuticles / Cheirolepidiaceae / Sheated bacteria / Amber / Cenomanian / France
Mots clés : Palynologie / Cuticules de gymnospermes / Cheirolepidiaceae / Bactéries gainées / Ambre / Cénomanien / France
© D. Néraudeau et al., Published by EDP Sciences 2020
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Late Cretaceous amber deposits are well distributed in western France, from the Anjou and Sarthe regions, at the North, (Ecommoy locality in Girard et al., 2013a, 2013b; Hucheloup locality in Fleury et al., 2017) to the Aude department, at the South (Fourtou locality in Girard et al., 2013a, 2013b; see Moreau et al., 2017, for a synthetic map of mid-Cretaceous french amber deposits). The more numerous amber deposits and the more rich in amber are located in the Charentes region, where Cenomanian sands and clays with lignite have been studied in several quarries, road works and coastal outcrops (Néraudeau et al., 2002, 2003, 2005, 2008). Conversely, amber from Mayenne has been the less studied. The only previous works were made by Durand and Louail (1971) about the discovery of a karst filling of fossiliferous Cenomanian lignites and sands in a substratum of Cambrian limestones at Neau, and by Azema et al. (1972) who performed a palynological analysis of the sediment. The latter study described lower to mid Cenomanian assemblages dominated by gymnosperm pollen grains and fern spores, and marked by the progressive increase of angiospermous forms. Finally, the rare mentions of Cenomanian amber at Neau have been provided by Durand and Louail (1971), and the few available data were then cited by other authors, such as Girard et al. (2013a, 2013b). We present here the first synthesis dedicated to the Cenomanian amber from Neau and its associated botanical macro-, meso- and microremains, along with palaeoenvironmental and stratigraphic considerations.
2.1 Field observations
The Neau quarry is located at about 30 km NW from Laval in the department of Mayenne, NW France (Fig. 1). The quarry is exploited by the Society Chaux & Dolomie Françaises/Lhoist France Ouest for the extraction of Cambrian dolomitic limestones and the production of lime.
At the top of the Cambrian limestones, several dissolution cavities are filled by Cenomanian erosive deposits (Figs. 2 and 3). According to the field observations made by the authors, the base of the karsts corresponds generally to a few metres of lignitic sand and clay (CnL facies on Figs. 2A and 3) including large pieces of fossil wood (trunk and branches fragments). The top of the karst filling consists of one to two metres of white sand (CnS facies on Figs. 2A and 3A–B), more or less oxidized and coloured in yellow at the contact with the lignite. Both Cambrian limestone palaeoreliefs and karsts are covered by discordant glauconitic sands (CnG facies on Figs. 2A and 3A–B) including more or less kaolinitic lenses. The base of lignitic deposits contains pyritised foraminifers that testify the coastal marine origin of these sediments (Durand and Louail, 1971). The marine remains disappear at the top of the Cenomanian sandy deposits. The presence of kaolinite indicates a typical lateritic weathering anterior to the Cenomanian (Durand and Louail, 1971). One sample of lignitic clay has been collected at the top of the facies CnL in the main karst (Fig. 3A–B), for palynological analyses. In addition, seven samples recovered from Neau amber-rich lignitic clay in 1972, and 39 corresponding palynological slides prepared and analyzed by Azema et al. (1972) were re-examined to complete our palynological analyses and to compare our biostratigraphical and palaeobotanical conclusions (samples S2, S3, S4, S7, S9, S11, S12 on Fig. 2B).
The amber can be collected by sieving of the lignites, but can also be sometimes collected on the outcrop surface after washout by the rain. The lignites and amber studied in this paper were collected during a field trip organized on June 4th 2014 by the Museum of Laval (J. Tréguier) and the University of Rennes I (D. Néraudeau), completed by additional collections made by John Brunet and D. Gendry.
Simplified geological map of the Neau area, in the Mayenne department, with location of the studied quarry.
Geological sections of the Cenomanian karsts from the Neau quarry. A. Synthetic section of the karsts with lignite and amber, observed by the authors (Cmb = Cambrian limestones; CnL = Cenomanian lignites; CnS = Cenomanian sand; CnG = Cenomanian Glauconitic facies). B. Geological section published by Azema et al. (1972), with location of their palynological samples S1 to S12.
Lignite and amber deposits from the Neau quarry. A. General view showing the Cenomanian lignites (CnL) in karsts incising the Cambrian limestones (Cmb); at the top of the quarry, Cenomanian glauconitic sands overlap both Cenomanian white sands (CnS) and Cambrian limestones. B. One Cenomanian karst showing at its top the contact between the lignites containing amber (CnL) and the glauconitic sands (CnG); the bag of the collector contains a large piece of fossil wood. C. Lateral view of a Cenomanian karst with the lignites (CnL) directly in erosive contact with the Cambrian limestones (Cmb) (photographs D. Néraudeau).
2.2 Amber, wood and cuticle preparation (Fig. 4)
Tiny amber grains have been collected by sieving of the lignitic clay, and then separated from wood and cuticle fragments (Fig. 4A). The lignitic marl was soaked in a solution of hydrogen peroxide (12%) and water for a few days. The disaggregated sediment was then washed with tap water through a column of sieves (2.0 mm, 1.0 mm and 0.5 mm meshes). The pieces of ambers as well as fossil plants (Fig. 4B–H) were picked out by naked eye or under a stereomicroscope Leica 125. Photographs were taken with a BMS digital USB camera (5 megapixels). Specimens are housed in the collections of the University of Rennes 1 under numbers IGR-PAL-2828 and IGR-PAL-22829 for the wood fragments and IGR-PAL-2830 to IGR-PAL-2836 and IGR-PAL-2844/IGR-PAL-2845 for the plant cuticles. An amber lot is housed under number IGR-PAL-2843. Amber slides used to illustrate the amber inclusions correspond to numbers IGR-PAL-2837 to IGR-PAL-2842. The amber grain containing wood fragments studied in the paper corresponds to number IGR-PAL-2846.
In the lignitic clay, plant remains are greatly disarticulated and vary in size including meso- to macro-remains (Fig. 4B–H). They consist of leafy axes (Fig. 4B–E) and cone scales of conifers (Fig. 4F) as well as fragmented leaves of ginkgophytes (Fig. 4G, H). Wood fragments are also abundant (Fig. 4A). The collection includes hundreds of plant specimens. They are preserved as coalified compressions with or without cuticles. Some plant microremains (pollen, woods) were also found as inclusions inside amber.
In order to characterize the amber grains, thin sections were prepared with a thickness slightly greater than the standard thickness of the petrographic thin section. The optical microscope used is a Zeiss Axioscope 40 with photographing device and observations were made with ×5 and ×10 objectives for large observation. The observations under confocal laser scanning microscope (CLSM) were essentially performed on a Leica TCS SP5 microscope. The images obtained allow viewing of the autofluorescent objects in false colours. 3D reconstruction was obtained by acquisition of stacks of closely spaced confocal optical sections at 0.10 μm to 0.20 µm intervals. Then these images were treated for optimization with the open source software Image J (Rasband, 1997–2013). Amber and wood examinations with Scanning Electron Microscope (SEM) were performed with the Hitachi SU3500 model.
In addition to the micro-fragments of wood found by sieving of the lignitic clay (Fig. 4A), several large pieces of trunk and branches have been collected during the field trip at the surface of the outcrop (Fig. 3B).
A. Amber, cuticle and wood remains extracted after soaking of sediment in a solution of hydrogen peroxide. B–E. Leafy axes of the conifer Frenelopsis sp. showing the characteristic tree short parts of the leaves (located by arrows), IGR-PAL-2830 to IGR-PAL-2833. F. Conifer cone scale IGR-PAL-2834. G–H. Fragments of leaves ascribed to Eretmophyllum obtusum showing the characteristic bifid veins (located by arrows), IGR-PAL-2835 and IGR-PAL-2836. Scale bars: A = 1 cm; B–D and G–H = 5 mm; E = 1 mm; F = 2 mm.
2.3 Amber analyses
Two pieces of Neau amber, an opaque and milky denoted form A and a translucent and orange denoted form B and a yellowish Baltic amber as reference were analyzed by thermally assisted hydrolysis and methylation (THM) also called thermochemolysis. Small portions of amber were crushed manually in an agate mortar. The powders (∼0.1 mg) were heated with TMAH (Tetramethylammonium Hydroxyde) at 400°C. THM was carried out using a Frontier Lab PY-2020iD pyrolyser coupled with a Shimadzu GCMS-QP2010 Plus system operating with a split ratio of 100. Separation was achieved using a capillary column SLB-5MS (60 m × 0.25 mm ID, 0.25 μm film thickness) with the carrier gas He with a flow of 1.1 mL/min. The operating conditions were as follows: initial temperature held at 50 °C for 2 minutes, increased to 310 °C at a rate of 4 °C/min for 34 minutes. Individual compounds were identified based on comparison of (i) MS data with the NIST2014 library and literature (Anderson, 1994, 1996, 2006; Dutta et al., 2011; Otto and Simoneit, 2002) and (ii) retention time with the reference Baltic amber.
The relative distribution of identified compounds was determined by measuring the area of a specific fragment, denoted m/z integration in Table 1. The peak area of the selected m/z for each compound was integrated and corrected by a mass spectra factor (Tab. 1) calculated as the reciprocal of the proportion of the fragment used for the integration and the entire fragmentogram. The molecular ratios were calculated using those corrected areas that allow an approximation of areas on the total ion chromatogram while preventing from the integration of co-eluting compounds.
List of identified compounds and their relative proportions in Neau ambers. Target compounds were identified based on m/z int and m/z identification. Areas were integrated using the m/z int, and the area on the total ion chromatogram was estimated using the mass spectra factor (MSF). Non-detected compounds are denoted "n.d.".
2.4 Palynomorphs
Seven samples were recovered from Neau amber-rich lignitic clay in 1972, and 39 corresponding palynological slides were prepared and analyzed by Azema et al. (1972; S2, S3, S4, S7, S9, S11, S12, see Fig. 2B). Because their study focused on several Cenomanian localities of western France, Azema et al. (1972) chose not to discuss extensively the palaeoenvironmental implications and the age attribution of the palynological assemblages of Neau. The palynomorphs illustrated are not accompanied by coordinates, and one cannot know which pollen grain or spore comes from Neau or from another locality. Thus, in order to determine more precisely the palaeoenvironmental and stratigraphic modalities associated with the formation/deposit of Neau resin − and later amber −, those 39 slides were re-examined, and the corresponding results are presented herein.
Several slides now correspond to partly dried residue, rendering observations difficult, but all seven samples yielded palynological assemblages, however often small. If the sample and corresponding slides were not particularly rich, all palynomorphs were counted and identified, as it is the case for S2 (N = 132), S7 (N = 27), S9 (N = 23), S11 (N = 135), and S12 (N = 106). The two remaining samples S3 and S4 provided rich assemblages. Three hundred palynomorphs were counted and identified, but all the palynomorphs were observed in order to log potential infrequent forms (Appendix S1). The 39 slides are housed in the collections of the University of Rennes 1 under numbers Cd1 to Cd39.
3 Plant remains from the lignitic clay
3.1 Coalified compressions and cuticles from the lignitic clay
Family Cheirolepidiaceae
Genus Frenelopsis Schenk, 1869 emend. J. Watson,1976
Frenelopsis sp.
(Fig. 4B–E)
Material. Forty-three specimens, from which IGR-PAL-2830 to IGR-PAL-2833 are figured.
Description. The material consists of isolated internodes constituting the leafy axes (Fig. 4B-D). The internodes are never connected. They are elongated, flattened, up to 13.0 mm long, and up to 3.5 mm wide. Each internode is formed by one whorl of three proximally fused leaves. Free parts of the leaves are only visible distally (Fig. 4B–E). They form three tiny tips which are triangular in shape, broader than long, up to 1.0 mm long, and up to 2.5 mm wide and show an obtuse apex (Fig. 4E). Surface of internodes shows numerous longitudinal rows of stomata.
Remarks. Cellular characters of the stomata are not preserved. Frenelopsis is one of the most abundant conifers from the Cenomanian deposits of Western France. This taxon was reported from many areas in Aude, Charente-Maritime, Vienne and Maine-et-Loire (see synthesis in Moreau et al., 2017 and references therein).
Family Incertae sedis
Cone scale Type 1
(Fig. 4F)
Material. One specimen, IGR-PAL-2834.
Description. The scale is longer than wide (i.e., 4.5 mm long and 3 mm wide), convex, shows an acuminate base, a broad truncate apex and an entire margin (Fig. 4F). The base displays a long free stalk (2.5 mm long and up to 1.5 mm wide). The adaxial surface displays several central and proximal grooves. They end before the truncate apex.
Remarks. The preservation is not sufficient to unambiguously identify the presence of ovule scars. Some isolated ovulate cone scales were previously reported from the lower Cenomanian of western France, in Charente-Maritime (e.g., Néraudeau et al., 2009). They were tentatively ascribed to Alvinia bohemica (Velen.) J. Kvaček. However, the shape of the cone scale from Mayenne differs from these specimens.
Family Karkeniaceae
Genus Eretmophyllum
Eretmophyllum obtusum (Velen.) J. Kvaček (1999)
(Fig. 4G–H and Fig. 5A–J)
Material. Sixteen specimens, from which IGR-PAL-2835 and IGR-PAL-2836 are figured.
Description. The material consists of up to 20 mm long and up to 11 mm wide fragmented lamina (Fig. 4G–H). The leaves are coriaceous and entire-margined. The apices are obtuse. Base of leaves and petiole are not preserved. The veins are dichotomously branched and run subparallel to leaf lamina and converge near the apex (Fig. 4G–H). The dichotomies form narrow angles. In the medial part, lamina display up to 12 parallel veins. The veins are up to 0.3 mm wide and are regularly spaced. Cuticle is heavily cutinized. Cuticle displays costal and intercostal bands, both bearing stomata apparatuses. Leaves are amphistomatic. Stomata are randomly oriented, scattered, and particularly abundant in intercostal bands (Fig. 5A). Stomata are haplocheilic, sunken and surrounded by 4 to 6 subsidiary cells (Fig. 5C–F). The diameter of stomatal apparatuses varies from 40 to 70 µm. The stomatal pits show a round or oval shape. Ordinary epidermal cells are square, rectangular, or polygonal, 20–110 µm long and form longitudinal rows. The anticlinal walls of ordinary epidermal cells are straight to slightly sinuous (Fig. 5B). Numerous rounded and spindle-shaped resin bodies are dispersed in the mesophyll (Fig. 5G). Rounded ones are up to 0.5 mm in diameter whereas spindle-shaped ones are up to 1.1 mm long (Fig. 5H–J).
Remarks. Pons et al. (1976) erected the species Eretmophyllum andegavense D.Pons, Boureau et Broutin based on material from the Cenomanian of Angers (western France). However, the distinction of Eretmophyllum (Velen.) J.Kvaček with Nehvizdya Hluštík is debated for a long time. Kvaček (1999) transfered Nehvizdya to the genus Eretmophyllum, and introduced a new combination, Eretmophyllum obtusum (Velen.) J. Kvaček. However, Gomez et al. (2000) attempted to distinguish Eretmophyllum from Nehvizdya on the basis of the presence or absence of papillae on subsidiary cells as the differential character. Gomez et al. (2000) tentatively transferred the species Eretmophyllum andegavense in the genus Nehvizdya. However, as pointed by Kvaček et al. (2005) the differential character used by Gomez et al. (2000) is not acceptable being variable among genera in the Ginkgoales. Here, we follow Kvaček et al. (2005) who suggested that Nehvizdya and Eretmophyllum cannot be splitted only based on the "papillae" argument. Although several studies (Gomez et al., 2004, 2008; Néraudeau et al., 2005) reported Nehvizdya andegavense from the Albian-Cenomanian of several localities in Charente-Maritime, we agree with Fleury et al. (2017) who used Eretmophyllum rather than Nehvizdya for material from the Cenomanian of western France (Maine et Loire).
Eretmophyllum obtusum. A–B. Details of cuticle showing the arrangement of cells, and the random orientation of stomatal apparatuses (white arrows), IGR-PAL-2844. C–F. Sketches of stomatal apparatuses showing arrangement of subsidiary cells. G. Arrangement of resin bodies (white arrows) preserved in the mesophyll between veins IGR-PAL-2845. H–J. Rounded and spindle-shaped resin bodies. Scale bars: A and H–J = 500 µm; B = 200 µm; C–F = 100 µm; G = 2 mm.
3.2 Palynomorphs from the lignitic clay
The seven palynological samples yielded a fairly diverse palynoflora composed of 71 species and ca. 1000 specimens (Appendix S1). Abundance charts of the five richest samples show that the proportion between spores (Fig. 6C–L) and pollen grains (Fig. 6M–Z) is well balanced, but spores are often slightly dominant (Fig. 6A). They usually represent around 60% of the assemblage, but can go up to 92% for S4. Most abundant spores correspond to Gleicheniidites senonicus (Gleicheniaceae), to smooth walled forms associated with the genera Cyathidites and Deltoidospora, and to massive cicatricose spores of Appendicisporites and Cicatricosisporites (Anemiaceae; Fig. 6A, E–J). Appendicisporites insignis (Fig. 6I–J) is the most common form of ornamented spores. Among subsidiary spores are those of the Lycophytes, mostly belonging to Camarozonosporites (Fig. 6D), a few bryophitic forms (Fig. 6C), spores associated with the Osmundaceae, such as Baculatisporites (Fig. 6K), and spores of uncertain botanical affinities, like Patellasporites tavaredensis (Fig. 6L) and Microreticulatisporites sacalii.
Gymnosperm pollen grains (Fig. 6M–O) are dominated by Circumpolles (Classopollis torosus) and small inaperturate or monoaperturate grains associated with the Cupressaceae (incl. Taxodiaceae), including Exesipollenites tumulus, Inaperturopollenites dubius, and Taxodiaceaepollenites hiatus (Fig. 6A). On the contrary, bisaccates (mostly Pinaceae/Podocarpaceae, Fig. 6M) and grains of Araucariaceae (Araucariacites, Fig. 6N) were rarely encountered, and seldom represent more than 5% of the assemblages, except for the youngest assemblage (Fig. 6A).
While the different groups of spores and gymnosperms pollen grains display a fairly fluctuant abundance throughout the five assemblages, S11 and S12 are marked by the sudden increase of angiosperm pollen grains (Fig. 6A). They represent from 3–5% of S2–S4 to 12–15% of S11–S12. Numerous representatives of Dichastopollenites were observed (uncertain affinity), as well as tricolpate (Tricolpites, Fig. 6V), tricolporate (Nyssapollenites, Fig. 6U), and tricolpoidate (Phimopollenites, Fig. 6X–Z) forms belonging to the Eudicots. Grains of Phimopollenites were particularly diversified and abundant. Less common forms include Stellatopllis cf. largissimus (Fig. 6S) and Artiopollis indivisus (Fig. 6T). No normapolles were observed. Very few dinocysts were logged in the oldest assemblages, mostly belonging to Surculosphaeridium longifurcatum (Fig. 6B). Except for the progessive increase of the abundance of the angiosperm pollen grains, and the curious abundance peak of Glecheiniidites in S4, no particular trend is noticed from S2 to S12, and the resulting interpretation will therefore consider the "Neau palynoflora" as a whole.
A. Abundance charts of the most productive palynological assemblages from the amber-rich lignitic clays of Neau. Charts are based on the botanical affinities of the various spores and pollen morphotypes. Encountered genera: 1: Aequitriradites, Stereisporites, Triporoletes; 2: Camarozonosporites, Densoisporites, Retitriletes; 3: Gleicheniidites, Ornamentifera; 4: Cyathidites, Deltoidospora, Dictyophyllidites, Matonisporites, Toroisporis; 5: Appendicisporites, Cicatricosisporites, Distaltriangulisporites; 6: Auritulinasporites, Baculatisporites, Concavissimisporites, Laevigatosporites, Microreticulatisporites, Patellasporites, Todisporites; 7: Parvisaccites, Piceaepollenites, Podocarpidites, Pristinuspollenites; 8: Araucariacites, Balmeiopsis, Callialasporites; 9: Classopollis; 10: Exesipollenites, Inaperturopollenites, Perinopollenites, Taxodiaceaepollenites; 11: Alisporites, Afropollis, Cycadopites, Eucommiidites, Monosulcites; 12: Clavatipollenites, Dichastopollenites, Pennipollis, Retimonocolpites, Stellatopollis, Transitoripollis; 13: Artiopollis, Nyssapollenites, Phimopollenites, Retitrescolpites, Tricolpites. Species list, counts and references are available on Appendix S1. B–Z. Dinocysts, spores and pollen grains recovered from Neau lignitic clays. Accompanying data are palynological preparation and England Finder coordinates. Scale bars represent 10 μm. B. Surculosphaeridium longifurcatum (Firtion) Davey et al., S3-Cd9, N30.4. C. Triporoletes cenomanianus (Agasie) Srivastava, S11-Cd28, R45.4. D. Camarozonosporites insignis Norris, S4-Cd16, J31.4. E. Cicatricosisporites cf. mohrioides Delcourt and Sprumont, S11-Cd31, P36.0. F. Cicatricosisporites annulatus Archangelsky and Gamerro, S3-Cd9, F29.2. G, H. Appendicisporites bilateralis Singh, S3-Cd7, K41.0. I, J. Appendicisporites insignis (Markova) Chlonova, S4-Cd11, J46.1. K. Baculatisporites sp., S3-Cd8, R48.1. L. Patellasporites tavaredensis Groot and Groot, S11-Cd28, J42.0. M. Podocarpidites biformis Rouse, S3-Cd6, M32.3. N. Araucariacites australis Cookson ex Cooper, S11-Cd31, L47.1. O. Eucommiidites minor Groot and Penny, S11-Cd29, P45.0. P. Transitoripollis anulisulcatus Góczán and Juhász, S3-Cd6, M31.0. Q. Dichastopollenites reticulatus May, S4-Cd14, S46.4. R. Dichastopollenites sp. 4 sensu Heimhofer et al. (2007), S11-Cd29, B40.0. S. Stellatopollis cf. largissimus Singh, S4-Cd16, K48.0. T. Artiopollis indivisus Agasie, S4-Cd16, K52.1. U. Nyssapollenites albertensis Singh, S3-Cd8, R48.3. V. Tricolpites cf. vulgaris (Pierce) Srivastava, S3-Cd7, H48.4. W. Tricolpites aff. virgeus (Groot, Penny and Groot) Hasenboehler, S11-Cd28, F35.0. X. Phimopollenites tectatus Singh, S3-Cd7, K47.1. Y. Phimopollenites megistus Singh, S4-Cd16, M33.1. Z. Phimopollenites cf. pannosus (Dettmann and Playford) Dettmann, S11-Cd33, L37.4.
4.1 General aspect (Figs. 7 and 8)
The collected amber grains are of variable appearance and size. Large pieces of amber are very uncommon and have been collected at the surface of the outcrop. They range from 1 to 3 cm in size. Three varieties of colour have been observed: milky brown (Fig. 7A), translucent honey (Fig. 7B) and opaque cork colour (Fig. 7C–D). A few ones are empty (Fig. 7D). The size of tiny amber grains collected by clay sieving varies generally from a few millimetres to one centimetre (Fig. 8A). Then, the appearance of the grains depends on the shape of the original resin drops or their posterior fragmentation, during transport or the conditions of deposit and sampling. Thus, the best preserved grains correspond to fine, more or less cylindrical flows or rather spherical drops with an attachment point. Others result from a more complex flow and show several protuberances. If some grains appear translucent with a dominant orange-yellow colour, very many grains are wholly or partly opaque with earthy or cork colours of beige to brown (Figs. 4A and 8A). The opacity is very irregularly distributed according to the grains appearance (Fig. 8B–E) corresponding to several phenomena: presence of bubbles and/or emulsions more or less coarse, colonization by filamentous microorganisms (Fig. 8H) or a conjugation of both (Fig. 8B, I). The external appearance revealed by the SEM observations shows that cracks are often present on the surface of the amber grains (Fig. 8F). In some cases the superposition of resin flows is clearly visible (Fig. 8G).
Large amber pieces from the Neau quarry. A. Milky brown variety. B. Translucent honey variety. C. Cork colour variety. D. Empty piece of cork colour variety; note the black colouring of the peripheral part, linked to the proliferation of the sheated bacteria Leptotrichites resinatus. Scale bar = 10 mm.
Amber features. A. Forms and aspects of the collected amber grains, some having kept the characteristics of the original resin drops; note the abundance of opaque grains with earthy colours. B–E. Sections of grains in thin sections showing various situations of more or less opaque grains. F. Cracked external surface of a grain under SEM. G. Stack of resin flows within a grain. H. Opaque grains marked by dense filamentous networks. I. Opaque grain containing many bubbles and colonization by filamentous networks.
4.2 Plant microremains included inside amber
4.2.1 Vegetal fibers and wood (Fig. 9)
The size of the large pieces of wood collected on the outcrop varies from several centimetres to about 1 m, and numerous ones show Teredo-borings typical for coastal marine environments in transgressive settings (Gingras et al., 2004), and tiny borings of unknown origin (Teredo, insect attacks?) (Fig. 9A, B). SEM observations of the wood fragments included in the amber evidenced pitting on the radial tracheid walls, preserved as pit chamber inner casts (Fig. 9C, D). While some up to 9 pits long row of contiguous pits occurred (Fig. 9D), locally pit rows seems to be interrupted (Fig. 9C). The regularity of the spacing between the preserved pits, however, argues more for non-preservation than for absence of pits. Consequently the tracheid radial pitting was interpreted as araucarian. The cross-fields are of the araucarioid type, with 5 to 7 contiguous alternate cupressoid oculipores (Fig. 9E). The fragmentary material did not allow to study growth-ring features, nor the occurrence or resin canals or axial parenchyma. According to these limited morphological observations, the most probable taxa are (from the most probable to the least one) (1) Agathoxylon; (2) Brachyoxylon; (3) Ginkgoxylon. The fact that these wood pieces are included in the amber could indicate that the resin producers were Araucariacae or Cheirolepidiaceae. These are indeed the only wood genera yet reported from the Mesozoic and combining araucarioid cross-fields and at least partly araucarian radial tracheid pitting (Philippe and Bamford, 2008).
All these three genera are known to produce resin inside their tracheids (Philippe, 1995), and the three of them were reported from the Cenomanian of Western France (Perrichot, 2005). The first and xylologically most probable one, Agathoxylon, was reported associated to all ambers with the same provenance. Despite its etymology genus Agathoxylon is not necessarily a univocal evidence of the Araucariaceae. After this has been suspected several times, it has recently been shown that Agathoxylon wood can also occur in Cheirolepidiaceae (Steart et al., submitted). Brachyoxylon is usually considered as related to the Cheirolepidiaceae (Macchour and Pons, 1995) and Ginkgoxylon to the Ginkgoalean (Jiang et al., 2016). Here in Neau, according to the non-woody remains all the three taxa occur (i.e. Araucariaceae, Cheirolepidiaceae and Ginkgoalean). The amber-embedded fragment of wood therefore does not make it possible to specify the taxonomic origin of this amber.
Optical (A–B) and SEM (C–F) photographs of wood fragments. A. Large piece of fossil wood showing large Teredo borings on the left and numerous tiny borings (insect attacks?) on the right, IGR-PAL-2828. B. Piece of branch showing tiny borings IGR-PAL-2829. C. Areolated pit inner casts; note that tori left a circular depression in the centre of the casts (magnification × 1700). D. Araucarian row of uniseriate contiguous radial pits (magnification × 1300). E. Five araucarioid cross-fields, with poorly preserved contiguous alternate cupressoid oculipores (magnification × 1600). F. An isolated areolated pit (foreground) and an araucarioid cross-field (background) (magnification × 3500). SEM observations have been made on specimen IGR-PAL-2846. Scale bar for A and B: 10 mm.
4.2.2 Pollen grains included in amber (Fig. 10)
Examination of some thin sections revealed the presence of gymnosperm pollen grains belonging to the genus Classopollis, which is associated with the extinct family of the Cheirolepidiaceae (Balme, 1995; Schrank, 2010; Fig. 10). They are often arranged in clusters (Fig. 10A–B, F), but isolated grains were also observed (Fig. 10C–D). Their rimula is discrete, but discernable. Azema et al. (1972) found numerous Classopollis grains within the lignitic clay of Neau, that they all identified as a new species called Classopollis tenuiparietalis. However, they state that C. tenuiparietalis is morphologically identical to the Aptian and Cenomanian Portuguese taxon Classopollis obidosensis Groot and Groot, creating this new form only to accommodate Cenomanian French pollen grains. Classopollis tenuiparietalis is thus considered invalid. As the morphological differences between C. obidosensis, C. classoides Pflug, and C. torosus (Reissinger), Couper are very tenuous, we consider them all synonymous of the first form described, Classopollis torosus (see diagnoses of Couper, 1958, pp. 156–157, and Groot and Groot, 1962, p. 161). This latter species is then adopted for the pollen grains from Neau amber.
Trapped palynomorphs have been mostly recovered from Eocene Baltic amber (Wetzel, 1953; Arnold, 1998; see Langenheim and Bartlett, 1971 for 1800s and early 1900s references). A few other studies on subsidiary Cenozoic amber bearing strata have also documented spores and pollen grains in Eocene amber from France (Breton et al., 1999; De Franceschi et al., 2000; Dejax et al., 2001), and Miocene amber from Peru and Mexico (Langenheim in Poinar, 1992, p. 78; Antoine et al., 2006). Mesozoic records are scarce, and concerns exclusively Cretaceous strata. Angiospermous pollen grains and spores were apparently recovered from Lower Cretaceous Lebanese amber, but neither precise reference nor illustrations are provided (Azar et al., 2010; Engel et al., 2011; Whalley in Poinar, 1992, p. 161). Several clusters of gymnosperm and angiosperm pollen grains were recovered from the Cenomanian Myanmar amber, always observed in association with various insects (Poinar, 2010; Cai et al., 2018; Grimaldi et al., 2019; Lin et al., 2019; Hinkelman and Vršanská, 2020). In Europe, Monsulcites grains were observed within late Albian amber from Spain (Peris et al., 2017). The Classopollis clusters described herein are the first pollen grains documented from Mezosoic French amber so far.
Palynomorphs inclusions in amber. A–F. Inclusions of Classopollis pollen grains in the Cenomanian amber of Neau (Mayenne). Generally pollen grains are grouped in vacuoles of the amber and can be numerous (A, B, E, F), IGR-PAL-2837 to IGR-PAL-2840. Only a few ones are isolated in the fossil resin (C, D), IGR-PAL-2841 and IGR-PAL-2842. Note the dense filamentous network due to the colonization of the resin by a sheathed bacterium (sb). A–D. Optical microscope. E–F. Confocal microscope (CLSM).
4.2.3 Microinclusions
The amber of Neau contains various inclusions of microorganisms (Saint Martin et al., under study) characterized by centripetal colonization of filamentous networks. They are essentially sheathed bacteria identifiable as Leptotrichites resinatus Schmidt 2005 whose colonization density in the initial resin results of the complete opacification of the amber grains (Figs. 7C, D, 8E, I, 10A–F), and often of black colouring of the peripheral parts of the amber drops, just below the crust surface (Fig. 7D). These microinclusions are very widespread in Cretaceous ambers (Schmidt and Schäfer, 2005; Saint Martin and Saint Martin, 2018). Smaller clumps of actinomycetes are also found to a lesser extent, located on the periphery of the amber grains.
4.2.4 Chemical characteristics
The total ion chromatograms of the THM-GC-MS analysis of the Neau resins are illustrated in Figure 11. The relative proportions of (i) the different categories of compounds and (ii) labdanoid diterpenes and compositional ratios are given in Table 2. The molecular fingerprint was composed of 66 molecules from three main families: (i) labdanoid diterpenes produced by the thermochemolysis of the A/B ring system of a polylabdanoid structure, (ii) methyl(hydro)naphthalene and methylphenanthrene and (iii) tricyclic diterpenes. Both pieces of ambers produced a different chemical fingerprint. Most of the compounds (80%) occurred in both fingerprints, but in different relative proportions.
Labdanoid diterpenes are the main chemical group in form A (64% of the analyzed compounds), while they only represent 20% of the analyzed compounds in form B (Tab. 2). The similarity of the retention times of the carboxylic acids compared with Baltic amber and the absence of dimethyl succinate classified these samples as Class Ib ambers. Labdanoid diterpens of form A are dominated by bicyclic acids (66%) with a large predominance of C15 over C14 (∑C14/∑C15 = 0.23). In form B, they are dominated by 1-methylbicyclic hydrocarbons (64% of labdanoid diterpens) with a slight predominance of C15 over C14 (SC14/SC15 = 0.88).
Methyl(hydro)naphthalene and methylphenanthrene are the main chemical group in form B (64% of analyzed compounds), while they represent 21% of the analyzed compounds in form A. This group included trimethylindene, ionene, methylionene and diagenetic products of sesqui- and diterpenoids. The distribution of these compounds is quite similar in both form with the predominance of 5 isomers of trimethylnaphthalene (38 and 36% in form A and B, respectively) and 2 isomers of dimethylnaphthalene (17 and 13% in form A and B, respectively). Amberene was detected in low amount in the program of form B and represented 0.5% of this chemical group.
The third chemical category was composed of tricyclic diterpenes. In form A, this group was dominated by methyl 16,17-dinordehydroabietate (23%), dimethylphenanthrene (19%) and methyl 8-abieten-18-oate (15%) with low occurrence of callitrisic acid derivatives. In form B, this group was dominated by dimethylphenanthrene (32%), methyl dehydroabietate (13%) and the isomers of trimethylphenanthrene (12%). Methyl callitrisate (5% and methyl 16,17-dinorcallitrisate (1%) were also detected.
Total ion chromatogram from the THM-GC-MS analysis of Neau amber form A (A) and form B (B). Numbered peaks refer to identified compounds in Table 1 and Appendix S2.
Relative proportions of the three categories of identified compounds and of labdanoid diterpenes. Compositional ratio calculated on the distribution of labdanoid diterpenes.
5.1 Singularity of the amber from Neau
The appearance of the Cenomanian amber of Neau is very similar to that of the amber grains generally collected in many Cretaceous French amber deposits of various ages. The same reduced size and the drop shape of the best preserved grains can be found in other Cenomanian French sites: e.g. Poitou (Valentin et al., this volume), Sarthe (Breton and Tostain, 2005; Breton, 2007; Girard et al., 2013a, 2013b). This feature is also common for the Turonian of Dordogne (Saint Martin et al., 2013a, 2013b; Néraudeau et al., 2016) and Aude (Breton et al., 2018), the Santonian of Provence (Saint Martin et al., 2012, 2013; Saint Martin and Saint Martin, 2018; Frau et al., this volume; Saint Martin et al., this volume), and the Campanian of Aude (Breton et al., 2013). On the other hand, they do not correspond to amber samples taken from the Albo-Cenomanian of Charente Maritime or the Upper Cretaceous from Vendée, where large nodules can be found (Néraudeau et al., 2008; Girard, 2010; Néraudeau et al., 2017).
Consequently, like in Dordogne, Poitou or Provence ambers, the very small size of the amber drops from Neau did not favour the preservation of arthropod inclusions as large amber drops from the Charentes and Vendée did. The only micro-inclusions that have been observed in the amber from Neau correspond to filamentous organisms such as sheathed bacteria and actinomycetes. But other micro-organisms, such as amoeba or diatoms seem to be lacking.
Conversely, palynological inclusions, which were never observed in French Cretaceous ambers, are well preserved in Neau amber (see Sect. 4.2.2). The lack of palynomorphs, known to be resistant to physical and chemical taphonomical processes, is difficult to explain for the other Cretaceous French ambers. Their presence in the Mayenne amber could be related to a season of resin flow more contemporaneous to the conifer pollination. Langenheim and Bartlett (1971) have noticed that the probability of finding pollen in amber can be increased when pollen was produced throughout the entire period of resin secretion. However, they also observed that several genera of palynomorphs were trapped throughout the year within resin, regardless of either time of pollination and period of resin production. As Cretaceous palynomorphs have been generally noticed when they are found in association with insects and plants (see Sect. 4.2.2), it could be possible that spores and pollen grains were trapped within other Cretaceous amber, but were not observed because they were not in the vicinity of larger fossils. However, the researches of Girard (2010), (2013, 2018) and Saint Martin et al. (2012, 2013a, 2013b) dedicated to the identification of every micro-inclusions in French Cretaceous ambers devoid of arthropod inclusions, have never observed pollen grains in these ambers, in spite of their diversity of geographical (centre-western, south-western or south-eastern France) and stratigraphical (Albian, Cenomanian, Turonian, Santonian, Campanian) origins. The case of Lebanese amber shows another original situation, the pollen grain species trapped in the Lower Cretaceous Hammana amber lacking in the palynological assemblage of the sediment containing the amber (Azar et al., 2010).
The chemical fingerprints of form A and B ambers composed of labdanoid diterpenes produced, methyl(hydro)naphthalene, methylphenanthrene and tricyclic diterpenes is typical of Cretaceous ambers (Anderson, 2006; Bray and Anderson, 2008; Menor-Salván et al., 2016; Nohra et al., 2015). Both chemical fingerprints shared 80% of the detected compounds and the 66 analyzed molecules fall in the three aforesaid chemical classes. Based on the higher proportion of methyl(hydro)naphthalene and methylphenanthrene (Clifford et al., 1995) and lower ∑C14/∑C15 (Clifford et al., 1999), the differences in the chemical fingerprints could be interpreted as a higher degree of maturation for form B than for form A. However both come from the same deposit, so the same diagenetic conditions could be assumed. Since 80% of the molecules are common to both fingerprints, a similar botanical precursor may be assumed. In such a situation, the differences between both fingerprints could be due to the initial composition of the resin that can present large seasonal and inter-specific variations (Langenheim, 2003) and/or from heterogeneities in the physic-chemical conditions of the deposit.
The chemical fingerprint of form A is characterized by (i) the predominance of labdanoid diterpenes with a predominance of bicyclic acids and (ii) the occurrence of tricyclic diterpenes coming from dehydroabietic and callitrisic acids with a predominance of dehydroabietic acid derivatives. It is similar to that described for the Cretaceous amber from the Raritan formation (Anderson, 2006) that has been assigned to the Cupressaceae. However the vegetal macrofossils from Neau are not from this family. Moreover the chemical fingerprint of the Cretaceous amber from Vendée (France) assigned to the Cupressaceae is characterized by a large predominance of callitrisic acid derivatives over dehydroabitic acid derivatives (Nohra et al., 2015).
Bisnorsimonellite also occurred in form A. The chemical fingerprint of this form A is similar to that described for the Charentese (France) Cretaceous amber (Nohra et al., 2015). The chemical fingerprint of the form B is characterized by the occurrence of traces of amberene and by a higher proportion of 16,17,18-trisnorabieta-8,11,13-triene versus 18-norabietatriene. It is similar to that described for the type 2 Cretaceous ambers from Spain (Menor-Salván et al., 2016). The extinct family Cheirolepidiaceae has been suggested as the potential producer of these ambers, which is in accordance with the vegetal macrofossils associated with the Neau ambers. Consequently Neau ambers may be assigned to the Cheirolepidiaceae.
The present data reinforce the chemical signature suggested for the ambers produced by the extinct family Cheirolepidiaceae. The combination of previous observations (Bray and Anderson, 2008; Menor-Salván et al., 2016; Nohra et al., 2015) and the present data suggests the following chemical fingerprint: (i) occurrence of labdanoid diterpenes, (ii) occurrence of tricyclic diterpenes coming from dehydroabietic and callitrisic acids with a predominance of dehydroabietic acid derivatives, (iii) a higher proportion of 16,17,18-trisnorabieta-8,11,13-triene versus 18-norabietatriene (Tab. 2), (iv) absence or occurrence in low proportion of amberene and (v) occurrence of ferruginol or its diagenetic products such as bisnorsimonellite.
5.2 Age of the lignitic clay(s)
Despite the revealing title of their study, Azema et al. (1972) did not consider all the palynological assemblages they observed to be mid-Cenomanian in age. This is the case of the palynoflora recovered from Neau, which they interpreted as lower to mid Cenomanian. They based their age attribution (1) on the presence of the same species of Classopollis in the clays of both Neau and Ecommoy, the latter being unequivocally mid-Cenomanian, and (2) on the absence of the form Lobelina, which would be indicative of an Albian age (Azema et al., 1972, p. 10). However, we consider herein that the specimens identified as Classopollis belong to the long-ranging form C. torosus (see Sect. 3.2). Moreover, the Circumpolle genus Lobelina created by Médus (1970) was later proven to be a nomen nudum (Jansonius and Hills, 1976), and is considered as a form of Classopollis. In any case, the use of Circumpolles to date Mesozoic deposits has not been proven satisfactory in spite of Médus efforts to produce a comprehensive morphologic and stratigraphic identification key (Médus, 1970). Thus, to confirm the age attribution made by Azema et al. (1972), supplementary palynological arguments must be made.
Several observations support a Cenomanian rather than Albian age for the lignitic clays of Neau. The presence of Artiopollis indivisus (Fig. 6T) is worth being noted, this form having been observed only in Late Cretaceous palynofloras so far, especially Cenomanian (Singh, 1983; Ravn and Witzke, 1995; Lupia, 1999). The occurring of Microreticulatisporites sacalii is sometime considered as a stratigraphic argument in favour of a Cenomanian age (Peyrot et al., 2019) because it has been almost exclusively found within Cenomanian strata (Deák and Combaz, 1967; Médus and Triat, 1969; Peyrot et al., 2019), but Ravn (1995) observed this species in late Albian assemblages of Wyoming. If this form is frequently encountered, it may be considered as relatively stratigraphically significant, when coupled with other stratigraphic arguments. The observation of numerous tricolpoidate and tricolporate forms, such as Phimopollenites and Nyssapollenites, is also indicative of Cenomanian rather than Albian assemblages. Specimens belonging to those genera, and more generally tricolporate pollen grains, appear very scarcely during the Albian, but become much more frequent and diverse during the Cenomanian (Doyle and Robbins, 1977; Hochuli et al., 2006). Actually, those tricolpoidate and tricolporate specimens were encountered more frequently in the palynoflora from Neau than in the lower Cenomanian palynofloras recovered from Charente-Maritime, Charente, and Vienne (Peyrot et al., 2019; Polette et al., 2019). The absence of indubitable mid-Cenomanian markers, such as Normapolles, has to be acknowledged. The lack of observation does not necessarily mean that Normapolle grains were not present in Neau palynoflora, and the absence of a form cannot be considered as stratigraphically significant. However, Normapolles complex diversified quite rapidly from the end of mid Cenomanian onward (Méon et al., 2004) and several species were usually encountered from other mid to late Cenomanian assemblages from western France (Azema et al., 1972; Néraudeau et al., 2017). If they were to be found in Neau lignites, they are certainly very scarce.
The palynoflora from Neau is then probably younger than the charentese palynofloras, and older than Normapolles-rich mid Cenomanian palynofloras from Vendée (western France; Azema et al., 1972; Néraudeau et al., 2017), agreeing with the regional stratigraphic correlations of Azema et al. (1972). A possible age of upper lower Cenomanian or lower mid Cenomanian (which is virtually the same) is then attributed to the Neau amber-bearing lignitic clays.
5.3 Palaeoenvironment
Such poorly diversified conifer-dominated plant assemblage is common in the Laurasian littoral floras during the Albian-Cenomanian. Albian-Cenomanian floras yielding the conifer Frenelopsis as well as the ginkgophyte Eretmophyllum (or Nehvizdya) were reported from several palaeobotanical sites of western France, including the Archingeay quarry and the Renardières quarry in Charente-Maritime (Néraudeau et al., 2005), and the Brouillard quarry in Maine-et-Loire (Pons, 1979; Néraudeau et al., 2013). The abundance of both the leafy axis Frenelopsis and the dispersed pollen grain Classopollis as well as the chemical signature of the amber suggest that Cheirolepidiaceae were one of the main component of the flora bordering the palaeokarsts from Neau. Although both are isolated in the sediment from Neau, Classopollis was reported attached on microsporangiate cones of Frenelopsis alata from other Cenomanian palaeobotanical sites of Europe (e.g. Kvaček, 2000). As it was remonstrated in the Albian-Cenomanian deposits of western France (e.g. Pons, 1979; Néraudeau et al., 2005, 2013; Girard et al., 2013a, 2013b; Moreau et al., 2014, 2017) and other European localities (e.g. Kvaček, 2000), the genus Frenelopsis is related to littoral environments commonly with strong marine influence. Ecophysiologically, the xerophytic characters of the conifer Frenelopsis clearly show that the flora from Neau was adapted to withstand intense sunlight and coastal environments exposed to desiccant conditions coupled in haline settings: sheathing leaves, thick cuticle, grooved epidermal cells, epidermal hairs, stomata in sunken lines, and stomata with two levels of papillae (Thévenard et al., 2005). These morphoanatomical characteristics allow a reduction of solar radiations, drying air circulations and evapotranspiration.
Classopollis shows a wide geographical distribution. The genus has been reported in high proportions from near-coastal settings, such as sandy bars or coastal islands with well-drained soils (Alvin, 1982; Abbink, 1998), as well as in upland slope habitats (Filatoff, 1975; Vakhrameev and Doludenko, 1977). However, the abundance of Classopollis in the Jurassic and Cretaceous of Russia and North America shows a marked decrease northward, at higher and cooler palaeolatitudes (Pocock, 1972). When recovered with Frenelopsis remains, the presence of this genus is likely to be indicative of warm coastal habitats. The observation of numerous Classopollis clusters within the amber from Neau suggests that their parent plants grew in the vicinity of the depositional environment. The presence of very scarce Surculosphaeridium longifurcatum and foraminifera lining supports the hypothesis of an environment submitted to occasional marine inputs (Appendix S1; Fig. 6A).
The composition of the palynological assemblages of Neau is very similar to that of the Cenomanian assemblages from western France described by Peyrot et al. (2019) and Polette et al. (2019), sharing numerous common species. The present study underlines the fact that all lower to mid-Cenomanian spore assemblages from western France are dominated by Anemiaceae, Gleicheniaceae, and Cyatheales, with often numerous lycopods, mostly belonging to Camarozonosporites (see Azema et al., 1972; Peyrot et al., 2019; Polette et al., 2019). Modern Cyatheales are concentrated at the tropics but can occupy varied habitats (Kramer in Kramer and Green, 1990). Their recurring presence at Neau agrees with a globally warm mid-Cretaceous climate, already suggested by the numerous Classopollis pollen grains (Kujau et al., 2013). Representatives of the Gleicheniaceae are considered to be opportunistic, pioneering tropical to subtropical plants, adapted to long droughts, growing in unstable habitats such as dry forests and wetlands that occasionally dry out (Coiffard et al., 2007; Mehltreter et al., 2012; Kujau et al., 2013). Modern Anemiaceae usually develop under warm and humid environments, and their Mesozoic relatives may have grown along riverbanks, or as understorey in forests (Dettmann and Clifford, 1991; Van Konijnenburg-Van Cittert, 2002). However, some species of Anemiaceae are adapted to more arid conditions, and may tolerate partial desiccation (Proctor and Tuba, 2002; Schrank, 2010). No suggestion has been previously made about the ecological requirements of the potential parent plant of Camarozonosporites, which has been associated with Lycopodiaceae (Ravn, 1995; Schrank, 2010). Extant forms usually develop in fairly sheltered, dark and humid environments, such as conifer forests understorey. They also can grow along riverbanks and streams, or as epiphytes on mossy tree trunks (Rusea et al., 2009). A few species, such as Lycopodiella cernua, are even adapted to more arid condition, and can develop in open and sunny areas (Rusea et al., 2009). While some representatives of Gleicheniaceae, Anemiaceae, and Lycopodiaceae correspond to drought-resistant plants, the majority of extant ferns flourishes in wet conditions, and a high spore content is generally used as indicator of humid settings. Subordinate elements of the palynoflora, such as Todisporites, or diversified Eudicots pollen assemblage support the hypothesis of the existence of a partly riparian hygrophilous plant community (Abbink et al., 2004; Peyrot et al., 2019). Other minor forms recovered from Neau palynoflora, such as Densoisporites and Alisporites, have been interpreted as indicators of tidaly influenced environments (Abbink et al., 2004). The recurring presence of several species of cupressaceous inaperturate pollen grains herein, including Inaperturopollenites dubius, Taxodiaceaepollenites hiatus, Perinopollenites halonatus, along with araucariaceous related forms (Appendix S1) could also suggest also the existence of conifer forests linked to wet lowlands, such as in low salinity back-swamp environments, based on the ecological requirement of some modern Cupressaceae (Schrank, 2010; Peyrot et al., 2019; Appendix S1).
Peyrot et al. (2019) and Polette et al. (2019) discussed extensively the hypothetical environmental settings corresponding to Cenomanian palynofloras from western France, and described various riparian to coastal plant communities which developed under humid and warm condition. They are associated with palynological assemblages grading from (1) assemblages clearly dominated by Classopollis which would indicate downstream and coastal environments associated with xeric communities (cheirolepids, some representatives of drought-tolerant Gleicheniaceae and Anemiaceae) to (2) assemblages dominated by diversified spores, bisaccates and angiosperm pollen grains which would represent more upstream depositional environments associated with riparian hygrophilous plant communities. The composition of the palaeobotanical and palynological assemblages from Neau is intermediate. The corresponding depositional environment was subjected to a very limited connection to the sea, while associated with both drought-resistant plants and hygrophilous ferns and angiosperms. It could well have corresponded to the upstream portion of a mangrove or the most inner part of a lagoon. Depositional settings associated with mangrove-type environments has now been abundantly suggested to accommodate lower to mid- Cenomanian plant communities of western Europe (Batten, 1974; Gomez et al., 2008; Peyrot et al., 2019; Polette et al., 2019). The abrupt increase of the abundance of angiosperm pollen grains is interpreted as a reflection of the group's radiation.
The authors are greatly indebted to the Society Chaux & Dolomie Françaises/Lhoist France Ouest for the authorization to access to the outcrop. They thank Paul Bessin and Valentin Prugneaux for their participation to the field trip. The preparation of thin sections was performed by Severin Morel (UMR 7207). We thank also Géraldine Toutirais (PTME, Muséum National d'Histoire Naturelle, Paris) for his assistance with scanning electron microscopy. The CLSM investigations were performed at the Institute of Biology Paris-Seine Imaging Facility that is strongly supported by the "Conseil Regional Île-de France", the French National Research Council (CNRS) and Sorbonne University.
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Cite this article as: Néraudeau D, Saint Martin J-P, Saint Martin S, Jeanneau L, Moreau J-D, Philippe M, Polette F, Gendry D, Brunet J, Tréguier J. 2020. Amber- and plant-bearing deposits from the Cenomanian of Neau (Mayenne, France), BSGF - Earth Sciences Bulletin 191: 39.
Appendix S1. Species list of palynomorphs recovered from the productive lower mid-Cenomanian clay deposits of Neau, along with potential botanical affinities and counts per sample.
Appendix S2. Molecules identified in the pyrolysates of Neau ambers. Individual compounds are labelled according to the identification of peaks in Table 1.
(Access here)
In the text
New fossil assemblage with amber, plants and vertebrates from the lower Cenomanian near Châtellerault (Vienne, western France)
Conifers from the Cenomanian amber of Fouras (Charente-Maritime, western France)
Thai amber: insights into early diatom history?
A review of amber and copal occurrences in Africa and their paleontological significance
Reassessment of amber-bearing deposits of Provence, southeastern France
BSGF - Earth Sciences Bulletin
Editor-in-Chief: Laurent JOLIVET - Editorial board
© SGF (Société Géologique de France)


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Toronto Real Estate Board RELEASE COMMERCIAL MARKET FIGURES July 2017
by Allen Mayer | Aug 3, 2017 | Real Estate News | 0 comments
GTA REALTORS® RELEASE COMMERCIAL MARKET FIGURES
TORONTO, August 3, 2017 — Toronto Real Estate Board President Tim Syrianos announced that TREB Commercial Network Members reported a combined 391,196 square feet of industrial, commercial/retail and office space leased through TREB's MLS® System in July 2017 – down from 879,946 in July 2016. Leasing results can be volatile on a month-to-month basis.
Average lease rates, for properties leased on a per square foot net basis with pricing disclosed, were up for all three major market segments. The average lease rate for industrial properties, which accounted for approximately two-thirds of space leased, was $7.53. This was up substantially from the average of $5.88 for July 2016, largely due to a lack of lease transactions for very large properties this year, which tend to lease for less per square foot.
"The latest headline GDP results for the Canadian economy have certainly been positive. However, thinking about southern Ontario in particular, there remains a reliance on the export of goods and services, especially to the United States. Export-related sectors tend to be tied to substantial business investment, including real estate. In the coming months, it will be important to monitor the impact of the recent increase in the value of the Canadian dollar," said Mr. Syrianos.
"It will also be important to watch how consumer-facing businesses, which are the drivers of the commercial/retail market segment, are impacted by the dip in housing transactions and the recent increase in borrowing costs," continued Mr. Syrianos.
The total number of sales for all three major market segments combined was 48 in July – down slightly from 55 sales reported during the same month in 2016. The average sale price was up substantially for the industrial market segment and down for the commercial/retail and office segments. These larger year-over-year changes in the average selling price were due to a change in the mix of properties sold this year compared to last, in terms of type, size and location.
"In the coming months, it will be important to monitor the impact of the recent increase in the value of the Canadian dollar (and) It will also be important to watch how consumer-facing businesses, which are the drivers of the commercial/retail market segment, are impacted by the dip in housing transactions and the recent increase in borrowing costs," said TREBPresident Tim Syrianos
provided as information only by Allen Mayer, Broker
Royal Lepage Real Estate Services Ltd., Brokerage
Allen Mayer is a Toronto Commercial Real Estate Agent

redpajama_set_name: RedPajamaCommonCrawl


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OC Ken Whisenhunt Opens Up About Lynn, Gordon, Rivers & More
Amid all the change surrounding the Los Angeles Chargers, the return of Ken Whisenhunt provides stability for one of the NFL's top offenses in 2016. Still, Whiz believes it can be even more explosive as the Bolts begin plans for the 2017 season.
The offensive coordinator spoke for the first time about teaming up with Head Coach Anthony Lynn, his return to the Bolts and plans for the coming months:
Chargers.com:First off, what went into your decision to return to the Chargers in 2017?
Whisenhunt:Well, there were a lot of positive things from last season and it was nice seeing some of the younger players step up and grow. Obviously, you have a quarterback like Philip Rivers that makes a big difference. I had known (Head Coach) Anthony (Lynn) and was comfortable with him. We talked about things before in the past, and it felt right. I had other opportunities but this felt right. I am grateful to the Spanos family for having me here, and I certainly feel like I have good relationship with (General Manager) Tom Telesco. So then add in knowing Anthony and what kind of coach he is, what kind of person he is and the opportunity to work with some of the guys I that really respect seemed like a good move.
Chargers.com:What has the last month been like working alongside Lynn?
Whisenhunt:Fortunately, some of the guys that were on the staff last year got to stay, and there is a lot to be said about continuity. I certainly give Anthony a lot of credit for doing that because we did have some good things happen last year with some of our young guys. Melvin Gordon stepped up, we had a good effort by Hunter Henry and obviously Tyrell (Williams) went over 1,000 yards, which is a pretty big accomplishment. As far as getting to know Anthony, he has been on a whirlwind tour so I haven't really had a chance to see him.
Chargers.com:In what ways will the continuity among the offensive staff help going forward?
Whisenhunt:I think it is good because normally when there is a change at head coach, everything starts over and there is a lot of work. But for us, a lot of the system is going to stay in place. We will get some input from some good coaches like Anthony who has been an offensive coach, which can help us get better. And there are areas where we do need to get better obviously, like with turnovers. We've got to clean that up. That is the number one thing we have to do, and we also have to be more efficient in the red zone. But there were a lot of positive things we want to build off of and tweak. For most of the season we were in the top five in scoring in the league, and to think if we can continue to build off of that and get even better, maybe we can end up like the Falcons.
Chargers.com:Melvin Gordon emerged as a top running back last year scoring 12 touchdowns and making the Pro Bowl. Most look at his rushing yards, but he really improved in all phases. What stood out to you about Melvin?
Whisenhunt:The big question about Melvin coming out of college was is he one dimensional? You knew he was a very talented football player but what kind of receiver could he be? Could he hold up in pass protection in the NFL? What Melvin did last year not only solidified the fact that he is a tremendous runner, but he went a long way to show that he can be a three down back. He is very effective in some of the screens and check downs. He did a much better job in pass protection, too. He will get more opportunities for big plays, but we obviously don't want Melvin taking as many snaps as he did last year. He shouldered the burden of some of our guys being injured at that position like Danny (Woodhead), Branden (Oliver), Dexter McCluster; the list goes on and on. What he's done is established that he can do it and be effective. Melvin technically didn't have 1,000 yards, but he (essentially is) a 1,000 yard rusher and if he doesn't get injured, he probably ends with 1,300 yards. The next step for him is, does he want to take it to the next level? Does he want to be one of the guys who can be one of the top backs in the league? He showed in stretches that he can, but now he has to continue to build on it.
Chargers.com:Joey Bosa has gotten a lot of buzz for his rookie year, and rightfully so, but Hunter Henry had a really big impact in his first year as well. He led all NFL tight ends with eight touchdown catches, and I know the team is really high on him. What is it about Hunter that makes him a special player?
Whisenhunt:It is hard for a young guy to come into the NFL and play that position, especially in an offense like this where there are so many things to do. To be proficient in run blocking, as a passer, as a movement guy in the backfield, out in space and so on. There were a lot of indications from him at Arkansas that he could do it, but give him credit for actually doing it as a rookie. A big part of it goes to Antonio Gates and how he worked with Hunter. There was good chemistry between those two. Hunter developed into an outstanding young tight end prospect and he has the chance to be one of the top players at his position because he can do so many things. He can block, he can catch, he is very productive in the red zone and he has the right mentality for work. He wants to get better. He was outstanding. Tom and those guys did a tremendous job with the first two picks in Joey and Hunter because they knocked it out of the park.
Chargers.com:You mentioned turnovers being the number one issue the offense needs to improve. Philip Rivers had another strong season, making the Pro Bowl and recording one of his highest touchdown totals. Yet he led the league in interceptions. Looking back at the tape, what were the reasons for those interceptions?
Whisenhunt:Let's face it; there were a number of injuries to skill position guys. Guys that were important to him like Danny, Branden and Keenan Allen. When you lose that, there is a little bit of a timing thing you have to get used to. During the latter part of the year, we were so banged up that we were pressing, trying to make plays and sometimes those types of interceptions happen. But you look at where we were midseason, there was talk of Philip being an MVP candidate because of the way he played. So I think part of it was a function of losing players and being injured and pressing, trying to carry the football team because he is such a special player. But, we obviously have to be better at that. He had a couple games where he had a lot of picks, and some of them were ugly. Those are the things we have to clean up. There were a couple of throws where he just threw them up (then) down the field trying to make a play, and those are the things we have to eliminate. As a quarterback, you are always going to have interceptions because there are tight windows and you have to fit the ball in there. But Philip, he is one of the best in the league, if not ever, at seeing it and making throws. So the ones that we gave up, the ones that we just didn't make the good throws on, those are the ones we need to get better at.
Chargers.com:With Tyrell Williams breaking out last season, and now getting Keenan Allen back, even though it is only February, how often do you find yourself scheming up ways to play them off each other?
Whisenhunt:You always get excited about having those guys. We know that we have some playmakers that we can utilize. We'll have some fun in the offseason workouts and seeing what everybody can do and going from there. If you look back to the first game starting against Kansas City, when we had everybody, we were pretty efficient moving the ball. A lot of guys made plays. If we can get back to that, we feel we can be pretty good. With Tyrell, I give him a lot of credit because he played through some injuries. You have to do that in this league. For him to be able to go out there and fight through it, that was a big part of (his success). And (Wide Receivers) Coach (Nick) Sirianni did a great job with him and all the receivers. So I have a lot of respect for Tyrell, and he's going to continue to grow and get better. It is exciting to have a big guy that has that much speed who is still learning at the position and can still get better.


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