1. Introduction
⌅The main objective of this work is to highlight, for the first time, the Variscan deformation characteristics of a set of distorted brachiopod fossils recently discovered in the area of “Val d’Or”, on the Atlantic coast of the Moroccan Meseta (X : 33,906231,Y : -6,986226). The strain analysis performed in this work provides some finite deformation parameters: elongations, quadratic elongations, and angular strain parameters, which, through the use of the Mohr construction, has yielded the axial ratio and orientation of the finite strain.
2. Geological Setting: West Mesetian Variscan Evolution
⌅The western Meseta of Morocco is mainly subdivided into four structural domains (Piqué, 1994Piqué, A. (1994). Géologie du Maroc : les domaines régionaux et leur évolution structurale. Ed. Pumag. 239 p.) representing the roots of the Variscan belt. The major deformation events are Namurian-Westphalian in age (Michard, 1976Michard, A. (1976). Elément de la géologie du Maroc. Notes et Mémoires du Service géologique du Maroc, 252, 422 p.), followed by mostly brittle deformations during the Permian (Ait Brahim and Tahiri, 1996Ait Brahim, L., and Tahiri, A. (1996). Rotation horaire des contraintes et mécanismes d’ouverture et de fermeture des bassins permiens du Maroc central. In: F. Medina (ed.): Le Permien et le Trias du Maroc, état des connaissances. Edit. Pumag, Marrakech, pp. 87-98.). From west to east we distinguish (figs. 1-A and B):
Coastal Block (MC): located in the westernmost part of the Meseta, this domain is stable, scarcely deformed (Michard, 1976Michard, A. (1976). Elément de la géologie du Maroc. Notes et Mémoires du Service géologique du Maroc, 252, 422 p.), and composed by continental platform rocks of the Early Paleozoic, namely middle Cambrian quartzites, schists and Ordovician shales. Near the shear zones affecting the region, those rocks are widely folded and show a slaty cleavage (El Attari, 2001El Attari, A. (2021). Etude lithostratigraphique et tectonique des terrains paléozoiques du môle côtiér (meseta occidentale, Maroc). Thése de Doctorat. Universite Mohammed V-Agdal. Faculté des Sciences de Rabat.). In the oued Rhebar, between Bouznika and Mohamedia, the middle Cambrian schists show a calc-alkaline volcanic complex generated during the Mesetian rift event, with orogenic signatures (El Hadi, 2006El Hadi, H., Tahiri, A., Cabrera, F. et al. (2006). Un exemple de volcanisme calco-alcalin de type orogénique mis en place en contexte de rifting (Cambrien de l’oued Rhebar, Meseta occidentale, Maroc). Comptes Rendus Geoscience, 338, 229-236.).
Benslimane Basin (BBS): defined by Lecointre (1926)Lecointre, G. (1926). Recherches géologiques dans la Meseta marocaine. Mém. Soc. Sci. natur. Maroc, 14, 158 p. and mapped by Destombes and Jeanette (1966)Destombes, J., and Jeanette, A. (1966). Mémoire explicatif de la carte géotechnique de la Meseta côtière à l’Est de Casablanca au 1/50000. Région de Mohammedia, Bouznika, Ben-Slimane. Notes et Mém. Serv. géol. Maroc, 180 bis, 104 p. as a NS sheared and compressed furrow, located at the East of the Coastal Block and separated from it by the West Meseta shear zone (WMSZ; figs. 1-A and B). This basin is formed by upper Famennian to upper Visean series that were affected by ductile, semi-brittle and brittle polyphasic deformation under a clockwise rotating principal stress σ1 (Nassri and El Adraoui, 2022Nassri, K., and El Adraoui, A. (2022). Rôle Des Alternances De Tectoniques Ductile Semi Fragile – Fragile Avec Σ1 Decrescendo En Rotation Horaire, Dans La Structuration Hercynienne De La Façade Nord De La Bande De Benslimane (Meseta Nw, Maroc). The International Congress on Educational Research, Materials Science & Engineering (ICEMSE) Saidia, Marocco, 25-27 November 2022, 71p. http://icsse2022.com/wp-content/uploads/2022/11/Proceeding.pdf.).
Cherrat Ridge (RCH): a N-S Devonian horst, it is mainly constituted by Silurian and Devonian platform carbonates. They were up-righted and sheared (Chalouan, 1977Chalouan, A. (1977). Stratigraphie et structure du Paléozoïque de l’Oued Cherrat : un segment du couloir de cisaillement de la Meseta Occidentale, Maroc. Thèse de 3éme cycle, U.L.P. Strasbourg, 92 p.) by a first Variscan deformation phase, D1, giving place to folds (trending N160ºE) and a fracture cleavage. A second Variscan phase, D2, originated folds (trending N045ºE), kinks and a crenulation cleavage. Towards the Atlantic Ocean, at Skhirate, Cherrat Ridge is offset towards the East by the E-W to NE-SW dextral strike-slip fault array of Skhirate.
Sidi Bettache Basin (BSB): Defined by Piqué (1979)Piqué, A. (1979). Evolution structurale d’un segment de la chaîne hercynienne : la Meseta marocaine nord-occidentale. Sci. Géol., Mém. 56, 243p., this basin is filled with thick series of Famennian-Tournaisian and upper Visean ages and subdivided into (Lakhloufi et al., 2002Lakhloufi, A., Hamoumi, N., Saquaque, A., et al. (2002). Évolution géodynamique des bassins de Sidi Bettache et de Brachwa-Maaziz et reinterpretation de l’histoire de l’Orogénese Hercynienne post-Viséenne au Maroc. 519 págs. Thèse Sciences Université Mohammed V., Rabat., 2008Lakhloufi, A., Hamoumi, N., Saquaque, A., et al. (2008). Tectónica compresiva sinsedimentaria de edad Viseense Superior en la cuenca de Sidi Bettache (Meseta noroccidental marroquí) Late Visean synsedimentary compressive tectonism into the Sidi Bettache Basin (northwestern Moroccan Meseta). Bol. R. Soc. Esp. Hist. Nat. Sec. Geol., 102(1-4), 71-92.):
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Sidi Bettache Basin s. s. (BSB): individualized during the upper Famennian.
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Brachwa-Maaziz Basin (BBM) filled with upper Visean deposits.
According to the authors cited before, the Sidi Bettache basin was formed first by Famennian NE-SW extension and later by upper Visean transpression (σ1 : NE-SW). This basin, which northwestern part is studied here, was strongly folded and metamorphosed mainly during the Namurian-Westphalian, and strongly sheared during later Permian phases.
3. Structural outline of the Northwestern Sidi Bettache Basin
⌅We studied here the coastal band of the Sidi Bettache basin, which extends into the central Meseta (figs. 1-A and B). It is formed by Famennian-Tournaisian detrital series covered by thick Upper Visean rocks, including claystones, recifal limestones, coastal sandstones, detrital quartzites, siltstones, mudstones and shales. Close to our sampling point in Val d’Or beach, some of these Visean series crop out in the Sable d’Or beach, showing mainly two phases of deformation:
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D1 folds trending N170ºE, with vertical or steep, west-dipping axial planes. Folds are accompanied by a slaty cleavage (S1) often parallel to their axial planes.
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D2 folds trending N-S, but accompanied by a penetrative crenulation cleavage striking N120ºE to N-S (Fig. 1-C). The localized variation of the directions of S2 can be interpreted as the result of rotational deformation (possibly dextral transpression). The folds generated by E-W shortening are then sheared by N120ºE dextral strike-slip faults and N160º-N168ºE sinistral strike-slip faults, indicating a late NW-SE compression.
The samples of brachiopods studied in this paper show exclusively ductile deformation associated with D2.
4. Methodology
⌅In this work we intend to determine the shape and orientation of the finite strain ellipse from deformed fossils (brachiopods) that presented bilateral symmetry before deformation. Finite deformation can be separated into different components: translation, rigid rotation, distortion, and volume or area change. The distortion and the change in volume or area constitute the strain (e.g., Fossen, 2010Fossen, H. (2010). Structural Geology. Cambridge University Press, 1-463. https://doi.org/10.1017/CBO9780511777806.). In two dimensions, strain can be described by several dimensionless quantities. To measure changes in the length of lines, parameters such as linear extension (e = (l1-l0)/l0), elongation (λ = l1/l0 = 1 + e), quadratic elongation (Λ = λ2), or logarithmic or natural deformation (ε = ln λ) can be used. In all cases, l1 and l0 indicate the final and initial length of the line, respectively. On the other side, the shear angle (y) measures the change in the angle between two initially perpendicular lines. In this work, y is considered positive in case of a clockwise rotation and negative otherwise. Finally, the shear strain parameter, g, is defined as g = tan y. Two-dimensional finite strain is best represented by the strain ellipse, which is the figure obtained by homogeneous strain of an initial circumference of unit radius. Accordingly, the half-length of the principal axes of the finite strain ellipse are λG > λP. A useful way to represent the shape of the finite strain ellipse and its dimensions with respect to the initial, circumference is the Cartesian diagram λG vs. λP (Fig. 2) (e.g., Ramsay, 1967Ramsay, J. G. (1967). Folding and fracturing of rocks. McGraw-Hill, New-York. 568 p.).
4.1. Mohr circle of deformation
⌅Each line of the ellipse (Fig. 3) forming an angle θ’ in the deformed state with the main axis λG is characterized by a reciprocal quadratic elongation: Λ’ = Λ’G cos2θ’ + Λ’P sin2θ’.
The corresponding shear is defined as: γ’ = (Λ’P - Λ’G) sin θ’. cosθ’. Equations Λ’ and γ’ are a way of expressing the equations of a circle. The reciprocal quadratic elongations Λ’, Λ’P and Λ’G are obtained by operating the inverse of the quadratic extensions: Λ’ = 1/Λ and
In order to determine the deformation ellipse, the previous equations are reformulated as (Ramsay, 1967Ramsay, J. G. (1967). Folding and fracturing of rocks. McGraw-Hill, New-York. 568 p., 1970Ramsay, J. G., and Graham, R. H. (1970). Strain variation in shear belts. Canadian Journal of Earth Sciences, 7(3), 786-813.; Viallon, 1991Vialon, P. (1991). Objet et démarche de la tectonophysique. Revue Française de géotechnique, Nº 56, 7-15.):
The analysis of the deformation becomes possible by the construction of the Mohr circle, the horizontal axis corresponds to the reciprocal quadratic elongation Λ’ and the axis of the coordinates represents the shears γ’ (Fig. 3).
4.2. Determination of the deformation ellipse
⌅The determination of the main axis of the ellipse by strain analysis is only possible if the viscosity of the matrix is close to that of deformed objects (Brun and Choukroune in Nicolas, 1984Nicolas, A. (1984). Pricipes de Tectonique, Ed. Masson, Paris, 196 p.; Michard, 1977Michard, A. (1977). Contraintes, déformations, fabriques- ULP,institut de Géologie-strasbourg 150 p., etc.). This condition is verified in our case, since the matrix (organic clay mud) and the material filling by moulding the shells of the Brachiopods Sprifer sp. are identical. We have used brachiopods as deformed objects for the measurement of angular shear deformation (Fig. 4). It should be noted that the Mohr diagram is not to scale.
The interest of the brachiopods, Spirifer sp. in particular, is the presence of two perpendicular lines in the undeformed state: hinge line and sinus symmetry line. After distortion of the fossils, though differently oriented, the shear angle ψ is measured as the angle deviating of the median sinus line relative to its originally perpendicular hinge axis. Plotting in the Mohr space the individual values of ψi of the different individuals makes it possible to find the ratio ΛG/ΛP and the shape and orientation of the deformation ellipse (figs. 3 and 4).
We have computed the angular deformation parameters on 14 selected brachiopod fossils distributed on five rock samples taken on an anticline structure (Fig. 1-C), a folded lumachellic layer interbeded in clay-mudstone strata affected by recumbent, west-vergent crenulation microfolds. Samples 1, 2, 3 are taken from the low-dipping limb (S0-1 in average N173, 25 E and S2: N003,90). Sample 4 is taken in the steeply-dipping limb (S0-1: N002, 80W and S2: N174, 70 E), while sample 5 is taken at the inner part of the hinge of the anticline (S0-1: N005, 85W and S2: N002,78 E) (figs. 1-C and 5).
Figure 5 shows five horizontal sections taken parallel to layers and slaty cleavage S0-1 (D1). Also, crenulation cleavage (lineation Lc, and S2) generated during phase D2 is indicated on each section. The photographs are taken with the north always oriented to the top. In each sample, two or three fossils were selected with complete hinges and symmetrical lines (figs. 6 and 7).
The results are summarized on a synthetic table (Table 1). A final synthesis will be raised and a conclusion-discussion will be presented as an attempt to identify the significance of this deformation in the genesis of the Variscan chain in a junction zone of five Variscan domains of the western Moroccan Meseta.
| Sample | Nº | ψ | γ | 2θ’ | Nhinge | Nsinus | Λ›G | Λ›p | Λ›p/ Λ’G | λG /λP | N λG | N λP |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | Fossil 1 Fossil 2 Fossil 3 |
+32º +28º +09º |
0,625 0,532 0,758 γm : 0,637 |
1-2 : 13º 2/3 : 67º 1/3 : 80º |
N009 N022 N030 |
N145 N136 N163 |
07 | 23 | 3,285 | 1,813 | N167 | N77 |
| 2 | Fossil 1 Fossil 2 Fossil 3 |
+16º -12º -20º |
0,286 -0,212 -0,363 γm : -0,289 |
1-2 : 100º 2-3 : 66º 1-3 : 166º |
N001 N137 N088 |
N113 N025 N002 |
7,4 | 16,3 | 2,202 | 1,483 | N175 | N85 |
| 3 | Fossil 1 Fossil 2 Fossil 3 |
+06º -25º -21º |
0,1051 -0,4663 -0,3838 γm : -0,745 |
1-2 : 123º 2-3 : 30º 1-3 : 93º |
N041 N111 N170 |
N175 N019 N042 |
13,2 | 33,3 | 2,523 | 1,59 | N29 | N119 |
| 4 | Fossil 1 Fossil 2 Fossil 3 |
-8º +25º +10º |
-0,1405 0,4663 0,1763 γm : 0,502 |
1-2 : 108º 2-3 : 66º 1-3 : 50º |
N153 N014 N177 |
N018 N150 N132 |
09,2 | 24,8 | 2,695 | 1,641 | N162 | N72 |
| 5 | Fossil 1 Fossil 2 |
-34º -13º |
-6,674 -0,231 γm : -0,905 |
1-2 : 70º | N002 N118 |
N042 N014 |
7,5 | 30,6 | 4,08 | 2,02 | N177 | N87 |
4.3. Wellmann method and Breddin graph
⌅The Wellman method (Wellman, 1962Wellman, H. G. (1962). A graphic method for analyzing fossil distortion caused by tectonic deformation. Geological Magazine, 99, 348-52.; Shah and Srivastava, 2007Shah., J., and Srivastava, D. C. (2007). Strain estimation from distorted vertebrate fossils: application of the wellman method. Geology Magazine, 144(1), 211-216.) uses objects with orthogonal lines of symmetry in the undeformed state, by drawing a reference line and then project on it parallel lines from endpoints to hinge and symmetry lines from each fossil. If the rock is unstrained, the lines will define a rectangle. If the rock is strained they will define parallelograms. At least the numbered corners of the parallelograms are joined to fit an ellipse with major and minor axis, which give the axial ratio R. If an ellipse cannot be fitted, then the strain is heterogeneous.
The input data in Breddin graph (Breddin, 1956Breddin, H. (1956). Die tektonische Deformation der Fossilien im Rheinischen Schiefergebirge. Zeitschrift Deutsche Geologische Gesellschaft, 106, 227-305.; Célérier and Séranne, 2001Célérier, B., and Séranne, M. (2001). Breddin’s graph for tectonic regimes. Journal of Structural Geology, 23, 789-801.) are the angular shear (ψ) and the orientations of the sheared line pairs with respect to long axis of the strain ellipse (φ). The R-value or ellipticity of the strain ellipse is found by fitting the points on the plot until they coincide on one of the curves.
5. Results
⌅This sample taken from the middle of the low-dipping limb of recumbent shows fossils deformed mainly by refolding S2 P2 (D2), crenulation especially in the intrados of the minor folds. Among 12 fossils, 3 individuals were selected 1-1, 1-2 and 1-3 (figs. 6-A and B). All the fossils are weakly S-shaped which seems to indicate a heterogeneous deformation. The fossils are commonly micro-folded (N-S trending hinges). The angles 2θ’ shown by their hinges are 13º, 67º, and 80º. The construction of the Mohr circle of deformation (Fig. 6-C) considering the parameters (ψ, 2θ’), permit to determine the reciprocal ratio Λ’P / Λ’G = 3.2857. The ratio λG/ λP (R) of the ellipse axis we look for is λG/ λP = (Λ’P / Λ’G)1/2 = 1.813.
The trend of λG is computed by counting 24º clockwise outside of the angle formed by hinge 1-1 and hinge 1-3, i.e., approximately λG is N167ºE and λP is N077ºE. We obtain so the axial ratio and the orientation of the ellipse axis.
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Sample 2: (Fig. 7-A)
This sample is the farthest from the hinge of the anticline, and presents great richness in fossils (brachiopods and lamellibranchs). The chosen individuals present two negative ψ values, namely -12º (2-2) and -20º (2-3), and a positive ψ value for 2-1, +16º. Angles 2θ’ formed by the three hinges are relatively high (66º, 100º, and 166º). The axial ratio λG/ λP (R) obtained from the Mohr circle is the lowest among all of the studied samples (1.483). The calculated axes of the finite strain ellipse yielded λG: N175ºE and λP: N085ºE.
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Sample 3: (Fig. 7-B)
Located at the middle part of the low-dipping limb of the anticline, it shows very big and thin individuals, in average, L (hinge): 3 cm, and l (sinus): 3.5 cm. Most of the shear angle values are negative, -21º (3-3), -25º (3-2) and +6º (3-1). The three hinges are intersected at 123º, 30º and 93º. The axial ratio λG/ λP (R) extracted from Mohr circle is 1.59 and the strikes of the ellipse axes are N029ºE (λG), and N119ºE (λP).
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Sample 4: (Fig. 7-C)
This sample is located at a second-order syncline, on the vertical limb of a larger anticline. The three individuals selected cut each other at 2θ’ of 108º, 66º and 50º; ψ is mostly positive +10º (4-3), +25º (4-2) and -8º (4-1). The ratio λG/ λP (R) obtained is 1.641, and the directions of strain ellipse axes are N162ºE (λG), and N072ºE (λP).
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Sample 5: (Fig. 7-D)
This sample was taken from the hinge of the anticline affected by penetrative crenulation cleavage, which folds intensively the fossils. Only two fossils are complete, 5-1 (ψ = -34º), and 5-2 (ψ = -13º), which hinges cut at 2θ’= 70º. The λG/ λP ratio (R) is the highest of all the studied samples, 2.02, and the directions of ellipse axes are N177ºE (λG), and N087ºE (λP).
From table 1, which summarizes the deformations of the fossil brachiopods of the five samples, we can note the following conclusions:
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Positive values of ψ vary between 6º to 32º, while the negative values vary between -12º to -34º.
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The λG/λP ratio (R) obtained from the Mohr diagram developed for each fossil group varies between 1.483 and 2.02.
5.1. Strain parameters analysis
⌅5.1.1. Relationship between ψ and 2θ’
⌅The class 60º-80º of the angle 2θ’, which is twice the angle between the hinge axis of the brachiopod fossils and the long axis of the finite strain ellipse, is the most representative in terms of variation of the deformation: ψ varies from +9º to +32º clockwise and from -8º to -34º counter-clockwise (Fig. 8). So, it is in the 2θ’ class of 60º-80º that we observe a maximum of rotation (+32º and -34º).
5.1.2. Average results
⌅The Mohr circles constructed for the samples show a homogeneous distribution of the shear angle ψ. The distances of the intersections of the circles from the center of the graph (Λ’, γ’) yield similar values, because the axial ratios λG/λP (R, the root of the ratio Λ’P/ Λ’G) show values varying only slightly between 1.483 and 2.02 (Table 1). The determination of the mean value of the final axial ratio of the ellipse of deformation in the sampling area, either calculating the average value or directly on the cumulated graph (Λ’, γ’), yield the same result: λG/λP = (Λ’P/ Λ’G)1/2 = 1.7.
The determination of the orientation of the principal axes of the finite strain ellipse from the Mohr circle gives the following average results (Table 1): NλG= N170, and NλP= N082.
5.1.3. λG/λP ratio and the structural context
⌅The sampling was performed around an N-S-trending, west-vergent anticline (Fig. 1-C). The maximum values of the λG/λP ratio correspond to the hinge of the fold, on its inner arc, where, assuming a mechanism of tangential longitudinal strain folding, shortening parallel to the layering is the highest (sample 5). Elsewhere from the fold’s hinge on the same lumachellic layer the ratio decreases (λG/λP (1) = 1.813 and λG/λP (4) = 1.642), which is also a characteristic of tangential longitudinal strain. These two samples are in symmetrical positions relative to the axial plane around the hinge. On the low-dipping limb, the value decreases to stabilize around 1.5: λG/λP (3) = 1.59 and λG/λP (2)= 1.483.
5.2. Results by using Wellmann method and Breddin graph
⌅Wellman method give a finite strain ellipse fitted by joining corners of the parallelograms. Its long axis is oriented N152 while its short axis is oriented N062. The axial ratio (R) is equal to 1.87 (Fig. 9-A).
Input data (y, φ) of table of Figure 9-B1 are plotted in the Breddin graph, giving R values varying between 1.2 and 2.5 (Fig. 9-B2). The axial ratio average is R= 1.7. Note that the average orientations of ellipse axes given by Mohr diagrams are N170 and N082, and λG/λP or R= 1.7.
The results obtained for the ratio R are similar for the three methods (see Table 1 (λG/λP) and Fig. 9): the average values of R=1.697 by Mohr circles, 1.698 by Breddin abacus, and 1.87 by Wellman’s method.
6. Conclusion - Discussion
⌅The bulk finite strain computed on strained, Upper Visean brachiopods in the northern area of the Sidi Bettache basin, permits to highlight a possible non-coaxial deformation attained by the brachiopod shells (Fig. 10). Strain was generated under E-W shortening, as a progressive deformation during folding and the development of crenulation cleavage (D2). The three methods used to determine the strain ellipse (Mohr, Wellmann and Breddin) yielded the same results: long and short axes of the finite strain ellipses: N152 to N170 and N62 to N82, respectively, while the average R value is of 1.7 (Mohr and Breddin) or 1.87 (Wellmann).
Deformation is partially computed and described by its strain parameters (ψ, γ, λG/λP) on deformed brachiopods. Distortion of shells took place probably within N-S trending shear zones formed under ductile dextral transpression (Fig. 10-B). These structures were recently recognized (Nassri and El Adraoui, 2022Nassri, K., and El Adraoui, A. (2022). Rôle Des Alternances De Tectoniques Ductile Semi Fragile – Fragile Avec Σ1 Decrescendo En Rotation Horaire, Dans La Structuration Hercynienne De La Façade Nord De La Bande De Benslimane (Meseta Nw, Maroc). The International Congress on Educational Research, Materials Science & Engineering (ICEMSE) Saidia, Marocco, 25-27 November 2022, 71p. http://icsse2022.com/wp-content/uploads/2022/11/Proceeding.pdf.; Nassri et al., 2023Nassri, K., El Adraoui, A., and Tahiri, A. (2023). Etude microtectonique des déformations synsédimentaires des terrains dévono-carbonifères de la plage de Skhirate (Nord de la bande de Benslimane, Meseta NO, Maroc). Hypothèse d’un bassin pull-apart en relai sur la branche Nord de la zone de cisaillement dextre de la Meseta occidentale (ZCMO). Bulletin de l’Institut Scientifique, Rabat, Section Sciences de la Terre, 2023, n° 45, 61-81.) in the neighboring domain (Benslimane basin) in which the Famennian-Visean series are exposed over a relatively large surface.
In the studied area, it is important to note the absence of semi-brittle tectonics by pressure-solution in shales, and lumachellic muds and dark clays show plastic behavior. According to Vialon (1991)Vialon, P. (1991). Objet et démarche de la tectonophysique. Revue Française de géotechnique, Nº 56, 7-15. isotropic layers must be subjected to a strong average stress (σ1-σ3). Indeed, clays contain water which, if it is not expelled during shortening, can make the process reversible or result in superimposed cleavages (Gratier, 1984Gratier, J. P. (1984). La déformation des roches par dissolution-cristallisation: aspects naturels et expérimentaux. Thèse de, Univ. Grenoble.; Vialon, 1979Vialon, P. (1979). Les déformations continues-discontinues des roches anisotropes. Eclog. Helveticae, 79(2), 531-549.). The appearance of schist anisotropy corresponds to a preferential orientation of the internal matter by continuous ductile deformation. In presence of fluids, two behaviors can occur during the generation of schists (Nicolas and Vialon, 1980Nicolas, A., and Vialon, P. (1980). Les mécanismes de déformation ductile dans les roches. Livre Jubil. 1830-1980, Mém. H. s. Soc. Géol. France, 10, 127-139.; Gratier, 1984Gratier, J. P. (1984). La déformation des roches par dissolution-cristallisation: aspects naturels et expérimentaux. Thèse de, Univ. Grenoble.):
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Reorientation by rotation of the objects (crystals, grains, shells) is synchronous with the loss of water, which leads to compaction and hardening of the clay.
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Pressure-solution cleavage (Rutter, 1983Rutter, E. H. (1983). Pressure-solution in nature, Theory and experiment. J. Geol. Soc. London, 140, 725-740.): in this case the shortening of grains parallel to the major stress axis gives changes in form and volume.
The deformations observed on the Upper Visean brachiopod schists correspond to the first case.
The studied area lies a few tens of meters from the N-S shear zone that separates Cherrat Ridge to the west from Sidi Bettache basin to the east (Fig. 1-B). This shear zone acted as a dextral ductile shear band, such as is the case for the Bouznika shear zone (Laamrani, 1993Laamrani El Idrissi, A. (1993). Relations déformations- Déplacements le long des failles hercyniennes : système de Bouznika et système de Cherrat-Benslimane et du Cherrat-Ykem. th Des de 3e cycle, Univ. Med V.,Fac,sc.,Rabat, 213 p.; El Attari, 2021El Attari, A. (2021). Etude lithostratigraphique et tectonique des terrains paléozoiques du môle côtiér (meseta occidentale, Maroc). Thése de Doctorat. Universite Mohammed V-Agdal. Faculté des Sciences de Rabat.).
In the northern part of Sidi Bettache basin, the pure ductile behavior of Carboniferous series can be explained by the proximity of the N-S Cherrat band, which contributed to the displacement to the north of the western Meseta. This type of structures is common elsewhere throughout the Variscan Orogen, such as in the neighboring Iberian Massif (Díez Fernández and Martínez Catalán, 2012Díez Fernández, R., and Martínez Catalán, J. R. (2012). Stretching lineations in high-pressure belts: the fingerprint of subduction and subsequent events (Malpica–Tui complex, NW Iberia). Journal of the Geological Society, 169, 531-543. https://doi.org/10.1144/0016-76492011-101.; Díez Fernández and Pereira, 2017Díez Fernández, R., and Pereira, M. F. (2017). Strike-slip shear zones of the Iberian Massif: are they coeval? Lithosphere, 9(5), 726-744. https://doi.org/10.1130/L648.1.), where they also occur alongside sinistral strike-slip shear zones during the latest stages of Variscan deformation (Díez Fernández et al., 2021Díez Fernández, R., Fernández, C., Arenas, R., and Novo-Fernández, I. (2021). On the Rootless Nature of a Devonian Suture in SW Iberia (Ossa-Morena Complex, Variscan Orogen): Geometry and Kinematics of the Azuaga Fault. Tectonics, 40(6), e2021TC006791. https://doi.org/10.1029/2021TC006791.). These structures are responsible for the displacement of previously deformed pieces of the Variscan Orogen, usually juxtaposing rock series with contrasting tectonothermal evolution and provenance.