TS2.2 | Dynamics and structural evolution of fold-and-thrust belts and accretionary prisms: an interdisciplinary approach
Dynamics and structural evolution of fold-and-thrust belts and accretionary prisms: an interdisciplinary approach
Convener: Christoph von Hagke | Co-conveners: Jonas Ruh, Esther Izquierdo Llavall, Sandra Borderie, Olivier Lacombe
Orals
| Wed, 17 Apr, 08:30–12:30 (CEST)
 
Room K1
Posters on site
| Attendance Thu, 18 Apr, 10:45–12:30 (CEST) | Display Thu, 18 Apr, 08:30–12:30
 
Hall X2
Orals |
Wed, 08:30
Thu, 10:45
Fold-and-thrust belts and accretionary prisms are key geological features occurring all around the globe. They mostly develop along convergent plate boundaries although they may also form along passive margins or other super-critical slopes by a gravitationally driven stress field. Fold-and-thrust belts can display a varied range of scales, may involve the whole continental lithosphere or just the uppermost sedimentary cover and can differ in their spatial extent, longevity of their formation and the rock types involved. Their geometry and kinematic evolution strongly depend on an ample variety of parameters (rheology, temperature, surface processes, structural inheritance, mechanical stratigraphy…), the understanding of their effects being fundamental for the comparison of different fold-and-thrust belts and the development of common predictive models.
Fold-and-thrust belts have been intensely investigated, aiming to decipher their short- and long-term evolution. However, there are important questions that remain not fully understood: i) What is the effect of structural inheritance, décollements, syn-tectonic sedimentation and the interplay between them on mountain building processes? ii) How are transient and long-term rheological/mechanical characteristics and processes affecting the evolution of fold-and-thrust belts? iii) How can we better define deep orogenic geometries and better reconstruct the burial, thermal and kinematic evolution of orogens?
The here proposed session tackles these questions by considering a multidisciplinary approach. We look forward to receiving abstracts focusing on the short- and long-term dynamics and the geometry and structural evolution of fold-and-thrust belts by means of different methodological approaches, including (but not limited to) field structural geology, cross-section construction and balancing, 3D structural modelling, seismics and seismology, analogue and numerical modelling, rock mechanics, geomorphology, thermochronology and geophysics.

Orals: Wed, 17 Apr | Room K1

Chairpersons: Christoph von Hagke, Jonas Ruh
08:30–08:35
08:35–08:45
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EGU24-3200
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On-site presentation
Rob Butler, Francisca Robledo, Phoebe Sleath, and Clare Bond

This presentation challenges the conventional theory that thrust systems necessarily grow by the upward propagation of tip-lines of faults away from a basal detachment. The model underpins mechanical considerations of thrust belt dynamics, explanations of thrust-related folding and commensurate forecasting of distributed deformation in the surrounding strata. Yet there have been few tests of the paradigm at the cross-section scale – not least because the quality of seismic imagery in most foreland thrust belts is insufficient to resolve structural geometries. Rather, the widespread application of the upward propagation (conventional) theory results from a variety of cognitive biases, especially restrictive citation of published literature.

Here we present interpretations of exceptional 3D seismic imagery from the eastern, lateral termination of the Jura fold-thrust belt of Switzerland. The area (the Baden-Irchel-Herdern Zone, referred to here as the BIHZ - broadly overlying the eponymous basement lineament) shows relatively little horizontal shortening and therefore preserves structures that would otherwise be overprinted by more extensive thrusting.  Contractional structures are developed in a multilayer of Mesozoic strata that comprise competent carbonates and incompetent mudrocks and marlstones. Interpretations based on 2D seismic profiles display thrusts sweeping through the Mesozoic strata as simple, continuous ramps, splaying from a basal detachment in Triassic evaporites. However, the higher-quality 3D seismic imagery does not support this type of interpretation. Within the BIHZ, statal reflectors are offset by small-offset (<50m) thrust segments. These do not map out as continuous fault surfaces, either in depth or in map-view. Some thrusts dip forelandward, others towards the hinterland. Collectively, these thrusts are layer-confined and, in plan-view, have highly sinuous forms. These geometries are indicative of having formed by linkage of originally distinct fault segments. Collectively this zone of segmented/low-displacement thrusting represents a “bead” of distributed deformation, restricted to the BIHZ. Presumably, if the area then evolved with greater contraction, part of the thrust array will become fully-linked and develop as a continuous structure – perhaps as elsewhere along the Jura arc. Those fault segments not incorporated into the now-continuous thrust would remain, forming a broad halo of distributed faulting in the surrounding rock. In this spatial context, the swathe of distributed deformation might be designated as a “damage zone” with respect to the main thrust but in fact, the distributed faulting would have no causative relationship to this main thrust.

Our interpretation of thrust system evolution derives from the “ramps first” model of Eisenstadt & DePaor (1987) – a structural concept that has received substantially less attention that the “conventional theory”. We do not wish to imply that there is a single mechanism by which thrusts nucleate and grow – the “conventional” theory may well apply in some situations. So too, may others. We do however emphasise the importance of considering a range of different behaviours and their resultant structural geometries when interpreting thrust systems. Some of these may yet to be described!

How to cite: Butler, R., Robledo, F., Sleath, P., and Bond, C.: Thrust system growth by segment linkage in sedimentary multilayers, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-3200, https://doi.org/10.5194/egusphere-egu24-3200, 2024.

08:45–08:55
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EGU24-8453
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ECS
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Highlight
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On-site presentation
Kristijan Rajič, Hugues Raimbourg, Vincent Famin, and Benjamin Moris-Muttoni

Tectonic mélanges, penetrative mixes of sediments and basalts, are often interpreted as fossil subduction plate interfaces. These formations, marked by intense deformation, contain witnesses of past earthquakes and commonly include remnants of the oceanic crust of the subducting plate. The original process that led to penetrative mixing of sediments and basalts is often controversial, and classically relies either on tectonic slicing of the downgoing plateduring subduction, or on pre-subduction, olistostrome-forming sedimentary mixing. In addition, magma emplacement in sediments of the downgoing plate may also explain the mixed lithologies of mélanges. This latter case should leave an aureole of contact metamorphism in sediments near basalts. In this work, we applied Raman Spectroscopy of Carbonaceous Material in the modern seafloor sediments where magmatism is reported, in order to evaluate the thermal influence from basalts onto carbonaceous material in the contacting sediments. Then, to check the potential contact metamorphism in mélanges, we employed the same methodology in several examples of sediment-basalt mélanges at (sub)-greenschist-facies conditions (Kodiak complex, Alaska; Shimanto Belt, Japan).

In modern ocean-floor settings, magmas intruding, and to a lesser extent, flowing onto sediments, resulted in higher crystallinity of carbonaceous material in a cm- to dm-thick contact aureole. In four of five studied mélanges, the crystallinity of carbonaceous material in metasediments increases toward basalts, indicating a ~1 cm-thick contact metamorphism aureole. Thus, we propose that for the studied mélanges the mixing likely occurred prior to subduction, with the preservation of contact metamorphism despite syn-subduction, low-temperature metamorphism.

As a consequence, the block-in-matrix structure observed in mélanges, as well as the occurrence of mafic bodies at seismogenic depths in accretionary prisms, is in many instances the result of pre-subduction structure, rather than tectonic slicing and step-down of the decollement into the oceanic crust. In particular, tectonic mélanges such as Mugi in Japan and Ghost Rocks in Alaska do not reflect simply the structure and thickness of the plate subduction interface, but a complex combination of pre-subduction geometry and tectonic processes during underplating and within the accretionary wedge.

Furthermore, in two studied paleo-accretionary complexes, deposition ages of the trench sediments forming the matrix of three examined mélanges overlap ages of magmatism within uncertainty. Considering that the basalts from these mélanges exhibit MORB signatures, this age overlap suggests that the mélanges possibly formed at the trench just before ridge subduction. We thus conclude that basalt-sediment mélanges stand as potential records documenting ancient ridge subduction events.

How to cite: Rajič, K., Raimbourg, H., Famin, V., and Moris-Muttoni, B.: The origin of tectonic mélanges and implication for the subduction interface processes, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-8453, https://doi.org/10.5194/egusphere-egu24-8453, 2024.

08:55–09:05
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EGU24-13025
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On-site presentation
Miller Zambrano, Stefano Mazzoli, and Jon Mosar

The Jura fold and thrust belt is characterised by dominant thin-skinned thrusting of the Mesozoic-Cenozoic sedimentary cover and variable interaction with inherited structures and deep-seated (i.e., sub-detachment) faults. In its central parts, this fold-and-thrust belt is detached from an underlying mechanically stiffer basement, along Triassic evaporites and displaced up to 30 km. The eastern termination of the fold and thrust belt is characterised by (i) a much lower amount of shortening (on the order of the hundreds of meters), (ii) a significant thickness reduction of evaporites of the Muschelkalk Group, and (iii) interaction of the décollement with steps associated with faults bounding an underlying Permo-Carboniferous graben (Constance-Frick Trough; CFT).

Using recently processed seismic data (Nördlich Lägern 3D), we document the role exerted by the inherited structures rooted in the Permo-Carboniferous basin fill and basement in the development of the different styles of deformation and structures in an area located northwest of the city of Zürich. The ENE-striking master normal fault bounding the CFT to the south displays evidence of reactivation, during both extensional and compressional episodes, illustrated by apparent normal steps, alignments with no apparent displacement, and gentle folding of the Permo-Carboniferous basin fill. The investigated seismic volume indicates that contractional deformation is concentrated in two major ENE trending fold-thrust zones involving the Triassic-Jurassic epicontinental platform succession and the stratigraphically overlying Cenozoic Molasse Basin deposits. The northern fold-thrust zone (NFTZ), manifested at the surface by the Siglisdorf anticline, consists of an up to 2 km wide pop-up structure linked to thrusting in the detached cover series. The structure is located in correspondence with steps in the topography of the base Mesozoic unconformity produced by south dipping ENE striking minor faults rooted in the Permo-Carboniferous sequence without affecting the detachment integrity. The southern fold-thrust zone (SFTZ), corresponding to the Baden-Irchel-Herdern Lineament, is located above a north dipping major fault of the Late Paleozoic half-graben. The overlying deformation structures in the SFTZ, comprising multiple thrusts and backthrusts, that form fish-tail structures in a narrow, steep zone involving the Mid-Triassic-Jurassic series, are interpreted as the result of layer-parallel shortening associated with buckling of the Mesozoic multilayer. In contrast, the Mesozoic succession is characterized by low deformation and absence of major faults in the area over the central part of the graben (comprised between the Weiach – Glattfelden – Eglisau Lineament – WGEL – to the north and the south fold-thrust zone). The WGEL separates a sub-horizontal to gently folded Mesozoic rock panel to the south from a gently dipping panel to the north. This suggests that fault reactivation may have been accompanied by mild basin shortening and inversion.

In conclusion, different modes of interaction between the Mesozoic multilayer (including the weak evaporite level at its base) and underlying Upper Paleozoic basin fill with inherited basement faults have produced a marked contrast in structural style among the detachment-dominated NFTZ, the buckling-dominated SFTZ, and a low deformation central area.

How to cite: Zambrano, M., Mazzoli, S., and Mosar, J.: Influence of Inherited Structures on Deformation Patterns in the Eastern Jura Fold and Thrust Belt: Insights from 3D Seismic Data, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-13025, https://doi.org/10.5194/egusphere-egu24-13025, 2024.

09:05–09:15
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EGU24-9604
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ECS
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On-site presentation
Thorben Schöfisch, Hemin Koyi, Antonio Teixell, and Bjarne Almqvist

The Aragüés thrust system, in the Southern Pyrenees, is a superb and well-exposed sequence of thrust imbricates to study the deformation and development of fault-propagating folds. The mechanisms of folding and thrusting, including the importance of material contrast during the development of the thrust sequence, are well-studied in this area. However, insights into the distribution and magnitude of penetrative strain remain unknown. Therefore, analysis of anisotropy of magnetic susceptibility (AMS) is used to reveal penetrative deformation within the sedimentary rocks of the Aragüés thrust system. Rock samples from 66 locations are collected across the Aragüés thrust imbricates with a focus on the layered limestone unit. A total of 489 cylinders were retrieved from the oriented hand samples and their AMS signal was measured. Thermomagnetic and magnetic remanence measurements show that the magnetic susceptibility of the samples is dominated by paramagnetic minerals and the magnetic lineation (axis of maximum susceptibility) is mainly parallel to subparallel to bedding. However, the more strongly magnetic samples (kmean: 3-5 x 10-4SI) show a magnetic lineation parallel to the general NNE-SSW shortening direction at the back- and forelimbs of fault-propagation folds. In contrast, the samples with a lower magnetic susceptibility (kmean: 1-3 x 10-4 SI), which are also closer to fold hinges, reveal a magnetic lineation perpendicular to the main shortening direction. We interpret the differences in fabric alignment and magnetic susceptibility to mineral composition and structural evolution. For example, the magnetic lineation parallel to the shortening direction is a consequence of flexural slip and flow along bedding surfaces or incompetent beds of the layered limestone units in the fold limbs. Additionally, a relationship between the magnetic lineation and the development of cleavage and stylolites within the limbs can be identified, but is not consistent. The magnetic lineation at the fold hinge is perpendicular to the main shortening direction and needs further investigation for strain accommodation prior to folding, an effect of buckling and/or development as intersection lineation. These first interpretations of the magnetic fabric provide additional insights into the deformation of the Aragüés thrust system and the development of fault-propagating folds. Moreover, the AMS data adds new information on penetrative strain in this region of the Southern Pyrenees and reveals a general tectonic overprint on grain-scale within sedimentary rocks during deformation.

How to cite: Schöfisch, T., Koyi, H., Teixell, A., and Almqvist, B.: Penetrative strain of the Aragüés fault-propagating folds in the Southern Pyrenees revealed by magnetic fabric analysis, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-9604, https://doi.org/10.5194/egusphere-egu24-9604, 2024.

09:15–09:35
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EGU24-4040
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solicited
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Highlight
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On-site presentation
Mary Ford

The Pyrenees is a collisional orogen built by inversion of an immature rift system during convergence of the Iberian and European plates from Late Cretaceous to late Cenozoic. The full mountain belt consists of the pro-wedge and foreland of the southern Pyrenees and the retro-wedge and foreland of the northern Pyrenees, where the inverted lower Cretaceous rift system is mainly preserved. Due to low overall convergence and absence of oceanic subduction, this immature orogen preserves one of the best geological records of early orogenesis, the transition from early convergence to main collision and the transition from collision to post-convergence. During these transitional periods major changes in orogen behavior reflect evolving lithospheric processes and tectonic drivers. These records are best preserved in the North Pyrenean Zone (NPZ), the retrowedge thrust belt and its adjacent syn-orogenic basin. This paper reviews along strike variations in structural and stratigraphic characteristics of the NPZ and adjacent basin evolution and explores the changing role in space and time of rheological, thermal and structural Inheritance and local and plate scale drivers.

How to cite: Ford, M.: Lateral and temporal variations in thrust belt behaviour in a low convergence retrowedge, north Pyrenees. , EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-4040, https://doi.org/10.5194/egusphere-egu24-4040, 2024.

09:35–09:45
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EGU24-7287
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On-site presentation
Josep Muñoz, Esther Izquierdo, Rosibeth Toro, Pablo Santolaria, Pablo Granado, Emilio Pueyo, and Antonio Casas

We present a new cross-section across the Jaca basin in the southern Pyrenees, aiming to analyze the temporal and spatial distribution of deformation in a fold-and-thrust belt. In this study, we have integrated all available subsurface data, including seismic sections and well data, with surface data to construct a balanced cross-section and partial restored cross-sections that illustrate the evolution of the south-Pyrenean fold-and-thrust belt.

Contractional deformation, initiating the development of the Pyrenean Mountain belt, started during Late Cretaceous times due to the reactivation of the Early Cretaceous hyperextended margin. Subsequently, deformation progressed during the Paleogene within the unstretched Iberian plate. In this region, the kinematics of the thrust wedge was controlled by inherited extensional faults and the unevenly distribution of Triassic evaporites above the basement.

Although deformation progressed toward the foreland, synchronous thrusting characterized the internal deformation of the thrust wedge. The localization and switching of deformation along the fold-and-thrust belt resulted from the interaction of unevenly distributed weak layers, including salt, and syntectonic sedimentation.

This work illustrates how detailed fieldwork, when combined with subsurface data and news concepts and methodologies (such as the use of drone imagery and analogue and numerical modelling), can significantly improve the understanding of the structure and evolution of fold-and-thrust belts.

How to cite: Muñoz, J., Izquierdo, E., Toro, R., Santolaria, P., Granado, P., Pueyo, E., and Casas, A.: Cover-basement relationships in a fold-and-thrust belt with inherited uneven weak horizons distribution: example from the southern Pyrenees across the Jaca basin, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-7287, https://doi.org/10.5194/egusphere-egu24-7287, 2024.

09:45–09:55
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EGU24-5837
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ECS
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On-site presentation
Augusto Maresca, Pablo Granado, Josep A. Muñoz, Gianreto Manatschal, Kei Ogata, and Stefano Tavani

The Apennines fold-and-thrust belt builds part of the Africa-Eurasia convergent plate boundary. It developed due to the Neogene subduction of the Alpine Tethys underneath Europe and to the subsequent involvement of the Adria microplate rifted margin into the collisional process. Since the Miocene, eastward retreat of the slab caused extensional deformation of the thrust pile, eventually leading to the opening of the Tyrrhenian back-arc basin. Multiple schools of thought exist about the structural style of the Apennines, each of which proposes rather irreconcilable models. The amount of shortening, the involvement of the crystalline basement, the architecture of the inherited rifted system with its degree of reactivation during convergence, and the role played by compressive inheritance during back-arc extension, are still under discussion.

In this contribution we focus on the crustal structure of the central Apennines, along a transect that stretches from the Sardinian shelf (West) to the center of the Adriatic Sea (Est). Our aim is to critically evaluate prior models and contextually to illuminate the deeper part of the belt, which is still seldom considered in modern-day Central Apennines solutions. Based on the most recent ideas on rift inheritance and thrust tectonics, we present a brand-new crustal balanced cross-section. We employ well-constrained surficial geological data from available public maps, as well as the most recent deep-reaching geophysical data (especially, tomography and seismological data), which are supplemented by thermochronological, biostratigraphic, and Sr-isotope datings. On top of that, data are encompassed in a coherent geodynamic framework that is supported by a geometrically balanced and consistent kinematic model. This way, we provide a comprehensive explanation for the regionally observed coupled forward migration of compressional and extensional domains, which is related to the slab pull/trench retreat system.

Our results point to a predominantly thin-skinned style for the orogen with a secondary basement involvement in the later collisional stage. Inherited extensional faults, developed during the Mesozoic rifting of Adria, were partially reactivated during convergence, and influence spacing and geometry of the compressional features. The main thrusts of the area are characterized by significant displacements, ranging from 10 to >50 km, and sole out into a basal décollement located at the base of the post-Variscan sedimentary sequence. Finally, post-thrusting back-arc extension is accommodated by faults that either displace the compressional décollement levels or reactivate them with an opposing kinematics.

How to cite: Maresca, A., Granado, P., Muñoz, J. A., Manatschal, G., Ogata, K., and Tavani, S.: Rift inheritance in a fold-and-thrust belt evolution: Central Apennine crustal balanced cross-section, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-5837, https://doi.org/10.5194/egusphere-egu24-5837, 2024.

09:55–10:05
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EGU24-15513
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ECS
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Virtual presentation
Basement inherited structures and their control on overburden sediments deformation: A study in the Eastern High Atlas and its northern foreland basins, Morocco
(withdrawn after no-show)
Ismail Es-sabbar, Khalid Amrouch, and Abderrahmane Soulaimani
10:05–10:15
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EGU24-10919
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On-site presentation
Andrea Zanchi, Stefano Zanchetta, Martina Rocca, Chiara Montemagni, Luca Aldega, Andrew Kylander-Clark, Andrea Fiorini, and Eugenio Carminati

The central Southern Alps (cSA) form a complex south-verging polyphase fold-and-thrust belt developed from the Late Cretaceous onward due to the Alpine convergence (Schönborn, 1992; Zanchetta et al., 2015). The oldest ages related to thrust stacking have been obtained from pseudotachylythes along the Orobic Thrust exposed in the northern part of the belt (Zanchetta et al., 2011), stacking the Variscan basement onto the Permian-Triassic cover.

Aim of this contribution is to present new U-Pb radiometric ages of calcite tectonites obtained in the central and southern portion of the belt, where no precise time constrains of thrust stacking are available. E-W trending Eocene dike swarms crosscutting thrust planes are the only indirect evidence of a pre-Eocene age of the oldest stages of the Alpine contraction (D’Adda et al., 2011).

The central part of the cSA shows a thick pile of thrust sheets deforming the Lower to Middle Triassic carbonate successions. Our new U-Pb calcite ages obtained on growth fibers along fault planes, veins and calc-mylonites sampled along some of the most important regional thrust planes mainly result in Late Cretaceous ages. We obtained similar ages also within the southern portion of the belt, where the Norian “Dolomia Principale” thrust sheets, override the Rhaetian Riva di Solto Shale immediately to the north of the frontal portion of the belt. Younger ages resulted from the Paleogene units which are involved in the exposed frontal part of the belt, which is mostly buried under the recent infilling of the Po Plain forming the Milan Belt.

These data confirm previous interpretations of the central Southern Alps as part of a Late Cretaceous doubly vergent pre-collisional belt (Zanchetta et al., 2012). Research supported by the FAST PRIN Project (2021-NAZ-0299, Italian MUR).

D'Adda, P., Zanchi A., Bergomi M. A., Berra F., Malusà M. G., Tunesi A., & Zanchetta S. (2011) - Polyphase thrusting and dyke emplacement in the central Southern Alps (Northern Italy), International Journal of Earth Sciences, 100, 1095–1113.

Schönborn, G. (1992) - Alpine tectonics and kinematic models of the central Southern Alps. Memorie di Scienze Geologiche, 44, 229-393.

Zanchetta S., D'Adda P., Zanchi A., Barberini V. & Villa I.M. (2011) - Cretaceous-Eocene compressions in the central Southern Alps (N Italy) inferred from 40Ar/39Ar dating of pseudotachylytes along regional thrust faults. Journal of Geodynamics, 51, 245-263.

Zanchetta, S., Garzanti, E., Doglioni, C., and Zanchi, A. (2012). The Alps in the Cretaceous: a doubly vergent pre-collisional orogen, Terra Nova, 24, 351–356, 2012.

Zanchetta S., Malusà M. & Zanchi A. (2015) - Precollisional development and Cenozoic evolution of the Southalpine retrobelt (European Alps). Lithosphere, 7, 662-681.

How to cite: Zanchi, A., Zanchetta, S., Rocca, M., Montemagni, C., Aldega, L., Kylander-Clark, A., Fiorini, A., and Carminati, E.: U-Pb calcite geochronology attests Late Cretaceous S-verging thrusting in the central Southern Alps, Italy, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-10919, https://doi.org/10.5194/egusphere-egu24-10919, 2024.

Coffee break
Chairpersons: Olivier Lacombe, Christoph von Hagke
10:45–10:50
10:50–11:00
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EGU24-4663
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ECS
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On-site presentation
Andrea Fiorini, Luca Aldega, Luigi Dallai, Eduardo Di Marcantonio, Martina Rocca, Stefano Tavani, Stefano Zanchetta, Andrea Zanchi, and Eugenio Carminati

Fold-and-thrust belts are usually deformed by major transverse zones oriented orthogonally to the main thrust faults. These structural discontinuities represent ancestral fault zones originated mainly during rifting and subsequently reactivated during orogenic shortening (Zanchi et al., 2012). Sectors displaying thicknesses and sedimentary facies changes within the syn-rifting successions are juxtaposed along transverse zones (Thomas, 1990). This variability results in diverse deformation and shortening styles, as thrusts exhibiting flat (detachment levels) or ramp (more competent lithologies) geometry occur at different depths.

Limited data exist on the origin of fluids circulating along transverse zones and how they control fluid flow at the regional scale. In this study, we analyse transverse zones in the Lecco area of the Central Southern Alps (Lombardy, Italy). This belt features N-S trending, km-scale transverse zones initiated as normal faults during Ladinian, Norian-Rhaetian and Early Jurassic rifting phases and subsequently reactivated as strike-slip faults and/or lateral ramps during the Alpine orogeny (Schönborn, 1992). Two transverse zones are foci of this work: the Lecco Line to the west, running along the southeastern branch of Como Lake, and the Faggio Line to the east.

Geological mapping and mesostructural analysis were conducted and geological cross sections were built to constrain the geometry and kinematics of such transverse zones. Inorganic thermal indicators were used to constrain the eroded overburden and the exhumation depth of the analysed fault zones. U-Pb radiometric dating on syntectonic calcite mineralizations allowed us to constrain the age of tectonic activity. Syntectonic calcite veins precipitated either during the Early Jurassic rifting phase or younger Alpine orogenic phases, testifying the complex and long-lasting tectonic history of these transverse zones. C and O stable isotopes analysis allowed us to assess the origin of fluids circulating within transverse zones and their degree of interaction with host rocks. Two significant findings emerged from these analyses: 1) calcite mineralizations with variable δ13C and δ18O values characterize these fault zones, pointing out different degrees of fluid-rock interactions and/or different origin of fluids circulating during rifting and orogenic shortening; 2) transverse zones and related structures bound sectors where mineralizations occasionally exhibit values within narrow ranges of δ13C and δ18O; conversely, in other sectors, isotopic values display significantly wider ranges. In conclusion, transverse zones in the Southern Alps are structural features with a complex tectonic and fluid flow history, as testified by the large variability of age and C-O stable isotopes values. Furthermore, they possibly exert a partial compartmentalization of fluid flow at the regional scale.

References:

- Schönborn, G. (1992). Alpine tectonics and kinematic models of the central Southern Alps. Memorie di Scienze Geologiche, 44, 229–393.

- Thomas, W. A. (1990). Controls on locations of transverse zones in thrust belts. Eclogae Geologicae Helvetiae, 83(3), 727-744.

- Zanchi, A., D’Adda, P., Zanchetta, S., & Berra, F. (2012). Syn-thrust deformation across a transverse zone: the Grem–Vedra fault system (central Southern Alps, N Italy). Swiss Journal of Geosciences, 105(1), 19-38.

How to cite: Fiorini, A., Aldega, L., Dallai, L., Di Marcantonio, E., Rocca, M., Tavani, S., Zanchetta, S., Zanchi, A., and Carminati, E.: Multiple tectonic phases and fluids variability along transverse zones of the Central Southern Alps (Lombardy, Italy), EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-4663, https://doi.org/10.5194/egusphere-egu24-4663, 2024.

11:00–11:10
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EGU24-12571
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ECS
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On-site presentation
Rudy Scarani, Angelo Cipriani, Niccolò Menegoni, Lorenzo Stori, Paolo Citton, Marco Romano, Umberto Nicosia, and Ausonio Ronchi

In the Nurra region (NW Sardinia), along the coast that stretches from Cala Viola to Cala del Turco bays, a stratigraphic sequence of continental sediments ranging from the upper Paleozoic to the lower Mesozoic is wonderfully exposed.

In the last twenty years this area has been a subject of renewed studies due to its exceptional stratigraphic and sedimentological features and thanks also to an exceptional paleontological record, encompassing trace fossils and body fossils, which provided key chronological data. The most recent investigations have been focused on stratigraphic and structural geology aspects, allowing to reconstruct the tectonic evolutionary history of Sardinia, from the middle Permian up to the Middle Triassic.

The redefinition of the stratigraphic and structural framework of the area became possible through integrating traditional geological surveys (mainly, field mapping, facies and structural analyses) with analyses conducted on 3D digital models of outcrops (DOMs) obtained via drone-based aerophotogrammetry. Investigations, both in the field and computer-based, have enabled the identification of the arrangement of cross-cutting relationships among fault systems.

Despite the absence of absolute geochronological constraints (e.g., dating of syn-kinematic mineralizations), it has nevertheless been possible to identify at least six to eight deformational events. These analyses have revealed the likely history of deformational processes in this sector of the Island, highlighting the tectonic events that have occurred from the Permian until at least the Pliocene, despite Pleistocene-Holocene tectonics cannot be excluded. The events can be summarized as follows:

  • Event 1: extensional tectonics related to the angular unconformity between Permian and Triassic deposits (age post early middle Permian to Early Triassic)
  • Event 2: extensional tectonics related to the rifting of the Ligurian-Piedmont Ocean and subsequent carbonates deposition (Middle Jurassic: Bajocian-Bathonian)
  • Event 3: extensional event related to the early Pyrenaic deformation and represented by an extensive angular unconformity/hiatus in carbonate platform (Early Cretaceous: Aptian-Albian)
  • Event 4: transpressive and compressive event related to deformative phase called “Laramian” tectonics (Late Cretaceous)
  • Event 5: compressive and consequent transcurrent tectonics related to the “Pyrenaic phase” (Eocene to Aquitanian age)
  • Event 6: extensional tectonics related to the opening of the Balearic basin and the rotation of the Sardinia-Corsica block (Burdigalian age)
  • Event 7: extensional tectonic phases occurred during two different sub-events (Serravalian age and the Pliocene age)
  • Event 8: extensional event occurred during the Pleistocene-Holocene

How to cite: Scarani, R., Cipriani, A., Menegoni, N., Stori, L., Citton, P., Romano, M., Nicosia, U., and Ronchi, A.: The Cala Viola-Torre del Porticciolo coastal area: classical geological survey and 3D digital outcrop models (DOMs) analysis to unravel the polyphase tectonics in NW Sardinia (Italy)., EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-12571, https://doi.org/10.5194/egusphere-egu24-12571, 2024.

11:10–11:30
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EGU24-12309
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ECS
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solicited
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Highlight
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On-site presentation
Philipp Balling, Bruno Tomljenović, Marijan Herak, and Kamil Ustaszewski

The overall SW-vergent and in-sequence structural architecture of the Dinarides fold and thrust belt resulted from collision of the Adriatic Microplate with Eurasia in the Late Cretaceous. Throughout Eo-Oligocene times, the deformation front extended outward, causing substantial crustal shortening within the External Dinarides. This part of the orogen is predominantly composed of Mesozoic carbonate platform rocks, originally deposited in an external passive margin setting. Analysis of fault kinematics and two balanced cross-sections suggests a Cenozoic deformation characterized by along-strike contraction. The 250 km long dextral transgressive Split-Karlovac Fault acts as a boundary, separating a southern, SW-vergent nappe stack forethrust dominated domain (as observed in the Split cross-section) from a northern western NE-vergent backthrust dominated segment (as observed in the southern Velebit cross-section). To understand the reasons for the contrasting along-strike deformation, a reevaluation of the temporal and spatial distribution of Paleo-Mesozoic lithofacies along- and across-strike on both sides of the Split-Karlovac Fault was conducted. Additionally, an assessment of the impact of mechanical stratigraphy on deformation styles in this section of the fold-thrust belt was undertaken.

The best-fit kinematic forward model for the central Velebit Mtn. portrays a 75 km wide triangle zone, which took up at least 47 km of Eo-Oligocene shortening. The triangle structure comprises a SW-vergent thick-skinned duplex system detached in the lower Paleozoic Adriatic basement and five thin-skinned backthrusts detached in the upper Paleozoic basement. These backthrusts nucleated at lateral facies boundaries, related to extensional half grabens that formed due to passive margin extension in Middle Triassic and Late Jurassic times. During Cenozoic folding and thrusting these inherited Mesozoic half graben boundary faults were selectively inverted into the NE-vergent backthrusts. This process contributed to the observed along-strike variations in the deformation style of the External Dinarides.

An analysis of instrumentally recorded earthquakes within the northwestern structural domain unveils contrasting seismic activity along the central and southern Velebit transects. In the central Velebit Mountain, the triangle structure currently predominantly undergoes strike-slip motion, with reverse faulting predominantly occurring to the east of the Split-Karlovac Fault. Conversely, seismic activity along the southern Velebit cross-section is concentrated in the structurally lowermost parts of the triangle zone and the foreland, while its structurally higher sections exhibit lower seismic activity. The prevalence of reverse faulting along this transect suggests the ongoing accommodation of shortening in this region.

How to cite: Balling, P., Tomljenović, B., Herak, M., and Ustaszewski, K.: Exploring mechanical stratigraphy's influence on deformation and seismicity: A 2D kinematic modelling study in the central External Dinarides, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-12309, https://doi.org/10.5194/egusphere-egu24-12309, 2024.

11:30–11:40
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EGU24-771
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ECS
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On-site presentation
Ioana Silvia Mihaela Tocariu, Alexandra Tamas, Dan Mircea Tamas, Daria Dohan, Alexandru Lapadat, Zsolt Schleder, and Csaba Krezsek

Studying the complex subsurface structures in fold-and-thrust belts, such as the Eastern Carpathian Bend Zone, remains challenging due to poor seismic data quality caused by steep and intricate structures alongside multiple detachment levels.

To address this, we have conducted eight analogue modelling experiments at the Structural Modelling Laboratory of Babes-Bolyai University with mechanical stratigraphy scaled to the area of interest. We used coloured quartz sand, glass microspheres and silicone to simulate brittle rocks, ductile shales, and salt, respectively. The materials were layered in a 120 cm long deformation box, which was shortened at a constant rate of one centimetre per hour. The experiments were monitored using timelapse photography and particle image velocimetry. The models were consolidated, serially sectioned, and photographed. MOVE software (Petroleum Experts) was used for importing the section images and interpreting the 3D structural style for the models.

The structural style of the experiments varied based on the change in parameters, such as layer thickness, materials, shortening amounts, as well as the timing of erosion and salt deposition. The following description will refer to the most common deformation features observed in the experiments but will use the equivalent formation names and ages. The most noteworthy features are the post-salt lower Miocene's decoupling from the pre-salt section, the lower Miocene upper Kliwa formation decoupling from the Oligocene lower Kliwa formation along the lower Miocene Podu Morii shales, and the distinct wavelengths for the post-salt, upper Kliwa, and pre-upper Kliwa structures.

Considering well data, outcrop data, analogue modelling observations, and the 3D model, we performed seismic interpretation. This guided seismic data interpretation revealed short-wavelength upper Kliwa disharmonic folding, Oligocene–Cretaceous thrust-related hanging-wall anticlines, and large thrust fault displacements leading to hanging-wall erosion and out-of-sequence reactivation of the thrust faults. The results of these experiments proved to be effective tools for comprehending the controlling factors of deformation in the Eastern Carpathian Bend Zone and can aid in the interpretation of subsurface data, especially in areas with poor seismic data quality.

How to cite: Tocariu, I. S. M., Tamas, A., Tamas, D. M., Dohan, D., Lapadat, A., Schleder, Z., and Krezsek, C.: Analogue Modelling to Support Seismic Interpretation in the Eastern Carpathian Bend Zone, Romania, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-771, https://doi.org/10.5194/egusphere-egu24-771, 2024.

11:40–11:50
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EGU24-3749
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ECS
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On-site presentation
Renas Koshnaw, Jonas Kley, István Dunkl, Fadhil Ameen, and Davit Vasilyan

Deep earth geodynamic processes shape surface geology, topography, and the earth’s crust evolution with consequences on erosion, deposition, climate, and biogeography. This research investigates the early-stage growth of the NW Zagros belt in the Kurdistan region of Iraq after the early Oligocene Arabia-Eurasia collision and the geologic signatures of potential SE-ward propagating Neotethys slab tearing. We will test two end-member hypotheses: (i) the slab has already detached, causing subsidence before slab tearing, followed by rapid regional uplift in the vicinity of the suture zone afterward, or (ii) the slab is still attached, causing no pulse of significant hinterland uplift but continuous regional lower plate subsidence. In the NW Zagros belt, where the Arabian and Eurasian plates are sutured along the Main Zagros fault, allochthonous thrust sheets of ophiolitic and arc-related terranes were emplaced onto post-collisional autochthonous units of clastic and lower-middle Miocene shallow marine carbonate rocks, now at ~1-1.5 km elevation. The allochthonous thrust sheets host pre-collisional acidic and mafic intrusions that provide exhumation rate constraints throughout collision, whereas the post-collisional marine carbonate rocks attest to a significant suture zone subsidence and uplift. Thermal history modeling of bedrock samples using zircon and apatite (U-Th)/He thermochronometers suggests an early uplift during ~30-25 Ma, with most apatite (U-Th)/He samples being reset during ~15-10 Ma. To quantitatively determine the depositional age of the lower-middle Miocene marine carbonate rocks, 87Sr/86Sr isotope chronstratigraphy will be conducted. Furthermore, the isopach maps of the middle and upper Miocene foreland deposits show a notable shift in the depocenter axis and an enhanced subsidence toward the SE, concurrent with the arrival of the Afar plume to the suture zone in the NW. These preliminary results argue for the formation of the NW Zagros orogenic wedge as early as ~30-25 Ma, followed by suture zone subsidence during the early-middle Miocene and then uplift again during ~15-10 Ma, possibly due to initiation of Neotethys slab-tearing and its subsequent propagation along the suture zone from the NW to the SE. These findings have implications for investigating the role of the Arabia-Eurasia land bridge formation and deformation on vertebrate distribution and paleoclimate response to orographic barrier development since the late Miocene in the Middle East.

How to cite: Koshnaw, R., Kley, J., Dunkl, I., Ameen, F., and Vasilyan, D.: Tectonothermal constraints on the early-stage orogenic wedge formation along the Arabia-Eurasia suture zone in the NW Zagros orogenic belt, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-3749, https://doi.org/10.5194/egusphere-egu24-3749, 2024.

11:50–12:00
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EGU24-3163
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ECS
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Virtual presentation
Fatemeh Gomar, Jonas B. Ruh, Mahdi Najafi, and Farhad Sobouti

Fold-thrust belts are complex tectonic domains formed in response to near- or far-field compressional stress fields in the Earth’s crust. The complexity of structural style in theses belts is controlled by multiple factors. The presence of mechanically weak layers, defined by rocks that exhibit lower strength than their surroundings, play a significant role in the formation and evolution of fold-and-thrust belts. In this research, a two-dimensional numerical finite difference model incorporating a visco-elasto-plastic/brittle rheology is utilized to investigate the structural evolution of the Fars arc in the southeast of the Zagros fold-thrust belt. The modeling includes the tectonic inversion process, from Permian-Triassic rifting of the Neo-Tethys Ocean to the Oligocene-to-present continental collision between the Arabian and Eurasian plates. The Eulerian grid dimensions were considered as 500 km in length and 60 km in thickness, respectively, comprising 1101×121 nodes. Each cell contains 16 Lagrangian markers that carry the information and properties of each layer. According to the stratigraphic column of the Fars arc, there are 30 km of basement overlain by a 2-km-thick salt layer with a 3-kilometer-thick Palaeozoic sedimentary sequence above the salt layer. Furthermore, to replicate the interplay between Earth's internal and surface dynamics, a 25-kilometer-thick layer representing air is incorporated at the uppermost part of the model to approximate a free surface. The experiments include three inherited basement faults. The role of pre-existing weak zones in extensional tectonics is the shaping of rift basin geometry, especially the formation of half grabens. In the convergence phase, fold-thrust-belts with a basal detachment layer and pre-existing faults produce folding at two distinct scales. The faulting in the basement develops long wavelength folds in the sedimentary cover, while the presence of a salt layer shapes the smaller wavelength folds and thin-skinned thrust faults that extend from the detachment layer to the surface. The reactivated faults play an important role in stress transfer, leading to the emergence of new faults and seismic events. The results indicate that deformed listric faults show a meaningful correlation with the depth distribution of earthquakes throughout the Fars arc. The outcome associated with the presence of a thick basal salt layer and involvement of the basement exhibit a correlation with the structural style of the Fars arc.

How to cite: Gomar, F., Ruh, J. B., Najafi, M., and Sobouti, F.: Numerical modeling of basement inheritance and salt decoupling effects on the structural evolution of the Zagros Fold-Thrust Belt, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-3163, https://doi.org/10.5194/egusphere-egu24-3163, 2024.

12:00–12:10
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EGU24-6848
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ECS
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On-site presentation
Aram Fathian, Hemin Koyi, Stefan Back, Hamid Nazari, Dan H. Shugar, Mohammad Ali Shokri, and Klaus Reicherter

The Fars Arc constitutes the southeastern segment of a tectonic recessions and salients array that characterizes the Zagros orogen. The delineation of the Fars Arc's western boundary is attributed to the prominent Kazerun fault system. However, further to the west, the southwestern periphery of the Arc (i.e., the Bushehr area) remains relatively unexplored, lacking documented evidence of tectonically active structures, as well as significant historical and instrumental seismic events. We combined tectonic geomorphology, remote sensing, and Quaternary geochronology to comprehensively study and identify tectonically active structures within the onshore area. Investigating the offshore area, we utilized 2D seismic-reflection data to interpret and image active subsurface structures in the Persian Gulf. We mapped and introduced several active faults in the Bushehr area, some of which are closely associated with active Quaternary anticlines, e.g., the Bushehr and Abtavil anticlines. Two generations of uplifted marine terraces, Terrace-I and Terrace-II across the Bushehr anticline, reveal a local uplift rate of approximately 0.8 mm/yr across the Bushehr Peninsula. The offshore 2D seismic-reflection data indicate ongoing deformation in the study area and show evidence of a recent sedimentary depocenter offshore of the Bushehr Peninsula. These observations define the present-day active deforming structures along the Zagros orogenic front in the Persian Gulf. The 2D seismic-reflection interpretations have characterized the active folding of the Bushehr anticline, indicating a minimum age of approximately 600 ka BP. The integration of on- and offshore geological analysis has revealed contemporaneous incipient deformation and syn-kinematic sedimentation, which significantly contributes to our understanding of geodynamics of the Zagros deformation front.

How to cite: Fathian, A., Koyi, H., Back, S., Nazari, H., H. Shugar, D., Shokri, M. A., and Reicherter, K.: Active tectonics within the southwestern edge of the Fars Arc, SW Iran, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-6848, https://doi.org/10.5194/egusphere-egu24-6848, 2024.

12:10–12:20
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EGU24-12111
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ECS
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On-site presentation
Aleksandra Smyrak-Sikora, Alvar Braathen, Per Terje Osmundsen, and Kim Senger

The Paleogene West Spitsbergen Fold-and-Thrust Belt, WSFTB, is present in Svalbard (Norwegian High Arctic archipelago; 74-81°N, 15-35°E). The WSFTB’s contraction reflects the Eurekan Orogeny and transpressional continental breakup along a transform fault zone, followed by opening of a seaway between the North Atlantic and Arctic oceans. The overall timing of the contraction is not well constrained, and many authors link it to the development of a deep and narrow foreland basin system filled with Uppermost Paleocene and Eocene to Oligocene(?) deposits, while the Lower Paleocene deposits are considered to be deposited in a regional subsidence prior to Eurekan deformation. The WSFTB divides into a thick-skinned, basement-involved fold-thrust complex in the west, passing into a central zone of thin-skinned, fold-thrust units with associated detachments developed in Permian evaporites and Mesozoic organic-rich mudstones, separated by a prominent duplex system that reflects a thrust-ramp transferring movements from Permian to Mesozoic detachments eastwards. Stress transfer also reactivated the steep, basement rooted Billefjorden and Lomfjorden fault zones farther east, showing up to 200 m of reverse stratigraphic offsets. These fault zones are long-lived structural elements exposing multiple reactivation events since the Late Palaeozoic.

Our study targets the Paleogene reactivation and especially the sequence of deformation of the Billefjorden Fault Zone, based in detailed interpretations of onshore seismic lines, and field mapping supported by acquired and interpreted mountain-scale digital outcrop models. Results suggest initial shortening by reactivation of deep-rooted extensional faults, seen as reverse offsets of stratigraphic units and formation of fault-propagation monoclines as anticlines-synclines pairs. Subsequent deformation involved the regional-scale (tens of km long) decollement zones hosted by the Mesozoic mudstones. West of the Billefjorden Fault Zone, the decollement is seen in the Jurassic Agardhfjellet Formation. Crossing the Billefjorden Fault Zone, this decollement is seen truncating the reverse fault (digital outcrop data) and fault propagation fold (seismic data) and displacing them 2 km to the east, where the decollement continuous in the uplifted mid-Triassic mudstones of the Botneheia Formation. This sequence of deformation, with the reactivated deep-rooted faults truncated by the decollement, contradicts previously published models that advocate for reactivation of deep-rooted faults taking place late during the deformation, synchronised with an uplift of thick-skinned basement-involved thrusts.

The timing of the deep-rooted faults reactivation is poorly constrained. In this study, we hypothesise that it can be as early as the early to middle Paleocene, corresponding to phase of regional compression at 61 Ma indicated, by the recent studies, for the Lower Paleocene Firkanten Formation. This contraction could also be determined from the westward thickening and locally NE and E sourcing deposits of the Firkanten Formation and overlying Basilica and Grumantbyen formations, which indicate an existing topographic high or a foreland bulge as suggested by some of the authors. The timing of the second stage is consistent with the main shortening phase in the Eocene.

How to cite: Smyrak-Sikora, A., Braathen, A., Osmundsen, P. T., and Senger, K.: Sequential reactivation of the Billefjorden Fault Zone during evolvement of the West Spitsbergen Fold and Thrust Belt, Svalbard., EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-12111, https://doi.org/10.5194/egusphere-egu24-12111, 2024.

12:20–12:30
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EGU24-20745
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On-site presentation
Panoramic transect of the Eastern Cordillera fold and thrust belt, northern Andes
(withdrawn)
Camilo Montes

Posters on site: Thu, 18 Apr, 10:45–12:30 | Hall X2

Display time: Thu, 18 Apr, 08:30–Thu, 18 Apr, 12:30
Chairpersons: Christoph von Hagke, Jonas Ruh, Olivier Lacombe
X2.55
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EGU24-19457
Esther Izquierdo Llavall, Rosibeth Toro, Emilio Pueyo, Antonio Casas, Josep Antón Muñoz, Concepción Ayala, Félix Manuel Rubio, and The GeoEU Pyrenean Team

Pre- or syn-orogenic décollements in the external domains of fold-and-thrust belts enhance the decoupling between basement and cover folds and thrusts. In this structural setting, deciphering the degree of basement involvement and the kinematic relationship between thin- and thick-skinned structures can be challenging. This work addresses the study of basement/cover deformation in the central-western Jaca basin, in the southern Pyrenees. The Jaca basin represents the early South Pyrenean foreland basin that was latter deformed, piggy-back thrusted, and incorporated into the South Pyrenean fold-and-thrust belt. Its formation and deformation was coeval with the sedimentation of a thick syn-orogenic sequence consisting of early-middle Eocene turbidites (Hecho Group), late Eocene marls (Arguis Fm.) and late Eocene-Oligocene (Campodarbe Fm.) and Miocene continental units (Uncastillo Fm.). At surface, these syn-orogenic units are affected by a series of NE-SW and E-W-trending folds and thrusts that display frequent along-strike relays and geometrical changes. Debate exists on the geometry, timing and role of basement structures underlying these emerging thrusts and folds.

To shed some light in these discussed geometrical aspects, we carried out a combined structural and gravimetric study covering the central-western part of the Jaca basin. Four serial, seismic-based cross sections have been constructed (from East to West, the Hecho, Ansó, Roncal and Salazar cross-sections). In the cross-sections area, gravimetric data have been acquired along a homogeneous and dense grid, the spacing between gravity sites being ~ 1km.

Conversely to previous interpretations, seismic profiles depict a Paleozoic basement that is significantly faulted and involved in the deep structure of the Jaca Basin. Basement units are affected by numerous south-directed thrusts that partly result from the reactivation of inherited Permian-Triassic extensional faults. They provoke a significant basement uplift from East (Hecho cross-section) to West, with the shallowest basement being identified underneath the central part of the study area (Illón and Leyre surface thrusts). South of this basement uplift (Guarga syncline), the base of the Meso-Cenozoic sequence deepens drastically in the footwall of a main basement-involved structure that accommodates a significant shortening and connects with cover units through a long thrust flat along Middle-upper Triassic evaporites. Gravity data, although influenced by the non-coaxial crustal structure in the region, are consistent with the basement geometry deduced from seismic profiles. The Bouguer anomaly shows a prominent minimum along the Axial Zone and the eastern Jaca basin, a relative positive anomaly marking the central basement uplift (Illón-Leyre thrusts, central-western Jaca basin) and a relative minimum to the south of it, corresponding to the area where the denser basement units reach their deepest position. Both gravity and seismic data reveal a degree of cover/basement coupling which is greater than proposed in previous studies. Basement structures are not cylindrical along the study area, resulting in along-strike changes in outcropping folds and thrusts.

How to cite: Izquierdo Llavall, E., Toro, R., Pueyo, E., Casas, A., Muñoz, J. A., Ayala, C., Rubio, F. M., and Pyrenean Team, T. G.: Basement geometry and cover-basement relationships in the central-western Jaca basin (southern Pyrenees): along-strike variations and role of structural inheritance, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-19457, https://doi.org/10.5194/egusphere-egu24-19457, 2024.

X2.56
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EGU24-16253
Stefano Zanchetta, Martina Rocca, Chiara Montemagni, Giulio Viola, Luca Aldega, and Andrea Zanchi

Despite the small volume they occupy in the crust, fault zones are of striking importance as they localize both seismic slip and aseismic deformation, as well as fluid migration at middle to shallow crustal levels. Regional-scale fault systems may benefit of long-lived activity as, due to their rheological weakness, they can be also reactivated by weak far-field stresses in a variety of tectonic settings. The architecture of fault zones that experienced multiple re-activation is complex and accurate structural analyses, including also the identification of (micro)structural facies (Brittle Structural Facies, BSF) and their crosscutting relationships, is mandatory to solve the spatial evolution and relative chronology of the fault zone.

The Orobic Thrust is a regional-scale fault zone, more than 80 km in length, representing one of the largest structures in the European Alps retro-belt. Along the thrust plane the Variscan basement is thrusted southward over the Upper Carboniferous to Lower Triassic volcano-sedimentary cover of the Southalpine Domain. In several areas the fault zone, ca. 250-300 m thick, is continuously exposed, allowing the detailed reconstruction of the fault architecture. A narrow (20-25 m) protomylonitic band marks the top of fault zone suggesting temperature of at least 300°C in the early stage of fault activity. Temperature in excess of 200°C are also supported by analysis of the thermal maturity of clay mineral assemblages (<2 µm size fraction) in terrigenous rocks in the footwall of the thrust plane. Four distinct BSF have been recognized: cataclasites, foliated cataclasites, pseudotachylyte bearing cataclastic bands and incoherent fault gouges. Apart from fault gouges occurring along discrete plane that appear to be undeformed, all the other 3 BSF display mutual crosscutting relationships, testifying for multiple switching between seismic slip and aseismic creep during fault history. The occurrence of pseudotachyltes and fault gouge allow to obtain absolute age constraints with 40Ar-39Ar and K-Ar illite dating, respectively. The ages obtained from pseudotachylytes span from 83 to 64 Ma whereas illite (<0.1 µm size fraction), separated from the gouge along a fault plane with a reverse kinematic at the core of the Orobic Thrust fault zone, provided and age of 53 Ma. Pseudotachylyte age distribution shows older ages 79-83 Ma occurring both at the top and the bottom of the fault zone, with a superposed pattern that display instead a bottom forward younging direction of ages between 76 and 64 Ma. Discrete fault planes decorated with gouges mark the end of the activity of the Orobic Thrust in the early Eocene.

Detailed meso-and microstructural analyses combined by absolute age constraints of the BSF allowed the reconstruction in space and time of the Orobic Thrust fault zone through its 30 Myrs long fault activity.

How to cite: Zanchetta, S., Rocca, M., Montemagni, C., Viola, G., Aldega, L., and Zanchi, A.: Evolution in space and time of a regional-scale fault: example from the Orobic Thrust (European Alps, Southalpine Domain), EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-16253, https://doi.org/10.5194/egusphere-egu24-16253, 2024.

X2.57
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EGU24-19944
Kateřina Schöpfer, Kurt Decker, Fatemeh Nazari, and Herfried Madritsch

The northwestern Alpine foreland in Switzerland and France comprises the Late Miocene Jura Mountains, considered a type example for thin-skinned thrusting where deformation of the sedimentary cover is decoupled from the basement along a regional basal detachment. To what extent basement faults were involved during its deformation is a matter of debate. We use 3D seismic data to investigate the deformation style along the easternmost tip of the Jura range in an unprecedented detail. Here, basement-rooted normal faults were repeatedly reactivated before thrust belt formation but also contemporaneously active as reverse/transpressional faults. They either propagated up into the Mesozoic succession without interruption (“hard linkage”) or apparently controlled the localisation of Mesozoic faults via smaller-scale shear zones (“soft linkage”). Our analysis of the resulting fault geometries questions the existence of a large-scale basal detachment in this area and points out the importance of thick-skinned fault reactivation.

How to cite: Schöpfer, K., Decker, K., Nazari, F., and Madritsch, H.: 3D-seismic evidence for thick-skinned tectonics in a ‘classic’ thin-skinned tectonics region (external Alpine foreland, Switzerland), EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-19944, https://doi.org/10.5194/egusphere-egu24-19944, 2024.

X2.58
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EGU24-16686
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ECS
Mariusz Fiałkiewicz, Marcin Olkowicz, Bartłomiej Grochmal, Marcin Dąbrowski, Bernhard Grasemann, and Oscar Fernandez

The presented study is a part of a broader project, which includes field as well as numerical investigations into the evolution of tectonic structures within fold-and-thrust belts, with a particular focus on the development of fault-related structures in layered rocks. The existing models for deformation in fold-and-thrusts belts predominantly adopt a kinematic approach, wherein layering is considered as passive. The kinematic approach neglects rheological effects such as mechanical anisotropy, which plays an important role in layered rocks commonly found within fold-and-thrusts belts.

To explore the role of mechanical anisotropy we have analysed folding and thrusting in the central Northern Calcareous Alps (NCA), which comprise the Permo-Mesozoic sediments of the Upper Austroalpine unit. The NCA represents a fold and thrust belt, in which folds are formed by processes along overthrusts (e.g. fault-bend folds or fault-propagation folds), but out-of-syncline overthrusts are also present. The tectonic evolution of NCA is strongly influenced by sedimentary facies. Nappes in the NCA were imbricated during Jurassic and Cretaceous thrusting. Our research has focused on the Scythian (Lower Triassic) mixed clastic-carbonate sediments of the Werfen Fm, located to the SW of Hallstatt at the base of the fold-and-thrust system, as well as on the Upper Jurassic limestones of the Oberalm Fm located SE of Bad Ischl that are deformed syndepositionally into thrusts and folds forming the shallowest part of the fold-and-thrust belt during the Jurassic deformation stage.

During fieldwork, documentation was gathered through the acquisition of orientation measurements of tectonic structures: folded bedding, faults with slickensides, fold axes, cleavage, joints, etc. Photographic documentation of tectonic structures was undertaken to produce georeferenced photogrammetric models. Digital outcrop models in the form of georeferenced textured polygon meshes, which allow the integration of spatial data with the results of detailed geological mapping, were created. All field observations, including outcrop images and measurements, were integrated in a 3D environment, which facilitated the collection of additional data from the digital models.

Sequential restoration and kinematic forward modelling of structures performed in Move software confirm the limitations inherent with kinematic modelling to represent real-world strain patterns. Hybrid modes of kinematic models provide more acceptable results and prove that rheological contrasts within the sedimentary pile exert a strong control in the distribution of folding and faulting. These observations made at the meter-scale, relate to structures that represent a scale of strain normally not represented in regional-scale (kilometer-scale) cross-sections and dealt with as ‘internal strain’. Our observations imply that strain distribution within sedimentary units can be strongly anisotropic and its distribution should be contemplated when performing kinematic modelling of regional-scale structures.

How to cite: Fiałkiewicz, M., Olkowicz, M., Grochmal, B., Dąbrowski, M., Grasemann, B., and Fernandez, O.: Kinematic modelling of fold and thrust structures in anisotropic layered rocks in examples from the Northern Calcareous Alps (Eastern Alps, Austria), EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-16686, https://doi.org/10.5194/egusphere-egu24-16686, 2024.

X2.59
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EGU24-6533
Christoph von Hagke, Arthur Bauville, Nils Chudalla, Sofia Brisson, Florian Wellmann, Dan Tamas, Alexandra Tamas, Piotr Krzywiec, and Alexander Malz

Fault vergence in fold-and-thrust belts and accretionary prisms is characterized by mainly forward verging thrusts and pop-up structures, and only few examples exist where backthrusting dominates. However, backthrusting and triangle zones are known from most if not all fold-thrust belts in the world. The circumstances under which backthrusts instead of forethrusts form are still incompletely understood. Previous studies suggest that the strength and dip of the basal décollement of Coulomb wedges plays a key role. However, a systematic study of these parameters is still missing. We present numerical models of brittle-ductile wedges, varying dip and strength of the basal décollement systematically. We show that a new parameter, cumulative vorticity, is well-suited to characterize wedges based on dominant fault vergence. We find that backthrust-dominated wedges form in setups of very low basal dip (≤ 0.5°) and a weak décollement. Increasing décollement strength or basal dip results in the formation of pop-up-dominated wedges, before forethrust dominated wedges form. While our models corroborate the idea that décollement strength and basal dip may control thrust vergence, comparison with natural examples indicates this cannot be the only explanation for the formation of backthrusts. We probe into this using a compilation of structures along strike the fold-thrust belt of the entire Alpine-Carpathian Belt. Our results show that indeed triangle zones are associated with weak décollements, while additionally syn-tectonic sedimentation, rheological changes across strike, or structural inheritance may play a role. In some cases, interpretations of backthrusts at depth is challenging due to geometric uncertainty. We show uncertainty modeling of triangle zones using a well-known example from the boundary between Eastern and Central Alps. These uncertainty estimates may be combined with thermochronological data with the goal to distinguish the presence or absence of triangle zones from exhumation estimates. When present, triangle zones and backthrusts may serve as mechanical gages, providing tight constraints on fold-thrust belt mechanics.

How to cite: von Hagke, C., Bauville, A., Chudalla, N., Brisson, S., Wellmann, F., Tamas, D., Tamas, A., Krzywiec, P., and Malz, A.: Triangle zones as mechanical gages - results from numerical models and the Alpine Carpathian Belt, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-6533, https://doi.org/10.5194/egusphere-egu24-6533, 2024.

X2.60
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EGU24-11995
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ECS
Matteo Pedini, Federico Cella, Claudio Di Celma, Stefano Mazzoli, and Pietro Paolo Pierantoni

Understanding how orogenic shortening transfers from the basement to the sedimentary cover is crucial in fold-and-thrust belts. Transfer distance dictates the thrusting style. In cases of 'long-distance rooting' such as the Jura Mts.-Swiss Mollasse Basin-Alps system, the sedimentary cover's shortening leads to a thin-skinned deformation style. Conversely, 'short-distance rooting', as observed in the ramp-dominated sectors of the Southern Alps, results in thick-skinned deformation. However, the distinction of thin- vs. thick-skinned styles of thrusting may be ambiguous. 'Long-distance rooting' may cause thin-skinned deformation at the belt front and thick-skinned deformation where the basement underplates, as seen in the Alpine region. The crucial aspect in fold-and-thrust belt dynamics is whether the basement is extensively underthrust and processed in the orogen's interior ('long-distance rooting'), or if displacement directly transfers from basement thrusts to the sedimentary cover on a local scale ('short-distance rooting'). This fundamental issue is addressed here for the Umbria-Marche zone of the Apennines, which style of thrusting has been the subject of a long-lasting debate. Interpretations proposed in the last decades mostly range from pure thin-skinned to composite models of basement-involved deformation and detachment-dominated thrusting of the sedimentary cover.

We aim to investigate whether the sedimentary cover is more shortened than the basement (i.e., a substantial component of ‘long-distance rooting’ of thrust displacement of the sedimentary cover) or do shortening of basement and cover balance at the scale of the foreland fold-and-thrust belt (i.e., ‘short-distance rooting’ characterizes the Umbria-Marche zone). We integrate the updated 1:50,000 scale geological map (CARG Project) of the Sibillini area (Visso and Ascoli Piceno Sheets) with a 10 m cell-size digital elevation model, the interpretation of vintage seismic lines and gravimetric data. We present a series of new balanced and restored cross-sections, including a crustal section along the trace of available seismic lines covering the entire Apennine and foothills area to the coastline, validated by gravimetric modelling, and thirteen cross-sections used to verify the geometric viability of sedimentary cover structures in the study area. The results of our work suggest coupled deformation of basement and sedimentary cover, which are characterized by similar amounts of shortening (consistent with ‘short-distance rooting’ of thrust displacement). The balanced cross-sections, integrated with a dense grid of (n. 25) additional sections perpendicular to the main structural trends, were used to construct a 3D structural model calibrated by surface geology. This allowed us to reconstruct the main fault surfaces, accounting for the along-strike variability of geological features observed from the map and offering a detailed representation of the geometrical arrangement of key horizons (base-top Calcare Massiccio Fm, top Maiolica Fm, top Scaglia Rossa Fm, top Bisciaro Fm) and their relationships with major faults. Our structural model provides new insights into the architecture, timing of the deformation, and kinematic evolution of the Umbria-Marche sector of the Apennines. This has major implications for a better understanding of deformation style, the role of structural inheritance, and post-thrusting extensional tectonics (which controls the seismotectonic setting of the study area).

How to cite: Pedini, M., Cella, F., Di Celma, C., Mazzoli, S., and Pierantoni, P. P.: Styles of deformation in the Umbria-Marche sector of the Apennines fold-and-thrust belt: new insights from balanced geological sections and 3D structural modelling, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-11995, https://doi.org/10.5194/egusphere-egu24-11995, 2024.

X2.61
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EGU24-20163
Late-stage collisional short-lived flysch sedimentation in the south Aegean (Greece).
(withdrawn)
Konstantinos Soukis, Sofia Laskari, Daniel Stockli, and Stylianos Lozios
X2.62
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EGU24-665
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ECS
Nowrad Ali, Edward R. Sobel, Humaad Ghani, and Anne Bernhardt

The Sulaiman and Kirthar fold-and-thrust belts constitute the western boundary of the India-Asia collision zone. The Sulaiman fold-thrust belt is composed of a passive margin sedimentary sequence of Mesozoic to Cenozoic platform carbonates and clastic sedimentary rocks overlain by younger Himalayan foreland basin molasse sediments. This study uses newly acquired zircon (U‐Th)/He (ZHe) data and surface geology observations to document the structural evolution of the north Sulaiman fold-thrust belt. The hinterland zone includes the Zhob Valley Suture thrust, emplaced ophiolites, and folded Mesozoic strata, while the foreland is characterized by folded Eocene to Pliocene strata and hinterland-verging back thrusts. The initial deformation of the North Sulaiman Fold-thrust belt was driven by an east-west compressional event, giving rise to structures oriented in a north-south direction. The formation of fault propagation folds such as the Drazinda Syncline and Domanda Anticline in the foreland region resulted from east-vergent deformational events. Following this eastward deformation, the west-verging East Domanda Fault was activated, forming a roof thrust within the tectonic wedge beneath the Domanda Anticline.

ZHe dates were obtained from Jurassic to Pliocene sandstone samples collected along the Drazinda-Zhob transect, crossing the Sulaiman Fold-thrust belt. ZHe ages from the Middle Jurassic (Chiltan Formation) and late Jurassic to early Cretaceous (Sembar Formation) samples are completely reset. ZHe ages from the late Cretaceous (Mughal Kot and Pab formations) to early Paleocene (Ranikot Formation) samples are partially reset to unreset; Eocene to Pliocene sample ages are unreset. ZHe ages for the Chiltan Formation range from 3.9-16.2 Ma with an average of 7.6 Ma. The ZHe ages for the Sembar Formation range from 5.5-41.4 Ma with an average of 15.2 Ma. The fully to partially reset ZHe ages for the Mughal Kot Formation range from 4.5 to 64.2 Ma with an average of 31.6 Ma. The ZHe ages of the Pab Formation samples range in age from 25.1-58.6 with an average of 44.9 Ma. A single partially reset ZHe age from the Ranikot Formation is 38.5 Ma. Thick and rapid sedimentation in the Late Cretaceous, Early Eocene and Miocene-Pliocene in the region resulted in sufficient burial of the Chiltan and Sembar formations to reset the ZHe system. Most of the reset ages from the Chiltan and Sembar formations range between 3.9-7.5 Ma, indicating rapid late Miocene to Early Pliocene uplift of the north Sulaiman Fold-thrust belt. This uplift is associated with development of the Sulaiman anticline and the associated Dhana Sar backthrust. Located along the western boundary of the Indian Plate, this area exhibits transpressional tectonics. The dominant east-west compression component coupled with left-lateral wrenching plays a key role in this rapid and young uplift in the north Sulaiman Fold-thrust belt.

How to cite: Ali, N., Sobel, E. R., Ghani, H., and Bernhardt, A.: First constraints on the timing of structural evolution of the north Sulaiman Fold-thrust belt, Pakistan , EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-665, https://doi.org/10.5194/egusphere-egu24-665, 2024.

X2.63
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EGU24-1068
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ECS
Ayan Patsa and Nibir Mandal

Many arcuate orogenic belts display complex patterns of fold structures. However, the kinematics of their development is poorly understood. This study aims to explore the origin of complex fold structures in the Proterozoic mobile belt of Cuddapah in peninsular India. This is a N-S trending thin-skinned fold-thrust belt, showing a spectacular crescent shape with westward convexity. The tectonic reconstructions suggest that the Cuddapah fold-thrust belts (CFTB) evolved through westward indentation of the westerly convex Nellore-Khammam schist belts (NKSB) during the collision between the Indian shield and the Antarctic block, interpreted as a consequence of the Rodinia Supercontinental event in Neoproterozoic time. The westward convergence resulted in the development of highly deformed Nallamalai fold belt (NFB) in the eastern part of CFTB, consisting of orogen-scale overturned folds with arcuate trends as well as higher order west-verging F1 folds on a wide range of spatial scales. Inclined to recumbent F1 folds are coaxially refolded by orogen-parallel F2 folds in outcrop scale. However, the superposition of steeply inclined E-W trending cross-folds (F3) that produced culminations and depressions on F1 and F2 indicates that the belt underwent orogen-parallel shortening in the course of its evolution. We performed laboratory experiments on a scaled representative CFTB model to understand such spatiotemporal evolution of the strain field in the CFTB. Two sets of experiments were run with a constant (2 cm/yr) and a temporally varying (2 cm/yr in Stage I to 1 cm/yr in Stage II) convergence velocity. The experimental results show that the CFTB during the initial periods of shortening undergoes mainly flattening deformations with maximum horizontal instantaneous stretching axes (ISAHmax), describing an arcuate trajectory in the eastern part that conforms to the indentor shape. In the later periods of the experimental runs (albeit at different times in the two experiments), the arcuate shape of the fixed wall causes a SW and NE-directed upper crustal flows from the elevated NE and SW parts of the CFTB, respectively. The flow convergence causes the strain field in the central part of the CFTB to develop a horizontal constriction. This kinematic transition leads to superposition of cross-folds on orogen-parallel folds, manifested in culmination (domes) and depression (basins) structures.

How to cite: Patsa, A. and Mandal, N.: Development of fold styles in the strongly arcuate Cuddapah fold-thrust belt, India: new insights from analogue models, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-1068, https://doi.org/10.5194/egusphere-egu24-1068, 2024.

X2.64
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EGU24-17684
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ECS
Umair Khan, Majid Khan, Wu Shiguo, and Jinwei Gao

The complex interplay between thrust wedge deformation, tectonically-induced fluid overpressures, and the complex phases of wedge-top sedimentary depositional systems in accretionary prisms presents a formidable challenge. The offshore Makran accretionary prism is the world's largest, formed by the convergence of Arabian plate underneath Eurasian plate in the Early Cretaceous, followed by Middle Miocene renewed subduction. The substantial tectonic shortening, imbricate thrust faulting triggered by Middle Miocene renewed subduction, coupled with a continuous influx of sediments, synergistically contributed to the remarkable accumulation of ~7.5 km thick sedimentary succession. In this research, geological and geophysical constraints derived from seismic and borehole stratigraphy, seismic attributes, depth structural maps, isopach maps and 3D structural geological models reveal that Middle Miocene renewed subduction controls thrust wedge deformation, deep fluid overpressure and the deformational pattern of wedge-top sedimentary depositional systems. The seismic data analysis suggested that the basement pre-kinematic Himalayan turbidities depositional system (HTDs) have been tectonically incorporated into the accretionary prism by Middle Miocene renewed subduction, which gave rise to complex folding and N-dipping imbricate thrusting features. These N-dipping imbricate thrust faults initiated sediment underplating and served as major structural pathways for deep fluid overpressure migration, resulting in the formation of fluid escape pipes. The fluid escape pipes exhibit conical and bifurcating geometries with inclination angles of approximately 73°, 90°, and 100°, signifying the upward migration of deep overpressured fluids. Furthermore, the Middle Miocene to Pliocene syn-kinematic piggyback and growth depositional system (PGDs) show progressive thickening (Max ~3600m) towards onshore Makran accretionary prism. It lies unconformable above the pre-kinematic HTDs and carries valuable sedimentation records, growth stratal patterns, onlap terminations, and truncations against growing structures, revealed the timing and spatial deformation of thrust faults in 3D space. In contrast, the Pleistocene to Recent post-kinematic progradational depositional system (PDs) exhibits clinoforms marked by top-lapping, on-lapping, and down-lapping reflection, which are primarily controlled by sediment recycling dynamics and sea level change since Pleistocene. It shows progressive thickening (Max ∼1800m) towards the Makran subduction zone and lies unconformably above the syn-kinematic PGDs. Abridging the analyses, the tectonic reconstruction and deformation mechanisms model shows four phases, e.g. (1) initiation of subduction and accretionary prism formation in Eocene, (2) N-dipping imbricate thrust faults and deep fluid overpressure triggered by Middle Miocene renewed subduction, (3) development of piggyback basins and growth stratal geometries in Middle Miocene to Pliocene, (4) thrust deformation ceases and development of progradational depositional system. This research will provide a strong foundation for comprehending the convergent tectonic mechanisms that shape accretionary prism geometry, tectonically-induced fluid overpressure, and the deformational patterns of wedge-top sedimentary depositional systems in active convergent margins (e.g. Nankai Trough, Cascadia, Barbados, and Hikurangi).

How to cite: Khan, U., Khan, M., Shiguo, W., and Gao, J.: Geodynamics and Structural Evolution of Makran Accretionary Prism, Arabian-Eurasian Convergent Plate Boundary, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-17684, https://doi.org/10.5194/egusphere-egu24-17684, 2024.

X2.65
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EGU24-7329
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ECS
Pauline Meyer, Francois Jouanne, Marie-Pierre Doin, Awais Ahmed, Adnan Alam Awan, and Jean-Louis Mugnier

The northwestern syntax of the Himalaya is a very rapidly deforming area at the edge of the India-Asia collision zone. Therefore, we quantify the current velocity field of the Potwar Plateau – Salt Range fold-and-thrust belt using GNSS horizontal surface velocities and Sentinel-1 interferometry line-of-sight velocities. From this velocity field which indicates a creep of the Potwar Plateau along the Main Himalayan Thrust, we infer a weak subhorizontal décollement level formed by a massive Precambrian salt layer. South of the Plateau, the Salt Range is uplifted along the Salt Range Thrust up to 5 mm/yr. The Kalabagh Fault, which forms the western boundary of the Salt Range and the Potwar Plateau, exhibits a creep rate along fault of 3.3 mm/yr. To characterize the slip distribution and coupling along the faults, we use numerical modelling with a set of dislocations in an elastic half-space. The preferred model shows the presence of a large asperity along the décollement level beneath the Potwar Plateau and several smaller asperities along the eastern basal thrust. These observations are consistent with the occurrence of the 2029 Mirpur earthquake of Mw 5.9 along the eastern part of the décollement level. Along the southern and superficial parts of the Salt Range Thrust, the model indicates a slip rate of 20 mm/yr which is greater than the 14 mm/yr slip rate along the Main Himalayan Thrust at depth. This observation suggests the existence of an internal southward flow of the massive salt layer along the upper part of the Salt Range Thrust. For the Kalabagh strike slip fault, an alternation of coupled and decoupled zones is observed, meaning that this fault can be characterised by creep and asperities where earthquakes and/or slow slip events can occur. Considering the lack of instrumental and historical large magnitude earthquakes in the area since the AD 25 Taxila earthquake, it can be concluded that the Main Himalayan Thrust and the Kalabagh Fault are likely to be affected by large magnitude earthquakes.

How to cite: Meyer, P., Jouanne, F., Doin, M.-P., Ahmed, A., Alam Awan, A., and Mugnier, J.-L.: Present-day quantification of seismic coupling along the décollement level beneath the Potwar Plateau region in Pakistan western Himalaya, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-7329, https://doi.org/10.5194/egusphere-egu24-7329, 2024.

X2.66
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EGU24-16812
Lucas Mesalles and Yuan-Hsi Lee

We present new zircon fission-track age and RSCM peak-metamorphic temperature estimates from the Taiwan slate-belt and northern Palawan. The two regions represent the conjugate margins of the South China Sea that have undergone inversion during two separate collisional episodes, from the latest Miocene until present-day (Taiwan) and in the Middle Miocene (Palawan). In both regions the slate/phyllite and (meta-) sandstone stratigraphic successions have undergone green-schist and sub-green-schist facies peak metamorphic temperatures with a consistent positive correlation between stratigraphic age and metamorphic grade. A similar pattern is observed in the resetting degree of ZFT-ages, with shallow stratigraphic levels displaying unreset to partially-reset ZFT ages, while older strata exposed at the core of regional anticlines are fully reset. Importantly, ZFT young-peak ages (i.e. pooled age of the youngest ZFT grain-age population) and fully reset ZFT-ages are consistent within error, and constrain the initiation of rock cooling and exhumation to 5.9±1.5Ma (weighted mean of 6 pooled ages) in the section studied in the Northern Hsuehshan Range (Taiwan), and to 14.7±0.5Ma (weighted mean of 7 pooled ages) in Northern Palawan. Taken together our data indicates that peak-metamorphic conditions in both regions were reached before the main exhumation event and precede thrust-stacking and topographic growth.  Metamorphism is possibly related to basinal evolution (“burial metamorphism”) during the opening of the South China Sea or to some other tectonothermal events unrelated to the late Cenozoic mountain building processes. Our findings have important implications for the commonly assumed orogenic origin of low-grade metamorphic belts, as this assumption is implicitly included in the tectonic evolutionary models of orogenic development and in models of orogenic gold deposits typically found in slate belts, to name a few.

How to cite: Mesalles, L. and Lee, Y.-H.: Chronology of deformation and metamorphism of an inverted passive margin: evidences of pre-orogenic peak-metamorphic conditions in Taiwan and Palawan island (The Philippines)., EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-16812, https://doi.org/10.5194/egusphere-egu24-16812, 2024.

X2.67
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EGU24-7239
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ECS
Li-Chen Hsieh and Yuan-Hsi Lee

The mechanisms of regional metamorphism in convergent orogens are still debated, with two perspectives on timing—either linked to convergence processes or pre-convergence rifting. The Hsuehshan Range in Taiwan experienced rifting from the Eocene to the Miocene, followed by a convergence since the late Miocene. In this study, we discuss the metamorphic mechanism of the Hsuehshan Range by combining Raman spectroscopy of carbonaceous material (RSCM) for the peak metamorphic temperatures and zircon fission track for the cooling ages, to constrain the burial temperature before the convergence.

In central Hsuehshan Range, RSCM temperatures peaked at 480°C, decreasing northward and southward. In the central-northern region, RSCM temperatures correlated positively with stratigraphic ages. However, in the southern region, east of the Tili Fault, temperatures increased eastward without matching stratigraphic ages.

In some areas, RSCM temperatures (260-300°C) indicate total reset during the late Cenozoic orogeny, while zircon fission-track ages show partial reset. Higher RSCM temperatures (>400°C) lack significant new biotite growth.

We propose that during the rifting stage, strata experienced peak metamorphism, followed by cooling before the late Cenozoic orogeny, thus explaining inconsistencies between RSCM temperatures and zircon fission track ages. The deposit thickness variations in the rifting basin that are contributed to the RSCM temperatures, show no apparent stratigraphic correlation.

How to cite: Hsieh, L.-C. and Lee, Y.-H.: Using Raman Spectroscopy of Carbonaceous Material to Explore the Metamorphic Temperature and its Tectonic Implications in the Southern Hsuehshan Range, Taiwan Orogen, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-7239, https://doi.org/10.5194/egusphere-egu24-7239, 2024.

X2.68
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EGU24-10775
Wolfram Geissler, Peter Klitzke, Graeme Eagles, Lutz Reinhardt, Maximilian Weber, Kai Berglar, and Antonia Ruppel

The Yermak Plateau is a submarine plateau that lies to the north of Svalbard. Strong magnetic anomalies over its northeastern part led early interpretations of an origin by volcanic processes in an oceanic setting, during the formation of the SW Eurasia Basin and the Fram Strait between Svalbard and Greenland. However, subsequent geophysical research delivered evidence that at least the southern and northwestern parts of the plateau might be underlain by extended continental crust. This implies that plate reconstructions for times before the opening of the Eurasia Basin should account for these continental fragments. Up until now, the true northward extent of this microcontinent and neighbouring parts of Svalbard, and their late Cretaceous and Paleogene relative locations, have been incompletely known.

Moreover, during the late Cretaceous and Paleogene, large areas along the Northern Canadian and North Greenland continental margins, as well as the West Svalbard and Southwest Barents Sea continental margins were affected by compressional and strike-slip deformation that culminated in at least two discrete phases together referred to as the Eurekan orogeny, which dates from 53 to 34 Ma. Considering that the continental fragments of Yermak Plateau were located to the north of Greenland or even north of the Canadian Arctic Islands, it is conceivable that the Eurekan deformation might have also left traces within or around the present-day Yermak Plateau.

Here we report on evidence from seismic reflection data from the Sophia Basin, which separates the Yermak Plateau from Svalbard. Evidence for compressional and transpressional features beneath a Neogene-Quaternary sedimentary cover can be correlated to the two Eurekan deformation phases. Reconstructing the Yermak Plateau towards the North Greenland margin by closing the Neogene-Quaternary Lena Trough spreading system based on aeromagnetic data, we also found further evidence for continuity of geological structures between North Greenland and the northwestern Yermak Plateau.

How to cite: Geissler, W., Klitzke, P., Eagles, G., Reinhardt, L., Weber, M., Berglar, K., and Ruppel, A.: Evidence for Eurekan deformation within and around the Yermak Plateau, Arctic Ocean, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-10775, https://doi.org/10.5194/egusphere-egu24-10775, 2024.

X2.69
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EGU24-11050
Peter Klitzke, Wolfram H. Geissler, Lutz Reinhardt, Antonia Ruppel, Martin Engels, and Rüdiger Lutz

The Morris Jesup Plateau is located offshore North Greenland and includes the Morris Jesup Rise in the west and the Morris Jesup Spur in the east. The Yermak Plateau north of Svalbard represents the conjugate margin of the Morris Jesup Plateau. Both margins are separated by the southernmost part of the Eurasia Basin with the Gakkel Ridge. The wider Eurasia Basin started to open in Paleocene-Eocene times. At those times, Greenland moved northwards due to active spreading both in the NE Atlantic and the Labrador Sea. This northward motion of Greenland resulted in the Eurekan compressional deformation between Greenland and Svalbard and limited or strongly influenced the opening of the Eurasia Basin towards the southwest. Only with the cessation of the Eurekan deformation in late Eocene times, the spreading system of the Eurasia Basin advanced southwards and finally separated the Yermak and Morris Jesup plateaus.

While Eurekan deformation is well documented onshore across the West Spitsbergen Fold-and-Thrust Belt and complex thrust and strike-slip zones in North and NE Greenland, only little is known about how these compressional/transpressional structures continue offshore across the North Greenland continental margin towards the Morris Jesup Plateau. Furthermore, the extent to which the Morris Jesup Plateau was affected by extension prior to its separation from the Yermak Plateau in the early Oligocene is poorly resolved. Answering these questions is essential to determine where the Morris Jesup and Yermak plateaus were situated along the North American margin in the late Mesozoic and earliest Cenozoic. Was the opening of the Eurasia Basin compensated by deformation within the plateaus, or did strike-slip movements reactivate the ancient Paleozoic Canadian Arctic transform system? Are there any indications for initial subduction to the North of Greenland as previously proposed on base of potential field data?

Here we report on the first multichannel seismic survey along with magnetic data of the southern Morris Jesup Plateau. The seismic data image transpressional and transtensional deformation likely associated with the two Eurekan deformation episodes, the transition to passive margin evolution as well as glacial sedimentation. We compare the results with two seismic lines of the northern Morris Jesup Plateau, which allow to discuss structural variations along the Morris Jesup Spur. 

How to cite: Klitzke, P., Geissler, W. H., Reinhardt, L., Ruppel, A., Engels, M., and Lutz, R.: Evidence for Eurekan deformation within and around the Morris Jesup Plateau, Arctic Ocean, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-11050, https://doi.org/10.5194/egusphere-egu24-11050, 2024.

X2.70
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EGU24-13635
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ECS
Lourenço Steel Hart, Ícaro Dias da Silva, Aitor Cambeses, João C. Duarte, and Manuel Francisco Pereira

Orogenesis involves a continuum of complex natural phenomena within the context of the Wilson Cycle, the backbone of modern plate tectonics. While topographic effects of present-day orogenic cycles are readily visible, eroded old orogens represent windows that expose the crust's interior and facilitate the study of complex lithospheric processes.

The object of this research lies within the Devonian-Carboniferous Variscan collisional orogen that extends from Southern Europe to Northern Africa. This orogenic belt resulted from the convergence and collision between the passive margin of north Gondwana and the active margin of southern Laurussia, forming the Pangea Supercontinent. The Iberian Massif, located in the core of Pangaea, is one of the best exposures of the Variscan orogen in Europe, and a unique natural laboratory to study deep-to-surface geodynamic phenomena. Studying this sector of the Pangea supercontinent raises new important questions about how modern collisional orogens evolve and how their crustal architecture develops.

Field and analytical data compiled in the last 20-30 years in Iberia has revealed a complex basin-cover architecture derived from the deformation and metamorphism of the Ediacaran to Carboniferous stratigraphy. Ongoing research in a critical and representative region of the SW Iberian Massif (i.e. Ossa-Morena Zone), reveals a close relationship between the deformation, metamorphism, magmatism and sedimentary processes involved in deep to shallow lithospheric dynamics, during both orogenic thickening and gravitational collapse. 

The systematic study of key outcrops was performed, to define first-order geological contacts between major tectono-metamorphic, stratigraphic and magmatic units. This information made it possible to define the architecture of the crust along a transverse across the central region of the Ossa-Morena Zone (Estremoz, Portugal). With the structural relationships well defined, the main units were sampled to control the ages of the orogenic events and to correlate the tectono-metamorphic fabrics found in the Variscan basement regionally. This research focused on SW Iberian Massif will give important constraints to develop state-of-the-art conceptual and numerical models of the tectonic evolution of the Variscan Orogen during the assembly of the Pangaea supercontinent. The combination of field and petrography data with numerical modelling can be very useful for better understanding the role of different lithospheric processes in orogenic building and gravitational collapse as Supercontinents are formed.

 

This work was funded by the Portuguese Fundação para a Ciência e a Tecnologia (FCT) I.P./MCTES through national funds (PIDDAC) – UIDB/50019/2020 (https://doi.org/10.54499/UIDB/50019/2020), through the scholarship UI/BD/154616/2023 and through UIDP/50019/2020 (https://doi.org/10.54499/UIDP/50019/2020), LA/P/0068/2020 (https://doi.org/10.54499/LA/P/0068/2020) and DL57/2016/CP1479/CT0030 (https://doi.org/10.54499/DL57/2016/CP1479/CT0030). M.F. Pereira acknowledges financial support from the FCT project (grant No. FCT/UIDB/ 04683/2020-ICT).

How to cite: Steel Hart, L., Dias da Silva, Í., Cambeses, A., Duarte, J. C., and Pereira, M. F.:  The northern Gondwana margin and Pangaea tectonics revisited: Preliminary results in the Ossa-Morena Zone (SW Iberian Massif), EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-13635, https://doi.org/10.5194/egusphere-egu24-13635, 2024.