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The rockslide systems along the Gepatsch reservoir in the Kaunertal valley are among the best investigated and monitored slopes in the Alps since TIWAG began operating the Kaunertal power plant in 1964. The rockslide systems consist of several individual slabs with variable activity. Only the deformation characteristics of the Hochmais slab shows transient behaviour and depends on external influences such as reservoir operation. No effects from heavy precipitation or snowmelt on the deformation characteristics were observed prior to 2019. The large amount of precipitation accumulated as snow in the winter of 2018/2019, combined with cool spring weather and low reservoir level, resulted in an increased deformation rate of the Hochmais slab due to excessive snowmelt in June 2019. The maximum deformation rate of several mm per week was the highest activity of the Hochmais slab since the end of the first impoundment period in 1966. In response to this exceptional situation, the engineers at TIWAG, in conjunction with external experts and the competent authorities, temporarily restricted the reservoir operation. The increased rates of deformation of the Hochmais slab decreased to the expected level in the late summer of 2019 [ABSTRACT FROM AUTHOR]

Worldwide, Ultrahigh Pressure (UHP) oceanic units are rare and to date only three were recognized: Tianshan (China), and Lago di Cignana and Lago Superiore Unit (Western Alps, Italy). The UHP oceanic units represent the only geological object directly exhumed from mantle depth and they record fundamental information about processes occurring in the deepest portions of the subduction interface. In this work, we describe the occurrence of a new UHP oceanic unit within the Western Alps (mid Susa Valley, Internal Piedmont Zone). We here report the finding of a UHP index mineral, i.e., coesite and we provide a detailed study of garnet inclusions in metapelites and metabasites part of the meta-sedimentary cover of the meta-ophiolites cropping out in the mid Susa Valley. The samples were investigated via optical microscope, Raman spectroscopy, Elastic Geothermometry and classic thermometry (Zr-in-rutile) in order to constrain the P-T evolution of the area. The finding of a new UHP unit in the Internal Piedmont Zone, together with the already described Lago di Cignana and Lago Superiore units, points towards the possible existence of a UHP oceanic slice that reached a similar peak-P (i.e., the return point) along the same subduction gradient. This slice was then removed from the slab and dismembered during exhumation, and it is now exposed as coesite-bearing units juxtaposed with lower pressure eclogite-facies ophiolites. Moreover, the large occurrence of coesite along the entire Internal Piedmont Zone significantly increases the extension of the UHP oceanic units. Hence, the model of a localized non-lithostatic pressure is at the state of the art difficult to apply to the oceanic units of the Western Alps. • We report a new occurrence of coesite within the eclogitic meta-ophiolites (Internal Piedmont Zone) of the Western Alps. • Elastic Geobarometry and Zr-in-rutile thermometry results confirm the PT path proposed in literature with pseudosections. • We propose a unique UHP level inside oceanic slab by linking the three UHP oceanic units outcropping on the Western Alps. [ABSTRACT FROM AUTHOR]

The stratigraphic development of foreland basins has mainly been related to surface loading in the adjacent orogens, whereas the control of slab loads on these basins has received much less attention. This has also been the case for interpreting the relationships between the Oligocene to Micoene evolution of the European Alps and the North Alpine foreland basin or Molasse basin. In this trough, periods of rapid subsidence have generally been considered as a response to the growth of the Alpine topography, and thus to the construction of larger surface loads. However, such views conflict with observations where the surface growth in the Alps has been partly decoupled from the subsidence history in the basin. In addition, surface loads alone are not capable of explaining the contrasts in the stratigraphic development particularly between its central and eastern portions. Here, we present an alternative view on the evolution of the Molasse basin. We focus on the time interval between c. 30 and 15 Ma and relate the basin-scale development of this trough to the subduction processes, and thus to the development of slab loads beneath the European Alps. At 30 Ma, the western and central portions of this basin experienced a change from deep marine underfilled (Flysch stage) to overfilled terrestrial conditions (Molasse stage). During this time, however, a deep marine Flysch-type environment prevailed in the eastern part of the basin. This was also the final sedimentary sink as sediment was routed along the topographic axis from the western/central to the eastern part of this trough. We interpret the change from basin underfill to overfill in the western and central basin as a response to oceanic lithosphere slab-breakoff beneath the Central and Western Alps. This is considered to have resulted in a growth of the Alpine topography in these portions of the Alps, an increase in surface erosion and an augmentation in sediment supply to the basin, and thus in the observed change from basin underfill to overfill. In the eastern part of the basin, however, underfilled Flysch-type conditions prevailed until 20 Ma, and subsidence rates were higher than in the western and central parts. We interpret that high subsidence rates in the eastern Molasse occurred in response to slab loads beneath the Eastern Alps, where the subducted oceanic slab remained attached to the European plate and downwarped the plate in the East. Accordingly, in the central and western parts, the growth of the Alpine topography, the increase in sediment flux and the change from basin underfill to overfill most likely reflect the response to slab delamination beneath the Central Alps. In contrast, in the eastern part, the possibly subdued topography in the Eastern Alps, the low sediment flux and the maintenance of a deep marine Flysch-type basin records a situation where the oceanic slab was still attached to the European plate. The situation changed at 20 Ma, when the eastern part of the basin chronicled a change from deep marine (underfilled) to shallow marine and then terrestrial (overfilled conditions). During the same time, subsidence rates in the eastern basin decreased, deformation at the Alpine front came to a halt and sediment supply to the basin increased possibly in response to a growth of the topography in the Eastern Alps. This was also the time when the sediment routing in the basin axis changed from an east-directed sediment dispersal prior to 20 Ma, to a west-oriented sediment transport thereafter and thus to the opposite direction. We relate these changes to the occurrence of oceanic slab breakoff beneath the Eastern Alps, which most likely resulted in a rebound of the plate, a growth of the topography in the Eastern Alps and a larger sediment flux to the eastern portion of the basin. Beneath the Central and Western Alps, however, the continental lithosphere slab remained attached to the European plate, thereby resulting in a continued downwarping of the plate in its central and western portions. This plate downwarping beneath the central and western Molasse together with the rebound of the foreland plate in the East possibly explains the inversion of the drainage direction. We thus propose that slab loads beneath the Alps were presumably the most important drivers for the development of the Molasse basin at the basin scale. [ABSTRACT FROM AUTHOR]

Based on recent results of AlpArray, we propose a new model of Alpine collision that involves subduction and detachment of thick (∼ 180 km) European lithosphere. Our approach combines teleseismic P-wave tomography and existing local earthquake tomography (LET), allowing us to image the Alpine slabs and their connections with the overlying orogenic lithosphere at an unprecedented resolution. The images call into question the conventional notion that downward-moving lithosphere and slabs comprise only seismically fast lithosphere. We propose that the European lithosphere is heterogeneous, locally containing layered positive and negative Vp anomalies of up to 5 %–6 %. We attribute this layered heterogeneity to seismic anisotropy and/or compositional differences inherited from the Variscan and pre-Variscan orogenic cycles rather than to thermal anomalies. The lithosphere–asthenosphere boundary (LAB) of the European Plate therefore lies below the conventionally defined seismological LAB. In contrast, the lithosphere of the Adriatic Plate is thinner and has a lower boundary approximately at the base of strong positive Vp anomalies at 100–120 km. Horizontal and vertical tomographic slices reveal that beneath the central and western Alps, the European slab dips steeply to the south and southeast and is only locally still attached to the Alpine lithosphere. However, in the eastern Alps and Carpathians, this slab is completely detached from the orogenic crust and dips steeply to the north to northeast. This along-strike change in attachment coincides with an abrupt decrease in Moho depth below the Tauern Window, the Moho being underlain by a pronounced negative Vp anomaly that reaches eastward into the Pannonian Basin area. This negative Vp anomaly is interpreted as representing hot upwelling asthenosphere that heated the overlying crust, allowing it to accommodate Neogene orogen-parallel lateral extrusion and thinning of the ALCAPA tectonic unit (upper plate crustal edifice of Alps and Carpathians) to the east. A European origin of the northward-dipping, detached slab segment beneath the eastern Alps is likely since its down-dip length matches estimated Tertiary shortening in the eastern Alps accommodated by originally south-dipping subduction of European lithosphere. A slab anomaly beneath the Dinarides is of Adriatic origin and dips to the northeast. There is no evidence that this slab dips beneath the Alps. The slab anomaly beneath the Northern Apennines, also of Adriatic origin, hangs subvertically and is detached from the Apenninic orogenic crust and foreland. Except for its northernmost segment where it locally overlies the southern end of the European slab of the Alps, this slab is clearly separated from the latter by a broad zone of low Vp velocities located south of the Alpine slab beneath the Po Basin. Considered as a whole, the slabs of the Alpine chain are interpreted as highly attenuated, largely detached sheets of continental margin and Alpine Tethyan oceanic lithosphere that locally reach down to a slab graveyard in the mantle transition zone (MTZ). [ABSTRACT FROM AUTHOR]

We perform a teleseismic P-wave travel-time tomography to examine the geometry and structure of subducted lithosphere in the upper mantle beneath the Alpine orogen. The tomography is based on waveforms recorded at over 600 temporary and permanent broadband stations of the dense AlpArray Seismic Network deployed by 24 different European institutions in the greater Alpine region, reaching from the Massif Central to the Pannonian Basin and from the Po Plain to the river Main. Teleseismic travel times and travel-time residuals of direct teleseismic P waves from 331 teleseismic events of magnitude 5.5 and higher recorded between 2015 and 2019 by the AlpArray Seismic Network are extracted from the recorded waveforms using a combination of automatic picking, beamforming and cross-correlation. The resulting database contains over 162 000 highly accurate absolute P-wave travel times and travel-time residuals. For tomographic inversion, we define a model domain encompassing the entire Alpine region down to a depth of 600 km. Predictions of travel times are computed in a hybrid way applying a fast TauP method outside the model domain and continuing the wave fronts into the model domain using a fast marching method. We iteratively invert demeaned travel-time residuals for P-wave velocities in the model domain using a regular discretization with an average lateral spacing of about 25 km and a vertical spacing of 15 km. The inversion is regularized towards an initial model constructed from a 3D a priori model of the crust and uppermost mantle and a 1D standard earth model beneath. The resulting model provides a detailed image of slab configuration beneath the Alpine and Apenninic orogens. Major features are a partly overturned Adriatic slab beneath the Apennines reaching down to 400 km depth still attached in its northern part to the crust but exhibiting detachment towards the southeast. A fast anomaly beneath the western Alps indicates a short western Alpine slab whose easternmost end is located at about 100 km depth beneath the Penninic front. Further to the east and following the arcuate shape of the western Periadriatic Fault System, a deep-reaching coherent fast anomaly with complex internal structure generally dipping to the SE down to about 400 km suggests a slab of European origin limited to the east by the Giudicarie fault in the upper 200 km but extending beyond this fault at greater depths. In its eastern part it is detached from overlying lithosphere. Further to the east, well-separated in the upper 200 km from the slab beneath the central Alps but merging with it below, another deep-reaching, nearly vertically dipping high-velocity anomaly suggests the existence of a slab beneath the eastern Alps of presumably the same origin which is completely detached from the orogenic root. Our image of this slab does not require a polarity switch because of its nearly vertical dip and full detachment from the overlying lithosphere. Fast anomalies beneath the Dinarides are weak and concentrated to the northernmost part and shallow depths. Low-velocity regions surrounding the fast anomalies beneath the Alps to the west and northwest follow the same dipping trend as the overlying fast ones, indicating a kinematically coherent thick subducting lithosphere in this region. Alternatively, these regions may signify the presence of seismic anisotropy with a horizontal fast axis parallel to the Alpine belt due to asthenospheric flow around the Alpine slabs. In contrast, low-velocity anomalies to the east suggest asthenospheric upwelling presumably driven by retreat of the Carpathian slab and extrusion of eastern Alpine lithosphere towards the east while low velocities to the south are presumably evidence of asthenospheric upwelling and mantle hydration due to their position above the European slab. [ABSTRACT FROM AUTHOR]

Based on recent results of AlpArray, we propose a new model of Alpine collision that involves subduction and detachment of thick (180-200 km) European tectosphere. Our approach combines teleseismic P-wave tomography and existing Local Earthquake Tomography (LET) allowing us to image the Alpine slabs and their connections with the overlying orogenic crust at an unprecedented resolution. The images call into question the conventional notion that slabs comprise only seismically fast lithosphere and suggest that the mantle of the downgoing European Plate is heterogeneous, containing both positive and negative Vp anomalies of up to 5-6%. We interpret these as compositional rather than thermal anomalies, inherited from the Variscan and pre-Variscan orogenic cycles. They make up a kinematic entity referred to as tectosphere, which presently dips beneath the Alpine orogenic front. In contrast to the European Plate, the tectosphere of the Adriatic Plate is thinner (100-120 km) and has a lower boundary approximately at the interface between positive and negative Vp anomalies. Horizontal and vertical tomographic slices reveal that beneath the Central and Western Alps, the downgoing European tectospheric slab dips steeply to the S and SE and is only locally still attached to the Alpine crust. However, in the Eastern Alps and Carpathians, the European slab is completely detached from the orogenic crust and dips steeply to the N-NE. This along-strike change in attachment coincides with an abrupt decrease in Moho depth below the Tauern Window, the Moho being underlain by a pronounced negative Vp anomaly that reaches eastward into the Pannonian Basin area. This negative Vp anomaly is interpreted to represent hot upwelling asthenosphere that was instrumental in accommodating Neogene orogen-parallel lateral extrusion of the ALCAPA tectonic unit (upper plate crustal edifice of Alps and Carpathians) to the east. A European origin of the northward-dipping, detached slab segment beneath the Eastern Alps is likely since its imaged down-dip length (300-500 km) matches estimated Tertiary shortening in the Eastern Alps accommodated by south-dipping subduction of European tectosphere. A slab anomaly beneath the Dinarides is of Adriatic origin and dips to the northeast. There is no evidence that this slab dips beneath the Alps. The slab anomaly beneath the northern Apennines, also of Adriatic origin, hangs subvertically and is detached from the Apenninic orogenic crust and foreland. Except for its northernmost segment where it locally overlies the southern end of the European slab of the Alps, this slab is clearly separated from the latter by a broad zone of low Vp velocities located south of the Alpine slab beneath the Po Basin. Considered as a whole, the slabs of the Alpine chain are interpreted as attenuated, largely detached sheets of continental margin and Alpine Tethyan lithosphere that locally reach down to a slab graveyard in the Mantle Transition Zone (MTZ). [ABSTRACT FROM AUTHOR]

We perform a teleseismic P-wave traveltime tomography to examine the geometry and structure of subducted lithosphere in the upper mantle beneath the Alpine orogen. The tomography is based on waveforms recorded at over 600 temporary and permanent broadband stations of the dense AlpArray Seismic Network deployed by 24 different European institutions in the greater Alpine region, reaching from the Massif Central to the Pannonian Basin and from the Po plain to the river Main. Teleseismic traveltimes and traveltime residuals of direct teleseismic P-waves from 331 teleseismic events of magnitude 5.5 and higher recorded between 2015 and 2019 by the AlpArray Seismic Network are extracted from the recorded waveforms using a combination of automatic picking, beamforming and cross-correlation. The resulting database contains over 162.000 highly accurate absolute P-wave traveltimes and traveltime residuals. For tomographic inversion, we define a model domain encompassing the entire Alpine region down to a depth of 600 km. Outside this domain, a laterally homogeneous standard earth model is assumed. Predictions of traveltimes are computed in a hybrid way applying a fast Tau-P method outside the model domain and continuing the wavefronts into the model domain using a fast marching method. For teleseismic inversion, we iteratively invert demeaned traveltime residuals for P-wave velocities in the model domain using a regular discretization with an average lateral spacing of about 25 km and a vertical spacing of 15 km. The inversion is regularized towards an initial model constructed from an a priori model of the crust and uppermost mantle and a standard earth model beneath. The resulting model provides a detailed image of slab configuration beneath the Alpine and Apenninic orogens. Major features are an overturned Adriatic slab beneath the Apennines reaching down to 400 km depth still attached in its northern part to the crust but exhibiting detachment towards the southeast. A fast anomaly beneath the western Alps indicates a short western Alpine slab that ends at about 100 km depth close to the Penninic front. Further to the east and following the arcuate shape of the western Periadriatic Fault System, a deep-reaching coherent fast anomaly with complex interior stucture generally dipping to the SE down to about 400 km suggests a slab of European origin extending eastward to the Giudicarie fault. This slab is detached from overlying lithosphere at its eastern end below a depth of about 100 km. Further to the east, well-separated from the slab beneath the western and central Alps, another deep-reaching, nearly vertically dipping high-velocity anomaly suggests the existence of a slab beneath the Eastern Alps of presumably European origin which is completely detached from the orogenic root. Our image of this slab does not require a polarity switch because of its nearly vertical dip and full detachment from the overlying lithosphere. Fast anomalies beneath the Dinarides are weak and concentrated to the northernmost part and shallow depths. Low-velocity regions surrounding the fast anomalies beneath the Alps to the west and northwest follow the same dipping trend as the overlying fast ones, indicating a kinematically coherent subducting tectosphere in this region. In contrast, low-velocity anomalies to the east suggest asthenospheric upwelling presumably driven by retreat of the Carpathian slab and extrusion of eastern Alpine lithosphere towards the east while low velocities to the south are presumably evidence of asthenospheric upwelling and mantle hydration due to the backarc position behind the European slab. [ABSTRACT FROM AUTHOR]

In this study, we present an estimate of the gravity signal of the slabs beneath the Alpine mountain belt. Estimates of the gravity effect of the subducting slabs are often omitted or simplified in crustal-scale models. The related signal is calculated here for alternative slab configurations at near-surface height and at a satellite altitude of 225 km. We apply three different modelling approaches in order to estimate the gravity signal from the subducting slab segments: (i) direct conversion of upper mantle seismic velocities to density distribution, which are then forward calculated to obtain the gravity signal; (ii) definition of slab geometries based on seismic crustal thickness and high-resolution upper mantle tomography for two competing slab configurations – the geometries are then forward calculated by assigning a constant density contrast and slab thickness; (iii) accounting for compositional and thermal variations with depth within the predefined slab geometry. Forward calculations predict a gravity signal of up to 40 mGal for the Alpine slab configuration. Significant differences in the gravity anomaly patterns are visible for different slab geometries in the near-surface gravity field. However, different contributing slab segments are not easily separated, especially at satellite altitude. Our results demonstrate that future studies addressing the lithospheric structure of the Alps should have to account for the subducting slabs in order to provide a meaningful representation of the geodynamic complex Alpine area. [ABSTRACT FROM AUTHOR]

Many convergent orogens, such as the eastern European Alps, display an asymmetric doubly vergent wedge geometry. In doubly vergent orogens, deepest exhumation occurs above the retro‐wedge. Deep‐seismic interpretations depict the European plate dipping beneath the Adriatic, suggesting the pro‐wedge location on the north side of the orogen. Our new thermochronometer data across the Eastern Alps confirm distinct shifts in the locus of exhumation associated with orogen‐scale structural reorganizations. Most importantly, we find a general Mid‐Miocene shift in exhumation (in the Tauern Window and the Southern Alps) and focus of modern seismicity across the Southern Alps. Taken together, these observations suggest a subduction polarity reversal at least since the Mid‐Miocene such that the present‐day pro‐wedge is located on the south side of the Alps. We propose a transient tectonic state of a slow‐and‐ongoing slab reversal coeval with motion along the Tauern Ramp, consistent with a present‐day northward migration of drainage divides. Plain Language Summary: When tectonic plates collide, they bend downwards and form two lithospheric wedges dipping in opposite directions, such as in the Eastern Alps. We present new crustal cooling data along a transect in the Eastern Alps confirming that surface rocks across the central Tauern Window originated from the deepest structural levels along the transect. South of the Tauern Window rocks were exhumed from higher depths compared to those north of it and were exhumed more recently, while seismic activity is also focused across the Southern Alps. These observations suggest a subduction polarity reversal because they are inconsistent with the original southern and northern locations of overriding and subducting plates, respectively, >15 million years ago. This interpretation is contrary to lithosphere‐scale tomography that shows no change in subduction polarity. Therefore, we propose a transient tectonic state, that is, a slow‐and‐ongoing subduction polarity reversal that initiated when Tauern Window rocks began their steep ascent to the surface along a deep‐seated fault known as the Tauern Ramp. This study bridges observations in the mantle, crust and on the surface over geologic time. Key Points: Thermochronologic data in the Eastern Alps is consistent with a transient tectonic state toward complete slab reversalThe pro‐wedge has switched from north to south of the Periadriatic Fault along TRANSALPMid‐Miocene motion along the Tauern Ramp is the consequence of slab‐reversal [ABSTRACT FROM AUTHOR]

Buoyancy forces associated with subducting lithosphere control the dynamics of convergent margins. In the postcollisional stage these forces are significantly reduced, yet mountain building and seismicity are ongoing, albeit at lower rates. We leverage advances of a newly developed seismo‐thermo‐mechanical modeling approach to simulate tectonic and seismicity processes in a self‐driven subduction and continental collision setting. We demonstrate that the rearrangement of forces due to slab breakoff, in the postcollisional stage, causes bending and rollback of the residual slab, suction forces, and mantle traction at the base of the upper plate, while stress coupling transfers to the shallow crust. Our results provide an explanation for the postcollisional evolution of the Central Alps, where the so‐called Slab Rollback Orogeny model explains the slow yet persistent upper plate advance, the height of the mountain range, and a seismicity pattern consistent with the different tectonic regimes throughout the orogen. Plain Language Summary: A long‐standing debate in tectonophysics evolves around whether vertical or horizontal forces are the primary drivers of mountain building processes. Here we explore this problem using 2‐D numerical models in a generic subduction and continental collision setting. Our results show how the postcollisional evolution of the orogen is controlled by a slow, but persistent, sinking and bending of the postbreakoff residual slab. The resulting seismicity pattern shows a broad pattern of different style of faulting, which are consistent with the local tectonic regimes. We find good correlations between our numerical results and the previously conflicting tectonic observations in the Central Alps and the adjacent foreland basin. Our results thus support the hypothesis that the postbreakoff remaining slab exerts a first‐order control on the motions and deformations of collisional orogens. Key Points: Two‐dimensional seismo‐thermo‐mechanical modeling is performed to investigate the driving forces during the postcollisional stagesPost‐breakoff residual slab proves sufficient to sustain slab rollback and retreat of the entire orogenThe proposed scenario is consistent with the postcollisional seismotectonic evolution of the central European Alps [ABSTRACT FROM AUTHOR]

After the onset of plate collision in the Alps, at 32–34 Ma, the deep structure of the orogen is inferred to have changed dramatically: European plate break-offs in various places of the Alpine arc, as well as a possible reversal of subduction polarity in the eastern Alps have been proposed. We review different high-resolution tomographic studies of the upper mantle and combine shear- and body-wave models to assess the most reliable geometries of the slabs. Several hypotheses for the tectonic evolution are presented and tested against the tomographic model interpretations and constraints from geologic and geodetic observations. We favor the interpretation of a recent European slab break-off under the western Alps. In the eastern Alps, we review three published scenarios for the subduction structure and propose a fourth one to reconcile the results from tomography and geology. We suggest that the fast slab anomalies are mainly due to European subduction; Adriatic subduction plays no or only a minor role along the Tauern window sections, possibly increasing towards the Dinarides. The apparent northward dip of the slab under the eastern Alps may be caused by imaging a combination of Adriatic slab, from the Dinaric subduction system, and a deeper lying European one, as well as by an overturned, retreating European slab. [ABSTRACT FROM AUTHOR]

Carbonate-silicate interaction within subduction channels influences the chemical and physical properties of subducting carbon and is crucial to understanding the fate of carbonates in subduction zones. However, geochemical evidence for such interaction is still limited. Here we investigate zinc isotopes (expressed as δ 66 Zn JMC-Lyon) to decipher potential carbonate-silicate interaction in subducting slabs given the remarkable Zn isotopic difference between silicate and carbonate components. A suite of high- to ultrahigh-pressure metasediments containing variable amounts of carbonates from the Schistes Lustrés nappe (western Alps) record subduction processes to various depths (∼15–90 km) in a cool geothermal condition (∼8 °C/km). Despite a broad range of metamorphic grades (0.8–2.9 GPa and 300–630 °C) and carbonate contents (0–49 wt%), the bulk metasediments have nearly constant δ 66 Zn values (av. 0.21 ± 0.05 ‰ , 2sd, n = 12), which are indistinguishable from their putative protoliths (0.25 ± 0.07 ‰ , 2sd, n = 5). The lack of systematic variation of bulk sediment δ 66 Zn with metamorphic grades implies a limited transfer of Zn during prograde metamorphism. Therefore, sediments will preserve their original Zn isotopic compositions after subduction into the mantle. By contrast, the carbonate components in sediments obtained by leaching exhibit a progressive decline in δ 66 Zn from 0.82 ± 0.01 ‰ to 0.20 ± 0.04 ‰ and a modest increase in Zn concentration with pressure. These variations are best interpreted as a result of prolonged closed-system Zn isotopic exchange between isotopically heavy carbonates and light silicate components in the subducting slab. Our results demonstrate that a considerable amount of carbonates in subducting sediments can be retained at least down to the depths of the sub-arc mantle (>90 km). The strong pressure-dependent Zn isotopic fractionation (R 2 = 0.87) during carbonate-silicate interaction makes Zn isotopes a novel proxy for the storage depth of subducting carbonates. • A systematic zinc isotope study on western Alpine metasediments. • Prograde metamorphism has limited impact on Zn isotopes of bulk subducting sediments. • Variation of δ 66 Zn in carbonates reflects interaction with silicates in a closed system. • Zn isotopes are an indicator for the storage depth of subducting carbonates. [ABSTRACT FROM AUTHOR]

Periadriatic Alpine magmatism has long been attributed to slab breakoff after Adria–Europe continental collision, but this interpretation is challenged by geophysical data suggesting the existence of a continuous slab. Here, we shed light on this issue based on a comprehensive dataset of zircon U–Pb ages and Hf isotopic compositions from the main western Periadriatic intrusives (from Traversella to Adamello). Our zircon U–Pb data provide the first evidence of Eocene magmatism in the Western Alps (42–41 Ma in Traversella), and demonstrate that magmatism started synchronously in different segments of the Alpine belt, when subduction was still active. Zircon U–Pb ages define younging trends perpendicular to the strike of the European slab, suggesting a progressive Eocene–Oligocene slab steepening. We propose that slab steepening enhanced the corner flow. This process was more effective near the torn edge of the European slab, and triggered Periadriatic magmatism in the absence of slab breakoff. [ABSTRACT FROM AUTHOR]

HP/UHP and LT metamorphic units that commonly occur in the inner parts of mountain belts result from the subduction of continental and oceanic material, most often exhumed prior to continental collision. The prograde pressure-temperature history of HP-UHP rocks strongly depends on the convergence rate and on the subduction zone geometry. The maximum pressure recorded provides a proxy for the depth of shearing off and stacking of HP metamorphic nappes. A 2-D thermal model of continental subduction at lithospheric scale is used to compute the length and pressure peak of detached HP metamorphic units as a function of the slab dip angle and the convergence rate. Model results are applied to the metamorphic nappe pile of the inner Alps. A mean convergence rate of 1 cm/year during the subduction of the Briançonnais terrane is indicated by the paleogeographic reconstructions between 46 and 38 Ma. On this basis, the available petrological data and lengths of metamorphic units are used to compute the variations of the slab dip angle. The slab dip angle is shown to increase, from the northeast to the southwest, along the Alpine arc with estimated values of 20° for Suretta, 30-45° for Monte Rosa and Gran Paradiso, and 60° for Dora Maira. From Eocene to Oligocene times, the increase in slab dip angle is controlled by changes of buoyancy, due to the spatial configuration of the Valaisan trough and the incoming of crustal material within the subduction zone. [ABSTRACT FROM AUTHOR]

Some (ultra)high-pressure metamorphic rocks that formed during continental collision preserve relict minerals, indicating a two-stage evolution: first, subduction to mantle depths and exhumation to the lower-crustal level (with simultaneous cooling), followed by intensive heating that can be characterized by a β-shaped pressure–temperature–time (P–T–t) path. Based on a two-dimensional (2D) coupled petrological–thermomechanical tectono-magmatic numerical model, we propose a possible sequence of tectonic stages that could lead to these overprinting metamorphic events along an orogenic β-shaped P–T–t path: the subduction and exhumation of continental crust, followed by slab retreat that leads to extension and subsequent asthenospheric upwelling. During the last stage, the exhumed crustal material at the crust–mantle boundary undergoes heating from the underlying hot asthenospheric mantle. This slab rollback scenario is further compared numerically with the classical continental collision scenario associated with slab breakoff, which is often used to explain the late heating impulse in the collisional orogens. The mantle upwelling occurring in the experiments with slab breakoff, which is responsible for the heating of the exhumed crustal material, is not related to the slab breakoff but can be caused either by slab bending before slab breakoff or by post-breakoff exhumation of the subducted crust. Our numerical modeling predictions align well with a variety of orogenic P–T–t paths that have been reported from many Phanerozoic collisional orogens, such as the Variscan Bohemian Massif, the Triassic Dabie Shan, the Cenozoic Northwest Himalaya, and some metamorphic complexes in the Alps. [ABSTRACT FROM AUTHOR]

The process of continent–continent collision in shaping mountain ranges and adjacent foreland basins has been discussed for many decades. The orogeny driving forces — whether vertical or horizontal — are central for our understanding and it seemed settled in favor of horizontal forces. For the central European Alps, however, this traditional concept fails to explain first-order observations of the mountain belt. Recent stratigraphic, palaeo-altimetry and lithosphere structural evidence suggest that a Slab Rollback Orogeny model is capable of explaining the construction of thick nappe successions and the large-scale evolution of the Swiss Alps (Kissling and Schlunegger, 2018). This new concept questions the traditionally assumed bulldozing effect of Adria indenter as a necessary component of the dynamic system and proposes the buoyancy forces of the postulated post-collisional rollback is sufficient to drive the evolution and to shape the Central Alps as we know them today. Here we explore these challenging questions using a high-resolution, rheologically consistent, two-dimensional visco-elasto-plastic thermo-mechanical numerical model (Dal Zilio et al., 2018), which simulates both tectonic and seismic processes in a subduction and subsequent continental collisional setting. Our numerical experiments reproduce the self-driven stages of oceanic subduction, continent-continent collision, and spontaneous oceanic lithosphere slab breakoff. The post-collisional evolution of the orogen shows how slow — but persistent — flexural bending of the post-breakoff residual slab in combination with the crustal delamination control the most recent stage of the orogen. Bending-related slab suction and coeval development of crust-mantle and intracrustal delamination and nappe stacking through the slab bending zone, leads to the appearance of crustal shortening on the foreland basin, and widening of the orogen. We find good correlations of our numerical results with the previously conflicting tectonic observations in the Central Alps and the foreland (Molasse) basin. In particular, we discuss how the current crustal seismicity pattern implies the occurrence of extensional forces at work beneath the Molasse Basin and within the Alps. Our results thus support the emerging hypothesis that the remaining slab exerts a first-order control on the motions and deformations of the orogen. In light of these results, we propose that the tectonic history of the Central Alps does require an alternative view.Dal Zilio, L., van Dinther, Y., Gerya, T. V., & Pranger, C. C. (2018). Seismic behaviour of mountain belts controlled by plate convergence rate. Earth and Planetary Science Letters, 482, 81-92.Kissling, E., & Schlunegger, F. (2018). Rollback orogeny model for the evolution of the Swiss Alps. Tectonics, 37(4), 1097-1115. [ABSTRACT FROM AUTHOR]

The ongoing formation of the alpine mountain belt is a major indicator of the active geological processes in the Mediterranean that for example causes volcanism in Italy as well as considerable hazard. To understand this complex system the European project AlpArray, with the German contribution 4D-MB, was funded in order to investigate the structure, dynamics and geology of the alpine area in more detail and through all scales. We focus on the large scale geodynamic processes that drive this complex system of multiple subduction zones, ranging from the surface to the mantle. We will present new preliminary results obtained by thermomechanical modelling of the area. The models are based on recent large-scale seismological studies. As such we take into account complex slab gemoetries slab gaps and delaminated slabs. The Moho is created as a combination of Tesauro et al. (2008), Spada et al. (2013) and Molinari et al. (2011). We present several instantaneous simulations with varying temperature structure, rheological parameters, boundary conditions and slab configurations, unraveling the sensitivity of the surface velocity to the existence and shape of slabs in order to answer, e.g. the question which slab is most important for the rotation of Adria? We compare the results to measured surface observables like GPS-velocities or stress directions. In addition we automatically optimize the misfit between the data and the simulation results using adjoint gradient based inversions for the rheology of the lithosphere and the slabs. Tesauro, Magdala, Mikhail K. Kaban, and Sierd APL Cloetingh. "EuCRUST‐07: A new reference model for the European crust." Geophysical Research Letters 35.5 (2008).Spada, M., et al. "Combining controlled-source seismology and receiver function information to derive 3-D Moho topography for Italy." Geophysical Journal International 194.2 (2013): 1050-1068.Molinari, Irene, and Andrea Morelli. "EPcrust: a reference crustal model for the European Plate." Geophysical Journal International 185.1 (2011): 352-364. [ABSTRACT FROM AUTHOR]

Despite being one of the most-studied orogens on Earth, recent deep-seismic data found profound heterogeneities in the deep mantle along-strike the Alpine orogen: in the Eastern Alps the subducting slab is steeply inclined, whereas in the Western Alps it is shallower and consistent with southward directed subduction after slab break-off possibly during Plio- to Pleistocene times. A goal of this study is to explore the long-term effects on the upper crustal structural and exhumation history by contrasting the western NFP-20E, central TRANSALP and eastern EASI seismic profiles utilising thermochronological and structural analyses. We achieve this in three steps: (1) by obtaining new low-temperature thermochronology data along the three profiles (apatite and zircon [U-Th/He]), (2) by modelling structural kinematics based on newly created balanced cross-sections for each profile, and (3) using these kinematics as input for an integrated thermo-kinematic forward model to predict cooling ages that can be compared to those measured at the surface. This approach will enable us to constrain rock uplift potentially associated with slab break-off in the Western Alps, and whether this mechanism is able to explain the overall higher topography in surface elevation compared to the Eastern Alps. Here we present new thermochronological ages along the NFP-20E and TRANSALP profiles together with preliminary thermo-kinematic forward models. These data are in accordance with recent exhumation focussed in the central part of the sections. The cooling ages show a slight north-to-south increase from ~5 Ma to ~10-15 Ma in apatite fission track ages and from ~10-15 Ma to ~20-25 Ma in zircon (U-Th/He) ages within the Tauern Window, and a sharp increase in cooling ages north of the Periadriatic Line. Apatite (U-Th/He) ages remain within ~5-10 Ma. North and South of the Tauern Window cooling ages tend to successively increase. We propose that the cooling age distribution measured at the surface is consistent with an in-sequence activation of mid-crustal ramps coeval with fault activity in the immediate hanging wall of the Periadriatic Line since the Oligocene. The unique setting, comparing the structural and exhumational history along sections above contrasting deep-seismic profiles, enables us to better understand, and possibly link, mantle processes and their influence on the crust and the surface during Palaeogene to Neogene Alpine orogenesis, while providing new insights into the formation of collisional mountain belts in general. [ABSTRACT FROM AUTHOR]

The long-lasting debate on the origin of Periadriatic magmatism in the European Alps has led to the formulation of one of the most successful theories of modern geology, the slab breakoff model (Davies and von Blanckenburg 1995) that is now extensively adopted worldwide (see review in Garzanti et al. 2018). In the Alpine region, recent tomographic data outline an unbroken European slab beneath the Western and the Central Alps (e.g., Zhao et al. 2016), which is incompatible with the hypothesis of oceanic slab detachment taking place in the early Oligocene, after continental collision between Adria and Europe (e.g., Schmid et al. 1996). In order to understand what triggers Alpine magmatism in the absence of slab breakoff, we present here the first comprehensive dataset of zircon U-Pb ages and Hf isotopic compositions from Periadriatic intrusives in the Western and Central Alps (Ji et al. 2019). Our data provide the first evidence of Eocene magmatism in the Western Alps (42-41 Ma in Traversella), and demonstrate that magmatism started synchronously in different segments of the Alpine belt, when subduction was still active. Zircon U-Pb ages define younging trends perpendicular to the strike of the European slab as imaged by seismic tomography, suggesting a progressive Eocene-Oligocene slab steepening. We propose that slab steepening enhanced the corner flow. This process was more effective near the edge of the European slab, and may have triggered Alpine magmatism in the absence of slab breakoff.CITED REFERENCESDavies JH and von Blanckenburg F (1995) Slab breakoff: a model of lithosphere detachment and its test in the magmatism and deformation of collisional orogens. Earth Planet Sci Lett 129, 85–102Garzanti E, Radeff G and Malusà MG (2018) Slab breakoff: A critical appraisal of a geological theory as applied in space and time. Earth-Sci Rev 177, 303-319Ji WQ, Malusà MG, Tiepolo M, Langone A, Zhao L and Wu FY (2019) Synchronous Periadriatic magmatism in the Western and Central Alps in the absence of slab breakoff. Terra Nova (in press)Schmid SM, Pfiffner OA, Froitzheim N, Schönborn G and Kissling E (1996) Geophysical–geological transect and tectonic evolution of the Swiss-Italian Alps. Tectonics 15, 1036–1064Zhao L, Paul A, Malusà MG, Xu X, Zheng T, Solarino S, Guillot S, Schwartz S, Dumont T, Salimbeni S, Aubert C, Pondrelli S, Wang Q and Zhu R (2016) Continuity of the Alpine slab unraveled by high-resolution P wave tomography. J Geophys Res Solid Earth 121, 8720-8737 [ABSTRACT FROM AUTHOR]

Collisional shortening across the entire Alpine belt has often been estimated in the Central Alpine sections, using sedimentary markers in the Southern Alps and more loosely constrained line-length balancing techniques in the Penninic and European domains. In the western Alps shortening has been assessed along numerous sections in the External Zone (European basement and cover), but shortening estimates for the entire Chain were always derived by projections of shortening amounts obtained in the Central Alps, either by assuming the amount of dextral displacement along the Insubric Line (Schmid and Kissling, 2000), or resolving the inferred amount of Central Alpine shortening on an assumed convergence direction in the western Alps (Handy et al., 2010).In the present study we estimate collisional shortening in the entire Alpine Chain, by reassessing displacements along the main structures of the orogen, without extrapolating displacements from one segment of the chain to the other. We note that collisional shortening progressively increases from less than 90 km in the south-western Alps, to nearly 200 km in the western Central Alps, where the Alpine chain starts to strike in an E-W direction. Therefore, we conclude that the convergence direction during the collisional phase must have been oriented NNW, as suggested by paleomagnetic studies, rather than WNW, as often inferred by tectonic investigations. The distribution of shortening described above is consistent with the distribution of collisional metamorphism: where the largest amounts of shortening are accommodated the nappes affected by the highest T of metamorphism are exhumed.The distribution of collisional shortening can also be used to constrain the interpretations of tomographic models on the geometry of slabs at depth. If the estimates of shortening are correct, along-strike variation of shortening are significant both along the upper and the lower plates. Based on these values it can be suggested that the central Alpine slab, well visible in all tomographic models, may largely consist of subducted European continental plate. In contrast, the eastern Alpine slab, in the area underlying the Tauern Window cannot be derived from the South-alpine continental plate, due to shortening amounts that are by far too small in this area, compared to the imaged slab length. Below the western Alps, some tomographic models image a slab break off whereas others image a continuous slab. Only the upper part of this slab, whether broken off or continuous, can be derived from the European plate based on the small amounts of inferred collisional shortening. References: Handy MR, Schmid SM, Bousquet R, Kissling E, Bernoulli D (2010). Earth Sci. Rev. 102:121–158.Schmid, S. M., and E. Kissling (2000). Tectonics, 19, 62–85, doi:10.1029/1999TC900057. [ABSTRACT FROM AUTHOR]