United States

In the western Ionian Basin, a wedge-shaped seismically transparent to chaotic unit has been mapped at the foot of the Malta Escarpment extending and thinning towards the east on the outer reaches of the Calabrian accretionary wedge. Its thickness, assuming realistic values of seismic velocity, exceed 800 m in the depocenter, and the volume is ~ 1600 km3. Its stratigraphic position has been assigned variably between the upper Messinian (deformed evaporites, mainly gypsum; Butler et al., 2015) and lower Pliocene (olistostrome; Polonia et al., 2011). A number of recent publications (Micallef et al., 2018, 2019; Garcia Castellanos et al., 2020; Spatola et al., 2020; Camerlenghi et al., 2020; Rebesco et al., in review) have proposed the hypothesis that this unit is the sedimentary expression of the Zanclean megaflood of the Mediterranean that ended the Messinian Salinity Crisis (e.g. Garcia-Castellanos et al., 2007). A number of observational, theoretical (numerical modelling) and conceptual arguments support his hypothesis, contributing to the discussion on the role of megafloods in the evolution of Earth terrestrial and marine sedimentary basins, and for comparison, on planets. We review the arguments in favor of the megaflood hypothesis and illustrate how we plan to verify it through scientific ocean drilling, proposing that a cross-disciplinary effort should be made to shed light on what could be the largest megaflood deposit so far identified on Earth and on the role of rapid  sealevel changes in marine sedimentary basin evolution.

SGI 2021

Megaflood deposits in sedimentary basins evolution. The case of the Messinian-Zanclean seismic stratigraphic unit in the Ionian basin

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L'Istituto Nazionale di Oceanografia e Geofisica Sperimentale - OGS e il Dipartimento di Matematica e Geoscienze dell'Università di Trieste sono orgogliosi di ospitare il 90° Congresso della Società Geologica Italiana a Trieste dal 14 al 16 settembre 2021. La modalità del congresso è interamente online.

Con il motto "Geologia senza frontiere" questo evento mira a promuovere le Scienze della Terra come disciplina scientifica proiettata nel futuro, oltre i confini geografici, politici e disciplinari, per comprendere meglio l'interno del Pianeta Terra e la struttura del sottosuolo, difendere la società da pericolosi eventi geologici, comprendere meglio la variabilità climatica, pianificare l'utilizzo delle georisorse in modo etico e nel rispetto dell'ambiente.


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The National Institute of Oceanography and Experimental Geophysics - OGS and the Department of Mathematics and Geosciences of the University of Trieste are proud to host the 90th Congress of the Italian Geological Society in Trieste on 14-16 September 2021.  The Congress will be held entirely online.

With the motto "Geology Without Borders" this event aims to promote Earth Sciences as a scientific discipline projected into the future, beyond geographical, political and disciplinary boundaries, to better understand the interior of Planet Earth and the structure of the subsurface, defend society from dangerous geological events, better understand climatic variability, plan the use of geo-resources in an ethical way and respecting the environment.


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Earth Sciences should be understood not only as necessary for a better understanding of the interior of the planet Earth, but also as a defense of society from dangerous geological events, for the understanding of climatic variations, for the planning and use of georesources in a ethical and respecting and protecting the environment.

technical paper

The role of sea-bottom topography in the dispersal of shallow water-derived calciturbidites across a submarine rift, as determined by the local extensional architecture, is under-investigated, namely with pelagic settings along ancient passive continental margins. A comparison with modern carbonate platform/basin analogues, or with siliciclastic systems, is not always feasible, as ancient carbonate systems were commonly home to anachronistic environments (e.g. the Western Tethyan Mesozoic). Geological mapping of the Jurassic rift basin exposed in the Apennines of Central Italy revealed a complex pattern of intrabasinal highs (pelagic carbonate platforms) and intervening basins, controlled by the high density, and oddly variable trends, of faults rooted in a shallow detachment layer corresponding to thick Triassic salt. A map pairing the occurrences of resedimented beds in pelagic successions with an updated palaeogeography becomes therefore the natural descriptor of the itineraries followed by sediment gravity flows. This qualitative method represents a companion, or even alternative, approach to the one strictly based on physical stratigraphy, and it greatly improves our knowledge of regional geology and rift-basin analysis. Our study focuses on: i) a reconstruction of the palaeotectonic architecture of the Umbria-Marche Basin in the Jurassic, and on ii) how this architecture produced a submarine topography which governed the dispersal of sediment, shed by the neighbouring Lazio-Abruzzo Carbonate Platform, for >40 million years. Geological mapping, coupled with the measurement and correlation of stratigraphic sections, shows that the marginal palaeoescarpments of pelagic carbonate platforms formed obstacles to the gravity flows as sediment load was discharged in confined basins at their toes and/or flows were deflected and forced along alternative itineraries. While turbidity currents were locally vigorous enough to climb the escarpments, leaving graded and laminated overbank deposits on the pelagic carbonate platform-tops, a “shelter” effect is evidenced by the resediment-free nature of those basins lying downflow, which were shielded by the highs. Our case study potentially represents the analogue of hydrocarbon fields both inland and in the offshore.

Role of Early Jurassic rift architecture in the dispersal of calciturbidites, as revealed by geological mapping in Central and Northern Apennines

A 2D and 3D re-interpretation of vintage seismic profiles acquired during the 1970s in the area of the Northern Tyrrhenian Sea between the Elba Island and the Argentario promontory was performend to build a 3D models of the main structures characterizing the Tuscan shelf. Stratigraphic information were extracted by the Pianosa island surface geology along with the Martina-1 and Mimosa-1 exploration wells. We identified eight seismostratigraphic units separated by eight unconformities. Among these seismostratigraphic units, two represent the pre-Neogenic foundation while six post-orogenic units represent the Neogenic succession covering the Tuscan shelf. The main shallow structures of the area are the narrow, mostly N-S and NE-SW trending Neogenic basins of Montecristo, Punta Ala and Uccellina, where the post-orogenic seismostratigraphic units deposited. Effort has been done to unravel the relationship between the position and evolution of the basins with previous compressive structures, mostly consisting in deep East-verging thrusts belonging to a previous compressional phase. Intringuingly, and partially in contrast with the literature works in the area, no evidence of listric and low angle fault systems were observed. A new evolutionary model of the Tuscany shelf was then proposed. In this view the formation of the Neogenic basins began in the upper Burdigalian initially as intermontane basins developed along the flanks of the antiforms formed during the compressive tectonics. The position of the basins, usually recovered at the forelimb vs. the backlimb of the thrust antiforms, influenced the  asymmetrical or symmetrical shape during their evolution. Starting from the Messinian, we observe a general collapse of the platform, which leads to the deepening of the basins driven by the normal high-angle bordering faults. This process continues up to the lower Pliocene, when the deactivation of all normal faults is recorded, and conditions of widespread subsidence are clear throughout the platform, together with the deposition of the two more post-orogenic units. In this contribution we reviewed the tectonic evolution of the northern Tyrrhenian Sea posing new questions both on the mechanisms responsible for the extensional processes and on the structures which impacted on such arrangement, also establishing a new starting point for a full unravelling of the Tuscan Shelf evolution.A 2D and 3D re-interpretation of vintage seismic profiles acquired during the 1970s in the area of the Northern Tyrrhenian Sea between the Elba Island and the Argentario promontory was performend to build a 3D models of the main structures characterizing the Tuscan shelf. Stratigraphic information were extracted by the Pianosa island surface geology along with the Martina-1 and Mimosa-1 exploration wells. We identified eight seismostratigraphic units separated by eight unconformities. Among these seismostratigraphic units, two represent the pre-Neogenic foundation while six post-orogenic units represent the Neogenic succession covering the Tuscan shelf. The main shallow structures of the area are the narrow, mostly N-S and NE-SW trending Neogenic basins of Montecristo, Punta Ala and Uccellina, where the post-orogenic seismostratigraphic units deposited. Effort has been done to unravel the relationship between the position and evolution of the basins with previous compressive structures, mostly consisting in deep East-verging thrusts belonging to a previous compressional phase. Intringuingly, and partially in contrast with the literature works in the area, no evidence of listric and low angle fault systems were observed. A new evolutionary model of the Tuscany shelf was then proposed. In this view the formation of the Neogenic basins began in the upper Burdigalian initially as intermontane basins developed along the flanks of the antiforms formed during the compressive tectonics. The position of the basins, usually recovered at the forelimb vs. the backlimb of the thrust antiforms, influenced the  asymmetrical or symmetrical shape during their evolution. Starting from the Messinian, we observe a general collapse of the platform, which leads to the deepening of the basins driven by the normal high-angle bordering faults. This process continues up to the lower Pliocene, when the deactivation of all normal faults is recorded, and conditions of widespread subsidence are clear throughout the platform, together with the deposition of the two more post-orogenic units. In this contribution we reviewed the tectonic evolution of the northern Tyrrhenian Sea posing new questions both on the mechanisms responsible for the extensional processes and on the structures which impacted on such arrangement, also establishing a new starting point for a full unravelling of the Tuscan Shelf evolution.

Tectonic-Sedimentary evolution of the Tuscan shelf: seismic-stratigraphic analysis of Neogenic succession in the norther Tyrrhenian sea (Elba Island - Argentario)

The Turkana depression (Ethiopia-Kenya) is a tectonic basin related to the Cretaceous-Early Cenozoic development of the South Sudan and the Anza grabens filled with a thick sequence of Cretaceous-Paleogene sediments reaching up to a thickness of 6–8 km. These two NW-SE trending depressions, which likely resulted from NE-SW extension, were later affected by W-E extension related to the Cenozoic East African Rift System. The influence of crustal thinning related to these NW-SE grabens on later W-E-related extension is testified by the marked change in style of deformation from the narrow rift valleys in Kenya and Ethiopia, to a distributed, basin-and-range-style faulting in the Turkana depression. Despite some local scale reactivation is visible, large scale reactivation of pre-existing NW-SE structures in the Turkana depression is not obvious, as it is extensively masked by the sedimentary and volcanic cover; consequently, contrasting hypothesis on the possible role exerted by discrete pre-existing fabrics have been proposed in the literature. To address this controversy, we performed analogue models to investigate whether inherited structures, largely obscured by sediments in the Turkana depression, might have been reactivated during subsequent tectonic phases. We run 2-layer, brittle-ductile models deformed in two successive phases: a first phase of NE-SW extension, followed by W-E extension. Different models were subjected to different amount of bulk extension during the first phase to investigate the influence of this parameter (and the importance of first-phase structures) on later reactivation. Our models indicate that the amount of deformation in the initial tectonic phase is key for structure reactivation in subsequent tectonic phases: the larger the deformation in the first phase, the higher the probability of reactivation. Comparison of the experimental results with nature suggest that, despite some local fault reactivation, large-scale structures were likely not reactivated in the Turkana depression. These outcomes represent a useful tool to decipher fault reactivation, not only in the Turkana depression but also in tectonic basins worldwide, especially where thick sedimentary covers may mask tectonic structures.

Reactivation or non-reactivation? Analogue models of multiphase rifting and applications to the Turkana depression, East Africa

We present PALEOSTRIPv1.0, a MATLAB open-source software designed to perform 1D, 2D and 3D backtracking of paleo-bathymetries. PALEOSTRIP comes with a Graphical User Interface (GUI) to facilitate computation of sensitivity tests and to allow the users to switch on and off all the different processes and thus separate the various aspects of backtracking. As such, all physical parameters can be modified from the GUI. It includes 3D flexural isostasy, 1D thermal subsidence and possibilities to correct for prescribed sea level and dynamical topography changes. In the following we detail the physics embedded within PALEOSTRIP and we show a few applications on a drilling site (1D), a transect (2D) and a map (3D), taking the Ross Sea (Antarctica) as a case study. PALEOSTRIP has been designed to be modular and to allow users to insert their own implementations.

A user-friendly 3D backtracking software to reconstruct paleo-bathymetries

We present a brand new multi-proxy dataset of thermal maturity indicators, which derive from the application of several analytical techniques on surface and subsurface sedimentary successions. The study area spans from the Greater Caucasus to the Adjara-Trialeti fold-and-thrust belt (FTB), comprising the intervening western Kura Basin, in Georgia, and represents a region of continental deformation in the hinterland of the Arabia-Eurasia collision zone. Original and published clay mineralogy, Raman spectroscopy and petrography on dispersed organic matter, and pyrolysis data are integrated for the first time in a coherent tectono-sedimentary scenario. Thermal maturity spans from the low diagenetic realm (60-80°C) in the Upper Miocene section of the Kura sedimentary fill, to the oil window in the Cretaceous to Lower Miocene successions of Adjara-Trialeti FTB, Kakheti ridge and Kura Basin (70-120°C), up to about 400°C in the Greater Caucasus core. Integration of different indicators, besides allowing the estimation of maximum burial temperatures acquired through time, enabled to draw the tectonic evolution of the area. Different maturity trends and thermal histories, coupled with structural and stratigraphic data, highlight that the study area comprises two domains derived from positive tectonic inversion: the E-W Adjara-Trialeti doubly-verging FTB from an Eocene back-arc rift basin and the SSW-verging Georgian Greater Caucasus from a Mesozoic rift basin. Between the two, thin-skinned south-verging thrusts deform the Kura Basin and the Kakheti ridge successions, originally deposited on an extensional structural high which was later flexured during compression. The similar thermal maturity degree in the Adjara-Trialeti FTB and the Kakheti ridge/Kura Basin areas has been acquired in different time spans: during Paleogene extension and during Miocene thin-skinned shortening, respectively. The results indicate that thermal maturation of the sedimentary successions in the Adjara-Trialeti FTB can be ascribed to burial during rift evolution. The same conclusion can be drawn for the axial zone of the Greater Caucasus, whereas tectonic overburden may have contributed to the thermal maturity of the rocks in the southern foothills of the Greater Caucasus: this area needs further work to assess its tectonic evolution.

Using multi-proxy thermal maturity datasets to validate deformation styles from the Adjara-Trialeti fold-and-thrust belt to the Greater Caucasus (Georgia)A

The tide-dominated Messina Strait (southern Italy) is a 3 km wide marine passageway, whose block-faulted borders form steep subaqueous zones incised by canyons and gullies. These erosional features retreat towards the shorelines and are often in direct connection with subaerial valley-bounded river deltas. High-energy density-flows generated by river floods periodically enter the canyon heads, attaining supercritical-flow regime and accreting large, upslope-migrating bedforms. Although these bedforms have been documented in recent studies, little attention has been paid to the definition of the type of delta entering canyon heads, the internal features of river-influenced deposits accumulated in the nearshore zone, and their interplay with tidal currents flowing axially to the strait. This study focuses on a Lower Pleistocene coarse-grained succession exposed along the north-eastern margin of the modern Messina Strait, investigated using conventional facies analysis and sedimentological logging, integrated with photogrammetric techniques and interpretation of drone-acquired imagery. Facies confinement between basement blocks suggests a subaqueous delta complex shed from the tectonically controlled margin of the ancient strait and entering shallowly submerged canyon heads. Basal breccias, conglomerates and pebbly sandstones exhibiting channel-form discontinuities and upslope dipping backsets are interpreted as cyclic-step and antidune deposits. Units composed of these facies are comprised between master erosional surfaces and tidal ravinement surfaces. The tidal ravinements suggest that canyon infill occurred during a major phase of sea-level rise, punctuated by minor falls and stillstands. These surfaces are overlain by mixed bioclastic–siliciclastic, arenitic, trough and planar cross-strata, representing dunes migrating roughly parallel to the palaeo-coastline and originated by tidal currents amplified by the narrowing of the ancient Messina Strait. Tidal-influenced sedimentation dominated over the fluvial-influenced processes during the late transgression, overfilling the canyon relief. The exceptionally good exposure of depositional architectures and facies characteristics is key to outline the general features of a specific type of delta system, fed by valley-bounded rivers and entering canyon heads in the nearshore of tectonically-controlled, tide-influenced steep strait margins. The pre-existing subaqueous incised topography forced the delta front to be split into lobe branches during the canyon infilling, hampering clinoform architectures and preserving large supercritical-flow sedimentary structures. This study suggests these as possible criteria for the recognition of similar systems in outcrop or subsurface.

Coarse-grained deltas approaching shallow-water canyon heads: A case study from the Lower Pleistocene Messina Strait, Southern Italy

Early Palaeozoic represents a crucial period in Earth history, marked by intervals of life spread alternated with short-lasting crisis in biological activity. The Zagros Basin (SW Iran) could be a key area for the study of this time interval, due to the widespread and well-exposed Cambrian-Ordovician successions; nevertheless, these are still poorly constrained from a sedimentological and stratigraphic point of view. This study, carried out through a high-resolution facies and microfacies analysis of the Zard Kuh section, aims to give a contribution to the palaeogeographic evolution of this area. The studied section (296 m thick) includes the upper Mila C Member and Ilebeyk Formation, referred to the late Cambrian (Furongian) based on acritarch assemblages. The upper Mila C Member (23 m thick) is mainly characterized by medium to thin-bedded bioclastic packstones to mudstones grading upward into a nodular limestone unit. A sharp horizon marks the contact with the overlying Ilebeyk Formation, represented by a shale-dominated interval in the lower part. These mudrocks grade upward into heterolithic lithofacies, generating a coarsening upward sequence with an increase of siltstone and sandstone intercalations in the lower-middle part. The coarser-grained layers display scoured basal surfaces, with common gutter casts, capped by plane parallel lamination and hummocky cross-stratification (HCS). In the middle part of Ilebeyk Formation, siliciclastic deposits are alternated with relatively thick carbonatic intervals, showing similar features with Mila C Member. The upper part of the Ilebeyk Formation is dominated by shales, overlain at the topmost by a 28 m thick unit of micaceous sandstone and siltstone. The sandstone layers include plane-parallel bedding, trough cross-stratification and long-wavelength HCS. Based on the facies and microfacies analysis, the depositional system of the studied section is interpreted as a mixed carbonate-siliciclastic ramp. In the Mila C Member and carbonatic unit of Ilebeyk Formation, small cycles characterized by erosive surfaces and fining upward fossiliferous biomicrites suggest deposition in middle ramp setting, affected by storm events. On the other hand, the nodular limestone intervals at the top of the carbonatic units point to deposition below the SWB under a transgressional regime. The shale to heterolithic parasequences from the Ilbeyk Formation are interpreted as autocyclic fluctuations of the depositional system from lower to upper offshore environment. In the uppermost part, the sandstone-dominated interval is attributed to shoreface setting, marking an abrupt change in the bathymetric conditions after a forced regression. The sedimentological features of the studied area can be correlated with other coeval depositional events at both regional (Arabian plate) and global (Laurentia and Baltica) scales, providing new constraints for the lower Palaeozoic evolution of the northeastern Gondwanan margin.

Facies analysis and depositional environment of a late Cambrian mixed carbonate-siliciclastic ramp from the Arabian Plate (Zagros Basin, Southwestern Iran)

An integrated analysis of subsurface dataset and outcropping successions permitted to define a stratigraphic and paleogeographic evolutionary model of the wedge-top Rossano and Crotone Basins during the Messinian Salinity Crisis (MSC). The presence of complete sea-level controlled successions, indicate the dominance of the eustatic signal in the basin evolution, in comparison with the synsedimentary tectonic input, which played only a secondary role consisting in the strong basinward shift of facies caused by fast decreasing in the accommodation space. In particular, during the late Tortonian - early Messinian the studied basins were characterized by open normal marine conditions, as suggested by the widespread deposition of deep-water claystones followed by diatomites (Tripoli Fm). The first basin restriction occurred during the early Messinian at ca. 5.96 Ma, as a consequence of the sea-level relative still stand, that triggered the deposition of a carbonate platform system (Calcare di Base Fm - CdB). The latter was characterized by sabkha to shallow-water environments, dominated by microbial carbonate and evaporite deposition, passing into a gentle slope to basin setting in which resedimented and pelagic deposits occurred. A successive regional sea-level drop, dated at ca. 5.60 Ma, induced a general exposure of the CdB platform system and the creation of a marked erosional surface generally known as the Messinian Erosional Surface (MES). Consequently, during the early LST, a thick prograding wedge deposited and, due to the reduction of the connections with the open sea, new more severe restricted conditions of the basins took place. Later, during the late LST, the massive deposition of salt dominated bodies reshaped the basin paleotopography and the depocentres were filled, thus sealing the previous irregularities of the paleo-seascape and creating roughly flat plains without deep depozones. Afterwards, a renewed transgression phase (TST) inundated again the basins, causing firstly the sedimentation of clay dominated deposits, and later, during a further HST, the reestablishment of evaporitic conditions and the deposition of widespread shallow-water sulphate deposits. Lastly, a new severe relative sea-level drop (LST) exposed again all the previous deposits, as testified by the superimposition of alluvial conglomerates along paleovalleys incised into the underlying HST sulphates. This event marks the transition to the so-called Lago-Mare event that typifies the last stage of the MSC, which definitely terminates with the reflooding of the Mediterranean at the Pliocene transition (ca. 5.33 Ma).

Relative sea-level variations and basin evolution during the Messinian Salinity Crisis (Crotone and Rossano Basins - North Calabria)

Incised valley-fill (IVF) systems play a key role in source-to-sink (S2S) sediment transport towards sedimentary basins (Blum et al., 2013). A buried paleovalley system, about 3.5 km wide and 50 m deep, was reconstructed below the Pescara River coastal plain (central Adriatic). The study area represents an onshore sector of the larger-scale S2S Po-Adriatic system and is located in front of the Mid-Adriatic Depression basin. The paleovalley profile, incised into the marine Upper Pliocene-Lower Pleistocene bedrock, and the 3D IVF facies architecture were reconstructed through a multi-proxy approach based on stratigraphic, sedimentological and palaeontological data. To refine stratigraphic and paleoenvironmental reconstructions, a new continuous core was recovered from the paleovalley depocenter and samples were collected for radiocarbon dating and facies analysis. At different depths below the surface, paleovalley flanks are characterized by fluvial terraces made of gravel bodies with upper flat surfaces. These terraces, most likely incised by the Pescara river during the stepwise sea-level fall that followed the last Interglacial (MIS 5e, about 125 ky BP), are interpreted as falling stage systems tract (FSST) deposits. The valley floor is composed of a laterally extensive gravel body, > 10 m thick, that accumulated during the Last Glacial Maximum (28-20 ky BP, MIS 2). This fluvial deposit represents the lowstand systems tract (LST). Above LST deposits, the transgressive systems tract (TST) shows a deepening-upward trend, from poorly-drained (alluvial) to estuarine facies associations (early to late TST). The estuarine succession is characterized by very soft (< 1 kg/cm²) and organic-rich silty clays, linked to the post-glacial sea-level rise, when the Pescara paleovalley was progressively drowned and an estuary formed in the study area. The uppermost part of the IVF and Pescara coastal plain Holocene succession is composed of coarse-grained (sands and gravels) fluvio-deltaic deposits. The base of this stratigraphic interval coincides with the beginning of deltaic progradation at the onset of the Holocene (MIS 1), and can be interpreted as the Maximum flooding surface (MFS). Thus, prograding fluvio-deltaic sediments are the highstand systems tract (HST). Glacio-eustatic fluctuations (over the last 125 ky) are considered the main driving factor that induced river down cutting during sea-level fall and subsequent valley filling during sea-level rise. This study represents the starting point of a more complex basin-scale study, where onshore data will be correlated to their offshore equivalents to better understand sediment dynamics within the Po-Adriatic S2S system.

The Pescara incised valley system: Insights from an onshore sector of the S2S Po-Adriatic sediment routing

A better understanding of the evolution of bottom current circulation and associated deposits is significant for many applications including paleoclimatology and geological hazard. Besides the large contourite drifts, bottom currents may generate fields of large sediment waves that, depending on their height and velocity of migration, may pose severe risk for infrastructures. Conversely, the time span of their paleoceanographic record is generally relatively short. We use bathymetry data, sub-bottom and seismic reflection profiles and legacy oceanographic data to analyse the sediment waves occurring in a deep environment (from 2400 to 3800 m water depth at the foot of the Malta Escarpment in the Mediterranean Sea) to understand their evolution in time, their significance for paleoceanography, and their relation to present day hydrographic conditions. In the absence of direct stratigraphic information, we use the information from nearby studies and from ODP Site 964 and DSDP Site 374 to constrain the age of the sedimentary successions. We discover that these waves (about 2.5 km in wavelength, 50 m in eight, with crest sub-perpendicular to the continental slope trend) have been steadily growing and migrating northward since about 500 ka, although an irregular growth and unsteady migration is distinguishable since about 1,800 ka. The waves are generated by predominantly alongslope southward flowing bottom currents compatible with modern hydraulic conditions (mean flow speed of ~5 cm s-1, peaks of 15 cm s-1). The rate of crest migration (~ 2.0-3.2 mm a-1) and the average sedimentation rate (0.64 - 0.69 mm a-1) are unusually high for deep sea environments away from turbidity currents paths. We infer that the steady development of sediment waves is produced by a drastic increase in sediment input to the Ionian Basin resulting from the tectonic uplift in NE Sicily and Calabria and the onset of a relatively steady, low energy bottom current regime following the Mid-Pleistocene Transition. We attempt to extract information on orbital cyclicity preserved in the seismic record from the power spectra of virtual seismic traces from the well preserved succession of 5 visually discernible, regularly spaced sub-units consisting of alternation of high-amplitude and low-reflectivity packages within the last 500 ka. Peaks in the power spectra can be identified around orbital obliquity and precession periodicities, while eccentricity appears not to be recorded. We discuss the results of seismic cyclicity analysis relative to uncertainties of stratigraphic and petrophysical constraints. The sediment waves along the foot of the Malta escarpment are an excellent candidate for the extraction of a long, continuous and high resolution sedimentary record of the paleo circulation changes and climate cycles in the Mediterranean Sea since about 500 ka.

Megaflood deposits in sedimentary basins evolution. The case of the Messinian-Zanclean seismic stratigraphic unit in the Ionian basin

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Role of Early Jurassic rift architecture in the dispersal of calciturbidites, as revealed by geological mapping in Central and Northern Apennines

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Megaflood deposits in sedimentary basins evolution. The case of the Messinian-Zanclean seismic stratigraphic unit in the Ionian basin

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Role of Early Jurassic rift architecture in the dispersal of calciturbidites, as revealed by geological mapping in Central and Northern Apennines

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Bottom current-controlled Quaternary sedimentation at the foot of the Malta Escarpment (Ionian Basin, Mediterranean)

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