Distal Turbidites and Tsunamigenic Landslides of Stromboli Volcano (Aeolian Islands, Italy) A. Di Roberto, M. Rosi, A. Bertagnini, M.P. Marani, and F. Gamberi Abstract On 30 December 2002, a 25–30 × 106 m3 landslide on the NW flank of Stromboli volcano produced a tsunami that caused relevant damage to the Stromboli village and to the neighboring islands of the Aeolian archipelago. The NW flank of Stromboli has been the site of several, cubic kilometer-scale, landslides during the past 13 ka. In this paper we present sedimentological and compositional data of deep-sea cores recovered from a site located about 24 km north of the island. Our preliminary results indicate that: (i) turbidity currents were effectively generated by the large-scale failures and (ii) volcanogenic turbidity current deposits retain clues of the landslide source and slope failure dynamics. By analogy with Hawaii and the Canary islands we confirm that deep-sea sediments can be effectively used to assess the age and scale of past landslide events giving an important contribution to the tsunami hazard assessment of this region. Keywords Landslide • turbidite • tsunami • Stromboli 1 Introduction Volcanic landslides have recently been identified as one of the most hazardous geological processes on Earth (Hürlimann and Ledesma 2007). Recent studies within the geological record and at many active volcanoes have documented that A. Di Roberto () and A. Bertagnini Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Pisa, Via della Faggiola, 32 – 56126 Pisa, Italy e-mail: diroberto@pi.ingv.it M. Rosi University of Pisa, Dipartimento di Scienze della Terra, Via S. Maria, 53 – 56126 Pisa, Italy M.P. Marani and F. Gamberi Istituto di Scienze Marine – CNR, Sede di Geologia Marina di Bologna, Via Gobetti 101 – 40129 Bologna, Italy D.C. Mosher et al. (eds.), Submarine Mass Movements and Their Consequences, Advances in Natural and Technological Hazards Research, Vol 28, © Springer Science + Business Media B.V. 2010 719 720 A. Di Roberto et al. volcanic landslides are frequent, with almost one event per 25 years during the last 500 years (Siebert 1992; McGuire 1996; Voight and Elsworth 1997). Debris avalanches, lahars, explosive eruptions and lateral blasts are all phenomena that can be directly connected to catastrophic flank failures of volcanoes. Along coastal regions or volcanic islands, the movement of landslide masses has the additional potential to produce large, sometimes devastating, tsunamis that can affect areas far from the source (e.g. Moore et al. 1989; Masson et al. 2006; McGuire 2006). Detailed offshore studies of volcanic islands show that deposits resulting from debris avalanches can comprise volumes of up to 5,000 km3, as observed in the Hawaii Islands (Moore et al. 1989), or in the Canary archipelago (Ablay and Hürlimann 2000; Masson et al. 2002; Wynn and Masson 2003; Masson et al. 2006). It is not necessary for a volcanic landslide to be large to produce hazards, and even relatively small volume landslides have the capacity to generate high run-up tsunamis (Masson et al. 2006) depending on their vicinity to the coastline, water depth, angle of the slide, density of the slide material, the speed with which the landslide moves and other factors (Murty 2004). As we have never observed a large volume flank collapse in real time the assessment of past volcano-induced tsunamigenic landslides has proved both difficult and controversial. Tsunami deposits are poorly preserved on land and can be difficult to distinguish from storm events in land and marine records. The poor preservation of tsunami deposits on land has led the paleoseismology community to turn to the marine environment, where, according to authors, a complete record of seismogenic tsunamis may be preserved as turbidite sequences in submarine canyons (e.g. Adams 1990; Goldfinger et al. 2003). Distal turbidites have also been employed to investigate volcanic landslides in Hawaii, the Canary archipelago, La Reunion Island (Garcia 1996; Ollier et al. 1998; Kanamatsu et al. 2002; Masson et al. 2002; Wynn and Masson 2003; Masson et al. 2006) and Aeolian Archipelago (Di Roberto et al. 2008). In this paper we analyze two sea-bottom sediment sections i.e. a gravity core and a box core collected offshore the volcanic island of Stromboli respectively prior and after the Dec. 30, 2002 landslide that affected the NW slope of the island. Such event produced a 25–30 × 106 m3 rock debris with associated tsunami wave that spread over most of the southern Tyrrhenian Sea. The work also aims at implementing the documentation of past potentially tsunami producing landslide events originated from Stromboli volcano during Holocene thus opening new perspectives for the assessment of the tsunami hazard in the southern Tyrrhenian sea. 2 Geological Background Stromboli is located in the Southern Tyrrhenian Sea, a few tens of kilometers offshore from the north coast of Sicily and the Italian peninsula (Fig. 1, inset). The island, with an elevation of 924 m, represents the subaerial part of a larger volcanic edifice extending to a maximum water depth of 2,600 m. Distal Turbidites and Tsunamigenic Landslides of Stromboli Volcano 721 Fig. 1 Shaded relief bathymetry of the Stromboli region with highlighted the main features of Stromboli sedimentary system; the star marks the sample site; SdF: Sciara del Fuoco. Inset shows location of Stromboli Island within the south Tyrrhenian sea Stromboli volcano was built during seven main periods of activity covering a time span of about 100 ka, i.e.: Paleostromboli I, II, and III (100-35 ka), Scari (35-25 ka), Vancori (25-13 ka), Neostromboli (13-6 ka), and Recent Stromboli (<6 ka) (HornigKjarsgaard et al. 1993; Gillot and Keller 1993). Transitions between each period are marked by significant modifications of the edifice structure (caldera collapses between 100 and 25 ka and flank collapses after 25 ka; Tibaldi 2001) and changes in magma compositions (Hornig-Kjarsgaard et al. 1993; Francalanci et al. 1993). The most striking geomorphological and volcanic structure of the island is the Sciara del Fuoco (SdF) a horseshoe-shaped collapse scar that occupies the NW sector of the island. SdF structure is considered the result of at least four flank collapses that occurred in the last 13 ka involving volumes of material ranging from 0.73 ± 0.22 to 2.23 ± 0.87 km3 (Tibaldi 2001). The younger collapse (<5,000 years ago; Kokelaar and Romagnoli 1995; Tibaldi 2001), with an estimated volume of about 0.7 km3, resulted in the present-day SdF morphology. SdF structure continues below sea level (Fig. 1) as a depression bounded by steep walls in continuity with the flanks of the 722 A. Di Roberto et al. sub-aerial SdF (Kokelaar and Romagnoli 1995). Further downslope, the SdF depression runs to the east of a large volcanoclastic fan extending from 1,000 m to 2,500 m water depth and with an estimated volume of about 4–6 km3 (Fig. 1; Gamberi et al. 2006). As deduced by recent physical modeling, the major flank collapses that produced the SdF had the potential to generate large and destructive tsunamis whose effects may extend throughout the Aeolian Islands and to the southern Italian coasts (Tinti et al. 2003). The most recent partial collapse of the SdF took place on 30 December 2002. Two relative small landslides, with a total volume of about 25–30 × 106 m3, detached from the submarine and subaerial part of SdF respectively and generated tsunami waves up to 10 m high on the Stromboli coasts and up to 2 m high on the neighboring islands (Tinti et al. 2005). The result was severe damage to Stromboli village and limited damage on the neighboring islands. The tsunami also weakly affected Milazzo harbor, located on the northern coast of Sicily, 100 km south of Stromboli (Maramai et al. 2005). The December 30, 2002 event and the historical record of the Stromboli volcano activity in the last century proves that besides major flank collapses, also smallscale tsunami-forming landslides may occur at Stromboli. Their higher frequency (five since 1906; Maramai et al. 2005) and the significant destructive power of the resulting tsunami waves, currently makes them among the most relevant natural hazards threatening the coastal areas of Stromboli volcano. 3 Marine Record of Stromboli Volcano Landslides Submarine deposits of the December 30, 2002 landslide were recently identified by seafloor imagery and sampling during the TTR14 cruise aboard the R.V. Professor Logachev in August, 2004 (Marani et al. 2008a, b). The proximal part consists of chaotic, coarse-grained deposits bordered and partially covered by sand. The deposits were interpreted as deriving from cohesionless, sandy-matrix, density flows (Marani et al. 2008b). 24 km north of Stromboli a 2–3 cm-thick sand bed was interpreted as the finer grained turbidite equivalent of the proximal deposits (Marani et al. 2008b). The identification of the distal landslide deposit was facilitated by repeat sampling in September, 2002 (VST02-16) and in August, 2004 (TTR14-342), respectively prior to- and post- the December 30, 2002 collapse. The sample site (VST02-16 Lat. 39°01.100′ Lon. N 15°09.298′ E WGS 84) is an even, flat area located on a topographic high at water depth of 2458 m, on the right (east) side of the Stromboli canyon about 200 m above the canyon floor (Gamberi et al. 2006; Marani et al. 2008b) and about 24 km from the SdF shore (Fig. 1). The site, located outside the direct influence of the sedimentary dynamics of the Stromboli canyon, is thus proved to record turbidity currents generated by landslide events of the SdF with a volume comparable to the volume of December 2002 landslide (tens × 106 m3). The two cores presented herein are 1 m and 38 cm long respectively (Fig. 2), and were collected from the same site, with a ±15 m accuracy in positioning. Distal Turbidites and Tsunamigenic Landslides of Stromboli Volcano Fig. 2 Image of collected cores: VST02-16 gravity core sampled about 4 months before the Dec. 30, 2002 Stromboli landslide; TTR14-342 box core sampled about 2 years after Dec. 30, 2002 Stromboli landslide 723 724 4 A. Di Roberto et al. Methods A detailed cores description was performed to characterize lithology, fabric, sedimentary structures, bedding thickness, and other pertinent features. 50 subsamples were picked at intervals of about 2–3 cm. Samples were washed in an ultrasonic bath for 10 min and subsequently, sieved at one-phi intervals for grainsize characterization. The 250–125 mm and 125–63 mm fractions were then mounted on thin section with epoxy resin for component analysis. A selection of 23 samples from VST02-16 and 11 samples from TTR14-342 were analyzed for component analysis (Fig. 3); 1,000 clasts of the most abundant grain size fractions were counted on each thin section. Fig. 3 Stratigraphic log, magnetic susceptibility and componentry results of VST02-16 core; Black-filled circles indicate samples that were processed for grain size analysis; white circles indicate samples that were processed for component analysis. Notice that leucitic lavas (Lc-lavas) and altered glass (Alt. glass) distribution is tightly linked to the sub-turbiditic units structures within thick sand beds between 96–48 and 30–17 cm Distal Turbidites and Tsunamigenic Landslides of Stromboli Volcano 725 Texture and composition of glass shards were also analyzed using a SEM-EDS Philips XL30 scanning electron microscope (accelerating voltage 20 kV, beam current 1 nA, working distance 10 mm), equipped with energy dispersive x-ray analysis (EDAX DX 4) at the Earth Science Department of Pisa University. For each sample a minimum amount of 30 glass particles were analyzed in raster mode, using windows ranging from 5 × 5 mm, in highly crystalline samples, to 30 × 30 mm in aphiric ones. The analytical error, measured on mineral and glass standards varies from 1 wt% (concentrations higher than 15 wt%) to 10 wt% (concentrations between 1–5 wt%), increasing at low concentrations. Results were compared with the glass composition of subaerial Stromboli volcanics available in literature for the past 13 ka. In order to infill such existing dataset, which was partially incomplete, some additional samplings were realized. These include 8 lava and 9 scoria samples recovered on the summit part of the volcano and in a 4 m deep stratigraphic trench dug on the NE flank of the island at 335 m a.s.l. (Lat. N 38°47.499′, Long. E 15°13.459′). 5 Results The description and analyses of the distal deposit of December 30, 2002 landslide that caps the TTR14-342 core (sampled in 2004) and that is absent in the 2002 core (Figs. 2 and 4) are reported in Marani et al. 2008b. The 1 m long gravity core sampled in 2002 (VST02-16) consists of a sequence of dark grey to black, decimetric to millimetric-thick beds of coarse to fine sands, interlaminated and interbedded with millimeter- to centimeter- thick brownish silty-clay (Fig. 2). Beds have sharp and slightly erosive basal contacts and commonly evidence normal grading into brown clay beds. Clay beds frequently contain mm-thick layers or lenses of black, fine sand to silt that are frequently disrupted by bioturbation. Brown clay are often capped by <0.5 cm-thick layer of pale-yellow hemipelagic clays. Samples range from moderate to poorly sorted (sΦ 0.705–1.371), coarse to very fine sands (MdF = 0.663 and 3.538). The two thicker beds, occurring at 96–48 cm and 30–17 cm are characterized by multiple, well-developed normally graded sand beds (Fig. 3). Grain size and component analysis data are shown in Fig. 3. Sand beds consists almost entirely of volcaniclastic fragments represented by lava (35–56 vol.%), pyroclastic fragments (22.5–37 vol.%), plagioclase crystals (3.8–14.5 vol.%), pyroxene (4.4–9 vol.%), olivine crystals (≤2 vol.%) and altered volcanic fragments (3–15.5% vol.%). Few subvulcanic, holocrystalline fragments occur. Biogenic and detrital clasts (mainly metamorphic rock fragments, muscovite and microcline crystals) account for less than 2 vol.% of the deposits suggesting that the site is poorly influenced by terrigenous sediment supply. Lava fragments are generally equant, bearing crystals of plagioclase, pyroxene and olivine set in a holocrystalline to partially glassy matrix. Pyroclastic fragments consist of mainly fresh, poorly vesicular, honey-colored glass containing abundant plagioclase microlites. 726 A. Di Roberto et al. Fig. 4 Glass shards composition plotted against stratigraphic height. Notice the similarity between the glass composition of (a) the lowermost half of the core and Neostromboli glasses, (b) the uppermost half of the core and products from recent and present products emitted by Stromboli volcano. (c) The glass composition of the topmost layer (core TTR14), attributable to the December 30 2002 landslide (Marani et al. 2008b) is reported to complete the chemical characterization of sediment sequence. Distal Turbidites and Tsunamigenic Landslides of Stromboli Volcano 727 In the uppermost layer subordinate highly vesicular, fresh and almost crystal free clear-glass clasts occur. Pyroclastic fragments have prominent angular shape with very delicate, sharp edges indicating the lack of any mechanical interaction due to reworking. A large compositional variability is evident when the glass compositions are plotted in the K2O-SiO2 diagram (Fig. 4), which is traditionally employed to classify magmas erupted from Stromboli during its volcanic history (Hornig-Kjarsgaard et al. 1993; Francalanci et al. 1993). Moreover great variations in glass composition occur between the lowermost half of the core and the uppermost one. Glass fragments of the lowermost part of the sequence (96–40 cm) have scattered composition largely covering the compositional range of Neostromboli products; minor compositions attributable to the Vancori periods also occur (Fig. 4). Glass fragments of the uppermost part of the cores (39–13 cm) have more homogeneous compositions; from 39 to 13 cm samples describe a short evolution trend from composition slightly enriched in K2O to composition strictly comparable with products of the Recent Stromboli (Fig.4). It is interesting to note that from 66 to 34 cm, within the deposits likely correlating Neostromboli period a significant amount of lava fragment bearing leucite microlites occurs; leucite (<100 mm) is usually replaced by analcime even if nuclei with original leucite composition still persist in few microlites. The first appearance of Lc-bearing lava fragments coincides with an abrupt increase in grain size corresponding to the base of one of the stacked sand beds between 96–48 cm. In the uppermost half of the core a consistent fraction of pyroclasts exhibit a few ten of mm-thick rim of leached glass (up to 50 wt.% loss in FeO, CaO, MgO and up to 11 wt.% gain of SiO2) likely indicating alteration of the glass by volcanic gas or acid rainwater. 6 Discussion The observed sedimentary structures indicate that the core is mainly composed of turbidity current deposits. The most interesting features revealed by grain size and component analysis are the multiple turbiditic-sub units contained within the two main sand units between 96–48 cm and 30–17 cm. Multiple, stacked and closely spaced sandy units with sharp base and gradational top, similar to those recovered in our sequence and interpreted as turbidites were recognized at about 320 km west of the island of Hawaii (Garcia 1996) and in Agadir basin about 300 km north of the western Canary Islands (Wynn and Masson 2003). Such deposits have been interpreted as the distal equivalent of large landslides developing with retrogressive or multi phase dynamics (Garcia 1996; Wynn and Masson 2003). Alternatively, stacked turbidites can also form as a consequence of turbidity current reflection off seafloor topography (Pickering et al. 1992) or from multiple turbidity currents reaching the sampling site along differential flow pathways (Masson 1994). 728 A. Di Roberto et al. In our case no submarine structure exists beyond the flank of Stromboli canyon upon which a turbidity current could reflect; in addition the SdF submarine valley represents the only pathway through which mass flows originating on the NW flank of Stromboli volcano are funneled in the Stromboli canyon. Thus in analogy with Hawaii and Canary Islands cases we interpret the sandy sub-units recovered in Stromboli core as the result of a rapid and progressive deposition from repeated turbidity currents (gravity flows) cogenetic to landslides on the NW flank of Stromboli volcano, dominated by retrogressive collapse dynamics. The almost complete absence of hemipelagic sediment deposited between each single sub-unit suggest a very rapid, geologically-instantaneous sequence of events. Geochemical data allow correlation of the turbidites. The sand interval occurring between 96 and 48 cm can be associated with the ∼5 ka old, Neostromboli collapse. This data is confirmed by the presence of Lc-bearing lava fragments in the turbidites. On Stromboli volcano, leucitic lavas crop out almost exclusively in the summit portion of the edifice and belongs only to the final phases of Neostromboli period (Speranza et al. 2008). Moreover, the occurrence of Lc-bearing lava limited to the uppermost stacked sand beds between 96 and 48 cm indicates that the flank collapse involved the summit portion of the volcano during its final phases thus enforcing the hypothesis that flank failure was dominated by retrogressive, multi phase dynamics. On the basis of geochemical and textural data the uppermost thick turbidite occurring at 30–17 cm can be correlated with a flank collapse that occurred during the Recent Stromboli period. An age of ~1 ka can be roughly estimate for this event considering that the landslide deposit is overlain by only 10 cm of mostly hemipelagic mud and that the sedimentation rate in this area was calculated in 9 cm/ka−1 during the last 10 ka (Di Roberto et al. 2008). Even during this collapse the summit of the edifice was likely involved as inferred by the presence of volcanic gas- or acid water-leached pyroclasts in the marine deposits. Such alteration suggests a crater source where an intense volcanic gas/fluid flux is present. Onshore studies have hypothesized that two large scale landslides occurred in the Recent Stromboli period and after the Neostromboli collapse (Tibaldi 2001). However, only one turbidite deposits in the offshore of Stromboli volcano can be correlated with a large-scale landslide event during the Recent Stromboli period. In this perspective marine archive seems to confirm the model proposed by Finizola et al. (2003) in which one of the flank collapses previously identified by Tibaldi (2001) is reinterpreted as a crater collapse (Collapses of the Pizzo pyroclastites into the Fossa craters) occurred after the transition from Neostromboli to Recent Stromboli cycles and before the collapse that gave the NW flank of Stromboli volcano the present form. Both collapses are interpreted to have occurred with multi-phase or retrogressive dynamics as evidenced by the occurrence of stacked sand beds. Recognized multiphase or retrogressive collapse behavior is crucial for modeling of tsunami-producing landslides at Stromboli volcano. In fact all numerical models presently proposed for Stromboli tsunamis assume landslide as a single sliding volumes detaching all at once from NW flank of Stromboli volcano and Distal Turbidites and Tsunamigenic Landslides of Stromboli Volcano 729 thus producing a single tsunami wave. Such an assumption likely results in an overestimation of initial tsunami wave amplitude and thus in a overestimation of the tsunami power. Several thinner, cm-scale turbidites occur in the recovered core thus testifying that also relative small-scale landslides occurred in the last 5 ka on the flank of Stromboli volcano. The average thickness of these turbidites is comparable to the thickness of December 30, 2002 landslide cogenetic turbidite indicating that events like December 30, 2002 have occurred also in the past. These events appear to have greater frequency with respect to that of the much larger failures since almost nine event occur in the last 5 ka. Five tsunami were registered in the last century on Stromboli volcano (Maramai et al. 2005) but only the most recent event of December 30, 2002 is recorded in the marine environment; this can be due to the peculiar morphology of seafloor in the sampling site that allows only the larger and most energetic landslides to be recorded. Alternatively we assume that some of these tsunamis were generated by different sources (earthquake, pyroclastic flows etc). 7 Conclusions and Implications for the Tsunami Hazard Assessment Identification of volcaniclastic turbidite offshore active volcanoes has been shown to be a powerful tool for acquiring information on the occurrence of failure events while providing baseline data for the future. In this work we have documented that during the last 5 ka several possibly tsunamigenic landslides originated from Stromboli volcano generated sandrich turbidity currents which travelled more than 24 km northwards and deposited up to 50 cm thick deposits above a topographic high 200 m above the canyon floor. At least two large events are recorded in marine record of which the former can be very likely correlated to the ∼5 ka old, Neostromboli flank collapse while the latter might correlate to the a younger flank collapse that occurred during the Recent Stromboli period (∼1 ka). Both collapses show multi-phase or retrogressive dynamics as evidenced by the occurrence of peculiar sedimentary structures and by component and geochemical data. Together with large landslides, almost nine small-scale landslides occurring with a greater frequency respect to that of the much larger failures were recorded by sediments, the last of whom is represented by December 30, 2002 event. The research shows that the complete documentation of past potentially tsunamiproducing landslide events of Stromboli is possible and opens new perspectives for the assessment of the tsunami hazard in the southern Tyrrhenian sea. By analogy with Hawaii and Canary islands we confirm that deep-sea sediments can be effectively used to assess age and scale of past landslide events giving an important contribution to the tsunami hazard assessment of this region. 730 A. Di Roberto et al. Acknowledgements We thank the captains and crew of R/V Urania and Logachev. M. Ivanov and the TTR14 and TTR15 cruise scientific parties are also acknowledged for their help in data acquisition. ADR grant was founded within “Piattaforma di ricerca multidisciplinare su terremoti e vulcani (AIRPLANE)” n. RBPR05B2ZJ, founded by Ministero dell’Istruzione dell’Università e della Ricerca. This work was supported by the DPC program: V2 – PAROXYSM. Authors are very grateful to G. De Alteriis and J. 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