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Natural Hazards and Earth System Sciences An interactive open-access journal of the European Geosciences Union
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NHESS | Articles | Volume 20, issue 8
Nat. Hazards Earth Syst. Sci., 20, 2157–2174, 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
Nat. Hazards Earth Syst. Sci., 20, 2157–2174, 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Research article 12 Aug 2020

Research article | 12 Aug 2020

Timing, drivers and impacts of the historic Masiere di Vedana rock avalanche (Belluno Dolomites, NE Italy)

Timing, drivers and impacts of the historic Masiere di Vedana rock avalanche (Belluno Dolomites, NE Italy)
Sandro Rossato1, Susan Ivy-Ochs2, Silvana Martin1, Alfio Viganò3, Christof Vockenhuber2, Manuel Rigo1, Giovanni Monegato4, Marco De Zorzi2, Nicola Surian1, Paolo Campedel3, and Paolo Mozzi1 Sandro Rossato et al.
  • 1Department of Geosciences, University of Padua, Via Gradenigo, 6, 35131 Padua, Italy
  • 2Laboratory of Ion Beam Physics, Otto-Stern-Weg 5, ETH-Honggerberg, 8093 Zurich, Switzerland
  • 3Servizio Geologico, Provincia autonoma di Trento, Via Zambra 42, 38122 Trento, Italy
  • 4National Research Council, Institute of Geosciences and Earth Resources, Padua, Italy

Correspondence: Sandro Rossato (

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The “Masiere di Vedana” rock avalanche, located in the Belluno Dolomites (NE Italy) at the foot of Mt. Peron, is reinterpreted as historic on the base of archeological information and cosmogenic 36Cl exposure dates. The deposit is 9 km2 wide, has a volume of ∼170 Mm3 corresponding to a pre-detachment rock mass of ∼130 Mm3, and has a maximum runout distance of 6 km and an HL ratio of ∼0.2. Differential velocities of the rock avalanche moving radially over different topography and path material lead to the formation of specific landforms (tomas and compressional ridges). In the Mt. Peron crown the bedding is subvertical and includes carbonate lithologies from Lower Jurassic (Calcari Grigi Group) to Cretaceous (Maiolica) in age. The stratigraphic sequence is preserved in the deposit with the formations represented in the boulders becoming younger with distance from the source area. In the release area the bedding, the SSE-verging frontal thrust planes, the NW-verging backthrust planes, the NW–SE fracture planes, and the N–S Jurassic fault planes controlled the failure and enhanced the rock mass fragmentation. The present Mt. Peron crown still shows hundreds-of-metres-high rock prisms bounded by backwall trenches. Cosmogenic 36Cl exposure ages, mean 1.90±0.45 ka, indicate failure occurred between 340 BCE and 560 CE. Although abundant Roman remains were found in sites surrounding the rock avalanche deposit, none were found within the deposit, and this is consistent with a late Roman or early Middle Ages failure. Seismic and climatic conditions as landslide predisposing factors are discussed. Over the last few hundred years, earthquakes up to Mw=6.3, including that at 365 CE, have affected the Belluno area. Early in the first millennium, periods of climate worsening with increasing rainfall occurred in the NE Alps. The combination of climate and earthquakes induced progressive long-term damage to the rock until a critical threshold was reached and the Masiere di Vedana rock avalanche occurred.

1 Introduction
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Landslides have an enormous impact on landscapes and can be a serious threat to human lives and buildings. Assessment of the potential for future events is distinctly dependent on knowledge of the conditions under which past failures occurred in the immediate vicinity (Samia et al.2017). This entails detailed analysis and interpretation of driving factors as well as possible triggers of past events (Eisbacher and Clague1984; Nicoletti and Sorriso-Valvo1991; Hungr2006; Strom2006; Hermanns and Longva2012). Bedrock bedding, faults, fractures and other discontinuities predispose a rock mass to fail (Stead and Wolter2015). Damage accumulation in rock (fatigue) contributes to the location of failure (Friedmann et al.2003; Brideau et al.2009; Parker et al.2013; Stead and Eberhardt2013; Preisig et al.2015), while seismic shakings (Keefer1993; Friedmann et al.2003; Dunning et al.2007; Cui et al.2011; Stead and Eberhardt2013) and periods of extreme rainfall (Guzzetti et al.2008; Tsai and Wang2011; Loew et al.2017; Preisig et al.2015) can trigger landslides.

Figure 1Simplified regional geological map (black dashed-line box indicates location of Fig. 3). The map is based on Bosellini et al. (1981), Masetti and Bianchin (1987), Bigi et al. (1990), and Costa et al. (1996). Epicentres of earthquakes from the last 2 millennia are shown with colour coding and year of occurrence (source: Parametric Catalogue of Italian Earthquakes, 2015 version Rovida et al.2016). The base map is the SRTM-derived digital elevation model (30 m cells) (source:, last access: 17 October 2019). The structural setting is shown in the upper left inset (based on Doglioni1990). AST: Alpine Sole thrust; BL: Belluno thrust; BS: Belluno syncline; CP: Coppolo-Pelf anticline; CVM: Val Carpenada–Val di Vido–Val Madonuta thrust; ESA: eastern Southern Alps thrust system; FPT: frontal Penninic thrust; IL: Insubric line; PG: Pala Alta–Gresal; PM: Pala Bassa–Val Medone; VS: Valsugana thrust; VV: Vittorio Veneto thrust.

From this perspective, the Italian landslide inventory project (IFFI; Trigila et al.2007;\\cartografia-on-line/, last access: 11 May 2020) is the ideal starting point for hazard maps. These are tools for landscape management and civil protection plans. They thus require continuous updating and accurate input data. In the study area (Fig. 1), the southern side of Mt. Peron (Belluno Dolomites, NE Italy) is classified in the most recent landslide hazard map (, last access: 11 May 2020) as an “attention area” (i.e. a failure is possible, but an evaluation is needed). In 2011 a rockfall (volume ∼1000 m3, blocks up to 2.5 m3) detached from the upper part of Mt. Peron, which led the Municipality of Peron to commission the evaluation of the hazard along its southern cliff (Di Giusto2012). Numerous partially detached rock prisms were recognised, up to 18 000 m3 and with trenches up to 50 cm wide. According to Di Giusto (2012), nine out of 16 pillars are at risk for failure in the case of an earthquake.

The IFFI catalogue, the landslide hazard map and the evaluation by Di Giusto focused on the Mt. Peron southern wall and the scree slope, neglecting the well-known deposit of Masiere di Vedana that lies on the southern plain (Abele1974; Eisbacher and Clague1984; Pellegrini et al.2006). This is also known as “Rovine di Vedana” (Mazzuoli1875; Squinabol1902; Montandon1933) or “Marocche di Vedana” (Dal Piaz1912; Venzo1939). The deposit covers an area of 8–9 km2, has a maximum thickness of 40 m and has an estimated volume of 100–120 Mm3 (Abele1974; Genevois et al.2006; Pellegrini et al.2006). The Masiere di Vedana is one of the largest catastrophic events in the Alps (Heim1932; Abele1974; Eisbacher and Clague1984), comparable with large events in the Himalayas (e.g. Hewitt2006; Hewitt et al.2008; Mitchell et al.2007), Rocky Mountains (e.g. Blais-Stevens et al.2011; Charrière et al.2016) and Andes (e.g. Hermanns et al.2004; Welkner et al.2010).

As there is no consensus on the age and dynamics of the Masiere di Vedana, a re-evaluation is needed in light of hazard assessment. The Masiere di Vedana deposit was interpreted as a glacial deposit (Hoernes1892), a landslide transported by a glacier during the late glacial (Mazzuoli1875; Squinabol1902; Dal Piaz1912; Venzo1939) and as the result of a catastrophic flood due to collapse of a natural dam (Taramelli1883). Some other authors proposed as origin for the deposit (1) the combined effect of a landslide over a glacier, followed by a second landslide that evolved into a rock avalanche (Pellegrini2000; Pellegrini et al.2006), and (2) a small rockslide followed by a larger rock avalanche (Genevois et al.2006). The age attribution for the deposit ranges from the late glacial (Pellegrini et al.2006) to historical times (Piloni1607; Miari1830).

Amongst all types of landslides, rock avalanches are particularly relevant, being both difficult to predict (Hungr2006) and representative of a very high risk for the population living in mountain areas (Guzzetti2000; Hungr2004; Geertsema et al.2006; Evans et al.2007; Sosio et al.2008; Cui et al.2011; Hermanns and Longva2012; Mitchell et al.2020). The moving masses are composed of dry debris, which in subaerial settings ranges from about 0.5 to more than 10 000 Mm3 (Crosta et al.2007). The initial phase, rockfall or rockslide, evolves into a flow-like movement of crumbling rock debris, sized from clay/silt up to decametric boulders, which can travel for several kilometres, even uphill, and overcome obstacles up to some hundreds of metres high (e.g. Hungr et al.2001; Mangeney et al.2010; Bowman et al.2012). Rock avalanche deposits are characterised by inverse grading of the sediment, with large blocks dominating the carapace, the inclusion of path material and, in some cases, preservation of the stratigraphic sequence (Hewitt2002; Strom2006).

The aim of this study is to provide dating and to evaluate driving factors, potential triggers, and process dynamics of the Masiere di Vedana rock avalanche, in light of a better assessment of the hazard, potential extent and runout in similar settings.

2 Geological setting
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The Masiere di Vedana lies at the mouth of the Cordevole Valley in a broad plain at the confluence of the Cordevole and Piave rivers (Fig. 1). Mt. Peron (1486 m a.s.l.) is the southwestern peak of the Schiara Group (highest peak: Mt. Schiara: 2565 m a.s.l.). Mt. Peron is composed, from the west to the east, by the Calcari Grigi Group (Lower–Middle Jurassic), Vajont Limestone (Middle Jurassic), Fonzaso Formation, and Rosso Ammonitico (Upper Jurassic) and Maiolica (Cretaceous) limestones. Their distinctive characteristics, useful for tracking the source of the Masiere di Vedana deposit, are thick-bedded, fossiliferous blue-grey limestones (Calcari Grigi Group); and thick-bedded, locally oolitic limestones and calcarenites (Vajont Limestone); thick-bedded siliceous limestones with clay interbeds (Fonzaso Fm.); pink to red nodular limestones rich in ammonites (Rosso Ammonitico); thick-bedded, white limestones with chert nodules (usually grey to black) containing nannofossils, calpionellids and radiolaria (Maiolica). Scaglia Rossa and the Cenozoic formations (Belluno flysch, Belluno glauconitic sandstone, Bastia siltstone, Libano sandstone and Bolago marl) crop out at the base of the Piz Vedana (Fig. 3), form the Castel Cuch ridge and underlie the fluvial plain between the Mis and Cordevole rivers. Outcrops of cemented Pleistocene fluvial gravels (“Roe” or “Sass Muss conglomerate”; Costa et al.1996) are located just to the west of the present course of the Cordevole River (near the town of Vignole in Fig. 3).

The investigated area is bounded by Alpine tectonic lineaments (Fig. 1): the Valsugana thrust fault to the north, and the S-verging Alpine folds and thrusts to the south (Doglioni1990). Mt. Peron belongs to the hanging wall of the WSW–ENE-oriented Belluno thrust, one of the main tectonic lineaments of the eastern Southern Alps (Doglioni1990; Galadini et al.2005), which crops out at the northern limb of the Belluno syncline. The sedimentary strata of the forelimb are sub-vertical to slightly overturned (Doglioni1990; Costa et al.1996), and they converge into the Belluno thrust. The Val Carpenada – Val di Vido – Val Madonuta thrust is the backthrust of the Belluno thrust (Costa et al.1996). To the east, reactivated Jurassic faults (Masetti and Bianchin1987) displaced the Val Carpenada – Val di Vido – Val Madonuta thrust (Fig. 1) and induced a wealth of fractures in the Mt. Peron rock wall (Fig. 2). The Mt. Peron is at the nucleus of an ENE–WSW-oriented anticline with a very steep forelimb, followed southwards by the Belluno syncline (Fig. 2a) that hosts Cenozoic sedimentary units (Costa et al.1996).

Figure 2Structural scheme of the Mt. Peron release scarp. (a) Schematic geological cross section. (b) Photograph with major structural elements and larger karst caves (black-and-white circles) highlighted. (c) Lower-hemisphere stereographic projection of principal structural elements. Colours in (b) and (c) correspond to the following: bedding (black), N–S reactivated Jurassic fault-related planes (grey), basal trenches and other high-angle fractures connected to the Belluno thrust (yellow) and backthrust (red), fractures related to the NNW–SSE fault system (light blue), their conjugates (pink), and high-angle fractures with the same orientation (green).


Figure 3Geological map of the study area, based on our own field surveys and previous studies (Pellegrini2000; Pellegrini and Caneve2005), overlying a 5 m cell DTM (open data released by Regione Veneto:, last access: 17 October 2019). The boundary of Mt. Peron rock avalanche deposits is marked with a solid white line, whilst the contact between Quaternary sediments and bedrock is shown with a solid black line. The locations of boulders sampled for dating (red stars) and/or thin-section analysis (green stars) are shown. Obtained 36Cl exposure ages are in kiloannum. Sites of Roman and pre-Roman archeological findings are indicated by red squares (from Capuis et al.1988). Solid lines in the left frame correspond to the traces of the stratigraphic profiles in Fig. 4. Location of stratigraphic sections (yellow ellipses; Fig. 5) and palaeo-Cordevole paths (black dashed arrows) are shown. The extent of Fig. 6 (dotted black box) and Fig. S4 (solid black box; Supplement) is indicated. In the lower right, a stratigraphic sketch of bedrock formations cropping out in the Belluno area is given (modified from Costa et al.1996).

3 Methods
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3.1 Field survey, structural analysis and remote sensing

Detailed geomorphological maps (Caneve1985; De Zorzi2013), aerial and satellite images (Google Earth and Bing databases), and DTM analysis (cell size: 5 m, vertical accuracy: 30 cm;, last access: 17 October 2019) were used to obtain topographic profiles and to estimate the area of the Masiere di Vedana deposit. The areal distribution of lithologies in the deposit was gauged by observation of boulders in the field and verified by thin-section analysis (Sect. S1 in the Supplement). Six boreholes, up to 3 m deep, were taken in the fine-grained sediments of the Torbe area (Fig. S2a) with a hand auger (Edelman combination type, EjikelkampTM), which allows the extraction of 10 cm wide cylindrical cores. Orientations of bedrock discontinuities, such as bedding, foliation, joints, fractures and faults, were measured in the southern wall of Mt. Peron.

3.2 Cosmogenic 36Cl exposure dating

Twelve different boulders located in topographically high positions with respect to the surroundings within the deposits were sampled for dating with cosmogenic 36Cl. For boulders VB13 (VB13a, VB13b) and VB14 (VB5 same boulder as VB14) two samples were taken. Samples were taken to cover the full extent of the deposit, from right near the source area to the distal sector.

For 36Cl sample preparation we used the method of isotope dilution as described by Ivy-Ochs et al. (2004). Total Cl and 36Cl were determined at the ETH AMS facility of the Laboratory for Ion Beam Physics (LIP) with the 6 MV tandem accelerator. The 36Cl∕Cl ratios of the samples were normalised to the ETH internal standard K382/4N with a value of 36Cl/Cl=17.36×10-12, which is calibrated against the primary 36Cl standard KNSTD5000 (Christl et al.2013; Vockenhuber et al.2019). Full process chemistry blanks (3.4×10-15) were subtracted from measured sample ratios. All 14 rock samples were processed. Only seven were measured successfully due to too high 36S, also in relation to the very low 36Cl concentrations in these samples. All measured data are presented here. Major and trace element concentrations were determined with X-ray fluorescence (XRF) (Sect. S3) and inductively coupled plasma mass spectrometry (ICP-MS) (Sect. S4), respectively. We calculated surface exposure ages with the LIP ETH in-house MATLAB code based on the parameters presented in detail in Alfimov and Ivy-Ochs (2009, and references therein). A production rate of 54.0±3.5 36Cl atoms (g Ca)−1 yr−1, which encompasses a muon contribution at the rock surface of 9.6 %, and a value of 760±150 neutrons (g air)−1 yr−1 were found. These values are in excellent agreement with production rates recently published by Marrero et al. (2016). Production from all major elements and through low-energy neutron capture in light of the trace elements (Table S4a) was fully considered. Production rates were scaled to the latitude, longitude and altitude of the sites based on Stone (2000). No correction was made for karst weathering of the boulder surfaces (see Styllas et al.2018). The extent of karst dissolution on the boulder surfaces varies significantly from boulder to boulder. Implementing a rate of 5 mm ka−1 would change the ages by less than 4 %, which does not affect any of the conclusions drawn here. Stated errors of the exposure ages (Table 1) include both analytical uncertainties and those of the production rates (Alfimov and Ivy-Ochs2009). Two different surfaces of boulder 13 were analysed (VB13a, 1.45±0.12; VB13b, 1.45±0.12 ka); the weighted mean of 1.45±0.08 ka is used for further discussion.

Table 1Sample site information, AMS data and 36Cl exposure ages. Samples VB3a and VB3c are not from the same boulder, whilst VB13a and VB13b are (weighted mean given). No erosion correction was made.

a Shielding includes surrounding topography and dip of sampled surface. b Sample from same surface on same boulder; mean age is 1.45±0.08 ka.

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4 Results
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4.1 Mt. Peron release area

The Mt. Peron scarp is 700 m wide and 600 m high, S-to-SW facing, and partially circular. No secondary scarps are present. Numerous faults and fractures are visible on the wall (Fig. 2b) and are grouped into five main discontinuity sets (Fig. 2c). These comprise (1) bedding, (2) WSW–ENE-directed frontal thrust planes, (3) NW-verging backthrust-related planes, (4) NW–SE-aligned local conjugate fracture plane sets, and (5) persistent N–S-oriented planes interpreted as reactivated Jurassic faults (Masetti and Bianchin1987). Bedding is nearly vertical, and its orientation ranges from 146∕78 to 170∕80 (dip directiondip angle). The Belluno thrust, average orientation 337∕64 (Costa et al.1996), crops out at the base of the steep wall, whilst other Belluno thrust planes (295∕53 to 340∕67) were measured higher up along the wall (Fig. 2b). The NW-verging planes related to the backthrust are 111∕15 to 175∕54 and steepen to 80 at higher elevations along the wall. The NW–SE-aligned fractures are 209∕16 to 245∕32 with an associated conjugate set, from 20∕44 to 62∕30, and nearly vertical fractures with a dip direction of 219 to 255. The N–S-striking fracture planes dip both to the east (75∕40 to 83∕75) and to the west (240∕71 to 299∕18). Today a myriad of large and small individual rock prisms bounded by these discontinuities are present in the upper part of the release area.

4.2 Masiere di Vedana rock avalanche deposit

The deposit covers an area of ∼9 km2 from the base of Mt. Peron southwards to Roe Basse (∼5 km) and westwards to Mis River (∼3 km; Fig. 3). By means of open sections, the thickness of the deposit is estimated ∼10 m in the proximal area (near boulder VB2, Fig. 3), ∼15 m in the central sector near Torbe, >30 m near the boundary between the Vedana and Masiere sectors (Ponte Mas section, Fig. 4), ∼5 m in the Masiere central sector, and ∼15 m in the southern (distal) sector (Suppiei section, Fig. 4). Using a mean thickness of 20 m, a rough estimation of the total debris volume of ∼170 Mm3 is obtained. Such a volume corresponds to a released rock mass of about 130 Mm3 (bulking coefficient of 25 %; see Genevois et al.2006). With a vertical drop (H) of about 1150 m (from the top of Mt. Peron: 1486 m a.s.l., to Roe Basse area: ∼340 m a.s.l.) and a travel distance (L) of about 5900 m (Fig. 3), we calculate an HL ratio of ∼0.2 (Fahrböschung angle of 11). Based on spatial pattern, boulder lithology and morphological character, we distinguish five sectors of the deposit: Peron, Vedana, Torbe, Masiere and Roe (Roe Alte and Roe Basse).

Figure 4Geologic profiles of the Mt. Peron rock avalanche deposits (modified from Costa et al.1996). Traces of the profiles are shown in the small DTM and in Fig. 3a, their extent being equal. The discussed sectors of the Mt. Peron rock avalanche, Vedana, Torbe, Masiere and Roe Alte, are indicated, along with the location of Ponte Mas and Suppiei stratigraphic sections (Fig. 5g and h). The vertical bedding and interpreted Belluno thrust are shown schematically. Note the preservation of bedrock stratigraphic order in the rock avalanche deposits from older to younger, i.e. from proximal to distal: Calcari Grigi Group, Vajont Limestone, Fonzaso Formation–Rosso Ammonitico–Maiolica.

The Peron sector includes the talus apron deposits at the foot of Mt. Peron, the rock avalanche deposits on the east side of the river and the terrace of the town of Peron (at about 380 m a.s.l.). Boulders at the foot of the slope range up to 20 m in diameter (Fig. 5a). Three boulders in the Peron sector were dated with cosmogenic 36Cl (Fig. 3; Table 1): VB3a (Rosso Ammonitico; 1.83±0.28 ka), VB3c (Fonzaso Fm.; 3.62±0.41 ka) and VB14a (Calcari Grigi Group; 2.39±0.39 ka). Based on the trend of all obtained ages, the age of VB3c is interpreted as an outlier, its age possibly reflecting the presence of inherited 36Cl due to pre-exposure. The town of Peron lies on a terrace made of rounded gravel layers with rare sand lenses that are interfingered with talus deposits (Caneve1985).

Figure 5Photos of the deposits (a decametric boulder, Peron alluvial terrace; b plurimetric boulder, Vedana sector; c metric boulders, Masiere sector; d toma relief in the Torbe sector; e open section of a toma, Torbe sector; f karst evidence on a boulder, Masiere sector) and stratigraphic sections described in the text (g Ponte Mas section: incorporation of the underlying glacial deposit (green) into the rock avalanche deposit (light blue) is shown; h Suppiei section: glacial sediments (green), covered by rock avalanche deposit (light blue), rest directly on bedrock (red); locations in Figs. 3 and 4).


In the Vedana sector, the rock avalanche deposit displays an irregular forested topography with relief on the order of tens of metres (Fig. 5b). Huge blocks hundreds of cubic metres in size, mostly made of Calcari Grigi, dominate the carapace. This covers the main body of the deposit made of shattered rocks, which is comprised of very angular clasts (up to tens of centimetres in diameter) in a matrix of silty sand. The VB2 boulder (Calcari Grigi) gave an age of 1.49±0.26 ka; it lies on top of an ∼10 m thick sequence of rock avalanche deposits. In the Ponte Mas quarry (Figs. 3 and 5g), an open section showed glacial till (up to 3 m thick) incorporated into the base of the rock avalanche deposit; its original bedding is completely obliterated. This sediment is >30 m thick and is composed of sub-rounded clasts (up to 20 cm in length), some of them striated, supported by a silty clay matrix. Clasts are sedimentary and volcanic, reflecting the catchment of the Cordevole palaeoglacier (see Pellegrini et al.2006). Several ENE–WSW-trending incisions cut through the Vedana and Torbe sectors (main ones highlighted in Fig. 3). Irregular patches of sandy-silty and fine gravel sediments are found in the Vedana low-lying areas between the blocky reliefs.

Figure 6Transverse ridges in the southwestern part of the Masiere sector (basemap source: © Google Earth). Location of image shown in Fig. 3. The rock avalanche moved (from north to south) over a slight topographic high made up of Pleistocene conglomerate (see Fig. 4); the ridges are interpreted as compressional. White stars indicate locations where the contact between the rock avalanche and the conglomerate is exposed.

The Torbe sector encompasses the distal northern lobe of the rock avalanche, characterised by 10 to 20 m high isolated hills and hummocks (Fig. 5d) that emerge from a flat topography. They are roughly aligned ENE–WSW, are circular at the base and have slope angles of 35–40. They are made of very angular Calcari Grigi boulders and clasts, with many jigsaw puzzle structures in a sandy, gravelly matrix (Fig. 5e). Such morphological structures are “toma” (Turnau1906; Abele1974; More and Wolkersdorfer2019). They are found in association with some large rockslides and are mainly made of landslide material, in many cases showing a gradation from very comminuted fragments in the outer part to less fractured material at the core (see von Poschinger and Ruegg2012; More and Wolkersdorfer2019). Six cores taken in the flat area between the hills (see Fig. 3 and Sect. S2) show up to 2 m of silty sand above the rock avalanche becoming more fine upwards. Torbe is crossed by the largest incision of the whole Masiere di Vedana (Fig. 3), ENE–WSW trending, ∼50 m wide and up to 20 m deep with respect to the mean topographic surface. Cenozoic lithologies crop out at the base of this incision, with the rock avalanche deposit being ∼15 m thick. A shallower incision, a few metres deep, is located at the base of the Piz Vedana slope, still conveying a small amount of water coming from the Vedana Lake.

The Masiere sector is strikingly different from Vedana and Torbe. It is a bleak, vegetation-free, desert-like sea of limestone blocks, mainly of dolomitised Vajont Limestone (Fig. 5c). Boulders up to 3 m in diameter and abundant angular and sub-angular clasts, with almost no matrix, are present in the surficial part. In the southern part of Masiere, numerous 2–3 m high and up to 150 m long ridges, aligned roughly E–W, are present (Fig. 6). The contact of the rock avalanche with the underlying Pleistocene conglomerate crops out near the southern boundary of the Masiere (white asterisks in Fig. 6), where the deposit is only ∼5 m thick. Next to the northern boundary of Masiere, the Cordevole River flows upon the Cenozoic rocks of the Castel Cuch ridge, covered elsewhere by the rock avalanche. An ENE–WSW-trending shallow incision (Fig. 3) with associated well-sorted, medium-to coarse-grained sandy deposits is present, almost parallel to Castel Cuch. A roughly N–S trending incision, a few metres deep, ∼10 m wide and about 500 m long, is located just to the west of the Cordevole River. The town of Mas is built upon a flat terrace, mainly made of sorted rounded gravels with a sandy matrix, that bounds the Masiere to the east.

Roe Alte and Roe Basse comprise the distal sector of the Masiere di Vedana to the south (Fig. 3), where there are angular clasts up to 20 cm in diameter and very few boulders immersed in a sandy matrix are scattered in the meadows. Boulders belong to the Fonzaso Formation, Rosso Ammonitico and Maiolica, with very few of them made of Vajont Limestone. Roe Basse is made of silty/sandy alluvial sediments deposited by the Gresal and other minor streams coming from the east, mantling the rock avalanche deposit on the northwestern side. The Suppiei section, 100 m long and 25 m high, on the left flank of the Cordevole River (Figs. 3 and 5h; Sect. 5), shows the Bolago Marl unconformably overlain by 0.5–2 m of glacial till. This is in turn covered, with a sharp and undulated contact, by up to 20 m of rock avalanche debris decimetric in size, with boulders (∼1 m diameter) on top. On the Roe Alte rocky upland, the rock avalanche is at most 2 m thick, with rare boulders (1–2 m diameter). Two boulders made of Vajont Limestone (Fig. 3) have been dated with 36Cl (VB12, 2.35±0.21 ka; VB13, 1.45±0.08 ka; Table 1). South of the town of Mas, the Cordevole River flows into narrow meanders entrenched ∼20 m into rock avalanche deposits, alluvial material, glacial sediments and bedrock. The terrace of the Vignole village is almost totally made of rock avalanche debris, despite being remarkably flat.

5 Interpretation and discussion
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5.1 Age of the Mt. Peron rock avalanche

36Cl surface exposure ages from boulders all across the deposit range from 1.45±0.08 to 2.39±0.38 ka (Table 1). All ages show a good overlap within uncertainties. A single sample (VB3c) gave a result markedly different from the others: 3.62±0.41 ka. Although this age may point to pre-exposure of the sampled boulder surface (see Sewell et al.2006; Merchel et al.2013), as for example seen at Lavini di Marco (Martin et al.2014), the possibility exists that this boulder is part of a partially buried older deposit located right at the foot of Mt. Peron. The poorly developed karst dissolution features (0.5–1 cm deep karren) on the tops of many boulders suggest as well that the deposit is relatively young. The average of 36Cl ages, excluding VB3c as an outlier, is 1.90±0.45 ka. The uncertainty of the mean is based on the cumulative probability of uncertainties for all samples based on a Gaussian probability distribution (one sigma level). Such a value indicates that the rock avalanche, considering the error range, occurred during historical times, between 340 BCE and 560 CE. These results are in stark contrast to previous reconstructions, which pointed to a late glacial age (Mazzuoli1875; Hoernes1892; Squinabol1902; Dal Piaz1912; Venzo1939; Genevois et al.2006; Pellegrini et al.2006). The dates 1113, 1114, and 1117 CE proposed for the main landslide event suggested by some authors (Piloni1607; Miari1830) may be associated with the Verona earthquake at 1117 CE. That event was clearly felt in the Belluno area, inducing numerous landslides (Guidoboni et al.2005), but its age is not consistent with the cosmogenic dates on the Masiere di Vedana. To search for independent constraints for the age of the main landslide event, detailed research in numerous archives and chronicles was undertaken. This area during Roman time was largely and uniformly inhabited by “incolae” for agricultural aims, being the area located next to the Claudia Augusta Altinate road connecting Feltre with Belluno (Fig. 1) (Alpago-Novello1957, 1988). The presence of a Roman bridge crossing the Cordevole River north of Mt. Peron indicates there was a connection to the main Claudia Augusta Altinate road. While numerous Neolithic and Roman archeological sites are reported around the Masiere di Vedana (Capuis et al.1988; Frassine et al.2016), no Roman or pre-Roman archaeological remains have been found within the rock avalanche deposits (Fig. 3). If the Masiere di Vedana deposit was settled after Roman times, previous settlements eventually located in the area would have been buried by the event. The oldest record for the post-event human presence is a hospice built in the 12th century CE (1155 CE; Magoga and Marin1998) on the fluvial terrace near the village of S. Gottardo (Fig. 3). Therefore, historical data indicate a time frame between late Roman times and the early Middle Ages.

The age uncertainties do not allow us to directly determine if the Masiere di Vedana deposit was due to a single failure or multiple events. The distribution of the available dates has no spatial pattern across the deposit, no physical boundaries occur and no buried soil layers have been found within the deposits. Moreover, the volume and HL ratio of the landslide (see Sect. 5.2 for further discussion), together with the morphology of the scarp and the absence of secondary scarps, indicate a single huge catastrophic event. Therefore, a single rock avalanche occurred in historical time, contradicting previous interpretations (e.g. Genevois et al.2006; Pellegrini et al.2006). Such a young age implies that glacial unloading was not responsible for the destabilisation of the southern side of Mt. Peron and makes a re-evaluation of the involved driving factors and potential triggers necessary.

5.2 Release, emplacement and post-event modification of the deposit

A schematic reconstruction of the reach of the Cordevole Valley involved in the rock avalanche can be depicted before, during and after the event. Before the rock avalanche, the Cordevole River flowed through a gentle rolling landscape along the foot of Piz Vedana and through a breach cutting the Castel Cuch bedrock ridge just north of the village of Mas (Figs. 3 and 7a). Topographic highs, like Castel Cuch and Roe Alte, were at that time mantled with glacial sediments attributable to the last glaciation.

Figure 7Curvilinear topographic profiles (10× vertical exaggeration) showing the relationship between the bigger incisions and the external main surfaces related to the rock avalanche and the post-event evolution. Profiles correspond to the present course of Cordevole creek (blue line in a) paired with the main topographic surfaces on its left bank (green line in a) and the main incision passing through the Torbe and Vedana sectors (blue line in b) paired with the main topographic surfaces on its left side (green line in b). Traces of the profiles are shown in the small DTM (open data released by Regione Veneto:, last access: 17 October 2019), which corresponds to Fig. 3.

The rock avalanche involved the detachment of about 130 Mm3 from the southern face of Mt. Peron. Initial movement was sliding along the NW-verging backthrust-related planes (Fig. 2). En bloc movement may have been only briefly sustained as the pervasive network of fractures favoured a massive collapse. The rock mass immediately evolved into a rock avalanche whose volume increased by fragmentation up to 170 Mm3 and spread out onto the flat plain below. The HL ratio of ∼0.2 (apparent friction angle of 11) and comparison with empirical and modelling plots of HL vs. volume (e.g. Spreafico et al.2018; Aaron and McDougall2019) mark the Mt. Peron event as extremely mobile. As a basis for comparison, the Fernpass rock avalanche has a HL of 0.9, a volume of 1 km3 and a significantly longer runout distance of 15.5 km (Prager et al.2009). It may be possible to glean information about the failure style from the distribution of boulder lithologies, which follows the stratigraphic order of the bedrock exposed in the source area. This has also been noted at the Tschirgant rock avalanche deposits in Austria (Dufresne et al.2016) and the Frank slide in Canada (Charrière et al.2016). In the Mt. Peron bedrock, the lithologic sequence from west to east is Calcari Grigi Group, Vajont Limestone, Fonzaso Fm., Rosso Ammonitico and Maiolica. This pattern is mirrored in the deposits (Figs. 3 and 4): Vedana and Torbe are dominated by Calcari Grigi Group, Masiere by Vajont Limestone, and Roe by Fonzaso Fm., Rosso Ammonitico and Maiolica. Experiments and modelling suggest that this kind of zonation is likely to occur when the sliding mass propagates as a flexible sheet, with laminar flow (Friedmann et al.2006).

Several landforms within the Masiere di Vedana provide further clues on the processes of propagation and emplacement. The tomas in the Torbe sector suggest differential velocities in the moving mass propagating on a water-saturated substrate (Strom2006; Prager et al.2009; Dufresne2012; Dufresne et al.2016; Aaron et al.2017). Tomas, with likely similar origin, are present in the distal deposits at Fernpass in Tyrol (Prager et al.2009) and at Flims (von Poschinger and Ruegg2012). Recently, More and Wolkersdorfer (2019) proposed for the toma hills at Fernpass an alternative origin from internal erosion by suffusion. However, at Masiere di Vedana the fluvial deposition above the rock avalanche suggests that the suffusion process can be ruled out. In contrast to the increased mobility seen in the Torbe sector, in the central Masiere area, landforms indicative of stalling are present (Fig. 6). The stacked subparallel transverse ridges, much like those noted at Tschirgant (Patzelt2012; Dufresne et al.2016; Ostermann et al.2017), with slight overrunning of the ridges in front by those behind, indicate slowing down of the moving mass due to longitudinal compression (Nicoletti and Sorriso-Valvo1991; Dunning et al.2005; Strom2006; Dufresne et al.2016). Outcrop relationships (Fig. 6) suggest that the Pleistocene conglomerate inhibited the rock mass flow, in combination with the slight uphill gradient. The ridges at Masiere were previously interpreted as neotectonic lineaments by Baggio and Marcolongo (1984).

After the event, the Cordevole River changed its channel several times. The rock avalanche blocked the river, creating accommodation space to the north, where possibly a temporary lake formed. The river was then forced to flow westward across the deposit as indicated by the palaeochannels in the Vedana and Torbe sectors (black arrows, Fig. 3), taking different paths at different times. Low-lying areas were progressively filled, as shown by the sequence recorded in core TB1 becoming more fine upwards (Fig. S2a). The Torbe, Vedana and Peron terraces are flat surfaces at ∼380 m a.s.l. (Fig. 7b). Afterwards, a further sedimentation was hindered by the trenching in Torbe. The Cordevole River finally breached the landslide deposit to the southeast, through the Castel Cuch ridge made of Cenozoic rocks (Fig. 3). The river initially flowed from Mas (about 375 m a.s.l.; green line in Fig. 7a) to the southern flank of Castel Cuch as suggested by the still recognisable palaeochannel (Fig. 3) filled with well-sorted, medium- to coarse-grained sand (Caneve1985). Subsequently, the Cordevole moved to the eastern side of the Pleistocene conglomerate cliff (Fig. 3). The final diversion of the river formed the Peron, Mas and Vignole terraces and currently flows some metres below with upstream migration of the knickpoint (Fig. 7).

5.3 Driving factors and potential hazard

In the Cordevole and Piave valleys many landslides have been recorded (Fig. 8) and have caused a great deal of damage and casualties (Rossato et al.2018). Rock avalanches such as Masiere di Vedana are difficult to predict (Hungr2006) and may be very destructive due to their huge volume and extreme runout (Guzzetti2000; Hungr2004; Geertsema et al.2006; Evans et al.2007; Sosio et al.2008; Cui et al.2011; Hermanns and Longva2012). In light of the results we obtained, the search for the drivers of the Masiere di Vedana rock avalanche is both timely and imperative. Even if what determines the moment of failure may be difficult to pinpoint, increased pore pressure and seismic ground shaking are the primary candidates in such cases (Wieczorek1996; Schuster and Wieczorek2002; Takahashi2001). However, rock avalanches may start without a definite external trigger, the progressive accumulation of rock fatigue being enough to overcome the resisting forces of the rock mass. This is the case, for example, of the Tsatichhu landslide (10 September 2003) in Bhutan (Dunning et al.2006) and the several Randa events (total of 30 Mm3) in 1991 in Switzerland (Loew et al.2012; Stead and Eberhardt2013).

Figure 8Largest and most damaging (in terms of human lives) landslides located near Mt. Peron (base map is a SRTM-derived digital elevation model with 30 m cells; source:, last access: 17 October 2019). Volumes of deposits correspond to the size of the symbols; casualties are shown with colour coding. AB: Alta Badia, several events between 11 500 BCE and present (Borgatti et al.2004); AL: Alleghe, 1771 CE (Ermini and Casagli2003); AN: Antelao, 1814 CE (Montandon1933); CM: Col Mandro, 1825 CE (Montandon1933); CO: Cortina d'Ampezzo, several events between 10 700 and 2000 BCE (Borgatti and Soldati2010); FA: Fadalto, late glacial to present (Pellegrini and Surian1996); LV: La Valle, 1701 CE (Montandon1933); MA: Marziai, 17 500–15 000 BCE (Pellegrini et al.2006); MS: Mt. Salta, 1674 CE (Montandon1933); PE: Pecol, 1841 CE (Montandon1933); MP: Mt. Peron, late Roman times – early Middle Ages (this work); SI: Siror, 1348 CE (Montandon1933); VA: Vajont, 1963 CE (Borgatti et al.2004); VC: Val Cia, 1882 CE (Montandon1933); VS: Valle San Lucano, 1908 CE (Aldighieri et al.2016).

The Belluno area has high mean annual rainfall (1643 mm in the time interval 1994–2018 at, last access: September 2019) and is prone to extreme rainfall events (e.g. >300 mm of rain at Sospirolo during a single event: 27 October–1 November 2018; ARPAV2018). Moreover, at the time of the Masiere di Vedana rock avalanche, between late Roman times and the early Middle Ages, the southeastern Alps and northeastern Italy were affected by various periods of climate degradation during which several extreme meteorological events occurred (Wirth et al.2013; Rossato et al.2015). One of these extreme events had an impact all over Europe between 50 and 250 CE, with marked intensity and widespread flooding recognisable in the stratigraphic records (Macklin et al.2006; Benito et al.2015; Rossato et al.2015; Cremonini et al.2013). This period of severe rainfall could possibly have been the trigger for the Masiere di Vedana rock avalanche or at least may have acted as a driving and destabilising factor. Likewise, the 1987 Val Pola rock avalanche in the central Alps was triggered by a period of exceptional rainfall (Crosta et al.2004).

The Veneto region is prone to earthquake activity, and the study area is categorised as level 2 seismic hazard (“possible strong earthquakes” in Ordinanza del PCM n. 3519/2006), as the historical record testifies (up to Mw=6.5Viganò et al.2013, 2015; Rovida et al.2016). Continuous instrumental monitoring of the Belluno area dates back only to 1977 (Sandron et al.2014). Preceding catalogued major seismic events in the region are based on either historical chronicles, dated building damage and/or observed rockfalls (Piloni1607; Taramelli1883; Guidoboni et al.2005, 2018). Within a radius of 30 km from Mt. Peron, eight earthquakes with Mw greater than 5.0, and one exceeding 6.0, were recorded (Fig. 1). The strongest (Mw=6.3) occurred just 20 km to the east of Mt. Peron on 29 June 1873 (Rovida et al.2016, and references therein). Severe damage to Belluno city was reported during the Asolo (25 February 1695 CE; Mw=6.4), Friuli (6 May 1976 CE; Mw=6.5) and Verona (3 January 1117 CE; Mw=6.5) earthquakes whose epicentres were located, respectively, 60, 65 and 140 km away (Guidoboni et al.2018). As for the time frame suggested by our chronology, historical records report an important seismic event in July 365 CE that resulted in damage to the city of Belluno (Piloni1607). These data suggest that the Belluno area is sensitive to seismic shakings originating even hundreds of kilometres away. Galadini et al. (2005) discuss evidence that active tectonics plays a key role in the reported intensification of slope instability registered in this area during the last 1500 years. The most important effect of the frequent seismic activity is the progressive increase in the rock fatigue, with the formation of failure surfaces and the removal of rock bridges and roughness on discontinuity planes (Friedmann et al.2003; Brideau et al.2009; Parker et al.2013; Stead and Eberhardt2013; Preisig et al.2015; Gischig et al.2016). Earthquakes have been suggested as triggers for several Alpine rock avalanches (e.g. Prager et al.2009; Grämiger et al.2016; Ivy-Ochs et al.2017; Köpfli et al.2018) and are known to have caused several rockfalls in the Belluno area (e.g. Piloni1607; Miari1830; Guidoboni et al.2005). Moreover, they are considered to be a possible trigger for failure of some pillars located on the southern side of Mt. Peron (Di Giusto2012).

The predisposition of the southwest Mt. Peron face to failure is attributable to the structural setting and the regional-scale framework. The entire Belluno Dolomites have experienced a long deformation history since the Miocene (Doglioni1990), related to regional-scale stress connected to the anticlockwise rotation of the Adria plate, indented with the Alpine orogeny (Márton et al.2003; D'Agostino et al.2008). The thrusts and backthrusts (WSW–ENE oriented) that encase Mt. Peron relate to this phase of activity, also creating the two conjugate fracture sets (NW–SE oriented) and inducing the reactivation of the Jurassic faults (N–S oriented) and the overturning of the beds. The area between the Belluno thrust to the south, the Val Carpenada – Val di Vido – Val Madonuta backthrust to the north, the Caorame Valley to the west and the Piave Valley to the east (Fig. 1) is structurally homogeneous and characterised by the same fracture sets identified at Mt. Peron (Bosellini et al.1981; Masetti and Bianchin1987; Bigi et al.1990; Costa et al.1996). In limestones, where these intersect, rock dissolution and caves can form (Filipponi et al.2009; Sauro et al.2013), further weakening the rock (Pánek et al.2009; Gutierrez et al.2014). The Mt. Peron southern wall is known locally as the “weeping rock” due to the numerous caves and karst springs along the steep rock face (Fig. 2b).

Our dating of the Masiere di Vedana landslide to late Roman times casts considerable doubt on the previous late glacial chronological assessment (e.g. Pellegrini et al.2006). Consequently, stress release following downwasting of the Last Glacial Maximum (LGM) Piave glacier, which had been previously considered the main driver of the rock avalanche, actually played no direct role in the process. Climatic and tectonic factors were much more important. In addition, the classification of the deposits as late glacial led to underplaying of the possible hazard at Mt. Peron. The situation at Mt. Peron, with steeply dipping-to-overturned bedding in a limestone massif crisscrossed by numerous faults and riddled with karst fissures, is presently the same that produced the massive failure of the Masiere di Vedana. Several-hundred-metre-high rock prisms along the top of the headscarp are partially detached along the discussed fracture systems and loom perilously over the inhabited valley below (Di Giusto2012). Our results suggest the need for a reconsideration of the hazard related to not only the southern Mt. Peron face, as the rock slopes still present evident structural weakness, but also the whole area lying between the Belluno thrust and its backthrusts, as intense rainfall and earthquakes can occur at any time.

6 Conclusions
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Data acquired in this study provide a new contribution to the knowledge of the timing, failure and propagation of the Masiere di Vedana rock avalanche. The rock avalanche (∼130 Mm3) detached from the southern slope of Mt. Peron. The deposit extends over an area of 9 km2, with a total volume of ∼170 Mm3. A HL ratio ∼0.2 is calculated, marking it as extremely mobile, which is also shown by the maximum runout of 6 km. Geomorphological, stratigraphic and historical evidence when combined with cosmogenic 36Cl exposure ages, mean age 1.90±0.45 ka, point to a single event that occurred in or after late Roman times but before the early Middle Ages.

The steep rock wall on the south face of Mt. Peron shows a pervasive deformation; numerous fractures and faults cross-cut the sub-vertical to slightly overturned carbonate Mesozoic bedrock. The WSW–ENE-directed backthrust planes, which are the most continuous ones, constituted the planes along which the rock mass initially slid, rapidly breaking up and evolving into a rock avalanche.

The stratigraphic sequence is preserved in the rock avalanche deposit. Lithologies that presently constitute the western part of the source area were deposited in the proximal sectors (Vedana, Torbe), while the more easterly outcropping ones reached the distal areas (Masiere, Roe Alte). Landforms of the deposit suggest differential velocities during emplacement. In the NW sector (Torbe) enhanced mobility likely due to interaction with water-saturated path material is evidenced by the numerous ENE–WSW-aligned tomas. In contrast, in the middle sector (Masiere) stacked transverse ridges point to stalling, perhaps related to the gentle uphill gradient and impeded propagation over Pleistocene conglomerates. Post-event evolution comprises formation of backwater alluvial terraces and the wandering of the Cordevole River in the rock avalanche deposits, with incision and aggradation phases.

Identified pivotal drivers are the overall structural setting, exceptional rainfall events and seismic shakings. Their combination produced a pervasive fracturation and weathering of the rock mass, with progressive increase in rock fatigue. No exceptional event may actually be required for such rock avalanches to occur, as accumulation of damage markedly lowers the energy needed to trigger failure.

Considering the new data provided, we highlight that the same driving factors responsible for the Masiere di Vedana rock avalanche are still present today at Mt. Peron. The area between the Belluno thrust and its backthrusts and from the Caorame to the Piave valleys is structurally analogous to Mt. Peron, and therefore re-evaluation of the landslide hazard may be warranted. The possible occurrence of huge rock avalanches and minor rockfalls is a scenario that is necessary to take into consideration in future hazard evaluation and mapping.

Data availability
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Data availability. 

All data are in the paper or in the Supplement.

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The supplement related to this article is available online at:

Author contributions
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Author contributions. 

All authors contributed to the discussion, field survey, data collection and improvement of the text, which has been written mostly by SR, SIO, SM and GM. Each author contributed to different parts, here listed: geomorphology: SR, SIO, GM, MDZ, NS, PM; geological and structural analysis: SM, AV, PC; remote sensing and GIS elaborations: SR; dating: SI, CV, SM; thin-section analysis: MR.

Competing interests
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Competing interests. 

The authors declare that they have no conflict of interest.

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The Ion Beam Physics group at ETH Zurich is thanked for support of fieldwork, laboratory work and AMS measurements. Andrea Cuman and Livio Ronchi are thanked for their support in the early phases of the research.

Financial support
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Financial support. 

This research has been supported by the Università degli Studi di Padova (grant no. Progetto di ricerca di Ateneo 2014, CPDA140511).

Review statement
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Review statement. 

This paper was edited by Paolo Tarolli and reviewed by two anonymous referees.

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Publications Copernicus
Short summary
Rock avalanches are extremely dangerous, causing much damage worldwide. The Masiere di Vedana is a rock avalanche deposit (9 km2, 170 Mm3) in NE Italy. We dated it back to late Roman to early Middle Ages. Identified drivers are the overall structural setting, exceptional rainfall events and seismic shakings. No exceptional event is required as a trigger. When dealing with heavily deformed bedrocks, especially in inhabited areas, the occurrence of a huge event like this must be considered.
Rock avalanches are extremely dangerous, causing much damage worldwide. The Masiere di Vedana is...
Final-revised paper