Literature DB >> 24966447

Early Holocene (8.6 ka) rock avalanche deposits, Obernberg valley (Eastern Alps): Landform interpretation and kinematics of rapid mass movement.

Marc Ostermann1, Diethard Sanders1, Susan Ivy-Ochs2, Vasily Alfimov3, Manfred Rockenschaub4, Alexander Römer4.   

Abstract

In the Obernberg valley, the Eastern Alps, landforms recently interpreted as moraines are re-interpreted as rock avalanche deposits. The catastrophic slope failure involved an initial rock volume of about 45 million m³, with a runout of 7.2 km over a total vertical distance of 1330 m (fahrböschung 10°). 36Cl surface-exposure dating of boulders of the avalanche mass indicates an event age of 8.6 ± 0.6 ka. A 14C age of 7785 ± 190 cal yr BP of a palaeosoil within an alluvial fan downlapping the rock avalanche is consistent with the event age. The distal 2 km of the rock-avalanche deposit is characterized by a highly regular array of transverse ridges that were previously interpreted as terminal moraines of Late-Glacial. 'Jigsaw-puzzle structure' of gravel to boulder-size clasts in the ridges and a matrix of cataclastic gouge indicate a rock avalanche origin. For a wide altitude range the avalanche deposit is preserved, and the event age of mass-wasting precludes both runout over glacial ice and subsequent glacial overprint. The regularly arrayed transverse ridges thus were formed during freezing of the rock avalanche deposits.

Entities:  

Keywords:  Alps; Cosmic ray exposure dating; Electrical tomography; LIDAR interpretation; Rock avalanche; Rock avalanche kinematics

Year:  2012        PMID: 24966447      PMCID: PMC4064935          DOI: 10.1016/j.geomorph.2012.05.006

Source DB:  PubMed          Journal:  Geomorphology (Amst)        ISSN: 0169-555X            Impact factor:   4.139


Introduction

Rockslides and rock avalanches include gravity-driven, rapid slope failures that are larger than about 105 to 106 m3 in volume (Evans et al., 2006). Most rock avalanches post-dating the Last Glacial Maximum (LGM) in the Alps are readily recognized by their shape and size as well as by an extremely poorly sorted composition ranging from cataclastic gouge to megablocks (Pollet and Schneider, 2004; Crosta et al., 2007). At a few locations, however, the interpretation of landforms composed of very poorly sorted deposits remains controversial. For instance, transverse and lateral ridges of rock avalanches may appear similar to terminal and lateral moraines of glaciers. Diamicts of fine-grained matrix hosting polished and striated rock fragments may, either, represent basal till, or may form in rock avalanches. In addition, rock avalanches can flow out over long distances, which may promote confusion with glacial sediments (cf. Hewitt, 1999). In the Obernberg valley, Austria, the character of a rock avalanche deposit led to diverse interpretations for more than a hundred years. In its distal part, which is about 2 km in length, the avalanche mass shows a regular arrangement of ridges and hillocks that are roughly transversal to valley axis. Frech (1903), who first investigated these deposits, interpreted their entirety as a rock avalanche. Paschinger (1953) agreed, but interpreted the ridges as a result of decay of underlying glacial ice. Later, based solely on the morphology of ridges and hillocks, the landforms were thought to be terminal moraines and kames (Magiera, 2000; Ebner et al., 2003; Wastl, 2007). Herein, we present a survey based on field investigations, volume estimation using airborne laser scanning image, a digital elevation model and electrical tomography, and proxy event ages produced by radiocarbon and cosmic ray-exposure dating. Our results indicate that the purported glacial landforms accumulated from a rock avalanche 8.6 ± 0.6 ka ago. We discuss: (a) a potential relation of rock avalanching with the 8.2-ka climatic phase in the Alps, and (b) the significance of transversal ridges with respect to rock avalanche kinematics.

The study area

The SW–NE trending Obernberg valley is a 9-km-long tributary of the Wipp valley, about 25 km south of Innsbruck (Fig. 1). Over most of its extent, the Wipp valley follows the Brenner extensional fault. The hangingwall of the Brenner fault consists of the Oetztal–Stubai basement complex with an overlying, parautochthonous Mesozoic succession and two superposed thrust nappes (Blaser and Steinach nappes); the footwall is comprised of variegated metamorphic successions of a different tectonostratigraphic unit (Fig. 1) (Fügenschuh et al., 1997). Neogene fission-track cooling ages in the footwall adjacent to the Brenner fault, and fault plane solutions of historical earthquakes suggest that the Brenner fault may still be active at a low rate (cf. Fügenschuh et al., 1997, 2000; Fügenschuh and Mancktelow, 2003; Reiter et al., 2003). The Obernberg rock avalanche detached from an isoclinally folded, Mesozoic series of calcitic to dolomitic marbles, calcitic phyllites and, subordinately, phyllites and quartzites (Fig. 2) (Rockenschaub et al., 2003). The dip/dip azimuth of schistosity in the isoclinally-folded series ranges from horizontal to 270–320°/10–20° (Reiser et al., 2010). The detachment scarp of the rock avalanche is located about 500 m west, and in the footwall of, an N–S striking normal fault (Portjoch fault) with a vertical throw of at least a few hundred meters. East of the Portjoch fault, the right flank of the See valley and that of the upper Obernberg valley consist mainly of quartz phyllite and mica schist of the Steinach nappe (Figs. 2 and 3). Whereas the mentioned Mesozoic series is deeply incised by many gullies, and the toes of slopes are covered with talus aprons, there is nearly no fluvial incision and talus formation within the Steinach nappe. The quartz phyllites there tend to form numerous slow moving, shallow to deep, mass movements (Fig. 3).
Fig. 1

The Obernberg rock avalanche and rockslides/rock avalanches (red areas) nearby, displayed on the tectonic map of Schmid et al. (2004), with a digital elevation model in the background. Earthquakes in this region according to the NEIC dataset (http://earthquake.usgs.gov/earthquakes) are indicated with multicolored and multi-sized dots. Dot size corresponds to earthquake magnitude, and dot color corresponds to the depth of the epicenters. GS: Gschnitz Stadial locus typicus.

Fig. 2

Geological map of the Obernberg region (modified after Rockenschaub et al., 2003). The area is subdivided into two tectonic and lithological units by the Portjoch normal fault (PJ). Yellow circles: sampling sites for surface exposure dating. Green circle: sampling site for radiocarbon dating. Orange bars: geoelectric profiles P1 to P6 (see also Fig. 4).

Fig. 3

Overview map of the Obernberg rock avalanche displayed on LIDAR-data (provided by TIRIS — Tyrolean spatial planning information system). The accumulation area has a color gradient displaying the estimated debris thickness distribution (light pink: 0–10 m; purple: 30–40 m). Lake Obernberg bathymetry is indicated in 5 m steps from pale blue to dark blue. Labeled white circles A to D denote areas motioned in the text. Green line from A (scarp area) to D (most distal part of the accumulation area): Cross-section shown in lower part of the figure.

During the Last Glacial Maximum in the Eastern Alps (LGM, ca. 24–19 ka), the upper margin of glacial ice sloped from about 2700 m a.s.l. in the heads of tributary valleys (Hinterenns and See valleys) to 2400 m a.s.l. in the central Obernberg valley; the summital Tribulaun range was a nunatak (Fig. 3) (Van Husen, 1987). In the Obernberg valley and its tributaries, the most widespread glacigenic sediment includes basal till and reworked basal till of the LGM. Subsequent to the LGM, after an early deglacial phase of rapid ice decay (Van Husen, 2004; Reitner, 2007), climatic amelioration and glacier shrinking were punctuated by stadials, that is, intermittent re-advances of valley glaciers (e.g. Kerschner, 1978; Van Husen, 1997; Ivy-Ochs et al., 2006). Along the northern (left) flank of the Obernberg valley, late-glacial ice-marginal deposits are preserved above the present valley floor, in an altitude range of 1820–1500 m a.s.l. These deposits may have accumulated during the Steinach Stadial, a phase of glacial re-advance older than 15,400 ± 470 14C yr BP (Magiera, 2000; Ivy-Ochs et al., 2006). In the neighboring Gschnitz valley, the type location of the Gschnitz Stadial, the terminal moraine complex is situated at the village Trins, at an elevation of 1410–1200 m a.s.l. (Fig. 1). The stabilization of the moraine complex has been attributed to no later than 15,400 ± 1400 years ago (Ivy-Ochs et al., 2006). In the Obernberg valley, probably as a result of a significantly smaller glacial catchment, no terminal moraine corresponding to the Gschnitz Stadial is present. Lake Obernberg is situated on rock avalanche deposits (Fig. 3). The lake shows substantial seasonal and inter-annual variations in level, as a result of poor sealing of the lake basin combined with a high permeability of the underlying rock avalanche deposits. During low stage, the lake is separated into two parts (Reiser et al., 2010). The lake basin probably became deeper with time due to subsurface entrainment of fine-grained matrix in groundwater flow.

Methods

Field mapping was conducted on a scale of 1:5000 using topographic maps and laserscan images. High resolution airborne laserscan-data and a digital elevation model (DEM) with a 1-m resolution were provided by TIRIS (www.tirol.gv.at/). These data have been implemented into a GIS-system and combined with orthophotos (TIRIS, BEV), topographic maps (Österreichische Karte 1:50.000, BEV, Blatt 148 Brenner), and geological maps (Geological map of Austria, 1:50,000, Blatt 175 Sterzing; Geologisch-tektonische Karte der östlichen Stubaier Alpen, 1:25.000). The coordinate system and projection used are WGS1984 and UTM Zone 32N. Volume calculations and cross-sections were made with AutoCAD 2010. For exposure dating with 36Cl, near Lake Obernberg in the proximal sector of the rock avalanche, the surfaces of four boulders were sampled (locations shown in Fig. 2). Unfortunately, the distal sector of the avalanche deposit with transversal ridges (C–D in Fig. 3) is devoid of suitable boulders (those lying well above the enclosing sediment). Sample preparation is described in Ivy-Ochs et al. (2009). Approximately 60 g of rock was dissolved, after addition of 2.4 mg of 35Cl carrier, with concentrated HNO3. Cl was isolated and freed of S with several pH change steps and addition of Ba(NO3)2, respectively. 36Cl and natural Cl (isotope dilution; Ivy-Ochs et al., 2004) were determined with accelerator mass spectrometry (Synal et al., 1997). Measured sample 36Cl/Cl ratios were normalized to the ETH internal standard K382/4N with a value of 36Cl/Cl = 1.736 × 10− 11 (normalized to the Nishiizumi standards in 2009) while the stable 37Cl/35Cl ratio was normalized to the natural 37Cl/35Cl ratio = 31.98% of the K382/4N standard and the machine blank. Measured sample ratios were also corrected for a procedural blank of 3 × 10− 15, which amounted to a correction of less than 2% for all samples. Major and trace element concentrations are given in Table 1. Concentrations of B and Gd were below the detection limit. Exposure ages (Table 2) were calculated based on a sea level/high latitude production rate of 48.8 ± 1.7 atoms 36Cl g(Ca)− 1 a− 1 for production from spallation of Ca, and 5.3 ± 0.5 36Cl g(Ca)− 1 a− 1 production due to muon capture on Ca (Stone et al., 1996, 1998) scaled after Stone (2000). Production of 36Cl through low energy capture of thermal and epithermal neutrons is calculated following Liu et al. (1994) and Phillips et al. (2001) using a production constant of 760 ± 120 neutrons (g air)− 1 a− 1 (Alfimov and Ivy-Ochs, 2009). Major element and samarium concentrations as well as major element concentrations (Table 1) were used to determine the fraction of low-energy neutrons available for capture by 35Cl to form 36Cl (Alfimov and Ivy-Ochs, 2009 and references therein). The contribution due to non-cosmogenic subsurface 36Cl production calculated after Fabryka-Martin (1988) was negligible. Shielding corrections were done following Dunne et al. (1999). We used a rock density of 2.4 g cm− 3.
Table 1

Major element data for the analyzed samples (determined by XRF at XRAL, Ontario, Canada).

Boulder no.Al2O3wt. %CaOwt. %Cr2O3wt. %Fe2O3wt. %K2Owt. %MgOwt. %MnOwt. %Na2Owt. %P2O5wt. %SiO2wt. %TiO2wt. %SumLOISmppmThppmUppm
OB10.153.30.010.010.020.590.010.010.010.210.0197.843.50.20.50.32
OB25.039.00.021.821.081.280.050.500.0519.600.230100.331.72.43.01.46
OB30.233.10.020.150.0319.20.010.010.010.410.0199.145.90.40.10.50
OB40.446.80.010.240.128.040.030.010.011.120.020100.543.70.40.10.50
Table 2

Results of 36Cl surface exposure dating.

Boulder no.Alt.[m]Easting
Northing
Thickness[cm]Shielding36Cl[105 atoms 36Cl/g rock]Cl[ppm]Exposure age[kyr]
[UTM WGS84 Z 32N]
OB11651682,9235,206,4602.50.957.27 ± 0.2031.3 ± 0.19.16 ± 0.40
OB21606682,7815,206,75210.977.06 ± 0.222.3 ± 0.112.09 ± 0.55
OB31616682,7025,207,17820.965.57 ± 0.2495.0 ± 1.58.24 ± 0.60
OB41610682,7995,207,3291.50.975.66 ± 0.2024.2 ± 0.78.32 ± 0.40
On the southern bank of Lake Obernberg, a paleosoil 1.2 m below the surface of a small alluvial fan was sampled for radiocarbon dating (Fig. 2). Radiocarbon ages (Table 3) were calibrated with OXCAL 4.0.1 (Bronk Ramsey, 2009) using the Int Cal 09 data set (Reimer et al., 2009).
Table 3

Results of radiocarbon dating.

SampleAlt. [m]EastingNorthingMaterial14C-age [kyr]cal-Age [kyr]
Vera — 4980 OB_14C_21608686,1915,206,273Paleosoil6.98 ± 45 [BP]7.79 ± 0.19
Vera — 4979 OB_14C_11608686,1915,206,273Wood0.12 ± 45 [BP]Modern
In the proximal part of the rock avalanche deposit, six electrical tomographic profiles were made with a GEOMON4D resistivity meter, an in-house development of the Geological Survey of Austria, with a gradient electrode array configuration (Fig. 2; see Table 4 for key parameters of profiles). Data inversions were performed with the AGI EarthImager 2D software according to a robust inversion method based on an L2-norm criterion. The results of the inverted profiles are shown in Fig. 4 after suppressing aberrant resistivity values obtained due to bad coupling between electrodes and the sometimes rocky material.
Table 4

Key parameters of the electrical tomography.

Electrical tomography profileLength [m]Orientation (first to last electrode)Elevation [m a.s.l.] (min. elv.–max. elv.)Unit electrode spacing [m]Horizontal scale pixels per unit spacing
P1736NNE–SSW1612–16728.009.97
P2690NE–SW1728–17507.5019.99
P3570NE–SW1751–17897.5012.08
P4532WNW–ESE1607–16257.0012.03
P5552W–E1581–16186.009.92
P6460NNW–SSE1591–16505.009.85
Fig. 4

Resistivity cross-sections (P1–P6) obtained by electrical tomography profiles (see Fig. 2). Values represented along the X-axis correspond to distance in meters form the starting point of the tomography profile. The Y-axis represents the elevation above sea level in meters. Parameters of each profile are given in Table 2.

Rock avalanche deposits

In the most proximal sector of the rock avalanche mass, a ridge up to 80 m in relief comprised of very poorly sorted bouldery sediment is present. Clasts of cobble to boulder size show in-situ fragmentation. Farther down, rock-avalanche deposits build lateral ridges along the Obernberg lakes. In addition, a continuous layer of bouldery deposit can be mapped for approximately 200 m in altitude onto the opposite, right-hand flank of the See valley (Fig. 3); the distribution of this deposit may suggest that it originated from a different mass-wasting event descended from the west-facing slope. The composition of clasts of folded marbles, however, indicates that it more likely derives from the detachment area of the Obernberg rock avalanche, i.e. from the eastern cliffs of the Tribulaun range. The medial part of the rock avalanche consists of a steeply sloping tongue of extremely-poorly sorted debris ranging up to boulders a few tens of meters in size (Figs. 3 and 5C). Finally, the distal part of the rock avalanche consists of a conspicuous array of hillocks and ridges that are described in more detail below (Figs. 3, 4 and 5). Rock avalanche deposits exposed at the surface cover an area of ~ 1.9 km2. Taking into account those parts of the avalanche that are buried by alluvial fans, talus slopes and colluvium, an area of ~ 3 km2 was calculated (Abele, 1974: 2.7 km2). The distance from the upper brink of the detachment scarp (2700 m a.s.l.) to the distal most toma hill (1370 m a.s.l.) is 7.2 km, yielding a fahrböschung angle of 10°. According to our calculation based on a digital elevation model, the total volume of rock avalanche deposits is 5.3 × 107 m³ (Paschinger, 1953: 5.7 × 107 m³). To reconstruct the rock volume detached from the scarp area (Fig. 3), we used a digital elevation model integrated with LIDAR data, aerial photos and topographic maps. The results give a maximum of close to 5.0 × 107 m3 of rock before detachment (Paschinger, 1953: 5.6 × 107 m3). This indicates a volume increase of 5.6% from rock to rock avalanche deposit, being higher than 1.2% of Paschinger (1953), but anomalously low relative to a volume increase of up to 25–30% reported for mass-wastings of carbonate rocks (Abele, 1974; Hungr and Evans, 2004). This may suggest that the initial volume was overestimated by isohypse fitting; a volume of ~ 4.0–4.5 × 107 m3 seems more realistic. With this deduced volume and a reconstructed area of 3 km2, the Obernberg rockslide lies within the range of volume/area ratio of other rockslides and rock avalanches; the same holds for the ratio of runout length to vertical drop versus volume (cf. Abele, 1974; Dade and Huppert, 1998). A minimum-age constraint of the mass-wasting event was obtained by radiocarbon dating of organic remnants found in alluvial fan deposits on the top of the rock avalanche deposits (Fig. 2). Two samples were taken: (a) Vera — 4980 (OB-14C_2) represents a paleosoil 120 cm below the surface of the alluvial fan, and (b) Vera — 4979 (OB-14C_1) is a piece of wood from about 20 cm below the recent fan surface (Table 3). From 36Cl surface exposure dating of four boulder surfaces, we obtained the following exposure ages: 9.16 ± 0.40 ka (OB1), 12.09 ± 0.55 ka (OB2), 8.24 ± 0.60 ka (OB3), and 8.32 ± 0.40 ka (OB4). The average age of 8.6 ± 0.6 ka indicates an early Holocene age for the rock avalanche event (Table 2). We attribute the outlier-age 12.09 ± 0.55 ka to inheritance which is often observed in rock avalanche boulders (Ivy-Ochs et al., 2009).

Transversal ridges and hillocks

The distal part of the rock avalanche between Untereinsalm (1540 m a.s.l.) and Obernberg Village (~ 1370 m a.s.l.) is characterized by an array of 40 hillocks and transversal ridges with up to 17 m in vertical relief (Figs. 3, 4 and 5). Because of the lack of both natural outcrops and drill logs, we could not establish whether the hillocks and ridges are contiguous with each other or rather represent isolated forms. For reasons discussed below, however, we assume that they are connected with each other in the subsurface. These ridges and hillocks were interpreted as terminal moraines and kames because of their morphology (Magiera, 2000; Ebner et al., 2003; Wastl, 2007). Cross-sections based on a digital elevation model with 1-m resolution show that the transversal ridges are arranged into two ‘domains’ each about 750 m in length (Fig. 5). Each domain consists of nine ridges, with the highest in the central part and progressively lower and elongated ones towards the distal and proximal margins. Two artificial outcrops (Fig. 7), each a few meters in height and about 10 m in length, provide insight into the internal fabric of ridges. Both outcrops show that the ridges consist of angular fragments of sand- to boulder-size clasts in disordered fabric; no systematic vertical/lateral sorting, stratification, and preferred orientation of clasts were observed. The fabric ranges, in a patchy pattern, from clast-supported with sparse interstitial matrix of structureless carbonate gouge to matrix-supported. Many clasts of coarse gravel- to boulder-size are fragmented in situ, with opposite fracture walls still fitting. Both the orientation and density of fractures are highly variable among and within individual clasts.
Fig. 5

Transversal ridges at Obernberg. A) Airborne laser scan image (by TIRIS) of the landscape at Obernberg. Red lines: 1-m contours for transversal ridges. Green lines: 10-m contours. B) Inset figure shows superposition of 14 cross-sections of transversal ridges. C) Cross-section from I to II (see A) through the transversal ridges, which show a very regular arrangement.

Fig. 7

Field photographs showing features related to the Obernberg rock avalanche. A) Overview of the scarp area of the Obernberg rock avalanche view towards W. The orange line represents the outline of the scarp. CM = calcareous marls, HD = Hauptdolomit. In the lower right corner rock avalanche debris is indicated in yellow. Notice the dissection of the upper part of the rock slope through faults and joints. B) Overview photo of Lake Obernberg with the northern lake basin in the foreground, view toward SW. The scarp area (red line) and the upper travel path (red arrow) in the background. Notice the big blocks in and around the lakes. Lake level is about 1.5 m below maximum. C) Chaotic fabric of angular clasts of calcareous marls and Hauptdolomit and fine grained matrix below a big block nearby the Lake Obernberg. Field book for scale. D) Hilly landscape at Obernberg view towards W. KT = Kleiner Tribulaun (2492 m a.s.l.). CS = church spire of the church of Obernberg situated on top of one of the transversal ridges. E) Artificial outcrop at one of the most distal transversal ridges. Angular clasts swimming in a fine grained matrix without any sorting. Stick = 1 m. F) Enlarged detail of E) showing a fractured clast of Hauptdolomit (jigsaw type). Visible stick = 44 cm.

Interpretation of the ground electrical tomography

Six multielectrode profiles were measured to get more detailed information on the depth and internal structure of the rock avalanche deposits. The locations of the profiles (P1–P6) are indicated in Fig. 2. The results of the geoelectric inversion of multi-electrode data on the profiles are shown in Fig. 4. To make comparison and interpretation easier, all profiles are depicted with the same color bar. P1 shows a relatively homogenous cover of rock avalanche debris, represented by high resistivity (> 3000 Ω m, red color in Fig. 4), reaching a maximum thickness of about 60 m, with an average thickness of about 50 m. The high resistivity can be explained by its high porosity, which is implied by the accumulation of large blocks (typical size of a few m3 scale). Below this surficial layer, resistivity decreases with depth, indicating finer and wetter material that could be the expression of increased matrix content and/or fluvio-glacial deposits (orange and yellow colors in Fig. 4). The bedrock is built up by quartz phyllite with an electr. resistivity around 500 Ω m (green color). In the NNE part of this profile, low electr. resistivities (< 50 Ω m, blue color) can be explained by the occurrence of a fault-zone. The rock debris cover at P2 reaches from about 20 m in the NE to a maximum extent of 45 m in the middle part of the profile. In the SW of the profile near Steineralm (1737 m a.s.l., Fig. 2) the bedrock (quartz phyllite) is at surface or below a very thin talus cover. Here a low resistivity zone can also be observed. This anomaly may be attributed to a technical reason: drainage pipe and power supply in the vicinity of Steineralm. P3 is characterized by up to 40 m thick rock avalanche debris in the NE. In the SW, in contrast, it consists of near-surface bedrock as well as water-saturated fluvial deposits and peaty material. P4 is situated along the “Maria am See” peninsula that divides the lake basin of Lake Obernberg into two parts. The situation here is more complex. The evaluation of the profile leads to the interpretation of a dry part and a water saturated part of the rock avalanche debris. The ridge consists of about 10–20 m unsaturated on top, and up to 20 m thick water saturated rock avalanche debris below. The bedrock is almost built up by quartz phyllite. Towards the NW, electric resistivity in the substratum increases (~ 1000 Ω m), indicating the transition to the carbonatic units in the W. P5 is situated on top of the steep valley step, where the northern most lake basin is dammed by rock debris. In the East, rock avalanche material is covered by a small alluvial cone (up to ~ 6 m in thickness) fed from a gully. The rock avalanche debris here reaches a thickness of ~ 25 m. In the central part of the profile, the prominent low resistivity anomaly can be interpreted as a fault-zone. This zone indicates the boundary of the carbonate bedrock (yellow and orange colors in Fig. 4) in the W and the quartz phyllite (green color) in the E. The high resistivity in the NW could also indicate a glacial or fluvial channel filled with rock avalanche debris. P6 crosses the up to 80 m high ridge developed along the SW bank of Lake Obernberg. The geoelectric survey clearly shows that the whole ridge is composed of rock avalanche debris. Toward the S of the profile one can see the water saturated part of the rock avalanche debris with aggradation deposits on the top, coming in from the S into the lake basin. The bedrock here has carbonatic lithologies.

Discussion

The kinematics of the Obernberg rock avalanche is described in chronological order from A to D (Figs. 2 and 6). (A) After detachment of the main volume of rock, the rock mass ran down a rectilinear slope ~ 30° in gradinet and 1200 m in length (Fig. 6A). Immediately after the detachment, the rock mass perhaps was still more-or-less intact and moved as a rockslide. We assume, however, that during run-down on the slope, the rock mass disintegrated by dynamic fragmentation and progressively turned into a rock avalanche (Davies and McSaveney, 1999; Davies et al., 1999).
Fig. 6

Sketch maps of the propagation of the Obernberg rock avalanche (A to D). The closer hatch in A indicates the assumed former outline of the intact rock slope. Explanations are given in the text.

(B) The rock avalanche ran across the valley floor and up onto the opposite slope ~ 12° in gradinet (Fig. 6B). Near Steineralm (1767 m a.s.l.), the rock-avalanche deposit consists of: (a) a surficial veneer of boulders of Hauptdolomit, resting on (b) calcareous marbles; this reflects the vertical distribution of these two lithologies in the scarp area (see Fig. 3). Transition from (B) to (C). After run-up of the frontal part of the rock avalanche onto the opposite slope, some of the swashed material may have flowed back (Fig. 6B); the following part of the moving rock avalanche bulged up, and was forced to swerve towards the N. As a result, longitudinal ridges and grooves formed in the marginal part of the avalanche. In addition, in flowing down the very steep upper part of the See valley, the rock avalanche probably gained kinetic energy again. (C) When the rock avalanche ran up the northern slope of the Obernberg valley, a part of it branched off and ran up, for a limited distance, into the Hinterenns valley (Fig. 6C; see also Fig. 3, point C). (D) The main body of the rock avalanche, however, continued to run down the Obernberg valley (Fig. 6D). There, kinetic energy dropped below the threshold for rock-avalanche movement, and the described arrays of transverse ridges formed. Taking into account the velocities for rock avalanches from Zambrano (2008) and a runout distance of 7.2 km, we infer that the event happened within a time span of 0.8 to 2 min. In the Alps, only a few mass-wasting events are dated into the range from ~ 9 to 7.5 ka. The age of 8.6 ± 0.6 ka of the Obernberg event may suggest a relation with the “8.2 ka cooling event” (cf. Rohling and Pälike, 2005). In the eastern part of the Eastern Alps, a cooling of ~ 3 °C into the 8.2 ka event needed 10–20 years, and cooler conditions then persisted from ~ 8.2 to 8.1 ka (Boch et al., 2009). The resolution of the numerical age of 8.6 ± 0.6 ka of the Obernberg rock avalanche event hence does not allow for an unequivocal correlation with the 8.2 ka cooling. In the eastern part of the Eastern Alps, there is no evidence for marked changes in seasonality or mean annual precipitation (Boch et al., 2009). Conversely, in the northern and western Alpine foreland, lake levels rose at about 8.2 kyr, probably due to increased precipitation and decreased summer temperatures (Magny et al., 2003). In NW-Germany, the onset of 8.2 ka event was characterized by a rapid switch to a phase of approximately 190 years of cooler and drier summers; similarly, winters were drier and cooler (Klitgaard-Kristensen et al., 1998; Prasad et al., 2009). If understood as a phase of cooler summers, the NW-Germany 8.2 ka event started between ~ 8.12 and 8.09 ka and ended at 7.93 ka (Prasad et al., 2009), i.e. nearly twice as long as in the eastern part of the Eastern Alps. This suggests that the response to the 8.2 ka event had a strong geographical component, provided that age assignments are sufficiently precise. Difficulties to capture the 8.2 ka event may also arise from the different methods of dating and the variegated records used (e.g., Alley and Ágústsdóttir, 2005; Kerschner et al., 2006; Prasad et al., 2009, and references therein). Because the climatic response of the central part of the western Eastern Alps to the 8.2 ka event is not documented to date, we thus refrain from suggesting a potential correlation of rock-avalanching with particular climatic conditions. In addition, only a minority of rockslides and rock avalanches of the Alps have been dated so far. This further impedes us to assess a potential correlation of palaeoclimate with catastrophic mass-wasting. In the Silvretta massif of the Central Alps, glaciers of N-facing cirques of the Kromer stadial (perhaps equivalent with the 8.2 ka phase) terminated at 2100 m a.s.l. or higher (Kerschner et al., 2006), i.e., in an altitude above the Obernberg rock-avalanche deposit. This further suggests that the rock avalanche did not run out over a glacier. We also found no evidence that the avalanche deposit was overridden by a glacier. Except for the present course of the Seebach stream (Fig. 3), the transverse ridges in the distal sector of the avalanche deposit were not dissected by fluvial activity. There is also no evidence for disintegration of the distal part of the avalanche mass by slow downslope movement after the event. Thus, at least the larger transverse ridges, as seen in Fig. 3, are well-preserved and in similar arrangement as they were immediately after the rock avalanching. However, smaller surface features such as scattered boulders or low ridges may have been removed upon agricultural amelioration for pasture. Compared with most other rock-avalanche masses in the Alps, the abundance and high regularity of the transversal ridges of the distal part of the Obernberg avalanche deposit are exceptional. The regularity may provide a record of the style of material movement (Fig. 6). The apparent excessive mobility of rock avalanches has been explained by sliding on, and/or lubrication of fine-grained deposits with incorporated snow, ice, and water (e.g., Abele, 1974; Goguel, 1978; Sartori et al., 2003; Hungr and Evans, 2004; De Blasio, 2009; Dufresne et al., 2010; Shugar and Clague, 2011). Another explanation for the high rock-avalanche mobility is based on the mechanics of the moving mass itself (e.g. Davies and McSaveney, 1999; Dufresne et al., 2010). Because a universal feature of large-volume catastrophic rock-slope failures is fragmentation (cf. Crosta et al., 2007), one key to the mobility of rock avalanches is comminution during downslope movement (Davies et al., 1999). Letting aside potential effects of snow or ice, or ‘lubrication’ by foreign materials, a rock mass probably moves as long as kinetic energy suffices to sustain dynamic fragmentation and resulting dilatancy by mutual particle impact (Imre et al., 2010). Propagation of kinetic energy may occur in acoustic waves that act to fluidize the moving particulate mass (Melosh, 1986; Collins and Melosh, 2003). We infer that the distal-most transverse ridge of the Obernberg rock-avalanche mass was the first to freeze, and the more proximal ridges formed subsequently by successive upslope propagation of freezing. Each transverse ridge thus may represent the terminal record of some kind of wave or surge that traveled downslope. Surging, i.e., fluctuations of both velocity and thickness of a flow associated with downflow propagation of roll waves, is observed in fluid flows, density flows, and debris flows of diverse compositions (e.g., Coussot and Meunier, 1996; Major, 1997; Balmforth and Mandre, 2004, and references therein). Roll waves do not require turbulence to develop, and can emerge also in granular flows (e.g., Daerr, 2001; Louge and Keast, 2001). Roll waves may overtake each other by run-up of faster surges into slower forerunners; overall, however, they strive towards quasi-periodic wave trains (all other conditions equal) (Forterre and Pouliquen, 2003). At least under certain experimental conditions, granular flows can evolve into a series of downslope-propagating roll waves pushing forward unmoved material resting in between the surges (Forterre and Pouliquen, 2003). No model of a granular flow undergoing dynamic disintegration, and explicitly treating the physical effects of disintegration from local scale up to the entire avalanche, exists as yet. Dynamic disintegration, perhaps the single most distinctive process in the movement of rock avalanches and rockslides, was analog modeled for a small volume of rock-like material in a centrifuge (Imre et al., 2010); however, this cannot reflect the potential behavior of a rock avalanche when in action as a whole over some period of time. Acoustic waves within rock fractures dissipate in areas close to the source (Melosh, 1996). In the distal part of a rock avalanche, acoustic waves from dynamic disintegration may become organized into downslope-propagating pulses, resulting in surging-style movement (cf. Collins and Melosh, 2003). The described transverse ridges thus may hint on the existence of surge-like flow behavior in the distal part of some rock avalanches.

Conclusions

Surface exposure dating of boulders indicates that the Obernberg rock avalanche occurred 8570 ± 630 years ago; this age is supported by a 14C age of 7785 ± 190 a cal BP of a palaeosol in alluvial fan deposits on the rock-avalanche deposits. The Obernberg rock avalanche is the first dated mass-wasting event in the Alps that potentially was associated with the 8.2 ka climatic cooling. The precise nature of the 8.2 ka event in the central part of the Eastern Alps, however, is insufficiently documented to sustain speculations on a triggering of the rock avalanche under a particular climatic condition. The distal 2 km of rock-avalanche deposits show an array of transverse ridges. These were previously interpreted as terminal moraines and kames. The internal fabric and nature of the sediment of the ridges are, however, incompatible with glacial moraines, but consistent with an origin from a rock avalanche. The transversal ridges are arranged into two highly regular higher-order waves, each of which consists of waxing and shrinking ridges. We suggest that the arrayed ridges reflect a mechanical aspect of the movement, perhaps propagation of waves towards the snout of the avalanche deposit.
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1.  Centennial-scale climate cooling with a sudden cold event around 8,200 years ago.

Authors:  Eelco J Rohling; Heiko Pälike
Journal:  Nature       Date:  2005-04-21       Impact factor: 49.962

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