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Acta Geologica Polonica, Vo l. 57 (2007), No. 2, pp. 305-323
Cavitation erosion – a possible cause of the mass
loss within thrust zones in the Tatra Mts., Poland
EDYTA JUREWICZ 1 , BOLES¸AW GIRE¡ 2 & JANUSZ STELLER 2
1 Faculty of Geology, University of Warsaw, Al. ˚wirki i Wigury 93, PL-02-089 Warsaw, Poland.
E-mail: edyta.jurewicz@uw.edu.pl
2 The Szewalski Institute of Fluid Flow Machinery , Polish Academy of Sciences , ul. Fiszera 14 ,
PL - 80-952 Gdaƒsk, Poland. E-mails : giren@imp.gda.pl , steller@imp.gda.pl
ABSTRACT:
J UREWICZ , E., G IRE¡ , B. & S TELLER , J. 2007. Cavitation erosion – a possible cause of the mass loss within
thrust zones in the Tatra Mts., Poland. Acta Geologica Polonica , 57 (3), 305-323. Warszawa.
In the Tatra Mts., thrust-napping and shearing were multi-stage re-activated processes. Their cyclic char-
acter was determined by increases and decreases in pore fluid pressure. During each cycle, new parts of
the rheologically heterogeneous wall-rock were selectively destroyed due to hydraulic fracturing, brec-
ciation and mylonitization, and moved out as a solution and/or suspension. As a result of these process-
es, including pressure solution, considerable mass loss could have taken place. All these processes took
place under the considerable influence of fluids. In this paper we consider the possible contribution of
cavitation erosion to mass loss processes. Displacement along an uneven thrust surface could create
chambers filled with fluid and sudden falls in local pressure promoting the inception of cavitation.
Cavitation damage, mainly mechanical in nature, could act synergistically with slurry abrasion and pres-
sure solution processes.
Our work is of a hypothetical character. To prove the possibility of cavitation erosion within shear
zones in the Tatra Mts. we conducted an experiment to show the low resistance of rock samples to cavi-
tation erosion. We also discuss and characterize the conditions essential to induce cavitation within thrust
zones at the base of nappes.
Key words: Cavitation erosion, Hydrotectonic pump, Fault slurry, Shear zone,
Tatra Mts.
INTRODUCTION
(S IBSON 1996). Fluids could be released to the shear
zone due to fracturing of country rocks. Other
processes, such as the dehydration of gypsum, could
also be a source of water. Fluidised rocks at the
base of nappes act as a low-viscosity tectonic lubri-
cant consisting of a suspension comprising salt solu-
The presence of fluids plays a key role during
shearing processes. A shear zone could be a path-
way of fluid migration, with the direction of fluid
flow governed by the maximum hydraulic gradient
306
EDYTA JUREWICZ & al .
tions, dissolved gases, rock fragments and matrix.
Fluids may cause a change in the predominant
mechanism of deformation due to hydrolytic weak-
ening or crack-seal-slip (P ETIT & al. 1999). Gases
can be released from solution as a result of a tem-
porary decrease in pressure or an increase in tem-
perature.
In the upper crust, fluid pressure is typically
normal and equal to hydrostatic pressure. H UBBERT
& R UBEY (1959) and S ECOR (1965) indicated the
importance of pore-fluid pressure in the mechanics
of sliding of large rock masses, especially in the case
of low-angle overthrusts. According to S IBSON
(2004), high fluid overpressures are easier to sus-
tain in compressional regimes that also allow the
highest amplitude fluid-pressure cycling.
In the Tatra Mts., nappe structures and nappe-
thrust surfaces are unique because of their geomet-
ric irregularity. Many investigations questioned the
cause of these geometric peculiarities. Earlier
works indicated that the morphology of the shear
zone was conditioned by anisotropy of the sedi-
mentary rocks and that the geometry of nappe
structures was connected with large-scale mass-loss
processes (J UREWICZ 2003, 2006; J UREWICZ &
S ¸ ABY 2004).
Shear zones in the Tatra Mts. connected with
Alpine nappe-thrusting processes cut layers of
sedimentary rocks as well as the crystalline core.
Only within shear zones originating in the sedi-
mentary cover of the Tatra Mts. could processes
of intense brecciation, mylonitization and pres-
Fig. 1. A – Main tectonic units of the Tatra Mts. and sampling points (after B AC -M OSZASZWILI & al. 1979). B – Tectonic contact of two
units (Giewont and Czerwone Wierchy) of the Tatric Nappe with clearly visible geometrical irregularity of the thrust surface; SW slope
of Giewont Mt. (geological interpretation after G ÑSIENICA -S ZOSTAK 1973)
391300274.002.png
CAVITATION EROSION
307
sure solution leading to mass-loss be observed
(J UREWICZ 2006). The surfaces of thrusts are usu-
ally corrugated and rough. From tectonically
deformed rocks uniquely preserved in dilation fis-
sures, we were able to reconstruct the shearing
processes resulting from repeated fault nucle-
ation by reactivation of pre-existing mechanical
discontinuities due to cyclic changes in pore-fluid
pressure (J UREWICZ 2003). The petrophysical
properties of the rocks and associated liquid spots
play an important role in the shearing processes.
In comparison with the sedimentary cover, the
main component of the crystalline core, a grani-
toid, shows low porosity and low solubility; the
shear surfaces dip typically at a low-angle and are
smooth and planar. This difference in petrophys-
ical properties results in the lack of comparable
processes within the granitoid core and in the sed-
imentary cover (J UREWICZ 2006).
The significant extent of mass loss associated
with thrust-napping surfaces within the Tatra Mts.
is difficult to explain by damage resulting from
fracturing and pressure solution processes alone.
We try to show below that cavitation erosion
could have been equally responsible for the wall
rock mass loss along the thrusts in the Tatra Mts.
as the above processes. Cavitation is a phenome-
non commonly associated with hydraulic equip-
ment; it is well known to mechanical and civil
engineers as a powerful erosive mechanism lead-
ing to severe damage to hydraulic equipment and
civil engineering structures (K NAPP & al. 1970,
G ALPERIN & al. 1977, K ENN 1983). Practical
implementations of cavitation include drilling
rocks in boreholes and cutting rocks in quarries.
Even if most geologists know cavitation, this
knowledge is of little use in explaining tectonic
processes. The difficulty is that we are looking for
something that does not exist now: the mass lost
and the inferred process or mechanism resulting
in the mass loss, i.e. cavitation erosion. Within the
shear zones there is no preserved record of cavi-
tation bubbles, but we can indicate the possibility
of the occurrence of cavitation during thrusting in
the Tatra Mts. and we are able to prove the low
resistance to cavitation of rocks from shear zones
and their vicinity. The authors are aware that, at
this stage in the investigation, their idea is only “a
working hypothesis”, and that further work is
required to substantiate it.
GEOLOGICAL SETTING
The Tatra Mountains are composed of a crys-
talline core, overlain by a Mesozoic sedimentary
cover and the Tatric, Kríˇna and Choˇ nappes,
which comprise many minor tectonic units (Text-
figs 1A, B). They represent the most northern mas-
sif of the Inner Carpathians. Nappe-folding pro-
ceeded from the south, gradually incorporating
increasingly northerly located sedimentary zones.
Thrusting of the Choˇ onto the Kríˇna Nappe
started after the Early Albian in the south, and
after the Early Cenomanian in the north (R AKÚS &
M ARSCHALKO 1997). The nappe-thrusting in the
Tatric took place during the Cenomanian and
Early Turonian (M I ˇ IK & al. 1985). As a final stage,
the autochthonous sedimentary cover of the crys-
talline core underwent folding. At the base of the
thrust nappes Middle Triassic dolomites and rocks
known as Rauhwacke or Zellendolomite usually
appeared (K OTA ¡ SKI 1956, P LA ˇ IENKA & S OTÁK
1996, J UREWICZ 2003). According to W ARREN
(1999), evaporite-lubricated protoliths of
Rauhwacke acted as detachment horizons during
thrusting and folding.
Pressure and temperature during thrusting
Processes of tectonic transport probably took
place in underwater conditions at full saturation of
rocks with seawater. Studies of fluid inclusions in
synkinematic quartz on slickensided low-angle fault
surfaces from the granitoid core (connected with
nappe-thrusting) proved that they originated at a
pressure of 145-170 MPa and a temperature of 212-
254°C (J UREWICZ & K OZ ¸ OWSKI 2003). Nappe-
thrusting processes of the Tatric Nappe took place
at a depth about 2 km nearer the surface (6-7 km
for the upper part of granitoid rocks minus the
thickness of autochthonous High-Tatric sedimenta-
ry cover c. 1.1 to 2.4 km by K OTA ¡ SKI 1959) and
hence temperatures and pressures could have been
lower; however temperatures determined from
chlorite and feldspar thermometers obtained from
the shear zone within the Tatric Nappe varied in the
range 300-350°C (J UREWICZ & S ¸ ABY 2004).
In a very similar situation, much higher temper-
atures (213-471°C) and pressures (20-540 MPa)
were obtained by M ILOVSKY ∂& al. (2003) from
investigation of fluid inclusions in the basal catacla-
sites of the Murá ˇ Nappe belonging to the
308
EDYTA JUREWICZ & al .
Silicicum cover nappe system (southern part of the
Central Western Carpathians). The wide range of
pressure values was interpreted by those authors as
a reflection of locally supralithostatic overpres-
sures. Such large amplitude fluid pressure fluctua-
tions determined on the basis of fluid inclusion
studies have also been noted by R OBERTS & al.
(1996) on fault-fracture veins associated with steep
reverse faults.
zones are diverse and complicated (Text-fig. 3). On
the Sto∏y Hill, the contact between the Tatric and
Kríˇna nappes is locally stylolitic (B AC -
M OSZASZWILI & al. 1981). The shear fissure is
closed. Triassic dolomites of the Kríˇna Nappe and
Urgonian limestones of the Tatric Nappe stick
closely to each other, without any damage zone or
cementing material, as if glued together (B AC -
M OSZASZWILI & al. 1981, J AROSZEWSKI 1982,
J UREWICZ 2003, J UREWICZ & S ¸ ABY 2004). In some
places a number of isolated megaclasts of Urgonian
limestones, belonging to the Tatric Nappe, and tec-
tonically incorporated into the Triassic dolomite of
the Kríˇna nappe, were noted in the hanging wall.
There is no tectonic deformation connected with
this incorporation. The thrust surface lacks the
slickensides that would enable kinematic analysis of
tectonic transport and reconstruction of the stress
field. Rocks in the vicinity of the stylolitic contact
show no evidence of strong deformation, with the
Character of the thrust zones
In many cases, rocks within the shear zones and
at the bases of the nappes do not show any features
which could indicate such high temperatures.
There is no evidence of metamorphism in the wall-
rocks. The surfaces of the thrusts are not planar.
Their complex course is clearly visible in the cross-
section (Text-fig. 1B) and directly in the field (Text-
fig. 2A). Structures appearing within the thrust
Fig. 2. A – Complicated course of the thrust zone at the base of the Czerwone Wierchy unit (Kozi Grzbiet Ridge). B – Tectonic con-
tact between Urgonian limestone of the Tatric Nappe (light) and Anisian dolomite of the Kríˇna Nappe (dark); Sto∏y Hill. C – Typical
slickensided fault plane, mineralized with quartz and epidote, originated within granitoid core of the Tatra Mts. D – Fragment of the
granitoid rock with fault plane coated with synkinematically-grown quartz and epidote
391300274.003.png 391300274.004.png 391300274.005.png 391300274.001.png
CAVITATION EROSION
309
exception of pressure solution within the limestone
and of hydraulic fractures within the dolomite
(Text-fig. 2B). This is connected with the radically
different mechanical behaviour of the limestone
and dolomite, which makes the dolomite less sus-
ceptible to dissolution and more prone to brittle
disintegration (P ASSCHIER & T ROUW 1996,
K ENNEDY & L OGAN 1997). To sum up, there is a
lack of evidence that this is the base of the nappe or
that this is the shear zone.
A different situation occurs e.g. at the base of
the Giewont Unit or in the Zadnie Kamienne shear
zone (J UREWICZ 2003, J UREWICZ & S ¸ ABY 2004),
where typical dynamometamorphic structures such
as foliation, stretching lineation and veining, associ-
ated with pressure solution, strain shadow and neo-
formed minerals, can be found (Text-figs 3D-F). In
some cases (e.g. in the base of the Czerwone
Wierchy Unit), these structures show signs of fold-
ing (Text-fig. 3F). Different characters of the shear
zones in the Tatra Mts. are inseperably linked to the
anisotropy of the rocks and the concomitant
anisotropy of the shear surfaces. Such variability of
tectonic structures appeared in the sedimentary
cover only. The main cause for the lack of a com-
parable structures within the granitoid core is the
planar character of the fault surfaces (Text-figs 2C,
D) and tightened fissures preventing fluid migra-
tion (J UREWICZ 2006). The above-mentioned fluid
inclusion investigation revealed rather narrow
ranges of pressure and temperature values, which
indicate rather uniform conditions of quartz forma-
tion and deformation. This is connected with the
relatively isotropic character of the granites in com-
parison to the lithologically diverse sedimentary
rocks, and with the fact that in many cases the acti-
vation took place only once. Due to the low solubil-
ity and low porosity of granite, as well as the lack of
sources of fluids, hydrotectonic phenomena and
associated cavitation erosion could not appear in
the crystalline core of the Tatra Mts.
various ways. The multistage character of rocks
deformations are connected with multiply activa-
tion of tectonic displacement depended on cyclical
changes in pore fluid pressure. The build-up of
pore fluid pressure leads to a decrease in stress to
an effective value (H UBBERT & R UBEY 1959) and to
rupturing by faulting associated with hydraulic frac-
turing. A model of fault development in carbonate
rocks based on repeated crack-seal-slip cycles was
described by P ETIT & al. (1999) and R ENARD & al.
(2000). Processes of such a kind, in which fluid
pressure plays a key role, were termed hydrotec-
tonic phenomena by J AROSZEWSKI (1982) and K OPF
(1982, 2003). In the Tatra Mts., the cyclical charac-
ter of nappe movement was described by J UREWICZ
(2003).
Newly-formed shear zones associated with a
fault-related fracture net provide a drainage path
for fluid migration (S IBSON 1996, 2004; G UDMUND -
SSON & al . 2001). In the case of the Tatra Mts., the
source of fluids could have been pores (which
appeared due to solution of salt crystals and filled
with meteoric water) or fluids could have originat-
ed from, for example, the dehydration of gypsum,
occurring in the so-called Anisian “cellular
dolomites” (K ASI ¡ SKI 1981) and in sediments of
Rauhwacke type (P LA ˇ IENKA & S OTÁK 1996,
M ILOVSKY ∂& al. 2003). It cannot be excluded that
the shear zone was a passageway for hydrothermal
solutions, this being supported by the presence of
hydrothermal feldspar crystallizing at a tempera-
ture of ~350°C (J UREWICZ & S ¸ ABY 2004). Fluids
and rock fragments filling the shear zone formed a
suspension circulating along the hydraulic gradient
(S IBSON 1996).
The presence of such a suspension, described by
K OPF (2003) as a “fault slurry”, causes a decrease in
friction, with the angle of internal friction decreas-
ing to values close to zero (J UREWICZ 2003).
According to B RODSKY & K ANAMORI (2001), the
lubrication effect of the fluid in all fluid-filled faults
facilitates tectonic transport and reduces the fric-
tion stress by as much as 30% relative to the hydro-
static value or 50% to the dry rock friction. M ARON
(2004) stated that friction at the interface between
the fault walls may additionally fall dramatically
due to high rates of slip, e.g. seismic in nature.
After displacement, the shear zone was gradu-
ally veined, cemented and immobilised. During this
time, ductile folding took place of material filling
the shear zone, comprising brecciated, mylonitized
Mechanism of tectonic transport and shearing-
related processes
The character and mechanism of deformations
within the shear zone at the base of the Tatric
nappes could be established from the investigation
of dilation fissures associated with the thrust sur-
face (J UREWICZ 2003, J UREWICZ & S ¸ ABY 2004).
The preserved rocks are tectonically deformed in
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