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Transcript
TECTONOPHYSICS
ELSEVIER
Tectonophysics
240 (1994) 29-43
The origin of the Dead Sea rift
Vladimir
Department
Lyakhovsky,
Zvi Ben-Avraham,
Moshe Achmon
ofGeophysics and Planetary Sciences, Raymond and Beverly Sackler Fuculty of Exact Sciences. Tel Al,il. Unir~er.sity,
Tel Ar,it, 69978, Israel
Received
14 April 1993; revised version
accepted
2 February
1994
Abstract
The Dead Sea rift is considered
to be a plate boundary of the transform type. Several key questions regarding its
structure and evolution are: Does sea floor spreading activity propagate from the Red Sea into the Dead Sea rift?
Did rifting activity start simultaneously
along the entire length of the Dead Sea rift, or did it propagate from several
centres? Why did the initial propagation
of the Red Sea into the Gulf of Suez stop and an opening of the Gulf of
Elat start?
Using crustal structure data from north Africa and the eastern Mediterranean
and approximating
the deformation of the lithosphere
by a deformation
of a multilayer thin sheet that overlies an inviscid half-space,
the regional
stress field in this region was calculated.
Using this approach
it is possible to take into account variations
ot
lithospheric
thickness and the transition from a continental
to an oceanic crust. By application of a strain-dependent
visco-elastic model of a solid with damage it is possible to describe the process of creation and evolution of narrow
zones of strain rate localization, corresponding
to the high value of the damage parameter,
i.e. fault zones.
Mathematical
simulation of the plate motion and faulting process suggests that the Dead Sea rift was created as a
result of a simultaneous
propagation
of two different transforms.
One propagated
from the Red Sea through the
Gulf of Elat to the north. The other transform started at the collision zone in Turkey and propagated
to the south.
1. Introduction
The Dead Sea rift is a plate boundary
between
the Sinai subplate and the Arabian plate (Fig. 1).
It extends over 1000 km from the southern tip of
the Sinai peninsula
to the Taurus Mountains
in
Turkey. The southern and central portions of the
Dead Sea rift trend north to north-northeast
and
approximately
follow a small circle (Le Pichon
and Franchetau,
1978; Joffe and Garfunkel,
1987).
This rift offers a unique opportunity
to study the
process of rift propagation
as well as other problems associated with continental
rifting. Geological and geophysical
evidence
from the Gulf of
0040.1951/94/$07.00
0 1994 Elsevier
SSDI 0040-1951(94)00106-J
Science
Elat, at the southern
part of the Dead Sea rift,
and other parts of the rift indicate that two kinds
of geodynamical
processes occur here simultaneously (Ben-Avraham,
1987). The first is a transform motion which has led to a total displacement of 105 km on the faults along the Dead Sea
rift since the time of its formation
less than 20
Ma (Freund et al., 1970; Garfunkel,
1981) and to
the formation
of a series of pull-apart
basins
along the entire length of the rift zone. The other
process is a propagation
of actual crustal spreading activity from the Red Sea northward
into the
Gulf of Elat (Ben-Avraham,
1985).
The origin of the Dead Sea rift is unclear.
B.V. All rights reserved
microplate
sea microplate
Fig. 1. Plate tectonic model for the eastern Mediterranean and surrounding areas (after McKenzie, 1972). The dashed line box indicates the Are;; studied; I = Sinal
2 = Red Sea; 3 = Gulf of Suez: 4 - Gulf of Elat. Arrows indicate motion of plates relative to Eurasian plate. Inset: main faults in northern Levant (after Walley,
1988).
FRICAN PLATE
Turkish
Black
V Lyakhovsky et al. / Tectonophysics 240 (1994) 29-43
Several models published recently have suggested
that rifting activity along the Dead Sea rift propagated from the northern
Red Sea in the south to
the north Wink et al., 1984; Steckler and ten
Brink, 1986). In the southern
part of the rift,
gravity, magnetic, seismic refraction and heat flow
data indicate a propagation
of the spreading
activity within the Gulf of Elat, from the Red Sea
northward
(Ben-Avraham,
1987). Only in the
southern part and possibly also in the central part
of the Gulf of Elat is actual mantle upwelling
now taking place.
The northern
part of the Dead Sea rift is
located close to the collisional
belts along the
Cyprian Arc and Taurus Mountains.
Stress generated in this zone can propagate
a long distance
into the interior of the adjacent plates. Based on
the analysis of crustal structure
variation
in the
eastern Mediterranean,
Ben-Avraham
and Grass0
(1991) offer an alternative
view on the formation
of the Dead Sea rift. They suggested
that the
initial cracking of the crust and faulting activity
have started at the collision zone in the north and
propagated
southward.
Rifting from the Red Sea
northward began later. A simulation
of a faulting
processes along the northern
Dead Sea and the
Levant margin (Ben-Avraham
and Lyakhovsky,
1992) suggests that the formation
of the major
structural elements could be explained as a result
of a simultaneous
propagation
of the Dead Sea
rift from the north and south.
In this paper we describe a simulation
of the
propagation
of rifting along the Dead Sea trend
by taking into account both an opening of the
Red Sea in the south and collisional processes in
Turkey in the north.
2. Plate tectonics
of the region
The geometry of the four major plates, African,
Arabian, Turkish (Anatolian)
and Black Sea (Fig.
1) was derived
from a model of the eastern
Mediterranean
and surrounding
areas proposed
by McKenzie (1972). The main sources of motion
in the region are the stresses exerted on it through
the northward motion of the Arabian and African
plates. Rifting in the Red Sea, a plate boundary
31
between Africa and Arabia, has been active since
the Oligocene (Cochran et al., 1986). The northern Red Sea is still in the late stage of continental rifting (Steckler and ten Brink, 1986). Rifting
in the Gulf of Suez, a northern
arm of the Red
Sea, began in the latest Oligocene/Miocene.
A
widespread
unconformity,
the Mid-Clysmic
event
at approximately
17 Ma (Garfunkel
and Bartov.
1977) marks a dramatic
change in its tectonic
evolution.
Motion
along the Dead Sea rift. which is
younger than 19 Ma, accommodates
3/4 of the
Africa-Arabian
opening (Steckler and ten Brink.
1986). There is no clear evidence of rifting activity along the Dead Sea rift prior to the MidClysmic event. Furthermore,
the reorganization
of the faulted blocks and change in subsidence
rate in the Gulf of Suez at this time is consistent
with the changes expected from the development
of a new plate boundary (Steckler and ten Brink.
1986). Geological evidence on the timing of events
in the Gulf of Suez and Gulf of Elat at the
southern
part of the Dead Sea rift. indicate that
the Gulf of Suez initiated
prior to the Gulf of
Elat as the northernmost
part of the Red Sea.
However, soon thereafter,
the Gulf of Elat developed and accommodated
most of the plate motion north of the Red Sea.
Seismic refraction
studies in the northeastern
and southwestern
Red Sea show that the adjacent
continental
crust is about 35 km thick and that it
decreases
to about 20 km under the coastline
over a distance of 30 km (Le Pichon and Gamier,
1988). Based on reconstruction
of the Red Sea
opening, Sultan et al. (lY92) suggested that prior
to rifting, the continental
crust underlying
the
Red Sea was also about 35 km thick.
The Dead Sea transform runs more than 1000
km from the Gulf of Elat in the south to the
Taurus-Zagros
convergence
zone in the north. A
total left-lateral
offset of about IO5 km in its
southern part is determined
by matching numerous rock bodies and structures
south of Lebanon
(Freund et al., 1970; Joffe and Garfunkel,
1987).
The southern
and central portion of the Dead
Sea rift trend north to north-northeast
and approximately
follow a small circle (Le Pichon and
Francheteau,
1978; Joffe and Garfunkel,
1987).
31
K Lyakhousky et al. / Tecfonophysics 240 (1994) 29-43
In the northern Dead Sea rift, the Yammuneh
Fault strikes N30”E and connects the central
Dead Sea rift with the north-trending Ghab Fault
(Walley, 1988). Besides the Yammuneh Fault,
several other faults can be related to the plate
boundary in this area.
Several hypotheses have been forwarded to
explain the tectonic framework and faulting processes in the northern Dead Sea rift. Ron (1987)
considered the Yammuneh Fault as a restraining
bend of the Dead Sea rift and suggested that the
regional shear in this area is accommodated by
secondary faulting and block rotation. Walley
(1988) objected to the assumption that the entire
displacement on the Dead Sea rift is transmitted
northward along the Yammuneh Fault and suggested that the left-lateral motion is transmitted
along a number of faults. Girdler (1990) has
suggested that the Dead Sea rift continues northward as the Ed Damur (Roum) Fault, which
follows a trend similar to the central Dead Sea
rift. He further suggested that the Roum Fault
extends into the Mediterranean south of Beirut
to meet the Gyprian Arc somewhere east of
Cyprus. According to this scheme, the Yammuneh Fault is not a plate boundary. One major
problem concerning the northern part of the Dead
Sea rift is that the displacement on the Yam-
muneh Fault or any other fault in this area is
relatively small, much less than the displacement
on the southern and central Dead Sea rift. According to Walley (1988) only 60 km of displacement took place along the Yammuneh Fault.
Large variations in crustal structure exist in
the Levant and eastern Mediterranean
(BenAvraham and Ginzburg, 1990). The Levant passive continental margin marks a transition from
the oceanic crust of the Levantine Basin to a
typical continental crust of the Levant (Makris et
al., 1983; Ginzburg and Ben-Avraham, 1987). The
Levant itself is probably composed of distinct
crustal domains of different origins. For example,
the crust of the Galilee-Lebanon
region, which is
bordered on the east by the Dead Sea transform,
is markedly different from the areas to the east
(the Palmyra zone in Syria) and south (the
Judea-Samaria
region)
(Ben-Avraham
and
Ginzburg, 1990). These crustal structure variations have probably caused a segmentation of the
collision zone in the north along the Cyprian Arc
and the Taurus Mountains. The segments are
separated by large fault zones (Ben-Avraham and
Grasso, 1991). Seismic refraction studies indicate
a sharp boundary between continental
and
oceanic crusts along the northern Levant margin
as compared with a wide transition zone along
Fig. 2. Palaeotectonic map of Turkey of the Late Eocene-Early
Miocene (after Sengor and Yilmaz, 1981).
33
V. Lyakhocsky et al. / Tectonophysics 240 (1994) 29-43
the southern Levant margin (Ginzburg
and BenAvraham, 1987). Seismic reflection data show the
existence
of probable
strike-slip
faulting
along
the northern
Levant margin (Ben-Avraham
and
Ginzburg,
1990).
The Turkish (Anatolian)
microplate
is located
between
the Eurasian,
African
and Arabian
plates. Its northern
boundary,
the north Anatolian Fault, is one of the major tectonic features
with well defined
fault trace. The age of the
north Anatolian
Fault is not well known. Ketin
(1968, 1969) suggested
that the fault has been
active since Pliocene-Quaternary
time with a total displacement
of a few tens of kilometres.
Sengor and Canitez (1982) suggested a time of
initiation
between
the Burdigalian
and
the
Pliocene
and cumulative
offset of 85-90 km.
Creep
measurements
and earthquake
studies
(Toksoz et al., 1979) indicate
that the current
average slip rate of the fault is about 2 cm/year.
The east Anatolian
Fault is generally considered to be a major strike-slip fault bounding
the
Anatolian
block and Arabian
plate (McKenzie,
1978; Jackson and McKenzie, 1984; Sengor et al.,
1985). This region has been and is still subject to
compressive
tectonics (Lyberis et al., 1992). The
sedimentary
cover displays a large, 5-10 km wide,
curved fold structure, located along the east Anatolian Fault. Further
south the Arabian
plate
seems to be undeformed.
Kasapoglu and Toksoz
(1983) suggested
that the initiation
of motion
along the Dead Sea transform
is older than the
beginning
of the strike-slip
motion on both the
east and the north Anatolian
Faults. A palaeotectonic map of Turkey by Sengor and Yilmaz (1981)
of the late Eocene-early
Miocene (Fig. 2) suggests that the Africa-Eurasia
convergence
took
place along a sinuous,
uniformly
north-dipping
subduction
zone beneath
southern
Turkey. This
subduction
zone was consuming
very young
oceanic lithosphere
of the Cungus basin along its
eastern extent, prior to the collision of Arabia
and Eurasia, whereas south of central and western Anatolia
much older lithosphere
was being
subducted.
Subduction
along the arcs south of
central and western Anatolia is still taking place
at present.
3. Stress field simulation
Simulation
of the faulting
processes
in the
crust raises two main problems:
(a) What is the
stress field distribution
in the crust? tb) Which
rheological
model of the crustal material is able
to describe the faulting process?
To calculate
the stress field distribution,
following England and McKenzie (1982, 1983) and
Vilotte et al. (1986), we approximate
the deformation of the lithosphere
by the deformation
of a
thin sheet that overlies an inviscid half-space.
Because the horizontal
dimensions
of the sheet
are much greater than the vertical dimension,
and the shear stresses are assumed to be zero on
the top and the bottom of the sheet, the deformation is approximated
by neglecting
the vertical
gradients of horizontal velocity components.
This
allows the deformation
of the sheet to be expressed in terms of vertical averages of the strain
rate and the deviatoric stress.
The lithosphere
itself has also its internal
structure. Typical continental
lithosphere
consists
of a number of layers. They are: a sedimentary
layer, granitic and basaltic layers (upper crust and
lower crust), and an upper mantle (Fig. 3). The
thickness
of each layer in the simulated
litho-
Distancedoni:
Fig. 3. Model of the layered
See Fig. 5 for the location
area.
profl!r
[km
structure of the continental
crust.
of the profile in the simulation
34
V. Lyukhocsky et al. / Tmtonophysics 240 (1994) 29-4.7
sphere is variable and the rheology also varies
from layer to layer. Thus, it is some possibility to
introduce a depth-dependent structure and rheology into two-dimensional in-plane stress simulation. Under the lithosphere we assume the existence of an inviscid asthenosphere.
Governing
equations of the in-plane stress approximation
were derived by a perturbation technique (Nayfen,
1981) for the integration of the equations of
motion of the lithosphere along a vertical axis. To
realize this procedure we defined the boundary
conditions and the rheology of each layer. The
upper boundary (topography) was assumed to be
free, i.e. forces acting on this boundary are equal
to zero. Forces and velocities are assumed to be
continuous on all internal boundaries. The existence of an inviscid, as compared with iithosphere, asthenosphere provides a state of a zero
shear force at the boundary between the asthenosphere and the lithosphere. The normal stresses
at the base of the lithosphere are defined in
accordance with the assumption of the local
isostasy equilibrium. The rheology of the sedimentary layer was described by a linear viscous
Newtonian body; for all the other layers, a viscoelastic model of a material with damage is described below. The effective viscosity of the sedimentary layer is assumed to be much smaller
than the average viscosity of the crystalline crust.
Thus, we had to simulate stress distribution in
two types of layers. The first type is the lowviscosity sedimentary layer, and the second type is
all the other layers with similar rheological properties. To describe a viscous flow velocity distribution (vi) in the first layer we used the NavierStokes equation in the following form:
(1)
div ( ui) = 0
where: p, = density of sediments; p = pressure;
7, = viscosity of sediments; gi = gravity acceleration vector (gi = (O,O,- g)>; i = index corresponding to the number of the coordinate axis, where
1,2 = horizontal
axes, 3 = vertical axis; A =
Laplace operator.
Neglecting higher-order terms of small parameter E = H/L (the ratio of average vertical size of
the lithosphere to its horizontal size). we intcgrated (1) and obtained the equations that dcscribe the velocity and stress fields in each layer
of the model. Velocity of the motion in the sedimentary layer relative to the crustal velocity vector V, under the sediments is (Mikhaylov. 1983):
/j,g
C’,
=
ah,
2t),a,(hz-x,)(hZ+-r,-2/r,)
I
1.’ 2
=
‘lg ah,(h,-x,)(h,+.r3-Zh,)
277, 3x2
(2)
-
c.3 =
To take into account erosion and sedimentation during the evolution of the upper surface,
the diffusion approach is applied. This approach
is widely used in geomorphology and civil engineering to simulate the long-term behaviour of
river systems. The diffusion model has been applied to the development of river delta’s in fjord
and glacial lakes (Syvitski et al., 1988). and to
foreland basins (Fleming and Jordan, 1989; Sinclair et al., 1991). Following Kenyon and Turcotte
(1985) an equation of motion of the upper boundary (h,) is:
dh,
-==J+AAh,+$
(3)
dt
The Laplace operator of h, with a transportation
coefficient A makes it possible to take into account a process of smoothing of the relief due to
denudation, and a function $(n,,x2,r), to introduce into the model a description of the erosion
and sedimentation processes.
Substituting (2) into (3) gives an equation for
the partial temporal derivation of the relief:
ah,
-=
at
’
+$-y:z+V,+hAh,+d
I
-
2
p,dh,
-h,f
377,
---
ah, ah,
ax, axI
1
Ah
+
I
p,g(h,
-h,)*
VI
(4)
V. Lyakhocsky
et al. / Tectonophysics
Eq. (4) is solved numerically for the known motion of the crust (F>. The first approximation of
the stress distribution in the sedimentary layer
gives a pressure equal to a lithostatic pressure
p=~,g(h,
-x,) an d a b sence of a deviatoric component due to the low viscosity.
According to the Maxwell visco-elastic constitutive relationship, the deviator of the stress tensor (sii) for the layers 2, 3, 4 is equal to:
240 (1994) 29-43
X
exp
snlZ= exp i
X exp
sn,,= exp
i
(8)
i
and lithostatic pressure:
(5)
X exp
where the index n = 2, 3, 4 denotes the consecutive layers, I_Lis the effective shear modulus and
77 the effective viscosity, which are functions of
the parameters of the layer, and t is time.
Using Eq. (5) we get the equations of motion
for the visco-elastic medium analogous to the
Navier-Stokes equation (1):
(6)
and ignoring a compressibility of material during
a long term deformation we add:
div (13,) =0
p = -
13pgdx-,
j iI1
These formulas allow the first approximation
of the deformation of the lithosphere to be expressed by neglecting vertical gradients of horizontaI velocity components in terms of strain rate
and deviatoric stress components. This method
also permits us to deduce an analytical solution
for sr3 and sz3 components of the stress tensor.
Using all components s,~ and the absence of
shear forces on the boundary between lithosphere and asthenosphere it is possible to achieve
equations of the motion of the lithosphere:
where:
Si,=S*,j(h2-h3)
In a similar way to the analysis of Eq. (I), we
get the first approximation of the velocity components:
[In, = V,(x,, x2)
+ss”i,(h,-h,)
+s4,,(h4-h5)
( 10)
and f, = effective internal forces caused by variations in layer thickness:
I!‘I7
I = Vz(xr, x2)
(7)
deviatoric stress components
(sij>:
(11)
For the steady-state case Eq. (10) gives an
effective viscosity of the lithosphere 77= n2(hz h,) + n&/z3 - h4) + n&/z4 - h,). This equation
and Eq. (11) for the internal forces are the multi-
layer analog of the one-layer approximation used
by Sonder and England (1989).
Eqs. (8-l 1) are the mathematical analog of a
2-dimensional
visco-elastic problem and are
solved numerically by the “FLAC” algorithm described below.
4. Model of a medium with damage
A long-term action of stress and temperature
will cause growth or healing of microcracks resulting in a changing of the rheological properties
of a solid. Recent investigations of a fracturing
process in granite by Yukutake (1989) and Lockner et al. (1991) show that this process can hardly
be described in terms of a classical Griffits model
of a single crack propagation. Lockner and Madden (1991) put forward a multiple-crack model of
brittle fracture. Many attempts have been made
to define and estimate suitable variables to describe the extent of fracturing. Such variables
should be able to characterize the processes of
fracturing quantitatively and should be suitable
for modeling from the point of view of continuum
mechanics. Among such approaches are Robinson’s (1952) linear cumulative creep damage law.
Hoffs
(1953) ductile creep rupture
theory,
Kachanov’s (1961, 1986) brittle rupture theory,
Rabotnov’s (1969) coupled damage creep theory
and many modifications of these theories. Following this approach and using the strain-dependent
moduli model, a description of the damage evolution of a fractured medium under long-term stress
has been put forward (Lyakhovsky and Myasnikov, 1985; Myasnikov et al., 1990; Lyakhovsky
et al., 1993). This model has made it possible to
simulate the evolution of fracturing under tectonic stress, resulting in the appearance of seismic boundaries of a rheological nature (Mints et
al., 1987; Lyakhovsky and Myasnikov, 1987, 1988)
and investigate a faulting process in the northern
Dead Sea rift (Ben-Avraham and Lyakhovsky,
1992).
In order to simulate a faulting process in terms
of continuum mechanics a nondimensional dam-
age parameter (Yis incorporated in a visco-elastic
Maxwell model. This parameter lies in the interval from 0 to 1 and describes the evolution of the
medium from an ideal undestroyed solid to an
absolutely destroyed material. Elastic moduli are
supposed to be linear functions of U. Assuming
the process of elastic deformation to be reversible
and following the principle of maximum rate of
entropy production, a phenomenological
equation for damage evolution was suggested (Lyakhovsky et al.. 1993):
da
= al: + bl, + cl,cj;
dt
where: t = time; I, = cii and I, = c,,ci, = the first
and the second invariants of the elastic strain
tensor lij. According to the multilayer approximation, an average value of the elastic deformation for each layer was taken to calculate the
damage distribution in each layer.
To simulate any flow it is necessary to define
an effective viscosity as a function of parameters
of a solid. Power law viscosity is usually assumed
for rocks in the ductile regime. Not much is
known about the viscosity in the brittle regime,
except that it is very strongly dependent on the
level of fracturing. To take into account a stronger
variation of viscosity in comparison with elastic
moduli, we assume the viscosity n to be an exponential function of the damage parameter (r:
q =A
exp( -Ba)
(13)
where A and B are constants.
Variation of Q between destroyed and undestroyed zones causes changes of the effective
viscosity of about lo4 times. Viscosity of the
upper crust, for instance, changes from about
10” Pa s for an undestroyed block up to 1O23Pa
s for a weak zone. A detailed description of the
model is presented by Lyakhovsky et al. (1993).
The application of this model makes it possible
to simulate the rheological transition from a ductile to a brittle regime and the process of creation
and evolution of narrow zones of strain rate localization, corresponding to a high value of damage
parameter, i.e. the evolution of fault zones.
V. Lyakhordy
5. Computation
techniques
Numerical simulation has been done using the
“FLAC” algorithm (Cundall and Board, 1988;
CundalI, 1989). The formulation is explicit in
time, using an updated Lagrangian scheme to
provide the capability for large strains. FLAC is
believed to offer advantages over conventional
finite element schemes in cases where flow and
material instability occur. Physical instability can
be modeled without numerical instability if internal terms are included in the equilibrium equations. The FLAC method has an advantage over
implicit methods because it is computation~~lly
inexpensive for each time step and it is memoryefficient because matrices storing the system of
equations are not required. An application of this
method to the simulation of a visco-elastic flow is
described in Poliakov et al. (1993).
The computational mesh consists of quadrilateral elements, which are subdivided into pairs of
constant-strain triangles, with different diagonals.
This overlay scheme ensures symmetry of the
solution by averaging results obtained on two
meshes (Cundall and Board, 1988). Linear triangular element shape functions L, are defined as:
L, =ux +xh,
iryc,
37
L’Ial. / Tectonophysics 240 (1994) 29-43
( 14)
where (lx, h,, ck are constants, and x and y are
grid coordinates. These shape functions are used
to interpolate the nodal velocities ~1:“’ within
each triangle element (e):
where nj is the j component of the unit vector
normal to each side of the element adjacent to
the node II. The length of each side is denoted by
Al. The minus sign is a consequence of Newton’s
third law. New velocities are computed by integrating the equation of motion over a given time
step Al:
(171
If a body is in a state of mechanical equilibrium,
the net forces on each node are zero; otherwise,
the nodes are accelerated. The new coordinates
of the grid nodes are computed by:
n,‘“‘( t + At) = xf”‘( t) + r~f”‘Ar
( 18)
and then the calculations are repeated for a new
configuration. Together with the deformation a
new damage distribution
is calculated using
known stresses. Thus, a visco-elastic deformation
of a damaged material is simulated.
When the mesh becomes too distorted it is
necessary to apply a special remeshing procedure.
An interpolation from the old nodes to a new
mesh must be done only at this stage. This is in
contrast to the Eulerian method where this interpofation must be performed at every time step.
An interpolation of velocities from the old mesh
to a new one is made by using shape functions L,
(Eq. 14). To interpolate media parameters, which
are constant inside each element, these parame-
This formula enables the calculation of the strain
inurements in each triangle and element stresses
using a constitutive law. All the parameters of the
media inside the element, such as damage, viscosity and elastic moduli are approximated by a
constant. When stresses in each triangle are
known, the forces at the node number 12 (I;;(“))
are calculated by projecting the stresses from ail
elements surrounding the node:
Fig. 4. The location of an element
additional
points for reinterpolation
of a regular mesh with
from a distorted mesh.
3x
K LyakhoLvky et al. / Tecronophysics 240 (1994) 29-43
ters are interpolated from the old elements to an
additional 15 points inside the new element of
the regular mesh (Fig. 4). An average value calculated over these points is projected onto the new
element. This method of interpolation makes it
possible to reduce the numerical diffusion caused
by a discrete mesh approximation.
Turkish mIcroplate
\
6. Results of computer simulation
In order to simulate the plate tectonic evolution of the region boxed in Fig. 1 two types of
lithosphere were introduced.
(1) The lithosphere of the Africa, Arabia,
Turkey and Black Sea microplates (Fig. 5) is
assumed to have a continental crust of about 35
km thickness. It has a 15 km thick granitic layer
with 2.7 g/cm3 density and a 20 km thick basaltic
layer with 2.9 g/cm3 density. The density of the
upper mantle is assumed to be 3.4 g/cm3. A very
thin sedimentary layer of about 0.5 km with 2.4
g/ cm3 density initially covers a continental-type
lithosphere. It should be mentioned here that the
African and Arabian plates were assumed to be
initially similar and homogeneous. Crustal structure variations between Galilee-Lebanon,
Judea
and Sinai were not taken into account. Therefore
it is difficult to expect an exact simulation of the
geometry of the newly created Dead Sea rift,
which locally must follow some pre-existing weak
zones and boundaries of blocks with different
crustal structure.
(2) An oceanic lithosphere with a 4 km thick
sedimentary layer and a 7 km thick basaltic layer
represents the eastern Mediterranean, which is
probably an oceanic part of the African plate,
and the Cungus basin, which was an oceanic
northern part of the Arabian plate. The north
Anatolian Fault and the Red Sea rift were introduced initially as the destroyed zones with a high
value of the damage parameter (Y. The initial
block geometry is based on the palaeotectonic
map shown in Fig. 2 and the rigid block kinematic
reconstruction made by Lyberis et al. (1992).
The boundary conditions shown in Fig. 5 correspond to the northward motion of Africa and
Arabia with a different rate. A free slip condition
i=o
$=5cm/y
>
Arabia
‘A
Afrlu
1~
V&J
I
vy=2cm/y
R=O
vy=5cm/y
Fig. 5. Outline of the main geological structures and boundary
conditions for the simulated area. See Fig. 3 for the initial
crustal structure of the simulated area along the profile A-A.
is enforced on the African and the Mediterranean parts of the western boundary. Therefore
the boundary of this section can move only in a
north-south direction. This boundary condition is
in agreement with a current northward motion of
the African plate and the modern tectonic stress
field in the Mediterranean region (Rebai et al.,
1992). The Turkish part of the western boundary
is assumed to be free, whereby westward motion
of the Turkish microplate is possible. The Black
Sea microplate is taken as fixed in its place. This
condition implies that all motions in the simulated area are defined with respect to the fixed
Black Sea microplate. The eastern boundary of
the simulated region south of the Black Sea microplate moves northward with a constant rate
and without any force acting in the western direction. These boundary conditions are in agreement
K Lyakhouky
et al. / Tectonophysics 240 (1994) 29-43
with the results of a finite element model of the
collision
of the Arabian
and Eurasian
plates
(Kasapoglu
and Toksoz, 1983).
At the initial stage of evolution at about MidMiocene
time (Fig. 6) the boundary
conditions
and the geometry of the lithospheric
units cause a
northward
motion of the Arabian
and African
plates with different rates. This motion results in
a zone of very high gradient
of the horizontal
velocities
(arrows in Fig. 6) or high horizontal
deformation
that
lies between
the
eastern
Mediterranean
and the Cungus basin in the south
and the undeformed
Turkish microplate
in the
north. The thin oceanic crust subducts the thick
and rigid continental
crust along the southern
margin of the Turkey plate. There is also a rotation of the Arabian
plate associated
with the
opening of the Red Sea and its propagation
in a
northwestern
direction.
This propagation
results
in the creation of a zone of low topography (Fig.
,:)()I1
IO0
_..
l(lCl
es
L
s
III00
‘=
>
ilO
Fig. 7. Topography
and horizontal velocities at the beginning
of the simulated collision between Arahia and Turkey. Dashed
line = axes of rifting propagation:
SR = Suez Rift: SDSR =
southern segment of the Dead Sea Rift.
Fig. 6. Topography
in metres
initial stage of the simulation.
and horizontal
velocities
at the
7), which may be interpreted
as the opening of
the Gulf of Suez.
The beginning
of the collisional
process between Arabia and Turkey influences
the stress
distribution
in the whole simulated
area. Northeast of the Red Sea a small anomaly
in the
topography
is developed.
The rheological
model
indicates that there is a transition
zone between
undestroyed
and initially destroyed
crust along
the Gulf of Suez. As a result the new direction of
the rifting process along the Dead Sea rift starts
not at the tip of the Gulf of Suez, where the
weakening
only begins, but slightly southward.
where the crust is already weak. The “partly
rifted” zone at the north end of the Red Sea rift
may be interpreted
as the future Gulf of Suez.
whose formation
started before the creation 01
the Dead Sea rift.
Continuation
of the collisional process (Fig. 8)
results in dramatic changes both in the evolution
I/: Lyukhor,sky et al. / Tectonophysics 240 (1994) 29-43
40
of the topography and in the distribution of horizontal velocities. There is no further propagation
of the Red Sea into the Gulf of Suez. On the
other hand, a newly created northeastern trending of the propagation of the Red Sea into the
Gulf of Elat becomes active. At the same time in
the north a new transform zone starts its propagation to the south at the boundary between the
zone of continental collision and the closing Cungus basin. The simulation, thus, suggests a simultaneous propagation of the Dead Sea rift from
the Red Sea in the south through the Gulf of
Elat northward and from the collision zone in the
north southward. In the simulated case, the Dead
Sea rift (Fig. 9) propagates along the shortest
straight line joining the northern Red Sea and
collision zone. Horizontal deformation of the
1600
1’100
i200
1000
800
600
400
200
Fig. 8. Topography and horizontal velocities at a developed
stage of the simulated collision between Arabia and Turkey.
The beginning of a rift propagation from the collision zone to
the south and from the Red Sea to the north can be clearly
seen. Dashed line = axes of rifting propagation: .!iR= Suez
Rift; SDSR = southern segment of the Dead Sea rift; NDSR
= northern segment of the Dead Sea rift.
Fig. 9. The last stage of the simulation. Localization of the
shear motion at the newly created Dead Sea rift. Dashed
line = axes of rifting propagation: SR = Suez rift; DSR = Dead
Sea rift.
simulated area corresponding to the latest stage
is shown in Fig. 10. There is a newly created high
deformation zone with a left-lateral motion, which
corresponds to the Dead Sea transform. A westward motion of the undeformed Turkish microplate accumulates on the east and north Anatolian Faults. There is also a newly created rightlateral strike-slip fault at the base of the northern
Levant margin. Similar to the northern Dead Sea,
this zone starts its propagation to the south at the
boundary between the zone of continental collision and the eastern Mediterranean basin. The
combination of the northern Dead Sea transform
and the fault zone along the Levant margin causes
the northward motion of the northwestern part of
the Arabian plate to be at a reduced rate as
compared with the areas east and west of it
(Ben-Avraham and Lyakhovsky, 1992).
It should also be noted that in spite of the
existence of a destroyed zone along the north
V. Lyakhorsky et al. / Tectonophysics 240 (1994) 29-43
I ijO0
I 100
-Y
1.3Jo
7
C
z
%
-
1000
800
1100
-100
“00
0
~00
4tirY’600
long.
HO0
1000
rift. It propagated
from the north to the south.
Active tectonics in the northern
part of the Arabian plate also causes a dramatic change of the
stress field around the northern
Red Sea. As a
result, rifting activity changes
its direction
of
propagation
from the Gulf of Suez into the Gulf
of Elat and a new plate boundary
of the transform type was created.
The simulation
suggests that the Dead Sea rift
is made of two different fault zones, which later
on were combined
into one feature. The simulation outlines only the general trend of the Dead
Sea rift. The exact geometry,
especially
in the
northern
part, is affected by local crustal structure variations.
The resulted
geometry
of the
Dead Sea rift follows the actual location of the
southern and central Dead Sea rift, but is derived
from the northern
Dead Sea rift. This suggests
that the crustal structure
of the African
and
Arabian plates in the south is homogeneous,
while
in the north it is variable.
[km]
Fig. 10. Horizontal
deformation
at the last stage of simulation.
Note the development
of a left-lateral
shear zone along the
Dead Sea rift and a right-lateral
shear zone along the northern Levant margin.
I = Dead Sea rift: 2 = north Anatolian
Fault: 3 = east Anatolian
Fault; 4 = shear zone at the Levant
continental
margin.
Anatolian
Fault, the simulation
shows no development of any significant
deformation
and topographic features along this zone until the closing
of the Cungus basin, which happened
at about
the same time as the creation of the Dead Sea
rift.
7. Discussion
31
and conclusion
This mathematical
model of the evolution
of
the Dead Sea rift suggests that the rift was created as a result of the propagation
of two fracture
zones at its northern
and southern ends towards
each other. Due to the collision of Arabia with
Eurasia and the strike-slip motion along the east
Anatolian
Fault a new fracture zone was created
and formed the northern
part of the Dead Sea
Acknowledgements
Critical
reading
by B. Colletta,
Y. Podladchikov, R. Guiraud,
J. Chery and F. Lucazeau
improved the manuscript.
Work by V. Lyakhovsky
was supported
by grants from the Israel Ministries of Science and of Absorption.
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