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doi:10.1144/0016-76492009-118 2010; v. 167; p. 731-749 Journal of the Geological Society
Amit Segev and Michael Rybakov
quiescence on the central and southern Levant continental marginEffects of Cretaceous plume and convergence, and Early Tertiary tectonomagmatic
Journal of the Geological Society
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© 2010 Geological Society of London
Journal of the Geological Society, London, Vol. 167, 2010, pp. 731–749. doi: 10.1144/0016-76492009-118.
731
Effects of Cretaceous plume and convergence, and Early Tertiary tectonomagmatic
quiescence on the central and southern Levant continental margin
AMIT SEGEV* & MICHAEL RYBAKOV
Geological Survey of Israel, 30 Malkhe Israel St. 95501 Jerusalem, Israel
*Corresponding author (e-mail address: [email protected])
Abstract: This study synthesizes geological and geophysical evidence concerning the structure and character
of the central and southern Jurassic Levant continental margin during Cretaceous–Tertiary time. From the
beginning of the Cretaceous and until Cenomanian time, the Levant margin was strongly affected by
extensional tectonics, cyclical igneous activity and rifting coupled with thermal and vertical fluctuations. It is
suggested here that during the Senonian–Maastrichtian convergence of Afro-Arabia and the Mesotethys, and
the Tauride part of Eurasia, the Herodotus basin oceanic crust subducted along the Eratosthenes Arc, below
the short-lived abandoned Levant back-arc basin. Such a plate configuration assumes regional shear zones, as
follows: (1) between the Eratosthenes Arc from the south and the Kyrenia Arc from the north: the NW–SE
Carmel–Azraq–Sirhan fault system; (2) between the Sinai and the African plates: the Suez fault system; (3)
between the Mesotethys and the African plates: the northern Egypt–Sinai–Negev west–east transversal fault
system. Distinct tectonomagmatic quiescence between Late Maastrichtian and Late Eocene time allowed
thermal relaxation and subsidence of the Levant margin until the apparent achievement of local isostatic
compensation and the consequent development of the longest transgression over the Afro-Arabian ramp.
Supplementary material: Details on the construction of the Bouguer gravity map are available at http://
www.geolsoc.org.uk/SUP18404.
The Levant basin and rifted margin formed during a Jurassic
tectonomagmatic event related to the opening of the Mesotethys
(Garfunkel 1998; Walley 1998; Segev 2000, 2002; Fig. 1). Such
margins, often called passive margins, are always formed in pairs
on either side of the oceanic spreading centre that appears after a
continental breakup, and they are commonly tectonically or
magmatically active for tens of millions of years during their
formation and become inactive after the oceanic spreading centre
retreats from the margins. In a simple situation, after such a
retreat, the principal horizontal (plate tectonics) and vertical
forces (mainly thermal uplift or subsidence) decrease and the
margins become passive. Many passive margins undergo renewed
tectonism during their ‘passive’ phase. Such events may form
fold belts (contraction), rifting and flood volcanism associated
with extension, regional uplift or doming, all within the intraplate
continental margin, which consequently result in an isostatically
highly non-compensated nature.
Rocchi et al. (2008) described several continental margins
surrounding the Atlantic Ocean (Senegal, Newfoundland–Grand
Banks, Iberian margin along the Tore–Madeira Rise, north-
western margin of Africa, offshore northeastern Brazil) that were
subjected to ‘delayed’ alkaline magmatism on their earlier
rifted–passive margins. Those workers suggested that this
igneous activity, tens of millions of years after the onset of
spreading, was linked to reactivation of oceanic fracture zones
and named such margins, in addition to volcanic and non-
volcanic margins, ‘delayed volcanic’ passive margins.
At present, the Levant’s central and southern continental
margin is a rifted margin of long duration situated offshore Sinai,
Israel and Lebanon (Fig. 1). Its upper c. 3 km sedimentary cover
was spatially divided by Ben-Avraham & Ginzburg (1986), Ben-
Avraham et al. (2002, 2006) and Schattner & Ben-Avraham
(2007) into two distinct regions, separated by the prominent
Carmel fault. Most of the Levant basin is underlain by oceanic
crust, covered by a 10–14 km thick sedimentary sequence (Ben-
Avraham et al. 2002), of which only the upper c. 3 km have been
studied in detail. On the basis of seismic refraction, deep
boreholes, receiver function and gravity data, as well as isostatic
and gravity 3D modelling, Segev et al. (2006) constructed the
3D layered structure of the Levant region. Moreover, they
delineated a high (up to 2500 m) positive local and regional
isostatic and residual gravity anomaly in Lebanon and northern
Israel caused by an elevated mantle lithosphere. They explained
it by the compressional push-up mechanism of the Dead Sea
Transform plate boundary, which according to their results meets
the Levant continental margin in northern Israel. This evidence
led Segev et al. (2006), Schattner & Ben-Avraham (2007) and
others to suggest that the present-day Levant continental margin
is active. Schattner & Ben-Avraham (2007) suggested a model of
a transform margin to explain the formation of the Levant margin
north of the Carmel fault.
The present study compiles and analyses existing geological,
geochronological and geophysical evidence relating to the early
evolutionary stages of the Levant margin and summarizes these
stages schematically in Figure 2a–c. These early stages, which
involved the Late Triassic–Jurassic formation of the Levant
rifted volcanic margin, were followed by the Early Cretaceous
intense plume-related tectonomagmatic activity (Wilson et al.
2000; Segev 2002, 2009). Our investigation adds new evidence
for understanding the configuration and evolution of the central
and southern Levant continental margin during: (1) Cretaceous
plume activity; (2) Late Cretaceous convergence (Fig. 2d); (3)
the Late Maastrichtian–Late Eocene tectonic quiescence (Fig.
2e). The present research uses: (1) new processing and inter-
pretation of gravity and magnetic data from the eastern Mediter-
ranean; (2) the lithostratigraphic changes across the margin and
their morphotectonic significance; (3) the cyclic tectonomag-
matic activity; (4) a detailed 3D crustal structure reconstructed to
pre-Cenozoic tectonism (from Segev et al. 2010), representing its
configuration during Mesozoic time. This study leads to a new
concept of the Cretaceous and Tertiary evolution of the Levant
basin and margin during one of its most enigmatic periods, the
transition from passive to active margin, plus a new approach to
the debate concerning the nature of the Levant basin.
The central Levant crustal structure
The present-day crustal structure and its characteristics
The transition zone between the Arabian continental plate and
the Levant marine basin, whether the latter is built of oceanic
crust (e.g. Makris et al. 1983; Makris & Wang 1994; Ben-
Avraham et al. 2002; Segev et al. 2006) or of a thin continental
crust (e.g. Woodside 1977; Hirsch et al. 1995; Gardosh et al.
2008; Netzeband et al. 2006) is still debated. Most interpreta-
tions of thin continental crust were based on commercial surveys,
which obtained numerous multichannel seismic reflection pro-
files, frequently recorded to 6 s (e.g. Sage & Letouzey 1996;
Gardosh et al. 2008; Netzeband et al. 2006). These profiles
provide detailed and reliable information about most of the
sedimentary sequence but information about depth to the base-
ment and the Moho, as well as the nature of the crystalline
crust, is lacking. The oceanic nature was suggested by a long-
range refraction experiment (Makris et al. 1983) and a seismic
refraction–wide-angle reflection experiment (Ben-Avraham et al.
2002). Furthermore, comparison between gravity modelling and
observations demonstrates that most of the Levant basin is
isostatically compensated (Segev et al. 2006) and the possibility
of thin continental crust beneath the Levant basin would decrease
the average calculated crustal density by more than 50 mGal and
would elevate the whole Levant basin by more than 400 m. The
Levant continental/oceanic thickness ratio of the crystalline crust
is c. 3:1, therefore extension of c. 300% is needed to produce
this thin continental crust. None of the fault systems suggested
by the seismic reflection profiles can explain such extension.
Consequently, the oceanic nature of the Levant marine basin
crust has been adopted here.
The Levant northwestward-thinning rifted and volcanic margin
has been estimated to have evolved in late Early Jurassic time
(Garfunkel & Derin 1984; Garfunkel 1998; Segev 2002). It was
formed as part of the evolution of the Neotethys and the
Mesotethys oceans (the latter also called southern Neotethys)
during two tectonomagmatic periods, the initial Permo-Triassic
stage and the principal Jurassic stage (Segev 2000, 2002), in
which the Levant region was subjected to cycles of dynamic
uplift and denudation, as well as rifting.
Fig. 1. Location of the main structural
elements of the Middle East (data from
Walley 1998; Bosworth et al. 1999; Abdel
Aal et al. 2000; Robertson 2000; Kazmin
2002; Rybakov et al. 2005; and references
therein) on the hypsometrically shaded
bathymetric and topographic image of the
eastern Mediterranean (compiled by Hall
2005). The division of the Levant region
into three segments (north, central and
south) should be noted. BB; Baer-Basit
ophiolite; H; Hatay ophiolite; KD, Kurd
Dag ophiolite.
A. SEGEV & M. RYBAKOV732
The continental part of the present-day Levant margin has a
crustal thickness of 36 � 1 km, and that of the marine part (the
Levant basin) is c. 23 km thick (Fig. 3; Makris et al. 1983; Ben-
Avraham et al. 2006; Segev et al. 2006). Several geophysical
studies have suggested that the crustal transition in the northern
Levant region is abrupt and located beneath the continental slope
(Ginzburg et al. 1975; Ben-Avraham & Ginzburg 1986; Ben-
Avraham et al. 2002, 2006); in Lebanon it is exposed onland
(Walley 1998). Furthermore, Schattner & Ben-Avraham (2007)
suggested a tectonic framework for the formation of the Levant
margin during the Mesozoic based on the present shallow crustal
structure. However, Segev et al. (2006) suggested that the recent
high topography of Lebanon and northern Israel reflects a
prominent high positive isostatic anomaly (see Fig. 3) caused
mainly by transpressional stresses along a right step (the
Yammouneh segment) of the sinistral Dead Sea Transform. In
general, the geological and geophysical evidence for the Levant
and the eastern Mediterranean clearly indicates an active Levant
margin since Late Eocene time. This activity was synchronous,
and perhaps related to, the Afar plume centred in Ethiopia and
Yemen (c. 2000 km south of the southern Levant region; White
& McKenzie 1989; Schilling et al. 1992; Ebinger et al. 1993;
Baker et al. 1996; Hofmann et al. 1997; Zeyen et al. 1997;
George et al. 1998), caused regional uplift from the Late Eocene
or Oligocene (Cloos 1954; Cox 1989; Collet et al. 2000; Pik et
al. 2003). This plume activity strongly affected the tectonic
regime of the Afro-Arabian plate and led to: (1) the Afro-
Arabian continental breakup and spreading in the Red Sea and
the Gulf of Aden; (2) the formation of the Dead Sea Transform
plate boundary; (3) the Tertiary–Recent northward convergent
phase between Africa–Sinai and Eurasia, as well as Arabia and
Eurasia. In the Israeli coastal region the uplift was c. 1000 m
(Segev, Lyakovsky & Schattner, in prep). Tertiary tectonics has
become localized along the Dead Sea Transform plate boundary
since Early Miocene time (Burdigalian, Garfunkel 1989; Garfun-
kel & Ben-Avraham 2001; Garfunkel & Beyth 2006), when it
Fig. 2. Schematic illustration of the tectonic
evolution of the Levant continental margins.
Legend is as for Figure 10. G,
Gondwanaland; P, Palmyrides; E,
Eratosthenes Block; T, Troodos ophiolite;
M, Mamonia complex; CY, Cyprus; H,
Hatay ophiolite; BB, Baer-Basit ophiolite;
N, Niklas ophiolite; KD, Kurd Dag
ophiolite; KA, Kyrenia Arc; EA,
Eratosthenes Arc; SMB, Syrian Arc mobile
belt; ASG, Azraq–Sirhan graben; EG,
Euphrates graben; S, Sinjar Trough; AG,
Anah graben; LB, Levant basin; HB,
Herodotus basin; PB, Phoenician basin; GS,
Gulf of Suez; GE, Gulf of Elat; DST, Dead
Sea Transform.
CENTRAL AND SOUTHERN LEVANT CONTINENTAL MARGIN 733
connected with the Levant margin in northern Israel. It is also
important to note the effect of a c. 4 km load of the Nile
sedimentary cone during the Pliocene calculated by Segev et al.
(2006) in the southeastern Mediterranean. Accommodation of
this within the Levant basin caused concentric oscillatory nega-
tive and positive anomalies, up to c. 400 m high, surrounding the
Nile sedimentary cone (Segev et al. 2006, fig. 6).
Tertiary–Recent tectonism has changed the shape of the
Levant upper crust. Furthermore, the original Jurassic configura-
tion could not have survived the intensive tectonic and magmatic
processes occurring during Cretaceous time (which had a time
span of c. 100 Ma), including the Senonian–Maastrichtian con-
vergence (Guiraud & Bosworth 1997; Bosworth et al. 1999;
Robertson 2000, 2002), which could have changed the Levant
crustal arrangement.
The prominent structural element of the central Levant region
in the subsurface is the very steep inclination of the Moho
boundary from about �32 km deep east of the Sea of Galilee to
about �25 km offshore Haifa, a difference of �7 km over a
distance of 50 km (Fig. 3).
Geophysical evidence
Previous magnetic and Bouguer gravity anomaly maps of the
eastern Mediterranean have been published by, among others,
Ben-Avraham & Ginzburg (1986, 1990), Makris & Wang (1994),
Makris et al. (1994; reduced-to-pole), Rybakov et al. (1997) and
Gardosh et al. (2008). The Bouguer gravity map depicted as
background in Figure 4 was prepared in the present study. Both
magnetic and gravity fields show significant differences between
the Herodotus and the Levant basins south of the Cenozoic
Hellenic and Cyprus subduction trenches. The significant lower
positive Bouguer gravity anomalies of the Levant basin cannot
be explained by a thicker section of the Pliocene Nile sedimen-
tary cone, as suggested by Makris & Wang (1994), because it
covers only a limited region extending mainly over the SE
Herodotus basin (Fig. 4). Nevertheless, the Levant basin accom-
modates huge amounts of dominantly Oligocene and later clastic
sediments that accumulated as a result of Afar dome erosion.
The differences between the Levant and the Herodotus basins
are even more significant on the magnetic map (Fig. 5). The
Levant basin has been interpreted by Makris et al. (1994) as
comprising oceanic crust with reverse magnetization that is older
than the normally magnetized ophiolites of Cretaceous age that
are sampled in Cyprus. The lack of linear oceanic-type magnetic
anomalies in this region has been explained by Ben-Avraham &
Ginzburg (1986) by: (1) a period with no polarity reversals of
the magnetic field; (2) destruction of the magnetic anomalies by
later compressional deformation; (3) no short-wavelength mag-
netic anomalies being observable at the surface because the
depth to the crystalline crust is over 14 km.
The eastern Levant basin is typified by values of �100 to
�250 nT; however, the oceanic crust of the western Levant basin
and westward of it acquired mainly normal magnetization (�50
to +250 nT), and a sharp transitional zone separates these two
regions. Furthermore, Ben-Avraham et al. (2002) suggested a
Fig. 3. Contour lines of depth to the Moho
(white lines), which represent the present
deep crustal structure of the Levant region,
overlaid on a residual elevation image
(black contours) calculated by flexural
(Vening Meinesz) isostasy related to the
Pliocene–Recent sedimentary loading and
unloading (from Segev et al. 2006). The
very high (up to 2500 m) positive isostatic
anomaly in Lebanon and northern Israel,
where the Moho contour lines cross the
Mediterranean coastline obliquely, should
be noted.
A. SEGEV & M. RYBAKOV734
different geomagnetic field inclination for the Israeli continental
crust, the Levant basin crust and the Eratosthenes microconti-
nent, indicating possible different genesis for these crusts.
The reverse magnetization of large parts of the eastern Levant
basin (Fig. 5) probably indicates their formation prior to the
Cretaceous Normal Polarity Superchron, which lasted between
Barremian (c. 127 Ma) and Santonian time (84 Ma; Gradstein et
al. 2004). The normally magnetized western Levant and the
Herodotus basins were probably formed during this superchron.
To shed light on this issue, we can take two examples of
subsurface magmatic causative bodies from Israel, as follows.
(1) The Late Triassic–Early Jurassic Saharonim basic intrusion
Fig. 4. Location of the main structural elements of the Middle East (see Fig. 1) on a Bouguer gravity anomaly map of the eastern Mediterranean. The
pink contour lines represent the isopach of the Nile sedimentary cone (Segev et al. 2006).
CENTRAL AND SOUTHERN LEVANT CONTINENTAL MARGIN 735
Fig. 5. Location of the main structural elements of the Middle East (see Fig. 1) on a pole- reduced total intensity magnetic map (modified by Rybakov,
after Makris et al. 1994; Rybakov et al. 1997; Gardosh et al. 2008) (for legend see Fig. 1).
A. SEGEV & M. RYBAKOV736
in the eastern Makhtesh Ramon yielded a negligible magnetic
anomaly and a high gravity anomaly. This body is located next
to the Early Cretaceous (116–108 Ma) Arod intrusion and is
associated with volcanic bodies in the western Makhtesh Ramon
that yielded both high magnetic and high gravity anomalies
(Segev et al. 1996). Moreover, Gvirtzman & Weinberger (1994)
found that some of these volcanic rocks have remanent magneti-
zation 6–15 times stronger than the induced magnetization.
(2) The c. 2 km thick Late Triassic–Early Jurassic Asher
Volcanics (Atlit-1 borehole), west of Mt. Carmel, yielded a
negligible aeromagnetic anomaly, in contrast to the Carmel high
positive magnetic anomalies that probably belong to the younger
Cretaceous magmatism (Rybakov 2008). The absence of a
magnetic high above the Asher Volcanics was explained by
Rybakov (2008) by a sequence of tuff layers magnetized in
various directions.
High positive magnetic anomalies up to 400 nT are spread
over the Levant continental and oceanic crusts. In Israel these
prominent anomalies were interpreted as representing mainly
subsurface basic igneous and volcanic bodies of various origins
(Ben-Avraham & Hall 1977; Recanati et al. 1989; Gvirtzman et
al. 1990; Kohn et al. 1993; Rybakov et al. 2000; Segev 2000,
2002; Segev & Eshet 2003). The first Phanerozoic magmatism in
Israel predominantly includes the Hebron magnetic anomaly
(Fig. 5, below Jerusalem), interpreted by Rybakov et al. (1995)
as a large basic volcano. The 200 m thick (Helez deep borehole)
Gevim quartz porphyry probably represents this volcanic phase,
which was radiometrically dated to be of Permian age (275 �47 Ma; Segev & Eshet 2003). The main Late Triassic–Early
Jurassic Asher magmatism and the Early Cretaceous Tayasir and
younger magmatic events were identified around Mt. Carmel and
in northern Israeli regions, and probably below the Palmyra fold
belt and in NW Jordan (Segev 2009).
Over the Herodotus basin crust the most prominent high
magnetic anomalies belong to the complex of the Eratosthenes
Seamount, which was previously interpreted by Makris & Wang
(1994) and Makris et al. (1994) as consisting of continental
crust. Recently, Rybakov et al. (2005, 2009) identified two
subsurface causative bodies by magnetic and gravity modelling:
(1) Eratosthenes, a 160 km 3 100 km, SW–NE-trending, high-
magnetic (500 nT) and low-gravity (25 mGal) body, interpreted
as a volcanic source; (2) Niklas, a 75 km 3 35 km, SW–NE-
trending, high-magnetic (200 nT) and high-gravity (100 mGal)
body, interpreted to be ophiolitic, although it could also be
interpreted as a dense mafic body. Rybakov et al. (2009) consid-
ered several previous models for the formation of the Era-
tosthenes and Niklas bodies (e.g. Woodside 1977; Ben-Avraham
1989; Robertson 1990; Krasheninnikov et al. 1994; Garfunkel
1998; Kempler 1998). He suggested that the Niklas body could
belong to a remnant of the large northeastern Mediterranean
ophiolite allochthon. According to Rybakov et al. the Troodos
ophiolite and Niklas bodies were probably connected during Late
Cretaceous obduction. Extending the Late Cretaceous ophiolite
allochthons toward the present-day central Levant basin, south of
the Cyprus Arc, raises the necessity of defining the subduction
and obduction zones of the Late Cretaceous.
Intensive geophysical surveys (seismic reflection and potential
fields) in the Levant basin and margin were carried out recently.
Gardosh et al. (2008) reported an extensive graben and horst
system extending throughout the Levant basin. This system was
later subjected to inversion and the formation of extensive,
Syrian Arc-type contractional structures throughout the Levant
basin and especially at the continental margin. Gardosh et al.
modelled several highly magnetized bodies, which were sug-
gested to correspond to extrusive volcanic rocks at relatively
shallow depth within the sedimentary succession. Several small
bodies in the northwestern part of the Levant basin correspond to
the Eratosthenes high. The origin of the elongated, NE–SW-
oriented anomaly in the central part of the basin, at the top of
the Jonah Ridge (horst), was interpreted by Folkman & Ben-Gai
(2004) as magmatism that occurred concurrently with the Syrian
Arc tectonism in Israel. Gardosh et al. (2008) related the Jonah
Ridge magmatism to Late Cretaceous and Tertiary eruptive
episodes.
The reconstructed Middle–Late Eocene crustal structure
Throughout the Jurassic and Cretaceous periods the Arabian
plate had a platform character for which a passive nature was
suggested (Bein & Gvirtzman 1977; Garfunkel & Derin 1984;
Garfunkel 1998; Fig. 6). During these periods, shallow marine
carbonate facies accumulated on the Arabian platform bounded
to the west by a hinge belt roughly coinciding with the present
Mediterranean coastline. A thick prism of deep-water continental
slope deposits accumulated west of the hinge belt (Bein & Weiler
1976; Bein & Gvirtzman 1977; Ginzburg & Gvirtzman 1979;
Walley 1998). The Afro-Arabian plate became ramp-like (Fig. 6;
Ahr 1973; Sass & Bein 1982; Buchbinder et al. 1988) only since
the Late Maastrichtian and mainly during Eocene time.
The 3D layered structure of three interfaces: (1) calculated
elevation, (2) top of the basement, and (3) the Moho interface of
a limited region of the central Levant pre-Tertiary tectonism
(pre-Dead Sea Transform) has been recently established by Segev
et al. (2010) and two of them (calculated elevation and the Moho
interface) are depicted in Figure 7. Segev et al. first restored a
lateral offset of 100 km along the Dead Sea Transform. Then
they calculated the expected elevation for a local isostatically
balanced model that considers: (1) a stable, cold and isostatically
compensated crust during Middle Eocene time with no magmatic
activity during this period; (2) insignificant change in the total
thickness of the crystalline crust since the Cretaceous. This
numerical procedure resulted in the vertically restored interface
of the top of the Avedat Group, which is considered to represent
the elevation at Middle Eocene time, as well as the restored
interfaces for the top of the crystalline basement and the Moho
boundary during the same period (Fig. 7).
The computed Middle–Late Eocene elevation matches the
SW–NE strike of the Moho and both interfaces define a ramp-
shaped structure with a significant structural high east of Mt.
Hermon (Fig. 7), similar to the geological observations of Sneh
(1988). The common inclination of this Middle–Late Eocene
elevation was between c. 28 (shelf) and c. 68 (slope), and during
the maximal transgression most parts of central Israel were
covered by c. 200 m (Jerusalem region) to c. 1800 m (Haifa
region) of seawater, according to a datum near the Dead Sea in
the elevation map of Figure 7.
Tectonics of the central and southern Levantcontinental margin
Vertical motions resulting from mantle plume activity;lithostratigraphy, morphotectonics and thermal history
When the Levant continental margin became close to isostatic
compensation it formed a ramp-shaped plate that was moderately
inclined toward the NW. This margin experienced pelagic deposi-
tion and was covered by chalk and fine clastic rocks of the Early
CENTRAL AND SOUTHERN LEVANT CONTINENTAL MARGIN 737
Tertiary Taqiye, Adulam, Maresha and lower Bet Guvrin Forma-
tions (Flexer 1968; Sneh 1988; Buchbinder et al. 1988; Fig. 8).
The Mesozoic central Levant continental margin (Fig. 7),
which obliquely crosses central and northern Israel, allows an
examination of the lithostratigraphic transitions from continental
to oceanic crust along an onshore south–north cross-section. The
lithostratigraphic changes across Israel (Fig. 8) indicate a variety
of environments of deposition and provide evidence of tectono-
magmatic events and regional unconformities associated with
denudation events. The geological history of northern Israel can
therefore be used to determine the morphotectonic events of the
upper part of the Levant continental margin since its formation
during Jurassic time.
In most parts of Israel the upper Jurassic succession (down to
the Oxfordian in the north and Bathonian in the south) was
truncated before the deposition of either basalt flows related to
the Tayasir Volcanics or younger Early Cretaceous siliciclastic
rock units (Hirsch et al. 1998; Fig. 8). The Lower Cretaceous
alternating sequence of siliciclastic and carbonate rocks forms a
belt along the northern margins of the Arabo-Nubian Shield.
The stratigraphic correlations suggest two principal regional
denudation events during the Cretaceous period (Segev et al.
2005; Segev 2009): (1) at the time of the pre-Tayasir Volcanics,
when the Upper Jurassic sequence was truncated; (2) in pre-
Aptian time, when most of the Berriasian–Barremian section,
including the Tayasir Volcanics, was eroded (see also Garfunkel
1989, 1998; in central Africa Guiraud et al. 2005 called this the
‘Austrian’ unconformity). These two regional Early Cretaceous
truncation episodes indicate the existence of a regional dome
structure (Fig. 6) that is probably centred close to northern Israel,
Lebanon and Syria, where it meets the Levant continental
margin. Coexisting regional unconformities were reported from
the African continent (Guiraud et al. 2005, and references
therein) in the framework of similar tectonic events (Levant–
Nubia plume, Segev 2002).
The geological record of the Berriasian–Barremian period
(Tayasir Volcanics and Helez Fm.) is preserved mainly in
coexisting grabens that survived the Late Barremian regional
truncation episode. The subaerial Tayasir volcanism and the later
Helez Formation siliciclastic deposits of central and northern
Israel represent a continental to shallow marine environment with
a strong influence from the nearby land (Blake 1936; Karcz
1965; Estes et al. 1978; Rosenfeld & Raab 1984; Rosenfeld et
al. 1995). At those times lagoons, swamps and dense vegetation
characterized the coastal region of Israel (Conway 1991; Nissen-
baum & Horowitz 1992). Moreover, sandstone intercalations up
to 15–20 m thick were encountered in the Yam-2, Yam West-1
and Yam West-2 wells offshore Israel. They are referred to as
‘Lower Sand’ of Hauterivian age and ‘Upper Sand’ of Barremian
age (Isramco Internal Report), and Gardosh et al. (2008)
interpreted these offshore sand beds, suggesting that the basin
floor should have been located westward of the offshore Yam
wells. Rosenfeld et al. (1998) and Rosenfeld & Hirsch (2005),
who used ostracode data, suggested that the mixed shallow
marine and continental Early Cretaceous environments also
typified the Israel offshore. This evidence demonstrates intensive
igneous and contemporaneous tectonic activity at the Levant
continental margin that uplifted it high above its isostatic
compensation state (c. �2000 m, in Fig. 7). It is reasonable to
assume even subaerial conditions for some parts of the Levant
basin during these Early Cretaceous uplift episodes.
Alkaline magmatism associated with sandstone of the same
age (140.7 � 0.4 Ma) as the Tayasir Volcanics has been reported
from the Mamonia Complex, SW Cyprus, by Chan et al. (2008).
Those workers suggested a possible expansion of the Levant
Early Cretaceous magmatism associated with alternating shallow
marine and subaerial environments far toward the NW.
The Aptian–Albian time interval was typified by cyclical
oscillations of continental clastic rock units (Amir, Avrona,
Malhata and Samar Formations) and shallow marine tongues
(Zuweira, Deragot and Uza Formations; see Fig. 8), becoming
mostly carbonates and marl of shallow marine environments
toward the NW to open marine deposits in the coastal plain and
offshore Israel. During this period, as in the Jurassic period, the
Arabian plate was a platform (Fig. 6), where shallow marine
carbonate facies accumulated as far as a hinge belt and deep-
Fig. 6. Schematic section across the Levant
continental margin (for location see A–A’
in Fig. 7). The crystalline crust (grey)
between the continuous brown lines
represents isostatically compensated crust
having ramp-shape elevation. The dashed
green lines delineating platform-shape crust
were estimated assuming similar crustal
thicknesses along its uplift by presumable
mantle upwelling. The dotted red lines
outline dome-shape crust typifying the
Early Cretaceous uplifts.
A. SEGEV & M. RYBAKOV738
water, continental slope deposits accumulated offshore from this
hinge belt (Bein & Gvirtzman 1977; Ginzburg & Gvirtzman
1979; Walley 1998).
During the Cenomanian, part of the study area was stable. The
Mount Carmel region, as well as sites in Lebanon, which were
located above the continental margin, were volcanically active,
and four phases of cyclical eruptions and local erosion episodes
have been identified (Ferry et al. 2007; Segev 2009; Segev &
Sass 2009).
Regional emergence of Israel during the Middle to Late
Turonian reflects an episode of subaerial exposure that produced
sandstone, conglomerate and karst (Weiler & Sass 1972;
Buchbinder et al. 1983; Kafri & Sandler 1992). Even more
extensive erosion occurred in the coastal mountains in Syria at
the same time (Filak et al. 2001).
After the Middle to Late Turonian short uplift episode,
regional subsidence caused deepening of the shallow marine
setting to an open marine and to a pelagic setting. This setting
characterized most of the Senonian to about Middle–Late
Eocene time (c. 40 Ma). This period is typified by the deposition
Fig. 7. Reconstructed Moho interface prior
to Tertiary deformation (red contour lines;
kilometres below mean sea level)
considered to represent the deep crustal
structure during Cretaceous time with the
calculated coexisting elevation (pink
contour lines; metres below mean sea
level). The vertical reconstruction is from
Segev, Lyakhovsky & Schattner (in prep),
who considered an isostatically
compensated crust during Middle–Late
Eocene time and insignificant changes in
the total thickness of the crystalline crust
since then. Both interfaces form a ramp-
shape plate margin (see Fig. 6). The
extension of Cretaceous magmatism over
the central and southern Levant continental
margin and the assumed location of the
Cretaceous Levant–Nubia plume (after
Segev et al. 2005) should be noted.
CENTRAL AND SOUTHERN LEVANT CONTINENTAL MARGIN 739
Fig. 8. Stratigraphic table of Israel since the Early Permian period depicting the lithology of the continental and offshore parts of Israel with the
radiometric ages of the magmatic events, the main tectonic and thermal events and the suggested state of the Levant continental margin.
A. SEGEV & M. RYBAKOV740
of chalk, marl, shale and chert, which are included in the Mount
Scopus and Avedat groups, with a common thickness in Israel of
c. 750 m (Segev, Lyakhovsky & Schattner, in prep).
Analysis of the subsidence history of the Levant region, as
well as studies of its thermal history, can be used as independent
tools for identifying vertical movements. Seven representative
columnar sections from southern Israel (Fig. 7) were used by
Gvirtzman (2003) to generate subsidence curves (Fig. 9). These
curves demonstrate three periods of rapid subsidence: (1) Middle
Triassic; (2) Middle Jurassic; (3) Cenomanian–Senonian. The
first event was associated with extensional faulting (Garfunkel
1989) during the formation of the Palmyra–Galilee graben. The
second represents extensional faulting during the formation of
the Levant volcanic continental margin, and the third represents
thermal subsidence after the Cretaceous tectonomagmatic activ-
ity (Segev 2009).
K-feldspar 40Ar/39Ar, zircon fission-track (ZFT), apatite fis-
sion-track (AFT) and apatite (U–Th)/He thermochronology were
conducted by Vermeesch et al. (2009) on detritus from Middle
Cambrian sandstones of the Shehoret Formation, southern Israel.
Their Phanerozoic thermal history identifies distinct thermal
events at c. 300 km south of the Levant margin, as follows.
Detrital ZFT ages are clustered around 380 Ma, consistent with
previous ZFT results (Kohn et al. 1993) and sediments of the
region (Segev et al. 1995), revealing that the Cambrian platform
sequence experienced a Middle Devonian thermal event and low-
grade metamorphism. All these studies suggested that the ob-
served Devonian ages represent a regional tectonothermal event.
Sixty single-grain detrital AFT ages are grouped at c. 270 Ma
with significant dispersion. This age fits well with the Early
Permian Gevim quartz porphyry (275 � 47 Ma; Segev & Eshet
2003) that overlies the crystalline basement of Central Israel,
which was totally exhumed at that time.
Inverse modelling of the AFT data suggests an episodic
burial–erosion history during the Mesozoic caused by low-
amplitude vertical motions. Seven detrital apatite (U–Th)/He
ages scatter between 33 and 77 Ma, whereas the c. 70 Ma age is
more likely to be accurate. This Campanian age marks the end
of the Cretaceous tectonomagmatic activity, whereas the Palaeo-
gene age marks the beginning of the Afar plume activity.
The first convergence phase between the Afro-Arabian andthe Mesotethys plates
The central and southern Levant region was submerged during
the Late Turonian–Early Santonian, when major regional com-
pressional tectonics initiated and resulted in the first stage of the
Syrian Arc deformation belt (Krenkel 1924; Bartov et al. 1980;
Honigstein et al. 1988; Guiraud & Bosworth 1997; Walley 1998;
Bosworth et al. 1999; Figs 1, 4 and 10). This belt consists of
NE–SW-trending asymmetric synclines and monoclines that
overlie deep-seated reverse faults (De Sitter 1962; Freund 1965;
Mimran 1976; Reches et al. 1981). Bosworth et al. (1999)
suggested the existence of Late Santonian (c. 84 Ma) far-field
compressional stress in central Egypt (Figs 4 and 10). The Syrian
Arc fold system demonstrates the formation of a tectonic mobile
belt above and along the central Levant continental margin
contemporaneously with the beginning of its subsidence. The
NW–SE contraction, which formed large folds with emergent
crests (Bartov et al. 1980; Cohen et al. 1990), slowed the speed
of the Levant northwestward drowning.
Contemporaneously with the NE–SW-trending folding and
deep-seated fault inversion, an east–west-trending Negev–
Central Sinai shear zone was activated (Bartov et al. 1980) with
a possible dextral motion. Bosworth et al. (1999) reported a
broad east–west-trending zone of dextral transpression, mostly as
inverted half-grabens, en echelon anticlines and strike-slip faults
crossing northern Egypt. The best documented strike-slip fault of
this system is the east–west Ragabet el-Naam (near Suez)–
Themed–Wadi Dana (Jordan) Fault (Fig. 1).
During the Campanian–Maastrichtian period the northern
Levant margin underwent intra-oceanic convergence (subduction,
obduction and collision) between the Tauride plate (Eurasia), or
Tethyan plate, and the NW Arabian plate (reviewed by Robertson
2000, 2002; Kazmin 2002). This convergence formed the major
structures of the northwestern Arabian plate, such as the SW–
NE Late Cretaceous thrust front in southern Turkey and the
Palmyra fold belt of the same direction (Salel & Seguret 1994).
During the same convergence the exposed Baer-Basit, Hatay,
Kurd Dagh and Amanos ophiolites (among others) were ob-
ducted onto the northwestern Arabian continental margin (e.g.
Al-Riyami et al. 2000; Al-Riyami & Robertson 2002) and the
Troodos ophiolite (e.g. Robertson 2000, 2002) was obducted over
the Cyprus microcontinent (Makris & Wang 1994; Makris et al.
1994).
The tectonic map of the continental parts of the Levant clearly
shows the consequences of the SE to NW convergence of the
northwestern Arabian plate with the Tethyan oceanic crust.
Although the thrust belts, fold belts and ophiolites are evidently
located in the northern Levant region, the geological and
geophysical observations in the central and southern Levant
region show the southwestward continuation of the Syrian Arc
mobile belt from the Palmyrides to Israel, Sinai (e.g. De Sitter
1962; Freund 1965; Mimran 1976; Reches et al. 1981) and its
further continuation in Egypt (Guiraud & Bosworth 1997; Bos-
worth et al. 1999). Bosworth et al. (1999) reported that this
compression event affects the entire African plate, in which pre-
Senonian sedimentary basins, mostly ENE–WSW-trending, were
folded and inverted, some of them along the Mesotethyan margin
from Morocco to Egypt. Bosworth et al. also described a
Fig. 9. Subsidence curves of seven composite columnar sections
(modified after Gvirtzman 2003, location shown in Fig. 7). The three
periods of rapid subsidence should be noted: (1) Middle Triassic;
(2) Middle Jurassic; (3) Aptian–Turonian (Cretaceous).
CENTRAL AND SOUTHERN LEVANT CONTINENTAL MARGIN 741
Campanian to Maastrichtian or Palaeocene extensive phase of
rifting in central and north Africa and northern Arabia (see
below).
Evidence from the continental regions makes re-examination
of the deeply buried tectonic setting of the eastern Mediterranean
by using geophysical data an interesting prospect. However, the
recent structural architecture of the Middle East (Fig. 1) is highly
modified by the later Cenozoic subduction along the Cyprus and
the Hellenic arcs, as well as the sinistral motion along the Dead
Sea Transform. These processes consumed important parts of the
eastern Mediterranean, thus making the present interpretation
much more difficult.
Synchronously with the above-mentioned convergence, two
parallel well-known graben systems, trending normal to the
Syrian mobile belt, developed on the northwestern Arabian plate
(Fig. 1): (1) the Euphrates graben in Syria and Iraq (EG in Fig.
2); (2) the Azraq–Sirhan graben (ASG in Fig. 2) in Saudi
Arabia, Jordan and northwestward toward Galilee, northern
Israel. This structure is bordered on the south by the Carmel
fault system with contemporaneous tectonic basins (grabens?) in
the north Samaria region (Rosenthal et al. 2000).
Although many researchers (e.g. Al-Riyami et al. 2000;
Robertson 2000, 2002; Al-Riyami & Robertson 2002; Robertson
et al. 2009) reported and discussed the Late Cretaceous subduc-
tion and obduction over the northern Levant region, most of
them did not consider the southwestward continuation of this
subduction complex. The Syrian Arc mobile belt over the central
and southern Levant margin represents the southwestward con-
Fig. 10. Three principal palaeotectonic alternatives for the Senonian–Late Maastrichtian. Abbreviations are as in the caption to Figure 2.
A. SEGEV & M. RYBAKOV742
tinuation of the convergent regime to Egypt (Bosworth et al.
1999). As this convergence represents the relative motion of the
Afro-Arabia and the Mesotethys plates, it is necessary to under-
stand the entire plate architecture of the eastern Mediterranean.
The significant differences between the northern (north of the
Carmel fault) and central–southern Levant tectonism during the
Late Cretaceous, as well as geological and geophysical evidence
from these regions, allow three alternative explanations (Fig. 10),
as follows.
(1) There was convergence in the northern Levant (Fig. 10a) at
the Kyrenia Arc only, and perhaps additional arcs, separated from
the central and southern Levant by strike-slip motion.
(2) There was convergence in both the northern and central–
southern Levant (Fig. 10b) with two arcs (Kyrenia and, herein
suggested, Eratosthenes) subducting in a similar NW direction as
suggested for the northern Levant, but separated by a different
rate of strike-slip motion (Kazmin (2002) suggested a similar
palaeotectonic scheme).
(3) There was convergence in both the northern and the
central–southern Levant (Fig. 10c) with two arcs (Kyrenia and
Eratosthenes) subducting in opposite directions, separated by a
strike-slip fault system. This configuration of the Eratosthenes
Arc requires additional strike-slip plate boundaries between
Africa and the Mesotethys, as well as between Africa and Sinai
(see also Rybakov et al. 1996). Accordingly, the Levant basin
was a short-lived abandoned back-arc basin.
The present Herodotus basin is deeper than the Levant basin
by c. 1000 m. Thus, at the end of the Turonian before deposition
of several thousands of metres of sediment in the Levant basin
and before the cooling of the Levant crust, it is more likely that
the Levant basin was higher and hotter than the Herodotus basin.
The simple observation of Doglioni et al. (1999) indicates that of
two plates the denser one subducts. This observation supports the
third alternative. Other supporting factors are as follows.
(1) A sharp magnetic transitional zone exists between the
Levant and the Herodotus oceanic crusts.
(2) Onland pre-Miocene fault systems occur between the Sinai
and the African plates along the present Suez fault system, which
can be seen by different magnetic patterns (Fig. 5). Similarly, a
c. 80 km southward reconstruction of the Sinai plate has been
suggested by Rybakov et al. (1996), who matched the east–west
magnetic anomalies on both sides of the Suez fault system.
Furthermore, the faults parallel to and above the African
continental margin (Figs 1, 4 and 5) were between Africa and the
Mesotethys crusts.
(3) Senonian volcanism occurred within the Levant basin
(Jonah Ridge; Figs 1, 4 and 5), which is located above the
suggested eastward subducting plate and on Mt. Carmel (Bat
Shelomo Volcanics) close to the Carmel fault system.
Period of tectonic quiescence associated with thermalsubsidence
During the Late Maastrichtian the Baer-Basit and Hatay ophio-
lites, located in the most active part of the northern Levant
region, were drowned and covered by marine calcareous sedi-
ments (Al-Riyami et al. 2000, 2002). Contemporaneously, the
Arabian plate was covered by mainly pelagic sediments. The
sedimentary sequence of the shallow marine Senonian restricted
basins, which are typified by cherts, chalk and phosphorites
(Reiss 1988; Soudry et al. 2006), was replaced by a deeper
Maastrichtian and Palaeocene shale, marl and chalk (all included
within the Mount Scopus Group, Fig. 8). These formations were
overlain mainly by the Early and Middle Eocene pelagic chalk of
the Avedat Group. The Syrian Arc folds were gradually covered
by the Avedat Group; however, the highest structures, such as the
Ramon anticline and the Golan Heights in northern Israel,
remained above sea level during most of this period.
Widespread intraformational Eocene to Early Oligocene con-
glomerates have been found in Sinai, the Eastern Desert of
Egypt, southern Jordan and southern Israel (Avni et al. 2007). In
places these conglomerates are overlain by and interfingered with
marine Eocene to Early Oligocene carbonate intercalations.
Generally, the deep marine Eocene sequences, including these
intraformational conglomerates, were preserved within down-
faulted blocks of Oligocene age having vertical movements up to
several hundred metres. These Eocene conglomerates indicate
tectonic activity synchronous with sedimentary instability. Avni
et al. (2007) suggested that the Eocene tectonics reactivated pre-
existing, east–west-, NW–SE- and north–south-trending fault
systems, representing an early stage of regional extensional
deformation. The Late Maastrichtian Palaeogene (c. 65–40 Ma)
lithostratigraphy, palaeogeography and tectonism suggest contin-
uous northwestward drowning, associated with fracturing, of the
study area as a result of thermal relaxation following the Early–
Middle Cretaceous plume activity.
Using this Palaeogene c. 25 Ma period of thermal relaxation
and tectonic quiescence, Segev et al. (2010) calculated the local
isostatic compensation of the crust in northern Israel and its
close vicinity. Their results suggest that the central and southern
Levant continental margin thermally subsided c. 2000 m offshore
Israel during this period (Fig. 7). It is therefore reasonable to
genetically connect the Early Tertiary normal faulting of the
central and southern Levant region to this thermal subsidence.
It is important to note that after the Jurassic establishment of
the Levant continental margin, the c. 25 Ma period between the
Late Maastrichtian (c. 65 Ma) and the Late Eocene (c. 40 Ma)
was a unique time of tectonomagmatic quiescence. Therefore
strictly speaking, only during this period was the Levant margin
passive (Segev et al. 2010).
Evolution of the Levant continental margin; discussion
The proposed scenario for the evolution of the Levant margin is
focused on the Cretaceous tectonomagmatic events (Table 1).
Initial setting and phase 1: Permian–Late Triassic (Fig. 2a)
The beginning of the Pangaea supercontinent dispersion led to
the opening of the Permo-Triassic Neotethys by northward
drifting of the Cimmeride microcontinent (Sengor et al. 1984;
Guiraud 1998; Stampfli 2000) and rifting towards the Levant
region (Ziegler 1990; Guiraud 1998; Segev 2002). The Palmyra
rift is one of the rifts (Brew et al. 1999) associated with regional
uplift and magmatism (Gevim Volcanics). This uplift caused
regional denudation of large areas in central and northern Israel
down to the crystalline basement. In these areas the sedimentary
succession begins with Permian rocks.
Phase 2: Late Triassic–Jurassic (the late stage asdescribed in Fig. 2b)
Deep erosion of Upper Triassic units and the absence of Lower
Jurassic rocks in the Levant, NE Africa and the Tauride block
indicate a major uplift and denudation of the Afro-Arabian
region (reviewed by Segev 2000, 2002) accompanied by alkaline
magmatism (Asher Volcanics). This Late Triassic–Early Jurassic
magmatism initiated at c. 207–205 Ma and continued in the
CENTRAL AND SOUTHERN LEVANT CONTINENTAL MARGIN 743
Early Jurassic during 191–189 Ma. The third Middle–Late
Jurassic magmatic event (Bhannes (Lebanon)–Devora (Israel)
Volcanics) took place during c. 160–170 Ma contemporaneously
with a large stratigraphic hiatus. The widespread Late Triassic–
Early Jurassic magmatism in the eastern Mediterranean and NE
Africa suggests that the main rift–drift event between the Afro-
Arabian plate and the Tauride block occurred mainly during the
Jurassic tectonomagmatic period. Throughout this period the
Mesotethys (or southern Neotethys, or present eastern Mediterra-
nean) began to open.
The predominantly reverse magnetization of large parts of the
eastern Levant basin (Fig. 5) is indicative of their pre-Barremian
(c. 127 Ma) formation, followed by the Cretaceous Normal
Polarity Superchron, which lasted until 84 Ma and which prob-
ably influenced the normal magnetized western Levant basin and
the Herodotus basin.
The original pre-Cenozoic orientation of the Levant margin
was east–west in the Egyptian part and SW–NE in Israel,
Lebanon and northeastward, as indicated by the reconstructed
Moho contour lines. This trend significantly differs from the
Miocene–Recent active transform margins. The thick (up to
.3000 m) Jurassic carbonate belt above the Levant margin
(Hirsch et al. 1998) indicates a platform profile of the NW
Arabian plate.
Phase 3: Early Cretaceous (Fig. 2c)
During the Berriasian–Barremian period the entire eastern
Mediterranean region was subjected to intensive updoming,
truncation and magmatism (the Tayasir Volcanics) with minor
and discontinued continental and shallow marine sedimentation.
Geological evidence strongly supports previous interpretations
that postulate a weak mantle plume (Levant–Nubian plume)
emplaced below the Levant continental margin (Garfunkel
1989; Stein & Hofmann 1992, 1994; Laws & Wilson 1997;
Wilson & Guiraud 1998; Segev 2000, 2002; Wilson et al. 2000;
Segev et al. 2005). Segev et al. (2005) centred the plume head
below northern Israel (Fig. 7). Igneous rocks are distributed
mainly over an area of c. 800 km 3 200 km in outcrops and in
the subsurface of Israel, Syria, Lebanon, Jordan, Sinai and the
Eastern Desert of Egypt, comprising various volcanic sequences
and small hypabyssal intrusions. Predictions based on the
mantle plume theory (Crough 1983; Cox 1989; White &
McKenzie 1989; Schubert et al. 2001), as well as geological
observations (Kent 1991; Sengor 2001), suggest that wide
regions, up to 2000 km, of the Earth’s lithosphere are uplifted
to the extent of 2000 m in response to a dynamic mantle
upwelling. According to Sengor (2001), there is no other
process on Earth that creates such domes of lithospheric flexure
within several million years. The sedimentary record of such
dome uplifts should be considerable, providing an independent
geologically based tool for observing plume activity, even if
much of the magmatic products has been removed (Rainbird &
Ernst 2001).
After Aptian time the Levant continental margin underwent
cyclical uplift and subsidence, whereas the Levant basin was
drowned and mainly covered by deep marine sediments. This
indicates that the Levant rifted margin was only partially cooled
and subsided during the Jurassic. In contrast, it was reactivated
during the c. 55 Ma duration of the Cretaceous plume activity.
The persistence of platform conditions until the Turonian, rather
than ramp-shape conditions (Fig. 6), is indicative of continuous
dynamic uplifting of the Levant margin during most of Cretac-
eous time.
Extensional tectonics and cyclical alkaline plume-related
magmatism typify the Berriasian–Cenomanian, although the
subsurface tectonic setting of these structures on both the
Arabian continental crust and the Levant oceanic crust is not yet
known. During this period the NW Arabian plate was subjected
to vertical changes from dome to platform shapes and vice versa
(Fig. 6). The continued opening of the Mesotethys during most
of Cretaceous time caused the formation of new oceanic crust
that predominantly acquired normal polarity, such as that of the
western Levant basin and the Herodotus basin.
Table 1. Summary of the Cretaceous tectonomagmatic events in the Levant region
Tectonomagmatic event, symboland name
Location Age (Ma) Sources
First, C.V.-1, Tayasir Volcanics Exposed: northern Israel: Mt. Hermon; Wadi El Malih, (Samaria).southern Israel: Makhtesh Ramon (Negev)
Berriasian–Hauterivian,141 � 1.6–133.5 � 1.5
1–11
Subsurface: Mt. Carmel; Samaria; GalileeMardin Plateau; Palmyrides of Syria; Euphrates graben, Iraq;Northeastern Desert, Egypt; Sirt, Libya; Mamonia Complex, SWCyprus
12–17
Second, C.V.-2, Shen Ramon–Gavnunim Exposed: southern Israel: Makhtesh Ramon, Har Arif (Negev) Basal Aptian 125–123 11, 18–22Subsurface: Mt. Carmel; northern IsraelCoastal Range, Jebel Ansariye, Syria; Wadi Al Karn, Lebanon 23–24
Third, C.V.-3, Ramon Volcanics Exposed: southern Israel: Makhtesh Ramon, Har Arif (Negev),Timna Valley; Arif en-Naqa, Sinai
Aptian–Albian 116.4 �3.4–108.8 � 1.2
25–30
Subsurface: Mt. Carmel, northern IsraelCoastal Range, Syria; Wadi Araba, Egypt 23, 39
Fourth, C.V.-4a, 4b, 4c, 4d, CarmelVolcanics
Northern Israel: Mt. Carmel; northern Lebanon; Coastal Range,Syria; Eastern Desert, Egypt
Cenomanian 99 � 1;98.2 � 1;
31–34, 11,
96.7 � 0.5; 95.4 � 0.5 23, 34–38Fifth, C.V.-5, Bat Shelomo Volcanics Northern Israel: Mt. Carmel Campanian 82 � 1 32, 34
1, Shimron & Lang 1989; 2, Shimron & Peltz 1993; 3, Mimran 1972; 4, Lang & Mimran 1985; 5, Garfunkel 1989; 6, Baer 1989; 7, Rophe et al. 1989; 8, Teutsch et al. 1996;9, Bonen 1980; 10, Katz & Eppelbaum 1999; 11, Segev 2000, 2009; 12, Wilson & Guiraud 1998; 13, Meneisy 1990; 14, Cahen et al. 1984; 15, Massa 1988; 16, Rossi et al.1992; 17, Chan et al. 2008; 18, Itamar & Steinitz 1988; 19, Lang et al. 1988; 20, Lang & Steinitz 1994; 21, Segev 2000; 22, Derin 1981; 23, Mouty et al. 1992; 24, Sharkov et
al. 1989; 25, Eyal 1996; 26, Segev et al. 2005; 27, Zemel et al. 1956; 28, Zak 1964; 29, Weissbrod et al. 1990; 30, Weissbrod & Segev 2003; 31, Picard & Kashai 1958;32, Sass 1980; 33, Sass & Bein 1982; 34, Segev et al. 2002; 35, Mouty & Saint-Marc 1982; 36, Meneisy & Kreuzer 1974; 37, Serencsits et al. 1981; 38, Ferry et al. 2007;39, Filak et al. 2001.
A. SEGEV & M. RYBAKOV744
Phase 4: Late Cretaceous (Fig. 2d)
Major regional convergence initiated during Late Turonian time,
when the first stage of the Syrian Arc deformation belt developed
at the central and southern Levant margin that had synchronously
begun to drown (Bartov et al. 1980; Honigstein et al. 1988). The
most intense convergence occurred between the Campanian and
Late Maastrichtian, when there was intra-oceanic subduction and
obduction at the northern Levant margin, as a result of collision
between the Mesotethys plate and the NW Arabian plate.
This SE–NW-trending collision resulted in the obduction of
ophiolites in the northern Levant margin and southern Turkey
and along a parallel westward trend in southern Turkey (Robert-
son 2000, 2002). Within the northeastern Mediterranean region
the Troodos ophiolite in Cyprus and perhaps the Niklas ophiolite
west of the Eratosthenes Seamount were related to the same
events (Rybakov et al. 2009). The Late Cretaceous plate-tectonic
regime reveals the convergence between the African–Arabian
plate from the SE and the Mesotethys and the Tauride plates
from the NW. The geological and geophysical evidence suggests
the existence of a convergent (subduction) plate boundary in the
present-day southeastern Mediterranean, called the Eratosthenes
Arc. It is also suggested that the available information points to
the possibility that the western Herodotus oceanic plate had
subducted southeastward, and thus the Levant basin was a short-
lived, abandoned back-arc basin.
Phase 5: Late Maastrichtian to Middle–Late Eocene(Fig. 2e)
After c. 15 Ma of Late Cretaceous convergence and before the
newly formed Cenozoic plate-tectonic regime, the entire Middle
East region experienced tectonomagmatic quiescence, a period
that lasted c. 25 Ma. Because the Cenozoic tectonism was most
probably genetically influenced by the Afar plume activity, it is
reasonable to search there for reasons why the short-lived Late
Cretaceous convergence terminated. However, during phase 5 the
Levant margin cooled and subsided until the NW Arabian plate
became a moderately inclined ramp. This tectonic quiescence
and thermal relaxation of the Levant continental margin reveal
the unique episode of its isostatic compensation.
Final setting, phase 6: Late Eocene–Recent (Fig. 2f)
The updoming of NE Africa and Arabia since the Late Eocene
terminated the previous tectonic quiescence and caused the
regression of the Mesotethys Ocean from the Afro-Arabian
continental margin. This uplift is probably related to the
dynamics of the Afar mantle plume, which resulted in rifting and
breakup between the African, Sinai and the Arabian plates. The
resulting Neogene rift–rift at the Gulf of Aden and the Red Sea
as well as the continuous opening of the southern Atlantic Ocean
caused the formation of a new plate-tectonic regime with a new
convergent pattern between the African and the Arabian plates
from the south and the Eurasian plate from the north. As part of
the new tectonic regime, the Dead Sea Transform plate boundary
connected with the Levant continental margin during the Early
Miocene (Burdigalian, Garfunkel 1989; Garfunkel & Ben-Avra-
ham 2001; Garfunkel & Beyth 2006) and then uplifted Lebanon
and northern Israel to c. 2500 m above their level of compensa-
tion. Moreover, since the Oligocene the area studied was
subjected to intensive flood volcanism over large regions. During
this tectonic period the Levant margin was reactivated, making it
an active transform margin (Dead Sea Transform).
Summary
This study focuses on the central and southern Levant continental
margin and synthesizes the relevant information from adjacent
continental and marine regions. A variety of geological evidence
relating to the shallow crust of the study area, and gravity and
magnetic anomaly maps of the eastern Mediterranean allow (1)
characterization and division of the eastern Mediterranean into
various regions, (2) better location of the basic Phanerozoic
igneous bodies, and (3) the suggestion of a new concept for the
Late Cretaceous convergence event. These, together with the
newly restored 3D crustal structure of the central Levant (after
Segev et al. 2010) clarify the Late Maastrichtian–Late Eocene
tectonic quiescence period and help in understanding the geo-
dynamic processes involved.
The geological record of the Levant region reveals the
complex effects of major tectomagmatic events that mainly
caused intensive vertical motion, deep truncation, rifting, inten-
sive magmatism, breakup and formation of new oceanic crusts.
However, it also exposed convergent episodes that led to
subduction, obduction, collision, thrusting, folding and strike-slip
motions. All these events significantly affect the region where
the Levant continental margin formed and developed. The
following summary traces the evolutionary geological scenario
of the formation and development of the Levant continental
margin through time.
(1) The Permo-Triassic breakup of the Pangaea supercontinent
led to the opening of the Neotethys north of the Tauride block
and to intensive rifting toward the northern part of the Gondwana
supercontinent, including the Levant region.
(2) The Late Triassic–Jurassic tectomagmatic event reveals the
breakup of the Tauride and other blocks from northern Gondwana
and the formation of the Levant rifted volcanic margin in the
southeastern part of the newly formed Mesotethys Ocean.
(3) The onland subsurface magmatic and volcanic rocks of the
Jurassic were found to have negligible magnetic anomalies
similar to the very low and mostly reverse magnetization of large
oceanic parts of the eastern Levant basin.
(4) The strike of the Levant margin was SW–NE in the
northwestern Arabian part and east–west in the northern African
part. The approximately south–north outline of the Levant coast-
line during part of the Cretaceous and at present is due to
tectonic activity and/or thermal uplifts.
(5) A Cretaceous mantle plume controlled the tectonomag-
matic tensional regime up to Late Turonian time. It is interpreted
as the cause for the Mesotethys oceanic crust change from
average negative magnetization of the eastern Levant basin to an
average positive magnetization westward.
(6) The Senonian–Maastrichtian (c. 15 Ma) convergence as a
result of the Kyrenia Arc is evident from the ophiolites and the
thrust zone in the northern Levant region. The continuation of
the Syrian Arc fold belt from the Palmyrides to Israel, Sinai and
Egypt therefore suggests the existence of another arc (Era-
tosthenes) in the central and southern Levant region. Accord-
ingly, the Levant basin was a short-lived abandoned back-arc
basin that accumulated a relatively thick sedimentary succession.
(7) A distinct tectonomagmatic quiescent period in the Middle
East, between Late Maastrichtian and Late Eocene time (c.
25 Ma), allowed the Afro-Arabian plate to thermally subside
until it approached its isostatic compensation and became a
moderately inclined ramp.
The authors wish to thank E. Sass for his collaboration on the geological
studies in the Mt. Carmel region and his productive discussions. The
CENTRAL AND SOUTHERN LEVANT CONTINENTAL MARGIN 745
paper benefited greatly from reviews by V. Lyakhovsky, S. Folkman and
J. Steinberg. Thanks are also due to T. Needham (editor), M. Gardosh
and an anonymous reviewer for their constructive reviews, and to B. Katz
and S. Shaiak for editing. This research was partially funded by the Israel
Science Foundation (ISF 753/08), and partially supported by grants from
the Earth Science Research Administration of the Ministry of National
Infrastructures, Israel (25-17-028; 25-17-048).
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Received 7 August 2009; revised typescript accepted 12 February 2010.
Scientific editing by Tim Needham.
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