Accretionary processes at subduction zones in the eastern mediterranean

Accretionary processes at subduction zones in the eastern mediterranean

Tecronophysics, 112 (1985) 551-561 Elsevier Science Publishers 551 B.V., Amsterdam - Printed in The Netherlands ACCRETIONARY PROCESSES AT SUBDUCT...

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Tecronophysics, 112 (1985) 551-561 Elsevier Science Publishers

551

B.V., Amsterdam

- Printed

in The Netherlands

ACCRETIONARY PROCESSES AT SUBDUCTION ZONES IN THE EASTERN MEDITERRANEAN

YAIR

’ and ZVI BEN-AVRAHAM

ROTSTEIN

2

’ Institute {or Petroleum Research and Geophysics, P. 0. Box I 717, Holon 581 I7 (Israel) ’ Department of Geophysics and Planetary Sciences, Tel Aviv University, Ramat Aviv, Tel Aviv 69976 (Israel) (Revised

version received

September

13, 1984)

ABSTRACT

Rotstein,

Y. and

Ben-Avraham,

Mediterranean.

The tectonic the collision exist today

present

history

of the eastern

and accretion

of oceanic

in the eastern

the plate

complexity

Mediterranean plateaus

continental subduction trenches. western subduction

at subduction

Structures

zones

and Processes

Mediterranean

boundary,

particularly

of this subduction of a large

in the Hellenic Subduction parts.

Inner

plateau

in the eastern in Subduction

Many

other

arc area. Their presence by the seismicity

and Cyprean

an older

style are affected

results

and bathymetry

arcs, is probably

arc. This plateau

has been

arc takes place in the outer

segments

lithosphere

of these

outward

trenches

following

trenches,

particularly

in the Pliny and Ptolemy served

the collision

as the main of oceanic

plateaus

oceanic

plateaus

in the unusual patterns.

thrusted

subduction

The of the

over the

the two arcs. Active

in the Ionian trenches

by

oceanic

the consequence

and pieces of it are to be found in the region between

of Mediterranean

zones migrated

with

tectonic

zones. Small but distinct

away from the plate boundary. in the Hellenic

zone, as is evidenced

continental

mass of Anatolia

as well as the present

at subduction

two arcs system in this region, the Hellenic

collision

processes

and IS. Sacks (Editors),

Tecronophysics, 112: 551-561.

Zones.

crowd

Z., 1985. Accretionary

In: K. Kobayashi

and Strabo

is limited trenches

to their

before

the

plateaus.

INTRODUCTION

The eastern Mediterranean is a small ocean basin known for its unusual’ tectonic complexity. It includes a short segment of the convergence boundary between Africa and Eurasia. Subduction in this segment is along two very small arcs, the Hellenic and Cyprean arcs. In both arcs subduction has been documented using bathymetric, earthquake and other data (e.g. Rabinowitz and Ryan, 1970; McKenzie, 1970, 1972; Papazachos, 1973). The Hellenic arc is associated with backarc basin and volcanism, while the Cyprean arc is not. The bathymetric and seismic patterns in the eastern 0040-1951/85/$03.30

0 1985 Elsevier Science Publishers

B.V.

552

Mediterranean

seem to be significantly

type” subduction

zones. This apparent

models for this region (e.g. McKenzie, Pichon

and Angelier,

of agreement discuss

1979; Rotstein

on even

the tectonic

the geometry

framework

more complex complexity

than in most simple “pacific

has resulted

in numerous

1972, 1978; Nur and Ben-Avraham, and Kafka,

1982). These models express a lack

of the plate

of this region

tectonic 1978; Le

boundary.

try to present

Most

papers

a model

which

which

is

consistent with first-order observations. To date, relatively little effort has been made to propose models which are consistent with second-order observations in order to explain the complex bathymetric and seismic patterns. In this paper, we briefly describe some of the unusual but well-known characteristics of the bathymetric and seismic patterns in the eastern Mediterranean. We then proceed to propose a tectonic model in which the collision and accretion of oceanic plateaus are important factors which, together with subduction, explain these patterns. The occurrence of collision and accretion of oceanic plateaus in the eastern Mediterranean may be of special importance to the overall understanding of these processes. This area consists of small and accessible basins which appear to include a large number of oceanic plateaus in various stages of maturation; in addition, both these basins and the landmasses surrounding them are well known. Thus, the eastern Mediterranean may prove to be an area which is well suited for studying this process in general and the effects of various boundary in particular.

size oceanic

plateaus

on the shape of the plate

BATHYMETRY

Virtually all subduction arcs are characterized by a subduction trench, a single and mostly continuous ocean deep which marks the flexure of the descending oceanic lithosphere. In the eastern Mediterranean, however, the situation is markedly different. Subduction has been documented in this region, Hellenic arc, yet a single continuous trench cannot be traced.

particularly in the Figure 1 shows the

main bathymetric features in the eastern Mediterranean. The Hellenic arc is characterized by multiple, parallel and en echelon ocean deeps which follow the arc; in addition, numerous short deeps which are perpendicular to the trend of the arc are also present. Separate elevated blocks appear to be the elements causing the fragmentation of the longer deeps parallel to the arc. Generally, in the Hellenic arc, instead of one long subduction trench there are several deeps which could, probably, qualify as subduction trenches. This nontypical pattern is, probably, tectonically related and warrants an explanation. Several other bathymetric observations are of interest, For example, the different trenches are not equal in depth; in fact the outer, Strabo, trench is but a cleft in the ocean floor (Jongsma, 1977), whereas the one next to it, the Pliny trench, is much more distinct. Equally important may be the observation of a halo of small and, in places, deep

553

basins north of the subduction be argued

that

equivalent

to backarc

zone of the eastern

some of these, particularly basins.

The deep Finike

other hand, are much more difficult Anatolia

landmass,

Mediterranean.

the shallow

to account

It could possibly

ones around

and Rhodes

basins

Cyprus.

(Fig.

for. The Finike basin. adjacent

is an E--W trench which is as deep as the Mediterranean

plane;

however. in spite of its depth, it is not in the subduction

north

of a large elevated

block,

the Anaximander

Seamount

are

1). on the to the abyssal

zone since it appears and

since

it is not

associated with deep seismicity. Somewhat similarly, the Rhodes basin is a deep basin, even deeper than the abyssal plane, adjacent to the Anatolia landmass: moreover. it is characterized by a distinct, positive Bouger gravity anomaly (Woodside, 1976) which is similar to the gravity signature of the central parts of the eastern Mediterranean. Finally, the eastern Mediterranean includes a large number of elevated terranes particularly in the Ionian basin and the Hellenic arc complex. Some of the more distinct elevated terranes in the Ionian basin are the Medina Ridge, Medina Bank and the Cyrene, Epicharmos and Archimedes seamounts. Other prominent elevated terranes also appear within the Hellenic arc complex; however, whereas in the Ionian basin the elevated blocks are spread throughout the basin, in the Hellenic arc a large number of blocks crowds a small area causing the complex pattern of bathymetric

highs and lows.

SEISMIC’ITY

Classical “pacific type” subduction ping seismic zone. Earthquakes in the have been thought to be in the form 1973). Figure 2 is an example of a subduction in the Hellenic arc. It is cross-section distribution

that,

although

of earthquakes

is characterized by a Benioff-Waddati dipHellenic arc reach a depth of over 160 km and of a dipping seismic zone (e.g. Papazachos, seismic cross-section which is used to infer clear from the distribution of events in this

a dipping

seismic

zone can indeed

is not a simple one. Normally,

be followed,

the dipping

the

seismic zone

is only several tens of kilometers thick, since it represents processes in the rigid upper part of the lithosphere. In the Hellenic arc, on the other hand, the zone of subcrustal

earthquakes

is unusually

thick, reaching

a thickness

of about

200 km,

which is over twice the estimated thickness of the lithosphere in this area (Papazachos, 1969). Such an observation raises the question of whether a simple two plate model can be applied in this area, The inconsistency of the simple plate model with the seismic data was noted earlier by Galanapoulus (1973) and has recently been investigated by several other workers (Leydecker et al., 1978; Richter and Strobach, 1978; Comninakis and Papazachos, 1980). They have re-analyzed the available data in an effort to determine whether the apparent complexity in the seismicity pattern is the result of poor data quality, particularly poor depth control. Their results generally support the observation that some kind of dipping seismic zone does exist

555

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400 .I . . ..*

mm

250

300

350

A?C

SW 200

100

I50

0

50

SO

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200

300

250

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Asthmomphwo 2110 -

Fig. 2. Cross-section Papazachos, denote

intermediate

intermediate between

showing

the pattern

of deep focus earthquakes

1973). The plot is of focal depths against earthquakes

earthquakes

the distance

with M > 4.9 which occurred

with 4.5 6 M 4 4.8 and

shallow

between

earthquakes

1965 and 1971. Vertical and lateral errors were estimated,

km for data prior

across

the Hellenic

from a line following

1911 and 1971 and dots denote with M > 4.5, which

by the original

to 1965 and up to 25 km for more recent data.

arc (following

the arc. Triangles

See original

compiler, paper

occurred

to be up to 40

for details of data

sources.

20° 22' 24O 26* 28" 30° 32" 34O 36O 38O 4o" 42O 38O 4o" 36O 38'

36' 32O 34O 3o" 32' cl

3o"

5.0-

53

A

4.5-4.9

A

I;;,“,:

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\1\

c

18O Fig. 3. Epicenters (following (hatched).

20°

of intermediate

Papazachos, Lateral

22O

24O and

1973) indicating

26*

deep focus

28O

earthquakes

a gap of seismicity

and vertical errors were estimated,

30° in the eastern

between

by the original

prior to 1965 and up to 25 km for more recent data. See original

32O

paper

Mediterranean

the Hellenic

compiler,

34O

and Cyprean

region arcs

to be up to 40 km for data

for details of sources.

556

in the Hellenic Particularly

arc, but that this zone is unusually interesting

lar to the Hellenic

arc which are presented

show that the dipping it is also discontinuous

wide and complex.

in this regard are the seismicity by Richter

cross-sections and Strobach

perpendicu(1978). These

seismic layer is not only thick and complex but that, in places, with a large and distinct

and lower parts of the dipping

seismic gap separating

seismic layer. A similar phenomenon

the upper

was observed

in

the northwestern corner of the Cyprean arc where it was assumed to be the result of collision and accretion processes (Rotstein and Kafka, 1982). Another observation which adds to the difficulty in using a simple subduction model in this area, is the obvious lateral discontinuity in the earthquake distribution. For example, in the Hellenic arc deep focus earthquakes extend eastwards as far as Rhodes. To the east, in the area which is thought to be the junction between the Hellenic and Cyprean arcs (e.g. McKenzie, 1972) deep focus earthquakes are missing (Papazachos, 1973 and Fig. 3). TECTONIC

SYNTHESIS

The first-order process in the eastern Mediterranean is undoubtedly the subduction of the African lithosphere beneath Eurasia (e.g., McKenzie, 1970, 1972). This simple, two plate model is still the most widely used in any tectonic analysis of this region; yet it clearly cannot account for the unusual complexity when small scale features are considered. Thus, a second-order process is possibly required to accompany the two plate model in order to account for the irregularities in the bathymetric and seismicity patterns. This process is the collision and accretion of oceanic plateaus at plate boundaries. The significance of this process has recently been described for several regions, particularly around the Pacific ocean (e.g., Coney et al., 1980; Ben-Avraham

et al., 1981).

It is very likely that oceanic plateaus have existed in the eastern Mediterranean and that they have had a significant role in shaping the present tectonic pattern in the area.

At present

there

are several

prominent

bathymetric

highs

or oceanic

plateaus in the eastern Mediterranean away from the zone of plate boundary. They appear mostly in the Ionian basin and are in the form of seamounts (e.g. Cyrene, Archimedes, Epicharmos, Eratosthenes) and other prominent highs (e.g. Medina Bank, Medina Rise). These structures are embedded in the floor of the eastern Mediterranean and move with it towards the zone of subduction. Their height, sometimes more than 1.5 km over the surrounding ocean floor, and at times their buoyancy will prevent subduction upon their arrival at the plate boundary. Instead, they can be expected to collide with the continental mass north of the plate boundary and eventually be accreted to it. This process of collision and accretion is probably associated with the emplacement of ophiolites. Ophiolites are found in Cyprus, Turkey and Greece (e.g., Gass and Masson-Smith, 1963; Robertson and Woodcock, 1981a; Smith and Woodcock, 1982). Their pres-

557

ence just north of the plate boundary clearly indicates previous occurrences of accretion of oceanic plateaus. Of particular interest is the Bey Daglari area in southern Anatolia. The ophiolites in this area (Pinar-Erden and Ilhan, 1977) have probably been emplaced by the collision of a large oceanic plateau which can be recognized today as an allochthonous terrane on land (Robertson and Woodcock, 1981b). Oceanic plateaus are thus found in this region both at sea and as accreted terranes on land. It is, therefore, reasonable to expect to find them also in the zone of plateau boundary; indeed, we propose that the many elevated blocks which crowd the Hellenic and Cyprean arcs are oceanic plateaus in various stages of collision and accretion. Some of the more prominent of these are the Gvados, Pliny and Strabo seamounts in the Hellenic arc, the Hecataeus Ridge in the Cyprean arc and the Anaximander Seamount between the two arcs (Fig. 4a). These larger structures and other smaller ones disrupted normal subduction in the area by their collision and we propose that this is the reason for the fragmented pattern of the subduction zone in the Hellenic area. It also resulted in multiple trenches, since new subduction zones tend to migrate behind the colliding oceanic plateaus. Hence, the outermost subduction trench, the Strabo trench, is the youngest and its features are the least developed. The same process can also be used to explain the main features of the seismicity pattern. New subduction behind a colliding and accreting block is associated with a new dipping seismic zone. The two dipping zones can result in the extraordinarily thick zone of deep seismicity observed in the Hellenic arc (Fig. 2). Under different circumstances, it could also appear as one dipping seismic zone with a distinct gap as observed, for example, in the northeastern corner of this arc (Richter and Strobach, 1978). A schematic history of collision and accretion in the eastern Mediterranean is outlined in Fig. 4; an important observation incorporated in this figure is the distinction between small and large oceanic plateaus. We assume that a small oceanic plateau which is accreted onto the continental mass has only a local effect on the shape of the arc. However, when a large oceanic plateau is involved, the situation is markedly different. A large oceanic plateau, pieces of which may possibly be found today in southern Anatolia, significantly affected the shape of the arc system. We suggest, in fact, that prior to the collision of this large oceanic plateau, the Hellenic and Cyprean arcs were parts of one subduction arc in which mostly normal (dip-slip) subduction took place. The collision of a large oceanic plateau created the present two arc system. By using this simple mechanism, it is possible to give a straightforward explanation for two important observations which are well documented but not yet accounted for. First is the observation that seismicity is no deeper than 60 km in the zone between the two arcs. This is an expected result if we assume that.this zone between the two arcs is occupied by an accreted block and that new subduction and deep earthquakes have migrated past this block to the south (Fig. 4c). Indeed,

558

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NATOLIA

Papazachos (1973 and Fig. 3) documented subcrustal earthquakes south of the Anaximander Seamount near the new subduction trench, the Strabo trench and its extension eastward. Secondly, using the same sequence of events, the oblique subduction in the Hellenic arc east of Crete can be explained. In this zone the relative plate motion is almost parallel to the arc. This has led several investigators to suggest that this zone serves, in effect, as an inclined transform fault (McKenzie, 1978; Dewey and Sengor, 1979; Le Pichon and Angelier, 1979). However, the great depth of earthquakes associated with this inclined seismic zone supports the idea that it did originate as a normal subduction zone in which dipslip motion was dominant. We assume, therefore, that subduction in this region originated under normal circumstances. Only during a later period, the collision of a large oceanic plateau caused the division into a two arc system, as well as the changes in sense of relative motion along the shifted segments of these arcs. According to this model, active consumption of newly subducted African lithosphere occurs only at the outermost trenches. Thus, in the west Hellenic arc, the entire Ionian trench may be active but, in the central and eastern segments of the Hellenic arc, only those portions of the Ptolemy and Pliny trenches which face the open Mediterranean sea are active. Other trenches are now either partially or completely shut off. They are probably associated with sinking or laterally moving subducted slabs at depth, but have little or no recent surface subduction associated with them. The young Strabo trench and its even less developed eastward extension into the center of the Levant basin and the Cyprean arc, represent presently active subduction east of Crete and thus approximate the present zone of active plate boundary between Africa and Eurasia. The Rhodes and Finike basins are deep basins north of this plate boundary. They were an integral part of the Mediterranean floor (Fig. 4) as their unusual depth indicates. The observation that the Rhodes basin is characterized by a relatively large gravity anomaly may be another indication that they represent pieces of Mediterranean lithosphere which were trapped behind the plate boundary during the process of collision and accretion.

Fig. 4. Schematic history of collision and accretion of oceanic plateaus in the plate boundary zone of the eastern Mediterranean:

a. Before collision.

Several oceanic plateaus existed in the eastern Mediterranean.

The plate boundary consists of a continuous

and undisturbed

arc. b. During collision

and accretion. A

large plateau between Crete and Cyprus bends the arc and is possibly breaking up. c. Present day tectonic elements. The former single arc is now broken into two arcs. Remains of the large oceanic plateau north of the Anaximander

Seamount may now be appearing as accreted terranes on land in southwest Turkey.

Several smaller accreted terranes crowd the Hellenic arc. The consuming plate boundary is in the outmost trenches which face the African plate. Dotted coast lines in (a) and (b) are for reference. only. Heavy broken lines in (c) represent old zones of subduction-dipstip present motions.

as inclined

transform

in (a) and oblique in (b), which act at

faults with little or no active subduction.

Arrows

mark relative plate

The process of accretion of oceanic plateaus is consistent with the available bathymetric, seismicity and gravity data from the eastern Mediterranean. It is probably, in effect, the only presently available unified model with which the details of the data may be compared;

yet in order to further

model, additional

studies are required.

seismic refraction

and other methods

Crustal

establish

the validity

studies of the oceanic

are essential.

of this

plateaus

using

Makris et al. (1983), for example,

used seismic refraction to show that the Eratosthenes Seamount is indeed a continental fragment and similar studies of some other seamounts may reveal similar structures. In addition, a detailed comparison between the presently active Strabo and Ionic trenches and the inner inactive parts of the Pliny and Ptolemy trenches may also contribute to the examination of the accretion model. Finally, detailed seismicity studies of the plate margin using local seismic networks may yield an accurate

and detailed

structure

of the subducting

slabs in this region.

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