163 The southern Caspian: A compressional depression floored by a trapped, modified ~ oceanic crust "... and a goat was drinking water from the Caspian Sea of a geographic map." (Sohrab Sepehry) 2MANUEL BERBERIAN Departmentof Earth Sciences, Bullard Laboratories, University of Cambridge,MadingleyRise, Madingley Rd., Cambridge CB3 0EZ, England Received March 4, 1981 Revision accepted July 14, 1982 The south Caspian intracontinental depression, floored by oceanic basement, is a relatively stable block, with minor deformation, surrounded by active fold-thrust belts of arcuate form (Talesh, Alborz, and KopehDaghMountains),which have undergone intense late Cainozoic crustal shortening. The basin is interpreted as a Neogene-Quaternary"compressional depression," boundedby multi-role mountain-borderingreverse faults, and apparently floored by a late Paleozoic - Triassic or late Mesozoic- early Tertiary "modified oceanic crust" trapped along an old geosuture. It maybe a relic of an old (Paleozoic-Triassic) ocean, or else a marginal sea developedbehind a Mesozoic-Paleogeneocean, and analysis of geological and geophysical data enables a schemeto be suggested. The general arcuate shape of the Alborz and the Talesh bordering mountainbelts follows the pattern of the supposedrigid and thickened ocean crust of south Caspian depression. A tectono-sedimentarystudy of the south Caspianregion, coupled with the body-wavemodellingof a recent earthquake along one of the borderingfaults, maysuggest a possible flattening of the fault with depth(listric thrust), and that the estimate of the focal depth of the regional earthquakesbased on teleseismic arrival time data is not accurate. Thedifference in elevation between the depressionand the borderingactive fold-thrust belts is causedby a difference in crustal structure andreverse faulting during a dominantcompressional tectonic regime. Thestudy mayadd support to the idea that old continental deep-seated multi-role faults, whichhavecontrolled the sedimentary facies and basins during different geological times and were responsible for the formation of the present physiographicfeature, are the site of the present seismicactivity in the orogenicbelts. Le foss6 tectonique intracontinental ~ socle ocranique de la rrgion Caspiennesud est constitu6 d’un bloc relativement stable, peu drformr, entour6 par des zones de failles imbriqures actives de forme arqure (montagnesTalesh, Alborz et KopehDagh) ota la cro~te fut considrrablement raccourcie au Crnozoiquesuprrieur. Oncroit que la drpression tectonique correspond ~ un affaissement caus6 par compressionet limit6 en bordurepar des montagnesrrsultant de failles inverses ~ comportement multiple, et dont le socle serait apparamment une "crofate ocranique modifire," d’~tge palrozoique suprrieur - triassique ou mrsozoique suprrieur - tertiaire infrrieur, coincre le long d’une anciennegrosuture. I1 est possible que ce soit une relique d’un vieil ocran (Palrozoique-Trias) ou autrement une mer marginale f0rmre derriere un ocran du Mrsozoique-Palrog~ne, et l’examen des donnres grologiques et grophysiques fournit la trame pour l’explication des 6v~nements.Les chainons de montagnesAlborz et Talesh en bordure prrsentent une allure grnrrale en forme d’arc et suivent la structure de cette prrsumre croOte ocranique 6paisse et rigide du foss6 tectonique de la rrgion caspienne sud. L’rtude tectono-srdimentaire de la Caspienne sud, secondre par une modrlisation basre sur l’interprrtation des ondes sismiques d’un tremblementde terre rrcent le long des failles en bordure, semble suggrrer un aplatissement de la faille en fonction de la profondeur (faille courbe) et que les hypocentres drterminrs ~ l’aide des tremblements de terre rrgionaux en se servant des donnres des temps d’arrivre trlrsismiques sont localisrs avec imprrcision. La diffrrence en 616vation entre le foss6 tectonique et la bordure des zones de failles imbriqures est causre par une diffrrence dans la structure de la crofite et par les failles inverses rrsultant de la phase culminantedu rrgime de compressiontectonique. La prrsente 6tude supporte l’idre que les failles continentales anciennes de grande profondeur et ~ comportement multiple, lesquelles ont influenc6 les fossrs tectoniques et les facies srdimentaires durant diffrrentes prriodes grologiques, et qui sont responsables des formes physiographiques actuelles, sont le lieu de l’activit6 sismique dans les chainons orogrniques. [Traduit par le journal] Can. J. Earth Sci. 20, 163-183 (1983) 1CambridgeEarth Sciences Contribution No. ES 161a. 2Present address: Geological Survey of Iran, P.O. Box1964, Tehran, Iran. 0008-4077/83/020163-21 $01.00/0 ©1983National Research Council of Canada/Conseil national de recherches du Canada 164 CAN. J. EARTHSCI. VOL. 20, 1983 Introduction The Caspian Sea forms a deep midland basin, with water depth up to 900 m, in the northern part of the Alpine-Himalayanorogenic belt, and is surrounded in the south by arcuate active fold-thrust belts (the Alborz Mountains). The downwardmotion of the basin seems to be linked with the uplift of the surroundingregion, and appears to have started early in the Cainozoic Era, with intense phases of activity in Neogeneand Pleistocene times. Thepresent depression can be divided into a northern, a central, and a southern region, separated by major basementfaults (Kornev etal. 1962; Fedynskyet al. 1972; Glazunovaet al. 1977). The northern part is partly floored by suboceanic basementdeveloped in the Precambrian Russian platform, with north-south fold trends that appear to havehad a controlling influence on its development. The central part is floored by a northwest-southeast trending Hercynian basement of continental character, superimposedon the north-south Precambrian trends. The southern part, which is the most enigmatic, is floored by a basaltic basement, 15-20 kmthick, surroundedby granitic crust. It is this part of the basin that is a geologicallyunusualfeature: an oceanic basin that is situated betweenactive fold-thrust mountains of the Alpine-Himalayan belt and has escaped obduction during collisional orogenies. The main purpose of this paper is to develop a systematic approach to a better understanding of the evolution of the south Caspian depression. Manyexplanations have been proposed for this region and are discussed, but someeither conflict with the observations or invoke arbitrary concepts. There are two particular problems in understanding the south Caspian depression: firstly, howan intracontinental deep basin can occur and exist within compressional regime, and secondly, how an old ocean-like crust can remain unsubducted in such an environment for such a long period. To explain the first problemthe writer proposesa "compressional depression" superimposed on a marginal basin, identifying some of the active faults associated with it that have been mappedfor the first time. For the second problem, the writer hypothesizes that the floor apparently consists of a "modifiedoceanic crust" rather than the commonlyassumedocean crust. This hypothesismayexplain the thickness of the basaltic layer and also suggests that it is sufficiently low in density to have escaped subduction. The writer then discusses the ancient and active tectonics of the region, and suggests mechanismsresponsible for the developmentof the surrounding arcuate active mountainbelts. basaltic basement15-20 kmthick, with P-wavevelocities of 6.6-7.0krn/s (Galperin et al. 1962; Malovitski 1968; Neprochnov 1968; Rezanov and Chamo1969; Malovitski et al. 1970; Fedynsky et al. 1972). The overlying sediments are 15-25 kmthick, with a refracting interface within them at a depth of 8-12km. The sediments belowthis interface are thought to be Mesozoic and Paleogene in age, and those above, Neogene and Quaternary in age (Neprochnov1968). Apparently intensive sedimentation in the south Caspiandepression took place in the Pliocene-Quatemaryperiod, with the thickness of the Pliocene sediments exceeding 5-8 km and that of the Quaternary sediments amounting to 1.5-2.0km (Fedynsky et al. 1972). The PlioceneQuarternaryincrease in the subsidencerate of the south Caspian depression corresponds to the uplift, folding, and thrusting of the bordering fold-thrust mountain belts. The depression is characterized by near-normal heat flow of about 0.8 x 10-6 to 1.4 x 10-6 Cal cm-2 s-1 (Lyubimovaet al. 1974). Theoretically calculated heat flow showsan increase from 1.3 in the upper mantle to 1.75 at a dePthof 15 kmin the south Caspiandepression (Ashirov et al. 1976), and a decrease to near normal at top sedimentary cover presumably because of the rapid sedimentation. The total crustal thickness in the south Caspian depression ranges from 40 kmnear the periphery of the depression to 30km near its centre (Yegorkin and Matushkin 1969). The depth to the asthenosphereis around80 kmin the depression, whereas towards the Caucasus it increases to 120-150km (Fedynskyet al. 1972). The depression is markedby positive Bouguergravity anomaly, which changes to a negative isostatic anomalytowards the southemcoastal plain and then switches back to positive in the Alborz Mountains(Fedynskyet al. 1972). The age of the basaltic basementof the depression is uncertain. Accordingto some(Amurskiet al. 1968)it is pre-Liassic (older than 195 Ma); according to others (Shikalibeily and Grigoriants 1980) it is Jurassic and overlain by Cretaceous volcanic rocks. Adamia(1975) and Adamiaet al. (1977, 1980)believe that the basaltic basement is Albian-Eocenein age. Despite the uncertainty in the age, most authors agree that the basaltic basement extends eastwards to the southweatern foredeep of the Great Balkhan and to the eastern coastal region of the southern Caspian Sea (Amurski et al. 1968;Fig. 2). The deepest well drilled by the National Iranian Oil Company in the southeastern (Gorgan) coastal plain the Caspian Sea was abandoned in Lower Jurassic sediments (the coal-beating ShemshakFormation) at 2. Structure of the south Caspian depression depth of about 6 km(Stocklin and Nabavi1973; Stocklin Deepseismic sounding data suggest that the southern 1974b; A. Afshar-Harb and I. Yassini, personal compart of the Caspian Sea (the south Caspian depression; munication, 1980). It demonstrates the absence of the Fig. 1) lacks a granitic layer and that the relatively thick Mesozoicand (or) Cainozoic layer in the southeastern undeformed sedimentary cover rests directly on a coastal plain of the south CaspianSea. Paleoreconstruc- BERBERIAN 165 192a,o2 19 FI~. 1. Documented faults (heavylines) and epicentral regions(stippled areas) of the majorknown earthquakesin the south Caspianregion and its borderingactive fold-thrust belts. Theoceanic part of the south Caspiandepression, coveredby Mesozoic-Cainozoic sediments(Komev et al. 1962)is hatched(Shikalibeilyand Grigoriants1980).Contoursof the baseof sedimentary coverin the southCaspiandepression(Malovitskiet al. 1970)are shownin kilometres.Basedmainlyon the present study and the seismotectonic mapof Iran (M.Berberian1976a,b, 1981)after modificationand correction.Sources--historical (pre-1900)earthquakes:Ambraseys (1974); Berberian(1976b,1977), Melville(1978;only for the 874and 1436events); 1895.07.09earthquakealong the southernmarginof the Turanplate: Ivanovski(1899), Gorshkov(1947), Savarenskyet al. (1953), Petrushevsky et al. (1954), Masarskii(1961), Lindenand Savarenskii(1961); the 1946.11.04earthquakein the region along the KopehDaghfault: Rezanov(1955); epicentral regions of 1945.05.11, 1957.07.02, and 1971.08.09 earthquakes: Tchalenko(1974); epicentral region and Ipak earthquake fault of 1962.09.01: Ambraseys(1963, after modification); epicentral region of 1970.07.03earthquakein the KopehDaghfold-thrust belt: Ambraseys et al. (1971); epicentral regionsof 1913.04.16and 1924.02.19earthquakesin the westernpart of the south Caspiandepression:Malinovski (1939,1940);epicentreof the 1953.02.12 Torudearthquake:Abdalian(1953).Fault-planesolution(equal-areaprojectionof lowerfocal hemisphere) of the 1978.11.04earthquakeis fromthis study; others are fromShirokova (1962),PetrescuandPurcaru (1964), McKenzie (1972), Jacksonand Fitch (1979). Compressional quadrantsare shownin black and dilatational in Heavybarbedlines with triangles = thrust; with short lines at right angle = high-anglereversefault. TransverseMercator projection. tion of the Iranian region based on the available 1968; Fedynsky et al. 1972), only 800m of the Neogene-Quaternarysediments was deposited along the paleogeographic data (Berberian and King 1981) indicates that if the basaltic layer is oceanicit couldbe a relic northern flank of the rising AlborzMountains,bordering of either the Hercynian(closed in Triassic) and (or) the southern part of the Caspiandepression(Sussli 1976; Fig. 3). Mesozoic (closed in Cretaceous) ocean, or else marginal sea developedbehind an island arc. The region 3. Previous interpretations has been mostly under compression at least since There are several hypotheses on the origin and Pliocene-Pleistocene times, and no long-term extensional regimeis knownto haveoccurredin the area since developmentof the south Caspian depression (Milanovsky 1963; Kosminskaya and Cheinmann1965; Rezanov then (see Section 4). It is important to emphasizethat while 10kin of the and Chamo1969). ManyRussian earth scientists beNeogene-Quaternary sediments (20-0 Ma) was accu- lieve that the oceanic-like seismic character of the mulating in the south Caspian depression (Neprochnov depression basementresulted from basification of for- 166 CAN.J. EARTH SCI. VOL. 20, 1983 lOOkm ~ I CENTRAL IRAN I FI6.2. Physiographicfeatures of the south Caspianregion. Topographic contourlines are in metres. Post-Neogene-early Quaternary fold axesin the Caspiandepression(Solovyev et al. 1959;Glazunova et al. 1977;ShikalibeilyandGrigoriants1980), andin Iran (M.Berberian1976a,1981;Huber1978)are shownby dashedlines. SouthCaspianbasaltic layer (Shikalibeily Grigoriants1980)is hatched.Majorfaults are shownbythick lines. ThePaleozoicshearedophiolites(blackpatch)andbasic ultrabasic plutons (cross) in the Taleshmountains,and the southeasterncontinuationof the Sevan-Akera-Qaradagh Cretaceous ophiolite m61ange belt (heavyhatches)are shownin the westernpart of the CaspianSea. I mer continental crust initiated by downwarpingduring the Tertiary Period. It has also beensuggested that the basementis a remnantof the ancient Tethys Sea (Kornev et al. 1962; Deweyet al. 1973). Rezanovand Chamo (1969) and Shikalibeily and Grigoriants (1980) regarded the south Caspiandepression as an eroded rigid massof continental character and a zone of multiple rifting. They explained the absence of a granitic layer in the depression as being due to the lack of Paleozoic and Mesozoicrocks and the 6.6-7.0 km/s layer was interpreted as a pre-Paleozoic metamorphic basement of continental compositionbut with a velocity similar to that of basalt. Accordingto Adamia(1975) and Adamia et al. (1977, 1980) the oceanic-like crust of the south Caspian results from Late Cretaceous - early Paleogene rifting processes, with Middle Eocene basalts in the lowercrust alone, and is not the relic of an older ocean. Apol’skiy (1975) believed that the south Caspian depression initiated during Late Jurassic - Early Cretaceous times at the southeasternend of a left-lateral fault, whichalso created the BlackSea at its northwesternend. Clark et al. (1975) have suggested that the westernpart of the south Caspian depression might be bounded by normalfaults buried beneaththe sedimentsof the coastal plain, and that the depression is downthrown along these normal faults. Geological cross sections across the southern (Huber 1978) and the western coastal plain of the south Caspian depression (Davies 1975) show that the basin is downthrown along normal faults dipping north and east, respectively, but neither of these references shows the faults on the geological maps. Most of these interpretations conflict with the geological-seismological data and with the structural evolution of the region, and their shortcomings are discussed in the following sections. 4. Deformationhistory of the region The western and the southern margins of the south Caspian depression are delimited by the Talesh and the Khazar (Caspian) mountain-bordering active reverse faults (Fig. 1). The Talesh fault, about 400 kmlong, truncates the eastern flank of the Talesh and the Little BERBERIAN h Vp Alborz MI. Mo S.C.D. , , U. Pe ~ 650 F~. 3. Comp~ison of the simplified column~sections of ¯ e sou~Caspiandepression(S.C.D.) ~d ~e Alborzbordering fold-t~st mountNnbelt. Mainlycompiled~omNeprochnov(1968), Stocklin (1974a), Sussli (1976), ~d (1978). Caucasus fold-thrust belts and has juxtaposed the Paleozoic-Mesozoic and Quartemary sediments of the Caspian coastal plain. Uplift of the northern flank of Alborz Mountainalong the 600 kmlength of the Khazar reverse fault in the south (Figs. 1, 2) has brought the Precambrian Gorgan schists (Gansser 1951; Huber 1957; Jenny 1977a,b; Salehi-Rad 1979; Delaloye etal. 1981) in contact with the Quaternary sediments of the southern coastal plain of the CaspianSea, indicating the large magnitudeof the vertical uplift. Thesharp escarpmentand abrupt changein elevation betweenthe level of the Caspian Sea (26 mbelow meansea level (msl)) the eastern flank of Talesh Mountainin the west (about 1800m above msl), and the Caspian Sea and the northern flank of Alborz Mountain(about 2000m) in the south, are striking topographic breaks that might have been caused by differences in crustal structure and reverse movements along the faults shownin Figs. 1 and 2, which have been postulated as normal faults in some geological cross sections. In both cases the faults were not mappedearlier. 167 Since the age of the oceanic basement of the south Caspian depression is uncertain at present, analyses of geological, structural, and geophysical data mayenable a scheme to be suggested. The present Talesh and Alborz fold-thrust mountainbelts (bordering the western and the southern parts of the south Caspian depression; Fig. 1) were the site of two major faultcontrolled subsiding sedimentary basins (with Gondwanian biostratigraphy) during the Paleozoic and the early Mesozoicregional extensional phases, whenthe whole Iranian basement was attenuated and stretched (Berberian 1979a; Berberian and King 1981). Apparently during late Paleozoic - Triassic time the Gondwanianfragments (including Alborz and Talesh) split from Gondwanaland,crossed the Hercynian Ocean (Paleo-Tethys), and collided with the Asian block what is nownortheast Iran (Berberian and King 1981). The Triassic suture zone is indicated by the Herat (Tapponnier et al. 1981), southern Kopeh Dagh (Stocklin 1974b, 1977; Majidi 1978, 1981), probably northern Alborzand eastern Talesh (Clark et al. 1975), and the southern Pontides line (Sengor et al. 1980; Sengor and Yilmaz 1981; Tekeli 1981; see Figs. 4, 10d). Following the Middle Triassic (220 Ma) collisional orogenies, compressionalmovements,and uplift of the whole region, the onset of the Mesozoicextensional phase was markedby Rhaetic rift volcanism (tholeiitic basaltic lava flows), estuarine, deltaic, and littoral conditions, and deposition of the coal-beating Shemshak Formationof Rhaetic-Liassic age (with Eurasiatic fauna and flora) in the Talesh (west), the Alborz(south), and the KopehDagh(east) regions. TheseEarly Jurassic extensional phases and subsidence, which were also recorded in the Caucasus, resulted in the spreading of the oceanic basin along the Sevan-Akerasuture zone (Adamiaet al. 1977; Figs. 4, 10jO. Conglomerateswith large detrital fragments in the ShemshakFormation of the Alborz and Talesh Mountains (Assereto 1966a), together with Liassic transgression of the formationover the PrecambrianGorganschists (in the northern Alborz) and over the pre-Triassic metamorphicrocks and the Permo-Carboniferoussediments (in the Talesh), indicate that the northern Alborz(south Caspianregion) was emergedduring the Triassic, and was subject to intense denudation. This observation is also documentedin the Russian side of the south Caspian region (Vereshchagin and Ronov1968). Jurassic andesitic porphyrite dykes cutting the ShemshakFormation, together with andesitic tufts, have been found in the upper levels of the ShemshakFormation in the Talesh Mountains (Clark et al. 1975). Sedimentaryconditions changedto a transgressive marine environmentwith deposition of carbonates during the Late Jurassic and Cretaceousin the Talesh and Alborz basins. 168 CAN. J. EARTHSCI. VOL. 20, 1983 LATE CRETACEOUS 0 200 ~ FiG. 4. Present distribution of the Mesozoiccalc-alkaline Andeantype magmaticarc (stippled) along the southern active continental marginof Central Iran (the Sanandaj-Sirjan belt (SS), north of the Zagrosgeo-suture), and the active continental margin of Caucasus, northwest Iran (north of the Sevan-Akera-Qaradagh geosuture). Note that the south Caspian depression region (markedby dotted line) is situated in the back-arc region of the Sevan-Akera-Qaradagh subduction system (marked dashed line), and is boundedin the north and" the south by the Hercynianand Triassic geo-sutures. TheMesozoicsubduction zones (Zagros, Sevan-Akera-Qamdagh, and Sistan geo-sutures) are markedby thick lines with triangles showingthe direction subduction. The Joghatai-Doruneh(in the northeast) and the Nain-Baft(in centre) Red Sea type spreading regions (with oceanic crust) are markedby a line with diverging open arrows. Absenceof a wide arc-trench gap north of the Zagros geo-suture may indicate a steep Mariana type subduction system during the MesozoicEra. Lambertconformal conic projection. Inset map: Modifiedreconstruction (Mercator projection) of the region during the Late Cretaceous Epoch, showingthe active subduction zones and the plate tectonic frameworkof the area. Oceanic crusts are stippled (H.Z.A. Ocean= High-ZagrosAlpine Ocean). Magmatic arc is represented by crosses, subductionsystemsare shownby thick lines with triangles, and spreadingridges by a line with small bar perpendicularto it. Thedashedline in the south Caspiandepressionrepresents the area of the Mesozoicfailed-rift system in the back-arc region of the Sevan-Akera-Qaradagh geo-suture zone in northwest Iran. Dotted lines are the present continental shorelines. See also the schematic cross sections in Fig. 10 d-g, which complementthis figure and showthe evolution of the area at various stages during the MesozoicEra. Basedon Adamiaet al. (1977, 1980), Berberian and Berberian (1981), M.Berberian etal. (1981), F. Berberian et al. (1982), Berberian and King(1981), Tapponnieretal. (1981), Tirrul etal. (1982), and other referen6es cited in the text. BERBERIAN Augite-olivine diabasic flows of Late Jurassic Early Cretaceous age are developed in central Alborz (east of Damavandvolcano and in the Chalus area; Gypsum-Melaphyre Formation and member 1 of the Chalus Formation; Allenbach 1966; Steiger 1966; Cartier 1971; Sussli 1976) and were followed by the deposition of Lower Cretaceous limestone. This sequencemaybe the lateral equivalent of the alkali basalttrachyte lavas with salt- and gypsum-bearing terrestrial deposits of the northern Little Caucasus(Adamiaet al. 1977). An approximately 40 m thick flow of olivine basalt is recorded in the lower Karsang Memberof the LowerCretaceous Tizkuh Formation in central Alborz (Assereto 1966b). In Azarbaijan (northwest and west Talesh Mountains, south of the Russian border) thick Jurassic-Cretaceous alkali basalt (hawaiite, mugearite), rhyolite, andesite, and tuff (Vach6 1968; Babakhani et al. 1977; Riou 1979), and Senonianalkaline subsaturated (Blairmorite) lavas (Didon and Germain 1976) were laid down. Discovery of the Late Cretaceous pelagic limestones, pillow basalts, and ophiolites along the "Qaradagh geo-suture" in northwest Iran (Berberian et al. 1981) illustrated the southeastern continuationof the Mesozoic Sevan-AkeraOcean in Iran (Fig. 4). The position and geometryof the Qaradaghgeo-suture (Berberian et al. 1981) with respect to the south Caspian oceanic basement may throw new light on the development of the depression. Aptian-Cenomanian (member 3 of the Chalus Formation), Cenomanian-Turonian (number 4), Turonian (member5 of the Chalus Formation) amygdaloidal pyroxene-olivine porphyrite to diabase and tuff (Sussli 1976) and Aptian-Albian and Senonian tholeiitic basaltic andesites are found in the western and central Alborz Mountains(Annells et al. 1975). Late Cretaceous (Senonian-Maastrichtian) andesitic (with somebasaltic) lavas and tuffs, and estuarine sediments cut by small dykes of porphyrites (similar composition to the andesites) are dominantin the Talesh Mountains, west of the Caspian(Clark et al. 1975). Thesevolcanodetrital facies seem to be the southeastern continuation of the UpperCretaceous shallow-marineterrigenous carbonates and volcanics of the Transcaucasian island arc, whichis developedonly in the area north of the Sevan-Akera suture zone (Adamia et al. 1977, 1980; Fig. 4). In eastern Alborz, Upper Cretaceous basalt, spilitic lavas, and andesitic basalts are recorded in a few places (GSI 1975; A. Saidi, personal communication, 1981; see Fig. 4). Triassic, Jurassic, and Cretaceous intrusive bodies are also exposedin the Talesh and western Alborz .Mountains (Fig. 4, Berberian and Berberian 1981). A Mesozoicactive continental margin with Andean- 169 type magmatic arc may be deduced to have been in existence along the Transcaucasus-Talesh - Western and Central Alborz belt. It should be noted that the Mesozoicvolcanic activity diminished towards central and eastern Alborz(Fig. 4). Volumetrically significant calc-alkaline volcanic rocks are restricted to the Azarbaijan, Talesh, and west-central Alborz Mountains. This may indicate that the Sevan-Akera-Qaradagh rifting and the subsequent northwardsubducting system terminated towards eastern Alborz. No evidence of completerifting and subduction-related volcanismis yet found in eastern Alborz. This mayimply that the pole of rotation for Sevan-Akera-Qaradagh oceanic rifting was close to the eastern end of the suture zone, i.e., east-central Alborz, for which no data are available. Alternatively the suture zone was possibly displaced by a transformfault. The Jurassic and Cretaceous facies variations have produceda clear regional zonation parallel to the major structural trends of the Talesh (Clark et al. 1975) and Alborz regions (Sussli 1976), with a considerable increase in thickness of the sediments. The "marked sedimentary zonations" and "differences in facies and thickness" of the sediments (deposited in a short geological time) are clear consequencesof the considerable downwarpingof the sedimentary basin and the controlling effect of the major normalfaults along which the Talesh and the Alborz sedimentary basins were formed. Similar conditions have been documentedin the Shotori fold-thrust belt of Central Iran (Berberian 1979a, 1982). Apparentlynear Late Cretaceous time, the northwestern Central Iranian and Caucasian blocks collided and ophiolites were obducted along the Sevan-AkeraQaradaghgeo-suture zone in the Little Caucasus and northwestern Iran (Adamiaet al. 1977, 1980; Knipper 1980; Berberian et al. 1981). The resulting plate collision, whichaffected the region during Late Cretaceous - Paleocene time, produced substantial compressional deformation, as well as perhaps somehorizontal movementsoblique to the direction of compression,for which no data are yet available. Becauseof these convergent movements,the motion of the Talesh and Khazarfaults that border the eastern and the northern parts of the Mesozoic, fault-controlled, subsiding sedimentary basin (of the Talesh and the Alborz) possibly changed from normal (in the Mesozoic) to reverse (in Cainozoic). Gradualrising of the early Talesh and early Alborz Mountains along these faults inherited from older geological times is evident by "lack of the Paleogene and the Neogenesedimentation" over most of the Talesh and Alborzhighs (Berberian and King 1981). No Paleogene volcanic activity is recorded in the Talesh or Alborz Mountains(Fig. 5). Strongly alkali 170 CAN.J. EARTH SCI. VOL.20, 1983 ’., LATE OLIGOCENE COMPLEX MAKRAN ~ f MAKRAN TRENCH FIG. 5. Present distribution of the Central Iranian Paleogenecalc-alkaline magmaticarc (stippled) and the synchronousalkali rift volcanism(randomdashed-line pattern). The complexdistribution of the Paleogenecalc-alkaline volcanism(stippled) indicate that a simple subduction system was not the only mechanismresponsible during this period. The wide zone of the Paleogenearc-trench gap north of the Zagros geo-suture mayindicate a low-angle subduction system for this period (see Fig. 10h). The Paleogenecalc-alkaline magmaticarc gradually gives wayto the synchronousalkali-rift volcanismin the north. The line with diverging open arrowsand patches of alkali-rift volcanics indicates approximateareas of the Paleogeneactive back-arc extension in northwestIran (Azarbaijan) and south of AlborzMountain.Theline with filled arrows indicates the formation of the south Caspian back-arc (marginal) basin and development of the oceanic crust. The Zagros geo-suture (subduction zone terminated in early Neogenetime) and the presently active Makrantrench are markedby thick lines with triangles showingthe dip of the subduction zone. The Late-Cretaceous-emplaced ophiolite m61angecomplex is marked by black patches. East-west parallel lines represent the Late Cretaceous - Tertiary accretionary complex along the continental margins. J. D. = Joghatai-Doruneh ophiolite m61angecomplex in the northeast. Lambert conformal conic projection. Inset map: Modified reconstruction (Mercator projection) of the region during Late Oligocenetime, showingthe formation of the south Caspianand the Black Sea marginal basins developedin the back-arc region of the Zagros subductionsystem. Crosses indicate the Paleogene Andeantype magmaticarc, and the black patches are the Late-Cretaceous-emplacedophiolites. Thick line with triangles is the subduction zone, and the lines with perpendicular bars indicate back-arc spreading systems. Thepresent continental shorelines are markedfor reference by dotted line. (See Fig. 10h, which complementsthis figure.) References as with Fig. 4 and those mentionedin the text. BERBERIAN 171 silica-undersaturated lavas (analcimites, phonolites) (Vindobonian-Sarmatian; 10-5 Ma) are at an elevation with silica-saturated or only slightly undersaturated of about 2000 m along the northern flank of Alborz lavas (ankaramites, alkali basalts, porphyritic latites, Mountain(Stocklin 1974a; Sussli 1976; Huber 1978). latites, alkali trachytes, andesites) of Paleocene-Eocene Similarly the Caspian-facies subaquatic continental age are dominantin the Azarbaijan area west of Talesh series (Pliocene; 5-1.8 Ma)lies at about 1000 mabove Mountain (Babakhani et al. 1977; GMSI1978; Riou sea level along the northern flank of the Alborz 1979; Babakhani 1981; Fig. 5). About 4kmof Eocene Mountains, south of the Khazar fault. The same beds alkali basalt and basanite with Late Eocenealkali basic were discoveredby deep drilling in the southern Caspian and ultrabasic dykes and small intrusive bodies was coastal plain (north of the Khazar fault) below some reported from the northern part of Talesh in Russia 1600-2000m of Pliocene and Quaternary sediments (Azizbekov et al. 1978). Eocene-Oligocene analcime (Faridi 1964; Mostofi and Paran 1964; Paran and basanite lavas were also developed in the southern Crichton 1966), indicating a rapidly subsiding basin. Alborz Mountains(Stalder 1971; Annells et al. 1975). The total vertical movementacross the Khazar fault The extensive "Paleogene alkaline volcanism" devel- since late Neogene time (2Ma), as indicated oped in northern Iran (northern Talesh, Azarbaijan, comparing the amount of throw in the Caspian-facies southern Alborz)indicates a "deep faulting and rifting" sedimentsdisplaced by the fault, is therefore estimated phase during an overall compressionalregime in Central to be at least 3000m. Total displacements of 2 km(for Iran (Fig. 5). Paleogene alkaline volcanism generally the Quaternary) and 600 m(for the past 300 000 years) lessened toward the south (i.e., Central Iran) where are reported from the southern coastal plain of the more "synchronous calc-alkaline volcanics" (mainly Caspian Sea (Paluska and Degens 1979). andesitic) predominate (Tarakian 1972; Dimitrijevic Similar to the formationof the Tabasand other Iranian 1973; Amidi 1975; Caillat et al. 1978; Fig. 5). The majordepressionsin responseto peripheral uplifts of the Central Iranian Paleogene volcanic activity was fol- fold-thrust mountainbelts (Berberian 1979a, 1982), the lowed by development of the northwest-southeast south Caspian depression underwentgradual subsidence Andean-type intrusive arc of Oligocene-Miocene age along the mountain-bordering reverse faults (Khazar (F. Berberian 1981; Berberian and Berberian 1981; and Talesh in the south and the west) during the Berberian et al. 1982). The occurrence of synchronous Pliocene-Pleistocene compressional orogenies. It subcalc-alkaline volcanics (a subduction product) in the sided as the Alborzand the Talesh fold-thrust mountain south and the predominantnorthern alkaline volcanism belts rose. The subsidence started in Eocene time mayindicate the formation of a "marginal basin" during (55 Ma) and continued to the present, with climaxes early Tertiary time along the Talesh - south Caspian in the Pliocene-Pleistocene. The Pliocene-Pleistocene elevation of the bordering fold-thrust mountainbelts is region (Fig. 5). During Middle and Late Miocene times marine therefore a manifestation of crustal shortening and Caspian-facies sediments covered only the northern thickening, and is not a basin-and-range type of su’uclimb of the rising AlborzMountains(deposition of about ture. The fluctuations and elevation changes of the 520mof Vindobonian-Sarmatian sediments; Sussli Caspian terraces and shorelines (Federov 1961; Leon1976). These sediments were unconformably covered tyev 1961, 1964; Kvasov1968; Ehlers 1971; Annells et by the Pliocene continental series (5-1.8 Ma)along the al. 1975; Paiuska and Degens 1979) are proof of northern foothills of the Alborz fold-thrust belt. The continuing Vertical movements of the region throughout Pliocene-Pleistocene compressional movementswere the QuaternaryPeriod. Despite an increasing subsidence involved in folding, reverse faulting, and further rate in Neogene-Quaternary times, no volcanic activity elevation of the Talesh and AlborzMountainsrelative to developed in the south Caspian depression during that the south Caspian depression. The Alborz fold-thrust period. The Pliocene-Quaternary tectonics (uplifting mountainbelt was elevated by northwardthrusting in the and folding of the bordering Alborz and Talesh Mounnorth and southwardthrusting in the south of the range. tains) and the present seismic activity (Fig. 1) indicate Similarly the Talesh fold-thrust mountainbelt rose along that the region is still under compressionalregime. eastward and westwarddipping reverse faults bordering the mountain belt. Surface geology (Stocklin 1974a; 5. Active tectonics, the Siahbil earthquake, and the Clark et al. 1975; Huber1978)indicates that folding and nature of the faults bordering the south Caspian depression thrusting of the Alborzand the Talesh fold-thrust belts represent a minimumhorizontal shortening of about 25 Nowroozi (1972), McKenzie (1972), Deweyet al. and 20%during the Pliocene-Pleistocene compres- (1973,) and Sborshchikovet al. (1981) postulated the existence of a south Caspian plate in their modelof sional movements. At present the folded Caspian marine sediments active tectonics of the area. Thereis no surface structure 172 CAN. J. EARTHSCI. VOL. 20, 1983 O0 O0 ¯ ¯ ¯ I,:.5.". ¯ - ¯ o~ ¯ O0 ¯ -. 50* ¯ ¯ Oo Oq-o -o q~O . . ~ O0 .. ~0 ¯ ¯ ¯ ¯ O0 ¯ ~o FIr. 6. Twentiethcentury instrumental epicentre (ISS 1918-1964;ISC 1964-1981)mapof the south Caspianregion indicatinghigh, shallowseismicactivity in the borderingactivefold-thrustbelts andlowerlevel of activity at the southCaspian depression,especiallyin the region of the basaltic layer. Theseismicityfollowsthe pattern of the fold-thrust belts. Early epicentral locations are poor, and epicentres of the 1970’shavea location error of about15 km(Berberian1979a,b). Mb 3.5-7.2; h = shallow. that could correspond to the western and southern boundariesof the introducedplate. Moreover,the recent folding (Fig. 2), faulting (Fig. 1), and seismic activity (Fig. 6) are not restricted to, or evenconcentrated on, the boundariesof the proposedplate. Scattered historical earthquakes and the 20th century instrumental earthquake locations of the south Caspian region lie along the bordering fold-thrust belts of the Talesh (in the west), the Alborz(in the south), and the KopehDagh in the east (Figs. 1, 6; see also M. Berberian 1976a, 1981). The inner part of the depression has a low level of seismic activity, and the region cannot be divided in the manner proposed by Nowroozi (1976). Regional geo!ogy, tectonics, and seismicity do not showeast or north dipping faults in the westernand southern borders of the Caspian Sea. The Talesh (Astara in Berberian 1976a) and the Khazar multi-role basement reverse faults are major active features associated with several damagingand destructive earthquakes during the last 1100 years (Fig. 1). Nofault-plane solutions have been available for earthquakes along the active faults described. The recent earthquake of Siahbil (1978.11.04) provided interesting results concerning the seismotectonic evolution of the area and the nature of the Talesh fault bordering the western part of the south Caspian depression. The earthquake of magnitude Ms= 6.0 (Mb = 6.1) took place on November4, 1978 at 15:22:19 CUT(Coordinated Universal Time) without any recorded foreshocks. The instrumental epicentre was reported by the National Earthquake Information Service of the United States Geological Survey (USGS) 37.674°N,48.90 I°E, with a focal depth of 34.0 km. The earthquake destroyed and damagedabout 20 villages along the Talesh fault (Fig. 1) and, unlike the previous earthquakes (Berberian 1979b), fortunately caused casualties (RLSO1978). The 1978 earthquake was not the first recordedseismicactivity alongthe Talesh fault. Thenorthern segmentof the fault was associated with an earthquake of Mb= 5.2 on April 16, 1913 (Malinovski 1940;see Fig. 1). Fault-plane solution of the 1978 earthquake using long-period vertical component P-wave first motion shows a low-angle (09°WSW)plane and a high-angle (81 °ENE)plane striking 168° (Fig. 7). Regionalgeological information, Landsat imagerystudy, damagedistribution (RLSO1978) along the Talesh fault (Fig. 1), the epicentral location of the earthquakeon the hangingwall block of the fault (NEIS1978)all mayindicate that the plane dipping west-southwestis the fault plane (Fig. 7). Unfortunately no surface break was observed in the field and no aftershock study wascarried out to constrain this argument. To myknowledgeno east dipping fault (the high-angleauxiliary plane) has been reported in the epicentral area. The auxiliary plane is well constrained BERBERIAN 173 1978.11.0~ 51AHBIL(Tolesh) C~syn obs ANP 1.2 ¯ ¯ ~=168’ SHL ~_~ -I 20s I- F~G.7. Synthetic (top) and observed(bottom) P-waveforms at 15 WWSS networkstations for the Siahbill 1978.11.04 earthquake alongthe Taleshfault, borderingthe westernpart of the southCaspiandepression.Eachstation canbe identifiedby its letter code.Thelong-periodP first motionpolarity is representedby the equal-areaprojectionof the lowerhalf of the focal sphere.Solidcircles are compressional first motion,openare dilatational. T = tensionaxis; P = pressureaxis. Thefoci are taken to be in the crust witha P-wave velocityof 6.8 km/s.Thehorizontalprojectionof the slip vectorsis shown bylines witharrows andnumbersoutside the focal sphere. Synthticwaveforms matchedthe observedwell at a focal depthof about20 ± 4 km(see Fig. 8). Thepredictedkink in the downward synthetic waveforms at WINandNAIis the P arrival, which is not present in the observedseismogram.COP,PTO,and ESKseemto have somebackgroundnoise. by the long-period first-motion observations, but the fault plane is less constrained(Fig. 7). In order to constrain the fault planes and to determine the source depth of the earthquake, far field waveform modelling was used (Jackson and Fitch 1981). For shallowearthquakesthe shapeof the first 10-20s of the long-period vertical components of the teleseismic P-waveformsis largely determined by direct P and its two surface reflections pPand sP. The polarities and relative amplitudes of these phases are determined by the fault-plane solution and their relative arrival times are controlled by the source depth (Helmberger1974; Langston and Helmberger 1975; Helmberger and Burdick 1979; Jackson and Fitch 1981). The comer frequency of the spectrum of the source function affects the waveformsin an identifiable way and is adjusted to give a goodfit. Thusthe initially determined fault-plane solution, the depth, and the comer frequency were the only source parameters altered in the modelling process. Figure 7 showsthe waveformschosenfor the best-fitting fault parameters. These have a fault of 168°, a depth of 20km, and a comer frequency of 0.1 Hz. The effect of changing comer frequency is shown in Fig. 8 and is firinly controlled by the pulse width to 0.1 Hz. Figure 9 shows the effect of depth change, and suggests an accuracy of better than 4 kmin the source-depth estimate (20 km). This is a slightly deeper event comparedwith similar observationsin other parts of Iran, and like other cases indicates that focal-depth estimates based on teleseismic 174 CAN. J. cop CHG EARTHSCI. VOL. 20, 1983 STU MAT obs d(kt=) |0 20s CHG COP STU ~ ~ ~ FIG. 8. Variation of synthetic waveforms with changeof comerfrequencyffc) at four selectedstations in Fig. 7. The observed waveformsare shownat top and bottom of each column,fc = 0.10 Hzseemsa reasonablefit withthe observed waveform. arrival-time data of the Iranian earthquakesare inaccurate (McKenzie 1972; Berberian and Papastamatiou 1978; Berberian 1979c; Berberian et al. 1979; Jackson 1980; Jackson and Fitch 1979, 1981). Similar variations of modelswith changing fault orientations suggest that the fault planes are well constrained. In conclusion a focal depth of 20 -+ 4 kmwith a fault plane at source dipping 09°WSW was constrained by detailed examination of the long-period teleseismic waveformmodelling of the Siahbil earthquakealong the Talesh active reverse fault, bordering the southwestern margin of the south Caspian depression. Despite the low-angle faulting at depth, the steep escarpmentand linearity of the fault at the surface reflect a mountain-bordering high-angle reverse character for the Talesh fault. Comparisonof different dips at the surface and at depth mayindicate that the fault dip decreases considerably with depth. 6. Discussion of the models The mechanism for generating the south Caspian depression is poorly understood, and most of the proposedideas fail to agree with the regional observations. This is mainlydue to the uncertainty in the age of the ocean basementand absence of detailed geological and petrochemical studies of the bordering mountain belts in Iran. Theessential conditionsto be fulfilled are that the compressionalregimewith reverse faulting and folding have dominated since at least Late Miocene time, and the pre-Jurassic (Amurski et al. 1968), Jurassic (Shikalibeily and Grigoriants 1980), or the Cretaceous - early Tertiary (Adamiaet al. 1977) thick basaltic crust was not subducted. It is difficult to assumea very thin (15 km), rigid continental basementcrust (i.e., metamorphicbasement at granulite or amphibolitegrade) for the south Caspian depression with P-velocities of about 6.6-7.0km/s. obs ~ 20s I-- FIG. 9. P-wavesynthetic seismogramsat four selected stations in Fig. 7 with varying depth (d). The observed waveformsare shownat top and bottom of each column. A source depthof about20 kmseemsa reasonablefit with the observed waveform. Metamorphic basements exist in northern Iran and southern Russia, but none of themhave the characteristics of the south Caspian basement,and the latter does not belong to either of them. The idea of diapiric intrusion of dense asthenospheric material into lower continental crust (oceanization of continental crust; Muller 1978) acting as a weight for lowering the basementis favoured by several Russian authors. The increase in the lower crust density by the invasion of subcrustal volumesof densebasic or ultrabasic intrusive rocks (Beloussov 1960, 1962, 1972, 1977), or metamorphismto the granulite or eclogite facies (Haxby et al. 1976) could be a possible initiating mechanism for the formation of the south Caspian depression. Several areas for which such an idea was proposed are now explained by other mechanisms. Moreover, it is not clear why such a mechanismwas initiated only in this special location. The dynamic effect of the mantle processes (Tamrazian 1976) unlikely to have been involved in the subsidence of the south Caspiandepression, since it is difficult to understand whysuch a mantle activity should exist beneath the south Caspian depression in particular rather than elsewhere. An upward migration of the Mohorovi~i6 discontinuity (Moho) due to phase changes and sedimentary loading (Rezanov and Chamo1969) does not appear plausible, because it is nowbelieved that the Mohois not a phase change (McKenzie1978b). The Baykal (Tapponnier and Molnar 1979), Hornelen 175 (Steel 1976), Maritime (Leeder 1976), and Dead-Sea rhombgraben (Garfunkel 1981; Garfunkel et al. 1981) type rifting associated with the large strike-slip movements seems not to be applicable to the south Caspian region. Large-scale strike-slip motions such as those now occurring in central Asia and Asia Minor could have occurred during previous geological times, but are not detectable by present paleogeographic and surface geological data. The detachment and sinking of the lower part of the lithosphere (the "cold blob" modelof McKenzie1978b) are unlikely to be applicable because the crust was not thick enoughduring early Tertiary time when the main loaded subsiding phase started. The present depth of the Mohounder the south Caspian depression is about 40km. By subtracting 20kmof sedimentary thickness, 20 kmof oceanic crust is obtained. Comparingthis amountwith the depth of the Mohounder the Alborz Mountains(in the south) or the Caucasusbelt (in the west), which is nowabout 45 (Peive and Yanshin 1979; Dehghani1981), requires large amountof stretching. The timing for subsidence caused by an extensional tectonic regimeand stretching of the crust is therefore critical, and shouldbe consistent with the geological history of the region. All existing data confirm that the south Caspian fault-controlled depression is underlain by an old basementof oceanic character: (i) lack of similarity with either the northern Iranian or the southern Russian geology;(ii) the special position of the depressionalong an old (late Paleozoic - Triassic) geo-suture, with obducted Hercynian-Triassic ophiolites (Talesh in the west (Clark et al. 1975) and Mashhad-Herat farther east (Majidi 1981;Tapponnieret al. 1981)); (iii) the depression’s situation in the back-arc region of the Late Cretaceous Sevan-Akera-Qaradagh ophiolite-radiolarite belt (Grigoryevet al. 1975; Adamiaet al. 1977, 1980; Knipper 1980; Berberian et al. 1981); and (iv) having the Black Sea oceanic crust (Adamiaet al. 1974, 1977; Letouzey et al. 1977; Biju-Duval et al. 1978) farther northwest in a similar situation. These four factors give somecredibility to the assumptionthat the south Caspian depression formedquite differently from its adjacent blocks, but its formation was linked with consumption of an oceanic crust. Absence of the Lg-wavephase propagation across the deep parts of the south Caspian depression (Kadinsky-Cadeet al. 1981) supports the oceanic type character of the depression. Becauseof its thickness (about 15-20km)it is difficult to consider it as being a renmantof a simpleoceancrust. Oceanic crusts are muchthinner (about 6 km), and the old, cold oceanic crusts are denser and gravitationally unstable with respect to the underlying hot mantle rock; therefore, they usually subduct in convergent zones (Parker and Oldenburg1973; Parson and Sclater 1977; McKenzie 1977, 1978b; Molnar and Atwater 1978). However,there are pieces of old oceanic crusts, like the Mesozoic oceanic plate of the eastern Bering Sea (Cooperet al. 1976a,b), that did not subduct into the mantle. The relatively thick and nonsubductedbasaltic crust could be analogousto a"modified oceanic crust" such as the oceanic plateaus (Carlson et al. 1980), Iceland type crust (Jacobyet al. 1980),or to the island arcs that never sank into the mantle. There are two sets of obducted ophiolite sequencesof different ages in the westernpart of the south Caspianoceanic crust: (1) The older sequence, consisting of sheared ophiolites-serpentinites, basic to ultrabasic plutonic bodies (gabbro and peridotite), LowerCarboniferous and Permian andesitic volcanics, and Paleozoic metamorphic rocks, has been found in the Talesh Mountains (Davies et al. 1972; Clark et al. 1975; Davies1975; see Fig. 2). Unfortunately the radiometric age of the ophiolites of the Talesh Mountainsis not known,and the evidence is not conclusive, but someof themare thought to be of probable late Paleozoicage; detrital fragments of the sheared serpentinites and metamorphicrocks are present in the LowerJurassic conglomerate(Clark et al. 1975). The Talesh late Paleozoic - Triassic ophiolites appear to mark the western continuation of the Mashhad-Herat Triassic suture line (Majidi 1978; Tapponnieret al. 1981; Figs. 2, 4). If the age of the oceanic crust of the south Caspian depression is preJurassic (Amurski et al. 1968) and the Triassic geosuture delineates its southern boundary, then it is plausible to consider the south Caspian depression basement as a part of an intra-oceanic island arc associated with the northwardsubduction of the Hercynian-Triassic ocean crust, which was possibly trapped along the suture zone. In this case the crust of the island arc, which is composed of volcanics and the arc sediments (Dickinson 1970, 1974; Mitchel and Reading 1971), could have a lower density than that of the upper mantle. This density difference, together with its thickness, presumablypreventedits completesinking into the mantle. An obducted fossil island arc with similar thickness was recently discovered in the Kuhistanregion along the India-Eurasia suture zone of northern Pakistan (Tahirkheli et al. 1979; Tahirkheli and Jan 1979). This discoverymayindicate that it is difficult to destroy the ancient island arcs that have lowerdensities than the mantle. (2) The younger ophiolite sequence is the "SevanAkera-Qaradaghophiolite m61angebelt" of Late Cretaceous age (Figs. 2, 4, 5), which was emplaced along the Little Caucasusmountainrange, west of the south Caspian depression (Gdgoryev et al. 1975; Yegorkina et al. 1976; Satian 1979; Knipper 1980; Berberian et al. 1981). The south Caspiandepression is situated in the "back-arc region" of the Sevan-Akera- 176 CAN.J. EARTHSCI. VOL; 20, 1983 ~ GONDWANALAND S SQ~pre 650Ma ? " b) 650-Z’00 Me d) 270-220 Ma "’"’-. ~HrZAGROS .: ~ ~ " .......... hz 80Ma. RedSea OCEAN ~ ..................... g) 85-60M~ NE : 9 ’ HERCYNIAN ~~ c)270Ma LAURASIA NE i ~-Turan 9 OCEAN PRECAMBRIAN ss60~nb60Ma " / "" ~ ~ ~ . ~ sTqlOOMa ~ " : ¯ -.. jd ~ ". f~ff SOUTH CASPIAN NE .. : i)5Ma-0 FIG.10. Schematic sequentialcross sections showingthe large-scalekinematicsand the simplifiedevolutionof the Iranian crust duringseveral collisional orogenics. Thecross sections complement Figs. 4, and 5 and the text. Northward motionof Central Iran, closure of the HercynianOceanin the northeast, and openingand closure of the High-Zagros AlpineOceanin southwest[ran duringvariouscollisional orogeniesprovidea plate tectonic framework for the structure of Iran anddevelopment of the southCaspianoceanicbasement.Widthsof the oceanbasins(black) are not representedat scale. 1 = metamorphism; 2 emplaced ophiolites; 3 = alkali-rift volcanism:4 = calc-alkaline magmatic arc; hz = High-Zagros (the northernmarginof the Zagrosbelt, southwestof the Zagrosgeo-suture);ss = Sanandaj-Sirjan belt, the southernactive continentalmarginof Central Iran, northeast of the Zagrosgeo-suture;al = AlborzMountains,northernmarginof Central Iran, south of Caspian;nb = Nain-Baft.jd = Joghatai-Doruneh ophiolite belts in Central[ran (also see Figs. 4, 5). Qaradaghgeo-suture (Fig. 5). The southern continua- AlborzMountains(see Fig. 5 and Section 4). This linear tion of this geo-suture was recently discovered in Iran belt was therefore a complexactive margin during the (Berberian et al. 1981). This geo-suture and the wide- Mesozoic Era, and the complex volcanism (Section 4) spread Mesozoicmagmaticarc along a linear zone can could have been connected with the formation of an be traced from the Transcaucasianisland arc (Adamiaet island-arc-marginal-basin system. al. 1977, 1980) southwardto the Talesh and parts of the Based on the geological data (Section 4) the south BERBERIAN Caspian depression is situated in a special region that has undergone at least two extensional phases during the Mesozoic(Fig. 4) and Paleogene(Fig. 5) with widespread developmentof alkali basalts and basanites. The Mesozoicextensional phase(s) was (were) related to formation of the Sevan-Akera-Qaradaghoceanic crust and its northern back-arc (marginal) basin development. The south Caspian depression could be considered as a failed-rift systemsuperimposedalong the Triassic collisional suture during the MesozoicEra, and its evolution was possibly terminated because of the Late Cretaceouscollisional orogenies (closure of the SevanAkera-Qaradagh ocean). Widespreadoccurrence of thick Paleogene alkaline volcanic rocks in the area west of the south Caspian region (northwest Iran, northern Talesh, and southern Alborz) may indicate development of the Paleogene extensional regime and "marginal basin" behind the Central Iranian Andeantype calc-alkaline magmatic-arc belt (Figs. 5, 10h). Developmentof the "predominant Paleogenealkali volcanics" in nothern Iran and in the Caspian region (far from the Zagros trench) and the "synchronous Andean-typecalc-alkaline volcanics" in Central Iran (close to the Zagros trench), with "transitional volcanic province" between them, becomes an interesting problem. Recent petrochemical and isotope study of the magmaticrocks in Central Iran (F. Berberian1981; Berberian et al. 1982) revealed that the Andeantype magmatism related to the subduction of the High-ZagrosAlpine Oceancrust underneath Central Iran lasted until early Neogenetime, whenan Arabian - Central Iranian continental collision took place. The Paleogenecalc-alkaline, transitional, and alkaline volcanic provinces in the north can be related to this subduction (Figs. 5, 10h). Apparentlythe south Caspian Mesozoicfailed rift (superimposedon the Triassic collisional suture zone) evolved as a true marginal basin during the Paleogeneback-arc rifting behind the Central Iranian Andeantype calc-alkaline magmaticarc. Presumablythe south Caspian basementsubsided further as a result of continued cooling and sedimentloading. Since at least Pliocene-Pleistocene time the south Caspian depression evolved as a depression boundedby major reverse faults. Data presented in this study indicate the establishment of the compressionalregime and introduce the bordering active reverse faults with their possible listric behaviourat depth. Theconvergent movementsand lithospheric response to loading of the depression (Watts and Ryan1976; Sweeney1976) with thick sedimentary deposits over a cold oceanic crust presumablyaccentuated the subsidence. At present the oceanic type basementof the south Caspian depression is limited by and downthrownalong the Khazar(in the south; this paper) and Apsheron-Balkhan (in the north; Shikalibeily and Grigodants 1980) reverse faults (Fig. 177 1). The Khazarfault coincides with a line dividing the northern zone of substantial negative isostatic anomalies from the southern (Alborz) zone of monotonous positive anomalies (Fedynskyetal. 1972). The Apsheron-Balkhan fault is clearly revealed by a gravity gradient and the pattern of the geomagnetic field, introducing a deep structure separating the south Caspian oceanic crust from the platform regions of the central Caspian (Fedynskyet al. 1972; Shikalibeily and Grigoriants 1980). The low level of seismic activity (Fig. 6) and the relatively undeformedthick sediments abovethe basaltic layer (Fig. 2) in the south Caspiandepressionindicate that, like the oceanic crusts, the old basementof the depressionis "inherentlyrigid." In contrast to this strong crust with minor deformation, the Talesh, Alborz, and the KopehDaghperipheral active fold-thrust belts with weak(continental) crust and inherited planes of weakness are folded, thrusted, and have higher seismic activity levels (Figs. 2, 6). The old oceanic type substratum of the depression presumably has not been remobilized during later deformational phases and possibly resisted fragmentation, althoughit was subject to the same forces as its bordering active fold-thrust belts. Minor folds observed in the upper sedimentary cover of the south Caspian depression should be involved in detachment tectonics with a d6collement zone at the base. Apparentlythe general arcuate pattem of the Alborzand Talesh bordering fold-thrust mountain belts (Fig. 2) follows the shape of the trapped modified ocean-crust basementof the south Caspian depression. Just as in the experimentalstudies on strain fields around rigid inclusions (Ghosh and Sengupta 1973; Ghosh 1975; Ghosh and Ramberg 1976), the Neogene-Quaternary fold patterns, with swerving of the fold axes around the south Caspian depression and bowingof the AlborzMountains(Fig. 2), mayoutline the strain field around the relatively rigid ocean-crust type basement. The superficial morphologyis somehowsimilar to the Tarim basin of central Asia (Molnar and Tapponnier 1978), whererifting does not occur and the depressionis surroundedby active folded and elevated belts. 7. Conclusions Notwithstanding manyassumptions due to the limited data available from Russian literature, an approachhas been attempted to tackle some of the seismotectonic problemsof the south Caspian region. A "compressional depression" superimposed on a "marginal basin," boundedby "reverse (listric?) basementfaults" inherited from older geological times and floored apparently by a "modified ocean-crust basement" seems to be a plausible mechanismfor the formation and elevation of the south Caspian depression during the convergent movementsof the Arabian and Eurasian plates. The stratig- 178 CAN. J. EARTHSCI. VOL. 20, 1983 raphyand structural history of the region showthat the subsidencewas associated with uplifting of the bordering fold-thrust mountain belts. Basementfaults that controlled the boundaries of the depression were formed prior to or during the initial subsidence. Apparently, throughout the Mesozoic and Cainozoic Eras, the basementfaults were reactivated with different mechanisms in response to different tectonic regimes produced by continental movements. The south Caspian depression opened as a marginal basin behind the Mesozoic Transcaucasian-Taleshwestern Alborz and the Paleogene Central Iranian Andeanarcs. Eventscan be divided into several overlapping and synchronousstages (Figs. 4, 5, 10): (a) Mesozoicrifting and formation of the SevanAkera-Qaradagh ocean between the European plate (active continental margin of the northern Little Caucasus) and the Central Iranian plate (passive continental marginof the southern Little Caucasus)(Fig. 10j’). (b) Mesozoic Andean-arc stage, characterized calc-alkaline volcanism north of the Sevan-AkeraQaradaghgeo-suture (Figs. 4, 10f). (c) Late Cretaceous collisional orogenyin northwest Iran and the formation of the Sevan-Akera-Qaradagh collisional geo-suture (Figs. 4, 10g). (d) Paleogene synchronous Andean-arc and back-arc stages, characterized by calc-alkaline volcanism(north of the Zagros geo-suture) and alkali basalt volcanism (northwesternIran), respectively. (Apparentlythe intraplate block faulting and predominantlyalkali basaltic volcanism(back-arc spreading stage) led to the formation of the south Caspianoceanic crust (Figs. 5, 10h).) (e) Neogenecollisional orogenyin southwestIran and formation of the Zagros collisional geo-suture, and overall shortening and thickening of the Iranian continental crust (Fig. 10i). (f) The south Caspian depression, with its modified oceanic crust, remaining open and subsiding further perhapsas a result of the continuedcoolingof its oceanic substratum and overthrusting of the bordering foldthrust mountainbelts (Fig. 10i). The assumedmodifiedocean-crust region of the south Caspiandepression, whichis not seismically active, is surrounded by arcuate active fold-thrust belts with a high seismic activity level. This study has demonstrated that the present physiographicand tectonic features are strongly influenced by the older tectonic elements. The axial direction of the arcuate Alborz and the Talesh fold-thrust belts bordering the trapped modified ocean crust was inherited at the onset of the regional compressional regime. These belts follow the shape of the trapped oceanic basement (which behaved as a rigid block) and apparentlystill control the orientation of the contemporaryfolding. Theactive tectonics of the area is dominatedby compressionalregime, and seismic activ- ity is widespread along several inherited mountainbordering reverse faults. Regional Pliocene-Quaternary geology,active faulting, and fault-plane solution of the earthquakes show predominantly reverse faulting and, therefore, crustal shortening and thickeningof the area, as well as the whole Persian plateau. With the limited data at hand, it is hopedthat the present reviewand the newdata presented in this paper on the bordering active reverse faults and the active tectonics of the region will initiate somefurther detailed study of the region. Acknowledgments This work was supported by the Departmentof Earth Sciences, CambridgeUniversity, and the Geological (and Mineral) Survey of Iran. I wouldlike to thank Berberian, G. C. P. King, K. Louden, D. P. McKenzie, P. Molnar, and C. Soufleris for critically reading the manuscript and for valuable discussions and comments. I benefited from discussions with P. C. England, D. Karig, R. H. Sibson, M. Sinha, S. Tanner and C. Williams. I acknowledge with thanks the comments received from X. LePichon. 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