Blueschists of the Amassia-Stepanavan Suture Zone (Armenia): linking Tethys subduction history from...
Transcript of Blueschists of the Amassia-Stepanavan Suture Zone (Armenia): linking Tethys subduction history from...
ORIGINAL PAPER
Blueschists of the Amassia-Stepanavan Suture Zone (Armenia):linking Tethys subduction history from E-Turkey to W-Iran
Yann Rolland Æ Sandra Billo Æ Michel Corsini ÆMarc Sosson Æ Ghazar Galoyan
Received: 11 June 2007 / Accepted: 10 November 2007 / Published online: 11 December 2007
� Springer-Verlag 2007
Abstract The Amassia–Stepanavan blueschist-ophiolite
complex of the Lesser Caucasus in NW Armenia is part of an
Upper Cretaceous-Cenozoic belt, which presents similar
metamorphic features as other suture zones from Turkey to
Iran. The blueschists include calcschists, metaconglomer-
ates, quartzites, gneisses and metabasites, suggesting a
tectonic melange within an accretionary prism. This blues-
chist melange is tectonically overlain by a low-metamorphic
grade ophiolite sequence composed of serpentinites, gabbro-
norite pods, plagiogranites, basalts and radiolarites. The
metabasites include high-P assemblages (glaucophane–
aegirine–clinozoisite–phengite), which indicate maximal
burial pressure of *1.2 GPa at *550�C. Most blueschists
show evidence of greenschist retrogression (chlorite—
epidote, actinolite), but locally epidote-amphibolite condi-
tions were attained (garnet—epidote, Ca/Na amphibole) at a
pressure of *0.6 GPa and a temperature of *500�C. This
LP–MT retrogression is coeval with exhumation and nappe-
stacking of lower grade units over higher grade ones.40Ar/39Ar phengite ages obtained on the high-P assemblages
range between 95 and 90 Ma, while ages obtained for
epidote-amphibolite retrogression assemblages range within
73.5–71 Ma. These two metamorphic phases are significant
of (1) HP metamorphism during a phase of subduction in the
Cenomanian–Turonian times followed by (2) exhumation in
the greenschist to epidote-amphibolite facies conditions
during the Upper Campanian/Maastrichtian due to the onset
of continental subduction of the South Armenian block
below Eurasia.
Keywords Armenia � Lesser Caucasus � Blueschists �HP metamorphism � 40Ar/39Ar dating
Introduction
The Alpine–Himalayan tectonic belt forms a puzzling
network of suture zones and micro-blocks from the eastern
Mediterranean area to the NW Himalayan belt (Sengor and
Yilmaz 1981; Tirrul et al. 1983; Ricou et al. 1985; Dercourt
et al. 1986; Ricou 1994; Okay and Tuysuz 1999; Stampfli
and Borel 2002, Fig. 1). From the above studies, the time
of ocean subductions, obductions, micro-plate accretions
and exhumations ranges mostly from the Upper Cretaceous
to the Eocene in that area. Still, it remains difficult to
correlate units from Turkey to Iran, because key geochro-
nological and metamorphic data still lack from the main
presumed suture zones. Further, lateral correlations of
continental terranes of presumed Gondwanian origin are
still controversial. This paper describes a High Pressure
(HP) complex, the Amassia-Stepanavan Blueschist Ophi-
olite complex (ASBOC) located in northern Armenia, from
which structural and Pressure–Temperature–time (P-T-t)
constraints are provided. These data are further used to
discuss lateral correlations between the known parts of the
Neo-Tethyan suture zone complex, in Turkey and Iran.
Y. Rolland (&) � S. Billo � M. Corsini � M. Sosson �G. Galoyan
Geosciences Azur, UMR 6526,
Universite de Nice-Sophia Antipolis CNRS,
Parc Valrose, 06108 Nice cedex 2, France
e-mail: [email protected]
S. Billo
DTP, UMR 5562, Observatoire Midi-Pyrenees,
14, avenue Edouard Belin, 31400 Toulouse, France
G. Galoyan
Institute of Geological Sciences,
National Academy of Sciences of Armenia,
24a Baghramian avenue, Yerevan 375019, Armenia
123
Int J Earth Sci (Geol Rundsch) (2009) 98:533–550
DOI 10.1007/s00531-007-0286-8
Between these two parts of the Neo-Tethyan belt, detailed
P-T constraints and HP metamorphic ages are scarcely
obtained on such rocks, so it remains difficult to establish
clear relationships with the East Mediterranean history to
that of the more documented Himalayan belt. In this con-
text, the relationships of the South Armenian Block with
Taurides to the West and Iran to the East are critical for
lateral correlations. In the present study we evaluate the
time of the South Armenian Block accretion with Eurasia
and the age of exhumation of the suture zone complex,
based on geological, P-T and 40Ar/39Ar phengite data.
Geological setting
The South Armenian Block is comprised between Turkey
and Iran blocks (Fig. 1). In the following, we summarize
the occurrences and known ages of HP metamorphism in
these two regions.
Turkey is formed by mainly four blocks, separated by
three main HP belts (e.g., Okay and Tuysuz 1999), namely:
(1) The Intra-Pontide suture, separating the Istambul
zone from the Sakarya Block to the NW;
(2) The Izmir-Ankara suture prolonged to the East by the
Izmir-Ankara-Erzincan suture separating the Sakarya
Block from the Anatolide-Taurides Block in the
centre;
(3) The Assyrian-Zagros suture separating the Anatolide–
Taurides from the Arabian plate to the SE and the
Pamphylian Suture in SSW Turkey.
In Turkey, the Intra-Pontide suture in the Sakarya
Zone preserves Permo-Triassic subduction complexes
PlatformEuropean margin (Pontides, “Sakarya series”)European margin including arc seriesMetamorphic massifsTauride-Anatolide and Armenian block(s)and accreted/obducted ophiolitesSuspected oceanic crust
Strike slip fault Thrust
SAS: Sevan-Akera SutureCACC: Central anatolian crystalline complex(Kirsehir massif)EAF: East anatolian fault(reactivating the Intra-Pontide suture)GC: Great CaucasusIAES: Izmir - Ankara - Erzinkan sutureIPS: Intra-Pontide SutureIZ: Istanbul ZoneKO: Khoy OphioliteMM: Menderes massifNAF: North anatolian faultSA: South armenian block
Studied area
East european Platform
Scythian Platform
Arabian Platform
Caspian Sea
Black Sea
45°N
40°N
35°N
25°E 30°E 35°E 40°E 45°E 50°E
45°N
CACC
MM
VR
GC
EAF
KO
SA S
Sanandaj-Sirjan zone
IAES
SAS
NAF
Zagros Suture
Assyrian
Suture
IPSIZ
V: Van LakeS: Sevan LakeR: Rezaiyeh Lake
Fig. 1 Tectonic map of the Middle East–Caucasus area, with main blocks and suture zones, after Avagyan et al. (2005), modified
534 Int J Earth Sci (Geol Rundsch) (2009) 98:533–550
123
unconformably overlain by Jurassic sediments (e.g., Okay
and Tuysuz 1999; Robertson et al. 2004; Okay and
Goncuoglu 2004).
The Izmir-Ankara suture is underlined by Mid- to Upper
Cretaceous HP–LT rocks. Dating of HP rocks from the
Kargi massif (Fig. 1) provided mean 40Ar/39Ar phengite
age of 104.5 ± 7.2 Ma (Okay et al. 2007), while ages
between 101 and 85 Ma were obtained with the same
method in the NW part of the Izmir-Ankara suture (Okay
et al. 1998; Sherlock et al. 1999). In contrast, Mid Paleo-
cene to Eocene ages were obtained in the southwest Izmir
suture (Rimmele et al. 2003).
Blueschists have also been found along the Zagros
Suture in SE Turkey (Oberhansli, pers. com.), but they
remain undated. Along the probable lateral continuation of
this SE Turkey suture, in western and southern Iran, sub-
duction age is constrained by the emplacement of supra-
subduction plagiogranites dated at 93–88 Ma by K–Ar
(Kananian et al. 2001), and by Mid–Upper Cretaceous40Ar/39Ar ages (Agard et al. 2006).
Further east, in Eastern Iran, blueschist to eclogite facies
metamorphism is also described (Fotoohi Rad et al. 2005),
and is ascribed to the age range 83–55 Ma (Tirrul et al.
1983), which correlates with ages of Tethyan subduction in
the Himalayan belt, which ends with the onset of Indian
continent subduction at c. 55 Ma (de Sigoyer et al. 2000).
The Sevan-Akera ophiolite belt
In the Lesser Caucasus belt of Armenia, the Sevan-Akera
suture (Aslanyan 1958; Gabrielyan 1959; Paffenholtz
1959) is the probable eastward extension of the Izmir-
Ankara-Erzincan suture in Anatolia (see above and Figs. 1,
2). It has been interpreted as a suture zone since the works
of Milanovski (1968). This suture is the northern tectonic
boundary of the South Armenian Block, which is presumed
of Gondwanian origin (Knipper 1975; Knipper and Khain
1980) with Eurasia. The South Armenia Block is a possible
eastward extension of the Eastern Taurides (Tauride-
Anatolide Block), and the ‘‘Eurasian margin’’ in Armenia/
Georgia may correspond to the Eastern Pontides/Sakarya
Zone. The geographic proximity and similarity in the
geological units would suggest a parallel evolution
Fig. 2 Sketch geological map
of Armenia, with location of the
studied area
Int J Earth Sci (Geol Rundsch) (2009) 98:533–550 535
123
between the northeastern Anatolia and Armenia (e.g.,
Knipper 1975; Adamia et al. 1980), but the age and origin
of the Armenian and Georgian Crystalline basements are
still not precisely constrained.
Ophiolites have been described in association with
blueschists and amphibolite facies metamorphic rocks
(Melikyan 1966; Knipper 1975; Sokolov 1977; Aslanyan
and Satian 1977; Morkovkina et al. 1977; Aghamalyan
1978, 1981; Knipper and Khain 1980; Abovyan 1981;
Zakariadze et al. 1983; 1990; Meliksetyan et al. 1984;
Tsameryan et al. 1988; Silantiev et al. 1996; Aghamalyan
2004). The age of oceanic closure and suturing is presumed
to be Upper Cretaceous on the basis of the unconformity of
platform-type Upper Coniacian limestones on the ophiolite
(Kniper 1975; Sokolov 1977), but as will be emphasized in
the present paper this age corresponds to the age of ophi-
olite obduction on the South Armenian Block, and not to
the suturing of the latter with Eurasia. In the Stepanavan
area, which is under study in this paper (Fig. 3), previous
works undertaken by Aghamalyan (1978, 1981) have
shown the following structural succession: (1) a basal part
comprising pelites interstratified with dacitic lava flows,
and hydrothermalized and silicified serpentinites (‘‘listwe-
nites’’); (2) a glaucophane-schist unit including blocks of
garnet amphibolites thrusted over (1); (3) ophiolitic
melanges comprising ultramafites, volcanic rocks and
radiolarites; (4) a conglomeratic and overlying limestone
unit overlying uncomformably the unit (3); (5) Paleocene-
Eocene series thrusted by (1–4). The age of the series (1–4)
is attributed a Lower to Upper Cretaceous age by analogy
with the neighbouring Amassia massif where brachiopods
have been described in limestones interstratified within
lava flows (Hakobyan 1976). Accordingly, whole-rock K–
Ar ages were obtained on blueschists, ranging from 90 to
80 Ma (Meliksetyan et al. 1984 and references therein).
However, these ages do not constrain neither the ophiolite
protolith age nor any precise metamorphic age of minerals,
from which only 40Ar/39Ar or U/Pb in relationship with PT
path determination could help resolve the complex history.
In the following, we provide a new description of the area,
and propose a different interpretation for the structure and
age of units. Concerning the issue of the age of meta-
morphic rocks, 40Ar/39Ar datings are provided in the
following ‘‘40Ar/39Ar dating’’ section.
Field analysis and sampling
On the basis of previous geological work in the area of
Stepanavan, we conducted two field campaigns for a pre-
cise mapping of the various units of the ASBOC in 2003
and 2004. A simplified version of the geological map is
presented in Fig. 3.
Lithologies
We observed five superposed units in the ASBOC, from
base to top (Figs. 3, 4):
(1) The lower structural unit is the ‘‘Blueschist Unit’’. It
is mainly composed of a strongly retrogressed calc-
schist matrix including boudins of metavolcanic rocks
and metasediments. Metavolcanics are glaucophane-
bearing mostly deriving from basalts. In rare loca-
tions, pillow-basalts and volcanic breccia can be
recognized within the Blueschist Unit. Metasediments
are comprised of micaschists, marbles, metaconglom-
erates, quartzites, and rare gneiss blocks. This
association suggests an active margin environment
where detrital deposits are intensely reworked an
accretionary prism.
(2) Structurally above the blueschists, the ‘‘Ophiolite
Unit’’ is a low-grade and complete ophiolite
sequence. A complete description of the ophiolite
series is provided by Galoyan et al. (2007), and main
features are briefly summarized below. This unit is a
preserved ophiolite section and not an ophiolitic
melange. It is composed of slightly metamorphozed
δ
V
V
V
V
V
V
V
V
V
V
V
V
STEPANAVAN
1 km
41°00’ 41°00’
44°23’44°16’
44°11’
δ
40°51’
V
AR.04.07
N
UVSU Volcano-sedimentary rocks (Paleogene)
Andesitic volcanites & volcano-sedimentary rocks
graywackesLimestones
Ophiolite Unit (LOT type : UB; basalts, gabbros, plagiogranites & radiolarites) - Upper Jur. to Lower Cret.
Conglomerates and fine sandstones
Blueschists Unit
Andesite-Dacite volcanics (Plio-IV)
Lower to Upper Cretaceous(LVSU)
Normal faults ThrustsFolds
A
B
AB
AR.03.57-58
AR.04.14
AR.03.50
AR.03.52
V
V
V
V
V
V
V
V
V VV
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
V
40°51’
V
AR.03.56
AR.03.54
Fig. 3 Geological map of the Stepanavan Blueschist Ophiolite
complex (ASBOC). d unconformities
536 Int J Earth Sci (Geol Rundsch) (2009) 98:533–550
123
serpentinites, gabbro-norite pods, plagiogranites, bas-
alts and radiolarites. The observed geometrical
relationships among lithologies include (a) sediments
unconformably lying on serpentinites, (b) small
relative volume of magmatic rocks versus serpenti-
nites, (c) cross-cutting plagiogranite dykes emplaced
within extensional shear zones. All the above features
suggest a Lherzolite Ophiolitic Type (LOT) sequence.
In the North, we observed the following succession:
serpentinite, flaser-gabbro basalt and radiolarites (see
lithological profile ‘‘log A’’ in Fig. 4). Whereas, in
the South we principally observed serpentinites
crosscut by pods of cumulative plutonic rocks com-
positionally evolving from gabbro-norites to
plagiogranites (‘‘log B’’ in Fig. 4). Dating of radio-
larian faunas interbedded in the pillow lavas provided
an Upper Jurassic age (Danelian et al. 2007).
Therefore, most of the ophiolite series protolith
should be Upper Jurassic as in the Sevan area
(Zakariadze et al. 1983).
(3) In stratigraphic contact with the ‘‘Ophiolite Unit’’, the
‘‘Lower Volcano-Sedimentary Unit’’ (or LVSU) is a
thick and highly variable succession of calc-alkaline
volcanic material and related sediments. It comprises
basal conglomerates or quartzites, red pelites,
limestones and finally grauwackes or basaltic to
andesitic lavas. Depending on the area, we observed
either: (1) the succession of a thick sandstone/
conglomerate layer and black graywackes interlay-
ered with several decameter-large limestone strata
(North, see ‘‘log A’’ in Fig. 4), or (2) the succession
quartzite and conglomeratic limestones, a reduced
pile of pelites, and a large thickness of pillowed
andesites, basaltic andesites and andesitic tuff (see
‘‘log A’’ in Fig. 4). The possible age range for this
succession is Lower Cretaceous-Paleocene, as it lies
unconformably on the ophiolite and predates the
following Paleocene-Eocene unconformity.
(4) The upper section is formed by the ‘‘Upper Volcano-
Sedimentary Unit’’ (UVSU), also in stratigraphic
(unconformity) contact with the below unit (LVSU).
It is comprised of basal conglomerates with volcanic
blocks and glauconite, tuffaceous limestones, and
andesites to rhyolites lavas. This series is presumably
Paleocene–Eocene (in reference to the Geological
Map of Armenia 1/5000 000) and lies unconformably
on the folded LVSU.
(5) Finally, an undated (probably Plio-Quaternary)
sequence of basalt lava flows and grauwacky material
lies just north to the blueschist windows. The down-
0 642 8
2000
3000
1000
(m)
blueschist unit
ophiolitic unitvolcano-sedimentaryUpper Cretaceous
unit(LVSU)
(km)
vvv
vv
v
vv v
v
foliation
δ
δUnconformity
v
South North
δUnconformity
Log B Log A
Log A Log B
blue-schists
metabasitesserpentinites
gabbros
basaltsradiolarites
sandstones & conglomerates
siltstones & grauwackes
limestones
siltstones & grauwackes
serpentinites
gabbros
basaltssandstones & limestones
siltstones & grauwackes
andesites
sandstones & limestones
andesites
metapelitesmarbles
Neogene volcanics(Plio-IV)
Paleogene volcanics(UVSU)
Fig. 4 Geological cross-section of the ASBOC, and lithological profiles in the northern and southern parts of the section. The location of the
section is indicated on Fig. 2
Int J Earth Sci (Geol Rundsch) (2009) 98:533–550 537
123
throw of the series is ascribed to N-dipping normal
faults, which crosscut the ASBOC on its northern rim
(Fig. 4).
Structure
At the geological map scale, the overall structure is that of a
folded nappe pile (Fig. 4). The blueschist unit appears
within two tectonic windows of ±1 km2. Exhumation of the
blueschists is partly due to the presence of steep reverse
north-verging faults. However, the rounded shape of the
windows, underlined by the metamorphic foliation can be
interpreted as ‘‘dome-like’’ structures. The domes presum-
ably formed by the succession of two phases of folding as is
emphasized by macro and micro-tectonic analysis. The
measurement of mineral and stretching lineations and
associated metamorphic foliations shows that at least two
ductile phases have deformed the ASBOC. A first genera-
tion of ductile structures was formed in the blueschist facies
as glaucophane + phengite minerals underline a first sub-
horizontal lineation striking N90–110�E, while a second
generation of greenschist facies (epidote, actinolite)
minerals form a mineral lineation striking N–S to NE–SW
with a steep dip (Fig. 5c). Main fold axes strike
N100-120�E on the map (Fig. 3). Similar orientations were
measured in the field on microfolds (Fig. 5a, b). Fold axes
are nearly horizontal and axial fold planes are vertical to
south-dipping. Both greenschist and blueschist facies foli-
ations are folded within N120�E folds as shown by the
computation of all foliation poles on stereographic projec-
tions (Fig. 5b). Therefore, fold structures indicate a late
tectonic event, featured by NNE–SSW sub-horizontal
shortening. This shortening direction agrees with that of
mineral lineations of the second phase, which indicates that
folding occurred later but in the same tectonic context as
nappe emplacement. Due to the intense strain and LP–MT
metamorphic overprint of this late phase it remains difficult
to identify the sense of shear related to the first HP mineral
lineation. The presence of dome structures and E–W
blueschist grade mineral lineations suggest that tectonic
motions might have been more E–W in the former HP strain
phase. However, no clear shear sense indicators could be
observed from field and thin section analyses, thus it
remains difficult to conclude about the sense of shear during
phases 1 and 2. Latest deformation is featured by NW–SE
north dipping normal faults crosscutting the ASBOC.
Fold axes
Greenschist facies stretching lineations
Blueschist facies stretching lineations
Poles to bedding
Poles to schistosity (greenschist facies)
Poles to schistosity (blueschist facies)
A
Fold Axis 105W6
Fold axis122E15
Stretching lineation. 1=E-WStretching lineation. 2=N-S
Legend:
C
B
Fig. 5 Wulf stereonets in lower
hemisphere, presenting the
orientations of main
microstructures. a Poles to
bedding; b poles to
metamorphic foliation; c poles
to mineral lineations
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Tectonic events
The structure and lithologies that were observed suggest
the following succession of tectonic events:
(1) A first high-P phase in blueschist facies conditions:
Tectonic motion at HP is supported by the orientation
of the HP stretching + mineral lineations. If these HP
lineations did not undergo any rotation at lower P, the
E–W strike of lineations could correspond to the
transport direction of subducted materials, which
would suggest a N–S trending subduction zone (and
thus an E or W directed subduction) at this stage.
(2) A second phase of top to the NE shearing: Tectonic
motion is related to the nappe-stacking event con-
temporaneous to the greenschist/epidote-amphibolite
facies. The HP units have been tectonically uplifted
during this event.
(3) In the same tectonic context, the nappe stack is folded
by a NNE–SSW trending shortening, still related to
top to the NNE sense of shear. The shortening related
to WNW–ESE folding resulted in uplift, exhumation
and erosion of the nappe stack.
(4) The nappe stack is unconformably overlain by the
Paleocene volcano-sedimentary sequence, which ori-
gin could be related to the onset of the collision.
(5) Post Paleocene (probably Eocene) N–S shortening is
emphasized by the long wavelength folds drawn by
this latter Paleocene volcano-sedimentary sequence.
(6) Later deformation stage is the relative uplift of the
blueschist sole, by denudation under extensional NE
dipping subvertical faults.
Analytical techniques
Mineral compositions were determined by electron probe
microanalysis (EPMA). The analyses are presented in
Table 1. They were carried out using a Cameca Camebax
SX100 electron microprobe at 15 kV and 1 nA beam
current, at the Blaise Pascal University (Clermont-Ferrand,
France). Natural samples were used as standards.
Geochronology was undertaken by laser 40Ar/39Ar dat-
ing of white micas. Results are presented in Table 2. White
micas were analyzed by EPMA prior to dating in order to
check mineral compositions homogeneity. Grains less than
1 mm were separated by careful selection by hand-picking
under a binocular microscope to prevent the presence of
altered grains. The samples were then irradiated in the
nuclear reactor at McMaster University in Hamilton
(Canada), in position 5c, along with Hb3gr hornblende
neutron fluence monitor, for which an age of 1072 Ma is
adopted (Turner et al. 1971). The total neutron flux density
during irradiation was 9.0 9 1018 neuton cm-2. The esti-
mated error bar on the corresponding 40Ar*/39ArK ratio is
±0.2% (1r) in the volume where the samples were set. All40Ar/39Ar measurements were proceed in the University of
Nice-Sophia Antipolis (UMR Geosciences Azur). Analyses
of phengite grains were undertaken by step heating with a
50 W CO2 Synrad 48-5 continuous laser beam. Measure-
ment of isotopic ratios was done with a VG3600 mass
spectrometer equipped with a Daly detector system.
Detailed procedures are described in Jourdan et al. (2004).
The typical blank values for extraction and purification of
the laser system are in the range 4.2–8.75, 1.2–3.9, and 2–6
cc STP for masses 40, 39 and 36, respectively. Mass dis-
crimination was monitored by regularly analyzing air
pipette volumes. Decay constants are those given by Stei-
ger and Jager (1977). Uncertainties on apparent ages are
given at the 2r level and do not include the error on the40Ar*/39Ark ratio of the monitor.
The criteria generally used in the laboratory for defining
a ‘‘plateau’’ age are the following: (1) it should contain at
least 70% of total 39Ar released; (2) there should be at least
three successive step-heating fractions in the plateau; (3) the
integrated age of the plateau (weighted average of apparent
ages of individual fractions comprising the plateau) should
agree with each apparent age of the plateau with a 2r error.
In this study, we also consider smaller plateaus than 70% of
total 39Ar, because the lower temperature age spectra are
generally lowered by a 39Ar loss effect.
Metamorphism of the Stepanavan Blueschists
High-P relics have been found within metabasites.
Metapelites appear to be Ca-rich and altered during their
retromorphosis, so we have focused our study on the
metabasic lithologies (CFMASH system).
Petrography
Stepanavan metabasic blueschists preserve several par-
ageneses, which are representative of the successive steps
of high-P metamorphism (see photographs on Fig. 6).
Samples, such as AR 03 50, show HP–LT parageneses
defined by (1) clinopyroxene—glaucophane – quartz
– pyrite ± phengite ± clinozoisite. HP–LT conditions are
also defined by the assemblage (2) glaucophane—clino-
zoisite ± phengite ± quartz. Clinopyroxene appears as
small dark green globular grains and glaucophane occurs as
equant porphyroblasts up to 2 mm in length. Phengite and
clinozoisite form elongated grains that define the foliation.
Quartz is not very abundant and commonly shows undulose
extinction.
Int J Earth Sci (Geol Rundsch) (2009) 98:533–550 539
123
Table 1 Representative electron-microprobe mineral analysis of blueschist samples
Sample AR 03 50 Sample AR 03 52a Sample AR 04 14 Sample AR 03 57
Aeg cro ph czo gl Cro czo grt rim1 grt core grt rim2 prg chl alb czo czo gl ph
SiO2 53.21 54.84 50.49 37.57 55.91 55.60 37.61 37.87 37.29 37.46 42.79 25.37 67.16 37.25 38.80 56.86 51.29
Al2O3 3.01 8.15 26.10 23.09 9.59 5.88 21.50 21.00 20.81 21.16 15.10 19.22 20.91 22.37 28.35 11.66 28.52
MgO 1.37 4.19 3.11 0.01 8.02 7.34 0.02 2.98 1.79 2.92 8.29 14.69 0.00 0.01 0.03 9.41 3.68
FeO 25.07 23.10 4.81 12.70 15.69 19.96 14.66 30.55 26.23 29.61 17.50 27.80 0.27 12.12 6.19 11.28 2.12
MnO 0.04 0.07 0.02 0.49 0.19 0.08 0.25 1.50 4.81 1.70 0.16 0.37 0.03 0.24 0.13 0.09 0.00
TiO2 0.05 0.08 0.18 0.15 0.13 0.05 0.06 0.10 0.20 0.13 0.51 0.02 0.01 0.06 0.25 0.17 0.21
CaO 3.89 0.53 0.03 22.64 1.02 0.81 22.82 6.61 7.79 6.59 9.17 0.12 1.57 22.52 24.10 1.40 0.03
Na2O 11.35 6.93 0.22 0.02 6.77 6.98 0.02 0.05 0.07 0.03 2.98 0.03 11.02 0.04 0.01 6.46 0.47
K2O 0.00 0.03 10.50 0.00 0.01 0.03 0.01 0.00 0.05 0.01 0.28 0.04 0.12 0.00 0.00 0.00 10.54
Total 98.00 97.92 95.46 96.67 97.32 96.71 96.95 100.67 99.05 99.62 96.78 87.67 101.08 94.61 97.84 97.33 96.86
Nb oxygen 6 23 11 12 23 23 12 12 12 12 23 14 8 12 12 23 11
Si 2.01 7.90 3.40 3.00 7.85 7.97 3.01 3.00 3.01 2.99 6.17 2.71 2.33 3.03 3.00 7.88 3.36
Al 0.13 1.38 2.07 2.17 1.59 0.99 2.03 1.96 1.98 1.99 2.57 2.42 0.86 2.15 2.58 1.90 2.20
Mg 0.08 0.90 0.31 - 1.68 1.57 - 0.35 0.22 0.35 1.78 2.34 - - - 1.94 0.36
Fe 0.79 2.78 0.27 0.85 1.84 2.39 0.98 2.02 1.77 1.98 2.11 2.48 0.01 0.83 0.40 1.31 0.12
Mn – 0.01 0.00 0.03 0.02 0.01 0.02 0.10 0.33 0.12 0.02 0.03 – 0.02 0.01 0.01 –
Ti – 0.01 0.01 0.01 0.01 0.01 – 0.01 0.01 0.01 0.06 – – – 0.01 0.02 0.01
Ca 0.16 0.08 – 1.94 0.15 0.12 1.96 0.56 0.67 0.56 1.42 0.01 0.06 1.97 2.00 0.21 –
Na 0.83 1.94 0.03 – 1.84 1.94 – 0.01 0.01 – 0.83 0.01 0.74 0.01 – 1.73 0.06
K – 0.01 0.90 – – 0.01 – – 0.01 – 0.05 0.01 0.01 – – – 0.88
Sample AR 03 58 Sample AR 03 52b
gl ph gl trem czo alb ph chl
SiO2 56.69 50.27 57.47 52.09 38.05 69.51 49.61 25.40
Al2O3 8.93 27.07 7.77 1.77 23.35 20.27 25.67 19.35
MgO 9.29 2.89 9.11 6.55 0.02 0.00 3.11 19.18
FeO 14.54 4.96 15.89 26.44 12.77 0.13 5.13 23.54
MnO 0.04 0.02 0.11 0.34 0.31 0.00 0.05 0.24
TiO2 0.06 0.22 0.05 0.01 0.18 0.00 0.31 0.00
CaO 0.73 0.03 0.50 3.32 22.81 0.24 0.03 0.07
Na2O 6.89 0.28 7.08 4.92 0.00 12.01 0.20 0.00
K2O 0.01 10.46 0.00 0.11 0.02 0.03 10.66 0.01
Total 97.16 96.20 97.99 95.54 97.51 102.20 94.76 87.78
Nb oxygen 23 11 23 23 12 8 11 14
Si 7.91 3.36 7.99 7.85 3.01 2.37 3.37 2.63
Al 1.47 2.13 1.27 0.31 2.18 0.82 2.05 2.36
Mg 1.93 0.29 1.89 1.47 – – 0.31 2.95
Fe 1.70 0.28 1.85 3.33 0.84 – 0.29 2.03
Mn 0.01 – 0.01 0.04 0.02 – – 0.02
Ti 0.01 0.01 0.01 0.00 0.01 – 0.02 0.00
Ca 0.11 0.00 0.07 0.54 1.93 0.01 0.00 0.01
Na 1.86 0.04 1.91 1.44 – 0.80 0.03 –
K – 0.89 – 0.02 – – 0.92 –
aeg aegyrine, alb albite, chl chlorite, Cro crossite, gl glaucophane; grt garnet, ph phengite, prg pargasite; trem tremolite, czo clinozoisite
540 Int J Earth Sci (Geol Rundsch) (2009) 98:533–550
123
Table 2 Phengite 40Ar/39Ar dating results from the ASBOC blueschists
Sample N� and Step N� Laser power (mW) Atmospheric content (%) 39Ar (%) 37ArCa/39ArK
40Ar*/39ArK Age (Ma ± 1r)
HP phengite samples
AR-03-56(1)
1 375 63,32 3,64 0,16 2,03 60,6 ± 1,3
2 396 13,83 6,15 0,09 2,56 76,0 ± 0,5
3 411 9,53 2,94 0,06 2,85 84,4 ± 1,1
4 426 5,64 23,01 0,08 3,07 90,8 ± 0,3
5 431 4,27 10,31 0,07 3,10 91,4 ± 0,4
6 437 3,64 14,09 0,12 3,15 93,0 ± 0,3
7 444 4,85 8,46 0,47 3,18 93,8 ± 0,4
8 458 7,13 8,22 1,64 3,19 94,1 ± 0,4
9 800 8,98 23,18 0,86 3,25 95,9 ± 0,3
AR-03-56(2)
1 342 35,72 5,77 0,12 2,11 61,7 ± 0,8
2 350 9,64 3,91 – 2,50 72,7 ± 0,7
3 359 6,69 14,00 0,10 2,82 81,8 ± 0,3
4 364 3,48 16,58 0,13 3,02 87,4 ± 0,2
5 369 2,83 19,78 0,19 3,12 90,3 ± 0,2
6 374 3,34 5,25 0,18 3,13 90,7 ± 0,4
7 382 5,81 10,12 0,86 3,17 91,8 ± 0,3
8 405 6,47 6,02 1,22 3,17 91,8 ± 0,4
9 442 6,67 4,68 1,35 3,19 92,4 ± 0,5
10 509 5,20 10,81 1,06 3,24 93,6 ± 0,3
11 549 10,17 2,45 1,95 3,30 95,3 ± 0,7
12 800 26,30 0,63 7,14 3,24 93,8 ± 3,2
AR-03-58(1)
1 340 9,53 5,07 – 2,48 72,2 ± 0,6
2 350 4,38 7,54 – 2,82 82,0 ± 0,5
3 358 1,80 9,84 – 2,99 86,7 ± 0,5
4 364 – 7,59 – 3,06 88,7 ± 0,6
5 369 0,67 11,72 – 3,10 89,8 ± 0,4
6 376 0,85 18,90 0,09 3,14 91,0 ± 0,3
7 381 0,32 9,52 0,13 3,19 92,3 ± 0,4
8 392 0,56 13,61 0,10 3,20 92,5 ± 0,4
9 409 2,56 6,59 0,51 3,16 91,4 ± 0,6
10 440 2,54 4,65 0,98 3,16 91,4 ± 0,7
11 800 2,65 4,98 3,07 3,11 90,2 ± 0,7
AR-04-07
1 350 17,00 10,26 0,01 2,86 86,2 ± 5,8
2 362 – 31,37 – 3,18 95,6 ± 1,6
3 376 – 39,96 – 3,18 95,5 ± 1,2
4 386 52,66 1,14 – 1,31 39,9 ± 63,6
5 424 6,76 10,52 – 2,93 88,3 ± 8,6
6 800 – 6,75 – 3,16 94,9 ± 7,5
LP–MT phengite samples
AR-03-54
1 350 16,54 19,46 0,02 2,26 66,0 ± 0,4
2 360 7,85 6,41 – 2,37 69,2 ± 0,6
3 368 9,19 8,63 – 2,37 69,0 ± 0,6
Int J Earth Sci (Geol Rundsch) (2009) 98:533–550 541
123
LP–MT parageneses are featured by (3) garnet–chlo-
rite—Ca/Na amphibole ± clinozoisite ± albite. Garnet is
partially replaced by pale-green chlorite. Amphibole occurs
as thin green crystals showing the foliation.
LP–LT parageneses are defined by (4) Ca/Na amphi-
bole–clinozoisite – chlorite – albite ± phengite.
Mineral chemistry
EPMA analysis of clinopyroxene shows that it is of
Aegirine composition (Acmite 0.66–0.75; Augite 0.11–
0.17; Jadeite 0.13–0.18, Table 1).
In LT–HP assemblages, blue amphibole is mainly of
glaucophane-crossite type (0.2 \ Na (A) \ 0.5; Fig. 7;
Table 1). In MT–LP assemblages, the amphiboles are of
pargasite composition (Si = 6.3–6.4; XMg = 0.3–0.4;
Table 1), while in LT–LP assemblages compositions are
within the tremolite-actinolite field.
Phengite is more celadonite-rich in LT–HP assemblages
(Si: 3.37–3.43) than in the LP assemblages (Si: 3.1–3.2;
Table 1).
In HP-LT assemblages, analysed epidote is of zoisite-
clinozoisite type (Table 1). In LP assemblages, epidote is
close to the pistascite pole.
The composition of garnet within LP–MT assem-
blages is featured by prograde zoning (Table 1; Fig. 8),
with increasing almandine (from 59.5 to 66.5%) and
pyrope (from 7 to 12%) contents and decreasing spes-
sartine (from 11 to 3.5%) and grossular (from 23 to
18.5%) contents towards mineral rims. This pattern is
indicative of thermal increase during retrogression (Spear
1988).
Alteration of garnet and amphibole into Fe-rich chlorite
(XFe = 0.43–0.49) is frequently observed.
Thermobarometry and PT paths
Average PT domains of studied assemblages can firstly be
deduced from the stability fields of main crystallizing
minerals. The main mineral reactions and PT stability
fields of mineral parageneses for metabasites in HP–LT
conditions are shown on Fig. 9 and Table 3. The peak
burial conditions are out of the lawsonite stability field, as
is evidenced by textural equilibrium of clinozoisite-bearing
assemblages and the absence of any lawsonite psewhich is
in agreement with temperatures [400�C at peak P (Hein-
rich and Althaus 1988; Fig. 9). The presence of
glaucophane implies maximal temperatures of 550�C at
peak P (Carman and Gilbert 1983). The jadeite content in
clinopyroxene (15–20%) provides a minimum pressure
estimate of 0.9 GPa, at 450�C, in the absence of albite
(Holland 1980). However, the absence of jadeite-rich
pyroxene in the overall set of thin sections suggests pres-
sures lower than 1.4 GPa. A minimum pressure estimate of
1.1 GPa is provided by the Si content in phengite (Si 3.38–
3.43) in pelitic rocks (gneiss sample AR0407) at 450�C
(Massone and Schreyer 1987). Therefore, the peak P con-
ditions can be approximated at 1.1 B P \ 1.4 GPa, and
400 \ T \ 550�C. These conditions are well within the
field of the epidote blueschist facies (Evans 1990).
Table 2 continued
Sample N� and Step N� Laser power (mW) Atmospheric content (%) 39Ar (%) 37ArCa/39ArK
40Ar*/39ArK Age (Ma ± 1r)
4 373 7,26 10,31 0,06 2,43 70,7 ± 0,6
5 379 5,87 17,37 – 2,54 73,9 ± 0,4
6 405 9,98 5,89 – 2,53 73,7 ± 0,9
7 443 7,87 8,61 – 2,52 73,4 ± 0,6
8 499 7,23 11,52 0,01 2,51 73,2 ± 0,6
9 800 6,03 11,80 0,01 2,52 73,2 ± 0,4
AR-03-58(2)
1 346 41,55 2,20 0,02 2,26 66,7 ± 3,6
2 357 38,30 2,26 0,01 2,27 66,9 ± 3,5
3 368 25,21 2,43 0,01 2,18 64,5 ± 2,9
4 385 30,29 6,96 0,01 2,22 65,7 ± 1,0
5 400 18,76 1,85 0,01 2,35 69,3 ± 4,1
6 416 15,81 11,51 0,01 2,31 68,2 ± 0,6
7 426 13,56 26,98 0,01 2,43 71,8 ± 0,4
8 432 17,26 2,54 0,02 2,36 69,5 ± 2,3
9 448 17,57 3,97 0,02 2,34 69,1 ± 1,8
10 700 17,25 39,30 0,03 2,40 71,0 ± 0,4
542 Int J Earth Sci (Geol Rundsch) (2009) 98:533–550
123
Thermobarometry was performed with multi-equilibria
approach, with the software THERMOCALC (v. 3.1;
Powell and Holland 1988), using the thermodynamic
dataset of Holland and Powell (1998). Thermobarometry
was undertaken in the CFMASH system, to precise the PT
conditions of peak P and of retrogression assemblages.
Only assemblages with textural evidence for equilibrium
were selected. Then, representative mineral analyses were
used. In the case of mineral zoning, as for garnet, only the
rim-rim compositions could be used, which allowed to
derive peak MT retrogression conditions but not the HP
peak conditions. Activities of mineral end-members used
for rock calculations are calculated with the help of the
program AX (T.J.B. Holland). Average temperatures were
calculated for different ranges of pressure and vice versa.
Representative results for the obtained mineral reactions,
fit, and deduced P-T intervals (at 2r) are shown in Table 3.
The calculations based on the HP parageneses provide
PT estimates of P = 1.2 ± 0.15 GPa and T = 545 ± 60�C.
0
10
20
50
60
70
rim
Abu
ndan
ce (
%)
(a)
(b)
(c)
(d)
rimcore
Fig. 8 Compositional profiles of two garnets of the MT–LP assem-
blage (sample AR-04–14; Table 1), with a almandine, b grossular, cspessartine and d pyrope contents. Note the correlated increase of
almandine and pyrope towards the rim, while spessartine and
grossular are enriched in the core of both garnets. Approximate size
of garnets 1 mm
Fig. 6 Microphotographs of studied samples. a Acmite-bearing-HP
blueschist (sample AR-03–50); b commonly observed HP blueschist
sample (sample AR-03–52a); c blueschist retrogressed in LP–MT
conditions (sample AR-04–14). Abbreviations following Kretz (1983)
0
10
20
30
40
50
60
70
80
90
100
0
100 Fe3+ / (Fe3+ + AlVI + Ti)
eF
001+2
eF(/
+ 2)
nM
+g
M+
AR 03 50
AR 03 52a
AR 03 57
AR 03 58
Ferroglaucophane
Glaucophane
Crossite
Riebeckite
Magnesioriebeckite
10090807060504030 2010
Fig. 7 Compositions of analyzed HP amphiboles plotted in the
diagram of Miyashiro (1957). The Fe3+ content was estimated on the
basis of structural formulae of 23 oxygens and 15 cations
Int J Earth Sci (Geol Rundsch) (2009) 98:533–550 543
123
P-T conditions on the LP–MT parageneses (computed with
garnet – chlorite – pargasite – albite – clinozoisite, sample
AR 04 14) are of P = 0.57 ± 0.02 GPa and
T = 505 ± 67�C. P-T conditions obtained on LT–LP
assemblages (computed with tremolite - clinozoisite -
albite - phengite) are variable and all at P \ 0.5 GPa and
T \ 400�C.
These estimates, when plotted on the PT diagram
(Fig. 9), are within the range of PT conditions deduced
from the stability fields of mineral phases discussed above,
and allow to precise the shape of the PT paths. The PT
paths are mostly in two phases: (1) burial and exhumation
within a relatively hot subduction-type geotherm (10–
15�C/km). Rocks were subducted to 40 ± 4 km, and were
exhumed rapidly to (or slightly above) the depth at which
the second (LP–MT) metamorphic event occurred. (2) The
LP–MT event is featured by a slight increase of tempera-
ture of about 100�C, up to *500�C at 0.6 GPa, which is in
agreement with zoning of garnet towards high-Fe, Mg rim
compositions. Peak LP–MT conditions are indicative of a
relaxed geotherm of 19–33�C/km, more in agreement with
a collision-type event, or to heat input related to synsub-
duction extension (e.g. Parrat et al. 2002). This thermal
increase is sensible at the contact between units, where
deformation was the most intense during the superposition
of the low-grade ophiolitic unit over the blueschist unit.
40Ar/39Ar dating
In the section above, maximal temperature conditions
estimated for the HP and LP–MT peaks are slightly above
(to within range) the closure temperature of the K–Ar
system in white mica (400 ± 50�C, Villa 1998). Thus, the40Ar/39Ar dating of white mica in equilibrium with each of
the parageneses allows estimating the crystallization age of
phengite, either (1) at the pressure peak, or (2) during the
LP–MT retrogression peak. For this reason, we selected
micas from samples exhibiting clear textural equilibrium
(1) in the HP metamorphic paragenesis (samples AR 03 56,
AR 03 58 and AR 04 07), and (2) in the LP–MT meta-
morphic paragenesis (samples AR 03 54 and AR 03 58).
Results are shown in Fig. 10 and Table 2.
40Ar/39Ar dating of HP peak phengite
The 40Ar/39Ar spectra of samples AR-03–56(1–2) exhibit a
staircase shape in the low-temperature part of the spectra
(Fig. 10a, b). This feature can be interpreted as partial 40Ar
loss during post-HP peak deformation, polymetamorphism,
or fluid circulation (Scaillet 1996). No age plateau was
obtained from samples Ar-03–56(1–2), because they dis-
play staircase shapes. However, HT 40Ar/39Ar steps
converge to an age of *95 Ma in the two spectra. So the
higher-T steps ages of *95 Ma of samples AR-03–56(1–
2) can be considered a minimum age for phengite crys-
tallization in these samples. The hypothesis of excess 40Ar
is unlikely because a similar age is obtained for HT steps in
both samples.40Ar/39Ar spectra of the other HP phengite samples
(Fig. 10c, d) are flatter, which allows estimating small
plateau and plateau ages. A small plateau-age was obtained
for sample AR-03–58(1), at 91.6 ± 0.4 Ma, with 35% of
released 39Ar. A plateau-age was obtained for sample AR-
04–07, at 93.9 ± 1.6 Ma, with 90% of released 39Ar. A
similar ‘‘within error’’ isochron age of 95.4 ± 0.4 Ma has
been obtained on this sample (AR-04–07), confirming the
age of *95 Ma. These plateau and isochron ages confirm
that the progressive staircase spectra of AR-03–56(1–2)
and AR-03–58(1) are due to partial resetting either during
early near-isothermal decompression or during the later
1,0
1,5
2,0
0,5
200 300 400 500 600 700 800
2,5
Jd10
Jd20
Jd30
Jd40Jd50Lw
s+Jd
Pa+Z
o+Q
z
Lws+ab
Si: 3,8
Pa+Zo+Qtz
Si:3,7
Pum
p+C
hl+Q
z
Si:3,6
Si:3,5
Sph +
Cz+
Act
+H20
TEMPERATURE (°C)
Si:3,4
GF
EBF AEA
LBF EBF
E
PR
ESS
UR
E (
GP
a)
AbJd
+ Qtz
PgJd50 +Ky
CoQtz
95-91 Ma
73.5-71 Ma
1
2
26°C/km
12°C/km
Glc+
Fig. 9 P-T diagram showing the stability fields of studied assem-
blages, and deduced P-T-t paths. The shaded domains correspond to
PT estimates derived from the stability fields of the two parageneses,
including the jadeite content in clinopyroxene and the Si content in
phengite. Ellipses are estimates obtained with Thermocalc. Ages
shown are those obtained by 40Ar/39Ar on phengite (this paper).
Limits of metamorphic facies after Evans (1990). AEA Albite-
Epidote-Amphibolite; E Eclogite; EBF Epidote-Blueschist Facies; GSGreenschist Facies; LBF Lawsonite Blueschist Facies
544 Int J Earth Sci (Geol Rundsch) (2009) 98:533–550
123
LP–MT stage, and do not result from excess 40Ar. From
these four samples, the age of HP metamorphism can be
bracketed between 95 and 91 Ma.
40Ar/39Ar dating of LP–MT peak phengite
The dating of LP–MT peak phengite is shown on Fig. 10e,
f. A small plateau was obtained from sample AR-03–54,
dated at 73.3 ± 0.5 Ma with 52% of released 39Ar. This
age is confirmed by the isochron age of 73.0 ± 1.4 Ma in
this sample. A plateau age was obtained from sample AR-
03–58(2) at 71.1 ± 0.5 Ma with 73% of released 39Ar.
From these two samples, the age of retrogression of
blueschists in the epidote-amphibolite facies is bracketed
between 71 and 73.5 Ma.
Discussion and Conclusions
P–T–t path and timing of deformation events
The complementary thermobarometric and 40Ar-39Ar geo-
chronological approaches allow the construction of P–T–t
paths, for two texturally defined sequences of assemblages:
(1) the HP rocks retrogressed into the greenschist facies, (2)
the HP rocks retrogressed into the epidote-amphibolite
facies (Fig. 9). The deduced rate of exhumation, using an
average density of 2.7 between the two phases is of 0.6–
1.5 mm a-1. This rate seems too slow for an uplift rate
within a subduction zone, as several works have shown that
the exhumation rate in these contexts is of the same order of
magnitude as the subduction rate (Rubatto and Hermann
2001). In addition, the relatively hot geotherm (26�C km-1)
Table 3 Representative results of Thermocalc calculations, for fit close to 1. Water and CO2 activities were fixed to 0.9 and 0.1, respectively
Parageneses Reactions Average
temperature
Average pressure
HP–LT (sample AR0350) fgl + 3hem = 2jd + 3mt + 4q + H2O
gl + 3cc + 2q = 3di + 2jd + H2O + 3CO2
fgl + 3cc + 2q = 3hed + 2jd + H2O + 3CO2
3mt + cz + 7cc + 12q + H2O = 3hed + 3ps + 7CO2
fgl + 3hem + ps = 2acm + 3mt + cz + 4q + H2O
mrb + hed + hem + 2cc = 3di + 2acm + mt + H2O + 2CO2
fgl + 4jd + 3mt + 10cc + 14q = 6hed + 6acm + 2cz + 10CO2
3fgl + 10mrb + 6ps = 6gl + 12di + 14acm + 9mt + 22q + 10H2O
7mrb + 13hed + 5mt + 4cz = 6fgl + 21di + 2acm + 11hem + 3H2O
3mrb + 6hed + 3mt + 2cz + CO2 = 3fgl + 9di + 6hem + cc + H2O
545 ± 60�C 1.25 ± 0.15 GPa
LP–MT (sample
AR0414)
2cz + 5cc + 3q = 3gr + H2O + 5CO2
6ts + 3clin = 11py + 4gr + 18H2O
8sp + ames + 5gr + 21q = 4ts + 7an
2ts + 3ames + 8q = 4an + 6py + 14H2O
4ts + 3ames + 6q = 4cz + 8py + 14H2O
9ts + 14cz + 38cc = 7sp + 4clin + 28gr + 38CO2
24cz + 5alm + 66cc + 36q = 3daph + 38gr + 66CO2
8ts + 15daph + 6ab + 4CO2 = 6parg + 25alm + 4cc + 62H2O
3ames + 2py + gr = 3sp + 3clin + 3an
ts + 3an + 2cc = 2cz + py + gr + 2CO2
505 ± 67�C 0.57 ± 0.02 GPa
LP–LT (sample
AR0352b)
2cz + pa + 2q = 4an + ab + 2H2O
3ftr + 2cz + 7pa + 3ab = 5fgl + 10an + 6H2O
5fgl + 6an + 8cc + 14q = 3ftr + 4cz + 10ab + 8CO2
5fgl + 2an + 4cc + 10q = 3ftr + 2pa + 8ab + 4CO2
2pa + 3cel + an + CO2 = gl + 3mu + cc + 3q + H2O
3ftr + 5gl + 18cz + 15mu + 21q = 5fgl + 15cel + 42an + 12H2O
2gl + 3ftr + 2ps + 7pa + 3ab = 5fgl + 2mrb + 10an + 6H2O
3ftr + 2gl + 2ps + 7pa + 3ab = 2mrb + 5fgl + 10an + 6H2O
10fgl + 6ps + 21pa + 30cel = 4gl + 6ftr + 6mrb + 30mu + 21ab + 18H2O
463 ± 30�C 0.35 ± 0.04 GPa
Mineral abbreviations are following Powell and Holland (1998). Estimates are given at 2r
Int J Earth Sci (Geol Rundsch) (2009) 98:533–550 545
123
deduced for the LP–MT retrogression is more in agreement
with crustal thickening during an early collisional stage than
with an ongoing subduction process. Similar increase of
temperature is obtained from Himalayan (de Sigoyer et al.
2000) and Alpine (Rolland et al. 2000) blueschists, where it
has been linked to thermal relaxation due to higher radio-
genic heat production related to collisional crustal stacking
(e.g., Vanderhaeghe et al. 1999). Such a collisional setting
during LP–MT metamorphism is also suggested by related
structures. The compressive deformation featured by
upright folds, in a horizontal NE–SW shortening context,
has to closely post-date the LP–MT (71–73 Ma) meta-
morphism, as it predates the deposition of the Paleocene-
Eocene UVSU. Such compressive deformation can be
ascribed to the accretion of the South Armenian Block to the
Eurasian margin, as it is the main shortening phase in the
Fig. 10 40Ar/39Ar phengite spectra of SBOC samples. a–d HP phengites samples. e–f LP–MT phengite samples
546 Int J Earth Sci (Geol Rundsch) (2009) 98:533–550
123
Lesser Caucasus. Consequently, we suggest that the time
gap between the two phases, the thermal increase during the
second metamorphic phase, and the tectonic style are due to
the collision of the South Armenian Block with the margin
of Eurasia at 71–73.5 Ma.
Large-scale geometry
The large-scale geometry of the South Armenian Block-
Eurasian margin boundary is interpreted in the light of data
presented in this paper (Fig. 11). The protrusion of blues-
chists and ophiolitic rocks in a top-to the North thrust
sequence, along a mainly north-dipping tectonic pile is
indicative of local back-thrusting. This may be facilitated
by a crustal back-stop at the northern edge of the Sevan-
Akera suture zone. The coincidence of north-dipping nor-
mal faults to the north of the ASBOC, with large amounts
of Plio-Quaternary volcano-sedimentary infill may coin-
cide with local extension at the back of a main Cretaceous
south-verging thrust ramp (Figs. 4, 11).
Geodynamic interpretations
The ASBOC is featured by the following geodynamic
history (Fig. 12):
(1) Formation of the ophiolite in the Upper Jurassic (age
given by radiolarians, Danelian 2007), which is
compatible with the age of the Sevan Ophiolite
(Zakariaze et al. 1983).
(2) Subduction of this oceanic crust segment during the
late Lower Cretaceous (at c. 95–91 Ma, 40Ar/39Ar
age of blueschists), and formation of the andesitic
volcanic arc as a result of the intra-oceanic subduc-
tion (Galoyan et al. 2007). Subduction might have
been west-or east-dipping as suggested by the
current geometry and the E–W orientation of linea-
tions. However, E–W lineations might have been
passively rotated during the main shortening phase.
Even though constant N–S convergence regime is
ascertained by paleomagnetism during this period
(e.g., Ricou 1994 and references therein), such E–W
motions might be explained by short-lived reactiva-
tion of transform faults oblique to convergence
direction. In the West, opening of a back-arc system
is ascertained by N–S, west dipping, normal faults.
These correspond to the eastern rim of the Black sea,
which is interpreted as a back-arc basin opened in
the Cretaceous (e.g., Boccaletti et al. 1974; Gorur
1988).
(3) The E–W convergence stops in the Late Upper
Cretaceous, and the whole tectonic pile is affected
by NNE–SSW shortening. Due to the intra-oceanic
setting of the volcanic arc, it is likely that a stage of
arc-continent accretion preceded the continent-conti-
nent collision (Fig. 12). The two events occur within
the range of LP–MT metamorphism. In a first stage,
nappe stacking at 73–71 Ma (40Ar/39Ar ages on
phengite) of variably metamorphosed units (greens-
chists above blueschists) suggests an ongoing
subduction context, dipping to the north. Further,
continent-continent collision (between 70 and 55 Ma)
between the South Armenian block to the South and
Eurasia to the North resulted in the blocking of the
subduction and in the formation of a penetrative E–W
fold belt. As is emphasized in Fig. 12, the very
peculiar structural aspect of the ‘‘blueschist windows’’
is allowed by a combination of thrusting towards the
south and back-thrusting towards the north.
(4) Cenozoic evolution is featured by Paleocene-Eocene
unconformity over the folded nappe stack. Large
wave-length folds, related thrusting towards the south
(e.g., the Spitak fault more to the South), and normal
faulting towards the north at the back of the ramp-
anticline structure resulting in the depression of the
Stepanavan area (Fig. 12).
Lateral correlations with other Tethyan suture zones
Timing of subduction in the ASBOC is similar as for NW
Turkey, ranging mostly from 105 to 85 Ma across the Izmir-
Ankara suture (Harris et al. 1994; Okay et al. 1998; Sherlock
++
++
+
+++
+
++ ++
++ ++
++ ++
++ ++
++ ++ ++
++
++
++ +
+++ + + +
CP-E
P-E
C
P-EP-Q
Armenian BlockEurasia
NorthSouth
20 km
J
BU
CC
C
Fig. 11 Schematic interpretative cross-section of the Armenian–Eurasian boundary. The capitals refer to geological formations. J Jurassic;
C Cretaceous; P-E Paleocene-Eocene; P-Q Plio-Quaternary. The black box indicates the location of the Stepanavan cross-section (Fig. 3 )
Int J Earth Sci (Geol Rundsch) (2009) 98:533–550 547
123
et al. 1999; Okay et al. in preparation). More to the SE,
supra-subduction plagiogranites were dated at 93–88 Ma by
K–Ar on whole rock by Kananian et al. (2001), and Mid-
Cretaceous 40Ar/39Ar ages are also reported from blueschists
in the Zagros region (Agard et al. 2006, 2007). These data
provide evidence that the same subduction front was active
from NW Turkey to N Armenia, contemporaneously to
subduction in the S Iran Zagros Subduction Zone.
The age of blueschist retrogression is not uniform along
this belt, which emphasizes different processes of exhu-
mation after peak pressure conditions were attained. In
northern Turkey, rapid exhumation postdates the HP peak,
so the rocks were not found to have a 2-phase evolution
showing that burial and exhumation are part of the same
subduction history within the accretionary prism (Okay
et al. 1998; Sherlock et al. 1999; Okay et al. in prepara-
tion). In the ASBOC of Armenia, a LP–MT phase is found
to postdate the HP peak by *20 Ma, which is in agreement
with a 2-phase exhumation with (1) subduction and (2)
early collision history as is found in the Alps and the
Himalayas.
Acknowledgments This work was supported by the MEBE (Middle
East Basin Evolution) program. Fieldwork was facilitated by the
support of the Armenian Academy of Science (Institute of Geological
Sciences). Financial support from the French Embassy in Armenia
and the French Ministry for Foreign Affairs has allowed Mr. Ghazar
Galoyan to complete his PhD in France. The help of G. Feraud and
J.L. Devidal during data acquisition in Nice and Clermont-Ferrand is
acknowledged. Reviews provided by A.I. Okay and S. Guillot helped
improve the quality of the manuscript.
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