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, DECEMBER 2011, 62, 6, 547—562 doi: 10.2478/v10096-011-0039-2
Introduction
The Quaternary alkaline volcanism of NW Iran has been
closely linked to the collision between the Afro-Arabian and
Eurasian plates. The northward motion of the Afro-Arabian
plate in the Late Mesozoic and Early Cenozoic was associat-
ed with subduction under the southern margin of Eurasia
(e.g. engör & Yilmaz 1981; Ricou 1994; Mohajjel et al.
2003; Agard et al. 2005; Azizi & Moinevaziri 2009; Saki
2010). Four structural zones developed in Iran as a result of
Neo-Tethys subduction beneath the Central Iran Microplate
(CIM) and the following collision of the Iranian and Afro-
Arabian plates (Fig. 1a). These structural zones include the
Urumieh-Dokhtar magmatic arc (UDMA), Sanandaj—Sirjan
Metamorphic Zone (SSMZ) and folded Zagros Zone (High
Zagros and Zagros Simply Folded Belt) (Alavi 2004). The
UDMA represents a continental arc that formed as a result of
the subduction of the Neotethyan oceanic crust under the
SSMZ in the Late Mesozoic (Alavi 1994).
This magmatic belt contains volcanic and plutonic rocks
of Eocene—Quaternary age that extend from NW to SE in
Iran. Magmatic activity in the UDMA started in the Late
Cretaceous and continued during the Eocene until Quaternary
period (Ahmadzadeh et al. 2010). However, the peak of
magmatic activity is thought to be of Eocene age (e.g. Stock-
lin 1974; Farhoudi 1978; Emami 1981; Jahangiri 2007).
Geochemical studies indicate that the Urumieh-Dokhtar
magmatic arc is generally composed of subduction-related
calc-alkaline rocks (e.g. Jung et al. 1976; Dupuy & Dostal
1978; Berberian et al. 1982; Azizi & Jahangiri 2008). Alka-
line rocks are also reported locally by Amidi et al. (1984),
Hassanzadeh (1993), Moradian et al. (1997), Hajalilou et al.
(2009), Khairkhah et al. (2009), Saadat et al. (2010), Saadat
& Stern (2011). These researchers have discussed the
geochemistry, origin, magmatic processes (such as fractional
crystallization, crustal contamination and magma mixing),
age and tectonic settings of Quaternary volcanic rocks in
Iran. The younger volcanic activity in the Urumieh-Dokhtar
magmatic arc is mainly alkaline in nature and is associated
with tectono-magmatic processes related to post-collisional,
intra-continental rifting events (Richards 2003). In this pa-
per, we present new geochemical characteristics and Sr, Nd
data on lavas from the Quaternary alkaline volcanism in
northwest Iran, filling a gap in the knowledge of the post-
Quaternary post-collision alkaline volcanism NW of Ahar
(NW Iran): geochemical constraints of fractional
crystallization process
RAHIM DABIRI
1*
, MOHAMAD HASHEM EMAMI
2
, HABIB MOLLAEI
3
, BIN CHEN
4
,
MANSOR VOSOGI ABEDINI
1
, NEMATALLAH RASHIDNEJAD OMRAN
5
and MITRA GHAFFARI
3
1
Department of Geology, Science and Research Branch, Islamic Azad University, Tehran, Iran; * r.dabiri@srbiau.ac.ir
2
Department of Geology, Islamshahr Branch, Islamic Azad University, Islamshahr, Iran
3
Department of Geology, Mashhad Branch, Islamic Azad University, Mashhad, Iran
4
School of Earth and Space Sciences, Peking University, Beijing 100871, P. R. China
5
Department of Geology, Tarbiat Modares University, P.O. Box 14115-175, Tehran, Iran
(Manuscript received January 5, 2011; accepted in revised form June 9, 2011)
Abstract: Major and trace elements and Sr—Nd isotopic data are presented for the Quaternary alkaline volcanism NW
of Ahar (NW Iran). The exposed rocks mainly consist of alkali basalts, trachybasalts, basaltic trachyandesites and
trachyandesites. Alkali basalts and trachybasalts display microlithic porphyritic texture with phenocrysts of olivine,
clinopyroxene, and plagioclase in microlithic groundmass. In the more evolved rocks (basaltic trachyandesites and
trachyandesites), amphibole and biotite have appeared. Major and trace element abundances vary along continuous
trends of decreasing MgO, TiO
2
, Fe
2
O
3
*
, CaO, Co, Cr, V and Zn, and increasing K
2
O, Al
2
O
3
, Ba and Th with increasing
SiO
2
. The Sr and Nd isotopic ratios vary from 0.704463 to 0.704921 and from 0.512649 to 0.512774, respectively.
Alkali basalts with high
143
Nd/
144
Nd ratio, low
87
Sr/
86
Sr ratio and high MgO, Ni and Cr contents indicate that they were
generated from relatively primitive magmas. Ba, Cr and La/Sm ratios versus Rb suggest that fractional crystallization
of alkali basalts could have played a significant role in the formation of evolved rocks. Assimilation and fractional crystal-
lization modelling, as well as Rb/Zr, Th/Yb and Ta/Yb ratios clearly indicate that crustal contamination accompanied by
the fractional crystallization played an important role in petrogenesis of the trachyandesites. The small compositional
differences between magma types, isotopic composition, mineralogy and nonlinear trends on Harker diagrams also indi-
cate that magma mixing was not an essential process in the evolution of the Ahar magmas. Petrogenetic modelling has
been used to constrain sources. Trace element ratio plots and REE modelling indicate that the alkali basalts were generated
from a spinel-peridotite source via small degrees ( ~ 2.5%) of fractional melting.
Key words: Quaternary, Iran, NW Ahar, geochemistry, alkaline volcanism, crustal contamination.
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collisional magmatism in NW Iran. We use these data to in-
fer the petrogenesis of these rocks in order to interpret their
melt sources and magmatic evolution.
Geological setting
The study area is located in NW Ahar, NW Iran (Fig. 1b).
In the classification of the structural units of Iran, this area is
Fig. 1. a – A simplified tectonic map
showing the main tectonomagmatic fea-
tures of the Iran and Eastern Anatolia
regions. UDMA – Urumieh-Dokhtar
magmatic arc, SSMZ – Sanandaj-Sir-
jan Metamorphic Zone, FZZ – Folded
Zagros Zone. b – Geological map of
the Ahar region. Simplified and modi-
fied after Babakhani et al. (1990).
a part of the Central Iranian magmatic arc (UDMA)
(Fig. 1a). A simplified geological map of NW Ahar is
shown in Fig. 2. The composition of volcanic rocks in this
area varies from calc-alkaline to alkaline during the Eocene
to Quaternary. The Quaternary volcanism is represented by
lava flows (Fig. 2). The volcanic sequences in the Ahar area
are correlatable with the eastern part of Turkey. According to
the study of Alberti et al. (1980), Innocenti et al. (1982),
Moinevaziri (1985), Mitchell et al. (1999) and Jamali et al.
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(2010) the last phase of volcanic activity in this area oc-
curred in Quaternary. The oldest unit of this region is Creta-
ceous (?)
basement
metamorphic
rocks
(micaschist,
meta-diabase and amphibolite), that is exposed in a very lim-
ited area. These rocks are covered by the Upper Cretaceous
volcanic and flysch type sedimentary rocks (Fig. 1b). The
Cenozoic magmatism started in the Paleocene and continued
in the Eocene with intensive volcanic activity that produced
widespread intermediate to felsic rocks. In the Oligocene—
Miocene large granitoid plutons were emplaced and this
caused extensive alteration and mineralization (Mollaei
1993; Mollaei et al. 2009). The Oligocene-Miocene intru-
sions mostly consist of coarse- to medium-grained grano-
diorite and monzonite, with local, younger diorite and
gabbro plutons. More alkaline, nepheline-syenitic to monzo-
syenitic bodies occur in Kaleybar and Razghah (in NW of
Iran) (Ashrafi 2009; Aghazadeh 2009; Tajbakhsh 2010). The
Quaternary basaltic and trachyandesitic rocks unconform-
ably cover the older magmatic units. This Quaternary alka-
line volcanism in northwest Iran occurred after Late Miocene
calc-alkaline magmatism (Jahangiri 2007). During the Late
Miocene to Quaternary, the Ahar-Arasbaran region, under-
went regional contraction, shortening first in the N-NW di-
rection and subsequently in the NNE direction. The
NNE-oriented crustal shortening was accompanied by WNW
stretching and extension and associated intensive alkaline
magmatism in a broad zone of dextral transtension in the
hinterland of the Arabia—Eurasia collision front (Mohajjel &
Fergusson 2000; Sosson et al. 2005; Masson et al. 2006;
Dilek et al. 2010; Jamali et al. 2010).
Fig. 2. A modified and simplified geological map (after Mehrpartou 1993) of the NW Ahar. The led circles show the sample locations.
Analytical techniques
A total of about 200 samples from Quaternary alkaline
rocks in the NW of Ahar were collected. One hundred twenty
thin sections were studied by Polarized microscope. Fifteen
representative samples were then selected for whole-rock
chemical analysis (Table 1). Samples weighed between
1—1.5 kg before crushing and powdering. Whole-rock major
elements were determined by X-ray fluorescence spectrometer
(XRF) and trace and rare earth elements (REE) were deter-
mined by lithium borate fusion ICP-MS at the ALS Chemex
Laboratories in Vancouver, Canada.
Sr and Nd isotopic analyses were performed at the Institute
of Geology and Geophysics (IGG) in Beijing, China. Mass
analyses were performed with a multi-collector VG354 mass
spectrometer. Rb, Sr, Sm and Nd concentrations were mea-
sured using the isotopic dilution method.
87
Sr/
86
Sr and
143
Nd/
144
Nd ratios were normalized against
86
Sr/
88
Sr = 0.1194
and
146
Nd/
144
Nd = 0.7219, respectively.
87
Sr/
86
Sr ratios were
adjusted to NBS-987 Sr standard = 0.710250 and
143
Nd/
144
Nd
ratios to La Jolla Nd standard = 0.511860. Uncertainties result-
ing from the concentration prior to isotopic dilution are ± 2 %
for Rb, ± 0.4—1 % for Sr and less than ± 0.5 % for Sm and Nd,
depending upon the concentration levels.
Petrographic studies
The volcanic rocks in the study area, according to mineral as-
semblages, can be divided into three sub-groups, based on the
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study of 120 samples. (I) Olivine basalt with grey to greyish
brown colours, which displays vitrophyric, porphyritic and in-
tersertal textures. Plagioclase, olivine and clinopyroxene form
the main phenocryst phases in these basaltic rocks. The micro-
crystalline matrix is dominated by plagioclase, clinopyroxene
and olivine. Rare nepheline also occurs in the groundmass of
some olivine basalts; (II) Olivine trachybasalt to trachybasalt
with porphyritic and trachytic textures occur. These samples
contain plagioclase, clinopyroxene, biotite and olivine. Their
groundmass consists of plagioclase, pyroxene, apatite and
opaque minerals; (III) Amphibole trachyandesites are dark
grey to black and have a trachytic, porphyritic and microlithic
textures. Plagioclase, clinopyroxene, amphibole and biotite are
Sample Ah-124 Ah-125 Ah-138 Ah-139 Ah-129 Ah-131 Ah-133 Ah-115 Ah-116 Ah-132 Ah-141 Ah-103 Ah-104 Ah-118 Ah-27
Rock
type AB AB AB AB TB TB TB BTA
BTA
BTA
BTA TA TA TA TA
SiO
2
(wt. %)
48.40 45.60 47.71 46.60 48.68 49.50 50.50 52.32 53.10 51.04 51.90 56.13 53.90 56.69 54.70
TiO
2
1.96 3.16 2.94 2.31 1.62 1.74 1.52 1.07 1.02 1.21 0.95 1.02 0.67 0.71 0.49
Al
2
O
3
15.09 15.50 14.97 15.73 15.96 15.50 17.40 18.05 18.50 15.00 16.45 18.90 18.63 18.55 19.40
Fe
2
O
3
8.93 9.34 9.05 9.65 9.40 8.40 8.60 6.89 7.25 8.22 7.98 4.56 5.70 5.06 5.61
MnO
0.15 0.14 0.12 0.22 0.14 0.13 0.12 0.15 0.14 0.11 0.15 0.14 0.11 0.07 0.07
MgO
7.31 8.08 8.30 8.40 6.07 5.69 4.60 3.32 2.28 3.89 4.50 1.75 2.78 1.14 1.82
CaO
9.44 9.96 8.30 9.13 9.22 8.63 8.78 8.37 6.20 7.80 7.47 5.32 6.43 4.20 5.40
Na
2
O
3.66 2.40 2.56 2.61 4.20 4.22 4.10 4.60 5.02 4.33 3.64 6.36 6.20 5.09 6.09
K
2
O
0.97 1.56 1.48 1.58 1.95 1.60 1.36 2.76 3.10 2.87 2.25 3.04 3.36 2.73 2.77
P
2
O
5
0.33 0.46 0.39 0.32 1.00 0.86 0.93 0.62 0.64 1.16 0.59 0.47 0.37 0.27 0.23
LOI
0.49 1.50 2.20 1.27 1.08 2.10 0.89 1.05 1.06 2.27 3.08 1.49 1.27 1.59 1.09
Total
96.73 97.70 98.01 97.82 99.32 98.37 98.80 99.20 98.31 97.90 98.96 99.18 99.42 96.10 97.67
Cs (ppm)
1.09 0.60 0.32 0.11 1.23 0.49 0.43 1.46 2.16 0.33 0.38 2.31 1.84 3.00 2.01
Rb
35.2 33.3 37.5 34.6 40.6 39.5 40.0 43.0 45.6 44.8 44.0 54.6 51.7 57.6 49.7
Ba
335
363
520
371
707
473
568
874
1020
944
708
1058
1190
1118
1082
Th
1.48 2.29 1.91 1.86 2.57 2.57 3.47 4.27 3.89 3.09 5.13 5.13 7.08 5.25 7.24
Ta
1.0 1.1 1.2 0.9 1.6 1.3 1.2 1.3 1.3 1.1 1.3 1.1 1.7 0.7 0.8
Nb
19.3 21.0 25.6 17.1 32.5 27.6 26.1 23.8 24.1 24.7 23.1 17.7 24.9 11.8 12.5
Sr
715
830
550
422
1430
1695
1445
1190
1300
1850
1450
2324
1604
1952
2180
Pb
5
9
11
10
11 8
8
17
18
8
11
13
18
15
18
Zr
268
260
249
253
207
253
204
189
136
168
158
160
154
96
85
Hf
4.2 4.1 3.7 2.5 4.5 3.8 3.5 4.5 4.5 4.0 5.7 4.2 5.4 3.2 3.3
Y
19.3 17.4 14.2 21.6 18.8 15.8 15.6 20.2 20.8 11.7 28.0 15.5 14.2 13.0 10.1
V
185
186
218
268
190
212
199
182
171
203
176
176
97
107
71
Cr
320
330
347
296
291
254
209
153
109
161
155
80
74
66
90
Co
35.4 42.1 28.7 30.7 39.5 45.9 25.7 23.7 21.1 29.1 22.4 14.3 20.4 14.3 15.3
Ni
266
244
286
215
185
174
181
159
186
177
162
36
59
16
28
Zn
106
130
121
95
124
130
118
99
79
142
95
51
85
54
63
La
44.8 50.1 43.0 50.0 63.5 56.3 42.4 42.4 50.1 44.2 75.0 46.0 52.7 30.5 36.0
Ce
37.8 58.0 53.7 29.5 97.5 111.5 103.5 93.8 108.5 115.0 128.0 93.2 129.8 104.8 81.3
Pr
5.34 7.11 5.69 3.97 14.50 12.95 11.70 10.30 11.90 12.80 14.50 9.27 9.97 7.43 6.46
Nd
22.7 33.2 26.2 18.1 57.1 50.0 44.9 39.9 44.9 48.3 56.2 33.0 36.7 23.1 22.8
Sm
10.57 11.39 8.63 9.40 13.72 11.92 8.40 8.71 9.46 8.66 13.11 9.16 9.94 5.69 6.12
Eu
1.82 1.91 2.26 1.55 2.37 2.21 2.02 1.97 2.12 1.82 2.75 1.70 1.63 1.15 0.98
Gd
5.93 6.46 7.03 4.46 7.86 7.08 6.38 6.45 6.90 5.89 9.13 6.02 5.85 3.95 3.31
Tb
0.76 0.76 0.81 0.69 0.89 0.82 0.74 0.81 0.85 0.61 1.19 0.79 0.78 0.52 0.39
Dy
3.56 3.65 3.48 4.17 4.11 3.62 3.48 3.94 4.16 2.66 5.71 4.18 3.28 2.66 2.05
Ho
0.66 0.65 0.60 0.83 0.71 0.62 0.61 0.74 0.81 0.44 1.04 0.82 0.79 0.50 0.39
Er
1.80 1.86 1.65 2.41 1.96 1.64 1.71 2.16 2.27 1.23 2.96 2.46 2.34 1.46 1.12
Tm
0.23 0.23 0.18 0.32 0.24 0.18 0.19 0.27 0.30 0.14 0.37 0.31 0.33 0.19 0.13
Yb
2.73 2.91 2.50 2.50 3.40 2.89 2.00 1.91 2.15 2.00 3.00 1.90 2.10 1.20 1.40
Lu
0.34 0.28 0.27 0.37 0.22 0.17 0.18 0.29 0.31 0.14 0.37 0.26 0.17 0.20 0.16
87
Sr/
86
Sr
0.704463 0.704697 0.704670 0.704800 0.704921 0.704763
143
Nd/
144
Nd
0.512774 0.512742 0.512696 0.512702 0.512651 0.512649
Nd
2.7 2.0
1.1
1.2
0.3
0.2
Table 1: Representative whole-rock analyses of the Ahar Quaternary volcanic rocks. AB – alkali basalt, TB – trachybasalt, BTA – ba-
saltic trachyandesite, TA – trachyandesite.
ubiquitous phenocrysts. The groundmass consists of microlithes
of plagioclase, amphibole and biotite with minor clinopyroxene.
Olivine occurs as phenocrysts and microphenocrysts in the
basalt and trachybasalt. Some olivine phenocrysts are embayed
and olivine also occurs as resorbed phenocrysts in the olivine
basalts (Fig. 3a). There are reaction rims around olivine phe-
nocrysts. The reaction rims around the olivines are composed
of fine-grained orthopyroxene, plagioclase and Fe-Ti oxide.
Clinopyroxenes are found in all rock types as phenocrysts and
microphenocrysts. In some clinopyroxene phenocrysts, matrix
fills embayments and the others have embayed margins sug-
gesting resorption (Fig. 3b). Clinopyroxene also occurs in glo-
meroporphyritic aggregates with plagioclase and Fe-Ti oxides.
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Plagioclase phenocrysts show clear evidence of multiple
evolution and periods of dissolution and growth. On the ba-
sis of textural criteria, plagioclase phenocrysts can be identi-
fied as one of three types: (a) unsieved, with no dissolution
texture, (b) sieve-cored, where the cores are riddled with
Fig. 3. a – Embayed olivine crystal in olivine basalt. b – Embayed augite crystal with melt inclusions; Aug – augite, Ol – olivine, Pl – pla-
gioclase in olivine basalt. c – Sieve texture in a plagioclase phenocryst that has overgrown with clear rim in amphibole trachyandesite. d – Sieve
texture in plagioclase phenocrysts with clear rim and core; Pl – plagioclase, Cpx – clinopyroxene in amphibole trachyandesite. e – Am-
phibole with thin rims of fine-grained Fe-Ti oxide, pyroxene and plagioclase; Amp – amphibole, Cpx – clinopyroxene, Pl – plagioclase
in amphibole trachyandesite. f – Breakdown reaction of amphibole to clinopyroxene, plagioclase and Fe-Ti oxides. Big crystals of Cpx
around represent an overgrowth; Cpx – clinopyroxene, Amp – amphibole in amphibole trachyandesite.
glass and overgrown with clear rims (Fig. 3c), and (c) sieve-
ringed, where a clear core is mantled by a resorption zone
followed by a clear rim (Fig. 3d).
Amphibole occurs as yellowish green to yellowish brown
pleochroism phenocrysts, that are observed as reacted pheno-
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crysts. They typically have thin rims of fine-grained pyroxene
and Fe-Ti oxide (Fig. 3e). This feature probably reflects vola-
tile loss during ascent of magma in conduits (Rutherford &
Hill 1993). Occasionally, amphiboles breakdown to clinopy-
roxene, plagioclase and Fe-Ti oxides in trachyandesite
(Fig. 3f). In some amphibole phenocrysts, groundmass micro-
lithes fill embayments. The biotites, typically euhedral grains,
occur as elongated crystals surrounded by opaque grains at the
rim. Fe-Ti oxides have magnetite compositions, are subhedral
and are present mainly in association with mafic minerals and
disseminated in the groundmass.
Geochemistry
Major and trace elements
Major and trace elements analyses were carried out on fif-
teen samples (Table 1). The Quaternary volcanic rocks in
Ahar have a wide range of chemical composition with SiO
2
contents ranging between 45 % and 57 %, and have been
classified on the basis of their alkali and silica contents using
the total alkali—SiO
2
diagram (TAS) of Le Maitre et al.
(1989). No major compositional gap or bimodality is ob-
served; instead, all the samples lie along a well defined and
relatively tight trend in the TAS diagram (Fig. 4). On this
diagram the composition of volcanic rocks is represented by
alkali basalt, trachybasalt, basaltic trachyandesite and tra-
chyandesite. This diagram also shows that all samples are
plotting in the alkaline field. In the Harker diagrams, as SiO
2
increases, Fe
2
O
3
, MgO, CaO and TiO
2
decrease, while K
2
O
and Al
2
O
3
increase (Fig. 5). Such negative and positive cor-
relations can be explained by removal of the ferromagnesian
phases such as olivine and pyroxene. Compatible trace ele-
ments such as Cr, Co, V and Zn show strong negative corre-
lation with increasing SiO
2
, whereas incompatible trace
elements (e.g. Ba, Th) correlate positively (Fig. 6). These
major and trace element trends are broadly consistent with
fractional crystallization plagioclase + pyroxene + Fe-Ti ox-
ides + amphibole + biotite removal, all of which are present
as phenocrysts in the Quaternary volcanic rocks in Ahar.
Primitive mantle-normalized trace elements patterns of the
study area are characterized by a Nb—Ta trough and are en-
riched in incompatible trace elements (Fig. 7). The negative
Nb—Ta anomaly for Ahar lavas is consistent with a melt
source that was metasomatized by Nb—Ta-depleted aqueous
fluids produced from a dehydrating slab with residual rutile.
Fig. 4. Total alkali-silica diagram (Le Maitre et al. 1989) for the
NW Ahar Quaternary volcanic rocks. Dividing line between alka-
line and subalkaline fields after Irvine & Barager (1971). AB – al-
kali basalt, TB – trachybasalt, BTA – basaltic trachyandesite,
TA – trachyandesite.
Fig. 5. Selected major element variations against SiO
2
content.
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When compared with the multi-element diagrams of the
study area volcanic rocks, alkali basalts are characterized by
a less marked enrichment in Rb, Ba, Th, K, Sr (Fig. 7). En-
richment in Rb, Ba, Th, K, Sr, Zr, Hf, Pb, Ta, LREE (La, Ce)
and negative anomalies in Co, V, Zn, Ti, Ni, Cu in the more
differentiated rocks (trachybasalts, basaltic trachyandesites
and trachyandesites) suggests that these rocks derived from
the alkali basalts.
Fig. 6. Selected trace element variations against SiO
2
content.
Fig. 7. Primitive mantle normalized alkali basalt, trachybasalt, basaltic trachyandesite and trachyandesite patterns for the Ahar Quaternary
volcanic rocks (normalized values from Sun & McDonough 1989).
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Isotope geochemistry
Six samples have been analysed for Sr and Nd isotopes. Sr
and Nd isotope ratios determined in this study are presented in
Figure 8, and representative analyses and
Nd
values are listed
in Table 1. The Nd isotopic compositions of
87
Sr/
86
Sr ratios
range from 0.704463 to 0.704921;
143
Nd/
144
Nd ratios range
from 0.512649 to 0.512774. The
Nd
values range Nd from 0.2
to 2.7. There is a clear relationship between geochemistry type
and isotopic characteristics. In the conventional
143
Nd/
144
Nd
vs.
87
Sr/
86
Sr diagram (Fig. 8), the alkali basalts plot in the de-
pleted quadrant of the mantle array, whereas the trachyandes-
ites plot in the enriched side. Basaltic trachyandesites and
trachybasalts lie between the alkali basalts and trachyandesites
(Fig. 8). All the samples plot within the mantle array and close
to the field of BSE (Bulk Silicate Earth). This suggestion is
compatible with the
Nd
values of the rocks, because a positive
value of epsilon for volcanic rocks implies a magma derived
from an isotopically depleted source (e.g. Rollinson 1993).
Low
87
Sr/
86
Sr and high
143
Nd/
144
Nd and low Ba and Rb in
contents indicate a mantle source also for these rocks. The
higher
87
Sr/
86
Sr and the lower
143
Nd/
144
Nd isotope ratios of
the trachyandesites may be interpreted in terms of crust—mag-
ma interaction. Sr—Nd isotopic compositions were compared
with data of young volcanics from north Iran and east Turkey
(Fig. 8). The isotopic data of the Ahar Quaternary volcanic
rocks are similar to the isotopic data reported from the Dama-
vand Quaternary stratovolcano (Liotard et al. 2008; Mirnejad
et al. 2010) in the central part of the Alborz magmatic belt
(AMB), Quaternary volcanism from the Iran/Turkey border-
lands (Kheirkhah et al. 2009) and Quaternary volcanic centers
in Eastern Anatolia (Buket & Temel 1998). The isotopic ratio
of the Lesser Caucasus alkaline Quaternary volcanic rocks
(Lebedev et al. 2003, 2007), Ararat Quaternary volcano
(Gülen 1984) and Neogene volcanic rocks of eastern Turkey
(Aydin et al. 2008) are different from the study rocks (Fig. 8).
The Ahar Quaternary volcanic rocks have high
87
Sr/
86
Sr and
low
143
Nd/
144
Nd compared to the Caucasus alkaline Quater-
nary volcanic rocks and Ararat Quaternary volcano and low
87
Sr/
86
Sr compared to the Neogene volcanic rocks of eastern
Turkey.
Discussion
Fractional crystallization
The new data reported in this study indicate that the Qua-
ternary volcanic rocks in Ahar have similar petrographical
and geochemical features and define typical alkaline trends
from alkaline basalts to trachyandesites. Major element vari-
ations are mainly controlled by the fractionation of olivine
and clinopyroxene, which strongly deplete the magma in
MgO, TiO
2
, Fe
2
O
3
*
, CaO and compatible trace elements
(e.g. Co, Cr, V and Zn) (Figs. 5, 6). Incompatible (Rb) ver-
sus incompatible (Ba) trace element variations are linear,
Fig. 8.
143
Nd/
144
Nd and
87
Sr/
86
Sr isotope variation diagram for the Ahar Quaternary
volcanic rocks. BSE (Bulk Silicate Earth) composition is from Hart et al. (1992).
Locations of depleted mantle (DM) and enriched mantles (EMI, EMII) are from
Zindler & Hart (1986). The samples from other Neogene alkaline volcanic suites
are also plotted for comparison, including the QVA (alkaline Quaternary volcanic
rocks, Ararat volcano; Gülen 1984), QVC (alkaline Quaternary volcanic rocks,
Lesser Caucasus; Lebedev et al. 2003, 2007), QVD (alkaline Quaternary volcanic
rocks, Damavand Volcano; Liotard et al. 2008; Mirnejad et al. 2010), QVEA
(Quaternary volcanic rocks, Eastern Anatolia; Buket & Temel 1998), QVIT (alka-
line Quaternary volcanic rocks, Iran/Turkey borderlands; Kheirkhah et al. 2009),
NVT (alkaline Neogene volcanic rocks, NE Turkey; Aydin et al. 2008) and QH
(Hocheifel volcanic rocks, Germany; Fekiacova et al. 2007).
Fig. 9. Cr (compatible element) and Ba (incompatible
element) against Rb for the Ahar Quaternary volcanic
rocks.
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with trends from low abundances in alkali basalts
towards higher abundances in trachyandesites
(Fig. 9). Compatible (Cr) versus incompatible (Rb)
element variations form curved rather than linear
trends (Fig. 9). Normalized REE patterns form par-
allel trends, and LREE contents increase from alkali
basalts to trachyandesites (Fig. 10). La/Sm data
points (Fig. 11) plot along a line, a feature restricted
to the process of fractional crystallization (Allegre
& Minster 1978). The above-mentioned character-
istics show that the Quaternary volcanic rocks in
Ahar evolved predominantly through fractional
crystallization of the petrographically observed
phenocryst assemblage (olivine + plagioclase + cli-
nopyroxene + amphibole + biotite + Fe-Ti oxides)
and fractional crystallization is the dominant pro-
cess for the Ahar rocks suite.
Role of crustal contamination
In order to constrain the role of crustal contami-
nation, we have utilized the assimilation and frac-
tional crystallization (AFC) model of DePaolo
(1981). The negative trend in the Sr-Nd isotope dia-
gram (Fig. 12) indicates that the magmas have been
affected by crustal contamination during their ascent
to the surface. We therefore attempted quantitative
modelling of AFC using the equations of DePaolo
(1981). In AFC modelling, the primitive mafic end-
member is the alkali basalt sample Ah-124, which
has a modal mineralogy of 8 % olivine, 1 % ortho-
pyroxene, 18 % clinopyroxene, 53 % plagioclase,
6 % alkali feldspar, and 5 % magnetite from CIPW
calculations (Table 2). It is further calculated from
the CIPW values of the parent mafic end-member
(Ah-124) that the bulk distribution coefficient for
Sr is 1.12, and for Nd 0.10 (D
Sr
= 1.12; D
Nd
= 0.10).
The upper crust has been selected for the contami-
nant end-member for the AFC modelling. Upper
crustal values are from Veizer & Compston (1974)
and O’Nions & Hamilton (1984). The ratios of the
rate of assimilation to the rate of crystallization
Fig. 10. Chondrite-normalized REE diagram for the alkali basalts and tra-
chyandesites (normalized values after Nakamura et al. 1974).
Table 2: Data used in the calculations of AFC modelling.
K
d
values for:
Starting
composition*
Calculated bulk partition
coefficient (D
o
) **
Olivine Opx Cpx Plag Mt
Sr 715
0.98
0.014 0.04 0.06 1.83
0.00
Nd 22.7
0.15
0.006 0.03 0.31 0.081 1.00
Th 1.48
0.015
0.04
0.13 0.03 0.01
0.00
Ta 1.0
0.07
0.04
0.15 0.013 0.018 1.00
Yb 2.73
0.2
0.014 0.34 0.62 0.067 0.9
K
d
values are from Rollinson (1993) and Keskin (1994).
Abbrevations: K
d
— mineral/melt partition coefficient, Cpx — clinopyroxene,
Plag — plagioclase, Mt — magnetite.
* — mafic parental end-member, sample Ah-124.
** — Of sample Ah-124 (Ol — 8 %, Opx — 1 %, Cpx — 18 %, Plag — 53 %,
K-spar — 6 %, Mt — 5 %).
Fig. 11. La/Sm variations against Rb for the Ahar Quater-
nary volcanic rocks.
Fig. 12. AFC modelling for
87
Sr/
86
Sr versus
143
Nd/
144
Nd isotopic compositions
for upper crustal (UC) end-member. Upper crustal values are from Veizer &
Compston (1974) and O’Nions & Hamilton (1984). Variations in r (the ratio of
the rate of assimilation/rate of crystallization) are shown with tick marks.
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(r values in Fig. 12) are from 0.1 to 0.9. Some samples are
located along AFC trajectories. Alkali basalts exhibit negli-
gible crustal contamination according to the diagram, since
they are located along the r = 0.1 trajectory (Fig. 12). The
contamination of the primitive end-member Ah-124 by the
continental crust gives rise first to trachybasalts and basaltic
trachyandesites and then, by a higher degree of contamina-
tion, to trachyandesites.
We have also prepared AFC modelling for Th/Yb versus
Ta/Yb diagram. This diagram has been found to be useful in
the determination of crustal contamination (Fig. 13). Th is
more affected than Ta and Yb during crustal contamination
processes. Therefore, rocks with crustal contamination show
high Th/Yb values (Wilson 1989). In this diagram, Yb is used
as a normalizing factor to minimize the effects of fractional
crystallization and crystal accumulation (Pearce 1983). The
composition of the upper crust has also been plotted on the
diagram. The fractional crystallization vector and AFC curve
(r = 0.4) for fractionation of a crystal assemblage consisting
of 8 % olivine, 1 % orthopyroxene, 18 % clinopyroxene,
53 % plagioclase, 6 % alkali feldspar, and 5 % magnetite
from the Ah-124 sample are also plotted (Fig. 13). The parti-
tion coefficients used are given in Table 2. The alkali basalt
to trachyandesite lavas of the Ahar exhibit a consistent dis-
placement from the mantle array towards higher Th/Yb val-
ues. The alkali basalts plot close to the mantle array field,
suggesting minimal crustal contamination (Fig. 14). The tra-
chyandesites have high ratios of Th/Yb (2.7—5.2). This sug-
gests that the role of crustal contamination in their magma
genesis cannot be ruled out.
The LILE (e.g. Rb and K) and Zr are incompatible with re-
spect to the major crystallizing phenocryst assemblage (pla-
gioclase, pyroxene, Fe-Ti oxides) and ratio like Rb/Zr do not
significantly change by simple fractional crystallization of this
assemblage. Variations in these ratios are preferably related to
Fig. 13. Th/Yb vs. Ta/Yb diagram (after Pearce 1983) for the Ahar Quaternary
volcanic rocks. AFC – assimilation and fractional crystallization, C – crustal
contamination, PM – primordial mantle composition, MORB – Mid-Ocean
Ridge Basalt.
crustal contamination by AFC processes (David-
son et al. 1987). Examination of the study volcanic
rocks shows that, in the alkali basalts, trachyba-
salts and basaltic trachyandesites, there is no sig-
nificant variation in the Rb/Zr ratio (Fig. 14). The
trachyandesites have a wider range of Rb/Zr val-
ues, which indicate that significant contamination
is involved in the evolution of these samples.
However, the trachyandesites have higher Sr and
lower Nd isotope ratios, and have higher Th/Yb ra-
tios and wider ranges in Rb/Zr values that clearly
indicate crustal contamination, which has played
an important role in the genesis of these rocks.
Magma mixing
Petrographic data provide evidence for magma
mixing in the Quaternary volcanic rocks in Ahar.
Some rocks contain disequilibrium mineral tex-
tures such as sieve textured plagioclases, and show
resorption of the ferromagnesian phases such as
olivine, pyroxene and amphibole. Fine-grained re-
sorption zones in plagioclase are probably caused
by superheating, as described by Tsuchiyama
(1985). The clear overgrowth rims on the sieved cores demon-
strate that the reaction took place before crystallization of the
inclusion groundmass began. Phenocrysts which are reacted
and resorbed in the study area formed when their host mag-
ma interacted with a more basic one. The olivine phenoc-
rysts exhibit normal zoning whereas some of the
plagioclases are reversely zoned. These features may be gen-
erated by fractionation of plagioclase in a magma chamber at
depth, with a sudden influx of more primitive phenocryst-
poor magma. The result is continuous normal zoning of oliv-
ine phenocrysts and reversed zoning of the previously
formed plagioclase phenocrysts as a result of the new liquid
composition (e.g. more primitive). Whole-rock major and
trace element chemistry is also an excellent method of deter-
mining mixing relationships (Reid et al. 1983; Srogi & Lutz
1997). Perfect mixing may be identified by linear trends for
Fig. 14. Rb/Zr variations against Rb for the Ahar Quaternary volca-
nic rocks.
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all elements in Harker diagrams, but nonlinear trends on
Harker variation diagrams are consistent with crystal frac-
tionation processes (Wall et al. 1987) (Figs. 5, 6).
Fig. 15. (a) Sm/Yb versus La/Yb and (b) Sm/Yb versus La/Sm diagrams
showing the melt curves obtained from fractional and batch melting equa-
tions of Shaw (1970). La, Sm and Yb concentrations of the spinel and garnet
peridotite are from McDonough (1990) and Sen & Leeman (1991), respec-
tively. Bulk partition coefcients are taken from Tables 3 and 4. Solid square
and star represent starting compositions of garnet and spinel peridotite at
0.1 % F, respectively.
Table 3: Data used in the batch and fractional melting calculations of spinel-
peridotite.
Spinel-peridotite
composition (K
d
)
Mineral/melt
partition coeficients
Bulk partititon
coeficients (D
0
)
Initial
concentration
Co (ppm)
Olivine Opx Cpx Spinel
(66 % Ol,
24 % Opx,
8 % Cpx,
2 % Spinel)
La
2.6
0.0067
–
0.056
0.01
0.0091
Sm
0.47
0.007
0.05 0.45
0.01
0.053
Yb
0.26
0.014
0.34
0.542
0.01 0.13
La, Sm and Yb concentrations are from McDonough (1990), modal mineralogy of
the spinel-peridotite are from Wilson (1989: p. 50) and mineral/melt partition
coeficients of the basaltic melts are from Fujimaki, Tatsumoto & Aoki (1984);
McKenzie & O’Nions (1991); Rollinson (1993: p. 108). Abbrevations: Opx —
orthopyroxene; Cpx — clinopyroxene; Ol — olivine.
It is very difficult to assess the extent of magma
mixing if the source was the same for all magmas.
However, magma mixing is not believed to be of
great importance in the evolution of Ahar magmas,
because: (1) the small compositional differences be-
tween magma types, (2) the identical isotopic signa-
tures of the erupted lavas, and (3) the domination of
normally zoned phenocrysts (olivine and plagio-
clase) over the occasional reversely zoned plagio-
clases (4) unlinear trends in Harker diagrams.
Determination of source characteristics
Whole-rock REE content is mainly controlled by
source composition and degree of partial melting
and as such it has been widely used to determine
the origin of the magmas, and the degree of, and
variation in mantle melting (e.g. Gurenko &
Chaussidon 1995; Johnson 1998; Münker 2000;
Green 2006; Zhao & Zhou 2007). The REE are
moderately incompatible during melting of mantle
peridotite according to their partitioning coeffi-
cient (Johnson 1998), and thus, their concentra-
tions and ratios are not greatly affected by mantle
depletion and fluid influx (Pearce & Peate 1995;
Münker 2000). Sm/Yb ratios can be used to con-
strain the source mineralogy of the alkaline mag-
mas, since Yb is compatible with garnet. Thus, we
have achieved REE modelling of the alkali basalt
samples (Fig. 15). In REE modelling, we use the
fractional and batch melting equations of Shaw
(1970). La, Sm and Yb concentrations, mineral/melt
(K
d
) and bulk (D
0
) partition coeffcients and modal
mineralogy of the spinel-peridotite and garnet-peri-
dotite are reported in Tables 3 and 4. The plot of
Sm/Yb versus La/Sm and La/Yb distinguishes be-
tween melting of garnet- and spinel-peridotite
sources (Fig. 15). Partial melting of a spinel-peri-
dotite source produces melts with lower Sm/Yb ra-
tios than a garnet-peridotite source. It is apparent
from Figure 15 that the alkali basalt clearly plots on
the fractional melting curve of spinel-peridotite.
REE modelling indicates that the alkali basalts
formed by partial melting of spinel-peridotite sourc-
es via degree of partial melting ranging from ~ 1 %
to ~ 3 %. In Table 5 – trace element contents, bulk
distribution coeficients and results obtained from
the calculations of 1 % to 5 % fractional melting of
the spinel-peridotite are reported. The results ob-
tained from 1 % to 5 % degree of partial melting
modelling were compared to the alkali basalt sam-
ples on the primitive mantle-normalized spidergram
(Fig. 16). It is clear in Figure 16 that the trace ele-
ment pattern obtained from the 2.5 % fractional
melting of the spinel-peridotite sample has the
highest similarity to the alkali basalt samples. We conclude
that the alkali basalt samples were generated by low degree
partial melting ( ~ 2.5 %) of a spinel-peridotite source.
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Table 4: Data used in the batch and fractional melting calculations of garnet-peridotite.
Garnet-peridotite
composition (K
d
)
Mineral/melt
partition coeficients
Bulk partititon
coeficients (D
0
)
Initial concentration
Co (ppm)
Olivine Opx Cpx Garnet (63 % Ol, 30 % Opx,
2 % Cpx, 5 % Garnet)
La
1.73
0.0067
– 0.056 0.0016
0.0054
Sm
1.12
0.007
0.05 0.45
0.217
0.039
Yb
0.51
0.014
0.34 0.542
6.167
0.43
La, Sm and Yb concentrations are from Sen & Leeman (1991), modal mineralogy of the
garnet-peridotite are from Wilson (1989: p. 50) and mineral/melt partition coeficients of
the basaltic melts are from Irving & Frey (1978), Fujimaki, Tatsumoto & Aoki (1984);
Rollinson (1993: p. 108). Abbrevations: Opx — orthopyroxene; Cpx — clinopyroxene;
Ol — olivine.
Fig. 16. Primitive mantle normalized (Sun & McDonough 1989) spidergrams calcu-
lated from the spinel-peridotite sample (McDonough 1990) at 1 to 5 % fractional
melting, compared with the alkali basalt samples. Trace element concentrations and
bulk partition coefcient (D
o
) of spinel-peridotite are taken from Table 5. Modal min-
eralogy of the spinel-peridotite as in Table 3.
Geodynamic implications
NW Iran is in the central part of the Arabian
lithospheric collisional zone, which experi-
enced N—S shortening and E—W extension
accompanied by intense faulting, strong
earthquakes and active volcanism (e.g.
Dewey et al. 1986; Karakhanian et al. 1997;
Talebian & Jackson 2002; Karakhanian et al.
2004; Copley & Jackson 2006). This region
was affected by a complex tectonic regime
from the Late Paleocene—Early Eocene
( engör & Kidd 1979; Topuz et al. 2005;
Karsli et al. 2007; Önal & Kaya 2007). The
melt generation modelling and geochemical
results presented above show that the source
of the alkaline rocks is enriched in LILE and
LREE relative to primitive mantle (PM) and
depleted MORB mantle (DMM).
Three main geodynamic models have been
suggested to explain the melting process of
the lithospheric mantle in NW Iran and SE
Turkey. They include mantle plume (Ershov
& Nikishin 2004), partial lithospheric delami-
nation (Pearce et al. 1990) and slab breakoff
(Keskin 2003; engör et al. 2003). For NW
Iran and the northern part of UDMA, the
melting of mantle lithosphere by heat from a
mantle plume is improbable, because there is
no evidence for a mantle plume origin. Ahar
Quaternary volcanic rocks have high
87
Sr/
86
Sr
and low
143
Nd/
144
Nd compared to rocks de-
rived from plumes (e.g. Quaternary Hocheifel
lavas (QH)) (Fig. 8). A mantle plume would
also be expected to produce a dynamic uplift
over an area 1000—2000 km in diameter
(White & McKenzie 1989; Hill et al. 1992;
Ritter & Christensen 2007). Furthermore, the
overall volcanic expression in NW Iran is
asymmetrical, extending in a NW—SE trend
sub-parallel to the general trend of the orogen-
ic belt. Therefore, a possible cause of the
melting of the lithospheric mantle beneath the
area can be explained by heat from asthenos-
pheric upwelling resulting from lithospheric
delamination or by detachment of subducted
slab following collision. Both mechanisms in-
volve ascent of asthenospheric mantle to re-
place the sinking material. These are not
mutually exclusive explanations (Keskin et al.
2006; Dokuz 2010). A partial lithospheric
delamination model is suggested by Pearce
et al. (1990) for volcanism in Eastern Anatolia
and recently by Liotard et al. (2008) for the
genesis of Quaternary alkaline volcanic
rocks in Damavand volcano. The slab brea-
koff model is proposed by Keskin (2003) and
engör et al. (2003) for genesis of collision
related Miocene to Quaternary volcanism in
Calculated composition
for fractional melting
Starting composition
(66 % Ol, 24 % Opx,
8 % Cpx, 2 % Spinel)
Spinel-peridotite
Bulk
partition
coeficients
(D
0
)
1 %F 2.5 %F 3.5 %F 4.5 %F 5 %F
Rb 1.9
0.01
70.11 17.09 6.59 2.51 1.55
Ba 33
0.04
714.66 469.12 353.05 264.92 229.22
Nb 4.8
0.01
168.48 21.73 5.45 1.35 0.67
Nd 2.67
0.08
31.09 25.82 22.78 20.07 18.83
Zr 21
0.04
397.57 280.65 221.84 174.93 155.19
Sm 0.47
0.053
8.47 6.11 4.91 3.93 3.51
Eu 0.16
0.07
2.13 1.71 1.47 1.27 1.18
Dy 0.51
0.05
8.17 6.18 5.12 4.24 3.85
Y 4.4
0.12
33.27 29.84 27.73 25.75 24.80
Yb 0.26
0.13
2.90 2.43 2.16 1.91 1.80
Lu
0.043
0.06
0.66 0.51 0.42 0.35 0.32
Table 5: Data obtained from the 1 % to 5 % fractional melting calculations of the
spinel-peridotite (McDonough 1990) end-member.
Modal mineralogy of the spinel-peridotite as in Table 3. The mineral/melt partition coefcients
of the basaltic melts are from Fujimaki, Tatsumoto & Aoki (1984); McKenzie & O’Nions
(1991); Rollinson (1993: p. 108). Abbrevations: Opx – orthopyroxene; Cpx – clino-
pyroxene; Ol – olivine.
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Eastern Anatolia and recently by Ghasemi & Talbot (2006)
and Omrani et al. (2008) for Pliocene-Quaternary volcanic
rocks at UDMA in the Zagros orogeny.
The northern part of UDMA has experienced calc-alkaline
magmatism during the Eocene period and alkaline and ul-
trapotassic magmatism during the Quaternary period
(Ahmadzadeh et al. 2010). Preliminary research indicates that
calc-alkaline magmatism during the Eocene is related to sub-
duction of Neo-Tethys oceanic crust beneath CIM. Opening of
the Red Sea and the Gulf of Aden and rotation of the Arabian
plate has been responsible for oblique convergence between
the Arabian plate and CIM and the final closure of the Neo-
Tethys Ocean. The final closure of Neo-Tethys and collision
between the Arabian plate and CIM took place before or dur-
ing the Late Miocene (Berberian & Berberian 1981; Berberian
et al. 1982; Dargahi 2007). In the northern part of UDMA,
cessation of magmatism occurred after the main period of con-
vergence, probably controlled by rollback processes and sub-
sequent breakoff of the subducted slab (Ghasemi & Talbot
2006; Jahangiri 2007). After the calc-alkaline volcanism, an
extensional transtensional regime was developed in the
Oligocene-Miocene period. As a result of extensional tran-
stensional regime, local volcanic activities occurred along the
main dextral faults, like the north-Tabriz dextral fault. The
volcanic activity along the north Tabriz dextral fault is repre-
sented by the Late Miocene and ultrapotassic and alkaline
mafic magmas with adakitic signatures during the Pliocene—
Quaternary (Ahmadzadeh et al. 2010).
These variations in the lava chemistry of the Cenozoic vol-
canic rocks (Eocene to Quaternary) indicate a geochemical
progression from calc-alkaline to more alkaline compositions
over time and a spatial shift from north to south towards the
Arabian plate. Considering the temporal and spatial relation-
ship between calc-alkaline, adakitic, ultrapotassic and alkaline
rocks, the northwestern UDMA is a special case of subduc-
tion-related, rollback magmatism and was possibly related to a
slab breakoff (detachment) system. Slab breakoff leads to the
generation of a shallow thermal perturbation and opening of
an asthenospheric window that in turn caused partial melting
of the subduction metasomatized lithospheric mantle beneath
the collision zone (Davies & von Blanckenburg 1995). The
findings of the recent northern part of UDMA (Taghizadeh-
Farahmand 2010) and eastern Turkey seismic experiment
(Al-Lazki et al. 2003; Gök et al. 2003; Zor et al. 2003) and
seismic velocity from the Zagros collision to UDMA and CIM
(Kaviani et al. 2007), along with the tomographic models, sug-
gest that velocity difference at shallow depth is due to higher
mantle temperatures and/or higher fluid content beneath NW
Iran and eastern Turkey. These observations, combined with
trace element and isotope characteristics of these volcanic se-
quences, suggest that their magmas were derived from partial
melting of subduction-metasomatized continental lithospheric
mantle in the spinel-peridotite field beneath the CIM.
Conclusions
The Ahar volcanic rocks range from alkali basalts to tra-
chyandesites and show a typical alkaline differentiation trend.
Major and trace element variations indicate fractional crystal-
lization. Alkali basalts crystallized from relatively primitive
magma as suggested by their mineralogy, geochemistry and
trace element ratios. AFC modelling, as well as trace element
ratios indicate that crustal contamination played an important
role in petrogenesis of the trachyandesites. The small compo-
sitional differences between magma types, identical isotopic
signatures, the domination of normally zoned phenocrysts and
nonlinear trends on Harker diagrams also suggest that magma
mixing is not of great importance in the evolution of the Ahar
magmas. Alkali basalts were derived from a spinel-peridotite
mantle source via a small degree ( ~ 2.5 %) of partial melting.
Acknowledgments: We are grateful to Drs. Patrik Konečný,
Jaroslav Lexa and Ioan Seghedi for their constructive reviews
that significantly improved the quality of this paper. This arti-
cle is derived from a PhD Thesis entitled, “Geochemistry and
petrology of Quaternary mafic volcanic rocks from NW Ahar,
NW Iran”. The authors appreciate the support received from
the Islamic Azad University, Sciences and Researches Branch.
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