Alkali Metasomatism and ThREE Mineralization in the Choghart deposit , Bafq district , Central Iran

The Choghart iron oxide-apatite (IOA) deposit is located 124 km southeast of Yazd, in the Bafq district within the Central Iranian microcontinent. The Choghart deposit is hosted by the rhyolitic rocks of the Early Cambrian volcano-sedimentary sequence (the Esfordi formation). Both host rocks and the orebodies are crosscut by diabase dykes. Tectonically, the Choghart rhyolites represent the continental margin setting and the Choghart diabase dykes formed in the back-arc basin environment, respectively, indicating that the evolution of the Bafq district is associated with subduction of Palaeotethys oceanic crust beneath the Central Iranian microcontinent followed by formation of continental arc related granitoids and rhyolites and then formation of backarc basin diabase dykes. Similar to the other subduction-related rhyolites, the Choghart rhyolite is enriched in Th and LREE compared to Ta, Nb, and HREE. The main host minerals of Th and REE in the Th-REE mineralization zone are thorite and sphene. Albitization is the most important alteration aspect related to Th-REE mineralization (mainly Th, La, Ce, Nd, and Y). In addition to albite, Th-REE mineralization is associated with actinolite, augite, diopside, minor microcline and orthoclase, plus magnetite, calcite, pyrite, rutile, and minor amounts of chalcopyrite. The negative Eu anomaly in Th mineralization zone, as well as the paragenetic occurrence of magnetite, pyrite and chalcopyrite with thorite suggest that Th-REE mineralization formed in relatively reduced condition. The presence of paragenetic calcite accompanied by thorite and sphene in the Th-REE mineralization zone indicates that Th and REE were likely transported by the carbonate complexes in the mineralizing fluids. The similarity between the chondrite-normalized REE patterns of the host rhyolite and the Th-REE mineralization zone suggests that post-magmatic driven fluids of continental margin rhyolitic magma played an important role in Th-REE mineralization.

Some of the iron oxide-apatite (IOA) ore deposits of the Bafq district contain REE-U-Th mineralization.The Bafq iron ore deposits display a range of mineralization styles including massive ore bodies, veins, stockworks and metasomatic replacements, of which their distribution is considerably different within the individual deposits (MOHAMMAD TORAB, 2008).The significance in the Bafq district is the occurrence of Th-REE (in the Choghart mine) and, REE-U-Th mineralization (anomaly 5 in the Saghand ore field) in peripheral alteration zones around the iron ore deposits and also the correlation between the areas compris-ing such metals and the distribution of the alkaline metasomatic rocks.U-Mo mineralization in the Narigan ore deposit is possesses, genetically, a granite related origin as an exception (IAEA, 2014) and it is not related to metasomatic processes (DAHLKAMP, 2009).
Metasomatic processes are proposed as performing geochemical roles in the concentration of REE-U-Th bearing minerals in some areas of the world (e.g. the Kirovograd-Krivoi Rog district of the Ukraine, Lagoa Real in Brazil and the Beaverlodge district of Canada, WILDE (2013).Na-metasomatism, among other types of metasomatic processes, are particularly effective in the concentration of such elements.This characteristic of metasomatism is marked by Na-bearing minerals, which are clearly in replacement relationships with primary magmatic minerals (PIRAJNO, 2009).The metasomatic and hydrothermal processes that occur with aqueous solutions, are the only endogenic processes in which the content of radioactive elements and primarily uranium reach economic grades TITAYEVA (1994).The rocks affected by this type of metasomatism were first described as Nagranites by TANATAR (1925) or as syenites by FELDMAN (1926).There has been a continuous interest in the association of Th, U and REE mineralization, and this type of metasomatism is related to the importance of albitization in the mineralization of radioactive elements.According to KINNAIRD (1985), Naenrichment is accompanied by concentrations of Fe, U, Th, Zr, Nb, Sn, Zn and HREE.Na-metasomatised rocks also tend to be enriched in Rb, Th, Nb, La, Ce, Hf, Zr, and Y with respect to Kmetasomatised rocks.The mineralization of natural radioactive elements controlled by the occurrence and development of the albitites is well studied in some localities such as the central Ukraine (CUNEY et al., 2012) and the Uranium City region in Canada (DAHLKAMP, 1993).High-temperature hydrothermal Th deposits are characterized by metasomatic replacements, accompanied by amphibolitization, aegirinization, biotitization, greisenization and filled open cavities (TITAYEVA, 1994).Obtained apatite ages confirm that IOA and the apatite-rich rocks (apatites) of the Bafq district formed coevally with the Early Cambrian magmatic (-metasomatic) events STOSCH et al. (2011).Alkali-metasomatism in the Chogart iron oxide-apatite (IOA) deposit occurred in peripheral alteration zones of the iron orebody.
It is observed by ground radiometric surveys using an RS-230 spectrometer that the radioactive anomaly of Th occurs at the margin of the Fe-orebody.Since no previous study has worked on Th-REE mineralization, the aim of this paper is to define the mineralogy of Th-REE bearing mineral assemblages and the role of alteration/s and metasomatic processes in their genesis.

GEOLOGICAL SETTING OF BAFQ DISTRICT
The geological setting of the Bafq district is described by RA-JABI et al. (2015).The crustal domain referred to as the Central Iranian microcontinent is a composite of three major structural zones, from E to W (ALAVI, 1991), the Lut, Tabas, and Yazd blocks (Figure 1a, b).The boundaries are defined by regionalscale faults (Figure 1).In addition, there is the Posht-e-Badam Block (ALAVI, 1991), a fault-bound, variably deformed and metamorphosed complex of supracrustal rocks that separates the Tabas and Yazd blocks (Figure 1).The Posht-e-Badam Block represents the area surrounded by three major fault systems (ALAVI, 1991) including the Chapedony, Kalmard and Kuhbanan faults.A Precambrian crystalline basement and Early Cambrian to Tertiary sedimentary cover are exposed in the block (FOSTER & JAFARZADEH, 1994).

Geologia Croatica
Kiruna-type iron ore deposits, are known to have formed from the Proterozoic to the Tertiary.They are commonly associated with calc-alkaline volcanic rocks and regional-to deposit-scale metasomatic alteration (STOSCH et al., 2011).

GEOLOGY OF THE CHOGHART DEPOSIT
The main roughly vertical, discordant, pipe-shaped magnetiteapatite orebody at Choghart, plunging 73°NNW, has been explored to a depth of 600 m, where it seems to interfinger with intrusive metasomatized and fragmented wall-rock.The thickness of the metasomatic zone differs widely.The orebody is hosted by volcanic members (rhyolitic to rhyodacitic in composition, as well as so-called quartz albitophyre) of the Infracambrian Esfordi Formation (MOORE & MODABBERI, 2003).
It is enveloped by metasomatic rocks with variable thickness.The ore body is crosscut by both diabase dykes and N-S trending normal faults.The iron concentration is not uniform throughout the ore body: the Fe content in the centre of the deposit is greater than 65% whereas it decreases to 45-20% towards the margins (MOORE & MODABBERI, 2003).The ore body is mostly surrounded by sodic-calcic hydrothermally altered rocks (Figure 3a, b), with minor albitite (5-30 cm wide).The P 2 O 5 content is very low (<0.2%) and it is enriched in the N-NE of the deposit.N-S, NW-SE and NE-SW trending normal faults cut each other and the ore body.The most well-known outstanding feature is the voluminous district-scale sodic-calcic alteration that developed in volcanic hostrocks.The Na-Ca alteration is enveloped as actinolite, apatite, magnetite, haematite, sodic plagioclase, chlorite, with or without epidote.Within the pervasively Na-Ca altered rhyolite and volcanoclastic rocks, there are locally patches with intense Na alteration with veins and veinlets of albite and a brecciated texture (TAGHIPOUR et al. 2013).Apatite is the most abundant gangue at Choghart.It is a distinctive, transparent, yellow-green fluor-apatite.Fine and coarse-grained apatite occur in varying proportions with magnetite, and apatite-bearing magnetite is the most abundant ore type at Choghart.At least two generations of apatite are discernible.The first, which is contemporaneous with the main phase of iron oxide formation, displays euhedral crystals ranging in size from a few millimetres to a few centimetres in diameter.It is intimately intergrown with magnetite.The second generation occurs as subhedral to anhedral crystals in lenses, dykes, and veinlets of varying size and thickness, which cut the magnetite-apatite ore (MOORE & MODABBERI, 2003).
Pyrite and quartz are distributed quite evenly in the orebody, either as solid inclusions in primary magnetite grains or as welldeveloped crystals in the orebody and the adjacent country rock.Some magnetite crystals are cemented by quartz and vice versa, indicating alternation of magnetite and quartz mineralization.Calcite, dolomite, secondary haematite and talc occur throughout the orebody as veinlets and cementing material of oxidized ore.Rutile and goethite are probably the result of the total transfor-the total transfor-total transfor-mation of the earlier formed martite (MOORE & MODABBERI, 2003).
The Th-REE enriched zone occurs within the south-eastern margin of the Fe-orebody between the F5 and F6 faults and it also cuts the sodic-calcic metasomatism/alteration as well as the host rhyolite (Figure 3a).The radioactive anomaly of thorium is observed in the margin of the Fe-orebody by ground radiometric and spectrometric surveys using an RS-230 spectrometer.Chem-an RS-230 spectrometer.Chem-RS-230 spectrometer.Chemical analyses of samples of this zone show Th-REE mineralization.The hydrothermal breccia and albitization (pink in colour), are both associated with Th-REE mineralization shown in Figure 4a, b.Carbonate-silica veins and veinlets cross cut the host rock, the Fe-orebody and Th-REE mineralization zone which indicates that they are formed after the Th-REE mineralization.

MATERIAL AND METHODS
Thirty-five samples were collected for petrographic, ore microscopic and geochemical studies from the Th-REE mineralization  zone (20 samples), volcanic host rock (10 samples) and diabase dykes (5 samples) at the Choghart deposit.The whole-rock concentrations of major oxides and trace elements were determined by inductively coupled plasma (ICP) optical emission spectroscopy (OES) and mass spectrometry (MS) at the Jaber-ebnehayyan laboratory of Nuclear Science and Technology Research Institute in Tehran, Iran.The detection limit for the main oxides and also the minor elements by ICP-OES is <10 ppm, and for the trace elements by ICP-MS is < 0.1 ppm.
In addition, the data obtained from previous studies in the Bafq district were also used to strengthen the discussion of results obtained from the present study (Table 1; RAMEZANI & TUCKER, 2003;MOHAMMAD TORAB, 2008;MIRZAEI BENI, 2014;RAJABI, et al., 2015).Petrographic and ore microscopic studies (including general recognition of mineral assemblages, alteration, metasomatic replacements and textures) were performed using an Olympus BX60 microscope at the petrography laboratory at the Shahid Beheshti University of Tehran.Based on optical microscope observations, 12 Th-REE mineralized thin-polished sections were selected for electron probe micro-analysis (EPMA).The detailed study of mineral assemblages, alteration, metasomatic replacements and textures was carried out at the mineralogy division of the Iranian Mineral Processing Research Centre (IMPRC) using a Cameca SX-100 electron mi-croprobe equipped with 5 wavelength-dispersive crystal spectrometers.Measurements were performed using an accelerating voltage of 15 kV, a beam current of 20 nA, beam size of ~5 µm and 15s counting time for major elements and an accelerating voltage of 25 kV, a beam current of 20 nA, beam size of ~3 µm and 30s counting time for trace elements.Natural oxides and silicates were used as standards and for calibration.Raw data were corrected for matrix effects with the ZAF correction procedure implemented by CAMECA.

Geochemistry of host rocks and mineralization
The rare earth elements (REE), high-field-strength elements (HFSE), Th and transition elements are usually immobile during intense hydrothermal alterations.In addition, the hydrothermal fluids do not have a great capacity to transport some of the major elements such as Ti and P (e.g.ZHOU, 1999).In contrast, Mg, Ca, Mg, Na, K, and some of the large ion lithophile elements (LILE; e.g.Sr, Ba and Rb) are mobile under hydrothermal conditions (e.g., mobility SMITH & SMITH, 1976).Immobile trace element geochemistry (including REE) is utilized here to deduce the tectonic setting of the igneous rocks.6c).Rhyolitic rocks of the Bafq district are noticeably enriched in Th and depleted in Ta, Nb and Ti (Figure 6d).Because the mantle was progressively modified by subducted oceanic crust, felsic volcanic rocks became enriched in Th and LREE compared to Ta, Nb, and HREE (SCHANDL & GORTON, 2002).
The Primitive-mantle-normalized geochemical patterns, arranged in order of incompatibly elements, indicate that the basaltic rocks of the Bafq district are more LREE-and HFSE (Th, Nb, Ta, Zr, Hf)-enriched rather than E-MORB or N-MORB (Figure 6d).
Considering the afore mentioned context, the Choghart rhyolite is similar to other felsic volcanic rocks and ECVSS granites formed in a continental margin setting, and like other continental margin rocks are noticeably enriched in Th and LREE compared to Ta, Nb, and the heavy rare earth elements.Likewise, the diabase dykes of Choghart have alkaline compositions similar to other diabase dykes and mafic rocks of the early Cambrian volcano-sedimentary sequence and were formed in a back-arc basin environment.Based on the results obtained during the study, the evolution of the Bafq district is genetically, related to the subduction of Palaeotethys oceanic crust beneath the Central Iranian microcontinent followed by formation of continental arc granitoids and rhyolites and then formation of back-arc basin diabase dykes (RAJABI et al., 2015).Diabase dykes were formed in a back-arc extensional setting after magnetite-apatite and Th-REE Since the volcanic host rocks of the Choghart deposit are affected by hydrothermal alteration, the immobile elements are employed for petrogenetic interpretations of the rhyolites in the Bafq district (Chahmir, Koushk, se-Chahun, Choghart, etc.).
On the log (Zr/TiO 2 ) vs. log (Nb/Y) plot of WINCHESTER & FLOYD (1977), effusive rocks range from rhyolite to dacite in composition (two samples of Choghart lie within trachy-andesite field), and the samples of diabase dykes from the Bafq district plot within the alkaline basalt field (two samples of Choghart plot within the basalt field) (Figure 5a, b).
HFSE ratios in felsic volcanic rocks reflect the regional tectonomagmatic evolution.Th/Ta, Th/Hf, Ta/Hf, Th/Yb, and Ta/Yb ratios help to define the tectonic setting of volcanism, separating oceanic arcs, active continental margins, and within-plate volcanic zones (SCHANDL & GORTON, 2002).The rhyolites of the Bafq district particularly Choghart are enriched in Th and the light rare earth elements compared to Ta, Nb, and the heavy rare earth elements that are related to subduction zones.Variable Th/Ta ratios within individual deposits show fractionation trends (Figure 5c; SCHANDL & GORTON, 2002).
The Ce/Nb vs. Th/Nb plot of SAUNDERS & TARNEY (1991) is useful in discriminating the tectonic environment of mafic rocks, because these elements are immobile during alteration processes.The diabase dyke samples of the Bafq district plot in the field of within-plate basalts (WPB); except for two samples of Choghart that plot out of this field in the field of continental margin volcanic arc basalt.This is possibly because of high con-.This is possibly because of high con-This is possibly because of high concentrations of Th (Figure 5d).Furthermore, Th and Ta behave coherently in non-subduction-related basalts, decoupling only in the subduction environment (WOOD, 1980).The Chondrite-normalized REE patterns (Fig. 7b) of Th-mineralization zone samples show a weak LREE/HREE fractionation and pronounced negative Eu anomaly.In addition, the similarity between the Chondrite-normalized REE patterns of the rhyolites and Th-mineralization zone in the Choghart mine is obvious.The negative Eu anomaly in the Th-mineralization zone of Choghart could be inherited from the fluid source.This implies that the fluid originated from rocks in which plagioclase has removed Eu 2+ or equilibrated with them, because Eu 2+ substitutes for Ca 2+ in plagioclase, early crystallizing plagioclase in magma will remove Eu 2+ from the system and thus a later exsolving fluid will be depleted in Eu.Additionally, if a fluid equilibrates with a plagioclase-bearing rock and doesn't dissolve pla-  gioclase, then the depletion in Eu will be inherited by the fluid.The negative Eu anomaly may reflect reducing conditions of the mineralizing fluid and depositional environment.Beside the RE-DOX conditions, the Eu 2+ /Eu 3+ ratio can be controlled by temperature (BAU & MÖLLER 1992).Since paragenetic magnetite, pyrite and chalcopyrite in mineral assemblages of the Th-mineralization zone were observed, the negative Eu anomaly is most likely due to the reducing conditions of the mineralizing fluid and depositional environment.According to Figure 7b, the chondritenormalized REE patterns of the Choghart rhyolite and Th-REE mineralization zone are similar, suggesting that Th and REE origi nated from continental margin Choghart rhyolitic magma.

Mineralogy
The microscope studies indicated that the main Th mineral in Th-REE mineralization zone is thorite (Figure 8a, b) which occurs in veinlets, either disseminated or as inclusions in other minerals such as albite and clinopyroxene.Minor amounts of thorite are associated with the sodic-calcic altered magnetite ore body.Sphene is the other host mineral of REE but is quantitatively less important than thorite.Two generations of sphene are recognized; the first, primary sphene which occurs as individual crystals and was likely precipitated directly from the mineralizing fluids (Figu re 9a), and the second generation of sphene that formed by alteration of ilmenite (Figure 8c).Calcium-and silica-rich mineralizing fluids cause the alteration of ilmenite that is converted to sphene and rutile.Iron released from ilmenite alteration precipitated as magnetite (Figure 8c).In some microscope sec-tions, ilmenite is observed to be converted to rutile and titanomagnetite (Figure 8c).Formation of magnetite, sphene and rutile suggests that probably the temperature of mineralizing fluids was relatively high.The occurrence of magnetite as a fracture filling in thorite indicates that it precipitated after thorite formation.
The silicate minerals accompanied by Th-REE mineralization include albite, amphibole and pyroxene.Following the nomenclature of LEAKE et al. (1997) and EPMA analyses (Table 2),  the amphibole belongs to the calcic group and is actinolite (except for 2 points which fall in the tremolite field, Figure 10).According to the nomenclature of MORIMOTO et al. (1989) and EPMA analyses (Table 3), all pyroxenes belong to Ca-rich pyroxene and fall mainly in the augite field and three samples have the composition of diopside (Figure 11).Also calcite, magnetite, pyrite, chalcopyrite and trace amounts of galena are associated with this type of mineralization.Two generations of galena are discernible; the first is contemporaneous with Th-REE mineralization (Figure 9b) and the second generation of galena formed after Th-REE mineraliza-  tion as a fracture filling of thorite (Figure 9c).Pb released from thorite (the decay product of Th) probably forms the second generation of galena, provided the activity of S is sufficient.The presence of magnetite, pyrite and chalcopyrite is likely due to relatively reduced conditions in the thorite depositional environment.
The paragenetic mineral assemblage of Th-REE mineralization of the Choghart iron oxide apatite deposit is shown in Figure 12.
The results of bulk chemical analyses show a high correlation of Ce, La, Y and Nd concentrations with the Th content.The EMPA analyses show that thorite contains mean values of 9460 ppm Ce, 1950 ppm La, 1810 ppm Y and 110 ppm Nd (Table 4).The EMPA analyses of sphene shows mean of 8050 ppm Ce, 3650 ppm Y while the contents of La and Y are below the detection limit (Table 5).

Alkali Metasomatism
Alkali metasomatism implies the transfer of the alkali ions, Na and K, from a fluid phase, generated during the cooling of an igneous body, to the adjoining rocks.Albitite, microclinite, fenites, and the core zones of potassic alteration of porphyry systems are This event is clearly associated with Th-REE mineralization at Choghart (Figure 13b).The replacement of alkali feldspar by albite (albitization or Na-feldspathization) shows the more common form of sodic metasomatism.This replacement may proceed from either preexisting perthites, or direct replacement of K-feldspar with late formed albites (POLLARD, 1983).
The replacement of K-feldspar by albite occurs pervasively accompanied with the Th-REE mineralization zone at Choghart (Figure 13c, 4b).Albitization of K-feldspar can be written as follows: KAlSi 3 O 8 +Na + =NaAlSi 3 O 8 +K + The development of albite-rich rocks (albitites) is typically accompanied by rare element mineralization (Nb, Ta, Sn, W, Li, Be).Sodium-enrichment is associated with elevated concentrations of Fe, U, Th, Zr, Nb, Sn, Zn, and HREE.Na-metasomatised rocks are also more prone to be enriched in Rb, Th, Nb, La, Ce, Hf, Zr, and Y with regard to K-metasomatised rocks (KINNAIRD, 1985).The Choghart Th-REE mineralization zone is enriched in Th, La, Ce, Nd, and Y.
The high-temperature post-magmatic processes can promote the mobilization and concentration of thorium.In these processes thorium is usually associated with rare-earth elements (the lanthanides).Most post-magmatic thorium-containing deposits are connected with pneumatic-hydrothermal or high-temperature hydrothermal processes.At present we know that Th-REE deposits have post-magmatic genesis (TITAYEVA, 1994).
The main paragenetic associations of thorium are the lanthanides.In high-temperature deposits Th is usually associated with Та, Nb, Ti, and occasionally with Mo, W, Sn, Be.In moderatetemperature deposits Th is paragenetically associated with Pb, Zn, Cu.The anion components such as Cl -, HCO 3 -, CO 3 2-, HS -, S 2-and F -are important and control the mobility of metals in post-magmatic fluids (TITAYEVA, 1994).
As mentioned above the Th-REE mineralization zone (thorite and sphene) in Choghart is associated with albitization, amphibolitization (actinolite), pyroxenitization (augite and diopside), carbonatization and minor K-feldespatization (microcline), as well as the occurrence of pyrite and minor amounts of chalcopyrite, considered to be a moderate-temperature post-magmatic Th-REE mineralization type.

Mineral formation conditions
Thermodynamic calculations have indicated that fluoride or mixed carbonate-fluoride complexes can dominate REE speciation (e.g., WOOD, 1990a, b).The scarcity of the F-bearing REE minerals (flourapatite) in the Th-REE mineralized zone of Choghart, however, implies that a high concentration of fluorine was probably, only locally, achieved and is not necessarily a component of the composite ore-forming fluids.
The presence of calcite along with calcic-amphibole andpyroxene (actinolite and augite, respectively), the high content of Ca in thorite (Table 6; up to 2.3% CaO) and the occurrence of sphene in the Choghart Th-REE mineralization zone imply that thorite crystallized from a Ca 2+ -and CO 3 2--bearing aqueous solution under conditions of low activity of F -.
Considering that dolomitic xenolites of the Esfordi formation are observed in the volcanic host rocks of the Choghart deposit, the portion of CO 2 in the mineralizing fluids is supplied by digestion of these xenolites.
According to the presence of paragenetic calcite accompanied with thorite and sphene in Th-REE mineralization, Th and REE transport was likely because of the presence of the carbonate complexes in mineralizing fluids.
According to TITAYEVA (1994) and PIRAJNO ( 2009) at the end of albitization processes, the thorium and uranium concentrations increase.Part of REE and U-Th is retained in microfissures filled with haematite and chlorite.The reddish colour is attributed to the presence of micro-haematite in micro-fractures.Although, WILDE (2013) has portrayed that the red or pink coloration is owing to the presence of fine-grained disseminated haematite or hydrothermal apatite.Our data revealed that albites from the Choghart Th-REE mineralization zone contain K-feldspar and minor Th silicate mineral inclusions (i.e.thorite) that give albite a more reddish colour (Figure 4B).MOORE & MODABBERI (2003) suggest that the separation of an iron oxide melt and the following hydrothermal processes dominated by alkali metasomatism have both been involved to in different degrees in the formation of the Choghart deposit.Alternatively, the Choghart rhyolite is enriched in Th and LREE similar to other continental margin felsic volcanic rocks.Chondritenormalized REE patterns of the Choghart rhyolite are similar to the Th-REE mineralization zone, indicating that Th and REE originated from a continental margin Choghart rhyolitic magma.

CONCLUSIONS
We suggest that in the Early Cambrian (about 533 Ma) calcalkaline granitoid magmatism associated with a subduction zone in the Choghart deposit initially formed a magnetite-apatite ore body and sodic-calcic alteration followed by penetration of the remaining magmatic fluids into the rhyolitic host rocks and also sodic-calcic alteration related to iron mineralization and partially brecciation.These fluids maintain elevated concentrations of metals such as Fe, Th and REE that were originally scavenged from the rhyolitic silicate melt due to the magmatic temperatures and high salinity of the fluid (REED et al., 2000;SIMON et al., 2004SIMON et al., , 2005SIMON et al., , 2006;;ZAJACZ et al., 2012;FRANK et al., 2011;MIGDISOV et al., 2014;HURTING & WILLIAMS-JONES, 2014).These fluids caused sodic metasomatism (albitization), carbonatization, actinolitization and pyroxenitization, minor K-feld-spatization (microcline) as well as generation of the minerals such as thorite and sphene.Alternatively, the Th-REE mineralization zone may have formed from entirely different fluids related to a later intrusion such as the resurgent central plutons.
The high CO 2 content of the fluid facilitates formation of metal-carbonate complexes.The presence of paragenetic calcite with thorite suggests that carbonate complexes most likely transferred the Th and REE.Considering that dolomitic xenoliths of the Esfordi Formation are observed in the volcanic host rocks of the Choghart deposit, the portion of CO 2 in the mineralizing fluids is supplied by digestion of these xenoliths.The negative Eu anomaly from the Th-REE mineralization zone and the presence of paragenetic magnetite, pyrite and chalcopyrite with thorite suggests relatively reduced conditions in the Th-REE mineralization environment.

Figure 1 .
Figure 1.(A) Simplified structural map of Iran (AGHANABATI, 1998) and location of the Bafq district in the Posht-e-Badam Block; (B) Eastern part of the Terranes map of the western Tethysides (RAJABI et al., 2012; modified by after STAMPFLI, 2009; according to BAGHERI & STAMPFLI, 2008).Note the location of the Iran Plate (Iranian Cimmerian terranes) between the Variscan domain in the north and the Arabian Plate in the southwest (ZTZ: Zagros Thrust Zone).

(
RAMEZANI & TUCKER, 2003) that partly metamorphosed to greenschist facies.During the Early Cambrian, granitic plutons intruded the Precambrian sequence of the Tashk Formation, and felsic to intermediate volcanic and volcano-sedimentary rocks of the Early Cambrian volcano-sedimentary sequence (ECVSS) were deposited.The 2000-2500 m thick ECVSS unconformably overlies the clastic sedimentary and tuffaceous rocks of the Tashk Formation.This contact is well exposed to the W and SW of the Narigan area.The ECVSS has also been termed the Cambrian Volcano-Sedi-

Figure 6 .
Figure 6.shows the Chondrite-and primitive-mantle-normalized REE patterns.The patterns for basaltic rocks (Figure 6a, b) display significant variation from LREE to HREE, similar to oceanic-island basalts (OIB).Most REE patterns of felsic rocks display enrichment in the LREE, with relatively flat HREE patterns (Figure6c).Rhyolitic rocks of the Bafq district are noticeably enriched in Th and depleted in Ta, Nb and Ti (Figure6d).Because the mantle was progressively modified by subducted oceanic crust, felsic volcanic rocks became enriched inTh and LREE compared to Ta, Nb, and HREE (SCHANDL & GORTON, 2002).The Primitive-mantle-normalized geochemical patterns, arranged in order of incompatibly elements, indicate that the basaltic rocks of the Bafq district are more LREE-and HFSE (Th, Nb, Ta, Zr, Hf)-enriched rather than E-MORB or N-MORB (Figure6d).Considering the afore mentioned context, the Choghart rhyolite is similar to other felsic volcanic rocks and ECVSS granites formed in a continental margin setting, and like other continental margin rocks are noticeably enriched in Th and LREE compared to Ta, Nb, and the heavy rare earth elements.Likewise, the diabase dykes of Choghart have alkaline compositions similar to other diabase dykes and mafic rocks of the early Cambrian volcano-sedimentary sequence and were formed in a back-arc basin environment.Based on the results obtained during the study, the evolution of the Bafq district is genetically, related to the subduction of Palaeotethys oceanic crust beneath the Central Iranian microcontinent followed by formation of continental arc granitoids and rhyolites and then formation of back-arc basin diabase dykes(RAJABI et al., 2015).Diabase dykes were formed in a back-arc extensional setting after magnetite-apatite and Th-REE

Figure 6 .
Figure 6.Chondrite and primitive mantle normalized rare earth elements and incompatible elements distribution patterns (Spider diagrams) (SUN and MC DONOUGH, 1989) for the Bafq district (A, B) diabase dykes and (C, D) rhyolitic rocks

Figure 7 .
Figure 7. (A) The K 2 O vs. Na 2 O diagram for Th-REE mineralized samples; (B) Comparison of chondrite-normalized REE patterns of the Choghart rhyolite and the Th-REE mineralization zone.

Figure 10 .
Figure 10.Classification of the calcic amphiboles in the Th-REE mineralization zone of Choghart.

Figure 11 .Figure 12 .
Figure 11.Classification of the Ca-rich pyroxene in the Th-REE mineralization zone of Choghart.

Table 1 .
Major and trace elements (REE, HFSE, LILE) of the felsic and basic rocks of the Bafq district (major oxides in percent and minor and trace elements in ppm;

Table 3 .
Representative electron microprobe analyses of pyroxene in some studied samples, Detection limit < 0.01%.

Table 2 .
Representative electron microprobe analyses of amphibole in some studied samples, Detection limit < 0.01%.