Vast stretches of granites with high strain equivalent gneisses, enclosing narrow linear greenstone belts, represent the Archaean granite-greenstone terrain of eastern block of Dharwar craton (EDC). The important greenstone belts of EDC include the Ramagiri-Penakacherla-Hungund-Kushtagi superbelt, Kolar-Kadiri-Julakava-Jonnagiri-Hutti-Muski superbelt, Veligallu-Gadwal superbelt, Tsundupalli schist belt and Nellore-Khammam super belt. Recent studies indicated these greenstone belts as composite tectonostratigraphic terranes of accreted plume-derived and convergent margin-derived magmatic sequences [1]. Earlier workers revealed four magma suites in the EDC: 1) Tonalite-trondjhemite-granodiorite gneiss suite (TTG); 2) Trondjhemite-granodiorite-monzogranite (TGM) suite; 3) Monzosyenite-syenogranite (MS) suite; and 4) Granite and k-feldspar granite suite (AFGS) i.e. shear controlled post orogenic granites and anarogenic (A-type) granites [2] - [15].

The present study area is the central part of the trident-shaped Ramagiri supracrustal belt (RSB), surrounded on all sides by granitoid gneisses and intrusive granites. Tectonic mélange of basaltic and felsic bimodal lavas intermixed with minor amounts of clastic sediments defines the RSB. The trident shape of the belt is due to alternating high-level diapiric intrusion of granitoids and rocks of schist belt [16] [17] [18] [19].

Detailed petrographic and geochemical characterizations of the granitoids around Kadiri, Kolar, Velligallu, and Nellore schist belt have been done by different authors and the petrogenesis of these granitoids with respect to the overall genesis of the schist belts has been worked out. [13] grouped the granites and gneisses of Penakacherla schist belt into TTG, TGM and MS suites, based on their lithological association. They also, evaluated their structural, petrographic, petrochemical characteristics, mutual field relationships and relationship with the schist belt.

However, a comparative petro-chemical characterization of the granitoids in the central part of trident shaped RSB, specifically, of the granitoids between central and western arm of RSB, is yet to be done. Hence, the present work details the distribution, field relations, petrography and geochemistry of the granites and gneisses in the central part of RSB in and around Balepalyam and Ramagiri village. Detailed field and petrographic studies of the granitoids observed in the study area are first used to club them under the established magma suites as per IUGS scheme, followed by the genetical classification of the granitoids. Also, emphasis has been given on the behavior of trace elements and REE of the various granitoids and geothermobarometry to determine their petrogenesis and their implication in bearing certain mineralization.

The study area is confined to the granitoids occupying the area around the central and western arms of RSB in its central part near Ramagiri and Balepalyam village. The central arm of the RSB is comprised of mainly chlorite schist, carbonaceous chlorite schist and massive and foliated metabasalt. The western arm of the schist belt is comprised of pillowed metabasalt, chlorite schist, carbonaceous chlorite schist, banded iron formation, quartzite, and ultramafites. Dolerite/gabbro dykes traverse all the units occurring in the area. Further they were intruded by kimberlites, lamprophyres and granophyres. The two arms are surrounded by different phases of granitoids (Figure 1).

Mineralogical observations during the present study broadly revealed three categories of granitoids in the area: Migmatite gneiss, granodiorite and monzogranite. The granodiorites and monzogranites are further categorized as equigranular and porphyritic based on the textural properties of the granitoids. Granodiorites are gneissic at places. The present study mainly compares the field, petrographic and geochemical characteristics of the broad categories of granodiorites, monzogranites and migmatite gneiss, with special emphasis on the petrogenesis of granodiorites and monzogranites.

Migmatite gneiss is grey, medium grained, mesocratic, defined by layers of melanosome and criss-cross patterned leucosomes (Figure 2(a)). These rocks show stromatic, ptygmatic and phlebitic structures. Melanosomes of the migmatite gneiss are comprised of fine to medium grained biotite (10%) and hornblendes (5%) while the leucosome part is mostly dominated by coarse grained quartz (30% - 35%), plagioclase (25% - 30%), k-feldspar (5% - 10%), and traces of magnetite, sphene, and pyrite (2%).

The granodiorites and monzogranites are spatially associated with each other and usually occur as vastly spread, large lenticular stocks. Granodiorites are mesocratic and grey colored with medium to coarse grained texture. The dominant mineralogy is quartz (20% - 25%), plagioclase (25% - 35%), and k-feldspar (12% - 15%), with subordinate amounts of hornblende (10%), biotite (2% - 3%) and traces of sphene and apatite. The rock occurs as both equigranular and porphyritic variety. Due to the equigranular mosaic of felsic and mafic minerals in the equigranular variety, the rock appears as salt and pepper texture (Figure 2(b)). The porphyritic granodiorites are characterized by large, lath-shaped plagioclase grains embedded in a groundmass of quartz, plagioclase, alkali feldspar and mafics (Figure 2(c)). The size of the phenocrysts varies from 0.5 cms to upto 3 cms. The monzogranites are weathered near the surface. The rock is recognized by its flesh-pink color, leucocratic nature and medium to coarse crystals of k-feldspar (30% - 35%), quartz (25% - 30%), plagioclase (20% - 25%) and traces of biotite (5%) and apatite (Figure 2(d), Figure 2(e)). K-feldspars occur as both large phenocrysts and groundmass. The k-feldspar phenocrysts are tabular, size varying from <5 mms to 5 cms and contain inclusion of sericitized plagioclase, biotite and granular quartz. This rock is devoid of synplutonic microgranitoid enclaves-dykelets. Arrangement of phenocrysts of feldspars in both granodiorites and monzogranites in a particular direction defines a crude magmatic foliation in the rock. The contact of the granodiorites and monzogranites with the schist belt is generally sharp and intrusive but tectonised at places due to later shearing (Figure 2(f)).

Presence of mafic microgranular enclaves (MME) is observed in all the three rocks (Figure 3(a), Figure 3(b)). However, in the monzogranites, presence of both MME and small dyke like bodies of mafic rich microgranitoids and enclavial bodies (MMDs) is observed (Figure 3b). They are few meters in length and their intrusive nature is indicated by the angularity of the length of the dykes. Rapakivi texture is also observed very prominently in some of the plagioclase phenocrysts within the monzogranite, indicating magma mixing and mingling (Figure 3(c)).

Several gold and pyrite bearing quartz veins (±tourmaline, ±scheelite) are observed in the area within the monzogranites.

Enclaves of dominantly metabasalt and amphibolites of RSB are observed in all these three types of granitoids, indicating the granitoids occupying areas between the central and western arm and west of western arm of schist belt to be younger than the rocks of RSB, possibly belonging to the TGM suite of PGC-II.

In thin section of migmatite gneiss, plagioclase is normally zoned and carries fine inclusions of sphene, apatite, zircon and rutile that lie in planes parallel to long axes or the twin planes of these plagioclase crystals (Figure 4(a)). Alternately arranged mafic and felsic minerals produces the gneissic structure and granoblastic texture (Figure 4(b)). K-feldspar megacrysts show intensive perthitization of exsolution origin and some include xenomorphic quartz crystals between the idiomorphic cores and their outer rims (Figure 4(c)). Porphyritic, myrmekitic and graphic textures are common in these rocks (Figure 4(d)). Biotite and hornblende show alteration to chlorite and epidote. Plagioclase and potash feldspar show alteration to saussurite and kaolinite respectively. The above observations suggest that the rock was originally metamorphosed to amphibolite grade and subsequently underwent retrogression.

The granodiorites show holocrystalline, seriate to hypidiomorphic texture and essentially consists of quartz, plagioclase, biotite, hornblende, potash feldspar. Epidote, apatite, sphene and opaques constitute the accessory minerals (Figure 5(a)). Quartz is present as strained grains and includes incipient sub-grains. Plagioclase crystals are idiomorphic or hypidiomorphic, mostly unzoned and poikilitic, moderately altered to sericites and epidotes. The plagioclase is characterized by lamellar, manabech and pericline twins, and the microcline perthite is of stringe perthitic nature. Plagioclase either occurs as large phenocrysts of 300 - 400 µm (Figure 5(b)) porphyritic variety and as equigranular grains of 50 - 100 µm. K-feldspar and quartz crystals are mostly allotriomorphic. Hornblende occurs as idiomorphic to hypidiomorphic rhombus with strong pleochroism and intergrown with granular quartz and biotite. Biotite occurs as dark reddish brown to yellowish brown pleochroic crystals in the groundmass.

Monzogranite shows hypidiomorphic texture, composed of subhedral microcline crystals of 300 to 500 µm in equigranular variety and 2 - 3 mms crystals in porphyritic variety (Figure 5(c), Figure 5(d)), sericitised plagioclase and allotriomorphic quartz. Chloritised biotite crystals occur as trace minerals. Exsolution and intergrowth textures like perthitic and granophyric are very common. These granites show microstructural deformation features, viz., strained quartz grains, kinked mica and deformation twins in plagioclase.

24 samples of granitoids have been studied as part of whole rock geochemistry. 04 nos of samples of migmatite gneiss, 08 nos of granodiorite samples and 12 nos of monzogranite samples are chemically analyzed along with their C.I.P.W. norm values (Table 1). Major oxide geochemistry of the granitoids was carried out in Chemical Division of Geological Survey of India, Southern Region, Hyderabad. Fresh, unaltered samples of 1 - 1.5 kgs weight were collected from each of the granitoids observed in the area. The samples were, then, crushed and pulverized to −120 micron size for chemical analysis. Major oxide data have been provided by X-Ray Fluorescence (XRF) instrument PANalyticalmagix 2424 (WD XRF) of power 2.4 kw at Chemical Division of Geological Survey of India, Southern Region, Hyderabad. Samples are prepared using the pressed pellet method. To ensure precision of data, the instrument is calibrated with 7 international standards (4 inhouse standards).

Mineral chemistry of the constituent mineral phases was determined by Electron ProbeMicro Analysis, EPMA SX100 of Cameca (France), with 5 vertically mounted Wavelength Dispersive Spectrometers for WDS analysis and LAB6 crystal, make installed Regional Petrological Laboratory of GSI, SR, Hyderabad is used for EPMA studies. Operating conditions of 15 keV accelerating voltage and 15 nA of beam current was used for major elements. A counting time of 10 seconds was used. For Xray measurements diffracting crystals like PET, TAP and LIF crystals were used depending on the measured elements. Beam diameter was set to 1 micron. Well known and internationally accepted standards developed by P&H Developers were used for calibration. Analytical uncertainty (standard deviation) during the calibrations and analysis of samples was <1%. During the analysis of silicate phases, K alpha lines were used for measurement for analysis of major elements like Si, Ti, Al, Cr, Mn, Fe, Ni, Mg K, Ca, Na and P.

All samples of granitoids of the study area are unaltered and fresh with CIA values varying from 49.12 to 57.82 for monzogranites, 46.05 to 58.61 for granodiorites and 48.9 to 51.53 for migmatite gneiss (Table 1). From the biplot of clr-transformed data of each sample, it is observed that the samples of monzogranite, granodiorite and migmatite gneiss trend perpendicular to the PC1 coordinate, which indicates all of them to be unweathered igneous rocks (Figure 6(a)). All the samples plot near the igneous rock trend line in the MFW ternary plot and away from the W index, indicting the samples to be fresh and unweathered (Figure 6(b); calculations as per [20]). All the samples have normative quartz and hypersthenes.

In the normative QAP classification diagram (Figure 7(a)), all the samples of monzogranites, plot in the monzogranite field while all the samples of granodiorite and migmatite gneiss falls either in the granodiorite field or near it. On the Ab–An–Or diagram [21], the samples plot within the expected fields (Figure 7(b)). Samples of migmatite gneiss are taken from both leucosome and melanosome part. It is observed that the samples of leucosome fall in the granite field and those of melanosome fall in the granodiorite field. The TAS classification of the granitoids follow similar trend wherein the monzogranite samples occupy the granite to monzogranite field and the granodiorite samples span from granodiorite to diorite (Figure 7(c)). All the samples plot in the sub alkaline field, defined by [22]. On the other hand, in the R1-R2 plot, monzogranite samples plot in the granite to alkali granite field and granodiorite samples plot in the granodiorite to tonalite field (Figure 7(d)). The samples of the granitoids are then plotted on a series of discrimination plots to identify and genetically classify the granites (Figure 8; after [23]). Based on the plots, it is observed that majority of the granitoids plot in the I- & S-type field. A few samples that though falls on the line separating the two fields, is not consistent in every diagram. All the samples are metaluminous to peraluminous in the molar Na₂O + Al₂O₃ + K₂O plot (Figure 9(a)), however, the samples of monzogranite have lower A/NK ratio than the samples of granodiorite and migmatite gneiss.

In the B-A plot and A/CNK-A/NK plot, the monzogranite samples plot either within or close to the peraluminous field and the granodiorite samples plot in the metaluminous field (Figure 9(b), Figure 9(d)). Samples of migmatite gneiss show variable character. The monzogranites samples fall close to the S-Type field than the granodiorite samples in the A/CNK-A/NK plot. The entire samples plot in S-type field in CaO-Al₂O₃ + Na₂O + K₂O-FeO_t + MgO ternary plot but the granodiorite samples have higher CaO content than the monzogranites (Figure 9(c)). Presence of hornblende in the granodiorites is also indicative of I-type granite affinity.

The samples plot in the High K-calc-alkaline and shoshonite series in the Co-Th plot (Figure 10(a)). On the SiO₂-K₂O plot, the monzogranite samples plot in the high-K calc-alkaline series and granodiorite samples plot in the calc-alkaline to high-K calc-alkaline series (Figure 10(b)). In the SiO₂ vs FeO_t/(FeO_t + MgO) plot and SiO₂ vs Na₂O + K₂O-CaO plot, the monzogranites plot in the ferroan field and straddle fields of alkali to calc-alkalic, respectively (Figure 10(c), Figure 10(d)). The granodiorites and migmatite gneiss are both ferroan and magnesian in nature and occur along the boundary between alkali and alkali-calcic field [24].

On the primitive mantle normalized multi-element spider diagrams, samples of granodiorite show similar patterns with more or less same degree of elemental enrichment. They show characteristic features common to I-type granites, viz., distinctive depletion of LILE’s like Ba, and HFSE’s like Nb, P and Ti relative to other trace elements (Figure 11(a)).

Chondrite normalized REE patterns reveal a distinction between monzogranite and granodiorite (Figure 11(b)), where samples of granodiorite show similar patterns with a lesser degree of REE fractionation ((La/Yb)_N =11.03 - 36.51) than monzogranite, which shows a higher degree of fractionation ((La/Yb)_N = 1.66 - 40.10). The granodiorite has high ΣREE (an average 327.905 ppm) content, and shows LREE enrichment ((La/Sm)_N = 3.1 - 6.8) with enriched but relatively flat HREE ((Gd/Yb)_N = 1.75 - 5.26) patterns and weak negative to positive Eu anomaly (Eu/Eu* = 0.62 - 1.18). Monzogranites, on the other hand, has relatively low ΣREE (an average 118.693 ppm) contents and exhibits strongly fractionated REE patterns with highly enriched LREE ((La/Sm)_N =1.74 - 9.76) and depleted HREE ((Gd/Yb)_N = 0.43 - 2.21) patterns having concave upward shape, and show strong negative Eu anomaly (Eu/Eu* = 0.23 - 0.89).

Major elements of the granodiorites and migmatite gneiss form well defined clusters and trends in Harker bivariate plots (Figure 12), where TiO₂, P₂O₅, CaO, FeO_t, MgO and MnO concentrations decrease monotonously with increasing amount of SiO₂. K₂O and Al₂O₃ display a weak positive correlation with SiO₂.

In monzogranites, all the oxides except Na₂O show decreasing concentration with respect of SiO₂. Na₂O, however, is independent of the SiO₂ in all the samples. The overall pattern of decreasing TiO₂, FeO_t, MgO and CaO with increasing SiO₂ is characteristic of fractionating granitic systems. The variation patterns of selected trace elements with respect to each other and SiO₂ however indicates fractionation in both monzogranites and granodiorites (Figure 13).

Sr and Zr generally decrease with increasing SiO₂ for all samples of granodiorites and migmatite gneiss whereas Rb and Ba show little correlation with increasing silica. In monzogranites, Ba, Sr and Zr negatively correlate with SiO₂. Rb and Ba are more enriched relative to Sr, and overall Rb/Sr ratios are high but

comparatively higher in monzogranite (0.62 - 4.08) than granodiorite (0.03 - 0.62). The major and trace elements along with inter-elemental variation diagrams suggest key role of fractional crystallization processes during petrogenesis of these granites, which is more in case of monzogranites. The Ba–Sr plot in logarithmic coordinates shows the presence of two distinct but broadly parallel linear trends, the first represented by monzogranitic and the second by granodioritic samples (Figure 13(g)).

The first trend is compatible with up to 15% fractional crystallization of a K-feldspar > plagioclase assemblage. The Ba-Rb plot in lograthmic coordinates confirms that K-feldspar with minor plagioclase fractional crystallization is a plausible model to explain the variation in the monzogranites (Figure 13(h)). This is also observed from (Zr + Nb + Ce + Y) vs (K₂O + Na₂O)/CaO plot where the samples of monzogranites are more fractionated than the granodiorites and thus fall in the fractionated felsic granite field while the granodiorites and migmatite gneiss samples plot in the normal I/S/M-type granites (Figure 8(b)). This can be explained by the high K content of the monzogranites.

On the Granite tectonic discrimination diagram of [33], barring a few, all the granitoids plot in CCG + IAG + CAG field (Group I; Figures 14(a)-(d)). Further discrimination within this group I can be accomplished only on the basis of Shand’s index (Figure 9(d)). Granitoids under CCG usually have A/CNK [AL₂O₃/(CaO + Na₂O + K₂O)] values greater than 1.15 [34]. But in the samples of present area, only few samples have values greater than 1.15. Majority of the samples have A/CNK values less than 1.15, which indicates a similar setup of the granitoids in the IAG + CAG group. However, it is not possible to discriminate between IAG and CAG through these diagrams. Accordingly, the most widespread trace-element plot is used to distinguish the tectonic setting of granitoids by the Rb v. (Y + Nb) plot of [35].

Based on this diagram, the granodiorites and monzogranites plot in the volcanic arc granites (VAG) field (Figure 15). According to [35] model (see also [36]), the high Rb component of VAG and/or post-COLG comes from enriched mantle or subducted crust, possibly augmented by Rb-rich, subduction-derived fluids. Incompatible elements, such as Nb + Y are diluted in the melt with higher melting. Hence, their low content in the granodiorites and monzogranites indicate higher melting in these granitoids. The R₁-R₂ scheme of [26], was specifically adapted by [37] into a tectonic framework by modifying the subdivisions postulated by [38]. In this scheme, the granodiorites and migmatite gneiss belong to the pre-plate collision field and the monzogranites straddle the field from post orogenic to syn-collision to Late orogenic fields (Figure 16).

Mineral chemistry of 2 samples of granodiorite and 2 samples of monzogranites are done to determine the dominant mineralogy of the rocks and to determine the emplacement pressure of each (Figure 17(a)). The elemental analyses of biotite, hornblende and feldspars are given in Table 2, Table 3.

Amphibole structural formula was calculated based on 23 oxygen atoms, according to the methods of [39] and [40] and feldspar structural formula are calculated based on 32 oxygen atoms. In the granodiorite samples, feldspars are mostly andesine to oligoclase and amphiboles are tschermakites and edenites (Figures 17(b)-(d)). The edenites are mostly observed within the titanite grains or in contact with the same. The monzogranites have dominantly sanidine and some anorthoclase in the rocks, apart from minor albites.

Zircon saturation temperatures (T_Zr) calculated from bulk rock compositions provides a simple and robust means of estimating magma temperatures [41] [42]. They have established experimentally that the partition coefficient of zircon D_Zr zircon melt is a function of the parameter M [(Na + K + 2Ca)/(Al*Si), all in cation fraction] and temperature. Therefore, using this formula, the Zr thermometry yields the temperature at which the granites of study area formed, i.e., an average T_Zr (˚C) ~775˚C for monzogranites, ~812.5˚C for granodiorite and ~785˚C for migmatite gneiss (Figure 18(a)).

The geobarometry of the granodiorites are attempted through the Al in hornblende barometry. The Al-in-hornblende barometer [43] [44] [45] [46] [47] [48] is controlled by the total Al-content of hornblende. The intensive parameters pressure, temperature, oxygen fugacity, as well as the whole rock composition and the coexisting phases determine the Al-content of hornblende. Based on these calibrations the pressure calculated for the hornblendes in the granodiorite of the present area can be summarized as in Table 4.

The granodiorites are I-type in character with some S-type contributions. Calcic amphiboles are typical for I-type intrusives (Figure 17(c), Figure 17(d)) [49]. According to [50] magmatic amphiboles contain less than 7.3 apfu of Si atoms, and amphiboles containing more than 7.3 apfu of Si atoms are derived via the subsolidus process [51]. All the amphiboles of granodiorites have Si atoms less than 7.3 apfu however; the edenites do not coexist with plagioclases (they are probably derived from magma that initially crystallized at a considerable depth). Hence, the tschermakites are considered for geobarometry.

Aiming to estimate the pressure, amphibole compositions of the granodiorites of present area were plotted in the diagram P (kbar) × Al_tot (Figure 18(b); based on all the calibrated values). The experimental data of [45] [47] and [48] are also shown. It is observed that the compositions of the tschermakites of granodiorites are more compatible with the experimental data of [45] and [48]. However, the geobarometer on calibration of [48] is applicable in a large variety of granitoid rocks containing the mineral assemblage amphibole + plagioclase (An_15-80) + biotite + alkali feldspar + quartz + magnetite + ilmenite/titanite + apatite. Such mineral association is found in the granodiorites of present area. Since, the granodiorites are emplaced at same tectonic level and no evidence of tectonic displacement is observed, hence it can be concluded that the emplacement pressure is about 7.85 [±0.6 kbar] to 8.43 [±0.6 kbar] kbar (avg. 8.14 ± 0.6 kbar).

Due to lack of significant geobarometer for estimating the crystallization pressure of the monzogranites, the same has been attempted by a numerical method based on two polynomial equations:

P = − 0.2426 × ( Qtz ) 3 + 26.392 × ( Qtz ) 2 − 980.74 × ( Qtz ) + 12563 (1)

P = 0.2426 × ( Ab + Or ) 3 − 46.397 × ( Ab + Or ) 2 + 2981.3 × ( Ab + Or ) − 64224 (2)

(R² = 0.9943)

where, P is pressure in MPa, and R denotes correlation coefficient [52]. It is noted that the pressure is correlated respectively with normative quartz (Qtz) content and with normative albite (Ab) plus orthoclase (Or) contents of granitic rocks. Normalization of CIPW norm (quartz, albite, orthoclase) contents to 100% is required before using Equations (1) and (2). The difference in pressure calculations between these two equations is ≤16 MPa for the range of normative quartz contents from 15 to 40 wt%. Keeping this in mind for considering samples for calculation of crystallization pressure based on the two equations, the following pressures have been obtained. (Table 5)

The pressure difference in two equations varies from 8.025 MPa to 10.919 MPa which is within the range for normative quartz contents from 27.24% to 35.85%. Based on these results the crystallization pressure of the monzogranites can be estimated within 0.77 kbar to 5.51 kbar. Even though the range is quite high, but it gives an idea about the fact that the monzogranites have crystallized at lower pressures indicating lower depth of their formation than the granodiorites.

The high-temperature nature of granodiorites also suggest that they have been generated either in the lower crustal or upper mantle region (Figure 19). The heat required for melting the parent rocks at such high temperatures must be provided by the mantle-derived melts either directly or indirectly, i.e., they may only provide the necessary heat for crustal melting or they may contribute mass through differentiation and assimilation of crustal melts [24]. The monzogranites have been generated from the crustal material. Thus, the I-type granodiorites have formed in volcanic arc setting by partial melting of the lower crust, promoted by heat from mantle-derived mafic melts producing a hybridized intermediate magma, that form granodiorite by fractional crystallization during its

ascent and cooling [53]. This metaluminous magnesian-rich magma eventually produces subduction-related granodiorites. Ubiquitous presence of mafic micro granular magmatic enclaves (MME) with cuspate and lobate margins within the granodiorites suggests interaction and mixing/mingling of comagmatic mafic-felsic melts. The generation of the S-type monzogranites has been dominated by continental crust recycling due to continued orogenic activities and hydrothermal influx, rather than the addition of new material from mantle sources.

The area between the central and western arm of RSB, is characterized by different phases of granitoids with different tectonic histories. Migmatite gneiss rocks show mixed characters geochemically with complexly deformed nature observed in field and petrography. The granodiorites are formed from a hybridized intermediate magma by mixing of a mantle derived mafic melts with partially melted lower crust materials in the lower crustal or upper mantle region in a subduction region owing to their high emplacement temperature-pressure, numerous MMEs and high ∑REE content. These granodiorites are thus formed during the orogeny. The monzogranites have generated at shallower depth within the crust by continued crustal recycling owing to continued orogenic activities and hydrothermal influx in the subduction zone. The monzogranites have relatively low ∑REE content and highly fractionated REE pattern. Owing to the high hydrothermal influx in the monzogranites, these S-type peraluminous granites are rich in hydrothermal ore minerals viz., tungsten, tin, molybdenum, copper, etc.

The work has been carried out under Mineral Exploration- M-II G4 stage exploration programme of Geological Survey of India, State Unit: Andhra Pradesh, SR, Hyderabad during field season programme 2020-21. The authors gratefully acknowledge Director General, Geological Survey of India, Addl. Director General and HOD, Geological Survey of India, Southern Region, Hyderabad for providing necessary facilities to carry out the work. The authors are extremely grateful to Shri. R.P. Nagar, Dy. Director General, State Unit: Andhra Pradesh, Southern Region, Hyderabad for his constructive suggestions during the course of work. The authors are thankful to the officers of Chemical Division and Petrology Division, Geological Survey of India, Southern Region, Hyderabad for analysis of the samples of granitoids collected during the field work. The authors are also indebted to the anonymous reviewers for their valuable scientific comments and suggestions.

The authors declare no conflicts of interest regarding the publication of this paper.

Kar, E., Ghosh, P. and Mishra, S. (2022) Comparative Geochemical and Petrographic Studies of the Various Granitoids between Central and Western Arm, in the Central Part of Ramagiri Schist Belt and Their Petrogenetic Histories. International Journal of Geosciences, 13, 382-413. https://doi.org/10.4236/ijg.2022.135021