Geoinformatics & Geostatistics: An OverviewISSN: 2327-4581

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Research Article, Geoinfor Geostat An Overview Vol: 12 Issue: 5

Evidence of Elliptical Intrusions and Sr, Hf, Pb and O-H Isotopes of the Khanbogd Alkali Granite Pluton: Construction of Underplating Magma Associated with The Duplex Thrust

Dash Batulzii1, Serjlkhumbe Amaramgalan2*, Holk Gregory3, Davaa Khishigsuren1, Jargal Lkhamsuren1 and Otgonhuu Javkhlan1

1School of Geology and Mining Engineering, Mongolian University Science and Technology, Ulan Bator, Mongolia

2Rio Tinto Kennecott LLC., South Jordan, Utah, United States of America

3Department of Geology, Californian State University, Long Beach, California, United States of America

*Corresponding Author: Serjlkhumbe Amaramgalan,
Rio Tinto Kennecott LLC., South Jordan, Utah, United States of America
E-mail: amaramgalans@riotinto.com

Received date: 09 September, 2024, Manuscript No. GIGS-24-147609;

Editor Assigned date: 11 September, 2024, PreQC No. GIGS-24-147609 (PQ);

Reviewed date: 25 September, 2024, QC No. GIGS-24-147609;

Revised date: 02 October, 2024, Manuscript No. GIGS-24-147609 (R);

Published date: 09 October, 2024, DOI: 10.4172/2327-4581.1000410.

Citation: Amaramgalan S, Batulzii D, Gregory H, Khishigsuren D, Lkhamsuren J, et al. Evidence of Elliptical Intrusions and Sr, Hf, Pb and O-H Isotopes of the Khanbogd Alkali Granite Pluton: Construction of Underplating Magma Associated with The Duplex Thrust. Geoinfor Geostat An Overview. 12:5.

Abstract

The Khanbogd peralkaline granite pluton, occupying more than 1000 km2, is located in southern Mongolia. Previously, two magmatic bodies called Western and Eastern and the flattened shape of this pluton were discovered. Several elliptical intrusions within the pluton have been detected in Landsat satellite images. These are at least four elliptical intrusions in the Western and two intrusions in the Eastern body. The granites of the inferred intrusions differed in Alumina Saturation Index (ASI) and Cross, Iddings, Pirrson and Washington (CIPW), 87Sr/86Sri and δ18O values. Fe-Mg minerals in studied granites are garnet, aegirine and arfvedsonites. The low dD values (-155% to -170%) of arfvedsonite support the argument for meteoric fluid involvement in the crystallization source. Two stages of aegirine crystallization were determined before and later arfvedsonite, which formed from a phase induced by meteoric water. The domain structure of arfvedsonite indicates its crystallization from a new lagging phase, which is similar to a peritectic phase. However, the peritectoid-like system is suggested for garnet and aegirine-I. Stage II aegirine, which appeared after arfvedsonite, shows its crystallization caused by a change in magnetization when the water is exhausted in the solidus. The diffusion effect, represented by the droplets of arfvedsonite and II stage aegirine in K-feldspar followed the processes. Further, meteoric fluids resulted in disequilibrium δ18O values between quartz and feldspar, which occurred in the postsolidus state. Accordingly, the K-feldspar surface has effects, such as fractured and stippled. Two adjacent intrusive bodies and undeformed host rocks at the front part of the pluton are consistent with underplating magmatic factors during duplex-type thrusting. Another factor is the multiple sources for the melt: mantle, reworked seafloor and arc rocks, which are identified by the ratio of 87Sr/86Sri and δ18Oqz values. An underplate magma source is a suitable interpretation explaining the principles of low non-stable isotopes for alkali granites.

Keywords: Alkali granite; Elliptic shape; ?18O isotope; Domain structure, Lagging phase, Peritectic, Duplex thrust; Underplating.

It is widely recognized that the geology of Mongolia is characterized by the accretion of arc complexes, which is accompanied by the emplacement of voluminous calc-alkaline granites into the arc [1]. However, anorogenic alkaline granites and syenite intrusions occur in Mongolia. One of them is the Khanbogd alkaline-granite pluton, consisting of aegirine-arfvedsonite, ferroedenite granites, pegmatites and dikes of ekerite, comendite and pantellerite. Petrogenetic models involving a mantle source have mainly been proposed for the origin of alkaline granites. The models include:

• Fractionation of mantle-derived magmas with or without interaction of crustal rocks [2-5].

• Partial melting of residue from i-type granites [6,7].

• Crustal melting accompanied by an influx of mantle fluids [8].

• Vapor absent dehydration melting from tonalite and biotiteamphibole gneiss [9,10].

• Partial melting of metasomatically altered crustal source rocks [11-13].

• Partial melting of lower crustal basalt and lithospheric mantle induced by a rising plume [14,15].

This model is based on research on peralkaline granites in central Mongolia. Bonin's hypothesis was different in that it assumed an underplating magmatic process for the origin of alkaline granites [16].

Vladykin et al., argued for model (i) for the origin of the Khanbogd plutonic complex. A more complete data set was used by Kovalenko et al. and they suggested a magma source from the melt via interactions of enriched, depleted mantle and crust materials [17-19].

The main goal of this study is to identify the features of alkaline granites in a flattened form intrusion, implying the nature of thrust faults. For this purpose, unpublished geochemical and radiogenic isotope data from Serjlkhumbe were used [20,21]. To integrate new chemical analysis with geological observations, we began to interpret ‘Landsat’ satellite images of the Khanbogd pluton. We have interpreted several elliptical incursions within two bodies that previous researchers have called the Western and Eastern bodies. The sample positions allowed us to examine chemical and isotopic data interpreted intrusions.

The flattened shape of this pluton and the O and H isotope data allowed us to accept the thrust-related magma model, which involves the melting of the mantle, oceanic crust and reworked arc rocks. The low dD values (-155% to -170%) of arfvedsonite support the argument for meteoric fluid involvement in the crystallization [22-26]. Plutonic rocks crystallized at shallow crustal depths are highly susceptible to interactions with meteoric-hydrothermal fluids, resulting in quartzfeldspar pairs out of oxygen isotope equilibrium and hydrogen isotope values below those in equilibrium with magmas [27,28].

Joekar-Niasar et al., supposed that the equilibrium change is an effect of the appearance of new phases like diffusion and their lagging behind the main crystallization. They note that the domain structure expresses the coexistence of lagging and main phase minerals because of different magnetization. We established this structure in studied granites [29].

Therefore, this manuscript presents our interpretation of satellite images of the Khanbogd pluton, petrographic, geochemical and isotopic data (Sr, Nd, Hf, Pb, O and H) of alkaline granites, as well as a new model of the Khanbogd pluton.

Materials and Methods

Mineral δ18O values were measured using the Thermo Finnigan Delta Plus-XP mass spectrometer at California State University, Long Beach. A modified version of the laser fluorination method of Sharp and the TC/EA method of Sharp et al., was employed for the acquisition of mineral δ18O and D values, respectively [23,24]. Analytical precision and accuracy for hydrogen and oxygen (dD ± 2.0% and δ18O ± 0.2%) isotopes were determined using the NBS- 30 biotite (dD = -65.7%) and Caltech Rose Quartz (δ18O = +8.45%) standards and reported relative to V-SMOW [30,31]. Whole rock major and 14 trace element (Ba, Ce, Cr, Ga, Nb, Ni, Pb, Rb, Sc, Sr, Th, V, Y, Zr) concentrations for 35 samples were analyzed by Rigaku RIX-2000 wavelength-depressive XRF spectrometer at Shimane University, e.g., [21]. REEs, Cs, Rb, Ba, Sr, Th, U, Nb, Ta, Pb, Zr, Hf, Li and Y analyses were carried out for selected samples by ICP-MS (Thermo ELEMENTAL, VGPQ3 at Shimane University), following the method described by Kimura et al. [32].

Sr and Nd isotopic ratios were determined for 36 samples by thermal ionization mass spectrometry (MAT262) at Shimane University, following the methods described in [33,34]. The isotopic compositions were measured in jumping multi-collection mode. The Sr isotope ratios of standard sample NBS987 (SrCO3) were used during the analysis. The isotope dilution method determined Sr isotope compositions and age dating due to the high Rb/Sr values and much lower average Sr concentrations (<10 ppm) of the Khanbogd plutonic complex. Samples were mixed with spike solution (87Rb/86Sr mixed spike, previously prepared at Shimane University of Japan). For the interpretation of the geological setting of Khanbogd pluton, 2-3-4, 4-5-1, 5-3-2 and 7-4-1 spectral bands image LandsatTM were used. The Nikon Eclipse 50iPol microscope was used for petrography research.

Geological background of the studied Khanbogd alkali granite pluton and its surroundings

The studied Khanbogd pluton is located near the southern border of Mongolia. This pluton intruded into a lower carboniferous sedimentary basin filled by the volcano-sedimentary strata e.g. [17,19]. According to the terrane-tectonic concept, this basin is located in the Gurvansaikhan terrane, e.g., (Figure 1) [35-37].

Figure 1: Location of the Khanbogd peralkaline granite pluton in the terrane-tectonic scheme of Mongolia and its surrounding geological formations. Modified from [84,1]. Terranes (1-4) per Badarch et al. [1].

Geological and mineralogical studies of previous researchers of the Khanbogd alkali granite pluton: Detailed mineralogical, geochemical, petrological and geophysical studies of alkaline granites of the Khanbogd pluton were carried out between 1970- 1980. Aegirine-arfvedsonite, aegirine granites, dikes of various compositions and rare-earth pegmatites were identified in two neighboring ring-shaped intrusive bodies; named Eastern and Western. Modeling of gravity data suggests a flattened shape for the Khanbogd complex. The 300 km3 Eastern body comprises mediumto fine-grained aegirine granite and is younger than the Western body. The 1000 km3 Western body is comprised of medium-to coarsegrained aegirine-arfvedsonite granites and small bodies of red granite that lack aegirine and arfvedsonite, but contain ferro-edenite.

Numerous REE-bearing pegmatites and various compositions of dikes, such as ekerite, pantellerite and comendites were discovered in the pluton. Elpidite (Na2Zr6Si6O15H2O) is a unique accessory mineral in these granites and pegmatites, e.g., [17]. Vladykin et al., discovered new zirconium oxide minerals from this pluton, such as armstrongite (CaZrSi6O153H2O) and mongolite (Na2ZrSi6O153H2O) in pegmatites. Kynicky et al., contributed to the study of REE-bearing minerals in pegmatites [38,39].

Granites of the western body have U/Pb zircon ages of 291 ± 1 to 290 ± 1 Ma and a Rb/Sr age of 287 ± 3 Ma [19]. However, other studies produced Rb/Sr ages 295-292 Ma from aegirinearfvedsonite granites of the Western Body, granites of both bodies and dikes. Lower to upper cretaceous red-bed continental sediments overlay Carboniferous, a bimodal basalt-comendite volcanic suite and Khanbogd pluton of Early Permian [40-43].

In the basin, where the Khanbogd pluton is located, leucogranites that analogs of felsic lavas of the bimodal volcanic suite are widespread. The U/Pb zircon age of a biotitic leucogranite near Khanbogd is 290 ± 1 Ma and the Rb/Sr whole-rock age of felsic volcanic is 291 ± 4 Ma. These emplacement ages between alkali granites, leucogranite and pantellerite indicate they are of coeval ages.

Interpretation of Landsat satellite images and the elliptic intrusions of alkaline granites in the Khanbogd pluton: We used a combination of ‘Landsat’ spectral bands 2-3-4, 4-5-1, 5-3-2 and 7-4- 1 to interpret the geological setting of the Khanbogd pluton. Four shapes, identical to the phases, are represented by different color images across the western body. The yellowish, pale red-pinkish, bluish and pale pinkish color tones are reflected from an arc-shaped stripe along the outer edge of the Western body (Figure 2).

Figure 2: Images of the Khanbogd granite pluton in the landsat bands and an interpreted intrusion using them landsat bands. Note: (a) -/2-3-4/; (b) -/4-5-1/; (c) -/5-3-2/; (d) -/7-4-1/; (e) interpreted elliptical intrusions and sample points (Interpretation by Batulzii, Holk and Bayartsengel).

This is marked I-W in Figure 2, which defines the first intrusion of the Western body. An elliptical shape with pale blue, blue, brown and pale red reflected color tones inside the arcuate strip is denoted as unit II-W. A narrow blackish zone is distinguished between an elliptical (II-W) and an arcuate (I-W) shape. This zone represents uplifted country rocks and marks the boundary of two granite intrusions I-W and II-W. The smaller irregular shape, displaying dark and pale blue, brown and bright reddish colors is the next phase in the relationship and is noted III-W. Images marked IV-W refer to small intrusions of ferro-edenite granites. Ferro-edinite granite dikes are common in II-W and III-W. Satellite images display a sharp contact between the western and eastern intrusive bodies. The cross-cutting relationships between granites indicate that the small elliptical Eastern body is younger than the Western body. Contrasting colors in the small body suggest there are two intrusions in the Eastern body marked as the I-E and II-E. The granites I-E, which occupy most of the eastern body are indicated by lighter colors. The II-E is characterized by its smaller size and blackish color. Interpreted elliptical intrusions in the studied Khanbogd pluton are shown in Figure 2e.

Texture of granite outcrops of distinguished intrusions, their relationships, dikes, roof pendant and mineralization: The interpreted intrusions differ primarily in the texture of their outcrops. Enhanced weathering along intersecting joints imparted a spheroidal surface appearance for intrusion I-W. This arcuate-shaped, I-W intrusion is mostly composed of coarse-grained, porphyritic and agpaitic aegirine-arfvedsonite granites. Outcrops of II-W are characterized by vertical joints that were intersected by shallowdipping, closer-spaced joints. Intrusion II-W is represented by pale pink, medium-to-coarse-grained, equigranular and porphyritic, aegirine-arfvedsonite granites. The content of elpidite in some places exceeds the content of accessory minerals. The outer contact zone II-W is not only controlled by the uplifted host rocks but also by banded pegmatite zones with quartz cores. Rough, fractured surfaces characterize the outcrops III-W. Primarily, structures were destroyed by dikes from IV-W. The outcrop of this intrusion was documented by Kovalenko et al., but the compositional character has not been studied [19]. Contrasting colors and textural shapes define the intrusive contact between units II-W and III-W. The contact where III-M intrudes II-M is visible by their colors and shapes. The intrusion III-M is composed of brown-reddish medium-grained aegirine-arfvedsonite granites. Intrusion IV-M is distinguished from others by their red color and outcrop shape formed by intersecting vertical and horizontal sets of joints. These red porphyritic granites have plagioclase phenocrysts, along K-feldspar and ferro-edinite (Figure 3).

Figure 3: Outcrop and hand specimen photos of alkali granites in the Western body of Khanbogd pluton. Note: (a) outcrop of intrusion I-W; (b) coarse-grained porphyritic texture greyish color aegirine-arfvedsonite granite in intrusions I-W; (c) outcrop of II-W, where dominated horizontal platy joint; (d) elpidite rich agpaitic, greyish color granite in intrusion II-W; (e) outcrop of III-W, intruded into II-W; (f) reddish color aegirine-arfvedsonite granite in III-W; (g) outcrop of IV-W, where cubic shape is formed from set of vertical and horizontal joints; (h) red color, ferro-edinite granite.

As mentioned above, two intrusions comprise the Eastern body. Scattered roof pendants indicated by a blackish color in the landsat images occur among the red granites of II-E.

Apophyses of II-E into I-E and I-W demonstrate its younger origin. Granites II-E are characterized by aegirine and red K-feldspar phenocrysts embedded in a fine-grained reddish groundmass. The older I-E is characterized by medium-grained spherical-textured lilac granites, where pinkish K-feldspar phenocrysts are in a lilac groundmass (Figure 4).

Figure 4: Outcrop and hand specimen photos of alkali granites in the Eastern body and outcrop of dike and pegmatites. Note: (a) host rock roof pendants among red granite intrusion I-E; (b) relationship between I-E and II-E: granite II-E intrude into I-E; (c) hand specimen of the porphyry texture red granite; (d) hand specimen of lilac granite; (е) comendite dike outcrop intruding III-W granite; (f) pantellerite lava lying in granite II-M; (g) ekerite composition sheet pegmatites in intrusion I-M; (h) outcrop of andesite roof pendant.

Dikes of various compositions have been identified in the Khanbogd pluton. Thus, in the arcuate intrusion, there are subparallel dikes of ekerites and pegmatites with arfvedsonite and elpidite. Red comendite dikes with large K-feldspar phenocrysts are common in granites II-W. Dark gray pantellerite dikes and elpidite-bearing smaller pegmatites are described from intrusions II-W and III-W.

However, Mongolian researcher Garamjav offered, that a shape-like ring of the Khanbogd pluton must be associated with the rise of magma in the form of a vortex. The primary structure study of the granites does not show a foliation structure, which has to follow a vortex event. The foliation is defined from some pegmatites and dikes [44,45].

The trachydacite in the roof pendant has a Carboniferous age of 330 Ma, that is dark brown in Landsat images. Following identifying several intrusions, we revise the location of REE mineralization. The horizontal pegmatites, consisting predominantly of large crystals of arfvedsonite-elpidites, occur in the southern part of the arc-shaped I-W intrusion. Zirconium and niobium oxides such as pyrochlore, monazite, armstrongite, mongolite and gittincite were described from pegmatites that are in II-W.

Oxygen and hydrogen isotope study

Oxygen isotope values from coexisting quartz, K-feldspar and arfvedsonite and δ D values of arfvedsonite from Khanbogd granite intrusions are indicated in Supplementary Table 1. The mineral δ18O values are compared to test for equilibrium to assess magma sources. Arfvedsonite dD values were used to determine whether granites were affected by the hydrous process.

The quartz and K-feldspar δ18O values are out of equilibrium with the feldspars being shifted to lower values. This indicates oxygen isotope exchange between a meteoric-hydrothermal fluid and feldspar [46].

The disequilibrium occurs because feldspar group minerals exchange oxygen much faster than quartz. Many of the quartz δ18O values cluster between 8 and 9.5 per mil. This narrows down the oxygen isotopic composition of the primary magma. The meteoric fluid system was short-lived because if it had been active over a longer period, the quartz would have been shifted to a lower δ18O value to be in equilibrium with the feldspar at a lower value [47].

However, some quartz δ18O values have also been shifted downward. These are common characteristics of intrusions emplaced into the shallow crust.

Few samples in the equilibrium field including granites II-E show the 18O/16O isotope ratios of quartz were changed to a lesser extent, more likely. Exceptionally, δ18O low values of quartz and K-feldspar are found in granites I-E and dikes (Figure 5).

Figure 5: Equilibrium fields of quartz and K-feldspar fractionation. Note: (a) plots in δ18O% qz– δ18O% kfs diagram; (b) plots in δ18O% qz– δ18O% arf diagram.

In addition, the real low dD values (-201 to -156) from arfvedsonite and ferro-edenite support the argument for the involvement of meteoric-hydrothermal fluids [22-26]. In the δ18 Oqz vs δ18O arf diagram, data for these minerals of all granites are plotted in an equilibrium field, except I-E and the dike data [45]. Across it, the data of some granites, particularly granites II-W, are plotted in the equilibrium field of T 700°C. Most granites are grouped in areas where the equilibrium T0 is between 700-5000C. According to Taylor [46], anatectic melting producing the formation of peraluminous leucogranite magmas must have occurred after a hydrothermal event that homogenized the 18O/16O and 87Sr/86Sr ratios of pelitic metasediments.

Therefore, the δ18O values of arfvedsonite were equilibrated with the magmatic δ18O values of quartz, although the dD values are much lower.

Water contents from arfvedsonite and ferro-edenite are generally low (<2.0%), however, an arfvedsonite of a comendite dike contains 7.4% H2O (Supplementary Table 1). An elpidite from a pegmatite has δD = ¬–87% and an H2O content of 8.3%, suggesting alteration by magmatic fluids (Supplementary Table 1).

Petrographical studies of the alkali granites

The alkali granites contain 65%-70% microcline, 25%-28% quartz and a lesser amount of albite (3%-5%), arfvedsonite and aegirine or ferro-edenite (3%-9%). Garnet is less than 2.0% in granites. Agpaite texture is common for studied granites. This study describes a domain structure indicative of a time gap caused by cold meteoric water accompanying nonequilibrium crystallization. The structure such as lobate, convolute and dislocation boundaries at the contact of K-feldspar and quartz were discussed as a domain structure by Joekar-Niasar, et al., Effects similar to such structures were considered as the result of changes in the 18O/16O ratio in K-feldspar and quartz by Holk and Tayle.

The contact between quartz and K-feldspar is different, sometimes direct and some are convolute and lobate (Figure 6). The fractured and stippled surfaces in the microcline are akin to the effects of oxygen isotope changes. Albite growth effects are observed in potassium feldspar. In the upper part of the photo, albite growth looks like drops and they are dense. Below, the drops are mixed with tabular albites and further on, needle-like intergrowths of albite are observed in K-feldspar. The dislocated boundaries between K-feldspar and quartz, new crystals along fracture zones in K-feldspar, are explained by effects associated with isotopic changes. Aegirine crystals occur between quartz and K-feldspar; less common, aegirine is grouped with either garnet or arfvedsonite. A changed surface in K-feldspar and a dislocated boundary at the contact of aegirine and K-feldspar are noted.

Figure 6: Petrographical studies of the alkali granites Note: (a) Lobate boundary between quartz (Qz) and fractured K-feldspar (Kfs); (b) convolute boundary between quartz and K-feldspar with albite growth; (c) dislocated boundary with new quartz along a fracture zone; (d) dislocated/lobate boundaries between aegirine, K-feldspar and quartz; (e) lobate boundary from arfvedsonite to I-stage aegirine; (f) domain boundary of arfvedsonite and aegirine in K-feldspar; (g) stage-II aegirine into arfvedsonite; (h) garnet corroded by aegirine; (i) ferro-edinite with relict garnets; (j) oxy-hornblende replacing ferro-edinite; (k) aegirine replaced by arfvedsonite; (l) garnet corroded by aegirine. Noncrossed nicol: b, e, h, i, j, k, l.

Between aegirine K-feldspar and aegirine arfvedsonite, convolute and lobate boundaries are often found, indicating a domain structure. Similar boundaries are observed in contact with potassium feldspar and aegirine, the latter being considered a peritectic phase mineral of alkali granites. Wedge-shaped aegirine crosses the arfvedsonite and ?-feldspar contact and the lobes around arfvedsonite were filled with aegirine plates. Thus, two-stage aegirine crystals are distinguished and differ in time, both before and after arfvedsonite. The thin needles and drops of arfvedsonite and aegirine-II in K-feldspar represent the diffusion domain. The stage-I aegirine is always associated with garnets in I-W, II-W and III-W granites. Garnets are easily marked in thin sections from III-W, corroded by aegirine.

The amphibole of granite IV-M refers to the ferro-edenite [47]. Granite composed by the microcline 60%-62%, quartz 25%-27%, plagioclase 9%-12%, ferro-edenite 2%-4%, approximately. This granite also contains garnets of various sizes. The droplets of ferroedenite in K-feldspar IV-M granites represent the domain structure. There is also brown oxygen-hornblende replacing the ferro-edinite.

The granites of the Eastern body are predominantly fine-grained, the amount of ferrous minerals is 2%-4% in the volume of granites. The fibrous and stellate form aegirine is characteristic of granites I-E. Arfvedsonite, which selectively replaces aegirine, is dark bluish compared to arfvedsonite in the granites of the Western body. The garnet with size from 0.03 × 0.01 mm is more conspicuous for granites II-E. A distinctive feature of these granites is absence of stage-II aegirine.

Geochemistry of the Khanbogd alkali granites

Chemical analysis of oxides and calculated CIPW norms of the granites are listed in Supplementary Table 2. Regardless of the presence of ferro-edenite, all granites in the TAS and AQPF diagrams are represented by alkali granites. The granites of all interpreted intrusions differ in their aluminum saturation index (ASI) e.g., [48,49].

Accordingly, granites of I-W, II-W and I-E intrusions are peralkaline. Granites III-W shows peraluminous affinity; the granites II-E vary from metaluminous to peraluminous. Identical affinity for them is cocrystallized aegirine and arfvedsonite, as well as the amount of garnet. Hence, ferro-edenite granites are plotted in the metaluminous granite field excluding one. Figures 7b- 7f show a correlation between oxides and differentiation index (D.I) e.g., [50]. The silica content in granites of all intrusions is 71.00%-78.36%. The granites of the Eastern body are characterized by a high DI and differ from the granites of the Western body. Ferro-edinite granites are distinguished by SiO2, CaO, MgO and K2O content from aegirine-arfvedsonite granites (Supplementary Table 2, Figures 7b-7f). FeOt variations indicate that the aegirine-arfvedsonite content in the granites of the Eastern body is less than in the granites of the Western body. Accordingly, they (I-E and II-E) are characterized by low Na2O, K2O and FeOt content compared to the Western body's granites. The studied granites also differ well in their CIPW norm calculated using the Hollocher program [51]. Granites I-M and II-M are acmite-Na-silicate (acmns) normative, except for a small amount of ferrosilite (fs) and enstatite (en) molecules. Ilmenite is in norm from these granites. The anorthite- hypersthene (an-hyp) molecule is calculated from aegirinearfvedsonite granite III-M. The an-hyp-di norm is acquired from ferro-edenite granites. Only acmite is calculated from granites I-E, which is peralkaline and an-hyp±di norm is calculated from II-E, which exhibit a metaluminous-peraluminous character. The norm of ilmenite (il) of the I-W and II-W granites implies that they derived from a more reduced environment than others, for which a near-neutral condition predominated. According to the K2O/Na2O ratio, all granites are rich in potassium; ekerite and pantellerite dikes are rich in Na and characterized by the acmite, Na-silicate and ilmenite norms. Comendites are potassium-rich and exhibit acmite or anorthite norm (Supplementary Table 2) (Figure 7) [52-56].

Figure 7: Correlation diagrams for Khanbogd alkali granites. Note: (a) Granite plots in the ASI diagram; (b-f) oxide vs differentiation index (D.I) plots; (g) calculated norms from alkali granites across different intrusions; (h) primitive mantle-normalized multi-element patterns of alkali granites; (i) chondrite-normalized REE patterns of alkali granites from various intrusions, with normalized values from Sun and McDonough; I-W (image); II-W(image); III-W(image); IV-W (image);I-E(image); II-E(image).

The trace and REE analysis of the granites are shown in Supplementary Table 3. The Li content is 31.75 ppm-71.02 ppm for granites I-W and 5.85 ppm-14.97 ppm for granites IV-W. Some samples contain high Zr content having zirconium oxides such as elpidite (Supplementary Table 3). In the trace element distribution diagram normalized to the primitive mantle, deep negative anomalies of Ba, Sr and Eu and positive anomalies of Th, U, Pb and Li are observed. The largest negative anomalies of Ba and Sr are detected in all patterns. Although, less pronounced negative anomalies of Ba, Sr and Eu are marked from ferro-edenite granites. The chondrite normalized REE patterns from granites are sub-symmetric, with Eu deep negative anomalies. In this diagram, the patterns of the ferroedenite granites are intermediate between those of the others and the Eu anomalies are at a higher level than the others.

The geochemistry of studied alkaline granites with low Sr, Ba, Eu, Ti and high Th, U and Pb contents resembles the vapor-absent melt crystallization from the High-Himalayan Mountains.

Sr, Nd, Hf, Pb, O and H isotopes of the alkali granites Khanbogd pluton

The initial 87Sr/86Sr and 143Nd/144Nd were calculated for samples on Rb-Sr whole rock isochron age of 295.7 Ma and the Sr isotope ratios were measured for most samples. The 295.7 Ma was obtained twice, first from all aegirine-arfvedsonite granites, including ekerite and comendite dikes and second from granites I-M, II-M and III-M (Supplementary Table 4). According to this measurement, 87Sr/86Sri values range from 0.6676 to 0.7077 for the aegirine-arfvedsonite granites, except for one value of 0.7287.143Nd/144Ndi values of the granites are moderately high, from 0.5125 to 0.5127. A slightly higher initial 87Sr/86Sr of 0.7051-0.7071 was obtained from ferro-edenite granites with their isolated plots of 269.6 ± 2.8 Ma (Supplementary Table 5). Also, 291 ± 7.2 Ma was detected from aegirine-arfvedsonite granites of two bodies, excluding dikes, (Supplementary Table 4). The received ages of 291 ± 7.2 and 295.7 ± 5.3 Ma are consistent with U/Pb zircon dating by Kovalenko et al., [19]. These are 290 ± 1 Ma for coarse-grained granite and 292 ± 1 Ma for a pegmatite I-M. The latest U/Pb ages of zircons were obtained from granites of the Eastern body during the prospecting project on U and REE. The studied site occupied the southern half of the Eastern body. Zircon U-Pb ages were analyzed at the Shandong testing center of China Metallurgical Geology Bureau in Jinan city of Shandong province, China. Samples were taken from drill cores. Obtained concordia ages are 287 ± 3.6 Ma, 288 ± 3.0 Ma and 289 ± 3.6 Ma.

All εNdt values are positive in the range 5.82-7.80 for aegirinearfvedsonite granites, 3.95-5.99 for ferro-edenite granites and 5.06-6.97 for dikes, (Supplementary Table 5). Isotopic plots in the 87Sr/86Sri-143Nd/144Ndi; 207Pb/204Pb-206Pb/204Pb; ?Nd(t)-?Hf(t) and Sri-δ18O% diagrams indicate that modified oceanic rocks were involved in the melting source of alkaline granites (Figure 8).

Figure 8: Isotope data plots from Serjlkhumbe. Note: (a) Plots in 87Sr/86Sri vs 143Nd/144Ndi diagram; (b) plots in Pb isotopic systematics upper and lower crust, orogen and mantle evolution curve by, Tick marks represent 0.1 Ga age intervals; (c) plots in ?Hf (t) vs ?Nd(t) diagram, N-MORB, Proterozoic continental crust, Proterozoic sediment data and mantle arrow are from; (d) data plots in 87Sr/86Sr - δ18Oqz diagram, modified from Magaritz et al., The dotted lines are approximate ranges of 87Sr/86Sri - δ18Oqz in mantle-derived rocks.

Results and Discussion

Fault zones controlled by uplifted country rocks indicate the emplacement of laccoliths, sills, sheets and ring dikes in response to magma injection along faulted country rocks or bedding in host rocks. This resulted in the Khanbogd pluton and identified several horizontal elliptical intrusions within the pluton. Our model for these alkali granites invokes magma underplating of duplex-type thrusts, consistent with the model of Konstantinovskaya and Malavielle. Evidence includes two adjacent intrusive bodies and undeformed Carboniferous volcanic rocks at the front of the pluton [57-60].

Geology and petrogenesis

Fault zones controlled by uplifted country rocks indicate the emplacement of laccoliths, sills, sheets and ring dikes in response to magma injection along faulted country rocks or bedding in host rocks. This resulted in the Khanbogd pluton and identified several horizontal elliptical intrusions within the pluton. Our model for these alkali granites invokes magma underplating of duplex-type thrusts, consistent with the model of Konstantinovskaya and Malavielle. Evidence includes two adjacent intrusive bodies and undeformed Carboniferous volcanic rocks at the front of the pluton.

The studied granites exhibit a variety of phenomena associated with meteoritic fluids. Much lower δD values of arfvedsonite (-141% to -171%) indicate the involvement of high-latitude meteorichydrothermal fluids [27]. These lowest dD values are also consistent with Late Paleozoic glaciation, noted in both hemispheres, in the Early Permian and Triassic timer e.g. [61].

The agpaite texture in studied granites indicates that quartz and K-feldspars crystallized first from the solid phase melt when the temperature reached their crystallization T0C. Accordingly, the residual solid phase was enriched with Mg-Fe components. A peritectic phase from vapor absent melt has been proposed for alkali pyroxene by the experimental data of Patino Douce. Garnet is a cocrystalized mineral with pyroxene in that experiment. This shows they may form from the peritectoid-like system, where two solid phases are suggested from the decomposing of the solid phase. The dominant aegirine crystals show, that pertictoid system transformed into a peritectic phase and continued aegirine crystallization. We intend that arfvedsonite can form from modified or initiated by the meteoric fluids peritectic phase. Most likely, the intersection of aegirine and arfvedsonite crystals indicates that the reaction producing aegirine has changed from an anhydrous to a hydrous state and formed arfvedsonite. The structures of aegirine and arfvedsonite, inferred from the peritectic and lagging phases, are similar. This may be due to the time gap that occurred in both cases. Crystals and droplets of stage-II aegirine may be associated with the diffusion of magnetization change from the hydrous to the anhydrous state in the crystallization source.

Further, meteoric hydrothermal fluids resulted in disequilibrium δ18O values between quartz and feldspar, which occurred in the postsolidus state [44]. Hydrothermal fluid was short-lived (<100ka), as evidenced by the faster exchanging feldspars having experienced a greater degree of 18O/16O exchange than co-existing quartz e.g., [62]. In addition, the effects in K-feldspar crystals are consistent with changes evidenced by hydrothermal fluids.

The vapor absent melt crystallization in granitoid from emplacement in thrust sense shear zones has been described since early e.g., [63,64]. The geochemistry characteristic of studied alkaline granites with low Sr, Ba, Eu, Ti and high Th, U and Pb is consistent with this crystallization.

Magma source of the Khanbogd alkali pluton and gravimetric model of another alkali-granite Bayan-Ulaan pluton

The 87Sr/86Sr-δ18O correlation diagram illustrates the sources: i) seafloor sediments, ii) depleted mantle and iii) Precambrian gneisses and paleozoic rock. Ocean-floor sediments are considered a resource of Rare Earth Elements e.g [65-68]. Therefore, the REE concentration in the alkaline granites of Khanbogd pluton does not negate the participation of modified ocean floor rocks in their magmatic source. The 87Sr/86Sri and 18O/16O ratios of studied granites are mainly suitable for the depleted mantle and source derived from the lower continental crust (Supplementary Table 4). Also, identical to the ratios of amphibolite and granulite [69]. The tonalites and granodiorite compositions studied by Blight e.g., [70] in southern Mongolian from Early Carboniferous arcs. These rocks and the rocks that produce them may be the melt source of the Khanbogd alkaline granite (Figure 9).

Figure 9: Model for Khanbogd pluton. Note: (a) Plots in 87Sr/86Sr291-δ18 Oqz diagram; (b) Suggested model for the emplacement of flattened form alkali granites of Khanbogd; (c) Trend curves of terrigenous sediment from, seafloor sediment from and depleted mantle from Eiler et al.

The much lower sri values of 0.6087-0.6089 were obtained from granite II-E intrusion. It was the last intrusion in the pluton. There is a small site with Mo mineralization on the southern margin of I-M intrusion, which has contacted II-E in its continuous. Therefore, the sri values 0.6087-0.6089 of intrusion II-E imply those changes by the ore-bearing hydrothermal fluids. Figure 9b presents our model for the studied Khanbogd pluton. The latest U/Pb ages from the Eastern body within 287-289±3.6 Ma are consistent with its formation later than the Western body [52].

A gravimetric model of another largest alkali-granite pluton, Bayan-Ulan, located in Central Mongolia, was done by geophysicists of the “Geo-Oron” company. As a result of modeling, a flattened shape was obtained for this pluton [71-74]. The Bayan-Ulan pluton occupies almost 1000 sq. km and is emplaced into an accretionary wedge complex. The underplate magma model has mainly been proposed for anorogenic igneous rocks of the rifting e.g [73-76]. According to Stel et al., this magmatic event is also observed in basins where crustal extension did not occur. The detrital zircon age of this complex correlated to the interval of Permian-Triassic [73,77-80]. The granites of the Bayan-Ulan pluton consist predominantly of quartz, K-feldspar and aegirine, with a minority of riebeckite and biotite. The U/Pb zircon age of 221 Ma was determined from alkaline granite [81-84]. The leucogranite is associated with alkali granites in this pluton. The measured dD values from riebeckite are in (-181) - (-210%) [85]. The δ18Oqz values ranged from -9.94% to -7.56% and δ18Okfs values from -0.06% to-8.53% are shown those mineral's disequilibrium [86-88].

Similar events, such as magma rising along horizontal faults and underplating magma sources, were suggested for the Permian alkaline granite plutons of China. This shows that the Permian alkali granite plutons were evidenced by similar processes, maybe by rifting in southern Mongolia and northern China [89].

Conclusion

The peralkaline Khanbogd plutonic complex, with an area over > 1000 sq. km, was formed by the sequential emplacement of several elliptic intrusions along the sub-horizontal fracture zones from duplex-type thrusting. The co-crystallization of aegirine and arfvedsonite or only arfvedsonites in alkali granites, shows the presence of hydrothermal fluid at their formation. The disequilibrium of δ18O values between quartz and feldspar caused by meteoric fluids is expressed by effects at their boundaries and the surface. These effects such as convolute, lobate and stippled surfaces are similar to the domain structure of arfvedsonite that resulted during the crystallization process. The intersection of aegirine and arfvedsonite crystals led us to conclude that the arfvedsonite could have formed from a changed peritectic phase producing aegirine. The convolute, lobate boundaries of aegirine and arfvedsonite imply that a time gap occurred in the initiation of both phases. Droplets, considered domains are formed from an opposition water-exhausted state, due to magnetization changes. The higher alkalinity associated with low Sr, Nd, Hf and Pb isotopes of alkali granites indicates their formation from an underplate melt during duplex thrust, where oceanic and mantle-sourced rocks were involved.

Funding

Field geological studies of this large pluton were re-examined as part of the project “Accretional Orogen of Southern Mongolia: A Comparison of the Central Asian Orogen (CAOB) in Mongolia and China - (NFSC2019/04). The geochemical analyses were carried out by Dr. Amaramgalan’s master's and doctoral thesis, provided by the Monbusho grant of the Japanese Ministry of Education and Culture.

Acknowledgments

We must thank our previous scientists, such as Vladykin. N.V. and Kovalenko. V.I. and others, who devoted many years of their work and life to the study of this pluton. Our great thanks to Professor Ochir Gerel who requested to study alkaline granites Khanbogd pluton. We also thank Professor Thomas K. Kelty for initiating our collaborative work with California State University Long Beach (CSULB) where the oxygen isotope analysis was conducted. A respected friend and colleague of many scientists and geologists, Prof. Yin An, remains in our memory, but his contribution to this manuscript is invaluable. Blessed memory to him. We specially thanked young geologists Tseveendorj Bayartsengel, Baatar Gendenjamts, Ganbat Turbat, Byambajav Tankhildulam, Dembee Unurzaya and director Ulamsain, Ya of “Geo-Oron” LLC and geologist of “Magnetic survey” LLC who cooperated and helped to develop this manuscript.

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