Au ‐ Ag ‐ S ‐ Se ‐ Cl ‐ Br Mineralization at the Corrida Deposit (Rus ‐ sia) and Physicochemical Conditions of Ore Formation

: The mineral and chemical compositions of ores from the Corrida epithermal Au ‐ Ag de ‐ posit (Chukchi Peninsula, Russia) were studied using the optical and scanning electron microscopy with X ‐ ray energy ‐ dispersion microanalysis. The deposit was formed at the time close to the period when the basic volume of acid magmas had been emplaced within the Okhotsk–Chukotka belt (84 to 80 Ma). The Au–Ag mineralization is distinguished with Au ‐ Ag sulphides and selenides (uy ‐ tenbogaardtite ‐ fischesserite solid solution, Se ‐ acanthite, S ‐ naumannite) and Ag halides of the chlorargyrite ‐ embolite ‐ bromargyrite series. The ores were formed in two stages. Using microther ‐ mometric methods, it has been established that the ore ‐ bearing quartz was formed in the medium ‐ temperature environment (340–160 ° С ) with the participation of low ‐ salt (3.55 to 0.18 wt. % NaCl eq.) hydrotherms, mostly of the NaCl composition with magnesium, iron and low ‐ density СО 2 . Ac ‐ cording to our results of thermodynamic modeling at temperatures from 300 to 25°C and data on mineral metasomatic alterations of the host rocks, the Au ‐ Ag ‐ S ‐ Se ‐ Cl ‐ Br mineralization was formed at decreasing temperature and fugacity of sulphur (logƒS 2 from − 6 to − 27), selenium (logƒSe 2 from − 14 to − 35), and oxygen (logƒ О 2 from − 36 to − 62), with near ‐ neutral solutions replaced by acid solu ‐ tions. Analysis of the obtained data shows that the Corrida refers to the group of the LS ‐ type epi ‐ thermal deposits. This deposit is a new example of epithermal deposits with significant quantities of Au–Ag chalcogenides (acanthite, uytenbogaardtite, fischesserite, naumannite and others).


Introduction
The exploitation of the Northern Sea Route and technological solutions of arranging production in the severe climatic conditions make the Arctic part of Eurasia increasingly interesting for investors [1]. Over the last 20 years, in Central and West Chukotka, more than 10 epithermal gold deposits have been explored and involved in mining production, though in the second half of the 20th century they were considered unfeasible. The resource base re-evaluation, which led to the successful exploration of mining objects, was based on their comprehensive study [2][3][4][5][6][7] and on the accumulated world insight into epithermal mineralization [8][9][10][11][12][13]. The Chukchi Peninsula is located to the east of the 180° meridian ( Figure 1). For some primarily infrastructure reasons, manifestations of different ore types, including epithermal Au-Ag ones, known ever since the 1970s, have so far been insufficiently studied. Some practical and research works generally characterize only their geological structure and the morphology of ore bodies exposed on the surface [14,15].
In 2013, E.E. Kolova participated in prospecting works arranged by a private geological company in East Chukotka. The greatest attention was drawn to the Corrida deposit (145 km to the east of the settlement of Egvekinot, in the Erguveyem River basin), discovered by geologists V.I. Plyasunov and G.A. Tynankergav in 1975.
The aim of this study is to investigate the features of Au-Ag-S-Se-Cl-Br mineralization at the epithermal Au-Ag Corrida deposit (Chukchi Peninsula, Russia) and to estimate the physicochemical conditions of its formation based on the fluid inclusions study and thermodynamic modeling.

Geological Situation
The Corrida deposit is located in the central part of the East-Chukotka flank zone of the Okhotsk-Chukotka volcanic belt (OCVB). It is the largest province of the Cretaceous calc-alkaline magmatism, localized at the joint of the North-Asian continent and the North Pacific, where it forms a marginal continental Andean-type belt [23]. The deposit was discovered by 1:50,000-scale geologic mapping in the Soviet-period [24].
The Corrida deposit belongs to the Erguveyem ore district [15], confined to the similarly named volcanic-tectonic structure of circular type, which is 90 km in diameter. It is built from periclinally deposited Late Cretaceous volcanites of the calc-alkaline series (Na2O/K2O ratio ranges between 1.5 and 5.6) [24]; among these, the Nyrvakinot Formation, composed of andesites (U-Pb zircon age ca. 88.1 Ма) and felsic volcanites of the Amgen' Formations (U-Pb zircon age ca. 84-80 Ма) prevail [23,25]. The stock (Figure 1) exposed in the central part of the volcanic structure is about 15 km in diameter, built from quartz syenites and monzonites of the Late Cretaceous Ekityn complex of the estimated age U-Pb 84 ± 1.2 Ма (Na2O/K2O ratio ranges between 0.5 and 3.0) [24]. Small intrusions and dykes of granites, granodiorites, monzonites, syenites, subvolcanic bodies of fluidal and spherolite rhyolites and andesites of the Early and Late Cretaceous age are widely spread [24]. The structure basement is composed of Late Triassic to Early Cretaceous volcanicterrigenous-siliceous masses and associated gabbroids and ophiolites of the Velmay island-arc terrane [26]; their debris is observed in coarsely fragmented tuffs in the basement of the Amgen' rocks [27]. All known occurrences in the Erguveyem ore district are located at the joints of circular fractures bounding the volcanic-tectonic structure with regional faults of the north-north-eastern strike.
The most intense alterations with clear vertical zoning are observed in the felsic tuffs of the Amgen' Formation. Coarse-grained tuffs with sericite and sericite-quartz alterations, with adularia-quartz veining including Au-Ag mineralization, occur within the elevation interval of 200-350 m. At 350-400 m, we observe intense argillic alteration and hematitization. Within 400-450 m, there are kaolinite-alunite-quartz advanced argillic alterations ("secondary quartzites" by Russian therminology) that host rare quartz veinlets with poor sulphide mineralization. Within the interval of 450-500 m, welded ash tuffs are weakly altered. The unaltered ignimbrites occur above 500 m.
The ore bodies present the adularia-quartz veining zones with rare thin (0.1-0.5 m) veins. The bodies have mostly northwestern and northeastern strike, north and north-east dip (50-60°) and extremely uneven thickness, from 5 to 15 m, with swells of up to 35 m. Along the strike, they are traced from the surface for 1.3 km. From data [24], it can be seen that gold grade in ores varies from 1 to 33 ppm, and silver grade from 116 to 622 ppm.
Veins and veinlets are built mostly from medium-, fine-grained, cryptocrystalline chalcedonic quartz, seldom associated with adularia. They often have colloform-banded, framboidal-platy, massive, porous, brecciform, and breccia structures, and seldom have drusy structures (Figure 2). In breccia aggregates, numerous rubbles are presented by host rocks (Figure 2) cemented by cryptocrystalline quartz. The ore mineralization is disseminated unevenly from fine and uniform to sporadic and nested.

Materials and Methods
The ore has been studied in polished sections under the AXIOPLAN Imagin microscope.( NEISRI FEB RAS, Magadan, Russia) The chemical compositions of the minerals were determined with the Camebax X-ray electron-probe microanalyzer (FEB RAS, Magadan, Russia) (analyst E.M. Goryacheva) (EDS) and QEMSCAN attached to the EVO50 scanning electron microscope (FEB RAS, Magadan, Russia) (SEM) with the Quantax Esprit system of X-ray energy-dispersion microanalysis system using the standard P/B-ZAF method (analyst T.V. Subbotnikova) The content range was 0.0n-100% with an error for the main components not exceeding 1 wt. %. Statistic calculations of native gold grades were made with the GOLD software (IVerison) developed by S.V. Preis.
Additional analyses of composition of sphalerite and associated minerals were carried out using a MIRA 3 LMU (Tescan Orsay Holding, Novosibirsk, Russia) with EDS INCA Energy 450+ (Analytical Center for Multi-elemental and Isotope Research, Siberian Branch, Russian Academy of Sciences, Novosibirsk, Russia, analyst N.S. Karmanov). The operation conditions were: an accelerating voltage of 20 kV, a probe current of 1 nA and a spectrum recording time of 20 s. The detection limits of elements were <0.1%. The uncertainty was ≤1% for major components (>10-15 wt.%) and <2% for minor ones (1-10 wt.%). These dates were used for thermodynamic modeling.
Microthermometry of fluid inclusions was conducted in NEISRI FEB RAS with the measuring set based on the THMSG-600 stage (made by Linkam, London, UK), Motic microscope, Moticam camcorder, Olympus x50 long-focus lens, and the control computer. Individual fluid inclusions (FI) were studied following the methodologies from [29,30]. The fill factor (FF) was calculated considering FI, flattened in shape, by the formula: FF = Sf ÷ Sv × 100, where Sf stands for the area of the fluid phase, and Sv, for that of the vacuole. The salt composition of solutions was determined by eutectic temperatures [31]; salt concentration, by the ice melting temperature (Тice. mel.), according to [32]. Salt concentrations as well as water vapor density and pressures were calculated using the FLINCOR software [33] according to the system outlined in [34]. Compositions of gas mixtures (CO2, N2, CH4) in fluid inclusions were determined by Raman analyses on the Lab Ram HR 800 Raman dispersion spectrometer in the wide spectrum range of 150-3800 cm −1 , with the exciting line 532 nm of the He-Ne laser and the spectral slit 1.8 cm −1 . Complex contours were disintegrated with the Origin 7.5 software. Raman-spectroscopy was carried out at the Analytical Center for Multielemental and Isotope Research, Siberian Branch, Russian Academy of Sciences, Novosibirsk, Russia.

Mineral Composition of Ores
The present research has established over 20 ore and 11 vein minerals at the Corrida deposit (Table 1). Quartz is the most widely spread mineral in lode-veinlet zones. Most narrow veins and veinlets, as well as lode central parts, are usually filled with medium-to finelygrained, sometimes platy, light quartz, often associated with adularia (Quartz Type 1) (Figure 2a  Adularia does not exceed 15% of lode fill; besides, it is observed in combination with sericite and kaolinite in near-lode metasomatic formations. It is light-crème in colour and is presented by hypidiomorphic aggregates, its position in rhythmically striped aggregates is clearly seen in the structure pattern ( Figure 2).
Pyrite and arsenopyrite fill fine impregnations (1-2 µm to 0.2 mm, seldom to 3-5 mm) both in lode bodies and in wallrock zones of metasomatic alterations. Joint locations of pyrite and arsenopyrite are observed extremely rarely: they are predominantly located separately. Pyrite is abundant and found in association with all established sulphides (Figures 3 and 4). The signs of pyrite cataclasis and recrystallization are widepsread. Arsenopyrite forms practically no mineral associations and often occurs as disseminated inclusions in fine-grained quartz. The pyrite composition is stoichiometric; in the arsenopyrite composition, Fe grades exceed stoichiometric while As and S ones are lower: Fe1.10As0.95S0.95 (Table 2).
Galena is marked in medium-fine-grained light quartz both as fine impregnations and pockets of up to 4-5 mm in size (Figure 3a,b). In the dark chalcedonic quartz, it is seldom observed in the shape of unevenly distributed submicroscopic grains. Acanthite is often developed on the edges of galena aggregates as well as on their joints. The Seanalog of galena, clausthalite, is found in the paragenesis with naumannite. They occur as submicroscopic impregnations in grey quartz ( Figure 4, Table 3,) and in direct proximity to acanthite, pyrite, and sphalerite ( Figure 4). In chalcedonic quartz, submicroscopic impregnations ( Figure 4, Table 3) consist of clausthalite, naumannite, uytenbogaardtite-fischesserite series, argyrodite, andorite, pyrargyrite, lenaite, and acanthite. There is also polybasite, which is characterized by a lower content of Ag, higher Cu and Fe contents, and absence of As. Rarely observed mineral mixtures of the argentopyrite-lenaite-sternbergite series are characterized by lower Fe and higher Ag contents ( Table 3).
The most common Ag-bearing mineral in ores is acanthite, which occurs in associations with galena (Figure 3b), naumannite, argyrodite, clausthalite, and jarosite. It has the non-stoichiometric composition, and often contains Se (1.3 to 15.7 wt.%) and Fe (up to 3 wt.%) ( Table 3). Naumannite shows up to 3 wt.% S. Native gold commonly occurs as submicroscopic particles in chalcedonic quartz associated with acanthite ( Figure 3) and galena; less often it forms larger (up to 0.5 mm), xenomorphic insets in medium-and fine-grained quartz (Figure 3h) in association with pyrite and sphalerite. The fineness of native gold varies from 330 to 720‰ (Table 4), and averages 458‰; values are distributed bimodally, with peaks at 300-400 and 550-600‰. Native silver is rare in association with acanthite and galena . Silver grains in quartz do not exceed 0.7 mm in size (Figure 3i).
Among ore mineralization, various chlorides and bromides of Ag are present as finely dispersed dissemination in chalcedony ( Figure 3, Table 5). They are frequently localized in fissures and interstitions, and associated with anglesite (Figure 4a,b,h) and jarosite. Mineralogical analysis showed three productive mineral associations in Corrida ores: pyrite-arsenopyrite-sphalerite-chalcopyrite with native gold and acanthite; galena with native gold and Au-Ag sulphides and selenides; limonite-anglesite with acanthite, silver chlorides and bromides. Basic Au-and Ag-bearing minerals are native gold (electrum) and, to a lesser extent, minerals of the uytenbogaardtite-fischesserite series, acanthite, and naumannite.

Fluid Inclusions
In quartz samples from ore bodies of the Corrida deposit, 55 individual primary and primary-secondary FI were studied (Table 6). Under the ambient temperature, all FI are two-phase, gas-liquid in their phase composition ( Figure 5). They vary in size from 5 to 20 µm, of which 28% smaller than 10 µm. FI are unevenly distributed, both in groups and individually, in the central zones of quartz crystals ( Figure 5), are elongated, and, more rarely, round in shape. About 23% can be referred to FI with a prevailing gas phase (FF lower than 67) (Table 6, Figure 5b). FI with different FF are typically localized in growth zones and can be considered syngenetic (Figure 5с). n-number of measurements with similar values, united in one group; FF-fluid inclusion fill factor: ratio of voluminous parts of the liquid phase to the gas one. In 4 out of 8 compositions of FI "gas" phases, Raman-spectroscopy established CO2 with density from 0.05 to 0.19 g/cm 3 (calculated according to [49]), with minor contents of N2 and CH4 ( Figure 6) and CO2/N2/CH4 ratios from 0.97/0/0.03 to 0.92/0.07/0.01. Most FI are homogenized within the temperature range of 163 to 340 °С (Table 6). FI with predominant gas phase (FF = 50) are homogenized at 237-300 °С (Table 6), and those with the liquid phase (FF = 89-92), at 158-205 °С. Homogenization temperatures are distributed bimodally, with peaks at 275-300 °С and 150-175 °С.
Cryometric research shows that the last ice crystal in FI melts at temperatures between −2.1 and −0.1 °С (Table 6, Figure 7), which corresponds to salt concentration in solutions from 3.55 to 0.18 wt.% NaCl eq. FI containing solutions with salt concentration from 3.5 to 2.4 wt.% NaCl eq. are homogenized at temperatures from 240 to 340 °С, and form a group on the diagram (Figure 7). FI have the eutectic temperature range of −32 to −20°C, which suggests the presence of NaCl with MgCl2 and FeCl2 in the solution (Table 6, Figure 7). Salt composition of the solutions from FI remains stable throughout the ore process (Figure 7).

Physicochemical Parameters (fO2, fS2, fSe2, pH) of Ore Formation
Based on the data of mineral compositions of ores and hydrothermal alterations as well as on the results of fluid inclusions study, some physicochemical parameters of mineralization (ƒS2, ƒSe2, ƒO2, and pH) have been evaluated.
The electrum-sphalerite geothermometer is used for calculating the temperature and S fugacity values. In the present research, we studied the homogeneous grains of native gold in paragenesis with sphalerite. The composition of native gold from this paragenesis varies within the range xAg = 0.630-0.731; mole fraction of FeS in sphalerite (xFeS) is between 0.019 and 0.055. The calculations show that the formation of this mineral assemblage, with the above-mentioned compositions of native gold and sphalerite, requires temperatures from 192 to 274 °С and lоgƒS2 from −15.6 to −11.4. Calculated by different equations [17,47], these characteristics are close in value (Table 7) and do not exceed the above-estimated boundary values of ƒS2. In evaluating sulphur fugacity, based on the composition of sphalerite associated with Ag-sulphoselenides and sulphosalts, we used mineral formation temperatures according to the data from the FI research (150-175 °C) that supposedly corresponds to the formation of later Ag-containing minerals. The presence of argentopyrite in the association indicates temperatures below 150 °C [50]. The mole fraction of FeS in sphalerite (xFeS) in this association varies between 0.020 and 0.120. Calculations using equations from [17,47] show that sphalerite forms within the range of temperatures from 150 to 175 °C and sulfur fugacity lоgƒS2 = −20.4-−16.0, which remains within the ƒS2 boundary values estimated above.
Hydrothermal-metasomatic alterations of Corrida host rocks are represented by hydromica-quartz metasomatites, argillisites, and secondary quartzites replacing them on higher horizons. According to the research on metasomatic rocks [51], weakly acid to nearneutral solutions are typical of argillization, and ultra-acid solutions are typical for secondary quartzites. Moreover, the presence of jarosite in ores at the final stages of Corrida mineralization also suggests participation of acid hydrothermal solutions [52]. At the original stages, mineral-forming solutions might have had weakly acid to near-neutral pH and were later replaced with acid and ultra-acid solutions.

Discussion
The research showed three productive mineral associations in the ores of the Corrida deposit: (1) pyrite-arsenopyrite-sphalerite-chalcopyrite with native gold and acanthite; (2) galena with native gold and silver and Au-Ag sulphides and selenides; (3) limonite-anglesite with acanthite and silver chlorides and bromides. A specific feature of the ores is a broad range of Au-Ag-S-Se-Cl-Br minerals. The observed mineral interrelations and bimodal distribution of native gold fineness values imply a two-stage model formation of Au-Ag ores at the Corrida deposit: plutogenic-volcanogenic and hypergenic; the first stage can be divided into two substages.
The FI study revealed that the lode body quartz was formed from low-salt (3.55 to 0.18 wt. % NaCl eq.) hydrotherms, saturated with ions of chlorine, sodium, magnesium, and iron at temperatures from 340 to 158 °С. A low level of salt concentration in hydrothermal solutions is characteristic of epithermal systems. This may be a consequence of the condensation of magmatic vapor [53][54][55], and the boiling process [56,57]. Most FI were trapped in two temperature intervals, which show that the first ore-forming stage contained two substages: 300-275 °С and 175-150 °С. It was found that three kinds of quartz filling ore formations were formed successively on cooling of the system: (1) light, medium-to fine-grained quartz (Type 1), building quartz-adularia lode-veinlet aggregates of the colloform-banded and crustified-platy structures (Sample 016c) (Figure 2a,b; Table 5), was formed at 340 to 192 °С; (2) fine-grained quartz (Type 2), forming aggregates of massive, brecciform, and porous structures, with mostly galena mineralization (Sample 053) (Figure 2c,d; Table 5), at 307 to 172 °С; (3) grey, cryptocrystalline (Type 3), which builds dark rhythms of colloform-banded and banded aggregates, serves as the cementing material for breccia formation, and contains submicroscopic impregnations of gold and silver minerals (Sample 1014В) (Figure 2e,f; Table 5), at 205 to 158 °С. In ore-forming solutions, trapped by the light quartz FI (Type 1), salt concentration is seven times as large (Table 5; Figure 7) as that in the grey quartz FI (Type 3). Simultaneously, low-density CO2 with minor N2 and CH4 ( Figure 6) was found only in the light quartz FI, which means that in the initial period, up to approximately 300 °С, the ore-forming fluid contained low-density gases. Vapor phases, according to [57,58], are capable of transporting gold in the form of colloid particles of heterogeneous trapping. Prokofiev et al. [59] determined the presence of gold as nanoparticles in fluid inclusions by optical and spectroscopic methods. The FI in quartz from the Corrida deposit are very small. We observed no gold as nanoparticles in them. Possible species of gold transport in the ore-forming epithermal system are chloride and hydrosulfide complexes [43,60,61]. Breccia ore formations, cemented by the low-temperature variety of quartz, indicate that the hypogene stage is complicated by tectonic, probably seismic, fluctuations.
According to experimental research and thermodynamic modeling results [51,52], in the core sample of hydrothermal-metasomatic alterations of host rocks, at the 400-500 m horizon, hydromica-quartz metasomatites and argillisites are replaced by kaolinite-alunite-quartz secondary quartzites and monoquartzites, which indicates the change of pH in the solutions from weakly acid-near-neutral to acid during mineral formation. The horizon, in which kaolinite-alunite-quartz metasomatism is manifested, presumably corresponds to the level of the Corrida ore system paleo surface, where geothermal processes were accompanied by boiling, solution oxidation, and formation of quartz platy aggregate [62]; these might have even had zero connection with the ore formation process ("overprinting ore") [9].
Thus, it was established that in the Corrida ore system, on the background of lowering temperature, boiling, decreasing fluid salt concentration, and pH changing from nearneutral to acid, the oxidation potential was increasing, sulphur activity was lowering, but selenium activity was growing. These factors resulted in the significant variation of sulphoselenides and selenides of Ag in ores. According to the results of thermodynamic modeling and experiments [63,64], at such physicochemical conditions, the role of selenium as an ideal precipitator of Ag is multiplied. Here, the buried waters of an oxygenfree marine paleobasin saturated with an organic matter could be the source of selenium [65]; the waters warmed to over 250 °С, and the biologically bound selenium could mobilize into a hydrothermal fluid [66]. Their deposition in the discussed area was favorably promoted by shallow deposition of the OCVB built by the flinty masses of the Velmay island-arc terrane, less permeable than the OCVB volcanites and, therefore, capable of confining water.
Comparatively high, for epithermal ores, initial temperature of ore-forming fluid, presence of low-density gases and broadly spread acanthite in ores suggest that an intrusion chamber could be the source of the ore-forming fluid [10]. Probably such chamber for the Corrida ore system was a stock built by syenites and monzonites of the Ekityn complex, of the estimated age 84 ± 1.2 Ма [24], which was formed during the evolution of the central part of the Erguveyem volcano-tectonic structure. The ore process occurred close to this time, which is indicated by hydrothermal-metasomatic alterations in the rocks of the Leurvaam and the Amgen' Formation (84-80 Ma) and complete absence of such alterations in the rocks of the Nunlingran Formation of the Campanian age [22,25]. These data allow one to estimate a possible period of the Corrida formation as 84 to 80 Ma [67], i.e., the time when the basic volume of OCVB acid magmas was formed [23,68].
The data obtained in the present study (adularia availability, colloform ore structures, development of arsenopyrite and sphalerite, wide range of Au-Ag minerals, absence of enargite, tennantite, tetrahedrite, and other sulfosalts characteristic for HS systems [17]) show near-neutral pH of ore-forming solutions in the basic part of the system. The presence of СО2 in the ore-forming fluid at the initial stage, as an indicator of redox reactions under interaction of fluid with rocks [18], allows us to classify the Corrida deposit as an LS-type deposit. It was determined, for this group of objects, that the most favorable temperature conditions for the formation of rich ores are 180-280 °С [9]; temperatures above 280 °С (in this case, maximum ore formation temperature 340 °С) imply a high ore potential of the system.

Conclusions
The studied Corrida Au-Ag deposit, located at the periphery of the Erguveyem volcanic-tectonic depression, belongs to the group of epithermal LS-type deposits. The mineral composition of ore bodies here is characterized by a broad range of Au-Ag-S±Se-Cl-Br minerals. Basic Au-and Ag-bearing minerals are native gold and, to a lesser extent, minerals of the uytenbogaardite-fishesserite series, acanthite and naumannite. The ores were formed in two stages. The first hypogenic stage was from 84 to 80 Ma. Basic ore mineralization was formed in the medium-to low-temperature environment (340-150 °С) from low-salt (3.55 to 0.18 wt. % NaCl eq.) chloride hydrotherms, in the context of fluid boiling, pH change from near-neutral to acid, decreasing sulfur, and increasing selenium contents. The buried waters of the oxygen-free marine paleobasin saturated with the organic matter could be the source of Se, Cl and Br.