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Photomicrographs of different types of multisolid inclusions (type 4) within the recrystallized quartz (Q1N). The marked phases were identi fi ed by Raman (LRMS). 

Photomicrographs of different types of multisolid inclusions (type 4) within the recrystallized quartz (Q1N). The marked phases were identi fi ed by Raman (LRMS). 

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Unusual paleofluid composition is reported for the Libcice orogenic-type gold deposit located in the Central Bohemian Plutonic Complex (CBPC), Czech Republic. Unexpected bicarbonate-rich fluids and their complex chemistry variations characterize primary fluid inclusions from the main gold-bearing quartz vein. A detailed microthermometry, Laser Rama...

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... the inclusions is variable (negative crystal shapes being the most common). Some inclusions contained 1 or 2 birefrigent crystals identi fi ed by Raman spectroscopy as nahcolite and calcite (Fig. 6). These solids can be found in about 25 – 40% of all the type 1 inclusions, but can easily be overlooked. In inclusions that look unaffected by recrystallization and/or leakage, the volume occupied by nahcolite and calcite crystals is relatively constant (~5 vol.%). In a few type 1 inclusions, other unidenti fi ed solids were sporadically present. The relatively constant volume ratio of nahcolite crystals in type 1 inclusions may be considered to be circumstantial evidence for their daughter nature. The apparent absence of nahcolite in some inclusions may re fl ect kinetic dif fi culties associated with nahcolite nucleation. We have noticed nahcolite nucleation after a cooling (freezing) cycle in a few inclusions. The partial homogenization of the carbonic phase (Th(car)), almost always to a liquid (L car +V car → L car ), ranges between − 21.6 °C and 29.5 °C. Final melting of solid CO 2 (Tm(car)) occurs between − 56.6 °C and − 64.1 °C and the fi nal clathrate dissolution Tm(Cla) occurs between 8.3 °C and 12.3 °C. Systematic variation of Th(car) was observed in individual quartz grains in some samples: grain cores usually show the highest Th(car) values, while the rims exhibit the lowest ones (Fig. 7). The majority of the inclusions decrepitated shortly before their fi nal fl uid homogenization or immediately after this temperature. Some inclusions homogenized at 280 – 315 °C (Th(total), usually to vapor). The observed dissolution temperature of nahcolite is within 80 – 90 °C. The calcite crystals trapped in the same inclusions do not dissolve until the inclusion decrepitation at about 255 °C. Type 2 inclusions (Fig. 4) are predominantly hosted by recrystallized quartz (Q1N), typically in the form of sparse 3D-distributed inclusions, possibly of primary origin (with respect to Q1N). Type 2 inclusions also rarely form secondary trails in relic quartz (Q1Ur). Of all type 2 inclusions present in a sample, usually those hosted by quartz enclosed inside a sulphide matrix (pyrite and/or pyrrhotine) were the largest and thus the most suitable for microthermometry (Fig. 2). Type 2 inclusions are always two-phase (aqueous liquid + carbonic vapor) at room temperature, are 3 to 70 μ m in size (commonly 10 – 25 μ m), and display regular or negative crystal shapes. The volume fraction of the aqueous liquid is 0.5 ± 0.2. Similarly to type 1 inclusions, one or more solid phases (nahcolite and/or carbonate) were identi fi ed and are present in 50 – 70% of type 2 inclusions. With respect to the density of the gaseous phase, two subtypes can be de fi ned. High density type 2 (TYPE 2a): Tm(car) from − 66.2 to − 60.0 °C (however not measurable in every inclusion), Th(car) from − 49 to +20 °C (always to L), and Tm(Cla) from +10.8 to +18.5 °C. Low-density type 2 (type 2b): the gas content of inclusions did not freeze even down to − 196 °C. Th(car) occurred from − 80 to − 11 °C (always to V) and Tm (Cla) from +14.3 to +19.5 °C. The inclusions probably correspond to the H 2 type of the Van den Kerkhof (1990) classi fi cation. Apart from the density, there is no difference in the size, shape, distribution and volume fraction of the aqueous phase of type 2a and type 2b inclusions. We are not able to separate type 2a and 2b inclusions by petrographic criteria alone. Therefore we cannot exclude that they represent two separate and genetically different inclusion types. The fi nal homogenization /Th(total)/ could not be measured due to partial leakage of majority inclusions above 250 °C (type 2a). In most inclusions, nahcolite remained in the inclusions up to their decrepitation without any evidence of dissolution. Only occasionally melting of nahcolite was observed between 84 °C and 90 °C. Important variations of the CO 2 /CH 4 ratio were found in both subtypes. However, there is no correlation between this parameter and the inclusion distribution at the grain scale (in contrast to type 1 inclusions in Q1Ur). Type 3 inclusions (Fig. 4) are secondary and mostly form short intragranular trails in Q1Ur and Q1N quartz. Rare trails crosscutting grain boundaries between quartz Q1Ur and Q1N were also found. Inclusions are two-phase (aqueous liquid + aqueous vapor) at room temperature, mostly oval shaped and show homogeneous volume fraction of aqueous liquid (0.9 – 0.95). The temperature of the fi rst/ initial melting (Ti) is from − 44 to − 37.0 °C and the fi nal melting of ice (Tm(Ice)) is between − 4 and − 1 °C, indicating that calcium is the main cation. There is no microthermometric evidence for the presence of gases. The total homogenization temperature (Th(total), usually to liquid) shows three maxima around 140, 180 and 260 °C. We have found numerous single-phase to multi-phase solid inclusions inside grains of recrystallized quartz Q1N (Fig. 5). Occa- sionally, a volumetrically insigni fi cant fl uid phase was also identi fi ed. Some solids are very dif fi cult to recognize or even to see by optical microscopy using a classical bright fi eld. Very careful observation incorporating both plane and crossed polarization was necessary to observe their presence. Type 4 inclusions (up to about 150 – 200 μ m in size) usually consist of 3 to 10 solid phases. Based on their petrographic criteria, they are considered primary with respect to Q1N. The most frequent solid phases (identi fi ed using Raman microspectroscopy) are chlorite, calcium carbonate and albite, with a size that usually varies from 20 to 50 μ m. Other solids (muscovite, rutile, pyrite, apatite, titanite, anatase ± some unidenti fi ed solids) occur randomly in different inclusions. It seems that there is a correlation between the number of type 4 inclusions present in the individual samples and the depth of the sample in the mine (i.e. distance to the granodiorite contact). The samples closest to the contact generally contain the highest number of multisolid inclusions. The fl uid phase (gas, aqueous or both) mostly wets the surface of the solids, which makes its optical identi fi cation dif fi cult and explains the absence of microthermometric data for these inclusions. However, H 2 O, CO 2 , CH 4 , N 2 , and H 2 were identi fi ed using Raman microspectrometry (see Section 6). Quantitative gas content measurements were performed on series of about 40 fl uid inclusions representing the primary inclusions (type 1) in the original quartz (Q1Ur) and the primary inclusions (type 2) in the recrystallized quartz (Q1N). Selected representative measurements are presented in Tables 1 and 2. Type 1 inclusions show (H 2 O) – CO 2 – CH 4 (±N 2 , H 2 S) composition with CO 2 as the main gas compound (98 to 89 mol% of gas content), CH 4 between 0.6 and 10 mol% and traces of N 2 and H 2 S around 0.5 and 0.1 mol%, respectively. Type 2 inclusions contain traces of C 2 H 6 , in addition to (H 2 O) – CO 2 – CH 4 (±N 2 , H 2 S). The variations in the CO 2 /CH 4 ratio are far more noticeable than in type 1 inclusions. The CO 2 concentration varies from 95 mol% to 14 mol% and CH 4 varies from 5 mol% to 86 mol%. The concentrations of N 2 and H 2 S are almost constant, around 0.5 and 0.1 mol%, respectively. C 2 H 6 is constantly present at trace levels (0.1 mol%) and was identi fi ed from its Raman peaks (C – H stretching at 2955 cm − 1 and C – C stretching at 990 cm − 1 ) (Fig. 6). No evidence for precipitated carbon inside the inclusions was found by LRM. Type 4 inclusions: the composition of the volumetrically accessory fl uid phase is highly variable — from nearly poor CH 4 in some cases to CH 4 – CO 2 mixtures (with or without H 2 O). In some inclusions, H 2 was identi fi ed (Fig. 6) in concentrations as high as 6 mol% (calculated using the standard methodology as described in Dubessy et al. (1989)). The aqueous phase was also checked for the presence of polyatomic ions, such as CO 2 3 − , HCO − 3 , SO 4 , PO 3 4 − and HS − , which are Raman active, permitting their identi fi cation and analysis in the fl uid phase (Rosasco and Roedder, 1979; Dubessy et al., 1983,1989). HCO − 3 in the aqueous phase of type 1 and type 2 inclusions was identi fi ed by its Raman peaks at 1013 cm − 1 and 1362 cm − 1 (Davis and Oliver, 1972; Oliver and Davis, 1973; Kruse and Franck, 1982; Frantz, 1998) (Fig. 6) which were obtained even with small integration times (2 s), indicating a high concentration around 1 mol/l. Dissolution of nahcolite at 80 – 90 °C indicates NaHCO 3 concentrations around 2 mol/l NaHCO 3 (Kogan et al., 1969; Vapnik and Moroz, 2002; Haynes, 2003). High-temperature Raman measurements also indicated the presence of HCO − 3 in solution after homogenization of selected inclusions at 326 °C. Calculation of the bicarbonate ion concentration from the Raman spectra is under development, so we were not able to quantify it precisely. These estimations suggest that HCO − 3 is probably the main anion in the solutions. In spite of the fact that only 25 – 40% of the inclusions demonstrably contain nahcolite crystals, the authors assume the nahcolite is of primary (i.e. daughter) origin, based on the relatively constant crystal/inclusion volume ratio (see above) and on the Th(total) of the fl uids over 300 °C which (most likely) excludes the presence of solid (i.e. trapped) nahcolite (Hoshino et al., 2006). The dissolution temperature of nahcolite in type 2 inclusions is highly variable, from 84 – 90 °C usually to above 250 °C, without any evidence of dissolution at this temperature. High dissolution temperatures can be interpreted either by high concentrations of bicarbonate, trapping of nahcolite together with the fl uid, or by metastability. According to previous data on fl uid inclusions, dissolution temperature around 80 °C in type 1 inclusions and industrial dissolution plants of nahcolite deposits, the ...
Context 2
... have found numerous single-phase to multi-phase solid inclusions inside grains of recrystallized quartz Q1N (Fig. 5). Occa- sionally, a volumetrically insignificant fluid phase was also identified. Some solids are very difficult to recognize or even to see by optical microscopy using a classical bright field. Very careful observation incorporating both plane and crossed polarization was necessary to observe their ...

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Citations

... In the Neoproterozoic Bohemian massif (Czech Republic), quartz from the Libice orogenic gold deposit hosts uncommon fluid inclusions rich in H 2 (< 6 mol. %) and bicarbonates (Hrstka et al., 2011). CH 4 content variability in the inclusions is interpreted as related to post-entrapment H 2 diffusion into the fluid inclusions. ...
... H 2 could indeed be trapped during inclusion formation in the presence of the metamorphic fluid involved in gold deposition. Alternatively, the fluid inclusion composition could be modified after entrapment due to later hydrogen diffusion into the inclusion (Mavrogenes and Bodnar, 1994;Hrstka et al., 2011;Goldfarb and Groves, 2015). As a result, 20 high H 2 concentrations in fluid inclusions in gold deposits could reflect postentrapment H 2 production, which is a process of interest here. ...
Article
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... These gold deposits are hosted in the Paleoproterozoic Houndé belt and the Neoproterozoic Nubian shield, respectively. In the Neoproterozoic Bohemian massif (Czech Republic), quartz from the Libčice orogenic gold deposit hosts uncommon fluid inclusions rich in H 2 (<6 mol%) and bicarbonates (Hrstka et al., 2011). CH 4 content variability in the inclusions is interpreted as related to postentrapment reaction of CO 2 with H 2 diffusing into the fluid inclusions. ...
... H 2 could indeed be trapped during inclusion formation in the presence of the metamorphic fluid involved in gold deposition. Alternatively, the fluid inclusion composition could be modified after entrapment due to later hydrogen diffusion into the inclusion (Goldfarb and Groves, 2015;Hrstka et al., 2011;Mavrogenes and Bodnar, 1994). As a result, high H 2 concentrations in fluid inclusions in gold deposits could reflect post-entrapment H 2 production, which is a process of interest here. ...
Preprint
A review of the localities in continental rocks where H2-rich gases have been reported, showed that they are mainly located near gold deposits. Two types of geomorphological features known as markers of gas venting in sedimentary basins were also systematically observed near orogenic gold deposits on satellite images. They consist in both barren ground depressions and high densities of small (< 20 m in diameter) circular- and comet-shaped white spots in 32 and 7 localities, respectively. Point pattern analysis revealed that the white spots are self-organized, and similar to previously described vegetation patterns including termite mounds and fairy circles. We proposed a geochemical model to account for this relationship between orogenic gold deposits, H2 emanations and geomorphological features. Fe-carbonates are ubiquitous mineral products associated with gold mineralization. They can further dissolve in the presence of aqueous fluid due to their high reactivity below 200°C to produce magnetite and up to ~ 1 mole of H2 per kg of rock along with ~ 3 mol/kg CO2. This process induces a solid volume decrease of 50 %. Therefore, we propose that Fe-carbonate dissolution is (1) the primary source of H2 in orogenic gold deposit areas, and (2) involved in the formation of the geomorphological structures reported here, providing a new framework to understand their seemingly complex formation. Ground depressions and white spots are possible tools for gold explorations. Actually, we identified four new areas where we suspect possible orogenic gold deposits. The association between H2-rich gas and ground depressions was also made near other formations containing Fe-carbonates such as iron formations and carbonatites. This suggests that H2 production through Fe-carbonate dissolution is not restricted to gold deposits. The global H2 production in crustal rocks associated with Fe-carbonate alteration is estimated to 3.10^5 mol/yr.
... In addition, the minerals composing the multiphase inclusion are tightly packed and are interlocked each other (Figure 3(l)). These chemical and textural features would eliminate the possibility that the minerals composing multiphase inclusion were accidentally trapped as pre-existing crystals during garnet growth like the cases reported by Hrstka et al. (2011). The multiphase inclusion represents polygonal shape that would be shape of negative crystal of garnet, and cuspate offshoot filled with phengite protruding from the corner of the polygonal shape (Figure 3(l)). ...
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... In Sudan, such fluids have been recorded in the Hamadi gold deposit (Cheng et al. 2017). The debate about the origin of CO 2rich fluid inclusions involves various possibilities (Klemd and Hirdes 1997;Chi et al. 2006;Klein and Fuzikawa 2010;Hrstka et al. 2011), including 1) specific fluid sources from high-grade metamorphism or early degassing of magmatic intrusions; 2) fluid-related processes such as selective vapour accumulation following fluid immiscibility; two fluids operating separately; or unmixing because of pressure fluctuations; and 3) postentrapment modifications of fluid inclusions. Recently, Gaboury (2013) proposed that CO 2 -rich fluids may be the result of the degradation of C 2 H 6 and the consumption of H 2 O, leading to the progressive enrichment of CO 2 in the fluids, following the reaction: ...
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... Mineralization of sphalerite in the Latala Deposit has occurred in shallow parts of sedimentaryvolcanic sequence (Padyar, 2017;Padyar et al., 2017a). One of the proposed mechanisms for the generation of H 2 attributes it to intense alteration including formation phyllosilicates involving redox reactions (Hrstka et al., 2011;Dubessy et al., 1988). During wall-rock reactions with fluid cooling in contact with intermediate-composition magmatic rocks, de-sulphidation of the fluid by iron in the wall rocks competes with the H + metasomatism effect of feldspar-destructive alteration (Heinrich, 2005). ...
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This paper presents the properties of fluid inclusions found in sphalerite from Latala epithermal base and precious metal deposit (Central Iran), which is hosted in Cenozoic volcanic-sedimentary host-rocks. The Latala Deposit represents an example of vein type, base metal deposits in the Miduk porphyry copper deposits (PCDs) in southern Urumieh-Dokhtar magmatic belt (UDMB). Mineralization in Latala epithermal base and precious metal vein type formed in 3 stages and sphalerite-quartz veins occur in stages 2 and 3. Stage 2 quartz-sphalerite veins are associated with chalcopyrite and zoned sphalerite, along with quartz+hematite, and Stage 3 quartz-sphalerite veins contain galena+sphalerite+chalcopyrite and quartz with overgrowth of calcite. Mineralization in Stage 3 occurs as replacement bodies and contains Fe-poor sphalerite without zoning in the outer parts of the deposit. This paper focuses on fluid inclusions in veins bearing sphalerite and quartz. The fluid inclusion homogenization temperatures and salinity in sphalerite (some with typical zoning) range from 144 to 285 ºC and from 0.2 wt.% to 7.6 wt.% NaCl eq. Sphalerite and fluid inclusions of the Latala base and precious metal deposit formed from relatively low-T and low-salinity solutions. Raman spectroscopy analyses indicate a high percentage of CO2 in the gas phase of fluid inclusions in Fe-poor sphalerites, as expected with melting temperature for CO2 of −56.6 ºC, and significant amounts of H2. Lack of reduced carbon species (methane and lighter hydrocarbons) was confirmed in the petrographic study using UV light and Raman spectros-copy. High amounts of H2 in fluid inclusions of Fe-poor sphalerite can be the result of different intensities of alteration and diffusion processes. The common occurrences of CO2 in fluid inclusions have originated from magma degassing and dissolution of carbonates. The δ³⁴S values for sulfide minerals in galena of sphalerite bearing veins vary between −9.8‰ and −1.0‰, and the δ³⁴S values calculated for H2S are between −7.1‰ and +0.6‰. These values correspond to magmatic sulfur whit possible interaction with wall rocks. Magmatic fluids were successively diluted during cooling and continuous ascent. Secondary boiling would lead to variable amounts of potassic or prophylactic alteration and the hydrogen diffusion into the inclusions hosted in sphalerite of Latala.
... The Bohemian Massif, Czech Republic, hosts several gold deposits of these genetic types, some with important economic grade (e.g., Mokrsko-West; Zachariáš et al. 2014), occurring in two prominent metallogenic zones (Morávek and Pouba 1987): (1) the Central Bohemian Metallogenetic Zone (CBMZ) and (2) the Kašperské Hory-Hartmanice Metallogenetic Zone. The former is associated with the Central Bohemian Plutonic Complex (CBPC) (e.g., Kasejovice-Bělčice deposits- Zachariáš and Pudilová 2002;Hrstka et al. 2011;Krásná Hora deposit-Němec and Zachariáš 2017) and its contacts with Neoproterozoic volcano-sedimentary rocks of the Teplá-Barrandian Unit (e.g., Mokrsko-Čelina deposit- Morávek et al. 1989;Zachariáš et al. 2014;Jílové deposit-Zachariáš et al. 2013; Petráčkova Hora deposit- . In comparison, the latter is represented by the Kašperské Hory gold deposit (Strnad et al. 2012), located farther southwest in high-grade metamorphic rocks of the Moldanubian Unit. ...
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... Al 2 Si 2 O 5 (OH) 4 + 2Na + + 2CO 2 + H 2 O = 2NaAlCO 3 (OH) 2 + 2SiO 2 + 2H + Boiling at high temperature and the common occurrence of CO 2 in fluid inclusions from the Latala epithermal system may suggest a magmatic source for the ore fluids, that may have originated from magma degassing and dissolution of carbonates (Coveney and Kelly, 1971;Sirbescu and Nabelek, 2003). High amounts of H 2 in fluid inclusions of Fe-poor sphalerite can be the result of different processes during alteration (Hrstka et al., 2011). Mineralization of sphalerite in Fig. 8. ...
... A B. Raman spectra of the gas phase in fluid inclusion of sphalerite suggesting the occurrence of a mixture of CO 2 (1285 cm -1 and 1388 cm -1 ), CO (2143 cm -1 ) and H 2 (4126 and 4156 cm -1 ). the Latala deposit has occurred at shallow parts in sedimentary-volcanic sequence. One of the proposed mechanisms for the generation of H 2 attributes it to intense alteration including formation phyllosilicates involving redox reactions (Hrstka et al., 2011). During fluid cooling in contact with intermediate-composition magmatic rocks, desulphidation of the fluid by iron in the wall rocks competes with the H + neutralising effect of feldspar-destructive alteration. ...
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Full-text available
The Cenozoic Urumieh-DokhtarMagmaticBelt (UDMB) of Iran is a major host to porphyry Cu-Mo-Au deposits (PCDs), represented by the world-class Sarcheshmeh deposit and Miduk deposit in the south and the Sungun deposit in the north. Vein type, base and/or precious metal deposits are also common and some are spatially associated with PCDs. Latala and Chahmessi are vein type, base and precious metal deposits in the north and southwest Miduk deposit. The area is covered mainly by Paleocene-Eocene volcanic and pyroclastic rocks of basaltic, basaltic-andesitic and trachy-andesitic compositions, and minor marls and limestones. The volcanic and pyroclastic rocks are intruded by Miocene shallow intrusions of quartz diorite, quartz monzonite and granodiorite compositions.The rocks are host to a set of ore-bearing quartz veins. Mineralization in both the Chahmessi and Latala deposits are controlled by faults and fractures. The role of the ring structures and faults in the distribution of hydrothermal alteration zones and mineralization is important in the Latala deposit. In these veins, euhedral quartz with sulfide mineralization occurs as open space fillings, minor replacement bodies and hydrothermal breccia. The veins consist of quartz, calcite, pyrite, chalcopyrite, galena, sphalerite, bornite and minor sulfosalts, particularly enargite. According to studies based on fluid inclusions in the Miduk porphyry, three types of fluids are responsible for mineralization. Homogenization temperatures and salinity in porphyry-type fluids vary from 566 to 162 °C and 61.3 to 1.2 wt% NaCl equiv. For the Latala vein type base and precious metals deposit, homogenization temperature and salinity vary from 380 to 131 °C and 10.6 to 0.17 wt% NaCl equiv. The gas phase in fluid inclusions of Latala is dominated by CO 2 but also shows the presence of CO and H 2 , characterizing reducing conditions associated with ore deposition. The change from lithostatic to hydrostatic regime, boiling and fluid dilution associated with the introduction of meteoric fluids provides an explanation for the widespread Th and salinity data. Calculated pressure for examples of Miduk fluid inclusions varies from 700 to 200 bars. These pressures correspond to depths of 2500 to 1500 metres for porphyry mineralization. The three-phase fluid inclusions, corresponding to magmatic fluid, show the highest pressure. The Latala base and precious metals deposit has formed at pressures between 200 and 100 bars, corresponding to a depth of less than 1 km. Sphalerite mineralization occurs in shallow parts of the sedimentary-volcanic sequence from magmatic fluids diluted by meteoric fluids and also occurs in more distal parts of the porphyry. The sulphur isotopic composition for sulfide minerals varies between-9.8 and-1.0‰, which correspond to values of magmatic sulfur. This suggests that magmatic water was responsible for transportation of metals in Latala. Epithermal mineral precipitation occurred upon dilution of the low-salinity magmatic fluid with meteoric water, which entered the hydrothermal system as it cooled and successively diluted during continued magmatic fluid ascent.
... Their generation has been attributed to metamorphic fluids, deep circulating meteoric water, magmatic fluids or other sources (e.g. Kerrich and Cassidy, 1994;Groves et al., 1998;Hagemann and Cassidy, 2000;Boiron et al., 2001;Goldfarb et al., 2001;Boiron et al., 2003;Goldfarb et al., 2005;Hrstka et al., 2011). In addition, the presence of variable amounts of non-aqueous volatiles, such as CH 4 -N 2 and their fraction variations (e.g. ...
... Their generation has been attributed to metamorphic fluids, deep circulating meteoric water, magmatic fluids or other sources (e.g. Kerrich and Cassidy, 1994;Groves et al., 1998;Hagemann and Cassidy, 2000;Boiron et al., 2001;Goldfarb et al., 2001;Boiron et al., 2003;Goldfarb et al., 2005;Hrstka et al., 2011). In addition, the presence of variable amounts of non-aqueous volatiles, such as CH 4 -N 2 and their fraction variations (e.g. ...
Article
The Hatu gold deposit is located in the West Junggar domain, Xinjiang, China. It contains 56 tonnes of gold. The deposit is hosted in the volcanic and sedimentary rocks of the Early Carboniferous Tailegula Group, and an ~E–W trending ductile shear zone controls the mineralization. The gold mineralization is hosted in quartz veins and hy-drothermally altered country rocks with b3 vol.% sulfides developed along the faults. The fluid inclusions are characterized by the presence of dominant CO 2 and minor CH 4 fluid. The δ 13 C VPDB values of CH 4 (−18.7‰ to −35.4‰) and CO 2 (−9.7‰ to −13.9‰) in fluid inclusions from quartz and their Δ 13 C CO 2 –CH 4 values (5.5‰ to 24.6‰) equilibrated at a temperature range from 299 °C to 1013 °C; these data indicate that the carbon had a dominantly sedimentary source with a minor contribution from the mantle. The oxygen and hydrogen isotope compositions (δ 18 O = 8.5‰ to 12.2‰, δD = −87‰ to −105‰) of water from fluid inclusions in quartz indicate that ore fluids comprised largely metamorphic water with a minor contribution of magmatic water. The δ 34 S values of sulfide from the mineral zones are between −2.3‰ and + 2.5‰, with the exception of two values (−9.7‰ and +7.4‰), showing a heterogeneous sulfur source. Fluid inclusions in pyrite and arsenopyrite that are intergrown with auriferous quartz have 3 He/ 4 He ratios of 0.2 to 0.3 Ra, and their 40 Ar/ 36 Ar ratios range from 310 to 650, indicating a crustal source for much of the ore fluids. We propose that the Hatu deposit is a structurally controlled orogenic gold system which is characterized by two different fluids one dominantly derived from a crustal source with a minor component of mantle derived fluids.
... Hydrogen, as well as longer-chain hydrocarbons than methane, are reported in the ore-related fluid inclusions for some orogenic gold deposits (Gaboury, 2013;Goldfarb et al., 1989;Guha et al., 1990). Hrstka et al. (2011), for example, reported as much as 6 mol% H 2 , as well as significant C 2 H 6 and HCO 3 − concentrations, from Laser Raman Micro Spectroscopy studies of individual fluid inclusions from the Libcice orogenic gold deposit in the Bohemian Massif, Czech Republic. However, the significance of hydrogen, ethane, propane, and other higher hydrocarbons is unclear, because these could easily be the products of reactions between C-, O-, and H-bearing volatiles in fluid inclusion cavities during uplift-related drops in pressure and temperature (Tsunogae and Dubessy, 2009). ...
... However, the significance of hydrogen, ethane, propane, and other higher hydrocarbons is unclear, because these could easily be the products of reactions between C-, O-, and H-bearing volatiles in fluid inclusion cavities during uplift-related drops in pressure and temperature (Tsunogae and Dubessy, 2009). In the Hrstka et al. (2011) study, heat from post-ore magmatism in the Bohemian Massif was suggested to have mobilized hydrogen from organic matter in the country rocks at temperatures N500°C, thus yielding H 2 rather than CH 4 , with the former diffusing into fluid inclusions closest to quartz grain boundaries during recrystallization of the quartz. Thus, such post-gold modification of ore-stage fluid inclusions by addition of H 2 might be expected in other sedimentary rock-hosted orogenic gold deposits, particularly where the sedimentary rocks are relatively reducing and there is nearby younger magmatism and associated contact metamorphism. ...
Article
Orogenic gold deposits of all ages, from Paleoarchean to Tertiary, show consistency in chemical composition. They are the products of aqueous-carbonic fluids, with typically 5–20 mol% CO2, although unmixing during extreme pressure fluctuation can lead to entrapment of much more CO2-rich fluid inclusions in some cases. Ore fluids are typically characterized by significant concentrations of CH4 and/or N2, common estimates of 0.01–0.36 mol% H2S, a near-neutral pH of 5.5, and salinities of 3–7 wt.% NaCl equiv., with Na > K > > Ca,Mg. This fluid composition consistency favors an ore fluid produced from a single source area and rules out mixing of fluids from multiple sources as significant in orogenic gold formation. Nevertheless, there are broad ranges in more robust fluid-inclusion trapping temperatures and pressures between deposits that support a model where this specific fluid may deposit ore over a broad window of upper to middle crustal depths.