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Physicochemical Conditions of the Formation of Elevated Indium Contents in the Ores of Tin–Sulfide and Base-Metal Deposits in Siberia and Far East : Evidence from Thermodynamic Modeling. / Gaskov, I. V.; Gushchina, L. V.

в: Geochemistry International, Том 58, № 3, 18.03.2020, стр. 291-307.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

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@article{1457e2a06a72481c869e3969b9e19489,
title = "Physicochemical Conditions of the Formation of Elevated Indium Contents in the Ores of Tin–Sulfide and Base-Metal Deposits in Siberia and Far East: Evidence from Thermodynamic Modeling",
abstract = "The base-metal (70–75 wt %) and tin–sulfide (10–15 wt %) deposits are the main indium suppliers in the world. However, the causes and conditions of In accumulation in the ores of these deposits are still unclear. To shed light on this problem, we simulated the physicochemical conditions of formation of base metal and tin–sulfide ores with elevated indium content. For this purpose, the average composition of ore–bearing hydrothermal solutions and parameters of ore precipitation at these deposits were determined using available literature data. Based on these data, obtained standard thermodynamic characteristics Gf 0 Hf 0 of chloride indium species ($${\text{InCl}}_{2}^{ + },$$ InCl3, InClOH+), coefficients required for calculations at elevated temperature and pressure, the formation of elevated indium contents in these ores was numerically simulated using “Gem–Selektor-3” and “Chiller” softwares. The results of thermodynamic modeling of the formation of quartz–cassiterite and tin–sulfide ores show that the higher In contents in tin–sulfide ores are related to their formation from acid (pH 4.3), high–chloride (6.6 m) solutions, which contain In (0.002 m) in form of (InCl3aq). The quartz–cassiterite ores were formed from near–neutral (pH 5.3), low–chloride (1.02 m) solution, in which In occurred as hydroxocomplexes InO2H and InO2 in concentrations no more than 0.00004 m, which, respectively, determined its low contents in these ores. Computer modeling of the formation of indium–bearing sulfide-base metal and barite-base metal deposits shows that they were formed form high–temperature chloride (1.3–4.3 m) hydrothermal solutions of near–neutral composition (pH 5.8–6). The main In speciations are hydroxocomplexes InO2H and InO2, which provide In concentrations of 5–9 × 10–5 m). However, due to the low indium concentrations in hydrothermal solutions, the forming sulfide minerals (sphalerite, pyrite, and chalcopyrite) differ in the lower indium contents compared to the minerals of tin–sulfide ores.",
keywords = "chemical forms of indium transfer, indium, ore–forming systems, thermodynamic modeling, COMPLEXES, HIGH-PRESSURES, IONS, FLUID INCLUSIONS, ELECTROLYTES, TEMPERATURES, PARTIAL MOLAL PROPERTIES, ore-forming systems, GEOCHEMISTRY, STANDARD, CHLORIDE",
author = "Gaskov, {I. V.} and Gushchina, {L. V.}",
year = "2020",
month = mar,
day = "18",
doi = "10.1134/S0016702920030052",
language = "English",
volume = "58",
pages = "291--307",
journal = "Geochemistry International",
issn = "0016-7029",
publisher = "PLEIADES PUBLISHING INC",
number = "3",

}

RIS

TY - JOUR

T1 - Physicochemical Conditions of the Formation of Elevated Indium Contents in the Ores of Tin–Sulfide and Base-Metal Deposits in Siberia and Far East

T2 - Evidence from Thermodynamic Modeling

AU - Gaskov, I. V.

AU - Gushchina, L. V.

PY - 2020/3/18

Y1 - 2020/3/18

N2 - The base-metal (70–75 wt %) and tin–sulfide (10–15 wt %) deposits are the main indium suppliers in the world. However, the causes and conditions of In accumulation in the ores of these deposits are still unclear. To shed light on this problem, we simulated the physicochemical conditions of formation of base metal and tin–sulfide ores with elevated indium content. For this purpose, the average composition of ore–bearing hydrothermal solutions and parameters of ore precipitation at these deposits were determined using available literature data. Based on these data, obtained standard thermodynamic characteristics Gf 0 Hf 0 of chloride indium species ($${\text{InCl}}_{2}^{ + },$$ InCl3, InClOH+), coefficients required for calculations at elevated temperature and pressure, the formation of elevated indium contents in these ores was numerically simulated using “Gem–Selektor-3” and “Chiller” softwares. The results of thermodynamic modeling of the formation of quartz–cassiterite and tin–sulfide ores show that the higher In contents in tin–sulfide ores are related to their formation from acid (pH 4.3), high–chloride (6.6 m) solutions, which contain In (0.002 m) in form of (InCl3aq). The quartz–cassiterite ores were formed from near–neutral (pH 5.3), low–chloride (1.02 m) solution, in which In occurred as hydroxocomplexes InO2H and InO2 in concentrations no more than 0.00004 m, which, respectively, determined its low contents in these ores. Computer modeling of the formation of indium–bearing sulfide-base metal and barite-base metal deposits shows that they were formed form high–temperature chloride (1.3–4.3 m) hydrothermal solutions of near–neutral composition (pH 5.8–6). The main In speciations are hydroxocomplexes InO2H and InO2, which provide In concentrations of 5–9 × 10–5 m). However, due to the low indium concentrations in hydrothermal solutions, the forming sulfide minerals (sphalerite, pyrite, and chalcopyrite) differ in the lower indium contents compared to the minerals of tin–sulfide ores.

AB - The base-metal (70–75 wt %) and tin–sulfide (10–15 wt %) deposits are the main indium suppliers in the world. However, the causes and conditions of In accumulation in the ores of these deposits are still unclear. To shed light on this problem, we simulated the physicochemical conditions of formation of base metal and tin–sulfide ores with elevated indium content. For this purpose, the average composition of ore–bearing hydrothermal solutions and parameters of ore precipitation at these deposits were determined using available literature data. Based on these data, obtained standard thermodynamic characteristics Gf 0 Hf 0 of chloride indium species ($${\text{InCl}}_{2}^{ + },$$ InCl3, InClOH+), coefficients required for calculations at elevated temperature and pressure, the formation of elevated indium contents in these ores was numerically simulated using “Gem–Selektor-3” and “Chiller” softwares. The results of thermodynamic modeling of the formation of quartz–cassiterite and tin–sulfide ores show that the higher In contents in tin–sulfide ores are related to their formation from acid (pH 4.3), high–chloride (6.6 m) solutions, which contain In (0.002 m) in form of (InCl3aq). The quartz–cassiterite ores were formed from near–neutral (pH 5.3), low–chloride (1.02 m) solution, in which In occurred as hydroxocomplexes InO2H and InO2 in concentrations no more than 0.00004 m, which, respectively, determined its low contents in these ores. Computer modeling of the formation of indium–bearing sulfide-base metal and barite-base metal deposits shows that they were formed form high–temperature chloride (1.3–4.3 m) hydrothermal solutions of near–neutral composition (pH 5.8–6). The main In speciations are hydroxocomplexes InO2H and InO2, which provide In concentrations of 5–9 × 10–5 m). However, due to the low indium concentrations in hydrothermal solutions, the forming sulfide minerals (sphalerite, pyrite, and chalcopyrite) differ in the lower indium contents compared to the minerals of tin–sulfide ores.

KW - chemical forms of indium transfer

KW - indium

KW - ore–forming systems

KW - thermodynamic modeling

KW - COMPLEXES

KW - HIGH-PRESSURES

KW - IONS

KW - FLUID INCLUSIONS

KW - ELECTROLYTES

KW - TEMPERATURES

KW - PARTIAL MOLAL PROPERTIES

KW - ore-forming systems

KW - GEOCHEMISTRY

KW - STANDARD

KW - CHLORIDE

UR - http://www.scopus.com/inward/record.url?scp=85082871769&partnerID=8YFLogxK

U2 - 10.1134/S0016702920030052

DO - 10.1134/S0016702920030052

M3 - Article

AN - SCOPUS:85082871769

VL - 58

SP - 291

EP - 307

JO - Geochemistry International

JF - Geochemistry International

SN - 0016-7029

IS - 3

ER -

ID: 23949397