Carbon dioxide in magmas and implications for hydrothermal systems
This review focuses on the solubility, origin, abundance, and degassing of carbon dioxide (CO^sub 2^) in magma-hydrothermal systems, with applications for those workers interested in intrusion-related deposits of gold and other metals. The solubility of CO^sub 2^ increases with pressure and magma al...
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description | This review focuses on the solubility, origin, abundance, and degassing of carbon dioxide (CO^sub 2^) in magma-hydrothermal systems, with applications for those workers interested in intrusion-related deposits of gold and other metals. The solubility of CO^sub 2^ increases with pressure and magma alkalinity. Its solubility is low relative to that of H^sub 2^O, so that fluids exsolved deep in the crust tend to have high CO^sub 2^/H^sub 2^O compared with fluids evolved closer to the surface. Similarly, CO^sub 2^/H^sub 2^O will typically decrease during progressive decompression- or crystallization-induced degassing. The temperature dependence of solubility is a function of the speciation of CO^sub 2^, which dissolves in molecular form in rhyolites (retrograde temperature solubility), but exists as dissolved carbonate groups in basalts (prograde). Magnesite and dolomite are stable under a relatively wide range of mantle conditions, but melt just above the solidus, thereby contributing CO^sub 2^ to mantle magmas. Graphite, diamond, and a free CO^sub 2^-bearing fluid may be the primary carbon-bearing phases in other mantle source regions. Growing evidence suggests that most CO^sub 2^ is contributed to arc magmas via recycling of subducted oceanic crust and its overlying sediment blanket. Additional carbon can be added to magmas during magma-wallrock interactions in the crust. Studies of fluid and melt inclusions from intrusive and extrusive igneous rocks yield ample evidence that many magmas are vapor saturated as deep as the mid crust (10-15 km) and that CO^sub 2^ is an appreciable part of the exsolved vapor. Such is the case in both basaltic and some silicic magmas. Under most conditions, the presence of a CO^sub 2^-bearing vapor does not hinder, and in fact may promote, the ascent and eruption of the host magma. Carbonic fluids are poorly miscible with aqueous fluids, particularly at high temperature and low pressure, so that the presence of CO^sub 2^ can induce immiscibility both within the magmatic volatile phase and in hydrothermal systems. Because some metals, including gold, can be more volatile in vapor phases than coexisting liquids, the presence of CO^sub 2^ may indirectly aid the process of metallogenesis by inducing phase separation.[PUBLICATION ABSTRACT] |
doi_str_mv | 10.1007/s001260100185 |
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The solubility of CO^sub 2^ increases with pressure and magma alkalinity. Its solubility is low relative to that of H^sub 2^O, so that fluids exsolved deep in the crust tend to have high CO^sub 2^/H^sub 2^O compared with fluids evolved closer to the surface. Similarly, CO^sub 2^/H^sub 2^O will typically decrease during progressive decompression- or crystallization-induced degassing. The temperature dependence of solubility is a function of the speciation of CO^sub 2^, which dissolves in molecular form in rhyolites (retrograde temperature solubility), but exists as dissolved carbonate groups in basalts (prograde). Magnesite and dolomite are stable under a relatively wide range of mantle conditions, but melt just above the solidus, thereby contributing CO^sub 2^ to mantle magmas. Graphite, diamond, and a free CO^sub 2^-bearing fluid may be the primary carbon-bearing phases in other mantle source regions. Growing evidence suggests that most CO^sub 2^ is contributed to arc magmas via recycling of subducted oceanic crust and its overlying sediment blanket. Additional carbon can be added to magmas during magma-wallrock interactions in the crust. Studies of fluid and melt inclusions from intrusive and extrusive igneous rocks yield ample evidence that many magmas are vapor saturated as deep as the mid crust (10-15 km) and that CO^sub 2^ is an appreciable part of the exsolved vapor. Such is the case in both basaltic and some silicic magmas. Under most conditions, the presence of a CO^sub 2^-bearing vapor does not hinder, and in fact may promote, the ascent and eruption of the host magma. Carbonic fluids are poorly miscible with aqueous fluids, particularly at high temperature and low pressure, so that the presence of CO^sub 2^ can induce immiscibility both within the magmatic volatile phase and in hydrothermal systems. 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The solubility of CO^sub 2^ increases with pressure and magma alkalinity. Its solubility is low relative to that of H^sub 2^O, so that fluids exsolved deep in the crust tend to have high CO^sub 2^/H^sub 2^O compared with fluids evolved closer to the surface. Similarly, CO^sub 2^/H^sub 2^O will typically decrease during progressive decompression- or crystallization-induced degassing. The temperature dependence of solubility is a function of the speciation of CO^sub 2^, which dissolves in molecular form in rhyolites (retrograde temperature solubility), but exists as dissolved carbonate groups in basalts (prograde). Magnesite and dolomite are stable under a relatively wide range of mantle conditions, but melt just above the solidus, thereby contributing CO^sub 2^ to mantle magmas. Graphite, diamond, and a free CO^sub 2^-bearing fluid may be the primary carbon-bearing phases in other mantle source regions. Growing evidence suggests that most CO^sub 2^ is contributed to arc magmas via recycling of subducted oceanic crust and its overlying sediment blanket. Additional carbon can be added to magmas during magma-wallrock interactions in the crust. Studies of fluid and melt inclusions from intrusive and extrusive igneous rocks yield ample evidence that many magmas are vapor saturated as deep as the mid crust (10-15 km) and that CO^sub 2^ is an appreciable part of the exsolved vapor. Such is the case in both basaltic and some silicic magmas. Under most conditions, the presence of a CO^sub 2^-bearing vapor does not hinder, and in fact may promote, the ascent and eruption of the host magma. Carbonic fluids are poorly miscible with aqueous fluids, particularly at high temperature and low pressure, so that the presence of CO^sub 2^ can induce immiscibility both within the magmatic volatile phase and in hydrothermal systems. Because some metals, including gold, can be more volatile in vapor phases than coexisting liquids, the presence of CO^sub 2^ may indirectly aid the process of metallogenesis by inducing phase separation.[PUBLICATION ABSTRACT]</description><subject>Alkalinity</subject><subject>Basalt</subject><subject>Carbon</subject><subject>Carbon dioxide</subject><subject>Crystallization</subject><subject>Degassing</subject><subject>Dolomite</subject><subject>Gold</subject><subject>High temperature</subject><subject>Igneous rocks</subject><subject>Immiscibility</subject><subject>Lava</subject><subject>Magma</subject><subject>Oceanic 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review focuses on the solubility, origin, abundance, and degassing of carbon dioxide (CO^sub 2^) in magma-hydrothermal systems, with applications for those workers interested in intrusion-related deposits of gold and other metals. The solubility of CO^sub 2^ increases with pressure and magma alkalinity. Its solubility is low relative to that of H^sub 2^O, so that fluids exsolved deep in the crust tend to have high CO^sub 2^/H^sub 2^O compared with fluids evolved closer to the surface. Similarly, CO^sub 2^/H^sub 2^O will typically decrease during progressive decompression- or crystallization-induced degassing. The temperature dependence of solubility is a function of the speciation of CO^sub 2^, which dissolves in molecular form in rhyolites (retrograde temperature solubility), but exists as dissolved carbonate groups in basalts (prograde). Magnesite and dolomite are stable under a relatively wide range of mantle conditions, but melt just above the solidus, thereby contributing CO^sub 2^ to mantle magmas. Graphite, diamond, and a free CO^sub 2^-bearing fluid may be the primary carbon-bearing phases in other mantle source regions. Growing evidence suggests that most CO^sub 2^ is contributed to arc magmas via recycling of subducted oceanic crust and its overlying sediment blanket. Additional carbon can be added to magmas during magma-wallrock interactions in the crust. Studies of fluid and melt inclusions from intrusive and extrusive igneous rocks yield ample evidence that many magmas are vapor saturated as deep as the mid crust (10-15 km) and that CO^sub 2^ is an appreciable part of the exsolved vapor. Such is the case in both basaltic and some silicic magmas. Under most conditions, the presence of a CO^sub 2^-bearing vapor does not hinder, and in fact may promote, the ascent and eruption of the host magma. Carbonic fluids are poorly miscible with aqueous fluids, particularly at high temperature and low pressure, so that the presence of CO^sub 2^ can induce immiscibility both within the magmatic volatile phase and in hydrothermal systems. Because some metals, including gold, can be more volatile in vapor phases than coexisting liquids, the presence of CO^sub 2^ may indirectly aid the process of metallogenesis by inducing phase separation.[PUBLICATION ABSTRACT]</abstract><cop>Heidelberg</cop><pub>Springer Nature B.V</pub><doi>10.1007/s001260100185</doi><tpages>13</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Alkalinity Basalt Carbon Carbon dioxide Crystallization Degassing Dolomite Gold High temperature Igneous rocks Immiscibility Lava Magma Oceanic crust Solubility Speciation |
title | Carbon dioxide in magmas and implications for hydrothermal systems |
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