This paper reports new FTIR data on the H2O and CO2 concentrations in glasses of 26 naturally quenched and experimentally partially homogenized melt inclusions in olivine (Fo(85-91)) phenocrysts from rocks of the Kliuchevskoi volcano. Measured H2O concentrations in the inclusions range from 0.02 to 4 wt.%. The wide variations in the H2O content of the inclusions, which do not correlate with the host olivine composition and contents of major elements in the melts, are explained by the H2O escape from inclusions via diffusion through the host olivine during the magma eruption and the following cooling. The largest H2O loss is characteristic of inclusions from lava samples which cooled slowly after eruption. The minimal H2O loss is observed for inclusions from rapidly quenched pyroclastic rocks. Parental magmas of the Kliuchevskoi volcano are estimated to contain 3.5 wt.% H2O. The new data imply a 40 degrees C lower mantle temperatures than that estimated earlier for the Kliuchevskoi primary melts. The concentrations of CO2 in glasses range from <0.01 to 0.13 wt.% and do not correlate with the type of studied inclusions and their composition. The calculated pressures of melt equilibria with H2O-CO2 fluid inside the inclusions are lower than 270 MPa. They are significantly lower than a pressure of 500 MPa calculated from the density (similar to 0.8 g/cm(3)) of cogenetic fluid inclusions in high-Fo olivine. The significant pressure drop inside the melt inclusions after their trapping in olivine might be due to the H2O loss and redistribution of CO2 from melt to daughter fluid phase. Compared with melt inclusions, cogenetic fluid inclusions provide independent information about the crystallization pressures of olivine and initial CO2 content in the Kliuchevskoi magma, which were estimated to be at least 500 MPa and 0.35 wt.%, respectively. The maximum CO2 concentrations in the primary Kliuchevskoi melts are estimated at 0.8-0.9 wt.%. The decompression crystallization of the Kliuchevskoi magmas starts at depths of 30-40 km and proceeds with a continuous decrease in CO2 content and an increase (up to 6-7 wt.%) and then a decrease (at <300 MPa) in H2O content in melts, which explains the origin of the whole spectrum of rocks and melt inclusions of the Kliuchevskoi volcano. (C) 2011, V.S. Sobolev IGM, Siberian Branch of the RAS. Published by Elsevier B.V. All rights reserved.
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Univ Calif Santa Barbara, Global Ctr Mantle Zool GCMZ, Dept Earth Sci, Isotope Geochem Facil, Santa Barbara, CA 93106 USAUniv Calif Santa Barbara, Global Ctr Mantle Zool GCMZ, Dept Earth Sci, Isotope Geochem Facil, Santa Barbara, CA 93106 USA
Anderson, Olivia E.
Jackson, Matthew G.
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Univ Calif Santa Barbara, Global Ctr Mantle Zool GCMZ, Dept Earth Sci, Isotope Geochem Facil, Santa Barbara, CA 93106 USAUniv Calif Santa Barbara, Global Ctr Mantle Zool GCMZ, Dept Earth Sci, Isotope Geochem Facil, Santa Barbara, CA 93106 USA
Jackson, Matthew G.
Pamukcu, Ayla S.
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Woods Hole Oceanog Inst, Woods Hole, MA 02543 USA
Stanford Univ, Geol Sci, Stanford, CA USAUniv Calif Santa Barbara, Global Ctr Mantle Zool GCMZ, Dept Earth Sci, Isotope Geochem Facil, Santa Barbara, CA 93106 USA
Pamukcu, Ayla S.
Rose-Koga, Estelle F.
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Inst Sci Terre Orleans ISTO, UO CNRS BRGM, INSU, 1A Rue Ferollerie, F-45071 Orleans, FranceUniv Calif Santa Barbara, Global Ctr Mantle Zool GCMZ, Dept Earth Sci, Isotope Geochem Facil, Santa Barbara, CA 93106 USA
Rose-Koga, Estelle F.
Le Roux, Veronique
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Woods Hole Oceanog Inst, Woods Hole, MA 02543 USA
Ctr Rech Petrog & Geochim, Nancy, FranceUniv Calif Santa Barbara, Global Ctr Mantle Zool GCMZ, Dept Earth Sci, Isotope Geochem Facil, Santa Barbara, CA 93106 USA
Le Roux, Veronique
Klein, Frieder
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Woods Hole Oceanog Inst, Woods Hole, MA 02543 USAUniv Calif Santa Barbara, Global Ctr Mantle Zool GCMZ, Dept Earth Sci, Isotope Geochem Facil, Santa Barbara, CA 93106 USA
Klein, Frieder
Koga, Kenneth T.
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Inst Sci Terre Orleans ISTO, UO CNRS BRGM, INSU, 1A Rue Ferollerie, F-45071 Orleans, FranceUniv Calif Santa Barbara, Global Ctr Mantle Zool GCMZ, Dept Earth Sci, Isotope Geochem Facil, Santa Barbara, CA 93106 USA
Koga, Kenneth T.
Gaetani, Glenn A.
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Inst Sci Terre Orleans ISTO, UO CNRS BRGM, INSU, 1A Rue Ferollerie, F-45071 Orleans, FranceUniv Calif Santa Barbara, Global Ctr Mantle Zool GCMZ, Dept Earth Sci, Isotope Geochem Facil, Santa Barbara, CA 93106 USA
Gaetani, Glenn A.
Price, Allison A.
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Univ Calif Santa Barbara, Global Ctr Mantle Zool GCMZ, Dept Earth Sci, Isotope Geochem Facil, Santa Barbara, CA 93106 USAUniv Calif Santa Barbara, Global Ctr Mantle Zool GCMZ, Dept Earth Sci, Isotope Geochem Facil, Santa Barbara, CA 93106 USA
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Nanjing Univ Sci & Technol, Sch Energy & Power Engn Nanjing, Nanjing 210094, Peoples R ChinaNanjing Univ Sci & Technol, Sch Energy & Power Engn Nanjing, Nanjing 210094, Peoples R China
Chen Longfei
Liu Dong
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Nanjing Univ Sci & Technol, Sch Energy & Power Engn Nanjing, Nanjing 210094, Peoples R ChinaNanjing Univ Sci & Technol, Sch Energy & Power Engn Nanjing, Nanjing 210094, Peoples R China
Liu Dong
Li Qiang
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Nanjing Univ Sci & Technol, Sch Energy & Power Engn Nanjing, Nanjing 210094, Peoples R ChinaNanjing Univ Sci & Technol, Sch Energy & Power Engn Nanjing, Nanjing 210094, Peoples R China
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Xi An Jiao Tong Univ, State Key Lab Multiphase Flow Power Engn, Xian 710049, Shaanxi, Peoples R ChinaXi An Jiao Tong Univ, State Key Lab Multiphase Flow Power Engn, Xian 710049, Shaanxi, Peoples R China
Li, Guoxing
Wang, Hexuan
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Xi An Jiao Tong Univ, State Key Lab Multiphase Flow Power Engn, Xian 710049, Shaanxi, Peoples R ChinaXi An Jiao Tong Univ, State Key Lab Multiphase Flow Power Engn, Xian 710049, Shaanxi, Peoples R China
Wang, Hexuan
Lu, Youjun
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Xi An Jiao Tong Univ, State Key Lab Multiphase Flow Power Engn, Xian 710049, Shaanxi, Peoples R ChinaXi An Jiao Tong Univ, State Key Lab Multiphase Flow Power Engn, Xian 710049, Shaanxi, Peoples R China