Anisotropic copper diffusion in olivine: Implications for Cu preservation in olivine and olivine-hosted melt inclusions
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作者:
Zhang, Li
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Univ Sci & Technol China, Sch Earth & Space Sci, CAS Key Lab Crust Mantle Mat & Environm, Hefei 230026, Peoples R China
CAS Ctr Excellence Comparat Planetol, Hefei, Peoples R ChinaUniv Sci & Technol China, Sch Earth & Space Sci, CAS Key Lab Crust Mantle Mat & Environm, Hefei 230026, Peoples R China
Zhang, Li
[1
,2
]
Wang, Fangyue
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Hefei Univ Technol, Sch Resources & Environm Engn, Hefei 230009, Peoples R ChinaUniv Sci & Technol China, Sch Earth & Space Sci, CAS Key Lab Crust Mantle Mat & Environm, Hefei 230026, Peoples R China
Wang, Fangyue
[3
]
Ni, Huaiwei
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机构:
Univ Sci & Technol China, Sch Earth & Space Sci, CAS Key Lab Crust Mantle Mat & Environm, Hefei 230026, Peoples R China
CAS Ctr Excellence Comparat Planetol, Hefei, Peoples R ChinaUniv Sci & Technol China, Sch Earth & Space Sci, CAS Key Lab Crust Mantle Mat & Environm, Hefei 230026, Peoples R China
Ni, Huaiwei
[1
,2
]
机构:
[1] Univ Sci & Technol China, Sch Earth & Space Sci, CAS Key Lab Crust Mantle Mat & Environm, Hefei 230026, Peoples R China
[2] CAS Ctr Excellence Comparat Planetol, Hefei, Peoples R China
[3] Hefei Univ Technol, Sch Resources & Environm Engn, Hefei 230009, Peoples R China
The rate of copper diffusion in olivine governs the preservation of copper in olivine and olivine-hosted melt inclusions, but Cu diffusivity in olivine has not been well determined especially regarding its anisotropy. In this study, Cu diffusion in single crystal olivine (Fo(91)Fa(09)) cuboid, prepared to comply with the three principle crystallographic axes, was investigated at 1273-1673 K and 1-2.5 GPa in a piston cylinder apparatus, using a diffusion-in approach with Cu or Cu2O as the source. Copper concentration profiles were analyzed by LA-ICP-MS scanning on the recovered samples along multiple directions. We found Cu diffusion in olivine to be appreciably anisotropic, with Cu diffusivity along the c axis being greater than that along the a axis by nearly an order of magnitude (D-c approximate to 3D(b) approximate to 7.5 D-a). The activation energy for Cu diffusion is similar to 210 kJ/mol, with little dependence on crystallographic orientation. Cu diffusivity at 2.5 GPa is only slightly lower than that at 1 GPa, yielding a small activation volume of 2.3 cm(3)/mol. While not being as rapid as the migration of H and interstitial Li, Cu diffusion, especially along the c axis, is significantly faster than the major elements of olivine (Fe-Mg, Si and O). Diffusion modeling indicates that the timescale for re-equilibration of Cu between olivine-hosted melt inclusion and external melt is relatively short (<60 yr at 1000 degrees C and <3000 yr at 800 degrees C) compared to the typical lifetime of magma chambers. Cu concentrations in olivine-hosted melt inclusions may therefore have been significantly modified from the pristine values. For Cu profiles preserved in olivine phenocryst, our determined Cu diffusivity can be used to constrain its residence time in magma chamber, and the diffusion anisotropy can provide a cross-check. (C) 2023 Elsevier Ltd. All rights reserved.
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CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USACALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
Newcombe, M. E.
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Fabbrizio, A.
Zhang, Youxue
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Univ Michigan, Dept Earth & Environm Sci, Ann Arbor, MI 48109 USACALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
Zhang, Youxue
Ma, C.
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CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USACALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
Ma, C.
Le Voyer, M.
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CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
Carnegie Inst Sci, Dept Terr Magnetism, Washington, DC 20015 USACALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
Le Voyer, M.
Guan, Y.
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CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USACALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
Guan, Y.
Eiler, J. M.
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CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USACALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
Eiler, J. M.
Saal, A. E.
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Brown Univ, Dept Geol Sci, Providence, RI 02912 USACALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
Saal, A. E.
Stolper, E. M.
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CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USACALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
机构:
Columbia Univ, Lamont Doherty Earth Observ, POB 1000,61 Route 9W, Palisades, NY 10964 USA
Smithsonian Inst, Natl Museum Nat Hist, MRC 119 NHB,10th & Constitut Ave, Washington, DC 20560 USAColumbia Univ, Lamont Doherty Earth Observ, POB 1000,61 Route 9W, Palisades, NY 10964 USA
Rasmussen, Daniel J.
Plank, Terry A.
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Columbia Univ, Lamont Doherty Earth Observ, POB 1000,61 Route 9W, Palisades, NY 10964 USAColumbia Univ, Lamont Doherty Earth Observ, POB 1000,61 Route 9W, Palisades, NY 10964 USA
Plank, Terry A.
Wallace, Paul J.
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Univ Oregon, Dept Earth Sci, 220 Cascade Hall, Eugene, OR 97403 USAColumbia Univ, Lamont Doherty Earth Observ, POB 1000,61 Route 9W, Palisades, NY 10964 USA
Wallace, Paul J.
Newcombe, Megan E.
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Univ Maryland, Dept Geol, 8000 Regents Dr, College Pk, MD 20742 USAColumbia Univ, Lamont Doherty Earth Observ, POB 1000,61 Route 9W, Palisades, NY 10964 USA
Newcombe, Megan E.
Lowenstern, Jacob B.
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US Geol Survey, 1300 SE Cardinal Court,Suite 100, Vancouver, DC 98683 USAColumbia Univ, Lamont Doherty Earth Observ, POB 1000,61 Route 9W, Palisades, NY 10964 USA