IS LOW-SPIN FE2+ PRESENT IN EARTH'S MANTLE?
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dc.contributor.author | Hofmeister A.M. | |
dc.date.accessioned | 2024-09-14T06:08:13Z | |
dc.date.available | 2024-09-14T06:08:13Z | |
dc.date.issued | 2006 | |
dc.identifier | https://www.elibrary.ru/item.asp?id=28060546 | |
dc.identifier.citation | Earth and Planetary Science Letters, 2006, 243, 1-2, 44-52 | |
dc.identifier.issn | 0012-821X | |
dc.identifier.uri | https://repository.geologyscience.ru/handle/123456789/45118 | |
dc.description.abstract | Recently, X-ray spectroscopy indicated that the low-spin (LS) electronic configuration of Fe2+ and Fe3+ ions substituting in silicate perovskite of various compositions, and also in magnesiowüstite is stable at room temperature above pressures of ~49 to 120 GPa [J. Badro, G. Fiquet, F. Guyot, J.-P. Rueff, V.V. Struzhkin, G. Vanko, G. Monaco, Iron partitioning in Earth's mantle: toward a deep lower mantle discontinuity, Science 300 (2003), 789-791.; J. Badro, J.-P. Rueff, G. Vanko, G. Monaco, G. Figuet, F. Guyot, Electronic transition in perovskite: possible non-convecting layers in the lower mantle, Science 305 (2004) 383-386.; J. Li, V.V. Struzhkin, H.K. Mao, J. Shu, R.J. Hemley, Y. Fei, B. Mysen, P. Dera, V. Prakapenka, G. Shen, Electronic spin state of iron in lower mantle perovskite, Proc. Natl. Acad. Sci. 101 (2004) 14027-14030.; J.M. Jackson, W. Sturhahn, G. Shen, J. Zhao, M.Y. Hu, D. Errandonea, J.D. Bass, Y. Fei, A synchrotron Mössbauer study of (Mg, Fe)SiO3 perovskite up to 120 GPa, Am. Mineral. 90 (2005) 199-205.; J.F. Lin, V.V. Struzhkin, S.D. Jacobsen, M.Y. Hu, P. Chow, J. Kung, H. Liu, H.K. Mao, R.J. Hemley, Spin transition of iron in magnesiowüstite in the Earth's lower mantle, Nature 436 (2005) 377-380.]. Simple thermodynamic relationships combined with crystal field theory provide a minimum Clausius-Clapeyron slope of ~0.23 to 0.4 GPa/K for the high-spin (HS) to low-spin transition of Fe ions in perovskite, consistent with lower mantle temperatures stabilizing the disordered HS state. This computation of ∂P/∂T utilizes experimentally determined parameters only (P and T at the transition), and is supported by microstructural analysis of the change in volume and entropy considerations. Similarly, (∂P/∂T)min ~0.18 to 0.31 GPa/K for magnesiowüstite. High spin Fe2+ should be stable in silicates throughout Earth's mantle for compositions of Fe/(Mg + Fe) ~0.1, consistent with disorder prevailing at high temperature, although partial conversion of octahedral Fe3+ to LS may occur. Similarly, partial conversion of octahedral Fe2+ in magnesiowüstite to the LS is possible for Fe-rich compositions, which transform at relatively low pressures. © 2006 Elsevier B.V. All rights reserved. | |
dc.subject | CRYSTAL FIELD THEORY | |
dc.subject | FE | |
dc.subject | LOWER MANTLE | |
dc.subject | SPIN-PAIRING | |
dc.subject | THERMODYNAMICS | |
dc.title | IS LOW-SPIN FE2+ PRESENT IN EARTH'S MANTLE? | |
dc.type | Статья | |
dc.identifier.doi | 10.1016/j.epsl.2005.12.013 |
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