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Carbonatite Melts and Electrical Conductivity in the Asthenosphere
Author(s)
Language
English
Obiettivo Specifico
3.3. Geodinamica e struttura dell'interno della Terra
Status
Published
JCR Journal
JCR Journal
Peer review journal
Yes
Title of the book
Issue/vol(year)
/322 (2008)
Publisher
AAAS
Pages (printed)
1363-1365
Issued date
November 2008
Keywords
Abstract
Electrically conductive regions in the Earth mantle have been interpreted to reflect the
presence of either silicate melt or water dissolved in olivine. On the basis of laboratory measurements we show that molten carbonates have electrical conductivities that are 3 orders of magnitude higher than those of molten silicate and 5 orders of magnitude higher than those of hydrated olivine. High conductivities in the asthenosphere probably indicate the presence of small amounts of carbonate melt in peridotite and can therefore be interpreted in terms of carbon concentration in the upper mantle. We show that the conductivity of the Oceanic asthenosphere can be explained by 0.1 volume % of carbonatite melts on average, which agrees with the CO2 content of Mid Ocean Ridge Basalts.
presence of either silicate melt or water dissolved in olivine. On the basis of laboratory measurements we show that molten carbonates have electrical conductivities that are 3 orders of magnitude higher than those of molten silicate and 5 orders of magnitude higher than those of hydrated olivine. High conductivities in the asthenosphere probably indicate the presence of small amounts of carbonate melt in peridotite and can therefore be interpreted in terms of carbon concentration in the upper mantle. We show that the conductivity of the Oceanic asthenosphere can be explained by 0.1 volume % of carbonatite melts on average, which agrees with the CO2 content of Mid Ocean Ridge Basalts.
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3. A.G. Jones, Lithos 48, 57-80 (1999).
4. R.L. Evans et al., Nature 437, 249-252 (2005).
5. K. Baba et al., J. Geophys. Res. 111, B02101 (2006).
6. F. Gaillard, G.I. Marziano, J. Geophys. Res. 110, B06204 (2006).
7. J. A. Tyburczy, H. S. Waff, J. Geophys. Res. 88, 2413–2430 (1983).
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Geochemistry, H. Keppler, J.R. Smyth, Eds. (MSA, 2006), vol. 62, chap.15.
9. F. Gaillard, Earth Planet. Sci. Lett. 218, 215–228, (2004).
10. A. Pommier, F. Gaillard, M. Pichavant, B. Scaillet, J. Geophys. Res. 113, B05205, (2008).
11. C. Aubaud, E. H. Hauri, M. M. Hirschmann, Geophys. Res. Lett. 31, L20611 (2004)
12. P. Tarits, S. Hautot, F. Perrier, Geophys. Res. Lett. 31, L06612 (2004).
13. S. Demouchy, S.D. Jacobsen, F. Gaillard, C.R. Stern, Geology 34, 429-432 (2006).
14. D.J. Wang, M. Mookherjee, Y.S. Xu, S-I. Karato, Nature 443, 977-980 (2006).
15. T. Yoshino, T. Matsuzaki, S. Yamashita, T. Katsura, Nature 443, 973-976 (2006).
16. A.E. Saal , E.H. Hauri , C.H. Langmuir, M.R. Perfit, Nature 419, 451-455 (2002).
17. P. Cartigny, F. Pineau, C. Aubaud, M. Javoy, Earth Planet. Sci. Lett. 265, 672-685 (2008)
18. B. Marty, I.N. Tolstikhin, Chem. Geol. 145, 233-248 (1998).
19. R. Dasgupta, M. M. Hirschmann, N.D. Smith, Geology 35, 135-138 (2007).
20. R. Dasgupta, M.M. Hirschmann, Nature 440, 659-661 (2006).
21. D.J. Frost, C. A. McCammon, An. Rev. Earth Planet. Sci. 36, 389-420 (2008).
22. S.S. Shcheka, M. Wiedenbeck, D.J. Frost, H. Keppler, Earth Planet. Sci. Lett. 245, 730-742
(2006).
23. W.G. Minarik, E.B. Watson, Earth Planet. Sci. Lett. 133, 423-437 (1995).
24. T. Hammouda, D. Laporte, Geology 28, 283–285 (2000).
25. T. Kojima, Y. Miyazaki, K. Nomura, K. Tanimoto, J. Electrochem. Soc. 155, F150-F156 (2008).
26. R. J. Sweeney, Earth Planet. Sci. Lett. 128, 259-270 (1994).
27. C. Simonnet, J. Phalippou, M. Malki, A. Grandjean, Rev. Sci. Inst. 74, 2085-2091 (2003).
28. D.P. Dobson et al., Earth Planet. Sci. Lett. 143, 207-215 (1996).
29. M. J. Genge, G.D. Price, A.P. Jones, Earth Planet. Sci. Lett. 131, 225-238 (1995).
30. Q. Liu, R.A. Lange, Contrib. Mineral. Petrol. 146, 370-381 (2003).
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