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Volumn 281, Issue 5373, 1998, Pages 85-87

Effects of water on the α-β transformation kinetics in San Carlos Olivine

Author keywords

[No Author keywords available]

Indexed keywords

GRAPHITE; MAGNESIUM HYDROXIDE; MINERAL; PLATINUM; SODIUM CHLORIDE; WATER;

EID: 0032479525     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.281.5373.85     Document Type: Article
Times cited : (108)

References (19)
  • 2
    • 0001739226 scopus 로고
    • For example, S Karato, M. S. Paterson, J. D. FitzGerald, J. Geophys. Res. 91, 8151 (1986); D. T. Griggs and J. D. Blacic, Science 147, 292 (1965).
    • (1965) Science , vol.147 , pp. 292
    • Griggs, D.T.1    Blacic, J.D.2
  • 5
    • 0028486376 scopus 로고
    • 4 [H. Morishima et al., Science 265, 1202 (1994)] at 1030°C. It is possible that pressures are higher when NaCl is used around the sample than in a normal multianvil calibration experiment at similar oil pressures because of the high coefficient of thermal expansion of NaCl.
    • (1994) Science , vol.265 , pp. 1202
    • Morishima, H.1
  • 8
    • 14444286075 scopus 로고    scopus 로고
    • note
    • The measured temperature is lower than that at the center of the heater by about 30°C at 1000°C based on measurements with two thermocouples. Therefore, we corrected the measured temperature of the sample by taking into account the effect of the temperature gradient in the furnace. The effect of pressure on the emf of the thermocouple was ignored in the present experiments.
  • 9
    • 14444277096 scopus 로고    scopus 로고
    • note
    • Microstructures of the recovered samples and crystal-lographic orientation relations between the reactant and product phases were examined with a 200-kV JEOL-2010 TEM.
  • 10
    • 14444273969 scopus 로고    scopus 로고
    • note
    • Electron microprobe analysis of the recovered samples revealed that small, iron-rich grains (less than 10 μm) with olivine stoichiometry exist within the reaction rim especially near the surface. The Mg/(Mg + Fe) ratios in these iron-rich grains range from about 81 to 85. This suggests that the iron-rich grains are ringwoodite, and the transformation occurred in the coexisting field of wadsleyite and ringwoodite at lower temperature before the desired value was reached.
  • 11
    • 0010245618 scopus 로고
    • F. Guyot, G. D. Gwamnesia, R. C. Liebermann, Geophys. Res. Lett. 18, 89 (1991); A. J. Brearley, D. C. Rubie, E. Ito, Phys. Chem. Miner. 18, 343 (1992); K. Fujino and T. Irifune, in High Pressure Research: Application to Earth and Planetary Sciences, Y. Syono and M. H. Manghnani, Eds. (American Geophysical Union, Washington, DC, 1992), pp. 237-244; A. J. Brearley and D. C. Rubie, Phys. Earth Planet. Int. 86, 45 (1994).
    • (1991) Geophys. Res. Lett. , vol.18 , pp. 89
    • Guyot, F.1    Gwamnesia, G.D.2    Liebermann, R.C.3
  • 12
    • 0000505156 scopus 로고
    • F. Guyot, G. D. Gwamnesia, R. C. Liebermann, Geophys. Res. Lett. 18, 89 (1991); A. J. Brearley, D. C. Rubie, E. Ito, Phys. Chem. Miner. 18, 343 (1992); K. Fujino and T. Irifune, in High Pressure Research: Application to Earth and Planetary Sciences, Y. Syono and M. H. Manghnani, Eds. (American Geophysical Union, Washington, DC, 1992), pp. 237-244; A. J. Brearley and D. C. Rubie, Phys. Earth Planet. Int. 86, 45 (1994).
    • (1992) Phys. Chem. Miner. , vol.18 , pp. 343
    • Brearley, A.J.1    Rubie, D.C.2    Ito, E.3
  • 13
    • 0010245618 scopus 로고
    • Y. Syono and M. H. Manghnani, Eds. American Geophysical Union, Washington, DC
    • F. Guyot, G. D. Gwamnesia, R. C. Liebermann, Geophys. Res. Lett. 18, 89 (1991); A. J. Brearley, D. C. Rubie, E. Ito, Phys. Chem. Miner. 18, 343 (1992); K. Fujino and T. Irifune, in High Pressure Research: Application to Earth and Planetary Sciences, Y. Syono and M. H. Manghnani, Eds. (American Geophysical Union, Washington, DC, 1992), pp. 237-244; A. J. Brearley and D. C. Rubie, Phys. Earth Planet. Int. 86, 45 (1994).
    • (1992) High Pressure Research: Application to Earth and Planetary Sciences , pp. 237-244
    • Fujino, K.1    Irifune, T.2
  • 14
    • 0028558087 scopus 로고
    • F. Guyot, G. D. Gwamnesia, R. C. Liebermann, Geophys. Res. Lett. 18, 89 (1991); A. J. Brearley, D. C. Rubie, E. Ito, Phys. Chem. Miner. 18, 343 (1992); K. Fujino and T. Irifune, in High Pressure Research: Application to Earth and Planetary Sciences, Y. Syono and M. H. Manghnani, Eds. (American Geophysical Union, Washington, DC, 1992), pp. 237-244; A. J. Brearley and D. C. Rubie, Phys. Earth Planet. Int. 86, 45 (1994).
    • (1994) Phys. Earth Planet. Int. , vol.86 , pp. 45
    • Brearley, A.J.1    Rubie, D.C.2
  • 15
    • 0019910802 scopus 로고
    • FTIR measurements were carried out in air. Thickness of the sample was 80 to 140 μm, and aperture size ranged from 50 μm by 50 μm to 500 μm by 500 μm. Water content of wadsteyite was estimated from the integration of the infrared spectra using the calibration by Paterson [M. S. Paterson, Bull. Mineral. 105, 20 (1982)].
    • (1982) Bull. Mineral. , vol.105 , pp. 20
    • Paterson, M.S.1
  • 17
    • 14444286313 scopus 로고    scopus 로고
    • M. Liu, L. Kerschhofer, and D. C. Rubie [Eos (Fall suppl.) 77, 716 (1996)] considered the effect of the strain energy associated with first-order transformation on the growth rate.
    • (1996) Eos (Fall Suppl.) , vol.77 , pp. 716
    • Liu, M.1    Kerschhofer, L.2    Rubie, D.C.3
  • 19
    • 14444273739 scopus 로고    scopus 로고
    • note
    • We thank D. C. Rubie, S. Karato, and J. P. Poirier for suggestions; H. Keppler, T. Terada, and M. Akizuki for the FTIR measurements; and T. Nagase and N. Miyajima for the TEM observation. This work was supported in part by a Grant-in-Aid for Scientific Research (A) (09304051) from the Japanese Ministry of Education, Science, Sports, and Culture (to E.O.).


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.