Cooling rates of porphyritic olivine chondrules in the Semarkona (LL3.00) ordinary chondrite: A model for diffusional equilibration of olivine during fractional crystallization

Meteoritics and Planetary Science

Volumn 44, Issue 4, 2009, Pages 521-530

  Miyamoto, M ^a   Mikouchi, T ^a   Jones, R H ^b  

^a UNIVERSITY OF TOKYO   (Japan)

^b UNIVERSITY OF NEW MEXICO   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 68149092035     PISSN: 10869379     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1945-5100.2009.tb00748.x     Document Type: Article

References (31)

1. Beattie P. 1993. Olivine melt and orthopyroxene melt equilibria. Contribution to Mineralogy and Petrology 115:102-111.
2. Brett R. and Sato M. 1984. Intrinsic oxygen fugacity measurements on seven chondrites, a pallasite, and a tektite and the redox state of meteorite parent bodies. Geochimica et Cosmochimica Acta 48:111-120.
3. Buening D. K. and Buseck P. R. 1973. Fe Mg lattice diffusion in olivine. Journal of Geophysical Research 78:6852-6862.
4. Chakraborty S. 1997. Rates and mechanisms of Fe Mg interdiffusion in olivine at 980 °C 1300 °C. Journal of Geophysical Research 102:12317-12331.
5. Connolly H. C. Jr., Desch S. J., Ash R. D., and Jones R. H. 2006. Transient heating events in the protoplanetary nebula. In Meteorites and the early solar system II, edited by Lauretta D. and McSween H. Y. Jr. Tucson: The University of Arizona Press. pp. 383 397.
6. Desch S. J. and Connolly H. C. Jr. 2002. A model of the thermal processing of particles in solar nebula shocks: Application to the cooling rates of chondrules. Meteoritics & Planetary Science 37: 183-183.
7. Elwell D. and Scheel H. J. 1975. Crystal growth from high temperature solutions. London: Academic Press Inc. 634 p.
8. Ghiorso M. and Sack R. 1995. Chemical mass transfer in magmatic processes IV. A revised and internally consistent thermodynamic model for the interpolation and extrapolation of liquid solid equilibria in magmatic systems at elevated temperatures and pressures. Contribution to Mineralogy and Petrology 119:197-212.
9. Grossman J. N. and Brearley A. J. 2005. The onset of metamorphism in ordinary and carbonaceous chondrites. Meteoritics & Planetary Science 40:87-122.
10. Hewins R. H. 1988. Experimental studies of chondrules. In Meteorites and the early solar system, edited by Kerridge J. F. and Matthews M. S. Tucson: The University of Arizona Press. pp. 660 679.
11. Hewins R. H., Connolly H. C. Jr., Lofgren G. E., and Libourel G. 2005. Experimental constraints on chondrule formation. In Chondrites and the protoplanetary disk, edited by Krot A. N., Scott E. R. D., and Reipurth B. ASP Conference Series, vol. 341. San Francisco: Astronomical Society of the Pacific. pp. 286 316.
12. Jones R. H. 1990. Petrology and mineralogy of Type II, FeO rich chondrules in Semarkona (LL3.0): Origin by closed system fractional crystallization with evidence for supercooling. Geochimica et Cosmochimica Acta 54:1785-1802.
13. Jones R. H. 1996. FeO rich, porphyritic pyroxene chondrules in unequilibrated ordinary chondrites. Geochimica et Cosmochimica Acta 60:3115-3138.
14. Jones R. H. and Lofgren G. E. 1993. A comparison of FeO rich, porphyritic olivine chondrules in unequilibrated chondrites and experimental analogues. Meteoritics 28:213-221.
15. Jurewicz A. J. G. and Watson E. B. 1988. Cations in olivine, Part 2: Diffusion in olivine xenocrysts, with applications to petrology and mineral physics. Contribution to Mineralogy and Petrology 99:186-201.
16. Lofgren G. E. 1996. A dynamic crystallization model for chondrule melts. In Chondrules and the protoplanetary disk, edited by Hewins R. H., Jones R. H., and Scott E. R. D. Cambridge: Cambridge University Press. pp. 187 196.
17. Misener D. J. 1974. Cationic diffusion in olivine to 1400 °C and 35 kbar. In Geochemical transport and kinetics, edited by Hofmann A. W., Giletti B. J., Yoder H. S. Jr., and Yund R. A. Carnegie Institute Washington Publication 634. pp. 117 129.
18. Miyamoto M. and Takeda H. 1994. Thermal history of lodranites Yamato 74357 and MAC 88177 as inferred from the chemical zoning of pyroxene and olivine. Journal of Geophysical Research 99:5669-5677.
19. Miyamoto M., McKay D. S., McKay G. A., and Duke M. B. 1986. Chemical zoning and homogenization of olivines in ordinary chondrites and implications for thermal histories of chondrules. Journal of Geophysical Research 91:12804-12816.
20. Miyamoto M., Mikouchi T., and Kaiden H. 1998. An analysis of iron magnesium zoning of olivine in a Semarkona (LL3.0) porphyritic olivine chondrule: Diffusional modification of primary zoning (abstract). Meteoritics & Planetary Science 33:A111 A112.
21. Miyamoto M., Mikouchi T., and Kaiden H. 1999. Diffusional modification of igneous zoning during crystal growth: analysis of Fe Mg zoning of olivine in Semarkona (LL3.0) porphyritic olivine chondrule (abstract #1323). 30th Lunar and Planetary Science Conference. CD ROM.
22. Miyamoto M., Mikouchi T., and Arai T. 2002. Comparison of Fe Mg interdiffusion coefficients in olivine. Antarctic Meteorite Research 15:143-151.
23. Miyamoto M., Koizumi E., and Mikouchi T. 2006. Verification of a model to calculate cooling rates in olivine by consideration of Fe Mg diffusion and olivine crystal growth II (abstract #1538). 37th Lunar and Planetary Science Conference. CD ROM.
24. 2+ interdiffusion in olivine (II). Physical Chemistry 88:140-145.
25. Nelder J. A. and Mead R. 1965. A simplex method for function minimization. Computer Journal 7:308-313.
26. Stolper E. 1977. Experimental petrology of eucritic meteorites. Geochimica et Cosmochimica Acta 41:587-611.
27. Tsuchiyama A., Nagahara H., and Kushiro I. 1980. Experimental reproduction of textures of chondrules. Earth and Planetaiy Science Letters 48:155-165.
28. Wasson J. T. 1993. Constraints on chondrule origins. Meteoritics 28:14-28.
29. Wasson J. T. 2004. Petrographic evidence for rapid heating and cooling during chondrule formation (abstract #9113). Workshop on Chondrules and the Protoplanetary Disk.
30. Wasson J. T. and Rubin A. E. 2003. Ubiquitous low FeO relict grains in type II chondrules and limited overgrowths on phenocrysts following the final melting event. Geochimica et Cosmochimica Acta 67:2239-2250.
31. Weinbruch S., Buttner H., Holzheid A., Rosenhauer M., and Hewins R. H. 1998. On the lower limit of chondrule cooling rate: The significance of iron loss in dynamic crystallization experiments. Meteoritics & Planetary Science 33:65-74.