Analysis of the ordinary chondrite of Dalgety Downs (L4): Mineralogy, geochemistry and Raman spectroscopy

Authors

  • Andrés Caño Blanes Departamento de Cristalografía y Mineralogía. Facultad de Ciencias Geológicas, UCM, Madrid
  • Rosario Lunar Hernández Departamento de Cristalografía y Mineralogía. Facultad de Ciencias Geológicas, UCM, Madrid; Instituto de Geociencias IGEO (CSIC, UCM), Madrid
  • Valentín García Baonza Instituto de Geociencias IGEO (CSIC, UCM), Madrid; Departamento de Física Química I, Facultad de Ciencias Químicas, UCM, Madrid
  • Jesús Martínez-Frías Instituto de Geociencias IGEO (CSIC, UCM), Madrid

DOI:

https://doi.org/10.55407/geogaceta102470

Keywords:

ordinary chondrites, chondrules, matrix, Raman spectroscopy

Abstract

The Dalgety Downs meteorite, found in the Western Australian Desert, is a poorly studied ordinary chondrite, that however contains valuable information about the Solar System primitive matter evolution and the processes that affect it. This specimen exhibits textural, mineralogical and geochemical characteristics in matrix and chondrules that reveal metamorphic processes of intermediate temperatures and moderate impact events, in addition to an intense alteration developed during its entry into the terrestrial atmosphere and later exposure to climate, in what is defined as the fusion crust. Among the methods employed in this study, Raman spectroscopy highlights as a mineralogical identification tool, a technique of high precision in the analysis of geological materials and that is expected to be used in upcoming space missions.

References

Bischoff, A. (2001a). Earth, Moon and Planets 85-86, 87-97. https://doi.org/10.1023/A:1017047311070

Bischoff, A. (2001b). Planetary and Space Science 49, 769-776. https://doi.org/10.1016/S0032-0633(01)00026-5

Bland, P. A., Zolensky, M. E., Benedix, G. K., y Sephton, M. A. (2006). Meteorites and the early solar system II, 853-867. https://doi.org/10.2307/j.ctv1v7zdmm.45

Easton, A. J., y Elliott, C. J. (1977). Meteoritics 12, 409-416. https://doi.org/10.1111/j.1945-5100.1977.tb00459.x

Englert, P. y Herr, W. (1978). Meteoritics 13, 454.

Herzog, G.F. y Cressy Jr, P.J. (1976). Meteoritics 11, 59-68. https://doi.org/10.1111/j.1945-5100.1976.tb00315.x

Herzog, G.F., Xue, S., Cloudt, S., Jull, A.J.T., Middleton, R. y Klein, J. (1995). Meteoritics 30(5), 518-519.

McSween, H.Y.Jr. (1999). Meteorites and their Parent Planets. Cambridge University Press, Cambridge, 310 p.

Miyamoto, M. y Ohsumi, K. (1995). Geophysical research letters 22(4), 437-440. https://doi.org/10.1029/94GL03281

Muñoz-Espadas, M.J. (2003). Mineralogía, texturas y cosmoquímica de cóndrulos en condritas H4, H5, L5 y LL5. Tesis doctoral, Universidad Complutense de Madrid, 324 p.

Stöffler, D., Keil, K. y Scott, E.R.D. (1991). Geochimica et Cosmochimica Acta 55, 3845-3867. https://doi.org/10.1016/0016-7037(91)90078-J

Van Schmus, W.R. y Wood, J.A. (1967). Geochimica et Cosmochimica Acta 31, 747-765. https://doi.org/10.1016/S0016-7037(67)80030-9

Wlotzka, F. (1993). Meteoritics 28, 460-460. https://doi.org/10.1111/j.1945-5100.1993.tb00262.x

Published

2021-06-12

How to Cite

Caño Blanes, A., Lunar Hernández, R., García Baonza, V., & Martínez-Frías, J. (2021). Analysis of the ordinary chondrite of Dalgety Downs (L4): Mineralogy, geochemistry and Raman spectroscopy . GEOGACETA, 69, 87–90. https://doi.org/10.55407/geogaceta102470

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