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Probing the chemical and mineralogical characteristics of the Martian meteorite NWA 7397 through μRaman and μXRF non-destructively

Published online by Cambridge University Press:  19 February 2018

Bruno Leonardo do Nascimento-Dias Open the ORCID record for Bruno Leonardo do Nascimento-Dias [Opens in a new window] ,
Douglas Galante Open the ORCID record for Douglas Galante [Opens in a new window] ,
Davi Oliveira  and
Marcelino Anjos
Bruno Leonardo do Nascimento-Dias*
Affiliation:
University of state of Rio of Janeiro, Rio de Janeiro, Brazil
Douglas Galante
Affiliation:
Brazilian Synchrotron Light Laboratory, Brazilian Center for Research in Energy and Materials, Campinas, Brazil
Davi Oliveira
Affiliation:
University of state of Rio of Janeiro, Rio de Janeiro, Brazil Federal University of Rio de Janeiro, Rio de Janeiro, Brazil
Marcelino Anjos
Affiliation:
University of state of Rio of Janeiro, Rio de Janeiro, Brazil Federal University of Rio de Janeiro, Rio de Janeiro, Brazil
*
Author for correspondence: Bruno Leonardo do Nascimento-Dias, E-mail: [email protected]
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Abstract

Martian meteorites have valuable information about past geological processes on Mars. In this particular case, the sample used was the Martian meteorite Northwest Africa (NWA) 7397. The main objective was to conduct preliminary analyses of the sample that was able to provide mineralogical characteristics in a non-destructive way. These meteorite NWA 7397 analyses were performed using two analytical techniques, μRaman and μXRF. Through the techniques used it was possible to suggest the presence of chromite, ilmenite, magnetite and forsterite minerals. These minerals seem to have a correspondence to one another in relation to the process that formed them. Thus, the information generated by these analytical techniques can contribute significantly by providing information on the history of Mars in order to have relevance to the areas of Astrobiology and Planetary Sciences.

Keywords

AstrobiologyMarsNWA 7397μRamanμXRF
Type
Research Article
Information
International Journal of Astrobiology , Volume 18 , Issue 1 , February 2019 , pp. 73 - 78
Copyright
Copyright © Cambridge University Press 2018 

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References

Bertin, EP (2012) Principles and Practice of X-Ray Spectrometric Analysis. Springer Science & Business Media.Google Scholar
Blumberg, BS (2003) The Nasa astrobiology institute: early history and organization. Astrobiology 3(3), 463–470.Google Scholar
BRUKER. M4 Tornado Bruker. Available at https://www.bruker.com/pt/products/x-ray-diffraction-and-elemental-analysis/micro-xrf-and-txrf/m4-tornado/technical-details.html (Accessed in October 2017).Google Scholar
Bucher, K and Frey, M (1994) Petrogenesis of Metamorphic Rocks, 6th edn., Berlin: Springer-Verlag, [S.l.] 318 p.Google Scholar
Deer, WA, Howie, RA and Zussman, J (1992) An Introduction to the Rock-Forming Minerals. Hong Kong: Longman Scientific & Technical.Google Scholar
Gladman, B (1997) Destination: Earth. Martian meteorite delivery. Icarus 130, 228–246.Google Scholar
Gladman, BJ, Burns, JA, Duncan, M, Lee, P and Levison, HF (1996) The exchange of impact ejecta between terrestrial planets. Science 271, 1378–1392.Google Scholar
Goodrich, CA (2002) Olivine-phyric Martian basalts: a new type of shergottite. Meteoritics & Planetary Science 37 (Suppl): B31–B34Google Scholar
Howarth, GH, Pernet-Fisher, JF, Balta, JB, Barry, PH, Bodnar, RJ and Taylor, LA (2014) Two-stage polybaric formation of the new enriched, pyroxene-oikocrystic, lherzoliticshergottite, NWA 7397. Meteoritics& Planetary Science 49(10), 1812–1830.Google Scholar
Hutchinson, IB, Parnell, P, Edwards, HGM, Jehlicka, J, Marshall, CP, Harris, LV and Ingley, R (2014) Potential for analysis of carbonaceous matter on Mars using Raman spectroscopy. Planetary and Space Science 103, 184–190.Google Scholar
Irving, A and Kuehner, S (2013) Northwest Africa 7397. The Meteoritical Society. Available at http://www.lpi.usra.edu/meteor/metbull.php?code=55749 (Accessed October 2017).Google Scholar
Mccubbin, FM and Jones, RH (2015) Extraterrestrial apatite: planetary geochemistry to astrobiology. Elements 11(3), 183–188.Google Scholar
Meteoritical Bullitin. Iniciative: The Meteoritical Society. Available at http://www.lpi.usra.edu/meteor/metbull.php (Accessed 21 de August de 2017).Google Scholar
Nascimento-Dias, BL, Oliveira, DF and Anjos, MJ (2017) The utilization and multidisciplinary relevance of X-ray spectroscopy. Revista Brasileira de Ensino de Física 39(4).Google Scholar
Nascimento-Dias, BL, Oliveira, DF, Machado, AS, Araújo, OM, Lopes, RT and Anjos, MJ (2018) Utilization of nondestructive techniques for analysis of the Martian meteorite NWA 6963 and its implications for astrobiology. X-Ray Spectrometry 47(1), 86–91.Google Scholar
Nasdala, L, Smith, DC, Kaindl, R and Ziemann, MA (2004) Raman spectroscopy: analytical perspectives in mineralogical research. Spectroscopic Methods in Mineralogy 6, 281–343.Google Scholar
Reynard, B, Rubie, D and Mineral, A (2017) Handbook of Minerals Raman Spectra of Lyon University. Iniciative: University of Lyon. Available at http://www.geologie-lyon.fr/Raman/ (Accessed October de 2017).Google Scholar
RRUFF Project website. Available at http://rruff.info/ (Accessed September de 2017).Google Scholar
Spear, FS (1995) Metamorphic Phase Equilibria and Pressure-Temperature-Time Paths. Washington: Mineralogical Society of America, [S.l.] 799p.Google Scholar
Szabó, GAJ, Babinski, M and Teixeira, W (2010) Rochas ígneas. In Teixeira, W, Toledo, MCM, Fairchild, TR, Taioli, F (eds). Decifrando A Terra, 2nd edn. São Paulo: IBEP [S.l], pp. 327–346.Google Scholar
Wang, A, Kuebler, KE, Jolliff, BL and Haskin, LA (2004) Raman spectroscopy of Fe-Ti-Cr-oxides, case study: Martian meteorite EETA79001. American Mineralogist 89(5–6), 665–680.Google Scholar