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Northwest Africa 7915: A New approved LL5 chondrite from Morocco

Treść / Zawartość
Identyfikatory
Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
A 415 g single meteorite was purchased in 2010 by T. Jakubowski from a dealer in Morocco. The meteorite was isometric in shape, ca. 8 cm in size, with distinct regmaglypts on the original ablated surface, and covered mostly in primary crust with one broken surface. The weight of the sample studied was 69 g. The meteorite is composed of several types of chondrules including porphyritic-Ol-Px, barred-Ol, radial-Px, granular and cryptocrystalline with distinct and diffused (not sharp) boundaries, and opaque grains and aggregates, enclosed in a very fine-grained matrix. The average compositions of minerals are: olivine (both in chondrules and matrix) − Fo70.4Fa29.1Te0.5, pyroxenes, represented by Mg-Fe (Ca-poor) orthopyroxene (and minor clinopyroxene?) − En73.9Fs24.1Wo2.0, feldspars (small in the matrix and in barred chondrules), with An12-37, and Or~3-4, taenite − Fe 70.80, Ni 25.50 and Co 1.67 wt. %, troilite − Fe0.98S1.00, chromite (Fe2+ 0.96Mg0.12Mn0.01Zn0.01) (Cr1.52Al0.23Fe3+ 0.02Ti0.10Si0.02)O4; altered accessory minerals including apatite and iron-rich secondary phases have also been identified and analyzed. The meteorite is of petrologic type 5, as evidenced by the observed recrystallization of the matrix, relatively good preservation of the chondrule structures, homogeneous composition of olivine and pyroxene, and the presence of only secondary small feldspar grains. The shock stage, S2, is based on the presence of undulatory extinction and irregular fractures in olivine crystals. The weathering grade, W3, is confirmed by the observation that kamacite is totally altered into secondary iron phases, whereas Nirich taenite, and troilite are only partly weathered. The specimen shows many bulk- and mineral-chemical parameters corresponding, mostly, to the LL chondrite group (e.g., Fe/SiO2 0.49, SiO2/MgO 1.62, Fa in olivine 29.05). However, concentrations of several other elements, including REE, are not fully consistent with the average values for the LL ordinary chondrites. Apparently, the parent body of the studied NWA 7915 meteorite was depleted in Dy, Tm, and Yb, compared to typical LL-type ordinary chondrite parent bodies. Also, relatively high concentrations of other elements, including Ba and Sr, have been measured, which may result from terrestrial weathering in hot desert conditions. The meteorite has been classified as LL5 ordinary chondrite, S2, W3, and registered in the Meteoritical Society database as NWA 7915. The type specimen is deposited in the Mineralogical Museum of the University of Wrocław.
Czasopismo
Rocznik
Strony
45--58
Opis fizyczny
Bibliogr. 23 poz., rys., tab.
Twórcy
autor
  • University of Wrocław, Institute of Geological Sciences, ul. Cybulskiego 30, 50-205 Wrocław, Poland
autor
  • University of Wrocław, Institute of Geological Sciences, ul. Cybulskiego 30, 50-205 Wrocław, Poland
  • ul. Drzewieckiego 44/7, 54-129 Wrocław, Poland
  • Wrocław University of Technology, Faculty of Geoengineering, Mining and Geology, Division of Geology and Mineral Waters, Wybrzeże S. Wyspiańskiego 27, 50-370 Wrocław, Poland
  • University of Wrocław, Institute of Geological Sciences, ul. Cybulskiego 30, 50-205 Wrocław, Poland
autor
  • Wrocław University of Technology, Faculty of Geoengineering, Mining and Geology, Division of Geology and Mineral Waters, Wybrzeże S. Wyspiańskiego 27, 50-370 Wrocław, Poland
Bibliografia
  • 1. Alexander C.M.O., Grossman J.N., Ebel D.S., Ciesla F.J., 2008 − The formation conditions of chondrules and chondrites. Science 320, 1617−1619.
  • 2. Brearley A.J., Jones R.H., 1998 − Chondritic meteorites. Planetary Materials, Reviews in Mineralogy and Geochemistry 36, 3.1−3.398.
  • 3. Davis A.M., Richter F.M., 2004 − Condensation and evaporation of solar system materials. [in:] Davis A.M. (ed.) – Treatise on Geochemistry, Vol 1., Meteorites, Comets and Planets, Elsevier, Oxford, 407−430.
  • 4. Ebel D.S., 2006 − Condensation of rocky material in astrophysical environments. [in:] Lauretta D.S., McSween H.Y. Jr. (eds.) – Meteorites and the Early Solar System II, University of Arizona Press, Tucson, 253−277.
  • 5. Grossman L., Larimer J.W., 1974 − Early chemical history of the solar system. Reviews of Geophysics and Space Physics 12, 71−101.
  • 6. Hezel D.C., Schlüter J., Kallweit H., Jull A.J.T., Al Fakeer O.Y., Al Shamsi M., Strekopytov S., 2011 – Meteorites from the United Arab Emirates: Description, weathering, and terrestrial ages. Meteoritics & Planetary Science 46 (2), 327−336.
  • 7. Hutchison R., 2006 – Meteorites. A Petrologic, Chemical and Isotopic Synthesis. Cambridge University Press, Cambridge, UK.
  • 8. Jarosewich E., 1990 – Chemical analyses of meteorites: a compilation of stony and iron meteorite analyses. Meteoritics 25, 323−337.
  • 9. Kallemeyn G.W., Rubin A.E., Wang D., Wasson J.T., 1989 − Ordinary chondrites: bulk chemical composition, classification, lithophile-element fractionations, and compositionpetrographic type relationships. Geochimica et Cosmochimica Acta 53, 2747−2767.
  • 10. Koblitz J., 2010 – MetBase®, ver. 7.3, Meteorite Data Retrieval Software. Ritterhude, Germany.
  • 11. Lauretta D.S., Nagahara H., Alexander C.M.O’D., 2006 – Petrology and Origin of Ferromagnesian Silicate Chondrules. [in:] Lauretta D.S., McSween H.Y. Jr. (eds.) – Meteorites and the Early Solar System II, University of Arizona Press, Tucson, 431−459.
  • 12. McSween H.Y., Huss G.R., 2010 – Cosmochemistry. Cambridge University Press, New York, USA.
  • 13. Mészáros M., Kereszturi Á., Ditrói-Puskás Z., 2014 – A new classification of Nyirábrany, an ordinary chondrite from Hungary. Meteorites 3 (1–2), 19−32.
  • 14. Rubin A.E., Scott E.R.D., Keil K., 1997 – Shock metamorphism of enstatite chondrites. Geochimica et Cosmochimica Acta 61 (4), 847−858.
  • 15. Stöffler D., Keil K., Scott E.R.D., 1991 – Shock metamorphism of ordinary chondrites. Geochimica et Cosmochimica Acta 55, 3845−3867.
  • 16. Van Schmuss W.R., Wood J.A., 1967 – A chemical-petrologic classification for the chondritic meteorites. Geochimica et Cosmochimica Acta 31 (5), 747−765.
  • 17. Velbel M.A., 2014 – Terrestrial weathering of ordinary chondrites in nature and continuing during laboratory storage and processing: Review and implications for Hayabusa sample integrity. Meteoritics & Planetary Science 49 (2), 154−171.
  • 18. Wanke H., Dreibus G., 1988 − Chemical composition and accretion history of terrestrial planets. Phylosophical Transactions of the Royal Society of London A325, 545−557.
  • 19. Wasson J.T., Kallemeyn G.W., 1988 – Composition of chondrites. Phylosophical Transactions of the Royal Society of London A325, 535–544.
  • 20. Weisberg M.K., McCoy T.J., Krot A.N., 2006 – Systematics and evaluation of meteorite classification. [in:] Lauretta D.S., McSween H.Y. Jr. (eds.) – Meteorites and the Early Solar System II, University of Arizona Press, Tucson, 19−52.
  • 21. Wlotzka F., 1993 – A Weathering Scale for the Ordinary Chondrites. Meteoritics 28 (3), 460−460.
  • 22. Yin Q.Z., 2005 − From dust to planets: the tale told by moderately volatile elements. [in:] Krot A.N., Scott E.R.D., Reipurth B. (eds.) – Chondrites and the Protoplanetary Disk, ASP Conference Series 341, Astronomical Society of the Pacifific, San Francisco, 632−644.
  • 23. Zurfluh F.J., Hofmann B.A., Gnos E., Eggenberger U., Greber N.D., Villa I.M., 2012 – Weathering and strontium contamination of meteorites recovered in the Sultanate of Oman. Meteorite, February 2012, 34−38.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-583617d7-3907-4ce8-951a-97f68210b2f6
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