Lut 009, an H4 (S2, W4) ordinary chondrite meteorite from Lut Desert of Iran

نویسندگان

1 Ph.D. Student, Aix-Marseille Université/CNRS/IRD, CEREGE UM34, Aix-en-Provence, France

2 Associate Professor, Department of Geology, Faculty of Sciences, University of Tehran, Iran

3 Professor, Aix-Marseille Université/CNRS/IRD, CEREGE UM34, Aix-en-Provence, France

4 Associate Researcher, Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, USA

چکیده

Lut 009 meteorite was found during a trip to Lut Desert of Iran in March,2012, at 30°20.38' N, 59°09.04' E. Chemical compositions of equilibrated olivine (Fa19.3 ± 0.5) and orthopyroxene (Fs16.7 ± 0.6) show that the meteorite sample belongs to H group of ordinary chondrites, while the texture (chondrule petrography and plagioclase size) suggests a petrologic type of 4. The Lut 009 has been very weakly shock altered and has a shock stage of S2. Fe-Ni is completely weathered whereas less than 5 percent of troilite is still present. Therefore, the meteorite has a weathering grade of W4. Magnetic susceptibility is log χ =4.75 (χ in 10-9 m3/kg) and, thus, consistent with a W4 H ordinary chondrite. Here we report description of Lut 009 in the first extended study on a meteorite from Lut Desert. Along with this sample, in-progress investigations of other meteorites from the desert will open a window into the characteristics of meteorite concentrations in this region.

کلیدواژه‌ها


عنوان مقاله [English]

Lut 009, an H4 (S2, W4) ordinary chondrite meteorite from Lut Desert of Iran

نویسندگان [English]

  • Hamed Pourkhorsandi 1
  • Hassan Mirnejad 2
  • Pierre Rochette 3
  • Jamshid Hassanzadeh 4
1 Ph.D. Student, Aix-Marseille Université/CNRS/IRD, CEREGE UM34, Aix-en-Provence, France
2 Associate Professor, Department of Geology, Faculty of Sciences, University of Tehran, Iran
3 Professor, Aix-Marseille Université/CNRS/IRD, CEREGE UM34, Aix-en-Provence, France
4 Associate Researcher, Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, USA
چکیده [English]

Lut 009 meteorite was found during a trip to Lut Desert of Iran in March,2012, at 30°20.38' N, 59°09.04' E. Chemical compositions of equilibrated olivine (Fa19.3 ± 0.5) and orthopyroxene (Fs16.7 ± 0.6) show that the meteorite sample belongs to H group of ordinary chondrites, while the texture (chondrule petrography and plagioclase size) suggests a petrologic type of 4. The Lut 009 has been very weakly shock altered and has a shock stage of S2. Fe-Ni is completely weathered whereas less than 5 percent of troilite is still present. Therefore, the meteorite has a weathering grade of W4. Magnetic susceptibility is log χ =4.75 (χ in 10-9 m3/kg) and, thus, consistent with a W4 H ordinary chondrite. Here we report description of Lut 009 in the first extended study on a meteorite from Lut Desert. Along with this sample, in-progress investigations of other meteorites from the desert will open a window into the characteristics of meteorite concentrations in this region.

کلیدواژه‌ها [English]

  • Iran
  • Lut Desert
  • Meteorite
  • Ordinary chondrite
Armstrong, J. T., 1988, Quantitative analysis of silicate and oxide minerals, comparison of Monte Carlo, ZAF, and U (qz) procedures, in: Newbury, D. E., (Ed.), Microbeam analysis. Proceedings of the 23rd Annual Conference of the Microbeam Analysis Society, San Francisco Press, San Francisco, 239-246.
Bland, P. A., Kelley, S. P., Berry, F. J., Cadogan, J. M. and Pillinger, C. T., 1997, Artificial weathering of the ordinary chondrite Allegan, Implications for the presence of Cl- as a structural component in akaganeite, Am. Mineral, 82, 1187-1197.
Bland, P. A., Zolensky, M. E., Benedix, G. K. and Sephton, M. A., 2006, Weathering of chondritic meteorites, in: Lauretta, D. S. and McSween, Jr., H. Y., (Eds.), Meteorites and the Early Solar System II, University of Arizona Press, Arizona, 853-867.
Buchwald, V. F. and Clarke, Jr., R. S., 1989, Corrosion of Fe-Ni alloys by Cl-containing akaganeite (β-FeOOH), the Antarctic meteorite case, Am, Mineral, 74, 657-667.
Ehsani, A. H. and Quiel, F., 2008, Remote sens, Environment, 112, 3284-3294.
Hutchison, R., 2004, Meteorites, a petrologic, chemical and isotopic synthesis, Cambridge University Press, Cambridge.
Koeberl, C. and Cassidy, W. A., 1991, Differences between Antarctic and non-Antarctic meteorites, An assessment, Geochim, Cosmochim, Ac(55), 3-18.
Lee, M. R. and Bland, P. A., 2004, Mechanisms of weathering of meteorites recovered from hot and cold deserts and the formation of phyllosilicates, Geochim, Cosmochim, Ac(68), 893-916.
Mahmoodi, F., 2002, The distribution of erg lands of Iran (in Persian), Forest and Range Protection Research Institute, Tehran.
Mildrexler, D. J., Zhao, M. and Running S. W., 2011, B. Am. Meteorol. Soc., 7, 855-860.
Pabot, H., 1967, Report to government of Iran, pasture development and range improvement through botanical and ecological studies, UNDP, Food and Agricultural Organization of the United Nations, Rome.
Pourkhorsandi, H. and Mirnejad, H., 2013, 44th Lunar and Planetary Science Conference, A1096.
Rochette, P., Gattacceca, J. and Lewandowski, M., 2012, Magnetic classification on meteorites and application to the Soltmany Fall. Meteorites, 2, 67-71.
Stöffler, D., Keil, K. and Scott E. R. D., 1991, Shock metamorphism of ordinary chondrites, Geochim, Cosmochim, Ac(55), 3845-3867.
Van Schmus, W. R. and Wood, J. A., 1967, A chemical-petrologic classification lot the chondritic meteorites, Geochim, Cosmochim, Ac(31), 747-765.
Wlotzka, F., 1993, A weathering scale for the ordinary chondrites, Meteoritics, 28, 460.