Mineralogy and crystallography of some Itokawa particles returned by the Hayabusa asteroidal sample return mission
详细信息    查看全文
  • 作者:Takashi Mikouchi ; Mutsumi Komatsu ; Kenji Hagiya…
  • 关键词:Itokawa ; Hayabusa ; Olivine ; Plagioclase ; SR ; XRD ; SR ; XANES ; LL chondrites
  • 刊名:Earth, Planets and Space
  • 出版年:2014
  • 出版时间:December 2014
  • 年:2014
  • 卷:66
  • 期:1
  • 全文大小:867KB
  • 参考文献:Abe M, Takagi Y, Kitazato K, Abe S, Hiroi T, Vilas F, Clark BE, Abell PA, Lederer SM, Jarvis KS, Nimura T, Ueda Y, Fujiwara A: Near-infrared spectral results of asteroid Itokawa from the Hayabusa spacecraft. Science 2006, 312:1334-338.CrossRef
    Akimoto S, Fujisawa H: Olivine-spinel solid solution equilibria in the system Mg 2 SiO 4 -Fe 2 SiO 4 . J Geophys Res 1968, 73:1467-479.CrossRef
    Bischoff A, Geiger T, Palme H, Spettel B, Schultz L, Scherer P, Schlüter J, Lkhamsuren J: Mineralogy, chemistry, and noble gas contents of Adzhi-Bogdo -an LL3- chondritic breccia with foreign clasts. Meteoritics 1993, 28:570-78.
    Bischoff A, Scott ERD, Metzler K, Goodrich CA: Nature and origins of meteoritic breccias. In Meteorites and the early solar system II. Edited by: Lauretta MS, McSween HYJr. Tucson: University of Arizona; 2006:679-12.
    Bischoff A, Horstmann M, Pack A, Laubenstein M, Haberer S: Asteroid 2008 TC3—Almahata Sitta: a spectacular breccia containing many different ureilitic and chondritic lithologies. Meteorit Planet Sci 2010, 45:1638-656.CrossRef
    Ebihara M, Sekimoto S, Shirai N, Hamajima Y, Yamamoto M, Kumagai K, Oura Y, Ireland TR, Kitajima F, Nagao K, Nakamura T, Naraoka H, Noguchi T, Okazaki R, Tsuchiyama A, Uesugi M, Yurimoto H, Zolensky ME, Abe M, Fujimura A, Mukai T, Yada T: Neutron activation analysis of a particle returned from asteroid Itokawa. Science 2011, 333:1119-121.CrossRef
    Fujiwara A, Kawaguchi J, Yeomans DK, Abe M, Mukai T, Okada T, Saito J, Yano H, Yoshikawa M, Scheeres DJ, Barnouin-Jha O, Cheng AF, Demura H, Gaskell RW, Hirata N, Ikeda H, Kominato T, Miyamoto H, Nakamura AM, Nakamura R, Sasaki S, Uesugi K: The rubble-pile asteroid Itokawa as observed by Hayabusa. Science 2006, 312:1330-334.CrossRef
    Goodrich CA, Bischoff A, O'Brien DP: Asteroid 2008 TC3 and the fall of Almahata Sitta, a unique meteorite breccia. Elements 2014, 10:31-7.CrossRef
    Hagiya K, Mikouchi T, Zolensky M, Ohsumi K, Terada Y, Yagi N, Takata M: Derivation of the cell parameters of meteoritic olivine in a thin section by energy-scanning X-ray diffraction with synchrotron radiation. Meteorit Planet Sci 2010,45(supplement s1):A5-A227. Abstract #5083
    Herrin JS, Zolensky ME, Ito M, Le L, Mittlefehldt DW, Jenniskens P, Ross AJ, Shaddad MH: Thermal and fragmentation history of ureilitic asteroids: insights from the Almahata Sitta fall. Meteorit Planet Sci 2010, 45:1789-803.CrossRef
    Horstmann M, Bischoff A: The Almahata Sitta polymict breccia and the late accretion of Asteroid 2008 TC3 - invited review. Chemie der Erde - Geochem 2014, 74:149-84.CrossRef
    Jamasja N, Ruzicka A: Shock and thermal history of Northwest Africa 4859, an annealed impact-melt breccia of LL chondrite parentage containing unusual igneous features and pentlandite. Meteorit Planet Sci 2010, 45:828-49.CrossRef
    Jenniskens P, Shaddad MH, Numan D, Elsir S, Kudoda AM, Zolensky M, Le L, Robinson GA, Friedrich JM, Rumble D, Steele A, Chesley SR, Fitzsimmons A, Duddy S, Hsieh HH, Ramsay G, Brown PG, Edwards WN, Tagliaferri E, Boslough MB, Spalding RE, Dantowitz R, Kozubal M, Pravec P, Borovicka J, Charvat Z, Vaubaillon J, Kuiper J, Albers J, Bishop JL, et al.: The impact and recovery of asteroid 2008 TC3. Nature 2009, 458:485-88.CrossRef
    Krot AN: Bringing part of an asteroid back home. Science 2011, 312:1098-099.CrossRef
    Mikouchi T, Zolensky ME, Ohnishi I, Suzuki T, Takeda H, Jenniskens P, Shaddad MH: Electron microscopy of pyroxene in the Almahata Sitta ureilite. Meteorit Planet Sci 2010, 45:1812-820.CrossRef
    Monkawa A, Mikouchi T, Koizumi E, Sugiyama K, Miyamoto M: Determination of the Fe oxidation state of the Chassigny kaersutite: a microXANES spectroscopic study. Meteorit Planet Sci 2006, 41:1321-329.CrossRef
    Nagao K, Okazaki R, Nakamura T, Miura YN, Osawa T, Bajo K, Matsuda S, Ebihara M, Ireland TR, Kitajima F, Naraoka H, Noguchi T, Tsuchiyama A, Yurimoto H, Zolensky ME, Uesugi M, Shirai K, Abe M, Yada T, Ishibashi Y, Fujimura A, Mukai T, Ueno M, Okada T, Yoshikawa M, Kawaguchi J: Irradiation history of Itokawa regolith material deduced from noble gases in the Hayabusa samples. Science 2011, 333:1128-131.CrossRef
    Nakamura T, Noguchi T, Tanaka M, Zolensky ME, Kimura M, Tsuchiyama A, Nakato A, Ogami T, Ishida H, Uesugi M, Yada T, Shirai K, Fujimura A, Okazaki R, Sandford SA, Ishibashi Y, Abe M, Okada T, Ueno M, Mukai T, Yoshikawa M, Kawaguchi J: Itokawa dust particles: a direct link between S-type asteroids and ordinary chondrites. Science 2011, 333:1113-116.CrossRef
    Nakamura T, Nakato A, Ishida H, Wakita S, Noguchi T, Zolensky ME, Tanaka M, Kimura M, Tshuchiyama A, Ogami T, Hashimoto T, Konno M, Uesugi M, Yada T, Shirai K, Fujimura A, Okazaki R, Sandford SA, Ishibashi Y, Abe M, Okada T, Ueno M, Kawaguchi J: Mineral chemistry of MUSES-C Regio inferred from analysis of dust particles collected from the first- and second-touchdown sites on asteroid Itokawa. Meteorit Planet Sci 201
  • 作者单位:Takashi Mikouchi (1)
    Mutsumi Komatsu (2)
    Kenji Hagiya (3)
    Kazumasa Ohsumi (4)
    Michael E Zolensky (5)
    Viktor Hoffmann (6) (7)
    James Martinez (8)
    Rupert Hochleitner (9)
    Melanie Kaliwoda (9)
    Yasuko Terada (4)
    Naoto Yagi (4)
    Masaki Takata (4)
    Wataru Satake (1)
    Yuya Aoyagi (1)
    Atsushi Takenouchi (1)
    Yuzuru Karouji (10)
    Masayuki Uesugi (10)
    Toru Yada (10)

    1. Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan
    2. Waseda Institute for Advanced Study, Waseda University, 1-6-1 Nishiwaseda, Shinjuku-ku, Tokyo, 169-8050, Japan
    3. School of Science, University of Hyogo, 3-2-1 Kouto, Kamigori-cho, Ako-gun, Hyogo, 678-1297, Japan
    4. Japan Synchrotron Radiation Research Institute (JASRI), 1-1-1 Kouto, Sayo-cho, Sayo-gun, Hyogo, 679-5198, Japan
    5. Astromaterials Research and Exploration Science, NASA Johnson Space Center, Houston, TX, 77058, USA
    6. Department of Earth and Environmental Sciences, Section Geophysics, Ludwig Maximillian’s University Munich (LMU), Theresienstr. 41, Munich, 80333, Germany
    7. Department of Geosciences, Eberhard Karls University of Tübingen, H?lderlinstr. 12, Tübingen, 72074, Germany
    8. ESCG Jacobs, Houston, TX, 77058, USA
    9. Mineralogical State Collection, Theresienstr 41, Munich, 80333, Germany
    10. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1, Yoshinodai, Chuo-ku, Sagamihara, Kanagawa, 252-5210, Japan
  • 刊物类别:Earth Sciences, general; Geology; Geophysics/Geodesy;
  • 刊物主题:Earth Sciences, general; Geology; Geophysics/Geodesy;
  • 出版者:Springer Berlin Heidelberg
  • ISSN:1880-5981
文摘
We studied seven Itokawa particles provided by the Japan Aerospace Exploration Agency (JAXA) as first International Announcement of Opportunity (AO) study mainly using electron and synchrotron radiation X-ray beam techniques. All the analyzed particles were collected from the first-touchdown site and composed of olivine and plagioclase with traces of Ca phosphate and chromite, and do not contain pyroxenes. Optical microscopy of these particles shows minor undulatory extinction of olivine and plagioclase, suggesting minor shock metamorphism (shock stage: S2). The electron microprobe analysis shows that olivine is Fo70-73 and plagioclase is An13-10Or5-7. The synchrotron radiation X-ray diffraction (SR-XRD) analysis of olivine crystals gives cell dimensions of a--.708 to 4.779 ?, b--0.271 to 10.289 ?, c--.017 to 6.024 ?, corresponding to the Fo content of Fo~70 by Vegard's law. This composition matches the result obtained by the electron microprobe analysis. The olivine compositions of the analyzed particles are consistent with those of LL chondrites. The cell dimensions of two plagioclase crystals (a--.180 to 8.194 ?, b--2.53 to 12.893 ?, c--.125 to 7.23 ?, α--2.6° to 93.00°, β--16.36° to 116.75°, γ--0.03° to 90.17°) indicate that their equilibration temperatures are 800°C?±-0°C. This temperature is near the peak metamorphic temperature recorded by equilibrated ordinary chondrites. The size of plagioclase crystals and the homogeneity of olivine compositions indicate that their petrologic type is ?. We also analyzed plagioclase by SR iron X-ray absorption near-edge structure (SR-XANES) and found that its Fe3+/(Fe2+ + Fe3+) ratio is approximately 0.5. Such high Fe3+ abundance indicates the formation under a relatively oxidizing environment. Thus, all these analyses have reconfirmed that the Itokawa particles returned by the Hayabusa spacecraft are very weakly shocked equilibrated LL chondrites, which matches the results of the preliminary examination team. Keywords Itokawa Hayabusa Olivine Plagioclase SR-XRD SR-XANES LL chondrites

© 2004-2018 中国地质图书馆版权所有 京ICP备05064691号 京公网安备11010802017129号

地址:北京市海淀区学院路29号 邮编:100083

电话:办公室:(+86 10)66554848;文献借阅、咨询服务、科技查新:66554700