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Analysis of Cation Composition in Dolomites on the Intact Particles Sampled from Asteroid Ryugu.
Morita, Mayu; Yui, Hiroharu; Urashima, Shu-Hei; Onose, Morihiko; Komatani, Shintaro; Nakai, Izumi; Abe, Yoshinari; Terada, Yasuko; Homma, Hisashi; Motomura, Kazuko; Ichida, Kiyohiro; Yokoyama, Tetsuya; Nagashima, Kazuhide; Aléon, Jérôme; O'D Alexander, Conel M; Amari, Sachiko; Amelin, Yuri; Bajo, Ken-Ichi; Bizzarro, Martin; Bouvier, Audrey; Carlson, Richard W; Chaussidon, Marc; Choi, Byeon-Gak; Dauphas, Nicolas; Davis, Andrew M; Fujiya, Wataru; Fukai, Ryota; Gautam, Ikshu; Haba, Makiko K; Hibiya, Yuki; Hidaka, Hiroshi; Hoppe, Peter; Huss, Gary R; Iizuka, Tsuyoshi; Ireland, Trevor R; Ishikawa, Akira; Itoh, Shoichi; Kawasaki, Noriyuki; Kita, Noriko T; Kitajima, Kouki; Kleine, Thorsten; Krot, Sasha; Liu, Ming-Chang; Masuda, Yuki; Moynier, Frédéric; Nguyen, Ann; Nittler, Larry; Pack, Andreas; Park, Changkun; Piani, Laurette.
Afiliação
  • Morita M; Analytical Technology Division, Horiba Techno Service Co., Ltd., Kyoto 601-8125, Japan.
  • Yui H; Department of Chemistry, Tokyo University of Science, Tokyo 162-8601, Japan.
  • Urashima SH; Department of Chemistry, Tokyo University of Science, Tokyo 162-8601, Japan.
  • Onose M; Analytical Technology Division, Horiba Techno Service Co., Ltd., Kyoto 601-8125, Japan.
  • Komatani S; Analytical Technology Division, Horiba Techno Service Co., Ltd., Kyoto 601-8125, Japan.
  • Nakai I; Department of Applied Chemistry, Tokyo University of Science, Tokyo 162-8601, Japan.
  • Abe Y; Graduate School of Engineering Materials Science and Engineering, Tokyo Denki University, Tokyo 120-8551, Japan.
  • Terada Y; Spectroscopy and Imaging Division, Japan Synchrotron Radiation Research Institute, Hyogo 679-5198, Japan.
  • Homma H; Osaka Application Laboratory, Rigaku Corporation, Osaka 569-1146, Japan.
  • Motomura K; Thermal Analysis Division, Rigaku Corporation, Tokyo 196-8666, Japan.
  • Ichida K; Analytical Technology Division, Horiba Techno Service Co., Ltd., Kyoto 601-8125, Japan.
  • Yokoyama T; Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo 152-8551, Japan.
  • Nagashima K; Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Ma̅noa, Honolulu, Hawaii 96822, United States.
  • Aléon J; Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, Sorbonne Université, Museum National d'Histoire Naturelle, Centre National de la Recherche Scientifique Unité Mixte de Recherche 7590, Institut de recherche pour le développement, Paris 75005, France.
  • O'D Alexander CM; Earth and Planets Laboratory, Carnegie Institution for Science, Washington, District of Columbia 20015, United States.
  • Amari S; McDonnell Center for the Space Sciences and Physics Department, Washington University, St. Louis, Missouri 63130, United States.
  • Amelin Y; Geochemical Research Center, The University of Tokyo, Tokyo 113-0033, Japan.
  • Bajo KI; Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, Guangzhou, GD 510640, China.
  • Bizzarro M; Department of Natural History Sciences, Hokkaido University, Sapporo 001-0021, Japan.
  • Bouvier A; Centre for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen K 1350, Denmark.
  • Carlson RW; Bayerisches Geoinstitut, Universität Bayreuth, Bayreuth 95447, Germany.
  • Chaussidon M; Earth and Planets Laboratory, Carnegie Institution for Science, Washington, District of Columbia 20015, United States.
  • Choi BG; Université Paris Cité, Institut de physique du globe de Paris, Centre National de la Recherche Scientifique, Paris 75005, France.
  • Dauphas N; Department of Earth Science Education, Seoul National University, Seoul 08826, Republic of Korea.
  • Davis AM; Department of the Geophysical Sciences and Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, United States.
  • Fujiya W; Department of the Geophysical Sciences and Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, United States.
  • Fukai R; Faculty of Science, Ibaraki University, Mito 310-8512, Japan.
  • Gautam I; Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara 252-5210, Japan.
  • Haba MK; Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo 152-8551, Japan.
  • Hibiya Y; Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo 152-8551, Japan.
  • Hidaka H; Department of General Systems Studies, University of Tokyo, Tokyo 153-0041, Japan.
  • Hoppe P; Department of Earth and Planetary Sciences, Nagoya University, Nagoya 464-8601, Japan.
  • Huss GR; Max Planck Institute for Chemistry, Mainz 55128, Germany.
  • Iizuka T; Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Ma̅noa, Honolulu, Hawaii 96822, United States.
  • Ireland TR; Department of Earth and Planetary Science, University of Tokyo, Tokyo 113-0033, Japan.
  • Ishikawa A; School of Earth and Environmental Sciences, University of Queensland, St Lucia, QLD 4072, Australia.
  • Itoh S; Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo 152-8551, Japan.
  • Kawasaki N; Division of Earth and Planetary Sciences, Kyoto University, Kyoto 606-8502, Japan.
  • Kita NT; Department of Natural History Sciences, Hokkaido University, Sapporo 001-0021, Japan.
  • Kitajima K; Department of Geoscience, University of Wisconsin─Madison, Madison, Wisconsin 53706, United States.
  • Kleine T; Department of Geoscience, University of Wisconsin─Madison, Madison, Wisconsin 53706, United States.
  • Krot S; Max Planck Institute for Solar System Research, Göttingen 37077, Germany.
  • Liu MC; Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Ma̅noa, Honolulu, Hawaii 96822, United States.
  • Masuda Y; Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, California 90095, United States.
  • Moynier F; Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo 152-8551, Japan.
  • Nguyen A; Université Paris Cité, Institut de physique du globe de Paris, Centre National de la Recherche Scientifique, Paris 75005, France.
  • Nittler L; Astromaterials Research and Exploration Science Division, National Aeronautics and Space Administration Johnson Space Center, Johnson Space Center, Houston, Texas 77058, United States.
  • Pack A; Earth and Planets Laboratory, Carnegie Institution for Science, Washington, District of Columbia 20015, United States.
  • Park C; Faculty of Geosciences and Geography, University of Göttingen, Göttingen D-37077, Germany.
  • Piani L; Division of Earth-System Sciences, Korea Polar Research Institute, Incheon 21990, Korea.
Anal Chem ; 96(1): 170-178, 2024 Jan 09.
Article em En | MEDLINE | ID: mdl-38155534
ABSTRACT
Characterization of the elemental distribution of samples with rough surfaces has been strongly desired for the analysis of various natural and artificial materials. Particularly for pristine and rare analytes with micrometer sizes embedded on specimen surfaces, non-invasive and matrix effect-free analysis is required without surface polishing treatment. To satisfy these requirements, we proposed a new method employing the sequential combination of two imaging modalities, i.e., microenergy-dispersive X-ray fluorescence (micro-XRF) and Raman micro-spectroscopy. The applicability of the developed method is tested by the quantitative analysis of cation composition in micrometer-sized carbonate grains on the surfaces of intact particles sampled directly from the asteroid Ryugu. The first step of micro-XRF imaging enabled a quick search for the sparsely scattered and micrometer-sized carbonates by the codistributions of Ca2+ and Mn2+ on the Mg2+- and Fe2+-rich phyllosilicate matrix. The following step of Raman micro-spectroscopy probed the carbonate grains and analyzed their cation composition (Ca2+, Mg2+, and Fe2+ + Mn2+) in a matrix effect-free manner via the systematic Raman shifts of the lattice modes. The carbonates were basically assigned to ferroan dolomite bearing a considerable amount of Fe2+ + Mn2+ at around 10 atom %. These results are in good accordance with the assignments reported by scanning electron microscopy-energy-dispersive X-ray spectroscopy, where the thin-sectioned and surface-polished Ryugu particles were applicable. The proposed method requires neither sectioning nor surface polishing; hence, it can be applied to the remote sensing apparatus on spacecrafts and planetary rovers. Furthermore, the non-invasive and matrix effect-free characterization will provide a reliable analytical tool for quantitative analysis of the elemental distribution on the samples with surface roughness and chemical heterogeneity at a micrometer scale, such as art paintings, traditional crafts with decorated shapes, as well as sands and rocks with complex morphologies in nature.

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2024 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2024 Tipo de documento: Article