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      Nanoscale infrared imaging analysis of carbonaceous chondrites to understand organic-mineral interactions during aqueous alteration

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          Significance

          Spatial relationships between organic matter and minerals are necessary for understanding the formation and evolution of organic matter during aqueous and thermal alteration in their parent bodies, as well as preaccretional history. Infrared spectroscopy is a powerful tool to analyze the molecular structures of organic matter and identification of minerals. However, its spatial resolution is limited due to the diffraction limit. Recently, the atomic force microscopy (AFM) based IR nanospectroscopy was developed and applied in various scientific fields to overcome the diffraction limit of IR. We applied the AFM-based IR nanospectroscopy to carbonaceous chondrites and studied organic-mineral associations at the ∼30 nm spatial resolution.

          Abstract

          Organic matter in carbonaceous chondrites is distributed in fine-grained matrix. To understand pre- and postaccretion history of organic matter and its association with surrounding minerals, microscopic techniques are mandatory. Infrared (IR) spectroscopy is a useful technique, but the spatial resolution of IR is limited to a few micrometers, due to the diffraction limit. In this study, we applied the high spatial resolution IR imaging method to CM2 carbonaceous chondrites Murchison and Bells, which is based on an atomic force microscopy (AFM) with its tip detecting thermal expansion of a sample resulting from absorption of infrared radiation. We confirmed that this technique permits ∼30 nm spatial resolution organic analysis for the meteorite samples. The IR imaging results are consistent with the previously reported association of organic matter and phyllosilicates, but our results are at much higher spatial resolution. This observation of heterogeneous distributions of the functional groups of organic matter revealed its association with minerals at ∼30 nm spatial resolution in meteorite samples by IR spectroscopy.

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          Author and article information

          Journal
          Proc Natl Acad Sci U S A
          Proc. Natl. Acad. Sci. U.S.A
          pnas
          pnas
          PNAS
          Proceedings of the National Academy of Sciences of the United States of America
          National Academy of Sciences
          0027-8424
          1091-6490
          15 January 2019
          2 January 2019
          : 116
          : 3
          : 753-758
          Affiliations
          [1] aFaculty of Engineering, Yokohama National University , 240-8501 Yokohama, Japan;
          [2] b Nihon Thermal Consulting Co., Ltd. , 160-0023 Tokyo, Japan;
          [3] cInstrumental Analysis Center, Yokohama National University , 240-8501 Yokohama, Japan;
          [4] dAstromaterials Research and Exploration Science, National Aeronautics and Space Administration Johnson Space Center , Houston, TX 77058
          Author notes
          1To whom correspondence should be addressed. Email: kebukawa@ 123456ynu.ac.jp .

          Edited by Mark H. Thiemens, University of California at San Diego, La Jolla, CA, and approved December 6, 2018 (received for review September 19, 2018)

          Author contributions: Y.K. designed research; Y.K., H.K., and M.K. performed research; H.K., N.U., and N.B. contributed new reagents/analytic tools; Y.K. analyzed data; and Y.K., M.E.Z., and K.K. wrote the paper.

          Author information
          http://orcid.org/0000-0001-8430-3612
          http://orcid.org/0000-0003-1226-0742
          http://orcid.org/0000-0002-9248-9899
          http://orcid.org/0000-0003-2951-1341
          Article
          PMC6338842 PMC6338842 6338842 201816265
          10.1073/pnas.1816265116
          6338842
          30602454
          aea8927d-4b94-4c4c-bbbe-8d8b35b798f4
          Copyright @ 2019

          Published under the PNAS license.

          History
          Page count
          Pages: 6
          Funding
          Funded by: MEXT | Japan Society for the Promotion of Science (JSPS) 501100001691
          Award ID: JP17H02991
          Award Recipient : Yoko Kebukawa Award Recipient : Kensei Kobayashi
          Funded by: MEXT | Japan Society for the Promotion of Science (JSPS) 501100001691
          Award ID: JP17H06458
          Award Recipient : Yoko Kebukawa Award Recipient : Kensei Kobayashi
          Funded by: MEXT | Japan Society for the Promotion of Science (JSPS) 501100001691
          Award ID: JP18K03722
          Award Recipient : Yoko Kebukawa Award Recipient : Kensei Kobayashi
          Funded by: NINS Astrobiology Center
          Award ID: AB281004
          Award Recipient : Yoko Kebukawa
          Funded by: NINS Astrobiology Center
          Award ID: AB291005
          Award Recipient : Yoko Kebukawa
          Funded by: NINS Astrobiology Center
          Award ID: AB301020
          Award Recipient : Yoko Kebukawa
          Categories
          Physical Sciences
          Earth, Atmospheric, and Planetary Sciences

          AFM-IR,IR spectroscopy,organic matter,meteorites
          AFM-IR, IR spectroscopy, organic matter, meteorites

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