TY - JOUR
T1 - Analytical dual-energy microtomography
T2 - A new method for obtaining three-dimensional mineral phase images and its application to Hayabusa samples
AU - Tsuchiyama, A.
AU - Nakano, T.
AU - Uesugi, K.
AU - Uesugi, M.
AU - Takeuchi, A.
AU - Suzuki, Y.
AU - Noguchi, R.
AU - Matsumoto, T.
AU - Matsuno, J.
AU - Nagano, T.
AU - Imai, Y.
AU - Nakamura, T.
AU - Ogami, T.
AU - Noguchi, T.
AU - Abe, M.
AU - Yada, T.
AU - Fujimura, A.
N1 - Funding Information:
The tomography experiment was performed under the approval of the SPring-8 Proposal Review Committee (2010B1531 and 2011A1388). We thank the Hayabusa sample curation team and the Hayabusa project team. We also thank Dr. A. Gucsik of Max Planck Institute for Chemistry, Mainz, Germany for reading the manuscript. We are grateful to Drs. D. Hezel, J.M. Friedrich and G. Flynn for improving the manuscript in the review step. Drs. D. Hezel and J.M. Friedrich also kindly checked the English of the paper. A. T. was supported by a Grant-in-aid of the Japan Ministry of Education, Culture, Sports, Science and Technology ( 19104012 ).
PY - 2013/9/1
Y1 - 2013/9/1
N2 - We developed a novel technique called "analytical dual-energy microtomography" that uses the linear attenuation coefficients (LACs) of minerals at two different X-ray energies to nondestructively obtain three-dimensional (3D) images of mineral distribution in materials such as rock specimens. The two energies are above and below the absorption edge energy of an abundant element, which we call the "index element". The chemical compositions of minerals forming solid solution series can also be measured. The optimal size of a sample is of the order of the inverse of the LAC values at the X-ray energies used. We used synchrotron-based microtomography with an effective spatial resolution of >200. nm to apply this method to small particles (30-180. μm) collected from the surface of asteroid 25143 Itokawa by the Hayabusa mission of the Japan Aerospace Exploration Agency (JAXA). A 3D distribution of the minerals was successively obtained by imaging the samples at X-ray energies of 7 and 8. keV, using Fe as the index element (the K-absorption edge of Fe is 7.11. keV). The optimal sample size in this case is of the order of 50. μm. The chemical compositions of the minerals, including the Fe/Mg ratios of ferromagnesian minerals and the Na/Ca ratios of plagioclase, were measured. This new method is potentially applicable to other small samples such as cosmic dust, lunar regolith, cometary dust (recovered by the Stardust mission of the National Aeronautics and Space Administration [NASA]), and samples from extraterrestrial bodies (those from future sample return missions such as the JAXA Hayabusa2 mission and the NASA OSIRIS-REx mission), although limitations exist for unequilibrated samples. Further, this technique is generally suited for studying materials in multicomponent systems with multiple phases across several research fields.
AB - We developed a novel technique called "analytical dual-energy microtomography" that uses the linear attenuation coefficients (LACs) of minerals at two different X-ray energies to nondestructively obtain three-dimensional (3D) images of mineral distribution in materials such as rock specimens. The two energies are above and below the absorption edge energy of an abundant element, which we call the "index element". The chemical compositions of minerals forming solid solution series can also be measured. The optimal size of a sample is of the order of the inverse of the LAC values at the X-ray energies used. We used synchrotron-based microtomography with an effective spatial resolution of >200. nm to apply this method to small particles (30-180. μm) collected from the surface of asteroid 25143 Itokawa by the Hayabusa mission of the Japan Aerospace Exploration Agency (JAXA). A 3D distribution of the minerals was successively obtained by imaging the samples at X-ray energies of 7 and 8. keV, using Fe as the index element (the K-absorption edge of Fe is 7.11. keV). The optimal sample size in this case is of the order of 50. μm. The chemical compositions of the minerals, including the Fe/Mg ratios of ferromagnesian minerals and the Na/Ca ratios of plagioclase, were measured. This new method is potentially applicable to other small samples such as cosmic dust, lunar regolith, cometary dust (recovered by the Stardust mission of the National Aeronautics and Space Administration [NASA]), and samples from extraterrestrial bodies (those from future sample return missions such as the JAXA Hayabusa2 mission and the NASA OSIRIS-REx mission), although limitations exist for unequilibrated samples. Further, this technique is generally suited for studying materials in multicomponent systems with multiple phases across several research fields.
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U2 - 10.1016/j.gca.2012.11.036
DO - 10.1016/j.gca.2012.11.036
M3 - Article
AN - SCOPUS:84880596898
SN - 0016-7037
VL - 116
SP - 5
EP - 16
JO - Geochimica et Cosmochimica Acta
JF - Geochimica et Cosmochimica Acta
ER -