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ReportsNear-Infrared Spectral Results of Asteroid Itokawa from the Hayabusa Spacecraft
The near-infrared spectrometer on board the Japanese Hayabusa spacecraft found a variation of more than 10% in albedo and absorption band depth in the surface reflectance of asteroid 25143 Itokawa. Spectral shape over the 1-micrometer absorption band indicates that the surface of this body has an olivine-rich mineral assemblage potentially similar to that of LL5 or LL6 chondrites. Diversity in the physical condition of Itokawa's surface appears to be larger than for other S-type asteroids previously explored by spacecraft, such as 433 Eros.
1 Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan.
2 Toho Gakuen University, 3-11 Heiwagaoka, Meito, Nagoya, Aichi 465-8515, Japan. 3 University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan. 4 Graduate School of Science and Technology, Kobe University, 1-1 Rokkodai, Nada, Kobe, Hyogo 657-8501, Japan. 5 Department of Geological Science, Brown University, Providence, RI 02912, USA. 6 MMT Observatory, Post Office Box 210065, University of Arizona, Tucson, AZ 85721, USA. 7 Department of Physics, Ithaca College, Ithaca, NY 14850, USA. 8 National Aeronautics and Space Administration, Lyndon B. Johnson Space Center, Houston, TX 77058, USA. 9 Department of Physics, California State University, 5500 University Parkway, San Bernardino, CA 92407, USA. 10 ESC Group/Hamilton Sundstrand, 2224 Bay Area Boulevard, Houston, TX 77058, USA.
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Science. ISSN 0036-8075 (print), 1095-9203 (online)