Detailed Images of Asteroid 25143 Itokawa from Hayabusa.

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Title: Detailed Images of Asteroid 25143 Itokawa from Hayabusa.
Authors: Saito, J., Miyamoto, H., Nakamura, R., Ishiguro, M., Michikami, T., Nakamura, A. M., Demura, H., Sasaki, S., Hirata, N., Honda, C., Yamamoto, A., Yokota, Y., Fuse, T., Yoshida, F., Tholen, D. J., Gaskell, R. W., Hashimoto, T., Kubota, T., Higuchi, Y., Nakamura, T.
Source: Science (pre-March 2025). 6/2/2006, Vol. 312 Issue 5778, p1341-1344. 4p.
Subjects: Near-earth asteroids, Space vehicles, Optical resolution, Cratering, Microstructure, Boulders, Geometric surfaces, Rubble, Solar system
Abstract: Rendezvous of the Japanese spacecraft Hayabusa with the near-Earth asteroid 25143 Itokawa took place during the interval September through November 2005. The onboard camera imaged the solid surface of this tiny asteroid (535 meters by 294 meters by 209 meters) with a spatial resolution of 70 centimeters per pixel, revealing diverse surface morphologies. Unlike previously explored asteroids, the surface of Itokawa reveals both rough and smooth terrains. Craters generally show unclear morphologies. Numerous boulders on Itokawa's surface suggest a rubble-pile structure. [ABSTRACT FROM AUTHOR]
Copyright of Science (pre-March 2025) is the property of American Association for the Advancement of Science and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
Database: Psychology and Behavioral Sciences Collection
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  Data: Detailed Images of Asteroid 25143 Itokawa from Hayabusa.
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  Data: <searchLink fieldCode="AR" term="%22Saito%2C+J%2E%22">Saito, J.</searchLink><br /><searchLink fieldCode="AR" term="%22Miyamoto%2C+H%2E%22">Miyamoto, H.</searchLink><br /><searchLink fieldCode="AR" term="%22Nakamura%2C+R%2E%22">Nakamura, R.</searchLink><br /><searchLink fieldCode="AR" term="%22Ishiguro%2C+M%2E%22">Ishiguro, M.</searchLink><br /><searchLink fieldCode="AR" term="%22Michikami%2C+T%2E%22">Michikami, T.</searchLink><br /><searchLink fieldCode="AR" term="%22Nakamura%2C+A%2E+M%2E%22">Nakamura, A. M.</searchLink><br /><searchLink fieldCode="AR" term="%22Demura%2C+H%2E%22">Demura, H.</searchLink><br /><searchLink fieldCode="AR" term="%22Sasaki%2C+S%2E%22">Sasaki, S.</searchLink><br /><searchLink fieldCode="AR" term="%22Hirata%2C+N%2E%22">Hirata, N.</searchLink><br /><searchLink fieldCode="AR" term="%22Honda%2C+C%2E%22">Honda, C.</searchLink><br /><searchLink fieldCode="AR" term="%22Yamamoto%2C+A%2E%22">Yamamoto, A.</searchLink><br /><searchLink fieldCode="AR" term="%22Yokota%2C+Y%2E%22">Yokota, Y.</searchLink><br /><searchLink fieldCode="AR" term="%22Fuse%2C+T%2E%22">Fuse, T.</searchLink><br /><searchLink fieldCode="AR" term="%22Yoshida%2C+F%2E%22">Yoshida, F.</searchLink><br /><searchLink fieldCode="AR" term="%22Tholen%2C+D%2E+J%2E%22">Tholen, D. J.</searchLink><br /><searchLink fieldCode="AR" term="%22Gaskell%2C+R%2E+W%2E%22">Gaskell, R. W.</searchLink><br /><searchLink fieldCode="AR" term="%22Hashimoto%2C+T%2E%22">Hashimoto, T.</searchLink><br /><searchLink fieldCode="AR" term="%22Kubota%2C+T%2E%22">Kubota, T.</searchLink><br /><searchLink fieldCode="AR" term="%22Higuchi%2C+Y%2E%22">Higuchi, Y.</searchLink><br /><searchLink fieldCode="AR" term="%22Nakamura%2C+T%2E%22">Nakamura, T.</searchLink>
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  Data: <searchLink fieldCode="JN" term="%22Science+%28pre-March+2025%29%22">Science (pre-March 2025)</searchLink>. 6/2/2006, Vol. 312 Issue 5778, p1341-1344. 4p.
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  Data: <searchLink fieldCode="DE" term="%22Near-earth+asteroids%22">Near-earth asteroids</searchLink><br /><searchLink fieldCode="DE" term="%22Space+vehicles%22">Space vehicles</searchLink><br /><searchLink fieldCode="DE" term="%22Optical+resolution%22">Optical resolution</searchLink><br /><searchLink fieldCode="DE" term="%22Cratering%22">Cratering</searchLink><br /><searchLink fieldCode="DE" term="%22Microstructure%22">Microstructure</searchLink><br /><searchLink fieldCode="DE" term="%22Boulders%22">Boulders</searchLink><br /><searchLink fieldCode="DE" term="%22Geometric+surfaces%22">Geometric surfaces</searchLink><br /><searchLink fieldCode="DE" term="%22Rubble%22">Rubble</searchLink><br /><searchLink fieldCode="DE" term="%22Solar+system%22">Solar system</searchLink>
– Name: Abstract
  Label: Abstract
  Group: Ab
  Data: Rendezvous of the Japanese spacecraft Hayabusa with the near-Earth asteroid 25143 Itokawa took place during the interval September through November 2005. The onboard camera imaged the solid surface of this tiny asteroid (535 meters by 294 meters by 209 meters) with a spatial resolution of 70 centimeters per pixel, revealing diverse surface morphologies. Unlike previously explored asteroids, the surface of Itokawa reveals both rough and smooth terrains. Craters generally show unclear morphologies. Numerous boulders on Itokawa's surface suggest a rubble-pile structure. [ABSTRACT FROM AUTHOR]
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  Data: <i>Copyright of Science (pre-March 2025) is the property of American Association for the Advancement of Science and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1126/science.1125722
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        Text: English
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        Type: general
      – SubjectFull: Space vehicles
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      – SubjectFull: Optical resolution
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