메뉴 건너뛰기




Volumn 312, Issue 5778, 2006, Pages 1341-1344

Detailed images of asteroid 25143 Itokawa from Hayabusa

(34)  Saito, J a,b   Miyamoto, H c,d   Nakamura, R e   Ishiguro, M a   Michikami, T f   Nakamura, A M g   Demura, H h   Sasaki, S i   Hirata, N g,h   Honda, C a   Yamamoto, A j   Yokota, Y a   Fuse, T i   Yoshida, F i   Tholen, D J k   Gaskell, R W l   Hashimoto, T a   Kubota, T a   Higuchi, Y m   Nakamura, T i   more..


Author keywords

[No Author keywords available]

Indexed keywords

ASTROPHYSICS; CAMERAS; OPTICAL RESOLVING POWER; SPACECRAFT; SURFACES;

EID: 33744786807     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1125722     Document Type: Article
Times cited : (239)

References (28)
  • 1
    • 33744808559 scopus 로고    scopus 로고
    • A. Fujiwara et al., Science 312, 1330 (2006).
    • (2006) Science , vol.312 , pp. 1330
    • Fujiwara, A.1
  • 3
    • 28444489698 scopus 로고    scopus 로고
    • A. Cellino et al., Icarus 179, 297 (2005).
    • (2005) Icarus , vol.179 , pp. 297
    • Cellino, A.1
  • 6
    • 33744782381 scopus 로고    scopus 로고
    • note
    • A test polarimetric observation at a solar phase angle of ∼10° was conducted during the earlier rendezvous phase; however, subsequent observations were canceled because of problems with the system's attitude control.
  • 7
    • 33744799499 scopus 로고    scopus 로고
    • note
    • A search for Itokawa's satellites was performed at a distance of about 1000 km. The field-of-view of AMICA was about 100 km by 100 km around Itokawa, and it fully covered the Hill sphere (∼40 km in radius). The limiting V-magnitude was about 9.5, corresponding to objects of less than ∼1 m in diameter. Preliminary analysis showed no bright satellite candidate.
  • 8
    • 0036252415 scopus 로고    scopus 로고
    • L. Prockter et al., Icarus 155, 75 (2002).
    • (2002) Icarus , vol.155 , pp. 75
    • Prockter, L.1
  • 10
    • 33744815293 scopus 로고    scopus 로고
    • note
    • The slope of the bulk population would be somewhat steeper (0.2 to 0.3) than that of the surface population. See (26).
  • 15
    • 0036250996 scopus 로고    scopus 로고
    • C. R. Chapman et al., Icarus 155, 104 (2002).
    • (2002) Icarus , vol.155 , pp. 104
    • Chapman, C.R.1
  • 16
    • 0036252250 scopus 로고    scopus 로고
    • S. Murchie et al., Icarus 155, 145 (2002).
    • (2002) Icarus , vol.155 , pp. 145
    • Murchie, S.1
  • 18
    • 16144367496 scopus 로고    scopus 로고
    • J. Veverka et al., Icarus 120, 66 (1996).
    • (1996) Icarus , vol.120 , pp. 66
    • Veverka, J.1
  • 23
    • 0141899672 scopus 로고    scopus 로고
    • W. Bottke et al., Eds. (Univ. of Arizona Press, Tucson)
    • B. E. Clark, B. Hapke, C. Pieters, D. Britt, in Asteroids III, W. Bottke et al., Eds. (Univ. of Arizona Press, Tucson, 2002), pp. 585-599.
    • (2002) Asteroids III , pp. 585-599
    • Clark, B.E.1    Hapke, B.2    Pieters, C.3    Britt, D.4
  • 25
    • 33744827172 scopus 로고    scopus 로고
    • note
    • Gravitational sliding of regolith materials with different brightnesses was also observed on Eros. See (27).
  • 27
    • 0036247395 scopus 로고    scopus 로고
    • P. C. Thomas et al., Icarus 155, 18 (2002).
    • (2002) Icarus , vol.155 , pp. 18
    • Thomas, P.C.1
  • 28
    • 33744824158 scopus 로고    scopus 로고
    • note
    • We thank the mission operation and spacecraft team of the Hayabusa project at ISAS/JAXA for their efforts that led to Hayabusa being the first Japanese spacecraft to rendezvous with and land on the asteroid. This research was supported by ISAS/JAXA, NASA, Kobe University through "The 21st Century Center of Excellence Program of the Origin and Evolution of Planetary Systems," and the University of Aizu.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.