小行星
航天器
天体生物学
天文
地质学
物理
大地测量学
天体物理学
作者
D. K. Yeomans,Peter G. Antreasian,A. F. Cheng,David Dunham,Robert W. Farquhar,R. W. Gaskell,Jon D. Giorgini,C. E. Helfrich,A. S. Konopliv,James McAdams,James Miller,W. M. Owen,P. C. Thomas,J. Veverka,B. G. Williams
出处
期刊:Science
[American Association for the Advancement of Science]
日期:1999-07-23
卷期号:285 (5427): 560-561
被引量:59
标识
DOI:10.1126/science.285.5427.560
摘要
The Near Earth Asteroid Rendezvous (NEAR) spacecraft flew within 3830 kilometers of asteroid 433 Eros on 23 December 1998. The gravitational perturbation on NEAR was evident in the spacecraft tracking data. Ground-based Doppler and range tracking of the spacecraft as well as spacecraft images of the asteroid's center of figure and surface features were used to determine the mass and rotation pole of Eros. The mass of Eros is (7.2 +/- 1.8) x 10(18) grams and, coupled with a volume estimate provided by the NEAR imaging team, this mass suggests a bulk density of 2.5 +/- 0.8 grams per cubic centimeter. The rotation pole position is 15.6 (+/-3.7) degrees in right ascension and 16.4 (+/-1.8) degrees in declination, which is consistent with ground-based and NEAR imaging team observations.
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