The landing of the NEAR-Shoemaker spacecraft on asteroid 433 Eros

被引:0
|
作者
J. Veverka
B. Farquhar
M. Robinson
P. Thomas
S. Murchie
A. Harch
P. G. Antreasian
S. R. Chesley
J. K. Miller
W. M. Owen
B. G. Williams
D. Yeomans
D. Dunham
G. Heyler
M. Holdridge
R. L. Nelson
K. E. Whittenburg
J. C. Ray
B. Carcich
A. Cheng
C. Chapman
J. F. Bell
M. Bell
B. Bussey
B. Clark
D. Domingue
M. J. Gaffey
E. Hawkins
N. Izenberg
J. Joseph
R. Kirk
P. Lucey
M. Malin
L. McFadden
W. J. Merline
C. Peterson
L. Prockter
J. Warren
D. Wellnitz
机构
[1] Space Sciences Building,Department of Geological Sciences
[2] Cornell University,Department of Earth and Environmental Sciences
[3] Applied Physics Laboratory,Department of Astronomy
[4] Johns Hopkins University,undefined
[5] Northwestern University,undefined
[6] 309 Locy Hall,undefined
[7] Jet Propulsion Laboratory,undefined
[8] Southwest Research Institute,undefined
[9] Science Center,undefined
[10] Rensselaer Polytechnic Institute,undefined
[11] US Geological Survey,undefined
[12] Hawaii Institute of Geophysics and Planetology,undefined
[13] University of Hawaii,undefined
[14] Malin Space Science Systems,undefined
[15] Inc.,undefined
[16] University of Maryland,undefined
来源
Nature | 2001年 / 413卷
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摘要
The NEAR-Shoemaker spacecraft was designed to provide a comprehensive characterization of the S-type asteroid 433 Eros (refs 1,2,3), an irregularly shaped body with approximate dimensions of 34 × 13 × 13 km. Following the completion of its year-long investigation, the mission was terminated with a controlled descent to its surface, in order to provide extremely high resolution images. Here we report the results of the descent on 12 February 2001, during which 70 images were obtained. The landing area is marked by a paucity of small craters and an abundance of ‘ejecta blocks’. The properties and distribution of ejecta blocks are discussed in a companion paper4. The last sequence of images reveals a transition from the blocky surface to a smooth area, which we interpret as a ‘pond’. Properties of the ‘ponds’ are discussed in a second companion paper5. The closest image, from an altitude of 129 m, shows the interior of a 100-m-diameter crater at 1-cm resolution.
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页码:390 / 393
页数:3
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