Estimating the mass of asteroid 433 Eros during the NEAR spacecraft flyby

Science

Volumn 285, Issue 5427, 1999, Pages 560-561

  Yeomans, D K ^a   Antreasian, P G ^a   Cheng, A ^b   Dunham, D W ^b   Farquhar, R W ^b   Gaskell, R W ^a   Giorgini, J D ^a   Helfrich, C E ^a   Konopliv, A S ^a   McAdams, J V ^b   Miller, J K ^a   Owen Jr , W M ^a   Thomas, P C ^c   Veverka, J ^c   Williams, B G ^a  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b JOHNS HOPKINS UNIVERSITY   (United States)

^c Department of Population Medicine and Diagnostic Sciences   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ASTEROID; GRAVITY ANOMALY; ROTATION;

ARTICLE; ASTRONOMY; ECHOLOCATION; IMAGE ANALYSIS; PRIORITY JOURNAL; SPACE FLIGHT;

ASTEROIDEA;

EID: 0033597899     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.285.5427.560     Document Type: Article

References (14)

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4. J. Veverka et al., ibid., p. 2109.
5. For an overview of the NEAR mission, see J. Astronaut. Sci. 43, 345 (1995). A science overview is given in the NEAR special issue of J. Geophys. Res. 102, 23695 (1997).
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13. B. Zellner, Icarus 28, 149 (1976).
14. We would like to acknowledge the technical assistance and helpful discussions provided by P.W. Chodas, A.B. Chamberlin, and M.S. Keesey, Important ground-based astrometric observations of Eros were provided by several observers including J. Ticha, M. Tichy, P. Shelus, T.J. Johnson, and J.G. Reis. A particularly accurate data set, reduced with respect to reference catalogs based on the Hipparcos star positions, was provided by C. Garradd (Loomberah, Australia) and by R. Stone and A. Monet at the U.S. Naval Observatory Flagstaff Station in Flagstaff, Arizona. A portion of the research reported here was done at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA.