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The Shape of 433 Eros from the NEAR-Shoemaker Laser Rangefinder
Maria T. Zuber,12*David E. Smith,2Andrew F. Cheng,3James B. Garvin,2Oded Aharonson,1Timothy D. Cole,3Peter J. Dunn,4Yanping Guo,3Frank G. Lemoine,2Gregory A. Neumann,12David D. Rowlands,2Mark H. Torrence4
Measurements from the Near Earth Asteroid Rendezvous
(NEAR)-Shoemaker Laser Rangefinder (NLR) indicate that asteroid
433 Erosis a consolidated body with a complex shape dominated by
collisions.The offset between the asteroid's center of mass and
center offigure indicates a small deviation from a homogeneous
internalstructure that is most simply explained by variations in
mechanicalstructure. Regional-scale relief and slope distributions
showevidence for control of topography by a competent substrate.
Impactcrater morphology is influenced by both gravity and structuralcontrol. Small-scale topography reveals ridges and grooves thatmay be
generated by impact-related fracturing.
1 Department of Earth, Atmospheric, and
Planetary Sciences, Massachusetts Institute of Technology, Cambridge,
MA 02139, USA.
2 Earth Sciences Directorate,
NASA-Goddard Space Flight Center, Greenbelt, MD 20771, USA.
3 Johns Hopkins University Applied Physics
Laboratory, Laurel, MD 20723-6099, USA.
4 Raytheon
Information Technology and Scientific Services, Landover, MD 20771, USA.
*
To whom correspondence should be addressed. E-mail:
zuber{at}mit.edu
The editors suggest the following Related Resources on Science sites:
In Science Magazine
PERSPECTIVES
Richard P. Binzel (22 September 2000) Science289 (5487), 2065.
[DOI: 10.1126/science.289.5487.2065] |Summary »|Full Text »
REPORTS
D. K. Yeomans, P. G. Antreasian, J.-P. Barriot, S. R. Chesley, D. W. Dunham, R. W. Farquhar, J. D. Giorgini, C. E. Helfrich, A. S. Konopliv, J. V. McAdams, J. K. Miller, W. M. Owen, Jr., D. J. Scheeres, P. C. Thomas, J. Veverka, and B. G. Williams (22 September 2000) Science289 (5487), 2085.
[DOI: 10.1126/science.289.5487.2085] |Abstract »|Full Text »|PDF »
REPORTS
J. Veverka, M. Robinson, P. Thomas, S. Murchie, J. F. Bell, III, N. Izenberg, C. Chapman, A. Harch, M. Bell, B. Carcich, A. Cheng, B. Clark, D. Domingue, D. Dunham, R. Farquhar, M. J. Gaffey, E. Hawkins, J. Joseph, R. Kirk, H. Li, P. Lucey, M. Malin, P. Martin, L. McFadden, W. J. Merline, J. K. Miller, W. M. Owen, Jr., C. Peterson, L. Prockter, J. Warren, D. Wellnitz, B. G. Williams, and D. K. Yeomans (22 September 2000) Science289 (5487), 2088.
[DOI: 10.1126/science.289.5487.2088] |Abstract »|Full Text »|PDF »
REPORTS
J. I. Trombka, S. W. Squyres, J. Brückner, W. V. Boynton, R. C. Reedy, T. J. McCoy, P. Gorenstein, L. G. Evans, J. R. Arnold, R. D. Starr, L. R. Nittler, M. E. Murphy, I. Mikheeva, R. L. McNutt, Jr., T. P. McClanahan, E. McCartney, J. O. Goldsten, R. E. Gold, S. R. Floyd, P. E. Clark, T. H. Burbine, J. S. Bhangoo, S. H. Bailey, and M. Petaev (22 September 2000) Science289 (5487), 2101.
[DOI: 10.1126/science.289.5487.2101] |Abstract »|Full Text »|PDF »
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