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The shape of 433 Eros from the NEAR-shoemaker laser Rangefinder

Author
ZUBER, Maria T1 2 ; SMITH, David E2 ; ROWLANDS, David D1 2 ; TORRENCE, Mark H4 ; CHENG, Andrew F3 ; GARVIN, James B2 ; AHARONSON, Oded1 ; COLE, Timothy D3 ; DUNN, Peter J4 ; YANPING GUO3 ; LEMOINE, Frank G2 ; NEUMANN, Gregory A2
[1] Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, United States
[2] Earth Sciences Directorate, NASA-Goddard Space Flight Center, Greenbelt, MD 20771, United States
[3] Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723-6099, United States
[4] Raytheon Information Technology and Scientific Services, Landover, MD 20771, United States
Source

Science (Washington, D.C.). 2000, Vol 289, Num 5487, pp 2097-2101 ; Illustration , Table

CODEN
SCIEAS
ISSN
0036-8075
Scientific domain
Multidisciplinary
Publisher
American Association for the Advancement of Science, Washington, DC
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Astéroïde Cannelure Champ gravimétrique Cratère impact Cratère météoritique Fracturation Géodésie Impact Linéation Morphologie Relief Topographie Astéroïde Eros 433 Collision NEAR Structure interne
Keyword (en)
asteroids grooves gravity field impact craters meteor craters fracturing geodesy impacts lineation morphology relief topography
Keyword (es)
Asteroide Campo gravitatorio Fracturación Geodesia Lineación Morfología Topografía
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E01 Earth sciences / 001E01D Cosmochemistry. Extraterrestrial geology / 001E01D01 Extraterrestrial geology

Discipline
Earth sciences
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
1500545

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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