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Forging Asteroid-Meteorite Relationships Through Reflectance SpectroscopyNear-infrared spectra were obtained for 196 asteroids as part of SMASSIR. SMASSIR focused on observing asteroids assumed to be one of the following: (1) olivine-rich, (2) objects with "Vesta-like spectra" (the "Vestoids"), and (3) postulated meteorite parent bodies.
Document ID
20000080717
Document Type
Conference Paper
Authors
Burbine, T. H. (Smithsonian Institution Washington, DC United States)
Binzel, R. P. (Massachusetts Inst. of Tech. Cambridge, MA United States)
Bus, S. J. (Massachusetts Inst. of Tech. Cambridge, MA United States)
Buchanan, P. C. (NASA Johnson Space Center Houston, TX United States)
Hinrichs, J. L. (Hawaii Univ. Honolulu, HI United States)
Meibom, A. (Hawaii Univ. Honolulu, HI United States)
Hiroi, T. (Brown Univ. Providence, RI United States)
Sunshine, J. M. (Science Applications International Corp. Chantilly, VA United States)
Date Acquired
August 19, 2013
Publication Date
March 1, 2000
Publication Information
Publication: Lunar and Planetary Science XXXI
Subject Category
Lunar and Planetary Science and Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle20000080557Analytic PrimaryLunar and Planetary Science XXXI