Small Main-Belt Asteroid Survey V2.1

Details Small Main-Belt Asteroid Survey V2.1 Small Main-Belt Asteroid Survey V2.1

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996pdss..168.....x&link_type=abstract

NASA Planetary Data System, EAR-A-M3SPEC-3-RDR-SMASS-V2.1

Physics

Scientific paper

The Small Main-belt Asteroid Spectrographic Survey (SMASS) was initiated in 1990 with the goal of obtaining spectra over the visual wavelength region for a substantial number of small (D < 20 km) main-belt asteroids. Observations were primarily made using the 2.4 m Hiltner telescope, located at the Michigan-Dartmouth-MIT (MDM) Observatory on the southwest ridge of Kitt Peak in Arizona. A total of 316 asteroids were included in the survey. The data have been published in Xu, et al. (Icarus 115, 1-35, 1995) and in this data set.

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