Small Main-Belt Asteroid Spectroscopic Survey (SMASS)
The Small Main-belt Asteroid Spectrographic Survey (SMASS) consists of visible spectra of 316 small main-belt asteroids observed primarily with the 2.4 m Hiltner telescope, located at the Michigan-Dartmouth-MIT (MDM) Observatory on Kitt Peak in Arizona. The data have been published in Xu, et al. (Icarus 115, 1-35, 1995).Release Date: 2020-08-31
Data Set Info
|PDS4 version||urn:nasa:pds:gbo.ast.smass.spectra::1.0||Browse||Download (1.9 MB)|
|PDS3 version||EAR-A-M3SPEC-3-RDR-SMASS-V2.1||Browse||Download (1.8 MB)|
The PDS4 bundle was migrated from the PDS3 data set in August 2020. The data content is unchanged.
Use the following citation to reference this data set:
"Xu, S., Binzel, R.P., Burbine, T.H., and Bus, S.J. (2020). Small Main-Belt Asteroid Survey V1.0. urn:nasa:pds:gbo.ast.smass.spectra::1.0. NASA Planetary Data System; https://doi.org/10.26033/2qgx-r057."