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SMASS ASTEROID SURVEY V1.0
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.
Complete Metadata
| bureauCode |
[ "026:00" ] |
|---|---|
| identifier | urn:nasa:pds:context_pds3:data_set:data_set.ear-a-m3spec-3-rdr-smass-v1.0_xpr2-xb6p |
| issued | 2018-06-26 |
| landingPage | https://pds.nasa.gov/ds-view/pds/viewDataset.jsp?dsid=EAR-A-M3SPEC-3-RDR-SMASS-V1.0 |
| programCode |
[ "026:005" ] |
| references |
[ "https://pds.nasa.gov" ] |
| theme |
[ "Earth Science" ] |
