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.

Data and Resources

This dataset has no data

Additional Info

Field Value
Maintainer Thomas Morgan
Last Updated April 1, 2025, 02:44 (UTC)
Created April 1, 2025, 02:44 (UTC)
accessLevel public
accrualPeriodicity irregular
bureauCode {026:00}
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harvest_object_id b240e01e-d9ce-46c0-9dc3-3db51d0540c6
harvest_source_id 61638e72-b36c-4866-9d28-551a3062f158
harvest_source_title DNG Legacy Data
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
modified 2023-01-26
programCode {026:005}
publisher National Aeronautics and Space Administration
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resource-type Dataset
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