JPL Technical Report Server

Ultraviolet Spectra and Geometric Albedos of 45 Asteroids

Show simple item record

dc.contributor.author Roettger, E. en_US
dc.contributor.author Buratti, B. en_US
dc.date.accessioned 2004-10-05T05:42:08Z
dc.date.available 2004-10-05T05:42:08Z
dc.date.issued 1994
dc.identifier.clearanceno 94-1242
dc.identifier.uri http://hdl.handle.net/2014/33303
dc.description.abstract Spectral reflectances and geometric albedos between 2300 and 3250 Angstroms are determined for 45 asteroids from data acquired by the International Ultraviolet Explorer satellite. The geometric albedos are consistently low, ranging from ~0.02 for C-type asteroids to ~0.08 for M-type asteroids. An exception is the single E-type asteriod (44 Nysa) with a geometric albedo of 0.3 at 2950 Angstroms. We find that the three major asteroid taxonomic classes persist into the UV. The taxonomic classes are distinguished primarily by their albedos, but S-types are generally redder than C- or M-types. The first ultraviolet phase curves of asteroids are presented. en_US
dc.format.extent 1781480 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other International Ultraviolet Explorer en_US
dc.title Ultraviolet Spectra and Geometric Albedos of 45 Asteroids en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account