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pubmed-article:17611536rdf:typepubmed:Citationlld:pubmed
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pubmed-article:17611536pubmed:issue7149lld:pubmed
pubmed-article:17611536pubmed:dateCreated2007-7-5lld:pubmed
pubmed-article:17611536pubmed:abstractTextHyperion, Saturn's eighth largest icy satellite, is a body of irregular shape in a state of chaotic rotation. The surface is segregated into two distinct units. A spatially dominant high-albedo unit having the strong signature of H2O ice contrasts with a unit that is about a factor of four lower in albedo and is found mostly in the bottoms of cup-like craters. Here we report observations of Hyperion's surface in the ultraviolet and near-infrared spectral regions with two optical remote sensing instruments on the Cassini spacecraft at closest approach during a fly-by on 25-26 September 2005. The close fly-by afforded us the opportunity to obtain separate reflectance spectra of the high- and low-albedo surface components. The low-albedo material has spectral similarities and compositional signatures that link it with the surface of Phoebe and a hemisphere-wide superficial coating on Iapetus.lld:pubmed
pubmed-article:17611536pubmed:languageenglld:pubmed
pubmed-article:17611536pubmed:journalhttp://linkedlifedata.com/r...lld:pubmed
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pubmed-article:17611536pubmed:authorpubmed-author:StephanKKlld:pubmed
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pubmed-article:17611536pubmed:authorpubmed-author:Dalle OreC...lld:pubmed
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pubmed-article:17611536pubmed:issnTypeElectroniclld:pubmed
pubmed-article:17611536pubmed:day5lld:pubmed
pubmed-article:17611536pubmed:volume448lld:pubmed
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pubmed-article:17611536pubmed:pagination54-6lld:pubmed
pubmed-article:17611536pubmed:year2007lld:pubmed
pubmed-article:17611536pubmed:articleTitleSurface composition of Hyperion.lld:pubmed
pubmed-article:17611536pubmed:affiliationNASA Ames Research Center, MS 245-6, NASA Ames Research Center, MS 211-3, Moffett Field, California 94035, USA. Dale.P.Cruikshank@nasa.govlld:pubmed
pubmed-article:17611536pubmed:publicationTypeJournal Articlelld:pubmed