pubmed-article:17611536 | rdf:type | pubmed:Citation | lld:pubmed |
pubmed-article:17611536 | lifeskim:mentions | umls-concept:C0672770 | lld:lifeskim |
pubmed-article:17611536 | lifeskim:mentions | umls-concept:C0205148 | lld:lifeskim |
pubmed-article:17611536 | lifeskim:mentions | umls-concept:C0486616 | lld:lifeskim |
pubmed-article:17611536 | pubmed:issue | 7149 | lld:pubmed |
pubmed-article:17611536 | pubmed:dateCreated | 2007-7-5 | lld:pubmed |
pubmed-article:17611536 | pubmed:abstractText | Hyperion, 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:17611536 | pubmed:language | eng | lld:pubmed |
pubmed-article:17611536 | pubmed:journal | http://linkedlifedata.com/r... | lld:pubmed |
pubmed-article:17611536 | pubmed:status | PubMed-not-MEDLINE | lld:pubmed |
pubmed-article:17611536 | pubmed:month | Jul | lld:pubmed |
pubmed-article:17611536 | pubmed:issn | 1476-4687 | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:StephanKK | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:NelsonR MRM | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:BauerJJ | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:BellucciGG | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:BaileyM JMJ | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:CruikshankD... | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:BrownR HRH | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:TossLL | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:ClarkR NRN | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:HansenC JCJ | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:CombeyWW | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:DaltonJ BJB | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:JaumannRR | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:MeyerA WAW | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:SicardiRR | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:MatsonD LDL | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:FormisanoVV | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:DrossartPP | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:McCordT BTB | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:HendrixA RAR | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:MennellaVV | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:NicholsonP... | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:CerroniPP | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:LangevinYY | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:BurattiB JBJ | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:CoradiniAA | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:BibringJ-PJP | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:CapaccioniFF | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:SotinCC | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:Dalle OreC... | lld:pubmed |
pubmed-article:17611536 | pubmed:author | pubmed-author:FilacchioneGG | lld:pubmed |
pubmed-article:17611536 | pubmed:issnType | Electronic | lld:pubmed |
pubmed-article:17611536 | pubmed:day | 5 | lld:pubmed |
pubmed-article:17611536 | pubmed:volume | 448 | lld:pubmed |
pubmed-article:17611536 | pubmed:owner | NLM | lld:pubmed |
pubmed-article:17611536 | pubmed:authorsComplete | Y | lld:pubmed |
pubmed-article:17611536 | pubmed:pagination | 54-6 | lld:pubmed |
pubmed-article:17611536 | pubmed:year | 2007 | lld:pubmed |
pubmed-article:17611536 | pubmed:articleTitle | Surface composition of Hyperion. | lld:pubmed |
pubmed-article:17611536 | pubmed:affiliation | NASA Ames Research Center, MS 245-6, NASA Ames Research Center, MS 211-3, Moffett Field, California 94035, USA. Dale.P.Cruikshank@nasa.gov | lld:pubmed |
pubmed-article:17611536 | pubmed:publicationType | Journal Article | lld:pubmed |