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Investigation of the Sinlap Crater on Titan Using VIMS and RADAR Data

hal.structure.identifierLaboratoire de Planétologie et Géodynamique [UMR 6112] [LPG]
dc.contributor.authorLE MOUÉLIC, S.
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorPAILLOU, Philippe
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorRODRIGUEZ, S.
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorCRAPEAU, M.
hal.structure.identifierLaboratoire de Planétologie et Géodynamique de Nantes [UMR 6112] [LPGN]
dc.contributor.authorSOTIN, C.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorHIRTZIG, M.
hal.structure.identifierLunar and Planetary Laboratory [Tucson] [LPL]
dc.contributor.authorBROWN, R. H.
hal.structure.identifierUS Geological Survey [Flagstaff]
dc.contributor.authorSODERBLOM, L. A.
hal.structure.identifierUS Geological Survey [Denver]
dc.contributor.authorCLARK, R. N.
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorBURATTI, B. J.
dc.date.created2006
dc.date.conference2006
dc.description.abstractEnFew impact craters have been observed so far on Titan by the CASSINI orbiter. A 80 km diameter crater (called Sinlap) has been observed by all three imaging instruments (ISS, VIMS and Radar). Observations at infrared and radar wavelengths provide very complementary information on the composition, topography and surface roughness of the surface materials. We first investigate the spectral characteristics of the Sinlap area using VIMS data, in order to map the spectral heterogeneities, highlighting the different compositional and physical characteristics of the materials excavated by the impact. These units are then compared to the radar observations acquired at T3. The differences between optical and radar properties are discussed in terms of composition and vertical heterogeneity
dc.language.isoen
dc.subject6094 Instruments and techniques
dc.subject6281 Titan
dc.subject6297 Instruments and techniques
dc.subject6094 Instruments and techniques
dc.title.enInvestigation of the Sinlap Crater on Titan Using VIMS and RADAR Data
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.conference.title2006AGUFM.P13A0156L - American Geophysical Union, Fall Meeting 2006, abstract #P13A-0156
bordeaux.countryUS
bordeaux.conference.citySan Francisco
bordeaux.peerReviewedoui
hal.identifierhal-00405534
hal.version1
hal.invitednon
hal.proceedingsnon
hal.popularnon
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00405534v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.au=LE%20MOU%C3%89LIC,%20S.&PAILLOU,%20Philippe&RODRIGUEZ,%20S.&CRAPEAU,%20M.&SOTIN,%20C.&rft.genre=unknown


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