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Cassini RADAR images at Hotei Arcus and western Xanadu, Titan: Evidence for geologically recent cryovolcanic activity

hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorWALL, S. D.
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorLOPES, R. M.
hal.structure.identifierProxemy Research Inc
dc.contributor.authorSTOFAN, E. R.
hal.structure.identifierWheeling Jesuit University
dc.contributor.authorWOOD, C. A.
hal.structure.identifierLunar and Planetary Laboratory [Tucson] [LPL]
dc.contributor.authorRADEBAUGH, J. L.
hal.structure.identifierDepartment of Planetary Sciences [Tucson]
dc.contributor.authorHÖRST, S. M.
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorSTILES, B. W.
hal.structure.identifierQueen Mary University of London [QMUL]
dc.contributor.authorNELSON, R. M.
dc.contributor.authorKAMP, L. W.
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorJANSSEN, M. A.
hal.structure.identifierJohns Hopkins University Applied Physics Laboratory [Laurel, MD] [APL]
dc.contributor.authorLORENZ, R. D.
hal.structure.identifierLunar and Planetary Laboratory [Tucson] [LPL]
dc.contributor.authorLUNINE, J.I.
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorFARR, T. G.
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorMITRI, G.
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.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorPAGANELLI, F.
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorMITCHELL, K. L.
dc.date.issued2009-02
dc.identifier.issn0094-8276
dc.description.abstractEnImages obtained by the Cassini Titan Radar Mapper (RADAR) reveal lobate, flowlike features in the Hotei Arcus region that embay and cover surrounding terrains and channels. We conclude that they are cryovolcanic lava flows younger than surrounding terrain, although we cannot reject the sedimentary alternative. Their appearance is grossly similar to another region in western Xanadu and unlike most of the other volcanic regions on Titan. Both regions correspond to those identified by Cassini's Visual and Infrared Mapping Spectrometer (VIMS) as having variable infrared brightness, strengthening the case that these are recent cryovolcanoes.
dc.language.isoen
dc.publisherAmerican Geophysical Union
dc.rights.urihttp://hal.archives-ouvertes.fr/licences/copyright/
dc.subject.enMarine Geology and Geophysics: Submarine tectonics and volcanism
dc.subject.enPlanetary Sciences: Solid Surface Planets: Origin and evolution
dc.title.enCassini RADAR images at Hotei Arcus and western Xanadu, Titan: Evidence for geologically recent cryovolcanic activity
dc.typeArticle de revue
dc.identifier.doi10.1029/2008GL036415
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.subject.halPlanète et Univers [physics]/Sciences de la Terre/Volcanologie
bordeaux.journalGeophysical Research Letters
bordeaux.page04203
bordeaux.volume36
bordeaux.issue4
bordeaux.peerReviewedoui
hal.identifierhal-00405364
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00405364v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Geophysical%20Research%20Letters&rft.date=2009-02&rft.volume=36&rft.issue=4&rft.spage=04203&rft.epage=04203&rft.eissn=0094-8276&rft.issn=0094-8276&rft.au=WALL,%20S.%20D.&LOPES,%20R.%20M.&STOFAN,%20E.%20R.&WOOD,%20C.%20A.&RADEBAUGH,%20J.%20L.&rft.genre=article


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