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dc.contributor.authorMASTROGIUSEPPE, Marco
dc.contributor.authorPOGGIALI, Valerio
hal.structure.identifierDivision of Geological and Planetary Sciences [Pasadena]
dc.contributor.authorHAYES, Alexander
hal.structure.identifierJohns Hopkins University Applied Physics Laboratory [Laurel, MD] [APL]
dc.contributor.authorLORENZ, Ralph
hal.structure.identifierLunar and Planetary Laboratory [Tucson] [LPL]
dc.contributor.authorLUNINE, Jonathan
dc.contributor.authorPICARDI, Giovanni
hal.structure.identifierDipartimento INFOCOM [Roma]
dc.contributor.authorSEU, Roberto
hal.structure.identifierAgenzia Spaziale Italiana [ASI]
dc.contributor.authorFLAMINI, Enrico
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorMITRI, Giuseppe
dc.contributor.authorNOTARNICOLA, Claudia
hal.structure.identifierSSE 2014
dc.contributor.authorPAILLOU, Philippe
hal.structure.identifierDepartment of Geophysics [Stanford]
hal.structure.identifierDepartment of Electrical Engineering [Stanford]
dc.contributor.authorZEBKER, Howard
dc.date.issued2014-03
dc.identifier.issn0094-8276
dc.description.abstractEnconstruct the depth profile--the bathymetry--of Titan's large sea Ligeia Mare from Cassini RADAR data collected during the 23 May 2013 (T91) nadir-looking altimetry flyby. We find the greatest depth to be about 160 m and a seabed slope that is gentler toward the northern shore, consistent with previously imaged shoreline morphologies. Low radio signal attenuation through the sea demonstrates that the liquid, for which we determine a loss tangent of 3 ± 1*10-5, is remarkably transparent, requiring a nearly pure methane-ethane composition, and further that microwave absorbing hydrocarbons, nitriles, and suspended particles be limited to less than the order of 0.1% of the liquid volume. Presence of nitrogen in the ethane-methane sea, expected based on its solubility and dominance in the atmosphere, is consistent with the low attenuation, but that of substantial dissolved polar species or suspended scatterers is not.
dc.language.isoen
dc.publisherAmerican Geophysical Union
dc.rights.urihttp://hal.archives-ouvertes.fr/licences/copyright/
dc.subject.enCassini
dc.subject.enRemote sensing
dc.subject.enPlanetary Sciences
dc.subject.enSolar System Objects
dc.subject.enTitan
dc.subject.enHydrology
dc.title.enThe bathymetry of a Titan sea
dc.typeArticle de revue
dc.identifier.doi10.1002/2013GL058618
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.journalGeophysical Research Letters
bordeaux.page1432-1437
bordeaux.volume41
bordeaux.peerReviewedoui
hal.identifierhal-00975219
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00975219v1
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