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The north polar lakes of Titan as observed by Cassini Radar
hal.structure.identifier | Jet Propulsion Laboratory [JPL] | |
dc.contributor.author | MITCHELL, K. L. | |
hal.structure.identifier | Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB] | |
hal.structure.identifier | Observatoire aquitain des sciences de l'univers [OASU] | |
hal.structure.identifier | Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB] | |
hal.structure.identifier | Université Sciences et Technologies - Bordeaux 1 [UB] | |
dc.contributor.author | PAILLOU, Philippe | |
hal.structure.identifier | US Geological Survey [Flagstaff] | |
dc.contributor.author | KIRK, R. L. | |
hal.structure.identifier | Lunar and Planetary Laboratory [Tucson] [LPL] | |
dc.contributor.author | LUNINE, J.I. | |
hal.structure.identifier | Proxemy Research Inc | |
dc.contributor.author | STOFAN, E. R. | |
hal.structure.identifier | Lunar and Planetary Laboratory [Tucson] [LPL] | |
dc.contributor.author | RADEBAUGH, J. | |
hal.structure.identifier | Jet Propulsion Laboratory [JPL] | |
dc.contributor.author | WALL, S. D. | |
hal.structure.identifier | Division of Geological and Planetary Sciences [Pasadena] | |
dc.contributor.author | HAYES, A. G. | |
hal.structure.identifier | Jet Propulsion Laboratory [JPL] | |
dc.contributor.author | LOPES, R. M. | |
hal.structure.identifier | Jet Propulsion Laboratory [JPL] | |
dc.contributor.author | STILES, B. W. | |
hal.structure.identifier | Jet Propulsion Laboratory [JPL] | |
dc.contributor.author | OSTRO, S. J. | |
hal.structure.identifier | Johns Hopkins University Applied Physics Laboratory [Laurel, MD] [APL] | |
dc.contributor.author | LORENZ, R. D. | |
hal.structure.identifier | Wheeling Jesuit University | |
dc.contributor.author | WOOD, C. A. | |
dc.contributor.author | CASSINI RADAR TEAM | |
dc.date.conference | 2007 | |
dc.description.abstractEn | Over the course of a year, Cassini RADAR obtained Synthetic Aperture Radar images covering 69 percent of Titan's polar region north of 65 degrees; the region being 1.4E6 km3 in extent, greater than double the land area of the USA. We observe several hundred lakes with a range of morphological expression, including areally massive and morphologically distinctive "seas", covering ~15% of the polar region. Lakes are extremely radar dark, consistent with a lossy liquid hydrocarbon. Preliminary laboratory estimates suggest that loss tangents in the range 10E4 to 2x10E3 are reasonable, which implies that one can see through at least a few to many tens of m of liquids before the noise floor is reached, consistent with observed brightening towards many lake shores. North polar lake volumes are most likely in the 8E3 - 1.4E6 km3 range. Uncertainties will be reduced as more data, both image-based and experimental, are obtained but we can conclude with a high degree of confidence that hydrocarbon lakes on Titan are more voluminous than known terrestrial oil reserves; current estimates range from 2248 - 3896 billion barrels of oil (J. Hakes, 2000, Long Term World Oil Supply, Meeting of the Am. Ass. Pet. Geol., 18th April 2000, New Orleans, LA, http://www.eia.doe.gov/pub/oil_gas/petroleum/presentations/2000/long_term_supply.), hence 357 - 619 km3 . Small lakes often occupy steep-sided depressions, and although thermal and cryovolcanic origins cannot be completely ruled out, we are seeing growing geomorphologic evidence for dissolution chemistry, indicative of karst-like geology. The dichotomy between small lakes over slightly more than one half of the region, and seas on the other half, may be best explained by a topographic anomaly causing sub-surface flow of materials from the lakes to the seas. This may also explain observations by the Cassini ISS team (E. Turtle et al., in prep.) of a putative massive sea extending considerably further south than other observed north polar lakes. | |
dc.language.iso | en | |
dc.subject.en | 9345 Large bodies of water (e.g. | |
dc.subject.en | 2400 IONOSPHERE (6929) | |
dc.subject.en | 2419 Ion chemistry and composition (0335) | |
dc.subject.en | 9345 Large bodies of water (e.g | |
dc.subject.en | lakes and inland seas) (0746) | |
dc.title.en | The north polar lakes of Titan as observed by Cassini Radar | |
dc.type | Communication dans un congrès | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP] | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP] | |
bordeaux.country | FR | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-00405463 | |
hal.version | 1 | |
hal.invited | non | |
hal.proceedings | non | |
hal.popular | non | |
hal.audience | Non spécifiée | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-00405463v1 | |
bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.au=MITCHELL,%20K.%20L.&PAILLOU,%20Philippe&KIRK,%20R.%20L.&LUNINE,%20J.I.&STOFAN,%20E.%20R.&rft.genre=unknown |
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