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A&A 417, L21-L24 (2004)
DOI: 10.1051/0004-6361:20040027
Letter
VLT/NACO adaptive optics imaging of Titan
E. Gendron1, A. Coustenis1, P. Drossart1, M. Combes1, M. Hirtzig1, F. Lacombe1, D. Rouan1, C. Collin1, S. Pau1, A-M. Lagrange2, D. Mouillet2, P. Rabou2, T. Fusco3 and G. Zins41 Observatoire de Paris, LESIA, UMR 8109 du CNRS, 5 place Jules Janssen, 92195 Meudon Cedex, France
2 Laboratoire d'Astrophysique, Observatoire de Grenoble, BP 53, 38041 Grenoble, France
3 ONERA - DOTA, 92322 Châtillon, France
4 ESO, Karl-Schwarzschild -Str. 2, 85748 Garching bei München, Germany
( Received 18 March 2003 / Accepted 17 January 2004)
Abstract
The advent of the NAOS/CONICA adaptive optics system at the ESO Very Large
Telescope recently gave us the opportunity
to map the surface of Titan
and to search for atmospheric variations at high spatial resolution
and contrast. We report here the first results from a series of
observations of Titan performed with this instrument in a number of
near-infrared narrow-band filters, covering various
altitude regions and three different longitudes
(out of the 16 days of Titan's orbit). We have achieved unequaled contrast on
images showing complex topography on Titan's trailing hemisphere and
have found robust evidence for the north-south asymmetry inversion.
The presence of other interesting
atmospheric features at Titan's South Pole is described.
Key words: instrumentation: adaptive optics -- planets and satellites: individual: Titan -- infrared: solar system
Offprint request: E. Gendron, Eric.Gendron@obspm.fr
© ESO 2004
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