Singular regional brightening events on Titan as seen by Cassini/VIMS

Titan, the largest satellite of Saturn, is the only satellite in the solar system with a dense atmosphere. The close and continuous observations of Titan by the Cassini spacecraft, in orbit around Saturn since July 2004, bring us evidences that Titan tropo-sphere and low stratosphere experience an exotic, but complete meteorological cycle similar to the Earth hy-drological cycle, with hydrocarbons evaporation, con-densation in clouds, and rainfall. Cassini monitoring campaigns also demonstrate that Titan’s cloud cover-age and climate vary with latitude. Titan’s tropics, with globally weak meteorological activity and widespread dune fields, seem to be slightly more arid than the poles, where extensive and numerous liquid reservoirs and sustained cloud activity were discovered. Only a few tropospheric clouds have been observed at Titan’s tropics during the southern summer [2-4]. As equinox was approaching (in August 2009), they oc-curred more frequently and appeared to grow in strength and size [5-7]

Studying Small Solar System Objects with Adaptive Optics in the Context of Space Missions

International audienc

Studying Small Solar System Objects with Adaptive Optics in the Context of Space Missions

International audienc

Titan's Clouds Detections : Observational Constraints from Adaptive Optics and Comparison to GCM Predictions

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Near-infrared Adaptive Optics observations of Titan in conjunction with Huygens' landing

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Near-infrared Adaptive Optics observations of Titan in conjunction with Huygens' landing

International audienc

Near-infrared Adaptive Optics observations of Titan in conjunction with Huygens' landing

International audienc