103 citations · 294 across the 4 of their papers we have counts for
4 papers
Global circulation as the main source of cloud activity on Titan
Sébastien Rodriguez, Stéphane Le Mouélic, Pascal Rannou +11
Clouds on Titan result from the condensation of methane and ethane and, as on other planets, are primarily structured by circulation of the atmosphere. At present, cloud activity m…
Cassini/VIMS hyperspectral observations of the HUYGENS landing site on Titan
S. Rodriguez, S. Le Mouélic, C. Sotin +7
Titan is one of the primary scientific objectives of the NASA ESA ASI Cassini Huygens mission. Scattering by haze particles in Titan's atmosphere and numerous methane absorptions d…
Diversity among other worlds: characterization of exoplanets by direct detection
J. Schneider, A. Boccaletti, A. Aylward +34
The physical characterization of exoplanets will require to take spectra at several orbital positions. For that purpose, a direct imaging capability is necessary. Direct imaging re…
Could we identify hot Ocean-Planets with CoRoT, Kepler and Doppler velocimetry?
F. Selsis, B. Chazelas, P. Borde +16
Planets less massive than about 10 MEarth are expected to have no massive H-He atmosphere and a cometary composition (50% rocks, 50% water, by mass) provided they formed beyond the…