100 citations · 126 across the 6 of their papers we have counts for
14 papers
An unidentified absorption feature at 5.11 m on the surface of Titan and Pluto from JWST spectroscopy
B. Bézard, E. Lellouch, M. Camarca +14
Titan possesses a thick N-CH atmosphere that makes it difficult to study its surface spectroscopically. The chemical composition of the solid surface of Titan thus remains…
Refractive indices of photochemical haze analogs for Solar System and exoplanet applications : a cross-laboratory comparative study between the PAMPRE and COSmIC experimental set-ups
Thomas Drant, Ella Sciamma-O'Brien, Lora Jovanovic +9
Previous observations of Titan, Pluto and Solar System gas giants along with recent observations of exoplanet atmospheres with the James Webb Space Telescope taught us that photoch…
Moonraker -- Enceladus Multiple Flyby Mission
O. Mousis, A. Bouquet, Y. Langevin +50
Enceladus, an icy moon of Saturn, possesses an internal water ocean and jets expelling ocean material into space. Cassini investigations indicated that the subsurface ocean could b…
Science goals and new mission concepts for future exploration of Titan's atmosphere geology and habitability: Titan POlar Scout/orbitEr and In situ lake lander and DrONe explorer (POSEIDON)
Sébastien Rodriguez, Sandrine Vinatier, Daniel Cordier +61
In response to ESA Voyage 2050 announcement of opportunity, we propose an ambitious L-class mission to explore one of the most exciting bodies in the Solar System, Saturn largest m…
Distribution and intensity of water ice signature in south Xanadu and Tui Regio
Maélie Coutelier, Daniel Cordier, Benoît Seignovert +5
Titan's surface was revealed by Cassini's instruments, showing the presence of liquid hydrocarbons in lakes, and features like dry riverbed. In order to study the sediment transpor…
Haze seasonal variations of Titan's upper atmosphere during the Cassini Mission
Benoît Seignovert, Pascal Rannou, Robert A. West +1
This study presents a 13 years survey of haze UV extinction profiles, monitoring the temporal evolution of the detached haze layer (DHL) in Titan's upper atmosphere (350-600 km). A…