International audienceThe factors contributing to the initial selection of a dune site near the Selk impact structure on Titan as the first landing site for the Dragonfly mission are described. These include arrival geometry and aerodynamic/ aerothermodynamic considerations, illumination, and Earth visibility, as well as the likely presence of exposed deposits of water-rich material, potentially including materials where molten ice has interacted with organics. Cassini observations of Selk are summarized and interpreted: near-infrared reflectance and microwave emission data indicate water-rich materials in and around the crater. Radar topography data shows the rim of Selk to have slopes on multi-km scales reaching only ∼2°degrees, an order ...
Only a small number of impact craters on Titan’s surface have been identified from observations by t...
Cassini's third and fourth radar flybys, T7 and T8, covered diverse terrains in the high southern an...
International audienceTitan, Saturn's biggest moon, is an ocean world, covered by organic materials ...
International audienceThe factors contributing to the initial selection of a dune site near the Selk...
The factors contributing to the initial selection of a dune site near the Selk impact structure on T...
International audienceThe Selk crater region is the future landing site of NASA's Dragonfly mission ...
International audienceObservations of Titan obtained by the Cassini Visual and Infrared Mapping Spec...
International audienceWe present an analysis of Titan data acquired by the Cassini Visual and Infrar...
International audienceRadar brightness of dunes changes with observation angles (incidence and azimu...
The surface of Titan is highly diverse with a remarkable landscape including dunes, streambeds, and ...
International audienceNASA's Dragonfly mission will send a rotorcraft lander to the surface of Titan...
International audienceThe first two swaths collected by Cassini's Titan Radar Mapper were obtained i...
International audienceTitan, the largest moon of Saturn, is the place in the Solar System showing th...
International audienceWe investigate the spectral behavior of nine Titan impact craters in order to ...
Only a small number of impact craters on Titan’s surface have been identified from observations by t...
Cassini's third and fourth radar flybys, T7 and T8, covered diverse terrains in the high southern an...
International audienceTitan, Saturn's biggest moon, is an ocean world, covered by organic materials ...
International audienceThe factors contributing to the initial selection of a dune site near the Selk...
The factors contributing to the initial selection of a dune site near the Selk impact structure on T...
International audienceThe Selk crater region is the future landing site of NASA's Dragonfly mission ...
International audienceObservations of Titan obtained by the Cassini Visual and Infrared Mapping Spec...
International audienceWe present an analysis of Titan data acquired by the Cassini Visual and Infrar...
International audienceRadar brightness of dunes changes with observation angles (incidence and azimu...
The surface of Titan is highly diverse with a remarkable landscape including dunes, streambeds, and ...
International audienceNASA's Dragonfly mission will send a rotorcraft lander to the surface of Titan...
International audienceThe first two swaths collected by Cassini's Titan Radar Mapper were obtained i...
International audienceTitan, the largest moon of Saturn, is the place in the Solar System showing th...
International audienceWe investigate the spectral behavior of nine Titan impact craters in order to ...
Only a small number of impact craters on Titan’s surface have been identified from observations by t...
Cassini's third and fourth radar flybys, T7 and T8, covered diverse terrains in the high southern an...
International audienceTitan, Saturn's biggest moon, is an ocean world, covered by organic materials ...