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Article Dans Une Revue Science Année : 2005

Cassini Radar Views the Surface of Titan

Y. Gim
  • Fonction : Auteur
R. Seu
  • Fonction : Auteur
L. C. Wye
  • Fonction : Auteur
H. Zebker
  • Fonction : Auteur

Résumé

The Cassini Titan Radar Mapper imaged about 1% of Titan's surface at a resolution of ~0.5 kilometer, and larger areas of the globe in lower resolution modes. The images reveal a complex surface, with areas of low relief and a variety of geologic features suggestive of dome-like volcanic constructs, flows, and sinuous channels. The surface appears to be young, with few impact craters. Scattering and dielectric properties are consistent with porous ice or organics. Dark patches in the radar images show high brightness temperatures and high emissivity and are consistent with frozen hydrocarbons.

Dates et versions

hal-03786408 , version 1 (23-09-2022)

Identifiants

Citer

Charles Elachi, Stephen D. Wall, M. Allison, Y. Anderson, R. Boehmer, et al.. Cassini Radar Views the Surface of Titan. Science, 2005, 308, pp.970-974. ⟨10.1126/science.1109919⟩. ⟨hal-03786408⟩
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