We present preliminary evidence that suggests a hemispheric albedo dichotomy on Titan, the largest planetary satellite in the Solar System. We have also studied the photometric properties of several dark circular features on Titan's surface to test if they might be of impact origin. The evidence is derived from photometric analysis of selected surface regions taken at different Titanian longitudes and solar phase angles using images from the Cassini Saturn Orbiter Visual and Infrared Mapping Spectrometer (VIMS). The VIMS instrument is able to image Titan's surface at spectral windows (e.g. 2.02 microns) in its atmosphere where methane, the principal atmospheric absorber is transparent. Additional information is included in the original exte...
Cassini observations of the surface of Titan offer unprecedented views of its surface through atmosp...
International audienceThe Cassini-Huygens instruments revealed that Titan, Saturn's largest moon, ha...
International audienceWe investigate the surface of Titan by means of two Cassini instruments used i...
International audienceThe Visual and Infrared Mapping Spectrometer (VIMS) instrument on the Cassini ...
Titan, the largest moon of Saturn, is the only satellite in the Solar System with a substantial atmo...
The joint NASA-ESA-ASI Cassini- Huygens mission reached the saturnian system on July 1st 2004. It st...
International audienceTitan shows its surface through many methane windows in the 1-5 mm region. Win...
We investigate Titan's low- and mid-latitude surface using spectro-imaging near-infrared data from C...
Cassini observations of the surface of Titan offer unprecedented views of its surface through atmosp...
International audienceThe Cassini-Huygens instruments revealed that Titan, Saturn's largest moon, ha...
International audienceWe investigate the surface of Titan by means of two Cassini instruments used i...
International audienceThe Visual and Infrared Mapping Spectrometer (VIMS) instrument on the Cassini ...
Titan, the largest moon of Saturn, is the only satellite in the Solar System with a substantial atmo...
The joint NASA-ESA-ASI Cassini- Huygens mission reached the saturnian system on July 1st 2004. It st...
International audienceTitan shows its surface through many methane windows in the 1-5 mm region. Win...
We investigate Titan's low- and mid-latitude surface using spectro-imaging near-infrared data from C...
Cassini observations of the surface of Titan offer unprecedented views of its surface through atmosp...
International audienceThe Cassini-Huygens instruments revealed that Titan, Saturn's largest moon, ha...
International audienceWe investigate the surface of Titan by means of two Cassini instruments used i...