… We mapped in detail Titan's South Belet region which spans from longitude 60E to 120E and
… mapping of Titan's South Belet region and associated geomorphological terrain units. This …

… Map of Titan from Cassini Image Science Subsystem (ISS) data. The sand dunes and sand
seas, appearing dark in ISS data, cover Titan’s entire equatorial region, … geomorphological …

… with the presumed crustal materials of Titan. The plains materials are consistent with …
geomorphological mapping results are consistent with the equatorial and mid-latitudes of Titan …

… mapping of the Afekan crater region, the South Belet region, and of the global geomorphological
map of Titan, … the detailed geomorphological map of the Soi crater region (Figure 7). As …

… striking geomorphological similarities to Earth, including a pervasive set of … On Titan, the
sand seas are concentrated in the equatorial region and are very large; for example, the Belet …

… on Titan is the Belet sand sea (220–300W, 20S-20N). The sediment supply in this region …
Quantifying the geomorphic work performed on the topography enables comparison of the …

… southern margins contain flow-like features that may be cryovolcanic in origin, perhaps
ascended from lithospheric faults related to regional … the oldest terrains on Titan and that its origin …

… Our mapping of the geomorphologic units on Titan is based … Labyrinth terrains cover
relatively small areas of Titan mostly … , which are close to the Belet sand sea implying possible …

… question by conducting geological mapping of Enceladus and Titan, the … in South Belet and
expands our understanding of processes typical of Titan’s equatorial and mid-latitude regions…

… , whereas the darkest equatorial regions such as Shangri-la, Fensal, and Belet are radar-dark …
In summary, the ‘menagerie’of Titan geological features and terrains defined by their radar …