Titan was a mostly unknown world prior to the Cassini spacecraft's arrival in July 2004. We
review the major scientific advances made by Cassini's Titan Radar Mapper (RADAR) …

One important, almost ubiquitous, tool for understanding the surfaces of solid bodies
throughout the solar system is the study of impact craters. While measuring a distribution of …

With the conclusion of the Cassini mission, we present an updated topographic map of Titan,
including all the available altimetry, SARtopo, and stereophotogrammetry topographic data …

Titan has an active methane-based hydrologic cycle that has shaped a complex geologic
landscape, making its surface one of most geologically diverse in the Solar System. Despite …

Abstract Thanks to the Cassini–Huygens mission, Titan, the pale orange dot of Pioneer and
Voyager encounters, has been revealed to be a dynamic, hydrologically shaped, organic …

Planetary surfaces beyond Earth's are impacted by surface hydrology, and exhibit fluvial and
lacustrine features. Titan in particular harbours a rich hydroclimate replete with valley …

Titan is Saturn's largest moon and has a dynamic surface with methane rivers carved by an
active hydrological cycle and sand seas shaped by aeolian processes. One way to study the …

We carried out geomorphological mapping in a mid-latitude area surrounding the Afekan
Crater region on Titan. We used Cassini RADAR (Synthetic Aperture Radar mode) data as …

Titan, with its organically rich and dynamic atmosphere and geology, and Enceladus, with its
active plume, both harbouring global subsurface oceans, are prime environments in which …

Saturn's moon Titan has all the ingredients needed to produce “life as we know it.” When
exposed to liquid water, organic molecules analogous to those found on Titan produce a …