Titan is the only moon with a substantial atmosphere, the only other thick N2 atmosphere
besides Earth's, the site of extraordinarily complex atmospheric chemistry that far surpasses …

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) …

A comprehensive calibration and mapping of the thermal microwave emission from Titan's
surface is reported based on radiometric data obtained at 2.18-cm wavelength by the …

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 …

Saturn's moon Titan was explored by the Cassini spacecraft from 2004 to 2017. While
Cassini revealed a lot about this Earth-like world, its radar observations could only provide …

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 …

Triboelectric, or frictional, charging is a ubiquitous yet poorly understood phenomenon in
granular flows. Recognized in terrestrial volcanic plumes and sand storms, such …