NASA's Dragonfly mission will send a rotorcraft lander to the surface of Titan in the mid-
2030s. Dragonfly's science themes include investigation of Titan's prebiotic chemistry …

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) …

Planetary Surface Processes is the first advanced textbook to cover the full range of geologic
processes that shape the surfaces of planetary-scale bodies. Using a modern, quantitative …

Data from laboratory flumes and natural streams show that the critical Shields stress for
initial sediment motion increases with channel slope, which indicates that particles of the …

Titan exhibits ample surface and crustal processes including lakes and seas, fluvial erosive
features, possibly subsurface reservoirs of liquid, and rainfall. Together these constitute …

Alluvial rivers are conveyor belts of fluid and sediment that provide a record of upstream
climate and erosion on Earth, Titan, and Mars. However, many of Earth's rivers remain …

Cassini radar images show a variety of fluvial channels on Titan's surface, often several
hundreds of kilometers in length. Some (predominantly at low-and mid-latitude) are radar …

This paper presents a relationship for calculating the drag coefficient of a spherical particle.
The results obtained were validated using experimental data, including comparison with …

A subset of the sinuous ridges (SRs) in the Aeolis/Zephyria Plana (AZP) region of Mars has
been previously hypothesized to be inverted fluvial features, although the precise induration …

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 …