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 …

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 …

Titan's surface and lower atmosphere support a hydrologic cycle that influences various
aspects of the icy moon's appearance and evolution. Here, we review the state of knowledge …

The Earth is no longer the only known celestial body containing one or more liquid phases.
The Cassini spacecraft has discovered seas of hydrocarbons at the surface of Titan, while a …

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 …

Cassini-Huygens provided a wealth of data with which to constrain numerical models of
Titan. Such models have been employed over the last decade to investigate various aspects …

Saturn's largest moon, Titan, hosts liquid hydrocarbon lakes and seas on its surface. During
the last close encounter with Titan (22 April 2017), the Cassini spacecraft used its RADAR …

Saturn's largest moon Titan is unique for its dense, methane‐rich atmosphere, with ongoing
complex organics chemistry, and the hydrocarbon lakes and seas on its frigid surface. Titan …