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 …

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 …

The shorelines of Titan's hydrocarbon seas trace flooded erosional landforms such as river
valleys; however, it is unclear whether coastal erosion has subsequently altered these …

Atmospheric photochemistry on Titan continuously transforms methane and nitrogen gases
into various organic compounds. This study explores the fate of these molecules when they …

Titan's northern high latitudes host many large hydrocarbon lakes. Like water lakes on Earth,
Titan's lakes are constantly subject to evaporation. This process strongly affects the …

Abstract On Titan, methane (CH 4) and ethane (C 2 H 6) are the dominant species found in
the lakes and seas. In this study, we have combined laboratory work and modeling to refine …

Titan, the largest moon of Saturn, has many lakes on its surface, formed mainly of liquid
methane. Like water lakes on Earth, these methane lakes on Titan likely profoundly affect …

We measured the solid–liquid–vapor (SLV) equilibrium of binary mixtures during
experiments that alternated between cooling the mixture and injecting the more-volatile …

This article presents a study to assess the characteristics of particles or bubbles possibly
present on Titan's lakes and seas using Cassini RADAR observations when operating in …

Titan is unique among the icy satellites in that it has a thick atmosphere, stable surficial
bodies of liquid, and a precipitation system that promotes interactions between the two …