Analogous to Earth's water cycle, Titan's methane-based hydrologic cycle supports standing
bodies of liquid and drives processes that result in common morphologic features including …

The entry of the Cassini-Huygens spacecraft into orbit around Saturn in July 2004 marked
the start of a golden era in the exploration of Titan, Saturn's giant moon. During the Prime …

The topography provided by altimetry, synthetic aperture radar‐topography, and stereo
radargrammetry has opened new doors for Titan research by allowing for quantitative …

We present a geomorphologic map of Titan's polar terrains. The map was generated from a
combination of Cassini Synthetic Aperture Radar (SAR) and Imaging Science Subsystem …

Abstract In May 2013 the Cassini RADAR altimeter observed channels in Vid Flumina, a
drainage network connected to Titan's second largest hydrocarbon sea, Ligeia Mare …

Abstract The Cassini/Huygens mission revealed a terrain type on Saturn's moon Titan of
dissected, elevated plateaux with a high density of valleys named labyrinth terrain. We …

We propose that cycling hydrocarbon rains on Saturn's moon Titan are likely to create
subsurface conduits through dissolution geology of the extensive organic and largely …

Some of Titan's small northern hemisphere lakes show raised rampart features (which are
distinct from raised rims), and appear as SAR-bright mound-like annuli extending away from …

Abstract Although the Ku-band Cassini RADAR was not primarily designed to probe Titan's
subsurface structure, it unexpectedly provided valuable data on penetration, notably …

Abstract Cassini Radar observations of Titan have revealed diverse landforms resulting from
a variety of geologic processes. Many landforms can be unambiguously interpreted as …