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 …

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 …

Simulation results are presented from a new general circulation model (GCM) of Titan, the
Titan Atmospheric Model (TAM), which couples the Flexible Modeling System (FMS) spectral …

The methane-based hydrologic cycle on Saturn's largest moon, Titan, is an extreme
analogue to Earth's water cycle. Titan is the only planetary body in the Solar System, other …

Over the past decade, the Cassini-Huygens mission to the Saturn system has revolutionized
our understanding of Titan and its climate. Veiled in a thick organic haze, Titan's visible …

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 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) …

There are few identifiable impact craters on Titan, especially in the polar regions. One
explanation for this observation is that the craters are being destroyed through fluvial …

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 …