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 …

We present an analysis of Titan data acquired by the Cassini Visual and Infrared Map**
Spectrometer (VIMS), making use of recent improvements in methane spectroscopic …

Titan is the only world we know, other than Earth, that has a liquid on its surface. It also has a
thick atmosphere composed of nitrogen and methane with a thick organic haze. There are …

Abstract Water–ice-poor, 5-μm-bright material on Saturn's moon Titan has previously been
geomorphologically identified as evaporitic. Here we present a global distribution of the …

Abstract The Undifferentiated Plains on Titan, first mapped by Lopes et al.(Lopes, RMC et
al., 2010. Icarus, 205, 540–588), are vast expanses of terrains that appear radar-dark and …

Linear sand dunes cover the equatorial latitudes of Saturn's moon Titan and are shaped by
global wind patterns,,. These dunes are thought to reflect present-day diurnal, tidal and …