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 …

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 …

Morphological evidence for ancient channelized flows (fluvial and fluvial-like landforms)
exists on the surfaces of all of the inner planets and on some of the satellites of the Solar …

Fluvial features on Titan have been identified in synthetic aperture radar (SAR) data taken
during spacecraft flybys by the Cassini Titan Radar Mapper (RADAR) and in Descent …

Ice resistance to tensile fracture influences surface morphodynamics on outer planetary
satellites such as Titan, yet measurements of tensile strength and fracture toughness of …

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) …

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 …

We carried out geomorphological map** in a mid-latitude area surrounding the Afekan
Crater region on Titan. We used Cassini RADAR (Synthetic Aperture Radar mode) data as …

Although Titan's surface shows clear evidence of erosional modification, such as fluvial
incision, evidence for tectonism has been less apparent. On Earth, fluvial networks with …