Water Ice and Methane Springs on Titan

A single Huygens DISR image that shows two new features on the surface of
Titan. A bright linear feature suggests an area where water ice may have
been extruded onto the surface. Also visible are short, stubby dark channels
that may have been formed by 'springs' of liquid methane rather than methane
'rain.'

Credit: ESA/NASA/JPL/University of Arizona