Bruce Murray Space Image Library

Flooded canyons on Titan

Flooded canyons on Titan
Flooded canyons on Titan NASA's Cassini spacecraft pinged the surface of Titan with microwaves, finding that some channels are deep, steep-sided canyons filled with liquid hydrocarbons. One such feature is Vid Flumina, the branching network of narrow lines in the upper-left quadrant of the image. The image was acquired on 26 September 2012, on Cassini's 87th close flyby of Titan. NASA / JPL-Caltech / Italian Space Agency (ASI)
Vid Flumina
Vid Flumina The canyons of Vid Flumina are seen in this view from Cassini's radar mapper. More information. NASA / JPL-Caltech / ASI

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