NASA’s Cassini

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.
Credits: NASA/JPL-Caltech/ASI

Leave a comment

Your email address will not be published. Required fields are marked *