Liquid methane-filled canyons hundreds to thousands of feet deep etch the surface of Saturn’s largest moon, according to researchers with NASA’s Cassini mission. Cassini pinged the surface of Titan with microwaves, finding that some channels are deep 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. Image credit: NASA / JPL-Caltech / ASI. Cassini...
