Recent images from the New Horizon spacecraft suggest that Charon's peculiar tectonic landscape could have been formed by expansion from the inside.
Having frozen, the ocean might have pushed outward, causing the moon's surface to stretch and fracture on a massive scale.
This has raised the question about how such an ocean would form in the first place. Scientists believe that as the outer layer of Charon is primarily water-ice, in the moon's youth it could have been heated by internal processes and radioactive elements. Some of the melting water apparently went underneath, into the moon's deeper layers to form a massive pool of water.

A close-up of the canyons on Charon, Pluto's big moon, taken by New Horizons during its close approach to the Pluto system last July
An image published by the space agency shows part of Charon's 1,800-km belt of chasms, one of the longest in our solar system. It reaches 4.5 miles (7.5km) deep - considerably more than the Grand Canyon on Earth, which is just over a mile (1.6km) in depth.
Flying over Charon:





