The side of Charon viewed by the passing New Horizons spacecraft in July 2015 is characterized by a system of “pull apart” tectonic faults, which are expressed as ridges, scarps, and valleys — the latter sometimes reaching more than 4 miles (6.5 kilometers) deep. Charon’s tectonic landscape shows that somehow the moon expanded in its past, and its surface fractured as it stretched.
Charon’s outer layer is primarily water ice. When the moon was young, this layer was warmed by the decay of radioactive elements as well as Charon’s own internal heat of formation. Scientists say Charon could have been warm enough to cause the water ice to melt deep down, creating a subsurface ocean. But as Charon cooled over time, this ocean would have frozen and expanded — as happens when water freezes — pushing the surface outward and producing the massive chasms we see today.
This image focuses on a section of the feature informally named Serenity Chasma, part of a vast equatorial belt of chasms on Charon. In fact, this system of chasms is one of the longest seen anywhere in the solar system, running at least 1,100 miles (1,800km) long and reaching 4.5 miles (7.5km) deep. By comparison, the Grand Canyon is 277 miles (446km) long and just over a mile (1.6km) deep.
The lower portion of the image shows color-coded topography of the same scene. Measurements of the shape of this feature tell scientists that Charon’s water-ice layer may have been at least partially liquid in its early history and has since refrozen.
This image was obtained by the Long-Range Reconnaissance Imager (LORRI) on New Horizons. North is up; illumination is from the top-left of the image. The image resolution is about 1,290 feet (394 meters) per pixel. The image measures 240 miles (386km) long and 110 miles (175km) wide. It was obtained at a range of approximately 48,900 miles (78,700km) from Charon, about an hour and 40 minutes before New Horizons’ closest approach to Charon on July 14, 2015.
