Natural satellite Charon
Charon
Always facing Pluto
About half Pluto's diameter. Both bodies are tidally locked to one another and orbit a shared center of mass outside Pluto.

- Mean radius
- 606 km
- Mean diameter
- 1,212 km
- Orbital semimajor axis
- 19,600 km
01 / Overview
Meet Charon
Charon is about half Pluto's diameter, forming an unusually balanced partnership. Mutual tidal locking keeps the same faces opposed as they orbit a center of mass outside Pluto. New Horizons revealed canyons and a reddish polar region: Charon has its own geological history, not a miniature copy of Pluto's.
02 / Key data
Core parameters
- Mean radius
- 606 km
- Mean diameter
- 1,212 km
- Orbital semimajor axis
- 19,600 km
- Orbital period
- 6.387 d
- Parent planet
- Pluto
Data and calculation notes
Radii are mean values; orbital data describe each world’s scale and motion.
03 / Further reading
A closer look
What makes this world distinctive5
James Christy discovered Charon in 1978.
Charon's diameter is about half Pluto's.
Pluto and Charon always keep the same faces toward each other.
New Horizons imaged Charon's canyons and other terrain in 2015.
Charon's north pole is covered in distinctive reddish-brown material.
Gravity and the interior14
A natural satellite forms naturally and orbits a larger body; an artificial satellite is built by people.
Tidal locking matches rotation to orbital motion; it does not mean no rotation.
A moon's orbit need not lie in the same plane as its planet's orbit around the Sun.
Differences in gravity across a moon can deform it through tides.
Repeated tidal deformation can turn orbital energy into internal heat.
Orbital resonance means periods near simple integer ratios, allowing repeated pulls between moons to build up.
Some moons formed in discs around planets; others may have been captured later.
Small moons are often irregular because their gravity cannot overcome the strength of their materials.
Large moons tend to be rounder because gravity shapes them.
Icy moons may have liquid oceans under their shells; a frozen surface does not mean a fully frozen interior.
Finding water or organic molecules is not the same as finding life.
A planet and moon both orbit their common center of mass; the heavier body's wobble is usually smaller.
Other bodies perturb a moon's orbit; a fixed ellipse is only an approximation.
Moons can be larger than some planets; classification is not based on diameter alone.
Surface and observation11
About half Pluto's diameter. Both bodies are tidally locked to one another and orbit a shared center of mass outside Pluto.
A moon's visible brightness usually comes from reflected sunlight.
Moons have sunlit and dark sides too; the side facing away from the planet is not permanently dark.
Crater counts help estimate surface ages, but resurfacing and the impact environment also matter.
A moon hiding a background star causes an occultation, useful for measuring size or probing an atmosphere.
A moon entering its planet's shadow experiences an eclipse, depending on the orbits' spatial alignment.
Tiny changes in a spacecraft's speed can reveal a moon's mass and gravity field.
Composition, grain size, and lighting all affect surface color; enhanced-color images differ from naked-eye views.
The day–night boundary is the terminator; long shadows nearby bring out terrain.
Surfaces with little or no atmosphere lack strong weather erosion and preserve old impact scars more easily.
A moon's observed phases come from changing angles between the Sun, moon, and observer.
04 / Sources
Trusted sources
NASA Science — CharonJPL — Orbital dataImage credits
Images reproject and light existing textures; they are not live observations.
Surface texture:cubicApocalypse / CelestiaContent · License · Rendered by ORBIT
