

Biggest Satellite in the Solar System: Discover Ganymede, the largest satellite in our solar system. Learn about its size, structure, and how it compares to other moons and even planets!
When we think of large celestial bodies, planets often come to mind. But did you know the largest satellite in the solar system is actually bigger than Mercury? Meet Ganymede, Jupiter’s largest moon and the biggest satellite orbiting any planet in our solar system.
Ganymede is so massive that it even generates its own magnetic field — a unique trait among moons. It was discovered in 1610 by Galileo Galilei and remains a subject of fascination for scientists and space agencies.
Despite its size, Ganymede is only about half as dense as Earth, owing to its composition of water ice and silicate rock.
Ganymede has three main layers:
Scientists believe there’s a subsurface ocean beneath the icy crust, possibly containing more water than all of Earth’s oceans combined. This raises exciting possibilities for extraterrestrial life.
Ganymede is the only moon known to have a magnetic field, which likely originates from its liquid iron core. This magnetic field interacts with Jupiter’s massive magnetosphere, creating stunning auroras around the moon’s poles.
Although its atmosphere is extremely thin, traces of oxygen and ozone have been detected, adding intrigue to its potential habitability.
These missions aim to understand the moon’s geology, subsurface ocean, and potential for harboring life.
Moon | Diameter (km) | Parent Planet | Notable Features |
---|---|---|---|
Ganymede | 5,268 | Jupiter | Magnetic field, subsurface ocean |
Titan | 5,151 | Saturn | Thick atmosphere, methane lakes |
Callisto | 4,821 | Jupiter | Oldest surface, heavily cratered |
Io | 3,643 | Jupiter | Volcanically active |
Moon (Earth) | 3,474 | Earth | Tidal locking, visible from Earth |
It orbits Jupiter, making it a natural satellite despite its massive size.
Not currently, but the subsurface ocean and thin oxygen atmosphere make it a target for future astrobiology missions.
Roughly 628 million kilometers when Jupiter is at opposition.
The surface is icy and rocky with grooves, craters, and ridges caused by tectonic and cryovolcanic activity.
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