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Saturn

Rings that are not solid, but countless orbiting fragments.

classification
Gas giant
system
Outer solar system
overview //

Saturn is the second-largest planet in the solar system, encircled by a broad, extremely thin ring system and orbited by a diverse family of moons.

technical data //
Mean radius
58,232 km
Surface gravity
10.44 m/s² at the 1-bar level
Orbital period
29.4 Earth years
Orbital distance
1.43 billion km from the Sun (mean)
Cloud-top temperature
about −178 °C at the 1-bar level

Only values with an established scientific consensus are listed. Where a quantity is uncertain or model-dependent, it is discussed in the sections below rather than stated as data.

what we know //
01

The rings are made of countless separate bodies

They are dominated by water ice, ranging from dust grains to house-sized blocks, each on its own orbit.

02

The rings are thin

Tens of metres thick in places, across a span of hundreds of thousands of kilometres.

03

Enceladus vents material into space

Plumes of water vapour and ice grains from Saturn's moon Enceladus feed the outer E ring.

how do we know? //

Long-duration orbital mission

Cassini observed the system for thirteen years, including passes between the planet and its rings.

Stellar and radio occultations

Watching starlight and radio signals dim as they pass through the rings reveals particle sizes and ring structure.

In-situ plume sampling

Cassini flew through the Enceladus plume and measured its composition directly.

methods archive →
open questions //
  • How old are the rings?Estimates from a few hundred million years to primordial remain debated.
  • What is the planet's true internal rotation rate?
  • Is Enceladus's subsurface ocean chemically hospitable?Suggestive, but unresolved.

Items above are unresolved. Hypotheses are labelled as such and are not presented as confirmed findings.

related missions //
continue exploring //