Saturn

Saturn

Planet· orbits the Sun

Saturn is the sixth planet and the second-largest, famous for its spectacular ring system of ice and rock. It is the least dense planet — it would float in water. Around its north pole sits a hexagon — a six-sided standing wave in a jet stream, first seen by Voyager in 1981 and stable for over forty years. In 2025 Hubble and ground-based telescopes found its southern counterpart: a ten-sided wave, a decagon, encircling the south pole at about 58–63°S. It drifts east at just 2.5 m/s inside a 116 m/s jet, its corners sway with a 32-day rhythm, and images from 2023–24 show it still taking shape (Sánchez-Lavega et al., Science Advances, September 2026) — so unlike the hexagon, it is new, evolving, and nobody yet knows whether it will last.

Open in 3D viewSee Saturn in the live, interactive 3D map

Key facts

Mass
5.68 × 10²⁶ kg
95.2 M⊕
Radius
58,232 km
9.14× wider than Earth
Surface gravity
11.2 m/s²
1.14× Earth's gravity
Day length
10.66 hours
Year
29.5 Earth years
10,759 Earth days
Distance from Sun
9.54 AU
Moons
291
known, incl. provisional (JPL SSD)

Science

Physical

Mass
5.68 × 10²⁶ kg · 95.2 M⊕
Radius
58,232 km · 9.14× wider than Earth
Density
687 kg/m³ · 0.69× water
Computed from mass and radius
Surface gravity
11.2 m/s² · 1.14× Earth's gravity
Computed from mass and radius
Escape velocity
36.1 km/s · 3.23× Earth's escape velocity
Computed from mass and radius
Axial tilt
26.73 °

Orbital

Distance from the Sun
9.43 AU
Computed from the position at the selected time
Semi-major axis
9.54 AU
Computed from the cached state vector
Eccentricity
0.05507
Computed from the cached state vector
Inclination
22.55 °
Computed from the cached state vector
Orbital period
29.46 years
Computed from the cached state vector
Perihelion
9.01 AU
Computed from the orbital elements
Aphelion
10.1 AU
Computed from the orbital elements
Mean orbital velocity
9.64 km/s
Computed from the orbital elements

Rotation

Rotation period
10.66 hours

Atmosphere

Composition
96% H₂, 3% He, traces of CH₄
Scale height
59.5 km

Rings

Composition & structure
Almost pure water ice (>90–95%) with a small rocky/carbonaceous contaminant that reddens them slightly. Particles span micron-scale dust to house-sized boulders, in a disk only tens of metres thick — the brightest, most massive ring system in the Solar System. Extensively mapped by Voyager (1980–81) and Cassini (2004–17).

Temperature

Mean
134 K (-139 °C)

Composition

Bulk composition
Hydrogen/helium with a rocky/icy core; iconic ring system

Radiation & temperature

Insolation
0.011 S⊕ · 1% of the sunlight Earth receives
Computed from the distance to the Sun (inverse-square; Earth's sunlight = 1), before any atmosphere.
Bond albedo
0.34 · reflects 34% of incoming sunlight
Equilibrium temperature
81 K (-192 °C)
Computed from albedo + distance from the Sun (airless black body)
Measured mean temperature
134 K (-139 °C)
Greenhouse warming
+53 K
Measured temperature minus the airless equilibrium — the greenhouse effect
Surface magnetic field
21 µT · 42% of Earth's magnetic field

Discovery & history

First known
Known since antiquity
Name
The Roman god of agriculture; to antiquity it was the most distant planet known.

Saturn, the slowest-moving of the naked-eye planets, marked the edge of the known Solar System for millennia. When Galileo saw it in 1610 his telescope was too crude to resolve the rings — he reported mysterious 'ears'. In 1655 Christiaan Huygens correctly identified a flat ring and discovered Titan. Centuries later the Cassini–Huygens mission orbited Saturn for 13 years, landing a probe on Titan and diving through the rings.

  1. 1979Pioneer 11Flyby

    First spacecraft to fly past Saturn.

  2. 1980Voyager 1Flyby

    Close study of the rings and a targeted flyby of Titan.

  3. 1981Voyager 2Flyby

    Imaged the rings in fine detail before heading on to Uranus and Neptune.

  4. 2004Cassini–HuygensOrbiter

    Orbited Saturn for 13 years; the Huygens probe landed on Titan in 2005.

Images

Images from open archives · credit shown per image