Moons · Space Codex

Enceladus

The most reflective world in the Solar System.

The moon that sprays its ocean into space

  • Last reviewed 10 Oct 2026
  • 6 sources

At a glance

Enceladus at a glance, with sources
MeasureValueSource
Dimensions257 × 251 × 248 kmNASA NSSDC Saturnian Satellite Fact Sheet (opens in a new tab)NASA NSSDC Saturnian Satellite Fact Sheet (opens in a new tab)
Mean radius252.1 kmJPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Mass1.08 × 10²⁰ kgDerived from the JPL GM value and mean radius.JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Surface gravity0.113 m/s² (0.0116 g)Derived from the JPL GM value and mean radius.JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Escape velocity239 m/sDerived from the JPL GM value and mean radius.JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Mean density1.61 g/cm³JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Distance from Saturn238,400 kmJPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)
Orbital period32.9 hoursJPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)
Geometric albedo1.0, the highest of any known bodyNASA NSSDC Saturnian Satellite Fact Sheet (opens in a new tab)NASA NSSDC Saturnian Satellite Fact Sheet (opens in a new tab)
Surface temperatureAbout −201 °CNASA Science: Enceladus (opens in a new tab)NASA Science: Enceladus (opens in a new tab)
Ice shellAbout 1–5 km thick at the south pole, about 20–25 km on averageNASA Science: Enceladus (opens in a new tab)NASA Science: Enceladus (opens in a new tab)
Geysers101 mapped along four 'tiger stripe' fracturesNASA JPL: Cassini reveals 101 geysers (opens in a new tab)NASA JPL: Cassini reveals 101 geysers (opens in a new tab)
Discovered1789 by William HerschelNASA Science: Enceladus (opens in a new tab)NASA Science: Enceladus (opens in a new tab)

Key points

Jets from cracks at its south pole vent an underground ocean into space, building one of Saturn's rings.

  • Reflects essentially all the sunlight that hits it
  • 101 geysers vent its ocean into space
  • Its plumes build Saturn's E ring

Plumes

Cassini found the plumes in 2005. Ice grains and gas leave the south-polar fractures at around 400 m/s; some fall back as snow, the rest feed Saturn's broad E ring. Cassini flew through the spray several times and tasted water, carbon dioxide, methane, ammonia, salts and tiny grains of silica.

A habitable ocean?

Silica nanograins form when hot water, above about 90 °C, reacts with rock, which points to hydrothermal vents on the seafloor. In 2023 researchers reported phosphate in plume grains at concentrations at least 100 times those of Earth's seawater; in 2025 a reanalysis found new complex organic molecules in freshly ejected grains.

Surface

The north is cratered and old, the south nearly crater-free. Four parallel fractures, each about 130 km long, cross the south pole; in true colour they are only faintly bluish-grey.

What we still don't know

Whether life could exist in an ocean this small, and how long the ocean has been liquid.

Missions

  1. 1977–

    Voyager 2

    NASAActive

    The only spacecraft to visit Uranus (1986) and Neptune (1989); interstellar since 5 Nov 2018.

    Mission page (opens in a new tab)

  2. 1997–2017

    Cassini–Huygens

    NASA / ESA / ASICompleted

    Orbited Saturn 2004–2017 and ended by diving into the planet.

First-hand · our 3D model

How we render it

Enceladus is a sphere wrapped in a global map built from USGS and NASA spacecraft mosaics. At full quality a plume rises from the south-polar fractures, drawn as an additive cone that only really shows when Enceladus is backlit, as in Cassini's images.

It is drawn at about 2.7% of Saturn's radius, enlarged from its true 0.43% so it stays visible. It orbits almost exactly in Saturn's equatorial plane, with a 1.37-day period kept in true ratio to its neighbours, and keeps one face towards Saturn.

Moon sizes and orbits are compressed so a whole system fits on screen, but never reordered: each moon is drawn at 0.72 × (true size ratio)^0.6 of its planet, capped so no large moon is drawn bigger than it really is, and orbit distances are log-compressed into a band that clears the planet's rings. Orbital periods keep their true ratios, every moon is tidally locked, and on lighter devices only the two largest moons of each planet are drawn.

  • SaturnRinged gas giant
  • TitanA moon with weather, rivers and seas
  • MimasThe 'Death Star' moon with a hidden ocean

Sources

  1. Postberg et al. 2023, Nature 618:489 (FU Berlin summary) (opens in a new tab)
  2. NASA NSSDC Saturnian Satellite Fact Sheet (opens in a new tab)
  3. JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
  4. JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)
  5. NASA Science: Enceladus (opens in a new tab)
  6. NASA JPL: Cassini reveals 101 geysers (opens in a new tab)

Last reviewed against these sources. Built from public NASA, ESA and JPL data; not affiliated with or endorsed by any agency.