Moons · Space Codex

Dione

A dense ice-and-rock moon whose trailing side is streaked with bright 'wisps', which Cassini revealed as walls of fractured ice hundreds of metres high.

Cratered moon laced with ice cliffs

  • Last reviewed 10 Oct 2026
  • 4 sources

At a glance

Dione at a glance, with sources
MeasureValueSource
Mean radius561.4 kmJPL Solar System Dynamics: satellite physical parameters (opens in a new tab)JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
Mass1.10 × 10²¹ 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 gravity0.232 m/s² (0.0237 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 velocity510 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 density1.48 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 Saturn377,700 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 period2.737 daysJPL 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 albedo0.7NASA NSSDC Saturnian Satellite Fact Sheet (opens in a new tab)NASA NSSDC Saturnian Satellite Fact Sheet (opens in a new tab)
Average temperatureAbout −186 °C (87 K)NASA Science: Dione (opens in a new tab)NASA Science: Dione (opens in a new tab)
Largest cratersUp to about 100 km acrossNASA Science: Dione (opens in a new tab)NASA Science: Dione (opens in a new tab)
ResonanceOrbits once for every two orbits of EnceladusNASA Science: Dione (opens in a new tab)NASA Science: Dione (opens in a new tab)
Co-orbital moonsHelene (60° ahead) and Polydeuces (60° behind)NASA Science: Dione (opens in a new tab)NASA Science: Dione (opens in a new tab)
Discovered21 Mar 1684 by Giovanni CassiniNASA Science: Dione (opens in a new tab)NASA Science: Dione (opens in a new tab)

Key points

  • Bright 'wisps' are ice cliffs hundreds of metres high
  • Locked in a 1:2 resonance with Enceladus
  • Shares its orbit with two tiny moons

Surface

Dione's leading hemisphere is heavily cratered; its trailing hemisphere carries bright streaks that Voyager could not resolve. Cassini, flying past from 2005, showed them to be fracture cliffs of clean ice, some several hundred metres high.

Interior

A rocky core makes up about a third of the moon. Its resonance with Enceladus may help keep Enceladus's interior warm.

What we still don't know

Whether Dione retains a thin liquid layer beneath its ice, as some interpretations of Cassini gravity data allow.

Missions

  1. 1977–

    Voyager 1

    NASAActive

    Jupiter 1979, Saturn 1980; interstellar space since 25 Aug 2012.

    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

Dione is a sphere wrapped in a global map built from USGS and NASA spacecraft mosaics.

It is drawn at about 4.4% of Saturn's radius, enlarged from its true 0.96% so it stays visible. It orbits almost exactly in Saturn's equatorial plane, with a 2.74-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.

Sources

  1. JPL Solar System Dynamics: satellite physical parameters (opens in a new tab)
  2. JPL Solar System Dynamics: satellite mean orbital elements (opens in a new tab)
  3. NASA NSSDC Saturnian Satellite Fact Sheet (opens in a new tab)
  4. NASA Science: Dione (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.