About Dione
Dione is Saturn’s fourth-largest moon, with a rocky core and icy mantle. Its trailing hemisphere displays striking bright, streaky “wispy terrain” — originally a mystery, but revealed by Cassini to be networks of bright ice cliffs hundreds of meters tall. Dione is in a 2:1 orbital resonance with Enceladus, which may contribute to tidal heating. Cassini gravity data hint at a subsurface ocean beneath ~100 km of ice.
Physical Properties
Orbit
Gallery
Hand-picked mission imagery of Dione sourced from NASA and partner archives. Click any photo for full resolution and source attribution.
Imagery on this page is provided by the original mission teams. Full attribution terms: Image Rights & Credits.
Sources & Further Reading
- NASA — official mission / factsheet page
- Wikipedia — extensive cross-referenced article
- NASA u2014 Dione
Numerical values (radius, mass, orbital elements, temperatures) are drawn from NASA NSSDC Planetary Fact Sheets, JPL Horizons, and the JPL Small-Body Database. Last refreshed: 2026-06-08 01:37:02.