About Hyperion
Hyperion is an irregularly shaped, heavily pitted moon of Saturn with an unusual “sponge-like” appearance caused by a very high bulk porosity — around 40%, the lowest density of any major moon. Its rotation is mathematically chaotic: tidal torques from Saturn and its orbital resonance with the much larger Titan produce a tumble that never repeats, making it one of only two non-synchronously-rotating moons whose attitude cannot be long-term predicted.
Physical Properties
Orbit
Missions to Hyperion
1 spacecraft tracked on Space Launch Live.
Gallery
Hand-picked mission imagery of Hyperion 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 Hyperion
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.