Key facts
- Scale fact
- 472 kmdiameter
- Composition
- Water ice and silicate rock
472 kmdiameter
Details
Miranda is the smallest and innermost of Uranus' major moons, but Voyager 2 revealed one of the strangest surfaces in the Solar System. Its patchwork coronae, ridges, valleys, and giant fault canyons make it geologically surprising for a moon only about 470 kilometers across.
Voyager 2 imaged Miranda as a patchwork of old cratered ground, younger-looking coronae, ridges and fault canyons as much as 20 kilometers deep. Competing models invoke internal upwelling, tidal heating and impacts to explain this terrain, but the single 1986 flyby did not determine one complete geological history.
Key facts
Links
Size neighbors
Sources
Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.
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About
Scale of Space is a scroll-based journey through the universe, placing objects on a single logarithmic scale so you can compare size across an unbroken range.
Guides explain selected parts of that range, while focused views filter the objects by subject.