Miranda

472 kmdiameter

Updated

472km
Visual creditVoyager 2 1986 / NASA / JPL-Caltech / Kevin M. Gill / CC BY 2.0Source: Wikimedia Commons

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

Category
Moons
Object class
Icy moon
Host
Uranus
Scale fact
472 kmdiameter
Composition
Water ice and silicate rock
Embed

Size neighbors

Objects near Miranda on the scale

On the logarithmic size axis, Miranda falls between Proteus and Enceladus. The band uses nearby Icy moon records.

Shared physical scale
895km
Mimas396 km
Miranda472 km
Tethys1,066 km
Dione1,124 km
Ariel1,160 km
Umbriel1,170 km

Sources

References for Miranda

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.

Continue with nearby objects or open the full scale.

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