Patchwork moon of UranusA world assembled from fragments
Miranda
Miranda looks like a collage of different landscapes, sliced by canyons and enormous cliffs.
- Host
- Uranus
- Type
- Small icy moon
- Mean diameter
- 472 km
- Mean orbital radius
- 129,390 km
- Orbital period
- 1.41 days
- Surface gravity
- 0.079 m/s²
- Key feature
- Verona Rupes
- Discovered
- 1948 · Gerard Kuiper
Miranda up close
NASA imagery
A geological patchwork
Miranda combines heavily cratered regions with bright oval coronae crossed by parallel ridges and grooves. The transitions are abrupt, making the moon look as though separate landscapes were pieced together.
The coronae may have formed through upwelling of warm ice or tectonic stretching. Their young appearance suggests Miranda was active after most of its older cratered surface had formed.
Cliffs beyond comparison
Verona Rupes is a fault scarp estimated to be as much as 20 kilometres high. In Miranda's weak gravity, an object falling from its top could take more than ten minutes to reach the base.
Voyager 2 remains the only spacecraft to have visited Miranda at close range. A future Uranus orbiter would be needed to resolve the moon's geological sequence.
Worth knowing
Miranda is named after a character in Shakespeare's The Tempest.
Its cliffs may be the tallest known in the Solar System.
Voyager 2 discovered Miranda's complex terrain during its only visit in 1986.
Watch and explore
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Miranda: Uranus's Strange Moon EVERLOOP
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Research & further reading
Mission imagery and measurements are interpreted alongside orbital data. Follow the source links for the current NASA overview and precise satellite parameters.