Miranda

Moon · Major moon of Uranus · orbits Uranus

Miranda is the smallest and innermost of Uranus’ five major moons, and its surface looks stitched together from spare parts - ancient cratered plains butt directly against huge chevron-shaped grooved regions called coronae. When Voyager 2 flew past in 1986, this little moon turned out to be the strangest sight in the whole Uranus system.

Open the 3D Solar System

Quick facts

The Frankenstein moon

A moon just 472 km across should have frozen solid long ago and stayed geologically dead. Yet Miranda’s jumbled patchwork says otherwise: it was probably caught for a time in an orbital resonance with Umbriel, and the resulting tidal heating sent warm ice welling up from inside, breaking and remaking parts of the crust. Even tiny worlds can be reworked - given the right gravitational choreography.

Physical characteristics

Diameter472 km
Mass6.600e+19 kg
Surface gravity0.08 m/s²
Density1.2 g/cm³
Tidally lockedYes
Mean temperature-200 °C
Geometric albedo0.32

Atmosphere and composition

AtmosphereNone detected.
CompositionWater ice mixed with silicate rock; the least dense of the five major Uranian moons.

Discovery

Discovered byGerard Kuiper
Year1948
How82-inch telescope at McDonald Observatory

Missions

Voyager 2 NASA · Flyby probe · 1977 · active
Launched 16 days before its twin, Voyager 2 is the only spacecraft ever to visit all four giant planets - Jupiter, Saturn, Uranus and Neptune. It entered interstellar space in 2018 and is still returning data.

Related objects

Sources