Uranus

50,724 kmdiameter

Updated

50,724km
Visual creditVoyager 2 1986 / NASA / JPL-Caltech / Public domainSource: Wikimedia Commons

Details

Uranus is an ice giant that rotates tipped over on its side, with its spin axis tilted by about 98 degrees. That extreme tilt makes its seasons unlike any other planet’s, leaving each pole pointed toward the Sun for decades at a time during its 84-year orbit.

Uranus’s rotation axis is tilted by about 98 degrees relative to its orbit, so each pole can face broadly toward the Sun for part of the planet’s 84-year orbit. The atmosphere is mostly hydrogen and helium with methane, while gravity and magnetic measurements indicate an interior richer in heavier volatile materials than Jupiter or Saturn. Voyager 2’s 1986 flyby remains the only close spacecraft survey.

Key facts

Category
Planets
Object class
Ice giant planet
Mass
~14.5 Earth masses
Host
Sun
Scale fact
50,724 kmdiameter
Estimated age
~4.5 billion years
Composition
Hydrogen, helium, water-ammonia-methane ices
Temperature
~76 K cloud tops
Embed

Size neighbors

Objects near Uranus on the scale

On the logarithmic size axis, Uranus falls between Neptune and NGC 4395 Black Hole. The band uses nearby Ice giant planet records.

Shared physical scale
38,789km
Neptune49,244 km
Uranus50,724 km

Sources

References for Uranus

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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