Uranus
- Nguyen Khoa
- Jun 18
- 2 min read
Uranus’s axial tilt, magnetic anomalies, and icy composition make it a puzzle for planetary scientists.

Introduction
Uranus is an ice giant famed for its unprecedented axial tilt – it rotates on its side at 97.77°, so it looks like it's rolling around the Sun. It has 13 thin rings, 28 moons, and ferocious winds. Uranus was the first planet to be found telescopically, by William Herschel in 1781.
Potential for Life
Although Herschel intended to name it after King George III, astronomers settled on Uranus, after the Greek god of the sky. Uranus is too cold, windy, and high-pressure to support life as we know it. Some moons might have oceans beneath their surfaces, but conditions are still harsh.
Properties
Property | Value |
Size and distance |
|
Orbit and Rotation |
|
Moons |
|
Rings |
|
Surface and Atmosphere
No solid surface
Atmosphere: mostly hydrogen, helium, methane
Red light is absorbed by methane, so Uranus looks blue-green.
Winds: 900 km/h
Coldest planet in some spots: -224.2°C
Magnetosphere
The magnetic field is 60° tilted and off-center.
Creates a twisted, corkscrew-shaped tail
Auroras are irregular and non-pole-oriented

Summary
Uranus is a cold, blue-green ice giant that rotates on its side with a 98° tilt, causing extreme seasons that last over 20 years. It was discovered in 1781 and is made of icy fluids, hydrogen, helium, and methane, giving it its unique color. Uranus has 13 rings, 28 moons (named after literary characters), and fierce winds up to 900 km/h. It has no solid surface and is one of the coldest planets, reaching –224°C. Its magnetic field is tilted and off-center, creating unusual, off-pole auroras and a twisted magnetic tail. While Uranus is uninhabitable, some of its moons may hide subsurface oceans.
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