SolarExplorer

Ice Giant

Uranus

Uranus is an ice giant unique for its extreme axial tilt. Its cyan color is due to atmospheric methane absorbing red light, and its atmosphere is the coldest in the solar system.

Equatorial Diameter

51,118 km

Surface Temperature

-210°C

Mass

8.681 × 10^25 kg

Surface Gravity

8.7 m/s²

Axial Tilt

97.77°

Rotation Period

17h 14m

Orbital Period

84 years

Moons

27 Known

Planetary Structure & Atmosphere

Uranus is an ice giant composed primarily of water, ammonia, and methane ices surrounding a small rocky core. Methane in its upper atmosphere absorbs red light, imparting a distinct pale cyan color. It spins almost entirely on its side with an axial tilt of 97.8°.

Atmospheric Composition

Hydrogen ($H_2$)82.5%
Helium ($He$)15.2%
Methane ($CH_4$) Ice2.3%

Cosmic Weight & Age Matrix

70 kg Human Weight
62.0 kg
0.886x Earth Gravity
20 Earth Years Equivalent
0.238 Years
Uranus Orbital Years (84 Yrs)
Escape Velocity
21.3 km/s
1.90x Earth Escape Velocity

Scientific Discoveries

  1. Uranus orbits the Sun on its side, with an axial tilt of 97.77 degrees.
  2. Due to its extreme tilt, one pole faces the Sun for 42 years, followed by 42 years of darkness.
  3. It was the first planet to be discovered by the use of a modern telescope, credited to William Herschel in 1781.
  4. It is theorized that extreme pressures within Uranus could break down methane and form diamond rain.
  5. Uranus has 13 known rings, which are very dark and narrow.
  6. When in opposition with the Sun relative to Earth, Uranus can become visible to the naked eye, appearing as a faint star under dark sky conditions.