Uranus

To the eye alone, Uranus is a dull planet. It looks like a featureless blue-green ball, with few of the dynamic cloud patterns that decorate Jupiter and Saturn. Yet Uranus may have the most interesting history of any planet in the solar system: A collision soon after its birth may have knocked the planet sideways.

Uranus

Uranus At a Glance

Discovery

1781, William Herschel

Name

Greek sky god, first ruler of the Titans

Average Distance from Sun

1,783,939,400 miles
2,870,972,200 km
19.2 Astronomical Units

Mass

14.4 times Earth's mass

Equatorial Diameter

31,764 miles
51,118 km

Length of Day

17 hours, 14 minutes

Length of Year

84 Earth years

Surface Gravity

0.86 that of Earth (If you weigh 100 pounds, you would weigh about 86 pounds on Uranus)

Known Moons

27 as of January 2006

The poles of most planets aim away from the plane of the solar system; like Earth's poles, they point roughly north and south. But the poles of Uranus point east and west, close to the plane of its orbit around the Sun. As a result, its north pole aims at the Sun at the beginning of northern summer, and away from the Sun at the start of southern summer. That gives the planet's northern and southern hemispheres 42 years of sunlight followed by 42 years of darkness. This sideways tilt also creates weather patterns unlike those on any other planet, with winds and clouds changing directions with the seasons.

Detecting and tracking the clouds on Uranus is difficult, however. Uranus is so far away that it appears as little more than a fuzzy green blob in ground-based telescopes. A layer of haze atop the atmosphere gives Uranus a uniform blue-green color, hiding most of the cloud formations that move around the planet. Not until recent years, when astronomers began using telescopes that could overcome the distorting effects of Earth's atmosphere, did they begin to see detailed features. Infrared and ultraviolet instruments attached to these telescopes penetrate the haze, allowing astronomers to see deeper into the planet's atmosphere.

Even then, there's not a lot to see. Uranus receives little heat from the Sun, and it does not produce much on its own, so there is no energy source to produce the dramatic cloud bands and weather systems seen on other worlds.

Like Jupiter and Saturn, an envelope of hydrogen and helium lies below the thin upper layers of Uranus' atmosphere. On Uranus, though, the layer of hydrogen and helium is not as thick as on the larger planets, extending perhaps only one-fifth of the distance down from its cloudtops.

 A liquid or partially frozen mixture of water, methane, and rocky minerals may lie beneath the hydrogen and helium. Unlike the region where the oceans and air meet on Earth, though, there probably isn't a sharp boundary between the layers of Uranus. The atmospheric pressure is so great that the liquid and gas merge in a slushy transition zone. This zone surrounds a dense, rocky core.

Narrow rings encircle Uranus, but their material is darker than charcoal, so astronomers didn't discover them until 1977, when the rings blocked the light of a star that was about to pass behind Uranus. The rings are the thinnest of any planet in the solar system, consisting of a single layer of particles. Some of the particles are as large as SUVs, though, which is far larger than most particles in the rings of other planets. These large particles suggest that the rings formed fairly recently, when a small moon was pulverized by a collision with a comet or asteroid.

Literary Moons: Titania, Oberon, Ariel, and Umbriel

For a man who made his reputation by counting and plotting the locations of thousands of stars, astronomer John Herschel had a poetic heart. In 1851, he named the four largest moons of Uranus. Instead of picking characters from mythology, he turned to the works of William Shakespeare and Alexander Pope. He named Oberon and Titania for the king and queen of the fairies from Shakespeare's A Midsummer Night's Dream. Ariel and Umbriel were spirits in Pope's The Rape of the Lock.

Titania is Uranus' largest moon. Small impact craters and long, tall cracks scar its icy crust. The cracks probably formed as the gravity of Uranus and its other moons pulled and twisted Titania.

The most interesting moon may be Miranda, which has canyons up to 12 miles (20 km) deep. It, too, may have been reshaped by the gravitational pull of Uranus and its moons.

Uranus's Moons

1. Cordelia
2. Ophelia
3. Bianca
4. Cressida
5. Desdemona
6. Juliet
7. Portia
8. Rosalind
9. Mab
10. Belinda
11. Perdita
12. Puck
13. Cupid
14. Miranda
15. Francisco
16. Ariel
17. Umbriel
18. Titania
19. Oberon
20. Caliban
21. Stephano
22. Trinculo
23. Sycorax
24. Margaret
25. Prospero
26. Setebos
27. Ferdinand
Viewing Guide

Visible in early October; requires very dark skies and good eyes.

Exploration

Only one spacecraft has ever visited Uranus. Voyager 2 flew past the giant planet in 1986.

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