Two views of Uranus

Two views of Uranus, one in true color (left) and the other in false color, compiled from images returned Jan. 17, 1986, by Voyager 2. The spacecraft was 9.1 million km (5.7 million miles) from the planet, several days from closest approach. Image:JPL - NASA

 

Two views of Uranus in false color

Two sides of Uranus, imaged through colored filters, showing long-lived clouds drifting across the surface. Image: Lawrence Sromovsky, UW-Madison

 

Uranus

Heaven's God and Gaya husband, the Earth's Goddess. It is the 7th planet from Sun and the 3rd in size of 4 Gaseous Giants.

Once considered one of the blander-looking planets, Uranus (pronounced YOOR un nus) has been revealed as a dynamic world with some of the brightest clouds in the outer solar system and 11 rings. The first planet found with the aid of a telescope, Uranus was discovered in 1781 by astronomer William Herschel. The seventh planet from the Sun is so distant that it takes 84 years to complete one orbit. Uranus, with no solid surface, is one of the gas giant planets (the others are Jupiter, Saturn, and Neptune).

The atmosphere of Uranus is composed primarily of hydrogen and helium, with a small amount of methane and traces of water and ammonia. Uranus gets its blue-green color from methane gas. Sunlight is reflected from Uranus' cloud tops, which lie beneath a layer of methane gas. As the reflected sunlight passes back through this layer, the methane gas absorbs the red portion of the light, allowing the blue portion to pass through, resulting in the blue-green color that we see. The planet's atmospheric details are very difficult to see in visible light. The bulk (80 percent or more) of the mass of Uranus is contained in an extended liquid core consisting primarily of 'icy' materials (water, methane, and ammonia), with higher-density material at depth.

In 1986, Voyager 2 observed faint cloud markings in the southern latitudes blowing westward between 100 and 600 kilometers (60 and 400 miles) per hour. In 2004, the Keck Observatory in Hawaii used advanced optics to capture highly detailed images of Uranus as the planet approached its southern autumnal equinox, when the equator will be vertically illuminated by the Sun.

Uranus' rotation axis is nearly horizontal as though Uranus has been knocked on its side, as compared to most other planets in our solar system. This unusual orientation may be the result of a collision with a planet-sized body early in the planet's history, which apparently radically changed Uranus' rotation. Additionally, while magnetic fields are typically in alignment with a planet's rotation, Uranus' magnetic field is tipped over: instead of aligning along the rotational axis, the magnetic axis is tilted nearly 60 degrees from the planet's axis of rotation, and is also offset from the center of the planet by one-third of the planet's radius. Unlike the magnetic fields of Earth, Jupiter, and Saturn, which can be thought of as acting like dipole bar magnets, the fields of Uranus (and Neptune also) are very irregular. Uranus' magnetic field is about 48 times more powerful than Earth's.

Even though Uranus is tipped on its side and experiences seasons that last over 20 years, the temperature differences on the summer and winter sides do not differ greatly because the planet is so far from the Sun. Near the cloud tops, the temperature of Uranus is -216 degrees Celsius (-357 degrees Fahrenheit).

Because of the planet's unusual orientation, Uranus' rings are perpendicular to its orbital path about the Sun. The 10 outer rings are dark, thin, and narrow, while the 11th ring is inside the others and is broad and diffuse. Uranus has 27 known moons, named mostly for characters from the works of William Shakespeare and Alexander Pope. Miranda is the strangest-looking Uranian moon, appearing as though it were made of spare parts. The high cliffs and winding valleys of the moon may indicate partial melting of the interior, with icy material occasionally drifting to the surface.

Uranus Data
Discovered By William Herschel
Date of Discovery 1781
Average Distance from the Sun 2,870,972,200 km
Perihelion (closest) 2,735,560,000 km
Aphelion (farthest) 3,006,390,000 km
Equatorial Radius 25,559 km
Equatorial Circumference 160,592 km
Volume (Earth 1) 63.1
Mass (Earth 1) 14.371
Density 1.30 g/cm3
Surface Area 8,115,600,000 km2
Equatorial Surface Gravity  8.43 m/s2
Escape Velocity 76,640 km/h
Sidereal Rotation Period (Length of Day) -0.7196 Earth days (retrograde)
Sidereal Orbit Period (Length of Year) 84.02 Earth years
Mean Orbit Velocity 24,607 km/h
Orbital Eccentricity 0.047168
Orbital Inclination to Ecliptic 0.770 degrees
Equatorial Inclination to Orbit 97.86 degrees
Orbital Circumference 17,620,000,000 km
Effective Temperature -216 °C
Atmospheric Constituents Hydrogen, Helium, Methane
Uranus Moons Uranus rings
1. Cordelia 1986U2R
2. Ophelia 6
3. Bianca 5
4. Cressida 4
5. Desdemona Alpha
6. Juliet Beta
7. Portia Eta
8. Rosalind Gamma
9. Cupid Delta
10. Belinda Lambda
11. Perdita Epsilon
12. Puck R/2003 U1
13. Mab R/2003 U2
14. Miranda  
15. Ariel  
16. Umbriel  
17. Titania  
18. Oberon  
19. Francisco  
20. Caliban  
21. Stephano  
22. Trinculo  
23. Sycorax  
24. Margaret  
25. Prospero  
26. Setebos  
27. Ferdinand  

 

Information from: SSE-JPL-NASA

spacer