Wednesday, January 19, 2011

Uranus



Uranus is the seventh planet from the sun in our solar system. This huge, icy planet is covered with clouds and is encircled by a belt of 11 rings and 22 known moons. Uranus' blue color is caused by the methane (CH4) in its atmosphere; this molecule absorbs red light.

ROTATIONAL AXIS
Uranus' rotational axis is strongly tilted on its side (97.9°). Instead of rotating with its axis roughly perpendicular to the plane of its orbit (like all the other planets in our Solar System), Uranus rotates on its side (along its orbital path). This tipped rotational axis gives rise to extreme seasons on Uranus.

Because of its almost-perpendicular axis orientation, there is a debate over which of Uranus' poles is its north pole. This debates leads to yet another: Is Uranus spinning in a retrograde orbit (like Venus) or not (like the other planets)?

SIZE
Uranus is about 31,690 miles (51,118 km) in diameter. This is about 4 times the diameter of the Earth.

This gas giant is the third-largest planet in our Solar System (after Jupiter and Saturn).

MASS AND GRAVITY
Uranus' mass is about 8.68 x 1025 kg. This is about 14 times the mass of the Earth. The gravity on Uranus is only 91% of the gravity on Earth. This is because it is such a large planet (and the gravitational force a planet exerts upon an object at the planet's surface is proportional to its mass and to the inverse of its radius squared).

A 100-pound person on Uranus would weigh 91 pounds.

LENGTH OF A DAY AND YEAR ON URANUS
Each day on Uranus takes 17.9 Earth hours. A year on Uranus takes 84.07 Earth years; it takes 84.07 Earth years for Uranus to orbit the sun once.

URANUS' ORBIT AND DISTANCE FROM THE SUN
Uranus is over 19 times as far from the Sun as the Earth is; it averages 19.18 A.U.

At aphelion (the farthest point in its solar orbit) it is 1,850,000,000 miles (3,003,000,000 km) from the Sun. At perihelion (the closest point in its solar orbit) it is 1,700,000,000 miles (2,739,000,000 km) from the Sun.

TEMPERATURE
The mean temperature on the surface of Uranus' cloud layer is -350°F (59 K). Uranus radiates very little heat in comparison with the other gas giants, Jupiter, Saturn and Neptune).

PLANETARY COMPOSITION AND ATMOSPHERE
Uranus is a frozen, gaseous planet with a molten core. Uranus' atmosphere consists of 83% hydrogen, 15% helium and 2% methane.



RINGS

Uranus and its rings photographed by an infrared camera.
Uranus has a belt of 11 faint, narrow rings composed of rock and dust. They circle Uranus is very elliptical orbits. These rings are only a fraction of the size of Saturn's rings, and were only discovered in 1977.




MOONS

Oberon, the largest moon of Uranus. Photo taken by NASA's Voyager mission in 1986.
Uranus has 5 large moons (2 were discovered by Wm. Herschel in 1781, 2 were discovered by Wm. Lassell in 1851, and one by G. Kuiper in 1948) and many small moons (which were discovered much later).



DISCOVERY OF URANUS
Uranus was discovered by the British astronomer William Herschel on March 13, 1781. Herschel also discovered two of the moons of Uranus (Titania and Oberon) and some of the moons of Saturn.

URANUS-EARTH COMPARISON



URANUS' NAME AND SYMBOL

This is the symbol of the planet Uranus.
This planet was originally named in 1781 by the British astronomer William Herschel - he called it Georgium Sidus (meaning "the Georgian planet") to honor the King George III of England. The name was later changed to Uranus, the ancient mythological god of the sky, Ouranos. The name Uranus was suggested by the German astronomer Johann Elert Bode.

SPACECRAFT VISITS
Uranus has been visited by NASA's Voyager 2, whose closest approach was on January 24, 1986. 


URANUS' ROTATIONAL TILT AND EXTREME SEASONS
Uranus' rotational axis is strongly tilted on its side (97.9°). Instead of rotating with its axis roughly perpendicular to the plane of its orbit (like all the other planets in our Solar System), Uranus rotates on its side (along its orbital path). This tipped rotational axis gives rise to extreme seasons on Uranus.




A catastrophic collision with another large body eons ago may have tipped Uranus over on its side. 

INSIDE URANUS
PLANETARY COMPOSITION AND ATMOSPHERE
Uranus is a frozen, gaseous planet.

Atmosphere: The planet is shrouded in an icy cloud layer (made up of frozen methane, ethane, and acetylene) circling this planet at 185 mph (300 kph. Uranus' icy atmosphere consist of 83% hydrogen,15% helium, and 2% methane. The outer layers of the atmosphere are the coldest; temperature and pressure rise under the cloud layer.

Partially-solid Layers: Beneath the atmosphere, there is a liquid layer of hydrogen and helium. As depth increases, this layer becomes more viscous, and then partly solid. This layer may be composed of compressed water with ammonia and methane.

Core: Uranus has a molten rocky core about 10,500 miles (17,000 km) in diameter and about 12,500°F (6927°C). This core may have a mass five times greater than the mass of the Earth. 

URANUS' RINGS

Uranus and its rings photographed by an infrared camera.
Uranus has a belt of 11 faint, narrow rings composed of rock and dust. They circle Uranus is very elliptical orbits. These rings are only a fraction of the size of Saturn's rings, and were only discovered in 1977.



RingDistance from the center of Uranus (km)Width of the ring (km)
Epsilon51,14020-96
1986 U1R50,0201 to 2
Delta48,2903 to 7
Gamma47,6301 to 4
Eta47,190less than 1 to 2
Beta45,6707 to 12
Alpha44,7207 to 12
Ring 442,5802 to 3
Ring 542,2302 to 3
Ring 641,8401 to 3
1986 U2R38,000.
 
Uranus Statistics
Discovered byWilliam Herschel
Date of discovery1781
Mass (kg)8.686e+25
Mass (Earth = 1)1.4535e+01
Equatorial radius (km)25,559
Equatorial radius (Earth = 1)4.0074
Mean density (gm/cm^3)1.29
Mean distance from the Sun (km)2,870,990,000
Mean distance from the Sun (Earth = 1)19.1914
Rotational period (hours)-17.9
Orbital period (years)84.01
Mean orbital velocity (km/sec)6.81
Orbital eccentricity0.0461
Tilt of axis (degrees)97.86
Orbital inclination (degrees)0.774
Equatorial surface gravity (m/sec^2)7.77
Equatorial escape velocity (km/sec)21.30
Visual geometric albedo0.51
Magnitude (Vo)5.52
Mean cloud temperature-193°C
Atmospheric pressure (bars)1.2
Atmospheric composition
Hydrogen
Helium
Methane

83%
15%
2%

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