1. Uranus

2. Uranus Uranus is the seventh planet from the Sun and the third-largest and fourth most massive planet in the Solar System. It is named after the ancient Greek deity of the sky (Uranus), the father of Kronos (Saturn) and grandfather of Zeus (Jupiter). Though it is visible to the naked eye like the five classical planets, it was never recognized as a planet by ancient observers because of its dimness and slow orbit. Uranus is the seventh planet from the Sun and the third-largest and fourth most massive planet in the Solar System. It is named after the ancient Greek deity of the sky (Uranus), the father of Kronos (Saturn) and grandfather of Zeus (Jupiter). Though it is visible to the naked eye like the five classical planets, it was never recognized as a planet by ancient observers because of its dimness and slow orbit.planetSunSolar SystemUranusKronosSaturnZeusJupiter classical planetsplanetSunSolar SystemUranusKronosSaturnZeusJupiter classical planets

3. Uranus has a mean distance from the Sun of 2.87 billion kilometers (1.78 billion miles). It rotates about its axis once every 17 hours 14 minutes. Uranus has at least 22 moons. Uranus has a mean distance from the Sun of 2.87 billion kilometers (1.78 billion miles). It rotates about its axis once every 17 hours 14 minutes. Uranus has at least 22 moons.

4. The atmosphere of Uranus is composed of 83% hydrogen, 15% helium, 2% methane and small amounts of acetylene and other hydrocarbons. Methane in the upper atmosphere absorbs red light, giving Uranus its blue-green color. The atmosphere is arranged into clouds running at constant latitudes, similar to the orientation of the more vivid latitudinal bands seen on Jupiter and Saturn.

5. Winds at mid-latitudes on Uranus blow in the direction of the planet's rotation. These winds blow at velocities of 40 to 160 meters per second (90 to 360 miles per hour). Radio science experiments found winds of about 100 meters per second blowing in the opposite direction at the equator. Winds at mid-latitudes on Uranus blow in the direction of the planet's rotation. These winds blow at velocities of 40 to 160 meters per second (90 to 360 miles per hour). Radio science experiments found winds of about 100 meters per second blowing in the opposite direction at the equator.

6. Uranus is a giant ball of gas and liquid. Its diameter at the equator is 31,763 miles (51,118 kilometers), over four times that of Earth. The surface of Uranus consists of blue-green clouds made up of tiny crystals of methane. The crystals have frozen out of the planet's atmosphere. Far below the visible clouds are probably thicker cloud layers made up of liquid water and crystals of ammonia ice. Uranus is a giant ball of gas and liquid. Its diameter at the equator is 31,763 miles (51,118 kilometers), over four times that of Earth. The surface of Uranus consists of blue-green clouds made up of tiny crystals of methane. The crystals have frozen out of the planet's atmosphere. Far below the visible clouds are probably thicker cloud layers made up of liquid water and crystals of ammonia ice.

7. Deeper still -- about 4,700 miles (7,500 kilometers) below the visible cloud tops -- may be an ocean of liquid water containing dissolved ammonia. At the very center of the planet may be a rocky core about the size of Earth. Scientists doubt Uranus has any form of life. Deeper still -- about 4,700 miles (7,500 kilometers) below the visible cloud tops -- may be an ocean of liquid water containing dissolved ammonia. At the very center of the planet may be a rocky core about the size of Earth. Scientists doubt Uranus has any form of life.

8. Uranus travels around the sun in an elliptical (oval-shaped) orbit, which it completes in 30,685 Earth days, or just over 84 Earth years. As it orbits the sun, Uranus also rotates on its axis, an imaginary line through its center. The planet's interior (ocean and core) takes 17 hours 14 minutes to spin around once on its axis. However, much of the atmosphere rotates faster than that. Uranus travels around the sun in an elliptical (oval-shaped) orbit, which it completes in 30,685 Earth days, or just over 84 Earth years. As it orbits the sun, Uranus also rotates on its axis, an imaginary line through its center. The planet's interior (ocean and core) takes 17 hours 14 minutes to spin around once on its axis. However, much of the atmosphere rotates faster than that.

9. The fastest winds on Uranus, measured about two-thirds of the way from the equator to the south pole, blow at about 450 miles per hour (720 kilometers per hour). Thus, this area toward the south pole makes one complete rotation every 14 hours. The fastest winds on Uranus, measured about two-thirds of the way from the equator to the south pole, blow at about 450 miles per hour (720 kilometers per hour). Thus, this area toward the south pole makes one complete rotation every 14 hours.

10. Uranus is the farthest planet that can be seen without a telescope. Its average distance from the sun is about 1,784,860,000 miles (2,872,460,000 kilometers), a distance that takes light about 2 hours 40 minutes to travel. Uranus is the farthest planet that can be seen without a telescope. Its average distance from the sun is about 1,784,860,000 miles (2,872,460,000 kilometers), a distance that takes light about 2 hours 40 minutes to travel.

11. Uranus is the planet tipped on its side. Uranus spins more like a barrel on its side than a top. This strange tilt may be the result of a collision with another body that tipped Uranus on its side. Uranus is the planet tipped on its side. Uranus spins more like a barrel on its side than a top. This strange tilt may be the result of a collision with another body that tipped Uranus on its side.

12. Uranus Temperature: Uranus is very cold — its average temperature is –350° F (–210° C). Temperature: Uranus is very cold — its average temperature is –350° F (–210° C). Uranus’ 5 biggest planets: Ariel, Umbriel, Titania, Oberon, and Miranda. There are at least 22 smaller moons. Uranus’ 5 biggest planets: Ariel, Umbriel, Titania, Oberon, and Miranda. There are at least 22 smaller moons.

13. Uranus is similar in composition to Neptune, and both have different compositions from those of the larger gas giants Jupiter and Saturn. As such, astronomers sometimes place them in a separate category, the "ice giants". Uranus's atmosphere, while similar to Jupiter's and Saturn's in being composed primarily of hydrogen and helium, contains a higher proportion of "ices" such as water, ammonia and methane, along with the usual traces of hydrocarbons Uranus is similar in composition to Neptune, and both have different compositions from those of the larger gas giants Jupiter and Saturn. As such, astronomers sometimes place them in a separate category, the "ice giants". Uranus's atmosphere, while similar to Jupiter's and Saturn's in being composed primarily of hydrogen and helium, contains a higher proportion of "ices" such as water, ammonia and methane, along with the usual traces of hydrocarbons Neptunegas giantsJupiterSaturnice giantshydrogenhelium waterammoniamethanehydrocarbons Neptunegas giantsJupiterSaturnice giantshydrogenhelium waterammoniamethanehydrocarbons

14. TRIVIA TRIVIA

15. QUESTION 1. What are the 5 biggest moons of URANUS? 1. What are the 5 biggest moons of URANUS?

16. ANSWER Ariel, Umbriel, Titania, Oberon, and Miranda Ariel, Umbriel, Titania, Oberon, and Miranda

17. QUESTION What is the order of Uranus from the sun?

18. ANSWER seventh

19. QUESTION What percent is Uranus’ hydrogen? What percent is Uranus’ hydrogen?

20. ANSWER 83% 83%

22. Reference http://www.nasa.gov/worldbook/uranus_worldbo ok.html http://www.nasa.gov/worldbook/uranus_worldbo ok.html http://www.nasa.gov/worldbook/uranus_worldbo ok.html http://www.nasa.gov/worldbook/uranus_worldbo ok.html http://en.wikipedia.org/wiki/Uranus http://en.wikipedia.org/wiki/Uranus http://en.wikipedia.org/wiki/Uranus http://www.astronomy.com/asy/default.aspx?c=a &id=1226 http://www.astronomy.com/asy/default.aspx?c=a &id=1226 http://www.astronomy.com/asy/default.aspx?c=a &id=1226 http://www.astronomy.com/asy/default.aspx?c=a &id=1226 http://solarsystem.nasa.gov/planets/profile.cfm? Object=Uranus http://solarsystem.nasa.gov/planets/profile.cfm? Object=Uranus http://solarsystem.nasa.gov/planets/profile.cfm? Object=Uranus http://solarsystem.nasa.gov/planets/profile.cfm? Object=Uranus http://www.solarviews.com/eng/uranus.htm http://www.solarviews.com/eng/uranus.htm http://www.solarviews.com/eng/uranus.htm http://images.search.yahoo.com/search/images?_a dv_prop=image&fr=yfp-t-501&va=uranus&sz= http://images.search.yahoo.com/search/images?_a dv_prop=image&fr=yfp-t-501&va=uranus&sz= http://images.search.yahoo.com/search/images?_a dv_prop=image&fr=yfp-t-501&va=uranus&sz http://images.search.yahoo.com/search/images?_a dv_prop=image&fr=yfp-t-501&va=uranus&sz