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Uranus is the seventh planet from the Sun and is the third largest in the solar system. It was discovered by
William Herschel in 1781. It has an equatorial diameter of 51,800 kilometres (32,190 miles) and orbits
the Sun once every 84.01 Earth years. It has a mean distance from the Sun of 2.87 billion kilometres (1.78
billion miles). The length of a day on Uranus is 17 hours 14 minutes. Uranus has at least 15 moons. The
two largest moons, Titania and Oberon, were discovered by William Herschel in 1787.
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 colour. 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. 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.
Uranus is distinguished by the fact that it is tipped on its side. Its unusual position is thought to be the
result of a collision with a planet-sized body early in the solar system's history. Voyager 2 found that one
of the most striking influences of this sideways position is its effect on the tail of the magnetic field,
which is itself tilted 60 degrees from the planet's axis of rotation. The magnetotail was shown to be
twisted by the planet's rotation into a long corkscrew shape behind the planet. The magnetic field source
is unknown; the electrically conductive, super-pressurized ocean of water and ammonia once thought to
lie between the core and the atmosphere now appears to be nonexistent. The magnetic fields of Earth and
other planets are believed to arise from electrical currents produced in their molten cores.
Uranus' Rings
In 1977, the first nine rings of Uranus were discovered. During the Voyager encounters, these rings were
photographed and measured, as were two other new rings and ringlets. Uranus' rings are distinctly
different from those at Jupiter and Saturn. The outermost epsilon ring is composed mostly of ice boulders
several feet across. A very tenuous distribution of fine dust also seems to be spread throughout the ring
system.
There may be a large number of narrow rings, or possibly incomplete rings or ring arcs, as small as 50
meters (160 feet) in width. The individual ring particles were found to be of low reflectivity. At least one
ring, the epsilon, was found to be grey in colour. The moons Cordelia and Ophelia act as shepherd
satellites for the epsilon ring.
Uranus Statistics:
Time taken to orbit the Sun in Earth years: 84.0
Average orbital velocity in miles/second (km/sec): 4.2 (6.8)
Angle between orbit of planet and orbit of Earth: 0.77º
Time taken to rotate on axis in Earth time: 16hr
Tilt of axis to perpendicular of orbital plane: 98º
Average distance from Sun in astronomical units*: 19.2
Average distance from Sun in miles (km): 1783 million (2870 million)
Average surface temperature in degrees Celsius: -218º (at cloud tops)
Density relative to water: 1.7
Equatorial diameter relative to Earth diameter**: 4.1
Equatorial diameter in miles (km): 32,300 (52,000)
Mass relative to Earth: 15
Escape velocity in miles/second (km/sec): 13.3 (21.41)
Number of known moons: 15
Number of known rings: 10
Date of discovery: 1781
* One astronomical unit is 92,956,000 miles (149,598,000km)
** Earth's diameter is 7,926 miles (12,756km) |