Uranus

(Redirected from Uranus (planet))

For other uses, see Uranus (disambiguation).
Uranus Image:Uranus2 symbol.ant.png
Image:Uranus.jpg

Click image for description

Discovery
Discovered by William Herschel
Discovered on March 13, 1781
Orbital characteristics (Epoch J2000)
Semi-major axis 2,870,972,220 km
19.191 263 93 AU
Orbital circumference 18.029 Tm
120.515 AU
Eccentricity 0.047 167 71
Perihelion 2,735,555,035 km
18.286 055 96 AU
Aphelion 3,006,389,405 km
20.096 471 90 AU
Orbital period 30,707.4896 d
(84.07 a)
Synodic period 369.65 d
Orbital speed 6.795 km/s
Max. orbital speed 7.128 km/s
Min. orbital speed 6.486 km/s
Inclination 0.769 86°
(6.48° to Sun's equator)
Longitude of the
ascending node
74.229 88°
Argument of the
perihelion
96.734 36°
Number of satellites 27
Physical characteristics
Equatorial diameter 51,118 km
(4.007 Earths)
Polar diameter 49,946 km
(3.929 Earths)
Oblateness 0.0229
Surface area 8.084×109 km2
(15.849 Earths)
Volume 6.834×1013 km3
(63.086 Earths)
Mass 8.6832×1025 kg
(14.536 Earths)
Mean density 1.318 g/cm3
Equatorial gravity 8.69 m/s2
(0.886 gee)
Escape velocity 21.29 km/s
Rotation period 0.718 333 333 d (17 h 14 min 24.000 00 s) 1
Rotation velocity 2.59 km/s = 9320 km/h (at the equator)
Axial tilt 97.77°
Right ascension
of North pole
77.31° (5 h 9 min 15 s)
Declination +15.175°
Albedo 0.51
Cloudtop avg. temp. 55 K
Surface temp.
min mean max
59 K 68 K N/A K
Adjective Uranian
Atmospheric characteristics
Atmospheric pressure 120 kPa (at the cloud level)
Hydrogen 83%
Helium 15%
Methane 1.99%
Ammonia 0.01%
Ethane 0.00025%
Acetylene 0.00001%
Carbon monoxide
Hydrogen sulfide
trace

Uranus (pronounced either /jəˈɹeɪnəs/ or /ˈjuɹənəs/) is the seventh planet from the Sun. It is a gas giant, the third largest by diameter and fourth largest by mass. It is named after Ouranos, the Greek god of the sky, and progenitor of the other gods. Its symbol is either ♅ (Unicode U+2645, mostly astrological) or Image:X - Uranus B.png (mostly astronomical).

Contents

Physical characteristics

Composition

Uranus is composed primarily of rocks and various ices, with only about 15% hydrogen and a little helium (in contrast to Jupiter and Saturn which are mostly hydrogen). Uranus (like Neptune) is in many ways similar to the cores of Jupiter and Saturn minus the massive liquid metallic hydrogen envelope. It appears that Uranus does not have a rocky core like Jupiter and Saturn but rather that its material is more or less uniformly distributed. Uranus' cyan color is due to the absorption of red light by atmospheric methane. The surface temperature of Uranus's cloud cover is approximately 55 K (-218 °C or -360 °F).

Axial tilt

One of the most distinctive features of Uranus is its axial tilt of ninety-eight degrees. Consequently, for part of its orbit one pole faces the Sun continually whilst the other pole faces away. At the other side of Uranus' orbit the orientation of the poles towards the Sun is reversed. Between these two extremes of its orbit the Sun rises and sets around the equator normally.

At the time of Voyager 2's passage in 1986, Uranus' south pole was pointed almost directly at the Sun. Note that the labelling of this pole as "south" is actually in some dispute. Uranus can either be described as having an axial tilt of slightly more than 90°, or it can be described as having an axial tilt of slightly less than 90° and rotating in a retrograde direction; these two descriptions are exactly equivalent as physical descriptions of the planet but result in different definitions of which pole is the North Pole and which is the South Pole.

One result of this odd orientation is that the polar regions of Uranus receive a greater energy input from the Sun than its equatorial regions. Uranus is nevertheless hotter at its equator than at its poles, although the underlying mechanism which causes this is unknown. The reason for Uranus' extreme axial tilt is also not known. It is speculated that perhaps during the formation of the planet it collided with an enormous protoplanet, resulting in the skewed orientation.

It appears that Uranus' extreme axial tilt also results in extreme seasonal variations in its weather. During the Voyager 2 flyby, Uranus' banded cloud patterns were extremely bland and faint. Recent Hubble Space Telescope observations, however, show a more strongly banded appearance now that the Sun is approaching Uranus' equator. By 2007 the Sun will be directly over Uranus's equator.

Magnetic Field

Uranus' magnetic field is odd in that it is not centered on the center of the planet and is tilted almost 60° with respect to the axis of rotation. It is probably generated by motion at relatively shallow depths within Uranus. Neptune has a similarly displaced magnetic field, suggesting that this is not necessarily a result of Uranus' axial tilt. The magnetotail is twisted by the planet's rotation into a long corkscrew shape behind the planet. The magnetic field's 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.

Discovery and naming of Uranus

Uranus was the first planet to be discovered that was not known in ancient times, although it had been observed on many previous occasions but was always dismissed as simply another star. The earliest recorded sighting was in 1690 when John Flamsteed catalogued it as 34 Tauri. Flamsteed observed Uranus twice again, in 1712 and 1715. Bradley observed it in 1748, 1750 and 1753; Mayer in 1756. Le Monnier observed it four times in 1750, twice in 1768, six times in 1769, and one last time in 1771. He was a victim of his own disorderliness: one of his observations was found consigned on a paper bag used to store hair powder!

Sir William Herschel discovered the planet on March 13, 1781, but reported it on April 26, 1781 as a "comet": Account of a Comet, By Mr. Herschel, F. R. S.; Communicated by Dr. Watson, Jun. of Bath, F. R. S., Philosophical Transactions of the Royal Society of London, Volume 71, pp. 492-501.

Herschel originally named it Georgium Sidus (George's Star) in honour of King George III of England. When it was pointed out that sidus means star and not planet, he rebaptised it the Georgian Planet. In any case, this name was not acceptable outside of Britain. Lalande proposed in 1784 to name it Herschel, at the same time that he created the planet's symbol ("a globe surmounted by your initial"); his proposal was readily adopted by French astronomers. Prosperin, of Uppsala, proposed the names Astraea, Cybele, and Neptune (now borne by two asteroids and a planet). Lexell, of St. Petersburg, compromised with George III's Neptune and Great-Britain's Neptune. Bernoulli, from Berlin, suggested Hypercronius and Transaturnis. Lichtenberg, from Göttingen, chimed in with Austräa, a goddess mentioned by Ovid (but who is traditionally associated with Virgo). The name Minerva was also proposed [1]. Finally, Bode, as editor of the Berliner Astronomisches Jahrbuch, opted for Uranus, after the Greek god; Hell followed suit by using it in the first ephemeris, published in Vienna. Examination of earliest issues of Monthly Notices of the Royal Astronomical Society from 1827 shows that the name Uranus was already the most common name used even by British astronomers by then, and probably earlier. The name Georgium Sidus or "the Georgian" were still used infrequently (by the British alone) thereafter. The final holdout was HM Nautical Almanac Office, which did not switch to Uranus until 1850.

Exploration of Uranus

NASA's Voyager 2, is the only spacecraft to have visited the planet and no other visits are planned. Launched in 1977, Voyager made its closest approach to Uranus on January 24, 1986, before continuing on its journey to Neptune.

Visibility

The brightness of Uranus is between magnitude +5.5 and +6.0, so it can be seen with the naked eye as a faint star under dark sky conditions. It can be easily found with binoculars. From Earth it has a diameter of 4". Even in large telescopes no details can be seen on its disc.

Appearance

Stationary, retrograde Opposition Distance
to Earth (AU)
Maximum
Brightness (mag)
Diameter Stationary, prograde Conjunction to Sun
June 10, 2004 August 27, 2004 19.04165 5.7 3.68" November 12, 2004 February 22, 2004
June 15, 2005 September 1, 2005 19.06043 5.7 3.67" November 16, 2005 February 25, 2005
June 19, 2006 September 5, 2006 19.07541 5.7 3.67" November 20, 2006 March 1, 2006
June 23, 2007 September 9, 2007 19.08609 5.7 3.67" November 24, 2007 March 5, 2007
June 27, 2008 September 13, 2008 19.09220 5.7 3.67" November 27, 2008 March 8, 2008
July 1, 2009 September 17, 2009 19.09299 5.7 3.67" December 2, 2009 March 13, 2009
July 6, 2010 September 21, 2010 19.08823 5.7 3.67" December 6, 2010 March 17, 2010
July 10, 2011 September 26, 2011 19.07756 5.7 3.67" December 10, 2011 March 21, 2011
July 13, 2012 September 29, 2012 19.06142 5.7 3.67" December 13, 2012 March 24, 2012
July 17, 2013 October 3, 2013 19.04002 5.7 3.68" December 18, 2013 March 29, 2013
July 22, 2014 October 7, 2014 19.01421 5.7 3.68" December 22, 2014 April 2, 2014
July 26, 2015 October 12, 2015 18.98441 5.7 3.69" December 26, 2015 April 6, 2015
July 30, 2016 October 15, 2016 18.95124 5.7 3.70" December 29, 2016 April 9, 2016
August 3, 2017 October 19, 2017 18.91472 5.7 3.70" January 2, 2018 April 14, 2017
August 7, 2018 October 24, 2018 18.87531 5.7 3.71" January 7, 2019 April 18, 2018
August 12, 2019 October 28, 2019 18.83289 5.7 3.72" January 11, 2020 April 22, 2019
August 15, 2020 October 31, 2020 18.78765 5.7 3.73" January 14, 2021 April 26, 2020

The rings of Uranus

Main article: Rings of Uranus

Uranus has a faint planetary ring system, composed of dark particulate matter up to 10 metres in diameter. This ring system was discovered in March 1977 by James L. Elliot, Edward W. Dunham, and Douglas J. Mink, using the Kuiper Airborne Observatory. The discovery was serendipitous; they planned to use the occultation of a star by Uranus to study the planet's atmosphere, but when they analysed their observations they found that the star had disappeared briefly from view five times both before and after it disappeared behind the planet. They concluded that there must be a ring system around the planet; it was directly detected when the Voyager 2 space probe passed Uranus in 1986.

The moons of Uranus

Main article: Uranus' natural satellites

Uranus has 27 known moons. Names for these moons are chosen from characters from the works of Shakespeare and Alexander Pope. The five main satellites are Miranda, Ariel, Umbriel, Titania and Oberon.

For a timeline of discovery dates, see Timeline of natural satellites.

Uranus in fiction

  • Mr. Vivenair (a pseudonym) published A Journey Lately Performed Through the Air in an Aerostatic Globe, Commonly Called an Air Balloon, From This Terraquaeous Globe to the Newly Discovered Planet, Georgium Sidus in 1784.
  • In the Buck Rogers series (1928–), Uranus is portrayed as having biodomes and robots.
  • R. R. Winterbotham's "Clouds over Uranus" was published by Astounding in March of 1937
  • In the 1962 film Journey to the Seventh Planet, astronauts on (sic) Uranus encounter a strange intelligence.
  • In the Doctor Who (1963–) serial The Daleks' Master Plan, Uranus is described as being the only location in the universe where the mineral Taranium can be acquired.
  • In H. P. Lovecraft's Cthulhu Mythos (1928–), Uranus is known as L'gy'hx and is inhabited by cubical metallic many-legged creatures who worship Lrogg. They entered in religious conflict with the Shan. (Ramsey Campbell's The Insects from Shaggai, 1964)
  • In the cartoon Sailor Moon (19921997), Uranus is the seventh "Sailor Scout".
  • In the animated series Futurama (19992003), in 2620 the name of Uranus was changed to Urectum to get rid of "That Stupid Joke" once and for all.
  • In Wayne W. Dyer's Gifts from Eykis (2002), Eykis is a female from Uranus who imparts wisdom and spirituality to Earth.

External links

Uranus' natural satellitesedit
Cordelia | Ophelia | Bianca | Cressida | Desdemona | Juliet | Portia | Rosalind | S/2003 U 2 | Belinda
S/1986 U 10 | Puck | S/2003 U 1 | Miranda | Ariel | Umbriel | Titania | Oberon | S/2001 U 3
Caliban | Stephano | Trinculo | Sycorax | Margaret | Prospero | Setebos | S/2001 U 2


Our Solar Systemedit
Sun | Mercury | Venus | Earth (Moon) | Mars | Asteroid belt
Jupiter | Saturn | Uranus | Neptune | Pluto | Kuiper belt | Scattered disc | Oort cloud
 See also astronomical objects and the solar system's list of objects, sorted by radius or mass
ar:اورانوس

bg:Уран (планета) ca:Urà (planeta) cs:Uran (planeta) cy:Wranws da:Uranus (planet) de:Uranus (Planet) et:Uraan (planeet) es:Urano (planeta) eo:Urano fa:اورانوس (سیاره) fr:Uranus (planète) ga:Úránas (pláinéad) gu:યુરેનસ (ગ્રહ) ko:천왕성 hr:Uran (planet) io:Urano id:Uranus it:Urano (astronomia) la:Uranus (planeta) lt:Uranas_(planeta) hu:Uránusz (bolygó) ms:Uranus nl:Uranus (planeet) ja:天王星 no:Uranus nn:Planeten Uranus pl:Uran (planeta) pt:Urano (planeta) ro:Uranus (planetă) ru:Уран (планета) simple:Uranus (planet) sk:Urán (planéta) sl:Uran (planet) sr:Уран (планета) fi:Uranus sv:Uranus (planet) th:ดาวยูเรนัส tr:Uranüs (gezegen) vi:Thiên Vương Tinh uk:Уран (планета) zh:天王星