Editing Uranus

{{Short description|Seventh planet from the Sun}}
{{About|the planet|the Greek god|Uranus (mythology)||Uranus (disambiguation)|and|Uranian (disambiguation)}}
{{Featured article}}
{{Pp-semi-indef}}
{{Pp-move}}
{{Use British English|date=October 2024}}
{{Use dmy dates|date=October 2024}}
{{Infobox planet
| name = Uranus
| symbol = [[File:Uranus symbol (bold).svg|24px|⛢|class=skin-invert]], [[File:Uranus monogram (bold).svg|24px|♅|class=skin-invert]]
| image = Uranus Voyager2 color calibrated.png
| caption = Uranus in true colour,{{efn|Based on {{Cite journal |last1=Irwin |first1=Patrick G J |last2=Dobinson |first2=Jack |last3=James |first3=Arjuna |last4=Teanby |first4=Nicholas A |last5=Simon |first5=Amy A |last6=Fletcher |first6=Leigh N |last7=Roman |first7=Michael T |last8=Orton |first8=Glenn S |last9=Wong |first9=Michael H |last10=Toledo |first10=Daniel |last11=Pérez-Hoyos |first11=Santiago |last12=Beck |first12=Julie |date=23 December 2023 |title=Modelling the seasonal cycle of Uranus's colour and magnitude, and comparison with Neptune |url=https://academic.oup.com/mnras/article/527/4/11521/7511973 |journal=Monthly Notices of the Royal Astronomical Society |language=en |volume=527 |issue=4 |pages=11521–11538 |doi=10.1093/mnras/stad3761 |issn=0035-8711|doi-access=free |hdl=20.500.11850/657542 |hdl-access=free }}}} as captured by ''[[Voyager 2]]''. Its pale, muted appearance is due to a shroud of haze above its clouds
| background = LightBlue
| discoverer = [[{{#property:P61}}]]
| discovered = {{#time:j F Y|{{#property:P575}}}}
| orbit_ref = <ref name="VSOP87" />{{efn | These are the mean elements from VSOP87, together with derived quantities.}}
| epoch = [[J2000]]
| aphelion = {{convert|3.00639|e9km|AU|lk=on|order=flip|comma=gaps|abbr=unit}}
| perihelion = {{convert|2.73556|e9km|AU|lk=off|order=flip|comma=gaps|abbr=unit}}
| time_periastron = 17–19 August 2050<ref>Jean Meeus, ''Astronomical Algorithms'' (Richmond, Virginia: Willmann-Bell, 1998) p271. Bretagnon's complete VSOP87 model. It gives the 17th @ 18.283075301au. http://vo.imcce.fr/webservices/miriade/?forms {{Webarchive|url=https://web.archive.org/web/20210907050257/http://vo.imcce.fr/webservices/miriade/?forms |date=7 September 2021 }} IMCCE Observatoire de Paris / CNRS Calculated for a series of dates, five or ten days apart, in August 2050, using an interpolation formula from ''Astronomical Algorithms''. Perihelion came very early on the 17th. INPOP planetary theory</ref><ref name=horizons-perihelion>{{Cite web|url=https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%27799%27&START_TIME=%272050-08-01%27&STOP_TIME=%272050-08-30%27&STEP_SIZE=%273%20hours%27&QUANTITIES=%2719%27|title=HORIZONS Planet-center Batch call for August 2050 Perihelion|website=ssd.jpl.nasa.gov|type=Perihelion for Uranus planet-center (799) occurs on 2050-Aug-19 at 18.28307512au during a rdot flip from negative to positive|publisher=NASA/JPL|access-date=7 September 2021|archive-date=7 September 2021|archive-url=https://web.archive.org/web/20210907215700/https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%27799%27&START_TIME=%272050-08-01%27&STOP_TIME=%272050-08-30%27&STEP_SIZE=%273%20hours%27&QUANTITIES=%2719%27|url-status=live}}</ref>
| semimajor = {{convert|2.870972|e9km|AU|lk=off|order=flip|comma=gaps|abbr=unit}}
| eccentricity = {{val|0.04717}}
| period = {{plainlist |
* {{val|84.0205|u=[[julian year (astronomy)|yr]]}}
* {{nowrap|{{val|fmt=commas|30688.5|u=days}}}}<ref name="nasafact" />
* {{nowrap|{{val|fmt=commas|42718}}}} Uranian [[solar day]]s<ref name="CSeligman" />
 }}
| synodic_period = 369.66&nbsp;days<ref name="fact" />
| avg_speed = 6.80&nbsp;km/s<ref name="fact" />
| inclination = {{ubl|{{val|0.773|u=°}} to [[ecliptic]]|6.48° to [[Sun]]'s [[equator]]|0.99° to [[invariable plane]]<ref name=Souami_Souchay_2012 />}}
| asc_node = {{val|74.006|u=°}}
| arg_peri = {{val|96.998857|u=°}}
| mean_anomaly = {{val|142.238600|u=°}}
| satellites = [[Moons of Uranus|28]]
| flattening = {{val|0.0229|0.0008}}{{efn | Calculated using data from Seidelmann, 2007.<ref name="Seidelmann Archinal A'hearn et al. 2007" /> }}
| equatorial_radius = {{nowrap|{{val|fmt=commas|25559|4|u=km}}}}<br />4.007&nbsp;Earths<ref name="Seidelmann Archinal A'hearn et al. 2007" />{{efn|name=atmospheric pressure}}
| polar_radius = {{nowrap|{{val|fmt=commas|24973|20|u=km}}}}<br />3.929&nbsp;Earths<ref name="Seidelmann Archinal A'hearn et al. 2007" />{{efn|name=atmospheric pressure}}
| mean_radius = {{nowrap|{{val|fmt=commas|25362|7|u=km}}}}<ref name="Seidelmann Archinal A'hearn et al. 2007" />{{efn|name=atmospheric pressure}}
| circumference = {{nowrap|{{val|fmt=commas|159354.1|u=km}}}}<ref name="nasafact" />
| surface_area = {{val|8.1156|e=9|u=km2}}<ref name="nasafact" />{{efn|name=atmospheric pressure}} <br /> 15.91&nbsp;Earths
| volume = {{val|6.833|e=13|u=km3}}<ref name="fact" />{{efn|name=atmospheric pressure}} <br /> 63.086&nbsp;Earths
| mass = {{val|8.6810|0.0013|e=25|u=kg}} <br /> 14.536&nbsp;Earths<ref name="Jacobson Campbell et al. 1992" /> <br />
[[standard gravitational parameter|GM]]={{nowrap|{{val|fmt=commas|5793939|13|u=km<sup>3</sup>/s<sup>2</sup>}}}}
| density = {{val|1.27|u=g/cm3}}<ref name="fact" />{{efn|name=atmospheric pressure2}}
| surface_grav = {{cvt|8.69|m/s2|g0|lk=out}}<ref name="fact" />{{efn|name=atmospheric pressure}}
| moment_of_inertia_factor = {{val|0.23|}}<ref name="PS15">{{cite book |last2=Lissauer |first2=Jack J. |last1=de Pater |first1=Imke |author-link1=Imke de Pater |title=Planetary Sciences |date=2015 |url=https://books.google.com/books?id=stFpBgAAQBAJ&pg=PA250 |page=250 |publisher=Cambridge University Press |location=New York |isbn=978-0521853712 |edition=2nd updated |access-date=17 August 2016 |archive-date=26 November 2016 |archive-url=https://web.archive.org/web/20161126120848/https://books.google.com/books?id=stFpBgAAQBAJ&pg=PA250 |url-status=live }}</ref> (estimate)
| escape_velocity = 21.3&nbsp;km/s<ref name="fact" />{{efn|name=atmospheric pressure}}
| rotation = {{val|−0.718649|u=days}}<br/>−{{RA|17|14|51}}<br/>([[retrograde motion|retrograde]])
| sidereal_day = {{val|-0.718661|u=days}}<br /> <span class="nowrap">−{{RA|17|14|52.310}} ± {{RA|||0.036}}<br/>(retrograde)<ref name="Lamy2025"/></span>
| rot_velocity = 2.59&nbsp;km/s
| axial_tilt = 82.23° (to orbit, retrograde).<ref name="fact"/> <!-- please read the section Axial tilt, this is correct -->
 97.77°(prograde, right-hand rule)
| right_asc_north_pole = {{RA|17|9|15}}<br />257.311°<ref name="Seidelmann Archinal A'hearn et al. 2007" /><ref name="iau2015">{{Cite journal |last1=Archinal |first1=B. A. |last2=Acton |first2=C. H. |last3=A'Hearn |first3=M. F. |last4=Conrad |first4=A. |last5=Consolmagno |first5=G. J. |last6=Duxbury |first6=T. |last7=Hestroffer |first7=D. |last8=Hilton |first8=J. L. |last9=Kirk |first9=R. L. |last10=Klioner |first10=S. A. |last11=McCarthy |first11=D. |last12=Meech |first12=K. |last13=Oberst |first13=J. |last14=Ping |first14=J. |last15=Seidelmann |first15=P. K. |date=2018 |title=Report of the IAU Working Group on Cartographic Coordinates and Rotational Elements: 2015 |url=http://link.springer.com/10.1007/s10569-017-9805-5 |journal=Celestial Mechanics and Dynamical Astronomy |language=en |volume=130 |issue=3 |page=22 |doi=10.1007/s10569-017-9805-5 |bibcode=2018CeMDA.130...22A |issn=0923-2958}}</ref>
| declination = −15.175°<ref name="Seidelmann Archinal A'hearn et al. 2007" /><ref name="iau2015" />
| albedo = 0.300 ([[Bond albedo|Bond]])<ref name="Pearl_et_al_Uranus"/><br />0.488 ([[Geometric albedo|geom.]])<ref name="Mallama_et_al"/>
| magnitude = 5.38<ref name="Mallama_and_Hilton" /> to 6.03<ref name="Mallama_and_Hilton" />
| abs_magnitude = −7.2<ref name="IMCCE">{{cite web | title=Encyclopedia - the brightest bodies | website=IMCCE | url=https://promenade.imcce.fr/en/pages5/572.html | access-date=29 May 2023 | archive-date=24 July 2023 | archive-url=https://web.archive.org/web/20230724225002/https://promenade.imcce.fr/en/pages5/572.html | url-status=live }}</ref>
| angular_size = 3.3″ to 4.1″<ref name="fact" />
| temp_name1 = 1&nbsp;[[bar (unit)|bar]] level<ref name="Podolak Weizman et al. 1995" />
| min_temp_1 = 
| mean_temp_1 = {{convert|76|K|C|disp=br()}}
| max_temp_1 = 
| temp_name2 = 0.1&nbsp;bar<br />([[tropopause]])<ref name="Lunine 1993" />
| min_temp_2 = 47&nbsp;K
| mean_temp_2 = 53&nbsp;K
| max_temp_2 = 57&nbsp;K
| pronounced = {{IPAc-en|audio=uranus.ogg|ˈ|jʊər|ə|n|ə|s}}<ref name="BBCOUP" /> or {{IPAc-en|audio=en-us-Uranus.ogg|j|ʊ|ˈ|r|eɪ|n|ə|s}}<ref name="OED" />
| adjectives = Uranian ({{IPAc-en|j|ʊ|ˈ|r|eɪ|n|i|ə|n}})<ref>{{OED|Uranian}}</ref>
| named_after = the Latin form ''Ūranus'' of the Greek god [[Uranus (mythology)|Οὐρανός]] ''Ouranos''
| atmosphere = yes
| atmosphere_ref = <ref name="Lunine 1993" /><ref name="Lindal Lyons et al. 1987" /><ref name="Conrath Gautier et al. 1987" />{{efn | Calculation of He, H<sub>2</sub> and CH<sub>4</sub> molar fractions is based on a 2.3% mixing ratio of methane to hydrogen and the 15/85 He/H<sub>2</sub> proportions measured at the tropopause. }}
| scale_height = 27.7&nbsp;km<ref name="fact" />
| atmosphere_composition = Below {{Cvt|1.3|bar|abbr=unit|sigfig=2}}:
{{indented plainlist|
* 83&nbsp;±&nbsp;3% [[hydrogen]]
* 15&nbsp;±&nbsp;3% [[helium]]
* 2.3% [[methane]]
* 0.009%&nbsp;(0.007–0.015%) [[hydrogen deuteride]]
* [[hydrogen sulfide]] ([[trace element|trace amount]])}}
Icy [[Volatile (astrogeology)|volatiles]]: {{cslist|[[ammonia]]|[[ice|water ice]]|[[ammonium hydrosulfide]]|[[methane hydrate]]}}
}}

'''Uranus''' is the seventh [[planet]] from the [[Sun]]. It is a gaseous [[cyan]]-coloured [[ice giant]]. Most of the planet is made of [[water]], [[ammonia]], and [[methane]] in a [[Supercritical fluid|supercritical phase of matter]], which astronomy calls "ice" or [[Volatile (astrogeology)|volatiles]]. [[Atmosphere of Uranus|The planet's atmosphere]] has a complex layered [[cloud]] structure and has the lowest minimum temperature ({{convert|49|K|C F|0}}) of all the [[Solar System]]'s planets. It has a marked [[axial tilt]] of 82.23° <!-- Please read the section "Axial tilt" and do not change; the next phrase describing the rotation as retrograde is related to the choice of axial tilt convention and follows the convention on the page [[Axial tilt]]. --> with a [[Retrograde and prograde motion|retrograde]] rotation period of 17 hours and 14 minutes. This means that in an 84-Earth-year [[orbital period]] around the Sun, its poles get around 42 years of continuous sunlight, followed by 42 years of continuous darkness.

Uranus has the third-largest diameter and fourth-largest mass among the Solar System's planets. Based on current models, inside its volatile [[Mantle (geology)|mantle]] layer is a rocky core, and surrounding it is a thick [[hydrogen]] and [[helium]] atmosphere. Trace amounts of [[hydrocarbon]]s (thought to be produced via [[hydrolysis]]) and [[carbon monoxide]] along with [[carbon dioxide]] (thought to have originated from [[comet]]s) have been detected in the upper atmosphere. There are many unexplained [[Climate of Uranus|climate phenomena in Uranus's atmosphere]], such as its peak wind speed of {{convert|900|km/h|mph|abbr=on|order=out}},<ref name="Sromovsky & Fry 2005" /> variations in its polar cap, and its erratic cloud formation. The planet also has very low [[internal heat]] compared to other giant planets, the cause of which remains unclear.

Like the other giant planets, Uranus has a [[Rings of Uranus|ring system]], a [[magnetosphere]], and many [[natural satellite]]s. The extremely dark ring system reflects only about 2% of the incoming light. Uranus's 28 natural satellites include 18 known [[regular moon]]s, of which 13 are small [[inner moon]]s. Further out are the larger five [[major moon]]s of the planet: [[Miranda (moon)|Miranda]], [[Ariel (moon)|Ariel]], [[Umbriel]], [[Titania (moon)|Titania]], and [[Oberon (moon)|Oberon]]. Orbiting at a much greater distance from Uranus are the ten known [[irregular moon]]s. The planet's magnetosphere is highly asymmetric and has many [[charged particle]]s, which may be the cause of the darkening of its rings and moons.

Uranus is visible to the naked eye, but it is very dim and was not classified as a planet until 1781, when it was first observed by [[William Herschel]]. About seven decades after its discovery, consensus was reached that the planet be named after the [[Uranus (mythology)|Greek god Uranus]] (Ouranos), one of the [[Greek primordial deities]]. As of 2025, it has been visited only once when in 1986 the ''[[Voyager 2]]'' probe flew by the planet.<ref>{{Cite web |title=Exploration {{!}} Uranus |url=https://solarsystem.nasa.gov/planets/uranus/exploration?page=0&per_page=10&order=launch_date+desc,title+asc&search=&tags=Uranus&category=33 |url-status=live |archive-url=https://web.archive.org/web/20200807125253/https://solarsystem.nasa.gov/planets/uranus/exploration/?page=0&per_page=10&order=launch_date+desc,title+asc&search=&tags=Uranus&category=33 |archive-date=7 August 2020 |access-date=8 February 2020 |website=NASA Solar System Exploration | date=10 November 2017 |quote=Jan. 24, 1986: NASA's Voyager&nbsp;2 made the first - and so far the only - visit to Uranus.}}</ref> Though nowadays it can be [[Optical resolution|resolved]] and observed by telescopes, there is much desire to revisit the planet, as shown by [[Planetary Science Decadal Survey]]'s decision to make the proposed [[Uranus Orbiter and Probe]] mission a top priority in the 2023–2032 survey, and the [[China National Space Administration|CNSA]]'s proposal to fly by the planet with a subprobe of ''[[Tianwen-4]]''.<ref name="TianwenPlSoc">{{cite news |last1=Jones |first1=Andrew |title=China's plans for outer Solar System exploration |url=https://www.planetary.org/articles/chinas-plans-for-outer-solar-system-exploration |access-date=24 January 2024 |work=The Planetary Society |date=21 December 2023 |language=en |archive-date=31 December 2023 |archive-url=https://web.archive.org/web/20231231044006/https://www.planetary.org/articles/chinas-plans-for-outer-solar-system-exploration |url-status=live }}</ref>

== History ==
[[File:Discovery of Uranus1781.png|thumb|Position of Uranus (marked with a cross) on 13 March 1781, the date of its discovery]]
Like the [[classical planet]]s, Uranus is visible to the naked eye, but it was never recognised as a planet by ancient observers because of its dimness and slow orbit.<ref>{{cite web | title=MIRA's Field Trips to the Stars Internet Education Program | work=Monterey Institute for Research in Astronomy | url=https://www.mira.org/fts0/planets/101/text/txt001x.htm | access-date=5 May 2021 | archive-date=1 May 2021 | archive-url=https://web.archive.org/web/20210501025331/http://www.mira.org/fts0/planets/101/text/txt001x.htm | url-status=live }}</ref> [[William Herschel]] first observed Uranus on 13 March 1781, leading to its discovery as a planet, expanding the known boundaries of the [[Solar System]] for the first time in history and making Uranus the first planet classified as such with the aid of a [[telescope]]. The discovery of Uranus also effectively doubled the size of the known Solar System because Uranus is around twice as far from the Sun as the planet [[Saturn]].

=== {{anchor|34 Tauri}}<!-- Used by an incoming redirect --> Discovery ===
[[File:William_Herschel01.jpg|thumb|upright|[[William Herschel]], discoverer of Uranus]]
Before its recognition as a planet, Uranus had been observed many times, but was generally misidentified as a star. The earliest possible known observation was by [[Hipparchus]], who in 128 BC might have recorded it as a star for his [[star catalogue]] that was later incorporated into [[Ptolemy]]'s ''[[Almagest]]''.<ref>{{Cite journal |last=Bourtembourg |first=René |date=November 2013 |title=Was Uranus Observed by Hipparchus? |journal=Journal for the History of Astronomy |language=en |volume=44 |issue=4 |pages=377–387 |bibcode=2013JHA....44..377B |doi=10.1177/002182861304400401 |issn=0021-8286 |s2cid=122482074}}</ref> The earliest definite sighting was in 1690, when [[John Flamsteed]] observed it at least six times, cataloguing it as 34 [[Taurus (constellation)|Tauri]]. The French astronomer [[Pierre Charles Le Monnier]] observed Uranus at least twelve times between 1750 and 1769,<ref>{{cite web | website=Astronomy Briefly | title=Uranus – About Saying, Finding, and Describing It | publisher=thespaceguy.com | url=http://www.thespaceguy.com/Uranus.htm | last=Dunkerson | first=Duane | access-date=5 May 2021 | archive-date=10 August 2011 | archive-url=https://web.archive.org/web/20110810072629/http://www.thespaceguy.com/Uranus.htm | url-status=live }}</ref> including on four consecutive nights.

[[William Herschel]] observed Uranus on 13 March 1781 from the garden of his house at 19 New King Street in [[Bath, Somerset]], England (now the [[Herschel Museum of Astronomy]]),<ref>{{cite web |title=Bath Preservation Trust |url=http://www.bath-preservation-trust.org.uk/ |access-date=29 September 2007 |archive-date=29 September 2018 |archive-url=https://web.archive.org/web/20180929004747/http://www.bath-preservation-trust.org.uk/ |url-status=live }}</ref> and initially reported it (on 26 April 1781) as a [[comet]].<ref>{{Cite journal |last1=Herschel |first1=W. |last2=Watson |first2=Dr. |date=1781 |title= Account of a Comet|journal= Philosophical Transactions of the Royal Society of London|volume=71 |pages=492–501 |bibcode=1781RSPT...71..492H |doi=10.1098/rstl.1781.0056 |s2cid=186208953}}</ref> With a homemade 6.2-inch reflecting telescope, Herschel "engaged in a series of observations on the [[parallax]] of the fixed stars."<ref name="Ref-1">Journal of the Royal Society and Royal Astronomical Society 1, 30, quoted in [[#Miner|Miner]], p. 8.</ref><ref>{{cite journal |title=Ice Giants: The Discovery of Nepture and Uranus |journal=Sky & Telescope |date=29 July 2020 |url=https://skyandtelescope.org/observing/ice-giants-neptune-and-uranus/ |access-date=21 November 2020 |publisher=American Astronomical Society |archive-date=22 November 2020 |archive-url=https://web.archive.org/web/20201122123848/https://skyandtelescope.org/observing/ice-giants-neptune-and-uranus/ |url-status=live }}</ref>

Herschel recorded in his journal: "In the quartile near [[Zeta Tauri|ζ Tauri]]&nbsp;... either [a] Nebulous star or perhaps a comet."<ref>Royal Astronomical Society MSS W.2/1.2, 23; quoted in [[#Miner|Miner]] p. 8.</ref> On 17 March he noted: "I looked for the Comet or Nebulous Star and found that it is a Comet, for it has changed its place."<ref>RAS MSS Herschel W.2/1.2, 24, quoted in [[#Miner|Miner]] p. 8.</ref> When he presented his discovery to the [[Royal Society]], he continued to assert that he had found a comet, but also implicitly compared it to a planet:<ref name="Ref-1"/>

{{blockquote|The power I had on when I first saw the comet was 227. From experience I know that the diameters of the fixed stars are not proportionally magnified with higher powers, as planets are; therefore I now put the powers at 460 and 932, and found that the diameter of the comet increased in proportion to the power, as it ought to be, on the supposition of its not being a fixed star, while the diameters of the stars to which I compared it were not increased in the same ratio. Moreover, the comet being magnified much beyond what its light would admit of, appeared hazy and ill-defined with these great powers, while the stars preserved that lustre and distinctness which from many thousand observations I knew they would retain. The sequel has shown that my surmises were well-founded, this proving to be the Comet we have lately observed.<ref name="Ref-1"/>}}

Herschel notified the Astronomer Royal [[Nevil Maskelyne]] of his discovery and received this flummoxed reply from him on 23 April 1781: "I don't know what to call it. It is as likely to be a regular planet moving in an orbit nearly circular to the sun as a Comet moving in a very eccentric ellipsis. I have not yet seen any coma or tail to it."<ref>RAS MSS Herschel W1/13.M, 14 quoted in [[#Miner|Miner]] p. 8.</ref>

Although Herschel continued to describe his new object as a comet, other astronomers had already begun to suspect otherwise. Finnish-Swedish astronomer [[Anders Johan Lexell]], working in Russia, was the first to compute the orbit of the new object.<ref name="lexell" /> Its nearly circular orbit suggested that it was a planet rather than a comet. Berlin astronomer [[Johann Elert Bode]] described Herschel's discovery as "a moving star that can be deemed a hitherto unknown planet-like object circulating beyond the orbit of Saturn".<ref>Johann Elert Bode, Berliner Astronomisches Jahrbuch, p. 210, 1781, quoted in [[#Miner|Miner]], p. 11.</ref> Bode concluded that its near-circular orbit was more like a planet's than a comet's.<ref>[[#Miner|Miner]], p. 11.</ref>

The object was soon accepted as a new planet. By 1783, Herschel acknowledged this to Royal Society president [[Joseph Banks]]: "By the observation of the most eminent Astronomers in Europe it appears that the new star, which I had the honour of pointing out to them in March 1781, is a Primary Planet of our Solar System."<ref name="Dreyer" /> In recognition of his achievement, [[George III of the United Kingdom|King George III]] gave Herschel an annual [[stipend]] of £200 ({{Inflation|UK|200|1783|fmt=eq|r=-3|cursign=£}}){{Inflation/fn|UK}} on condition that he moved to [[Windsor, Berkshire|Windsor]] so that the Royal Family could look through his telescopes.<ref name="Miner12" />

=== Name ===
The name Uranus references the ancient Greek deity of the sky [[Uranus (mythology)|Uranus]] ({{langx|grc|[[wikt:οὐρανός#Ancient Greek|Οὐρανός]]}}), known as [[Caelus]] in Roman mythology, the father of [[Cronus]] ([[Saturn (mythology)|Saturn]]), grandfather of [[Zeus]] ([[Jupiter (god)|Jupiter]]) and the great-grandfather of [[Ares]] ([[Mars (mythology)|Mars]]), which was rendered as {{lang|la|Uranus}} in Latin ({{IPA|la|ˈuːranʊs|IPA}}).<ref name="OED" /> It is the only one of the eight planets whose English name derives from a figure of [[Greek mythology]]. The pronunciation of the name ''Uranus'' preferred among [[astronomers]] is {{IPAc-en|ˈ|jʊər|ə|n|ə|s}} {{respell|YOOR|ə|nəs}},<ref name="BBCOUP" /> with the [[Long u|long "u"]] of English and stress on the first syllable as in Latin {{lang|la|Uranus}}, in contrast to {{IPAc-en|j|ʊ|ˈ|r|eɪ|n|ə|s}} {{respell|yoo|RAY|nəs}}, with stress on the second syllable and a [[vowel length#Traditional long and short vowels in English orthography|long ''a'']], though both are considered acceptable.{{efn|Because, in the English-speaking world, the latter sounds like "your [[anus]]", the former pronunciation also saves embarrassment: as [[Pamela L. Gay|Pamela Gay]], an astronomer at [[Southern Illinois University Edwardsville]], noted on her podcast, to avoid "being made fun of by any small schoolchildren&nbsp;... when in doubt, don't emphasise anything and just say {{IPA|/ˈjʊərənəs/}}. And then run, quickly."<ref>{{Cite web |last=Cain |first=Frasier |date=12 November 2007 |title=Uranus |url=http://www.astronomycast.com/astronomy/episode-62-uranus/ |url-status=live |archive-url=https://web.archive.org/web/20090426084001/http://www.astronomycast.com/astronomy/episode-62-uranus/ |archive-date=26 April 2009 |access-date=20 April 2009 |website=AstronomyCast}}</ref> }}

Consensus on the name was not reached until almost 70 years after the planet's discovery. During the original discussions following discovery, Maskelyne asked Herschel to "do the astronomical world the {{sic|faver}} to give a name to your planet, which is entirely your own, [and] which we are so much obliged to you for the discovery of".<ref>RAS MSS Herschel W.1/12.M, 20, quoted in [[#Miner|Miner]], p. 12</ref> In response to Maskelyne's request, Herschel decided to name the object {{lang|la|Georgium Sidus}} (George's Star), or the "Georgian Planet" in honour of his new patron, King George III.<ref>{{cite journal |url=http://vesuvius.jsc.nasa.gov/er/seh/hersc.html |title=Voyager at Uranus |date=1986 |journal=NASA JPL |pages=400–268 |volume=7 |issue=85 |url-status=dead |archive-url=https://web.archive.org/web/20060210222142/http://vesuvius.jsc.nasa.gov/er/seh/hersc.html |archive-date=10 February 2006}}</ref> He explained this decision in a letter to Joseph Banks:<ref name="Dreyer" />

{{blockquote|In the fabulous ages of ancient times the appellations of Mercury, Venus, Mars, Jupiter and Saturn were given to the Planets, as being the names of their principal heroes and divinities. In the present more philosophical era it would hardly be allowable to have recourse to the same method and call it Juno, Pallas, Apollo or Minerva, for a name to our new heavenly body. The first consideration of any particular event, or remarkable incident, seems to be its chronology: if in any future age it should be asked, when this last-found Planet was discovered? It would be a very satisfactory answer to say, 'In the reign of King George the Third'.}}

Herschel's proposed name was not popular outside Britain and Hanover, and alternatives were soon proposed. Astronomer [[Jérôme Lalande]] proposed that it be named ''Herschel'' in honour of its discoverer.<ref name="Francisca" /> Swedish astronomer [[Erik Prosperin]] proposed the names ''[[Astraea]],'' ''[[Cybele]]'' (now the names of asteroids), and ''[[Neptune (mythology)|Neptune]]'', which later became the name of the [[Neptune|next planet to be discovered]]. [[Georg Christoph Lichtenberg|Georg Lichtenberg]] from [[Göttingen]] also supported ''Astraea'' (as ''Austräa''), but she is traditionally associated with [[Virgo (astrology)|Virgo]] instead of Taurus. ''Neptune'' was supported by other astronomers who liked the idea of commemorating the victories of the British [[Royal Navy|Royal Naval]] fleet in the course of the [[American Revolutionary War]] by calling the new planet either ''Neptune George III'' or ''Neptune Great Britain'', a compromise Lexell suggested as well.<ref name="lexell" /><ref name=":0">{{Cite journal |last=Gingerich |first=O. |date=1958 |title=The Naming of Uranus and Neptune, Astronomical Society of the Pacific Leaflets, Vol. 8, No. 352, p.9 |url=https://articles.adsabs.harvard.edu//full/1958ASPL....8....9G/0000009.000.html |access-date=1 June 2023 |journal=Leaflet of the Astronomical Society of the Pacific |volume=8 |issue=352 |page=9 |bibcode=1958ASPL....8....9G |archive-date=1 June 2023 |archive-url=https://web.archive.org/web/20230601144624/https://articles.adsabs.harvard.edu//full/1958ASPL....8....9G/0000009.000.html |url-status=live }}</ref> [[Daniel Bernoulli]] suggested ''Hypercronius'' and ''Transaturnis''. ''[[Minerva]]'' was also proposed.<ref name=":0" />
[[File:Johann_elert_bode_painting.jpg|right|thumb|upright|[[Johann Elert Bode]], the astronomer who suggested the name ''Uranus'']]
In a March 1782 treatise, [[Johann Elert Bode]] proposed ''Uranus'', the Latinised version of the [[Greek mythology|Greek god]] of the sky, [[Uranus (mythology)|Ouranos]].<ref name=Bode>{{harvnb|Bode|1784|pp=88–90}}: [In original German]: {{blockquote|{{lang|de|Bereits in der am 12ten März 1782 bei der hiesigen naturforschenden Gesellschaft vorgelesenen Abhandlung, habe ich den Namen des Vaters vom Saturn, nemlich Uranos, oder wie er mit der lateinischen Endung gewöhnlicher ist, Uranus vorgeschlagen, und habe seit dem das Vergnügen gehabt, daß verschiedene Astronomen und Mathematiker in ihren Schriften oder in Briefen an mich, diese Benennung aufgenommen oder gebilligt. Meines Erachtens muß man bei dieser Wahl die Mythologie befolgen, aus welcher die uralten Namen der übrigen Planeten entlehnen worden; denn in der Reihe der bisher bekannten, würde der von einer merkwürdigen Person oder Begebenheit der neuern Zeit wahrgenommene Name eines Planeten sehr auffallen. Diodor von Cicilien erzahlt die Geschichte der Atlanten, eines uralten Volks, welches eine der fruchtbarsten Gegenden in Africa bewohnte, und die Meeresküsten seines Landes als das Vaterland der Götter ansah. Uranus war ihr, erster König, Stifter ihres gesitteter Lebens und Erfinder vieler nützlichen Künste. Zugleich wird er auch als ein fleißiger und geschickter Himmelsforscher des Alterthums beschrieben... Noch mehr: Uranus war der Vater des Saturns und des Atlas, so wie der erstere der Vater des Jupiters.}}}} [Translated]: {{blockquote|Already in the pre-read at the local Natural History Society on 12th March 1782 treatise, I have the father's name from Saturn, namely Uranos, or as it is usually with the Latin suffix, proposed Uranus, and have since had the pleasure that various astronomers and mathematicians, cited in their writings or letters to me approving this designation. In my view, it is necessary to follow the mythology in this election, which had been borrowed from the ancient name of the other planets; because in the series of previously known, perceived by a strange person or event of modern times name of a planet would very noticeable. Diodorus of Cilicia tells the story of Atlas, an ancient people that inhabited one of the most fertile areas in Africa, and looked at the sea shores of his country as the homeland of the gods. Uranus was her first king, founder of their civilized life and inventor of many useful arts. At the same time he is also described as a diligent and skilful astronomers of antiquity ... even more: Uranus was the father of Saturn and the Atlas, as the former is the father of Jupiter.}}</ref> Bode argued that the name should follow the mythology so as not to stand out as different from the other planets, and that Uranus was an appropriate name as the father of the first generation of the [[Titans]].<ref name=Bode/> He also noted the elegance of the name in that just as [[Saturn (mythology)|Saturn]] was the father of [[Jupiter (mythology)|Jupiter]], the new planet should be named after the father of Saturn.<ref name="Miner12" /><ref name=Bode/><ref name="planetsbeyond" /><ref>{{cite web |title=Astronomy in Berlin |publisher=Brian Daugherty |url=http://bdaugherty.tripod.com/astronomy/bode.html |access-date=24 May 2007 |last=Daugherty |first=Brian |archive-url=https://web.archive.org/web/20141008052101/http://bdaugherty.tripod.com/astronomy/bode.html |archive-date=8 October 2014 |url-status=dead }}</ref> However, he was apparently unaware that ''Uranus'' was only the Latinised form of the deity's name, and the Roman equivalent was Caelus. In 1789, Bode's [[Royal Swedish Academy of Sciences|Royal Academy]] colleague [[Martin Klaproth]] named his newly discovered element [[uranium]] in support of Bode's choice.<ref>{{Cite web |last=Finch |first=James |date=2006 |title=The Straight Scoop on Uranium |url=http://www.allchemicals.info/articles/Uranium.php |url-status=dead |archive-url=https://web.archive.org/web/20081221011537/http://www.allchemicals.info/articles/Uranium.php |archive-date=21 December 2008 |access-date=30 March 2009 |publisher=AllChemicals}}</ref> Ultimately, Bode's suggestion became the most widely used, and became universal in 1850 when [[HM Nautical Almanac Office]], the final holdout, switched from using ''Georgium Sidus'' to ''Uranus''.<ref name="planetsbeyond" />

Uranus has two [[astronomical symbol]]s. The first to be proposed, [[File:Uranus symbol (fixed width).svg|16px|⛢]],{{efn|name=symbol later}} was proposed by [[Johann Gottfried Köhler]] at Bode's request in 1782.<ref name=platinum>''Astronomisches Jahrbuch für das Jahr 1785.'' George Jacob Decker, Berlin, p. 191.</ref> Köhler suggested that the new planet be given the symbol for [[platinum]], which had been described scientifically only 30 years before. As there was no [[alchemical symbol]] for platinum, he suggested <span style="{{Transform-rotate|180}}">⛢</span> or <span style="{{Transform-rotate|90}}">⛢</span>, a combination of the planetary-metal symbols ☉ (gold) and ♂ (iron), as platinum (or 'white gold') is found mixed with iron. Bode thought that an upright orientation, ⛢, fit better with the symbols for the other planets while remaining distinct.<ref name=platinum/> This symbol predominates in modern astronomical use in the rare cases that symbols are used at all.<ref>{{Cite journal |last1=Chen |first1=Jingjing |last2=Kipping |first2=David |date=2017 |title=Probabilistic Forecasting of the Masses and Radii of Other Worlds |journal=The Astrophysical Journal |volume=834 |issue=1 |pages=17 |arxiv=1603.08614 |doi=10.3847/1538-4357/834/1/17 |doi-access=free |bibcode=2017ApJ...834...17C |issn=0004-637X }}</ref><ref>[https://solarsystem.nasa.gov/resources/680/solar-system-symbols/ Solar System Symbols] {{Webarchive|url=https://web.archive.org/web/20210318010355/https://solarsystem.nasa.gov/resources/680/solar-system-symbols/ |date=18 March 2021 }}, NASA/JPL</ref> The second symbol, [[File:Uranus monogram (fixed width).svg|16px|♅]],{{efn|name=symbol first}} was suggested by Lalande in 1784. In a letter to Herschel, Lalande described it as "{{lang|fr|un globe surmonté par la première lettre de votre nom}}" ("a globe surmounted by the first letter of your surname").<ref name="Francisca" /> The second symbol is nearly universal in astrology.

In [[English language|English-language]] [[popular culture]], humour is often derived from the common pronunciation of Uranus's name, which resembles that of the phrase "your [[anus]]".<ref>{{cite news |last=Craig |first=Daniel |date=20 June 2017 |title=Very nice job with these Uranus headlines, everyone |url=http://www.phillyvoice.com/very-nice-job-these-uranus-headlines-everyone/ |work=The Philly Voice |location=Philadelphia |access-date=27 August 2017 |archive-date=28 August 2017 |archive-url=https://web.archive.org/web/20170828062818/http://www.phillyvoice.com/very-nice-job-these-uranus-headlines-everyone/ |url-status=live }}</ref>

Uranus is called by a variety of names in other languages. Uranus's name is literally translated as the "[[Heavenly King]] star" in [[Chinese language|Chinese]] ({{Lang-zh|c=天王星|p=Tiānwángxīng|labels=no}}), [[Japanese language|Japanese]] (天王星), [[Korean language|Korean]] (천왕성), and [[Vietnamese language|Vietnamese]] (''sao Thiên Vương'').<ref>{{cite book |first=Jan Jakob Maria |last=De Groot |year=1912 |title=Religion in China: universism. a key to the study of Taoism and Confucianism |series=American lectures on the history of religions |volume=10 |page=300 |publisher=G. P. Putnam's Sons |url=https://books.google.com/books?id=ZAaP7dyjCrAC&pg=PA300 |access-date=8 January 2010 |archive-date=22 July 2011 |archive-url=https://web.archive.org/web/20110722005812/http://books.google.com/books?id=ZAaP7dyjCrAC&pg=PA300 |url-status=live }}</ref><ref>{{cite book |first=Thomas |last=Crump |year=1992 |title=The Japanese numbers game: the use and understanding of numbers in modern Japan |url=https://archive.org/details/japanesenumbersg00crum |url-access=limited |pages=[https://archive.org/details/japanesenumbersg00crum/page/n53 39]–40 |publisher=Routledge |isbn=978-0-415-05609-0}}</ref><ref>{{cite book |first=Homer Bezaleel |last=Hulbert |year=1909 |title=The passing of Korea |page=[https://archive.org/details/passingkorea01hulbgoog/page/n538 426] |publisher=Doubleday, Page & company |url=https://archive.org/details/passingkorea01hulbgoog |access-date=8 January 2010}}</ref><ref>{{cite journal |url=http://amateurastronomy.org/EH/Oct97.txt |title=Asian Astronomy 101 |journal=Hamilton Amateur Astronomers |date=1997 |volume=4 |issue=11 |access-date=5 August 2007 |url-status=dead |archive-url=https://web.archive.org/web/20030514154035/http://amateurastronomy.org/EH/Oct97.txt |archive-date=14 May 2003 }}</ref> In [[Thai language|Thai]], its official name is {{lang|th-Latn|Dao Yurenat}} ({{lang|th|ดาวยูเรนัส}}), as in English. Its other name in Thai is {{lang|th-Latn|Dao Maruettayu}} ({{lang|th|ดาวมฤตยู}}, Star of Mṛtyu), after the [[Sanskrit language|Sanskrit]] word for 'death', {{lang|sa-Latn|[[Mrtyu]]}} ({{lang|sa|मृत्यु}}). In [[Mongolian language|Mongolian]], its name is {{lang|mn-Latn|Tengeriin Van}} ({{lang|mn-Cyrl|Тэнгэрийн ван}}), translated as 'King of the Sky', reflecting its namesake god's role as the ruler of the heavens. In [[Hawaiian language|Hawaiian]], its name is {{lang|haw|Hele{{okina}}ekala}}, the Hawaiian rendering of the name 'Herschel'.<ref>{{cite web |url=http://ulukau.org/elib/cgi-bin/library?e=d-0ped-000Sec--11haw-50-20-frameset-search-uranus-1-011escapewin&a=d&cl=&d=D0.3.3.22&toc=0&p=frameset&p2=search&l=en |title=Hawaiian Dictionary, Mary Kawena Pukui, Samuel H. Elbert |access-date=18 December 2018 |archive-date=30 August 2021 |archive-url=https://web.archive.org/web/20210830233325/http://ulukau.org/elib/cgi-bin/library?e=d-0ped-000Sec--11haw-50-20-frameset-search-uranus-1-011escapewin&a=d&cl=&d=D0.3.3.22&toc=0&p=frameset&p2=search&l=en |url-status=live }}</ref>

== Formation ==
{{main|Formation and evolution of the Solar System}}

{{For|details of the evolution of Uranus's orbit|Nice model}}

It is argued that the differences between the ice giants and the gas giants arise from their formation history.<ref name="Thommes1999" /><ref name="Brunini1999" /><ref name="dangelo2021">{{Cite journal |last1=D'Angelo |first1=Gennaro |last2=Weidenschilling |first2=Stuart J. |last3=Lissauer |first3=Jack J. |last4=Bodenheimer |first4=Peter |date=February 2021 |title=Growth of Jupiter: Formation in disks of gas and solids and evolution to the present epoch |journal=[[Icarus (journal)|Icarus]] |volume=355 |pages=114087 |arxiv=2009.05575 |bibcode=2021Icar..35514087D |doi=10.1016/j.icarus.2020.114087 |s2cid=221654962}}</ref> The Solar System is hypothesised to have formed from a rotating disk of gas and dust known as the [[presolar nebula]]. Much of the nebula's gas, primarily hydrogen and helium, formed the Sun, and the dust grains collected together to form the first protoplanets. As the planets grew, some of them eventually accreted enough matter for their gravity to hold on to the nebula's leftover gas.<ref name="Thommes1999" /><ref name="Brunini1999" /><ref name="dangelo_bodenheimer_2013">{{Cite journal |last1=D'Angelo |first1=Gennaro |last2=Bodenheimer |first2=Peter |date=6 November 2013 |title=Three-dimensional Radiation-hydrodynamics Calculations of the Envelopes of Young Planets Embedded in Protoplanetary Disks |journal=[[The Astrophysical Journal]] |volume=778 |issue=1 |pages=77 |arxiv=1310.2211 |bibcode=2013ApJ...778...77D |doi=10.1088/0004-637X/778/1/77 |issn=0004-637X |s2cid=118522228}}</ref> The more gas they held onto, the larger they became; the larger they became, the more gas they held onto until a critical point was reached, and their size began to increase exponentially.<ref name="dl2018">{{Cite book |last1=D'Angelo |first1=G. |title=Handbook of Exoplanets |last2=Lissauer |first2=J. J. |date=2018 |publisher=[[Springer International Publishing AG]] |isbn=978-3-319-55332-0 |editor-last=Deeg |editor-first=H. |pages=2319–2343 |chapter=Formation of Giant Planets |bibcode=2018haex.bookE.140D |doi=10.1007/978-3-319-55333-7_140 |editor-last2=Belmonte |editor-first2=J. |arxiv=1806.05649 |s2cid=116913980}}</ref> The ice giants, with only a few [[Earth mass]]es of nebular gas, never reached that critical point.<ref name="Thommes1999" /><ref name="Brunini1999" /><ref name="Sheppard Jewitt Kleyna 2006" /> Recent simulations of [[planetary migration]] have suggested that both ice giants formed closer to the Sun than their present positions, and moved outwards after formation (the [[Nice model]]).<ref name="Thommes1999" />

== Orbit and rotation ==
Uranus orbits the Sun once every 84 years. As viewed against the background of stars, since being discovered in 1781,<ref>{{Cite news |last=McKie |first=Robin |date=16 July 2022 |title=Journey to the mystery planet: why Uranus is the new target for space exploration |url=https://www.theguardian.com/science/2022/jul/16/uranus-mission-space-exploration-nasa |url-status=live |archive-url=https://web.archive.org/web/20240106022932/https://www.theguardian.com/science/2022/jul/16/uranus-mission-space-exploration-nasa |archive-date=6 January 2024 |access-date=28 April 2024 |work=The Observer |language=en-GB |issn=0029-7712}}</ref> the planet has returned to the point of its discovery northeast of the binary star [[Zeta Tauri]] twice—in March 1865 and March 1949—and will return to this location again in April 2033.<ref>{{Cite web |last=Fahad |first=Engr |date=26 December 2022 |title=Uranus Size and Uranus Distance from the Sun |url=https://www.electroniclinic.com/uranus-size-and-uranus-distance-from-the-sun/ |url-status=live |archive-url=https://web.archive.org/web/20230301094631/https://www.electroniclinic.com/uranus-size-and-uranus-distance-from-the-sun/ |archive-date=1 March 2023 |access-date=28 April 2024 |website=Electronic Clinic |language=en-US}}</ref>

Its average distance from the Sun is roughly {{convert|20|AU|e9km+e9mi|sigfig=1|abbr=unit|lk=on}}. The difference between its minimum and maximum distance from the Sun is 1.8 AU, larger than that of any other planet, though not as large as that of dwarf planet [[Pluto]].<ref name=AA>Jean Meeus, ''Astronomical Algorithms'' (Richmond, VA: Willmann-Bell, 1998) p 271. From the 1841 aphelion to the 2092 one, perihelia are always 18.28 and aphelia always 20.10 astronomical units</ref> The intensity of sunlight varies inversely with the square of the distance—on Uranus (at about 20 times the distance from the Sun compared to Earth), it is about 1/400 the intensity of light on Earth.<ref>{{cite web | title=Next Stop: Uranus | publisher=Astronomical Society of the Pacific | work=The Universe in the Classroom | url=https://astrosociety.org/file_download/inline/be6d544d-9619-4a20-9614-9f3d097fc32d | date=1986 | access-date=4 May 2021 | archive-date=4 May 2021 | archive-url=https://web.archive.org/web/20210504003407/https://astrosociety.org/file_download/inline/be6d544d-9619-4a20-9614-9f3d097fc32d | url-status=live }}</ref>

The orbital elements of Uranus were first calculated in 1783 by [[Pierre-Simon Laplace]].<ref name="georgeforbes" /> With time, discrepancies began to appear between predicted and observed orbits, and in 1841, [[John Couch Adams]] first proposed that the differences might be due to the gravitational tug of an unseen planet. In 1845, [[Urbain Le Verrier]] began his own independent research into Uranus's orbit. On 23 September 1846, [[Johann Gottfried Galle]] located a new planet, later named [[Neptune]], at nearly the position predicted by Le Verrier.<ref>{{cite web | title=Mathematical discovery of planets | last1=O'Connor | first1=J J. | last2=Robertson | first2=E. F. | website=MacTutor | name-list-style=amp | url=http://www-groups.dcs.st-and.ac.uk/~history/HistTopics/Neptune_and_Pluto.html | date=September 1996 | access-date=13 June 2007 | archive-date=20 August 2011 | archive-url=https://web.archive.org/web/20110820080638/http://www-groups.dcs.st-and.ac.uk/~history/HistTopics/Neptune_and_Pluto.html | url-status=live }}</ref>

The rotational period of the interior of Uranus is 17&nbsp;hours, 14&nbsp;minutes, and 52&nbsp;seconds<ref name="Lamy2025">{{cite journal |last1=Lamy |first1=L. |last2=Prangé |first2=R. |last3=Berthier |first3=J. |last4=Tao |first4=C. |last5=Kim |first5=T. |last6=Roth |first6=L. |last7=Barthélémy |first7=M. |last8=Chaufray |first8=J.-Y. |last9=Rymer |first9=A. |last10=Dunn |first10=W. R. |last11=Wibisono |first11=A. D. |last12=Melin |first12=H. |title=A new rotation period and longitude system for Uranus |journal=Nature Astronomy |date=7 April 2025 |pages=1–8 |doi=10.1038/s41550-025-02492-z |url=https://www.nature.com/articles/s41550-025-02492-z |language=en |issn=2397-3366}}</ref> which was determined by tracking the rotational motion of Uranus's aurorae.<ref>{{cite news |url=https://science.nasa.gov/missions/hubble/hubble-helps-determine-uranus-rotation-rate-with-unprecedented-precision/?utm_source=FBPAGE&utm_medium=NASA%27s+Hubble+Space+Telescope&utm_campaign=NASASocial&linkId=794640986&fbclid=IwY2xjawJjwbFleHRuA2FlbQIxMAABHtFT6KdfU0L0HFsadSMK22xZx4PCRt3vCs3qB5C9mUNKQOYUIWP_EjYeweQy_aem_qbiW_Oe3wOw9UvtY1f0FiA |title=Hubble Helps Determine Uranus' Rotation Rate with Unprecedented Precision |publisher=NASA Hubble Space Telescope imaging team|date=9 April 2025 |access-date=9 April 2025}}</ref> As on all [[giant planet]]s, its upper atmosphere experiences strong winds in the direction of rotation. At some latitudes, such as about 60 degrees south, visible features of the atmosphere move much faster, making a full rotation in as little as 14 hours.<ref>{{Cite web |last1=Gierasch |first1=Peter J. |last2=Nicholson |first2=Philip D. |name-list-style=amp |date=2004 |title=Uranus |url=http://www.warrentboe.org/_files/TeacherPages/792/Uranus_Article.pdf |url-status=live |archive-url=https://web.archive.org/web/20150402112123/http://www.warrentboe.org/_files/TeacherPages/792/Uranus_Article.pdf |archive-date=2 April 2015 |access-date=8 March 2015 |website=World Book}}</ref>

=== Axial tilt ===
[[File:Uranus orientation 1985-2030.gif|thumb|Simulated Earth view of Uranus from 1986 to 2030, from southern summer solstice in 1986 to equinox in 2007 and northern summer solstice in 2028.]]
The Uranian axis of rotation is approximately parallel to the plane of the Solar System, with an [[axial tilt]] of 82.23°.<!-- To match the description on the page [[Axial tilt]], 82.23° and not 97.77° is used throughout this page. See the following explanation. --> Depending on which pole is considered north, the tilt can be described either as 82.23° or as 97.77°. The former follows the [[International Astronomical Union]] [[axial tilt|definition]] that the north pole is the pole which lies on Earth's North's side of the [[invariable plane]] of the [[Solar System]]. Uranus has [[Retrograde and prograde motion|retrograde]] rotation when defined this way. Alternatively, the convention in which a body's north and south poles are defined according to the [[right-hand rule]] in relation to the direction of rotation, Uranus's axial tilt may be given instead as 97.77°, which reverses which pole is considered north and which is considered south and giving the planet prograde rotation.<ref>{{cite web |url=http://roger.ecn.purdue.edu/~masl/documents/masl/coords.html |title=Coordinate Frames Used in MASL |date=2003 |access-date=13 June 2007 |archive-url=https://web.archive.org/web/20041204061125/http://roger.ecn.purdue.edu/~masl/documents/masl/coords.html <!--Added by H3llBot--> |archive-date=4 December 2004}}</ref> This gives it seasonal changes completely unlike those of the other planets. Pluto and asteroid [[2 Pallas]] also have extreme axial tilts. Near the [[solstice]], one pole faces the Sun continuously and the other faces away, with only a narrow strip around the equator experiencing a rapid day–night cycle, with the Sun low over the horizon. On the other side of Uranus's orbit, the orientation of the poles towards the Sun is reversed. Each pole gets around 42&nbsp;years of continuous sunlight, followed by 42&nbsp;years of darkness.<ref>{{Cite web |last=Sromovsky |first=Lawrence |date=2006 |title=Hubble captures rare, fleeting shadow on Uranus |url=http://www.news.wisc.edu/releases/12826.html |url-status=dead |archive-url=https://web.archive.org/web/20110720221646/http://www.news.wisc.edu/releases/12826.html |archive-date=20 July 2011 |access-date=9 June 2007 |website=University of Wisconsin Madison}}</ref> Near the time of the [[equinox]]es, the Sun faces the equator of Uranus, giving a period of day–night cycles similar to those seen on most of the other planets.

One result of this axis orientation is that, averaged over the Uranian year, the near-polar regions of Uranus receive a greater energy input from the Sun than its equatorial regions. Nevertheless, Uranus is hotter at its equator than at its poles. The underlying mechanism that causes this is unknown. The cause of Uranus's unusual axial tilt is also not known with certainty, but the usual speculation is that during the formation of the Solar System, an Earth-sized [[protoplanet]] collided with Uranus, causing the skewed orientation.<ref>{{Cite book |title=Uranus |date=1991 |publisher=[[University of Arizona Press]] |isbn=978-0-8165-1208-9 |editor-last=Bergstralh |editor-first=Jay T. |location=Tucson |pages=485–486 |editor-last2=Miner |editor-first2=Ellis D. |editor-last3=Matthews |editor-first3=Mildred Shapley}}</ref> Research by Jacob Kegerreis of [[Durham University]] suggests that the tilt resulted from a rock larger than Earth crashing into the planet 3 to 4&nbsp;billion years ago.<ref>{{cite news |url=https://www.apnews.com/d1e2c440af57450ab82b62d035adac61 |title=Science Says: A big space crash likely made Uranus lopsided |work=[[Associated Press]] |last=Borenstein |first=Seth |date=21 December 2018 |access-date=17 January 2019 |archive-date=19 January 2019 |archive-url=https://web.archive.org/web/20190119121444/https://www.apnews.com/d1e2c440af57450ab82b62d035adac61 |url-status=live }}</ref> Uranus's south pole was pointed almost directly at the Sun at the time of ''Voyager&nbsp;2''{{'s}} flyby in 1986.<ref>{{cite journal |url=http://www.hnsky.org/iau-iag.htm |title=Report of the IAU/IAG working group on cartographic coordinates and rotational elements of the planets and satellites: 2000 |volume=82 |issue=1 |pages=83 |journal=Celestial Mechanics and Dynamical Astronomy |date=2000 |access-date=13 June 2007 |bibcode=2002CeMDA..82...83S |last1=Seidelmann |first1=P. K. |last2=Abalakin |first2=V. K. |last3=Bursa |first3=M. |last4=Davies |first4=M. E. |last5=De Bergh |first5=C. |last6=Lieske |first6=J. H. |last7=Oberst |first7=J. |last8=Simon |first8=J. L. |last9=Standish |first9=E. M. |last10=Stooke |first10=P. |last11=Thomas |first11=P. C. |doi=10.1023/A:1013939327465 |s2cid=189823009 |archive-date=12 May 2020 |archive-url=https://web.archive.org/web/20200512151452/http://www.hnsky.org/iau-iag.htm |url-status=dead |url-access=subscription }}</ref><ref>{{cite web |url=http://pds.jpl.nasa.gov/documents/sr/stdref_021015/Chapter02.pdf |title=Cartographic Standards |work=NASA |access-date=13 June 2007 |url-status=dead |archive-url=https://web.archive.org/web/20040407151631/http://pds.jpl.nasa.gov/documents/sr/stdref_021015/Chapter02.pdf |archive-date=7 April 2004 }}</ref>

{| class="wikitable" style="text-align: center; margin-left: 20px;"
|+List of solstices and equinoxes<ref>{{cite conference |last=Hammel |first=Heidi B. |date=5 September 2006 |title=Uranus nears Equinox |url=http://www.apl.ucl.ac.uk/iopw/uworkshop_060905.pdf |archive-url=https://web.archive.org/web/20090225084057/http://www.apl.ucl.ac.uk/iopw/uworkshop_060905.pdf |archive-date=25 February 2009 |book-title=A report from the 2006 Pasadena Workshop}}</ref>
|-
! Northern hemisphere
! Year
! Southern hemisphere
|-
| Winter solstice
| 1902, 1986, 2069
| Summer solstice
|-
| Vernal equinox
| 1923, 2007, 2092
| Autumnal equinox
|-
| Summer solstice
| 1944, 2028
| Winter solstice
|-
| Autumnal equinox
| 1965, 2050
| Vernal equinox
|}

=== Visibility from Earth ===
[[File:UranusAndMoon 20221108 fromJP (crop).jpg|thumb|Uranus seen through an amateur telescope, shortly after lunar [[occultation]], during the [[November 2022 lunar eclipse]]]]
The mean [[apparent magnitude]] of Uranus is 5.68 with a standard deviation of 0.17, while the extremes are 5.38 and 6.03.<ref name="Mallama_and_Hilton" /> This range of brightness is near the limit of [[naked eye]] visibility. Much of the variability is dependent upon the planetary latitudes being illuminated from the Sun and viewed from the Earth.<ref name="Schmude_et_al" /> Its [[angular diameter]] is between 3.4 and 3.7&nbsp;arcseconds, compared with 16 to 20&nbsp;arcseconds for Saturn and 32 to 45&nbsp;arcseconds for Jupiter.<ref name="ephemeris" /> At [[Opposition (astronomy)|opposition]], Uranus is visible to the naked eye in dark skies, and becomes an easy target even in urban conditions with binoculars.<ref name="fact" /> On larger amateur telescopes with an objective diameter of between 15 and 23&nbsp;cm, Uranus appears as a pale cyan disk with distinct [[limb darkening]]. With a large telescope of 25&nbsp;cm or wider, cloud patterns, as well as some of the larger satellites, such as [[Titania (moon)|Titania]] and [[Oberon (moon)|Oberon]], may be visible.<ref>{{Cite web |last=Nowak |first=Gary T. |date=2006 |title=Uranus: the Threshold Planet of 2006 |url=http://www.vtastro.org/Articles/uranus2006.html |archive-url=https://web.archive.org/web/20110727233304/http://www.vtastro.org/Articles/uranus2006.html |archive-date=27 July 2011 |access-date=14 June 2007 |website=Vtastro.org}}</ref>

== Internal structure ==
[[File:Uranus, Earth size comparison 2.jpg|thumb|Size comparison of Earth and Uranus]]
Uranus's mass is roughly 14.5 times that of Earth, making it the least massive of the giant planets. Its diameter is slightly larger than Neptune's at roughly four times that of Earth. A resulting density of 1.27&nbsp;g/cm<sup>3</sup> makes Uranus the second least dense planet, after Saturn.<ref name="Seidelmann Archinal A'hearn et al. 2007" /><ref name="Jacobson Campbell et al. 1992" /> This value indicates that it is made primarily of various ices, such as water, ammonia, and methane.<ref name="Podolak Weizman et al. 1995" /> The total mass of ice in Uranus's interior is not precisely known, because different figures emerge depending on the model chosen; it must be between 9.3&nbsp;and 13.5&nbsp;Earth masses.<ref name="Podolak Weizman et al. 1995" /><ref name="Podolak Podolak et al. 2000" /> [[Hydrogen]] and [[helium]] constitute only a small part of the total, with between 0.5 and 1.5&nbsp;Earth masses.<ref name="Podolak Weizman et al. 1995" /> The remainder of the non-ice mass (0.5 to 3.7&nbsp;Earth masses) is accounted for by [[rock (geology)|rocky material]].<ref name="Podolak Weizman et al. 1995" />

The standard model of Uranus's structure is that it consists of three layers: a rocky ([[silicate]]/[[iron–nickel alloy|iron–nickel]]) [[core (geology)|core]] in the centre, an icy [[mantle (geology)|mantle]] in the middle, and an outer gaseous hydrogen/helium envelope.<ref name="Podolak Weizman et al. 1995" /><ref name="Faure2007" /> The core is relatively small, with a mass of only 0.55&nbsp;Earth masses and a radius less than 20% of the planet; the mantle comprises its bulk, with around 13.4&nbsp;Earth masses, and the upper atmosphere is relatively insubstantial, weighing about 0.5&nbsp;Earth masses and extending for the last 20% of Uranus's radius.<ref name="Podolak Weizman et al. 1995" /><ref name="Faure2007" /> Uranus's core [[density]] is around 9&nbsp;g/cm<sup>3</sup>, with a [[pressure]] in the centre of 8&nbsp;million&nbsp;[[bar (unit)|bars]] (800 [[gigapascal|GPa]]) and a temperature of about 5000&nbsp;[[kelvin|K]].<ref name="Podolak Podolak et al. 2000" /><ref name="Faure2007" /> The ice mantle is not in fact composed of ice in the conventional sense, but of a hot and dense fluid consisting of water, ammonia and other [[Volatile (astrogeology)|volatiles]].<ref name="Podolak Weizman et al. 1995" /><ref name="Faure2007" /> This fluid, which has a high electrical conductivity, is sometimes called a water–ammonia ocean.<ref name="Atreya2006" />

[[File:Uranus diagram.svg|thumb|Diagram of the interior of Uranus, listing each layer's composition|center|450x450px]]

The extreme pressure and temperature deep within Uranus may break up the methane molecules, with the carbon atoms condensing into crystals of [[diamond]] that rain down through the mantle like hailstones.<ref>{{cite web |url=http://www.spacedaily.com/news/carbon-99d.html |title=Is It Raining Diamonds on Uranus |website=Space Daily |date=1 October 1999 |access-date=17 May 2013 |archive-date=22 May 2013 |archive-url=https://web.archive.org/web/20130522005929/http://www.spacedaily.com/news/carbon-99d.html |url-status=live }}</ref><ref>{{Cite journal |title=Formation of diamonds in laser-compressed hydrocarbons at planetary interior conditions |journal=Nature Astronomy |last1=Kraus |first1=D. |last2=Vorberger |first2=J. |last3=Pak |first3=A. |last4=Hartley |first4=N. J. |last5=Fletcher |first5=L. B. |last6=Frydrych |first6=S. |last7=Galtier |first7=E. |last8=Gamboa |first8=E. J. |last9=Gericke |first9=D. O. |last10=Glenzer |first10=S. H. |last11=Granados |first11=E. |last12=MacDonald |first12=M. J. |last13=MacKinnon |first13=A. J. |last14=McBride |first14=E. E. |last15=Nam |first15=I. |last16=Neumayer |first16=P. |last17=Roth |first17=M. |last18=Saunders |first18=A. M. |last19=Schuster |first19=A. K. |last20=Sun |first20=P. |last21=van Driel |first21=T. |last22=Döppner |first22=T. |last23=Falcone |first23=R. W. |display-authors=1 |volume=1 |issue=9 |pages=606–611 |date=September 2017 |doi=10.1038/s41550-017-0219-9 |bibcode=2017NatAs...1..606K |s2cid=46945778 |url=https://cloudfront.escholarship.org/dist/prd/content/qt1k79p6pk/qt1k79p6pk.pdf?t=p5nsjk |access-date=23 October 2018 |archive-date=25 July 2018 |archive-url=https://web.archive.org/web/20180725002534/https://cloudfront.escholarship.org/dist/prd/content/qt1k79p6pk/qt1k79p6pk.pdf?t=p5nsjk |url-status=live }}</ref> This phenomenon is similar to diamond rains that are theorised by scientists to exist on [[Jupiter]], [[Saturn]], and [[Neptune]].<ref>{{cite web|url=https://www.businessinsider.com/diamond-rain-saturn-jupiter-2016-4|title=Lightning storms make it rain diamonds on Saturn and Jupiter|last1=Kane|first1=Sean|website=Business Insider|date=29 April 2016|access-date=22 May 2019|archive-date=26 June 2019|archive-url=https://web.archive.org/web/20190626211704/https://www.businessinsider.com/diamond-rain-saturn-jupiter-2016-4|url-status=live}}</ref><ref>{{cite news|url=https://www.washingtonpost.com/news/speaking-of-science/wp/2017/08/25/it-rains-solid-diamonds-on-uranus-and-neptune/|title=It rains solid diamonds on Uranus and Neptune|last1=Kaplan|first1=Sarah|newspaper=The Washington Post|date=25 March 2017|access-date=22 May 2019|archive-date=27 August 2017|archive-url=https://web.archive.org/web/20170827011901/https://www.washingtonpost.com/news/speaking-of-science/wp/2017/08/25/it-rains-solid-diamonds-on-uranus-and-neptune/|url-status=live}}</ref> Very-high-pressure experiments at the [[Lawrence Livermore National Laboratory]] suggest that an ocean of metallic liquid carbon, perhaps with floating solid 'diamond-bergs', may comprise the base of the mantle.<ref name="Eggert">{{Cite journal |last1=Eggert |first1=J. H. |last2=Hicks |first2=D. G. |last3=Celliers |first3=P. M. |last4=Bradley |first4=D. K. |last5=McWilliams |first5=R. S. |last6=Jeanloz |first6=R. |last7=Miller |first7=J. E. |last8=Boehly |first8=T. R. |last9=Collins |first9=G. W. |display-authors=etal |date=January 2010 |title=Melting temperature of diamond at ultrahigh pressure |journal=[[Nature Physics]] |language=en |volume=6 |issue=1 |pages=40–43 |bibcode=2010NatPh...6...40E |doi=10.1038/nphys1438 |issn=1745-2473 |doi-access=free}}</ref><ref name="Bland, Eric">{{cite news |last1=Bland |first1=Eric |title=Outer planets may have oceans of diamond |url=http://www.abc.net.au/science/articles/2010/01/18/2794635.htm |access-date=9 October 2017 |work=ABC Science |date=18 January 2010 |language=en-AU |archive-date=15 June 2020 |archive-url=https://web.archive.org/web/20200615182200/http://www.abc.net.au/science/articles/2010/01/18/2794635.htm |url-status=live }}</ref><ref>{{cite journal |url=http://www.astronomynow.com/news/n1001/21diamond/ |title=Oceans of diamond possible on Uranus and Neptune |last1=Baldwin |first1=Emily |journal=Astronomy Now |date=21 January 2010 |access-date=6 February 2014 |url-status=dead |archive-url=https://web.archive.org/web/20131203065217/http://www.astronomynow.com/news/n1001/21diamond/ |archive-date=3 December 2013 }}</ref>

The bulk compositions of Uranus and Neptune are different from those of Jupiter and [[Saturn]], with ice dominating over gases, hence justifying their separate classification as [[ice giant]]s. There may be a layer of ionic water where the water molecules break down into a soup of hydrogen and oxygen ions, and deeper down [[superionic water]] in which the oxygen crystallises but the hydrogen ions move freely within the oxygen lattice.<ref>{{cite news |url=https://www.newscientist.com/article/mg20727764.500-weird-water-lurking-inside-giant-planets/ |title=Weird water lurking inside giant planets |work=New Scientist |first=David |last=Shiga |issue=2776 |date=1 September 2010 |access-date=11 February 2018 |archive-date=12 February 2018 |archive-url=https://web.archive.org/web/20180212143537/https://www.newscientist.com/article/mg20727764.500-weird-water-lurking-inside-giant-planets/ |url-status=live }}</ref>

Although the model considered above is reasonably standard, it is not unique; other models also satisfy observations. For instance, if substantial amounts of hydrogen and rocky material are mixed in the ice mantle, the total mass of ices in the interior will be lower, and, correspondingly, the total mass of rocks and hydrogen will be higher. Presently available data does not allow a scientific determination of which model is correct.<ref name="Podolak Podolak et al. 2000" /> The fluid interior structure of Uranus means that it has no solid surface. The gaseous atmosphere gradually transitions into the internal liquid layers.<ref name="Podolak Weizman et al. 1995" /> For the sake of convenience, a revolving [[oblate spheroid]] set at the point at which atmospheric pressure equals 1&nbsp;bar (100&nbsp;kPa) is conditionally designated as a "surface". It has equatorial and [[Geographical pole|polar]] radii of {{convert|25559|±|4|km|mi|abbr=on}} and {{convert|24973|±|20|km|mi|abbr=on}}, respectively.<ref name="Seidelmann Archinal A'hearn et al. 2007" /> This surface is used throughout this article as a zero point for altitudes.

=== Internal heat ===
Uranus's [[internal heat]] appears markedly lower than that of the other giant planets; in astronomical terms, it has a low [[thermal flux]].<ref name="Sromovsky & Fry 2005" /><ref name="Hanel Conrath et al. 1986" /> Why Uranus's internal temperature is so low is still not understood. Neptune, which is Uranus's near twin in size and composition, radiates 2.61 times as much energy into space as it receives from the Sun,<ref name="Sromovsky & Fry 2005" /> but Uranus radiates hardly any excess heat at all. The total power radiated by Uranus in the [[far infrared]] (i.e. heat) part of the spectrum is {{val|1.06|0.08}} times the solar energy absorbed in its [[atmosphere]].<ref name="Lunine 1993" /><ref name="Pearl Conrath et al. 1990" /> Uranus's heat flux is only {{val|0.042|0.047|ul=W/m2}}, which is lower than the internal heat flux of Earth of about {{val|0.075|ul=W/m2}}.<ref name="Pearl Conrath et al. 1990" /> The lowest temperature recorded in Uranus's [[tropopause]] is {{convert|49|K|C F}}, making Uranus the coldest planet in the Solar System.<ref name="Lunine 1993" /><ref name="Pearl Conrath et al. 1990" />

One of the hypotheses for this discrepancy suggests the Earth-sized impactor theorised to be behind Uranus's axial tilt left the planet with a depleted core temperature, as the impact caused Uranus to expel most of its primordial heat.<ref>{{Cite magazine |last=Hawksett |first=David |date=2005 |title=Ten Mysteries of the Solar System: Why is Uranus So Cold? |magazine=[[Astronomy Now]] |page=73}}</ref> Another hypothesis is that some form of barrier exists in Uranus's upper layers that prevents the core's heat from reaching the surface.<ref name="Podolak Weizman et al. 1995" /> For example, [[convection]] may take place in a set of compositionally different layers, which may inhibit upward [[Heat conduction|heat transport]];<ref name="Lunine 1993" /><ref name="Pearl Conrath et al. 1990" /> perhaps [[double diffusive convection]] is a limiting factor.<ref name="Podolak Weizman et al. 1995" />

In a 2021 study, the ice giants' interior conditions were mimicked by compressing water that contained minerals such as [[olivine]] and [[ferropericlase]], thus showing that large amounts of [[magnesium]] could be dissolved in the liquid interiors of Uranus and Neptune. If Uranus has more of this magnesium than Neptune, it could form a [[thermal insulation]] layer, thus potentially explaining the planet's low temperature.<ref>{{cite journal|last1=Taehyun|first1=Kim|display-authors=et al|title=Atomic-scale mixing between MgO and H2O in the deep interiors of water-rich planets|url=https://www.researchsquare.com/article/rs-78494/v1.pdf?c=1631891793000|journal=[[Nature Astronomy]]|year=2021|volume=5|issue=8|pages=815–821|doi=10.1038/s41550-021-01368-2|bibcode=2021NatAs...5..815K|s2cid=238984160|access-date=20 May 2021|archive-date=26 February 2024|archive-url=https://web.archive.org/web/20240226144821/https://assets.researchsquare.com/files/rs-78494/v1/59e27b87-a2e1-4af2-8d68-877406ccb609.pdf?c=1637596106|url-status=live}}</ref>

== Atmosphere ==
{{main|Atmosphere of Uranus}}
Although there is no well-defined solid surface within Uranus's interior, the outermost part of Uranus's gaseous envelope that is accessible to remote sensing is called its [[atmosphere]].<ref name="Lunine 1993" /> Remote-sensing capability extends down to roughly 300&nbsp;km below the {{convert|1|bar|kPa|abbr=on}} level, with a corresponding pressure around {{convert|100|bar|MPa|abbr=on}} and temperature of {{convert|320|K|C F}}.<ref name="de Pater Romani et al. 1991" /> The tenuous [[thermosphere]] extends over two planetary radii from the nominal surface, which is defined to lie at a pressure of 1 bar.<ref name="Herbert Sandel et al. 1987" /> The Uranian atmosphere can be divided into three layers: the [[troposphere]], between altitudes of {{convert|-300|and|50|km|mi|abbr=on}} and pressures from 100 to 0.1&nbsp;bar (10&nbsp;MPa to 10&nbsp;kPa); the [[stratosphere]], spanning altitudes between {{convert|50|and|4000|km|mi|abbr=on}} and pressures of between {{nowrap|0.1 and 10<sup>−10</sup>&nbsp;bar}} (10&nbsp;kPa to 10&nbsp;[[micropascal|μPa]]); and the thermosphere extending from 4,000&nbsp;km to as high as 50,000&nbsp;km from the surface.<ref name="Lunine 1993" /> There is no [[mesosphere]].

=== Composition ===
[[File:Tropospheric profile Uranus new.svg|thumb|400x400px|Diagram of the Uranus atmosphere's composition and layers, along with the graph of its pressure]]
The composition of Uranus's atmosphere is different from its bulk, consisting mainly of [[molecular hydrogen]] and helium.<ref name="Lunine 1993" /> The helium [[Gas composition|molar fraction]], i.e. the number of helium [[atom]]s per molecule of gas, is {{val|0.15|0.03}}<ref name="Conrath Gautier et al. 1987" /> in the upper troposphere, which corresponds to a mass fraction {{val|0.26|0.05}}.<ref name="Lunine 1993" /><ref name="Pearl Conrath et al. 1990" /> This value is close to the protosolar helium mass fraction of {{val|0.275|0.01}},<ref name="Lodders 2003" /> indicating that helium has not settled in its centre as it has in the gas giants.<ref name="Lunine 1993" /> The third-most-abundant component of Uranus's atmosphere is methane ({{chem2|CH4}}).<ref name="Lunine 1993" /> Methane has prominent [[absorption band]]s in the [[visible spectrum|visible]] and [[near-infrared]] (IR), making Uranus [[aquamarine (color)|aquamarine]] or [[cyan]] in colour.<ref name="Lunine 1993" /> Methane molecules account for 2.3% of the atmosphere by molar fraction below the methane cloud deck at the pressure level of {{convert|1.3|bar|kPa|abbr=on}}; this represents about 20 to 30&nbsp;times the carbon abundance found in the Sun.<ref name="Lunine 1993" /><ref name="Lindal Lyons et al. 1987" /><ref name="Tyler 1986" />

The mixing ratio{{efn | Mixing ratio is defined as the number of molecules of a compound per a molecule of hydrogen. }} is much lower in the upper atmosphere due to its extremely low temperature, which lowers the saturation level and causes excess methane to freeze out.<ref name="Bishop Atreya et al. 1990" /> The abundances of less volatile compounds such as ammonia, water, and [[hydrogen sulfide]] in the deep atmosphere are poorly known. They are probably also higher than solar values.<ref name="Lunine 1993" /><ref name="de Pater Romani et al. 1989" /> Along with methane, trace amounts of various [[hydrocarbon]]s are found in the stratosphere of Uranus, which are thought to be produced from methane by [[photolysis]] induced by the solar [[ultraviolet]] (UV) radiation.<ref name="Summers & Strobel 1989" /> They include [[ethane]] ({{chem2|C2H6}}), [[acetylene]] ({{chem2|C2H2}}), [[methylacetylene]] ({{chem2|CH3C2H}}), and [[diacetylene]] ({{chem2|C2HC2H}}).<ref name="Bishop Atreya et al. 1990" /><ref name="Burgdorf Orton et al. 2006" /><ref name="Encrenaz 2003" /> Spectroscopy has also uncovered traces of water vapour, [[carbon monoxide]], and [[carbon dioxide]] in the upper atmosphere, which can only originate from an external source such as infalling dust and [[comet]]s.<ref name="Burgdorf Orton et al. 2006" /><ref name="Encrenaz 2003" /><ref name="Encrenaz Lellouch et al. 2004" />

=== Troposphere ===
The troposphere is the lowest and densest part of the atmosphere and is characterised by a decrease in temperature with altitude.<ref name="Lunine 1993" /> The temperature falls from about {{convert|320|K|C F|0}} at the base of the nominal troposphere at −300&nbsp;km to {{convert|53|K|C F|0}} at 50&nbsp;km.<ref name="de Pater Romani et al. 1991" /><ref name="Tyler 1986" /> The temperatures in the coldest upper region of the troposphere (the [[tropopause]]) actually vary in the range between {{convert|49|and|57|K|C F|0}} depending on planetary latitude.<ref name="Lunine 1993" /><ref name="Hanel Conrath et al. 1986" /> The tropopause region is responsible for the vast majority of Uranus's thermal [[far infrared]] emissions, thus determining its [[effective temperature]] of {{convert|59.1|±|0.3|K|C F|1}}.<ref name="Hanel Conrath et al. 1986" /><ref name="Pearl Conrath et al. 1990" />

The troposphere is thought to have a highly complex cloud structure; water clouds are hypothesised to lie in the pressure range of {{convert|50|to|100|bar|MPa|sigfig=1|abbr=on}}, [[ammonium hydrosulfide]] clouds in the range of {{convert|20|to|40|bar|MPa|sigfig=1|abbr=on}}, ammonia or [[hydrogen sulfide]] clouds at between {{convert|3|and|10|bar|MPa|sigfig=1|abbr=on}} and finally directly detected thin methane clouds at {{convert|1|to|2|bar|MPa|sigfig=1|abbr=on}}.<ref name="Lunine 1993" /><ref name="Lindal Lyons et al. 1987" /><ref name="de Pater Romani et al. 1991" /><ref name="Atreya Wong 2005" /> The troposphere is a dynamic part of the atmosphere, exhibiting strong winds, bright clouds, and seasonal changes.<ref name="Sromovsky & Fry 2005" />

=== Upper atmosphere ===
[[File:Adding to Uranus's legacy.tif|thumb|Uranus's upper atmosphere imaged by HST during the Outer Planet Atmosphere Legacy (OPAL) observing program.<ref>{{cite web |title=Adding to Uranus's legacy |url=https://www.spacetelescope.org/images/potw1906a/ |url-status=live |archive-url=https://web.archive.org/web/20190212011708/https://www.spacetelescope.org/images/potw1906a/ |archive-date=12 February 2019 |access-date=11 February 2019 |website=www.spacetelescope.org |language=en}}</ref>]]
The middle layer of the Uranian atmosphere is the [[stratosphere]], where temperature generally increases with altitude from {{convert|53|K|C F|0}} in the [[tropopause]] to between {{convert|800|and|850|K|C F|0}} at the base of the thermosphere.<ref name="Herbert Sandel et al. 1987" /> The heating of the stratosphere is caused by absorption of solar UV and IR radiation by methane and other [[hydrocarbon]]s,<ref name="Young et al. 2001" /> which form in this part of the atmosphere as a result of methane [[photolysis]].<ref name="Summers & Strobel 1989" /> Heat is also conducted from the hot thermosphere.<ref name="Young et al. 2001" /> The hydrocarbons occupy a relatively narrow layer at altitudes of between 100 and 300&nbsp;km corresponding to a pressure range of 1,000 to 10&nbsp;Pa and temperatures of between {{convert|75|and|170|K|C F|0}}.<ref name="Bishop Atreya et al. 1990" /><ref name="Burgdorf Orton et al. 2006" />

The most abundant hydrocarbons are methane, [[acetylene]], and [[ethane]] with [[mixing ratio]]s of around {{10^|-7}} relative to hydrogen. The mixing ratio of [[carbon monoxide]] is similar at these altitudes.<ref name="Bishop Atreya et al. 1990" /><ref name="Burgdorf Orton et al. 2006" /><ref name="Encrenaz Lellouch et al. 2004" /> Heavier hydrocarbons and [[carbon dioxide]] have mixing ratios three orders of magnitude lower.<ref name="Burgdorf Orton et al. 2006" /> The abundance ratio of water is around 7{{e|-9}}.<ref name="Encrenaz 2003" /> Ethane and acetylene tend to condense in the colder lower part of the stratosphere and tropopause (below 10&nbsp;mBar level) forming haze layers,<ref name="Summers & Strobel 1989" /> which may be partly responsible for the bland appearance of Uranus. The concentration of hydrocarbons in the Uranian stratosphere above the haze is significantly lower than in the stratospheres of the other giant planets.<ref name="Bishop Atreya et al. 1990" /><ref name="Herbert & Sandel 1999" />
[[File:PIA25951-Uranus-NorthPole-Cyclone-October2021.jpg|thumb|left|250px|Planet Uranus – North Pole – Cyclone ([[Very Large Array|VLA]]; October 2021)]]
The outermost layer of the Uranian atmosphere is the thermosphere and corona, which has a uniform temperature of around {{convert|800|K|C}} to {{convert|850|K|C}}.<ref name="Lunine 1993" /><ref name="Herbert & Sandel 1999" /> The heat sources necessary to sustain such a high level are not understood, as neither the solar UV nor the [[aurora (astronomy)|auroral]] activity can provide the necessary energy to maintain these temperatures. The weak cooling efficiency due to the lack of hydrocarbons in the stratosphere above 0.1&nbsp;mBar pressure levels may contribute too.<ref name="Herbert Sandel et al. 1987" /><ref name="Herbert & Sandel 1999" /> In addition to molecular hydrogen, the thermosphere-corona contains many free hydrogen atoms. Their small mass and high temperatures explain why the corona extends as far as {{convert|50000|km|mi|abbr=on}}, or two Uranian radii, from its surface.<ref name="Herbert Sandel et al. 1987" /><ref name="Herbert & Sandel 1999" />

This extended corona is a unique feature of Uranus.<ref name="Herbert & Sandel 1999" /> Its effects include a [[drag (physics)|drag]] on small particles orbiting Uranus, causing a general depletion of dust in the Uranian rings.<ref name="Herbert Sandel et al. 1987" /> The Uranian thermosphere, together with the upper part of the stratosphere, corresponds to the [[ionosphere]] of Uranus.<ref name="Tyler 1986" /> Observations show that the ionosphere occupies altitudes from {{convert|2000|to|10000|km|mi|abbr=on}}.<ref name="Tyler 1986" /> The Uranian ionosphere is denser than that of either Saturn or Neptune, which may arise from the low concentration of hydrocarbons in the stratosphere.<ref name="Herbert & Sandel 1999" /><ref name="Trafton Miller et al. 1999" /> The ionosphere is mainly sustained by solar UV radiation and its density depends on the [[Space weather|solar activity]].<ref name="Encrenaz Drossart et al. 2003" /> [[Auroral]] activity is insignificant as compared to Jupiter and Saturn.<ref name="Herbert & Sandel 1999" /><ref name="Lam Miller et al. 1997" />

== Climate ==
{{main|Climate of Uranus}}

At ultraviolet and visible wavelengths, Uranus's atmosphere is bland in comparison to the other giant planets, even to Neptune, which it otherwise closely resembles.<ref name="Sromovsky & Fry 2005" /> When ''Voyager&nbsp;2'' flew by Uranus in 1986, it observed a total of 10 [[cloud]] features across the entire planet.<ref name="Smith Soderblom et al. 1986" /><ref name="planetary" /> One proposed explanation for this dearth of features is that Uranus's [[internal heat]] is markedly lower than that of the other giant planets, being the coldest planet in the Solar System.<ref name="Lunine 1993" /><ref name="Pearl Conrath et al. 1990" />

=== Banded structure, winds and clouds ===
[[File:Uranus-timelapse.gif|thumb|''Voyager 2''<nowiki/>'s timelapse of Uranus's dynamic atmosphere]]
In 1986, ''Voyager&nbsp;2'' found that the visible southern hemisphere of Uranus can be subdivided into two regions: a bright polar cap and dark equatorial bands.<ref name="Smith Soderblom et al. 1986" /> Their boundary is located at about −45° of [[latitude]]. A narrow band straddling the latitudinal range from −45 to −50° is the brightest large feature on its visible surface.<ref name="Smith Soderblom et al. 1986" /><ref name="Hammel de Pater et al. Uranus in 2003, 2005" /> It is called a southern "collar". The cap and collar are thought to be a dense region of methane clouds located within the pressure range of 1.3 to 2&nbsp;bar.<ref name="Rages Hammel et al. 2004" /> Besides the large-scale banded structure, ''Voyager&nbsp;2'' observed ten small bright clouds, most lying several degrees to the north from the collar.<ref name="Smith Soderblom et al. 1986" /> In all other respects, Uranus looked like a dynamically dead planet in 1986.

''Voyager&nbsp;2'' arrived during the height of Uranus's southern summer and could not observe the northern hemisphere. At the beginning of the 21st century, when the northern polar region came into view, the Hubble Space Telescope (HST) and [[Keck telescopes|Keck]] telescope initially observed neither a collar nor a polar cap in the northern hemisphere.<ref name="Hammel de Pater et al. Uranus in 2003, 2005" /> So Uranus appeared to be asymmetric: bright near the south pole and uniformly dark in the region north of the southern collar.<ref name="Hammel de Pater et al. Uranus in 2003, 2005" /> In 2007, when Uranus passed its equinox, the southern collar almost disappeared, and a faint northern collar emerged near 45° of latitude.<ref name="Sromovsky Fry et al. 2009" /> In 2023, a team employing the [[Very Large Array]] observed a dark collar at 80° latitude, and a bright spot at the north pole, indicating the presence of a [[polar vortex]].<ref>{{Cite journal |last1=Akins |first1=Alex |last2=Hofstadter |first2=Mark |last3=Butler |first3=Bryan |last4=Friedson |first4=A. James |last5=Molter |first5=Edward |last6=Parisi |first6=Marzia |last7=de Pater |first7=Imke |date=28 May 2023 |title=Evidence of a Polar Cyclone on Uranus From VLA Observations |journal=[[Geophysical Research Letters]] |volume=50 |issue=10 |arxiv=2305.15521 |bibcode=2023GeoRL..5002872A |doi=10.1029/2023GL102872 |issn=0094-8276 |s2cid=258883726}}</ref>
[[File:Uranus Dark spot.jpg|thumb|The first dark spot observed on Uranus. Image obtained by the HST [[Advanced Camera for Surveys|ACS]] in 2006.|left]]
In the 1990s, the number of the observed bright cloud features grew considerably, partly because new high-resolution imaging techniques became available.<ref name="Sromovsky & Fry 2005" /> Most were found in the northern hemisphere as it started to become visible.<ref name="Sromovsky & Fry 2005" /> An early explanation—that bright clouds are easier to identify in its dark part, whereas in the southern hemisphere the bright collar masks them—was shown to be incorrect.<ref name="Karkoschka ('Uranus') 2001" /><ref name="Hammel de Pater et al. Uranus in 2004, 2005" /> Nevertheless, there are differences between the clouds of each hemisphere. The northern clouds are smaller, sharper and brighter.<ref name="Hammel de Pater et al. Uranus in 2004, 2005" /> They appear to lie at a higher altitude.<ref name="Hammel de Pater et al. Uranus in 2004, 2005" /> The lifetime of clouds spans several orders of magnitude. Some small clouds live for hours; at least one southern cloud may have persisted since the ''Voyager&nbsp;2'' flyby.<ref name="Sromovsky & Fry 2005" /><ref name="planetary" /> Recent observation also discovered that cloud features on Uranus have a lot in common with those on Neptune.<ref name="Sromovsky & Fry 2005" /> For example, the dark spots common on Neptune had never been observed on Uranus before 2006, when the first such feature dubbed [[Climate of Uranus#Uranus Dark Spot|Uranus Dark Spot]] was imaged.<ref name="DarkSpot" /> The speculation is that Uranus is becoming more Neptune-like during its equinoctial season.<ref name="Hammel2007" />

The tracking of numerous cloud features allowed determination of [[Zonal and meridional|zonal]] winds blowing in the upper troposphere of Uranus.<ref name="Sromovsky & Fry 2005" /> At the equator winds are retrograde, which means that they blow in the reverse direction to the planetary rotation. Their speeds are from {{convert|-100|to|-50|m/s|km/h mph|order=out|abbr=on}}.<ref name="Sromovsky & Fry 2005" /><ref name="Hammel de Pater et al. Uranus in 2003, 2005" /> Wind speeds increase with the distance from the equator, reaching zero values near ±20° latitude, where the troposphere's temperature minimum is located.<ref name="Sromovsky & Fry 2005" /><ref name="Hanel Conrath et al. 1986" /> Closer to the poles, the winds shift to a prograde direction, flowing with Uranus's rotation. Wind speeds continue to increase reaching maxima at ±60° latitude before falling to zero at the poles.<ref name="Sromovsky & Fry 2005" /> Wind speeds at −40° latitude range from {{convert|150|to|200|m/s|km/h mph|order=out|abbr=on}}. Because the collar obscures all clouds below that parallel, speeds between it and the southern pole are impossible to measure.<ref name="Sromovsky & Fry 2005" /> In contrast, in the northern hemisphere maximum speeds as high as {{convert|240|m/s|km/h mph|order=out|abbr=on}} are observed near +50° latitude.<ref name="Sromovsky & Fry 2005" /><ref name="Hammel de Pater et al. Uranus in 2003, 2005" /><ref name="Hammel Rages et al. 2001" />

In 1986, the ''Voyager 2'' Planetary Radio Astronomy (PRA) experiment observed 140 lightning flashes, or Uranian electrostatic discharges with a frequency of 0.9-40&nbsp;MHz.<ref name="Atmospheric Electricity at the Ice">{{cite journal |last1=Aplin |first1=K.L. |last2=Fischer |first2=G. |last3=Nordheim |first3=T.A. |last4=Konovalenko | first4=A. |last5=Zakharenko |first5=V. |last6=Zarka |first6= P.|title=Atmospheric Electricity at the Ice Giants |journal=Space Science Reviews |date=2020 |volume=216 |issue=2 |page=26 |doi=10.1007/s11214-020-00647-0 |arxiv=1907.07151 |bibcode=2020SSRv..216...26A }}</ref><ref name="Radio detection of uranian lightnin">{{cite journal |last1=Zarka |first1=P. |last2=Pederson |first2=B.M. |title=Radio detection of uranian lightning by Voyager 2 |journal=Nature |date=1986 |volume=323 |issue=6089 |pages=605–608 |doi=10.1038/323605a0  |bibcode=1986Natur.323..605Z }}</ref> The UEDs were detected from 600,000&nbsp;km of Uranus over 24 hours, most of which were not visible .<ref name="Atmospheric Electricity at the Ice"/> However, microphysical modelling suggests that Uranian lightning occurs in convective storms occurring in deep troposphere water clouds.<ref name="Atmospheric Electricity at the Ice"/><ref name="ReferenceA">{{cite journal |last1=Aglyamov |first1=Y.S. |last2=Lunine |first2=J. |last3=Atreya |first3=S. |last4=Guillot | first4=T. |last5=Becker |first5=H.N. |last6=Levin |first6=S.|last7=Bolton |first7=S.J. |title=Atmospheric Electricity at the Ice Giants |journal=Space Science Reviews |date=2020 |volume=216 |issue=2 |doi=10.1007/s11214-020-00647-0 |arxiv=1907.07151 |bibcode=2020SSRv..216...26A }}</ref> If this is the case, lightning will not be visible due to the thick cloud layers above the troposphere.<ref name="Radio detection of uranian lightnin"/> The UEDs were detected from 600,000&nbsp;km of Uranus, most of which were not visible .<ref name="Atmospheric Electricity at the Ice"/> Uranian lightning has a power of around 10<sup>8</sup> W, emits 1×10^7 J - 2×10^7 J of energy, and lasts an average of 120 ms. There is a possibility that the power of Uranian lightning varies greatly with the seasons caused by changes in convection rates in the clouds<ref name="Radio detection of uranian lightnin"/> The UEDs were detected from 600,000&nbsp;km of Uranus, most of which were not visible.<ref name="Atmospheric Electricity at the Ice"/> Uranian lightning is much more powerful than lightning on Earth and comparable to Jovian lightning.<ref name="Radio detection of uranian lightnin"/> During the Ice Giant flybys, "Voyager 2" detected lightning more clearly on Uranus than on Neptune due to the planet's lower gravity and possible warmer deep atmosphere.<ref name="ReferenceA"/>

=== Seasonal variation ===
[[File:Uranus clouds.jpg|thumb|upright|Uranus in 2005. Rings, southern collar and a bright cloud in the northern hemisphere are visible (HST ACS image).]]

For a short period from March to May 2004, large clouds appeared in the Uranian atmosphere, giving it a Neptune-like appearance.<ref name="NYT-20240104">{{cite news |last=Ferreira |first=Becky |title=Uranus and Neptune Reveal Their True Colors - Neptune is not as blue as you've been led to believe, and Uranus's shifting colors are better explained, in new research. |url=https://www.nytimes.com/2024/01/04/science/uranus-neptune-colors-blue.html |date=4 January 2024 |work=[[The New York Times]] |url-status=live |archiveurl=https://archive.today/20240105004738/https://www.nytimes.com/2024/01/04/science/uranus-neptune-colors-blue.html |archivedate=5 January 2024 |accessdate=5 January 2024 }}</ref><ref name="Hammel de Pater et al. Uranus in 2004, 2005" /><ref>{{cite web |last=Devitt |first=Terry |url=http://www.news.wisc.edu/10402 |title=Keck zooms in on the weird weather of Uranus |publisher=University of Wisconsin-Madison |date=2004 |access-date=24 December 2006 |archive-url=https://web.archive.org/web/20110813072359/http://www.news.wisc.edu/10402 |archive-date=13 August 2011 |url-status=dead }}</ref> Observations included record-breaking wind speeds of {{convert|229|m/s|km/h mph|order=out|abbr=on}} and a persistent thunderstorm referred to as "Fourth of July fireworks".<ref name="planetary" /> On 23 August 2006, researchers at the Space Science Institute (Boulder, Colorado) and the University of Wisconsin observed a dark spot on Uranus's surface, giving scientists more insight into Uranus atmospheric activity.<ref name="DarkSpot" /> Why this sudden upsurge in activity occurred is not fully known, but it appears that Uranus's extreme axial tilt results in extreme seasonal variations in its weather.<ref name="weather" /><ref name="Hammel2007" /> Determining the nature of this seasonal variation is difficult because good data on Uranus's atmosphere has existed for less than 84 years, or one full Uranian year. [[Photometry (astronomy)|Photometry]] over the course of half a Uranian year (beginning in the 1950s) has shown regular variation in the brightness in two [[spectral band]]s, with maxima occurring at the solstices and minima occurring at the equinoxes.<ref name="Lockwood & Jerzykiewicz 2006" /> A similar periodic variation, with maxima at the solstices, has been noted in [[microwave]] measurements of the deep troposphere begun in the 1960s.<ref name="Klein & Hofstadter 2006" /> [[Stratosphere|Stratospheric]] temperature measurements beginning in the 1970s also showed maximum values near the 1986 solstice.<ref name="Young et al. 2001" /> The majority of this variability is thought to occur owing to changes in viewing geometry.<ref name="Karkoschka ('Uranus') 2001" />

There are some indications that physical seasonal changes are happening in Uranus. Although Uranus is known to have a bright south polar region, the north pole is fairly dim, which is incompatible with the model of the seasonal change outlined above.<ref name="Hammel2007" /> During its previous northern solstice in 1944, Uranus displayed elevated levels of brightness, which suggests that the north pole was not always so dim.<ref name="Lockwood & Jerzykiewicz 2006" /> This information implies that the visible pole brightens some time before the solstice and darkens after the equinox.<ref name="Hammel2007" /> Detailed analysis of the visible and microwave data revealed that the periodical changes in brightness are not completely symmetrical around the solstices, which also indicates a change in the [[meridional]] albedo patterns.<ref name="Hammel2007" />

In the 1990s, as Uranus moved away from its solstice, Hubble and ground-based telescopes revealed that the south polar cap darkened noticeably (except the southern collar, which remained bright),<ref name="Rages Hammel et al. 2004" /> whereas the northern hemisphere demonstrated increasing activity,<ref name="planetary" /> such as cloud formations and stronger winds, bolstering expectations that it should brighten soon.<ref name="Hammel de Pater et al. Uranus in 2004, 2005" /> This indeed happened in 2007 when it passed an equinox: a faint northern polar collar arose, and the southern collar became nearly invisible, although the zonal wind profile remained slightly asymmetric, with northern winds being somewhat slower than southern.<ref name="Sromovsky Fry et al. 2009" />

The mechanism of these physical changes is still not clear.<ref name="Hammel2007" /> Near the summer and winter solstices, Uranus's hemispheres lie alternately either in full glare of the Sun's rays or facing deep space. The brightening of the sunlit hemisphere is thought to result from the local thickening of the methane clouds and haze layers located in the troposphere.<ref name="Rages Hammel et al. 2004" /> The bright collar at −45° latitude is also connected with methane clouds.<ref name="Rages Hammel et al. 2004" /> Other changes in the southern polar region can be explained by changes in the lower cloud layers.<ref name="Rages Hammel et al. 2004" /> The variation of the microwave [[Emission (electromagnetic radiation)|emission]] from Uranus is probably caused by changes in the deep tropospheric [[Circulation (fluid dynamics)|circulation]], because thick polar clouds and haze may inhibit convection.<ref name="Hofstadter & Butler 2003" /> Now that the spring and autumn equinoxes are arriving on Uranus, the dynamics are changing and convection can occur again.<ref name="planetary" /><ref name="Hofstadter & Butler 2003" />

== Magnetosphere ==
[[File:PIA23683-Uranus-MagneticField-20200325.gif|thumb|upright=1.4|The magnetic field of Uranus<br />(animated; 25 March 2020)]]
Before the arrival of ''Voyager&nbsp;2'', no measurements of the Uranian [[magnetosphere]] had been taken, so its nature remained a mystery. Before 1986, scientists had expected the [[magnetic field]] of Uranus to be in line with the [[solar wind]], because it would then align with Uranus's poles that lie in the [[ecliptic]].<ref name="Ness Acuña et al. 1986" />

''Voyager''{{'}}s observations revealed that Uranus's magnetic field is peculiar, both because it does not originate from its geometric centre, and because it is tilted at 59° from the axis of rotation.<ref name="Ness Acuña et al. 1986" /><ref name="Russell993" /> In fact, the magnetic dipole is shifted from Uranus's centre towards the south rotational pole by as much as one-third of the planetary radius.<ref name="Ness Acuña et al. 1986" /> This unusual geometry results in a highly asymmetric magnetosphere, where the magnetic field strength on the surface in the southern hemisphere can be as low as 0.1&nbsp;[[Gauss (unit)|gauss]] (10&nbsp;[[microtesla|μT]]), whereas in the northern hemisphere it can be as high as 1.1&nbsp;gauss (110&nbsp;μT).<ref name="Ness Acuña et al. 1986" /> The average field at the surface is 0.23&nbsp;gauss (23&nbsp;μT).<ref name="Ness Acuña et al. 1986" />
[[File:Uranian Magnetic field.gif|left|thumb|A diagram showing Uranus's asymmetric magnetosphere]]
Studies of ''Voyager&nbsp;2'' data in 2017 suggest that this asymmetry causes Uranus's magnetosphere to connect with the solar wind once a Uranian day, opening the planet to the Sun's particles.<ref>{{cite web |last=Maderer |first=Jason |date=26 June 2017 |title=Topsy-Turvy Motion Creates Light Switch Effect at Uranus |url=http://www.news.gatech.edu/2017/06/26/topsy-turvy-motion-creates-light-switch-effect-uranus |url-status=live |archive-url=https://web.archive.org/web/20170707101644/http://www.news.gatech.edu/2017/06/26/topsy-turvy-motion-creates-light-switch-effect-uranus |archive-date=7 July 2017 |access-date=8 July 2017 |publisher=Georgia Tech}}</ref> In comparison, the magnetic field of Earth is roughly as strong at either pole, and its "magnetic equator" is roughly parallel with its geographical equator.<ref name="Russell993" /> The dipole moment of Uranus is 50&nbsp;times that of Earth.<ref name="Ness Acuña et al. 1986" /><ref name="Russell993" /> Neptune has a similarly displaced and tilted magnetic field, suggesting that this may be a common feature of ice giants.<ref name="Russell993" /> One hypothesis is that, unlike the magnetic fields of the terrestrial and gas giants, which are generated within their cores, the ice giants' magnetic fields are generated by motion at relatively shallow depths, for instance, in the water–ammonia ocean.<ref name="Atreya2006" /><ref>{{Cite journal |last1=Stanley |first1=Sabine |author-link1=Sabine Stanley |last2=Bloxham |first2=Jeremy |date=March 2004 |title=Convective-region geometry as the cause of Uranus' and Neptune's unusual magnetic fields |url=http://mahi.ucsd.edu/johnson/ES130/stanley2004-nature.pdf |url-status=dead |journal=[[Nature (journal)|Nature]] |volume=428 |issue=6979 |pages=151–153 |bibcode=2004Natur.428..151S |doi=10.1038/nature02376 |issn=0028-0836 |pmid=15014493 |s2cid=33352017 |archive-url=https://web.archive.org/web/20070807213745/http://mahi.ucsd.edu/johnson/ES130/stanley2004-nature.pdf |archive-date=7 August 2007 |access-date=5 August 2007}}</ref> Another possible explanation for the magnetosphere's alignment is that there are oceans of liquid diamond in Uranus's interior that would deter the magnetic field.<ref name="Bland, Eric" />

It is, however, unclear whether the observed asymmetry of Uranus's magnetic field represents the typical state of the magnetosphere, or a coincidence of observing it during unusual [[space weather]] conditions. A post-analysis of Voyager data from 2024 suggests that the strongly asymmetric shape of the magnetosphere observed during the fly-by represents an anomalous state, as the measured values of solar wind density at the time were unusually high, which could have compressed Uranus's magnetosphere. The interaction with the solar wind event could also explain the apparent paradox of presence of strong electron [[Van Allen radiation belt|radiation belts]] despite the otherwise low magnetospheric [[Plasma (physics)|plasma]] density measured. Such conditions are estimated to occur less than 5% of the time.<ref>{{cite web |url=https://www.nasa.gov/missions/voyager-program/voyager-2/mining-old-data-from-nasas-voyager-2-solves-several-uranus-mysteries/ |title=Mining Old Data From NASA's Voyager 2 Solves Several Uranus Mysteries |date=11 November 2024 |publisher=[[NASA]] |access-date=26 December 2024}}</ref><ref>{{cite journal |last1=Jasinski |first1=Jamie M. |last2=Cochrane |first2=Corey J. |last3=Jia |first3=Xianzhe |last4=Dunn |first4=William R. |last5=Roussos |first5=Elias |last6=Nordheim |first6=Tom A. |last7=Regoli |first7=Leonardo H. |last8=Achilleos |first8=Nick |last9=Krupp |first9=Norbert |last10=Murphy |first10=Neil |year=2024 |title=The anomalous state of Uranus's magnetosphere during the Voyager 2 flyby |journal=[[Nature Astronomy]] |volume=9 |issue=1 |pages=66–74 |doi=10.1038/s41550-024-02389-3 |bibcode=2025NatAs...9...66J |s2cid=273973089 |doi-access=free|pmid=39866552 |pmc=11757144 }}</ref>

Despite its curious alignment, in other respects the Uranian magnetosphere is like those of other planets: it has a [[bow shock]] at about 23 Uranian radii ahead of it, a [[magnetopause]] at 18 Uranian radii, a fully developed [[magnetotail]], and [[radiation belt]]s.<ref name="Ness Acuña et al. 1986" /><ref name="Russell993" /><ref name="Krimigis Armstrong et al. 1986" /> Overall, the structure of Uranus's magnetosphere is different from Jupiter's and more similar to Saturn's.<ref name="Ness Acuña et al. 1986" /><ref name="Russell993" /> Uranus's [[magnetotail]] trails behind it into space for millions of kilometres and is twisted by its sideways rotation into a long corkscrew.<ref name="Ness Acuña et al. 1986" /><ref>{{cite web |date=2003 |title=Voyager: Uranus: Magnetosphere |url=http://voyager.jpl.nasa.gov/science/uranus_magnetosphere.html |url-status=dead |archive-url=https://web.archive.org/web/20110827125820/http://voyager.jpl.nasa.gov/science/uranus_magnetosphere.html |archive-date=27 August 2011 |access-date=13 June 2007 |publisher=NASA}}</ref>[[File:Alien aurorae on Uranus (remastered).jpg|thumb|Aurorae on Uranus taken by the [[Space Telescope Imaging Spectrograph]] (STIS) installed on [[Hubble Space Telescope|Hubble]].<ref>{{cite web |title=Alien aurorae on Uranus |url=https://www.spacetelescope.org/images/potw1714a/ |url-status=live |archive-url=https://web.archive.org/web/20170403160412/http://spacetelescope.org/images/potw1714a/ |archive-date=3 April 2017 |access-date=3 April 2017 |website=www.spacetelescope.org}}</ref>]]Uranus's magnetosphere contains [[charged particle]]s: mainly [[proton]]s and [[electron]]s, with a small amount of [[Dihydrogen cation|H<sub>2</sub><sup>+</sup>]] ions.<ref name="Russell993" /><ref name="Krimigis Armstrong et al. 1986" /> Many of these particles probably derive from the thermosphere.<ref name="Krimigis Armstrong et al. 1986" /> The ion and electron energies can be as high as 4 and 1.2&nbsp;[[megaelectronvolt]]s, respectively.<ref name="Krimigis Armstrong et al. 1986" /> The density of low-energy (below 1&nbsp;[[kiloelectronvolt]]) ions in the inner magnetosphere is about 2&nbsp;cm<sup>−3</sup>.<ref name="Bridge1986" /> The particle population is strongly affected by the Uranian moons, which sweep through the magnetosphere, leaving noticeable gaps.<ref name="Krimigis Armstrong et al. 1986" /> The particle [[flux]] is high enough to cause darkening or [[space weathering]] of their surfaces on an astronomically rapid timescale of 100,000&nbsp;years.<ref name="Krimigis Armstrong et al. 1986" /> This may be the cause of the uniformly dark colouration of the Uranian satellites and rings.<ref name="summary" />

Uranus has relatively well developed aurorae, which are seen as bright arcs around both magnetic poles.<ref name="Herbert & Sandel 1999" /> Unlike Jupiter's, Uranus's aurorae seem to be insignificant for the energy balance of the planetary thermosphere.<ref name="Lam Miller et al. 1997" /> They, or rather their [[trihydrogen cation]]s' infrared spectral emissions, have been studied in-depth as of late 2023.<ref name="Thomas Melin Stallard Chowdhury 2023 pp. 1473–1480">{{cite journal | last1=Thomas | first1=Emma M. | last2=Melin | first2=Henrik | last3=Stallard | first3=Tom S. | last4=Chowdhury | first4=Mohammad N. | last5=Wang | first5=Ruoyan | last6=Knowles | first6=Katie | last7=Miller | first7=Steve | title=Detection of the infrared aurora at Uranus with Keck-NIRSPEC | journal=Nature Astronomy | volume=7 | issue=12 | date=23 October 2023 | issn=2397-3366 | doi=10.1038/s41550-023-02096-5 | pages=1473–1480| arxiv=2311.06172 | bibcode=2023NatAs...7.1473T }}</ref>

In March 2020, NASA astronomers reported the detection of a large atmospheric magnetic bubble, also known as a [[plasmoid]], released into [[outer space]] from the planet Uranus, after reevaluating old data recorded by the ''[[Voyager&nbsp;2]]'' [[space probe]] during a flyby of the planet in 1986.<ref name="NASA-20200325">{{cite news |last=Hatfield |first=Mike |date=25 March 2020 |title=Revisiting Decades-Old Voyager&nbsp;2 Data, Scientists Find One More Secret - Eight and a half years into its grand tour of the solar system, NASA's Voyager&nbsp;2 spacecraft was ready for another encounter. It was Jan. 24, 1986, and soon it would meet the mysterious seventh planet, icy-cold Uranus. |work=[[NASA]] |url=https://www.nasa.gov/feature/goddard/2020/revisiting-decades-old-voyager-2-data-scientists-find-one-more-secret |url-status=live |access-date=27 March 2020 |archive-url=https://web.archive.org/web/20200327030510/https://www.nasa.gov/feature/goddard/2020/revisiting-decades-old-voyager-2-data-scientists-find-one-more-secret |archive-date=27 March 2020}}</ref><ref name="NYT-20200327">{{cite news |last=Andrews |first=Robin George |date=27 March 2020 |title=Uranus Ejected a Giant Plasma Bubble During Voyager&nbsp;2's Visit - The planet is shedding its atmosphere into the void, a signal that was recorded but overlooked in 1986 when the robotic spacecraft flew past. |work=[[The New York Times]] |url=https://www.nytimes.com/2020/03/27/science/uranus-bubble-voyager.html |url-status=live |access-date=27 March 2020 |archive-url=https://web.archive.org/web/20200327215013/https://www.nytimes.com/2020/03/27/science/uranus-bubble-voyager.html |archive-date=27 March 2020}}</ref>

== Moons ==
{{main|Moons of Uranus}}

{{see also|Timeline of discovery of Solar System planets and their moons}}
[[File:Uranian_moon_montage,_albedo_corrected.png|thumb|300x300px|Major moons of Uranus in order of increasing distance (left to right), at their proper relative sizes and [[albedo]]s. From left to right, they are Miranda, Ariel, Umbriel, Titania, and Oberon. (collage of ''Voyager&nbsp;2'' photographs)]]
[[File:Annotated_Moons_of_Uranus.png|thumb|Uranus along with its five major moons and nine inner moons as taken by the [[James Webb Space Telescope]]'s [[NIRCam]].]]
Uranus has 28 known [[natural satellites]].<ref name="Sheppardmoons2024" /> The names of these satellites are chosen from characters in the works of [[Shakespeare]] and [[Alexander Pope]].<ref name="Faure2007" /><ref name="Nineplanets" /> The five main satellites are [[Miranda (moon)|Miranda]], [[Ariel (moon)|Ariel]], [[Umbriel]], [[Titania (moon)|Titania]], and [[Oberon (moon)|Oberon]].<ref name="Faure2007" /> The Uranian satellite system is the least massive among those of the giant planets; the combined mass of the five major satellites would be less than half that of [[Triton (moon)|Triton]] (largest moon of [[Neptune]]) alone.<ref name="Jacobson Campbell et al. 1992" /> The largest of Uranus's satellites, Titania, has a radius of only {{convert|788.9|km|mi|abbr=on}}, or less than half that of the [[Moon]], but slightly more than Rhea, the second-largest satellite of Saturn, making Titania the [[List of natural satellites by diameter|eighth-largest moon]] in the Solar System. Uranus's satellites have relatively low [[albedo]]s; ranging from 0.20 for Umbriel to 0.35 for Ariel (in green light).<ref name="Smith Soderblom et al. 1986" /> They are ice–rock conglomerates composed of roughly 50% ice and 50% rock. The ice may include ammonia and [[carbon dioxide]].<ref name="summary" /><ref name="Hussmann2006" />

Among the Uranian satellites, Ariel appears to have the youngest surface, with the fewest impact craters, and Umbriel the oldest.<ref name="Smith Soderblom et al. 1986" /><ref name="summary" /> Miranda has fault canyons {{convert|20|km|mi|abbr=on}} deep, terraced layers, and a chaotic variation in surface ages and features.<ref name="Smith Soderblom et al. 1986" /> Miranda's past geologic activity is thought to have been driven by [[tidal heating]] at a time when its orbit was more eccentric than currently, probably as a result of a former 3:1 [[orbital resonance]] with Umbriel.<ref name="Tittemore Wisdom 1990" /> [[Rift|Extensional]] processes associated with upwelling [[diapir]]s are the likely origin of Miranda's 'racetrack'-like [[Corona (planetary geology)|coronae]].<ref>{{cite journal |last1=Pappalardo |first1=R. T. |last2=Reynolds |first2=S. J. |last3=Greeley |first3=R. |title=Extensional tilt blocks on Miranda: Evidence for an upwelling origin of Arden Corona |journal=Journal of Geophysical Research |volume=102 |issue=E6 |pages=13,369–13,380 |date=1997 |url=http://www.agu.org/pubs/crossref/1997/97JE00802.shtml |doi=10.1029/97JE00802 |bibcode=1997JGR...10213369P |doi-access=free |access-date=8 December 2007 |archive-date=27 September 2012 |archive-url=https://web.archive.org/web/20120927014719/http://www.agu.org/pubs/crossref/1997/97JE00802.shtml |url-status=live }}</ref><ref>{{cite web |last=Chaikin |first=Andrew |author-link=Andrew Chaikin |title=Birth of Uranus's Provocative Moon Still Puzzles Scientists |work=Space.Com |publisher=ImaginovaCorp. |date=16 October 2001 |url=http://www.space.com/scienceastronomy/solarsystem/miranda_creation_011016-1.html |archive-url=https://web.archive.org/web/20080709020909/http://www.space.com/scienceastronomy/solarsystem/miranda_creation_011016-1.html |archive-date=9 July 2008 |access-date=7 December 2007}}</ref> Ariel is thought to have once been held in a 4:1 resonance with Titania.<ref name="Tittemore 1990" />

Uranus has at least one [[horseshoe orbit]]er occupying the [[Sun]]–Uranus {{L3}} [[Lagrangian point]]—a gravitationally unstable region at 180° in its orbit, [[83982 Crantor]].<ref name="coorbital1">{{cite journal |last=Gallardo |first=T. |title=Atlas of the mean motion resonances in the Solar System |journal=Icarus |volume=184 |issue=1 |pages=29–38 |date=2006 |doi=10.1016/j.icarus.2006.04.001 |bibcode=2006Icar..184...29G}}</ref><ref name="coorbital2">{{cite journal |last1=de la Fuente Marcos |first1=C. |last2=de la Fuente Marcos |first2=R. |title=Crantor, a short-lived horseshoe companion to Uranus |journal=Astronomy and Astrophysics |volume=551 |pages=A114 |date=2013 |doi=10.1051/0004-6361/201220646 |url=http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/abs/2013/03/aa20646-12/aa20646-12.html |bibcode=2013A&A...551A.114D |arxiv=1301.0770 |s2cid=118531188 |access-date=29 September 2021 |archive-date=30 August 2021 |archive-url=https://web.archive.org/web/20210830233403/https://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=%2Farticles%2Faa%2Fabs%2F2013%2F03%2Faa20646-12%2Faa20646-12.html |url-status=live }}</ref> Crantor moves inside Uranus's co-orbital region on a complex, temporary horseshoe orbit. {{mpl|2010 EU|65}} is also a promising Uranus horseshoe [[Trojan (celestial body)|librator]] candidate.<ref name="coorbital2" />

== Rings ==
{{main|Rings of Uranus}}

[[File:Annotated_Uranian_rings.png|thumb|Uranus's rings, inner moons, and atmosphere as imaged by the [[James Webb Space Telescope]]'s [[NIRCam|near-infrared camera]].|left]]The Uranian rings are composed of extremely dark particles, which vary in size from micrometres to a fraction of a metre.<ref name="Smith Soderblom et al. 1986" /> Thirteen distinct rings are presently known, the brightest being the ε ring. All except the two rings of Uranus are extremely narrow—they are usually a few kilometres wide. The rings are probably quite young; the dynamics considerations indicate that they did not form with Uranus. The matter in the rings may once have been part of a moon (or moons) that was shattered by high-speed impacts. From numerous pieces of debris that formed as a result of those impacts, only a few particles survived, in stable zones corresponding to the locations of the present rings.<ref name="summary" /><ref name="Esposito2002" />

William Herschel described a possible ring around Uranus in 1789. This sighting is generally considered doubtful, because the rings are quite faint, and in the two following centuries none were noted by other observers. Still, Herschel made an accurate description of the epsilon ring's size, its angle relative to Earth, its red colour, and its apparent changes as Uranus travelled around the Sun.<ref>{{cite news |title=Uranus rings 'were seen in 1700s' |work=BBC News |url=http://news.bbc.co.uk/2/hi/science/nature/6569849.stm |date=19 April 2007 |access-date=19 April 2007 |archive-date=3 August 2012 |archive-url=https://web.archive.org/web/20120803104312/http://news.bbc.co.uk/2/hi/science/nature/6569849.stm |url-status=live }}</ref><ref>{{cite web |title=Did William Herschel Discover The Rings of Uranus in the 18th Century? |work=Physorg.com |url=http://www.physorg.com/news95949762.html |date=2007 |access-date=20 June 2007 |archive-date=11 February 2012 |archive-url=https://web.archive.org/web/20120211075055/http://www.physorg.com/news95949762.html |url-status=live }}</ref> The ring system was definitively discovered on 10 March 1977 by [[James L. Elliot]], Edward W. Dunham, and [[Jessica Mink]] using the [[Kuiper Airborne Observatory]]. The discovery was serendipitous; they planned to use the [[occultation]] of the star SAO 158687 (also known as HD 128598) by Uranus to study its [[atmosphere]]. When their observations were analysed, they found that the star had disappeared briefly from view five times both before and after it disappeared behind Uranus. They concluded that there must be a ring system around Uranus.<ref name="Elliot1977" /> Later, they detected four additional rings.<ref name="Elliot1977" /> The rings were directly imaged when ''Voyager&nbsp;2'' passed Uranus in 1986.<ref name="Smith Soderblom et al. 1986" /> ''Voyager&nbsp;2'' also discovered two additional faint rings, bringing the total number to eleven.<ref name="Smith Soderblom et al. 1986" />

In December 2005, the [[Hubble Space Telescope]] detected a pair of previously unknown rings. The largest is located twice as far from Uranus as the previously known rings. These new rings are so far from Uranus that they are called the "outer" ring system. Hubble also spotted two small satellites, one of which, [[Mab (moon)|Mab]], shares its orbit with the outermost newly discovered ring. The new rings bring the total number of Uranian rings to 13.<ref>{{cite web |title=NASA's Hubble Discovers New Rings and Moons Around Uranus |work=Hubblesite |url=http://hubblesite.org/newscenter/archive/releases/2005/33/ |date=2005 |access-date=9 June 2007 |archive-date=5 March 2012 |archive-url=https://web.archive.org/web/20120305175554/http://hubblesite.org/newscenter/archive/releases/2005/33/ |url-status=live }}</ref> In April 2006, images of the new rings from the [[Keck Observatory]] yielded the colours of the outer rings: the outermost is blue and the other one red.<ref name="dePater2006" /><ref>{{cite web |title=Blue ring discovered around Uranus |publisher=UC Berkeley News |last=Sanders |first=Robert |url=http://www.berkeley.edu/news/media/releases/2006/04/06_bluering.shtml |date=6 April 2006 |access-date=3 October 2006 |archive-date=6 March 2012 |archive-url=https://web.archive.org/web/20120306060105/http://www.berkeley.edu/news/media/releases/2006/04/06_bluering.shtml |url-status=live }}</ref> One hypothesis concerning the outer ring's blue colour is that it is composed of minute particles of water ice from the surface of Mab that are small enough to scatter blue light.<ref name="dePater2006" /><ref>{{Cite web |last=Battersby |first=Stephen |date=April 2006 |title=Blue ring of Uranus linked to sparkling ice |url=https://www.newscientist.com/article/dn8960-blue-ring-of-uranus-linked-to-sparkling-ice.html |url-status=live |archive-url=https://web.archive.org/web/20110604035019/http://www.newscientist.com/article/dn8960-blue-ring-of-uranus-linked-to-sparkling-ice.html |archive-date=4 June 2011 |access-date=9 June 2007 |website=New Scientist}}</ref> In contrast, Uranus's inner rings appear grey.<ref name="dePater2006" />

Although the Uranian rings are very difficult to directly observe from Earth, advances in digital imaging have allowed several amateur astronomers to successfully photograph the rings with red or infrared filters; telescopes with apertures as small as {{Convert|36|cm|abbr=in}} may be able to detect the rings with proper imaging equipment.<ref>{{Cite web |title=Amateur detection of Uranus' rings – British Astronomical Association |url=https://britastro.org/journal_contents_ite/amateur-detection-of-uranus-rings |access-date=22 August 2023 |language=en-GB |archive-date=22 August 2023 |archive-url=https://web.archive.org/web/20230822064521/https://britastro.org/journal_contents_ite/amateur-detection-of-uranus-rings |url-status=live }}</ref>

== Exploration ==
{{main|Exploration of Uranus}}
[[File:Uranus seen from Saturn by Cassini.jpg|thumb|Uranus as seen from the [[Cassini–Huygens|''Cassini'' spacecraft]] at [[Saturn]]]]
Launched in 1977, ''Voyager&nbsp;2'' made its closest approach to Uranus on 24 January 1986, coming within {{convert|81500|km|mi|abbr=on}} of the cloudtops, before continuing its journey to Neptune. The spacecraft studied the structure and chemical composition of Uranus's atmosphere,<ref name="Tyler 1986" /> including its unique weather, caused by its extreme axial tilt. It made the first detailed investigations of its five largest moons and discovered 10 new ones. ''Voyager 2'' examined all nine of the [[Rings of Uranus|system's known rings]] and discovered two more.<ref name="Smith Soderblom et al. 1986" /><ref name="summary" /><ref>{{cite web |title=Voyager: The Interstellar Mission: Uranus |work=JPL |url=http://voyager.jpl.nasa.gov/science/uranus.html |date=2004 |access-date=9 June 2007 |archive-date=7 August 2011 |archive-url=https://web.archive.org/web/20110807215103/http://voyager.jpl.nasa.gov/science/uranus.html |url-status=live }}</ref> It also studied the magnetic field, its irregular structure, its tilt and its unique corkscrew [[magnetosphere|magnetotail]] caused by Uranus's sideways orientation.<ref name="Ness Acuña et al. 1986" />

No other spacecraft has flown by Uranus since then, though there have been many [[proposed Uranus missions|proposed missions]] to revisit the Uranus system. The possibility of sending the [[Cassini–Huygens|''Cassini'' spacecraft]] from Saturn to Uranus was evaluated during a mission extension planning phase in 2009, but was ultimately rejected in favour of destroying it in the Saturnian atmosphere,<ref name="spilker" /> as it would have taken about twenty years to get to the Uranian system after departing Saturn.<ref name="spilker" /> A Uranus entry probe could use [[Pioneer Venus Multiprobe]] heritage and descend to 1–5 atmospheres.<ref name="uop" /> A [[Uranus orbiter and probe]] was recommended by the 2013–2022 [[Planetary Science Decadal Survey]] published in 2011; the proposal envisaged launch during 2020–2023 and a 13-year cruise to Uranus.<ref name="uop" /> The committee's opinion was reaffirmed in 2022, when a Uranus probe/orbiter mission was placed at the highest priority, due to the lack of knowledge about [[ice giant]]s.<ref>{{cite web |title=Planetary Science and Astrobiology Decadal Survey 2023-2032 |url=https://www.nationalacademies.org/our-work/planetary-science-and-astrobiology-decadal-survey-2023-2032 |access-date=17 May 2022 |website=National Academies |archive-date=29 March 2021 |archive-url=https://web.archive.org/web/20210329003054/https://www.nationalacademies.org/our-work/planetary-science-and-astrobiology-decadal-survey-2023-2032 |url-status=live }}</ref> Most recently, the CNSA's ''Tianwen-4'' Jupiter orbiter, launching in 2029, is planned to have a subprobe that will detach and get a gravity assist instead of entering orbit, flying by Uranus in March 2045 before heading to interstellar space.<ref name="TianwenPlSoc"/> China also has plans for a potential ''Tianwen-5'' that may orbit either Uranus or Neptune that have yet to come to fruition.<ref name="TianwenPlSoc"/>

== In culture ==
{{Prose|section|date=April 2025}}
As well as being a popular [[Uranus in fiction|subject in fiction]], Uranus has inspired artistic works including [[Lydia Sigourney]]'s 1827 poem {{ws|[[s:Poems (Sigourney, 1827)/The Georgian Planet|The Georgian Planet]]|ps=no}} and a movement in [[Gustav Holst]]'s orchestral suite ''[[The Planets]]'', written between 1914 and 1916. Herschel's discovery of the planet is also referenced in the lines "Then felt I like some watcher of the skies/When a new planet swims into his ken", from [[John Keats]]'s poem "[[On First Looking into Chapman's Homer]]".<ref>{{cite web |last=Melani |first=Lilia |date=12 February 2009 |title=On First Looking into Chapman's Homer |url=https://academic.brooklyn.cuny.edu/english/melani/cs6/homer.html |url-status=live |archive-url=https://web.archive.org/web/20210412194155/http://academic.brooklyn.cuny.edu/english/melani/cs6/homer.html |archive-date=12 April 2021 |access-date=5 May 2021 |publisher=City University of New York}}</ref> The planet's discovery also inspired the naming of the chemical element [[uranium]], itself discovered in 1789 by the German chemist [[Martin Heinrich Klaproth]].<ref>{{cite web |last=Hobart |first=David E. |date=23 July 2013 |title=Uranium |url=https://periodic.lanl.gov/92.shtml |url-status=live |archive-url=https://web.archive.org/web/20210512173625/https://periodic.lanl.gov/92.shtml |archive-date=12 May 2021 |access-date=5 May 2021 |work=Periodic Table of the Elements |publisher=Los Alamos National Laboratory}}</ref>

In modern [[astrology]], the planet Uranus (symbol [[File:Uranus monogram.svg|22px|alt=Uranus monogram]]) is the ruling planet of [[Aquarius (astrology)|Aquarius]]; prior to the discovery of Uranus, the ruling planet of Aquarius was Saturn. Because Uranus is [[cyan]] and Uranus is associated with electricity, the colour [[electric blue (color)|electric blue]], which is close to cyan, is associated with the sign Aquarius.<ref>{{cite book | last1=Parker | first1=Derek | author-link1=Derek Parker | last2=Parker | first2=Julia | author-link2=Julia Parker (astrologer) | title=Aquarius | series=Planetary Zodiac Library | date=1996 | publisher=DK Publishing | page=12 | isbn=9780789410870 }}</ref>

[[Operation Uranus]] was the successful [[military operation]] in [[World War II]] by the [[Red Army]] to take back [[Stalingrad]] and marked the turning point in the land war against the [[Wehrmacht]]. It was part of a series of operations named after planets, including [[Operation Mars|Mars]] and [[Operation Little Saturn|Saturn]].

== See also ==
<!-- Please keep entries in alphabetical order and add a short description [[WP:SEEALSO]] -->
{{div col|colwidth=20em}}
* {{mpl|2011 QF|99}} and {{mpl|2014 YX|49}}, the only two known Uranus trojans
* [[Colonization of Uranus|Colonisation of Uranus]]
* [[Extraterrestrial diamonds]] (thought to be abundant in Uranus)
* [[Outline of Uranus]]
* [[List of gravitationally rounded objects of the Solar System#Planets|Statistics of planets in the Solar System]]
* [[Uranus (astrology)|Uranus in astrology]]
* [[Uranus in fiction]]{{div col end}}
<!-- please keep entries in alphabetical order -->

== Notes ==
{{notelist
| notes =
{{efn
| name = atmospheric pressure
| Refers to the level of 1 bar atmospheric pressure.
}}

{{efn
| name = atmospheric pressure2
| Based on the volume within the level of 1 bar atmospheric pressure.
}}

{{efn
| name = symbol first
| Cf. [[File:Uranus monogram (fixed width).svg|20px|alt=♅|H monogram for Uranus]] (not supported by all fonts)
}}

{{efn
| name = symbol later
| Cf. [[File:Uranus symbol (fixed width).svg|20px|alt=⛢|Platinum symbol for Uranus]] (not supported by all fonts)
}}

}}

== References ==
{{Reflist
| refs =
<ref name="CSeligman">{{cite web |last=Seligman |first=Courtney |title=Rotation Period and Day Length |url=http://cseligman.com/text/sky/rotationvsday.htm |access-date=13 August 2009 |archive-date=28 July 2011 |archive-url=https://web.archive.org/web/20110728200555/http://cseligman.com/text/sky/rotationvsday.htm |url-status=live }}</ref>

<ref name="fact">{{cite web |url=https://nssdc.gsfc.nasa.gov/planetary/factsheet/uranusfact.html |title=Uranus Fact Sheet |publisher=NASA |last=Williams |first=Dr. David R. |access-date=10 August 2007 |date=31 January 2005 |archive-date=13 July 2017 |archive-url=https://web.archive.org/web/20170713094239/https://nssdc.gsfc.nasa.gov/planetary/factsheet/uranusfact.html |url-status=live }}</ref>

<ref name=Souami_Souchay_2012>{{cite journal
 | title=The solar system's invariable plane
 | last1=Souami | first1=D. | last2=Souchay | first2=J.
 | journal=Astronomy & Astrophysics
 | volume=543 | id=A133 | pages=11 | date=July 2012
 | doi=10.1051/0004-6361/201219011 | bibcode=2012A&A...543A.133S | doi-access=free }}</ref>

<ref name="Seidelmann Archinal A'hearn et al. 2007">
{{cite journal| doi = 10.1007/s10569-007-9072-y| last1 = Seidelmann| first1 = P. Kenneth| last2 = Archinal| first2 = Brent A.| last3 = A'Hearn<!-- written A'hearn here, mostly A'Hearn elsewhere -->| first3 = Michael F.| display-authors = 3| last4 = Conrad| first4 = Albert R.| last5 = Consolmagno| first5 = Guy J.| last6 = Hestroffer| first6 = Daniel| last7 = Hilton| first7 = James L.| last8 = Krasinsky| first8 = Georgij A.| last9 = Neumann| first9 = Gregory A.| last10=Oberst | first10=Jürgen | last11=Stooke | first11=Philip J. | last12=Tedesco | first12=Edward F. | last13=Tholen | first13=David J. | last14=Thomas | first14=Peter C. | last15=Williams | first15=Iwan P. | year = 2007| title = Report of the IAU/IAG Working Group on cartographic coordinates and rotational elements: 2006| journal = Celestial Mechanics and Dynamical Astronomy| volume = 98| issue = 3| pages = 155–180| bibcode = 2007CeMDA..98..155S| s2cid = 122772353| ref = {{sfnRef|Seidelmann Archinal A'hearn et al.|2007}}| doi-access = free}}
</ref>

<ref name="nasafact">
{{cite web |url=http://solarsystem.nasa.gov/planets/profile.cfm?Object=Uranus&Display=Facts |archive-url=https://web.archive.org/web/20031214200402/http://solarsystem.nasa.gov/planets/profile.cfm?Object=Uranus&Display=Facts |url-status=dead |archive-date=14 December 2003 |title=NASA: Solar System Exploration: Planets: Uranus: Facts & Figures |publisher=NASA |last=Munsell |first=Kirk |access-date=13 August 2007 |date=14 May 2007}}
</ref>

<ref name="Jacobson Campbell et al. 1992">
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<ref name="ephemeris">
{{cite web |title=Twelve Year Planetary Ephemeris: 1995–2006 |last=Espenak |first=Fred |work=NASA |url=http://sunearth.gsfc.nasa.gov/eclipse/TYPE/TYPE.html |archive-url=https://web.archive.org/web/20070626153349/http://sunearth.gsfc.nasa.gov/eclipse/TYPE/TYPE.html |archive-date=26 June 2007 |date=2005 |url-status=dead |access-date=14 June 2007}}
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<ref name="Lunine 1993">
{{cite journal |doi=10.1146/annurev.aa.31.090193.001245 |last=Lunine |first=Jonathan I. |date=September 1993 |title=The Atmospheres of Uranus and Neptune |journal=Annual Review of Astronomy and Astrophysics |volume=31 |pages=217–263 |bibcode=1993ARA&A..31..217L }}
</ref>

<ref name="OED">
{{OED|Uranus}}
</ref>

<ref name="BBCOUP">Because the vowel ''a'' is short in both Greek and Latin, the former pronunciation, {{IPA|/ˈjʊərənəs/}}, is the expected one. The [[BBC Pronunciation Unit]] notes that this pronunciation "is the preferred usage of astronomers":
{{Cite book |title=Oxford BBC Guide to Pronunciation: The Essential Handbook of the Spoken Word |date=2006 |publisher=[[Oxford University Press]] |isbn=978-0-19-280710-6 |editor-last=Holmquist Olausson |editor-first=Lena |location=Oxford |page=404 |editor-last2=Sangster |editor-first2=Catherine}}</ref>

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<ref name="Miner12">[[#Miner|Miner]], p. 12
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== Further reading ==
* {{cite web |title=Stinky 'mushball' hailstones on Uranus may explain an atmospheric anomaly there (and on Neptune, too) |first=Tereza |last=Pultarova |date=1 October 2021 |website=Space.com |url=https://www.space.com/uranus-mushballs-hailstones-stinky-gas-neptune-atmosphere-anomaly}}
* {{cite book |ref=Miner |last=Miner |first=Ellis D. |date=1998 |title=Uranus: The Planet, Rings and Satellites |location=New York |publisher=[[John Wiley and Sons]] |isbn=978-0-471-97398-0}}
* {{cite magazine |title=Uranus: Voyager Visits a Dark Planet |first=Rick |last=Gore |magazine=[[National Geographic (magazine)|National Geographic]] |pages=178–194 |volume=170 |issue=2 |date=August 1986 |issn=0027-9358 |oclc=643483454}}
* {{Cite book |last=Alexander |first=Arthur Francis O'Donel |author-link=Arthur Francis O'Donel Alexander |url=https://archive.org/details/planeturanushist0000alex |title=The Planet Uranus: A History of Observation, Theory and Discovery |date=1965 |publisher=[[American Elsevier Publ. Comp.]] |location=New York |url-access=registration}}
* {{Cite book |last=Bode |first=Johann Elert |author-link=Johann Elert Bode |url=https://archive.org/details/bub_gb_ZqA5AAAAcAAJ |title=Von Dem Neu Entdeckten Planeten |publisher=Bey dem Verfasser |year=1784 |location=Berlin |language=de |trans-title=From the Newly Discovered Planet |bibcode=1784vdne.book.....B |doi=10.3931/e-rara-1454}}

== External links ==
{{Sister project links|Uranus|b=no|n=no|s=no}}
* [http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=35653 Uranus] at European Space Agency
* [https://solarsystem.nasa.gov/planets/uranus/overview/ Uranus] at NASA's Solar System Exploration site
* [http://photojournal.jpl.nasa.gov/targetFamily/Uranus Uranus] at [[Jet Propulsion Laboratory]]'s planetary photojournal (photos)
* [http://www.ciclops.org/ir_index/81/Voyager_at_Uranus Voyager at Uranus] {{Webarchive|url=https://web.archive.org/web/20150104173418/http://www.ciclops.org/ir_index/81/Voyager_at_Uranus |date=4 January 2015 }} (photos)
* [http://www.solarviews.com/raw/uranus/urfamily.jpg Uranian system montage] (photo)
* {{cite web |last=Gray |first=Meghan |title=Uranus |url=http://www.sixtysymbols.com/videos/uranus.htm |work=Sixty Symbols |publisher=[[Brady Haran]] for the [[University of Nottingham]] |author2=Merrifield, Michael |date=2010}}
* [https://gravitysimulator.org/solar-system/uranus-and-its-rings-and-major-moons Interactive 3D gravity simulation of the Uranian system] {{Webarchive|url=https://web.archive.org/web/20200611221238/https://gravitysimulator.org/solar-system/the-uranian-system/ |date=11 June 2020 }}
* {{Citation | title=Uranus Rings photos |date=18 December 2023 |website=James Webb Space Telescope | publisher=NASA |url=https://webbtelescope.org/contents/news-releases/2023/news-2023-150 | access-date=19 December 2023}}

{{Uranus}}
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[[Category:Uranus| ]]
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[[Category:Discoveries by William Herschel]]
[[Category:Flamsteed objects|Tauri, 034]]
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