File:Uranus_Voyager2_color_calibrated.png · Wikimedia Commons · See Wikimedia Commons
Uranus
Sign in to saveAlso known as Sol VII, Georgium Sidus, Sol h, the Georgian Planet, Georgian Planet, the, 34 Tauri, Planet Uranus, Sol 7
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 phase of matter, which astronomy calls "ice" or volatiles. The planet's atmosphere has a complex layered cloud structure and has the lowest minimum temperature () of all the Solar System's planets. It has a marked axial tilt of 82.23° with a 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
Uranus is the seventh planet from the Sun and a gaseous ice giant with a cyan color, composed mainly of water, ammonia, and methane in a supercritical state, making it one of the coldest planets in our Solar System. It matters as a scientific subject because its extreme axial tilt of 82.23° and unusual rotation create distinctive seasonal patterns unlike any other planet, providing insights into planetary formation and the diversity of worlds in our Solar System.
AI-generated from the Wikipedia summary — may contain errors.
Key facts
- Planet.name
- Uranus
- Planet.symbol
- 24px|⛢|class=skin-invert, 24px|♅|class=skin-invert
- Planet.image
- Uranus Voyager2 color calibrated.png
- Planet.caption
- Uranus in true colour, as captured by Voyager 2 on January 24, 1986. Its pale, muted appearance is due to a shroud of haze above its clouds.
- Planet.background
- LightBlue
- Planet.discoverer
- [[]]
- Planet.epoch
- J2000
- Planet.time_periastron
- 17–19 August 2050
- Planet.synodic_period
- 369.66 days
- Planet.avg_speed
- 6.80 km/s
- Planet.satellites
- 29
- Planet.equatorial_radius
- 4.007 Earths
- Planet.polar_radius
- 3.929 Earths
- Planet.surface_area
- 15.91 Earths
- Planet.volume
- 63.086 Earths
- Planet.mass
- 14.536 Earths GM=
- Planet.moment_of_inertia_factor
- (estimate)
- Planet.escape_velocity
- 21.3 km/s
via Wikipedia infobox
Research
287 papers- Multiple Probe Measurements at Uranus Motivated by Spatial Variability.ReviewSpace science reviews · 2024Wong MH, Rowe-Gurney N, Markham S et al.DOI: 10.1007/s11214-024-01050-9
- Plasma Environment, Radiation, Structure, and Evolution of the Uranian System (PERSEUS): A Dedicated Orbiter Mission Concept to Study Space Physics at Uranus.ReviewSpace science reviews · 2023Cohen IJ, Smith EJ, Clark GB et al.DOI: 10.1007/s11214-023-01013-6
- We've misunderstood Uranus all these years.Nature · 2025DOI: 10.1038/d41586-025-01074-3
- Uranus should be NASA's top target, report finds.Science (New York, N.Y.) · 2022Voosen PDOI: 10.1126/science.abq6108
- Photochemical Haze Formation on Titan and Uranus: A Comparative Review.ReviewInternational journal of molecular sciences · 2025Dubois DDOI: 10.3390/ijms26157531
- The upper atmospheres of Uranus and Neptune.Philosophical transactions. Series A, Mathematical, physical, and engineering sciences · 2020Melin HDOI: 10.1098/rsta.2019.0478
- Auroral emissions from Uranus and Neptune.Philosophical transactions. Series A, Mathematical, physical, and engineering sciences · 2020Lamy LDOI: 10.1098/rsta.2019.0481
- Neptune and Uranus: ice or rock giants?Philosophical transactions. Series A, Mathematical, physical, and engineering sciences · 2020Teanby NA, Irwin PGJ, Moses JI et al.DOI: 10.1098/rsta.2019.0489
via PubMed
Wikidata facts
- Demonym
- Uranian
- Area
- 8115600000
- Distance from Earth
- 3150000000
- Diameter
- 51118
- Radius
- 24973
- Mass
- 86810
- Orbital period
- 30688.5
- Image
- Uranus Voyager2 color calibrated.png
Show 28 more facts
- Commons category
- Uranus (planet)
- time of discovery or invention
- 1781-03-13
- orbital eccentricity
- 0.04725744
- flattening
- 0.0229
- Commons gallery
- Uranus
- semi-major axis of an orbit
- 19.18916464
- orbital inclination
- 1.02
- argument of periapsis
- 170.95427630
- longitude of ascending node
- 74.01692503
- synodic period
- 369.66
- magnetic moment
- 3899999999999999773507584
- apoapsis
- 3006318143
- periapsis
- 2734998229
- catalog code
- 34 Tau
- surface gravity
- 8.7
- density
- 1.271
- mean anomaly
- 142.238
- volume as quantity
- 68330000000000
- right ascension
- 257.311
- declination
- -15.175
- apparent magnitude
- 5.32
- angular diameter
- 4.1
- temperature
- 57
- albedo
- 0.300
- Unicode character
- ♅
- Stack Exchange tag
- astronomy.stackexchange.com/tags/uranus
- IPA transcription
- ˈuːʁanʊs
- rotation period
- 17
Sources (14)
via Wikidata · CC0
~53 min read
Article
26 sectionsContents
- History
- {{anchor|34 Tauri}}<!-- Used by an incoming redirect --> Discovery
- Name
- Formation
- Orbit and rotation
- Axial tilt
- Visibility from Earth
- Internal structure
- Internal heat
- Atmosphere
- Composition
- Troposphere
- Upper atmosphere
- Climate
- Banded structure, winds and clouds
- Seasonal variation
- Magnetosphere
- Moons
- Rings
- Exploration
- In culture
- See also
- Notes
- References
- Further reading
- External links
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 phase of matter, which astronomy calls "ice" or volatiles. The planet's atmosphere has a complex layered cloud structure and has the lowest minimum temperature () of all the Solar System's planets. It has a marked axial tilt of 82.23° with a 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 layer is a rocky core, and a thick hydrogen and helium atmosphere surrounds it. Trace amounts of hydrocarbons (thought to be produced via hydrolysis) and carbon monoxide along with carbon dioxide (thought to have originated from comets) have been detected in the upper atmosphere. There are many unexplained climate phenomena in Uranus's atmosphere, such as its peak wind speed of , 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.
Gallery (52)
Available in 239 languages
- Español
- Français
- Deutsch
- 中文
- 日本語
- Русский
- Português
- Italiano
- العربية
- हिन्दी
- abstract
- Afrikaans
- Albanian
- Albanian
- Amharic
- Angika
- Aragonese
- Armenian
Show 220 more
- Arpitan
- Assamese
- Asturian
- Awadhi
- azb
- Azerbaijani
- Bahasa Indonesia
- Balinese
- Bangla
- Banjar
- Bashkir
- Basque
- bat_smg
- Bavarian
- be_x_old
- Belarusian
- Betawi
- Bhojpuri
- Bikol
- Bosnian
- Breton
- btm
- Bulgarian
- Buriat
- Burmese
- Catalan
- cdo
- Cebuano
- Central Kurdish
- Chechen
- Cherokee
- Church Slavic
- Chuvash
- Colognian
- Cornish
- Crimean Tatar
- Croatian
- Czech
- Danish
- dty
- Dzongkha
- Egyptian Arabic
- eml
- Esperanto
- Estonian
- Extremaduran
- Faroese
- Fiji Hindi
- Fijian
- Filipino
- Finnish
- fiu_vro
- Galician
- Gan Chinese
- gcr
- Georgian
- Gilaki
- Greek
- Guarani
- Gujarati
- guw
- Haitian Creole
- Hakka Chinese
- Hawaiian
- Hebrew
- Hungarian
- hyw
- Icelandic
- Ido
- Iloko
- Inari Sami
- Interlingua
- Interlingue
- Inuktitut
- Irish
- Jamaican Creole English
- Javanese
- Kannada
- Kanuri
- Kara-Kalpak
- Kashmiri
- Kashubian
- Kazakh
- kbp
- Khmer
- Komi
- Kongo
- Kurdish
- Kyrgyz
- Latin
- Latvian
- Lezghian
- Ligurian
- Limburgish
- Lingala
- Lingua Franca Nova
- Lithuanian
- lld
- Lojban
- Lombard
- Low German
- Luxembourgish
- Macedonian
- Madurese
- Maithili
- Malagasy
- Malay
- Malayalam
- Maltese
- Manipuri
- Manx
- Marathi
- Mazanderani
- Minangkabau
- Mingrelian
- Mirandese
- Moksha
- Mongolian
- Moroccan Arabic
- N’Ko
- nah
- Navajo
- nds_nl
- Neapolitan
- Nederlands
- Nepali
- Nigerian Pidgin
- Northern Frisian
- Northern Sami
- Norwegian
- Norwegian Nynorsk
- Novial
- Occitan
- Odia
- Old English
- olo
- Oromo
- Ossetic
- Pampanga
- Papiamento
- Pashto
- Picard
- Piedmontese
- Polski
- ppl
- Punjabi
- Quechua
- roa_rup
- Romanian
- Romansh
- Romany
- Rusyn
- Sanskrit
- Santali
- Sardinian
- Saterland Frisian
- Scots
- Scottish Gaelic
- Serbian
- Serbian (Latin)
- Shona
- Sicilian
- Silesian
- simple
- Sindhi
- Sinhala
- skr
- Slovak
- Slovenian
- Somali
- Southern Sotho
- Standard Moroccan Tamazight
- Sundanese
- Svenska
- Swahili
- Tachelhit
- Tajik
- Talysh
- Tamil
- Tatar
- Telugu
- Tibetan
- Tiếng Việt
- Tok Pisin
- Toki Pona
- Tumbuka
- Türkçe
- Turkmen
- Tuvinian
- Tyap
- Udmurt
- Ukrainian
- Urdu
- Uyghur
- Uzbek
- Venetian
- Veps
- Volapük
- Walloon
- Waray
- Welsh
- West Flemish
- Western Frisian
- Western Panjabi
- Wolof
- Wu Chinese
- Xhosa
- Yakut
- Yiddish
- Yoruba
- Zaza
- Zeelandic
- zh_classical
- zh_min_nan
- zh_yue
- Zhuang
- Zulu
- فارسی
- ไทย
- 한국어
via Wikidata sitelinks · CC0