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(Dagiti 34 nga agtengnga a rebision babaen dagiti 11 nga agar-aramat a saan a naipakita)
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{{Infobox planeta
{{Planetbox begin |
| bgcolour = #FFC8A0
nagan=Jupiter}} [[File:Jupiter symbol.ant.png|25px|Simbolo nga astronomia ti Jupiter]]
| name = Hupiter
{{Planetbox imahen |
imahen=[[File:Jupiter.jpg|250px]] |
| symbol = [[File:Jupiter symbol (bold).svg|24px|alt=♃|Astronomika a simbolo iti Hupiter]]
| image = [[File:Jupiter by Cassini-Huygens.jpg|frameless]]
capsion=Jupiter }}
| caption = Maysa a komposito [[Cassini–Huygens|Cassini]] nga imahen iti Hupiter. Ti nangisit a turik iti anniniwan ket ti [[Europa (bulan)|Europa]].
{{Planetbox orbit|
| orbit_ref =
epoca=J2000 |
<ref name=horizons>{{cite web
semimajor_axis=[[1 E11 m|778,412,027]] [[kilometre|km]]<br />5.203 363 01 [[Astronomical nga unit|AU]] |
|last = Yeomans|first = Donald K.|date = 2006-07-13
orbital_circumference=4.888 [[Tera|T]][[metre|m]]<br />32.675 AU |
|url = http://ssd.jpl.nasa.gov/?horizons
eccentricity=0.048 392 66 |
|title = HORIZONS System|publisher = NASA JPL
perihelion=740,742,598 km <br />4.951 558 43 AU |
|accessdate = 2007-08-08}} — At the site, go to the "web interface" then select "Ephemeris Type: Elements", "Target Body: Jupiter Barycenter" and "Center: Sun".</ref><ref name=barycenter>Orbital elements refer to the barycenter of the Jupiter system, and are the instantaneous [[osculating orbit|osculating]] values at the precise [[J2000]] epoch. Barycenter quantities are given because, in contrast to the planetary centre, they do not experience appreciable changes on a day-to-day basis from to the motion of the moons.</ref>
aphelion=816,081,455 km<br />5.455 167 59 AU |
| epoch = [[J2000]]
orbital period=[[1 E8 s|4333.2867 d]]<br />(11.86 [[tawen a julian (astronomia)|a]]) |
| aphelion = {{convert|816520800|km|AU|abbr=on}}
synod=-398.88 d |
| perihelion = {{convert|740573600|km|AU|abbr=on}}
avg os=13.056 km/s |
| semimajor = {{convert|778547200|km|AU|abbr=on}}
max os=13.712 km/s |
| eccentricity = 0.048775
min os=12.446 km/s |
inclination=1.305 30°<br />(6.09° agingga ti ecuador ti Init) |
| inclination = 1.305° aginggan ti [[Ecliptic]]<br />6.09° ti ekuador ti [[Init]]<br />0.32° ti [[Saan a nagbalbaliw a dalumpinas]]<ref name=meanplane>{{cite web
|date=2009-04-03
long=100.556 15° |
|title=Ti MeanPlane (Saan a nagbalbaliw a dalumpinas) iti Sistema Solar ng aagbalballasiw iti barisentro
arg=274.197 70° |
|url=http://home.surewest.net/kheider/astro/MeanPlane.gif
sat= 63 }}
|accessdate=2009-04-10
{{Planetbox fisica|
}} (naaramid ti [http://chemistry.unina.it/~alvitagl/solex/ Solex 10] {{Webarchive|url=https://web.archive.org/web/20150524145440/http://chemistry.unina.it/~alvitagl/solex/ |date=2015-05-24 }} insurat babaen ni Aldo Vitagliano; kitaen pay ti [[Saan a nagbalbaliw a dalumpinas]])</ref>
edi=[[1 E8 m|142,984 km]] [http://www.onasch.de/astro/showobject.php?lang=en&obj=p05]<br />(11.209 a [[Daga]]) |
| asc_node = 100.492°
pdi= 133,709 km<br />(10.517 a Daga) |
| arg_peri = 275.066°
surfacearea=[[1 E16 m²|6.14{{e|10}}]] [[square kilometre|km<sup>2</sup>]]<br />(120.5 a Daga)|
| mean_anomaly = 18.818°
obl= 0.064 87 |
| period = 4,332.59&nbsp;[[aldaw]]<br />11.8618&nbsp;[[hulian a tawen (astronomia)|tawen]]<br />10,475.8 Hupiter [[solar nga aldaw]]<ref name="planet_years">{{cite web|url = http://cseligman.com/text/sky/rotationvsday.htm|title = Panagtayyek a Panawen ken Kaatiddog ti Aldaw|last = Seligman |first = Courtney|accessdate = 2009-08-13}}</ref>
vol=1.431{{e|15}} [[cubic kilometro|km<sup>3</sup>]]<br />(1321.3 a Daga) |
| synodic_period = 398.88&nbsp;al-aldaw
mass=[[1 E27 kg|1.899{{e|27}}]] [[kilogram|kg]]<br />(317.8 a Daga) |
| avg_speed = 13.07&nbsp;km/s
avg dens=1.326 g/cm<sup>3</sup> |
| satellites = [[Dagiti kasisigud a satelite ti Hupiter|64]]
eq grav=23.12 [[Acceleration|m/s<sup>2</sup>]]<br />(2.358 [[gee]]) |
| physical_characteristics = yes
esc vel= 59.54 km/s |
| flattening = 0.06487 ± 0.00015 <!-- calculated from data in ref name="SeidelmannArchinalA'hearn_2007" -->
rp=0.413 538 021 d (9 h 55 min 29.685 s) [http://www.hnsky.org/iau-iag.htm <sup>1</sup>] |
| equatorial_radius = 71,492 ± 4&nbsp;km<ref name=1bar>Manggitudo ti agpang iti 1 bar nga atmosperiko a presion</ref> <br />11.209 [[Daga (planeta)|Daga]]
rv=12.6 km/s = 45,300 km/h <br />(manipud ti ecuador)|
| polar_radius = 66,854 ± 10&nbsp;km<ref name=1bar/> <br />10.517&nbsp;Ti Daga
axial tilt=3.13° |
| mean_radius = 69,911 ± 6&nbsp;km<<ref name=1bar/> <br />
north pole=268.05° (17 h 52 min 12 s)|
| surface_area = 6.1419×10<sup>10</sup>&nbsp;km<sup>2</sup><ref name=1bar/><ref name="nasafact">{{cite web |url=http://solarsystem.nasa.gov/planets/profile.cfm?Object=Jupiter&Display=Facts |title=Sistema a Solar Panagsukisok: Hupiter: Dagiti Kinapudno ken Bilang |work=NASA |date=7 Mayo 2008}}</ref><br />121.9 Ti Daga
dec=64.49° |
| volume = 1.4313×10<sup>15</sup>&nbsp;km<sup>3</sup><ref name=1bar/> <br />1321.3&nbsp;Ti daga
albedo=0.52 |
| mass = 1.8986×10<sup>27</sup>&nbsp;kg<br />317.8&nbsp;Ti Daga<br />1/1047 Init<ref name=ssd-constants>{{cite web
mintemp=110 [[kelvin|K]] |
|title=Astrodynamic a Taginayon
meantemp=[[1 E2 K|152 K]] |
|publisher=JPL a Dinamiko a Sistema a Solar
maxtemp=N/A K }}
|date=2009-02-27
{{Planetbox atmosphere Jupiter|
|url=http://ssd.jpl.nasa.gov/?taginayon
kemika1=[[Atmospheric pressure]] |
|accessdate = 2007-08-08}}</ref>
value1=70 [[Pascal|kPa]] |
| density = 1.326&nbsp;g/cm<sup>3</sup><ref name=1bar/>
kemika2=[[Hydrogen]] |
| surface_grav = 24.79&nbsp;[[Panagpardasan|m/s<sup>2</sup>]]<ref name=1bar/><br />2.528&nbsp;[[g-force|g]]
value2=~86% |
| escape_velocity = 59.5&nbsp;km/s<ref name=1bar/>
kemika3=[[Helium]] |
| sidereal_day = 9.925&nbsp;h<ref>{{cite web|author = Seidelmann, P. K.|author2 = Abalakin, V. K.|author3 = Bursa, M.|author4 = Davies, M. E.|author5 = de Burgh, C.|author6 = Lieske, J. H.|author7 = Oberst, J.|author8 = Simon, J. L.|author9 = Standish, E. M.|author10 = Stooke, P.|author11 = Thomas, P. C.|year = 2001|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|publisher = HNSKY Planetarium Program|accessdate = 2007-02-02|archive-date = 2019-05-14|archive-url = https://web.archive.org/web/20190514222418/http://www.hnsky.org/iau-iag.htm|url-status = dead}}</ref> (9 h 55 m 30 s)
value3=~14% |
| rot_velocity = 12.6&nbsp;km/s<br />45,300&nbsp;km/h
kemika4=[[Methane]] |
| axial_tilt = 3.13°
value4=0.1% |
| right_asc_north_pole = 268.057°<br />17&nbsp;h 52&nbsp;min 14&nbsp;
kemika5=[[Water]] vapor |
| declination = 64.496°
value5=0.1%] |
| albedo = 0.343 ([[Piansa nga albedo|Piansa]])<br />
kemika6=[[Ammonia]]|
0.52 ([[Geometric albedo|geom.]])
value6=0.02% |
| magnitude = -1.6 to -2.94
kemika7=[[Ethane]] |
| angular_size = 29.8" — 50.1"
value7=0.0002% |
| pronounce =
kemika8=[[Phosphine]] |
| adjectives = Jovian
value8=0.0001% |
| temperatures = yes
kemika9=[[Hydrogen sulfide]]|
| temp_name1 = 1 bar level
value9=&lt;0.00010% }}
| min_temp_1 =
{{Planetbox end}}
| mean_temp_1 = 165&nbsp;[[Kelvin|K]]
Ti '''Jupiter''' ti maikalima a [[planeta]] manipud iti [[Init]] ket isu ti kadakkelan iti ikub ti [[Sistema a Solar]].
| max_temp_1 =
| temp_name2 = 0.1 bar
| min_temp_2 =
| mean_temp_2 = 112&nbsp;K
| max_temp =
| atmosphere = yes
| atmosphere_ref =
| surface_pressure = 20–200&nbsp;[[Pascal (paset)|kPa]]<ref>{{cite journal
|author=Anonymous|title=Probe Nephelometer
|journal=Galileo Messenger|publisher=NASA/JPL
|date=Marso 1983|issue=6
|url=http://www2.jpl.nasa.gov/galileo/messenger/oldmess/2Probe.html
|accessdate = 2007-02-12}}</ref> (ulep a&nbsp;rutap)
| scale_height = 27&nbsp;km
| atmosphere_composition =
<table>
<tr><td>
89.8±2.0%</td><td>[[hidróheno]] (H<sub>2</sub>)
</td></tr><tr><td>
10.2±2.0%</td><td>[[helio]]
</td></tr><tr><td>
~0.3%</td><td>[[metano]]
</td></tr><tr><td>
~0.026%</td><td>[[amoníako]]
</td></tr><tr><td>
~0.003%</td><td>[[hidróheno deuteride]] (HD)
</td></tr><tr><td>
0.0006%</td><td>[[etano]]
</td></tr><tr><td>
0.0004%</td><td>[[danum]]
</td></tr><tr><td>
'''Ices''':</td><td>
</td></tr><tr><td>
</td><td>[[amoníako]]
</td></tr><tr><td>
</td><td>[[danum]]
</td></tr><tr><td>
</td><td>[[ammonio hydrosulpuro]](NH<sub>4</sub>SH)
</td></tr></table>
}}
Ti '''Hupiter''' ti maikalima a [[planeta]] manipud iti [[Init]] ket isu ti kadakkelan iti ikub ti [[Sistema a Solar]].


== Pakasaritaan ==
== Pakasaritaan ==


Ti Jupiter ket masirmataan iti nalawag a rabii. Isu ti maikapat a kasellagan a gandat a masurot iti [[Init]], [[Bulan]], ken iti [[Venus]]. Impanagan dagiti [[Romano]] iti diosenda a ni [[Jupiter (dios)|Jupiter]] ket ti [[simbolo astronomico]na ket maysa a ladawan ti kimat a simbolo ni diosen a Jupiter.
Ti Hupiter ket masirmataan iti nalawag a rabii. Isu ti maikapat a kasellagan a gandat a masurot iti [[Init]], [[Bulan]], ken iti [[Venus]]. Impanagan dagiti [[Taga-ugma a Roma|Romano]] iti diosenda a ni [[Hupiter (dios)|Hupiter]] ket ti [[simbolo nga astronomiko]] na ket maysa a ladawan ti kimat a simbolo ti diosen a Hupiter.


== [[Bulbulan iti Jupiter]] ==
==Bulbulan ==


[[Bulbulan iti Jupiter|Bulbulan ti Hupiter]]
[[File:Jupiter.moons2.jpg|thumb|left|300px|Dagiti uppat nga kadakkelan a bulan ti Jupiter: manipud ti ngato: [[Callisto (bulan)|Callisto]], [[Ganymede (bulan)|Ganymede]], [[Europa (bulan)|Europa]] ken [[Io (bulan)|Io]].]]


Addaan 63 a [[Bulan (astronomia)|bulan]] ti Jupiter. Dagiti uppat a kadakkelan--ti [[Callisto (bulan)|Callisto]], [[Ganymede (bulan)|Ganymede]], [[Europa (bulan)|Europa]] ken [[Io (bulan)|Io]]-- ket matawagan no dadduma a "bulbulan ni [[Galileo Galilei|Galileo]]."
[[Papeles:Jupiter.moons2.jpg|thumb|left|Dagiti uppat nga kadakkelan a bulan ti Hupiter: manipud ti ngato: [[Callisto (bulan)|Callisto]], [[Ganymede (bulan)|Ganymede]], [[Europa (bulan)|Europa]] ken [[Io (bulan)|Io]].]]


Addaan ti 63 a [[Bulan (astronomia)|bulan]] ti Hupiter. Dagiti uppat a kadakkelan ti [[Callisto (bulan)|Callisto]], [[Ganymede (bulan)|Ganymede]], [[Europa (bulan)|Europa]] ken [[Io (bulan)|Io]] ket matawagan no dadduma a "bulbulan ni [[Galileo Galilei|Galileo]]."
{{clearleft}}
=== Bulbulan ni Galileo ===
=== Bulbulan ni Galileo ===

==Dagiti nagibasaran==
{{Reflist}}
{{pungol-nangruna}}

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==Overview==
==Overview==


[[Image:Jupiter-Earth-Spot_comparison.jpg|thumb|left|200px|Approximate size comparison of Earth, Jupiter, and the Great Red Spot]]
[[Image:Jupiter-Earth-Spot_comparison.jpg|thumb|left|Approximate size comparison of Earth, Jupiter, and the Great Red Spot]]


Jupiter is 2.5 times more [[mass]]ive than all the other planets combined, so massive that its [[Center of mass#Barycenter|barycenter]] with the Sun actually lies above the Sun's surface (1.068 [[solar radius|solar radii]] from the Sun's center). It is 318 times more massive than [[Earth]], with a [[diameter]] 11 times that of Earth, and a [[volume]] 1300 times that of [[Earth]]. Quite naturally, Jupiter's [[gravity|gravitational]] influence has dominated the evolution of the solar system: most planets' orbits lie closer to Jupiter's [[orbital plane (astronomy)|orbital plane]] than the Sun's [[celestial sphere|equatorial plane]] ([[Mercury (planet)|Mercury]] is the only planet which is closer to the Sun's equator in orbital tilt), the majority of [[short-period comet]]s belong to Jupiter's family (a result due to both Jupiter's mass and its relative speed), the [[Kirkwood gap]]s in the [[asteroid belt]] are mostly due to Jupiter, and Jupiter is even thought to have been possibly responsible for the [[late heavy bombardment]] of the inner solar system's history. Some have described the solar system as consisting of the Sun, Jupiter, and assorted debris.<ref name="clarke2061">{{cite book|author=Clarke, Arthur C.|year=1989|title=2061: Odyssey Three|publisher=Del Rey|id=ISBN 0-345-35879-1}}</ref> Some describe Jupiter as the solar system's vacuum cleaner, due to its immense [[gravity well]].
Jupiter is 2.5 times more [[mass]]ive than all the other planets combined, so massive that its [[Center of mass#Barycenter|barycenter]] with the Sun actually lies above the Sun's surface (1.068 [[solar radius|solar radii]] from the Sun's center). It is 318 times more massive than [[Earth]], with a [[diameter]] 11 times that of Earth, and a [[volume]] 1300 times that of [[Earth]]. Quite naturally, Jupiter's [[gravity|gravitational]] influence has dominated the evolution of the solar system: most planets' orbits lie closer to Jupiter's [[orbital plane (astronomy)|orbital plane]] than the Sun's [[celestial sphere|equatorial plane]] ([[Mercury (planet)|Mercury]] is the only planet which is closer to the Sun's equator in orbital tilt), the majority of [[short-period comet]]s belong to Jupiter's family (a result due to both Jupiter's mass and its relative speed), the [[Kirkwood gap]]s in the [[asteroid belt]] are mostly due to Jupiter, and Jupiter is even thought to have been possibly responsible for the [[late heavy bombardment]] of the inner solar system's history. Some have described the solar system as consisting of the Sun, Jupiter, and assorted debris.<ref name="clarke2061">{{cite book|author=Clarke, Arthur C.|year=1989|title=2061: Odyssey Three|publisher=Del Rey|isbn= 0-345-35879-1}}</ref> Some describe Jupiter as the solar system's vacuum cleaner, due to its immense [[gravity well]].


As impressive as Jupiter's mass is, [[extrasolar planet]]s have been discovered with much greater masses. There is no clear-cut definition of what distinguishes a large planet such as Jupiter from a [[brown dwarf]], although the latter possesses rather specific [[spectral line]]s. Currently, if an object is above 12 Jupiter masses, large enough to burn [[deuterium]], it is considered a brown dwarf; below that mass, it is a planet. Jupiter is thought to have about as large a diameter as a planet of its composition can; adding extra mass would result in further gravitational compression, in theory leading to stellar ignition. This has led some astronomers to term it a "failed star" -- although Jupiter would need to be about seventy-five times as large to become a star, the smallest red dwarf is only about 30% larger than Jupiter. In light of this, it is also interesting to note that it radiates more heat than it receives from the Sun. This additional heat radiation is produced by the [[Kelvin-Helmholtz mechanism]]. As another symptom of this process, the planet shrinks at the rate of a few millimeters each year. When it was younger and hotter, Jupiter was much larger than it is today, though previously [[Saturn]] would have been even bigger than Jupiter due to its lower mass: Saturn has a much weaker gravitational pull and with more heat, both planets would have been more bloated (and because of Saturn's lower core mass, it would have been more bloated). In general, the more massive the core, the smaller the planet in size.
As impressive as Jupiter's mass is, [[extrasolar planet]]s have been discovered with much greater masses. There is no clear-cut definition of what distinguishes a large planet such as Jupiter from a [[brown dwarf]], although the latter possesses rather specific [[spectral line]]s. Currently, if an object is above 12 Jupiter masses, large enough to burn [[deuterium]], it is considered a brown dwarf; below that mass, it is a planet. Jupiter is thought to have about as large a diameter as a planet of its composition can; adding extra mass would result in further gravitational compression, in theory leading to stellar ignition. This has led some astronomers to term it a "failed star" -- although Jupiter would need to be about seventy-five times as large to become a star, the smallest red dwarf is only about 30% larger than Jupiter. In light of this, it is also interesting to note that it radiates more heat than it receives from the Sun. This additional heat radiation is produced by the [[Kelvin-Helmholtz mechanism]]. As another symptom of this process, the planet shrinks at the rate of a few millimeters each year. When it was younger and hotter, Jupiter was much larger than it is today, though previously [[Saturn]] would have been even bigger than Jupiter due to its lower mass: Saturn has a much weaker gravitational pull and with more heat, both planets would have been more bloated (and because of Saturn's lower core mass, it would have been more bloated). In general, the more massive the core, the smaller the planet in size.
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[[Category:Astronomia]]
[[Category:Pangted]]

{{Link FA|en}}
{{Link FA|es}}
{{Link FA|fr}}
{{Link FA|sl}}


[[Kategoria:Hupiter]]
[[af:Jupiter (planeet)]]
[[als:Jupiter (Planet)]]
[[am:ጁፒተር]]
[[an:Chupiter (planeta)]]
[[ang:Þunor (dweligend)]]
[[ar:المشتري]]
[[arz:جوبيتر]]
[[as:বৃহস্পতি গ্ৰহ]]
[[ast:Xúpiter (planeta)]]
[[az:Yupiter (planet)]]
[[ba:Юпитер (планета)]]
[[bar:Jupiter (Planet)]]
[[bat-smg:Jopėteris (planeta)]]
[[be:Планета Юпітэр]]
[[be-x-old:Юпітэр (плянэта)]]
[[bg:Юпитер (планета)]]
[[bn:জুপিটার]]
[[br:Yaou (planedenn)]]
[[bs:Jupiter]]
[[ca:Júpiter (planeta)]]
[[chr:ᏧᏈᏓ]]
[[cs:Jupiter (planeta)]]
[[csb:Jupiter]]
[[cv:Юпитер (планета)]]
[[cy:Iau (planed)]]
[[da:Jupiter (planet)]]
[[de:Jupiter (Planet)]]
[[el:Δίας (πλανήτης)]]
[[eml:Zòbia]]
[[en:Jupiter]]
[[eo:Jupitero (planedo)]]
[[es:Júpiter (planeta)]]
[[et:Jupiter]]
[[eu:Jupiter (planeta)]]
[[ext:Júpiti (praneta)]]
[[fa:مشتری (سیاره)]]
[[fi:Jupiter]]
[[fiu-vro:Jupitõr (hod'otäht)]]
[[fo:Jupiter]]
[[fr:Jupiter (planète)]]
[[frp:Jupitèr (planèta)]]
[[frr:Jupiter]]
[[fy:Jupiter]]
[[ga:Iúpatar (pláinéad)]]
[[gan:木星]]
[[gd:Am Bliogh]]
[[gl:Xúpiter]]
[[gu:ગુરુ (ગ્રહ)]]
[[gv:Jupiter]]
[[haw:Ka‘āwela]]
[[he:צדק (כוכב לכת)]]
[[hi:बृहस्पति]]
[[hif:Brahaspati]]
[[hr:Jupiter (planet)]]
[[ht:Jipitè (planèt)]]
[[hu:Jupiter]]
[[hy:Յուպիտեր]]
[[ia:Jupiter (planeta)]]
[[id:Yupiter]]
[[io:Jupitero]]
[[is:Júpíter (reikistjarna)]]
[[it:Giove (astronomia)]]
[[ja:木星]]
[[jbo:iupiter]]
[[jv:Yupiter]]
[[ka:იუპიტერი (პლანეტა)]]
[[kaa:Yupiter (planeta)]]
[[kk:Юпитер]]
[[km:ភពព្រហស្បតិ៍]]
[[kn:ಗುರು (ಗ್ರಹ)]]
[[ko:목성]]
[[ksh:Juppitter (Planneet)]]
[[ku:Berçîs]]
[[kv:Юпитер]]
[[kw:Yow (planet)]]
[[ky:Юпитер]]
[[la:Iuppiter (planeta)]]
[[lb:Jupiter (Planéit)]]
[[li:Jupiter (planeet)]]
[[lij:Giòve (astronomia)]]
[[lt:Jupiteris (planeta)]]
[[lv:Jupiters (planēta)]]
[[mdf:Юпитерь (шары тяште)]]
[[mk:Јупитер]]
[[ml:വ്യാഴം]]
[[mn:Бархасбадь]]
[[mr:गुरू ग्रह]]
[[ms:Musytari]]
[[mt:Ġove (pjaneta)]]
[[mwl:Júpiter (planeta)]]
[[my:ကြာသပတေးဂြိုဟ်]]
[[nah:Huēyitzitzimicītlalli]]
[[nds:Jupiter (Planet)]]
[[ne:बृहस्पतिग्रह]]
[[nl:Jupiter (planeet)]]
[[nn:Planeten Jupiter]]
[[no:Jupiter]]
[[nov:Jupitere (planete)]]
[[nv:Jíbitoo]]
[[oc:Jupitèr (planeta)]]
[[or:ବୃହସ୍ପତି]]
[[os:Юпитер (планетæ)]]
[[pa:ਬ੍ਰਹਿਸਪਤ]]
[[pam:Jupiter]]
[[pl:Jowisz]]
[[pms:Gieuv (pianeta)]]
[[pnb:مشتری]]
[[ps:مشتري]]
[[pt:Júpiter (planeta)]]
[[qu:Pirwa]]
[[rm:Jupiter (planet)]]
[[ro:Jupiter]]
[[ru:Юпитер]]
[[rue:Юпітер (планета)]]
[[sah:Юпитер]]
[[scn:Giovi (pianeta)]]
[[sd:وِسپَتُ]]
[[se:Jupiter]]
[[sh:Jupiter (planeta)]]
[[si:බ්‍රහස්පති ග්‍රහයා]]
[[simple:Jupiter]]
[[sk:Jupiter]]
[[sl:Jupiter]]
[[so:Cirjeex]]
[[sq:Jupiteri]]
[[sr:Јупитер]]
[[stq:Jupiter]]
[[su:Jupiter]]
[[sv:Jupiter]]
[[sw:Mshtarii]]
[[szl:Jowisz]]
[[ta:வியாழன் (கோள்)]]
[[te:గురుడు]]
[[tg:Муштарӣ]]
[[th:ดาวพฤหัสบดี]]
[[tl:Hupiter (planeta)]]
[[tr:Jüpiter]]
[[tt:Юпитер (планета)]]
[[ug:يۇپىتېر]]
[[uk:Юпітер (планета)]]
[[ur:مشتری]]
[[uz:Yupiter]]
[[vi:Sao Mộc]]
[[war:Hupiter]]
[[wo:Yupiter]]
[[xal:Пүрвə һариг]]
[[yi:יופיטער]]
[[yo:Júpítérì]]
[[za:Ndaundeiqfaex]]
[[zh:木星]]
[[zh-classical:木星]]
[[zh-min-nan:Bo̍k-chheⁿ]]
[[zh-yue:木星]]

Kinaudi a rebision manipud idi 13:04, 31 Enero 2024

Hupiter ♃
Maysa a komposito Cassini nga imahen iti Hupiter. Ti nangisit a turik iti anniniwan ket ti Europa.
Dagiti panangikeddeng
Dagiti pangilasinJovian
Dagiti pakailasinan ti panaglikmut[3][4]
Panawen J2000
Aphelion816,520,800 km (5.458104 AU)
Perihelion740,573,600 km (4.950429 AU)
778,547,200 km (5.204267 AU)
Eksentrisidad0.048775
4,332.59 aldaw
11.8618 tawen
10,475.8 Hupiter solar nga aldaw[1]
398.88 al-aldaw
13.07 km/s
18.818°
Paglikigan1.305° aginggan ti Ecliptic
6.09° ti ekuador ti Init
0.32° ti Saan a nagbalbaliw a dalumpinas[2]
100.492°
275.066°
Dagiti ammo a satelite64
Dagiti pisikal a pakailasinan
Promedio a rayus
69,911 ± 6 km<[5]
Rayus ti ekuador
71,492 ± 4 km[5]
11.209 Daga
Rayus ti polar
66,854 ± 10 km[5]
10.517 Ti Daga
Panagdalumpinas0.06487 ± 0.00015
6.1419×1010 km2[5][6]
121.9 Ti Daga
Tomo1.4313×1015 km3[5]
1321.3 Ti daga
Masa1.8986×1027 kg
317.8 Ti Daga
1/1047 Init[7]
Promedio a densidad
1.326 g/cm3[5]
24.79 m/s2[5]
2.528 g
59.5 km/s[5]
9.925 h[8] (9 h 55 m 30 s)
Kapardas ti panagtayyek ti ekuador
12.6 km/s
45,300 km/h
3.13°
Panagpangato ti kanawan ti amianan nga ungto
268.057°
17 h 52 min 14 
Deklinasion ti amianan nga ungto
64.496°
Albedo0.343 (Piansa)
0.52 (geom.)
temp. ti rabaw min mean max
1 bar level 165 K
0.1 bar 112 K
-1.6 to -2.94
29.8" — 50.1"
Atmospeara
Presion ti rabaw
20–200 kPa[9] (ulep a rutap)
27 km
Pakabuklan babaen ti tomo
89.8±2.0%hidróheno (H2)
10.2±2.0%helio
~0.3%metano
~0.026%amoníako
~0.003%hidróheno deuteride (HD)
0.0006%etano
0.0004%danum
Ices:
amoníako
danum
ammonio hydrosulpuro(NH4SH)

Ti Hupiter ti maikalima a planeta manipud iti Init ket isu ti kadakkelan iti ikub ti Sistema a Solar.

Pakasaritaan[urnosen | urnosen ti taudan]

Ti Hupiter ket masirmataan iti nalawag a rabii. Isu ti maikapat a kasellagan a gandat a masurot iti Init, Bulan, ken iti Venus. Impanagan dagiti Romano iti diosenda a ni Hupiter ket ti simbolo nga astronomiko na ket maysa a ladawan ti kimat a simbolo ti diosen a Hupiter.

Bulbulan[urnosen | urnosen ti taudan]

Bulbulan ti Hupiter

Dagiti uppat nga kadakkelan a bulan ti Hupiter: manipud ti ngato: Callisto, Ganymede, Europa ken Io.

Addaan ti 63 a bulan ti Hupiter. Dagiti uppat a kadakkelan ti Callisto, Ganymede, Europa ken Io ket matawagan no dadduma a "bulbulan ni Galileo."

Bulbulan ni Galileo[urnosen | urnosen ti taudan]

Dagiti nagibasaran[urnosen | urnosen ti taudan]

  1. ^ Seligman, Courtney. "Panagtayyek a Panawen ken Kaatiddog ti Aldaw". Naala idi 2009-08-13.
  2. ^ "Ti MeanPlane (Saan a nagbalbaliw a dalumpinas) iti Sistema Solar ng aagbalballasiw iti barisentro". 2009-04-03. Naala idi 2009-04-10. (naaramid ti Solex 10 Naiyarkibo 2015-05-24 iti Wayback Machine insurat babaen ni Aldo Vitagliano; kitaen pay ti Saan a nagbalbaliw a dalumpinas)
  3. ^ Yeomans, Donald K. (2006-07-13). "HORIZONS System". NASA JPL. Naala idi 2007-08-08. — At the site, go to the "web interface" then select "Ephemeris Type: Elements", "Target Body: Jupiter Barycenter" and "Center: Sun".
  4. ^ Orbital elements refer to the barycenter of the Jupiter system, and are the instantaneous osculating values at the precise J2000 epoch. Barycenter quantities are given because, in contrast to the planetary centre, they do not experience appreciable changes on a day-to-day basis from to the motion of the moons.
  5. ^ a b c d e f g h Manggitudo ti agpang iti 1 bar nga atmosperiko a presion
  6. ^ "Sistema a Solar Panagsukisok: Hupiter: Dagiti Kinapudno ken Bilang". NASA. 7 Mayo 2008.
  7. ^ "Astrodynamic a Taginayon". JPL a Dinamiko a Sistema a Solar. 2009-02-27. Naala idi 2007-08-08.
  8. ^ Seidelmann, P. K.; Abalakin, V. K.; Bursa, M.; Davies, M. E.; de Burgh, C.; Lieske, J. H.; Oberst, J.; Simon, J. L.; Standish, E. M.; Stooke, P.; Thomas, P. C. (2001). "Report of the IAU/IAG Working Group on Cartographic Coordinates and Rotational Elements of the Planets and Satellites: 2000". HNSKY Planetarium Program. Naiyarkibo manipud iti kasisigud idi 2019-05-14. Naala idi 2007-02-02.
  9. ^ Anonymous (Marso 1983). "Probe Nephelometer". Galileo Messenger. NASA/JPL (6). Naala idi 2007-02-12.
Simbolo ti pungol

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