Hupiter: Paggiddiatan a nagbaetan dagiti rebision
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ZéroBot (tungtungan | aramid) m r2.7.1) (Robot: Agnaynayon ckb:هەسارەی موشتەری |
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| (Dagiti 21 nga agtengnga a rebision babaen dagiti 9 nga agar-aramat a saan a naipakita) | |||
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| bgcolour = #FFC8A0 |
| bgcolour = #FFC8A0 |
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| name = Hupiter |
| name = Hupiter |
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| symbol = [[File:Jupiter symbol.svg| |
| symbol = [[File:Jupiter symbol (bold).svg|24px|alt=♃|Astronomika a simbolo iti Hupiter]] |
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| image = [[File:Jupiter by Cassini-Huygens.jpg| |
| image = [[File:Jupiter by Cassini-Huygens.jpg|frameless]] |
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| caption = Maysa a komposito [[Cassini–Huygens|Cassini]] nga imahen iti Hupiter. Ti nangisit a turik iti anniniwan ket ti [[Europa (bulan)|Europa]]. |
| caption = Maysa a komposito [[Cassini–Huygens|Cassini]] nga imahen iti Hupiter. Ti nangisit a turik iti anniniwan ket ti [[Europa (bulan)|Europa]]. |
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| orbit_ref = |
| orbit_ref = |
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| Linia 20: | Linia 20: | ||
|title=Ti MeanPlane (Saan a nagbalbaliw a dalumpinas) iti Sistema Solar ng aagbalballasiw iti barisentro |
|title=Ti MeanPlane (Saan a nagbalbaliw a dalumpinas) iti Sistema Solar ng aagbalballasiw iti barisentro |
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|url=http://home.surewest.net/kheider/astro/MeanPlane.gif |
|url=http://home.surewest.net/kheider/astro/MeanPlane.gif |
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|accessdate=2009-04-10 |
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|accessdate=2009-04-10}} (naaramid ti [http://chemistry.unina.it/~alvitagl/solex/ Solex 10] insurat babaen ni Aldo Vitagliano; kitaen pay ti [[Saan a nagbalbaliw a dalumpinas]])</ref> |
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}} (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> |
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| asc_node = 100.492° |
| asc_node = 100.492° |
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| arg_peri = 275.066° |
| arg_peri = 275.066° |
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| Linia 44: | Linia 45: | ||
| surface_grav = 24.79 [[Panagpardasan|m/s<sup>2</sup>]]<ref name=1bar/><br />2.528 [[g-force|g]] |
| surface_grav = 24.79 [[Panagpardasan|m/s<sup>2</sup>]]<ref name=1bar/><br />2.528 [[g-force|g]] |
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| escape_velocity = 59.5 km/s<ref name=1bar/> |
| escape_velocity = 59.5 km/s<ref name=1bar/> |
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| sidereal_day = 9.925 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) |
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| sidereal_day = 9.925 h<ref>{{cite web |
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|author = 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. |
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|year = 2001|url = http://www.hnsky.org/iau-iag.htm |
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|title = Report of the IAU/IAG Working Group on Cartographic Coordinates and Rotational Elements of the Planets and Satellites: 2000 |
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|publisher = HNSKY Planetarium Program |
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|accessdate = 2007-02-02}}</ref> (9 h 55 m 30 s) |
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| rot_velocity = 12.6 km/s<br />45,300 km/h |
| rot_velocity = 12.6 km/s<br />45,300 km/h |
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| axial_tilt = 3.13° |
| axial_tilt = 3.13° |
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| Linia 58: | Linia 54: | ||
| magnitude = -1.6 to -2.94 |
| magnitude = -1.6 to -2.94 |
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| angular_size = 29.8" — 50.1" |
| angular_size = 29.8" — 50.1" |
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| pronounce = |
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| pronounce = {{IPAc-en|audio=en-us-Jupiter.ogg|ˈ|dʒ|uː|p|ɪ-|t|ər}}<ref>Jupiter, entry in the Oxford English Dictionary, prepared by J. A. Simpson and E. S. C. Weiner, vol. 8, second edition, Oxford: Clarendon Press, 1989. ISBN 0-19-861220-6 (vol. 8), ISBN 0-19-861186-2 (set.)</ref> |
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| adjectives = Jovian |
| adjectives = Jovian |
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| temperatures = yes |
| temperatures = yes |
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|author=Anonymous|title=Probe Nephelometer |
|author=Anonymous|title=Probe Nephelometer |
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|journal=Galileo Messenger|publisher=NASA/JPL |
|journal=Galileo Messenger|publisher=NASA/JPL |
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| |
|date=Marso 1983|issue=6 |
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|url=http://www2.jpl.nasa.gov/galileo/messenger/oldmess/2Probe.html |
|url=http://www2.jpl.nasa.gov/galileo/messenger/oldmess/2Probe.html |
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|accessdate = 2007-02-12}}</ref> (ulep a rutap) |
|accessdate = 2007-02-12}}</ref> (ulep a rutap) |
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== Pakasaritaan == |
== Pakasaritaan == |
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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 (dios)|Hupiter]] ket ti [[simbolo nga astronomiko]] na ket maysa a ladawan ti kimat a simbolo ti diosen a Hupiter. |
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. |
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==Bulbulan == |
==Bulbulan == |
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[[Bulbulan iti Jupiter|Bulbulan ti Hupiter]] |
[[Bulbulan iti Jupiter|Bulbulan ti Hupiter]] |
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[[ |
[[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]].]] |
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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]]." |
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]]." |
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=== Bulbulan ni Galileo === |
=== Bulbulan ni Galileo === |
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==Dagiti nagibasaran== |
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==Pinagibasaran== |
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{{Reflist |
{{Reflist}} |
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==Overview== |
==Overview== |
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[[Image:Jupiter-Earth-Spot_comparison.jpg|thumb|left |
[[Image:Jupiter-Earth-Spot_comparison.jpg|thumb|left|Approximate size comparison of Earth, Jupiter, and the Great Red Spot]] |
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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| |
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]]. |
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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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{{Sistema Solar}} |
{{Sistema Solar}} |
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[[ |
[[Kategoria:Hupiter]] |
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{{Link FA|en}} |
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{{Link FA|es}} |
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{{Link FA|fr}} |
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{{Link FA|sl}} |
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[[af:Jupiter (planeet)]] |
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[[als:Jupiter (Planet)]] |
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[[am:ጁፒተር]] |
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[[an:Chupiter (planeta)]] |
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[[ang:Þunor (dweligend)]] |
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[[ar:المشتري]] |
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[[arz:المشترى]] |
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[[as:বৃহস্পতি গ্ৰহ]] |
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[[ast:Xúpiter (planeta)]] |
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[[az:Yupiter (planet)]] |
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[[ba:Юпитер (планета)]] |
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[[bar:Jupiter (Planet)]] |
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[[bat-smg:Jopėteris (planeta)]] |
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[[be:Планета Юпітэр]] |
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[[be-x-old:Юпітэр (плянэта)]] |
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[[bg:Юпитер (планета)]] |
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[[bn:বৃহস্পতি গ্রহ]] |
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[[bo:ཕུར་བུ།]] |
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[[br:Yaou (planedenn)]] |
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[[bs:Jupiter]] |
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[[ca:Júpiter (planeta)]] |
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[[chr:ᏧᏈᏓ]] |
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[[ckb:هەسارەی موشتەری]] |
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[[cs:Jupiter (planeta)]] |
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[[csb:Jupiter]] |
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[[cv:Юпитер (планета)]] |
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[[cy:Iau (planed)]] |
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[[da:Jupiter (planet)]] |
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[[de:Jupiter (Planet)]] |
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[[diq:Jupiter]] |
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[[el:Δίας (πλανήτης)]] |
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[[eml:Zòbia]] |
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[[en:Jupiter]] |
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[[eo:Jupitero (planedo)]] |
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[[es:Júpiter (planeta)]] |
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[[et:Jupiter]] |
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[[eu:Jupiter (planeta)]] |
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[[ext:Júpiti (praneta)]] |
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[[fa:مشتری (سیاره)]] |
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[[fi:Jupiter]] |
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[[fiu-vro:Jupitõr (hod'otäht)]] |
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[[fo:Jupiter]] |
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[[fr:Jupiter (planète)]] |
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[[frp:Jupitèr (planèta)]] |
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[[frr:Jupiter]] |
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[[fy:Jupiter]] |
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[[ga:Iúpatar (pláinéad)]] |
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[[gan:木星]] |
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[[gd:Am Bliogh]] |
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[[gl:Xúpiter]] |
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[[gn:Húpiter]] |
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[[gu:ગુરુ (ગ્રહ)]] |
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[[gv:Jupiter]] |
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[[haw:Ka‘āwela]] |
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[[he:צדק (כוכב לכת)]] |
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[[hi:बृहस्पति]] |
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[[hif:Brahaspati]] |
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[[hr:Jupiter (planet)]] |
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[[ht:Jipitè (planèt)]] |
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[[hu:Jupiter]] |
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[[hy:Յուպիտեր (մոլորակ)]] |
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[[ia:Jupiter (planeta)]] |
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[[id:Yupiter]] |
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[[io:Jupitero]] |
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[[is:Júpíter (reikistjarna)]] |
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[[it:Giove (astronomia)]] |
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[[ja:木星]] |
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[[jbo:iupiter]] |
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[[jv:Yupiter]] |
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[[ka:იუპიტერი (პლანეტა)]] |
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[[kaa:Yupiter (planeta)]] |
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[[kk:Юпитер]] |
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[[km:ភពព្រហស្បតិ៍]] |
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[[kn:ಗುರು (ಗ್ರಹ)]] |
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[[ko:목성]] |
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[[ksh:Juppitter (Planneet)]] |
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[[ku:Berçîs]] |
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[[kv:Юпитер]] |
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[[kw:Yow (planet)]] |
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[[ky:Юпитер]] |
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[[la:Iuppiter (planeta)]] |
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[[lb:Jupiter (Planéit)]] |
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[[lez:Юпитер]] |
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[[li:Jupiter (planeet)]] |
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[[lij:Giòve (astronomia)]] |
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[[lt:Jupiteris (planeta)]] |
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[[lv:Jupiters (planēta)]] |
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[[mdf:Юпитерь (шары тяште)]] |
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[[mk:Јупитер]] |
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[[ml:വ്യാഴം]] |
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[[mn:Бархасбадь]] |
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[[mr:गुरू ग्रह]] |
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[[ms:Musytari]] |
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[[mt:Ġove (pjaneta)]] |
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[[mwl:Júpiter (planeta)]] |
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[[my:ကြာသပတေးဂြိုဟ်]] |
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[[nah:Huēyitzitzimicītlalli]] |
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[[nds:Jupiter (Planet)]] |
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[[nds-nl:Jupiter (planeet)]] |
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[[ne:बृहस्पतिग्रह]] |
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[[nl:Jupiter (planeet)]] |
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[[nn:Planeten Jupiter]] |
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[[no:Jupiter]] |
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[[nov:Jupitere (planete)]] |
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[[nv:Jíbitoo]] |
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[[oc:Jupitèr (planeta)]] |
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[[or:ବୃହସ୍ପତି]] |
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[[os:Юпитер (планетæ)]] |
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[[pa:ਬ੍ਰਹਿਸਪਤ]] |
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[[pam:Jupiter]] |
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[[pl:Jowisz]] |
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[[pms:Gieuv (pianeta)]] |
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[[pnb:مشتری]] |
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[[ps:مشتري]] |
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[[pt:Júpiter (planeta)]] |
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[[qu:Pirwa]] |
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[[rm:Jupiter (planet)]] |
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[[ro:Jupiter]] |
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[[ru:Юпитер]] |
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[[rue:Юпітер (планета)]] |
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[[sa:गुरुग्रहः]] |
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[[sah:Юпитер]] |
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[[scn:Giovi (pianeta)]] |
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[[se:Jupiter]] |
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[[sh:Jupiter (planeta)]] |
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[[si:බ්රහස්පති ග්රහයා]] |
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[[simple:Jupiter]] |
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[[sk:Jupiter]] |
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[[sl:Jupiter]] |
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[[so:Cirjeex]] |
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[[sq:Jupiteri]] |
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[[sr:Јупитер]] |
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[[stq:Jupiter]] |
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[[su:Jupiter]] |
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[[sv:Jupiter]] |
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[[sw:Mshtarii]] |
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[[szl:Jowisz]] |
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[[ta:வியாழன் (கோள்)]] |
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[[te:గురుడు]] |
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[[tg:Муштарӣ]] |
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[[th:ดาวพฤหัสบดี]] |
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[[tl:Hupiter (planeta)]] |
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[[tr:Jüpiter]] |
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[[tt:Юпитер (планета)]] |
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[[ug:يۇپىتېر]] |
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[[uk:Юпітер (планета)]] |
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[[ur:مشتری]] |
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[[uz:Yupiter]] |
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[[vi:Sao Mộc]] |
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[[war:Hupiter]] |
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[[wo:Yupiter]] |
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[[xal:Пүрвə һариг]] |
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[[yi:יופיטער]] |
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[[yo:Júpítérì]] |
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[[za:Ndaundeiqfaex]] |
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[[zh:木星]] |
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[[zh-classical:木星]] |
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[[zh-min-nan:Bo̍k-chheⁿ]] |
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[[zh-yue:木星]] |
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Kinaudi a rebision manipud idi 13:04, 31 Enero 2024
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| Dagiti panangikeddeng | |||||||||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Dagiti pangilasin | Jovian | ||||||||||||||||||||||
| Dagiti pakailasinan ti panaglikmut[3][4] | |||||||||||||||||||||||
| Panawen J2000 | |||||||||||||||||||||||
| Aphelion | 816,520,800 km (5.458104 AU) | ||||||||||||||||||||||
| Perihelion | 740,573,600 km (4.950429 AU) | ||||||||||||||||||||||
| 778,547,200 km (5.204267 AU) | |||||||||||||||||||||||
| Eksentrisidad | 0.048775 | ||||||||||||||||||||||
| 4,332.59 aldaw 11.8618 tawen 10,475.8 Hupiter solar nga aldaw[1] | |||||||||||||||||||||||
| 398.88 al-aldaw | |||||||||||||||||||||||
Napipia a kapardas ti panaglikmut | 13.07 km/s | ||||||||||||||||||||||
| 18.818° | |||||||||||||||||||||||
| Paglikigan | 1.305° 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 satelite | 64 | ||||||||||||||||||||||
| 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 | ||||||||||||||||||||||
| Panagdalumpinas | 0.06487 ± 0.00015 | ||||||||||||||||||||||
| 6.1419×1010 km2[5][6] 121.9 Ti Daga | |||||||||||||||||||||||
| Tomo | 1.4313×1015 km3[5] 1321.3 Ti daga | ||||||||||||||||||||||
| Masa | 1.8986×1027 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] | |||||||||||||||||||||||
Panawen ti panagtayyek ti sidereal | 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° | ||||||||||||||||||||||
| Albedo | 0.343 (Piansa) 0.52 (geom.) | ||||||||||||||||||||||
| |||||||||||||||||||||||
| -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 |
| ||||||||||||||||||||||
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]
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]
- ^ Seligman, Courtney. "Panagtayyek a Panawen ken Kaatiddog ti Aldaw". Naala idi 2009-08-13.
- ^ "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)
- ^ 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".
- ^ 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.
- ^ a b c d e f g h Manggitudo ti agpang iti 1 bar nga atmosperiko a presion
- ^ "Sistema a Solar Panagsukisok: Hupiter: Dagiti Kinapudno ken Bilang". NASA. 7 Mayo 2008.
- ^ "Astrodynamic a Taginayon". JPL a Dinamiko a Sistema a Solar. 2009-02-27. Naala idi 2007-08-08.
- ^ 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.
- ^ Anonymous (Marso 1983). "Probe Nephelometer". Galileo Messenger. NASA/JPL (6). Naala idi 2007-02-12.
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