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Jupiter

*** Shopping-Tip: Jupiter

: ''For the god, see Jupiter (god). For other uses of this term, see Jupiter (disambiguation). {{Planet Infobox/Jupiter}} '''Jupiter''' is the fifth planet from the Sun and by far the Solar system by size largest within the solar system. Jupiter and the other gas giants—Saturn, Uranus, and Neptune—are sometimes referred to as "Jovian planets."

Overview
Jupiter is usually the fourth brightest object in the sky (after the Sun, the Moon and Venus); however at times Mars appears brighter than Jupiter. Image:Jupiter-Earth-Spot_comparison.jpg thumb|left|200px|Approximate size comparison of Earth, Jupiter, and the Great Red Spot. Jupiter is 2.5 times larger than all the other planets combined, so large that its Center of mass#Barycenter barycenter with the Sun actually lies above the Sun's surface (1.068 solar radii from the Sun's center). It is 318 times larger than Earth, with a diameter 11 times that of Earth, and with a volume 1300 times that of Earth. Quite naturally, Jupiter's gravitational influence has dominated the evolution of the solar system: most planets' orbits lie closer to Jupiter's orbital plane than the Sun's equatorial plane, the majority of short-period comets belong to Jupiter's family (a result due to both Jupiter's mass and its relative speed), the Kirkwood gaps 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.{{cite book|author=Clarke, Arthur C.|year=1989|title=2061: Odyssey Three|publisher=Del Rey|id=ISBN 0345358791}} Some describe Jupiter as the solar system's vacuum cleaner, due to its immense gravity well. As impressive as Jupiter's mass is, extrasolar planets 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 star, although the latter possesses rather specific spectral lines. Currently, if a very large object is above 12 Jupiter masses, large enough to burn deuterium, it is considered a brown dwarf star; 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 times as large to become a star. Jupiter also has the fastest rotation rate of any planet within the solar system, making a complete rotation on its axis in slightly less than ten hours, which results in an equatorial bulge easily seen through an Earth-based amateur telescope. Jupiter is perpetually covered with a layer of clouds, composed of ammonia crystals and possibly ammonium hydrosulfide, and it may not have any solid surface. Its best known feature is the Great Red Spot, a storm larger than Earth which was first observed by Galileo four centuries ago. Indeed, mathematical models suggest that the storm is stable and may be a permanent feature of the planet.{{cite journal |url=http://www.nature.com/nature/journal/v331/n6158/abs/331689a0.html;jsessionid=EB6990ACE69E14E754FC2B2635B5301C |title=Laboratory simulation of Jupiter's Great Red Spot |first=Jöel |last=Sommeria |coauthors=Steven D. Meyers & Harry L. Swinney |journal=Nature |volume=331 |pages=689 - 693 |month=25 February |year=1988 |id={{doi|10.1038/331689a0}}}} In 2000, three small spots merged to form a larger spot named Oval BA, which later acquired a red hue very similar to that of the Great Red Spot.{{cite web |url=http://science.nasa.gov/headlines/y2006/02mar_redjr.htm |title=Jupiter's New Red Spot |year=2006 |format=HTML |accessdate=2006-03-09}}

Historical observations
Jupiter has been known since ancient times and is visible to the naked eye in the night sky. The Ancient Rome Romans named the planet after the Roman mythology Roman god Jupiter (god) Jupiter (also called Jove). The astronomical symbol for the planet is a stylized representation of the god's lightning bolt. The China Chinese, Korean, Japanese, and Vietnamese refer to the planet as the ''wood star'', 木星,{{cite web |url=http://www.crystalinks.com/jupiter.html |title=JUPITER |format=HTML |accessdate=2006-03-09}} based on the Chinese Five Elements (curiously enough, through a small telescope, it does somewhat resemble a circular slice of wood in appearance, with the Great Red Spot Red Spot being a "knot"). In Vedic Astrology, Hindu astrologers refer to Jupiter as "Guru" which means the "Wise One". In 1610, Galileo Galilei discovered the four largest natural satellite moons of Jupiter, Io (moon) Io, Europa (moon) Europa, Ganymede (moon) Ganymede and Callisto (moon) Callisto (now known as the Galilean moons) using a telescope, the first observation of moons other than Earth's. This was also the first discovery of a celestial motion not apparently centered on the Earth. It was a major point in favor of Copernicus' heliocentric theory of the motions of the planets; Galileo's outspoken support of the Copernican theory got him in trouble with the Inquisition.

Physical characteristics


Planetary composition
Jupiter is composed of a relatively small Rock (geology) rocky core, surrounded by metallic hydrogen, surrounded by phase (matter) liquid hydrogen, which is surrounded by gaseous hydrogen. There is no clear boundary or surface between these different phases of hydrogen; the conditions blend smoothly from gas to liquid as one descends.

Atmosphere
Image:Jupiter from Voyager 1.jpg False-color.html"_title="Meaning of thumb thumb|left|[[False-color_detail of Jupiter's atmosphere, imaged by ''Voyager 1'', showing the Great Red Spot and a passing white oval..html" title="Meaning of left|[[False-color">thumb|left|[[False-color detail of Jupiter's atmosphere, imaged by ''Voyager 1'', showing the Great Red Spot and a passing white oval.">left|[[False-color">thumb|left|[[False-color detail of Jupiter's atmosphere, imaged by ''Voyager 1'', showing the Great Red Spot and a passing white oval. Jupiter's atmosphere is composed of ~81% hydrogen and ~18% helium by number of atoms. The atmosphere is ~75%/24% by mass; with ~1% of the mass accounted for by other substances - the interior contains denser materials such that the distribution is ~71%/24%/5%. The atmosphere contains trace amounts of methane, water vapor, ammonia, and "rock". There are also traces of carbon, ethane, hydrogen sulfide, neon, oxygen, phosphine, and sulfur. The outermost layer of the atmosphere contains crystals of frozen ammonia. This atmospheric composition is very close to the composition of the solar nebula. Saturn has a similar composition, but Uranus (planet) Uranus and Neptune have much less hydrogen and helium. Jupiter's upper atmosphere undergoes differential rotation, an effect first noticed by Giovanni Domenico Cassini Giovanni Cassini (1690). The rotation of Jupiter's polar region polar atmosphere is ~5 minutes longer than that of the equatorial atmosphere. In addition, bands of clouds of different latitudes, known as tropical regions flow in opposing directions on the prevailing winds. The interactions of these conflicting Atmospheric circulation circulation patterns cause storms and turbulence. Wind speeds of 600 km/h are not uncommon. A particularly violent storm, about three times Earth's diameter, is known as the Great Red Spot, and has persisted through more than three centuries of human observation. The only spacecraft to have descended into Jupiter's atmosphere to take scientific measurements is the ''Galileo spacecraft Galileo'' probe (see #Galileo mission Galileo mission). It sent an atmospheric probe into Jupiter upon arrival in 1995, then itself entered Jupiter's atmosphere and burned up in 2003. {{seealso|Cloud pattern on Jupiter}}

Planetary rings
{{main|Rings of Jupiter}} Jupiter has a faint planetary ring system composed of smoke-like dust particles knocked from its moons by meteor impacts. The main ring is made of dust from the satellites Adrastea and Metis. Two wide gossamer rings encircle the main ring, originating from Thebe and Amalthea. There is also an extremely tenuous and distant outer ring that circles Jupiter backwards. Its origin is uncertain, but this outer ring might be made of captured interplanetary dust.

Magnetosphere
Jupiter has a very large and powerful magnetosphere. In fact, if one could see Jupiter's magnetic field from Earth, it would appear five times as large as the full moon in the sky despite being so much farther away. This magnetic field collects a large flux of particle radiation in Jupiter's radiation belts, as well as producing a dramatic gas torus and flux tube associated with Io. Jupiter's magnetosphere is the largest planetary structure in the solar system. The ''Pioneer'' probes confirmed that Jupiter's enormous magnetic field is 10 times stronger than Earth's and contains 20,000 times as much energy. The sensitive instruments aboard found that the Jovian magnetic field's "north" magnetic pole is at the planet’s geographic south pole, with the axis of the magnetic field tilted 11 degrees from the Jovian rotation axis and offset from the center of Jupiter in a manner similar to the axis of the Earth's field. The ''Pioneers'' measured the bow shock of the Jovian magnetosphere to the width of 26 million kilometres (16 million miles), with the magnetic tail extending beyond Saturn’s orbit. The data showed that the magnetic field fluctuation fluctuates rapidly in size on the sunward side of Jupiter because of pressure variations in the solar wind, an effect studied in further detail by the two ''Voyager'' spacecraft. It was also discovered that streams of high-energy atomic particles are ejected from the Jovian magnetosphere and travel as far as the orbit of the Earth. Energetic protons were found and measured in the Jovian radiation belt and Current (electricity) electric currents were detected flowing between Jupiter and some of its moons, particularly Io.

Exploration of Jupiter
A number of probes have visited Jupiter.

Pioneer flyby missions
''Pioneer 10'' flew past Jupiter in December of 1973, followed by ''Pioneer 11'' exactly one year later. They provided important new data about Jupiter's magnetosphere, and took some low-resolution photographs of the planet.

Voyager flyby missions
Image:Jupiter gany.jpg January 24.html" title="Meaning of thumb thumb|200px|right|''Voyager 1'' took this photo of the planet Jupiter on [[January 24, while still more than 25 million miles (40 million kilometres) away. Click image for full caption..html" title="Meaning of 200px|right|''Voyager 1'' took this photo of the planet Jupiter on [[January 24">thumb|200px|right|''Voyager 1'' took this photo of the planet Jupiter on [[January 24, while still more than 25 million miles (40 million kilometres) away. Click image for full caption.">200px|right|''Voyager 1'' took this photo of the planet Jupiter on [[January 24">thumb|200px|right|''Voyager 1'' took this photo of the planet Jupiter on [[January 24, while still more than 25 million miles (40 million kilometres) away. Click image for full caption. ''Voyager 1'' flew by in March 1979 followed by ''Voyager 2'' in July of the same year. The ''Voyagers'' vastly improved the understanding of the Galilean moons and discovered Jupiter's rings. They also took the first close up images of the planet's atmosphere.

Ulysses flyby mission
In February 1992, ''Ulysses probe Ulysses'' solar probe performed a flyby of Jupiter at a distance of 450,000 km (6.3 Jovian radii). The flyby was required to attain a polar orbit around the Sun. The probe conducted studies on Jupiter's magnetosphere. Since there are no cameras onboard the probe, no images were taken. In February 2004, the probe came again in the vicinity of Jupiter. This time distance was much greater, about 240 million km.

Galileo mission
So far the only spacecraft to orbit Jupiter is the ''Galileo spacecraft Galileo'' orbiter, which went into orbit around Jupiter in December 7 1995. It orbited the planet for over seven years and conducted multiple flybys of all of the Galilean moons and Amalthea (moon) Amalthea. The spacecraft also witnessed the impact of Comet Shoemaker-Levy 9 into Jupiter as it approached the planet in 1994, giving a unique vantage point for this spectacular event. However, while the information gained about the Jovian system from the ''Galileo'' mission was extensive in its own right, its originally-designed capacity was limited by the failed deployment of its high-gain radio transmitting antenna. Image:PIA04866_modest.jpg Cassini-Huygens thumb|right|Jupiter as seen by the space probe [[Cassini-Huygens|Cassini. This is the most detailed global color portrait of Jupiter ever assembled..html" title="Meaning of Cassini.html" title="Meaning of thumb|right|Jupiter as seen by the space probe [[Cassini-Huygens|Cassini">thumb|right|Jupiter as seen by the space probe [[Cassini-Huygens|Cassini. This is the most detailed global color portrait of Jupiter ever assembled.">Cassini.html" title="Meaning of thumb|right|Jupiter as seen by the space probe [[Cassini-Huygens|Cassini">thumb|right|Jupiter as seen by the space probe [[Cassini-Huygens|Cassini. This is the most detailed global color portrait of Jupiter ever assembled. An atmospheric probe was released from the spacecraft in July, 1995. The probe entered the planet's atmosphere in December 7 1995. It parachuted through 150 km of the atmosphere, collecting data for 57.6 minutes, before being crushed by the extreme pressure to which it was subjected. It would have melted and vaporized shortly thereafter. The ''Galileo'' orbiter itself experienced a more rapid version of the same fate when it was deliberately steered into the planet on September 21, 2003 at a speed of over 50 km/s, in order to avoid any possibility of it crashing into and possibly contaminating Europa (moon) Europa, one of the Jovian moons.

Cassini flyby mission
In 2000, the ''Cassini-Huygens Cassini'' probe, ''en route'' to Saturn, flew by Jupiter and provided some of the highest-resolution images ever made of the planet.

Future probes
NASA is planning a mission to study Jupiter in detail from a polar orbit. Named ''Juno (spacecraft) Juno'', the spacecraft is planned to launch by 2010. After the discovery of a liquid ocean on Jupiter's moon Europa (moon) Europa, there has been great interest to study the icy moons in detail. A mission proposed by NASA was dedicated to study them. The Jupiter Icy Moons Orbiter JIMO (Jupiter Icy Moons Orbiter) was expected to be launched sometime after 2012. However, the mission was deemed too ambitious and its funding was canceled. In 2007, Jupiter will also be briefly visited by the ''New Horizons'' probe, ''en route'' to Pluto.

Natural satellites
{{main|Jupiter's natural satellites}} Image:Jupiter.moons1.jpg Great Red Spot.html" title="Meaning of thumb thumb|right|300px|Jupiter's 4 Galilean moons, in a composite image comparing their sizes and the size of Jupiter ([[Great Red Spot visible). From the top they are: Callisto (moon) Callisto, Ganymede (moon) Ganymede, Europa (moon) Europa and Io (moon) Io..html" title="Meaning of right|300px|Jupiter's 4 Galilean moons, in a composite image comparing their sizes and the size of Jupiter ([[Great Red Spot">thumb|right|300px|Jupiter's 4 Galilean moons, in a composite image comparing their sizes and the size of Jupiter ([[Great Red Spot visible). From the top they are: Callisto (moon) Callisto, Ganymede (moon) Ganymede, Europa (moon) Europa and Io (moon) Io.">right|300px|Jupiter's 4 Galilean moons, in a composite image comparing their sizes and the size of Jupiter ([[Great Red Spot">thumb|right|300px|Jupiter's 4 Galilean moons, in a composite image comparing their sizes and the size of Jupiter ([[Great Red Spot visible). From the top they are: Callisto (moon) Callisto, Ganymede (moon) Ganymede, Europa (moon) Europa and Io (moon) Io. Jupiter has at least 63 moons. For a complete listing of these moons, please see Jupiter's natural satellites. For a timeline of their discovery dates, see Timeline of natural satellites. The four large moons, known as the "Galilean moons", are Io (moon) Io, Europa (moon) Europa, Ganymede (moon) Ganymede and Callisto (moon) Callisto.

Galilean moons
The orbits of Io, Europa, and Ganymede, the largest moon in the solar system, form a pattern known as a Laplace resonance; for every four orbits that Io makes around Jupiter, Europa makes exactly two orbits and Ganymede makes exactly one. This resonance causes the gravity gravitational effects of the three moons to distort their orbits into elliptical shapes, since each moon receives an extra tug from its neighbors at the same point in every orbit it makes. image:JupiterandIo.jpg Hubble Space Telescope thumb|250px|left|A picture of Jupiter and its moon Io taken by [[Hubble Space Telescope|Hubble. The black spot is Io's shadow..html" title="Meaning of Hubble.html" title="Meaning of thumb|250px|left|A picture of Jupiter and its moon Io taken by [[Hubble Space Telescope|Hubble">thumb|250px|left|A picture of Jupiter and its moon Io taken by [[Hubble Space Telescope|Hubble. The black spot is Io's shadow.">Hubble.html" title="Meaning of thumb|250px|left|A picture of Jupiter and its moon Io taken by [[Hubble Space Telescope|Hubble">thumb|250px|left|A picture of Jupiter and its moon Io taken by [[Hubble Space Telescope|Hubble. The black spot is Io's shadow. The tidal force from Jupiter, on the other hand, works to circularize their orbits. This constant tug of war causes regular flexing of the three moons' shapes, Jupiter's gravity stretches the moons more strongly during the portion of their orbits that are closest to it and allowing them to spring back to more spherical shapes when they're farther away. This flexing causes tidal heating of the three moons' cores. This is seen most dramatically in Io's extraordinary volcanic activity, and to a somewhat less dramatic extent in the geologically young surface of Europa indicating recent resurfacing. {| class="wikitable" |- style="background:#efefef;" ! colspan="6" | The Galilean moons, compared to Earth's moon Moon Luna |- |- style="background:#efefef;" ! colspan="2" | Name
(Asteroid pronunciation key Pronunciation key) ! Diameter
(km) ! Mass
(kg) ! Orbital radius (km) ! Orbital period (days) |- style="background:#ccccff;" align="center" | '''Io (moon) Io''' || ''eye'-oe''
{{IPA|ˈaɪəʊ}} || 3643
(105% Luna) || 8.9×1022
(120% Luna) ||421 700
(110% Luna) ||1.77
(6.5% Luna) |- style="background:#ccccff" align="center" | '''Europa (moon) Europa''' || ''ew-roe'-pÉ™''
{{IPA|jʊərəʊpə}} || 3122
(90% Luna) || 4.8×1022
(65% Luna) || 671 034
(175% Luna) || 3.55
(13% Luna) |- style="background:#ccccff" align="center" | '''Ganymede (moon) Ganymede''' || ''gan'-É™-meed''
{{IPA|ˈgænəmid}} || 5262
(150% Luna) || 14.8×1022
(200% Luna) || 1 070 412
(280% Luna) || 7.15
(26% Luna) |- style="background:#ccccff" align="center" | '''Callisto (moon) Callisto''' || ''kÉ™-lis'-toe''
{{IPA|kəˈlɪstəʊ}} || 4821
(140% Luna) || 10.8×1022
(150% Luna) || 1 882 709
(490% Luna) || 16.69
(61% Luna) |}

Classification of Jupiter's moons
Before the discoveries of the Voyager missions, Jupiter's moons were arranged neatly into four groups of four. Since then, the large number of new small outer moons has complicated this picture. There are now thought to be six main groups, although some are more distinct than others. A basic division is between the eight inner regular moons with nearly circular orbits near the plane of Jupiter's equator, which are believed to have formed with Jupiter, and an unknown number of small irregular moons, with elliptical and inclined orbits, which are believed to be captured asteroids or fragments of captured asteroids. Image:Europa-moon.jpg Europa_(moon) thumb|right|150px|[[Europa (moon)|Europa, one of Jupiter's many natural satellite moons..html" title="Meaning of Europa.html" title="Meaning of thumb|right|150px|[[Europa (moon)|Europa">thumb|right|150px|[[Europa (moon)|Europa, one of Jupiter's many natural satellite moons.">Europa.html" title="Meaning of thumb|right|150px|[[Europa (moon)|Europa">thumb|right|150px|[[Europa (moon)|Europa, one of Jupiter's many natural satellite moons. #Regular moons ##The inner group of four small moons all have diameters of less than 200 km, orbit at radii less than 200,000 km, and have orbital inclinations of less than half a degree. ##The four Galilean moons were all discovered by Galileo Galilei, orbit between 400,000 and 2,000,000 km, and include some of the largest moons in the solar system. #Irregular moons ##Themisto (moon) Themisto is in a group of its own, orbiting halfway between the Galilean moons and the next group. ##The Himalia group is a tightly clustered group of moons with orbits around 11-12,000,000 km from Jupiter. ##Carpo (moon) Carpo is another isolated case; at the inner edge of the Ananke group, it revolves in the direct sense. ##The Ananke group is a group with rather indistinct borders, averaging 21,276,000 km from Jupiter with an average inclination of 149 degrees. ##The Carme group is a fairly distinct group that averages 23,404,000 km from Jupiter with an average inclination of 165 degrees. ##The Pasiphaë group is a dispersed and only vaguely distinct group that covers all the outermost moons. It is thought that the groups of outer moons may each have a common origin, perhaps as a larger moon or captured body that broke up.

Life on Jupiter
It is considered highly unlikely that there is any extraterrestrial life life on Jupiter, as there is little to no water in the atmosphere and any possible solid surface deep within Jupiter would be under extraordinary pressures. However, in 1976, before the Voyager program Voyager missions, Carl Sagan hypothesized (with Edwin E. Salpeter) that ammonia-based life could evolve in Jupiter's upper atmosphere. Sagan and Salpeter based this hypothesis on the ecology of terrestrial seas which have simple Photosynthesis photosynthetic plankton at the top level, fish at lower levels feeding on these creatures, and marine predators which hunt the fish. The Jovian equivalents Sagan and Salpeter hypothesized were "sinkers", "floaters", and "hunters". The "sinkers" would be plankton-like organisms which fall through the atmosphere, existing just long enough that they can reproduce in the time they are kept afloat by convection. The "floaters" would be giant bags of gas functioning along the lines of hot air balloons, using their own metabolism (feeding off sunlight and free molecules) to keep their gas warm. The "hunters" would be almost squid-like creatures, using jets of gas to propel themselves into "floaters" and consume them.{{cite web |url=http://www.daviddarling.info/encyclopedia/J/Jupiterlife.html |title=Jupiter, life on |publisher=Encyclopedia of Astrobiology, Astronomy & Spaceflight |format=HTML |accessdate=2006-03-09}} These ideas are only hypotheses and there is currently no way to prove or disprove them.

Trojan asteroids
In addition to its moons, Jupiter's gravitational field controls numerous asteroids which have settled into the Lagrangian points preceding and following Jupiter in its orbit around the sun. These are known as the Trojan asteroids, and are divided into List of Trojan asteroids (Greek camp) Greek and List of Trojan asteroids (Trojan camp) Trojan "camps" to commemorate the ''Iliad''. The first of these, 588 Achilles, was discovered by Max Wolf in 1906; since then hundreds more have been discovered. The largest is 624 Hektor.

Cometary impact
Image:Jupitersatelliteimpact.jpg Comet.html" title="Meaning of right right|thumb|[[Comet impacts on the surface of Jupiter. The dark clouds resulting from these impacts are larger than Earth itself..html" title="Meaning of thumb|right|thumb|[[Comet impacts on the surface of Jupiter. The dark clouds resulting from these impacts are larger than Earth itself.">thumb|[[Comet">right|thumb|[[Comet impacts on the surface of Jupiter. The dark clouds resulting from these impacts are larger than Earth itself. During the period July 16 to July 22, 1994, over twenty fragments from the comet comet Shoemaker-Levy 9 Shoemaker-Levy 9 hit Jupiter's southern hemisphere, providing the first direct observation of a collision between two solar system objects. It is thought that due to Jupiter's large mass and location near the inner solar system it receives the most frequent comet impacts of the solar system's planets.

See also
* Planets in astrology#Jupiter Jupiter in astrology * Aspects of Jupiter - for data of opposition, conjunction to sun, etc. * Jupiter in fiction

References
* Bagenal, F. & Dowling, T. E. & McKinnon, W. B. (Eds.). (2004). ''Jupiter: The planet, satellites, and magnetosphere''. Cambridge: Cambridge University Press. * {{cite book|last=Beebe|first=Reta|title=Jupiter: The Giant Planet|origyear=1997|edition=Second|year=2002|publisher=Smithsonian Institute Press|location=Washington, D.C.|ISBN=1560986859}}

External links
{{commons|Jupiter}}
- NASA's Jupiter fact sheet
- A Trip Into Space Data and photos on Jupiter
- Jupiter's Inner Moons
- 3D VRML Jupiter globe and its satellites Io, Callisto, Europa and Ganymede
- Planets - Jupiter A kid's guide to Jupiter.
- "Jupiter: The Giant Planet" One of ''World Book Encyclopedia'''s monthly features, this one on Jupiter. {{Jupiter Footer}} {{Footer_SolarSystem}} Category:Jupiter * {{Link FA|cs}} {{Link FA|es}} {{Link FA|fr}} af:Jupiter (planeet) als:Jupiter (Planet) ang:Iupiter ar:مشتري bg:Юпитер (планета) bn:জà§?পিটার bs:Jupiter ca:Júpiter (planeta) cs:Jupiter (planeta) cy:Iau (planed) da:Jupiter (planet) de:Jupiter (Planet) et:Jupiter (planeet) es:Júpiter (planeta) eo:Jupitero eu:Jupiter fr:Jupiter (planète) ga:Iúpatar (pláinéad) gl:Xúpiter (planeta) gu:ગà«?રà«? (ગà«?રહ) ko:목성 kw:Yow (planet) hr:Jupiter (planet) io:Jupitero id:Jupiter is:Júpíter (reikistjarna) it:Giove (astronomia) he:צדק (כוכב לכת) la:Iuppiter (planeta) lv:Jupiters lt:Jupiteris (planeta) hu:Jupiter (bolygó) mk:Јупитер mt:Ä ove (pjaneta) ms:Musytari nl:Jupiter (planeet) ja:木星 ka:იუპიტერი (პლáƒ?ნეტáƒ?) no:Jupiter (planet) nn:Planeten Jupiter pam:Jupiter pl:Jowisz pt:Júpiter (planeta) ro:Jupiter (planetă) ru:Юпитер (планета) scn:Giovi simple:Jupiter (planet) sk:Jupiter (planéta) sl:Jupiter (planet) sr:Јупитер (планета) fi:Jupiter sv:Jupiter tl:Jupiter ta:வியாழனà¯? (கோளà¯?) th:ดาวพฤหัสบดี vi:Má»™c Tinh tr:Jüpiter (gezegen) uk:Юпітер (планета) zh:木星 {{catmore1|Jupiter (planet)}} {{Footer_SolarSystem}} Category:Planets of the Solar System als:Kategorie:Jupiter (Planet) bg:КатегориÑ?:Юпитер bs:Category:Jupiter ca:Categoria:Júpiter cs:Kategorie:Jupiter de:Kategorie:Jupiter (Planet) et:Kategooria:Jupiter es:Categoría:Júpiter eo:Kategorio:Jupitero fr:Catégorie:Jupiter ko:분류:목성 it:Categoria:Giove la:Categoria:Iuppiter nl:Categorie:Jupiter ja:Category:木星 nn:Kategori:Jupiter pl:Kategoria:Jowisz pt:Categoria:Júpiter ru:КатегориÑ?:Юпитер sk:Kategória:Jupiter (planéta) sl:Kategorija:Jupiter sr:Категорија:Јупитер fi:Luokka:Jupiter tr:Kategori:Jüpiter (gezegen) zh:Category:木星

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[The article Jupiter is based on the the dictionary Wikipedia, the free encyklopedia. There you will find a list of all editors and the possibility to edit the original text of the article Jupiter.
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