

|
![]() Click image for description |
|||||||
|---|---|---|---|---|---|---|---|
| Orbital characteristics (Epoch J2000) | |||||||
| Semi-major axis | 778,412,027 km 5.203 363 01 AU |
||||||
| Orbital circumference | 4.888 Tm 32.675 AU |
||||||
| Eccentricity | 0.048 392 66 | ||||||
| Perihelion | 740,742,598 km 4.951 558 43 AU |
||||||
| Aphelion | 816,081,455 km 5.455 167 59 AU |
||||||
| Orbital period | 4333.2867 d (11.86 a) |
||||||
| Synodic period | 398.88 d | ||||||
| Avg. Orbital Speed | 13.056 km/s | ||||||
| Max. Orbital Speed | 13.712 km/s | ||||||
| Min. Orbital Speed | 12.446 km/s | ||||||
| Inclination | 1.305 30° (6.09° to Sun's equator) |
||||||
| Longitude of the ascending node |
100.556 15° | ||||||
| Argument of the perihelion |
274.197 70° | ||||||
| Number of satellites | 63 | ||||||
| Physical characteristics | |||||||
| Equatorial diameter | 142,984 km [1] (11.209 Earths) |
||||||
| Polar diameter | 133,709 km (10.517 Earths) |
||||||
| Oblateness | 0.064 87 | ||||||
| Surface area | 6.14×1010 km2 (120.5 Earths) |
||||||
| Volume | 1.431×1015 km3 (1321.3 Earths) |
||||||
| Mass | 1.899×1027 kg (317.8 Earths) |
||||||
| Mean density | 1.326 g/cm3 | ||||||
| Equatorial gravity | 23.12 m/s2 (2.358 gee) |
||||||
| Escape velocity | 59.54 km/s | ||||||
| Rotation period | 0.413 538 021 d (9 h 55 min 29.685 s) 1 | ||||||
| Rotation velocity | 12.6 km/s = 45,300 km/h (at the equator) |
||||||
| Axial tilt | 3.13° | ||||||
| Right ascension of North pole |
268.05° (17 h 52 min 12 s) | ||||||
| Declination | 64.49° | ||||||
| Albedo | 0.52 | ||||||
| Surface temp. |
|
||||||
| Adjective | Jovian | ||||||
| Atmospheric characteristics | |||||||
| Atmospheric pressure | 70 kPa | ||||||
| Hydrogen | ~86% | ||||||
| Helium | ~14% | ||||||
| Methane | 0.1% | ||||||
| Water vapor | 0.1% | ||||||
| Ammonia | 0.02% | ||||||
| Ethane | 0.0002% | ||||||
| Phosphine | 0.0001% | ||||||
| Hydrogen sulfide | <0.00010% | ||||||
Jupiter is the fifth planet from the Sun and by far the largest within our solar system. Some have described the solar system as consisting of the Sun, Jupiter, and assorted debris,[2]; some describe Jupiter as the solar system's vacuum cleaner, due to its immense gravity well. It and the other gas giants - Saturn, Uranus, and Neptune, are sometimes referred to as "Jovian planets." The Romans named the planet after the Roman god Jupiter (also called Jove). The astronomical symbol for the planet is a stylized representation of the god's lightning bolt.
The Chinese, Korean, Japanese, and Vietnamese cultures refer to the planet as the wood star, 木星 [3], based on the Chinese Five Elements (although, curiously enough, through a small telescope, it does somewhat resemble a circular slice of wood in appearance, with the Red Spot being a "knot").
Contents |
Jupiter has been known since ancient times and is visible to the naked eye in the night sky. In 1610, Galileo Galilei discovered the four largest moons of Jupiter using a telescope, the first observation of moons other than Earth's.
Jupiter is 2.5 times more massive than all the other planets combined, so massive that its barycenter with the Sun actually lies above the Sun's surface (1.068 solar radii from the Sun's center). It is 318 times more massive 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 (see illustration), the majority of short-period comets belong to Jupiter's family (a result due to both Jupiter's mass and its relative celerity), 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.
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 and massive planet such as Jupiter from a brown dwarf star, although the latter possesses rather specific spectral lines. 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 massive to become a star.
Jupiter also has the fastest rotation rate of any planet within the solar system, making a complete revolution on its axis in slightly less than ten hours, which results in a flattening easily seen through an Earth-based amateur telescope. Its best known feature is probably 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 a permanent feature of the planet. Jupiter is perpetually covered with a layer of clouds, and may not have any solid surface.
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, while at others Jupiter appears brighter than Venus). It has been known since ancient times. Galileo Galilei's discovery, in 1610, of Jupiter's four large moons Io, Europa, Ganymede and Callisto (now known as the Galilean moons) was 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.
Jupiter is composed of a relatively small rocky core, surrounded by metallic hydrogen, surrounded by 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.
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 vapour, 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 and Neptune have much less hydrogen and helium.
Jupiter's upper atmosphere undergoes differential rotation, an effect first noticed by Giovanni Cassini (1690). The rotation of Jupiter's 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 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 probe (see Galileo mission).
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.
Jupiter has a very large and powerful magnetosphere. In fact, if you 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 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 electric currents were detected flowing between Jupiter and some of its moons, particularly Io.
Source: The Calculated Sky
A number of probes have visited Jupiter.
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 1 flew by in March 1979 followed by Voyager 2 in July of the same year. The Voyagers vastly improved our understanding of the Galilean moons and discovered Jupiter's rings. They also took the first close up images of the planet's atmosphere.
In February 1992, Ulysses solar probe performed a flyby of Jupiter at a distance of 900,000 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.
So far the only spacecraft to orbit Jupiter is the 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. 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, the information gained about the Jovian system from the Galileo mission was limited by the failed deployment of its high-gain radio transmitting antenna.
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, one of the Jovian moons.
In 2000, the Cassini probe, en route to Saturn, flew by Jupiter and provided some of the highest-resolution images ever made of the planet.
NASA is planning a mission to study Jupiter in detail from a polar orbit. Named Juno, the spacecraft is planned to launch by 2010.
After the discovery of a liquid ocean on Jupiter's 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 JIMO (Jupiter Icy Moons Orbiter) was expected to be launched sometime after 2012. However, the mission was deemed too ambitious and its funding was cancelled.
In 2007, Jupiter will also be briefly visited by the New Horizons probe, en route to Pluto.
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, Europa, Ganymede and Callisto.
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 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.
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.
| The Galilean moons, compared to Earth's moon Luna | |||||
|---|---|---|---|---|---|
| Name |
Diameter (km) |
Mass (kg) |
Orbital radius (km) | Orbital period (days) | |
| Io | eye'-oe ˈaɪɔʊ |
3643 (105% Luna) |
8.9×1022 (120% Luna) |
421 700 (110% Luna) |
1.77 (6.5% Luna) |
| Europa | ew-roe'-pa juˈrɔʊpə |
3122 (90% Luna) |
4.8×1022 (65% Luna) |
671 034 (175% Luna) |
3.55 (13% Luna) |
| Ganymede | gan'-i-meed ˈgænəmid |
5262 (150% Luna) |
14.8×1022 (200% Luna) |
1 070 412 (280% Luna) |
7.15 (26% Luna) |
| Callisto | ka-lis'-toe kəˈlɪstɔʊ |
4821 (140% Luna) |
10.8×1022 (150% Luna) |
1 882 709 (490% Luna) |
16.69 (61% Luna) |
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.
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.
It is considered highly unlikely that there is any life on Jupiter, as there is little to no water in the atmosphere and any solid surface Jupiter would be under extraordinary pressures. However, in 1976, before the 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 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 Saltpeter hypothesized were "sinkers", "floaters", and "hunters". 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. [4] These ideas are only hypotheses and there is currently no way to prove or disprove them.
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 Greek and 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.
During the period July 16 to July 22, 1994, over twenty fragments from the comet 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.
Although the theory of the intentional detonation of Jupiter predates the internet, the web spawned at least one theory of its own. On October 19, 2003 a black spot was photographed on Jupiter by Belgian astronomer Olivier Meeckers [5]. Although not an unusual occurrence, this one caught the fancy of some science fiction fans and conspiracy theorists, who went as far as speculating that the spot was evidence of nuclear activity on Jupiter, caused by Galileo's plunge into the planet a month prior [6]. Galileo carried about 15.6 kg [7] of plutonium-238 as its power source, in the form of 144 pellets of plutonium dioxide, a ceramic [8] [9]. The individual pellets (which would be expected to separate during entry) initially contained about 108 grams of 238Pu each (about 10% would have decayed away by the time Galileo entered Jupiter), and are short of the required critical mass by a factor of about 100 [10].
| Jupiter's natural satellitesedit |
|---|
| Inner satellites | Galilean moons: Io, Europa, Ganymede, and Callisto | Themisto | Himalia group | Carpo | S/2003 J 12 | Ananke group | Carme group | Pasiphaë group | S/2003 J 2 |
| The Solar System |
|---|
| Sun - Mercury - Venus - Earth (Moon) - Mars - Asteroid belt - Jupiter |
| Saturn - Uranus - Neptune - Pluto - Kuiper belt - Scattered disc - Oort cloud |
| See also astronomical objects and the solar system's list of objects, sorted by radius or mass. |