Jump to content

Jupiter

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by 207.200.116.11 (talk) at 05:31, 8 December 2005 (Planetary composition). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

Template:Planet Infobox/Jupiter 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,[1]; 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, 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").

Overview

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. As impressive as it 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.

File:Poles.png
Jupiter is so massive it clusters the orbital poles of the other planets around its own.

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 years 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.

Physical characteristics

Planetary composition

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. Life has also been found on jupiter!! Scientist are testing the species as you read this!

Atmosphere

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 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 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).

Planetary rings

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 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.

Appearance

Stationary, retrograde Opposition Distance to Earth (AU) Maximum brightness Diameter Stationary, prograde Conjunction to Sun
January 4, 2004 March 4, 2004 4.42570 -2.5 mag 44.50" May 5, 2004 September 21, 2004
February 2, 2005 April 3, 2005 4.45664 -2.5 mag 44.19" June 5, 2005 October 23, 2005
March 5, 2006 May 4, 2006 4.41269 -2.5 mag 44.63" July 6, 2006 November 21, 2006
April 6, 2007 June 5, 2007 4.30436 -2.6 mag 45.75" August 7, 2007 December 23, 2007
May 9, 2008 July 9, 2008 4.16097 -2.7 mag 47.33" September 8, 2008 January 24, 2009
June 15, 2009 August 14, 2009 4.02777 -2.9 mag 48.89" October 13, 2009 February 28, 2010
July 24, 2010 September 21, 2010 3.95392 -2.9 mag 49.81" November 19, 2010 April 6, 2011
August 30, 2011 October 29, 2011 3.96975 -2.9 mag 49.61" December 26, 2011 May 13, 2012
October 4, 2012 December 3, 2012 4.06853 -2.8 mag 48.41" January 30, 2013 June 19, 2013
November 7, 2013 January 5, 2014 4.21044 -2.7 mag 46.77" March 6, 2014 July 24, 2014
December 9, 2014 February 6, 2015 4.34623 -2.6 mag 45.31" April 8, 2015 August 26, 2015
January 8, 2016 March 8, 2016 4.43536 -2.5 mag 44.40" May 9, 2016 September 26, 2016
February 6, 2017 April 7, 2017 4.45491 -2.5 mag 44.21" June 10, 2017 October 26, 2017
March 9, 2018 May 9, 2018 4.39983 -2.5 mag 44.76" July 11, 2018 November 26, 2018
April 10, 2019 June 10, 2019 4.28388 -2.6 mag 45.97" August 11, 2019 December 27, 2019
May 14, 2020 July 14, 2020 4.13931 -2.8 mag 47.58" September 12, 2020 January 29, 2021

Source: The Calculated Sky

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

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 our 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 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.

Galileo mission

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.

Jupiter as seen by the space probe 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, one of the Jovian moons.

Cassini flyby mission

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.

Future probes

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's moons

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, Ganymede, Europa and 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, Europa, Ganymede and 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 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.

A picture of Jupiter and its moon Io taken by 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.

The Galilean moons, compared to Earth's moon Luna
Name

(Pronunciation key)

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)

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.

Europa, one of Jupiter's many moons.
  1. Regular moons
    1. 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.
    2. 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.
  2. Irregular moons
    1. Themisto is in a group of its own, orbiting halfway between the Galilean moons and the next group.
    2. The Himalia group is a tightly clustered group of moons with orbits around 11-12,000,000 km from Jupiter.
    3. Carpo is another isolated case; at the inner edge of the Ananke group, it revolves in the direct sense.
    4. The Ananke group is a group with rather indistinct borders, averaging 21,276,000 km from Jupiter with an average inclination of 149 degrees.
    5. The Carme group is a fairly distinct group that averages 23,404,000 km from Jupiter with an average inclination of 165 degrees.
    6. 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 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. [2] 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 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.

Cometary impact

A 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 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.

Jupiter in fiction and film

Jupiter and Internet conspiracists

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 [3]. 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 [4]. Galileo carried about 15.6 kg [5] of plutonium-238 as its power source, in the form of 144 pellets of plutonium dioxide, a ceramic [6] [7]. 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 [8].

See also

References

  • Bagenal, F. & Dowling, T. E. & McKinnon, W. B. (Eds.). (2004). Jupiter: The planet, satellites, and magnetosphere. Cambridge: Cambridge University Press.
  • ^ . ISBN 0345358791. {{cite book}}: Missing or empty |title= (help); Unknown parameter |Author= ignored (|author= suggested) (help); Unknown parameter |Publisher= ignored (|publisher= suggested) (help); Unknown parameter |Title= ignored (|title= suggested) (help); Unknown parameter |Year= ignored (|year= suggested) (help)
(moon navigator) | Jupiter | Metis | ...

Template:Jupiter Footer

Template:Link FA