Galilean moons - wikipedia Galilean moons Montage of Jupiter 's four Galilean moons, in a composite image depicting part of Jupiter and their relative sizes ( positions are illustrative, not actual ). From top to bottom : Io, Europa, Ganymede, Callisto. Two Hubble Space Telescope views of a rare triple transit of Jupiter by Europa, Callisto and Io ( 24 January 2015 ). The Galilean moons are the four largest moons of Jupiter -- Io, Europa, Ganymede, and Callisto. They were first seen by Galileo Galilei in January 1610, and recognized by him as satellites of Jupiter in March 1610. They were the first objects found to orbit another planet. Their names derive from the lovers of Zeus. They are among the largest objects in the Solar System with the exception of the Sun and the eight planets, with a radius larger than any of the dwarf planets. Ganymede is the largest moon in the Solar System, and is even bigger than the planet Mercury, though only around half as massive. The three inner moons -- Io, Europa, and Ganymede -- are in a 4 : 2 : 1 orbital resonance with each other. Because of their much smaller size, and therefore weaker self - gravitation, all of Jupiter 's remaining moons have irregular forms rather than a spherical shape. The Galilean moons were discovered in either 1609 or 1610 when Galileo made improvements to his telescope, which enabled him to observe celestial bodies more distinctly than ever. Galileo 's discovery showed the importance of the telescope as a tool for astronomers by proving that there were objects in space that can not be seen by the naked eye. More importantly, the incontrovertible discovery of celestial bodies orbiting something other than Earth dealt a serious blow to the then - accepted Ptolemaic world system, or the geocentric theory in which everything orbits around Earth. Galileo initially named his discovery the Cosmica Sidera ( `` Cosimo 's stars '' ), but the names that eventually prevailed were chosen by Simon Marius. Marius discovered the moons independently at the same time as Galileo, and gave them their present names, which were suggested by Johannes Kepler, in his Mundus Jovialis, published in 1614. Contents 1 History 1.1 Discovery 1.2 Dedication to the Medicis 1.3 Name 1.4 Determination of longitude 2 Members 2.1 Io 2.2 Europa 2.3 Ganymede 2.4 Callisto 3 Comparative structure 3.1 Size 3.2 Latest flyby 4 Origin and evolution 5 Visibility 6 Orbit animation 7 See also 8 References 9 External links History Discovery Galileo Galilei, the discoverer of the four moons As a result of improvements Galileo Galilei made to the telescope, with a magnifying capability of 20 ×, he was able to see celestial bodies more distinctly than was ever possible before. This allowed Galilei to discover in either December 1609 or January 1610 what came to be known as the Galilean moons. On January 7, 1610, Galileo wrote a letter containing the first mention of Jupiter 's moons. At the time, he saw only three of them, and he believed them to be fixed stars near Jupiter. He continued to observe these celestial orbs from January 8 to March 2, 1610. In these observations, he discovered a fourth body, and also observed that the four were not fixed stars, but rather were orbiting Jupiter. Galileo 's discovery proved the importance of the telescope as a tool for astronomers by showing that there were objects in space to be discovered that until then had remained unseen by the naked eye. More importantly, the discovery of celestial bodies orbiting something other than Earth dealt a blow to the then - accepted Ptolemaic world system, which held that Earth was at the center of the universe and all other celestial bodies revolved around it. Galileo 's Sidereus Nuncius ( Starry Messenger ), which announced celestial observations through his telescope, does not explicitly mention Copernican heliocentrism, a theory that placed the Sun at the center of the universe. Nevertheless, Galileo accepted the Copernican theory. A Chinese historian of astronomy, Xi Zezong, has claimed that a `` small reddish star '' observed near Jupiter in 362 BCE by Chinese astronomer Gan De may have been Ganymede, predating Galileo 's discovery by around two millennia. Dedication to the medicis The Medician stars in the Sidereus Nuncius ( the ' starry messenger ' ), 1610. The moons are drawn in changing positions. In 1605, Galileo had been employed as a mathematics tutor for Cosimo de ' Medici. In 1609, Cosimo became Grand Duke Cosimo II of Tuscany. Galileo, seeking patronage from his now - wealthy former student and his powerful family, used the discovery of Jupiter 's moons to gain it. On February 13, 1610, Galileo wrote to the Grand Duke 's secretary : `` God graced me with being able, through such a singular sign, to reveal to my Lord my devotion and the desire I have that his glorious name live as equal among the stars, and since it is up to me, the first discoverer, to name these new planets, I wish, in imitation of the great sages who placed the most excellent heroes of that age among the stars, to inscribe these with the name of the Most Serene Grand Duke. '' Galileo asked whether he should name the moons the `` Cosmian Stars '', after Cosimo alone, or the `` Medician Stars '', which would honor all four brothers in the Medici clan. The secretary replied that the latter name would be best. On March 12, 1610, Galileo wrote his dedicatory letter to the Duke of Tuscany, and the next day sent a copy to the Grand Duke, hoping to obtain the Grand Duke 's support as quickly as possible. On March 19, he sent the telescope he had used to first view Jupiter 's moons to the Grand Duke, along with an official copy of Sidereus Nuncius ( The Starry Messenger ) that, following the secretary 's advice, named the four moons the Medician Stars. In his dedicatory introduction, Galileo wrote : Scarcely have the immortal graces of your soul begun to shine forth on earth than bright stars offer themselves in the heavens which, like tongues, will speak of and celebrate your most excellent virtues for all time. Behold, therefore, four stars reserved for your illustrious name... which... make their journeys and orbits with a marvelous speed around the star of Jupiter... like children of the same family... Indeed, it appears the Maker of the Stars himself, by clear arguments, admonished me to call these new planets by the illustrious name of Your Highness before all others. Name A Jovilabe : an apparatus from the mid-18th century for demonstrating the orbits of Jupiter 's satellites Galileo initially called his discovery the Cosmica Sidera ( `` Cosimo 's stars '' ), in honour of Cosimo II de ' Medici ( 1590 -- 1621 ). At Cosimo 's suggestion, Galileo changed the name to Medicea Sidera ( `` the Medician stars '' ), honouring all four Medici brothers ( Cosimo, Francesco, Carlo, and Lorenzo ). The discovery was announced in the Sidereus Nuncius ( `` Starry Messenger '' ), published in Venice in March 1610, less than two months after the first observations. Other names put forward include : I. Principharus ( for the `` prince '' of Tuscany ), II. Victripharus ( after Vittoria della Rovere ), III. Cosmipharus ( after Cosimo de ' Medici ) and IV. Fernipharus ( after Duke Ferdinando de ' Medici ) -- by Giovanni Battista Hodierna, a disciple of Galileo and author of the first ephemerides ( Medicaeorum Ephemerides, 1656 ) ; Circulatores Jovis, or Jovis Comites -- by Johannes Hevelius ; Gardes, or Satellites ( from the Latin satelles, satellitis, meaning `` escorts '' ) -- by Jacques Ozanam. The names that eventually prevailed were chosen by Simon Marius, who discovered the moons independently at the same time as Galileo : he named them at the suggestion of Johannes Kepler after lovers of the god Zeus ( the Greek equivalent of Jupiter ) : Io, Europa, Ganymede and Callisto, in his Mundus Jovialis, published in 1614. Galileo steadfastly refused to use Marius ' names and invented as a result the numbering scheme that is still used nowadays, in parallel with proper moon names. The numbers run from Jupiter outward, thus I, II, III and IV for Io, Europa, Ganymede, and Callisto respectively. Galileo used this system in his notebooks but never actually published it. The numbered names ( Jupiter x ) were used until the mid-20th century when other inner moons were discovered, and Marius ' names became widely used. Determination of longitude See also : History of longitude Galileo was able to develop a method of determining longitude based on the timing of the orbits of the Galilean moons. The times of the eclipses of the moons could be precisely calculated in advance, and compared with local observations on land or on ship to determine the local time and hence longitude. The main problem with the technique was that it was difficult to observe the Galilean moons through a telescope on a moving ship ; a problem that Galileo tried to solve with the invention of the celatone. The method was used by Cassini and Picard to re-map France. Members Some models predict that there may have been several generations of Galilean satellites in Jupiter 's early history. Each generation of moons to have formed would have spiraled into Jupiter and been destroyed, due to tidal interactions with Jupiter 's proto - satellite disk, with new moons forming from the remaining debris. By the time the present generation formed, the gas in the proto - satellite disk had thinned out to the point that it no longer greatly interfered with the moons ' orbits. Other models suggest that Galilean satellites formed in a proto - satellite disk, in which formation timescales were comparable to or shorter than orbital migration timescales. Io is anhydrous and likely has an interior of rock and metal. Europa is thought to contain 8 % ice and water by mass with the remainder rock. These moons are, in increasing order of distance from Jupiter : Name Image Model of interior Diameter ( km ) Mass ( kg ) Density ( g / cm ) Semi-major axis ( km ) Orbital period ( d ) ( relative ) Inclination ( ° ) Eccentricity Io Jupiter I 7003366000000000000 ♠ 3660. 0 7003363740000000000 ♠ × 3637. 4 7003363060000000000 ♠ × 3630. 6 7022893000000000000 ♠ 8.93 × 10 7000352800000000000 ♠ 3.528 7005421800000000000 ♠ 421 800 1.769 ( 1 ) 0.050 0.0041 Europa Jupiter II 7003312160000000000 ♠ 3121. 6 7022480000000000000 ♠ 4.8 × 10 3.014 7005671100000000000 ♠ 671 100 3.551 ( 2 ) 0.471 0.0094 Ganymede Jupiter III 7003526820000000000 ♠ 5268. 2 7023148000000000000 ♠ 1.48 × 10 1.942 7006107040000000000 ♠ 1070400 7.155 ( 4 ) 0.204 0.0011 Callisto Jupiter IV 7003482060000000000 ♠ 4820. 6 7023108000000000000 ♠ 1.08 × 10 1.834 7006188270000000000 ♠ 1882700 16.69 ( 9.4 ) 0.205 0.0074 Further information : Moons of Jupiter Io Main article : Io ( moon ) Tupan Patera on Io Io ( Jupiter I ) is the innermost of the four Galilean moons of Jupiter and, with a diameter of 3642 kilometers, the fourth - largest moon in the Solar System. It was named after Io, a priestess of Hera who became one of the lovers of Zeus. Nevertheless, it was simply referred to as `` Jupiter I '', or `` The first satellite of Jupiter '', until the mid-20th century. With over 400 active volcanos, Io is the most geologically active object in the Solar System. Its surface is dotted with more than 100 mountains, some of which are taller than Earth 's Mount Everest. Unlike most satellites in the outer Solar System ( which have a thick coating of ice ), Io is primarily composed of silicate rock surrounding a molten iron or iron sulfide core. Although not proven, recent data from the Galileo orbiter indicate that Io might have its own magnetic field. Io has an extremely thin atmosphere made up mostly of sulfur dioxide ( SO ). If a surface data or collection vessel were to land on Io in the future, it would have to be extremely tough ( similar to the tank - like bodies of the Soviet Venera landers ) to survive the radiation and magnetic fields that originate from Jupiter. Europa Main article : Europa ( moon ) Europa Europa ( Jupiter II ), the second of the four Galilean moons, is the second closest to Jupiter and the smallest at 3121.6 kilometers in diameter, which is slightly smaller than the Moon. The name comes from a mythical Phoenician noblewoman, Europa, who was courted by Zeus and became the queen of Crete, though the name did not become widely used until the mid-20th century. It has a smooth and bright surface, with a layer of water surrounding the mantle of the planet, thought to be 100 kilometers thick. The smooth surface includes a layer of ice, while the bottom of the ice is theorized to be liquid water. The apparent youth and smoothness of the surface have led to the hypothesis that a water ocean exists beneath it, which could conceivably serve as an abode for extraterrestrial life. Heat energy from tidal flexing ensures that the ocean remains liquid and drives geological activity. Life may exist in Europa 's under - ice ocean. So far, there is no evidence that life exists on Europa, but the likely presence of liquid water has spurred calls to send a probe there. Recurring plume erupting from Europa. The prominent markings that criss - cross the moon seem to be mainly albedo features, which emphasize low topography. There are few craters on Europa because its surface is tectonically active and young. Some theories suggest that Jupiter 's gravity is causing these markings, as one side of Europa is constantly facing Jupiter. Also, volcanic water eruptions splitting the surface of Europa, and even geysers have been considered as a cause. The color of the markings, reddish - brown, is theorized to be caused by sulfur, but scientists can not confirm that, because no data collection devices have been sent to Europa. Europa is primarily made of silicate rock and likely has an iron core. It has a tenuous atmosphere composed primarily of oxygen. Ganymede Main article : Ganymede ( moon ) Ganymede Ganymede ( Jupiter III ), the third Galilean moon is named after the mythological Ganymede, cupbearer of the Greek gods and Zeus 's beloved. Ganymede is the largest natural satellite in the Solar System at 5262.4 kilometers in diameter, which makes it larger than the planet Mercury -- although only at about half of its mass since Ganymede is an icy world. It is the only satellite in the Solar System known to possess a magnetosphere, likely created through convection within the liquid iron core. Ganymede is composed primarily of silicate rock and water ice, and a salt - water ocean is believed to exist nearly 200 km below Ganymede 's surface, sandwiched between layers of ice. The metallic core of Ganymede suggests a greater heat at some time in its past than had previously been proposed. The surface is a mix of two types of terrain -- highly cratered dark regions and younger, but still ancient, regions with a large array of grooves and ridges. Ganymede has a high number of craters, but many are gone or barely visible due to its icy crust forming over them. The satellite has a thin oxygen atmosphere that includes O, O, and possibly O ( ozone ), and some atomic hydrogen. Callisto Main article : Callisto ( moon ) Callisto 's Valhalla impact crater as seen by Voyager Callisto ( Jupiter IV ) is the fourth and last Galilean moon, and is the second largest of the four, and at 4820.6 kilometers in diameter, it is the third largest moon in the Solar System, and barely smaller than Mercury, though only a third of the latter 's mass. It is named after the Greek mythological nymph Callisto, a lover of Zeus who was a daughter of the Arkadian King Lykaon and a hunting companion of the goddess Artemis. The moon does not form part of the orbital resonance that affects three inner Galilean satellites and thus does not experience appreciable tidal heating. Callisto is composed of approximately equal amounts of rock and ices, which makes it the least dense of the Galilean moons. It is one of the most heavily cratered satellites in the Solar System, and one major feature is a basin around 3000 km wide called Valhalla. Callisto is surrounded by an extremely thin atmosphere composed of carbon dioxide and probably molecular oxygen. Investigation revealed that Callisto may possibly have a subsurface ocean of liquid water at depths less than 300 kilometres. The likely presence of an ocean within Callisto indicates that it can or could harbour life. However, this is less likely than on nearby Europa. Callisto has long been considered the most suitable place for a human base for future exploration of the Jupiter system since it is furthest from the intense radiation of Jupiter. Comparative structure Comparison of ( a part of ) Jupiter and its four largest natural satellites Jovian Radiation Moon rem / day Io 3600 Europa 540 Ganymede 8 Callisto 0.01 Fluctuations in the orbits of the moons indicate that their mean density decreases with distance from Jupiter. Callisto, the outermost and least dense of the four, has a density intermediate between ice and rock whereas Io, the innermost and densest moon, has a density intermediate between rock and iron. Callisto has an ancient, heavily cratered and unaltered ice surface and the way it rotates indicates that its density is equally distributed, suggesting that it has no rocky or metallic core but consists of a homogeneous mix of rock and ice. This may well have been the original structure of all the moons. The rotation of the three inner moons, in contrast, indicates differentiation of their interiors with denser matter at the core and lighter matter above. They also reveal significant alteration of the surface. Ganymede reveals past tectonic movement of the ice surface which required partial melting of subsurface layers. Europa reveals more dynamic and recent movement of this nature, suggesting a thinner ice crust. Finally, Io, the innermost moon, has a sulfur surface, active volcanism and no sign of ice. All this evidence suggests that the nearer a moon is to Jupiter the hotter its interior. The current model is that the moons experience tidal heating as a result of the gravitational field of Jupiter in inverse proportion to the square of their distance from the giant planet. In all but Callisto this will have melted the interior ice, allowing rock and iron to sink to the interior and water to cover the surface. In Ganymede a thick and solid ice crust then formed. In warmer Europa a thinner more easily broken crust formed. In Io the heating is so extreme that all the rock has melted and water has long ago boiled out into space. Surface features of the four members at different levels of zoom in each row Size Galilean moons compared with other Solar System bodies, although pixel scale is not accurate at this resolution. Latest flyby Jupiter and Io Io Europa Ganymede Callisto Jupiter and Galilean moons circa 2007, imaged by New Horizons during flyby. ( greyscale colour ) Origin and Evolution The relative masses of the Jovian moons. Those smaller than Europa are not visible at this scale, and combined would only be visible at 100 × magnification. Jupiter 's regular satellites are believed to have formed from a circumplanetary disk, a ring of accreting gas and solid debris analogous to a protoplanetary disk. They may be the remnants of a score of Galilean - mass satellites that formed early in Jupiter 's history. Simulations suggest that, while the disk had a relatively high mass at any given moment, over time a substantial fraction ( several tenths of a percent ) of the mass of Jupiter captured from the Solar nebula was processed through it. However, the disk mass of only 2 % that of Jupiter is required to explain the existing satellites. Thus there may have been several generations of Galilean - mass satellites in Jupiter 's early history. Each generation of moons would have spiraled into Jupiter, due to drag from the disk, with new moons then forming from the new debris captured from the Solar nebula. By the time the present ( possibly fifth ) generation formed, the disk had thinned out to the point that it no longer greatly interfered with the moons ' orbits. The current Galilean moons were still affected, falling into and being partially protected by an orbital resonance which still exists for Io, Europa, and Ganymede. Ganymede 's larger mass means that it would have migrated inward at a faster rate than Europa or Io. Visibility Jupiter and its four Galilean moons as seen with an amateur telescope Jupiter with the Galilean moons -- Io, Ganymede, Europa, and Callisto ( near maximum elongation ), respectively -- and the full Moon as seen around conjunction on 10 April 2017 All four Galilean moons are bright enough to be viewed from Earth without a telescope, if they appear farther away from Jupiter. ( They are, however, easily visible with even low - powered binoculars. ) They have apparent magnitudes between 4.6 and 5.6 when Jupiter is in opposition with the Sun, and are about one unit of magnitude dimmer when Jupiter is in conjunction. The main difficulty in observing the moons from Earth is their proximity to Jupiter, since they are obscured by its brightness. The maximum angular separations of the moons are between 2 and 10 arcminutes from Jupiter, which is close to the limit of human visual acuity. Ganymede and Callisto, at their maximum separation, are the likeliest targets for potential naked - eye observation. Orbit animation GIF animation of the resonance of Io, Europa, and Ganymede The three inner Galilean moons revolve in a 1 : 2 : 4 resonance. See also Astronomy portal Moons of Jupiter Jupiter 's moons in fiction Colonization of the Jovian System References Jump up ^ Drake, Stillman ( 1978 ). Galileo At Work. Chicago : University of Chicago Press. ISBN 0 - 226 - 16226 - 5. ^ Jump up to : Galilei, Galileo, Sidereus Nuncius. Translated and prefaced by Albert Van Helden. Chicago & London : University of Chicago Press 1989, 14 -- 16 Jump up ^ Pasachoff, Jay M. ( 2015 ). `` Simon Marius 's Mundus Iovialis : 400th Anniversary in Galileo 's Shadow ''. Journal for the History of Astronomy. 46 ( 2 ) : 218 -- 234. Bibcode : 2015AAS... 22521505P. doi : 10.1177 / 0021828615585493. Jump up ^ Van Helden, Albert ( March 1974 ). `` The Telescope in the Seventeenth Century ''. Isis. The University of Chicago Press on behalf of The History of Science Society. 65 ( 1 ) : 38 -- 58. doi : 10.1086 / 351216. JSTOR 228880. Jump up ^ Galilei, Galileo ( 1610 ). The Starry Messenger ( PDF ). Venice. ISBN 0 - 374 - 37191 - 1. Archived ( PDF ) from the original on 2012 - 02 - 07. On the seventh day of January in this present date 1610... Jump up ^ `` Satellites of Jupiter ''. The Galileo Project. Rice University. 1995. Archived from the original on 4 February 2012. Retrieved 9 August 2007. Jump up ^ Zezong, Xi, `` The Discovery of Jupiter 's Satellite Made by Gan De 2000 years Before Galileo '', Chinese Physics 2 ( 3 ) ( 1982 ) : 664 -- 67. Jump up ^ `` Jovilabe ''. Museo Galileo. Archived from the original on 16 April 2015. Retrieved 15 April 2015. Jump up ^ Cosimo is the Italian form of the Greek name Cosmas itself deriving from cosmos ( whence the neuter plural adjective cosmica ). Sidera is the plural form of the Latin noun sidus `` star, constellation ''. Jump up ^ Annuaire de l'Observatoire royal de Bruxelles. L'Académie royale des sciences, des lettres et des beaux - arts de Belgique. 1879. p. 263. ^ Jump up to : Marazzini, C. ( 2005 ). `` The names of the satellites of Jupiter : from Galileo to Simon Marius ''. Lettere Italiana. 57 ( 3 ) : 391 -- 407. Jump up ^ Howse, Derek. Greenwich Time and the Discovery of the Longitude. Oxford : Oxford University Press, 1980, 12. Jump up ^ Howse, Derek ( 1997 ). Greenwich Time and the Longitude. Philip Wilson. pp. 26, 31. ^ Jump up to : Canup, Robin M. ; Ward, William R. ( 2008 - 12 - 30 ). Origin of Europa and the Galilean Satellites. University of Arizona Press. p. 59. arXiv : 0812.4995. Bibcode : 2009euro. book... 59C. ISBN 978 - 0 - 8165 - 2844 - 8. ^ Jump up to : Chown, Marcus ( 7 March 2009 ). `` Cannibalistic Jupiter ate its early moons ''. New Scientist. Archived from the original on 23 March 2009. Retrieved 18 March 2009. Jump up ^ d'Angelo, Gennaro ; Podolak, Morris ( 2015 ). `` Capture and Evolution of Planetesimals in Circumjovian Disks ''. The Astrophysical Journal. 806 ( 2 ) : 203. arXiv : 1504.04364. Bibcode : 2015ApJ... 806... 203D. doi : 10.1088 / 0004 - 637X / 806 / 2 / 203. Jump up ^ Computed using the IAU - MPC Satellites Ephemeris Service μ value Jump up ^ Moons of Jupiter Archived 2017 - 06 - 08 at the Wayback Machine. NASA Jump up ^ Computed from IAG Travaux 2001 Archived 2011 - 08 - 10 at WebCite. Jump up ^ Lopes, Rosaly M.C ; Kamp, Lucas W ; Smythe, William D ; Mouginis - Mark, Peter ; Kargel, Jeff ; Radebaugh, Jani ; Turtle, Elizabeth P ; Perry, Jason ; Williams, David A ; Carlson, R.W ; Douté, S. ; the Galileo NIMS ; SSI Teams ( 2004 ). `` Lava lakes on Io : Observations of Io 's volcanic activity from Galileo NIMS during the 2001 fly - bys ''. Icarus. 169 : 140 -- 74. Bibcode : 2004Icar... 169... 140L. doi : 10.1016 / j. icarus. 2003.11. 013. Jump up ^ Schenk, Paul ; Hargitai, Henrik ; Wilson, Ronda ; McEwen, Alfred ; Thomas, Peter ( 2001 ). `` The mountains of Io : Global and geological perspectives from Voyager and Galileo ''. Journal of Geophysical Research : Planets. 106 : 33201 -- 22. Bibcode : 2001JGR... 10633201S. doi : 10.1029 / 2000JE001408. Jump up ^ Porco, C.C. ; West, Robert A. ; McEwen, Alfred ; Del Genio, Anthony D. ; Ingersoll, Andrew P. ; Thomas, Peter ; Squyres, Steve ; Dones, Luke ; Murray, Carl D. ; Johnson, Torrence V. ; Burns, Joseph A. ; Brahic, Andre ; Neukum, Gerhard ; Veverka, Joseph ; Barbara, John M. ; Denk, Tilmann ; Evans, Michael ; Ferrier, Joseph J. ; Geissler, Paul ; Helfenstein, Paul ; Roatsch, Thomas ; Throop, Henry ; Tiscareno, Matthew ; Vasavada, Ashwin R. ( 2003 ). `` Cassini Imaging of Jupiter 's Atmosphere, Satellites, and Rings '' ( PDF ). Science. 299 ( 5612 ) : 1541 -- 7. Bibcode : 2003Sci... 299.1541 P. doi : 10.1126 / science. 1079462. PMID 12624258. Archived ( PDF ) from the original on 2017 - 09 - 22. Jump up ^ McEwen, A.S. ; Keszthelyi, L. ; Spencer, J.R. ; Schubert, G. ; Matson, D.L. ; Lopes - Gautier, R. ; Klaasen, K.P. ; Johnson, T.V. ; Head, J.W. ; Geissler, P. ; Fagents, S. ; Davies, A.G. ; Carr, M.H. ; Breneman, H.H. ; Belton, M.J.S. ( 1998 ). `` High - Temperature Silicate Volcanism on Jupiter 's Moon Io ''. Science. 281 ( 5373 ) : 87 -- 90. Bibcode : 1998Sci... 281... 87M. doi : 10.1126 / science. 281.5373. 87. PMID 9651251. Jump up ^ Fanale, F.P. ; Johnson, T.V. ; Matson, D.L. ( 1974 ). `` Io : A Surface Evaporite Deposit ? ''. Science. 186 ( 4167 ) : 922 -- 5. Bibcode : 1974Sci... 186... 922F. doi : 10.1126 / science. 186.4167. 922. PMID 17730914. Jump up ^ Hefler, Michael ( 2001 ). `` Europa : In Depth ''. NASA, Solar system Exploration. NASA, Jet Propulsion Laboratory. Archived from the original on 14 November 2015. Retrieved 9 August 2007. Jump up ^ Schenk, P.M. ; Chapman, C.R. ; Zahnle, K. ; Moore, J.M. ; Chapter 18 : Ages and Interiors : the Cratering Record of the Galilean Satellites, in Jupiter : The Planet, Satellites and Magnetosphere, Cambridge University Press, 2004 Jump up ^ Hamilton, C.J. `` Jupiter 's Moon Europa ''. Archived from the original on 2012 - 01 - 24. Jump up ^ Tritt, Charles S. ( 2002 ). `` Possibility of Life on Europa ''. Milwaukee School of Engineering. Archived from the original on 9 June 2007. Retrieved 10 August 2007. Jump up ^ `` Tidal Heating ''. geology.asu.edu. Archived from the original on 2006 - 03 - 29. Retrieved 2007 - 10 - 20. Jump up ^ Phillips, Cynthia ( 28 September 2006 ). `` Time for Europa ''. Space.com. Archived from the original on 24 January 2012. Retrieved 5 January 2014. Jump up ^ `` Hubble sees recurring plume erupting from Europa ''. www.spacetelescope.org. Archived from the original on 25 April 2017. Retrieved 24 April 2017. Jump up ^ Greenberg, Richard ; Geissler, Paul ; Hoppa, Gregory ; Tufts, B. Randall ; Durda, Daniel D. ; Pappalardo, Robert ; Head, James W. ; Greeley, Ronald ; Sullivan, Robert ; Carr, Michael H. ( 1998 ). `` Tectonic Processes on Europa : Tidal Stresses, Mechanical Response, and Visible Features ''. Icarus. 135 ( 1 ) : 64 -- 78. Bibcode : 1998Icar... 135... 64G. doi : 10.1006 / icar. 1998.5986. Jump up ^ Carlson, R.W. ; M.S. Anderson ( 2005 ). `` Distribution of hydrate on Europa : Further evidence for sulfuric acid hydrate ''. Icarus. 177 ( 2 ) : 461 -- 471. Bibcode : 2005Icar... 177... 461C. doi : 10.1016 / j. icarus. 2005.03. 026. Jump up ^ `` Satellites of Jupiter ''. The Galileo Project. Archived from the original on 2012 - 02 - 04. Retrieved 2007 - 11 - 24. Jump up ^ `` Ganymede ''. nineplanets.org. October 31, 1997. Archived from the original on February 4, 2012. Retrieved 2008 - 02 - 27. Jump up ^ Kivelson, M.G. ; Khurana, K.K. ; Volwerk, M. ( 2002 ). `` The Permanent and Inductive Magnetic Moments of Ganymede ''. Icarus. 157 ( 2 ) : 507 -- 22. Bibcode : 2002Icar... 157... 507K. doi : 10.1006 / icar. 2002.6834. Jump up ^ `` Solar System 's largest moon likely has a hidden ocean ''. Jet Propulsion Laboratory. NASA. 2000 - 12 - 16. Archived from the original on 2012 - 02 - 04. Retrieved 2008 - 01 - 11. Jump up ^ Hall, D.T. ; Feldman, P.D. ; McGrath, M.A. ; Strobel, D.F. ( 1998 ). `` The Far ‐ Ultraviolet Oxygen Airglow of Europa and Ganymede ''. The Astrophysical Journal. 499 : 475. Bibcode : 1998ApJ... 499... 475H. doi : 10.1086 / 305604. Jump up ^ Eviatar, Aharon ; m. Vasyliūnas, Vytenis ; a. Gurnett, Donald ( 2001 ). `` The ionosphere of Ganymede ''. Planetary and Space Science. 49 ( 3 -- 4 ) : 327 -- 36. Bibcode : 2001P&SS... 49... 327E. doi : 10.1016 / S0032 - 0633 ( 00 ) 00154 - 9. Jump up ^ Musotto, S ; Varadi, Ferenc ; Moore, William ; Schubert, Gerald ( 2002 ). `` Numerical Simulations of the Orbits of the Galilean Satellites ''. Icarus. 159 ( 2 ) : 500 -- 4. Bibcode : 2002Icar... 159... 500M. doi : 10.1006 / icar. 2002.6939. Jump up ^ Carlson, R.W. ( 1999 ). `` A Tenuous Carbon Dioxide Atmosphere on Jupiter 's Moon Callisto '' ( PDF ). Science. 283 ( 5403 ) : 820 -- 1. Bibcode : 1999Sci... 283... 820C. doi : 10.1126 / science. 283.5403. 820. hdl : 2014 / 16785. PMID 9933159. Archived ( PDF ) from the original on 2008 - 10 - 03. Jump up ^ Liang, Mao - Chang ; Lane, Benjamin F. ; Pappalardo, Robert T. ; Allen, Mark ; Yung, Yuk L. ( 2005 ). `` Atmosphere of Callisto ''. Journal of Geophysical Research. 110 : E02003. Bibcode : 2005JGRE... 110.2003 L. doi : 10.1029 / 2004JE002322. Jump up ^ Zimmer, C ; Khurana, Krishan K. ; Kivelson, Margaret G. ( 2000 ). `` Subsurface Oceans on Europa and Callisto : Constraints from Galileo Magnetometer Observations '' ( PDF ). Icarus. 147 ( 2 ) : 329 -- 47. Bibcode : 2000Icar... 147... 329Z. doi : 10.1006 / icar. 2000.6456. Archived ( PDF ) from the original on 2009 - 03 - 27. Jump up ^ Lipps, Jere H. ; Delory, Gregory ; Pitman, Joseph T. ; Rieboldt, Sarah ( 2004 ). `` Astrobiology of Jupiter 's icy moons ''. Instruments, Methods, and Missions for Astrobiology VIII. Instruments. Instruments, Methods, and Missions for Astrobiology VIII. 5555. p. 78. Bibcode : 2004SPIE. 5555... 78L. doi : 10.1117 / 12.560356. Jump up ^ Trautman, Pat ; Bethke, Kristen ( 2003 ). `` Revolutionary Concepts for Human Outer Planet Exploration ( HOPE ) '' ( PDF ). NASA. Archived from the original ( PDF ) on 2012 - 01 - 19. ^ Jump up to : Ringwald, Frederick A. ( 29 February 2000 ). `` SPS 1020 ( Introduction to Space Sciences ) ''. California State University, Fresno. Archived from the original on 20 September 2009. Retrieved 5 January 2014. ^ Jump up to : Canup, Robert M. ; Ward, William R. ( 2009 ). `` Origin of Europa and the Galilean Satellites ''. Europa. University of Arizona Press. pp. 59 -- 83. ISBN 978 - 0 - 8165 - 2844 - 8. Jump up ^ Alibert, Y. ; Mousis, O. ; Benz, W. ( 2005 ). `` Modeling the Jovian subnebula I. Thermodynamic conditions and migration of proto - satellites ''. Astronomy & Astrophysics. 439 ( 3 ) : 1205 -- 13. arXiv : astro - ph / 0505367. Bibcode : 2005A&A... 439.1205 A. doi : 10.1051 / 0004 - 6361 : 20052841. Jump up ^ Yeomans, Donald K. ( 2006 - 07 - 13 ). `` Planetary Satellite Physical Parameters ''. JPL Solar System Dynamics. Archived from the original on 2010 - 01 - 18. Retrieved 2008 - 08 - 23. Jump up ^ Jupiter is about 750 times brighter than Ganymede and about 2000 times brighter than Callisto. Ganymede : ( 5th root of 100 ) ^ ( 4.4 Ganymede APmag − ( − 2.8 Jup APmag ) ) = 758 Callisto : ( 5th root of 100 ) ^ ( 5.5 Callisto APmag − ( − 2.8 Jup APmag ) ) = 2089 Jump up ^ Jupiter near perihelion 2010 - Sep - 19 : 656.7 ( Callisto angular separation arcsec ) − 24.9 ( jup angular radius arcsec ) = 631 arcsec = 10 arcmin External links Animation of Galileo 's observation, march 1613 Sky & Telescope utility for identifying Galilean moons Wikimedia Commons has media related to Moons of Jupiter. Moons of Jupiter Listed in approximately increasing distance from Jupiter. Provisional designations in italics. Inner moons Metis Adrastea Amalthea Thebe Galilean moons Io Europa Ganymede Callisto Themisto group Themisto Himalia group Leda Himalia S / 2018 J 1 S / 2017 J 4 Lysithea Elara Dia Carpo group Carpo S / 2016 J 2 group S / 2016 J 2 Ananke group S / 2003 J 12 ( ? ) Euporie Jupiter LX Jupiter LV Jupiter LII Thelxinoe Euanthe Helike Orthosie S / 2017 J 7 Jupiter LIV S / 2017 J 3 Iocaste S / 2003 J 16 Praxidike Harpalyke Mneme Hermippe Thyone S / 2017 J 9 Ananke Carme group S / 2011 J 1 ( ? ) Herse Aitne Kale Taygete S / 2003 J 19 Chaldene S / 2003 J 10 ( ? ) Erinome Kallichore S / 2017 J 5 S / 2017 J 8 Kalyke Carme S / 2017 J 2 Pasithee Jupiter LI Eukelade Arche Isonoe S / 2003 J 9 Jupiter LVII Pasiphae group S / 2017 J 6 Jupiter LVIII S / 2003 J 23 Aoede Callirrhoe Eurydome Kore Cyllene Jupiter LVI Jupiter LIX S / 2003 J 4 ( ? ) Pasiphae Hegemone Sinope Sponde Autonoe Megaclite S / 2003 J 2 ( ? ) Rings of Jupiter In fiction Natural satellites of the Solar System Planetary satellites Terrestrial Martian Jovian Saturnian Uranian Neptunian Other satellites Minor - planet moons Plutonian Haumean Makemakean Eridian Largest satellites ( mean radius ≥ 100 km ) size Ganymede largest / 2634 km / 0.413 Earths Titan Callisto Io Moon Europa Triton Titania Rhea Oberon Iapetus Charon Umbriel Ariel Dione Tethys ( Dysnomia ) Enceladus Miranda Proteus Mimas ( Hi'iaka ) Nereid Hyperion Phoebe abc 's Ariel Callisto Charon Dione ( Dysnomia ) Enceladus Europa Ganymede ( Hi'iaka ) Hyperion Iapetus Io Mimas Miranda Moon Nereid Oberon Phoebe Proteus Rhea Tethys Titan Titania Triton Umbriel Discovery timeline Inner moons Irregular moons List Naming Regular moons Trojan moons NOTE : Italicized moons are not close to being in hydrostatic equilibrium ; ( bracketed ) moons may or may not be close to being in hydrostatic equilibrium. Jupiter Outline of Jupiter Geography Atmosphere Great Red Spot Magnetosphere Rings Moons Inner moons Adrastea Amalthea Metis Thebe Galilean moons Callisto Europa Ganymede Io Irregular moons Ananke group Carme group Himalia group Pasiphae group Ungrouped moons Carpo Themisto S / 2003 J 2 S / 2003 J 12 S / 2011 J 1 S / 2016 J 2 Astronomy General Jupiter - crossing minor planets Solar eclipses Trojans Greek camp Trojan camp Impact events Comet Shoemaker -- Levy 9 2009 Jupiter impact event 2010 Jupiter impact event Exploration and orbiting missions Current Juno Past Cassini Galileo New Horizons Pioneer program Pioneer 10 Pioneer 11 Ulysses Voyager program Voyager 1 Voyager 2 Future Jupiter Icy Moons Explorer ( 2022 ) Europa Clipper ( 2025 ) Proposed Io Volcano Observer ( 2021 ) Laplace - P ( 2023 ) Smara ( 2030 ) Related Fiction Jovian Jupiter Moons Mythology Book Portal The Solar System The Sun Mercury Venus Earth Mars Ceres Jupiter Saturn Uranus Neptune Pluto Haumea Makemake Eris Planets and Dwarf planets Terrestrial planets Mercury Venus Earth Mars Giant planets Jupiter Saturn Uranus Neptune Dwarf planets Ceres Pluto Haumea Makemake Eris Rings Jovian Saturnian ( Rhean ) Charikloan Chironean Uranian Neptunian Haumean Moons Terrestrial Moon other near - Earth objects Martian Phobos Deimos Jovian Ganymede Callisto Io Europa all 79 Saturnian Titan Rhea Iapetus Dione Tethys Enceladus Mimas Hyperion Phoebe all 62 Uranian Titania Oberon Umbriel Ariel Miranda all 27 Neptunian Triton Proteus Nereid all 14 Plutonian Charon Nix Hydra Kerberos Styx Haumean Hiʻiaka Namaka Makemakean S / 2015 ( 136472 ) 1 Eridian Dysnomia Lists Solar System objects By size By discovery date Minor planets Gravitationally rounded objects Possible dwarf planets Natural satellites Comets Small Solar System bodies Meteoroids Minor planets moons Comets Damocloids Mercury - crossers Venus - crossers Venus trojans Near - Earth objects Earth - crossers Earth trojans Mars - crossers Mars trojans Asteroid belt Asteroids first discovered : Ceres Pallas Juno Vesta Families Notable asteroids Kirkwood gap Main - belt comets Jupiter trojans Jupiter - crossers Centaurs Saturn - crossers Uranus trojans Uranus - crossers Neptune trojans Cis - Neptunian objects Trans - Neptunian objects Neptune - crossers Plutoids Kuiper belt Plutinos Cubewanos Scattered disc Detached objects Sednoids Hills cloud Oort cloud Hypothetical objects Vulcan Vulcanoids Phaeton Planet V Theia Fifth giant Planets beyond Neptune Tyche Nemesis Planet Nine Exploration ( outline ) Discovery Astronomy Timeline Spaceflight Robotic spacecraft Human spaceflight List of crewed spacecraft Colonization List of probes Timeline Mercury Venus Moon Mars Ceres Asteroids Mining Comets Jupiter Saturn Uranus Neptune Pluto Deep space Outline of the Solar System Portals Solar System Astronomy Earth sciences Mars Jupiter Uranus Cosmology Solar System → Local Interstellar Cloud → Local Bubble → Gould Belt → Orion Arm → Milky Way → Milky Way subgroup → Local Group → Virgo Supercluster → Laniakea Supercluster → Observable universe → Universe Each arrow ( → ) may be read as `` within '' or `` part of ''. Galileo Galilei Scientific career Observational astronomy Galileo affair Galileo 's escapement Galilean invariance Galilean moons Galilean transformation Leaning Tower of Pisa experiment Phases of Venus Celatone Thermoscope Works The Assayer De Motu Antiquiora Dialogue Concerning the Two Chief World Systems `` Discourse on the Tides '' `` Letter to the Grand Duchess Christina '' Sidereus Nuncius Two New Sciences Family Vincenzo Galilei ( father ) Michelagnolo Galilei ( brother ) Vincenzo Gamba ( son ) Maria Celeste ( daughter ) Marina Gamba ( mistress ) Related `` And yet it moves '' Villa Il Gioiello Galileo 's paradox Sector Museo Galileo Galileo 's telescopes Tribune of Galileo In popular culture Life of Galileo ( 1943 play ) Lamp At Midnight ( 1947 play ) Galileo ( 1968 film ) Galileo ( 1975 film ) Starry Messenger ( 1996 book ) Galileo 's Daughter : A Historical Memoir of Science, Faith, and Love ( 1999 book ) Galileo Galilei ( 2002 opera ) Galileo 's Dream ( 2009 novel ) Retrieved from `` https://en.wikipedia.org/w/index.php?title=Galilean_moons&oldid=852882485 '' Categories : Galilean moons Copernican Revolution Moons of Jupiter Hidden categories : Webarchive template wayback links Webarchive template webcite links Commons category with local link different than on Wikidata Good articles Talk Contents About Wikipedia Afrikaans Alemannisch Azərbaycanca Беларуская Български Brezhoneg Català Čeština Dansk Deutsch Ελληνικά Español Esperanto فارسی Français Gaeilge Galego 한국어 Հայերեն हिन्दी Hrvatski Bahasa Indonesia Íslenska Italiano עברית ქართული Latviešu Lëtzebuergesch Magyar मराठी Bahasa Melayu Nederlands 日本 語 Norsk Norsk nynorsk Occitan Plattdüütsch Polski Português Română Русский Scots සිංහල Simple English Slovenčina Српски / srpski Srpskohrvatski / српскохрватски Suomi Svenska தமிழ் Татарча / tatarça ไทย Тоҷикӣ Türkçe Українська Tiếng Việt 中文 49 more Edit links This page was last edited on 1 August 2018, at 00 : 45 ( UTC ). 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Question: of the four galilean moons which is the closest to jupiter
Answer: Io