Ganymede moon Language Watch Edit For other uses see Ganymede Ganymede a satellite of Jupiter Jupiter III is the largest and most massive of the Solar System s moons The ninth largest object in the Solar System it is the largest without a substantial atmosphere It has a diameter of 5 268 km 3 273 mi making it 26 larger than the planet Mercury by volume although it is only 45 as massive 16 Possessing a metallic core it has the lowest moment of inertia factor of any solid body in the Solar System and is the only moon known to have a magnetic field Outward from Jupiter it is the seventh satellite and the third of the Galilean moons the first group of objects discovered orbiting another planet 17 Ganymede orbits Jupiter in roughly seven days and is in a 1 2 4 orbital resonance with the moons Europa and Io respectively GanymedeGanymede photographed by Juno in 2021Discovery 1 2 Discovered byGalileo GalileiDiscovery dateJanuary 7 1610DesignationsPronunciation ˈ ɡ ae n ɪ m iː d 3 Named afterGanymhdhs GanymedesAlternative namesJupiter IIIAdjectivesGanymedian 4 Ganymedean 5 6 ɡ ae n ɪ ˈ m iː d i en Orbital characteristicsPeriapsis1069 200 km a Apoapsis1071 600 km b Semi major axis1070 400 km 7 Eccentricity0 0013 7 Orbital period7 154552 96 d 7 Average orbital speed10 880 km sInclination2 214 to the ecliptic 0 20 to Jupiter s equator 7 Satellite ofJupiterGroupGalilean moonPhysical characteristicsMean radius2634 1 0 3 km 0 413 Earths 8 Surface area8 72 107 km2 0 171 Earths c Volume7 66 1010 km3 0 0704 Earths d Mass1 4819 1023 kg 0 025 Earths 8 Mean density1 936 g cm3 8 Surface gravity1 428 m s2 0 146 g e Moment of inertia factor0 3115 0 0028 9 Escape velocity2 741 km s f Rotation periodsynchronousAxial tilt0 0 33 10 Albedo0 43 0 02 11 Surface temp min mean maxK 70 13 110 13 152 14 Apparent magnitude4 61 opposition 11 4 38 in 1951 12 AtmosphereSurface pressure0 2 1 2 µPa 15 Composition by volumeOxygen 15 Ganymede is composed of approximately equal amounts of silicate rock and water It is a fully differentiated body with an iron rich liquid core and an internal ocean that may contain more water than all of Earth s oceans combined 18 19 20 21 Its surface is composed of two main types of terrain Dark regions saturated with impact craters and dated to four billion years ago cover about a third of it Lighter regions crosscut by extensive grooves and ridges and only slightly less ancient cover the remainder The cause of the light terrain s disrupted geology is not fully known but was likely the result of tectonic activity due to tidal heating 8 Ganymede s magnetic field is probably created by convection within its liquid iron core 22 The meager magnetic field is buried within Jupiter s far larger magnetic field and would show only as a local perturbation of the field lines Ganymede has a thin oxygen atmosphere that includes O O2 and possibly O3 ozone 15 Atomic hydrogen is a minor atmospheric constituent Whether Ganymede has an ionosphere associated with its atmosphere is unresolved 23 Ganymede s discovery is credited to Galileo Galilei the first to observe it on January 7 1610 1 g Its name was soon suggested by astronomer Simon Marius after the mythological Ganymede a Trojan prince desired by Zeus the Greek counterpart of Jupiter who carried him off to be the cupbearer of the gods 25 Beginning with Pioneer 10 several spacecraft have explored Ganymede 26 The Voyager probes Voyager 1 and Voyager 2 refined measurements of its size while Galileo discovered its underground ocean and magnetic field The next planned mission to the Jovian system is the European Space Agency s Jupiter Icy Moon Explorer JUICE due to launch in 2022 After flybys of all three icy Galilean moons it is planned to enter orbit around Ganymede 27 Size comparison of Earth the Moon top left and Ganymede bottom left Contents 1 History 2 Name 3 Orbit and rotation 4 Physical characteristics 4 1 Size 4 2 Composition 4 3 Surface features 4 4 Internal structure 4 4 1 Subsurface oceans 4 4 2 Core 4 5 Atmosphere and ionosphere 4 6 Magnetosphere 4 7 Radiation environment 5 Origin and evolution 6 Exploration 6 1 Completed flybys 6 2 Future missions 6 3 Proposed missions 7 See also 8 Notes 9 References 10 External linksHistory EditChinese astronomical records report that in 365 BC Gan De detected what might have been a moon of Jupiter probably Ganymede with the naked eye 28 29 However Gan De reported the color of the companion as reddish which is puzzling since the moons are too faint for their color to be perceived with the naked eye 30 Shi Shen and Gan De together made fairly accurate observations of the five major planets 31 32 On January 7 1610 Galileo Galilei used a telescope to observe what he thought were three stars near Jupiter including what turned out to be Ganymede Callisto and one body that turned out to be the combined light from Io and Europa the next night he noticed that they had moved On January 13 he saw all four at once for the first time but had seen each of the moons before this date at least once By January 15 Galileo came to the conclusion that the stars were actually bodies orbiting Jupiter 1 2 g Name EditGalileo claimed the right to name the moons he d discovered He considered Cosmian Stars and settled on Medicean Stars in honor of Cosimo II de Medici 25 The French astronomer Nicolas Claude Fabri de Peiresc suggested individual names from the Medici family for the moons but his proposal was not taken up 25 Simon Marius who had originally claimed to have found the Galilean satellites 33 tried to name the moons the Saturn of Jupiter the Jupiter of Jupiter this was Ganymede the Venus of Jupiter and the Mercury of Jupiter another nomenclature that never caught on From a suggestion by Johannes Kepler Marius suggested a different naming system based on Greek mythology 25 Quin etiam impensius amavit Ganymedem puerum formosum Trois Regis filium adeo etiam assumpta aquilae figura illum humeris impositum in cœlum transportavit prout fabulantur poetae a me vocatur Tertius ob luminis Majestatem Ganymedes Io Europa Ganimedes puer atque Calisto lascivo nimium perplacuere Jovi Then there was Ganymede the handsome son of King Tros whom Jupiter having taken the form of an eagle transported to heaven on his back as poets fabulously tell The Third moon is called Ganymede by me on account of its majesty of light Io Europa the boy Ganymede and Callisto greatly pleased lustful Zeus 34 35 This name and those of the other Galilean satellites fell into disfavor for a considerable time and were not in common use until the mid 20th century In much of the earlier astronomical literature Ganymede is referred to instead by its Roman numeral designation Jupiter III a system introduced by Galileo in other words the third satellite of Jupiter Following the discovery of moons of Saturn a naming system based on that of Kepler and Marius was used for Jupiter s moons 25 Ganymede is the only Galilean moon of Jupiter named after a male figure like Io Europa and Callisto he was a lover of Zeus The Galilean satellites retain the Italian spellings of their names In the cases of Io Europa and Callisto these are identical to the Latin but the Latin form of Ganymede is Ganymedes In English the final e is silent perhaps under the influence of French unlike later names taken from Latin and Greek Orbit and rotation Edit Laplace resonance of Ganymede Europa and Io conjunctions are highlighted by color changes Ganymede orbits Jupiter at a distance of 1 070 400 km third among the Galilean satellites 17 and completes a revolution every seven days and three hours Like most known moons Ganymede is tidally locked with one side always facing toward the planet hence its day is seven days and three hours 36 Its orbit is very slightly eccentric and inclined to the Jovian equator with the eccentricity and inclination changing quasi periodically due to solar and planetary gravitational perturbations on a timescale of centuries The ranges of change are 0 0009 0 0022 and 0 05 0 32 respectively 37 These orbital variations cause the axial tilt the angle between rotational and orbital axes to vary between 0 and 0 33 10 Ganymede participates in orbital resonances with Europa and Io for every orbit of Ganymede Europa orbits twice and Io orbits four times 37 38 Conjunctions alignment on the same side of Jupiter between Io and Europa occur when Io is at periapsis and Europa at apoapsis Conjunctions between Europa and Ganymede occur when Europa is at periapsis 37 The longitudes of the Io Europa and Europa Ganymede conjunctions change with the same rate making triple conjunctions impossible Such a complicated resonance is called the Laplace resonance 39 The current Laplace resonance is unable to pump the orbital eccentricity of Ganymede to a higher value 39 The value of about 0 0013 is probably a remnant from a previous epoch when such pumping was possible 38 The Ganymedian orbital eccentricity is somewhat puzzling if it is not pumped now it should have decayed long ago due to the tidal dissipation in the interior of Ganymede 39 This means that the last episode of the eccentricity excitation happened only several hundred million years ago 39 Because Ganymede s orbital eccentricity is relatively low on average 0 0015 38 tidal heating is negligible now 39 However in the past Ganymede may have passed through one or more Laplace like resonances h that were able to pump the orbital eccentricity to a value as high as 0 01 0 02 8 39 This probably caused a significant tidal heating of the interior of Ganymede the formation of the grooved terrain may be a result of one or more heating episodes 8 39 There are two hypotheses for the origin of the Laplace resonance among Io Europa and Ganymede that it is primordial and has existed from the beginning of the Solar System 40 or that it developed after the formation of the Solar System A possible sequence of events for the latter scenario is as follows Io raised tides on Jupiter causing Io s orbit to expand due to conservation of momentum until it encountered the 2 1 resonance with Europa after that the expansion continued but some of the angular moment was transferred to Europa as the resonance caused its orbit to expand as well the process continued until Europa encountered the 2 1 resonance with Ganymede 39 Eventually the drift rates of conjunctions between all three moons were synchronized and locked in the Laplace resonance 39 Physical characteristics Edit Depiction of Ganymede centered over 45 W longitude dark areas are Perrine upper and Nicholson lower regiones prominent craters are Tros upper right and Cisti lower left Three high resolution views of Ganymede taken by Voyager 1 near closest approach on July 9 1979 Size Edit See also List of Solar System objects by size Ganymede is the largest and most massive moon in the Solar System 41 Its diameter of 5 268 km is 0 41 times that of Earth 0 77 times that of Mars 1 02 times that of Saturn s Titan Solar System s second largest moon 1 08 times Mercury s 1 09 times Callisto s 1 45 times Io s and 1 51 times the Moon s Its mass is 10 greater than Titan s 38 greater than Callisto s 66 greater than Io s and 2 02 times that of the Moon 42 Composition Edit The average density of Ganymede 1 936 g cm3 suggests a composition of about equal parts rocky material and mostly water ices 8 Some of the water is liquid forming an underground ocean 43 The mass fraction of ices is between 46 and 50 which is slightly lower than that in Callisto 44 Some additional volatile ices such as ammonia may also be present 44 45 The exact composition of Ganymede s rock is not known but is probably close to the composition of L LL type ordinary chondrites 44 which are characterized by less total iron less metallic iron and more iron oxide than H chondrites The weight ratio of iron to silicon ranges between 1 05 and 1 27 in Ganymede whereas the solar ratio is around 1 8 44 Surface features Edit See also List of geological features on Ganymede Ganymede Juno 7 June 2021 Ganymede dark side Juno 7 June 2021 Tros crater taken by Juno on 7 June 2021 Enhanced color Galileo spacecraft image of Ganymede s trailing hemisphere 46 The crater Tashmetum s prominent rays are at lower right and the large ejecta field of Hershef at upper right Part of dark Nicholson Regio is at lower left bounded on its upper right by Harpagia Sulcus Ganymede s surface has an albedo of about 43 47 Water ice seems to be ubiquitous on its surface with a mass fraction of 50 90 8 significantly more than in Ganymede as a whole Near infrared spectroscopy has revealed the presence of strong water ice absorption bands at wavelengths of 1 04 1 25 1 5 2 0 and 3 0 mm 47 The grooved terrain is brighter and has a more icy composition than the dark terrain 48 The analysis of high resolution near infrared and UV spectra obtained by the Galileo spacecraft and from Earth observations has revealed various non water materials carbon dioxide sulfur dioxide and possibly cyanogen hydrogen sulfate and various organic compounds 8 49 Galileo results have also shown magnesium sulfate MgSO4 and possibly sodium sulfate Na2SO4 on Ganymede s surface 36 50 These salts may originate from the subsurface ocean 50 The craters Gula and Achelous bottom in the grooved terrain of Ganymede with ejecta pedestals and ramparts The Ganymedian surface albedo is very asymmetric the leading hemisphere i is brighter than the trailing one 47 This is similar to Europa but the reverse for Callisto 47 The trailing hemisphere of Ganymede appears to be enriched in sulfur dioxide 51 52 The distribution of carbon dioxide does not demonstrate any hemispheric asymmetry although it is not observed near the poles 49 53 Impact craters on Ganymede except one do not show any enrichment in carbon dioxide which also distinguishes it from Callisto Ganymede s carbon dioxide gas was probably depleted in the past 53 Ganymede s surface is a mix of two types of terrain very old highly cratered dark regions and somewhat younger but still ancient lighter regions marked with an extensive array of grooves and ridges The dark terrain which comprises about one third of the surface 54 contains clays and organic materials that could indicate the composition of the impactors from which Jovian satellites accreted 55 The heating mechanism required for the formation of the grooved terrain on Ganymede is an unsolved problem in the planetary sciences The modern view is that the grooved terrain is mainly tectonic in nature 8 Cryovolcanism is thought to have played only a minor role if any 8 The forces that caused the strong stresses in the Ganymedian ice lithosphere necessary to initiate the tectonic activity may be connected to the tidal heating events in the past possibly caused when the satellite passed through unstable orbital resonances 8 56 The tidal flexing of the ice may have heated the interior and strained the lithosphere leading to the development of cracks and horst and graben faulting which erased the old dark terrain on 70 of the surface 8 57 The formation of the grooved terrain may also be connected with the early core formation and subsequent tidal heating of Ganymede s interior which may have caused a slight expansion of Ganymede by 1 6 due to phase transitions in ice and thermal expansion 8 During subsequent evolution deep hot water plumes may have risen from the core to the surface leading to the tectonic deformation of the lithosphere 58 Radiogenic heating within the satellite is the most relevant current heat source contributing for instance to ocean depth Research models have found that if the orbital eccentricity were an order of magnitude greater than currently as it may have been in the past tidal heating would be a more substantial heat source than radiogenic heating 59 Cratering is seen on both types of terrain but is especially extensive on the dark terrain it appears to be saturated with impact craters and has evolved largely through impact events 8 The brighter grooved terrain contains many fewer impact features which have been only of a minor importance to its tectonic evolution 8 The density of cratering indicates an age of 4 billion years for the dark terrain similar to the highlands of the Moon and a somewhat younger age for the grooved terrain but how much younger is uncertain 60 Ganymede may have experienced a period of heavy cratering 3 5 to 4 billion years ago similar to that of the Moon 60 If true the vast majority of impacts happened in that epoch whereas the cratering rate has been much smaller since 42 Craters both overlay and are crosscut by the groove systems indicating that some of the grooves are quite ancient Relatively young craters with rays of ejecta are also visible 42 61 Ganymedian craters are flatter than those on the Moon and Mercury This is probably due to the relatively weak nature of Ganymede s icy crust which can or could flow and thereby soften the relief Ancient craters whose relief has disappeared leave only a ghost of a crater known as a palimpsest 42 One significant feature on Ganymede is a dark plain named Galileo Regio which contains a series of concentric grooves or furrows likely created during a period of geologic activity 62 Ganymede also has polar caps likely composed of water frost The frost extends to 40 latitude 36 These polar caps were first seen by the Voyager spacecraft Theories on the formation of the caps include the migration of water to higher latitudes and bombardment of the ice by plasma Data from Galileo suggests the latter is correct 63 The presence of a magnetic field on Ganymede results in more intense charged particle bombardment of its surface in the unprotected polar regions sputtering then leads to redistribution of water molecules with frost migrating to locally colder areas within the polar terrain 63 A crater named Anat provides the reference point for measuring longitude on Ganymede By definition Anat is at 128 longitude 64 The 0 longitude directly faces Jupiter and unless stated otherwise longitude increases toward the west 65 Internal structure Edit Ganymede appears to be fully differentiated with an internal structure consisting of an iron sulfide iron core a silicate mantle and outer layers of water ice and liquid water 8 66 67 The precise thicknesses of the different layers in the interior of Ganymede depend on the assumed composition of silicates fraction of olivine and pyroxene and amount of sulfur in the core 44 66 68 Ganymede has the lowest moment of inertia factor 0 31 8 among the solid Solar System bodies This is a consequence of its substantial water content and fully differentiated interior Subsurface oceans Edit Artist s cut away representation of the internal structure of Ganymede Layers drawn to scale In the 1970s NASA scientists first suspected that Ganymede has a thick ocean between two layers of ice one on the surface and one beneath a liquid ocean and atop the rocky mantle 8 19 66 69 70 In the 1990s NASA s Galileo mission flew by Ganymede and found indications of such a subsurface ocean 43 An analysis published in 2014 taking into account the realistic thermodynamics for water and effects of salt suggests that Ganymede might have a stack of several ocean layers separated by different phases of ice with the lowest liquid layer adjacent to the rocky mantle 19 20 21 71 Water rock contact may be an important factor in the origin of life 19 The analysis also notes that the extreme depths involved 800 km to the rocky seafloor mean that temperatures at the bottom of a convective adiabatic ocean can be up to 40 K higher than those at the ice water interface In March 2015 scientists reported that measurements with the Hubble Space Telescope of how the aurorae moved confirmed that Ganymede has a subsurface ocean 43 A large salt water ocean affects Ganymede s magnetic field and consequently its aurora 18 71 72 73 The evidence suggests that Ganymede s oceans might be the largest in the entire Solar System 74 There is some speculation on the potential habitability of Ganymede s ocean 70 75 Core Edit The existence of a liquid iron nickel rich core 67 provides a natural explanation for the intrinsic magnetic field of Ganymede detected by Galileo spacecraft 76 The convection in the liquid iron which has high electrical conductivity is the most reasonable model of magnetic field generation 22 The density of the core is 5 5 6 g cm3 and the silicate mantle is 3 4 3 6 g cm3 44 66 68 76 The radius of this core may be up to 500 km 76 The temperature in the core of Ganymede is probably 1500 1700 K and pressure up to 10 GPa 99 000 atm 66 76 Atmosphere and ionosphere Edit In 1972 a team of Indian British and American astronomers working in Java Indonesia and Kavalur India claimed that they had detected a thin atmosphere during an occultation when it and Jupiter passed in front of a star 77 They estimated that the surface pressure was around 0 1 Pa 1 microbar 77 However in 1979 Voyager 1 observed an occultation of the star k Centauri during its flyby of Jupiter with differing results 78 The occultation measurements were conducted in the far ultraviolet spectrum at wavelengths shorter than 200 nm which were much more sensitive to the presence of gases than the 1972 measurements made in the visible spectrum No atmosphere was revealed by the Voyager data The upper limit on the surface particle number density was found to be 1 5 109 cm 3 which corresponds to a surface pressure of less than 2 5 µPa 25 picobar 78 The latter value is almost five orders of magnitude less than the 1972 estimate 78 False color temperature map of Ganymede Despite the Voyager data evidence for a tenuous oxygen atmosphere exosphere on Ganymede very similar to the one found on Europa was found by the Hubble Space Telescope HST in 1995 15 79 HST actually observed airglow of atomic oxygen in the far ultraviolet at the wavelengths 130 4 nm and 135 6 nm Such an airglow is excited when molecular oxygen is dissociated by electron impacts 15 which is evidence of a significant neutral atmosphere composed predominantly of O2 molecules The surface number density probably lies in the 1 2 7 108 cm 3 range corresponding to the surface pressure of 0 2 1 2 µPa 15 j These values are in agreement with the Voyager s upper limit set in 1981 The oxygen is not evidence of life it is thought to be produced when water ice on Ganymede s surface is split into hydrogen and oxygen by radiation with the hydrogen then being more rapidly lost due to its low atomic mass 79 The airglow observed over Ganymede is not spatially homogeneous like that over Europa HST observed two bright spots located in the northern and southern hemispheres near 50 latitude which is exactly the boundary between the open and closed field lines of the Ganymedian magnetosphere see below 80 The bright spots are probably polar auroras caused by plasma precipitation along the open field lines 81 The existence of a neutral atmosphere implies that an ionosphere should exist because oxygen molecules are ionized by the impacts of the energetic electrons coming from the magnetosphere 82 and by solar EUV radiation 23 However the nature of the Ganymedian ionosphere is as controversial as the nature of the atmosphere Some Galileo measurements found an elevated electron density near Ganymede suggesting an ionosphere whereas others failed to detect anything 23 The electron density near the surface is estimated by different sources to lie in the range 400 2 500 cm 3 23 As of 2008 the parameters of the ionosphere of Ganymede are not well constrained Additional evidence of the oxygen atmosphere comes from spectral detection of gases trapped in the ice at the surface of Ganymede The detection of ozone O3 bands was announced in 1996 83 In 1997 spectroscopic analysis revealed the dimer or diatomic absorption features of molecular oxygen Such an absorption can arise only if the oxygen is in a dense phase The best candidate is molecular oxygen trapped in ice The depth of the dimer absorption bands depends on latitude and longitude rather than on surface albedo they tend to decrease with increasing latitude on Ganymede whereas O3 shows an opposite trend 84 Laboratory work has found that O2 would not cluster or bubble but dissolve in ice at Ganymede s relatively warm surface temperature of 100 K 173 15 C 85 A search for sodium in the atmosphere just after such a finding on Europa turned up nothing in 1997 Sodium is at least 13 times less abundant around Ganymede than around Europa possibly because of a relative deficiency at the surface or because the magnetosphere fends off energetic particles 86 Another minor constituent of the Ganymedian atmosphere is atomic hydrogen Hydrogen atoms were observed as far as 3 000 km from Ganymede s surface Their density on the surface is about 1 5 104 cm 3 87 Magnetosphere Edit Magnetic field of the Jovian satellite Ganymede which is embedded into the magnetosphere of Jupiter Closed field lines are marked with green color The Galileo craft made six close flybys of Ganymede from 1995 to 2000 G1 G2 G7 G8 G28 and G29 22 and discovered that Ganymede has a permanent intrinsic magnetic moment independent of the Jovian magnetic field 88 The value of the moment is about 1 3 1013 T m3 22 which is three times larger than the magnetic moment of Mercury The magnetic dipole is tilted with respect to the rotational axis of Ganymede by 176 which means that it is directed against the Jovian magnetic moment 22 Its north pole lies below the orbital plane The dipole magnetic field created by this permanent moment has a strength of 719 2 nT at Ganymede s equator 22 which should be compared with the Jovian magnetic field at the distance of Ganymede about 120 nT 88 The equatorial field of Ganymede is directed against the Jovian field meaning reconnection is possible The intrinsic field strength at the poles is two times that at the equator 1440 nT 22 Aurorae on Ganymede auroral belt shifting may indicate a subsurface saline ocean The permanent magnetic moment carves a part of space around Ganymede creating a tiny magnetosphere embedded inside that of Jupiter it is the only moon in the Solar System known to possess the feature 88 Its diameter is 4 5 Ganymede radii 89 The Ganymedian magnetosphere has a region of closed field lines located below 30 latitude where charged particles electrons and ions are trapped creating a kind of radiation belt 89 The main ion species in the magnetosphere is single ionized oxygen O 23 which fits well with Ganymede s tenuous oxygen atmosphere In the polar cap regions at latitudes higher than 30 magnetic field lines are open connecting Ganymede with Jupiter s ionosphere 89 In these areas the energetic tens and hundreds of kiloelectronvolt electrons and ions have been detected 82 which may cause the auroras observed around the Ganymedian poles 80 In addition heavy ions precipitate continuously on Ganymede s polar surface sputtering and darkening the ice 82 The interaction between the Ganymedian magnetosphere and Jovian plasma is in many respects similar to that of the solar wind and Earth s magnetosphere 89 90 The plasma co rotating with Jupiter impinges on the trailing side of the Ganymedian magnetosphere much like the solar wind impinges on the Earth s magnetosphere The main difference is the speed of plasma flow supersonic in the case of Earth and subsonic in the case of Ganymede Because of the subsonic flow there is no bow shock off the trailing hemisphere of Ganymede 90 In addition to the intrinsic magnetic moment Ganymede has an induced dipole magnetic field 22 Its existence is connected with the variation of the Jovian magnetic field near Ganymede The induced moment is directed radially to or from Jupiter following the direction of the varying part of the planetary magnetic field The induced magnetic moment is an order of magnitude weaker than the intrinsic one The field strength of the induced field at the magnetic equator is about 60 nT half of that of the ambient Jovian field 22 The induced magnetic field of Ganymede is similar to those of Callisto and Europa indicating that Ganymede also has a subsurface water ocean with a high electrical conductivity 22 Given that Ganymede is completely differentiated and has a metallic core 8 76 its intrinsic magnetic field is probably generated in a similar fashion to the Earth s as a result of conducting material moving in the interior 22 76 The magnetic field detected around Ganymede is likely to be caused by compositional convection in the core 76 if the magnetic field is the product of dynamo action or magnetoconvection 22 91 Despite the presence of an iron core Ganymede s magnetosphere remains enigmatic particularly given that similar bodies lack the feature 8 Some research has suggested that given its relatively small size the core ought to have sufficiently cooled to the point where fluid motions hence a magnetic field would not be sustained One explanation is that the same orbital resonances proposed to have disrupted the surface also allowed the magnetic field to persist with Ganymede s eccentricity pumped and tidal heating of the mantle increased during such resonances reducing heat flow from the core leaving it fluid and convective 57 Another explanation is a remnant magnetization of silicate rocks in the mantle which is possible if the satellite had a more significant dynamo generated field in the past 8 Radiation environment Edit The radiation level at the surface of Ganymede is considerably lower than at Europa being 50 80 mSv 5 8 rem per day an amount that would cause severe illness or death in human beings exposed for two months 92 Origin and evolution Edit A sharp boundary divides the ancient dark terrain of Nicholson Regio from the younger finely striated bright terrain of Harpagia Sulcus Ganymede probably formed by an accretion in Jupiter s subnebula a disk of gas and dust surrounding Jupiter after its formation 93 The accretion of Ganymede probably took about 10 000 years 94 much shorter than the 100 000 years estimated for Callisto The Jovian subnebula may have been relatively gas starved when the Galilean satellites formed this would have allowed for the lengthy accretion times required for Callisto 93 In contrast Ganymede formed closer to Jupiter where the subnebula was denser which explains its shorter formation timescale 94 This relatively fast formation prevented the escape of accretional heat which may have led to ice melt and differentiation the separation of the rocks and ice The rocks settled to the center forming the core 67 In this respect Ganymede is different from Callisto which apparently failed to melt and differentiate early due to loss of the accretional heat during its slower formation 95 This hypothesis explains why the two Jovian moons look so dissimilar despite their similar mass and composition 69 95 Alternative theories explain Ganymede s greater internal heating on the basis of tidal flexing 96 or more intense pummeling by impactors during the Late Heavy Bombardment 97 98 99 100 In the latter case modeling suggests that differentiation would become a runaway process at Ganymede but not Callisto 99 100 After formation Ganymede s core largely retained the heat accumulated during accretion and differentiation only slowly releasing it to the ice mantle 95 The mantle in turn transported it to the surface by convection 69 The decay of radioactive elements within rocks further heated the core causing increased differentiation an inner iron iron sulfide core and a silicate mantle formed 76 95 With this Ganymede became a fully differentiated body 67 By comparison the radioactive heating of undifferentiated Callisto caused convection in its icy interior which effectively cooled it and prevented large scale melting of ice and rapid differentiation 101 The convective motions in Callisto have caused only a partial separation of rock and ice 101 Today Ganymede continues to cool slowly 76 The heat being released from its core and silicate mantle enables the subsurface ocean to exist 45 whereas the slow cooling of the liquid Fe FeS core causes convection and supports magnetic field generation 76 The current heat flux out of Ganymede is probably higher than that out of Callisto 95 Exploration EditSeveral spacecraft have performed close flybys of Ganymede four Pioneer and Voyager spacecraft made a single flyby each between 1973 and 1979 the Galileo spacecraft made six passes between 1996 and 2000 and the Juno spacecraft performed two flybys in 2019 and 2021 102 No spacecraft has yet orbited Ganymede but there have been multiple proposals to do so including the JUICE mission which is currently under construction as of 2021 update Completed flybys Edit Ganymede from Pioneer 10 1973 The first spacecraft to approach close to Ganymede was Pioneer 10 which performed a flyby in 1973 as it passed through the Jupiter system at high speed Pioneer 11 made a similar flyby in 1974 26 Data sent back by the two spacecraft was used to determine the moon s physical characteristics 103 and provided images of the surface with up to 400 km 250 mi resolution 104 Pioneer 10 s closest approach was 446 250 km about 85 times Ganymede s diameter 105 Voyager 1 and Voyager 2 both studied Ganymede when passing through the Jupiter system in 1979 Data from those flybys were used to refine the size of Ganymede revealing it was larger than Saturn s moon Titan which was previously thought to have been bigger 106 Images from the Voyagers provided the first views of the moon s grooved surface terrain 107 The Pioneer and Voyager flybys were all at large distances and high speeds as they flew on unbound trajectories through the Jupiter system Better data can be obtained from a spacecraft which is orbiting Jupiter as it can encounter Ganymede at a lower speed and adjust the orbit for a closer approach In 1995 the Galileo spacecraft entered orbit around Jupiter and between 1996 and 2000 made six close flybys of Ganymede 36 These flybys were denoted G1 G2 G7 G8 G28 and G29 22 During the closest flyby G2 Galileo passed just 264 km from the surface of Ganymede 5 of the moon s diameter 22 which remains the closest approach by any spacecraft During the G1 flyby in 1996 Galileo instruments detected Ganymede s magnetic field 108 Data from the Galileo flybys was used to discover the sub surface ocean which was announced in 2001 22 36 High spatial resolution spectra of Ganymede taken by Galileo were used to identify several non ice compounds on the surface 49 The New Horizons spacecraft also observed Ganymede but from a much larger distance as it passed through the Jupiter system in 2007 en route to Pluto The data were used to perform topographic and compositional mapping of Ganymede 109 110 Like Galileo the Juno spacecraft orbited around Jupiter On 2019 December 25 Juno performed a distant flyby of Ganymede during its 24th orbit of Jupiter at a range of 97 680 to 109 439 kilometers 60 696 to 68 002 mi This flyby provided images of the moon s polar regions 111 In June 2021 Juno performed a second flyby at a closer distance of 1 038 kilometers 645 mi 102 112 This encounter was designed to provide a gravity assist to reduce Juno s orbital period from 53 days to 43 days Additional images of the surface were collected 102 Future missions Edit The Jupiter Icy Moon Explorer JUICE will be the first to enter orbit around Ganymede itself As of 2021 update JUICE is under construction with launch planned for June 2022 It is intended to perform its first flyby of Ganymede in 2029 then enter orbit of the moon in 2032 It will de orbit and crash into Jupiter when the spacecraft fuel begins to run out probably in 2034 to avoid potential contamination of Ganymede s subsurface ocean a form of planetary protection 113 114 Proposed missions Edit A Voyager spaceprobe Several other missions have been proposed to flyby or orbit Ganymede but were either not selected for funding or cancelled before launch The Jupiter Icy Moons Orbiter would have studied Ganymede in greater detail 115 However the mission was canceled in 2005 116 Another old proposal was called The Grandeur of Ganymede 55 A Ganymede orbiter based on the Juno probe was proposed in 2010 for the Planetary Science Decadal Survey 117 The mission was not supported with the Decadal Survey preferring the Europa Clipper mission instead citation needed The Europa Jupiter System Mission EJSM had a proposed launch date in 2020 and was a joint NASA and ESA proposal for exploration of many of Jupiter s moons including Ganymede In February 2009 it was announced that ESA and NASA had given this mission priority ahead of the Titan Saturn System Mission 118 EJSM was to consist of the NASA led Jupiter Europa Orbiter the ESA led Jupiter Ganymede Orbiter and possibly a JAXA led Jupiter Magnetospheric Orbiter The NASA and JAXA components were later cancelled and ESA s appeared likely to be cancelled too 114 but in 2012 ESA announced it would go ahead alone The European part of the mission became the Jupiter Icy Moon Explorer JUICE see above 119 The Russian Space Research Institute proposed a Ganymede lander GL astrobiology mission called Laplace P 120 possibly in partnership with JUICE 120 121 If selected it would be launched in 2023 120 needs update See also Edit Solar System portal Astronomy portal Cold trap astronomy Jupiter s moons in fiction List of craters on Ganymede List of geological features on Ganymede List of natural satellites Lunar and Planetary InstituteNotes Edit Periapsis is derived from the semimajor axis a and eccentricity e a 1 e displaystyle a cdot 1 e Apoapsis is derived from the semimajor axis a and eccentricity e a 1 e displaystyle a cdot 1 e Surface area derived from the radius r 4 p r 2 displaystyle 4 pi r 2 Volume derived from the radius r 4 p r 3 3 displaystyle 4 pi r 3 3 Surface gravity derived from the mass m the gravitational constant G and the radius r G m r 2 displaystyle Gm r 2 Escape velocity derived from the mass m the gravitational constant G and the radius r 2 G m r displaystyle textstyle sqrt 2Gm r a b It is probable that the German astronomer Simon Marius discovered it independently the same year 24 A Laplace like resonance is similar to the current Laplace resonance among the Galilean moons with the only difference being that longitudes of the Io Europa and Europa Ganymede conjunctions change with rates whose ratio is a non unity rational number If the ratio is unity then the resonance is the Laplace resonance The leading hemisphere is the hemisphere facing the direction of orbital motion the trailing hemisphere faces the reverse direction The surface number density and pressure were calculated from the column densities reported in Hall et al 1998 assuming a scale height of 20 km and temperature 120 K References Edit a b c Galilei Galileo translated by Edward Carlos March 1610 Barker Peter ed Sidereus Nuncius PDF University of Oklahoma History of Science Archived from the original PDF on December 20 2005 Retrieved January 13 2010 a b In Depth Ganymede NASA Solar System Exploration Retrieved June 16 2021 Ganymede Oxford English Dictionary Online ed Oxford University Press Subscription or participating institution membership required Ganymede Merriam Webster Dictionary Quinn Passey amp E M Shoemaker 1982 Craters on Ganymede and Callisto in David Morrison ed Satellites of Jupiter vol 3 International Astronomical Union pp 385 386 411 Journal of Geophysical Research v 95 1990 E M Shoemaker et al 1982 Geology of Ganymede in David Morrison ed Satellites of Jupiter vol 3 International Astronomical Union pp 464 482 496 a b c d Planetary Satellite Mean Orbital Parameters Jet Propulsion Laboratory California Institute of Technology a b c d e f g h i j k l m n o p q r s t u v Showman Adam P Malhotra Renu October 1 1999 The Galilean Satellites PDF Science 286 5437 77 84 doi 10 1126 science 286 5437 77 PMID 10506564 Schubert G Anderson J D Spohn T McKinnon W B 2004 Interior composition structure and dynamics of the Galilean satellites In Bagenal F Dowling T E McKinnon W B eds Jupiter the planet satellites and magnetosphere New York Cambridge University Press pp 281 306 ISBN 978 0521035453 OCLC 54081598 a b Bills Bruce G 2005 Free and forced obliquities of the Galilean satellites of Jupiter Icarus 175 1 233 247 Bibcode 2005Icar 175 233B doi 10 1016 j icarus 2004 10 028 a b Yeomans Donald K July 13 2006 Planetary Satellite Physical Parameters JPL Solar System Dynamics Retrieved November 5 2007 Yeomans Chamberlin Horizon Online Ephemeris System for Ganymede Major Body 503 California Institute of Technology Jet Propulsion Laboratory Retrieved April 14 2010 4 38 on 1951 Oct 03 a b Delitsky Mona L Lane Arthur L 1998 Ice chemistry of Galilean satellites PDF J Geophys Res 103 E13 31 391 31 403 Bibcode 1998JGR 10331391D doi 10 1029 1998JE900020 Archived from the original PDF on October 3 2006 Orton G S Spencer G R et al 1996 Galileo Photopolarimeter radiometer observations of Jupiter and the Galilean Satellites Science 274 5286 389 391 Bibcode 1996Sci 274 389O doi 10 1126 science 274 5286 389 S2CID 128624870 a b c d e f Hall D T Feldman P D et al 1998 The Far Ultraviolet Oxygen Airglow of Europa and Ganymede The Astrophysical Journal 499 1 475 481 Bibcode 1998ApJ 499 475H doi 10 1086 305604 Ganymede Fact Sheet www2 jpl nasa gov Retrieved January 14 2010 a b Jupiter s Moons The Planetary Society Archived from the original on December 31 2007 a b Staff March 12 2015 NASA s Hubble Observations Suggest Underground Ocean on Jupiter s Largest Moon NASA News Retrieved March 15 2015 a b c d Clavin Whitney May 1 2014 Ganymede May Harbor Club Sandwich of Oceans and Ice NASA Jet Propulsion Laboratory Retrieved May 1 2014 a b Vance Steve Bouffard Mathieu Choukroun Mathieu Sotina Christophe April 12 2014 Ganymede s internal structure including thermodynamics of magnesium sulfate oceans in contact with ice Planetary and Space Science 96 62 70 Bibcode 2014P amp SS 96 62V doi 10 1016 j pss 2014 03 011 a b Staff May 1 2014 Video 00 51 Jupiter s Club Sandwich Moon NASA Retrieved May 2 2014 a b c d e f g h i j k l m n o Kivelson M G Khurana K K et al 2002 The Permanent and Inductive Magnetic Moments of Ganymede PDF Icarus 157 2 507 522 Bibcode 2002Icar 157 507K doi 10 1006 icar 2002 6834 hdl 2060 20020044825 a b c d e Eviatar Aharon Vasyliunas Vytenis M et al 2001 The ionosphere of Ganymede ps Planet Space Sci 49 3 4 327 336 Bibcode 2001P amp SS 49 327E doi 10 1016 S0032 0633 00 00154 9 Ganymede satellite of Jupiter Encyclopaedia Britannica Retrieved November 19 2019 a b c d e Satellites of Jupiter The Galileo Project Retrieved November 24 2007 a b Pioneer 11 Solar System Exploration Archived from the original on September 2 2011 Retrieved January 6 2008 Amos Jonathan May 2 2012 Esa selects 1bn euro Juice probe to Jupiter BBC News Retrieved May 2 2012 Chamberlain V D 1981 Astronomical content of American Plains Indian winter counts Bulletin of the Astronomical Society 13 793 Bibcode 1981BAAS 13 793C Brecher K 1981 Ancient Astronomy in Modern China Bulletin of the Astronomical Society 13 793 Bibcode 1981BAAS 13 793B Yi Long Huang 1997 Gan De In Helaine Selin ed Encyclopaedia of the history of science technology and medicine in non western cultures Springer p 342 ISBN 978 0 7923 4066 9 Yinke Deng March 3 2011 Ancient Chinese Inventions Cambridge University Press p 68 ISBN 978 0 521 18692 6 Xi Ze zong 1981 The Discovery of Jupiter s Satellite Made by Gan De 2000 Years Before Galileo Acta Astrophysica Sinica 1 2 87 Bibcode 1981AcApS 1 85X Retrieved March 22 2017 Discovery Cascadia Community College Archived from the original on September 20 2006 Retrieved November 24 2007 Marius Simon 1614 Mundus Iovialis anno MDCIX detectus ope perspicilli Belgici hoc est quatuor Jovialium planetarum cum theoria tum tabulae Nuremberg Sumptibus amp Typis Iohannis Lauri p B2 recto and verso images 35 and 36 with erratum on last page image 78 Retrieved June 30 2020 The Discovery of the Galilean Satellites Views of the Solar System Space Research Institute Russian Academy of Sciences Archived from the original on November 18 2007 Retrieved November 24 2007 a b c d e Miller Ron Hartmann William K May 2005 The Grand Tour A Traveler s Guide to the Solar System 3rd ed Thailand Workman Publishing pp 108 114 ISBN 978 0 7611 3547 0 a b c Musotto Susanna Varadi Ferenc Moore William Schubert Gerald 2002 Numerical Simulations of the Orbits of the Galilean Satellites Icarus 159 2 500 504 Bibcode 2002Icar 159 500M doi 10 1006 icar 2002 6939 a b c Phillips Cynthia October 3 2002 High Tide on Europa SPACE com Archived from the original on October 17 2002 a b c d e f g h i Showman Adam P Malhotra Renu 1997 Tidal Evolution into the Laplace Resonance and the Resurfacing of Ganymede PDF Icarus 127 1 93 111 Bibcode 1997Icar 127 93S doi 10 1006 icar 1996 5669 Peale S J Lee Man Hoi 2002 A Primordial Origin of the Laplace Relation Among the Galilean Satellites Science 298 5593 593 597 arXiv astro ph 0210589 Bibcode 2002Sci 298 593P doi 10 1126 science 1076557 PMID 12386333 S2CID 18590436 Ganymede NASA Solar System Exploration Retrieved June 15 2021 a b c d Ganymede nineplanets org October 31 1997 Retrieved February 27 2008 a b c Chang Kenneth March 12 2015 Suddenly It Seems Water Is Everywhere in Solar System New York Times Retrieved March 12 2015 a b c d e f Kuskov O L Kronrod V A 2005 Internal structure of Europa and Callisto Icarus 177 2 550 569 Bibcode 2005Icar 177 550K doi 10 1016 j icarus 2005 04 014 a b Spohn T Schubert G 2003 Oceans in the icy Galilean satellites of Jupiter PDF Icarus 161 2 456 467 Bibcode 2003Icar 161 456S doi 10 1016 S0019 1035 02 00048 9 Archived from the original PDF on February 27 2008 Galileo has successful flyby of Ganymede during eclipse Spaceflight Now Retrieved January 19 2008 a b c d Calvin Wendy M Clark Roger N Brown Robert H Spencer John R 1995 Spectra of the ice Galilean satellites from 0 2 to 5 µm A compilation new observations and a recent summary J Geophys Res 100 E9 19 041 19 048 Bibcode 1995JGR 10019041C doi 10 1029 94JE03349 Ganymede the Giant Moon Wayne RESA Archived from the original on December 2 2007 Retrieved December 31 2007 a b c McCord T B Hansen G V et al 1998 Non water ice constituents in the surface material of the icy Galilelean satellites from Galileo near infrared mapping spectrometer investigation J Geophys Res 103 E4 8 603 8 626 Bibcode 1998JGR 103 8603M doi 10 1029 98JE00788 a b McCord Thomas B Hansen Gary B Hibbitts Charles A 2001 Hydrated Salt Minerals on Ganymede s Surface Evidence of an Ocean Below Science 292 5521 1523 1525 Bibcode 2001Sci 292 1523M doi 10 1126 science 1059916 PMID 11375486 S2CID 40346198 Domingue Deborah Lane Arthur Moth Pimol 1996 Evidence from IUE for Spatial and Temporal Variations in the Surface Composition of the Icy Galilean Satellites Bulletin of the American Astronomical Society 28 1070 Bibcode 1996DPS 28 0404D Domingue Deborah L Lane Arthur L Beyer Ross A 1998 IEU s detection of tenuous SO2 frost on Ganymede and its rapid time variability Geophys Res Lett 25 16 3 117 3 120 Bibcode 1998GeoRL 25 3117D doi 10 1029 98GL02386 a b Hibbitts C A Pappalardo R Hansen G V McCord T B 2003 Carbon dioxide on Ganymede J Geophys Res 108 E5 5 036 Bibcode 2003JGRE 108 5036H doi 10 1029 2002JE001956 Patterson Wesley Head James W et al 2007 A Global Geologic Map of Ganymede PDF Lunar and Planetary Science XXXVIII 1098 a b Pappalardo R T Khurana K K Moore W B 2001 The Grandeur of Ganymede Suggested Goals for an Orbiter Mission PDF Lunar and Planetary Science XXXII 4062 Bibcode 2001iaop work 62P Showman Adam P Stevenson David J Malhotra Renu 1997 Coupled Orbital and Thermal Evolution of Ganymede PDF Icarus 129 2 367 383 Bibcode 1997Icar 129 367S doi 10 1006 icar 1997 5778 a b Bland Showman A P Tobie G March 2007 Ganymede s orbital and thermal evolution and its effect on magnetic field generation PDF Lunar and Planetary Society Conference 38 1338 2020 Bibcode 2007LPI 38 2020B Barr A C Pappalardo R T Pappalardo Stevenson 2001 Rise of Deep Melt into Ganymede s Ocean and Implications for Astrobiology PDF Lunar and Planetary Science Conference 32 1781 Bibcode 2001LPI 32 1781B Huffmann H et al 2004 Internal Structure and Tidal Heating of Ganymede PDF Geophysical Research Abstracts 6 a b Zahnle K Dones L 1998 Cratering Rates on the Galilean Satellites PDF Icarus 136 2 202 222 Bibcode 1998Icar 136 202Z doi 10 1006 icar 1998 6015 PMID 11878353 Archived from the original PDF on February 27 2008 Ganymede Lunar and Planetary Institute 1997 Casacchia R Strom R G 1984 Geologic evolution of Galileo Regio Journal of Geophysical Research 89 B419 B428 Bibcode 1984LPSC 14 419C doi 10 1029 JB089iS02p0B419 a b Khurana Krishan K Pappalardo Robert T Murphy Nate Denk Tilmann 2007 The origin of Ganymede s polar caps Icarus 191 1 193 202 Bibcode 2007Icar 191 193K doi 10 1016 j icarus 2007 04 022 USGS Astrogeology Rotation and pole position for planetary satellites IAU WGCCRE Archived from the original on October 24 2011 Retrieved August 28 2017 Planetary Names Target Coordinate Systems planetarynames wr usgs gov International Astronomical Union Archived from the original on May 27 2016 Retrieved May 21 2016 a b c d e Sohl F Spohn T Breuer D Nagel K 2002 Implications from Galileo Observations on the Interior Structure and Chemistry of the Galilean Satellites Icarus 157 1 104 119 Bibcode 2002Icar 157 104S doi 10 1006 icar 2002 6828 a b c d Bhatia G K Sahijpal S 2017 Thermal evolution of trans Neptunian objects icy satellites and minor icy planets in the early solar system Meteoritics amp Planetary Science 52 12 2470 2490 Bibcode 2017M amp PS 52 2470B doi 10 1111 maps 12952 a b Kuskov O L Kronrod V A Zhidikova A P 2005 Internal Structure of Icy Satellites of Jupiter PDF Geophysical Research Abstracts 7 p 01892 Bibcode 2010aogs 19 365K doi 10 1142 9789812838162 0028 ISBN 9789812838162 a b c Freeman J 2006 Non Newtonian stagnant lid convection and the thermal evolution of Ganymede and Callisto PDF Planetary and Space Science 54 1 2 14 Bibcode 2006P amp SS 54 2F doi 10 1016 j pss 2005 10 003 Archived from the original PDF on August 24 2007 a b Underground ocean on Jupiter s largest moon EarthSky March 15 2015 Retrieved August 14 2015 a b Hubble observations suggest underground ocean on Jupiter s largest moon Ganymede NASA PhysOrg March 12 2015 Retrieved March 13 2015 Underground ocean on Jupiter s largest moon Ganymede Saur Joachim Duling Stefan Roth Lorenz Jia Xianzhe Strobel Darrell F Feldman Paul D Christensen Ulrich R Retherford Kurt D McGrath Melissa A Musacchio Fabrizio Wennmacher Alexandre Neubauer Fritz M Simon Sven Hartkorn Oliver 2015 The Search for a Subsurface Ocean in Ganymede with Hubble Space Telescope Observations of its Auroral Ovals Journal of Geophysical Research Space Physics 120 3 1715 1737 Bibcode 2015JGRA 120 1715S doi 10 1002 2014JA020778 Wenz John October 4 2017 Overlooked Ocean Worlds Fill the Outer Solar System Scientific American Griffin Andrew March 13 2015 Ganymede oceans on Jupiter s moon could have been home to alien life The Independent Archived from the original on March 13 2015 Retrieved February 19 2018 a b c d e f g h i j Hauck Steven A Aurnou Jonathan M Dombard Andrew J 2006 Sulfur s impact on core evolution and magnetic field generation on Ganymede J Geophys Res 111 E9 E09008 Bibcode 2006JGRE 111 9008H doi 10 1029 2005JE002557 a b Carlson R W Bhattacharyya J C et al 1973 Atmosphere of Ganymede from its occultation of SAO 186800 on 7 June 1972 PDF Science 182 4107 53 5 Bibcode 1973Sci 182 53C doi 10 1126 science 182 4107 53 PMID 17829812 S2CID 33370778 a b c Broadfoot A L Sandel B R et al 1981 Overview of the Voyager Ultraviolet Spectrometry Results through Jupiter Encounter PDF Journal of Geophysical Research 86 A10 8259 8284 Bibcode 1981JGR 86 8259B doi 10 1029 JA086iA10p08259 a b Hubble Finds Thin Oxygen Atmosphere on Ganymede Jet Propulsion Laboratory NASA October 23 1996 Archived from the original on May 4 2009 Retrieved February 17 2017 a b Feldman Paul D McGrath Melissa A et al 2000 HST STIS Ultraviolet Imaging of Polar Aurora on Ganymede The Astrophysical Journal 535 2 1085 1090 arXiv astro ph 0003486 Bibcode 2000ApJ 535 1085F doi 10 1086 308889 S2CID 15558538 Johnson R E 1997 Polar Caps on Ganymede and Io Revisited Icarus 128 2 469 471 Bibcode 1997Icar 128 469J doi 10 1006 icar 1997 5746 a b c Paranicas C Paterson W R et al 1999 Energetic particles observations near Ganymede J Geophys Res 104 A8 17 459 17 469 Bibcode 1999JGR 10417459P doi 10 1029 1999JA900199 Noll Keith S Johnson Robert E et al July 1996 Detection of Ozone on Ganymede Science 273 5273 341 343 Bibcode 1996Sci 273 341N doi 10 1126 science 273 5273 341 PMID 8662517 S2CID 32074586 Calvin Wendy M Spencer John R December 1997 Latitudinal Distribution of O2 on Ganymede Observations with the Hubble Space Telescope Icarus 130 2 505 516 Bibcode 1997Icar 130 505C doi 10 1006 icar 1997 5842 Vidal R A et al 1997 Oxygen on Ganymede Laboratory Studies Science 276 5320 1839 1842 Bibcode 1997Sci 276 1839V doi 10 1126 science 276 5320 1839 PMID 9188525 S2CID 27378519 Brown Michael E 1997 A Search for a Sodium Atmosphere around Ganymede Icarus 126 1 236 238 Bibcode 1997Icar 126 236B CiteSeerX 10 1 1 24 7010 doi 10 1006 icar 1996 5675 Barth C A Hord C W et al 1997 Galileo ultraviolet spectrometer observations of atomic hydrogen in the atmosphere of Ganymede Geophys Res Lett 24 17 2147 2150 Bibcode 1997GeoRL 24 2147B doi 10 1029 97GL01927 S2CID 123038216 a b c Kivelson M G Khurana K K et al 1997 The magnetic field and magnetosphere of Ganymede PDF Geophys Res Lett 24 17 2155 2158 Bibcode 1997GeoRL 24 2155K doi 10 1029 97GL02201 a b c d Kivelson M G Warnecke J et al 1998 Ganymede s magnetosphere magnetometer overview PDF J Geophys Res 103 E9 19 963 19 972 Bibcode 1998JGR 10319963K doi 10 1029 98JE00227 a b Volwerk M Kivelson M G Khurana K K McPherron R L 1999 Probing Ganymede s magnetosphere with field line resonances PDF J Geophys Res 104 A7 14 729 14 738 Bibcode 1999JGR 10414729V doi 10 1029 1999JA900161 Hauck Steven A Dombard A J Solomon S C Aurnou J M 2002 Internal structure and mechanism of core convection on Ganymede PDF Lunar and Planetary Science XXXIII 1380 Bibcode 2002LPI 33 1380H Podzolko M V Getselev I V March 8 2013 Radiation Conditions of a Mission to Jupiterʼs Moon Ganymede International Colloquium and Workshop Ganymede Lander Scientific Goals and Experiments IKI Moscow Russia Moscow State University Retrieved January 6 2020 a b Canup Robin M Ward William R 2002 Formation of the Galilean Satellites Conditions of Accretion PDF The Astronomical Journal 124 6 3404 3423 Bibcode 2002AJ 124 3404C doi 10 1086 344684 a b Mosqueira Ignacio Estrada Paul R 2003 Formation of the regular satellites of giant planets in an extended gaseous nebula I subnebula model and accretion of satellites Icarus 163 1 198 231 Bibcode 2003Icar 163 198M doi 10 1016 S0019 1035 03 00076 9 a b c d e McKinnon William B 2006 On convection in ice I shells of outer Solar System bodies with detailed application to Callisto Icarus 183 2 435 450 Bibcode 2006Icar 183 435M doi 10 1016 j icarus 2006 03 004 Showman A P Malhotra R March 1997 Tidal evolution into the Laplace resonance and the resurfacing of Ganymede Icarus 127 1 93 111 Bibcode 1997Icar 127 93S doi 10 1006 icar 1996 5669 S2CID 55790129 Baldwin E January 25 2010 Comet impacts explain Ganymede Callisto dichotomy Astronomy Now Retrieved March 1 2010 Researchers offer explanation for the differences between Ganymede and Callisto moons Phys Org January 24 2010 Retrieved February 3 2017 a b Barr A C Canup R M March 2010 Origin of the Ganymede Callisto dichotomy by impacts during an outer solar system late heavy bombardment PDF 41st Lunar and Planetary Science Conference 2010 Houston Retrieved March 1 2010 a b Barr A C Canup R M January 24 2010 Origin of the Ganymede Callisto dichotomy by impacts during the late heavy bombardment PDF Nature Geoscience 3 March 2010 164 167 Bibcode 2010NatGe 3 164B doi 10 1038 NGEO746 a b Nagel K A Breuer D Spohn T 2004 A model for the interior structure evolution and differentiation of Callisto Icarus 169 2 402 412 Bibcode 2004Icar 169 402N doi 10 1016 j icarus 2003 12 019 a b c Chang Kenneth June 8 2021 NASA Just Visited the Solar System s Biggest Moon The Juno spacecraft completed a close flyby of Ganymede Jupiter s biggest moon as it transitions into a new phase of its mission The New York Times Retrieved June 10 2021 Exploration of Ganymede Terraformers Society of Canada Archived from the original on March 19 2007 Retrieved January 6 2008 Chapter 6 Results at the New Frontiers SP 349 396 Pioneer Odyssey NASA August 1974 Pioneer 10 Full Mission Timeline D Muller Archived from the original on July 23 2011 Retrieved May 25 2011 Voyager 1 and 2 ThinkQuest Archived from the original on December 26 2007 Retrieved January 6 2008 The Voyager Planetary Mission Views of the Solar System Archived from the original on February 3 2008 Retrieved January 6 2008 New Discoveries From Galileo Jet Propulsion Laboratory Retrieved January 6 2008 Pluto Bound New Horizons Spacecraft Gets A Boost From Jupiter Space Daily Retrieved January 6 2008 Grundy W M Buratti B J et al 2007 New Horizons Mapping of Europa and Ganymede Science 318 5848 234 237 Bibcode 2007Sci 318 234G doi 10 1126 science 1147623 PMID 17932288 S2CID 21071030 Ganymede Southwest Research Institute January 9 2020 Retrieved January 10 2020 Nasa spacecraft captures first closeups of Jupiter s largest moon in decades The Guardian Associated Press June 8 2021 Retrieved June 9 2021 Dougherty Grasset 2011 Jupiter Icy Moon Explorer PDF Parent page OPAG October 2011 Presentations a b Cosmic Vision 2015 2025 Proposals ESA July 21 2007 Retrieved February 20 2009 Jupiter Icy Moons Orbiter JIMO The Internet Encyclopedia of Science Retrieved January 6 2008 Peplow M February 8 2005 NASA budget kills Hubble telescope Nature doi 10 1038 news050207 4 Retrieved December 24 2011 Planetary Science Decadal Survey Mission amp Technology Studies Space Studies Board Ganymede Orbiter PDF Rincon Paul February 20 2009 Jupiter in space agencies sights BBC News Retrieved February 20 2009 ESA Selection of the L1 mission PDF ESA April 17 2012 Retrieved April 15 2014 a b c International Colloquium and Workshop Ganymede Lander scientific goals and experiments Russia Space Research Institute IKI Roscosmos November 2012 Retrieved November 20 2012 Amos Jonathan November 20 2012 Russia and Europe joint Mars bid agreement approved BBC News External links EditWikimedia Commons has media related to Ganymede moon Ganymede Profile at NASA s Solar System Exploration site Ganymede page at The Nine Planets Ganymede page at Views of the Solar System Ganymede Crater Database from the Lunar and Planetary Institute Images of Ganymede at JPL s Planetary Photojournal Movie of Ganymede s rotation from the National Oceanic and Atmospheric Administration Ganymede map from Scientific American article Ganymede map with feature names from Planetary Photojournal Ganymede nomenclature and Ganymede map with feature names from the USGS planetary nomenclature page Paul Schenk s 3D images and flyover videos of Ganymede and other outer solar system satellites Terraforming Ganymede with Robert A Heinlein part 1 article by Gregory Benford 2011 Part 2 Ganymede Orbiter Concept Global Geologic Map of Ganymede USGS Google Ganymede 3D interactive map of the moonRetrieved from https en wikipedia org w index php title Ganymede moon amp oldid 1028963828, wikipedia, wiki, book,


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