Ganymede is composed of silicate rock and water in approximately equal proportions. It is a fully differentiated body with an iron-rich, liquid core, and an internal ocean that potentially contains more water than all of Earth's oceans combined.[19][20][21][22] Its surface is composed of two main types of terrain.
The first of the two main surface types are the lighter regions, which are generally crosscut by extensive grooves and ridges, dating from slightly less than 4 billion years ago. They cover about two-thirds of Ganymede. The cause of the light terrain's disrupted geology is not fully known, but it is speculated that this may be the result of tectonic activity due to tidal heating. Next are the dark regions that cover about a third of Ganymede. These dark regions are saturated with impact craters and are dated to four billion years ago.[9] Ganymede orbits Jupiter in roughly seven days and is in a 1:2:4 orbital resonance with the moons Europa and Io, respectively.
Possessing a metallic core, it has the lowest moment of inertia factor of any solid body in the Solar System. Ganymede's magnetic field is probably created by convection within its liquid iron core, also created by Jupiter's tidal forces.[23] 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 oxygenatmosphere that includes O, O2, and possibly O3 (ozone).[17]Atomic hydrogen is a minor atmospheric constituent. Whether Ganymede has an ionosphere associated with its atmosphere is unresolved.[24]
Ganymede's discovery is credited to Simon Marius and Galileo Galilei, who both observed it in 1610,[2][g] as the third of the Galilean moons, the first group of objects discovered orbiting another planet.[26] Its name was soon suggested by astronomer Simon Marius, after the mythologicalGanymede, a Trojan prince desired by Zeus (the Greek counterpart of Jupiter), who carried him off to be the cupbearer of the gods.[27] Beginning with Pioneer 10, several spacecraft have explored Ganymede.[28] 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), which was launched in 2023.[29] After flybys of all three icy Galilean moons, it is planned to enter orbit around Ganymede.[30]
^ abGalilei, 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.
^"In Depth | Ganymede". NASA Solar System Exploration. Archived from the original on July 28, 2018. Retrieved June 16, 2021.
^Quinn Passey & 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.
^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.
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