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Jupiter[History | Information | Moons | Data] HistoryJupiter is named after the Roman king of the gods. It is more than twice
as massive as all the other planets in the solar system combined. InformationJupiter is a giant ball of hydrogen-based gasses whose density is only
slightly greater than water. Its surface clouds form alternating bands that spin in
opposite directions. White bands are known as zones and dark bands are known as belts.
They are caused by material rising from the center, cooling, and sinking back to the
center. This action takes place on earth also, just much slower (plate tectonics). The
coriolis effect on the surface causes the winds to spin in opposite directions. Organic
chemicals cause the color differences. MoonsJupiter has 16 named moons, 4 of which can be seen from Earth. These were
discovered by Galileo, and named the Galilean satellites: Io, Europa, Ganymede, and Callisto.
The moons of Jupiter mimicked the formation of the planets in the solar system, the
lighter moons farther out, the heavier ones close to the center.
[Top] Io: This moon is the most volcanically active of these 4 moons. The intense gravitational field of Jupiter pulls and distorts Io to such an extent that internal friction heats the planet up. The internal heat returns to the surface as volcanoes, which produces sulfur, making the surface reddish-orange. Europa: An icy crust covers the liquid mantle of this planet. Some scientists believe that this moon might be able to support life. Its surface was recently shown to contain a great deal of Epsom salts. Ganymede: This moon is the largest in the solar system, larger than the planet Mercury. Callisto: This is the last Galilean moon and is similar in composition to Ganymede but not as large. [Top] Data
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