Space Science
Jupiter Science
JUPITER
JUPITER is the fifth planet from the
Sun and the innermost of the four giant planets. It is the largest and the most
massive planet, with a diameter of about 11 times that of the earth and a mass
about 2.5times the combined mass of seven other planets. Jupiter is thought to
have a small rocky core surrounded by an inner mantle of metallic hydrogen
(liquid hydrogen that acts like a metal). Outside the inner mantle is an outer
mantle of liquid hydrogen and helium that merges into the gaseous atmosphere.
Jupiter’s rapid rate of rotation causes the clouds in its atmosphere to form
belts and zones that encircle the planet parallel to the equator. Belts are
dark, low lying, relatively warm clouds layers, and zones are bright, and high
altitude, cooler clouds layers. Within the belts and zones, turbulence causes
the formation of cloud features such as white ovals and red spots, both of
which are huge storm system. The most prominent cloud feature is a storm called
the Great Red Spot, which consist of a spiralling column of clouds three times
wider than the Earth that rises about eight kilometres above the upper cloud
layer. Jupiter has a thin, faint, main ring, inside which is a tenuous halo
ring of tiny particles. Beyond the main ring’s outer edge is a broad and faint
two-part gossamer ring. There are 63b known Jovian Moons.
The four largest
Moons (called the Galileans) are Ganymede, and Callisto, Io, and Europa. Ganymede
and Callisto are cratered and icy. Europa is smooth and icy and is thought to
have a subsurface water ocean. Io is covered in bright red, orange, and yellow
splotches. This colouring is caused by sulphurous material from active
volcanoes that shoot plumes of lava hundreds of kilometres above the surface.



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