Scientists accept that Jupiter is mainly composed of large quantities of hydrogen and helium. There is some consideration as to whether there is the presence of a solid rocky core that contains elements that are much heavier. The quick rotation of Jupiter pulls the planet into an oblate spheroid. This means that there is a bulging appearance about the planets equator. The outer atmosphere is divided into multiple bands at variant latitudes. Due to the movement of the planet and the location of these bands storms are produced where the bands converge with each other. As the boundaries of one band intersect with the boundaries of another closer band, the resulting interaction produces a hostile climate. The energy produced by the interaction is translated into storm like conditions. The most visible of these storms is the Great Red Spot. This storm was identified as early as the 17th century by astronomers in that age. The Great Red Spot therefore has had the benefit of centuries of inquiry into its existence. This has however produced a highly speculative environment for which recent missions of unmanned craft have provided clarity and guidance.
The most useful data on the great Red Spot of Jupiter have come from the mission of Pioneer 11 (Jupiter 2011). At its widest point the Great Red Spot is at least as three times the diameter of the planet earth, additionally the edge of the spot spins in a counter clockwise direction at an average speed of 225 miles per hour (Jupiter 2011). The storm is not a constant colour but changes hue and the change in hue is linked to two elements. The amount of sulfur and phosphorus in Jupiter's clouds determine the color of the Red Spot.
The storm has also been...
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