Atmospheric super-rotation
State where a planet's atmosphere rotates faster than the planet itself / From Wikipedia, the free encyclopedia
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Atmospheric super-rotation is a phenomenon where a planet's atmosphere rotates faster than the planet itself. This behavior is observed in the atmosphere of Venus, atmosphere of Titan, atmosphere of Jupiter, and atmosphere of Saturn. Venus exhibits the most extreme super-rotation, with its atmosphere circling the planet in four Earth days, much faster than its planet's own rotation. The phenomenon of atmospheric super-rotation can influence a planet's climate and atmospheric dynamics.