Differential rotation is when a planet's equator and polar regions rotate at different rates.

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Differential rotation is a commonly observed phenomenon in the outer gas giants of the solar system, such as Jupiter and Saturn. The equator of these planets rotates faster than the polar regions, resulting in a noticeable bulge at the equator. Differential rotation is a real phenomenon that occurs on many planets in our solar system, including Jupiter, Saturn, and the Sun. The equator rotates faster than the polar regions, resulting in differential rotation.

Differential Rotation Is When a Planet's Equator and Polar Regions