Equator To Poles Variation

Equator-to-poles variation describes how a physical quantity changes with latitude between Earth’s equator and poles, an important pattern in planetary physics and geophysics. For apparent gravitational acceleration, the variation results from Earth’s rotation, which produces a greatest centrifugal effect at the equator, and from Earth’s oblate shape, which places the poles closer to the planet’s center. Consequently, measured gravity is generally lower near the equator and higher near the poles. Understanding this latitude-dependent change improves gravimetric measurements, satellite orbit calculations, geodetic surveys, and models of Earth’s interior and global physical systems.

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