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Physics · Ch 3 — Laws of Motion

Centrifugal Force due to Rotation of the Earth

3.7.6

Centrifugal Force due to Rotation of the Earth

Although the Earth is usually treated as (approximately) an inertial frame, it is strictly non-inertial — it spins about its own axis with angular velocity ω=2πT\omega=\dfrac{2\pi}{T} (T≈24T\approx24 hours ≈86,400\approx86{,}400 s, so ω≈7.27×10−5 rad s−1\omega\approx7.27\times10^{-5}\text{ rad s}^{-1}). Any object resting on the Earth's surface therefore experiences a small outward centrifugal force, directed perpendicular to (and away from) the Earth's rotation axis.

For a person of mass mm standing at latitude φ\varphi, the perpendicular distance from the rotation axis is r=Rcos⁡φr=R\cos\varphi (RR = Earth's radius), so the centrifugal force is

Fc=mω2Rcos⁡φ.F_c=m\omega^2R\cos\varphi.

This is largest at the equator (φ=0°\varphi=0°, r=Rr=R, maximum) and zero at the poles (φ=90°\varphi=90°, r=0r=0). For a 60 kg60\text{ kg} person at Chennai (latitude ≈13°\approx13°):

Fc≈60×(7.27×10−5)2×6.4×106×cos⁡13°≈1.97 NF_c\approx60\times(7.27\times10^{-5})^2\times6.4\times10^6\times\cos13°\approx1.97\text{ N} …