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Physics · Ch 7 — Gravitation

Variation of g Due to Rotation of the Earth

7.7

Variation of g Due to Rotation of the Earth

The Earth spins on its own axis once approximately every 2424 hours, and this rotation provides a third reason -- entirely separate from altitude or depth -- why the acceleration due to gravity actually measured (or felt as weight) at different points on the Earth's surface is not perfectly uniform.

Consider an object of mass mm resting on the Earth's surface at latitude λ\lambda (measured from the equator, so λ=0\lambda = 0 at the equator and λ=90∘\lambda = 90^\circ at either pole). Because the Earth is rotating, this object is not really at rest at all -- it is moving in a horizontal circle of radius Rcos⁡λR\cos\lambda about the Earth's rotation axis (this radius shrinks steadily from a maximum of RR at the equator down to zero exactly at the poles, where a point on the axis itself does not move in a circle at all). Moving in this circle at the Earth's own angular speed ω=2π/T\omega = 2\pi/T (with T≈24 hT \approx 24\ \text{h}) requires a net inward (centripetal) force of magnitude mω2(Rcos⁡λ)m\omega^2(R\cos\lambda), directed horizontally toward the rotation axis.

This required centripetal force is supplied by a small part of the true gravitational pull GMm/R2=mgGMm/R^2 = mg -- so the force the ground actually needs to supply upward on the object (its measured, apparent weight, mg′mg') is slightly LESS than the full gravitational pull mgmg, by exactly the component of that required centripetal force that acts along the local vertical (the radial direction at that latitude). Resolving the horizontal centripetal requirement mω2Rcos⁡λm\omega^2 R\cos\lambda along the local vertical introduces one further factor of cos⁡λ\cos\lambda, giving

mg′=mg−mω2Rcos⁡2λ⟹g′=g−ω2Rcos⁡2λmg' = mg - m\omega^2 R\cos^2\lambda \quad \Longrightarrow \quad g' = g - \omega^2 R\cos^2\lambda

Two limiting cases make the physical meaning of this formula clear:

  • At the equator (λ=0∘\lambda = 0^\circ, so cos⁡λ=1\cos\lambda = 1): g′=g−ω2Rg' = g - \omega^2 R, the MAXIMUM possible reduction, since the full radius RR is doing the swinging and the entire centripetal requirement acts straight along the local vertical.
  • At either pole (λ=90∘\lambda = 90^\circ, so cos⁡λ=0\cos\lambda = 0): g′=gg' = g, i.e. NO reduction at all -- a point exactly on the Earth's rotation axis does not move in a circle as the Earth spins, and so needs no centripetal force whatsoever. …