Gravitation Near Earth's Surface — Question 5

Section 13-3 · Physics pages 1940–1941

Question 5 Rotation tilts effective gravity away from the radial direction At latitude λ on a spherical rotating planet, use outward radial unit vector ˆr and northward tangent ˆλ. The centrifugal acceleration in the rotating frame has components Ω2R cos2 λ outward and −Ω2R sin λ cos λ northward. Gravitational acceleration is −g0ˆr. −ˆr −ˆλ⃗ geff β Local vector components at northern latitude; the equatorward tilt is exaggerated for clarity. (a) Find effective gravity and the small angle it makes with inward radial at northern latitudes. (b) At λ = 45◦and Ω2R/g0 = .004, calculate the tilt and its direction.
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Question 5 - Solution Rotation tilts effective gravity away from the radial direction −ˆr −ˆλ⃗ geff β (a) Derivation and calculation Adding gravitational and centrifugal accelerations gives⃗ geff= −(g0 −Ω2R cos2 λ)ˆr −Ω2R sin λ cos λ ˆλ . For positive inward radial component, define q = Ω2R/g0: tan β = q sin λ cos λ 1 −q cos2 λ, β ≃q sin λ cos λ (q ≪1). (b) Result and interpretation At 45◦, both sin λ cos λ and cos2 λ equal 1/2. Thus tan β = .004/2 1 −.004/2 = .002 .998. β = 0.00200401 rad = 0.114821◦. The negative northward component tilts the plumb direction toward the equator. Physical check The tilt vanishes at the equator and poles, and everywhere as Ω→0.

Question 5

Rotation tilts effective gravity away from the radial direction

At latitude λ\lambda on a spherical rotating planet, use outward radial unit vector r̂\hat r and northward tangent λ̂\hat\lambda. The centrifugal acceleration in the rotating frame has components Ω2Rcos⁡2λ\Omega^2R\cos^2\lambda outward and −Ω2Rsin⁡λcos⁡λ-\Omega^2R\sin\lambda\cos\lambda northward. Gravitational acceleration is −g0r̂-g_0\hat r.

Diagram shown in the original SVG worksheet.

  1. Find effective gravity and the small angle it makes with inward radial at northern latitudes.

  2. At λ=45∘\lambda=45^\circ and Ω2R/g0=.004\Omega^2R/g_0=.004, calculate the tilt and its direction.

Question 5 - Solution

Rotation tilts effective gravity away from the radial direction

Diagram shown in the original SVG worksheet.

(a) Derivation and calculation

Adding gravitational and centrifugal accelerations gives g→eff=−(g0−Ω2Rcos⁡2λ)r̂−Ω2Rsin⁡λcos⁡λλ̂.\boxed{\vec g_{\mathrm{eff}}=-(g_0-\Omega^2R\cos^2\lambda)\hat r -\Omega^2R\sin\lambda\cos\lambda\,\hat\lambda}. For positive inward radial component, define q=Ω2R/g0q=\Omega^2R/g_0: tan⁡β=qsin⁡λcos⁡λ1−qcos⁡2λ,β≃qsin⁡λcos⁡λ(q≪1).\tan\beta=\frac{q\sin\lambda\cos\lambda}{1-q\cos^2\lambda},\qquad \beta\simeq q\sin\lambda\cos\lambda\quad(q\ll1).

(b) Result and interpretation

At 45∘45^\circ, both sin⁡λcos⁡λ\sin\lambda\cos\lambda and cos⁡2λ\cos^2\lambda equal 1/21/2. Thus tan⁡β=.004/21−.004/2=.002.998.\tan\beta=\frac{.004/2}{1-.004/2}=\frac{.002}{.998}. β=0.00200401rad=0.114821∘.\boxed{\beta=0.00200401\ \mathrm{rad}=0.114821^\circ}. The negative northward component tilts the plumb direction toward the equator.

Physical check

The tilt vanishes at the equator and poles, and everywhere as Ω→0\Omega\to0.