Gravitation Near Earth's Surface — Question 9

Section 13-3 · Physics pages 1948–1949

Question 9 Vertical free-fall separation grows because the lower body accelerates more Two small freely falling objects are initially separated vertically by ℓ≪R, close to the surface of a nonrotating spherical Earth. Their initial relative velocity is zero. Use g0 = 10 m/s2, R = 6.4 × 106 m and ℓ= 2 m. ℓ Local radial view; the lower object has the slightly greater downward acceleration. (a) Find their initial relative acceleration, keeping first order in ℓ/R. (b) Estimate the increase in separation after 1 s, over which field changes can be neglected.
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Question 9 - Solution Vertical free-fall separation grows because the lower body accelerates more ℓ (a) Derivation and calculation Take outward radial coordinate positive, so ar = −GM/r2. For separation ℓ, ¨ℓ≃dar dr ℓ= 2GM R3 ℓ= 2g0ℓ R . ¨ℓ= 2(10)(2) 6.4 × 106 = 6.25 × 10−6 m/s2 . (b) Result and interpretation With zero initial relative speed and approximately constant tidal acceleration, ∆ℓ≃1 2 ¨ℓt2 = 1 2(6.25 × 10−6)(1)2. ∆ℓ= 3.125 × 10−6 m = 3.125 µm . The lower particle falls faster, increasing their vertical separation. Physical check The fractional separation change is 1.5625 × 10−6, consistent with the short-time linearization.

Question 9

Vertical free-fall separation grows because the lower body accelerates more

Two small freely falling objects are initially separated vertically by ℓ≪R\ell\ll R, close to the surface of a nonrotating spherical Earth. Their initial relative velocity is zero. Use g0=10m/s2g_0=10\,\mathrm{m/s^2}, R=6.4×106mR=6.4\times10^6\,\mathrm m and ℓ=2m\ell=2\,\mathrm m.

Diagram shown in the original SVG worksheet.

  1. Find their initial relative acceleration, keeping first order in ℓ/R\ell/R.

  2. Estimate the increase in separation after 1s1\,\mathrm s, over which field changes can be neglected.

Question 9 - Solution

Vertical free-fall separation grows because the lower body accelerates more

Diagram shown in the original SVG worksheet.

(a) Derivation and calculation

Take outward radial coordinate positive, so ar=−GM/r2a_r=-GM/r^2. For separation ℓ\ell, ℓ̈≃dardrℓ=2GMR3ℓ=2g0ℓR.\ddot\ell\simeq\frac{da_r}{dr}\ell =\frac{2GM}{R^3}\ell=\frac{2g_0\ell}{R}. ℓ̈=2(10)(2)6.4×106=6.25×10−6m/s2.\boxed{\ddot\ell=\frac{2(10)(2)}{6.4\times10^6} =6.25\times10^{-6}\ \mathrm{m/s^2}}.

(b) Result and interpretation

With zero initial relative speed and approximately constant tidal acceleration, Δℓ≃12ℓ̈t2=12(6.25×10−6)(1)2.\Delta\ell\simeq\frac12\ddot\ell t^2 =\frac12(6.25\times10^{-6})(1)^2. Δℓ=3.125×10−6m=3.125μm.\boxed{\Delta\ell=3.125\times10^{-6}\ \mathrm m=3.125\ \mu\mathrm m}. The lower particle falls faster, increasing their vertical separation.

Physical check

The fractional separation change is 1.5625×10−61.5625\times10^{-6}, consistent with the short-time linearization.