Gravitation Inside Earth — Question 8

Section 13-4 · Physics pages 1966–1967

Question 8 An ideal diameter tunnel turns interior gravity into harmonic motion A narrow frictionless evacuated diameter tunnel is drilled through a uniform, nonrotating planet of radius R and surface gravity gs. Neglect removed mass. A particle is released from rest at one surface. You may use the solution x(t) = x0 cos(ωt) for ¨x = −ω2x. start Cross-section of a spherically symmetric mass distribution. (a) Find the motion and the time to reach the opposite surface. (b) Find the speed at the center and explain its mass independence.
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Question 8 - Solution An ideal diameter tunnel turns interior gravity into harmonic motion start (a) Derivation and calculation Inside a uniform planet, signed displacement x obeys ¨x = −gs R x = −ω2x, ω = √ gs/R. With x(0) = R and ˙x(0) = 0, x(t) = R cos(ωt) , topposite = π ω = π √ R/gs . (b) Result and interpretation Differentiating gives v(t) = −Rω sin(ωt). At the first center crossing, ωt = π/2, so |vcenter| = Rω = √ gsR . The particle mass cancels from m¨x = −mgsx/R, giving the same motion for every test mass. Physical check The speed vanishes at both surfaces and is greatest at the center; these conclusions require the ideal uniform, nonrotating planet.

Question 8

An ideal diameter tunnel turns interior gravity into harmonic motion

A narrow frictionless evacuated diameter tunnel is drilled through a uniform, nonrotating planet of radius RR and surface gravity gsg_s. Neglect removed mass. A particle is released from rest at one surface. You may use the solution x(t)=x0cos⁡(ωt)x(t)=x_0\cos(\omega t) for ẍ=−ω2x\ddot x=-\omega^2x.

Diagram shown in the original SVG worksheet.

  1. Find the motion and the time to reach the opposite surface.

  2. Find the speed at the center and explain its mass independence.

Question 8 - Solution

An ideal diameter tunnel turns interior gravity into harmonic motion

Diagram shown in the original SVG worksheet.

(a) Derivation and calculation

Inside a uniform planet, signed displacement xx obeys ẍ=−gsRx=−ω2x,ω=gs/R.\ddot x=-\frac{g_s}{R}x=-\omega^2x,\qquad \omega=\sqrt{g_s/R}. With x(0)=Rx(0)=R and ẋ(0)=0\dot x(0)=0, x(t)=Rcos⁡(ωt),topposite=πω=πR/gs.\boxed{x(t)=R\cos(\omega t)},\qquad \boxed{t_{\mathrm{opposite}}=\frac\pi\omega=\pi\sqrt{R/g_s}}.

(b) Result and interpretation

Differentiating gives v(t)=−Rωsin⁡(ωt).v(t)=-R\omega\sin(\omega t). At the first center crossing, ωt=π/2\omega t=\pi/2, so |vcenter|=Rω=gsR.\boxed{|v_{\mathrm{center}}|=R\omega=\sqrt{g_sR}}. The particle mass cancels from mẍ=−mgsx/Rm\ddot x=-mg_sx/R, giving the same motion for every test mass.

Physical check

The speed vanishes at both surfaces and is greatest at the center; these conclusions require the ideal uniform, nonrotating planet.