Gravitation and the Principle of Superposition — Question 10

Section 13-2 · Physics pages 1930–1931

Question 10 A force-free center does not make an extended detector force-free Two equal fixed sources M lie at x = ±a. A light rigid detector holds two equal test masses m at x = ±b, where 0 < b < a. Ignore their mutual gravity. M M m m Schematic; labels, not drawing lengths, specify the data. (a) Find the net gravitational force on the detector and the outward force on either end mass. (b) Find the tension the connecting rod must provide and its leading small-b form.
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Question 10 - Solution A force-free center does not make an extended detector force-free M M m m (a) Derivation and calculation At the right end, the nearer right source pulls more strongly: FR = GMm [ 1 (a −b)2 − 1 (a + b)2 ] = 4GMmab (a2 −b2)2 . Reflection symmetry gives FL = −FR, so Fnet = 0 , |Fend| = 4GMmab (a2 −b2)2 . (b) Result and interpretation To keep either end stationary, inward rod tension balances the outward force: T = 4GMmab (a2 −b2)2 . For b/a ≪1, T = 4GMmb a3 [1 −(b/a)2]−2 ≃4GMmb a3 . Zero net force permits nonzero internal tidal stress. Physical check Tension tends to zero with detector size and increases as either end approaches a source.

Question 10

A force-free center does not make an extended detector force-free

Two equal fixed sources MM lie at x=±ax=\pm a. A light rigid detector holds two equal test masses mm at x=±bx=\pm b, where 0<b<a0<b<a. Ignore their mutual gravity.

Diagram shown in the original SVG worksheet.

  1. Find the net gravitational force on the detector and the outward force on either end mass.

  2. Find the tension the connecting rod must provide and its leading small-bb form.

Question 10 - Solution

A force-free center does not make an extended detector force-free

Diagram shown in the original SVG worksheet.

(a) Derivation and calculation

At the right end, the nearer right source pulls more strongly: FR=GMm[1(a−b)2−1(a+b)2]=4GMmab(a2−b2)2.F_R=GMm\left[\frac1{(a-b)^2}-\frac1{(a+b)^2}\right] =\frac{4GMmab}{(a^2-b^2)^2}. Reflection symmetry gives FL=−FRF_L=-F_R, so Fnet=0,|Fend|=4GMmab(a2−b2)2.\boxed{F_{\mathrm{net}}=0},\qquad \boxed{|F_{\mathrm{end}}|=\frac{4GMmab}{(a^2-b^2)^2}}.

(b) Result and interpretation

To keep either end stationary, inward rod tension balances the outward force: T=4GMmab(a2−b2)2.\boxed{T=\frac{4GMmab}{(a^2-b^2)^2}}. For b/a≪1b/a\ll1, T=4GMmba3[1−(b/a)2]−2≃4GMmba3.T=\frac{4GMmb}{a^3}[1-(b/a)^2]^{-2} \simeq\boxed{\frac{4GMmb}{a^3}}. Zero net force permits nonzero internal tidal stress.

Physical check

Tension tends to zero with detector size and increases as either end approaches a source.