Gravitation Inside Earth — Question 4

Section 13-4 · Physics pages 1958–1959

Question 4 An outward-increasing density produces a quadratic interior field A spherical planet of radius R has density ρ(r) = ρ0r/R. Use dM = 4πr2ρ(r) dr and the shell theorem. r/R g/g(R) 1/2 1 1/4 1 Interior gravitational magnitude for the specified outward-increasing density. (a) Find enclosed mass, total mass and interior gravity. (b) Find g(R/2)/g(R) and explain why the uniform-density rule would fail.
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Question 4 - Solution An outward-increasing density produces a quadratic interior field r/R g/g(R) 1/2 1 1/4 1 (a) Derivation and calculation Integrate shells using a dummy radius s: M(r) = ∫r 0 4πs2ρ(s) ds = 4πρ0 R ∫r 0 s3 ds = πρ0r4 R . Consequently, M = πρ0R3 , g(r) = GM(r) r2 = πGρ0 R r2 . (b) Result and interpretation Normalizing by the surface value, g(R) = πGρ0R, g(r) g(R) = (r/R)2. g(R/2)/g(R) = 1/4 . The uniform-density rule would instead use M(r) ∝r3 and give 1/2; here M(r) ∝r4. Physical check The total mean density is 3ρ0/4, below the surface density ρ0.

Question 4

An outward-increasing density produces a quadratic interior field

A spherical planet of radius RR has density ρ(r)=ρ0r/R\rho(r)=\rho_0r/R. Use dM=4πr2ρ(r)drdM=4\pi r^2\rho(r)\,dr and the shell theorem.

Diagram shown in the original SVG worksheet.

  1. Find enclosed mass, total mass and interior gravity.

  2. Find g(R/2)/g(R)g(R/2)/g(R) and explain why the uniform-density rule would fail.

Question 4 - Solution

An outward-increasing density produces a quadratic interior field

Diagram shown in the original SVG worksheet.

(a) Derivation and calculation

Integrate shells using a dummy radius ss: M(r)=∫0r4πs2ρ(s)ds=4πρ0R∫0rs3ds=πρ0r4R.M(r)=\int_0^r4\pi s^2\rho(s)\,ds =\frac{4\pi\rho_0}{R}\int_0^rs^3\,ds =\frac{\pi\rho_0r^4}{R}. Consequently, M=πρ0R3,g(r)=GM(r)r2=πGρ0Rr2.\boxed{M=\pi\rho_0R^3},\qquad \boxed{g(r)=\frac{GM(r)}{r^2}=\frac{\pi G\rho_0}{R}r^2}.

(b) Result and interpretation

Normalizing by the surface value, g(R)=πGρ0R,g(r)g(R)=(r/R)2.g(R)=\pi G\rho_0R,\quad \frac{g(r)}{g(R)}=(r/R)^2. g(R/2)/g(R)=1/4.\boxed{g(R/2)/g(R)=1/4}. The uniform-density rule would instead use M(r)∝r3M(r)\propto r^3 and give 1/21/2; here M(r)∝r4M(r)\propto r^4.

Physical check

The total mean density is 3ρ0/43\rho_0/4, below the surface density ρ0\rho_0.