A small point of mass m is placed at a distance 2R from the centre ‘O’ of a big uniform solid sphere of mass M and radius R. The gravitational force on ‘m’ due to M is F1. A spherical part of radius R/3 is removed from the big sphere as shown in the figure and the gravitational force on m due to remaining part of M is found to be F2. The value of ratio F1 : F2 is: (1) 16 : 9 (2) 11 : 10 (3) 12 : 11 (4) 12 : 9

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Published July 8, 2025
Physics
Gravitation
Newton's law of gravitation
Superposition principle
Cavity problems

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Detailed Explanation

Key Concepts

  1. Inverse-square law: F=GMmr2F = G \frac{M m}{r^{2}}
  2. Shell theorem: For any point outside a uniform solid sphere, the entire mass can be considered at the centre.
  3. Superposition (addition & subtraction): The net gravitational field equals the vector sum of fields produced by each mass element. If mass is removed, treat it as adding a negative mass at its own centre.

Logical chain to solve

  1. Whole sphere (before removal) Distance from point mass to centre O: 2R2R F1=GMm(2R)2=GMm4R2F_1 = G \frac{M m}{(2R)^2}=G \frac{M m}{4R^2}

  2. Describe the cavity Radius of cavity: R/3R/3
    Volume ratio: (R/3)3:R3=1:27(R/3)^3 : R^3 = 1:27
    Mass removed: M/27M/27 (since density is uniform).

  3. Locate the cavity centre (given/figure): on the line joining O and mm, at a distance 2R3\dfrac{2R}{3} from O.
    Distance from cavity centre to mm: (2R2R3)=4R3\bigl(2R - \frac{2R}{3}\bigr)=\frac{4R}{3}

  4. Force due to the removed part (take its mass as negative):

    Fcav=G(M/27)m(4R3)2=GMm48R2F_{\text{cav}}= G\frac{(M/27)m}{\left(\dfrac{4R}{3}\right)^2}=G\frac{M m}{48R^2} (direction is the same as F1F_1 toward O).

  5. Subtract to find the new force

    F2=F1Fcav=GMm4R2GMm48R2=GMmR2(14148)=GMmR21148F_2 = F_1 - F_{\text{cav}} = G\frac{M m}{4R^2}-G\frac{M m}{48R^2}=G\frac{M m}{R^2}\left(\frac{1}{4}-\frac{1}{48}\right)=G\frac{M m}{R^2}\frac{11}{48}

  6. Ratio

    F1:F2=1248:1148=12:11F_1:F_2 = \frac{12}{48} : \frac{11}{48} = 12 : 11

Simple Explanation (ELI5)

What’s happening?

Imagine you have a huge, perfectly round laddu (the big sphere) that pulls a tiny chocolate chip (the small mass mm) toward its centre because of gravity.

  1. First case: The laddu is whole, so the pull (force) is F1F_1.
  2. Second case: You scoop out a small ball–shaped bite (a cavity) from the laddu. Now the remaining laddu pulls the chip with a slightly different force, F2F_2.

Because every bit of the laddu attracts the chip, removing some dough means subtracting that little bit of attraction. We use the idea that a sphere attracts as if all its weight was concentrated at its centre. The scoop you removed also acted like a mini-laddu whose pull you now have to ‘take away’.
So, F2F_2 is just

pull of whole laddu minus pull of the scooped-out bite.

Do the maths carefully and the numbers turn out so that the first force (F1F_1) and the new force (F2F_2) are in the ratio 12 : 11.

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Step-by-Step Solution

Step-by-step Calculation

  1. Force before removing the cavity

    F1=GMm(2R)2=GMm4R2F_1 = G\frac{M m}{(2R)^2}=G\frac{M m}{4R^{2}}

  2. Mass of the removed sphere

    Mcav=ρ(4π3)(R3)3=127MM_{\text{cav}} = \rho \cdot \left(\frac{4\pi}{3}\right)\left(\frac{R}{3}\right)^3 = \frac{1}{27}\,M

  3. Distance of point mass from cavity centre

    rcav=2R2R3=4R3r_{\text{cav}} = 2R - \frac{2R}{3} = \frac{4R}{3}

  4. Force that the cavity alone would exert

    Fcav=G(M27)m(4R3)2=GMm48R2F_{\text{cav}} = G\frac{\left(\frac{M}{27}\right)m}{\left(\dfrac{4R}{3}\right)^2} = G\frac{M m}{48R^{2}}

  5. Net force after cavity is removed

    F2=F1Fcav=GMm4R2GMm48R2=GMmR2(14148)=GMmR21148F_2 = F_1 - F_{\text{cav}} = G\frac{M m}{4R^{2}} - G\frac{M m}{48R^{2}} = G\frac{M m}{R^{2}}\left(\frac{1}{4}-\frac{1}{48}\right)=G\frac{M m}{R^{2}}\frac{11}{48}

  6. Ratio

    F1:F2=1248:1148=12:11F_1:F_2 = \frac{12}{48} : \frac{11}{48} = 12:11

Hence the correct option is (3) 12 : 11.

Examples

Example 1

Designing artificial gravity gradients in space stations by adding/removing mass segments

Example 2

Detecting underground caves (lower density cavities) via gravimetric surveys

Example 3

Calculating net electrostatic field when a small charged hole is drilled in a conductor

Example 4

Finding magnetic field inside a cylindrical cavity carved in a uniformly magnetised material

Example 5

Gravitational balancing of Lagrange–point satellites by accounting for missing Earth mass near mountain ranges

Visual Representation

References

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