Q.

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
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a

12 : 9

b

16 : 9

c

12 : 11

d

11 : 10

answer is C.

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Detailed Solution

To determine the ratio F1:F2F_1 : F_2, we analyze the gravitational force acting on the mass mm before and after removing the smaller spherical part.

Step 1: Gravitational Force Before Removing the Small Sphere

The force F1F_1 is due to the entire sphere of mass MM and radius RR, and the mass mm is located at a distance 2R2R from the center.

The gravitational force due to a sphere acts as if the entire mass were concentrated at the center:

F1=GMm(2R)2F_1 = \frac{G M m}{(2R)^2}

 F1=GMm4R2F_1 = \frac{G M m}{4R^2}

Step 2: Gravitational Effect of the Removed Sphere

The removed sphere has a radius of R/3R/3. The mass of a sphere is proportional to the volume, so the mass MM' of the removed part is:

M=M×(volume of removed spherevolume of original sphere)M' = M \times \left(\frac{\text{volume of removed sphere}}{\text{volume of original sphere}}\right)

 M=M×(43π(R/3)343πR3)M' = M \times \left(\frac{\frac{4}{3} \pi (R/3)^3}{\frac{4}{3} \pi R^3}\right) 

M=M×(127)=M27M' = M \times \left(\frac{1}{27}\right) = \frac{M}{27}

Now, we calculate the gravitational force FF' due to this removed sphere on mm. The center of the removed sphere was at a distance RR from the center of the big sphere. The force due to this removed mass at 2R2R is:

F'=GM'm(R+R3)2=G(M/27)m169R2

 F'=GMm48R2

Step 3: Gravitational Force After Removing the Small Sphere

By the superposition principle, the net force F2F_2 due to the remaining part is:

F2=F1FF_2 = F_1 - F'

 F2=GMm4R2GMm48R2

 F2=444×48×GMmR2

Since F1=GMm4R2, the ratio F1:F2F_1 : F_2 is:

F1:F2=4×484×44=1211

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