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Question: There is a concentric hole of the radius \(R\) in a solid sphere of radius \(2R\) . Mass of the rema...

There is a concentric hole of the radius RR in a solid sphere of radius 2R2R . Mass of the remaining portion is MM . What is the gravitational potential at the center?

A) 5GM7R - \dfrac{{5GM}}{{7R}}
B) 7GM14R - \dfrac{{7GM}}{{14R}}
C) 3GM7R - \dfrac{{3GM}}{{7R}}
D) 9GM14R - \dfrac{{9GM}}{{14R}}

Explanation

Solution

To solve the above question you should be familiar with gravitational potential. Let us define gravitational potential first. The gravitational potential is defined as the work done to move a unit of mass from infinity to the gravitational field of another body. In the above question, the gravitational field is of the earth. We know the formula for the gravitational potential of a solid sphere at the center, that is, 3GM2R - \dfrac{{3GM}}{{2R}} , where MM is the mass of the solid sphere and RR is the radius of the sphere. But the problem here is that we are not concerned with a solid sphere. Therefore first we will calculate the mass of the remaining sphere of radius 2R2R and then that of the solid sphere of radius 2R2R. Once we get these two then we can easily calculate the desired gravitational potential.

Complete step by step solution:
Step 1: First calculate the mass of the remaining sphere of the radius 2R2R in terms of volume and density. Let us assume the density of the sphere is ρ\rho ,
M=ρ×V\therefore M = \rho \times V
We know that the volume of a sphere of the radius 2R2R will be 43π(2R)3\dfrac{4}{3}\pi {(2R)^3} . But the hole in the sphere is of the radius RR . Therefore we will subtract the volume of the hole from the volume of the solid sphere to get the volume of the remaining part.
M=ρ×43π[(2R)3R3]\therefore M = \rho \times \dfrac{4}{3}\pi [{(2R)^3} - {R^3}]
M=ρ×43π×7R3\Rightarrow M = \rho \times \dfrac{4}{3}\pi \times 7{R^3}
………… equation (1).
Step 2: Similarly calculate the mass of the solid sphere of the radius 2R2R in terms of volume and density. Let the mass of the solid sphere of radius 2R2R be MM' .
M=ρ×V2\therefore M' = \rho \times {V_2}
M=ρ×43π(2R)3\Rightarrow M' = \rho \times \dfrac{4}{3}\pi {(2R)^3}
M=ρ×43π×8R3\Rightarrow M' = \rho \times \dfrac{4}{3}\pi \times 8{R^3}
…………equation (2)
Step 3: Divide equation (2) by equation (1).
MM=87\therefore \dfrac{{M'}}{M} = \dfrac{8}{7}
M=87M\Rightarrow M' = \dfrac{8}{7}M
This is the mass of the solid sphere of radius 2R2R .
Step 4: To find the mass of the sphere of the radius RR of the same matter we will subtract the mass of the remaining part MMfrom the mass of the solid sphere of the radius 2R2R . Let the mass of the sphere of the radius RR is MM'' . then,
M=[87MM]\therefore M'' = - [\dfrac{8}{7}M - M]
M=17M\Rightarrow M'' = - \dfrac{1}{7}M
Here mass will be taken negatively because the negative mass is imposed.
Step 5: We know that the formula for the gravitational potential of a solid sphere is 3GM2R - \dfrac{{3GM}}{{2R}} . Therefore the gravitational potential of the remaining sphere UU will be
U=3GM2R3GM2R\therefore U = - \dfrac{{3GM'}}{{2R}} - \dfrac{{3GM''}}{{2R}}
U=3G2[M2R+MR]\Rightarrow U = - \dfrac{{3G}}{2}[\dfrac{{M'}}{{2R}} + \dfrac{{M''}}{R}]
Substitute the values of MM' and MM''
U=3G2[87M2R17MR]\therefore U = - \dfrac{{3G}}{2}\left[ {\dfrac{{\dfrac{8}{7}M}}{{2R}} - \dfrac{{\dfrac{1}{7}M}}{R}} \right]
U=3G2[4M7RM7R]\Rightarrow U = - \dfrac{{3G}}{2}\left[ {\dfrac{{4M}}{{7R}} - \dfrac{M}{{7R}}} \right]
U=9GM14R\Rightarrow U = - \dfrac{{9GM}}{{14R}}

Hence option D is correct.

Note: We know the formula for gravitational potential of only slandered shapes like sphere, circular disk, cube, etc. but in this case, the sphere was not solid. While solving this problem always remember that if you are taking the mass of the imagined sphere as negative then you have to add the gravitational potential of both. But if you are taking that mass as positive then you have to subtract the gravitational potential of the imagined sphere from the potential of the solid bigger sphere.