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JEE Advanced 2014 · Gravitation

A planet of radius R=110×(radius of Earth)R = \frac{1}{10} \times (\text{radius of Earth}) has the same mass density as Earth. Scientists dig a well of depth R5\frac{R}{5} on it and lower a wire of the same length and a linear mass density 10−3 kg m−110^{-3}\,\text{kg m}^{-1} into it. If the wire is not touching anywhere, the force applied at the top of the wire by a person holding it in place is (take the radius of Earth =6×106 m= 6 \times 10^{6}\,\text{m} and the acceleration due to gravity on Earth is 10 ms−210\,\text{ms}^{-2})

Answer: B. 108 N108\,\text{N}

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Written solution

Step 1: Find the acceleration due to gravity at the surface of the planet.

The acceleration due to gravity at the surface of a planet with uniform mass density ρ\rho is given by:

gs=43πGρRg_s = \frac{4}{3}\pi G\rho R

Since the planet has the same mass density as Earth, the surface gravity is directly proportional to its radius:

gs=gE(RRE)g_s = g_E \left(\frac{R}{R_E}\right)

Substitute the given values gE=10 m/s2g_E = 10\text{ m/s}^2 and R=RE10R = \frac{R_E}{10}:

gs=10×110=1 m/s2g_s = 10 \times \frac{1}{10} = 1\text{ m/s}^2

Step 2: Express the acceleration due to gravity as a function of depth.

At a distance rr from the center of the planet (r≤Rr \le R), the acceleration due to gravity is:

g(r)=gsrRg(r) = g_s \frac{r}{R}

Let xx be the depth below the surface, so that r=R−xr = R - x:

g(x)=gs(1−xR)g(x) = g_s \left(1 - \frac{x}{R}\right)

Step 3: Set up the integral for the total weight of the wire.

The tension TT at the top of the wire is equal to the total gravitational force acting on the wire. For an infinitesimal element of length dxdx at depth xx, the mass is dm=λ dxdm = \lambda \, dx.

dT=g(x) dm=λgs(1−xR)dxdT = g(x) \, dm = \lambda g_s \left(1 - \frac{x}{R}\right) dx

Integrate from the surface x=0x = 0 to the bottom of the well x=R5x = \frac{R}{5}:

T=∫0R/5λgs(1−xR)dxT = \int_{0}^{R/5} \lambda g_s \left(1 - \frac{x}{R}\right) dx T=λgs[x−x22R]0R/5T = \lambda g_s \left[ x - \frac{x^2}{2R} \right]_{0}^{R/5} T=λgs(R5−R50)T = \lambda g_s \left(\frac{R}{5} - \frac{R}{50}\right) T=λgs9R50T = \lambda g_s \frac{9R}{50}

Step 4: Calculate the numerical value of the force.

The radius of the planet is:

R=RE10=6×10610=6×105 mR = \frac{R_E}{10} = \frac{6 \times 10^6}{10} = 6 \times 10^5\text{ m}

Substitute λ=10−3 kg/m\lambda = 10^{-3}\text{ kg/m}, gs=1 m/s2g_s = 1\text{ m/s}^2, and R=6×105 mR = 6 \times 10^5\text{ m} into the expression for TT:

T=10−3×1×9×6×10550T = 10^{-3} \times 1 \times \frac{9 \times 6 \times 10^5}{50} T=540050T = \frac{5400}{50} T=108 NT = 108\text{ N}

Answer: The force applied at the top of the wire to hold it in place is 108 N108\text{ N}.

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