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NCERT Exemplar · Q39

Q.A tunnel is dug through the centre of the Earth. Show that a body of mass 'mm' when dropped from rest from one end of the tunnel will execute simple harmonic motion.

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A body dropped through a tunnel across the Earth experiences a restoring force proportional to its displacement from the centre — exactly the condition for simple harmonic motion — with a period of about 84 minutes.

The key insight is that only the mass of the Earth inside the body's current radius pulls on it. Outside that radius, the shell of Earth above cancels its own gravity — a result of Newton's shell theorem. So as the body falls toward the centre, the gravitational force shrinks linearly with distance, not as 1/r21/r^2. That linear restoring force is the hallmark of SHM.

Let's work through it.

  1. Set up the problem.

    Earth is a uniform sphere of radius RR and mass MM. A tunnel is drilled straight through the centre, from one surface to the other. A body of mass mm is dropped from rest at the surface (r=Rr = R). We want to show its motion is SHM.

  2. Gravitational force inside a uniform sphere.

    For a point at distance rr from the centre (r≤Rr \le R), the gravitational force on mm is due only to the mass MrM_r enclosed within radius rr. By the shell theorem, the spherical shell outside rr contributes zero net force.

    The enclosed mass is proportional to volume:

Mr=M⋅r3R3M_r = M \cdot \frac{r^3}{R^3}

  1. Write the force. Newton's law of gravitation gives:

F=−GMrmr2=−Gmr2⋅Mr3R3=−GMmR3 rF = -\frac{G M_r m}{r^2} = -\frac{G m}{r^2} \cdot M \frac{r^3}{R^3} = -\frac{G M m}{R^3} \, r

The negative sign means the force points toward the centre (restoring).

This is a linear restoring force: F=−krF = -k r with k=GMmR3k = \frac{G M m}{R^3}.

F=−GMmR3 rF = -\frac{G M m}{R^3} \, r

  1. Relate to SHM. For any system where F=−kxF = -k x, the motion is simple harmonic with angular frequency ω=k/m\omega = \sqrt{k/m}. Here x=rx = r, so:

ω=GMR3\omega = \sqrt{\frac{G M}{R^3}}

The equation of motion is:

md2rdt2=−GMmR3r⇒d2rdt2+GMR3r=0m \frac{d^2 r}{dt^2} = -\frac{G M m}{R^3} r \quad \Rightarrow \quad \frac{d^2 r}{dt^2} + \frac{G M}{R^3} r = 0 …

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