Question:

An earth's satellite near the surface of the earth takes about 90 min per revolution. A satellite orbiting the moon also takes about 90 min per revolution. Then which of the following is true? (\(\rho\)m is the density of the moon and ρe is the density of the earth).

Updated On: Apr 11, 2025
  • \(\rho_m<\rho_e\)
  • \(\rho_m>\rho_e\)
  • \(\rho_m=\rho_e\)
  • No conclusion can be made about the densities
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The Correct Option is C

Solution and Explanation

The time period of a satellite in orbit depends on the mass of the celestial body it is orbiting and the radius of the orbit.

The formula for the time period is: 

$T = 2\pi \sqrt{\frac{a^3}{GM}}$

Squaring both sides:

$T^2 = \frac{4\pi^2 a^3}{GM}$

Rearranging gives:

$\frac{a^3}{M} = \text{constant}$

Since both satellites (one orbiting Earth and the other orbiting the Moon) have the same time period, we get:

$\frac{a_e^3}{M_e} = \frac{a_m^3}{M_m}$

We know that mass $M$ of a spherical body is related to density $\rho$ by:

$M = \rho \cdot \frac{4}{3} \pi R^3$

Assuming the satellites are close to the surfaces, we take $a \approx R$, so:

$\frac{M}{a^3} \approx \rho \cdot \frac{4}{3} \pi$

This implies:

$\frac{M_e}{a_e^3} = \frac{M_m}{a_m^3} \Rightarrow \rho_e = \rho_m$

Therefore, the correct option is (C): $\rho_m = \rho_e$

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Concepts Used:

Gravitational Potential Energy

The work which a body needs to do, against the force of gravity, in order to bring that body into a particular space is called Gravitational potential energy. The stored is the result of the gravitational attraction of the Earth for the object. The GPE of the massive ball of a demolition machine depends on two variables - the mass of the ball and the height to which it is raised. There is a direct relation between GPE and the mass of an object. More massive objects have greater GPE. Also, there is a direct relation between GPE and the height of an object. The higher that an object is elevated, the greater the GPE. The relationship is expressed in the following manner:

PEgrav = mass x g x height

PEgrav = m x g x h

Where,

m is the mass of the object,

h is the height of the object

g is the gravitational field strength (9.8 N/kg on Earth) - sometimes referred to as the acceleration of gravity.