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Question: A satellite is revolving around a planet in a circular orbit close to its surface. Let '$\rho$' be t...

A satellite is revolving around a planet in a circular orbit close to its surface. Let 'ρ\rho' be the mean density and 'R' be the radius of the planet. Then the period of the satellite is (G = universal constant of gravitation)

A

4πρG\sqrt{\frac{4\pi}{\rho G}}

B

πρG\sqrt{\frac{\pi}{\rho G}}

C

3πρG\sqrt{\frac{3\pi}{\rho G}}

D

2πρG\sqrt{\frac{2\pi}{\rho G}}

Answer

3πρG\sqrt{\frac{3\pi}{\rho G}}

Explanation

Solution

For a satellite in a circular orbit of radius R (planet's surface), the time period is

T=2πR3GMT = 2\pi\sqrt{\frac{R^3}{GM}}

The planet's mass MM is given by

M=ρ43πR3M = \rho \cdot \frac{4}{3}\pi R^3

Substitute MM into the period formula:

T=2πR3G(ρ43πR3)=2π1Gρ43π=2π34πGρT = 2\pi\sqrt{\frac{R^3}{G\left(\rho\cdot\frac{4}{3}\pi R^3\right)}} = 2\pi\sqrt{\frac{1}{G\rho\cdot\frac{4}{3}\pi}} = 2\pi\sqrt{\frac{3}{4\pi G\rho}}

Simplify:

T=4π234πGρ=3πGρT = \sqrt{\frac{4\pi^2\cdot 3}{4\pi G\rho}} = \sqrt{\frac{3\pi}{G\rho}}

Thus, the correct answer is Option C.