Question:

Two particles of equal mass m go round a circle of radius R under the action of their mutual gravitational attraction. The speed of each particle is:

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The force that brings an article in circular motion is equal to the centripetal force. The centripetal force acts towards the circle's centre.

Updated On: Sep 3, 2024
  • $\frac{1}{2}\sqrt{\frac{Gm}{R}}$
  • $\sqrt{\frac{4Gm}{R}}$
  • $\sqrt{\frac{Gm}{2R}}$
  • $\frac{1}{2R}\sqrt{\frac{1}{Gm}}$
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The Correct Option is A

Approach Solution - 1

The force that brings an article in circular motion is equal to the centripetal force. The centripetal force acts towards the circle's centre. In the question, both particles with the same mass moves in a circle, hence the gravitational force must be equal to the centripetal force.

Complete step-by-step answer:

Mass of each particle = M

Gravitational force is given by \(F=\frac{Gm_{1}m_{2}}{x^{2}}\)

where x refers to the distance between two bodies. 

In the question, the distance between two bodies is equal to the diameter of the circle, i.e. 2R. 

Putting the values in the equation, we get, \(F=\frac{GM^{2}}{4R^{2}}\) 

Now, this must be equal to the centripetal force which is: \(F=\frac{Mv^{2}}{R}\)

Putting them equally we get,

\(\frac{GM^{2}}{4R^{2}}=\frac{Mv^2}{R}\)

\(⇒v^2=\frac{GM}{4R}\)

\(\therefore v=\frac{1}{2}\sqrt\frac{GM}{R}\)

So, the correct answer is Option A.

Note: The gravitational force is an attractive force. The centripetal force is generated whenever the body moves in a circular motion. The distance between the two bodies will be 2R as they are diametrically opposite at each point in time, otherwise, it will be impossible for them to undergo circular motion under the influence of gravitational force.

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Approach Solution -2

Both particles diametrically move in opposite positions along the circular path with a radius of R. The gravitational force provides the required centripetal force.

Particles that are diametrically opposite

From the given condition 
\(\frac{Gmm}{\left(2R\right)^{2}}=\frac{mv^{2}}{R}, v=\frac{Gm}{4R}\)

v = \(\frac{1}{2}\sqrt{\frac{Gm}{R}}\)

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Concepts Used:

Newtons Law of Gravitation

Gravitational Force

Gravitational force is a central force that depends only on the position of the test mass from the source mass and always acts along the line joining the centers of the two masses.

Newton’s Law of Gravitation:

According to Newton’s law of gravitation, “Every particle in the universe attracts every other particle with a force whose magnitude is,

  • Directly proportional to the product of their masses i.e. F ∝ (M1M2) . . . . (1)
  • Inversely proportional to the square of the distance between their center i.e. (F ∝ 1/r2) . . . . (2)

By combining equations (1) and (2) we get,

F ∝ M1M2/r2

F = G × [M1M2]/r2 . . . . (7)

Or, f(r) = GM1M2/r2 [f(r)is a variable, Non-contact, and conservative force]