Question:

A ''double star'' is a composite system of two stars rotating about their center of mass under their mutual gravitational attraction. Let us consider such a ''double star'' which has two stars of masses 'm' and '2m' at a separation '1'. If T is the time period of rotation about their enter of mass then.

Updated On: Jul 5, 2022
  • $T=2\pi\sqrt\frac{l^3}{mG}$
  • $T=2\pi\sqrt\frac{l^3}{2mG}$
  • $T=2\pi\sqrt\frac{l^3}{3mG}$
  • $T=2\pi\sqrt\frac{l^3}{4mG}$
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The Correct Option is C

Solution and Explanation

consider origin at pratical of mass 2m, we have centre of mass is 1/3 and 21/3 from m. $\frac{2l}{3} \, \omega^2 = \frac{Gm(2m)}{l^2}$ then find T
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Concepts Used:

Gravitation

In mechanics, the universal force of attraction acting between all matter is known as Gravity, also called gravitation, . It is the weakest known force in nature.

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,

  • F ∝ (M1M2) . . . . (1)
  • (F ∝ 1/r2) . . . . (2)

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

F ∝ M1M2/r2

F = G × [M1M2]/r2 . . . . (7)

Or, f(r) = GM1M2/r2

The dimension formula of G is [M-1L3T-2].