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MHT CET 2019 (2 May, Shift 2) · Moment of Inertia & Radius of Gyration

Moment of Inertia & Radius of Gyration question from MHT CET 2019 (2 May, Shift 2)

Q156MHT CET 2019 · 2 MAY · SHIFT 2Easy

Moment of Inertia & Radius of Gyration

Three point masses each of mass ' mm ' are kept at the corners of an equilateral triangle of side ' LL '. The system rotates about the center of the triangle without any change in the separation of masses during rotation. The period of rotation is directly proportional to (cos⁡30∘=sin⁡60∘=32)\left(\cos 30^\circ = \sin 60^\circ = \frac{\sqrt{3}}{2}\right)

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Answer: (a)

  1. The separation stays fixed because mutual gravity supplies the centripetal force. Each mass is at r=L3r = \frac{L}{\sqrt{3}} from the centre.
  2. Net pull on one mass toward the centre: 2Gm2L2cos⁡30∘=3Gm2L22\frac{Gm^2}{L^2}\cos 30^\circ = \frac{\sqrt{3}Gm^2}{L^2}
  3. mω2L3=3Gm2L2⇒ω2=3GmL3m\omega^2 \frac{L}{\sqrt{3}} = \frac{\sqrt{3}Gm^2}{L^2} \Rightarrow \omega^2 = \frac{3Gm}{L^3}
  4. T=2πω=2πL33Gm⇒T∝L3/2T = \frac{2\pi}{\omega} = 2\pi\sqrt{\frac{L^3}{3Gm}} \Rightarrow T \propto L^{3/2}
  5. So the answer is (b) L3/2L^{3/2}.
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