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MHT CET 2024 (16 May, Shift 1) · Satellites - Orbital Velocity & Period

Satellites - Orbital Velocity & Period question from MHT CET 2024 (16 May, Shift 1)

Q19MHT CET 2024 · 16 MAY · SHIFT 1Easy

Satellites - Orbital Velocity & Period

A satellite is orbiting just above the surface of the planet of density ' ρ\rho ' with periodic time ' TT '. The quantity T2ρT^2\rho is equal to ( G=G = universal gravitational constant)

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Answer: (c)

  1. Just above the surface: T2=4π2R3GMT^2 = \frac{4\pi^2 R^3}{GM} with M=43πR3ρM = \frac{4}{3}\pi R^3\rho.
  2. T2=4π2R3G⋅43πR3ρ=3πGρT^2 = \frac{4\pi^2 R^3}{G \cdot \frac{4}{3}\pi R^3 \rho} = \frac{3\pi}{G\rho}
  3. T2ρ=3πGT^2\rho = \frac{3\pi}{G}
  4. So the answer is (c) 3πG\frac{3\pi}{G}.
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