Physics Circle home Student Login

Home›Chapters›Gravitation PYQs›Satellites - Orbital Velocity & Period›Question 22

MHT CET 2024 (10 May, Shift 1) · Satellites - Orbital Velocity & Period

Satellites - Orbital Velocity & Period question from MHT CET 2024 (10 May, Shift 1)

Q22MHT CET 2024 · 10 MAY · SHIFT 1Medium

Satellites - Orbital Velocity & Period

A small planet is revolving around a very massive star in a circular orbit of radius ' RR ' with a period of revolution ' TT '. If the gravitational force between the planet and the star were proportional to 'R−5/2R^{-5/2}', then 'TT' would be proportional to

Show answer and solution

Answer: (d)

  1. Force gives the centripetal force: mω2R∝R−5/2m\omega^2 R \propto R^{-5/2}.
  2. ω2∝R−7/2\omega^2 \propto R^{-7/2}, and T∝1ωT \propto \frac{1}{\omega}, so T2∝R7/2T^2 \propto R^{7/2}.
  3. T∝R7/4T \propto R^{7/4}
  4. So the answer is (d).
Report a mistake

More questions on Satellites - Orbital Velocity & Period