Physics Circle home Student Login

Home›Chapters›Gravitation PYQs›Kepler's Laws & Planetary Motion›Question 1

NEET 2026 (Re-neet) · Kepler's Laws & Planetary Motion

Kepler's Laws & Planetary Motion question from NEET 2026 (Re-neet)

Q1NEET 2026 · RE-NEETEasy

Kepler's Laws & Planetary Motion

In a solar system, the time-period of revolution of a planet tracing a circular orbit of radius RR is proportional to:

Show answer and solution

Answer: (c)

  1. Gravity gives the centripetal force: GMmR2=m4π2T2R⇒T2=4π2GMR3\dfrac{GMm}{R^2} = m\dfrac{4\pi^2}{T^2}R \Rightarrow T^2 = \dfrac{4\pi^2}{GM}R^3.
  2. T∝R3/2T \propto R^{3/2}
  3. So the answer is (c) R3/2R^{3/2}.
Report a mistake

More questions on Kepler's Laws & Planetary Motion