Physics Circle home Student Login

Home›Chapters›Gravitation PYQs›Satellites - Orbital Velocity & Period›Question 58

JEE Main 2020 (2 Sep, Shift 1) · Satellites - Orbital Velocity & Period

Satellites - Orbital Velocity & Period question from JEE Main 2020 (2 Sep, Shift 1)

Q58JEE Main 2020 · 2 SEP · SHIFT 1Difficult

Satellites - Orbital Velocity & Period

The mass density of a spherical galaxy varies as Kr\frac{K}{r} over a large distance ‘r’ from its centre. In that region, a small star is in a circular orbit of radius R. Then the period of revolution, T depends on R as:

Show answer and solution

Answer: (a)

  1. Mass inside radius rr: M(r)=∫0rKr4πr2dr=2πKr2M(r) = \int_0^r \frac{K}{r} 4\pi r^2 dr = 2\pi K r^2.
  2. Field at RR: g=GM(R)R2=2πGKg = \frac{GM(R)}{R^2} = 2\pi G K, a constant.
  3. v2R=2πGK⇒v∝R\frac{v^2}{R} = 2\pi G K \Rightarrow v \propto \sqrt{R}.
  4. T=2πRv∝R⇒T2∝RT = \frac{2\pi R}{v} \propto \sqrt{R} \Rightarrow T^2 \propto R.
  5. So the answer is (a) T2∝RT^2 \propto R.
Report a mistake

More questions on Satellites - Orbital Velocity & Period