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Newtonian Gravitation MCQs – Practice Test 5 PDF Download

MCQ: 21

Total energy of an orbiting satellite depends on semimajor axis of its orbit and not its eccentricity, when orbit is

  1. circular
  2. elliptical
  3. triangular
  4. rectangular
MCQ: 22

Ratio T2/a3 for Pluto is equals to

  1. 5.01x10-34 y2/m3
  2. 3.01x10-34 y2/m3
  3. 2.96x10-34 y2/m3
  4. 2.99x10-34 y2/m3
MCQ: 23

Radius of Ceres is equals to

  1. 3.8x105 m
  2. 6.37x106 m
  3. 6.96x108 m
  4. 1x104 m
MCQ: 24

Neutron star has a mass of

  1. 2x1030 kg
  2. 1.99x1030 kg
  3. 2x1020 kg
  4. 5.98x1024 kg
MCQ: 25

If M is earth's mass, r is the distance between them and G is gravitational constant then by Newton's law of gravitation gravitational acceleration is equals to

  1. GM/r
  2. rG/M
  3. GMr
  4. GM/r2

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