Home › Grade XI Physics › Gravitation
MCQsGrade XI50 questions

Gravity and Gravitation — 50 MCQs

Comprehensive 50-question MCQ set on gravitational field, orbital motion, escape velocity, satellite dynamics and planetary phenomena (arranged easy to very hard).

Ch. 7 Gravitation · Updated 2026-09-27

  1. 1. According to Newton's law of gravitation, the gravitational force between two point masses is inversely proportional to:

    easy
  2. 2. The SI value of the universal gravitational constant G is approximately:

    easy
  3. 3. The gravitational force between two masses is always:

    easy
  4. 4. The SI unit of gravitational field strength is:

    easy
  5. 5. The relation connecting acceleration due to gravity g, the universal gravitational constant G, the mass of the Earth M, and its radius R is:

    easy
  6. 6. The SI unit of gravitational potential is:

    easy
  7. 7. The gravitational potential energy of a bound two-mass system is always:

    easy
  8. 8. As altitude above the Earth's surface increases, the value of g:

    easy
  9. 9. As depth below the Earth's surface increases, the value of g:

    easy
  10. 10. At the exact centre of the Earth, the value of g is:

    easy
  11. 11. The centre of mass of a system of particles depends only on:

    easy
  12. 12. The centre of gravity of a body depends on:

    easy
  13. 13. The orbital velocity of a satellite in a circular orbit of radius r around a planet of mass M is given by:

    easy
  14. 14. The escape velocity from a planet's surface, expressed in terms of g and R, is:

    easy
  15. 15. For a satellite to be geostationary, its time period must equal:

    easy
  16. 16. The value of the universal gravitational constant G was first experimentally determined by:

    medium
  17. 17. If the distance between two point masses is doubled, the gravitational force between them becomes:

    medium
  18. 18. If both masses in a gravitating pair are doubled and the distance between them is halved, the new gravitational force is how many times the original?

    medium
  19. 19. The gravitational field strength at a distance of 2R from the centre of a planet of radius R (surface gravity g) is:

    medium
  20. 20. The value of g at a height equal to the Earth's radius R above the surface (i.e. at a distance 2R from the centre) is:

    medium
  21. 21. The value of g at a depth of R/2 below the Earth's surface (uniform-density approximation) is:

    medium
  22. 22. The ratio of escape velocity to orbital velocity at the same radius is:

    medium
  23. 23. If the orbital radius of a satellite is increased to 4 times its original value, its orbital velocity becomes:

    medium
  24. 24. If the orbital radius of a satellite is increased to 4 times its original value, its time period becomes:

    medium
  25. 25. If the orbital radius of a satellite is doubled, its kinetic energy becomes:

    medium
  26. 26. If the orbital radius of a satellite is doubled, the magnitude of its potential energy becomes:

    medium
  27. 27. The total mechanical energy E of an orbiting satellite is related to its kinetic energy KE by:

    medium
  28. 28. The binding energy of a satellite of mass m orbiting at radius r around a planet of mass M is given by:

    medium
  29. 29. The approximate height of a geostationary orbit above the Earth's surface is:

    medium
  30. 30. The approximate orbital period of a typical GPS satellite is:

    medium
  31. 31. The minimum number of GPS satellites a receiver must detect simultaneously to determine its full three-dimensional position and correct its own clock is:

    medium
  32. 32. The centre of mass and centre of gravity of a body coincide when:

    medium
  33. 33. In the vector form of Newton's law of gravitation, the negative sign indicates that the force is:

    medium
  34. 34. The approximate escape velocity from the Earth's surface is:

    medium
  35. 35. The gravitational potential at an infinite distance from any mass is taken to be:

    medium
  36. 36. Two satellites orbit the same planet at radii r and 4r respectively. The ratio of their time periods T(4r):T(r) is:

    hard
  37. 37. A satellite's orbital radius is reduced to half its original value. Its orbital velocity:

    hard
  38. 38. Two planets have the same average density but different radii R₁ and R₂. The ratio of their surface gravitational accelerations g₁:g₂ is:

    hard
  39. 39. If the Earth's radius were halved while its mass remained unchanged, the new surface value of g would become:

    hard
  40. 40. A hypothetical planet has twice the mass and twice the radius of Earth. Compared to Earth's escape velocity vₑ, the escape velocity from this planet's surface is:

    hard
  41. 41. Two identical point masses m are fixed at the two ends of a light rod of length d. A third mass is placed exactly at the midpoint of the rod. The net gravitational force on the third mass due to the two end masses is:

    hard
  42. 42. The energy that must be supplied to raise a satellite of mass m from a circular orbit of radius r to a circular orbit of radius 2r, around a planet of mass M, is:

    hard
  43. 43. Using the formula for variation of g with depth, the depth below the Earth's surface at which g reduces to exactly half its surface value is:

    hard
  44. 44. Using the exact (non-approximated) expression for variation of g with altitude, the height above the Earth's surface at which g reduces to exactly one-fourth of its surface value is:

    hard
  45. 45. A satellite orbits a planet of mass M at radius r with time period T. An identical satellite orbits a different planet of mass 4M at the same orbital radius r. Its time period will be:

    hard
  46. 46. Regarding the relativistic time corrections applied to GPS satellite clocks, which statement is correct?

    hard
  47. 47. If the mass of a planet is doubled while a satellite's orbital radius r is kept unchanged, the satellite's new orbital velocity becomes:

    hard
  48. 48. A satellite is placed in a circular equatorial orbit at a radius smaller than the geostationary radius, moving in the same direction as the Earth's rotation. Relative to a fixed point on the Earth's surface, this satellite will appear to:

    hard
  49. 49. As the orbital radius r of a satellite decreases, its binding energy:

    hard
  50. 50. A hypothetical planet has twice the mass of Earth and half the radius of Earth. The escape velocity from this planet's surface, compared to Earth's escape velocity vₑ, is:

    hard