JEE Main & Advanced / Physics / Chapter 10

Gravitation

Move from Newton's law to field, potential, escape speed, and satellite motion with a JEE-centered understanding of gravitational systems.

Original Notes2 Core SectionsJEE Revision Style
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JEE Intro

How to Think About Gravitation

Move from Newton's law to field, potential, escape speed, and satellite motion with a JEE-centered understanding of gravitational systems.

This chapter is written as original Learn at My Place teaching copy. The aim is to give you the JEE decision-making layer: what equation to trust, what approximation is valid, and where exam traps usually appear.

Read the full note once, then revisit the quick revision block before solving your own practice questions.

Problem Method

How to Solve Gravitation Questions

1. Model the Situation

Draw the body, path, field, graph, or interaction first. Label known quantities and choose sign convention before writing equations.

2. Pick the Governing Law

Decide whether the problem is about conservation, force balance, energy, momentum, fields, or graph interpretation.

3. Check the Edge Case

Verify units, limiting values, direction, and whether approximation assumptions are valid for JEE Main and Advanced options.

Section A

Notes: Gravitation

Original teaching copy for Learn at My Place

1. Universal Gravitation, Field, and Potential

The force between two masses is:

F=Gm1m2r2F = G\frac{m_1m_2}{r^2}
It is always attractive and acts along the line joining the masses.

Gravitational field and potential due to a point mass MM are:

g=GMr2,V=GMrg = \frac{GM}{r^2}, \qquad V = -\frac{GM}{r}
The negative sign in potential matters because zero is taken at infinity.

2. Variation of g, Satellite Motion, and Escape Speed

For small height hh above Earth, gg decreases approximately as ghg(12h/R)g_h \approx g(1-2h/R). For depth dd inside a uniform Earth model, gd=g(1d/R)g_d = g(1-d/R).

For a circular orbit of radius rr:

vo=GMr,T=2πr3GMv_o = \sqrt{\frac{GM}{r}}, \qquad T = 2\pi\sqrt{\frac{r^3}{GM}}
Escape velocity from the surface is:
ve=2gRv_e = \sqrt{2gR}

Quick Revision

Last 5-Minute Recall

JEE exam rule: First identify the governing principle. Most errors happen because students choose the wrong framework before they start the algebra.
Newton's inverse-square law
Field and potential as two complementary viewpoints
Variation of g with height and depth
Orbital speed, time period, and escape velocity
Verified question bank

Gravitation questions with answers

Open any of these 81 quality-checked JEE questions to review all four options, the correct answer, and the worked explanation.

  1. Question 1 · EasyNewton's Law
  2. Question 2 · EasyG vs g
  3. Question 3 · Easyg at Altitude
  4. Question 4 · Easyg at Depth
  5. Question 5 · MediumGravitational Potential
  6. Question 6 · MediumGravitational PE
  7. Question 7 · MediumSuperposition
  8. Question 8 · Easyg at Equator vs Poles
  9. Question 9 · EasyKepler's First Law
  10. Question 10 · EasyKepler's Second Law
  11. Question 11 · MediumKepler's Third Law
  12. Question 12 · MediumGravitational Field
  13. Question 13 · MediumShell Theorem
  14. Question 14 · MediumInside Shell
  15. Question 15 · HardBinding Energy
  16. Question 16 · MediumWeight at Altitude
  17. Question 17 · EasyGravitational Constant G
  18. Question 18 · MediumGravitational Force — Ratio
  19. Question 19 · HardZero Gravity Point
  20. Question 20 · HardField Inside Solid Sphere
  21. Question 21 · EasyOrbital Speed
  22. Question 22 · EasyTime Period of Satellite
  23. Question 23 · EasyEscape Velocity
  24. Question 24 · MediumGeostationary Orbit
  25. Question 25 · MediumOrbital Energy
  26. Question 26 · MediumEscape vs Orbital Speed
  27. Question 27 · EasyWeightlessness in Orbit
  28. Question 28 · MediumKepler III — Calculation
  29. Question 29 · HardSatellite — Speed Increase Effect
  30. Question 30 · MediumEscape Velocity — Moon
  31. Question 31 · HardTransfer Orbit
  32. Question 32 · MediumAngular Momentum in Orbit
  33. Question 33 · HardGravitational PE Change
  34. Question 34 · EasyPolar Satellite
  35. Question 35 · HardPeriod at Earth's Surface
  36. Question 36 · MediumGravitational Force — Ratio
  37. Question 37 · MediumEscape Velocity — No Atmosphere
  38. Question 38 · EasyWeight vs Mass
  39. Question 39 · HardBlack Hole Escape
  40. Question 40 · MediumGravitational PE at Surface
  41. Question 41 · Hardg at Combined Height+Depth
  42. Question 42 · MediumSatellite Period Ratio
  43. Question 43 · HardOrbital KE and PE
  44. Question 44 · HardEscape from Orbit
  45. Question 45 · Mediumg variation — numerical
  46. Question 46 · HardTwo-body Gravity
  47. Question 47 · MediumKepler's 3rd Numerical
  48. Question 48 · HardField Between Two Masses
  49. Question 49 · HardHohmann Transfer Energy
  50. Question 50 · HardGravitational PE — Two Masses
  51. Question 51 · MediumSatellite — Larger Orbit Slower
  52. Question 52 · HardTidal Force
  53. Question 53 · MediumPeriod of Low Orbit
  54. Question 54 · HardGravitational Acceleration — Rotating Earth
  55. Question 55 · MediumInertial Frame Falling
  56. Question 56 · HardGravitational Self Energy
  57. Question 57 · MediumJEE — g Depth vs Altitude
  58. Question 58 · MediumJEE — Satellite Energy Sign
  59. Question 59 · MediumJEE — Kepler Period Ratio
  60. Question 60 · EasyJEE — Weightlessness
  61. Question 61 · MediumJEE — Geosynchronous Period
  62. Question 62 · HardJEE — Gravity on Surface
  63. Question 63 · MediumJEE — Escape Velocity Ratio
  64. Question 64 · HardJEE — Orbital Speed at Height
  65. Question 65 · HardJEE — Angular Momentum Orbit
  66. Question 66 · HardJEE — Gravitational Field of Ring
  67. Question 67 · MediumJEE — Variation g Poles to Equator
  68. Question 68 · HardJEE — Total Energy Conservation Orbit
  69. Question 69 · MediumJEE — Field Inside Hollow Sphere
  70. Question 70 · HardAdvanced — Tunnelling Through Earth
  71. Question 71 · HardAdvanced — Binary Star Orbits
  72. Question 72 · HardAdvanced — Gravitational Lensing
  73. Question 73 · HardAdvanced — Dark Matter
  74. Question 74 · HardAdvanced — Vis-Viva Equation
  75. Question 75 · HardAdvanced — Tidal Locking
  76. Question 76 · HardAdvanced — Lagrange Points
  77. Question 77 · HardAdvanced — Escape from Orbit
  78. Question 78 · HardAdvanced — Geoid
  79. Question 79 · HardAdvanced — Period Change with Density
  80. Question 80 · HardAdvanced — Rocket in Orbit
  81. Question 81 · HardAdvanced — Gravitational Redshift
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