NDA Physics · Free notes
Gravitation — NDA Physics
Gravitation is 19 past-year NDA questions across 2017–2026, a compact, formula-driven earner. It is the universal pull every mass exerts on every other mass — the force that holds you to the ground, keeps the Moon in orbit, and shapes the solar system. For the NDA it splits into three movements: (1) Newton's Law of Gravitation — the inverse-square law F = Gm₁m₂/r², the universal constant G, and the action-reaction nature of the force; (2) Gravitational Field and Potential — surface gravity g = GM/R², how g depends on a planet's mass, radius and density, the field-versus-potential distinction, and weightlessness in orbit; (3) Orbits, Kepler and Escape — Kepler's third law T² ∝ a³, orbital and escape speeds, and what actually keeps a satellite up. Almost every mark comes from one of a handful of formulas and from scaling them correctly when a planet's mass, radius or density is changed by a factor. Learn the formulas, track the powers, and the marks follow.
The handout has every subtopic, worked example, formula and trap with answers shown. The formula sheet is the chapter’s formulas and traps alone, on one page.
Subtopic notes
Newton's Law of Gravitation
8 PYQsEvery two point masses attract each other with a force proportional to the product of their masses and inversely proportional to the square of the distance between them — F = Gm₁m₂/r² — where G is the same universal constant everywhere in the universe.
Gravitational Field and Potential
7 PYQsThe acceleration due to gravity at a planet's surface is g = GM/R² (equivalently g = (4/3)πGρR); gravitational potential measures energy per unit mass, and a region of equal potential does no work on a body moved through it.
Orbits, Kepler and Escape
4 PYQsA planet's orbital period and size obey Kepler's third law T² ∝ a³; a satellite stays up on the gravitational force alone (needing no fuel), and escaping a planet's pull requires a launch speed v_e = √(2GM/R) = √(2gR).
Formula & revision sheet
13 formulas · 1 reference tables · 17 gotchas across all subtopics — the exam-eve cheat-sheet
Formula & revision sheet
13 formulas · 1 reference tables · 17 gotchas across all subtopics — the exam-eve cheat-sheet
Formulas (3)
Reference tables (1)
The universal gravitational constant G5 rows
| Property | Value / Statement |
|---|---|
| SI unit | N·m²/kg² (newton metre-squared per kilogram-squared)Q NDA 2025 — the unit of G is N-m²/kg², derived from G = Fr²/(m₁m₂). |
| Dimensional formula | M⁻¹L³T⁻² |
| Approximate value | 6.674 × 10⁻¹¹ N·m²/kg² |
| Universality | Same for ALL pairs of bodies, everywhere; independent of mass, distance, location, or local gQ NDA 2017 — G is a universal constant; it does NOT depend on the local value of g. |
| Force, in contrast, is NOT universal | F itself depends on the masses and separation, so it differs for every pair of bodiesQ NDA 2018 — the false statement is 'gravitational force is the same for all pairs of bodies'. The force varies; only G is constant. |
Watch out for (5)
- Distance enters as a square, masses do not→ Newton's law of gravitation — the inverse-square law
- G is universal, but the FORCE is not→ The universal gravitational constant G
- Don't confuse G with g→ The universal gravitational constant G
- Square only the distance factor→ Scaling the force — changing masses and distance together
- The bigger mass does NOT exert the bigger force→ Gravitational force is action-reaction — equal and opposite
Formulas (6)
- Surface gravity — g = GM/R² · Surface gravity
- Surface gravity from density — g = (4/3)πGρR · Surface gravity from density
- Average density of a composite body · Average density of a composite body
- Gravitational field versus potential · Work and equal potential
- Weightlessness in orbit — zero normal reaction · Apparent weight = normal reaction
- g is the same for all bodies — free fall and weight · Weight and spring extension scale with g
Watch out for (7)
- Radius enters as a square in g, just like in F→ Surface gravity — g = GM/R²
- Same density does NOT mean same gravity→ Surface gravity from density — g = (4/3)πGρR
- Average density is volume-weighted, not the mean of densities→ Average density of a composite body
- Equal potential, not equal field, decides the work→ Gravitational field versus potential
- Weightless does NOT mean gravity-free→ Weightlessness in orbit — zero normal reaction
- In vacuum, mass and shape don't change the fall time→ g is the same for all bodies — free fall and weight
- Spring extension follows g, not just the mass→ g is the same for all bodies — free fall and weight
Formulas (4)
Watch out for (5)
- It's T² ∝ a³, not T ∝ a→ Kepler's third law — T² ∝ a³
- Orbital speed is set by the orbit, not the satellite→ Orbital velocity — v_o = √(GM/R)
- Halving R while quadrupling ρ leaves v_e UNCHANGED→ Escape velocity — v_e = √(2GM/R) and how it scales
- Escape velocity is independent of the projectile's mass and launch angle→ Escape velocity — v_e = √(2GM/R) and how it scales
- Orbiting needs no fuel — gravity does the work→ What keeps a satellite up — no fuel required
PYQ weightage by concept
14 concepts · 19 PYQs — where the marks actually sit, so you know what to drill first
PYQ weightage by concept
14 concepts · 19 PYQs — where the marks actually sit, so you know what to drill first
| Concept | PYQs | Share |
|---|---|---|
| The universal gravitational constant G | 3 | 16% |
| Scaling the force — changing masses and distance together | 2 | 11% |
| Gravitational force is action-reaction — equal and opposite | 2 | 11% |
| Newton's law of gravitation — the inverse-square law | 1 | 5% |
| Concept | PYQs | Share |
|---|---|---|
| g is the same for all bodies — free fall and weight | 2 | 11% |
| Surface gravity — g = GM/R² | 1 | 5% |
| Surface gravity from density — g = (4/3)πGρR | 1 | 5% |
| Average density of a composite body | 1 | 5% |
| Gravitational field versus potential | 1 | 5% |
| Weightlessness in orbit — zero normal reaction | 1 | 5% |
| Concept | PYQs | Share |
|---|---|---|
| Kepler's third law — T² ∝ a³ | 2 | 11% |
| Escape velocity — v_e = √(2GM/R) and how it scales | 1 | 5% |
| What keeps a satellite up — no fuel required | 1 | 5% |
| Orbital velocity — v_o = √(GM/R)foundation | — | — |
Test yourself on a real paper
Sit a past NDA paper, timed and marked the way the exam marks it. You see your score and every answer the moment you finish. Free to start.