Calculate the gravitational force between masses, the gravitational acceleration on a planet’s surface and at a height, and explain the difference between mass and weight.
Newton’s law of universal gravitation: every particle with mass in the universe attracts every other particle with a force which is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centres.
F = G m₁m₂ ÷ r² G = 6,67 × 10⁻¹¹ N·m²·kg⁻²
Many multiple-choice questions ask what happens to F when a quantity changes. Use the formula as a ratio:
| Change | Effect on F |
|---|---|
| One mass doubled | F doubles |
| Both masses doubled | F × 4 |
| Distance doubled | F ÷ 4 |
| Distance tripled | F ÷ 9 |
| Distance halved | F × 4 |
On a planet of mass M and radius R, the weight of an object is the gravitational force on it, so mg = GMm ÷ R² and
g = GM ÷ r² (r = R at the surface; r = R + h at a height h above the surface)