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AP® Physics 1: Algebra-Based · Unit 2 · Topic 2.6

Gravitational Force: Revision Notes (Physics 1 2.6)

One-page recap of universal gravitation, field strength, weight, apparent weight and inertial versus gravitational mass for the algebra-based course, with the mistakes that cost marks.

Short on time? This page is the recap. For diagrams, graphs and worked examples, use the full study guide. This is the algebra-based course: no calculus is needed.

Recap

  • Any two masses attract. The force acts along the line joining their centres of mass and can be drawn from each centre of mass.
  • The two forces are a third-law pair: equal and opposite, whatever the masses.
  • A field gives the force per kilogram at each point. Gravitational field strength g is in N/kg, which equals m/s².
  • Weight is the gravitational force from a planet or moon on a nearby small object: mg.
  • g is effectively constant when the object’s distance from the centre changes by only a tiny fraction (anything near the ground).
  • Apparent weight is the normal force. It differs from mg whenever the system accelerates. A system appears weightless when gravity is the only force on it (free fall), or when no forces act.
  • Equivalence principle: in an accelerating frame, you cannot tell apparent weight from real gravity.
  • Inertial mass (resists changes in motion) and gravitational mass (feels gravity) are equal by experiment, so all objects fall with the same acceleration.

Key relationships

Relationship Symbols and units Use it to
F_g = G m₁m₂ / r² G = 6.67 × 10⁻¹¹ N·m²/kg², r in m force between two masses
g = F_g / m = GM / r² N/kg = m/s² field strength at distance r from mass M
weight = mg g = 9.8 N/kg at Earth’s surface gravitational force near a planet
F_N = m(g + a_y), +y up a_y signed apparent weight in a lift
F_g ∝ 1/r² factor-of-change: 2r → ¼ force

Assumptions behind the numbers

  • Planets and spheres act as if all their mass is at their centre (for points outside them).
  • Near Earth’s surface, g = 9.8 N/kg (10 N/kg where stated).
  • The ground is an inertial frame; a lift that accelerates is not.

Mistakes to avoid

  1. Using surface-to-surface distance. Use centre to centre, so add the planet’s radius to a height.
  2. Forgetting to square r. Halving r gives four times the force.
  3. Saying the larger body pulls harder. The forces are equal; the smaller body accelerates more.
  4. Linking scale readings to velocity. Only the acceleration matters.
  5. “No gravity in orbit.” g is still large; there is just no normal force.
  6. Mixing mass and weight. kg is not N.

Quick self-check

  1. The distance between two objects is tripled. By what factor does the gravitational force change? (It becomes one ninth.)
  2. A 70 kg astronaut stands on the Moon, where g = 1.6 N/kg. What is her weight there? (about 110 N)
  3. Take +y up. A 50 kg person stands on a scale in a lift accelerating downward at 2.0 m/s². What does the scale read? (390 N)

Next: practice questions.

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