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Orbits and escape speed test with answers for AP Physics C (free PDF download)

Quick answer: Gravitational potential energy is U = −GMm/r, with zero at infinity. This AP Physics C test on orbits and escape speed has 8 questions worth 20 marks, to do in 45 minutes: field strength, low Earth orbit and effect of drag. The mark scheme is on a separate page; free printable PDF.

Orbits and escape speed test with answers for AP Physics C (free PDF download)

This test covers gravitational potential energy, circular and elliptical orbits and escape speed in the style of AP Physics C: Mechanics. Show each step, use calculus where asked and give units. Take G = 6.67 × 10⁻¹¹ N m²/kg² and the data given. The total is 20 marks.

Level: AP Physics C (Mechanics and E&M, calculus-based) · Curriculum: AP PC:M Unit 7

Time: 45 minutes · 8 questions · Total: 20 marks · Calculator allowed

Question 2 Low Earth orbit (3 marks)

A satellite orbits 600 km above Earth (R = 6.37 × 10⁶ m, GM = 3.98 × 10¹⁴ N m²/kg²).
  1. Write the equation linking gravity and centripetal force. (1 mark)
  2. Calculate the orbital speed. (1 mark)
  3. Calculate the period. (1 mark)

Question 3 Effect of drag (2 marks)

Explain why a satellite in a low circular orbit speeds up as air drag slowly lowers it.

Question 4 Escape from the Moon (3 marks)

Derive and calculate the escape speed from the Moon (M = 7.35 × 10²² kg, R = 1.74 × 10⁶ m, G = 6.67 × 10⁻¹¹ N m²/kg²).

Question 5 Energies of an orbit (3 marks)

A satellite of mass 800 kg is in a circular orbit of radius 1.2 × 10⁷ m. Calculate (a) its kinetic energy, (b) its potential energy, (c) its total energy. Use GM = 3.98 × 10¹⁴.

Question 6 Comet speeds (3 marks)

A comet on an elliptical orbit: at the closest point to the Sun it moves at 20 kilometres per second and at the farthest point it is four times further awaySunclosest: 20 km/sfarthest: 4 r_p
Question 6: speed at the two extremes of the orbit.
A comet moves at 20 km/s at its closest point to the Sun (distance r_p). Its farthest point is 4r_p from the Sun (figure). Explain why the speed differs and calculate the speed at the farthest point.

Question 7 Deriving U (2 marks)

Starting from F = −GMm/r², show by integration that the gravitational potential energy is U = −GMm/r, taking U = 0 at infinity.

Question 8 Kepler’s third law (2 marks)

A planet orbits a star at 4.0 times the distance of another planet. Calculate the ratio of their periods.

See the orbits and escape speed test answers and mark scheme

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