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Gravity and Newton's Laws: How Apollo Saved Fuel to the Moon

1Why Coasting Is Free: Newton's First Law on the Way to the Moon2Gravity as a Free Engine: Newton's Law of Gravitation on the Translunar Coast3Designing the Path: Free-Return Trajectory and the Oberth Effect4The Remaining Burns: Lunar Orbit Insertion and Transearth Injection
Designing the Path: Free-Return Trajectory and the Oberth Effect

Same Burn, Different Speed, Different Result

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The free-return path saves fuel by removing a burn entirely. But some burns cannot be removed — so the next lever is where you fire them. Watch two identical spacecraft receive identical engine burns.
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The Oberth effect states that a rocket burn produces a larger change in the spacecraft's kinetic energy when the burn is performed at high speed than when the same burn is performed at low speed.

  • Kinetic energy depends on the square of speed: \(E_k = \tfrac{1}{2}mv^2\). A fixed velocity change \(\Delta v\) added at a higher speed therefore changes \(E_k\) by a larger amount.
  • Equivalently, the same propellant produces a larger change in orbital energy when the engine fires while the spacecraft is moving fastest.
  • Practical consequence: for a given mission goal, burning near the fastest point of an orbit — periapsis — requires less propellant than burning near the slowest point — apoapsis.

Key point: the Oberth effect is not a new force. It is a consequence of how kinetic energy depends on speed, and it makes burn timing a fuel-saving decision.

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