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The idea was first clearly described by Hermann Oberth in his 1923 book, although hints also appeared in Tsiolkovsky's work. The law works due to the nonlinear dependence of kinetic energy on speed. Imagine you push a cart. If it is barely moving, your push adds almost no energy to it — most of the energy turns into heat in your shoes. If the cart is racing, you push off the ground, transferring momentum while remaining nearly in place, and almost all the work turns into its acceleration. In space, the planet's gravitational field plays the role of the ground, and the rocket exhaust provides the 'push.' The faster the rocket relative to the planet, the greater the percentage of fuel energy converted into motion.

How it works

A space probe approaching Jupiter fires its engine at the point of closest approach. There, its speed is maximal, and the same fuel impulse changes the trajectory more. Thus, using the Oberth effect, one can reach the outer planets with less cost.

💡 Oberth first proposed using an 'orbital refueling system' — refueling at high speed, which could allow reaching high velocities without enormous single-use rockets.
\Delta K \approx m v \Delta v
ΔK is the increase in the rocket's kinetic energy; m is the rocket mass at the moment of the impulse; v is the current rocket speed; Δv is the speed increment due to the engine firing (Δv << v)
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