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Astronomy Principles and Practice Fourth Edition.pdf

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Interplanetary transfer orbits 197<br />

Figure 14.8. An incremental change V in the velocity V.<br />

Figure 14.9. An incremental change in velocity along the original velocity direction.<br />

Figure 14.10. A Hohmann transfer orbit APB between two circular, co-planar orbits.<br />

However, if the increment V is applied as in figure 14.9, along the instantaneous velocity vector<br />

V , then the maximum increase in kinetic energy is achieved for a given burn, i.e. the full effect of V<br />

is added to V . Obviously if it is desired to decrease the kinetic energy, the velocity increment V<br />

would be applied in the opposite direction to V .<br />

Hohmann showed that, in practice, the most economical transfer orbit between circular, coplanar<br />

orbits was an elliptical orbit cotangential to inner <strong>and</strong> outer orbits at perihelion <strong>and</strong> aphelion<br />

respectively. It is shown in figure 14.10 as ellipse APB. Only one-half of the transfer orbit is used.<br />

At A, the rocket-engine is fired to produce a velocity increment V A , applied tangentially to place the<br />

vehicle in the transfer orbit. The vehicle coasts round the half-ellipse APB, reaching aphelion at B.<br />

If no further change in energy took place, the vehicle would coast onwards along the mirror half of<br />

APB to return eventually to A. A second impulse is, therefore, required to produce a second velocity<br />

increment V B . This is again obtained by firing the rocket-engine tangentially <strong>and</strong> the rocket enters<br />

the outer circular orbit of radius a 2 AU.<br />

Such transfer orbits are known as Hohmann least-energy two-impulse cotangential orbits.<br />

We now show how to calculate various parameters associated with the transfer.

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