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guidance, flight mechanics and trajectory optimization

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ii<br />

2<br />

I<br />

2<br />

4!m<br />

4000<br />

3500<br />

3000<br />

250C I-<br />

rood I--<br />

)-<br />

I-<br />

I-<br />

‘5<br />

0 CUAORATIC THEORY<br />

P LlhEAR THEORY<br />

-<br />

-<br />

AV<br />

AV -827.52 FPS<br />

Figure 1.5<br />

Extreme Case Comparison<br />

Figures 1.5 illustrate a rather extreme case of velocity difference in<br />

which even the quadratic theory breaks down rapidly. However, even if this<br />

case for relative distance is less than 2500 miles, the predictions are quite<br />

accurate.<br />

2.1.6 The Effects of Perturbations on Rendezvous<br />

Satellite orbits are perturbed from pure conic sections by forces due to<br />

the earth's atmosphere, the non-sphericity of the earth, the attraction of the<br />

moon or sun, <strong>and</strong> the radiation pressure of solar radiation. As was indicated<br />

earlier, the term A g really represents the difference between the accele-<br />

rations of the two objects due to all forces. The earth's atmosphere could<br />

29<br />

3n

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