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Propulsion















                     Figure 3-9.  Geostationary orbital transfer. The plane-change maneuver is   71
                     performed out at the apogee of the transfer orbit to minimize the Av required.


                     Geostationary Transfer. Figure 3-9 illustrates the transfer of  a satellite
                     from a typical low-earth "parking" orbit of 28.5" inclination to a geosta-
                     tionary orbit.
                       The first maneuver establishes the spacecraft on a transfer orbit which is
                     an ellipse that lies in the same plane as the parking orbit with its perigee at
                     the same altitude  as the parking orbit and its apogee at geostationary altitude.
                     This should be recognized as a Hohmann transfer orbit described in Chapter
                     2. Note that in order to intersect the final desired equatorial geostationary
                     orbit, the apogee (and, thus, the perigee) of the 28.5" inclined transfer orbit
                     must be located over the equator. As the satellite approaches this point over
                     the equator, a perigee kick motor (PKM) is fired to inject the spacecraft into
                     the transfer orbit from the parking orbit. The change in velocity required at
                     this point can be found from the relationships given in Chapter 2.
                       At  the transfer orbit apogee, two changes to the orbit must  occur in
                     order to establish a geostationary orbit. First, the elliptical transfer orbit
                     must be circularized at the geostationary altitude. If this is done as a sep-
                     arate maneuver within the same plane as the transfer orbit, the Av required
                     would be the same as for a Hohmann transfer. However, to be geostation-
                     ary, the orbit must also be equatorial, so the plane of our spacecraft orbit
                     must be changed from 28.5" to 0". The Av relationship for a simple plane,
                     given earlier in Chapter 2, is repeated here to illustrate an important point:
                                             Ai
                       "simple   plane change = 2v sin -                       (2 - 22)
                                             2
                       This  relationship  reminds  us  that  plane  changes  performed  at  low
                     orbital velocities minimize the required Av. That is why, in geostationary
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