Page 110 - Satellite Communications, Fourth Edition
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90   Chapter Three

                              are published at regular intervals, Fig. 3.7 showing typical values. The
                              period for a geostationary satellite is 23 h, 56 min, 4 s, or 86,164 s. The
                              reciprocal of this is 1.00273896 rev/day, which is about the value tabu-
                              lated for most of the satellites in Fig. 3.7. Thus these satellites are geo-
                              synchronous, in that they rotate in synchronism with the rotation of the
                              earth. However, they are not geostationary. The term geosynchronous
                              satellite is used in many cases instead of geostationary to describe these
                              near-geostationary satellites. It should be noted, however, that in gen-
                              eral a geosynchronous satellite does not have to be near-geostationary,
                              and there are a number of geosynchronous satellites that are in highly
                              elliptical orbits with comparatively large inclinations (e.g., the Tundra
                              satellites).
                                Although in principle the two-line elements could be used as described
                              in Chap. 2 to determine orbital motion, the small inclination makes it
                              difficult to locate the position of the ascending node, and the small
                              eccentricity makes it difficult to locate the position of the perigee.
                              However, because of the small inclination, the angles w and Ω can be
                              assumed to be in the same plane.
                                Referring to Fig. 2.9 it will be seen that with this assumption the
                              subsatellite point will be            east of the line of Aries. The longi-
                              tude of the subsatellite point (the satellite longitude) is the easterly






                              INTELSAT 901
                              1 26824U 01024A   05122.92515626 -.00000151  00000-0  10000-3 0  7388
                              2 26824   0.0158 338.7780 0004091  67.7508 129.4375  1.00270746 14318
                              INTELSAT 902
                              1 26900U 01039A   05126.99385197  .00000031  00000-0  10000-3 0  6260
                              2 26900   0.0156 300.5697 0002640 112.8823 231.2391  1.00271845 13528
                              INTELSAT 903
                              1 27403U 02016A   05125.03556931  .00000000  00000-0  10000-3 0  6249
                              2 27403   0.0362 171.6123 0002986 232.5077 157.1571  1.00265355 11412
                              INTELSAT 904
                              1 27380U 02007A   05125.62541657  .00000043  00000-0  00000+0 0  5361
                              2 27380   0.0202   0.0174 0003259  40.3723 108.3316  1.00272510 11761
                              INTELSAT 905
                              1 27438U 02027A   05125.03693822  .00000000  00000-0  10000-3 0  5812
                              2 27438   0.0205 164.2424 0002820 218.0675 189.4691  1.00265924 10746
                              INTELSAT 906
                              1 27513U 02041A   05126.63564565  .00000012  00000-0  00000+0 0  4817
                              2 27513   0.0111 324.7901 0003200  99.2828  93.4848  1.00272600  9803
                              INTELSAT 907
                              1 27683U 03007A   05124.32309516  .00000000  00000-0  10000-3 0  3108
                              2 27683   0.0206  13.5522 0009594  61.6856 235.7624  1.00266570  8131
                              INTELSAT 1002
                              1 28358U 04022A   05124.94126775 -.00000018  00000-0  00000+0 0  1527
                              2 28358   0.0079 311.0487 0000613  59.4312 190.2817  1.00271159  3289
                              Figure 3.7 Two-line elements for some geostationary satellites.
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