Page 59 - Communications Satellites Global Change Agents
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2.  EVOLUTION  OF SATELLITE  TECHNOLOGY                        35

           Arthur Clarke has  a truly magical gift  for writing  solid  works  of  science  and
         engineering while also spinning yarns of science fiction, including 2001: A Space
         Odyssey.  In  1945 he was an unknown; consequently, his brief but  seminal article
         was largely ignored. Yet the entire vision was there. In succinct but clear terms, he
         spelled out a remarkably practical vision of what the future  of space applications
        might bring. He described how we might someday  establish a global  communica-
        tions system with just three  satellites by calculating the speed necessary  to launch
        a "space station" into geostationary  orbit and establish  radio  stations  beyond  the
        ionosphere. The satellite application he used as a way of illustration was the relay
        of TV signals, although TV was then in its infancy. Today, TV relay still  remains
        the  most  dramatic  application  of  communications  satellites.
           Clarke  described  a  special  orbit,  which  was the  only one whereby  a  satellite
        precisely  encircles  the  earth  once  a  day  without losing altitude or  escaping  the
        world's gravitational field and thus flying off into space. This magical orbit where
        the "g" force is exactly 0.22  meters/second 2  allows a satellite to remain stationary
        with respect to a constant point on the earth's  equator. Thus, a satellite, once  posi-
        tioned  in orbit  some  22,230  miles or  35,870  kilometers  above  the  equator (with
        only  modest  orbital adjustments from  microjets  to  correct  for small north-south
        or  east-west  excursions)  will  stay  in  place  for  long  periods  of  time.  A
        geosynchronous  satellite,  located  in  what  is  now  called  a  GEO  orbit,  thus  be-
        comes  much  like a  very,  very tall radio  relay tower  in the  sky.  The  satellite re-
        ceives the faint up-link signal, filters out noise and interference, translates it to the
        down-link frequency (to prevent interference), amplifies it, and then retransmits  it
        back  to  earth  (see  Fig. 2.1).
           With such a high tower, a radio transmission can reach across  the oceans  and,
        in  fact,  "see"  40%  of  the  way  around  the  earth  at  the  equator.  Clarke's  land-
        breaking (or rather  space-breaking)  article explained  how three  such  satellite ra-
        dio  stations  equally spaced  above  the  equator  could  connect  the  world  together
        and  serve  the  entire  planet  except  at  the  polar  caps.
           Due to the earth's curvature, a microwave  tower  over  500 miles  (or over  800
        kilometers) high would be required to "see"  across the Atlantic Ocean and a much
        taller one still to  "see"  across  the Pacific Ocean.  Of course  such towers  were not
        economically  or  technically  feasible.  Yet,  Arthur  Clarke  discussed  how  it  was
        possible  to  build  one  that  was  over  22,230  miles  (or  35,870  kilometers)  high.
        Such  a  relay  tower  in  space  could  do  what  a  physical tower  built  up  from  the
        earth's  surface  could  not  do  in  a practical manner.
           Brilliance  and vision is not always immediately  recognized. Galileo,  Colum-
        bus, Kopernicus, Goddard, and many others found their "new ideas" ridiculed or
        ignored  at  first.  Such  was the  case  with Clarke,  whose  article  was only  recog-
        nized for its greatness  in retrospect.  This was,  in part, due to Clarke's own be-
        liefs that these radio towers  in space  would need human crews to constantly re-
        place  burnt-out  radio  tubes,  and  that  space  travel  and  reliable  rocket  systems
        were  simply  too  far  in the  future  to be  seriously  considered  in the  short  term.
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