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See the accompanying graph (below) showing the relationship between h and d Transparency Master |
It is possible to determine the maximum visual contact distance from a ground based observer to a satellite in orbit around the Earth.
This maximum distance occurs at the instant that the satellite appears above the horizon. For low Earth orbit this distance approximates the radius of the visual footprint of the satellite. The figure to the left shows a satellite in a circular polar orbit travelling from horizon to horizon and exactly through the zenith (the point in the sky directly overhead). For convenience we have placed the observer at the North Pole, however the choice of location is arbitrary and the derived rules apply to all satellites, regardless of their orbit. If the satellite is orbiting at height h above the Earth, whose radius is re then simple geometric arguments show that the distance d from the observer to the satellite as it "just" rises above the local horizon is given by
d = retan
(eq.1)
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is defined as
= arccos(re/(re+h))
NOTE: arccos = cos-1 or inv cos on some calculators.
For any reasonable values of h, the satellite's altitude above the Earth's surface, the angle
can be computed and then d determined.
The graph below is a plot of equation (eq.1) above.
Transparency Master |
For low Earth orbits the distance to the horizon is the visual footprint of the satellite.
At the precise moment that the satellite comes into the view of the ground based observer, the ground based observer also comes into view from the satellite. The only difference is that the horizon of the ground based observer is fixed, whereas the horizon of the satellite moves along with the satellite. |
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