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[APML] OT: Satellite orbital taxonomy
At 10:07 PM 5/22/2002, Paul M. Rybski wrote:
> ...that was why this location was such a good one in which to park a
> spy satellite. To find a geosynchronous satellite, you park a telescope
> at a specific altitude and azimuth, don't move it and make lots of
> integrations. During those integrations, stars will track through your
> field and possibly ruin an exposure of a fixed target. The more stars,
> the better. Couple trailing stars with a faint object moving
> orthogonally to the stars and you create a spy satellite that is very
> difficult to find. Then add orbit changes to this motion and you end up
> with a devilishly difficult object to find. I know because I had to do
> it and succeeded. But not without a very large (2.7 meter aperture)
> telescope and not without knowing the orbit of the satellite. With that
> same large telescope but without knowledge of the orbit, I would not have
> had a prayer of finding this very faint object, even away from the Milky
> Way plane. Note that a US quarter ($0.25 piece) placed a geosynchronous
> distance will exhibit a maximum magnitude of 18. My object was fainter
> than that most of the time. However, during maneuvering, the object
> could glint after sunset or before sunrise just like the object in the
> photo under discussion...
Paul,
That's really interesting. That info isn't classified? Obviously not I guess.
When you say that the target was darker than a quarter, it must have been
completely painted flat black (or even flocked), right? Was it solar
powered? How can solar collector panels be made stealthy? Is that why you
saw a glint?
Such satellites must have limited expected service life. Don't they use up
their propellant to change orbit? How long will it take for a typical one
of these satellite's orbit to decay?
--
Matt BenDaniel
matt@starmatt.com
http://starmatt.com
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