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square17320509
In general the reflecting optical telescope has a large-aperture concave mirror for gathering and focusing light from astronomical bodies. As you've known, larger the size of mirror becomes, more difficult making such mirror with sufficient accuracy. Here is an alternative method to avert such difficulty;

http://hecoaustralia.fortunecity.com/telescope/reflect.htm
Montec
Hello square17320509

Would not the reduction in aperture of the "scanning beam" reduce the light gathering ability of the telescope?

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square17320509
QUOTE (Montec+Nov 19 2007, 07:17 PM)
Hello square17320509

Would not the reduction in aperture of the "scanning beam" reduce the light gathering ability of the telescope?

smile.gif

That's it cool.gif As mentioned in my site, it would require the exposure time longer than that of ordinary reflecting telescope.
Montec
Hello square17320509

May I suggest multiple scanning beams with computer integrated image software as a solution. Something similar to a DLP projection system but only in reverse.

smile.gif

square17320509
QUOTE (Montec+Nov 21 2007, 09:00 PM)
Hello square17320509

May I suggest multiple scanning beams with computer integrated image software as a solution. Something similar to a DLP projection system but only in reverse.

smile.gif

Oh, that's a nice idea! But I think ususal CCD is still available for the image sensor rather than using expensive devices such as DLP.
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