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What is the minimum diameter of a mirror on a telescope that would allow you to resolve objects with angular separation of 3.5 cross times 10 to the power of negative 5 end exponent radians ? Assume an average wavelength of 550 nm for the light received.

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Answer:

the angular magnification of the telescope can be expressed as m 5 CQ36.9, one tree is a distance x from the lens and the other is at 2x.

Explanation:

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