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A) improve the angular resolution of radio telescopes.
B) speed up the processing of CCD images.
C) decrease the effects of light pollution in getting darker sky backgrounds.
D) yield better seeing conditions with optical telescopes.
E) increase the sensitivity of infrared telescopes to longer wavelengths.
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A) they record colors better than film can.
B) they can cover larger areas of the sky than film can.
C) their images never fade, as film can.
D) they record much more light in a given exposure time.
E) their images do not have to be developed as film does.
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A) aperture
B) magnification
C) resolution
D) interference
E) light grasp
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A) 9
B) 16
C) 4
D) 2
E) 8
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A) separate light into its component wavelengths.
B) measure the brightness of stars very accurately.
C) collect a large amount of light and bring it into focus.
D) make distant objects appear nearby.
E) magnify distant objects.
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A) have the same light gathering power.
B) have more light gathering power.
C) have more chromatic aberration.
D) have a larger hole in the center of its mirror.
E) be easier to build.
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A) Lenses absorb light, while mirrors do not.
B) Lenses are subject to chromatic aberration.
C) Heavy lenses, which can only be supported at their edges, tend to deform under their own weight.
D) A lens must have two precision surfaces; a mirror needs only one.
E) Lenses are harder to focus than mirrors.
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A) Einstein
B) Kepler
C) Chandra
D) Hubble
E) Fermi
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