Earth's atmosphere is fully transparent only to visible and radio light.
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Q121: The light-gathering power of a telescope increases
Q122: Resolving power refers to the ability of
Q123: An achromatic lens brings all colors to
Q124: Both optical and radio telescopes can suffer
Q125: The amount of energy a photon carries
Q127: Far-ultraviolet rays have short wavelengths, low energies,
Q128: Spectrographs use a prism or a grating
Q129: Telescopes in space do not have the
Q130: All radio telescopes are refracting telescopes.
Q131: One of the advantages of charge-coupled devices
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