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Observing over the entire electromagnetic spectrum
•Different phenomena produce different wavelength waves
–Ordinary stars:  Visible light
–Cool planets or dust clouds:  Infrared light
–Moving charged particles, cool molecules:  Radio waves
–Very hot objects:  X-Rays and Gamma Rays
–Quasars: ALL wavelengths
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•Only visible, some IR, and radio make it through atmosphere
–Need to observe from space for other wavelengths
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•Going into space also lets you obtain more detailed images
–On Earth telescope size isn’t only limit on image resolution
–Temperature fluctuations in atmosphere cause “seeing” (blurring)