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Published byCecil Cook Modified over 8 years ago
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Light, Optics and Telescopes The Electromagnetic Spectrum
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Photons of different energies radiate at different wavelengths or frequencies wavelength x frequency = velocity of light ( c) = c
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Atmospheric Windows Visible and radio
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Physical Properties of Light Refraction
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Reflection Refraction is wavelength dependent
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Formation of an image
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Telescopes -- Refractors Yerkes Observatory – Lake Geneva, Williams Bay Wisconsin
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20 th Century Large Reflectors Mt Wilson 100-inch – 100 yrs old Cerro Tololo 4 -meter Palomar 200-inch
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Modern Observatories Cerro Tololo Interamerican Obs.
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Kitt Peak National Obs. Tucson Arizona
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Very Large Telescopes Mauna Kea ESO – VLT
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MMT on Mt. Hopkins, AZ
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Minnesota’s $5M (private) investment in a very large telescope (> $100M) Large Binocular Telescope (LBT) Mt. Graham Arizona Design Other partners -- University of Arizona, Germany, Italy, Ohio State University, University of Virginia, Notre Dame
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Radio Telescopes
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Arecibo Very Large Array – VLA
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Telescopes in Space -- other wavelengths – UV, X ray, gamma ray and far-IR
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