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Telescopes
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Telescope History Galileo Galilei built first refractive telescope in 1609 Isaac Newton built the first reflective telescope in 1668
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1st Reflecting Telescope by Isaac Newton
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Optical Telescopes Telescopes that contain mirrors, lenses, or both
Three properties: Light-gathering power Resolving power Magnifying power
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Optical Telescopes Telescopes with larger mirrors/lenses:
Can“see”farther into space Have greater resolution Magnification can be changed by using different eyepieces Usually placed on mountain tops to reduce city lights
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Refracting Telescopes
Telescope uses two lens to bend or refract light Simplest of all telescopes First refracting telescope capable of magnifying objects 30 times.
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Objective Lens Most important lens is the objective lens
Bends the light from a distant object and focuses the light at the focus to produce an image The objective lens produces a very small, bright image of an object Focus= central point Focal length= distance between the focus and the objective lens
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Eyepiece Lens The second lens used in a refractive telescope
Eyepiece magnifies image produced by the objective lens
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Simple Refracting Telescope
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Disadvantages Shorter wavelengths of light are bent more than the longer ones Chromatic aberration: Weakens image and creates a halo of color around it When red light is in focus, a bluish halo appears. Very hard to produce a large piece of high-quality, bubble-free glass
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Yerkes Observatory Largest Refracting Telescope
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Yerkes Observatory Williams Bay, Wisconsin
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Refracting Telescope at Lick Observatory Southern California
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Lick Observatory
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Reflecting Telescopes
Uses a concave (curved) mirror that focuses the light in front of it Mirror is coated in a highly reflective material, an aluminum compound Two mirrors- one large & concave and one small & flat
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Reflecting Telescope
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Advantages No Chromatic aberration because reflected light is not dispersed into its component colors. Glass does not need to be high-quality because light does not pass through it. Disadvantage–secondary mirror blocks some light entering the telescope.
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Mount Palomar Observatory California
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Mirror for Hale Telescope at Mount Palomar Observatory
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Hale Telescope
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Keck Telescopes World’s Largest Reflecting Telescopes Hawaii
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Schematic of Keck Multiple Mirros Telescope (MMT)
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Kitt Peak Observatory Arizona
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La Palma Observatory Canary Islands, Spain
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McDonald Observatory Texas
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Cerro Tololo Observatory Chile
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Invisible Light Stars produce light wavelengths that are not visible to our eyes Gamma rays, X-rays, ultraviolet radiation, infrared radiation, and radio waves Most of these can not get past our atmosphere… so we must get our cameras above it!
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Radio Telescopes These big dishes are used to detect radio waves
Focuses incoming radio waves on an antenna and transmits these to an amplifier.
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Radio Signals Radio signals are weak so it requires a very large dish
These telescopes have poor resolution Radio Interferometer= Wire several telescopes together
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Advantages Less affected by turbulence in the atmosphere, clouds, and weather No protective dome is required = cheaper Can be used and “viewed” 24 hours a day Radio signals can pass through intersteller dust clouds
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Disadvantages Can be affected by human-made radio interference
Usually placed in valleys to block interference
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Largest Radio Telescope in World Arecibo, Puerto Rico
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VLA Radio Telescope Socorro, New Mexico
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VLA
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Space Telescopes Orbit above Earth’s atmosphere and produce clearer images
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Hubble Space Telescope
Built by NASA and sent in April 1990 10 billion times more light-gathering power than the human eye Given us amazing images of space
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Other Space Telescopes
Chandra X-Ray Observatory NASA uses to study X-rays Launched in 1999 Gather data about black holes Compton Gamma-Ray Observatory Used to study visible light and gamma rays In 2018, NASA will launch James Webb Space Telescope to study infrared radiation Run into many obstacles and budget problems
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