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Telescopes. Refractors and Reflectors Various Designs Important Properties Modern Advances Beyond Visible Light. Basic Optics - Refraction. Light is bent or refracted when it changes speed going through a lens or prism. Where the refracted rays meet is the “focal point.” - PowerPoint PPT Presentation

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  • TelescopesRefractors and ReflectorsVarious DesignsImportant PropertiesModern AdvancesBeyond Visible Light

  • Basic Optics - RefractionLight is bent or refracted when it changes speed going through a lens or prism.Where the refracted rays meet is the focal point.Distance from the lens to the focal point is the focal length.

  • Basic Optics - ReflectionWhen light strikes a mirror it is reflected at an angle equal to its incident angle.Rays of light striking a curved mirror will meet at a focal point.The distance from the vertex of the mirror to the focal point is the focal length.

  • Reflectors and RefractorsA reflector telescope has a mirror as its objective.A refractor telescope has a lens as its objective.The main function of a telescope is to gather light.

  • Chromatic AberrationDifferent wavelengths focus at different distancesWorlds Largest Refractor - Yerkes Observatory

  • Reflectors

  • Why Mirrors?Light gathering power - size matters!lgp increases with the square of the radiusMore lgp, more resolution!Magnification is third!

  • 200 Hale Telescope Mt. Palomar

  • Comparing lgp lgp depends upon the area of the lens or mirror; A = r2

    lgp = (Dbig/Dsmall)2

  • Calculating Magnificationfobjfeye

    M =Mmax = 20 x Dcm

  • Practical Limit of MagnificationSmaller focal length eyepieces give greater magnification.They also limit light & increase diffraction.At some point the image is too poor to be useful.

    Mmax = 20X____cmx D

  • Resolving PowerThe ability of a telescope to distinguish two objects.Measured in arcseconds ( 1 arcsecond is 1/3600)a =11.58_______D (in cm)

  • Modern AdvancesBinocular TelescopesLBT - two 8.4 m mirrors with adaptive opticsLGP of an 11.8 m mirrorDetail of a 22.4 m mirrorSurpasses HST in clarity

  • Adaptive OpticsCorrect for atmospheric turbulenceUse the light from a guide star or laser to determine what the atmosphere is doing to the light passing through it.Distortable mirror will change shape to correct the image.

  • Beyond Visible LightRadio Telescopes

  • VLA Telescope

  • UV and X-Ray TelescopesSOHOChandra

  • HST and James Webb

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