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TELESCOPES

HOW THEY WORK | WHY WE USE THEM

HOW DO TELESCOPES WORK?

FOR YOUR NOTEBOOK:

Lesson 2 Notes and Vocabulary:


  1. Perspective - the height, width, and depth of an object from the viewer

  2. Telescope - an optical instrument designed to make distant objects appear nearer

    • Goals:

      • Gather as much light as possible

      • Increase the apparent size of the object

    • Parts:

      • Lens - curved piece of glass that refracts light which can magnify or reduce the image of the perceived object

      • Mirrors - reflective surfaces that can be used to bend light the way we want it.

    • Early Telescope:  

      • Had and OBJECTIVE LENS - Lens facing the object that rays refract through.  Convex in shape to focalize the rays.

      • Rays cross each other so the image appears upside-down!

      • Rays hit a second Convex Lens called EYE PIECE Lens which straightens the rays

    • Newer Telescope

      • Instead of a Convex Object Lens, it uses a Concave Mirror

      • Rays enter, hit the mirror, bend toward another mirror which bounces the light to the eye piece lens.

  • Hubble Space Telescope

    • Advantage is that it eliminates Atmospheric Distortion.  In space, we don’t have atmosphere/air, so nothing distorts our image of the rest of space.  

  • Crazy Amazing Humans:  they’ve created other telescopes out there using cameras that receive other types of radiation to create images.  We can learn about stars and planets using heat signatures and even X Ray to Gamma Ray signatures.

HUBBLE SPACE TELESCOPE

VERY EARLY TELESCOPE

EARLY TECH | CURRENT USE | BINOCULARS

EARLY TECH | CURRENT USE | HIGHER POWER BINOCULARS

WHAT WE USE NOW TO SEE SPACE FROM EARTH

MODERN RADIO WAVE TELESCOPE

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