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Optical Telescopes

3.1. Using Technology to See the Visible Telescopes allow us to see objects that are very distant in space. Optical Telescopes. In 1608, Hans Lippershey made one of the first telescopes – but it was Galileo Galilei who made practical use of it. Optical telescopes are ‘light collectors’.

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Optical Telescopes

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  1. 3.1. Using Technology to See the VisibleTelescopes allow us to see objects that are very distant in space.

  2. Optical Telescopes • In 1608, Hans Lippershey made one of the first telescopes – but it was Galileo Galilei who made practical use of it. • Optical telescopes are ‘light collectors’. • The series of lenses or mirrors enable the optical device to collect and focus the light from stars.

  3. Refracting Telescopes • A refracting telescope works just like a magnifying glass. • It uses a convex glass lens (to bend light and bring it into focus. • This lens is thicker in the center than it is toward its edges, which bends the light more at the edge of the lens than light coming through the center. • This allows all of the light to come together at a focus point. • If someone looks into the eyepiece, a concave lens magnifies the image.

  4. Problems • Refracting telescopes have two main problems—images are not always clear because the light is being bent and the size of the lens is limited (which limits the power of the telescope). • Yerkes Observatory- Largest reflecting telescope in the world.

  5. Reflecting Telescopes • Reflecting telescopes use curved mirrors instead of convex lenses to collect and focus light. • A large concave mirror (the center is thinner than the edges) collects and reflects the light to make an image. • Once the image forms, the lens in the eyepiece magnifies the image. • Reflecting telescopes are very helpful for viewing dim or dark objects. • Large reflecting telescopes can see objects that are a millionth or a billionth the brightness of the faintest star that can be seen by the human eye alone!

  6. Reflecting Telescopes • One of the newest innovations for ground-based optical reflecting telescopes is the use of segmented mirrors (a segmented-mirror telescope uses several lightweight-segments to build one large mirror).

  7. Interferometry: Combining Telescopes For Greater Power • The technique of using a number of telescopes in combination is called interferometry. • When working together, these telescopes can detect objects in space with better clarity and at greater distances than any current Earth-based observatory.

  8. Hubble Space Telescope • To improve the views of space, astronomers are able to access images from a telescope in space. • Free from the interferences of weather, clouds humidity and even high winds.

  9. Hubble Facts • Hubble Space Telescope, launched in 1990, orbits 600 kms above the Earth, collecting images of extremely distant objects. • It is a cylindrical reflecting telescope, 13 m long and 4.3 m in diameter. • It is modular (parts can be removed and replaced) and is serviced by shuttle astronauts.

  10. Images from Hubble

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