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Chapter 6 Optics and Telescopes

Chapter 6 Optics and Telescopes. Guiding Questions. Why is it important that telescopes be large? Why do most modern telescopes use a mirror rather than a lens? Why are observatories in such remote locations?

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Chapter 6 Optics and Telescopes

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  1. Chapter 6 Optics and Telescopes

  2. Guiding Questions • Why is it important that telescopes be large? • Why do most modern telescopes use a mirror rather than a lens? • Why are observatories in such remote locations? • Do astronomers use ordinary photographic film to take pictures of the sky? Do they actually look through large telescopes? • How do astronomers use telescopes to measure the spectra of distant objects? • Why do astronomers need telescopes that detect radio waves and other non-visible forms of light? • Why is it useful to put telescopes in orbit?

  3. Two Basic Types of Telescopes • Refractors • Use lenses to concentrate incoming light at a focus. • Reflectors • Use mirrors to concentrate incoming light at a focus. The goal is always the same – gather as much light as possible and concentrate it at a focus.

  4. Concept of Refraction: light slows and changes direction when it enters a denser medium.

  5. A refracting telescope uses a lens to concentrate incoming light at a focus.

  6. A refracting telescope actually uses two a lenses: an objective and an eyepiece. The two lenses are separated by the sum of their focal lengths.

  7. A lens creates an extended image of an extended object.lenses reverse images

  8. Three main functions of a telescope • Brighter image “light gathering power” isproportional to the area of the objective lens (pr2)

  9. Three main functions of a telescope • Brighter image “light gathering power” isproportional to the area of the objective lens (pr2) • Finer detail “resolution” or resolving power is proportional to the radius of the lens (r)

  10. Poor and Great Resolution (improved by using adaptive optics) Telescope images are degraded by the blurring effects of the atmosphere and by light pollution

  11. Three main functions of a telescope • Brighter image “light gathering power” isproportional to the area of the objective lens (pr2) • Finer detail “resolution” or resolving power is proportional to the radius of the lens (r) • Bigger image magnification = (objective lens focal length / eyepiece lens focal length).

  12. Spherical aberration Chromatic aberration Sagging due to gravity distorting the lens Unwanted refractions opaque to certain wavelengths of light Refracting telescopes have drawbacks

  13. Special achromatic compound lenses and lens coatings can often fix this aberration.

  14. REFLECTING telescopes solve many problems of refracting telescopes. Reflecting telescopes use a mirror instead of a lens to focus images.

  15. The secondary mirror in the tube does not cause a hole in the image. It does however make it a little dimmer because it reduces the total amount of light reaching the primary mirror.

  16. Drawback of Using Spherical Mirrors in Reflecting Telescope • Spherical Aberration • (can be corrected with a correcting lens)

  17. The largest research telescopes in the world are reflectors. The Keck I telescope on Mauna Kea on the Big Island of Hawaii uses 36 hexagonal mirrors to make a total diameter of 10 m. (Note the astronomers standing on either side of the platform.)

  18. A Charge-Coupled Device (CCD) An electronic device counts the photons arriving at a telescope’s focus

  19. Ordinary Photographs vs. CCDs

  20. Spectrographs record the spectra of astronomical objects.

  21. Spectrographs can be built into telescopes.

  22. Observations at wavelengths other than visible light are revealing previously invisible sights. Visible light image radio wavelength image

  23. Infrared observations reveal hot gases. UV infrared Map of Orion region Ordinary visible

  24. Telescopes in orbit around the Earth detect radiation that cannot penetrate the atmosphere.

  25. Other Space ObservatoriesChandra X-ray ObservatoryXMM-Newton X-ray ObservatoryCompton Gamma Ray Observatory

  26. The Entire Sky at the Visible Wavelengths

  27. The Entire Sky at the 21-cm Wavelengths

  28. The Entire Sky at the Infrared Wavelengths

  29. The Entire Sky at the X-ray Wavelengths

  30. The Entire Sky at the Gamma Ray Wavelengths

  31. Guiding Questions • Why is it important that telescopes be large? • Why do most modern telescopes use a large mirror rather than a large lens? • Why are observatories in such remote locations? • Do astronomers use ordinary photographic film to take pictures of the sky? Do they actually look through large telescopes? • How do astronomers use telescopes to measure the spectra of distant objects? • Why do astronomers need telescopes that detect radio waves and other non-visible forms of light? • Why is it useful to put telescopes in orbit?

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