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.

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

8. 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.

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

10. Three main functions of a telescope
Brighter image
“light gathering power” is proportional to the area of the objective lens (pr2)

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

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

15. Three main functions of a telescope
Brighter image
“light gathering power” is proportional 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).

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

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

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

21. 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.

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

23. 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.)

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

26. Ordinary Photographs vs. CCDs

27. Spectrographs record the spectra of astronomical objects.

28. Spectrographs can be built into telescopes.

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

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

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

36. Other Space Observatories Chandra X-ray Observatory XMM-Newton X-ray Observatory Compton Gamma Ray Observatory

37. The Entire Sky at the Visible Wavelengths

38. The Entire Sky at the 21-cm Wavelengths

39. The Entire Sky at the Infrared Wavelengths

40. The Entire Sky at the X-ray Wavelengths

41. The Entire Sky at the Gamma Ray Wavelengths

42. 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?