1. Light & Telescopes (Chapter 5) All of what we know and understand about the stars is the result of observation and analysis of light.

2. Student Learning Objectives Describe the properties of light Identify types and properties of telescopes

3. What are the properties of light?  Electromagnetic waves carry information as well as energy.  Light speed is constant in a vacuum (in space) 3 x 10 8 m/s 186,000 miles/sec 670 million mph

6.  The energy we are now observing from objects in space was generated at some time in the past. Sun 8 min. Proxima Centauri 4.2 LY Sirius 8.6 LY Andromeda Galaxy 2.5 x 10 6 LY

7. Practice: In a science fiction movie, when a spaceship explodes, we see and hear the explosion instantly. What are the mistakes in this scenario?

8. Wave Properties  Electromagnetic waves have a wavelength ( ) and frequency ( ). c =

10.  Electromagnetic radiation exhibits wave-particle duality.  Photons  No mass  Pure energy  Each photon of light carries energy.  The more photons, the higher the intensity. E = hc E = h

11. Electromagnetic Radiation http://www.chromoscope.net/ E Gamma Rays X-Rays Ultraviolet Visible Infrared Radio http://spaceplace.nasa.gov/ir-photo-album/en/

12.  We interpret particular wavelengths of visible light as particular colors! RedBlue 7000 Å5500 Å4000 Å CoolerHotter Less EnergyMore Energy ROY G BVROY G BV

13. Some of the Information in The Light Energy output Temperature Chemical composition Distance Relative Motion

14. Atmospheric Windows

15. Practice 1) What is the speed of a radio wave? 2) Which wavelength is longer? a.95.1 MHz b.1220 MHz

16. More Practice 3) Which star would be hotter, a blue star or a red star? 4) What affects the intensity of the light we receive from stars?

17. What are the main features of optical telescopes?  Reflection is a bounce (mirrors)  Refraction is a change in velocity (lenses)

18. Reflecting Telescope  Reflecting telescopes utilize a mirror.

19.  Refracting telescopes utilize a lens. Refracting Telescope

20. Newtonian Reflector Mirror  The objective or primary lens/mirror of the telescope is the most important part.

21. Refractor Issues  All refractors produce chromatic aberration (“color deviation or distortion”). Interesting Note: A very long focal length will minimize chromatic aberration. This is why the early refracting telescopes (like Galileo’s) were made very long.

22. Reflector Issues  Reflectors may produce a fuzzy image due to spherical aberration (curvature distortion). Hubble Images

23.  Advanced optical telescopes use floppy mirror segments controlled by a computer.Why?

24. Practice 1)What is the main purpose of a telescope? 2)Where are the telescopes that astronomers use? 3)Are there any telescopes that can be used during the day?

25. Mauna Kea, Hawaii (Elevation 14,000 Feet)

26. What are the functions of telescopes?  Light Gathering Power Ability of the telescope to collect photons. LGP = (Diameter) 2

27.  Resolving Power Ability of the telescope to “see” fine detail, and distinguish individual objects from each other  = (2.06 x 10 5 ) Diameter Larger D and Smaller sharper images

28. Image Credit: Richard Bloch An image of two stars through a telescope with low angular resolution An image of two stars through a telescope with high angular resolution.

29.  Magnifying Power Telescopes enlarge the image.  Atmosphere & Light affect observations. Mars with naked eye

31. Practice 1) Which telescope would allow you to see fainter objects? a.Small diameter telescope b.Large diameter telescope c.Either as long as there is good magnification 2) What are the advantages of space based telescopes?

33. What is a radio telescope?  A large parabolic dish gathers radio waves and reflects this energy to a central focus. Star formation regions SETI program

34. Interferometers  A single radio telescope has very poor angular resolution.  An interferometer is a set of radio telescopes connected together.  Constructive light Interference

35. NRAO

36. Detectors  Photometers: count photons Measure Intensity  CCD - Charge-Coupled Device: produce electronic images with millions of light detectors (pixels on a small silicon wafer) Measure Intensity per Pixel Camera!

37.  Spectrographs: use a grating to split light into individual wavelengths White Light → Rainbow  Adaptive optics: is a computer program that corrects for bad seeing Removes blurring caused by atmosphere Sun's Visible Spectrum

38. Image Credit: Canada-France-Hawaii Telescope

39. Image Credit: Gemini Observatory

40. Practice 1)What do people use everyday that has a CCD camera? 2)Optics are lenses and mirrors. How do adaptive optics differ from regular optics? 3)What are two tools that astronomers can use to produce the clearest image possible?