Astronomy                 Natural Science 1001

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Ed Wehling
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3. Light

Primary goals

  • Describe characteristics of light
  • Describe light that we receive from objects in space
  • Describe the Doppler effect and its applications

Basic characteristics of light   [sections 5.1 and 5.2  p. 138-143]

  • Why is the study of light so important to Astronomy?
  • Wave properties 
    --Describe wavelength
  • Particle properties 
    --Describe photons
  • Energy of light
  • Electromagnetic spectrum 
    --What are the regions of the electromagnetic spectrum?
    --How do they vary in wavelength and energy?
    --Links
       --How a spectrometer works (2nd bullet on right)
       --IR video

        --The Milky Way in different wavelengths
  • How do light and matter interact?
  • How can light tell us what stuff is made of?
  • Videos
    --research video 
    2 min What are gamma rays?

What do we see when we look in space?

For the next three headings [Section 5.4   p. 150-155]
Explanation D2L

Emission line spectrum   

  • What would we look at in space to see an emission line spectrum?
  • What does an emission line spectrum look like?

Continuous spectrum

  • What would we look at in space to see a continuous spectrum?
  • Describe the shape of the spectrum.
  • What is the relationship between total amount of light emitted by an object and the surface temperature of the object?
  • What is the relationship between the average energy of photons emitted by an object and the surface temperature of the object?

Absorption line spectrum

  • What would we look at in space to see an absorption line spectrum?
  • What does an absorption line spectrum look like?
  • Links
    --Some star spectra

Revisit Chemical Fingerprints

  • Videos
    --research video  3 min  how spectra are used to learn more about exoplanets (so-so)

Telescopes and the Electromagnetic Spectrum

Doppler Effect      [Section 5.5  p. 156-160]     Explanation D2L

  • Definitions
    --Red-shifting and blue-shifting
    --What happens to the light emitted by objects that are traveling
    away from each other? What does that light look like?
    --What happens to the light emitted by objects that are traveling
    toward from each other? What does that light look like?
    --Link
      --interactive of Doppler spectral shift of a star
  • Applications
     --Explain how the Doppler effect can help us determine the
    relative speed of two objects toward or away from each other
    --Explain how the Doppler effect can help us determine the
    rotation speed of an object

    For the rest of the topic see: [p. 368-371, 376]
    --We look into the sky and see one point of light. Explain how the Doppler effect can help us determine that there are actually
    two objects orbiting each other.
     --Explain how the Doppler effect can help us find
    planets around other stars.     Explanation D2L

    --Link
      --Radial velocity simulator from U Nebraska
      --YouTube

Other

 


©2000-2019     D. Edward Wehling                   Comments should go to ed.wehling@anokaramsey.edu

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