Ed
Wehling
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Astronomy
Meteorology
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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
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