1. Electromagnetic Radiation
LACC §4.2, 4.3, 4.5
• Electromagnetic (EM) Radiation as a wave
• Electromagnetic (EM) Radiation as a particle
• Interactions between EM Radiation
(e.g. light) and Matter
All we know about objects beyond our solar
system comes (almost) solely from examining
the radiation (e.g. light) they emit.
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2. Electromagnetic Radiation
is a wave
• EM radiation is pure energy (it has no mass)
• EM radiation results from the motion of
charged objects
• EM radiation travels at the speed of light
through a vacuum (and at lesser speeds
through matter)
• EM radiation is completely described by its
frequency, intensity, and direction of travel.
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3. Waves: Diffraction
If the wavelength is of a If the wavelength does
similar size to a gap ... not match the size of
then the wave will the gap, then only a little
diffract as shown diffraction will occur
below. at the edge of the wave.
http://www.gcsescience.com/pwav37.htm
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4. Waves: Interference
http://www.twow.net/ObjText/OtkCaLdQmB.htm
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5. Waves: Interference
The diffraction pattern of light The same when the beam passes
observed on a distant screen through two identical closely
when a He-Ne beam passes spaced slits.
through a single narrow slit;
http://www1.union.edu/newmanj/lasers/Light%20as%20a%20Wave/
light_as_a_wave.htm
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6. EM Radiation as a Wave
v = fλ
v = velocity
f = frequency
λ = wavelength
Q: What is v for light?
A: c, the speed of light
= 3x108 m/s
= 186,400 miles/s
http://www.bbemg.ulg.ac.be/UK/2Basis/freqlength.html
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7. E.g. Light
http://www.uark.edu/ua/pirelli/html/color_freq_wavelength.html
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8. Electromagnetic Radiation
is a particle
• atoms and molecules absorb and emit photons
• a photon is a single packet of EM energy
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9. Atoms Emit Photons
E = hf
E = energy
h = Plank’s constant
f = frequency
h = 6.626x10-34 J•s
This makes Plank’s constant
the smallest(?) constant in
physics.
http://www.astrosociety.org/education/publications/tnl/35/light3.html
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10. Atoms Absorb and Emit
Individual Photons
http://steve.files.wordpress.com/2006/03/Absorption%20emission.jpg
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11. The EM Spectrum
•
Credit: Philip Ronan who has
given permission to copy,
distribute and/or modify this
document under the terms of
the GNU Free Documentation
License, Version 1.2 or any
later version.
•
Download site: Wikipedia:
Image:EM spectrum.svg.
http://www.nhn.ou.edu/~jeffery/course/c_energy/energyl/lec001.html
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12. EM Radiation:
Wave or Particle?
Waves Particles
• interactions between • interactions between
waves results in particles result in
interference patters collisions
• radiate out from a • are “shot” out in
source specific directions
• can bend around • travel in straight
corners lines
• can bend around • are blocked by
obstacles obstacles
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13. Electromagnetic Radiation
LACC §4.2, 4.3, 4.5
• Electromagnetic (EM) Radiation as a wave
(v = fλ)
• Electromagnetic (EM) Radiation as a particle
(i.e. photons, E=hf)
• Interactions between EM Radiation
(e.g. light) and Matter: absorption/emission
of EM radiation by atoms/molecules
All we know about objects beyond our solar
system comes (almost) solely from examining
the radiation (e.g. light) they emit.
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14. LACC HW: Franknoi, Morrison, and
Wolff, Voyages Through the Universe,
3rd ed.
• Ch. 4, pp. 106-107: 11. Choose your answers from: radio |
microwave | infrared | visible | ultraviolet | X-ray | gamma ray.
Due at the beginning of next week’s first class.
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15. Spectroscopy
LACC §4.2, 4.3, 4.5
• Thermal Spectra: Wien’s Law, Stefan-
Boltaman Law
• Types of Spectra: there are 3 types of spectra
• Spectroscopy: what can it tell us?
All we know about objects beyond our solar
system comes (almost) solely from examining the
electromagnetic radiation (e.g. light) they emit.
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16. Thermal Radiation
http://astro.unl.edu/classaction/animations/light/meltednail.html
Blackbody Curves or Melting
http://cse.ssl.berkeley.edu/bmendez/
ay10/2002/notes/pics/bt2lf0612_a.jpg
http://astro.unl.edu/classaction/animations/light/bbexplorer.html
Blackbody Curves (NAAP)
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17. Thermal Radiation
T = Temperature
λ = peak wavelength
Wein’s law
http://feps.as.arizona.edu/outreach/bbwein.html
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18. Thermal Radiation
F= T 4
F = energy flux
σ = Stefan-Boltzmann
constant
T = temperature
Stefan-Boltzmann
law
http://csep10.phys.utk.edu/astr162/lect/light/radiation.html
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19. Types of Observed Spectra
http://instruct1.cit.cornell.edu/courses/astro101/lectures/images/lec07_04.jpg
http://astro.unl.edu/classaction/animations/light/threeviewsspectra.html
Three Views Spectrum Demonstrator
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20. Atomic Energy Levels
of Hydrogen
http://www.daviddarling.info/
encyclopedia/H/
hydrogen_spectrum.html
http://astro.unl.edu/classaction/animations/light/hydrogenatom.htmlBlackbody Curves (NAAP)
Hydrogen Atom Simulator (NAAP)
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21. EM Rad. & Space--Our Sun
http://www.weasner.com/etx/guests/2004/guests_spectra.html
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22. EM Rad. & Space--Orion N.
http://mais-ccd-spectroscopy.com/Planetary%20Nebula.htm
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23. EM Rad. & Space--M.W.
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24. Images vs. Spectra
Which is better, the image of an astronomical
object, or the spectrum of an astronomical
object?
What about photometry?
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25. Spectroscopy
LACC §4.2, 4.3, 4.5
• Types of Spectra: Continuous, Emission Line,
Absorption Line
• Thermal (or Blackbody) Spectra: Wien’s Law
(Temperature), Stefan-Boltaman Law (Power)
• Spectroscopy: Temperature, Composition,
Doppler Shift, Density
All we know about objects beyond our solar
system comes (almost) solely from examining the
electromagnetic radiation (e.g. light) they emit.
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26. LACC HW: Franknoi, Morrison, and
Wolff, Voyages Through the Universe,
3rd ed.
• Ch. 4, pp. 106-107: 23, 24.
• Ch 5: Tutorial Quizzes accessible from:
www.brookscole.com/cgi-brookscole/course_products_bc.pl?
http://
fid=M20b&product_isbn_issn=9780495017899&discipline_number=19
Due at the beginning of next class period.
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