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Announcements

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Second test will be next week (W, Th) Looks like a great weekend ... Rosette nebula. Helix nebula. Emission of spectral lines. Hydrogen energy levels. Energy ... – PowerPoint PPT presentation

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Title: Announcements


1
Announcements
  • Homework 5 due Monday
  • Solutions to test are posted near south entrance
    to Science Lab building (until next test)
  • Second test will be next week (W, Th)
  • Looks like a great weekend for projects! (Due
    two weeks from today)

2
Spectroscopy
  • 29 September 2006

3
Today
  • Splitting light into separate colors
    (wavelengths)
  • Spectra of thermal light sources
  • Spectra of nonthermal light sources
  • Absorption spectra
  • How does motion of a light source affect its
    spectrum?

4
Thermal Light Sources(Hot, opaque objects)
  • Emit a continuous spectrum (all colors present)
  • Hotter implies brighter
  • Hotter implies bluer in color
  • Brightness color dont depend much on what the
    object is made of
  • Examples incandescent light filaments (3000 K)
    electric heating coils (1500 K) coals in a
    campfire (1500 K) your body (310 K) the sun
    minus its outer layers (6000 K)

5
Graphs of thermal spectrum
6
Orion star colors
7
Infrared light is real!
8
Emission Spectra (nonthermal)from hot,
transparent gases
9
Hydrogen emission spectrum(Balmer lines)
10
Rosette nebula
11
Helix nebula
12
Emission of spectral lines
13
Hydrogen energy levels
Energy --gt
14
Nonthermal Light Sources(Especially hot,
transparent gases)
  • Emit only a few precise wavelengths (colors)
  • Temperature matters less than chemical
    composition
  • Each element has its own spectral signature
  • Examples mercury and sodium vapor lights
    lasers (just one wavelength) interstellar gas
    clouds

15
Thermal source plus cool gas
16
Absorption lines in suns spectrum
17
Three types of spectra
18
Spectrum photo vs. graph
19
What if a wave source is moving?
Doppler effect
20
Doppler-shifted absorption spectra
shift in wavelength speed of source,
as of speed
of light
21
Doppler-shifted absorption spectra
shift in wavelength speed of source,
as of speed
of light
22
Doppler-shifted absorption spectra
Shorter wavelengths implies its moving toward us
Wavelengths are shifted by about 10 units
(Angstroms) out of 4000, or 1 part in 400.
Therefore this object is moving toward us at
1/400 the speed of light (750 km/s)
23
The Physics of Light
  • Speed 300,000 km/s
  • Brightness of a source is measured in watts (a
    unit of power, energy/time)
  • Diffraction indicates wavelike behavior
  • Made of tiny units called photons
  • Wavelength determines color and photon energy
  • Hot, opaque object emits continuous spectrum,
    brighter and bluer if hotter
  • Hot, transparent gas emits bright-line spectrum
  • Thermal source viewed through cooler gas has
    dark-line absorption spectrum
  • Doppler-shifted spectral lines indicate motion of
    source toward or away from us
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