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5 Cards in this Set

  • Front
  • Back

Droppler shift

Red shifting: object going away from us, wavelength is longer


Blue shifting: object no c in toward us, wavelength is shorter

Blackbodies

Perfect absorber of light at all wavelengths


Blackbody radiation

Energy emitted by black body

3 quantities we get from examining spectrum of a star

1. Velocity


2. Composition


3. Temperature

Kirchoffs' Laws of spectra

Continous spectrum (all colors) Solid, liquid, or a hot dense gas.



Emission line spectrum (abrupt spikes in brightness) Electrons falling from high energy to low.



Absorption line spectrum (wavelengths with little light) Electrons jumping from low levels to high.