Lecture 7:Spectroscopy & Astrophysics Flashcards
1)properties of blackbody radiation 2)Wein's and Stefan Boltzmann's laws 3)Kirchhoff’s laws and properties (emission/ absorption lines) of spectra 4)Doppler effect of light
List the type of rays in order starting from lowest wavelength to highest wavelength
Thermal energy comes from kinetic energy of its internal particles. The greater its thermal energy, the hotter the object is
A blackbody is an ideal object that does not reflect any light and thus emits electromagnetic radiation in all wavelengths entirely as a result of its
temperature
Blackbody radiation: it refers to the light emitted by a blackbody
Wein’s law: The blackbody radiation consists of a continuous spectrum that peaks at a certain wavelength (or frequency
Peak of blackbody radiation = wavelength of maximum emission =>
wavelength at which the object looks brightest (gives colours to objects)
Stefan-Boltzmann’s law: The higher an object’s temperature, the more intensely the object emits electromagnetic radiation at all wavelengths and
the shorter the wavelength at which it emits most strongly
Explain Kirchoff’s three laws to do with the line spectrum of objects.
Explain the Lyman, Balmer, Paschen series of electron transitions
What is doppler effect?
When is blue shift seen when is red shift seen?