Difference: Spectroscopy_Project (3 vs. 4)

Revision 413 Dec 2015 - JosephBayley

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Spectrocopy Project

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The main aims of this project are to observe a star to obtain its spectrum, then analyse this to find its composition and which line broadening methods are dominant in the star.
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The main aims of this project are to observe a star to obtain its spectrum, then analyse this to find where the lines come from and then determine which line broadening mechanisms are dominant in the star.

  • The project starts with calibrating the spectrometer so that the spectral lines can be measured.
  • The spectrum of a chosen star is then recorded and investigated.
  A link to the logbook for calibration, observation and meetings can be found here:
 
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