Spectrocopy Project

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:


-- JosephBayley - 16 Nov 2015

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Topic revision: r4 - 13 Dec 2015 - JosephBayley

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