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Spectra of the bright stars of Cassiopeia

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About this observation
Observer
Hugh Allen
Time of observation
11/02/2018 - 20:30
Object
Bright stars of Cassiopeia
Observing location
Oakhill Somerset
Equipment
8" Meade LX90 at f6.3
Alpy 600 spectroscope
Ati 314L mono camera
Spectra processed in BASS software
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Over the last few months I have been spending much of my spectroscopic observing time following the eclipse of VV Cep. This night  I decided to relax with a little project on the contrasting spectra of the bright stars of Cassiopeia. They include the famous gamma Cassiopeiae whose spectrum shows intensely bright hydrogen Balmer emission lines first observed by Angelo Secchi, one of the 19th century pioneers of astronomical spectroscopy. The other stars wonderfully illustrate how photospheric temperature affects the shape of the spectrum and the expression of elemental absorption lines, ranging from 18,000 Kelvin (spectral type B3) down to 5,200 Kelvin (spectral type K0). Cassiopeia is a beautiful constellation both visually and spectroscopically.

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