Some Early Stellar Spectra

⏱️ 2 minute read
MS125 connected to telescope

Introduction

Several years ago I connected the MS125 spectrometer to a 12 inch Meade LX200 telescope to test its suitability for recording stellar spectra. In order manually to guide on the star’s image the Oriel Sighting Optic was employed which you can clearly see in the photo here:

Exposure times were limited to under 5 minutes and several spectra were multiple integrations of 0.1 second exposure in order to build up each spectral acquisition.

Sirius
Sirius in the visible region showing all the principal hydrogen absorption lines H Alpha, Beta, Gamma, Delta and Epsilon
The emission spectrum of Messier 42, the Great Orion Nebula. H-alpha and H-Beta emission lines can be seen and 6563 Angstrom and 4861 Angstrom respectively, as well as emission lines due to doubly ionized O atoms (OIII) at 4959 and 5007 Angstrom which give this nebula its green tinge when observed visually. The narrow shoulder on the H-alpha line is due to singly ionized N atoms (Nii) at 6584 Angstrom.
Aldebaran
Alpha Tauri (Aldebaran), spectral type K5+ III
Betelgeuse
Betelguse (Alpha Orionis), spectral class M1-2
Capella
Capella (Alpha Aurigae), spectral type G3 III
Methane absorption Jupiter
Visible spectrum of the Sun and Jupiter showing the broad absorption band in the Jovian spectrum that is absent in the solar spectrum, and is due to methane absorption in Jupiter's atmosphere.

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