Stellar Spectroscopy

Simple Stellar Spectroscopy achieved by viewing starlight through a fine diffraction grating (similar to a prism producing a rainbow) and analysing the diffracted image using RSpec software. Spectroscopy gives information on the type and composition of stars by analysis of the emission or absorption lines present in the resultant spectrum. This can be done mounting the diffraction grating as a filter on an ordinary digital camera and lens setup or a specific astronomical telescope.

The Star Analyser 100 is a diffraction grating with grooves that are spaced at 100 lines/mm. The grating is mounted in a standard 1.25″ filter cell and is protected on both sides with anti-reflection coated glass. Star Analysers can be obtained here https://rspec-astro.com/star-analyser/.

Examples below are my first few attempts…

VEGA:

Alpha Lyrae]

Vega is the brightest star in the northern constellation of Lyra and it is the fifth-brightest star in the night sky.

Spectral type A0Va. Main sequence.

SADR:

[Gamma Cygni]

Stellar Classification F8 Iab.

Deneb:

[Alpha Cygnii]

Deneb is a bluish-white star of spectral type A2Ia, with a surface temperature of 8,500 kelvin. Deneb is the brightest star in Cygnus and the 19th brightest star in the night sky.

Altair:

[Alpha Aquillae]

Altair is a type-A main-sequence star with about 1.8 times the mass of the Sun and 11 times its luminosity. Altair is the brightest star in the constellation of Aquila and the twelfth-brightest star in the night sky.

Spectral type A7V

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