Stellar Spectra

In the constellation CYGNUS you can find the fine double star Albireo. It is the head of the flying swan on his long craned neck. Even with a small telescope you will see a double star with a wonderful contrast of colour. The brighter star gleams orange, the dimmer in a beautiful light blue.
CYGNUS Albireo
What is the reason for the different colours? You may find a similar phenomenon at home if you have an electric light bulb with a dimmer. If you dim your lamp down you will see the filament glowing dark orange. At full power the lamp is more yellow or white. But the light bulb is not really white. Comparing the light bulb with the sun we will find the bulb shines orange and the sun in a light yellow.

Hence we have two sequenzes:
Colour dark orange orange yellow
Temperature 2000 K 3500 K 6000 K

The colour of the integral light of the stars tells us about the temperatures of the stars!
Now, if we break up the light into the colours of the rainbow we might even learn more about the physical properties of the stars.

(And if you think about your lamps, the colours of the stars and their brightness, you might learn something about the radii of these stars :-)

Next: The Formation of Stellar Spectra

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