Classifying Stars

This lesson covers:

1The classification of stars by temperature and colour

2Absolute and apparent magnitude

3The Hertzsprung-Russell diagram

Star temperature and colour


When gazing at the stars, not all stars look the same. Some appear brighter and/or a different colour. Astronomers examine the light emitted by stars and categorise them by colour and temperature.


Hot stars appear blue or white in colour. Cooler stars appear red. Our sun has a temperature of 5,800 K and so appears yellow-white to us on Earth.


The amount of energy emitted by a star per second is known as its luminosity. The brighter the star, the higher the luminosity.


Chart showing star colour and corresponding surface temperature in Kelvin. Blue stars are above 11,000 K, blue-white stars are between 7,500 and 11,000 K, white stars are between 6,000 and 7,500 K, yellow-white stars are between 5,000 and 6,000 K, orange stars are between 3,500 and 5,000 K, and red stars are below 3,500 K.

Apparent magnitude


When observed from Earth, some stars appear brighter than others. This could either be because they emit more light, or because they are closer to us.


We measure this brightness using the apparent magnitude scale which is a measure of how bright a star appears from Earth.


Oddly, the lower the number, the brighter the star appears from Earth.


An apparent magnitude of -1 would appear significantly brighter than a star with an apparent magnitude of +2.


Absolute magnitude


Absolute magnitude on the other hand is a measure of the intrinsic brightness of a star (its luminosity), at a specific distance from Earth. Specifically, it is the apparent magnitude a star would have if it were observed from a standard distance of 10 parsecs (about 32.6 light-years).

Diagram illustrating absolute magnitude with two stars at different distances from Earth.

In the example above, star A and star B are identical, but Star A will appear brighter to an observer on Earth because it is closer. In other words, star A will have a lower apparent magnitude (remember that apparent magnitude has the weird scale where lower values mean brighter).


However, because both stars are identical, if they were the same distance from earth (e.g. 10 parsecs), then they would be equally bright. Both stars therefore have the same absolute magnitude.


The Hertzsprung-Russell diagram

The Hertzsprung-Russell diagram showing the relationship between the temperature and luminosity of stars.

x-axis


The x axis of the Hertzsprung-Russell diagram is temperature in Kelvin. (Note that the values decreases as you go along the x-axis).


Hot stars will therefore be on the left and cool stars will be on the right.

Which colour is associated with hot stars?

White

Yellow

Red

Blue

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What does the apparent magnitude scale measure?

Star temperature

Star brightness from Earth

Star luminosity

Star distance from Earth

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What is the main difference between absolute magnitude and apparent magnitude?

Absolute magnitude compares star distance from Earth, while apparent magnitude compares star distance from the sun

Absolute magnitude compares star brightness from Earth, while apparent magnitude compares star brightness at a standard distance

Absolute magnitude compares star brightness at a standard distance, while apparent magnitude compares star brightness from Earth

Absolute magnitude compares star temperature, while apparent magnitude compares star color

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What does the x-axis of the Hertzsprung-Russell diagram represent?

Star luminosity

Star brightness from Earth

Star temperature

Star distance from Earth

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Where are the hottest stars located on the Hertzsprung-Russell diagram?

Right

Bottom

Top

Left

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