How are stars classified?
From white dwarfs to red giants, discover how astronomers have categorised the cosmos
Within our galaxy alone there are over 100 billion stars, so how do astronomers keep track of what’s what in the universe? From the late 19th century stars were classified based on ‘hydrogen lines’. These lines are gaps in the light spectrometry of stars, as the gases in their atmosphere absorbs certain light wavelengths. Those with the biggest hydrogen lines were classed as ‘A’ stars, descending in size going through the alphabet.
It wasn’t until the relationship between temperature, mass and luminosity was discovered that a new system was created. Astronomer Annie Jump Cannon condensed and reordered the system to O,B,A,F,G,K,M. Stars were arranged from hottest at O to coolest at M. This order is still used today.
In the current MK system, stars are also attributed a figure to indicate temperature scale, and a Roman numeral to indicate luminosity. For example, the Sun is a G2V star. ‘G’, places the Sun in a group of stars ranging in temperature between 5700 – 4700°C. ‘2’, indicates a subscale within the G group, 0 being the hottest and 9 being the coolest, and finally ‘V’ shows its place on the scale of luminosity – with ‘I’ being the brightest.
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Types of star
This article was originally published in How It Works issue 128
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