Scientists classify stars based on several key characteristics, including their temperature, luminosity, size, and spectral type, which is determined by the absorption lines in their spectrum. The Hertzsprung-Russell diagram is a common tool used to visualize the relationship between a star's luminosity and temperature, allowing for further categorization into groups such as main sequence stars, giants, and white dwarfs. Additionally, the chemical composition of a star can also influence its classification.
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