A scatter plot showing the relationship between stars' absolute magnitude (brightness) and spectral class (temperature), revealing distinct groupings like the main sequence, red giants, and white dwarfs. It serves as the fundamental tool for understanding stellar evolution and the life cycles of stars.
Named after Danish astronomer Ejnar Hertzsprung and American astronomer Henry Norris Russell who independently developed similar diagrams around 1910-1913. The diagram revolutionized astronomy by showing that stars follow predictable evolutionary paths rather than being randomly distributed in brightness and color.
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