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Hertzsprung-Russell Diagram: Understanding Stellar Evolution and Classification #3730242 (License: Personal Use)
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This Hertzsprung-Russell (HR) diagram visualizes stellar properties across evolutionary stages: the diagonal main sequence hosts hydrogen-fusing stars like our Sun; upper-right red giants and supergiants are cooler but highly luminous; lower-left white dwarfs are hot yet dim remnants. Color gradients and labeled clusters-including spectral classes O through M-illustrate how temperature correlates with color and spectral type.
Used in astronomy education, research, and outreach to teach stellar evolution, classify observed stars, and interpret telescope data; ideal for users seeking foundational astrophysics knowledge or visual aids for academic content.
Related Cliparts: Explore the Hertzsprung-Russell diagram-a cornerstone of astrophysics-mapping stars by surface temperature and luminosity to reveal their life cycles.
(view all Hertzsprung-Russell Diagram: Understanding Stellar Evolution and Classification)
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