Hertzsprung–Russell diagram β€” temperature (X) vs luminosity (Y, log)
Surface temperature
O/B hotM cool

🌌 Astrophysics: Stellar Evolution (2D)

Spectral class: G
Temperature: 5800 K
Luminosity: 1.0 Lβ˜‰
Radius: 1.0 Rβ˜‰
Stage: Main sequence
FPS: β€”