Stefan-Boltzmann Law.
AI-generated estimates. No guarantee of accuracy. We assume no liability for decisions based on these results. Independent verification is recommended.
Luminosity is the total amount of energy emitted by a star, galaxy, or other astronomical object per unit time. It depends on the radius and surface temperature of the star.
L = 4πR²σT⁴
(σ = 5.67×10⁻⁸ W/m²K⁴)
AI-generated estimates. No guarantee of accuracy. We assume no liability for decisions based on these results. Independent verification is recommended.