Mass-Luminosity Relation
- The more massive stars are generally the more luminous
- Luminosity varies as the fourth power of the mass
- Can be used to find the distance to binary star systems
Formula
- $\frac{L}{L_{sun}} = (\frac{M}{M_{sun}})^a$
- $L_{sun}$ and $M_{sun}$ are the luminosity and mass of the Sun
- $1 < a < 6$