Most stars occupy a very small volume in luminosity - mass space. In this section we will derive the analytic relations between those variables. We will assume that stars are characterised by a mass , radius , density , luminosity , typical temperature , typical pressure and photon mean free path .
From the condition of hydrostatic equilibrium
The luminosity can be estimated in the following way: the energy density is assumed to be that of black body where is the radiation constant. The volume of the star is . The time it take a photon to cross is . Hence the luminosity can be estimated as
The density can be expressed in terms of the mass and radius
If the material is dominated by gas pressure, then
If, instead, the material is dominated by radiation pressure
If the gas is fully ionised, then Thomson opacity can be used
If not, then Kramer's opacity gives a better approximation
In the next sections we will discuss each combination.