For a family in stellar homology, dimensionless radial profiles are fixed. Mass conservation and hydrostatic equilibrium then give the central scalings
The ideal gas equation of state, with fixed mean molecular weight, consequently gives
where fixed dimensional constants such as are suppressed in homology relations.
The proton–proton chain law gives the nuclear luminosity
On the other hand, radiative diffusion in a star gives
Using the Kramers opacity law ,
Thermal equilibrium requires . Their common mass factor cancels, leaving , and hence
This model captures the gas-pressure support, pp-chain burning, and strongly mass-dependent luminosity of the lower main sequence, including the Sun approximately. Its fully radiative assumption is an idealization: the Sun has a convective envelope, and sufficiently low-mass red dwarfs become largely or fully convective, so real radii are not exactly constant.
For a homologous star, hydrostatic equilibrium, mass conservation, and the ideal gas equation give the central scalings
where is the mean molecular weight. Integrating the nuclear energy-generation law over a fixed homologous profile gives
Radiative stellar structure gives independently
Equating the two luminosities yields
At fixed zero-age composition, the stars are therefore homologous with
The effective temperature satisfies , so . The zero-age main sequence consequently has
It is a steep line rising toward high luminosity and high temperature on a Hertzsprung-Russell diagram.
For fully ionized hydrogen and helium with ,
while . At fixed mass,
and the corresponding radius relation is
At the pure-hydrogen zero-age point ,
whereas
Hence
and
As hydrogen is consumed, falls, so both and rise. In the usual diagram with temperature increasing leftward, the evolutionary track initially moves upward and leftward from the zero-age main sequence.