Eddington Luminosity Calculator

The Eddington luminosity also referred to as the Eddington limit, is the maximum luminosity any astronomical body can achieve when there is a balance between the force of radiation acting outward and the gravitational force acting inward. The state of balance is called hydrostatic equilibrium. Enter the stellar and solar mass in the Eddington luminosity calculator to find the Eddington limit.

m3/kg-1/s-2
m/s

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An Eddington limiting luminosity produced by the stellar object can be calculated based on the solar mass and stellar mass with this simple online Eddington luminosity calculator.