How to use this tool
Check the units, enter your values, and run the tool. Results follow the assumptions and method below.
Calculation method
Blackbody luminosity
4*pi*radius^2*5.670374419e-8*temperature^4Stefan–Boltzmann luminosity of a spherical star at its effective temperature.
Stefan–Boltzmann luminosity of a spherical star at its effective temperature.
Enter your values and run the tool to see your result.
Check the units, enter your values, and run the tool. Results follow the assumptions and method below.
4*pi*radius^2*5.670374419e-8*temperature^4