function radiusFromLuminosity
universe/src/catalog/photometry.ts:286
radiusFromLuminosity(solarLuminosities: number, temperature: number) → number
Stefan-Boltzmann, in solar units: R/R☉ = √(L/L☉) · (T☉/T)².
- solarLuminositiesnumber
- Undocumented
- temperaturenumber
- Undocumented
Returnsnumber