Cross-Section Hydrostatic Simulation
Equilibrium: Radiation Supported
Astrophysical Model Parameters
z ≈ 8.5 (660 Myr Post-BB)
Core Eddington (Γ)
12.5×
Photosphere Radius
14.2 AU
Surface Temp
4,200 K
Total Luminosity
4.8×10⁷ L☉
Quasi-Star Lifespan
720 kyr
Remnant BH Seed
10⁴ - 10⁵ M☉
JWST NIRCam Photometric Signature
Strong red excess in F356W/F444W relative to F150W due to cool 4,200 K envelope spanning 14.2 AU. Unlike standard Population III supergiants powered by CNO/fusion, radiation pressure from the internal black hole furnace inflates a convective sphere matching solar-system dimensions.