Loading Stellar Simulator...
Main Sequence Star
A main sequence star is in the stable part of its life, fusing hydrogen into helium in its core.
Current Fusion Process
Hydrogen → Helium
Star Composition
Hydrogen: 70%, Helium: 28%, Other: 2%
Layers
Core: 15 million K, fusion reactions
Radiative Zone: Energy transport via radiation
Convective Zone: Energy transport via convection
Photosphere: Visible surface
Chromosphere: Lower atmosphere
Corona: Extended outer atmosphere