Source: wikibot/neon-burning-process
= Neon-burning process
{wiki=Neon-burning_process}
The neon-burning process is a phase in stellar evolution that occurs in the cores of massive stars, typically those with initial masses greater than about 8 times that of the Sun. This process occurs after hydrogen and helium burning phases and takes place when the core temperature reaches approximately 1 billion Kelvin (10^9 K). During neon burning, neon (Ne) is converted into heavier elements through nuclear fusion.