by engineerretired » Thu Nov 05, 2009 11:15 am
From my college astronomy notes (simplified version):
The Sun converts about 700 billion tons of hydrogen to helium every SECOND. Sounds like a lot but
when consider that the mass of the Sun is 1,989 billion billion billion kilograms, it is a very tiny amount.
As the temperature rises in the core, the density decreases, reaction rate goes down. Reduced reaction
rate (hydrogen fusion) causes core density to increase. It is a self-stabilizing cycle.
The sun has to be at least as old as the Solar System by definition, 4.5 billion years old. It should last about another 5 billion years, a few million years as a red giant, a few billion years as a white dwarf.
Hope this helps.