•Luminosity of sun: 3.8 ´ 1026 J/s
•
•H
burned rate:
•
•H atoms available:
•
•Lifetime:
•
•
•In reality not all the atoms we start with are H, and
only those near the center are
available for fusion. The
structure of the sun will change
when about 10% of the above total have been used, so after about 10 billion years.