A star initially has 1040 deutrons. It produces energy via the processes
H2+,H2⟶,H3+pH2+H3⟶2He4+nThe masses of the nuclei are as followsM(H2)=2.014 amu: M(p)=1.007 amu: M(n)=1.008 amu; M(He4)=4.00 lamu
If the average power radiated by the star is 1016 w,the deutron supply of the star is exhausted in a time of the order of