- #1
Ranguna
- 13
- 0
Is it possible to calculate how much Helium a star can produce when it reaches the end of the main-sequence, right before it starts burning Helium ( given if it has enough mass to do so) ?
And if it is possible then is it also possible to calculate how many materials a star can produce given it's mass ?
I'm kind of starting my journey into physics so forgive me if I write anything that might not be scientifically correct.
Thanks for reading.
And if it is possible then is it also possible to calculate how many materials a star can produce given it's mass ?
I'm kind of starting my journey into physics so forgive me if I write anything that might not be scientifically correct.
Thanks for reading.