During the fusion process, how is mass converted into energy?
1 Answer
Explanation:
This is calculated using the famous equation of Einstein,
E = m c^2E=mc2
In Fusion reaction like the ones taking place in the core of a Star, there is enough pressure to fuse hydrogen nuclei to form one helium nucleus.
So, 4 hydrogen nuclei are fused together to form one Helium nucleus. But, where does the energy come from that keeps the Sun from collapsing?.
When 4 Hydrogen nuclei are merged together they show a certain discrepancy in the mass when a Helium atom is formed, i.e the mass of 4 Hydrogen atoms before Fusion is higher than the mass of the Helium atom after the reaction this mass defect is converted into energy by
"mass of a hydrogen atom " = " 1.00794 u"mass of a hydrogen atom = 1.00794 u
"mass of one helium atom " = " 4.002602 u"mass of one helium atom = 4.002602 u
Where
The mass defect,
Delta m = 4 xx m_H - m_(He)
= 4 xx "1.00794 u" - "4.002602 u"
= "0.029158 u " or" "4.8416859 * 10^(-29)"kg"
In the equation
This means that you have
E = 4.8416859 * 10^(-29)"kg" * (3 * 10^8)^2"m"^2"s"^(-2)
E = 4.35751731 * 10^(-12)" J per reaction"