During the fusion process, how is mass converted into energy?

1 Answer

E = mc^2E=mc2

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 E = mc^2E=mc2.

"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 u = 1.6605 xx 10^(-27)"kg"u=1.6605×1027kg.

The mass defect, Deltam, will be

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 E = mc^2, c is the speed of light in a vacuum, approximately equal to 3 * 10^8"m s"^(-1).

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"