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1800-102-2727Ever looked at the sun on a terribly humid day and wondered where is all that heat coming from? The answer for this is nuclear fusion. The stars we see at night have been formed as a result of a phenomenon called the Stellar life cycle; when dust and gas particles attract to each other due to gravity, they accumulate and form a star. In both of these examples, energy is released as a result of changes inside a nucleus; a process called nuclear fusion. In a nuclear fusion reaction, more energy is released in comparison to a nuclear fission reaction. In this article, we will explore nuclear fusion in detail.
Table of Contents
When two lighter nuclei fuse together to form a heavier nucleus, it is termed as a fusion reaction. The difference in mass between the parent and daughter nuclei is called binding energy. In a fusion reaction, since the daughter nucleus formed is more stable, it has higher binding energy per nucleon than the parent nuclei. A good example would be the fusion of two hydrogen nuclei to form a helium nucleus, which happens in the sun.
1H1 + 1H1 → 1H2 + e+ + v + 0.42 MeV
e+ + e- → γ + γ + 1.02 MeV
1H2 + 1H1 → 2He3 + γ + 5.49 MeV
2He3 + 2He3 → 2He4 + 1H1 + 1H1 + 12.86 MeV
e+ → Positron
e- → Electron
1H1 → Hydrogen nucleus
1H2 → Deuterium nucleus.
1H3 →Tritium Nucleus.
v → Neutrino
γ → Gamma rays
Both deuterium and tritium are isotopes of hydrogen.
Q1) What is X in the following reaction?
1H2 + 1H1 → 2X3 + γ + 5.49 MeV
Solution) 1H2 + 1H1 → 2He3 + γ + 5.49 MeV
Q2) What is Y in the following reaction?
1H1 + 1H1 → 1Y2 + e+ + γ + 0.42 MeV
Solution) Y is 1H2.
Q3) Complete the following reaction?
6C12 + 2He4 → ? + γ
Solution) 6C12 + 2He4 → 8O16 + γ
Q4) Calculate the total energy released in the nuclear fusion reaction of the sun?
Solution) 1H2 + 1H2 → 1H2 + e++ γ + 0.42 MeV
e+ + e- → γ + γ + 1.02 MeV
1H2 + 1H1 → 2He3 + γ + 5.49 MeV
2He3 + 2He3 → 2He4 + 1H1 + 1H1 + 12.86 MeV
Total energy = 0.42 + 1.02 + 5.49 + 12.86 = 19.79 MeV
Question1. The binding energy per nucleon of the daughter nucleus is more than that of the parent nucleus in a fusion reaction. Why?
Answer. The daughter nucleus is more stable, hence more binding energy per nucleon.
Question2. Define nuclear fusion?
Answer. When two lighter nuclei fuse to form a heavier nucleus, it is called a fusion reaction.
Question3. Explain how stars are born?
Answer. Dust slowly accumulates after falling under the influence of gravity, and begin to accelerate inwards and collision occurs. Due to the collision, heat is produced, which starts the nuclear fusion process and the star begins to fuse H into He. This is how a star is born.
Question4. Write the fusion reaction of deuterium nuclei forming helium.
Answer. 1H2 + 1H2 → 2He4 + Energy.
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