CBSE Class 12 Physics 2025: question 21
Set in the CBSE Class 12 board exam of 2025, paper 55/7/1, section B, question 21, for 2 marks. Try it first; the hints and our step-by-step solution are below.
Q21 · 2 marks · Very short answerNuclei
Briefly explain how energy is produced in stars, giving two examples of the nuclear reactions involved.
Source: official question paper from cbse.gov.in (PDF). See it in the full 2025 board paper, set 55/7/1.
Hints
Open one hint at a time and try again before the next.
Hint 1
Is it fission or fusion that powers the Sun?
Hint 2
Think of the proton–proton cycle that converts hydrogen into helium.
Step-by-step solution
Each step shows the marks it earns, as an examiner would award them. Checked by an independent re-solve from the question paper.
- ½ mark
Energy in stars comes from thermonuclear fusion. The core temperature is about K, so light nuclei (mainly hydrogen) have enough kinetic energy to overcome Coulomb repulsion and fuse.
- ½ mark
The heavier nucleus formed has a higher binding energy per nucleon, so its mass is less than the total mass of the reacting nuclei. This mass defect is released as energy .
- ½ mark
Example 1 (proton–proton cycle): MeV.
- ½ mark
Example 2: MeV. Further, MeV. Overall, four protons combine to form one He nucleus and about 26.7 MeV is released.
Answer: By nuclear fusion of hydrogen into helium (proton–proton cycle), e.g. ¹H + ¹H → ²H + e⁺ + ν, and ³He + ³He → ⁴He + 2¹H.
Where the marks are
- Identifies thermonuclear fusion at very high temperature (½ mark)
- Explains the release of energy through mass defect / higher binding energy per nucleon (½ mark)
- Any two correct fusion reactions (½ + ½ mark)
Revise the chapter
- Chapter: Nuclei (notes, formulas, where marks are lost and every past question)
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