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Question

What is the source of energy in the Sun or other stars?

This question was previously asked in
RRB NTPC 2019 CBT 1 Question Paper (8-Mar-2021) (Shift 2)
The correct answer is
Nuclear Fusion

Stellar Energy Source: Understanding Nuclear Fusion

The primary source of energy in the Sun and other stars is a process called nuclear fusion.

Core Fusion Process

In the intensely hot and dense core of stars, light atomic nuclei are forced together and fuse to form heavier nuclei. For stars like our Sun, this predominantly involves the fusion of hydrogen nuclei (protons) into helium nuclei.

Energy Release Mechanism

This nuclear fusion process releases a vast amount of energy. A tiny fraction of the mass of the fusing nuclei is converted directly into energy, according to the mass-energy equivalence principle described by Albert Einstein's equation $E=mc^2$. This energy radiates outwards, making the star shine.

Why Other Options Are Incorrect

  • Nuclear Fission: This is the splitting of heavy atomic nuclei (like uranium), which is used in nuclear power plants but is not the main energy source for stars like the Sun.
  • Burning of Helium/Hydrogen Gas: Burning refers to chemical combustion, a much lower-energy process than nuclear reactions. While stars fuse hydrogen and later helium, it's through nuclear fusion, not simple burning.

Conclusion

Therefore, nuclear fusion is the correct explanation for the immense energy output of stars.

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