
The reaction responsible for the production of light energy from the sun will be:
(A) Fission
(B) Fusion
(C) Nuclear
(D) None of these
Answer
226.8k+ views
Hint Energy is produced in the sun via nuclear fusion. 2 hydrogen isotopes collide with each other at a very high speed. The extreme heat already present in the sun acts as a catalyst for the reaction to proceed. Once the reaction occurs, a single neutron is ejected as a by-product and the helium atom is formed. This reaction results in a lot of heat being liberated.
Complete step by step answer:
The solar energy or the light energy of the sun comes from constant chemical reactions happening within the sun. Sun is a star made up of mostly hydrogen and helium atoms. The chemical reaction involved here can be represented by the following diagram:
During nuclear fusion, the high pressure and temperature in the core of the sun cause the hydrogen nuclei to separate from their electrons. These hydrogen nuclei then fuse to form a single helium atom.
Hence, Option (B) is correct.
Note Two hydrogen atoms fuse into each other to give a helium atom and a lot of energy. This energy is released because a helium atom is much more stable than a hydrogen atom and the binding energy of the resultant helium nuclei is much greater than the initial binding energy of the hydrogen nuclei.
Complete step by step answer:
The solar energy or the light energy of the sun comes from constant chemical reactions happening within the sun. Sun is a star made up of mostly hydrogen and helium atoms. The chemical reaction involved here can be represented by the following diagram:
During nuclear fusion, the high pressure and temperature in the core of the sun cause the hydrogen nuclei to separate from their electrons. These hydrogen nuclei then fuse to form a single helium atom.
Hence, Option (B) is correct.
Note Two hydrogen atoms fuse into each other to give a helium atom and a lot of energy. This energy is released because a helium atom is much more stable than a hydrogen atom and the binding energy of the resultant helium nuclei is much greater than the initial binding energy of the hydrogen nuclei.
Recently Updated Pages
States of Matter Chapter For JEE Main Chemistry

Mass vs Weight: Key Differences Explained for Students

Circuit Switching vs Packet Switching: Key Differences Explained

Conduction Explained: Definition, Examples & Science for Students

Balancing of Redox Reactions - Important Concepts and Tips for JEE

Atomic Size - Important Concepts and Tips for JEE

Trending doubts
JEE Main 2026: City Intimation Slip and Exam Dates Released, Application Form Closed, Syllabus & Eligibility

JEE Main 2026 Application Login: Direct Link, Registration, Form Fill, and Steps

Understanding the Angle of Deviation in a Prism

Hybridisation in Chemistry – Concept, Types & Applications

How to Convert a Galvanometer into an Ammeter or Voltmeter

Ideal and Non-Ideal Solutions Explained for Class 12 Chemistry

Other Pages
JEE Advanced Marks vs Ranks 2025: Understanding Category-wise Qualifying Marks and Previous Year Cut-offs

Laws of Motion Class 11 Physics Chapter 4 CBSE Notes - 2025-26

JEE Advanced 2026 - Exam Date (Released), Syllabus, Registration, Eligibility, Preparation, and More

Mechanical Properties of Fluids Class 11 Physics Chapter 9 CBSE Notes - 2025-26

Thermodynamics Class 11 Physics Chapter 11 CBSE Notes - 2025-26

Units And Measurements Class 11 Physics Chapter 1 CBSE Notes - 2025-26

