Here are the essential concepts you must grasp in order to answer the question correctly.
Energy-Mass Equivalence
Energy-mass equivalence is a principle derived from Einstein's theory of relativity, encapsulated in the equation E=mc². This concept states that mass can be converted into energy and vice versa, highlighting the relationship between mass and energy. In the context of the sun, this principle explains how the mass lost during nuclear fusion is transformed into the energy radiated by the sun.
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Nuclear Fusion
Nuclear fusion is a process where two light atomic nuclei combine to form a heavier nucleus, releasing a significant amount of energy in the process. This reaction powers stars, including the sun, where hydrogen nuclei fuse to form helium. Understanding fusion is crucial for calculating the energy output of the sun and its implications for mass loss over time.
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Percentage Calculation
Percentage calculation is a mathematical process used to express a number as a fraction of 100. In this context, it involves determining what fraction of the sun's total mass is converted into energy. This requires dividing the mass equivalent of the energy output by the sun's total mass and multiplying by 100 to obtain the percentage, providing insight into the efficiency of the sun's energy production.
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