How Did Scientists Explain the Sun's Energy Before Nuclear Fusion?

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SUMMARY

Before the understanding of nuclear fusion, scientists theorized various mechanisms to explain the sun's energy output. Notably, Lord Kelvin proposed that the sun was a massive liquid body gradually cooling by radiating energy. Additionally, early theories suggested that the sun resembled a giant burning coal ball. However, these hypotheses were ultimately dismissed due to the insufficient energy output that coal could provide over extended periods, leading to a deeper inquiry into the sun's true nature.

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  • Basic understanding of thermodynamics
  • Familiarity with historical scientific theories
  • Knowledge of energy output calculations
  • Awareness of nuclear fusion principles
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  • Research Lord Kelvin's theories on stellar energy
  • Explore the transition from classical to modern astrophysics
  • Study the principles of nuclear fusion in stars
  • Investigate historical misconceptions about solar energy
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Historians of science, astrophysicists, educators, and anyone interested in the evolution of theories regarding solar energy and stellar physics.

timman_24
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The history of our understanding of the sun is a very rich area. Ancients believed the sun was a god while we now know the sun is an enormous body of fusion. What I would like to discuss is how the scientists thought the sun worked after the development of the basics of thermodynamics but before the understanding of subatomic interactions. I believe between the years of 1800-1900's.

I'm sure there were many very fascinating theories, do any of you guys know some of these?

To get us started, Kelvin theorized the Sun was a large body of liquid that was slowly cooling by radiating its energy.
 
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From a book I have, I remember them talking about thinking that the sun was a huge ball of something like Coal that was burning. But in the end, once the output of the sun was calculated, there was no way that coal could be putting out that much energy for anywhere near a long enough time.
 

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