How was the core temperature of sun estimated ?

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SUMMARY

The core temperature of the Sun is estimated to be approximately 15,000,000 °C. Scientists derive this value by creating models of the Sun that align with observational data. A fundamental model considers the fusion process occurring in a small volume at the core, where energy is transported to the surface as light. By analyzing the Sun's light emission and applying Newton's gravity alongside the ideal gas equation (IGE), researchers can calculate the necessary temperature and density gradients to maintain stability within the Sun.

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  • Understanding of stellar models and astrophysics
  • Familiarity with Newton's law of gravitation
  • Knowledge of the ideal gas equation (IGE)
  • Basic concepts of nuclear fusion and energy transport
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  • Study the principles of nuclear fusion and its role in stellar dynamics
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Astronomers, astrophysicists, and students studying stellar evolution and thermodynamics will benefit from this discussion.

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It was estimated that the heat inside the core of the Sun inside around 15 000 000 °C - this value is extremely enormous. How did scientists estimate this value?
 
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In general: you make models of the sun, and then you see which one agrees with all observations, and check which temperature this model predicts for the core.

A very simple model that gives a good approximation: fusion happens within a small volume in the core, and a part of the released energy is transported to the surface afterwards until it can escape as light. We know how much light the sun emits, and you can calculate the necessary temperature and density gradients inside that is required to transport this power and to keep the sun stable. Work from the surface inwards and you get an estimate for the core temperature.

Another nice approach is the fusion rate - this is known from the total power as well, and it can be compared to the fusion rate the sun would have at different temperatures.
 
It is not necessary to know anything about fusion to estimate the Sun's central temperature. Very good estimates were made even before fusion was ever understood. After all, the Sun is just a self-gravitating ball of gas. It's Newton's gravity and the ideal gas equation. Find the central pressure and density and the temperature is found by the IGE.
 

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