How was the core temperature of sun estimated ?

In summary, scientists estimate the heat inside the core of the Sun to be around 15,000,000 °C by creating models and comparing them to observations. By calculating the necessary temperature and density gradients to transport the sun's emitted light and keep it stable, they can work from the surface inwards to estimate the core temperature. Another approach is to compare the fusion rate of the Sun to its total power at different temperatures. It is not necessary to understand fusion to estimate the central temperature of the Sun, as it can be calculated using Newton's gravity and the ideal gas equation based on central pressure and density.
  • #1
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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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  • #2
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.
 
  • #3
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.
 

1. How can we measure the temperature of the sun's core?

The temperature of the sun's core is estimated by using mathematical models and measurements of the sun's surface and atmosphere. Scientists also use data from solar observatories and satellites to study the sun's internal structure and radiation output, which help determine the core temperature.

2. What methods do scientists use to estimate the temperature of the sun's core?

Scientists use a variety of methods to estimate the temperature of the sun's core, including spectroscopy, helioseismology, and nuclear reaction rates. Spectroscopy involves analyzing the light emitted by the sun to determine its temperature. Helioseismology uses sound waves to study the movement and structure of the sun's interior, which can provide information about its temperature. Nuclear reaction rates help scientists understand the processes happening in the sun's core and can also provide clues about its temperature.

3. How accurate are the estimates of the sun's core temperature?

The estimates of the sun's core temperature are considered to be very accurate, with a margin of error of only a few percent. This is due to the combination of multiple methods used to estimate the temperature, as well as advancements in technology and data collection.

4. Has the estimated temperature of the sun's core changed over time?

Yes, the estimated temperature of the sun's core has changed over time as scientists have developed new methods and technology for studying the sun. In the past, estimates were much lower than they are today, as scientists did not have access to the same level of data and technology that we have now. However, as our understanding of the sun has improved, so has the accuracy of the estimated core temperature.

5. Why is it important to know the temperature of the sun's core?

Understanding the temperature of the sun's core is crucial for studying the sun's behavior and its impact on our planet. It also helps scientists better understand the processes happening in the sun's interior, which can provide insights into other stars and the universe as a whole. Additionally, knowing the temperature of the sun's core is important for predicting solar activity and potential disruptions to Earth's communication and navigation systems.

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