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Answer :
Final answer:
To estimate the Sun's surface temperature, use the solar constant and Stefan-Boltzmann law, along with the Earth-Sun distance and Sun's radius, to calculate the total solar power output and surface area, thus determining the temperature.
Explanation:
To estimate the temperature of the Sun's surface, you can use the solar constant and the Stefan-Boltzmann law. The solar constant is the amount of solar power per unit area received at the Earth's distance from the Sun. Additional data needed would be the Earth-Sun distance to calculate the total solar power output and the Sun's radius for calculating its surface area.
With the total solar power and the Stefan-Boltzmann law, which states that the power radiated per unit area of a black body is proportional to the fourth power of its temperature, you can estimate the surface temperature of the Sun.
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