How Do the Temperatures of Star 1 and Star 2 Compare?

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SUMMARY

The discussion focuses on comparing the temperatures of Star 1 and Star 2 based on their energy emission rates and radii. Star 1 emits energy at a rate twice that of Star 2 and has a radius three times larger. According to the Stefan-Boltzmann law, the temperature of Star 1 is determined to be approximately 0.37 times that of Star 2. This conclusion is derived from the relationship between energy emission, surface area, and temperature.

PREREQUISITES
  • Understanding of the Stefan-Boltzmann law
  • Basic knowledge of stellar physics
  • Familiarity with concepts of energy emission and surface area
  • Ability to perform mathematical comparisons of physical quantities
NEXT STEPS
  • Study the Stefan-Boltzmann law in detail
  • Explore the relationship between surface area and energy emission in stars
  • Learn about the properties of different types of stars
  • Investigate the methods for calculating stellar temperatures
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Students in physics, astrophysics enthusiasts, and anyone interested in understanding stellar properties and energy emissions.

DracoMalfoy
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Homework Statement


Star 1 emits energy at a rate that is 2 times that of Star 2. If Star 1 also has a radius that is 3 times larger than Star 2, how do the temperatures of the stars compare?

a. Star 1's temperature is 2.58 that of Star 2.

b. Star 1's temperature is 3.75 that of Star 2.

c. Star 1's temperature is 0.69 that of Star 2.

d. Star 1's temperature is 0.37 that of Star 2.

e. Star 1's temperature is 0.12 that of Star 2.

Homework Equations

The Attempt at a Solution



This is supposed to be a physics class.. I am not sure why we were given this question. The teacher didnt even give us any equations for questions like this. so i have no idea,.. pls help
 
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well Physics is about objects in the real world :biggrin:
jokes aside, a star emits electromagnetic radiation from its surface due to the temperature of the (very hot :smile:) material - similar to a hot filament in a light bulb.
hotter material will emit more radiation energy per unit time.
a larger star will have more surface area and thus also emit more energy per unit time.
so the amount of radiation energy emitted per unit time will depend on the temperature and the amount of surface area of the star.
 

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