Calculating Luminosity and Temperature of the Sun from Pluto

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SUMMARY

The discussion focuses on calculating the Sun's luminosity and temperature based on measurements from Pluto, specifically using the surface temperature of 58 K, a distance of 33 AU, and an albedo of 0.5. The initial calculation yielded a luminosity of 3.13 W and an effective surface temperature of 3193 K, which is significantly lower than the actual value. The error was identified as a miscalculation in the area used to determine the Sun's luminosity, which should be based on the total flux at Pluto's orbit multiplied by the surface area of a sphere (4π times the radius squared).

PREREQUISITES
  • Understanding of black body radiation and the Stefan-Boltzmann Law
  • Knowledge of astronomical units (AU) and their application in distance calculations
  • Familiarity with the concept of albedo and its impact on energy absorption
  • Basic skills in algebra for manipulating equations and solving for variables
NEXT STEPS
  • Review the Stefan-Boltzmann Law and its application in astrophysics
  • Learn how to calculate luminosity using the formula for flux and surface area
  • Study the concept of albedo and its effects on planetary temperatures
  • Explore the relationship between a star's luminosity, radius, and temperature using the appropriate equations
USEFUL FOR

Astronomy students, astrophysicists, and educators seeking to understand the calculations involved in determining stellar properties from planetary observations.

EzequielSeattle
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Hey all, I think that I'm doing this problem correctly but I'm getting an answer that's a couple thousand Kelvins off. Sorry if I should have posted this in the "advanced" section.

1. Homework Statement

Part of a flat region of Pluto has the Sun directly overhead. Its surface temperature is 58 K. You have determined Pluto is 33 AU away from the sun, and the region of interest has an albedo of 0.5. Use all of this information to determine the Sun's luminosity temperature. Assume the Sun and Pluto are perfect black bodies.

Homework Equations


P/A of a black body is equal to σT4, where σ = 5.67x10-8 W*m-2*K-4.

The Attempt at a Solution


Pluto's temperature is 58 K. By the equation above, its power/area radiated outward is σ*584, which is 0.642 W*m-2. Because its albedo is 0.5, it receives double this power from the sun, so the power per area from the sun hitting the surface is 1.283 W*m-2.

Because this power will fall off as the radius squared from the sun, I multiplied this by the square of 33 AU, which is 2.437x1025 square meters. I came away with a total luminosity of 3.13 W. Then, using the same equation above, I get that the effective surface temperature of the Sun is 3193 K, which is almost 3000 K away from the true value. Am I doing something wrong, or is this because of the imprecise variables that I was given in the problem?

Thanks in advance.
 
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EzequielSeattle said:
Pluto's temperature is 58 K. By the equation above, its power/area radiated outward is σ*584, which is 0.642 W*m-2. Because its albedo is 0.5, it receives double this power from the sun, so the power per area from the sun hitting the surface is 1.283 W*m-2.
Why do you care for the power radiated from Pluto's surface, though?
 
The power radiated from Pluto's surface is equal to half of the total power it receives from the Sun, because the albedo is 0.5. Right?
 
Right, sorry. I posted without thinking. Give me a moment to go through it again.
Tentatively, I'd probably look at the difference in areas that receive and reradiate the energy.
 
EzequielSeattle said:
Because this power will fall off as the radius squared from the sun, I multiplied this by the square of 33 AU, which is 2.437x1025 square meters.
I think this is the issue right here. To get the total power produced by the Sun, you need to take the flux you've just calculated at Pluto's orbit, and multiply it by the area of a sphere at that distance. That is, 4π times the radius squared. This gives the correct luminosity for the Sun.

I'm not sure what method you used to get the temp. from luminosity, though. Don't you need to know the Sun's radius? In any case, with the correct luminosity you should get the correct temperature.
 

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