Effect of Earth-Sun Distance Variance on Effective Temperature

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SUMMARY

The discussion focuses on the effect of the Earth's varying distance from the Sun on its effective temperature. The minimum distance occurs in January, while the maximum distance is approximately 3.3% larger in July. The effective temperature can be calculated using the equation $$ T_E^4 = \frac{(1 - \alpha) F_0}{4 \sigma} $$, where F0 represents the solar flux, which decreases as the distance increases. Participants seek clarification on how to calculate the change in solar flux and its impact on effective temperature due to this distance variance.

PREREQUISITES
  • Understanding of effective temperature equations
  • Familiarity with solar flux calculations
  • Knowledge of the Stefan-Boltzmann law
  • Basic concepts of Earth's orbital mechanics
NEXT STEPS
  • Research the relationship between distance and solar flux using the inverse square law
  • Study the derivation of the effective temperature equation in astrophysics
  • Explore the implications of seasonal changes in solar radiation on climate
  • Investigate the mathematical modeling of Earth's orbit and its effects on temperature
USEFUL FOR

Students in astrophysics, climate science researchers, and educators looking to understand the relationship between solar distance and effective temperature variations.

il27

Homework Statement



The distance between the Sun and the Earth varies during the year: it is a minimum in January, and about 3.3% larger at its maximum in July. What is the corresponding change in the Earth's effective temperature?

Homework Equations



Energy absorbed: $$ E_{abs} = \pi R^2 (1- \alpha) F_0 $$
energy emitted: $$ E_{emit} = 4 \pi R^2 \sigma (T_E)^4 $$

The Attempt at a Solution



I tried finding the effective temperature equation:

The effective temperature equation:

$$ T_E^4 = \frac{(1 - \alpha) F_0}{4 \sigma} $$

but I am stuck on how to account for the changing distances between the sun and the earth.
Please help, thank you!
 
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F0, the flux of solar radiation at the Earth, is dependent on the distance between the Earth and the Sun. Do you know how much F0 changes if the Earth-Sun distance doubles, for example?
 
phyzguy said:
F0, the flux of solar radiation at the Earth, is dependent on the distance between the Earth and the Sun. Do you know how much F0 changes if the Earth-Sun distance doubles, for example?

Oh okay. the solar constant would decrease right?
what is the equation to find the solar contsant where it relies on the distance between the sun and the earth?
 
help
 
i think i understand the equation. i use the effective temperature equation but find two different solar constant values.
however, what does it mean when it is a minimum in January, and about 3.3% larger at its maximum in July?
is the minimum the distance between the sun and the earth? while 3.3% larger than that is 3.3% added to the distance?
 
il27 said:
i think i understand the equation. i use the effective temperature equation but find two different solar constant values.
however, what does it mean when it is a minimum in January, and about 3.3% larger at its maximum in July?
is the minimum the distance between the sun and the earth? while 3.3% larger than that is 3.3% added to the distance?

Yes. Whatever the distance is in January, it is 3.3% larger in July. When the distance increases by 3.3%, how much does the solar flux decrease?
 

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