A satellite, the sun and the satellites heat protector

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SUMMARY

The equilibrium temperature of a spacecraft's baffle, which protects it from solar radiation, is determined by the formula $$T_b=\Big(\frac{\alpha_d^2}{8}\Big)^{\frac{1}{4}}T_s$$ where T_s is the Sun's temperature at 5800K and $\alpha_d$ is the angular diameter of the Sun as observed from the spacecraft. The discussion emphasizes the importance of using the solar flux equation, $$\text{Flux} = \frac{L}{2\pi d^2}$$, where L represents the Sun's luminosity and d is the distance from the Sun to the baffle. Participants suggest employing a small angle approximation to simplify calculations, although it is noted that this may not be strictly necessary for deriving the final result.

PREREQUISITES
  • Understanding of thermal equilibrium concepts
  • Familiarity with solar flux calculations
  • Knowledge of angular diameter measurements
  • Basic proficiency in algebraic manipulation of equations
NEXT STEPS
  • Explore the derivation of the solar flux equation in detail
  • Research the implications of small angle approximations in physics
  • Study the principles of thermal radiation and heat transfer
  • Investigate the effects of varying distances from the Sun on spacecraft design
USEFUL FOR

Aerospace engineers, astrophysicists, and students studying thermal dynamics in spacecraft design will benefit from this discussion.

Olly_price
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Homework Statement



A spacecraft is protected from the Sun’s radiation by a planar baffle whose size is much greater than that of the spacecraft itself. The baffle is aligned perpendicular to the direction of the Sun. Show that the equilibrium temperature of the baffle is $$T_b=\Big(\frac{\alpha_d^2}{8}\Big)^{\frac{1}{4}}T_s$$ where T_s is the heat of the sun and is 5800K, $\alpha_d$ is the angular diameter of the Sun as seen from the spacecraft .

Homework Equations



Flux of the sun = L / $2\pi d^2$ where $d$ is the distance of the Sun from the baffle and L is the luminosity of the Sun.
Any classical equations involving thermal equilibriums etc.

The Attempt at a Solution



I was thinking of using the flux of the Sun stated above, and then the flux of the Sun's radiation on the baffle, considering the Sun's rays projected onto the baffle. Some form of ratios may help, but I didn't get anywhere.

I also tried using some geometries involving the angular diameter but could not successfully isolate $\alpha$. Perhaps we need to take a small angle approximation?
 
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Olly_price said:
I was thinking of using the flux of the Sun stated above, and then the flux of the Sun's radiation on the baffle
You can use that approach. It is probably useful to introduce some variable for its area. It will cancel out later but it makes the formulas easier to follow.
Olly_price said:
Perhaps we need to take a small angle approximation?
The final result looks like it uses that approximation, yes, but it should not be necessary to get a result.
 

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