- #1
CricK0es
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Homework Statement
It's not a piece of homework, I'm doing a project and I've been wondering how I may be able to show it mathematically. I've covered the material before but it was a long long time ago...
Homework Equations
The Attempt at a Solution
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A-Thinking about modelling my "ship" as a spherical ball of radius, 1m.
B- Use Stefan-Boltzmann Law to determine how much energy is radiated, under the assumption it's a blackbody, at its maximum temperature.
C- Then assuming the radiated energy is equal to the incoming energy from the sun.
D- Calculating the distance required for these two values to be equal.
I feel like it's fairly hand wavey but it doesn't have to be particularly accurate, just a ball park figure. But for D, is it sufficient to use the inverse square law for intensity, or would I have to be more rigorous. As in, treating every point on the surface of the sun as a point source and integrating... Probably too complicated for what I'm looking for.
Anywho. Any help would be appreciated and thank you in advance.
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