Planet Cooling Homework: Calculating Time to Cool Down from 100K to 50K

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The discussion focuses on calculating the time it takes for a planet with a surface temperature of 100K and a radius of 500 km to cool down to 50K, neglecting solar heating. Participants emphasize the need to set up a differential equation due to the non-constant power loss as the temperature decreases. The relationship between thermal energy and temperature is explored, with suggestions to express energy in terms of temperature and to use separation of variables for solving the equation. The mass of the planet, assumed to be made of iron, is calculated using its density and volume to determine the number of particles. The final cooling time estimate discussed is around 10^42 years, highlighting the complexity of the calculations involved.
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Homework Statement



How much time does it take a planet with surface temperature of 100K and a radius of 500 km to cool down to 50K, ignoring solar heating. Assume E_thermal = 3/2 NkT and that the surface radiates as a blackbody. Calculate this by using the relationship between thermal energy and temperature and the relationship between the rate of energy loss dE/dt and temperature.

Homework Equations



E_thermal = 3/2 NkT

Power emitted/Area = σT^4

The Attempt at a Solution



Power = Energy/Time

Energy/Area*Time = σT^4

Energy = σT^4 * A*t

Subbing for thermal energy

3/2 NkT = σT^4 * A*t

T = (3NKt/2A)^(1/3)
I feel like I've missed something and the T should be a delta T but I'm not sure where I've going wrong.

Thanks for any help,
 
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Something to consider: the power is not constant in this problem, because cooling causes the planet's surface temperature to get lower, which causes it to radiate less. So, you probably have to set up an integral here.

Edit: Er, actually, a differential equation, I think.
 
I get

dE/dt = σT^4 * A

d(3/2 NkT)/dt = σT^4 * A

and take out the constant and solve using separation of variables?
 
ma18 said:
Yes it supposed to be a differential equation but I tried doing that and I didn't get anywhere.

I get

dE/dt = σT^4 * A

then what?

Well, what is E(T)? That will allow you to express everything in terms of T.
 
ma18 said:
I get

dE/dt = σT^4 * A

d(3/2 NkT)/dt = σT^4 * A

and take out the constant and solve using separation of variables?

Oh, you edited your post. Yes. I think that is the right approach.
 
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Thanks!
 
Is it reasonable to assume that the planet is a sphere?

I am given that the planet is made of iron (know the density and mass of iron). Using p = m/V I would calcluate the mass of the planet and then get the number of particles N.

Is there any other way to get N?
 
ma18 said:
Is it reasonable to assume that the planet is a sphere?

Yes. In fact, since you've only been given one dimension, you can't really assume anything else.

ma18 said:
I am given that the planet is made of iron (know the density and mass of iron). Using p = m/V I would calcluate the mass of the planet and then get the number of particles N.

Is there any other way to get N?

This sounds like the way to get N.
 
I get time to be negative :(Tf
∫dt/T^4
Ti

[(1/Ti^3)-(1/Tf^3)]

Since Ti>Tf
 
  • #10
Plus I get a timescale of 10^42 years
 
  • #11
Regarding the first problem: you could just be out by a negative sign. Remember that the power radiated is equal to the rate of decrease in thermal energy.

Second problem: it is an algebraic or arithmetic error. Please post all of your work so far.
 
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  • #12
I got it, thanks for all your help. I like this method, much better than other places which just give you the answer.
 
  • #13
Just out of curiosity, what did you get as the cooling time to 50 K?
 
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