Try it on paper first. A hint, the key idea and the worked solution are here when you need them.
A solid copper sphere of radius is painted black (treat it as a black body). It hangs on a thin thread in an evacuated enclosure whose walls are kept at . A tiny heater inside the sphere keeps it at . Copper has density and specific heat ; take . Ignore heat flow along the thread, and take the sphere's temperature to be the same throughout.
Have you tried it?
Work it out on paper first. It is fine to get stuck or make a mistake: that is how we learn. When you are ready, go through the solution one step at a time, and check each step against your own.
Plan. Balance the net radiation against the heater, then against the loss of stored heat. Integrate for the time.
Step 1. The sphere. Its surface area is , its mass , and its heat capacity .
Step 2. The heater (a). The sphere radiates and takes in from the walls. The heater makes up the difference:
Step 3. The first rate (b). .
Step 4. The time (c). Separate the variables in :
Here , and with the given formula () the integral is . So .
Step 5. A larger sphere (d). The heat capacity grows as and the area as , so grows as . The same cooling takes twice as long: .
Answer: (a) . (b) . (c) . (d) .
Check. The rate falls from at to at . Cooling the whole at the first rate would take ; at the last rate it would take much longer. The answer, , lies between, nearer the start because the rate is high there.
Watch out. Newton's law of cooling (a rate proportional to ) only works for small temperature differences. Here the differences are large, so the full law is needed.
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