Roger44 said:
"you can only heat a blackbody target using a blackbody source to the same temperature as the source. So however much you concentrate the light with lenses/mirrors you can't use the sun to heat something to a higher temperature than the surface of the sun. Because at that point the target would emit back at the sun"
Are you sure of this? My first rection would be to say if you focused the light from a large 1000K black body onto a small target, then the target would rapidly rise to a temperature well above the source.
This was a great thought experiment. I have sorted it out in my mind taking into account some other posts in this thread. Let me try an explanation
Case 1. No focusing
Imagine a blackbody radiator with one mother of a lot of internal energy, at a temperature of 5780 K. (A bit like the Sun, for our purposes.) Let it be a sphere with surface area of 6 * 10
18 m
2. (That's a radius of 6.91*10
8 m.)
Imagine it in a massive empty space filled with a bath of radiation, with a characteristic temperature of about 2.7 K. (A bit like interstellar space and the cosmic background.)
Imagine a small sphere, a super cold blackbody radiator, 1 meter in radius, situated about 1.5*10
11 m from the Sun. (That's near enough to the distance of the Earth from the Sun.) Assume is it an efficient conductor of heat, so it is all one temperature.
What temperature can you expect this small sphere to reach when it comes into equilibrium with the surrounding radiation?
The radiation from the surface of the Sun will be σT
4 which is 6.33*10
7 W/m
2. This spreads out as it leaves the Sun, by the square of the distance, so by the time it gets out to the 1 meter sphere the flux is reduced to be
6.33 \times 10^7 \left(\frac{6.91\times 10^8}{1.5 \times 10^{11}} \right)^2 = 1343 \; W/m^2
That you should recognize as the solar constant at Earth's orbit. There's negligible energy coming from space, and the sphere has to radiate all that again, but it receives energy over a cross section of pi.r^4 and radiates it over a surface area of 4.pi.r^2, so the radiated flux from the sphere is one quarter of the solar constant. From this we get the temperature T
b of the ball as follows:
T_b = \left( \frac{1343}{4\sigma} \right)^{0.25} = 277.4 \; K
The sphere is just above the freezing point of water.
Case 2. Big mirrors for a solar furnace
Now we bring in some perfect mirrors, line them all up behind the little ball, and focus them all directly on to the ball. These mirrors have a cross section area against the Sun of that is 10
5 times greater than the surface area of the ball.
Without the mirrors, the ball is getting 1343/4 watts for each square meter of its own surface area. But the mirrors are getting 1343 * 10
5 Watts for each square meter of the ball's own surface area. So the ball has to heat up to shed 1.343 * 10
8 W/m
2, which gives a temperature of
\left(\frac{1.343\times 10^8}{\sigma}\right)^{0.25} = 6976 \; K
Bingo. We've heated the ball up to be hotter than the Sun. Clearly, this is wrong. It is a violation of thermodynamics. So what was the error?
Case 3. Huge mirrors for a solar furnace
To see where the above goes wrong, imagine an enormous ellipsoidal mirror enclosing the Sun and the ball, and with each one at a focus of the ellipsoid. All the energy from the Sun is now being focused on to that tiny ball.
But here's the problem. The Sun is a finite site: about 6.91*10
8 meters in radius. So the radiating surface is not all at the focus of the ellipsoid. The best you can possibly get has a focus that gives a pseudo-surface around the ball radiating in with a characteristic temperature of the surface of the Sun and in all directions from that virtual surface. And that, my friends, cannot be focused any more tightly to get all the radiation impinging on a ball 1m in radius.
Similarly, in case 2, the error was thinking any number of mirrors would be able to get all the light from every point on the surface of a huge ball like the Sun focused down into a tiny sphere, with an energy flux greater than the blackbody radiating surface at 5780 K.
Case 4. Huge blackbody enclosing the system.
Added in edit... This is the example proposed by the4thamigo_uk as follows:
the4thamigo_uk said:
If you look back at my imaginary black body inside another black body example there is no focussing going on. So in this case what is the physics?
Imagine now no focusing; just have the whole system surrounded by an enormous blackbody surface, but one which has a small heat capacity compared with the Sun. That is, to heat up the surrounding body does not require so much energy as to deplete the Sun's store of internal energy.
The Sun keeps radiating with energy having a Planck radiation spectrum of 5780 K. This will be absorbed by the surrounding surface, which will heat up comparatively quickly (because it has a low heat capacity) and begin radiating itself. When it stops heating up, it will be in equilibrium with the incoming energy, so it radiates precisely what it receives. The whole cavity will be filled with radiation at a characteristic temperature of 5780 K. The "Sun" will now be receiving back again the same energy that it is emitting, so it is no longer cooling down. Because it has a large heat capacity, its own temperature did not fall significantly in the time it took the cavity to come to equilibrium.
(Note in this example I am not thinking of any generation of new heat energy from fusion reactions; just thinking about blackbody radiators.)
A small blackbody sphere 1m in radius, anywhere in this cavity, will also come to equilibrium with the surrounding radiation bath, at the same temperature.
Cheers -- sylas