Simple black body radiation theory (adapted from http://www.atmos.washington.edu/2002Q4/211/notes_greenhouse.html):
The earth receives a certain amount of heat per unit area from the sun - this amount is about 1370 W/m$^2$ for parts of the earth facing the sun when there is no atmosphere. But the earth presents a "disk" with area $\pi R^2$ to the sun, when it is in fact a sphere with an area of $4\pi R^2$. This means that on average the power received per unit area over 24 hours is 1/4 of that, or about 340 W.
Now some of the sun's power is reflected by earth - about 30%. The power left to get rid of by "gray body radiation" is about 240 W/m$^2$.
Using Stefan-Boltmann, with again an emissivity of 0.7, we solve for the "equivalent" temperature of Earth:
$$\Phi = \epsilon \sigma T^4\\
240 = 0.7 \cdot 5.67 \cdot 10^{-8} T^4\\
T = 278 K$$
If you ignore the emissivity, the value would be even lower - 255 K. This is well below the temperature of Earth (mean value 288 K), suggesting that the atmosphere is indeed helping keep the temperature up. The effect of the atmosphere on surface temperature is much more extreme on Venus (100's of degrees K), where the layer of carbon dioxide is very thick.
Of course all kinds of simplifying assumptions went into the above. For example, the poles will be significantly colder when there is no atmospheric convection to bring heat from the lower latitudes - and the temperature fluctuations between day and night could be enormous. The hotter surface during the day will emit relatively more power (because of that 4th power) so the mean would be lower than the "effective" temperature I calculated above. Either way - the atmosphere absorbs more strongly in the IR than in the visible, and this means that it is easier for sunlight to get in, than for emitted thermal radiation to get out. This helps keep the planet warm. Your school board, in this case, had the right answer.
But the bottom line is - the atmosphere makes earth livable. Changing the composition will change the conditions on earth. But the balance is precarious. Let's not disturb it if we can help it.
model, thermal equilibrium fixes the average of T⁴. With this constraint, the greater the thermal amplitude, the lower the average temperature. I certainly have missed many other effects...
– Edgar Bonet Mar 04 '15 at 15:25