lomiller
Penultimate Amazing
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- Jul 31, 2007
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Actually, complete transparency makes the adiabatic lapse rate irrelevant. You get an adiabatic lapse rate when you get vertical convection, and to get any significant vertical convection you need to gain heat from below and lose it from above. You can gain heat at the ground from direct thermal contact, but you can only really lose it at the top from radiation. And if you're completely transparent, you don't radiate..
This would only hold true if the atmosphere was completely opaque to IR, because IR is emitted in a random direction which means large amounts are emitted towards the surface. So, once again we are back to the dependence on greenhouse gasses.
Sure, but you need to know how much atmosphere you have to calculate that second part. That's my point: more atmosphere means a hotter surface temp. Composition matters too, but if Venus had the amount of atmosphere we have, even with the composition it currently has, it would be a lot cooler than it is now.
What you need to know is how much greenhouse gas you have in the atmosphere, since non-greenhouse gasses don’t interact with IR by definition. If Venus has an equally thick atmosphere composed entirely of a non-greenhouse gas like Nitrogen (and the planets reflectivity was unchanged) it would be about the same temperature as the moon regardless of pressure.
Venus has many times more greenhouse gas in it’s atmosphere then the earth has atmosphere so obviously we couldn’t reach those same levels without more atmosphere which would result in more pressure, but pressure remains an ancillary effect, not a cause.
The surface of a planet most certainly CAN cool by convection. Below the point at which the atmosphere becomes opaque to IR, that can easily be the dominant cooling mechanism
Only if the top of the atmosphere is cooling by some other means. AFAIK convection IS the dominant cooling mechanism for the surface, nonetheless top of atmosphere radiative balance ultimately determines surface temperature.
That convection brings warm gasses up to high altitudes where it can then radiate heat into space, but the transfer of heat from the ground to the upper atmosphere very much involves convection. And since we're talking about surface temperatures, it's wrong to exclude convection from the discussion.
This gets you into territory where you need extremely complex models to resolve anything. Such models are well beyond anything we could hope to discuss here but we know what these models tell us and their results are in the same ballpark as the simple top of atmosphere calculation.
http://www.realclimate.org/index.php/archives/2007/08/the-co2-problem-in-6-easy-steps/