On my blog, I am explaining why the faster rotating planets are warmer.
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I actually think this is quite interesting, though I'm not sure anyone who hadn't thought about similar things would understand your posts.
To restate your point, the relevant conserved quantity when dealing with surface temperature equilibria problems is not temperature T but T^4, because Stefan's Law says that the power radiated from a blackbody goes as the 4th power of temperature. So a planet with dense pockets of high temperature surrounded by regions of low temperature will have a lower average temperature than a planet with the same rate of radiatio...
This is the supposedly-bimonthly-but-we-missed-April-and-June-2013 'What are you working On?' thread. Previous threads are here. So here's the question:
What are you working on?
Here are some guidelines: