Jotapay wrote:
Here is a representation of CO2 over geologic time. Note that we are currently around 390 ppm CO2 in the atmosphere which is pretty low, relatively speaking. Temps are also no where near past record highs. Combine that with the bad data that researchers are working with and I think it's easy to see why the current hysteria is a little overblown.
Even this data is uncertain and incomplete, as noted in the graph.
Main sequence stars burn hydrogen into helium as a fuel. As they age the ratio of hydrogen to helium tilts in favour of helium, which is twice as dense, The denisty of the core is the critical factor in the burn rate of the star. This has all been well understood and pretty mainstream astrophysics from the 50s. The consaquence of this is that a star like the sun produces more energy as it ages, or when you run the clock backwards it cools as you go further back into time. The figure given for the past 500 million years is about 1% per 100 million years. So if one takes for example 100million years ago, we can give a ball park figure.
The current temperature is about 287K.
The greenhouse effect is about 33K
So the current direct solar energy is about 254K
At 1% less solar energy this would be roughly 251K
If we take the CO2 level at being 1700ppm we can make rough estimates of the additional global warming, 280ppm is given as the preindustrial level and each doubling generates an estimated 2K. At about 2.5 times preindustrial levels this would be 5K of additional heating or just slightly above current the current level of 251K + 33K + 5K =289K. Many other factors also contribute including changes in albedo and so on, but the figures give an indication that higher levels of CO2 during the Phanerozoic are necessary to prevent a global freeze.