
astrodon
Audioholic
I have been debating for some time as to whether to add to this thread since there have been so many angry comments made. Being an astrophysicist who specializes in the study of the "atmospheres" (i.e., the outer layers) of cool stars, and who has done some research in planetary atmospheres, let me make a few points.
1. Over the past century, there has been a "one-to-one" correlation between the increase of atmospheric CO2 and average atmospheric temperature rise averaged on a seasonal cycle. One need only examine a textbook on meteorology or freshman astronomy to see this data. Coincidentally, the industrial revolution started around the same epoch of this correlation. Both data were relatively flat over time prior to this.
2. Occasional large volcanic epsidoes have had some impact on the average atmospheric temperature, but these episodes have not had a lasting (i.e., more than a year or few) impact on the atmosphere.
3. The Sun's luminosity has remained relatively constant over the past 400 years (since mankind started measuring it). There are minor (less than 0.01 percent) changes due to the solar activity (sunspot/facula) cycle. The Sun is not causing this temperature increase. (And if it was, this would be far worse than manmade greenhouse gases causing this temperature increase -- we would be toast within a single generation.) The Sun's luminosity is negligibly increasing over time (fortunately) -- the Earth still has about a billion years in the habital zone (the region around a star where temperatures allow liquid water to form and exist for long periods of time).
4. From what we understand about the formation of the solar system (and this understanding is quite good now-a-days), the original Earth atmosphere had a similar percentage of molecular abundances as the current abundances of Venus and Mars, about 95-98% CO2, 2-5% N2, and trace amounts of argon and water vapor. Unlike Venus and Mars, the distance that the Earth is from the Sun allows water to exist primarily in a liquid state (however see the note below). Fortunately, liquid H2O chemically interacts with gaseous CO2 and the oceans acted as a filter reducing the CO2 abundance over time. As a matter of fact, much of this original CO2 atmosphere is now locked up in limestone rock and various clays. Fortunately back when the Earth had a substantial CO2 atmosphere, the Sun's luminosity was about 90% of its current value (we know this from a detailed understanding of stellar evolution and studying other one-solar mass stars that have formed within the past billion years), otherwise the Earth may had experienced a runaway greenhouse effect like it's neighbor Venus experienced (which is a whole other talk). Mars was too far away from the Sun for such a runaway greenhouse effect to take place. Also, without the greenhouse effect from this original Earth atmosphere, the Earth's surface would have been too cold to support liquid water during the Sun's early days on the main sequence (the era of a star when it fuses hydrogen into helium in its core) -- by the way, the Sun's main sequence lifetime is about 10 billion years. Since the solar system is about 5 billion years old, the Sun is mid-aged.
The bottom line is that the evidence is overwhelming that mankind is the cause of the current increasing atmospheric temperature.
This global warming problem is perhaps something that should concern us. Carl Sagan pointed out back in the 70s that if the atmospheric temperature increases too much (about 5 K or 10 F), the original atmospheric CO2 that is currently locked in the Earth's surface could start to sublimate (solid to gas phase change) out which could send Earth's surface into a runaway greenhouse event similar to what happened on Venus early in the history of the solar system. And once this sublimation starts, there is no stopping it. This would boil and fry the Earth's surface in a very short period of time (likely less than 100 years). So it's not just flooded coastlines that we might have to worry about.
The moral of this story: Isn't it better to be safe than sorry? Especially if your unable to fix the problem once it gets going?
Finally to clarify some misunderstandings. Global long-term climate changes are easier to model than short-term weather. The physics of weather is very non-linear and one needs to employ methods of chaos theory to model it (which results in answers described as probabilities). The physics of long-term climate evolution is not as complicated as short-term weather variation and has much smaller uncertainties (or standard deviations for those of you who are math-minded) as compared to weather uncertainties.
I hope this doesn't generate too much wrath in my direction.
1. Over the past century, there has been a "one-to-one" correlation between the increase of atmospheric CO2 and average atmospheric temperature rise averaged on a seasonal cycle. One need only examine a textbook on meteorology or freshman astronomy to see this data. Coincidentally, the industrial revolution started around the same epoch of this correlation. Both data were relatively flat over time prior to this.
2. Occasional large volcanic epsidoes have had some impact on the average atmospheric temperature, but these episodes have not had a lasting (i.e., more than a year or few) impact on the atmosphere.
3. The Sun's luminosity has remained relatively constant over the past 400 years (since mankind started measuring it). There are minor (less than 0.01 percent) changes due to the solar activity (sunspot/facula) cycle. The Sun is not causing this temperature increase. (And if it was, this would be far worse than manmade greenhouse gases causing this temperature increase -- we would be toast within a single generation.) The Sun's luminosity is negligibly increasing over time (fortunately) -- the Earth still has about a billion years in the habital zone (the region around a star where temperatures allow liquid water to form and exist for long periods of time).
4. From what we understand about the formation of the solar system (and this understanding is quite good now-a-days), the original Earth atmosphere had a similar percentage of molecular abundances as the current abundances of Venus and Mars, about 95-98% CO2, 2-5% N2, and trace amounts of argon and water vapor. Unlike Venus and Mars, the distance that the Earth is from the Sun allows water to exist primarily in a liquid state (however see the note below). Fortunately, liquid H2O chemically interacts with gaseous CO2 and the oceans acted as a filter reducing the CO2 abundance over time. As a matter of fact, much of this original CO2 atmosphere is now locked up in limestone rock and various clays. Fortunately back when the Earth had a substantial CO2 atmosphere, the Sun's luminosity was about 90% of its current value (we know this from a detailed understanding of stellar evolution and studying other one-solar mass stars that have formed within the past billion years), otherwise the Earth may had experienced a runaway greenhouse effect like it's neighbor Venus experienced (which is a whole other talk). Mars was too far away from the Sun for such a runaway greenhouse effect to take place. Also, without the greenhouse effect from this original Earth atmosphere, the Earth's surface would have been too cold to support liquid water during the Sun's early days on the main sequence (the era of a star when it fuses hydrogen into helium in its core) -- by the way, the Sun's main sequence lifetime is about 10 billion years. Since the solar system is about 5 billion years old, the Sun is mid-aged.
The bottom line is that the evidence is overwhelming that mankind is the cause of the current increasing atmospheric temperature.
This global warming problem is perhaps something that should concern us. Carl Sagan pointed out back in the 70s that if the atmospheric temperature increases too much (about 5 K or 10 F), the original atmospheric CO2 that is currently locked in the Earth's surface could start to sublimate (solid to gas phase change) out which could send Earth's surface into a runaway greenhouse event similar to what happened on Venus early in the history of the solar system. And once this sublimation starts, there is no stopping it. This would boil and fry the Earth's surface in a very short period of time (likely less than 100 years). So it's not just flooded coastlines that we might have to worry about.
The moral of this story: Isn't it better to be safe than sorry? Especially if your unable to fix the problem once it gets going?
Finally to clarify some misunderstandings. Global long-term climate changes are easier to model than short-term weather. The physics of weather is very non-linear and one needs to employ methods of chaos theory to model it (which results in answers described as probabilities). The physics of long-term climate evolution is not as complicated as short-term weather variation and has much smaller uncertainties (or standard deviations for those of you who are math-minded) as compared to weather uncertainties.
I hope this doesn't generate too much wrath in my direction.