lpetrich
Contributor
Life On Earth To Hit Brick Wall In Another 500 Million Years
But as James Kasting points out, this thermostat is running out, and it will take the Earth's plant life with it.
It must be noted that it has only limited relevance for the CO2 that we are spewing into the atmosphere, because its reaction time is typically around a million years.
The decline is from the carbonate-silicate thermostat and the slow brightening of the Sun. Here is how the carbonate-silicate thermostat works. If the Earth has too little CO2, it tends to accumulate as volcanoes spew more and more of it into the air. But as it does so, it causes more and more of a greenhouse effect, heating the Earth's surface up. More heat, more weathering, and more consumption of CO2. That keeps the Earth's average surface temperature roughly constant over geological time. It has enabled tropical forests to exist for as long as there have been trees - the last 380 million years.Thus, as the sun’s luminosity grows and earth’s CO2 concentrations fall towards 150 parts per million (ppm), says Kasting, most of the world’s plants and trees will likely disappear. He says it’s possible that some of the biotic slack might be taken up by plants --- such as corn, sugar cane and tropical grasses --- that are able to function under such low CO2 concentrations.
“But it will be a very different planet,” said Kasting.
Kasting’s models point to the remaining plants going extinct 900 million years from now when CO2 levels falls below 10 parts per million (ppm).
But as James Kasting points out, this thermostat is running out, and it will take the Earth's plant life with it.
It must be noted that it has only limited relevance for the CO2 that we are spewing into the atmosphere, because its reaction time is typically around a million years.
But, in fact, Kasting says the inner edge of the habitable zone is “actually not that easy to find,” since it depends on clouds and relative humidity, neither of which, he says, can be easily calculated in a one-dimensional climate model. Yet, in any case, he notes this precipitous drop in earth’s atmospheric CO2 should occur at about the same projected rate.
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Although the sun won’t envelop earth for at least another five billion years, or long after our star turns into an expanding Red Giant, Kasting says the “punchline” is that earth won’t remain habitable through to the end of the sun's hydrogen-burning (or main sequence) phase.
“Bad things start to happen much earlier than that,” said Kasting.
Kasting suggests one alternative would be to geo-engineer our way around our sun's luminosity increase by constructing space-based solar shield.