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The habitable zone on Earth will not last forever. Like most stars, the Sun exists in a stable configuration balanced between gravity pulling inward and pressure (maintained by heat from nuclear burning) pushing outward. This balance is self-regulating. Any slight change in one force will be off set by the other as long as there is enough fuel to maintain the burning. The solar system will undergo drastic change with the depletion of the hydrogen fuel. At the end of the evolution, the Earth may be still around, but any evidence that a biosphere once existed on the planet will have long since been melted
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Figure 09-28 The End of Life on Earth [view large image] |
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and re-crystallized into oblivion. Figure 09-28 presents an updated history of life on Earth from the 2016 issue of New Scientist. The scenario combines fossil evidences in the past and the theory of solar evolution for the future. |
Essentially, once life reaches its maximum prosperity, the decline is just the opposite of advance, i.e., from land to sea, from multicelluar to unicelluar, the final existence will linger hopelessly in underground cave to escape the scorching sun. The end of even such simple life would come about 7.5 billion years from now.