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S. Franck, W. von Bloh, C. Bounama, and H.-J. Schellnhuber
In: V. Burdyuzha and G. Khozin (Eds.), The Future of the Universe
and the Future of our Civilization, World Scientific, Singapore, 309-315 (2000)
Potsdam Institute for Climate Impact Research (PIK),
Telegrafenberg, P.O. Box 60 12 03,
14412 Potsdam, Germany.
A geosphere-biosphere model to analyze the evolution of the Earth system on a global scale
from the geological past to the planetary future up to 1.5 billion years is presented. The Earth-system model consists of the components solid Earth, hydrosph
ere, atmosphere, and biosphere. It evolves under the external influence of increasing solar luminosity. The model is
based on a quasi-equilibrium formulation of the large-scale global carbon balance between the
main sources and the main sinks as modified by the biosphere. The state of parameters of the
Earth system determines the ``terrestrial life corridor'' for the existence of a
photosynthesis-based biosphere. In the case of the geostatic approximation the
results of Caldeira and Kasting (1992)
concerning the life span of the biosphere are reproduced. The
consideration of geodynamics in the new model reveals to a higher atmospheric carbon content for the past but a
much stronger decrease for the future. This leads to a reduction of the life span of the biosphere of up to some hundred million years (Franck et al., 2000). The habitable zone and the
optimum position of an Earth-like planet with maximum life span of any photosynthesis-based biosphere are calculated.
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