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The biosphere has greatly shaped the past evolution of the Earth system. Here I argue that life evolved to maximize planetary entropy production. The evolution of the Earth system through time has thus evolved as far away from thermodynamic equilibrium as possible. I describe the implications of this hypothesis for the evolution of the global cycles of water and carbon and the implied consequences for biospheric evolution. This thermodynamic perspective of Earth’s biospheric evolution extends the views of Vernadski and Lovelock and puts it on a quantitative foundation.
Axel Kleidon (2009) studied this question.