Computer Science
Scientific paper
Feb 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ncimc...3...37s&link_type=abstract
Nuovo Cimento C, Serie 1, vol. 3C, Jan.-Feb. 1980, p. 37-44.
Computer Science
3
Black Body Radiation, Carnot Cycle, Planetary Radiation, Rotating Spheres, Thermodynamic Efficiency, Electromagnetic Interactions, Entropy, Planetary Surfaces, Radiative Transfer, Solar Terrestrial Interactions, Surface Reactions
Scientific paper
Consideration is given to the thermodynamics of the relationship between the external and internal interactions of a black planet with an external source of energy. Thermodynamic equations are derived for the case of a spherical planet with a skin made of a black, rigid, perfect heat conductor covered by a net of boundary lines representing a certain geometry, which is in a circular orbit around a star emitting a black-body spectrum. The approach thus provides a quantitative description of the work efficiency of a compound system with a natural separation between the entropy-producing channels and the zero-entropy channel, and results in a generalization of the concept of Carnot efficiency.
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