Abstract
As stars evolve and brighten, the radial zone within which liquid water can exist at the surface of an Earth-like planet expands outward. Using a new planetary climate model we have calculated the evolution of these habitable zones around several main sequence stars of masses between 0.50 and 1.25 solar masses. This evolution is presented in the form of a habitability continuum diagram for each star. We also give results for post main sequence evolution of the habitable zone around a 1.0 M⋅ star. The inner radius of the habitable zone is determined by the moist greenhouse effect and the outer radius is taken to be the distance at which a dense CO2 atmosphere begins to condense. Preliminary results indicate that the range of planetary radii for which liquid water can exist for > 4.5 Byr is considerably broader than previously calculated.
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References
Hart, M. H., The evolution of the atmosphere of the Earth, Icarus 33, 23–39 (1978).
Hart, M. H., Habitable zones about main sequence stars, Icarus 37 351–357 (1979).
Huang, S., Occurrence of life in the universe, American Scientist 47, 397–402 (1959).
Huang, S., Life outside the Solar System, Sci. Amer. 202, 55–63 (1960).
Iben, I., Stellar Evolution. VI. Evolution from the main sequence to the red-giant branch for stars of mass 1 M⋅, 1.25 M⋅, and 1.5 M⋅, Ap. J. 147, 624–649 (1967a).
Iben, I., Stellar evolution within and off the main sequence, Ann. Rev. Astron. Astrophys. 5, 571–626 (1967b).
Iben, I., Post main sequence evolution of single stars, Ann. Rev. Astron. Astrophys. 12, 215–256 (1974).
Iben, I. and Renzini, A., Asymptotic giant branch evolution and beyond, Ann. Rev. Astron. Astrophys. 21, 271–342 (1983).
Kasting, J. F., Pollack, J. B., and Ackerman, T. P., Response of Earth's atmosphere to increases in solar flux and implications for loss of water from Venus, Icarus 57, 335–355 (1984a).
Kasting, J. F., Pollack, J. B., and Crisp, D., Effects of high CO2 levels on surface temperature and atmospheric oxidation state of the early Earth, J. Atmos. Chem. 1, 403–428 (1984b).
Kasting, J. F., Runaway and moist greenhouse atmospheres and the evolution of Earth and Venus, Icarus 74, 472–494 (1988a).
Kasting, J. F., Toon, O., and Pollack, J. B., Sci. Amer. Feb., 90 (1988b).
Lovelock, J. E., and Watson, A. J., The regulation of carbon dioxide and climate, Planet Space Sci., 30, 795–802, 1982.
Schwartzman, D. W., and Volk, T., Geophysiology and habitable zones around Sun-like stars, this volume (1991).
Schwartzman, D. W., and Volk, T., Biotic enhancement of weathering and the habitability of Earth, Nature 340, 457–460 (1989).
Whitmire, D. P. and Reynolds, R. T., The fiery fate of the Solar System, Astronomy 18, 20–29, April (1990)
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© 1991 Springer-Verlag
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Whitmire, D.P., Reynolds, R.T., Kasting, J.F. (1991). Habitable zones for earth-like planets around main sequence stars. In: Heidmann, J., Klein, M.J. (eds) Bioastronomy. Lecture Notes in Physics, vol 390. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-54752-5_210
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DOI: https://doi.org/10.1007/3-540-54752-5_210
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